![1.12. Given points A(10, 12, −6), B(16, 8, −2), C(8, 1, −4), and D(−2, −5, 8), determine:
a) the vector projection of RAB + RBC on RAD: RAB + RBC = RAC = (8, 1, 4) − (10, 12, −6) =
(−2, −11, 10) Then RAD = (−2, −5, 8) − (10, 12, −6) = (−12, −17, 14). So the projection will
be:
(RAC · aRAD)aRAD = (−2, −11, 10) ·
(−12, −17, 14)
√
629
(−12, −17, 14)
√
629
= (−6.7, −9.5, 7.8)
b) the vector projection of RAB + RBC on RDC: RDC = (8, −1, 4) − (−2, −5, 8) = (10, 6, −4). The
projection is:
(RAC · aRDC)aRDC = (−2, −11, 10) ·
(10, 6, −4)
√
152
(10, 6, −4)
√
152
= (−8.3, −5.0, 3.3)
c) the angle between RDA and RDC: Use RDA = −RAD = (12, 17, −14) and RDC = (10, 6, −4).
The angle is found through the dot product of the associated unit vectors, or:
θD = cos−1
(aRDA · aRDC) = cos−1 (12, 17, −14) · (10, 6, −4)
√
629
√
152
= 26◦
1.13. a) Find the vector component of F = (10, −6, 5) that is parallel to G = (0.1, 0.2, 0.3):
F||G =
F · G
|G|2
G =
(10, −6, 5) · (0.1, 0.2, 0.3)
0.01 + 0.04 + 0.09
(0.1, 0.2, 0.3) = (0.93, 1.86, 2.79)
b) Find the vector component of F that is perpendicular to G:
FpG = F − F||G = (10, −6, 5) − (0.93, 1.86, 2.79) = (9.07, −7.86, 2.21)
c) Find the vector component of G that is perpendicular to F:
GpF = G−G||F = G−
G · F
|F|2
F = (0.1, 0.2, 0.3)−
1.3
100 + 36 + 25
(10, −6, 5) = (0.02, 0.25, 0.26)
1.14. The four vertices of a regular tetrahedron are located at O(0, 0, 0), A(0, 1, 0), B(0.5
√
3, 0.5, 0), and
C(
√
3/6, 0.5,
√
2/3).
a) Find a unit vector perpendicular (outward) to the face ABC: First find
RBA × RBC = [(0, 1, 0) − (0.5
√
3, 0.5, 0)] × [(
√
3/6, 0.5, 2/3) − (0.5
√
3, 0.5, 0)]
= (−0.5
√
3, 0.5, 0) × (−
√
3/3, 0, 2/3) = (0.41, 0.71, 0.29)
The required unit vector will then be:
RBA × RBC
|RBA × RBC|
= (0.47, 0.82, 0.33)
b) Find the area of the face ABC:
Area =
1
2
|RBA × RBC| = 0.43
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![1.17c. (continued) Now
1
2
(aAM + aAN ) =
1
2
[(0.697, 0.627, −0.348) + (−0.507, 0.406, 0.761)] = (0.095, 0.516, 0.207)
Finally,
abis =
(0.095, 0.516, 0.207)
|(0.095, 0.516, 0.207)|
= (0.168, 0.915, 0.367)
1.18. Given points A(ρ = 5, φ = 70◦, z = −3) and B(ρ = 2, φ = −30◦, z = 1), find:
a) unit vector in cartesian coordinates at A toward B: A(5 cos 70◦, 5 sin 70◦, −3) = A(1.71, 4.70, −3), In
the same manner, B(1.73, −1, 1). So RAB = (1.73, −1, 1) − (1.71, 4.70, −3) = (0.02, −5.70, 4) and
therefore
aAB =
(0.02, −5.70, 4)
|(0.02, −5.70, 4)|
= (0.003, −0.82, 0.57)
b) a vector in cylindrical coordinates at A directed toward B: aAB · aρ = 0.003 cos 70◦ − 0.82 sin 70◦ =
−0.77. aAB · aφ = −0.003 sin 70◦ − 0.82 cos 70◦ = −0.28. Thus
aAB = −0.77aρ − 0.28aφ + 0.57az
.
c) a unit vector in cylindrical coordinates at B directed toward A:
Use aBA = (−0, 003, 0.82, −0.57). Then aBA ·aρ = −0.003 cos(−30◦)+0.82 sin(−30◦) = −0.43, and
aBA · aφ = 0.003 sin(−30◦) + 0.82 cos(−30◦) = 0.71. Finally,
aBA = −0.43aρ + 0.71aφ − 0.57az
1.19 a) Express the field D = (x2 + y2)−1(xax + yay) in cylindrical components and cylindrical variables:
Have x = ρ cos φ, y = ρ sin φ, and x2 + y2 = ρ2. Therefore
D =
1
ρ
(cos φax + sin φay)
Then
Dρ = D · aρ =
1
ρ
cos φ(ax · aρ) + sin φ(ay · aρ) =
1
ρ
cos2
φ + sin2
φ =
1
ρ
and
Dφ = D · aφ =
1
ρ
cos φ(ax · aφ) + sin φ(ay · aφ) =
1
ρ
[cos φ(− sin φ) + sin φ cos φ] = 0
Therefore
D =
1
ρ
aρ
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![1.19b. Evaluate D at the point where ρ = 2, φ = 0.2π, and z = 5, expressing the result in cylindrical and
cartesian coordinates: At the given point, and in cylindrical coordinates, D = 0.5aρ. To express this in
cartesian, we use
D = 0.5(aρ · ax)ax + 0.5(aρ · ay)ay = 0.5 cos 36◦
ax + 0.5 sin 36◦
ay = 0.41ax + 0.29ay
1.20. Express in cartesian components:
a) the vector at A(ρ = 4, φ = 40◦, z = −2) that extends to B(ρ = 5, φ = −110◦, z = 2): We
have A(4 cos 40◦, 4 sin 40◦, −2) = A(3.06, 2.57, −2), and B(5 cos(−110◦), 5 sin(−110◦), 2) =
B(−1.71, −4.70, 2) in cartesian. Thus RAB = (−4.77, −7.30, 4).
b) a unit vector at B directed toward A: Have RBA = (4.77, 7.30, −4), and so
aBA =
(4.77, 7.30, −4)
|(4.77, 7.30, −4)|
= (0.50, 0.76, −0.42)
c) a unit vector at B directed toward the origin: Have rB = (−1.71, −4.70, 2), and so −rB =
(1.71, 4.70, −2). Thus
a =
(1.71, 4.70, −2)
|(1.71, 4.70, −2)|
= (0.32, 0.87, −0.37)
1.21. Express in cylindrical components:
a) the vector from C(3, 2, −7) to D(−1, −4, 2):
C(3, 2, −7) → C(ρ = 3.61, φ = 33.7◦, z = −7) and
D(−1, −4, 2) → D(ρ = 4.12, φ = −104.0◦, z = 2).
Now RCD = (−4, −6, 9) and Rρ = RCD · aρ = −4 cos(33.7) − 6 sin(33.7) = −6.66. Then
Rφ = RCD · aφ = 4 sin(33.7) − 6 cos(33.7) = −2.77. So RCD = −6.66aρ − 2.77aφ + 9az
b) a unit vector at D directed toward C:
RCD = (4, 6, −9) and Rρ = RDC · aρ = 4 cos(−104.0) + 6 sin(−104.0) = −6.79. Then Rφ =
RDC · aφ = 4[− sin(−104.0)] + 6 cos(−104.0) = 2.43. So RDC = −6.79aρ + 2.43aφ − 9az
Thus aDC = −0.59aρ + 0.21aφ − 0.78az
c) a unit vector at D directed toward the origin: Start with rD = (−1, −4, 2), and so the vector toward
the origin will be −rD = (1, 4, −2). Thus in cartesian the unit vector is a = (0.22, 0.87, −0.44).
Convert to cylindrical:
aρ = (0.22, 0.87, −0.44) · aρ = 0.22 cos(−104.0) + 0.87 sin(−104.0) = −0.90, and
aφ = (0.22, 0.87, −0.44) · aφ = 0.22[− sin(−104.0)] + 0.87 cos(−104.0) = 0, so that finally,
a = −0.90aρ − 0.44az.
1.22. A field is given in cylindrical coordinates as
F =
40
ρ2 + 1
+ 3(cos φ + sin φ) aρ + 3(cos φ − sin φ)aφ − 2az
where the magnitude of F is found to be:
|F| =
√
F · F =
1600
(ρ2 + 1)2
+
240
ρ2 + 1
(cos φ + sin φ) + 22
1/2
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![Sketch |F|:
a) vs. φ with ρ = 3: in this case the above simplifies to
|F(ρ = 3)| = |Fa| = [38 + 24(cos φ + sin φ)]1/2
b) vs. ρ with φ = 0, in which:
|F(φ = 0)| = |Fb| =
1600
(ρ2 + 1)2
+
240
ρ2 + 1
+ 22
1/2
c) vs. ρ with φ = 45◦, in which
|F(φ = 45◦
)| = |Fc| =
1600
(ρ2 + 1)2
+
240
√
2
ρ2 + 1
+ 22
1/2
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![CHAPTER 2
2.1. Four 10nC positive charges are located in the z = 0 plane at the corners of a square 8cm on a side.
A fifth 10nC positive charge is located at a point 8cm distant from the other charges. Calculate the
magnitude of the total force on this fifth charge for ǫ = ǫ0:
Arrange the charges in the xy plane at locations (4,4), (4,-4), (-4,4), and (-4,-4). Then the fifth charge
will be on the z axis at location z = 4
√
2, which puts it at 8cm distance from the other four. By
symmetry, the force on the fifth charge will be z-directed, and will be four times the z component of
force produced by each of the four other charges.
F =
4
√
2
×
q2
4πǫ0d2
=
4
√
2
×
(10−8)2
4π(8.85 × 10−12)(0.08)2
= 4.0 × 10−4
N
2.2. A charge Q1 = 0.1 µC is located at the origin, while Q2 = 0.2 µC is at A(0.8, −0.6, 0). Find the
locus of points in the z = 0 plane at which the x component of the force on a third positive charge is
zero.
To solve this problem, the z coordinate of the third charge is immaterial, so we can place it in the
xy plane at coordinates (x, y, 0). We take its magnitude to be Q3. The vector directed from the first
charge to the third is R13 = xax + yay; the vector directed from the second charge to the third is
R23 = (x − 0.8)ax + (y + 0.6)ay. The force on the third charge is now
F3 =
Q3
4πǫ0
Q1R13
|R13|3
+
Q2R23
|R23|3
=
Q3 × 10−6
4πǫ0
0.1(xax + yay)
(x2 + y2)1.5
+
0.2[(x − 0.8)ax + (y + 0.6)ay]
[(x − 0.8)2 + (y + 0.6)2]1.5
We desire the x component to be zero. Thus,
0 =
0.1xax
(x2 + y2)1.5
+
0.2(x − 0.8)ax
[(x − 0.8)2 + (y + 0.6)2]1.5
or
x[(x − 0.8)2
+ (y + 0.6)2
]1.5
= 2(0.8 − x)(x2
+ y2
)1.5
2.3. Point charges of 50nC each are located at A(1, 0, 0), B(−1, 0, 0), C(0, 1, 0), and D(0, −1, 0) in free
space. Find the total force on the charge at A.
The force will be:
F =
(50 × 10−9)2
4πǫ0
RCA
|RCA|3
+
RDA
|RDA|3
+
RBA
|RBA|3
where RCA = ax − ay, RDA = ax + ay, and RBA = 2ax. The magnitudes are |RCA| = |RDA| =
√
2,
and |RBA| = 2. Substituting these leads to
F =
(50 × 10−9)2
4πǫ0
1
2
√
2
+
1
2
√
2
+
2
8
ax = 21.5ax µN
where distances are in meters.
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![2.4. Let Q1 = 8 µC be located at P1(2, 5, 8) while Q2 = −5 µC is at P2(6, 15, 8). Let ǫ = ǫ0.
a) Find F2, the force on Q2: This force will be
F2 =
Q1Q2
4πǫ0
R12
|R12|3
=
(8 × 10−6)(−5 × 10−6)
4πǫ0
(4ax + 10ay)
(116)1.5
= (−1.15ax − 2.88ay) mN
b) Find the coordinates of P3 if a charge Q3 experiences a total force F3 = 0 at P3: This force in
general will be:
F3 =
Q3
4πǫ0
Q1R13
|R13|3
+
Q2R23
|R23|3
where R13 = (x − 2)ax + (y − 5)ay and R23 = (x − 6)ax + (y − 15)ay. Note, however, that
all three charges must lie in a straight line, and the location of Q3 will be along the vector R12
extended past Q2. The slope of this vector is (15 − 5)/(6 − 2) = 2.5. Therefore, we look for P3
at coordinates (x, 2.5x, 8). With this restriction, the force becomes:
F3 =
Q3
4πǫ0
8[(x − 2)ax + 2.5(x − 2)ay]
[(x − 2)2 + (2.5)2(x − 2)2]1.5
−
5[(x − 6)ax + 2.5(x − 6)ay]
[(x − 6)2 + (2.5)2(x − 6)2]1.5
where we require the term in large brackets to be zero. This leads to
8(x − 2)[((2.5)2
+ 1)(x − 6)2
]1.5
− 5(x − 6)[((2.5)2
+ 1)(x − 2)2
]1.5
= 0
which reduces to
8(x − 6)2
− 5(x − 2)2
= 0
or
x =
6
√
8 − 2
√
5
√
8 −
√
5
= 21.1
The coordinates of P3 are thus P3(21.1, 52.8, 8)
2.5. Let a point charge Q125 nC be located at P1(4, −2, 7) and a charge Q2 = 60 nC be at P2(−3, 4, −2).
a) If ǫ = ǫ0, find E at P3(1, 2, 3): This field will be
E =
10−9
4πǫ0
25R13
|R13|3
+
60R23
|R23|3
where R13 = −3ax +4ay −4az and R23 = 4ax −2ay +5az. Also, |R13| =
√
41 and |R23| =
√
45.
So
E =
10−9
4πǫ0
25 × (−3ax + 4ay − 4az)
(41)1.5
+
60 × (4ax − 2ay + 5az)
(45)1.5
= 4.58ax − 0.15ay + 5.51az
b) At what point on the y axis is Ex = 0? P3 is now at (0, y, 0), so R13 = −4ax + (y + 2)ay − 7az
and R23 = 3ax + (y − 4)ay + 2az. Also, |R13| = 65 + (y + 2)2 and |R23| = 13 + (y − 4)2.
Now the x component of E at the new P3 will be:
Ex =
10−9
4πǫ0
25 × (−4)
[65 + (y + 2)2]1.5
+
60 × 3
[13 + (y − 4)2]1.5
To obtain Ex = 0, we require the expression in the large brackets to be zero. This expression
simplifies to the following quadratic:
0.48y2
+ 13.92y + 73.10 = 0
which yields the two values: y = −6.89, −22.11
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![2.9. A 100 nC point charge is located at A(−1, 1, 3) in free space.
a) Find the locus of all points P (x, y, z) at which Ex = 500 V/m: The total field at P will be:
EP =
100 × 10−9
4πǫ0
RAP
|RAP |3
where RAP = (x + 1)ax + (y − 1)ay + (z − 3)az, and where |RAP | = [(x + 1)2 + (y − 1)2 +
(z − 3)2]1/2. The x component of the field will be
Ex =
100 × 10−9
4πǫ0
(x + 1)
[(x + 1)2 + (y − 1)2 + (z − 3)2]1.5
= 500 V/m
And so our condition becomes:
(x + 1) = 0.56 [(x + 1)2
+ (y − 1)2
+ (z − 3)2
]1.5
b) Find y1 if P (−2, y1, 3) lies on that locus: At point P , the condition of part a becomes
3.19 = 1 + (y1 − 1)2
3
from which (y1 − 1)2 = 0.47, or y1 = 1.69 or 0.31
2.10. Charges of 20 and -20 nC are located at (3, 0, 0) and (−3, 0, 0), respectively. Let ǫ = ǫ0.
Determine |E| at P (0, y, 0): The field will be
EP =
20 × 10−9
4πǫ0
R1
|R1|3
−
R2
|R2|3
where R1, the vector from the positive charge to point P is (−3, y, 0), and R2, the vector from
the negative charge to point P , is (3, y, 0). The magnitudes of these vectors are |R1| = |R2| =
9 + y2. Substituting these into the expression for EP produces
EP =
20 × 10−9
4πǫ0
−6ax
(9 + y2)1.5
from which
|EP | =
1079
(9 + y2)1.5
V/m
2.11. A charge Q0 located at the origin in free space produces a field for which Ez = 1 kV/m at point
P (−2, 1, −1).
a) Find Q0: The field at P will be
EP =
Q0
4πǫ0
−2ax + ay − az
61.5
Since the z component is of value 1 kV/m, we find Q0 = −4πǫ061.5 × 103 = −1.63 µC.
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![2.11. (continued)
b) Find E at M(1, 6, 5) in cartesian coordinates: This field will be:
EM =
−1.63 × 10−6
4πǫ0
ax + 6ay + 5az
[1 + 36 + 25]1.5
or EM = −30.11ax − 180.63ay − 150.53az.
c) Find E at M(1, 6, 5) in cylindrical coordinates: At M, ρ =
√
1 + 36 = 6.08, φ = tan−1(6/1) =
80.54◦, and z = 5. Now
Eρ = EM · aρ = −30.11 cos φ − 180.63 sin φ = −183.12
Eφ = EM · aφ = −30.11(− sin φ) − 180.63 cos φ = 0 (as expected)
so that EM = −183.12aρ − 150.53az.
d) Find E at M(1, 6, 5) in spherical coordinates: At M, r =
√
1 + 36 + 25 = 7.87, φ = 80.54◦ (as
before), and θ = cos−1(5/7.87) = 50.58◦. Now, since the charge is at the origin, we expect to
obtain only a radial component of EM. This will be:
Er = EM · ar = −30.11 sin θ cos φ − 180.63 sin θ sin φ − 150.53 cos θ = −237.1
2.12. The volume charge density ρv = ρ0e−|x|−|y|−|z| exists over all free space. Calculate the total charge
present: This will be 8 times the integral of ρv over the first octant, or
Q = 8
∞
0
∞
0
∞
0
ρ0e−x−y−z
dx dy dz = 8ρ0
2.13. A uniform volume charge density of 0.2 µC/m3 (note typo in book) is present throughout the spherical
shell extending from r = 3 cm to r = 5 cm. If ρv = 0 elsewhere:
a) find the total charge present throughout the shell: This will be
Q =
2π
0
π
0
.05
.03
0.2 r2
sin θ dr dθ dφ = 4π(0.2)
r3
3
.05
.03
= 8.21 × 10−5
µC = 82.1 pC
b) find r1 if half the total charge is located in the region 3 cm < r < r1: If the integral over r in part
a is taken to r1, we would obtain
4π(0.2)
r3
3
r1
.03
= 4.105 × 10−5
Thus
r1 =
3 × 4.105 × 10−5
0.2 × 4π
+ (.03)3
1/3
= 4.24 cm
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![2.18. (continued)
b) Find E at Q(2, 3, 4): This field will in general be:
EQ =
ρl
2πǫ0
R+Q
|R+Q|
−
R−Q
|R−Q|
where R+Q = (2, 3, 4)−(0, −.6, 4) = (2, 3.6, 0), and R−Q = (2, 3, 4)−(0, .6, 4) = (2, 2.4, 0).
Thus
EQ =
ρl
2πǫ0
2ax + 3.6ay
22 + (3.6)2
−
2ax + 2.4ay
22 + (2.4)2
= −625.8ax − 241.6ay V/m
2.19. A uniform line charge of 2 µC/m is located on the z axis. Find E in cartesian coordinates at P (1, 2, 3)
if the charge extends from
a) −∞ < z < ∞: With the infinite line, we know that the field will have only a radial component
in cylindrical coordinates (or x and y components in cartesian). The field from an infinite line on
the z axis is generally E = [ρl/(2πǫ0ρ)]aρ. Therefore, at point P :
EP =
ρl
2πǫ0
RzP
|RzP |2
=
(2 × 10−6)
2πǫ0
ax + 2ay
5
= 7.2ax + 14.4ay kV/m
where RzP is the vector that extends from the line charge to point P, and is perpendicular to the z
axis; i.e., RzP = (1, 2, 3) − (0, 0, 3) = (1, 2, 0).
b) −4 ≤ z ≤ 4: Here we use the general relation
EP =
ρldz
4πǫ0
r − r′
|r − r′|3
where r = ax + 2ay + 3az and r′ = zaz. So the integral becomes
EP =
(2 × 10−6)
4πǫ0
4
−4
ax + 2ay + (3 − z)az
[5 + (3 − z)2]1.5
dz
Using integral tables, we obtain:
EP = 3597
(ax + 2ay)(z − 3) + 5az
(z2 − 6z + 14)
4
−4
V/m = 4.9ax + 9.8ay + 4.9az kV/m
The student is invited to verify that when evaluating the above expression over the limits −∞ <
z < ∞, the z component vanishes and the x and y components become those found in part a.
2.20. Uniform line charges of 120 nC/m lie along the entire extent of the three coordinate axes. Assuming
free space conditions, find E at P (−3, 2, −1): Since all line charges are infinitely-long, we can write:
EP =
ρl
2πǫ0
RxP
|RxP |2
+
RyP
|RyP |2
+
RzP
|RzP |2
where RxP , RyP , and RzP are the normal vectors from each of the three axes that terminate on point
P . Specifically, RxP = (−3, 2, −1) − (−3, 0, 0) = (0, 2, −1), RyP = (−3, 2, −1) − (0, 2, 0) =
(−3, 0, −1), and RzP = (−3, 2, −1) − (0, 0, −1) = (−3, 2, 0). Substituting these into the expression
for EP gives
EP =
ρl
2πǫ0
2ay − az
5
+
−3ax − az
10
+
−3ax + 2ay
13
= −1.15ax + 1.20ay − 0.65az kV/m
21
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![2.21. Two identical uniform line charges with ρl = 75 nC/m are located in free space at x = 0, y = ±0.4 m.
What force per unit length does each line charge exert on the other? The charges are parallel to the z
axis and are separated by 0.8 m. Thus the field from the charge at y = −0.4 evaluated at the location
of the charge at y = +0.4 will be E = [ρl/(2πǫ0(0.8))]ay. The force on a differential length of the
line at the positive y location is dF = dqE = ρldzE. Thus the force per unit length acting on the line
at postive y arising from the charge at negative y is
F =
1
0
ρ2
l dz
2πǫ0(0.8)
ay = 1.26 × 10−4
ay N/m = 126 ay µN/m
The force on the line at negative y is of course the same, but with −ay.
2.22. A uniform surface charge density of 5 nC/m2 is present in the region x = 0, −2 < y < 2, and all z. If
ǫ = ǫ0, find E at:
a) PA(3, 0, 0): We use the superposition integral:
E =
ρsda
4πǫ0
r − r′
|r − r′|3
where r = 3ax and r′ = yay + zaz. The integral becomes:
EP A =
ρs
4πǫ0
∞
−∞
2
−2
3ax − yay − zaz
[9 + y2 + z2]1.5
dy dz
Since the integration limits are symmetric about the origin, and since the y and z components of
the integrand exhibit odd parity (change sign when crossing the origin, but otherwise symmetric),
these will integrate to zero, leaving only the x component. This is evident just from the symmetry
of the problem. Performing the z integration first on the x component, we obtain (using tables):
Ex,PA =
3ρs
4πǫ0
2
−2
dy
(9 + y2)
z
9 + y2 + z2
∞
−∞
=
3ρs
2πǫ0
2
−2
dy
(9 + y2)
=
3ρs
2πǫ0
1
3
tan−1 y
3
2
−2 = 106 V/m
The student is encouraged to verify that if the y limits were −∞ to ∞, the result would be that of
the infinite charged plane, or Ex = ρs/(2ǫ0).
b) PB(0, 3, 0): In this case, r = 3ay, and symmetry indicates that only a y component will exist.
The integral becomes
Ey,P B =
ρs
4πǫ0
∞
−∞
2
−2
(3 − y) dy dz
[(z2 + 9) − 6y + y2]1.5
=
ρs
2πǫ0
2
−2
(3 − y) dy
(3 − y)2
= −
ρs
2πǫ0
ln(3 − y) 2
−2 = 145 V/m
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![2.27. Given the electric field E = (4x − 2y)ax − (2x + 4y)ay, find:
a) the equation of the streamline that passes through the point P (2, 3, −4): We write
dy
dx
=
Ey
Ex
=
−(2x + 4y)
(4x − 2y)
Thus
2(x dy + y dx) = y dy − x dx
or
2 d(xy) =
1
2
d(y2
) −
1
2
d(x2
)
So
C1 + 2xy =
1
2
y2
−
1
2
x2
or
y2
− x2
= 4xy + C2
Evaluating at P (2, 3, −4), obtain:
9 − 4 = 24 + C2, or C2 = −19
Finally, at P , the requested equation is
y2
− x2
= 4xy − 19
b) a unit vector specifying the direction of E at Q(3, −2, 5): Have EQ = [4(3) + 2(2)]ax − [2(3) −
4(2)]ay = 16ax + 2ay. Then |E| =
√
162 + 4 = 16.12 So
aQ =
16ax + 2ay
16.12
= 0.99ax + 0.12ay
2.28. Let E = 5x3 ax − 15x2y ay, and find:
a) the equation of the streamline that passes through P (4, 2, 1): Write
dy
dx
=
Ey
Ex
=
−15x2y
5x3
=
−3y
x
So
dy
y
= −3
dx
x
⇒ ln y = −3 ln x + ln C
Thus
y = e−3 ln x
eln C
=
C
x3
At P , have 2 = C/(4)3 ⇒ C = 128. Finally, at P ,
y =
128
x3
24
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![3.2c. (continued) The total charge enclosed in the sphere (and the outward flux from it) is now
Ql + Qp = 2(1.94)(−50 × 10−9
) + 2(1.73)(80 × 10−9
) + 12 × 10−9
= 348 nC
3.3. The cylindrical surface ρ = 8 cm contains the surface charge density, ρs = 5e−20|z| nC/m2.
a) What is the total amount of charge present? We integrate over the surface to find:
Q = 2
∞
0
2π
0
5e−20z
(.08)dφ dz nC = 20π(.08)
−1
20
e−20z
∞
0
= 0.25 nC
b) How much flux leaves the surface ρ = 8 cm, 1 cm < z < 5cm, 30◦ < φ < 90◦? We just integrate
the charge density on that surface to find the flux that leaves it.
= Q′
=
.05
.01
90◦
30◦
5e−20z
(.08) dφ dz nC =
90 − 30
360
2π(5)(.08)
−1
20
e−20z
.05
.01
= 9.45 × 10−3
nC = 9.45 pC
3.4. The cylindrical surfaces ρ = 1, 2, and 3 cm carry uniform surface charge densities of 20, −8, and 5
nC/m2, respectively.
a) How much electric flux passes through the closed surface ρ = 5 cm, 0 < z < 1 m? Since the
densities are uniform, the flux will be
= 2π(aρs1 + bρs2 + cρs3)(1 m) = 2π [(.01)(20) − (.02)(8) + (.03)(5)] × 10−9
= 1.2 nC
b) Find D at P (1 cm, 2 cm, 3 cm): This point lies at radius
√
5 cm, and is thus inside the outermost
charge layer. This layer, being of uniform density, will not contribute to D at P . We know that in
cylindrical coordinates, the layers at 1 and 2 cm will produce the flux density:
D = Dρaρ =
aρs1 + bρs2
ρ
aρ
or
Dρ =
(.01)(20) + (.02)(−8)
√
.05
= 1.8 nC/m2
At P , φ = tan−1(2/1) = 63.4◦. Thus Dx = 1.8 cos φ = 0.8 and Dy = 1.8 sin φ = 1.6. Finally,
DP = (0.8ax + 1.6ay) nC/m2
28
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![3.5. Let D = 4xyax + 2(x2 + z2)ay + 4yzaz C/m2 and evaluate surface integrals to find the total charge
enclosed in the rectangular parallelepiped 0 < x < 2, 0 < y < 3, 0 < z < 5 m: Of the 6 surfaces to
consider, only 2 will contribute to the net outward flux. Why? First consider the planes at y = 0 and 3.
The y component of D will penetrate those surfaces, but will be inward at y = 0 and outward at y = 3,
while having the same magnitude in both cases. These fluxes will thus cancel. At the x = 0 plane,
Dx = 0 and at the z = 0 plane, Dz = 0, so there will be no flux contributions from these surfaces.
This leaves the 2 remaining surfaces at x = 2 and z = 5. The net outward flux becomes:
=
5
0
3
0
D x=2
· ax dy dz +
3
0
2
0
D z=5
· az dx dy
= 5
3
0
4(2)y dy + 2
3
0
4(5)y dy = 360 C
3.6. Two uniform line charges, each 20 nC/m, are located at y = 1, z = ±1 m. Find the total flux leaving a
sphere of radius 2 m if it is centered at
a) A(3, 1, 0): The result will be the same if we move the sphere to the origin and the line charges to
(0, 0, ±1). The length of the line charge within the sphere is given by l = 4 sin[cos−1(1/2)] =
3.46. With two line charges, symmetrically arranged, the total charge enclosed is given by Q =
2(3.46)(20 nC/m) = 139 nC
b) B(3, 2, 0): In this case the result will be the same if we move the sphere to the origin and keep
the charges where they were. The length of the line joining the origin to the midpoint of the line
charge (in the yz plane) is l1 =
√
2. The length of the line joining the origin to either endpoint
of the line charge is then just the sphere radius, or 2. The half-angle subtended at the origin by
the line charge is then ψ = cos−1(
√
2/2) = 45◦. The length of each line charge in the sphere
is then l2 = 2 × 2 sin ψ = 2
√
2. The total charge enclosed (with two line charges) is now
Q′ = 2(2
√
2)(20 nC/m) = 113 nC
3.7. Volume charge density is located in free space as ρv = 2e−1000r nC/m3 for 0 < r < 1 mm, and ρv = 0
elsewhere.
a) Find the total charge enclosed by the spherical surface r = 1 mm: To find the charge we integrate:
Q =
2π
0
π
0
.001
0
2e−1000r
r2
sin θ dr dθ dφ
Integration over the angles gives a factor of 4π. The radial integration we evaluate using tables;
we obtain
Q = 8π
−r2e−1000r
1000
.001
0
+
2
1000
e−1000r
(1000)2
(−1000r − 1)
.001
0
= 4.0 × 10−9
nC
b) By using Gauss’s law, calculate the value of Dr on the surface r = 1 mm: The gaussian surface
is a spherical shell of radius 1 mm. The enclosed charge is the result of part a. We thus write
4πr2Dr = Q, or
Dr =
Q
4πr2
=
4.0 × 10−9
4π(.001)2
= 3.2 × 10−4
nC/m2
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![3.8. Uniform line charges of 5 nC/m ar located in free space at x = 1, z = 1, and at y = 1, z = 0.
a) Obtain an expression for D in cartesian coordinates at P (0, 0, z). In general, we have
D(z) =
ρs
2π
r1 − r′
1
|r1 − r′
1|2
+
r2 − r′
2
|r2 − r′
2|2
where r1 = r2 = zaz, r′
1 = ay, and r′
2 = ax + az. Thus
D(z) =
ρs
2π
[zaz − ay]
[1 + z2]
+
[(z − 1)az − ax]
[1 + (z − 1)2]
=
ρs
2π
−ax
[1 + (z − 1)2]
−
ay
[1 + z2]
+
(z − 1)
[1 + (z − 1)2]
+
z
[1 + z2]
az
b) Plot |D| vs. z at P , −3 < z < 10: Using part a, we find the magnitude of D to be
|D| =
ρs
2π
1
[1 + (z − 1)2]2
+
1
[1 + z2]2
+
(z − 1)
[1 + (z − 1)2]
+
z
[1 + z2]
2 1/2
A plot of this over the specified range is shown in Prob3.8.pdf.
3.9. A uniform volume charge density of 80 µC/m3 is present throughout the region 8 mm < r < 10 mm.
Let ρv = 0 for 0 < r < 8 mm.
a) Find the total charge inside the spherical surface r = 10 mm: This will be
Q =
2π
0
π
0
.010
.008
(80 × 10−6
)r2
sin θ dr dθ dφ = 4π × (80 × 10−6
)
r3
3
.010
.008
= 1.64 × 10−10
C = 164 pC
b) Find Dr at r = 10 mm: Using a spherical gaussian surface at r = 10, Gauss’ law is written as
4πr2Dr = Q = 164 × 10−12, or
Dr(10 mm) =
164 × 10−12
4π(.01)2
= 1.30 × 10−7
C/m2
= 130 nC/m2
c) If there is no charge for r > 10 mm, find Dr at r = 20 mm: This will be the same computation
as in part b, except the gaussian surface now lies at 20 mm. Thus
Dr(20 mm) =
164 × 10−12
4π(.02)2
= 3.25 × 10−8
C/m2
= 32.5 nC/m2
3.10. Let ρs = 8 µC/m2 in the region where x = 0 and −4 < z < 4 m, and let ρs = 0 elsewhere. Find D at
P (x, 0, z), where x > 0: The sheet charge can be thought of as an assembly of infinitely-long parallel
strips that lie parallel to the y axis in the yz plane, and where each is of thickness dz. The field from
each strip is that of an infinite line charge, and so we can construct the field at P from a single strip as:
dDP =
ρs dz′
2π
r − r′
|r − r′|2
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![3.10 (continued) where r = xax + zaz and r′ = z′az We distinguish between the fixed coordinate of P , z,
and the variable coordinate, z′, that determines the location of each charge strip. To find the net field at
P, we sum the contributions of each strip by integrating over z′:
DP =
4
−4
8 × 10−6 dz′ (xax + (z − z′)az)
2π[x2 + (z − z′)2]
We can re-arrange this to determine the integral forms:
DP =
8 × 10−6
2π
(xax + zaz)
4
−4
dz′
(x2 + z2) − 2zz′ + (z′)2
− az
4
−4
z′ dz′
(x2 + z2) − 2zz′ + (z′)2
Using integral tables, we find
DP =
4 × 10−6
π
(xax + zaz)
1
x
tan−1 2z′ − 2z
2x
−
1
2
ln(x2
+ z2
− 2zz′
+ (z′
)2
) +
2z
2
1
x
tan−1 2z′ − 2z
2x
az
4
−4
which evaluates as
DP =
4 × 10−6
π
tan−1 z + 4
x
− tan−1 z − 4
x
ax +
1
2
ln
x2 + (z + 4)2
x2 + (z − 4)2
az C/m2
The student is invited to verify that for very small x or for a very large sheet (allowing z′ to approach
infinity), the above expression reduces to the expected form, DP = ρs/2. Note also that the expression
is valid for all x (positive or negative values).
3.11. In cylindrical coordinates, let ρv = 0 for ρ < 1 mm, ρv = 2 sin(2000πρ) nC/m3 for 1 mm < ρ <
1.5 mm, and ρv = 0 for ρ > 1.5 mm. Find D everywhere: Since the charge varies only with radius,
and is in the form of a cylinder, symmetry tells us that the flux density will be radially-directed and will
be constant over a cylindrical surface of a fixed radius. Gauss’ law applied to such a surface of unit
length in z gives:
a) for ρ < 1 mm, Dρ = 0, since no charge is enclosed by a cylindrical surface whose radius lies
within this range.
b) for 1 mm < ρ < 1.5 mm, we have
2πρDρ = 2π
ρ
.001
2 × 10−9
sin(2000πρ′
)ρ′
dρ′
= 4π × 10−9 1
(2000π)2
sin(2000πρ) −
ρ
2000π
cos(2000πρ)
ρ
.001
or finally,
Dρ =
10−15
2π2ρ
sin(2000πρ) + 2π 1 − 103
ρ cos(2000πρ) C/m2
(1 mm < ρ < 1.5 mm)
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![3.14b. find Dρ for ρ > 1 mm: The Gaussian cylinder now lies outside the charge, so
2πρDρ = π(.001)2
(5 × 10−9
) ⇒ Dρ =
2.5 × 10−15
ρ
C/m2
c) What line charge ρL at ρ = 0 would give the same result for part b? The line charge field will be
Dr =
ρL
2πρ
=
2.5 × 10−15
ρ
(part b)
Thus ρL = 5π × 10−15 C/m. In all answers, ρ is expressed in meters.
3.15. Volume charge density is located as follows: ρv = 0 for ρ < 1 mm and for ρ > 2 mm, ρv = 4ρ µC/m3
for 1 < ρ < 2 mm.
a) Calculate the total charge in the region 0 < ρ < ρ1, 0 < z < L, where 1 < ρ1 < 2 mm: We find
Q =
L
0
2π
0
ρ1
.001
4ρ ρ dρ dφ dz =
8πL
3
[ρ3
1 − 10−9
] µC
where ρ1 is in meters.
b) Use Gauss’ law to determine Dρ at ρ = ρ1: Gauss’ law states that 2πρ1LDρ = Q, where Q is
the result of part a. Thus
Dρ(ρ1) =
4(ρ3
1 − 10−9)
3ρ1
µC/m2
where ρ1 is in meters.
c) Evaluate Dρ at ρ = 0.8 mm, 1.6 mm, and 2.4 mm: At ρ = 0.8 mm, no charge is enclosed by a
cylindrical gaussian surface of that radius, so Dρ(0.8mm) = 0. At ρ = 1.6 mm, we evaluate the
part b result at ρ1 = 1.6 to obtain:
Dρ(1.6mm) =
4[(.0016)3 − (.0010)3]
3(.0016)
= 3.6 × 10−6
µC/m2
At ρ = 2.4, we evaluate the charge integral of part a from .001 to .002, and Gauss’ law is written
as
2πρLDρ =
8πL
3
[(.002)2
− (.001)2
] µC
from which Dρ(2.4mm) = 3.9 × 10−6 µC/m2.
3.16. Given the electric flux density, D = 2xy ax + x2 ay + 6z3 az C/m2:
a) use Gauss’ law to evaluate the total charge enclosed in the volume 0 < x, y, z < a: We call the
surfaces at x = a and x = 0 the front and back surfaces respectively, those at y = a and y = 0
the right and left surfaces, and those at z = a and z = 0 the top and bottom surfaces. To evaluate
the total charge, we integrate D · n over all six surfaces and sum the results:
= Q = D · n da =
a
0
a
0
2ay dy dz
front
+
a
0
a
0
−2(0)y dy dz
back
+
a
0
a
0
−x2
dx dz
left
+
a
0
a
0
x2
dx dz
right
+
a
0
a
0
−6(0)3
dx dy
bottom
+
a
0
a
0
6a3
dx dy
top
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![3.22. Let D = 8ρ sin φ aρ + 4ρ cos φ aφ C/m2.
a) Find div D: Using the divergence formula for cylindrical coordinates (see problem 3.21), we find
∇ · D = 12 sin φ.
b) Find the volume charge density at P (2.6, 38◦, −6.1): Since ρv = ∇ · D, we evaluate the result of
part a at this point to find ρvP = 12 sin 38◦ = 7.39 C/m3.
c) How much charge is located inside the region defined by 0 < ρ < 1.8, 20◦ < φ < 70◦,
2.4 < z < 3.1? We use
Q =
vol
ρvdv =
3.1
2.4
70◦
20◦
1.8
0
12 sin φρ dρ dφ dz = −(3.1 − 2.4)12 cos φ
70◦
20◦
ρ2
2
1.8
0
= 8.13 C
3.23. a) A point charge Q lies at the origin. Show that div D is zero everywhere except at the origin. For
a point charge at the origin we know that D = Q/(4πr2) ar. Using the formula for divergence in
spherical coordinates (see problem 3.21 solution), we find in this case that
∇ · D =
1
r2
d
dr
r2 Q
4πr2
= 0
The above is true provided r > 0. When r = 0, we have a singularity in D, so its divergence is not
defined.
b) Replace the point charge with a uniform volume charge density ρv0 for 0 < r < a. Relate ρv0
to Q and a so that the total charge is the same. Find div D everywhere: To achieve the same net
charge, we require that (4/3)πa3ρv0 = Q, so ρv0 = 3Q/(4πa3) C/m3. Gauss’ law tells us that
inside the charged sphere
4πr2
Dr =
4
3
πr3
ρv0 =
Qr3
a3
Thus
Dr =
Qr
4πa3
C/m2
and ∇ · D =
1
r2
d
dr
Qr3
4πa3
=
3Q
4πa3
as expected. Outside the charged sphere, D = Q/(4πr2) ar as before, and the divergence is zero.
3.24. Inside the cylindrical shell, 3 < ρ < 4 m, the electric flux density is given as
D = 5(ρ − 3)3
aρ C/m2
a) What is the volume charge density at ρ = 4 m? In this case we have
ρv = ∇ · D =
1
ρ
d
dρ
(ρDρ) =
1
ρ
d
dρ
[5ρ(ρ − 3)3
] =
5(ρ − 3)2
ρ
(4ρ − 3) C/m3
Evaluating this at ρ = 4 m, we find ρv(4) = 16.25 C/m3
b) What is the electric flux density at ρ = 4 m? We evaluate the given D at this point to find
D(4) = 5 aρ C/m2
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![3.24c. How much electric flux leaves the closed surface 3 < ρ < 4, 0 < φ < 2π, −2.5 < z < 2.5? We note
that D has only a radial component, and so flux would leave only through the cylinder sides. Also, D
does not vary with φ or z, so the flux is found by a simple product of the side area and the flux density.
We further note that D = 0 at ρ = 3, so only the outer side (at ρ = 4) will contribute. We use the result
of part b, and write the flux as
= [2.5 − (−2.5)]2π(4)(5) = 200π C
d) How much charge is contained within the volume used in part c? By Gauss’ law, this will be the
same as the net outward flux through that volume, or again, 200π C.
3.25. Within the spherical shell, 3 < r < 4 m, the electric flux density is given as
D = 5(r − 3)3
ar C/m2
a) What is the volume charge density at r = 4? In this case we have
ρv = ∇ · D =
1
r2
d
dr
(r2
Dr) =
5
r
(r − 3)2
(5r − 6) C/m3
which we evaluate at r = 4 to find ρv(r = 4) = 17.50 C/m3.
b) What is the electric flux density at r = 4? Substitute r = 4 into the given expression to
find D(4) = 5 ar C/m2
c) How much electric flux leaves the sphere r = 4? Using the result of part b, this will be =
4π(4)2(5) = 320π C
d) How much charge is contained within the sphere, r = 4? From Gauss’ law, this will be the same
as the outward flux, or again, Q = 320π C.
3.26. Given the field
D =
5 sin θ cos φ
r
ar C/m2
,
find:
a) the volume charge density: Use
ρv = ∇ · D =
1
r2
d
dr
(r2
Dr) =
5 sin θ cos φ
r2
C/m3
b) the total charge contained within the region r < 2 m: To find this, we integrate over the volume:
Q =
2π
0
π
0
2
0
5 sin θ cos φ
r2
r2
sin θ dr dθ dφ
Before plunging into this one notice that the φ integration is of cos φ from zero to 2π. This yields
a zero result, and so the total enclosed charge is Q = 0.
c) the value of D at the surface r = 2: Substituting r = 2 into the given field produces
D(r = 2) =
5
2
sin θ cos φ ar C/m2
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![3.29b. Evaluate the surface integral side for the corresponding closed surface: We call the surfaces at x = 3
and x = 2 the front and back surfaces respectively, those at y = 3 and y = 2 the right and left surfaces,
and those at z = 3 and z = 2 the top and bottom surfaces. To evaluate the surface integral side, we
integrate D · n over all six surfaces and sum the results. Note that since the x component of D does not
vary with x, the outward fluxes from the front and back surfaces will cancel each other. The same is
true for the left and right surfaces, since Dy does not vary with y. This leaves only the top and bottom
surfaces, where the fluxes are:
D · dS =
3
2
3
2
−4xy
32
dxdy
top
−
3
2
3
2
−4xy
22
dxdy
bottom
= (9 − 4)(9 − 4)
1
4
−
1
9
= 3.47 C
3.30. If D = 15ρ2 sin 2φ aρ + 10ρ2 cos 2φ aφ C/m2, evaluate both sides of the divergence theorem for the
region 1 < ρ < 2 m, 1 < φ < 2 rad, 1 < z < 2 m: Taking the surface integral side first, the six sides
over which the flux must be evaluated are only four, since there is no z component of D. We are left
with the sides at φ = 1 and φ = 2 rad (left and right sides, respectively), and those at ρ = 1 and ρ = 2
(back and front sides). We evaluate
D · dS =
2
1
2
1
15(2)2
sin(2φ) (2)dφdz
front
−
2
1
2
1
15(1)2
sin(2φ) (1)dφdz
back
−
2
1
2
1
10ρ2
cos(2) dρdz
left
+
2
1
2
1
10ρ2
cos(4) dρdz
right
= 6.93 C
For the volume integral side, we first evaluate the divergence of D, which is
∇ · D =
1
ρ
∂
∂ρ
(15ρ3
sin 2φ) +
1
ρ
∂
∂φ
(10ρ2
cos 2φ) = 25ρ sin 2φ
Next
vol
∇ · D dv =
2
1
2
1
2
1
25ρ sin(2φ) ρdρ dφ dz =
25
3
ρ3
2
1
− cos(2φ)
2
2
1
= 6.93 C
3.31. Given the flux density
D =
16
r
cos(2θ) aθ C/m2
,
use two different methods to find the total charge within the region 1 < r < 2 m, 1 < θ < 2 rad,
1 < φ < 2 rad: We use the divergence theorem and first evaluate the surface integral side. We are
evaluating the net outward flux through a curvilinear “cube”, whose boundaries are defined by the
specified ranges. The flux contributions will be only through the surfaces of constant θ, however, since
D has only a θ component. On a constant-theta surface, the differential area is da = r sin θdrdφ,
where θ is fixed at the surface location. Our flux integral becomes
D · dS = −
2
1
2
1
16
r
cos(2) r sin(1) drdφ
θ=1
+
2
1
2
1
16
r
cos(4) r sin(2) drdφ
θ=2
= −16 [cos(2) sin(1) − cos(4) sin(2)] = −3.91 C
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![3.31. (continued) We next evaluate the volume integral side of the divergence theorem, where in this case,
∇ · D =
1
r sin θ
d
dθ
(sin θ Dθ ) =
1
r sin θ
d
dθ
16
r
cos 2θ sin θ =
16
r2
cos 2θ cos θ
sin θ
− 2 sin 2θ
We now evaluate:
vol
∇ · D dv =
2
1
2
1
2
1
16
r2
cos 2θ cos θ
sin θ
− 2 sin 2θ r2
sin θ drdθdφ
The integral simplifies to
2
1
2
1
2
1
16[cos 2θ cos θ − 2 sin 2θ sin θ] drdθdφ = 8
2
1
[3 cos 3θ − cos θ] dθ = −3.91 C
3.32. If D = 2r ar C/m2, find the total electric flux leaving the surface of the cube, 0 < x, y, z < 0.4: This
is where the divergence theorem really saves you time! First find
∇ · D =
1
r2
d
dr
(r2
× 2r) = 6
Then the net outward flux will be
vol
∇ · D dv = 6(0.4)3
= 0.38 C
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![CHAPTER 4
4.1. The value of E at P (ρ = 2, φ = 40◦, z = 3) is given as E = 100aρ −200aφ +300az V/m. Determine
the incremental work required to move a 20 µC charge a distance of 6 µm:
a) in the direction of aρ: The incremental work is given by dW = −q E · dL, where in this case,
dL = dρ aρ = 6 × 10−6 aρ. Thus
dW = −(20 × 10−6
C)(100 V/m)(6 × 10−6
m) = −12 × 10−9
J = −12 nJ
b) in the direction of aφ: In this case dL = 2 dφ aφ = 6 × 10−6 aφ, and so
dW = −(20 × 10−6
)(−200)(6 × 10−6
) = 2.4 × 10−8
J = 24 nJ
c) in the direction of az: Here, dL = dz az = 6 × 10−6 az, and so
dW = −(20 × 10−6
)(300)(6 × 10−6
) = −3.6 × 10−8
J = −36 nJ
d) in the direction of E: Here, dL = 6 × 10−6 aE, where
aE =
100aρ − 200aφ + 300az
[1002 + 2002 + 3002]1/2
= 0.267 aρ − 0.535 aφ + 0.802 az
Thus
dW = −(20 × 10−6
)[100aρ − 200aφ + 300az] · [0.267 aρ − 0.535 aφ + 0.802 az](6 × 10−6
)
= −44.9 nJ
e) In the direction of G = 2 ax − 3 ay + 4 az: In this case, dL = 6 × 10−6 aG, where
aG =
2ax − 3ay + 4az
[22 + 32 + 42]1/2
= 0.371 ax − 0.557 ay + 0.743 az
So now
dW = −(20 × 10−6
)[100aρ − 200aφ + 300az] · [0.371 ax − 0.557 ay + 0.743 az](6 × 10−6
)
= −(20 × 10−6
) 37.1(aρ · ax) − 55.7(aρ · ay) − 74.2(aφ · ax) + 111.4(aφ · ay)
+ 222.9] (6 × 10−6
)
where, at P , (aρ · ax) = (aφ · ay) = cos(40◦) = 0.766, (aρ · ay) = sin(40◦) = 0.643, and
(aφ · ax) = − sin(40◦) = −0.643. Substituting these results in
dW = −(20 × 10−6
)[28.4 − 35.8 + 47.7 + 85.3 + 222.9](6 × 10−6
) = −41.8 nJ
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![4.2. Let E = 400ax − 300ay + 500az in the neighborhood of point P (6, 2, −3). Find the incremental work
done in moving a 4-C charge a distance of 1 mm in the direction specified by:
a) ax + ay + az: We write
dW = −qE · dL = −4(400ax − 300ay + 500az) ·
(ax + ay + az)
√
3
(10−3
)
= −
(4 × 10−3)
√
3
(400 − 300 + 500) = −1.39 J
b) −2ax + 3ay − az: The computation is similar to that of part a, but we change the direction:
dW = −qE · dL = −4(400ax − 300ay + 500az) ·
(−2ax + 3ay − az)
√
14
(10−3
)
= −
(4 × 10−3)
√
14
(−800 − 900 − 500) = 2.35 J
4.3. If E = 120 aρ V/m, find the incremental amount of work done in moving a 50 µm charge a distance
of 2 mm from:
a) P (1, 2, 3) toward Q(2, 1, 4): The vector along this direction will be Q − P = (1, −1, 1) from
which aPQ = [ax − ay + az]/
√
3. We now write
dW = −qE · dL = −(50 × 10−6
) 120aρ ·
(ax − ay + az
√
3
(2 × 10−3
)
= −(50 × 10−6
)(120) (aρ · ax) − (aρ · ay)
1
√
3
(2 × 10−3
)
At P, φ = tan−1(2/1) = 63.4◦. Thus (aρ · ax) = cos(63.4) = 0.447 and (aρ · ay) = sin(63.4) =
0.894. Substituting these, we obtain dW = 3.1 µJ.
b) Q(2, 1, 4) toward P (1, 2, 3): A little thought is in order here: Note that the field has only a radial
component and does not depend on φ or z. Note also that P and Q are at the same radius (
√
5)
from the z axis, but have different φ and z coordinates. We could just as well position the two
points at the same z location and the problem would not change. If this were so, then moving
along a straight line between P and Q would thus involve moving along a chord of a circle whose
radius is
√
5. Halfway along this line is a point of symmetry in the field (make a sketch to see
this). This means that when starting from either point, the initial force will be the same. Thus the
answer is dW = 3.1 µJ as in part a. This is also found by going through the same procedure as
in part a, but with the direction (roles of P and Q) reversed.
4.4. Find the amount of energy required to move a 6-C charge from the origin to P (3, 1, −1) in the field
E = 2xax − 3y2ay + 4az V/m along the straight-line path x = −3z, y = x + 2z: We set up the
computation as follows, and find the the result does not depend on the path.
W = −q E · dL = −6 (2xax − 3y2
ay + 4az) · (dxax + dyay + dzaz)
= −6
3
0
2xdx + 6
1
0
3y2
dy − 6
−1
0
4dz = −24 J
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![4.16. Uniform surface charge densities of 6, 4, and 2 nC/m2 are present at r = 2, 4, and 6 cm, respectively,
in free space.
a) Assume V = 0 at infinity, and find V (r). We keep in mind the definition of absolute potential
as the work done in moving a unit positive charge from infinity to location r. At radii outside all
three spheres, the potential will be the same as that of a point charge at the origin, whose charge
is the sum of the three sphere charges:
V (r) (r > 6 cm) =
q1 + q2 + q3
4πǫ0r
=
[4π(.02)2(6) + 4π(.04)2(4) + 4π(.06)2(2)] × 10−9
4πǫ0r
=
(96 + 256 + 288)π × 10−13
4π(8.85 × 10−12)r
=
1.81
r
V where r is in meters
As the unit charge is moved inside the outer sphere to positions 4 < r < 6 cm, the outer sphere
contribution to the energy is fixed at its value at r = 6. Therefore,
V (r) (4 < r < 6 cm) =
q1 + q2
4πǫ0r
+
q3
4πǫ0(.06)
=
0.994
r
+ 13.6 V
In moving inside the sphere at r = 4 cm, the contribution from that sphere becomes fixed at its
potential function at r = 4:
V (r) (2 < r < 4 cm) =
q1
4πǫ0r
+
q2
4πǫ0(.04)
+
q3
4πǫ0(.06)
=
0.271
r
+ 31.7 V
Finally, using the same reasoning, the potential inside the inner sphere becomes
V (r) (r < 2 cm) =
0.271
.02
+ 31.7 = 45.3 V
b) Calculate V at r = 1, 3, 5, and 7 cm: Using the results of part a, we substitute these distances (in
meters) into the appropriate formulas to obtain: V (1) = 45.3 V,
V (3) = 40.7 V, V (5) = 33.5 V, and V (7) = 25.9 V.
c) Sketch V versus r for 0 < r < 10 cm.
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![4.21d. |E|P : taking the magnitude of the part c result, we find |E|P = 75.0 V/m.
e) aN : By definition, this will be
aN
P
= −
E
|E|
= −0.095 ax − 0.304 ay + 0.948 az
f) D: This is D
P
= ǫ0E
P
= 62.8 ax + 202 ay − 629 az pC/m2.
4.22. It is known that the potential is given as V = 80r0.6 V. Assuming free space conditions, find:
a) E: We use
E = −∇V = −
dV
dr
ar = −(0.6)80r−0.4
ar = −48r−0.4
ar V/m
b) the volume charge density at r = 0.5 m: Begin by finding
D = ǫ0E = −48r−0.4
ǫ0 ar C/m2
We next find
ρv = ∇ · D =
1
r2
d
dr
r2
Dr =
1
r2
d
dr
−48ǫ0r1.6
= −
76.8ǫ0
r1.4
C/m3
Then at r = 0.5 m,
ρv(0.5) =
−76.8(8.854 × 10−12)
(0.5)1.4
= −1.79 × 10−9
C/m3
= −1.79 nC/m3
c) the total charge lying within the surface r = 0.6: The easiest way is to use Gauss’law, and integrate
the flux density over the spherical surface r = 0.6. Since the field is constant at constant radius,
we obtain the product:
Q = 4π(0.6)2
(−48ǫ0(0.6)−0.4
) = −2.36 × 10−9
C = −2.36 nC
4.23. It is known that the potential is given as V = 80ρ.6 V. Assuming free space conditions, find:
a) E: We find this through
E = −∇V = −
dV
dρ
aρ = −48ρ−.4
V/m
b) the volume charge density at ρ = .5 m: Using D = ǫ0E, we find the charge density through
ρv
.5
= [∇ · D].5 =
1
ρ
d
dρ
ρDρ
.5
= −28.8ǫ0ρ−1.4
.5
= −673 pC/m3
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![4.23c. the total charge lying within the closed surface ρ = .6, 0 < z < 1: The easiest way to do this calculation
is to evaluate Dρ at ρ = .6 (noting that it is constant), and then multiply by the cylinder area: Using part
a, we have Dρ
.6
= −48ǫ0(.6)−.4 = −521 pC/m2. Thus Q = −2π(.6)(1)521×10−12 C = −1.96 nC.
4.24. Given the potential field V = 80r2 cos θ and a point P (2.5, θ = 30◦, φ = 60◦) in free space, find at P :
a) V : Substitute the coordinates into the function and find VP = 80(2.5)2 cos(30) = 433 V.
b) E:
E = −∇V = −
∂V
∂r
ar −
1
r
∂V
∂θ
aθ = −160r cos θar + 80r sin θaθ V/m
Evaluating this at P yields Ep = −346ar + 100aθ V/m.
c) D: In free space, DP = ǫ0EP = (−346ar + 100aθ )ǫ0 = −3.07 ar + 0.885 aθ nC/m2.
d) ρv:
ρv = ∇ · D = ǫ0∇ · E = ǫ0
1
r2
∂
∂r
r2
Er +
1
r2 sin θ
∂
∂θ
(Eθ sin θ)
Substituting the components of E, we find
ρv = −
160 cos θ
r2
3r2
+
1
r sin θ
80r(2 sin θ cos θ) ǫ0 = −320ǫ0 cos θ = −2.45 nC/m3
with θ = 30◦.
e) dV/dN: This will be just |E| evaluated at P , which is
dV
dN P
= | − 346ar + 100aθ | = (346)2 + (100)2 = 360 V/m
f) aN : This will be
aN = −
EP
|EP |
= −
−346ar + 100aθ
(346)2 + (100)2
= 0.961 ar − 0.278 aθ
4.25. Within the cylinder ρ = 2, 0 < z < 1, the potential is given by V = 100 + 50ρ + 150ρ sin φ V.
a) Find V , E, D, and ρv at P (1, 60◦, 0.5) in free space: First, substituting the given point, we find
VP = 279.9 V. Then,
E = −∇V = −
∂V
∂ρ
aρ −
1
ρ
∂V
∂φ
aφ = − [50 + 150 sin φ] aρ − [150 cos φ] aφ
Evaluate the above at P to find EP = −179.9aρ − 75.0aφ V/m
Now D = ǫ0E, so DP = −1.59aρ − .664aφ nC/m2. Then
ρv = ∇ ·D =
1
ρ
d
dρ
ρDρ +
1
ρ
∂Dφ
∂φ
= −
1
ρ
(50 + 150 sin φ) +
1
ρ
150 sin φ ǫ0 = −
50
ρ
ǫ0 C
At P , this is ρvP = −443 pC/m3.
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![4.29. A dipole having a moment p = 3ax − 5ay + 10az nC · m is located at Q(1, 2, −4) in free space. Find
V at P (2, 3, 4): We use the general expression for the potential in the far field:
V =
p · (r − r′)
4πǫ0|r − r′|3
where r − r′ = P − Q = (1, 1, 8). So
VP =
(3ax − 5ay + 10az) · (ax + ay + 8az) × 10−9
4πǫ0[12 + 12 + 82]1.5
= 1.31 V
4.30. A dipole, having a moment p = 2az nC · m is located at the origin in free space. Give the magnitude
of E and its direction aE in cartesian components at r = 100 m, φ = 90◦, and θ =: a) 0◦; b) 30◦; c)
90◦. Begin with
E =
p
4πǫ0r3
[2 cos θ ar + sin θ aθ ]
from which
|E| =
p
4πǫ0r3
4 cos2
θ + sin2
θ
1/2
=
p
4πǫ0r3
1 + 3 cos2
θ
1/2
Now
Ex = E · ax =
p
4πǫ0r3
[2 cos θ ar · ax + sin θ aθ · ax] =
p
4πǫ0r3
[3 cos θ sin θ cos φ]
then
Ey = E · ay =
p
4πǫ0r3
2 cos θ ar · ay + sin θ aθ · ay =
p
4πǫ0r3
[3 cos θ sin θ sin φ]
and
Ez = E · az =
p
4πǫ0r3
2 cos θ ar · az + sin θ aθ · az =
p
4πǫ0r3
2 cos2
θ − sin2
θ
Since φ is given as 90◦, Ex = 0, and the field magnitude becomes
|E(φ = 90◦
)| = E2
y + E2
z =
p
4πǫ0r3
9 cos2
θ sin2
θ + (2 cos2
θ − sin2
θ)2
1/2
Then the unit vector becomes (again at φ = 90◦):
aE =
3 cos θ sin θ ay + (2 cos2 θ − sin2 θ) az
9 cos2 θ sin2 θ + (2 cos2 θ − sin2 θ)2 1/2
Now with r = 100 m and p = 2 × 10−9,
p
4πǫ0r3
=
2 × 10−9
4π(8.854 × 10−12)106
= 1.80 × 10−5
Using the above formulas, we find at θ = 0◦, |E| = (1.80 × 10−5)(2) = 36.0 µV/m and aE = az.
At θ = 30◦, we find |E| = (1.80 × 10−5)[1.69 + 1.56]1/2 = 32.5 µV/m and aE = (1.30ay +
1.25az)/1.80 = 0.72 ax + 0.69 az. At θ = 90◦, |E| = (1.80×10−5)(1) = 18.0 µV/m and aE = −az.
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![CHAPTER 5
5.1. Given the current density J = −104[sin(2x)e−2yax + cos(2x)e−2yay] kA/m2:
a) Find the total current crossing the plane y = 1 in the ay direction in the region 0 < x < 1,
0 < z < 2: This is found through
I =
S
J · n
S
da =
2
0
1
0
J · ay
y=1
dx dz =
2
0
1
0
−104
cos(2x)e−2
dx dz
= −104
(2)
1
2
sin(2x)
1
0
e−2
= −1.23 MA
b) Find the total current leaving the region 0 < x, x < 1, 2 < z < 3 by integrating J · dS over
the surface of the cube: Note first that current through the top and bottom surfaces will not exist,
since J has no z component. Also note that there will be no current through the x = 0 plane, since
Jx = 0 there. Current will pass through the three remaining surfaces, and will be found through
I =
3
2
1
0
J · (−ay)
y=0
dx dz +
3
2
1
0
J · (ay)
y=1
dx dz +
3
2
1
0
J · (ax)
x=1
dy dz
= 104
3
2
1
0
cos(2x)e−0
− cos(2x)e−2
dx dz − 104
3
2
1
0
sin(2)e−2y
dy dz
= 104 1
2
sin(2x)
1
0
(3 − 2) 1 − e−2
+ 104 1
2
sin(2)e−2y
1
0
(3 − 2) = 0
c) Repeat part b, but use the divergence theorem: We find the net outward current through the surface
of the cube by integrating the divergence of J over the cube volume. We have
∇ · J =
∂Jx
∂x
+
∂Jy
∂y
= −10−4
2 cos(2x)e−2y
− 2 cos(2x)e−2y
= 0 as expected
5.2. Let the current density be J = 2φ cos2 φaρ − ρ sin 2φaφ A/m2 within the region 2.1 < ρ < 2.5,
0 < φ < 0.1 rad, 6 < z < 6.1. Find the total current I crossing the surface:
a) ρ = 2.2, 0 < φ < 0.1, 6 < z < 6.1 in the aρ direction: This is a surface of constant ρ, so only
the radial component of J will contribute: At ρ = 2.2 we write:
I = J · dS =
6.1
6
0.1
0
2(2) cos2
φ aρ · aρ 2dφdz = 2(2.2)2
(0.1)
0.1
0
1
2
(1 + cos 2φ) dφ
= 0.2(2.2)2 1
2
(0.1) +
1
4
sin 2φ
0.1
0
= 97 mA
b) φ = 0.05, 2.2 < ρ < 2.5, 6 < z < 6.1 in the aφ direction: In this case only the φ component of
J will contribute:
I = J · dS =
6.1
6
2.5
2.2
−ρ sin 2φ φ=0.05
aφ · aφ dρ dz = −(0.1)2 ρ2
2
2.5
2.2
= −7 mA
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![5.2c. Evaluate ∇ · J at P (ρ = 2.4, φ = 0.08, z = 6.05):
∇ · J =
1
ρ
∂
∂ρ
(ρJρ) +
1
ρ
∂Jφ
∂φ
=
1
ρ
∂
∂ρ
(2ρ2
cos2
φ) −
1
ρ
∂
∂φ
(ρ sin 2φ) = 4 cos2
φ − 2 cos 2φ
0.08
= 2.0 A/m3
5.3. Let
J =
400 sin θ
r2 + 4
ar A/m2
a) Find the total current flowing through that portion of the spherical surface r = 0.8, bounded by
0.1π < θ < 0.3π, 0 < φ < 2π: This will be
I = J · n
S
da =
2π
0
.3π
.1π
400 sin θ
(.8)2 + 4
(.8)2
sin θ dθ dφ =
400(.8)22π
4.64
.3π
.1π
sin2
dθ
= 346.5
.3π
.1π
1
2
[1 − cos(2θ)] dθ = 77.4 A
b) Find the average value of J over the defined area. The area is
Area =
2π
0
.3π
.1π
(.8)2
sin θ dθ dφ = 1.46 m2
The average current density is thus Javg = (77.4/1.46) ar = 53.0 ar A/m2.
5.4. The cathode of a planar vacuum tube is at z = 0. Let E = −4 × 106 az V/m for z > 0. An electron
(e = 1.602 × 10−19 C, m = 9.11 × 10−31 kg) is emitted from the cathode with zero initial velocity at
t = 0.
a) Find v(t): Using Newton’s second law, we write:
F = ma = qE ⇒ a =
(−1.602 × 10−19)(−4 × 106)az
(9.11 × 10−31)
= 7.0 × 1017
az m/s2
Then v(t) = at = 7.0 × 1017t m/s.
b) Find z(t), the electron location as a function of time: Use
z(t) =
t
0
v(t′
)dt′
=
1
2
(7.0 × 1017
)t2
= 3.5 × 1017
t2
m
c) Determine v(z): Solve the result of part b for t, obtaining
t =
√
z
√
3.5 × 1017
= 1.7 × 109√
z
Substitute into the result of part a to find v(z) = 7.0 × 1017(1.7 × 10−9)
√
z = 1.2 × 109√
z m/s.
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![5.9a. Using data tabulated in Appendix C, calculate the required diameter for a 2-m long nichrome wire that
will dissipate an average power of 450 W when 120 V rms at 60 Hz is applied to it:
The required resistance will be
R =
V 2
P
=
l
σ(πa2)
Thus the diameter will be
d = 2a = 2
lP
σπV 2
= 2
2(450)
(106)π(120)2
= 2.8 × 10−4
m = 0.28 mm
b) Calculate the rms current density in the wire: The rms current will be I = 450/120 = 3.75 A.
Thus
J =
3.75
π 2.8 × 10−4/2
2
= 6.0 × 107
A/m2
5.10. A steel wire has a radius of 2 mm and a conductivity of 2 × 106 S/m. The steel wire has an aluminum
(σ = 3.8 × 107 S/m) coating of 2 mm thickness. Let the total current carried by this hybrid conductor
be 80 A dc. Find:
a) Jst . We begin with the fact that electric field must be the same in the aluminum and steel regions.
This comes from the requirement that E tangent to the boundary between two media must be
continuous, and from the fact that when integrating E over the wire length, the applied voltage
value must be obtained, regardless of the medium within which this integral is evaluated. We can
therefore write
EAl = Est =
JAl
σAl
=
Jst
σst
⇒ JAl =
σAl
σst
Jst
The net current is now expressed as the sum of the currents in each region, written as the sum of
the products of the current densities in each region times the appropriate cross-sectional area:
I = π(2 × 10−3
)2
Jst + π[(4 × 10−3
)2
− (2 × 10−3
)2
]JAl = 80 A
Using the above relation between Jst and JAl, we find
80 = π (2 × 10−3
)2
1 −
3.8 × 107
6 × 106
+ (4 × 10−3
)2 3.8 × 107
6 × 106
Jst
Solve for Jst to find Jst = 3.2 × 105 A/m2.
b)
JAl =
3.8 × 107
6 × 106
(3.2 × 105
) = 2.0 × 106
A/m2
c,d) Est = EAl = Jst /σst = JAl/σAl = 5.3 × 10−2 V/m.
e) the voltage between the ends of the conductor if it is 1 mi long: Using the fact that 1 mi = 1.61×103
m, we have V = El = (5.3 × 10−2)(1.61 × 103) = 85.4 V.
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![5.19b. (continued) Now
E = −∇V = −40xyz ax − 20x2
z ay − [20xy − 20z] az
Then, at the given point, we have
D(2, 7/8, 1) = ǫ0E(2, 7/8, 1) = −ǫ0[70 ax + 80 ay + 50 az] C/m2
We know that since this is the higher potential surface, D must be directed away from it, and so
the charge density would be positive. Thus
ρs =
√
D · D = 10ǫ0 72 + 82 + 52 = 1.04 nC/m2
c) Give the unit vector at this point that is normal to the conducting surface and directed toward the
V = 0 surface: This will be in the direction of E and D as found in part b, or
an = −
7ax + 8ay + 5az
√
72 + 82 + 52
= −[0.60ax + 0.68ay + 0.43az]
5.20. A conducting plane is located at z = 0 in free space, and a 20 nC point charge is present at Q(2, 4, 6).
a) If V = 0 at z = 0, find V at P (5, 3, 1): The plane can be replaced by an image charge of -20 nC
at Q′(2, 4, −6). Vectors R and R′ directed from Q and Q′ to P are R = (5, 3, 1) − (2, 4, 6) =
(3, −1, −5) and R′ = (5, 3, 1) − (2, 4, −6) = (3, −1, 7). Their magnitudes are R =
√
35 and
R′ =
√
59. The potential at P is given by
VP =
q
4πǫ0R
−
q
4πǫ0R′
=
20 × 10−9
4πǫ0
√
35
−
20 × 10−9
4πǫ0
√
59
= 7.0 V
b) Find E at P :
EP =
qR
4πǫ0R3
−
qR′
4πǫ0(R′)3
=
(20 × 10−9)(3, −1, −5)
4πǫ0(35)3/2
−
(20 × 10−9)(3, −1, 7)
4πǫ0(59)3/2
=
20 × 10−9
4πǫ0
(3ax − ay)
1
(35)3/2
−
1
(59)3/2
−
7
(59)3/2
+
5
(35)3/2
az
= 1.4ax − 0.47ay − 7.1az V/m
c) Find ρs at A(5, 3, 0): First, find the electric field there:
EA =
20 × 10−9
4πǫ0
(5, 3, 0) − (2, 4, 6)
(46)3/2
−
(5, 3, 0) − (2, 4, −6)
(46)3/2
= −6.9az V/m
Then ρs = D · n
surf ace
= −6.9ǫ0az · az = −61 pC/m2.
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![5.22b. Find |ρs| at B(0, 0, 0) (note error in problem statement): First, E at the origin is done as per the setup
in part a, except the vectors are directed from the charges to the origin:
EB =
10−9
4πǫ0
(4)(−7, −1, 2)
(54)3/2
−
(3)(−4, −2, −1)
(21)3/2
−
(4)(7, −1, 2)
(54)3/2
+
(3)(4, −2, −1)
(21)3/2
Now ρs = D · n|surf ace = D · ax in our case (note the other components cancel anyway as they must,
but we still need to express ρs as a scalar):
ρsB = ǫ0EB · ax =
10−9
4π
(4)(−7)
(54)3/2
−
(3)(−4)
(21)3/2
−
(4)(7)
(54)3/2
+
(3)(4)
(21)3/2
= 8.62 pC/m2
5.23. A dipole with p = 0.1az µC · m is located at A(1, 0, 0) in free space, and the x = 0 plane is perfectly-
conducting.
a) Find V at P (2, 0, 1). We use the far-field potential for a z-directed dipole:
V =
p cos θ
4πǫ0r2
=
p
4πǫ0
z
[x2 + y2 + z2]1.5
The dipole at x = 1 will image in the plane to produce a second dipole of the opposite orientation
at x = −1. The potential at any point is now:
V =
p
4πǫ0
z
[(x − 1)2 + y2 + z2]1.5
−
z
[(x + 1)2 + y2 + z2]1.5
Substituting P (2, 0, 1), we find
V =
.1 × 106
4πǫ0
1
2
√
2
−
1
10
√
10
= 289.5 V
b) Find the equation of the 200-V equipotential surface in cartesian coordinates: We just set the
potential exression of part a equal to 200 V to obtain:
z
[(x − 1)2 + y2 + z2]1.5
−
z
[(x + 1)2 + y2 + z2]1.5
= 0.222
5.24. The mobilities for intrinsic silicon at a certain temperature are µe = 0.14 m2/V · s and µh =
0.035 m2/V · s. The concentration of both holes and electrons is 2.2 × 1016 m−3. Determine both
the conductivity and the resistivity of this silicon sample: Use
σ = −ρeµe + ρhµh = (1.6 × 10−19
C)(2.2 × 1016
m−3
)(0.14 m2
/V · s + 0.035 m2
/V · s)
= 6.2 × 10−4
S/m
Conductivity is ρ = 1/σ = 1.6 × 103 · m.
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![5.25. Electron and hole concentrations increase with temperature. For pure silicon, suitable expressions are
ρh = −ρe = 6200T 1.5e−7000/T C/m3. The functional dependence of the mobilities on temperature is
given by µh = 2.3 × 105T −2.7 m2/V · s and µe = 2.1 × 105T −2.5 m2/V · s, where the temperature,
T , is in degrees Kelvin. The conductivity will thus be
σ = −ρeµe + ρhµh = 6200T 1.5
e−7000/T
2.1 × 105
T −2.5
+ 2.3 × 105
T −2.7
=
1.30 × 109
T
e−7000/T
1 + 1.095T −.2
S/m
Find σ at:
a) 0◦ C: With T = 273◦K, the expression evaluates as σ(0) = 4.7 × 10−5 S/m.
b) 40◦ C: With T = 273 + 40 = 313, we obtain σ(40) = 1.1 × 10−3 S/m.
c) 80◦ C: With T = 273 + 80 = 353, we obtain σ(80) = 1.2 × 10−2 S/m.
5.26. A little donor impurity, such as arsenic, is added to pure silicon so that the electron concentration
is 2 × 1017 conduction electrons per cubic meter while the number of holes per cubic meter is only
1.1×1015. If µe = 0.15 m2/V · s for this sample, and µh = 0.045 m2/V · s, determine the conductivity
and resistivity:
σ = −ρeµe + ρhµh = (1.6 × 10−19
) (2 × 1017
)(0.15) + (1.1 × 1015
)(0.045) = 4.8 × 10−3
S/m
Then ρ = 1/σ = 2.1 × 102 · m.
5.27. Atomic hydrogen contains 5.5×1025 atoms/m3 at a certain temperature and pressure. When an electric
field of 4 kV/m is applied, each dipole formed by the electron and positive nucleus has an effective
length of 7.1 × 10−19 m.
a) Find P: With all identical dipoles, we have
P = Nqd = (5.5 × 1025
)(1.602 × 10−19
)(7.1 × 10−19
) = 6.26 × 10−12
C/m2
= 6.26 pC/m2
b) Find ǫR: We use P = ǫ0χeE, and so
χe =
P
ǫ0E
=
6.26 × 10−12
(8.85 × 10−12)(4 × 103)
= 1.76 × 10−4
Then ǫR = 1 + χe = 1.000176.
5.28. In a certain region where the relative permittivity is 2.4, D = 2ax − 4ay + 5az nC/m2. Find:
a) E =
D
ǫ
=
(2ax − 4ay + 5az) × 10−9
(2.4)(8.85 × 10−12)
= 94ax − 188ay + 235az V/m
b) P = D − ǫ0E = ǫ0E(ǫR − 1) =
(2ax − 4ay + 5az) × 10−9
2.4
(2.4 − 1)
= 1.2ax − 2.3ay + 2.9az nC/m2
c) |∇V | = |E| = [(94.1)2
+ (188)2
+ (235)2
]1/2
= 315 V/m
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![5.31 (continued)
f) DN2 = DN1 = ǫR1ǫ0EN1 = 3(8.85 × 10−12)(80) = 2.12 nC/m2.
g) DT 2 = ǫR2ǫ0ET 1 = 5(8.85 × 10−12)(67.1) = 2.97 nC/m2.
h) D2 = ǫR1ǫ0EN1ax + ǫR2ǫ0ET 1 = 2.12ax − 2.66ay − 1.33az nC/m2.
i) P2 = D2 − ǫ0E2 = D2 [1 − (1/ǫR2)] = (4/5)D2 = 1.70ax − 2.13ay − 1.06az nC/m2.
j) the angle θ2 between E2 and a normal to the surface: Use
cos θ2 =
E2 · ax
E2
=
D2 · ax
D2
=
2.12
(2.12)2 = (2.66)2 + (1.33)2
= .581
Thus θ2 = cos−1(.581) = 54.5◦.
5.32. In Fig. 5.18, let D = 3ax − 4ay + 5az nC/m2 and find:
a) D2: First, the electric field in region 1 is
E1 =
3
2ǫ0
ax −
4
2ǫ0
ay +
5
2ǫ0
az × 10−9
V/m
Since, at the dielectric interface, tangential electric field and normal electric flux density are
continuous, we may write
D2 = ǫR2ǫ0ET 1 + DN1 =
5
2
3ax −
5
2
4ay + 5az = 7.5ax − 10ay + 5az nC/m2
b) DN2 = 5az, as explained above.
c) DT 2 = ǫR2ǫ0ET 2 = ǫR2ǫ0ET 1 = 7.5ax − 10ay nC/m2.
d) the energy density in each region:
we1 =
1
2
ǫR1ǫ0E1 · E1 =
1
2
(2)ǫ0
3
2ǫ0
2
+
4
2ǫ0
2
+
5
2ǫ0
2
× 10−18
= 1.41 µJ/m3
we2 =
1
2
ǫR2ǫ0E2 · E2 =
1
2
(5)ǫ0
3
2ǫ0
2
+
4
2ǫ0
2
+
5
5ǫ0
2
× 10−18
= 2.04 µJ/m3
e) the angle that D2 makes with az: Use D2 · az = |D2| cos θ = Dz = 5. where |D2| =
(7.5)2 + (10)2 + (5)2 1/2
= 13.5. So θ = cos−1(5/13.5) = 68◦.
f) D2/D1 = (7.5)2 + (10)2 + (5)2 1/2
/ (3)2 + (4)2 + (5)2 1/2
= 1.91.
g) P2/P1: First P1 = ǫ0E1(ǫR1 − 1) = 1.5ax − 2ay + 2.5az nC/m2.
Then P2 = ǫ0E2(ǫR2 − 1) = 6ax − 8ay + 4az nC/m2. So
P2
P1
=
[(6)2 + (8)2 + (4)2]1/2
[(1.5)2 + (2)2 + (2.5)2]1/2
= 3.04
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![5.33. Two perfect dielectrics have relative permittivities ǫR1 = 2 and ǫR2 = 8. The planar interface between
them is the surface x − y + 2z = 5. The origin lies in region 1. If E1 = 100ax + 200ay − 50az
V/m, find E2: We need to find the components of E1 that are normal and tangent to the boundary, and
then apply the appropriate boundary conditions. The normal component will be EN1 = E1 · n. Taking
f = x − y + 2z, the unit vector that is normal to the surface is
n =
∇f
|∇f |
=
1
√
6
ax − ay + 2az
This normal will point in the direction of increasing f , which will be away from the origin, or into region
2 (you can visualize a portion of the surface as a triangle whose vertices are on the three coordinate
axes at x = 5, y = −5, and z = 2.5). So EN1 = (1/
√
6)[100 − 200 − 100] = −81.7 V/m. Since the
magnitude is negative, the normal component points into region 1 from the surface. Then
EN1 = −81.65
1
√
6
[ax − ay + 2az] = −33.33ax + 33.33ay − 66.67az V/m
Now, the tangential component will be
ET 1 = E1 − EN1 = 133.3ax + 166.7ay + 16.67az
Our boundary conditions state that ET 2 = ET 1 and EN2 = (ǫR1/ǫR2)EN1 = (1/4)EN1. Thus
E2 = ET 2 + EN2 = ET 1 +
1
4
EN1 = 133.3ax + 166.7ay + 16.67az − 8.3ax + 8.3ay − 16.67az
= 125ax + 175ay V/m
5.34. Let the spherical surfaces r = 4 cm and r = 9 cm be separated by two perfect dielectric shells, ǫR1 = 2
for 4 < r < 6 cm and ǫR2 = 5 for 6 < r < 9 cm. If E1 = (2000/r2)ar V/m, find:
a) E2: Since E is normal to the interface between ǫR1 and ǫR2, D will be continuous across the
boundary, and so
D1 =
2ǫ0(2000)
r2
ar = D2
Then
E2 =
D2
5ǫ0
=
2
5
2000
r2
ar =
800
r2
ar V/m
b) the total electrostatic energy stored in each region: In region 1, the energy density is
we1 =
1
2
ǫR1ǫ0|E1|2
=
1
2
(2)ǫ0
(2000)2
r4
J/m3
In region 2:
we2 =
1
2
ǫR2ǫ0|E2|2
=
1
2
(5)ǫ0
(800)2
r4
J/m3
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![5.34. (continued)
The energies in each region are then
Region 1 : We1 = (2000)2
ǫ0
2π
0
π
0
.06
.04
1
r2
r2
sin θ dr dθ dφ
= 4πǫ0(2000)2 1
.04
−
1
.06
= 3.7 mJ
Region 2 : We2 = (800)2 5
2
ǫ0
2π
0
π
0
.09
.06
1
r2
r2
sin θ dr dθ dφ
= 4πǫ0(800)2 5
2
1
.06
−
1
.09
= 0.99 mJ
5.35. Let the cylindrical surfaces ρ = 4 cm and ρ = 9 cm enclose two wedges of perfect dielectrics, ǫR1 = 2
for 0 < φ < π/2, and ǫR2 = 5 for π/2 < φ < 2π. If E1 = (2000/ρ)aρ V/m, find:
a) E2: The interfaces between the two media will lie on planes of constant φ, to which E1 is parallel.
Thus the field is the same on either side of the boundaries, and so E2 = E1.
b) the total electrostatic energy stored in a 1m length of each region: In general we have wE =
(1/2)ǫRǫ0E2. So in region 1:
WE1 =
1
0
π/2
0
9
4
1
2
(2)ǫ0
(2000)2
ρ2
ρ dρ dφ dz =
π
2
ǫ0(2000)2
ln
9
4
= 45.1 µJ
In region 2, we have
WE2 =
1
0
2π
π/2
9
4
1
2
(5)ǫ0
(2000)2
ρ2
ρ dρ dφ dz =
15π
4
ǫ0(2000)2
ln
9
4
= 338 µJ
5.36. Let S = 120 cm2, d = 4 mm, and ǫR = 12 for a parallel-plate capacitor.
a) Calculate the capacitance:
C = ǫRǫ0S/d = [12ǫ0(120 × 10−4)]/[4 × 10−3] = 3.19 × 10−10 = 319 pF.
b) After connecting a 40 V battery across the capacitor, calculate E, D, Q, and the total stored
electrostatic energy: E = V/d = 40/(4 × 10−3) = 104 V/m. D = ǫRǫ0E = 12ǫ0 × 104 =
1.06 µC/m2. Then Q = D · n|surf ace × S = 1.06 × 10−6 × (120 × 10−4) = 1.27 × 10−8C =
12.7 nC. Finally We = (1/2)CV 2
0 = (1/2)(319 × 10−12)(40)2 = 255 nJ.
c) Thesourceisnowremovedandthedielectriciscarefullywithdrawnfrombetweentheplates. Again
calculate E, D, Q, and the energy: With the source disconnected, the charge is constant, and thus
so is D: Therefore, Q = 12.7 nC, D = 1.06 µC/m2, and E = D/ǫ0 = 104/8.85 × 10−12 =
1.2 × 105 V/m. The energy is then
We =
1
2
D · E × S =
1
2
(1.06 × 10−6
)(1.2 × 105
)(120 × 10−4
)(4 × 10−3
) = 3.05 µJ
d) What is the voltage between the plates? V = E × d = (1.2 × 105)(4 × 10−3) = 480 V.
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![5.48. A potential function in free space is given by
V = −20 + 10 ln
(5 + y)2 + x2
(5 − y)2 + x2
a) Describe the 0-V equipotential surface: Setting the given expression equal to zero, we find
(5 + y)2 + x2
(5 − y)2 + x2
= e2
= 7.39
So 6.39x2 + 6.39y2 − 83.9y + 160 = 0. Completing the square in the y trinomial leads to
x2 + (y − 6.56)2 = 18.1 = (4.25)2, which we recognize as a right circular cylinder whose axis
is located at x = 0, y = 6.56, and whose radius is 4.25.
b) Describe the 10-V equipotential surface: In this case, the given expression is set equal to ten,
leading to
(5 + y)2 + x2
(5 − y)2 + x2
= e3
= 20.1
So 19.1x2 + 19.1y2 − 211y + 477 = 0. Following the same procedure as in part a, this becomes
x2 + (y − 5.52)2 = 5.51 = (2.35)2, which we recognize again as a right circular cylinder with
axis at x = 0, y = 5.52, and of radius 2.35.
5.49. A 2 cm diameter conductor is suspended in air with its axis 5 cm from a conducting plane. Let the
potential of the cylinder be 100 V and that of the plane be 0 V. Find the surface charge density on the:
a) cylinder at a point nearest the plane: The cylinder will image across the plane, producing an
equivalent two-cylinder problem, with the second one at location 5 cm below the plane. We will
take the plane as the zy plane, with the cylinder positions at x = ±5. Now b = 1 cm, h = 5
cm, and V0 = 100 V. Thus a =
√
h2 − b2 = 4.90 cm. Then K1 = [(h + a)/b]2 = 98.0, and
ρL = (4πǫ0V0)/ ln K1 = 2.43 nC/m. Now
D = ǫ0E = −
ρL
2π
(x + a)ax + yay
(x + a)2 + y2
−
(x − a)ax + yay
(x − a)2 + y2
and
ρs, max = D · (−ax)
x=h−b,y=0
=
ρL
2π
h − b + a
(h − b + a)2
−
h − b − a
(h − b − a)2
= 473 nC/m2
b) plane at a point nearest the cylinder: At x = y = 0,
D(0, 0) = −
ρL
2π
aax
a2
−
−aax
a2
= −
ρL
2π
2
a
ax
from which
ρs = D(0, 0) · ax = −
ρL
πa
= −15.8 nC/m2
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![6.16. The square washer shown in Fig. 6.19 is 2.4 mm thick and has outer dimensions of 2.5 × 2.5 cm
and inner dimensions of 1.25 × 1.25 cm. The inside and outside surfaces are perfectly-conducting. If
the material has a conductivity of 6 S/m, estimate the resistance offered between the inner and outer
surfaces (shown shaded in Fig. 6.19). A few curvilinear squares are suggested: First we find the surface
resistance, Rs = 1/(σt) = 1/(6 × 2.4 × 10−3) = 69.4 /sq. Having found this, we can construct
the total resistance by using the fundamental square as a building block. Specifically, R = Rs(Nl/Nw)
where Nl is the number of squares between the inner and outer surfaces and Nw is the number of squares
around the perimeter of the washer. These numbers are found from the curvilinear square plot shown
below, which covers one-eighth the washer. The resistance is thus R
.
= 69.4[4/(8 × 5)]
.
= 6.9 .
6.17. A two-wire transmission line consists of two parallel perfectly-conducting cylinders, each having a
radius of 0.2 mm, separated by center-to-center distance of 2 mm. The medium surrounding the wires
has ǫR = 3 and σ = 1.5 mS/m. A 100-V battery is connected between the wires. Calculate:
a) the magnitude of the charge per meter length on each wire: Use
C =
πǫ
cosh−1(h/b)
=
π × 3 × 8.85 × 10−12
cosh−1 (1/0.2)
= 3.64 × 10−9
C/m
Then the charge per unit length will be
Q = CV0 = (3.64 × 10−11
)(100) = 3.64 × 10−9
C/m = 3.64 nC/m
b) the battery current: Use
RC =
ǫ
σ
⇒ R =
3 × 8.85 × 10−12
(1.5 × 10−3)(3.64 × 10−11)
= 486
Then
I =
V0
R
=
100
486
= 0.206 A = 206 mA
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![7.22c. Use a development similar to that of Sec. 7.4 to show that C = dQ/dV0 = ǫS/8a ( note error in
problem statement): First, the overall potential difference is
V0 = Vx→∞ − Vx→−∞ = 2 ×
2a2ρv0
ǫ
=
4a2ρv0
ǫ
From this we find a =
√
(ǫV0)/(4ρv0). Then the total charge on one side will be
Q = S
∞
0
ρv0
x
a
e−x/a
dx = Sρv0 ae−x/a −x
a
− 1
∞
0
= Sρv0 a =
1
2
S ǫV0ρv0
Now
C =
dQ
dV0
=
d
dV0
1
2
S ǫV0ρv0 =
S
4
ρv0 ǫ
V0
But a =
√
(ǫV0)/(4ρv0), from which (ρv0/V0) = ǫ/(4a2). Substituting this into the capacitance
expression gives
C =
S
4
ǫ2
4a2
=
ǫS
8a
7.23. A rectangular trough is formed by four conducting planes located at x = 0 and 8 cm and y = 0 and 5
cm in air. The surface at y = 5 cm is at a potential of 100 V, the other three are at zero potential, and the
necessary gaps are placed at two corners. Find the potential at x = 3 cm, y = 4 cm: This situation is
the same as that of Fig. 7.6, except the non-zero boundary potential appears on the top surface, rather
than the right side. The solution is found from Eq. (39) by simply interchanging x and y, and b and d,
obtaining:
V (x, y) =
4V0
π
∞
1,odd
1
m
sinh(mπy/d)
sinh(mπb/d)
sin
mπx
d
where V0 = 100 V, d = 8 cm, and b = 5 cm. We will use the first three terms to evaluate the potential
at (3,4):
V (3, 4)
.
=
400
π
sinh(π/2)
sinh(5π/8)
sin(3π/8) +
1
3
sinh(3π/2)
sinh(15π/8)
sin(9π/8) +
1
5
sinh(5π/2)
sinh(25π/8)
sin(15π/8)
=
400
π
[.609 − .040 − .011] = 71.1 V
Additional accuracy is found by including more terms in the expansion. Using thirteen terms, and
using six significant figure accuracy, the result becomes V (3, 4)
.
= 71.9173 V. The series converges
rapidly enough so that terms after the sixth one produce no change in the third digit. Thus, quoting
three significant figures, 71.9 V requires six terms, with subsequent terms having no effect.
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![7.28b. Show that P = Aρn + Bρ−n satisfies the ρ equation: From part a, the radial equation is:
ρ2 d2P
dρ2
+ ρ
dP
dρ
− n2
P = 0
Substituting Aρn, we find
ρ2
n(n − 1)ρn−2
+ ρnρn−1
− n2
ρn
= n2
ρn
− nρn
+ nρn
− n2
ρn
= 0
Substituting Bρ−n:
ρ2
n(n + 1)ρ−(n+2)
− ρnρ−(n+1)
− n2
ρ−n
= n2
ρ−n
+ nρ−n
− nρ−n
− n2
ρ−n
= 0
So it works.
c) Construct the solution V (ρ, φ). Functions of this form are called circular harmonics. To assemble
the complete solution, we need the radial solution for the case in which n = 0. The equation to
solve is
ρ
d2P
dρ2
+
dP
dρ
= 0
Let S = dP/dρ, and so dS/dρ = d2P/dρ2. The equation becomes
ρ
dS
dρ
+ S = 0 ⇒ −
dρ
ρ
=
dS
S
Integrating, find
− ln ρ + ln A0 = ln S ⇒ ln S = ln
A0
ρ
⇒ S =
A0
ρ
=
dP
dρ
where A0 is a constant. So now
dρ
ρ
=
dP
A0
⇒ Pn=0 = A0 ln ρ + B0
We may now construct the solution in its complete form, encompassing n ≥ 0:
V (ρ, φ) = (A0 ln ρ + B0)(C0φ + D0)
n=0 solution
+
∞
n=1
[Anρn
+ Bnρ−n
][Cn cos(nφ) + Dn sin(nφ)]
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![CHAPTER 8
8.1a. Find H in cartesian components at P (2, 3, 4) if there is a current filament on the z axis carrying 8 mA
in the az direction:
Applying the Biot-Savart Law, we obtain
Ha =
∞
−∞
IdL × aR
4πR2
=
∞
−∞
Idz az × [2ax + 3ay + (4 − z)az]
4π(z2 − 8z + 29)3/2
=
∞
−∞
Idz[2ay − 3ax]
4π(z2 − 8z + 29)3/2
Using integral tables, this evaluates as
Ha =
I
4π
2(2z − 8)(2ay − 3ax)
52(z2 − 8z + 29)1/2
∞
−∞
=
I
26π
(2ay − 3ax)
Then with I = 8 mA, we finally obtain Ha = −294ax + 196ay µA/m
b. Repeat if the filament is located at x = −1, y = 2: In this case the Biot-Savart integral becomes
Hb =
∞
−∞
Idz az × [(2 + 1)ax + (3 − 2)ay + (4 − z)az]
4π(z2 − 8z + 26)3/2
=
∞
−∞
Idz[3ay − ax]
4π(z2 − 8z + 26)3/2
Evaluating as before, we obtain with I = 8 mA:
Hb =
I
4π
2(2z − 8)(3ay − ax)
40(z2 − 8z + 26)1/2
∞
−∞
=
I
20π
(3ay − ax) = −127ax + 382ay µA/m
c. Find H if both filaments are present: This will be just the sum of the results of parts a and b, or
HT = Ha + Hb = −421ax + 578ay µA/m
This problem can also be done (somewhat more simply) by using the known result for H from an
infinitely-long wire in cylindrical components, and transforming to cartesian components. The Biot-
Savart method was used here for the sake of illustration.
8.2. A current filament of 3ax A lies along the x axis. Find H in cartesian components at P (−1, 3, 2): We
use the Biot-Savart law,
H =
IdL × aR
4πR2
where IdL = 3dxax, aR = [−(1 + x)ax + 3ay + 2az]/R, and R =
√
x2 + 2x + 14. Thus
HP =
∞
−∞
3dxax × [−(1 + x)ax + 3ay + 2az]
4π(x2 + 2x + 14)3/2
=
∞
−∞
(9az − 6ay) dx
4π(x2 + 2x + 14)3/2
=
(9az − 6ay)(x + 1)
4π(13)
√
x2 + 2x + 14
∞
−∞
=
2(9az − 6ay)
4π(13)
= 0.110az − 0.073ay A/m
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![8.3. Two semi-infinite filaments on the z axis lie in the regions −∞ < z < −a (note typographical error in
problem statement) and a < z < ∞. Each carries a current I in the az direction.
a) Calculate H as a function of ρ and φ at z = 0: One way to do this is to use the field from an
infinite line and subtract from it that portion of the field that would arise from the current segment
at −a < z < a, found from the Biot-Savart law. Thus,
H =
I
2πρ
aφ −
a
−a
I dz az × [ρ aρ − z az]
4π[ρ2 + z2]3/2
The integral part simplifies and is evaluated:
a
−a
I dz ρ aφ
4π[ρ2 + z2]3/2
=
Iρ
4π
aφ
z
ρ2 ρ2 + z2
a
−a
=
Ia
2πρ ρ2 + a2
aφ
Finally,
H =
I
2πρ
1 −
a
ρ2 + a2
aφ A/m
b) What value of a will cause the magnitude of H at ρ = 1, z = 0, to be one-half the value obtained
for an infinite filament? We require
1 −
a
ρ2 + a2
ρ=1
=
1
2
⇒
a
√
1 + a2
=
1
2
⇒ a = 1/
√
3
8.4a.) A filament is formed into a circle of radius a, centered at the origin in the plane z = 0. It carries a
current I in the aφ direction. Find H at the origin: We use the Biot-Savart law, which in this case
becomes:
H =
loop
IdL × aR
4πR2
=
2π
0
Ia dφ aφ × (−aρ)
4πa2
= 0.50
I
a
az A/m
b.) A filament of the same length is shaped into a square in the z = 0 plane. The sides are parallel to the
coordinate axes and a current I flows in the general aφ direction. Again, find H at the origin: Since
the loop is the same length, its perimeter is 2πa, and so each of the four sides is of length πa/2.
Using symmetry, we can find the magnetic field at the origin associated with each of the 8 half-sides
(extending from 0 to ±πa/4 along each coordinate direction) and multiply the result by 8: Taking one
of the segments in the y direction, the Biot-Savart law becomes
H =
loop
IdL × aR
4πR2
= 8
πa/4
0
Idy ay × −(πa/4) ax − y ay
4π y2 + (πa/4)2 3/2
=
aI
2
πa/4
0
dy az
y2 + (πa/4)2 3/2
=
aI
2
y az
(πa/4)2 y2 + (πa/4)2
πa/4
0
= 0.57
I
a
az A/m
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![8.5. The parallel filamentary conductors shown in Fig. 8.21 lie in free space. Plot |H| versus y, −4 < y < 4,
along the line x = 0, z = 2: We need an expression for H in cartesian coordinates. We can start with the
known H in cylindrical for an infinite filament along the z axis: H = I/(2πρ) aφ, which we transform
to cartesian to obtain:
H =
−Iy
2π(x2 + y2)
ax +
Ix
2π(x2 + y2)
ay
If we now rotate the filament so that it lies along the x axis, with current flowing in positive x, we obtain
the field from the above expression by replacing x with y and y with z:
H =
−Iz
2π(y2 + z2)
ay +
Iy
2π(y2 + z2)
az
Now, with two filaments, displaced from the x axis to lie at y = ±1, and with the current directions as
shown in the figure, we use the previous expression to write
H =
Iz
2π[(y + 1)2 + z2]
−
Iz
2π[(y − 1)2 + z2]
ay +
I(y − 1)
2π[(y − 1)2 + z2]
−
I(y + 1)
2π[(y + 1)2 + z2]
az
We now evaluate this at z = 2, and find the magnitude (
√
H · H), resulting in
|H| =
I
2π
2
y2 + 2y + 5
−
2
y2 − 2y + 5
2
+
(y − 1)
y2 − 2y + 5
−
(y + 1)
y2 + 2y + 5
2 1/2
This function is plotted below
8.6a. A current filament I is formed into circle, ρ = a, in the z = z′ plane. Find Hz at P (0, 0, z) if I flows
in the aφ direction: Use the Biot-Savart law,
H =
IdL × aR
4πR2
where in this case IdL = Idφaφ, aR = [−aaρ + (z − z′)az]/R, and R = a2 + (z − z′)2. The
setup becomes
H =
2π
0
Iadφ aφ × [−aaρ + (z − z′)az]
4π[a2 + (z − z′)2]3/2
=
2π
0
Ia[aaz + (z − z′)aρ] dφ
4π[a2 + (z − z′)2]3/2
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![At this point we need to be especially careful. Note that we are integrating a vector with an aρ component
around a complete circle, where the vector has no φ dependence. This sum of all aρ components will be
zero – even though this doesn’t happen when we go ahead with the integration without this knowledge.
The problem is that the integral “interprets” aρ as a constant direction, when in fact – as we know – aρ
continually changes direction as φ varies. We drop the aρ component in the integral to give
H =
2π
0
Ia2az dφ
4π[a2 + (z − z′)2]3/2
=
πa2Iaz
2π[a2 + (z − z′)2]3/2
=
m
2π[a2 + (z − z′)2]3/2
A/m
where m = πa2Iaz is the magnetic moment of the loop.
b) Find Hz at P caused by a uniform surface current density K = K0aφ, flowing on the cylindrical
surface, ρ = a, 0 < z < h. The results of part a should help: Using part a, we can write down the
differential field at P arising from a circular current ribbon of differential height, dz′, at location
z′. The ribbon is of radius a and carries current K0dz′aφ A:
dH =
πa2K0dz′az
2π[a2 + (z − z′)2]3/2
A/m
The total magnetic field at P is now the sum of the contributions of all differential rings that
comprise the cylinder:
Hz =
h
0
πa2K0dz′
2π[a2 + (z − z′)2]3/2
=
a2K0
2
h
0
dz′
[a2 + z2 − 2zz′ + (z′)2]3/2
=
a2K0
2
2(2z′ − 2z)
4a2 a2 + z2 − 2zz′ + (z′)2
h
0
=
K0(z′ − z)
2 a2 + (z′ − z)2
h
0
=
K0
2
(h − z)
a2 + (h − z)2
+
z
√
a2 + z2
A/m
8.7. Given points C(5, −2, 3) and P (4, −1, 2); a current element IdL = 10−4(4, −3, 1) A · m at C pro-
duces a field dH at P .
a) Specify the direction of dH by a unit vector aH : Using the Biot-Savart law, we find
dH =
IdL × aCP
4πR2
CP
=
10−4[4ax − 3ay + az] × [−ax + ay − az]
4π33/2
=
[2ax + 3ay + az] × 10−4
65.3
from which
aH =
2ax + 3ay + az
√
14
= 0.53ax + 0.80ay + 0.27az
b) Find |dH|.
|dH| =
√
14 × 10−4
65.3
= 5.73 × 10−6
A/m = 5.73 µA/m
c) What direction al should IdL have at C so that dH = 0? IdL should be collinear with aCP ,
thus rendering the cross product in the Biot-Savart law equal to zero. Thus the answer is al =
±(−ax + ay − az)/
√
3
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![8.14. A toroid having a cross section of rectangular shape is defined by the following surfaces: the cylinders
ρ = 2 and ρ = 3 cm, and the planes z = 1 and z = 2.5 cm. The toroid carries a surface current density
of −50az A/m on the surface ρ = 3 cm. Find H at the point P (ρ, φ, z): The construction is similar
to that of the toroid of round cross section as done on p.239. Again, magnetic field exists only inside
the toroid cross section, and is given by
H =
Iencl
2πρ
aφ (2 < ρ < 3) cm, (1 < z < 2.5) cm
where Iencl is found from the given current density: On the outer radius, the current is
Iouter = −50(2π × 3 × 10−2
) = −3π A
This current is directed along negative z, which means that the current on the inner radius (ρ = 2) is
directed along positive z. Inner and outer currents have the same magnitude. It is the inner current that
is enclosed by the circular integration path in aφ within the toroid that is used in Ampere’s law. So
Iencl = +3π A. We can now proceed with what is requested:
a) PA(1.5cm, 0, 2cm): The radius, ρ = 1.5 cm, lies outside the cross section, and so HA = 0.
b) PB(2.1cm, 0, 2cm): This point does lie inside the cross section, and the φ and z values do not
matter. We find
HB =
Iencl
2πρ
aφ =
3aφ
2(2.1 × 10−2)
= 71.4 aφ A/m
c) PC(2.7cm, π/2, 2cm): again, φ and z values make no difference, so
HC =
3aφ
2(2.7 × 10−2)
= 55.6 aφ A/m
d) PD(3.5cm, π/2, 2cm). This point lies outside the cross section, and so HD = 0.
8.15. Assume that there is a region with cylindrical symmetry in which the conductivity is given by σ =
1.5e−150ρ kS/m. An electric field of 30 az V/m is present.
a) Find J: Use
J = σE = 45e−150ρ
az kA/m2
b) Find the total current crossing the surface ρ < ρ0, z = 0, all φ:
I = J · dS =
2π
0
ρ0
0
45e−150ρ
ρ dρ dφ =
2π(45)
(150)2
e−150ρ
[−150ρ − 1]
ρ0
0
kA
= 12.6 1 − (1 + 150ρ0)e−150ρ0 A
c) Make use of Ampere’s circuital law to find H: Symmetry suggests that H will be φ-directed only,
and so we consider a circular path of integration, centered on and perpendicular to the z axis.
Ampere’s law becomes: 2πρHφ = Iencl, where Iencl is the current found in part b, except with ρ0
replaced by the variable, ρ. We obtain
Hφ =
2.00
ρ
1 − (1 + 150ρ)e−150ρ
A/m
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![8.18. (continued) To find the magnetic field in region 1, we apply Ampere’s circuital law to the path c −
d − e − f − c, again noting that H will be zero along the two horizontal segments and along the right
vertical segment. This leaves only the left vertical segment, e − f , pointing in the +x direction, and
along which is field, Hx1. The counter-clockwise direction of the path integral is chosen using the
right-hand convention, where we take the normal to the path in the +z direction, which is the same as
the current direction. Assuming the height of the path is x, we find
Hx1 x = x
2
y1
8(2 − y)dy = x 16y − 4y2
2
y1
= x 16(2 − y1) − 4(4 − y2
1)
Replacing y1 with y, we find
Hx1 = 4[8 − 4y − 4 + y2
] ⇒ H1(1 < y < 2) = 4(y − 2)2
ax A/m
H1 lies in the positive x direction, since the result of the integration is net positive.
H in region 2 is now found through the line integral over the path d − g − h − c, enclosing all of region
1 within x and part of region 2 from y = y2 to 1:
Hx2 x = x
2
1
8(2 − y) dy + x
1
y2
8y dy = x 4(1 − 2)2
+ 4(1 − y2
2) = 4(2 − y2
2) x
so that in terms of y,
H2(0 < y < 1) = 4(2 − y2
)ax A/m
y
x
1 20-1-2
a
b c
d
e
f
g
h
x x . .
I1I2I3I4
4 3 2 1
y2 y1
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![8.18. (continued) The procedure is repeated for the remaining two regions, −2 < y < −1 and −1 < y < 0,
by taking the integration path with its right vertical segment within each of these two regions, while
the left vertical path is a − b. Again the integral is taken counter-clockwise, which means that the
right vertical path will be directed along −x. But the current is now in the opposite direction of that
for y > 0, making the enclosed current net negative. Therefore, H will be in the opposite direction
from that of the right vertical path, which is the positive x direction. The magnetic field will therefore
be symmetric about the y = 0 plane. We can use the results for regions 1 and 2 to construct the field
everywhere:
H = 0 (y > 2) and (y < −2)
H = 4(2 − |y|2
)ax A/m (0 < |y| < 1)
H = 4(|y| − 2)2
ax A/m (1 < |y| < 2)
8.19. Calculate ∇ × [∇(∇ · G)] if G = 2x2yz ax − 20y ay + (x2 − z2) az: Proceding, we first find ∇ · G =
4xyz − 20 − 2z. Then ∇(∇ · G) = 4yz ax + 4xz ay + (4xy − 2) az. Then
∇ × [∇(∇ · G)] = (4x − 4x) ax − (4y − 4y) ay + (4z − 4z) az = 0
8.20. The magnetic field intensity is given in the square region x = 0, 0.5 < y < 1, 1 < z < 1.5 by
H = z2ax + x3ay + y4az A/m.
a) evaluate H · dL about the perimeter of the square region: Using dL = dxax + dyay + dzaz,
and using the given field, we find, in the x = 0 plane:
H · dL =
1
.5
0 dy +
1.5
1
(1)4
dz +
.5
1
0 dy +
1
1.5
(.5)4
dz = 0.46875
b) Find ∇ × H:
∇ × H =
∂Hz
∂y
−
∂Hy
∂z
ax +
∂Hx
∂z
−
∂Hz
∂x
ay +
∂Hy
∂x
−
∂Hx
∂y
az
= 4y3
ax + 2zay + 3x2
az
c) Calculate (∇ × H)x at the center of the region: Here, y = 0.75 and so (∇ × H)x = 4(.75)3 =
1.68750.
d) Does (∇×H)x = [ H·dL]/Area Enclosed? Using the part a result, [ H·dL]/Area Enclosed =
0.46875/0.25 = 1.8750, which is off the value found in part c. Answer: No. Reason: the limit
of the area shrinking to zero must be taken before the results will be equal.
8.21. Points A, B, C, D, E, and F are each 2 mm from the origin on the coordinate axes indicated in Fig.
8.23. The value of H at each point is given. Calculate an approximate value for ∇ × H at the origin:
We use the approximation:
curl H
.
=
H · dL
a
where no limit as a → 0 is taken (hence the approximation), and where a = 4 mm2. Each curl
component is found by integrating H over a square path that is normal to the component in question.
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![8.23. (continued)
b) Integrate J over the circular surface ρ = 1, 0 < φ < 2π, z = 0, to determine the total current
passing through that surface in the az direction: The integral is:
I = J · dS =
2π
0
1
0
60ρaz · ρ dρ dφaz = 40π A
c) Find the total current once more, this time by a line integral around the circular path ρ = 1,
0 < φ < 2π, z = 0:
I = H · dL =
2π
0
20ρ2
aφ ρ=1
· (1)dφaφ =
2π
0
20 dφ = 40π A
8.24. Evaluate both sides of Stokes’theorem for the field G = 10 sin θ aφ and the surface r = 3, 0 ≤ θ ≤ 90◦,
0 ≤ φ ≤ 90◦. Let the surface have the ar direction: Stokes’ theorem reads:
C
G · dL =
S
(∇ × G) · n da
Considering the given surface, the contour, C, that forms its perimeter consists of three joined arcs of
radius 3 that sweep out 90◦ in the xy, xz, and zy planes. Their centers are at the origin. Of these three,
only the arc in the xy plane (which lies along aφ) is in the direction of G; the other two (in the −aθ and
aθ directions respectively) are perpendicular to it, and so will not contribute to the path integral. The
left-hand side therefore consists of only the xy plane portion of the closed path, and evaluates as
G · dL =
π/2
0
10 sin θ π/2
aφ · aφ 3 sin θ π/2
dφ = 15π
To evaluate the right-hand side, we first find
∇ × G =
1
r sin θ
d
dθ
[(sin θ)10 sin θ] ar =
20 cos θ
r
ar
The surface over which we integrate this is the one-eighth spherical shell of radius 3 in the first octant,
bounded by the three arcs described earlier. The right-hand side becomes
S
(∇ × G) · n da =
π/2
0
π/2
0
20 cos θ
3
ar · ar (3)2
sin θ dθ dφ = 15π
It would appear that the theorem works.
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![8.30. A solid nonmagnetic conductor of circular cross-section has a radius of 2mm. The conductor is inho-
mogeneous, with σ = 106(1 + 106ρ2) S/m. If the conductor is 1m in length and has a voltage of 1mV
between its ends, find:
a) H inside: With current along the cylinder length (along az, and with φ symmetry, H will be φ-
directed only. We find E = (V0/d)az = 10−3az V/m. Then J = σE = 103(1 + 106ρ2)az A/m2.
Next we apply Ampere’s circuital law to a circular path of radius ρ, centered on the z axis and
normal to the axis:
H · dL = 2πρHφ =
S
J · dS =
2π
0
ρ
0
103
(1 + 106
(ρ′
)2
)az · azρ′
dρ′
dφ
Thus
Hφ =
103
ρ
ρ
0
ρ′
+ 106
(ρ′
)3
dρ′
=
103
ρ
ρ2
2
+
106
4
ρ4
Finally, H = 500ρ(1 + 5 × 105ρ3)aφ A/m (0 < ρ < 2mm).
b) the total magnetic flux inside the conductor: With field in the φ direction, a plane normal to B will
be that in the region 0 < ρ < 2 mm, 0 < z < 1 m. The flux will be
=
S
B·dS = µ0
1
0
2×10−3
0
500ρ + 2.5 × 108
ρ3
dρdz = 8π ×10−10
Wb = 2.5 nWb
8.31. The cylindrical shell defined by 1 cm < ρ < 1.4 cm consists of a non-magnetic conducting material
and carries a total current of 50 A in the az direction. Find the total magnetic flux crossing the plane
φ = 0, 0 < z < 1:
a) 0 < ρ < 1.2 cm: We first need to find J, H, and B: The current density will be:
J =
50
π[(1.4 × 10−2)2 − (1.0 × 10−2)2]
az = 1.66 × 105
az A/m2
Next we find Hφ at radius ρ between 1.0 and 1.4 cm, by applying Ampere’s circuital law, and
noting that the current density is zero at radii less than 1 cm:
2πρHφ = Iencl =
2π
0
ρ
10−2
1.66 × 105
ρ′
dρ′
dφ
⇒ Hφ = 8.30 × 104 (ρ2 − 10−4)
ρ
A/m (10−2
m < ρ < 1.4 × 10−2
m)
Then B = µ0H, or
B = 0.104
(ρ2 − 10−4)
ρ
aφ Wb/m2
Now,
a = B · dS =
1
0
1.2×10−2
10−2
0.104 ρ −
10−4
ρ
dρ dz
= 0.104
(1.2 × 10−2)2 − 10−4
2
− 10−4
ln
1.2
1.0
= 3.92 × 10−7
Wb = 0.392 µWb
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![8.31b) 1.0 cm < ρ < 1.4 cm (note typo in book): This is part a over again, except we change the upper limit
of the radial integration:
b = B · dS =
1
0
1.4×10−2
10−2
0.104 ρ −
10−4
ρ
dρ dz
= 0.104
(1.4 × 10−2)2 − 10−4
2
− 10−4
ln
1.4
1.0
= 1.49 × 10−6
Wb = 1.49 µWb
c) 1.4 cm < ρ < 20 cm: This is entirely outside the current distribution, so we need B there: We
modify the Ampere’s circuital law result of part a to find:
Bout = 0.104
[(1.4 × 10−2)2 − 10−4]
ρ
aφ =
10−5
ρ
aφ Wb/m2
We now find
c =
1
0
20×10−2
1.4×10−2
10−5
ρ
dρ dz = 10−5
ln
20
1.4
= 2.7 × 10−5
Wb = 27 µWb
8.32. The free space region defined by 1 < z < 4 cm and 2 < ρ < 3 cm is a toroid of rectangular
cross-section. Let the surface at ρ = 3 cm carry a surface current K = 2az kA/m.
a) Specify the current densities on the surfaces at ρ = 2 cm, z = 1cm, and z = 4cm. All surfaces
must carry equal currents. With this requirement, we find: K(ρ = 2) = −3 az kA/m. Next, the
current densities on the z = 1 and z = 4 surfaces must transistion between the current density
values at ρ = 2 and ρ = 3. Knowing the the radial current density will vary as 1/ρ, we find
K(z = 1) = (60/ρ)aρ A/m with ρ in meters. Similarly, K(z = 4) = −(60/ρ)aρ A/m.
b) Find H everywhere: Outside the toroid, H = 0. Inside, we apply Ampere’s circuital law in the
manner of Problem 8.14:
H · dL = 2πρHφ =
2π
0
K(ρ = 2) · az (2 × 10−2
) dφ
⇒ H = −
2π(3000)(.02)
ρ
aφ = −60/ρ aφ A/m (inside)
c) Calculate the total flux within the toriod: We have B = −(60µ0/ρ)aφ Wb/m2. Then
=
.04
.01
.03
.02
−60µ0
ρ
aφ · (−aφ) dρ dz = (.03)(60)µ0 ln
3
2
= 0.92 µWb
8.33. Use an expansion in cartesian coordinates to show that the curl of the gradient of any scalar field G is
identically equal to zero. We begin with
∇G =
∂G
∂x
ax +
∂G
∂y
ay +
∂G
∂z
az
and
∇ × ∇G =
∂
∂y
∂G
∂z
−
∂
∂z
∂G
∂y
ax +
∂
∂z
∂G
∂x
−
∂
∂x
∂G
∂z
ay
+
∂
∂x
∂G
∂y
−
∂
∂y
∂G
∂x
az = 0 for any G
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![8.34. A filamentary conductor on the z axis carries a current of 16A in the az direction, a conducting shell
at ρ = 6 carries a total current of 12A in the −az direction, and another shell at ρ = 10 carries a total
current of 4A in the −az direction.
a) Find H for 0 < ρ < 12: Ampere’s circuital law states that H·dL = Iencl, where the line integral
and current direction are related in the usual way through the right hand rule. Therefore, if I is in
the positive z direction, H is in the aφ direction. We proceed as follows:
0 < ρ < 6 : 2πρHφ = 16 ⇒ H = 16/(2πρ)aφ
6 < ρ < 10 : 2πρHφ = 16 − 12 ⇒ H = 4/(2πρ)aφ
ρ > 10 : 2πρHφ = 16 − 12 − 4 = 0 ⇒ H = 0
b) Plot Hφ vs. ρ:
c) Find the total flux crossing the surface 1 < ρ < 7, 0 < z < 1: This will be
=
1
0
6
1
16µ0
2πρ
dρ dz +
1
0
7
6
4µ0
2πρ
dρ dz =
2µ0
π
[4 ln 6 + ln(7/6)] = 5.9 µWb
8.35. A current sheet, K = 20 az A/m, is located at ρ = 2, and a second sheet, K = −10 az A/m is located
at ρ = 4.
a.) Let Vm = 0 at P (ρ = 3, φ = 0, z = 5) and place a barrier at φ = π. Find Vm(ρ, φ, z) for
−π < φ < π: Since the current is cylindrically-symmetric, we know that H = I/(2πρ) aφ,
where I is the current enclosed, equal in this case to 2π(2)K = 80π A. Thus, using the result of
Section 8.6, we find
Vm = −
I
2π
φ = −
80π
2π
φ = −40φ A
which is valid over the region 2 < ρ < 4, −π < φ < π, and −∞ < z < ∞. For ρ > 4, the
outer current contributes, leading to a total enclosed current of
Inet = 2π(2)(20) − 2π(4)(10) = 0
With zero enclosed current, Hφ = 0, and the magnetic potential is zero as well.
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![8.35b. Let A = 0 at P and find A(ρ, φ, z) for 2 < ρ < 4: Again, we know that H = Hφ(ρ), since the current
is cylindrically symmetric. With the current only in the z direction, and again using symmmetry, we
expect only a z component of A which varies only with ρ. We can then write:
∇ × A = −
dAz
dρ
aφ = B =
µ0I
2πρ
aφ
Thus
dAz
dρ
= −
µ0I
2πρ
⇒ Az = −
µ0I
2π
ln(ρ) + C
We require that Az = 0 at ρ = 3. Therefore C = [(µ0I)/(2π)] ln(3), Then, with I = 80π, we finally
obtain
A = −
µ0(80π)
2π
[ln(ρ) − ln(3)] az = 40µ0 ln
3
ρ
az Wb/m
8.36. Let A = (3y − z)ax + 2xzay Wb/m in a certain region of free space.
a) Show that ∇ · A = 0:
∇ · A =
∂
∂x
(3y − z) +
∂
∂y
2xz = 0
b) At P (2, −1, 3), find A, B, H, and J: First AP = −6ax + 12ay. Then, using the curl formula in
cartesian coordinates,
B = ∇ × A = −2xax − ay + (2z − 3)az ⇒ BP = −4ax − ay + 3az Wb/m2
Now
HP = (1/µ0)BP = −3.2 × 106
ax − 8.0 × 105
ay + 2.4 × 106
az A/m
Then J = ∇ × H = (1/µ0)∇ × B = 0, as the curl formula in cartesian coordinates shows.
8.37. Let N = 1000, I = 0.8 A, ρ0 = 2 cm, and a = 0.8 cm for the toroid shown in Fig. 8.12b. Find Vm in
the interior of the toroid if Vm = 0 at ρ = 2.5 cm, φ = 0.3π. Keep φ within the range 0 < φ < 2π:
Well-within the toroid, we have
H =
NI
2πρ
aφ = −∇Vm = −
1
ρ
dVm
dφ
aφ
Thus
Vm = −
NIφ
2π
+ C
Then,
0 = −
1000(0.8)(0.3π)
2π
+ C
or C = 120. Finally
Vm = 120 −
400
π
φ A (0 < φ < 2π)
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![8.42. Show that ∇2(1/R12) = −∇1(1/R12) = R21/R3
12. First
∇2
1
R12
= ∇2 (x2 − x1)2
+ (y2 − y1)2
+ (z2 − z1)2
−1/2
= −
1
2
2(x2 − x1)ax + 2(y2 − y1)ay + 2(z2 − z1)az
[(x2 − x1)2 + (y2 − y1)2 + (z2 − z1)2]3/2
=
−R12
R3
12
=
R21
R3
12
Also note that ∇1(1/R12) would give the same result, but of opposite sign.
8.43. Compute the vector magnetic potential within the outer conductor for the coaxial line whose vector
magnetic potential is shown in Fig. 8.20 if the outer radius of the outer conductor is 7a. Select the
proper zero reference and sketch the results on the figure: We do this by first finding B within the outer
conductor and then “uncurling” the result to find A. With −z-directed current I in the outer conductor,
the current density is
Jout = −
I
π(7a)2 − π(5a)2
az = −
I
24πa2
az
Since current I flows in both conductors, but in opposite directions, Ampere’s circuital law inside the
outer conductor gives:
2πρHφ = I −
2π
0
ρ
5a
I
24πa2
ρ′
dρ′
dφ ⇒ Hφ =
I
2πρ
49a2 − ρ2
24a2
Now, with B = µ0H, we note that ∇ × A will have a φ component only, and from the direction and
symmetry of the current, we expect A to be z-directed, and to vary only with ρ. Therefore
∇ × A = −
dAz
dρ
aφ = µ0H
and so
dAz
dρ
= −
µ0I
2πρ
49a2 − ρ2
24a2
Then by direct integration,
Az =
−µ0I(49)
48πρ
dρ +
µ0Iρ
48πa2
dρ + C =
µ0I
96π
ρ2
a2
− 98 ln ρ + C
As per Fig. 8.20, we establish a zero reference at ρ = 5a, enabling the evaluation of the integration
constant:
C = −
µ0I
96π
[25 − 98 ln(5a)]
Finally,
Az =
µ0I
96π
ρ2
a2
− 25 + 98 ln
5a
ρ
Wb/m
A plot of this continues the plot of Fig. 8.20, in which the curve goes negative at ρ = 5a, and then
approaches a minimum of −.09µ0I/π at ρ = 7a, at which point the slope becomes zero.
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![8.44. By expanding Eq.(58), Sec. 8.7 in cartesian coordinates, show that (59) is correct. Eq. (58) can be
rewritten as
∇2
A = ∇(∇ · A) − ∇ × ∇ × A
We begin with
∇ · A =
∂Ax
∂x
+
∂Ay
∂y
+
∂Az
∂z
Then the x component of ∇(∇ · A) is
[∇(∇ · A)]x =
∂2Ax
∂x2
+
∂2Ay
∂x∂y
+
∂2Az
∂x∂z
Now
∇ × A =
∂Az
∂y
−
∂Ay
∂z
ax +
∂Ax
∂z
−
∂Az
∂x
ay +
∂Ay
∂x
−
∂Ax
∂y
az
and the x component of ∇ × ∇ × A is
[∇ × ∇ × A]x =
∂2Ay
∂x∂y
−
∂2Ax
∂y2
−
∂2Ax
∂z2
+
∂2Az
∂z∂y
Then, using the underlined results
[∇(∇ · A) − ∇ × ∇ × A]x =
∂2Ax
∂x2
+
∂2Ax
∂y2
+
∂2Ax
∂z2
= ∇2
Ax
Similar results will be found for the other two components, leading to
∇(∇ · A) − ∇ × ∇ × A = ∇2
Axax + ∇2
Ayay + ∇2
Azaz ≡ ∇2
A QED
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![9.2 (continued) Motion along negative y through the field would cause further deflection into the negative
x direction. We can construct the differential equations for the forces in x and in y as follows:
Fxax = m
dvx
dt
ax = qvyay × Baz = qBvyax
Fyay = m
dvy
dt
ay = qvxax × Baz = −qBvxay
or
dvx
dt
=
qB
m
vy (1)
and
dvy
dt
= −
qB
m
vx (2)
To solve these equations, we first differentiate (2) with time and substitute (1), obtaining:
d2vy
dt2
= −
qB
m
dvx
dt
= −
qB
m
2
vy
Therefore, vy = A sin(qBt/m) + A′ cos(qBt/m). However, at t = 0, vy = 0, and so A′ = 0, leaving
vy = A sin(qBt/m). Then, using (2),
vx = −
m
qB
dvy
dt
= −A cos
qBt
m
Now at t = 0, vx = vx0 = 3 × 105. Therefore A = −vx0, and so vx = vx0 cos(qBt/m), and
vy = −vx0 sin(qBt/m). The positions are then found by integrating vx and vy over time:
x(t) = vx0 cos
qBt
m
dt + C =
mvx0
qB
sin
qBt
m
+ C
where C = 0, since x(0) = 0. Then
y(t) = −vx0 sin
qBt
m
dt + D =
mvx0
qB
cos
qBt
m
+ D
We require that y(0) = 0, so D = −(mvx0)/(qB), and finally y(t) = −mvx0/qB [1 − cos (qBt/m)].
Summarizing, we have, using q = −3×10−7 C, m = 3×10−16 kg, B = 30×10−3 T, and vx0 = 3×105
m/s:
x(t) =
mvx0
qB
sin
qBt
m
= −10−2
sin(−3 × 10−7
t) m
y(t) = −
mvx0
qB
1 − cos
qBt
m
= 10−2
[1 − cos(−3 × 107
t)] m
vx(t) = vx0 cos
qBt
m
= 3 × 105
cos(−3 × 107
t) m/s
vy(t) = −vx0 sin
qBt
m
= −3 × 105
sin(−3 × 107
t) m/s
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![9.2 (continued) The answers are now:
a) At t = 3 × 10−6 s, x = 8.9 mm, y = 14.5 mm, and z = 0.
b) At t = 3 × 10−6 s, vx = −1.3 × 105 m/s, vy = 2.7 × 105 m/s, and so
v(t = 3 µs) = −1.3 × 105
ax + 2.7 × 105
ay m/s
whose magnitude is v = 3 × 105 m/s as would be expected.
c) Kinetic energy is K.E. = (1/2)mv2 = 1.35 µJ at all times.
9.3. A point charge for which Q = 2 × 10−16 C and m = 5 × 10−26 kg is moving in the combined fields
E = 100ax − 200ay + 300az V/m and B = −3ax + 2ay − az mT. If the charge velocity at t = 0 is
v(0) = (2ax − 3ay − 4az) × 105 m/s:
a) give the unit vector showing the direction in which the charge is accelerating at t = 0: Use
F(t = 0) = q[E + (v(0) × B)], where
v(0) × B = (2ax − 3ay − 4az)105
× (−3ax + 2ay − az)10−3
= 1100ax + 1400ay − 500az
So the force in newtons becomes
F(0) = (2×10−16
)[(100+1100)ax+(1400−200)ay+(300−500)az] = 4×10−14
[6ax+6ay−az]
The unit vector that gives the acceleration direction is found from the force to be
aF =
6ax + 6ay − az
√
73
= .70ax + .70ay − .12az
b) find the kinetic energy of the charge at t = 0:
K.E. =
1
2
m|v(0)|2
=
1
2
(5 × 10−26
kg)(5.39 × 105
m/s)2
= 7.25 × 10−15
J = 7.25 fJ
9.4. An electron (qe = −1.60219 × 10−19 C, m = 9.10956 × 10−31 kg) is moving at a constant velocity
v = 4.5 × 107ay m/s along the negative y axis. At the origin it encounters the uniform magnetic field
B = 2.5az mT, and remains in it up to y = 2.5 cm. If we assume (with good accuracy) that the electron
remains on the y axis while it is in the magnetic field, find its x-, y-, and z-coordinate values when
y = 50 cm: The procedure is to find the electron velocity as it leaves the field, and then determine its
coordinates at the time corresponding to y = 50 cm. The force it encounters while in the field is
F = qv × B = (−1.60219 × 10−19
)(4.5 × 107
)(2.5 × 10−3
)(ay × az) = −1.80 × 10−14
ax N
This force will be constant during the time the electron traverses the field. It establishes a negative
x-directed velocity as it leaves the field, given by the acceleration times the transit time, tt :
vx =
Ftt
m
=
−1.80 × 1014 N
9.10956 × 10−31 kg
2.5 × 10−2 m
4.5 × 107 m/s
= −1.09 × 107
m/s
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![9.9. A current of −100az A/m flows on the conducting cylinder ρ = 5 mm and +500az A/m is present
on the conducting cylinder ρ = 1 mm. Find the magnitude of the total force acting to split the outer
cylinder apart along its length: The differential force acting on the outer cylinder arising from the field
of the inner cylinder is dF = Kouter × B, where B is the field from the inner cylinder, evaluated at the
outer cylinder location:
B =
2π(1)(500)µ0
2π(5)
aφ = 100µ0 aφ T
Thus dF = −100az × 100µ0aφ = 104µ0aρ N/m2. We wish to find the force acting to split the outer
cylinder, which means we need to evaluate the net force in one cartesian direction on one half of the
cylinder. We choose the “upper” half (0 < φ < π), and integrate the y component of dF over this
range, and over a unit length in the z direction:
Fy =
1
0
π
0
104
µ0aρ · ay(5 × 10−3
) dφ dz =
π
0
50µ0 sin φ dφ = 100µ0 = 4π × 10−5
N/m
Note that we did not include the “self force” arising from the outer cylinder’s B field on itself. Since the
outer cylinder is a two-dimensional current sheet, its field exists only just outside the cylinder, and so no
force exists. If this cylinder possessed a finite thickness, then we would need to include its self-force,
since there would be an interior field and a volume current density that would spatially overlap.
9.10. Two infinitely-long parallel filaments each carry 50 A in the az direction. If the filaments lie in the
plane y = 0 at x = 0 and x = 5mm (note bad wording in problem statement in book), find the vector
force per meter length on the filament passing through the origin: The force will be
F =
1
0
IdL × B
where IdL is that of the filament at the origin, and B is that arising from the filament at x = 5mm
evaluated at the location of the other filament (along the z axis). We obtain
F =
1
0
50 dzaz ×
−50µ0ay
2π(5 × 10−3)
= 0.10 ax N/m
9.11. a) Use Eq. (14), Sec. 9.3, to show that the force of attraction per unit length between two filamentary
conductors in free space with currents I1az at x = 0, y = d/2, and I2az at x = 0, y = −d/2, is
µ0I1I2/(2πd): The force on I2 is given by
F2 = µ0
I1I2
4π
aR12 × dL1
R2
12
× dL2
Let z1 indicate the z coordinate along I1, and z2 indicate the z coordinate along I2. We then have
R12 = (z2 − z1)2 + d2 and
aR12 =
(z2 − z1)az − day
(z2 − z1)2 + d2
Also, dL1 = dz1az and dL2 = dz2az The “inside” integral becomes:
aR12 × dL1
R2
12
=
[(z2 − z1)az − day] × dz1az
[(z2 − z1)2 + d2]1.5
=
∞
−∞
−d dz1 ax
[(z2 − z1)2 + d2]1.5
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![9.11a. (continued) The force expression now becomes
F2 = µ0
I1I2
4π
∞
−∞
−d dz1 ax
[(z2 − z1)2 + d2]1.5
× dz2az = µ0
I1I2
4π
1
0
∞
−∞
d dz1 dz2 ay
[(z2 − z1)2 + d2]1.5
Note that the “outside” integral is taken over a unit length of current I2. Evaluating, obtain,
F2 = µ0
I1I2d ay
4πd2
(2)
1
0
dz2 =
µ0I1I2
2πd
ay N/m
as expected.
b) Show how a simpler method can be used to check your result: We use dF2 = I2dL2 × B12, where
the field from current 1 at the location of current 2 is
B12 =
µ0I1
2πd
ax T
so over a unit length of I2, we obtain
F2 = I2az ×
µ0I1
2πd
ax = µ0
I1I2
2πd
ay N/m
This second method is really just the first over again, since we recognize the inside integral of the
first method as the Biot-Savart law, used to find the field from current 1 at the current 2 location.
9.12. A conducting current strip carrying K = 12az A/m lies in the x = 0 plane between y = 0.5 and y = 1.5
m. There is also a current filament of I = 5 A in the az direction on the z axis. Find the force exerted
on the:
a) filament by the current strip: We first need to find the field from the current strip at the filament
location. Consider the strip as made up of many adjacent strips of width dy, each carrying
current dIaz = Kdy. The field along the z axis from each differential strip will be dB =
[(Kdyµ0)/(2πy)]ax. The total B field from the strip evaluated along the z axis is therefore
B =
1.5
0.5
12µ0ax
2πy
dy =
6µ0
π
ln
1.5
0.5
ax = 2.64 × 10−6
ax Wb/m2
Now
F =
1
0
IdL × B =
1
0
5dz az × 2.64 × 10−6
ax dz = 13.2 ay µN/m
b) strip by the filament: In this case we integrate K ×B over a unit length in z of the strip area, where
B is the field from the filament evaluated on the strip surface:
F =
Area
K × B da =
1
0
1.5
0.5
12az ×
−5µ0ax
2πy
dy =
−30µ0
π
ln(3) ay = −13.2 ay µN/m
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![9.14a (continued) The force acting on the segment farther from the y axis will be
F2 = IL × B = 30(3 × 10−2
)ay × −350µ0ax = 315µ0 az N
The torque about the origin is now T = R1 × F1 + R2 × F2, where R1 is the vector directed from the
origin to the midpoint of the nearer y-directed segment, and R2 is the vector joining the origin to the
midpoint of the farther y-directed segment. So R1(cm) = ax + 3.5ay and R2(cm) = 3ax + 3.5ay.
Therefore
T0,0,0 = [(ax + 3.5ay) × 10−2
] × −315µ0 az + [(3ax + 3.5ay) × 10−2
] × 315µ0 az
= −6.30µ0ay = −7.92 × 10−6
ay N−m
b) at the center of the loop: Use T = IS × B where S = (2 × 3) × 10−4 az m2. So
T = 30(6 × 10−4
az) × (−350µ0 ax) = −7.92 × 10−6
ay N−m
9.15. A solid conducting filament extends from x = −b to x = b along the line y = 2, z = 0. This filament
carries a current of 3 A in the ax direction. An infinite filament on the z axis carries 5 A in the az
direction. Obtain an expression for the torque exerted on the finite conductor about an origin located
at (0, 2, 0): The differential force on the wire segment arising from the field from the infinite wire is
dF = 3 dx ax ×
5µ0
2πρ
aφ = −
15µ0 cos φ dx
2π
√
x2 + 4
az = −
15µ0x dx
2π(x2 + 4)
az
So now the differential torque about the (0, 2, 0) origin is
dT = RT × dF = x ax × −
15µ0x dx
2π(x2 + 4)
az =
15µ0x2 dx
2π(x2 + 4)
ay
The torque is then
T =
b
−b
15µ0x2 dx
2π(x2 + 4)
ay =
15µ0
2π
ay x − 2 tan−1 x
2
b
−b
= (6 × 10−6
) b − 2 tan−1 b
2
ay N · m
9.16. Assume that an electron is describing a circular orbit of radius a about a positively-charged nucleus.
a) By selecting an appropriate current and area, show that the equivalent orbital dipole moment is
ea2ω/2, where ω is the electron’s angular velocity: The current magnitude will be I = e
T , where
e is the electron charge and T is the orbital period. The latter is T = 2π/ω, and so I = eω/(2π).
Now the dipole moment magnitude will be m = IA, where A is the loop area. Thus
m =
eω
2π
πa2
=
1
2
ea2
ω //
b) Show that the torque produced by a magnetic field parallel to the plane of the orbit is ea2ωB/2:
With B assumed constant over the loop area, we would have T = m × B. With B parallel to the
loop plane, m and B are orthogonal, and so T = mB. So, using part a, T = ea2ωB/2.
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![9.17. (continued) As for the magnetic moment, we have
m = IS =
eω
2π
πa2
=
1
2
ωea2 .
=
1
2
ea2
ω0 −
eB
2me
=
1
2
ω0ea2
−
1
4
e2a2B
me
//
Finally, for a = 6 × 10−11 m, B = 0.5 T, we have
ω
ω
=
eB
2me
1
ω
.
=
eB
2me
1
ω0
=
1.60 × 10−19 × 0.5
2 × 9.1 × 10−31 × 3.4 × 1016
= 1.3 × 10−6
where ω0 = 3.4 × 1016 sec−1 is found from Problem 16. Finally,
m
m
=
e2a2B
4me
×
2
ωea2
.
=
eB
2meω0
= 1.3 × 10−6
9.18. Calculate the vector torque on the square loop shown in Fig. 9.16 about an origin at A in the field B,
given:
a) A(0, 0, 0) and B = 100ay mT: The field is uniform and so does not produce any translation of the
loop. Therefore, we may use T = IS × B about any origin, where I = 0.6 A and S = 16az m2.
We find T = 0.6(16)az × 0.100ay = −0.96 ax N−m.
b) A(0, 0, 0) and B = 200ax + 100ay mT: Using the same reasoning as in part a, we find
T = 0.6(16)az × (0.200ax + 0.100ay) = −0.96ax + 1.92ay N−m
c) A(1, 2, 3) and B = 200ax +100ay −300az mT: We observe two things here: 1) The field is again
uniform and so again the torque is independent of the origin chosen, and 2) The field differs from
that of part b only by the addition of a z component. With S in the z direction, this new component
of B will produce no torque, so the answer is the same as part b, or T = −0.96ax + 1.92ay N−m.
d) A(1, 2, 3) and B = 200ax + 100ay − 300az mT for x ≥ 2 and B = 0 elsewhere: Now, force
is acting only on the y-directed segment at x = +2, so we need to be careful, since translation
will occur. So we must use the given origin. The differential torque acting on the differential wire
segment at location (2,y) is dT = R(y) × dF, where
dF = IdL × B = 0.6 dy ay × [0.2ax + 0.1ay − 0.3az] = [−0.18ax − 0.12az] dy
and R(y) = (2, y, 0) − (1, 2, 3) = ax + (y − 2)ay − 3az. We thus find
dT = R(y) × dF = ax + (y − 2)ay − 3az × [−0.18ax − 0.12az] dy
= −0.12(y − 2)ax + 0.66ay + 0.18(y − 2)az dy
The net torque is now
T =
2
−2
−0.12(y − 2)ax + 0.66ay + 0.18(y − 2)az dy = 0.96ax + 2.64ay − 1.44az N−m
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![magnetic field strength H
(1)
c
.
= 270 A/m. We check this by applying Ampere’s circuital law to the
magnetic circuit:
H · dL = H(1)
c Lc + H(1)
g d
where H
(1)
c Lc = (270)(8×10−2) = 22, and where H
(1)
g d = (1)¨g = (2.8×10−4)(7.1×105) =
199. But we require that
H · dL = 200 A · t
whereas the actual result in this first calculation is 199 + 22 = 221, which is too high. So, for a
second trial, we reduce B to B
(2)
c = 1 Wb/m2. This yields H
(2)
c = 200 A/m from Fig. 9.11, and
thus (2) = 2.5 × 10−4 Wb. Now
H · dL = H(2)
c Lc + (2)
Rg = 200(8 × 10−2
) + (2.5 × 10−4
)(7.1 × 105
) = 194
This is less than 200, meaning that the actual flux is slightly higher than 2.5 × 10−4 Wb.
I will leave the answer at that, considering the lack of fine resolution in Fig. 9.11.
9.32. Determine the total energy stored in a spherical region 1cm in radius, centered at the origin in free
space, in the uniform field:
a) H1 = −600ay A/m: First we find the energy density:
wm1 =
1
2
B1 · H1 =
1
2
µ0H2
1 =
1
2
(4π × 10−7
)(600)2
= 0.226 J/m3
The energy within the sphere is then
Wm1 = wm1
4
3
πa3
= 0.226
4
3
π × 10−6
= 0.947 µJ
b) H2 = 600ax + 1200ay A/m: In this case the energy density is
wm2 =
1
2
µ0 (600)2
+ (1200)2
=
5
2
µ0(600)2
or five times the energy density that was found in part a. Therefore, the stored energy in this field
is five times the amount in part a, or Wm2 = 4.74 µJ.
c) H3 = −600ax + 1200ay. This field differs from H2 only by the negative x component, which is a
non-issue since the component is squared when finding the energy density. Therefore, the stored
energy will be the same as that in part b, or Wm3 = 4.74 µJ.
d) H4 = H2 + H3, or 2400ay A/m: The energy density is now wm4 = (1/2)µ0(2400)2 =
(1/2)µ0(16)(600)2 J/m3, which is sixteen times the energy density in part a. The stored en-
ergy is therefore sixteen times that result, or Wm4 = 16(0.947) = 15.2 µJ.
e) 1000ax A/m+0.001ax T: The energy density is wm5 = (1/2)µ0[1000+.001/µ0]2 = 2.03 J/m3.
Then Wm5 = 2.03[(4/3)π × 10−6] = 8.49 µJ.
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![9.35. The cones θ = 21◦ and θ = 159◦ are conducting surfaces and carry total currents of 40 A, as shown in
Fig. 9.18. The currents return on a spherical conducting surface of 0.25 m radius.
a) Find H in the region 0 < r < 0.25, 21◦ < θ < 159◦, 0 < φ < 2π: We can apply Ampere’s
circuital law and take advantage of symmetry. We expect to see H in the aφ direction and it would
be constant at a given distance from the z axis. We thus perform the line integral of H over a circle,
centered on the z axis, and parallel to the xy plane:
H · dL =
2π
0
Hφaφ · r sin θaφ dφ = Iencl. = 40 A
Assuming that Hφ is constant over the integration path, we take it outside the integral and solve:
Hφ =
40
2πr sin θ
⇒ H =
20
πr sin θ
aφ A/m
b) How much energy is stored in this region? This will be
WH =
v
1
2
µ0H2
φ =
2π
0
159◦
21◦
.25
0
200µ0
π2r2 sin2 θ
r2
sin θ dr dθ dφ =
100µ0
π
159◦
21◦
dθ
sin θ
=
100µ0
π
ln
tan(159/2)
tan(21/2)
= 1.35 × 10−4
J
9.36. A filament carrying current I in the az direction lies on the z axis, and cylindrical current sheets of 5az
A/m and −2az A/m are located at ρ = 3 and ρ = 10, respectively.
a) Find I if H = 0 for ρ > 10. Ampere’s circuital law says, for ρ > 10:
2πρH = 2π(3)(5) − 2π(10)(2) + I = 0
from which I = 2π(10)(3) − 2π(3)(5) = 10π A.
b) Using this value of I, calculate H for all ρ, 3 < ρ < 10: Again, using Ampere’s circuital law, we
find
H(3 < ρ < 10) =
1
2πρ
[10π + 2π(3)(5)] aφ =
20
ρ
aφ A/m
c) Calculate and plot WH versus ρ0, where WH is the total energy stored within the volume 0 < z < 1,
0 < φ < 2π, 3 < ρ < ρ0: First the energy density will be wH = (1/2)µ0H2 = 200µ0/ρ2 J/m3.
Then the energy is
WH =
1
0
2π
0
ρ0
3
200µ0
ρ2
ρ dρ dφ dz = 400πµ0 ln
ρ0
3
= (1.58 × 10−3
) ln
ρ0
3
J
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![Then
emf = −
d
dt
=
0.16
3
(3)(5t +2t3
)2
(5+6t2
) = −(0.16)[5(.4)+2(.4)3
]2
[5+6(.4)2
] = −4.32 V
b) x = 0.6 m: Have 0.6 = 5t + 2t3, from which we find t = 0.1193. Thus
emf = −(0.16)[5(.1193) + 2(.1193)3
]2
[5 + 6(.1193)2
] = −.293 V
10.6. A perfectly conducting filament containing a small 500- resistor is formed into a square, as illustrated
in Fig. 10.6. Find I(t) if
a) B = 0.3 cos(120πt −30◦) az T: First the flux through the loop is evaluated, where the unit normal
to the loop is az. We find
=
loop
B · dS = (0.3)(0.5)2
cos(120πt − 30◦
) Wb
Then the current will be
I(t) =
emf
R
= −
1
R
d
dt
=
(120π)(0.3)(0.25)
500
sin(120πt − 30◦
) = 57 sin(120πt − 30◦
) mA
b) B = 0.4 cos[π(ct − y)] az µT where c = 3 × 108 m/s: Since the field varies with y, the flux is
now
=
loop
B · dS = (0.5)(0.4)
.5
0
cos(πy − πct) dy =
0.2
π
[sin(πct − π/2) − sin(πct)] µWb
The current is then
I(t) =
emf
R
= −
1
R
d
dt
=
−0.2c
500
[cos(πct − π/2) − cos(πct)] µA
=
−0.2(3 × 108)
500
[sin(πct) − cos(πct)] µA = 120 [cos(πct) − sin(πct)] mA
10.7. The rails in Fig. 10.7 each have a resistance of 2.2 /m. The bar moves to the right at a constant speed
of 9 m/s in a uniform magnetic field of 0.8 T. Find I(t), 0 < t < 1 s, if the bar is at x = 2 m at t = 0
and
a) a 0.3 resistor is present across the left end with the right end open-circuited: The flux in the
left-hand closed loop is
l = B × area = (0.8)(0.2)(2 + 9t)
Then, emfl = −d l/dt = −(0.16)(9) = −1.44 V. With the bar in motion, the loop resistance is
increasing with time, and is given by Rl(t) = 0.3 + 2[2.2(2 + 9t)]. The current is now
Il(t) =
emfl
Rl(t)
=
−1.44
9.1 + 39.6t
A
Note that the sign of the current indicates that it is flowing in the direction opposite that shown in
the figure.
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![b) Repeat part a, but with a resistor of 0.3 across each end: In this case, there will be a contribution
to the current from the right loop, which is now closed. The flux in the right loop, whose area
decreases with time, is
r = (0.8)(0.2)[(16 − 2) − 9t]
and emfr = −d r/dt = (0.16)(9) = 1.44 V. The resistance of the right loop is Rr(t) =
0.3 + 2[2.2(14 − 9t)], and so the contribution to the current from the right loop will be
Ir(t) =
−1.44
61.9 − 39.6t
A
The minus sign has been inserted because again the current must flow in the opposite direction
as that indicated in the figure, with the flux decreasing with time. The total current is found by
adding the part a result, or
IT (t) = −1.44
1
61.9 − 39.6t
+
1
9.1 + 39.6t
A
10.8. Fig. 10.1 is modified to show that the rail separation is larger when y is larger. Specifically, let the
separation d = 0.2 + 0.02y. Given a uniform velocity vy = 8 m/s and a uniform magnetic flux density
Bz = 1.1 T, find V12 as a function of time if the bar is located at y = 0 at t = 0: The flux through the
loop as a function of y can be written as
= B · dS =
y
0
.2+.02y′
0
1.1 dx dy′
=
y
0
1.1(.2 + .02y′
) dy′
= 0.22y(1 + .05y)
Now, with y = vt = 8t, the above becomes = 1.76t(1 + .40t). Finally,
V12 = −
d
dt
= −1.76(1 + .80t) V
10.9. A square filamentary loop of wire is 25 cm on a side and has a resistance of 125 per meter length. The
loop lies in the z = 0 plane with its corners at (0, 0, 0), (0.25, 0, 0), (0.25, 0.25, 0), and (0, 0.25, 0) at
t = 0. The loop is moving with velocity vy = 50 m/s in the field Bz = 8 cos(1.5 × 108t − 0.5x) µT.
Develop a function of time which expresses the ohmic power being delivered to the loop: First, since
the field does not vary with y, the loop motion in the y direction does not produce any time-varying
flux, and so this motion is immaterial. We can evaluate the flux at the original loop position to obtain:
(t) =
.25
0
.25
0
8 × 10−6
cos(1.5 × 108
t − 0.5x) dx dy
= −(4 × 10−6
) sin(1.5 × 108
t − 0.13x) − sin(1.5 × 108
t) Wb
Now, emf = V (t) = −d /dt = 6.0 × 102 cos(1.5 × 108t − 0.13x) − cos(1.5 × 108t) , The total
loop resistance is R = 125(0.25 + 0.25 + 0.25 + 0.25) = 125 . Then the ohmic power is
P (t) =
V 2(t)
R
= 2.9 × 103
cos(1.5 × 108
t − 0.13x) − cos(1.5 × 108
t) Watts
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![10.19. In the first section of this chapter, Faraday’s law was used to show that the field E = −1
2 kB0ρekt aφ
results from the changing magnetic field B = B0ekt az (note that the factor of ρ appearing in E was
omitted from the original problem statement).
a) Show that these fields do not satisfy Maxwell’s other curl equation: Note that B as stated is constant
with position, and so will have zero curl. The electric field, however, varies with time, and so
∇ × H = ∂D
∂t would have a zero left-hand side and a non-zero right-hand side. The equation is
thus not valid with these fields.
b) If we let B0 = 1 T and k = 106 s−1, we are establishing a fairly large magnetic flux density in 1
µs. Use the ∇ × H equation to show that the rate at which Bz should (but does not) change with
ρ is only about 5 × 10−6 T/m in free space at t = 0: Assuming that B varies with ρ, we write
∇ × H = −
∂Hz
∂ρ
aφ = −
1
µ0
dB0
dρ
ekt
= ǫ0
∂E
∂t
= −
1
2
ǫ0k2
B0ρekt
Thus
dB0
dρ
=
1
2
µ0ǫ0k2
ρB0 =
1012(1)ρ
2(3 × 108)2
= 5.6 × 10−6
ρ
which is near the stated value if ρ is on the order of 1m.
10.20. Point C(−0.1, −0.2, 0.3) lies on the surface of a perfect conductor. The electric field intensity at C is
(500ax − 300ay + 600az) cos 107t V/m, and the medium surrounding the conductor is characterized
by µR = 5, ǫR = 10, and σ = 0.
a) Find a unit vector normal to the conductor surface at C, if the origin lies within the conductor:
At t = 0, the field must be directed out of the surface, and will be normal to it, since we have a
perfect conductor. Therefore
n =
+E(t = 0)
|E(t = 0)|
=
5ax − 3ay + 6az
√
25 + 9 + 36
= 0.60ax − 0.36ay + 0.72az
b) Find the surface charge density at C: Use
ρs = D · n|surf ace = 10ǫ0 500ax − 300ay + 600az cos(107
t) · .60ax − .36ay + .72az
= 10ǫ0 [300 + 108 + 432] cos(107
t) = 7.4 × 10−8
cos(107
t) C/m2
= 74 cos(107
t) nC/m2
10.21. The surfaces ρ = 3 and 10 mm, and z = 0 and 25 cm are perfect conductors. The region en-
closed by these surfaces has µ = 2.5 × 10−6 H/m, ǫ = 4 × 10−11 F/m, and σ = 0. Let H =
(2/ρ) cos(10πz) cos(ωt) aφ A/m. Make use of Maxwell’s equations to find
a) ω: We start with
∇ × H = −
∂Hφ
∂z
aρ =
20π
ρ
sin(10πz) cos(ωt) aρ = ǫ
∂E
∂t
We then find
E =
20π
ρǫ
sin(10πz) cos(ωt) dt aρ =
20π
ωρǫ
sin(10πz) sin(ωt) aρ
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![10.23. (continued)
These, along with the permittivities and conductivities, are substituted to obtain
(4 × 10−3
)(10) cos(109
t) − 10−3
[A cos(109
t) + B sin(109
t)]
=
∂
∂t
10−11
[A cos(109
t) + B sin(109
t)] − (2 × 10−11
)(10) cos(109
t)
= −(10−2
A sin(109
t) + 10−2
B cos(109
t) + (2 × 10−1
) sin(109
t)
We now equate coefficients of the sin and cos terms to obtain two equations:
4 × 10−2
− 10−3
A = 10−2
B
−10−3
B = −10−2
A + 2 × 10−1
These are solved together to find A = 20.2 and B = 2.0. Thus
EN2 = 20.2 cos(109
t) + 2.0 sin(109
t) az = 20.3 cos(109
t + 5.6◦
)az V/m
Then
DN2 = ǫ2EN2 = 203 cos(109
t + 5.6◦
)az pC/m2
and
JN2 = σ2EN2 = 20.3 cos(109
t + 5.6◦
)az mA/m2
10.24. Given the fields V = 80z cos x cos 3 × 108t. kV and A = 26.7z sin x sin 3 × 108t ax mWb/m in free
space, find E and H: First, find E through
E = −∇V −
∂A
∂t
where
−∇V = 80 cos(3 × 108
t)[z sin xax − cos xaz] kV/m
and
−∂A/∂t = −(3 × 108
)(26.7)z sin x cos(3 × 108
t)ax mV/m
Finally,
E = − 7.9 × 106
z sin x ax + 8.0 × 104
cos x az cos(3 × 108
t) V/m
Now
B = ∇ × A =
∂Ax
∂z
ay = 26.7 sin x sin(3 × 108
t)ay mWb/m2
Then
H =
B
µ0
= 2.12 × 104
sin x sin(3 × 108
t) ay A/m
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![10.25. In a region where µR = ǫR = 1 and σ = 0, the retarded potentials are given by V = x(z − ct) V and
A = x[(z/c) − t]az Wb/m, where c = 1/
√
µ0ǫ0.
a) Show that ∇ · A = −µǫ(∂V/∂t):
First,
∇ · A =
∂Az
∂z
=
x
c
= x
√
µ0ǫ0
Second,
∂V
∂t
= −cx = −
x
√
µ0ǫ0
so we observe that ∇ · A = −µ0ǫ0(∂V/∂t) in free space, implying that the given statement would
hold true in general media.
b) Find B, H, E, and D:
Use
B = ∇ × A = −
∂Ax
∂x
ay = t −
z
c
ay T
Then
H =
B
µ0
=
1
µ0
t −
z
c
ay A/m
Now,
E = −∇V −
∂A
∂t
= −(z − ct)ax − xaz + xaz = (ct − z)ax V/m
Then
D = ǫ0E = ǫ0(ct − z)ax C/m2
c) Show that these results satisfy Maxwell’s equations if J and ρv are zero:
i. ∇ · D = ∇ · ǫ0(ct − z)ax = 0
ii. ∇ · B = ∇ · (t − z/c)ay = 0
iii.
∇ × H = −
∂Hy
∂z
ax =
1
µ0c
ax =
ǫ0
µ0
ax
which we require to equal ∂D/∂t:
∂D
∂t
= ǫ0cax =
ǫ0
µ0
ax
iv.
∇ × E =
∂Ex
∂z
ay = −ay
which we require to equal −∂B/∂t:
∂B
∂t
= ay
So all four Maxwell equations are satisfied.
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![CHAPTER 11
11.1. Show that Exs = Aejk0z+φ is a solution to the vector Helmholtz equation, Sec. 11.1, Eq. (16), for
k0 = ω
√
µ0ǫ0 and any φ and A: We take
d2
dz2
Aejk0z+φ
= (jk0)2
Aejk0z+φ
= −k2
0Exs
11.2. Let E(z, t) = 200 sin 0.2z cos 108tax + 500 cos(0.2z + 50◦) sin 108tay V/m. Find:
a) E at P (0, 2, 0.6) at t = 25 ns: Obtain
EP (t = 25) = 200 sin [(0.2)(0.6)] cos(2.5)ax + 500 cos [(0.2)(0.6) + 50(2π)/360] sin(2.5)ay
= −19.2ax + 164ay V/m
b) |E| at P at t = 20 ns:
EP (t = 20) = 200 sin [(0.2)(0.6)] cos(2.0)ax + 500 cos [(0.2)(0.6) + 50(2π)/360] sin(2.0)ay
= −9.96ax + 248ay V/m
Thus |EP | = (9.96)2 + (248)2 = 249 V/m.
c) Es at P: Es = 200 sin 0.2zax − j500 cos(0.2z + 50◦)ay. Thus
EsP = 200 sin [(0.2)(0.6)] ax − j500 cos [(0.2)(0.6) + 2π(50)/360] ay
= 23.9ax − j273ay V/m
11.3. An H field in free space is given as H(x, t) = 10 cos(108t − βx)ay A/m. Find
a) β: Since we have a uniform plane wave, β = ω/c, where we identify ω = 108 sec−1. Thus
β = 108/(3 × 108) = 0.33 rad/m.
b) λ: We know λ = 2π/β = 18.9 m.
c) E(x, t) at P (0.1, 0.2, 0.3) at t = 1 ns: Use E(x, t) = −η0H(x, t) = −(377)(10) cos(108t −
βx) = −3.77 × 103 cos(108t − βx). The vector direction of E will be −az, since we require that
S = E × H, where S is x-directed. At the given point, the relevant coordinate is x = 0.1. Using
this, along with t = 10−9 sec, we finally obtain
E(x, t) = −3.77 × 103
cos[(108
)(10−9
) − (0.33)(0.1)]az = −3.77 × 103
cos(6.7 × 10−2
)az
= −3.76 × 103
az V/m
11.4. In phasor form, the electric field intensity of a uniform plane wave in free space is expressed as
Es = (40 − j30)e−j20zax V/m. Find:
a) ω: From the given expression, we identify β = 20 rad/m. Then ω = cβ = (3 × 108)(20) =
6.0 × 109 rad/s.
b) β = 20 rad/m from part a.
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![11.4. (continued)
c) f = ω/2π = 956 MHz.
d) λ = 2π/β = 2π/20 = 0.314 m.
e) Hs: In free space, we find Hs by dividing Es by η0, and assigning vector components such that
Es × Hs gives the required direction of wave travel: We find
Hs =
40 − j30
377
e−j20z
ay = (0.11 − j0.08)e−j20z
ay A/m
f) H(z, t) at P (6, −1, 0.07), t = 71 ps:
H(z, t) = Re Hsejωt
= 0.11 cos(6.0 × 109
t − 20z) + 0.08 sin(6.0 × 109
t − 20z) ay
Then
H(.07, t = 71ps) = 0.11 cos (6.0 × 109
)(7.1 × 10−11
) − 20(.07)
+ .08 sin (6.0 × 109
)(7.1 × 10−11
) − 20(.07) ay
= [0.11(0.562) − 0.08(0.827)]ay = −6.2 × 10−3
ay A/m
11.5. A 150-MHz uniform plane wave in free space is described by Hs = (4 + j10)(2ax + jay)e−jβz A/m.
a) Find numerical values for ω, λ, and β: First, ω = 2π × 150 × 106 = 3π × 108 sec−1. Second,
for a uniform plane wave in free space, λ = 2πc/ω = c/f = (3 × 108)/(1.5 × 108) = 2 m.
Third, β = 2π/λ = π rad/m.
b) Find H(z, t) at t = 1.5 ns, z = 20 cm: Use
H(z, t) = Re{Hsejωt
} = Re{(4 + j10)(2ax + jay)(cos(ωt − βz) + j sin(ωt − βz)}
= [8 cos(ωt − βz) − 20 sin(ωt − βz)] ax − [10 cos(ωt − βz) + 4 sin(ωt − βz)] ay
. Now at the given position and time, ωt − βz = (3π × 108)(1.5 × 10−9) − π(0.20) = π/4. And
cos(π/4) = sin(π/4) = 1/
√
2. So finally,
H(z = 20cm, t = 1.5ns) = −
1
√
2
12ax + 14ay = −8.5ax − 9.9ay A/m
c) What is |E|max? Have |E|max = η0|H|max, where
|H|max = Hs · H∗
s = [4(4 + j10)(4 − j10) + (j)(−j)(4 + j10)(4 − j10)]1/2
= 24.1 A/m
Then |E|max = 377(24.1) = 9.08 kV/m.
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![11.8. Let the fields, E(z, t) = 1800 cos(107πt − βz)ax V/m and H(z, t) = 3.8 cos(107πt − βz)ay A/m,
represent a uniform plane wave propagating at a velocity of 1.4 × 108 m/s in a perfect dielectric. Find:
a) β = ω/v = (107π)/(1.4 × 108) = 0.224 m−1.
b) λ = 2π/β = 2π/.224 = 28.0 m.
c) η = |E|/|H| = 1800/3.8 = 474 .
d) µR: Have two equations in the two unknowns, µR and ǫR: η = η0
√
µR/ǫR and β = ω
√
µRǫR/c.
Eliminate ǫR to find
µR =
βcη
ωη0
2
=
(.224)(3 × 108)(474)
(107π)(377)
2
= 2.69
e) ǫR = µR(η0/η)2 = (2.69)(377/474)2 = 1.70.
11.9. A certain lossless material has µR = 4 and ǫR = 9. A 10-MHz uniform plane wave is propagating in
the ay direction with Ex0 = 400 V/m and Ey0 = Ez0 = 0 at P (0.6, 0.6, 0.6) at t = 60 ns.
a) Find β, λ, vp, and η: For a uniform plane wave,
β = ω
√
µǫ =
ω
c
√
µRǫR =
2π × 107
3 × 108
(4)(9) = 0.4π rad/m
Then λ = (2π)/β = (2π)/(0.4π) = 5 m. Next,
vp =
ω
β
=
2π × 107
4π × 10−1
= 5 × 107
m/s
Finally,
η =
µ
ǫ
= η0
µR
ǫR
= 377
4
9
= 251
b) Find E(t) (at P ): We are given the amplitude at t = 60 ns and at y = 0.6 m. Let the maximum
amplitude be Emax, so that in general, Ex = Emax cos(ωt − βy). At the given position and time,
Ex = 400 = Emax cos[(2π × 107
)(60 × 10−9
) − (4π × 10−1
)(0.6)] = Emax cos(0.96π)
= −0.99Emax
So Emax = (400)/(−0.99) = −403 V/m. Thus at P, E(t) = −403 cos(2π × 107t) V/m.
c) Find H(t): First, we note that if E at a given instant points in the negative x direction, while the
wave propagates in the forward y direction, then H at that same position and time must point in
the positive z direction. Since we have a lossless homogeneous medium, η is real, and we are
allowed to write H(t) = E(t)/η, where η is treated as negative and real. Thus
H(t) = Hz(t) =
Ex(t)
η
=
−403
−251
cos(2π × 10−7
t) = 1.61 cos(2π × 10−7
t) A/m
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![11.12. The plane wave Es = 300e−jkxay V/m is propagating in a material for which µ = 2.25 µH/m, ǫ′ = 9
pF/m, and ǫ′′ = 7.8 pF/m. If ω = 64 Mrad/s, find:
a) α: We use the general formula, Eq. (35):
α = ω
µǫ′
2
1 +
ǫ′′
ǫ′
2
− 1
1/2
= (64 × 106
)
(2.25 × 10−6)(9 × 10−12)
2
1 + (.867)2 − 1
1/2
= 0.116 Np/m
b) β: Using (36), we write
β = ω
µǫ′
2
1 +
ǫ′′
ǫ′
2
+ 1
1/2
= .311 rad/m
c) vp = ω/β = (64 × 106)/(.311) = 2.06 × 108 m/s.
d) λ = 2π/β = 2π/(.311) = 20.2 m.
e) η: Using (39):
η =
µ
ǫ′
1
1 − j(ǫ′′/ǫ′)
=
2.25 × 10−6
9 × 10−12
1
√
1 − j(.867)
= 407 + j152 = 434.5ej.36
f) Hs: With Es in the positive y direction (at a given time) and propagating in the positive x direction,
we would have a positive z component of Hs, at the same time. We write (with jk = α + jβ):
Hs =
Es
η
az =
300
434.5ej.36
e−jkx
az = 0.69e−αx
e−jβx
e−j.36
az
= 0.69e−.116x
e−j.311x
e−j.36
az A/m
g) E(3, 2, 4, 10ns): The real instantaneous form of E will be
E(x, y, z, t) = Re Esejωt
= 300e−αx
cos(ωt − βx)ay
Therefore
E(3, 2, 4, 10ns) = 300e−.116(3)
cos[(64 × 106
)(10−8
) − .311(3)]ay = 203 V/m
11.13. Let jk = 0.2 + j1.5 m−1 and η = 450 + j60 for a uniform plane wave propagating in the az
direction. If ω = 300 Mrad/s, find µ, ǫ′, and ǫ′′: We begin with
η =
µ
ǫ′
1
1 − j(ǫ′′/ǫ′)
= 450 + j60
and
jk = jω µǫ′ 1 − j(ǫ′′/ǫ′) = 0.2 + j1.5
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![11.13. (continued) Then
ηη∗
=
µ
ǫ′
1
1 + (ǫ′′/ǫ′)2
= (450 + j60)(450 − j60) = 2.06 × 105
(1)
and
(jk)(jk)∗
= ω2
µǫ′
1 + (ǫ′′/ǫ′)2 = (0.2 + j1.5)(0.2 − j1.5) = 2.29 (2)
Taking the ratio of (2) to (1),
(jk)(jk)∗
ηη∗
= ω2
(ǫ′
)2
1 + (ǫ′′
/ǫ′
)2
=
2.29
2.06 × 105
= 1.11 × 10−5
Then with ω = 3 × 108,
(ǫ′
)2
=
1.11 × 10−5
(3 × 108)2 1 + (ǫ′′/ǫ′)2
=
1.23 × 10−22
1 + (ǫ′′/ǫ′)2
(3)
Now, we use Eqs. (35) and (36). Squaring these and taking their ratio gives
α2
β2
=
1 + (ǫ′′/ǫ′)2
1 + (ǫ′′/ǫ′)2
=
(0.2)2
(1.5)2
We solve this to find ǫ′′/ǫ′ = 0.271. Substituting this result into (3) gives ǫ′ = 1.07 × 10−11 F/m.
Since ǫ′′/ǫ′ = 0.271, we then find ǫ′′ = 2.90 × 10−12 F/m. Finally, using these results in either (1) or
(2) we find µ = 2.28 × 10−6 H/m. Summary: µ = 2.28 × 10−6 H/m,
ǫ′ = 1.07 × 10−11 F/m, and ǫ′′ = 2.90 × 10−12 F/m.
11.14. A certain nonmagnetic material has the material constants ǫ′
R = 2 and ǫ′′/ǫ′ = 4 × 10−4 at ω = 1.5
Grad/s. Find the distance a uniform plane wave can propagate through the material before:
a) it is attenuated by 1 Np: First, ǫ′′ = (4 × 104)(2)(8.854 × 10−12) = 7.1 × 10−15 F/m. Then,
since ǫ′′/ǫ′ << 1, we use the approximate form for α, given by Eq. (51) (written in terms of ǫ′′):
α
.
=
ωǫ′′
2
µ
ǫ′
=
(1.5 × 109)(7.1 × 10−15)
2
377
√
2
= 1.42 × 10−3
Np/m
The required distance is now z1 = (1.42 × 10−3)−1 = 706 m
b) the power level is reduced by one-half: The governing relation is e−2αz1/2 = 1/2, or z1/2 =
ln 2/2α = ln 2/2(1.42 × 10−3) = 244 m.
c) the phase shifts 360◦: This distance is defined as one wavelength, where λ = 2π/β
= (2πc)/(ω ǫ′
R) = [2π(3 × 108)]/[(1.5 × 109)
√
2] = 0.89 m.
11.15. A 10 GHz radar signal may be represented as a uniform plane wave in a sufficiently small region.
Calculatethewavelengthincentimetersandtheattenuationinneperspermeterifthewaveispropagating
in a non-magnetic material for which
a) ǫ′
R = 1 and ǫ′′
R = 0: In a non-magnetic material, we would have:
α = ω
µ0ǫ0ǫ′
R
2
1 +
ǫ′′
R
ǫ′
R
2
− 1
1/2
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![11.15. (continued) and
β = ω
µ0ǫ0ǫ′
R
2
1 +
ǫ′′
R
ǫ′
R
2
+ 1
1/2
With the given values of ǫ′
R and ǫ′′
R, it is clear that β = ω
√
µ0ǫ0 = ω/c, and so
λ = 2π/β = 2πc/ω = 3 × 1010/1010 = 3 cm. It is also clear that α = 0.
b) ǫ′
R = 1.04 and ǫ′′
R = 9.00 × 10−4: In this case ǫ′′
R/ǫ′
R << 1, and so β
.
= ω ǫ′
R/c = 2.13 cm−1.
Thus λ = 2π/β = 2.95 cm. Then
α
.
=
ωǫ′′
2
µ
ǫ′
=
ωǫ′′
R
2
√
µ0ǫ0
ǫ′
R
=
ω
2c
ǫ′′
R
ǫ′
R
=
2π × 1010
2 × 3 × 108
(9.00 × 10−4)
√
1.04
= 9.24 × 10−2
Np/m
c) ǫ′
R = 2.5 and ǫ′′
R = 7.2: Using the above formulas, we obtain
β =
2π × 1010
√
2.5
(3 × 1010)
√
2
1 +
7.2
2.5
2
+ 1
1/2
= 4.71 cm−1
and so λ = 2π/β = 1.33 cm. Then
α =
2π × 1010
√
2.5
(3 × 108)
√
2
1 +
7.2
2.5
2
− 1
1/2
= 335 Np/m
11.16. The power factor of a capacitor is defined as the cosine of the impedance phase angle, and its Q is
ωCR, where R is the parallel resistance. Assume an idealized parallel plate capacitor having a dielecric
characterized by σ, ǫ′, and µR. Find both the power factor and Q in terms of the loss tangent: First,
the impedance will be:
Z =
R 1
jωC
R + 1
jωC
= R
1 − jRωC
1 + (RωC)2
= R
1 − jQ
1 + Q2
Now R = d/(σA) and C = ǫ′A/d, and so Q = ωǫ′/σ = 1/l.t. Then the power factor is P.F =
cos[tan−1(−Q)] = 1/ 1 + Q2.
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![11.22. The inner and outer dimensions of a copper coaxial transmission line are 2 and 7 mm, respectively.
Both conductors have thicknesses much greater than δ. The dielectric is lossless and the operating
frequency is 400 MHz. Calculate the resistance per meter length of the:
a) inner conductor: First
δ =
1
√
πf µσ
=
1
π(4 × 108)(4π × 10−7)(5.8 × 107)
= 3.3 × 10−6
m = 3.3µm
Now, using (70) with a unit length, we find
Rin =
1
2πaσδ
=
1
2π(2 × 10−3)(5.8 × 107)(3.3 × 10−6)
= 0.42 ohms/m
b) outer conductor: Again, (70) applies but with a different conductor radius. Thus
Rout =
a
b
Rin =
2
7
(0.42) = 0.12 ohms/m
c) transmission line: Since the two resistances found above are in series, the line resistance is their
sum, or R = Rin + Rout = 0.54 ohms/m.
11.23. A hollow tubular conductor is constructed from a type of brass having a conductivity of 1.2 × 107 S/m.
The inner and outer radii are 9 mm and 10 mm respectively. Calculate the resistance per meter length
at a frequency of
a) dc: In this case the current density is uniform over the entire tube cross-section. We write:
R(dc) =
L
σA
=
1
(1.2 × 107)π(.012 − .0092)
= 1.4 × 10−3
/m
b) 20 MHz: Now the skin effect will limit the effective cross-section. At 20 MHz, the skin depth is
δ(20MHz) = [πf µ0σ]−1/2
= [π(20 × 106
)(4π × 10−7
)(1.2 × 107
)]−1/2
= 3.25 × 10−5
m
This is much less than the outer radius of the tube. Therefore we can approximate the resistance
using the formula:
R(20MHz) =
L
σA
=
1
2πbδ
=
1
(1.2 × 107)(2π(.01))(3.25 × 10−5)
= 4.1 × 10−2
/m
c) 2 GHz: Using the same formula as in part b, we find the skin depth at 2 GHz to be δ = 3.25×10−6
m. The resistance (using the other formula) is R(2GHz) = 4.1 × 10−1 /m.
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![11.32. Suppose that the length of the medium of Problem 11.31 is made to be twice that as determined in
the problem. Describe the polarization of the output wave in this case: With the length doubled, a
phase shift of π radians develops between the two components. At the input, we can write the field as
Es(0) = E0(ax + ay). After propagating through length L, we would have,
Es(L) = E0[e−jβxL
ax + e−jβyL
ay] = E0e−jβxL
[ax + e−j(βy−βx)L
ay]
where (βy − βx)L = −π (since βx > βy), and so Es(L) = E0e−jβxL[ax − ay]. With the reversal of
the y component, the wave polarization is rotated by 90◦, but is still linear polarization.
11.33. Given a wave for which Es = 15e−jβzax +18e−jβzejφay V/m, propagating in a medium characterized
by complex intrinsic impedance, η.
a) Find Hs: With the wave propagating in the forward z direction, we find:
Hs =
1
η
−18ejφ
ax + 15ay e−jβz
A/m
b) Determine the average power density in W/m2: We find
Pz,avg =
1
2
Re Es × H∗
s =
1
2
Re
(15)2
η∗
+
(18)2
η∗
= 275 Re
1
η∗
W/m2
11.34. Given the general elliptically-polarized wave as per Eq. (73):
Es = [Ex0ax + Ey0ejφ
ay]e−jβz
a) Show, using methods similar to those of Example 11.7, that a linearly polarized wave results when
superimposing the given field and a phase-shifted field of the form:
Es = [Ex0ax + Ey0e−jφ
ay]e−jβz
ejδ
where δ is a constant: Adding the two fields gives
Es,tot = Ex0 1 + ejδ
ax + Ey0 ejφ
+ e−jφ
ejδ
ay e−jβz
=
Ex0ejδ/2
e−jδ/2
+ ejδ/2
2 cos(δ/2)
ax + Ey0ejδ/2
e−jδ/2
ejφ
+ e−jφ
ejδ/2
2 cos(φ−δ/2)
ay
e−jβz
This simplifies to Es,tot = 2 Ex0 cos(δ/2)ax + Ey0 cos(φ − δ/2)ay ejδ/2e−jβz, which is lin-
early polarized.
b) Find δ in terms of φ such that the resultant wave is polarized along x: By inspecting the part a
result, we achieve a zero y component when 2φ − δ = π (or odd multiples of π).
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![12.11. (continued) So we now have
Ŵ = 0.5ej0.2π
=
ηu − η0
ηu + η0
We solve for ηu to find
ηu = η0(1.70 + j1.33) = 641 + j501
12.12. A 50MHz uniform plane wave is normally incident from air onto the surface of a calm ocean. For
seawater, σ = 4 S/m, and ǫ′
R = 78.
a) Determine the fractions of the incident power that are reflected and transmitted: First we find the
loss tangent:
σ
ωǫ′
=
4
2π(50 × 106)(78)(8.854 × 10−12)
= 18.4
This value is sufficiently greater than 1 to enable seawater to be considered a good conductor
at 50MHz. Then, using the approximation (Eq. 65, Chapter 11), the intrinsic impedance is
ηs =
√
πf µ/σ(1 + j), and the reflection coefficient becomes
Ŵ =
√
πf µ/σ (1 + j) − η0
√
πf µ/σ (1 + j) + η0
where
√
πf µ/σ = π(50 × 106)(4π × 10−7)/4 = 7.0. The fraction of the power reflected is
Pr
Pi
= |Ŵ|2
=
[
√
πf µ/σ − η0]2 + πf µ/σ
[
√
πf µ/σ + η0]2 + πf µ/σ
=
[7.0 − 377]2 + 49.0
[7.0 + 377]2 + 49.0
= 0.93
The transmitted fraction is then
Pt
Pi
= 1 − |Ŵ|2
= 1 − 0.93 = 0.07
b) Qualitatively, how will these answers change (if at all) as the frequency is increased? Within
the limits of our good conductor approximation (loss tangent greater than about ten), the reflected
power fraction, using the formula derived in part a, is found to decrease with increasing frequency.
The transmitted power fraction thus increases.
12.13. A right-circularly-polarized plane wave is normally incident from air onto a semi-infinite slab of plex-
iglas (ǫ′
R = 3.45, ǫ′′
R = 0). Calculate the fractions of the incident power that are reflected and trans-
mitted. Also, describe the polarizations of the reflected and transmitted waves. First, the impedance of
the plexiglas will be η = η0/
√
3.45 = 203 . Then
Ŵ =
203 − 377
203 + 377
= −0.30
The reflected power fraction is thus |Ŵ|2 = 0.09. The total electric field in the plane of the interface
must rotate in the same direction as the incident field, in order to continually satisfy the boundary
condition of tangential electric field continuity across the interface. Therefore, the reflected wave will
have to be left circularly polarized in order to make this happen. The transmitted power fraction is now
1 − |Ŵ|2 = 0.91. The transmitted field will be right circularly polarized (as the incident field) for the
same reasons.
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![12.28. Over a certain frequency range, the refractive index of a certain material varies approximately linearly
with frequency: n(ω)
.
= na + nb(ω − ωa), where na, nb, and ωa are constants. Using β = nω/c:
a) determine the group velocity as a function (or perhaps not a function) of frequency:
vg = (dβ/dω)−1, where
dβ
dω
=
d
dω
naω
c
+
nb(ω − ωa)ω
c
=
1
c
[na + nb(2ω − ωa)]
so that
vg(ω) = c [na + nb(2ω − ωa)]−1
b) determine the group dispersion parameter, β2:
β2 =
d2β
dω2 ω0
=
d
dω
1
c
[na + nb(2ω − ωa)]
ω0
= 2nb/c
c) Discuss the implications of these results, if any, on pulse broadening: The point of this problem was
to show that higher order terms (involving d3β/dω3 and higher) in the Taylor series expansion,
Eq. (89), do not exist if the refractive index varies linearly with ω. These higher order terms
would be necessary in cases involving pulses of exremely large bandwidth, or in media exhibiting
complicated variations in their ω-β curves over relatively small frequency ranges. With d2β/dω2
constant, the three-term Taylor expansion of Eq. (89) describes the phase constant of this medium
exactly. The pulse will broaden and will acquire a frequency sweep (chirp) that is precisely linear
with time. Additionally, a pulse of a given bandwidth will broaden by the same amount, regardless
of what carrier frequency is used.
12.29. A T = 5 ps transform-limited pulse propagates in a dispersive channel for which β2 = 10 ps2/km.
Over what distance will the pulse spread to twice its initial width? After propagation, the width is
T ′ = T 2 + ( τ)2 = 2T . Thus τ =
√
3T , where τ = β2z/T . Therefore
β2z
T
=
√
3T or z =
√
3T 2
β2
=
√
3(5 ps)2
10 ps2/km
= 4.3 km
12.30. A T = 20 ps transform-limited pulse propagates through 10 km of a dispersive channel for which β2 =
12 ps2/km. The pulse then propagates through a second 10 km channel for which β2 = −12 ps2/km.
Describe the pulse at the output of the second channel and give a physical explanation for what hap-
pened.
Our theory of pulse spreading will allow for changes in β2 down the length of the channel. In fact, we
may write in general:
τ =
1
T
L
0
β2(z) dz
Having β2 change sign at the midpoint, yields a zero τ, and so the pulse emerges from the output
unchanged! Physically, the pulse acquires a positive linear chirp (frequency increases with time over
the pulse envelope) during the first half of the channel. When β2 switches sign, the pulse begins to
acquire a negative chirp in the second half, which, over an equal distance, will completely eliminate
the chirp acquired during the first half. The pulse, if originally transform-limited at input, will emerge,
again transform-limited, at its original width. More generally, complete dispersion compensation is
achieved using a two-segment channel when β2L = −β′
2L′, assuming dispersion terms of higher order
than β2 do not exist.
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![CHAPTER 13
13.1. The parameters of a certain transmission line operating at 6 × 108 rad/s are L = 0.4 µH/m, C =
40 pF/m, G = 80 mS/m, and R = 20 /m.
a) Find γ , α, β, λ, and Z0: We use
γ =
√
ZY = (R + jωL)(G + jωC)
= [20 + j(6 × 108)(0.4 × 10−6)][80 × 10−3 + j(6 × 108)(40 × 10−12)]
= 2.8 + j3.5 m−1
= α + jβ
Therefore, α = 2.8 Np/m, β = 3.5 rad/m, and λ = 2π/β = 1.8 m. Finally,
Z0 =
Z
Y
=
R + jωL
G + jωC
=
20 + j2.4 × 102
80 × 10−3 + j2.4 × 10−2
= 44 + j30
b) If a voltage wave travels 20 m down the line, what percentage of the original amplitude remains,
and by how many degrees is it phase shifted? First,
V20
V0
= e−αL
= e−(2.8)(20)
= 4.8 × 10−25
or 4.8 × 10−23
percent!
Then the phase shift is given by βL, which in degrees becomes
φ = βL
360
2π
= (3.5)(20)
360
2π
= 4.0 × 103
degrees
13.2. A lossless transmission line with Z0 = 60 is being operated at 60 MHz. The velocity on the line is
3 × 108 m/s. If the line is short-circuited at z = 0, find Zin at:
a) z = −1m: We use the expression for input impedance (Eq. 12), under the conditions Z2 = 60
and Z3 = 0:
Zin = Z2
Z3 cos(βl) + jZ2 sin(βl)
Z2 cos(βl) + jZ3 sin(βl)
= j60 tan(βl)
where l = −z, and where the phase constant is β = 2πc/f = 2π(3 × 108)/(6 × 107) =
(2/5)π rad/m. Now, with z = −1 (l = 1), we find Zin = j60 tan(2π/5) = j184.6 .
b) z = −2 m: Zin = j60 tan(4π/5) = −j43.6
c) z = −2.5 m: Zin = j60 tan(5π/5) = 0
d) z = −1.25 m: Zin = j60 tan(π/2) = j∞ (open circuit)
13.3. The characteristic impedance of a certain lossless transmission line is 72 . If L = 0.5 µH/m, find:
a) C: Use Z0 =
√
L/C, or
C =
L
Z2
0
=
5 × 10−7
(72)2
= 9.6 × 10−11
F/m = 96 pF/m
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![13.3b) vp:
vp =
1
√
LC
=
1
(5 × 10−7)(9.6 × 10−11)
= 1.44 × 108
m/s
c) β if f = 80 MHz:
β = ω
√
LC =
2π × 80 × 106
1.44 × 108
= 3.5 rad/m
d) The line is terminated with a load of 60 . Find Ŵ and s:
Ŵ =
60 − 72
60 + 72
= −0.09 s =
1 + |Ŵ|
1 − |Ŵ|
=
1 + .09
1 − .09
= 1.2
13.4. A lossless transmission line having Z0 = 120 is operating at ω = 5 × 108 rad/s. If the velocity on
the line is 2.4 × 108 m/s, find:
a) L: With Z0 =
√
L/C and v = 1/
√
LC, we find L = Z0/v = 120/2.4 × 108 = 0.50 µH/m.
b) C: Use Z0v =
√
L/C/
√
LC ⇒ C = 1/(Z0v) = [120(2.4 × 108)]−1 = 35 pF/m.
c) Let ZL be represented by an inductance of 0.6 µH in series with a 100- resistance. Find Ŵ and
s: The inductive impedance is jωL = j(5 × 108)(0.6 × 10−6) = j300. So the load impedance
is ZL = 100 + j300 . Now
Ŵ =
ZL − Z0
ZL + Z0
=
100 + j300 − 120
100 + j300 + 120
= 0.62 + j0.52 = 0.808 40◦
Then
s =
1 + |Ŵ|
1 − |Ŵ|
=
1 + 0.808
1 − 0.808
= 9.4
13.5. Two characteristics of a certain lossless transmission line are Z0 = 50 and γ = 0 + j0.2π m−1 at
f = 60 MHz.
a) Find L and C for the line: We have β = 0.2π = ω
√
LC and Z0 = 50 =
√
L/C. Thus
β
Z0
= ωC ⇒ C =
β
ωZ0
=
0.2π
(2π × 60 × 106)(50)
=
1
3
× 1010
= 33.3 pF/m
Then L = CZ2
0 = (33.3 × 10−12)(50)2 = 8.33 × 10−8 H/m = 83.3 nH/m.
b) A load, ZL = 60 + j80 is located at z = 0. What is the shortest distance from the load to a
point at which Zin = Rin + j0? I will do this using two different methods:
The Hard Way: We use the general expression
Zin = Z0
ZL + jZ0 tan(βl)
Z0 + jZL tan(βl)
We can then normalize the impedances with respect to Z0 and write
zin =
Zin
Z0
=
(ZL/Z0) + j tan(βl)
1 + j(ZL/Z0) tan(βl)
=
zL + j tan(βl)
1 + jzL tan(βl)
where zL = (60 + j80)/50 = 1.2 + j1.6.
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![13.5b. (continued) Using this, and defining x = tan(βl), we find
zin =
1.2 + j(1.6 + x)
(1 − 1.6x) + j1.2x
(1 − 1.6x) − j1.2x
(1 − 1.6x) − j1.2x
The second bracketed term is a factor of one, composed of the complex conjugate of the denomi-
nator of the first term, divided by itself. Carrying out this product, we find
zin =
1.2(1 − 1.6x) + 1.2x(1.6 + x) − j[(1.2)2x − (1.6 + x)(1 − 1.6x)]
(1 − 1.6x)2 + (1.2)2x2
We require the imaginary part to be zero. Thus
(1.2)2
x − (1.6 + x)(1 − 1.6x) = 0 ⇒ 1.6x2
+ 3x − 1.6 = 0
So
x = tan(βl) =
−3 ± 9 + 4(1.6)2
2(1.6)
= (.433, −2.31)
We take the positive root, and find
βl = tan−1
(.433) = 0.409 ⇒ l =
0.409
0.2π
= 0.65 m = 65 cm
The Easy Way: We find
Ŵ =
60 + j80 − 50
60 + j80 + 50
= 0.405 + j0.432 = 0.59 0.818
Thus φ = 0.818 rad, and we use the fact that the input impedance will be purely real at the location
of a voltage minimum or maximum. The first voltage maximum will occur at a distance in front
of the load given by
zmax =
φ
2β
=
0.818
2(0.2π)
= 0.65 m
13.6. The propagation constant of a lossy transmission line is 1 + j2 m−1, and its characteristic impedance
is 20 + j0 at ω = 1 Mrad/s. Find L, C, R, and G for the line: Begin with
Z0 =
R + jωL
G + jωL
= 20 ⇒ R + jωL = 400(G + jωC) (1)
Then
γ 2
= (R + jωL)(G + jωC) = (1 + j2)2
⇒ 400(G + jωC)2
= (1 + j2)2
(2)
where (1) has been used. Eq. 2 now becomes G + jωC = (1 + j2)/20. Equating real and imaginary
parts leads to G = .05 S/m and C = 1/(10ω) = 10−7 = 0.1 µF/m.
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![13.32. A lossless line is operating with Z0 = 40 , f = 20 MHz, and β = 7.5π rad/m. With a short circuit
replacing the load, a minimum is found at a point on the line marked by a small spot of puce paint.
With the load installed, it is found that s = 1.5 and a voltage minimum is located 1m toward the source
from the puce dot.
a) Find ZL: First, the wavelength is given by λ = 2π/β = 2/7.5 = 0.2667m. The 1m distance
is therefore 3.75λ. With the short installed, the Vmin positions will be at multiples of λ/2 to the
left of the short. Therefore, with the actual load installed, the Vmin position as stated would be
3.75λ + nλ/2, which means that a maximum voltage occurs at the load. This being the case, the
normalized load impedance will lie on the positive real axis of the Smith chart, and will be equal
to the standing wave ratio. Therefore, ZL = 40(1.5) = 60 .
b) What load would produce s = 1.5 with |V |max at the paint spot? With |V |max at the paint spot
and with the spot an integer multiple of λ/2 to the left of the load, |V |max must also occur at the
load. The answer is therefore the same as part a, or ZL = 60 .
13.33. In Fig. 13.14, let ZL = 40 − j10 , Z0 = 50 , f = 800 MHz, and v = c.
a) Find the shortest length, d1, of a short-circuited stub, and the shortest distance d that it may be
located from the load to provide a perfect match on the main line to the left of the stub: The Smith
chart construction is shown on the next page. First we find zL = (40 − j10)/50 = 0.8 − j0.2
and plot it on the chart. Next, we find yL = 1/zL by transforming this point halfway around the
chart, where we read yL = 1.17+j0.30. This point is to be transformed to a location at which the
real part of the normalized admittance is unity. The g = 1 circle is highlighted on the chart; yL
transforms to two locations on it: yin1 = 1 − j0.32 and yin2 = 1 + j0.32. The stub is connected
at either of these two points. The stub input admittance must cancel the imaginary part of the line
admittance at that point. If yin2 is chosen, the stub must have input admittance of −j0.32. This
point is marked on the outer circle and occurs at 0.452 λ on the WTG scale. The length of the stub
is found by computing the distance between its input, found above, and the short-circuit position
(stub load end), marked as Psc. This distance is d1 = (0.452−0.250)λ = 0.202 λ. With f = 800
MHz and v = c, the wavelength is λ = (3×108)/(8×108) = 0.375 m. The distance is thus d1 =
(0.202)(0.375) = 0.758 m = 7.6 cm. This is the shortest of the two possible stub lengths, since
if we had used yin1, we would have needed a stub input admittance of +j0.32, which would have
required a longer stub length to realize. The length of the main line between its load and the stub
attachment point is found on the chart by measuring the distance between yL and yin2, in moving
clockwise (toward generator). This distance will be d = [0.500 − (0.178 − 0.138)] λ = 0.46 λ.
The actual length is then d = (0.46)(0.375) = 0.173m = 17.3 cm.
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![14.21a. (continued)
Dividing by the magnitude, (0.608)2 + (0.330)2 = 0.692, we obtain the unit vector at t = 0:
aN (0) = −0.879ar + 0.477aθ . We next convert this to cartesian components:
aNx = aN (0) · ax = −0.879 sin θ cos φ + 0.477 cos θ cos φ =
1
√
2
(−0.879 + 0.477) = −0.284
aNy = aN (0) · ay = −0.879 sin θ sin φ + 0.477 cos θ sin φ = 0 since φ = 0
aNz = aN (0) · az = −0.879 cos θ − 0.477 sin θ =
1
√
2
(−0.879 − 0.477) = −0.959
The final result is then
aN (0) = −0.284ax − 0.959az
b) What fraction of the total average power is radiated in the belt, 80◦ < θ < 100◦? We use the
far-zone phasor fields, (84) and (85), and first find the average power density:
Pavg =
1
2
Re[EθsH∗
φs] =
I2
0 d2η
8λ2r2
sin2
θ W/m2
We integrate this over the given belt, an at radius r:
Pbelt =
2π
0
100◦
80◦
I2
0 d2η
8λ2r2
sin2
θ r2
sin θ dθ dφ =
πI2
0 d2η
4λ2
100◦
80◦
sin3
θ dθ
Evaluating the integral, we find
Pbelt =
πI2
0 d2η
4λ2
−
1
3
cos θ sin2
θ + 2
100
80
= (0.344)
πI2
0 d2η
4λ2
The total power is found by performing the same integral over θ, where 0 < θ < 180◦. Doing
this, it is found that
Ptot = (1.333)
πI2
0 d2η
4λ2
The fraction of the total power in the belt is then f = 0.344/1.333 = 0.258.
14.22. Prepare a curve, r vs. θ in polar coordinates, showing the locus in the φ = 0 plane where:
a) the radiation field |Eθs| is one-half of its value at r = 104 m, θ = π/2: Assuming the far field
approximation, we use (84) to set up the equation:
|Eθs| =
I0dη
2λr
sin θ =
1
2
×
I0dη
2 × 104λ
⇒ r = 2 × 104
sin θ
b) the average radiated power density, Pr,av, is one-half of its value at r = 104 m, θ = π/2. To find
the average power, we use (84) and (85) in
Pr,av =
1
2
Re{EθsH∗
φs} =
1
2
I2
0 d2η
4λ2r2
sin2
θ =
1
2
×
1
2
I2
0 d2η
4λ2(108)
⇒ r =
√
2 × 104
sin θ
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 = −(1.24 × 10−2)(ay + az) V/m.
e) Find |E| at (1000, 0, 0) at t = 0: Taking the magnitude of the part d result, we find |E| =
1.75 × 10−2 V/m.
257
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Solucionario teoria-electromagnetica-hayt-2001
- 1. StuDocu no está patrocinado ni avalado por ningún colegio o universidad. solucionario teoria electromagnetica -hayt (2001 ) Electromagnetismo (Universidad de Costa Rica) StuDocu no está patrocinado ni avalado por ningún colegio o universidad. solucionario teoria electromagnetica -hayt (2001 ) Electromagnetismo (Universidad de Costa Rica) Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 2. http://www. .com Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 3. CHAPTER 1 1.1. Given the vectors M = −10ax + 4ay − 8az and N = 8ax + 7ay − 2az, find: a) a unit vector in the direction of −M + 2N. −M + 2N = 10ax − 4ay + 8az + 16ax + 14ay − 4az = (26, 10, 4) Thus a = (26, 10, 4) |(26, 10, 4)| = (0.92, 0.36, 0.14) b) the magnitude of 5ax + N − 3M: (5, 0, 0) + (8, 7, −2) − (−30, 12, −24) = (43, −5, 22), and |(43, −5, 22)| = 48.6. c) |M||2N|(M + N): |(−10, 4, −8)||(16, 14, −4)|(−2, 11, −10) = (13.4)(21.6)(−2, 11, −10) = (−580.5, 3193, −2902) 1.2. Given three points, A(4, 3, 2), B(−2, 0, 5), and C(7, −2, 1): a) Specify the vector A extending from the origin to the point A. A = (4, 3, 2) = 4ax + 3ay + 2az b) Give a unit vector extending from the origin to the midpoint of line AB. The vector from the origin to the midpoint is given by M = (1/2)(A + B) = (1/2)(4 − 2, 3 + 0, 2 + 5) = (1, 1.5, 3.5) The unit vector will be m = (1, 1.5, 3.5) |(1, 1.5, 3.5)| = (0.25, 0.38, 0.89) c) Calculate the length of the perimeter of triangle ABC: Begin with AB = (−6, −3, 3), BC = (9, −2, −4), CA = (3, −5, −1). Then |AB| + |BC| + |CA| = 7.35 + 10.05 + 5.91 = 23.32 1.3. The vector from the origin to the point A is given as (6, −2, −4), and the unit vector directed from the origin toward point B is (2, −2, 1)/3. If points A and B are ten units apart, find the coordinates of point B. With A = (6, −2, −4) and B = 1 3 B(2, −2, 1), we use the fact that |B − A| = 10, or |(6 − 2 3 B)ax − (2 − 2 3 B)ay − (4 + 1 3 B)az| = 10 Expanding, obtain 36 − 8B + 4 9 B2 + 4 − 8 3 B + 4 9 B2 + 16 + 8 3 B + 1 9 B2 = 100 or B2 − 8B − 44 = 0. Thus B = 8± √ 64−176 2 = 11.75 (taking positive option) and so B = 2 3 (11.75)ax − 2 3 (11.75)ay + 1 3 (11.75)az = 7.83ax − 7.83ay + 3.92az 1 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 4. 1.4. given points A(8, −5, 4) and B(−2, 3, 2), find: a) the distance from A to B. |B − A| = |(−10, 8, −2)| = 12.96 b) a unit vector directed from A towards B. This is found through aAB = B − A |B − A| = (−0.77, 0.62, −0.15) c) a unit vector directed from the origin to the midpoint of the line AB. a0M = (A + B)/2 |(A + B)/2| = (3, −1, 3) √ 19 = (0.69, −0.23, 0.69) d) the coordinates of the point on the line connecting A to B at which the line intersects the plane z = 3. Note that the midpoint, (3, −1, 3), as determined from part c happens to have z coordinate of 3. This is the point we are looking for. 1.5. A vector field is specified as G = 24xyax + 12(x2 + 2)ay + 18z2az. Given two points, P (1, 2, −1) and Q(−2, 1, 3), find: a) G at P : G(1, 2, −1) = (48, 36, 18) b) a unit vector in the direction of G at Q: G(−2, 1, 3) = (−48, 72, 162), so aG = (−48, 72, 162) |(−48, 72, 162)| = (−0.26, 0.39, 0.88) c) a unit vector directed from Q toward P : aQP = P − Q |P − Q| = (3, −1, 4) √ 26 = (0.59, 0.20, −0.78) d) the equation of the surface on which |G| = 60: We write 60 = |(24xy, 12(x2 + 2), 18z2)|, or 10 = |(4xy, 2x2 + 4, 3z2)|, so the equation is 100 = 16x2 y2 + 4x4 + 16x2 + 16 + 9z4 2 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 5. 1.6. For the G field in Problem 1.5, make sketches of Gx, Gy, Gz and |G| along the line y = 1, z = 1, for 0 ≤ x ≤ 2. We find G(x, 1, 1) = (24x, 12x2 + 24, 18), from which Gx = 24x, Gy = 12x2 + 24, Gz = 18, and |G| = 6 √ 4x4 + 32x2 + 25. Plots are shown below. 1.7. Given the vector field E = 4zy2 cos 2xax + 2zy sin 2xay + y2 sin 2xaz for the region |x|, |y|, and |z| less than 2, find: a) the surfaces on which Ey = 0. With Ey = 2zy sin 2x = 0, the surfaces are 1) the plane z = 0, with |x| < 2, |y| < 2; 2) the plane y = 0, with |x| < 2, |z| < 2; 3) the plane x = 0, with |y| < 2, |z| < 2; 4) the plane x = π/2, with |y| < 2, |z| < 2. b) the region in which Ey = Ez: This occurs when 2zy sin 2x = y2 sin 2x, or on the plane 2z = y, with |x| < 2, |y| < 2, |z| < 1. c) the region in which E = 0: We would have Ex = Ey = Ez = 0, or zy2 cos 2x = zy sin 2x = y2 sin 2x = 0. This condition is met on the plane y = 0, with |x| < 2, |z| < 2. 1.8. Two vector fields are F = −10ax +20x(y −1)ay and G = 2x2yax −4ay +zaz. For the point P (2, 3, −4), find: a) |F|: F at (2, 3, −4) = (−10, 80, 0), so |F| = 80.6. b) |G|: G at (2, 3, −4) = (24, −4, −4), so |G| = 24.7. c) a unit vector in the direction of F − G: F − G = (−10, 80, 0) − (24, −4, −4) = (−34, 84, 4). So a = F − G |F − G| = (−34, 84, 4) 90.7 = (−0.37, 0.92, 0.04) d) a unit vector in the direction of F + G: F + G = (−10, 80, 0) + (24, −4, −4) = (14, 76, −4). So a = F + G |F + G| = (14, 76, −4) 77.4 = (0.18, 0.98, −0.05) 3 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 6. 1.9. A field is given as G = 25 (x2 + y2) (xax + yay) Find: a) a unit vector in the direction of G at P (3, 4, −2): Have Gp = 25/(9 + 16) × (3, 4, 0) = 3ax + 4ay, and |Gp| = 5. Thus aG = (0.6, 0.8, 0). b) the angle between G and ax at P : The angle is found through aG · ax = cos θ. So cos θ = (0.6, 0.8, 0) · (1, 0, 0) = 0.6. Thus θ = 53◦. c) the value of the following double integral on the plane y = 7: 4 0 2 0 G · aydzdx 4 0 2 0 25 x2 + y2 (xax + yay) · aydzdx = 4 0 2 0 25 x2 + 49 × 7 dzdx = 4 0 350 x2 + 49 dx = 350 × 1 7 tan−1 4 7 − 0 = 26 1.10. Use the definition of the dot product to find the interior angles at A and B of the triangle defined by the three points A(1, 3, −2), B(−2, 4, 5), and C(0, −2, 1): a) Use RAB = (−3, 1, 7) and RAC = (−1, −5, 3) to form RAB · RAC = |RAB||RAC| cos θA. Obtain 3 + 5 + 21 = √ 59 √ 35 cos θA. Solve to find θA = 65.3◦. b) Use RBA = (3, −1, −7) and RBC = (2, −6, −4) to form RBA · RBC = |RBA||RBC| cos θB. Obtain 6 + 6 + 28 = √ 59 √ 56 cos θB. Solve to find θB = 45.9◦. 1.11. Given the points M(0.1, −0.2, −0.1), N(−0.2, 0.1, 0.3), and P (0.4, 0, 0.1), find: a) the vector RMN : RMN = (−0.2, 0.1, 0.3) − (0.1, −0.2, −0.1) = (−0.3, 0.3, 0.4). b) the dot product RMN · RMP : RMP = (0.4, 0, 0.1) − (0.1, −0.2, −0.1) = (0.3, 0.2, 0.2). RMN · RMP = (−0.3, 0.3, 0.4) · (0.3, 0.2, 0.2) = −0.09 + 0.06 + 0.08 = 0.05. c) the scalar projection of RMN on RMP : RMN · aRMP = (−0.3, 0.3, 0.4) · (0.3, 0.2, 0.2) √ 0.09 + 0.04 + 0.04 = 0.05 √ 0.17 = 0.12 d) the angle between RMN and RMP : θM = cos−1 RMN · RMP |RMN ||RMP | = cos−1 0.05 √ 0.34 √ 0.17 = 78◦ 4 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 7. 1.12. Given points A(10, 12, −6), B(16, 8, −2), C(8, 1, −4), and D(−2, −5, 8), determine: a) the vector projection of RAB + RBC on RAD: RAB + RBC = RAC = (8, 1, 4) − (10, 12, −6) = (−2, −11, 10) Then RAD = (−2, −5, 8) − (10, 12, −6) = (−12, −17, 14). So the projection will be: (RAC · aRAD)aRAD = (−2, −11, 10) · (−12, −17, 14) √ 629 (−12, −17, 14) √ 629 = (−6.7, −9.5, 7.8) b) the vector projection of RAB + RBC on RDC: RDC = (8, −1, 4) − (−2, −5, 8) = (10, 6, −4). The projection is: (RAC · aRDC)aRDC = (−2, −11, 10) · (10, 6, −4) √ 152 (10, 6, −4) √ 152 = (−8.3, −5.0, 3.3) c) the angle between RDA and RDC: Use RDA = −RAD = (12, 17, −14) and RDC = (10, 6, −4). The angle is found through the dot product of the associated unit vectors, or: θD = cos−1 (aRDA · aRDC) = cos−1 (12, 17, −14) · (10, 6, −4) √ 629 √ 152 = 26◦ 1.13. a) Find the vector component of F = (10, −6, 5) that is parallel to G = (0.1, 0.2, 0.3): F||G = F · G |G|2 G = (10, −6, 5) · (0.1, 0.2, 0.3) 0.01 + 0.04 + 0.09 (0.1, 0.2, 0.3) = (0.93, 1.86, 2.79) b) Find the vector component of F that is perpendicular to G: FpG = F − F||G = (10, −6, 5) − (0.93, 1.86, 2.79) = (9.07, −7.86, 2.21) c) Find the vector component of G that is perpendicular to F: GpF = G−G||F = G− G · F |F|2 F = (0.1, 0.2, 0.3)− 1.3 100 + 36 + 25 (10, −6, 5) = (0.02, 0.25, 0.26) 1.14. The four vertices of a regular tetrahedron are located at O(0, 0, 0), A(0, 1, 0), B(0.5 √ 3, 0.5, 0), and C( √ 3/6, 0.5, √ 2/3). a) Find a unit vector perpendicular (outward) to the face ABC: First find RBA × RBC = [(0, 1, 0) − (0.5 √ 3, 0.5, 0)] × [( √ 3/6, 0.5, 2/3) − (0.5 √ 3, 0.5, 0)] = (−0.5 √ 3, 0.5, 0) × (− √ 3/3, 0, 2/3) = (0.41, 0.71, 0.29) The required unit vector will then be: RBA × RBC |RBA × RBC| = (0.47, 0.82, 0.33) b) Find the area of the face ABC: Area = 1 2 |RBA × RBC| = 0.43 5 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 8. 1.15. Three vectors extending from the origin are given as r1 = (7, 3, −2), r2 = (−2, 7, −3), and r3 = (0, 2, 3). Find: a) a unit vector perpendicular to both r1 and r2: ap12 = r1 × r2 |r1 × r2| = (5, 25, 55) 60.6 = (0.08, 0.41, 0.91) b) a unit vector perpendicular to the vectors r1 − r2 and r2 − r3: r1 − r2 = (9, −4, 1) and r2 − r3 = (−2, 5, −6). So r1 − r2 × r2 − r3 = (19, 52, 32). Then ap = (19, 52, 32) |(19, 52, 32)| = (19, 52, 32) 63.95 = (0.30, 0.81, 0.50) c) the area of the triangle defined by r1 and r2: Area = 1 2 |r1 × r2| = 30.3 d) the area of the triangle defined by the heads of r1, r2, and r3: Area = 1 2 |(r2 − r1) × (r2 − r3)| = 1 2 |(−9, 4, −1) × (−2, 5, −6)| = 32.0 1.16. Describe the surfaces defined by the equations: a) r · ax = 2, where r = (x, y, z): This will be the plane x = 2. b) |r × ax| = 2: r × ax = (0, z, −y), and |r × ax| = z2 + y2 = 2. This is the equation of a cylinder, centered on the x axis, and of radius 2. 1.17. Point A(−4, 2, 5) and the two vectors, RAM = (20, 18, −10) and RAN = (−10, 8, 15), define a triangle. a) Find a unit vector perpendicular to the triangle: Use ap = RAM × RAN |RAM × RAN | = (350, −200, 340) 527.35 = (0.664, −0.379, 0.645) The vector in the opposite direction to this one is also a valid answer. b) Find a unit vector in the plane of the triangle and perpendicular to RAN : aAN = (−10, 8, 15) √ 389 = (−0.507, 0.406, 0.761) Then apAN = ap × aAN = (0.664, −0.379, 0.645) × (−0.507, 0.406, 0.761) = (−0.550, −0.832, 0.077) The vector in the opposite direction to this one is also a valid answer. c) Find a unit vector in the plane of the triangle that bisects the interior angle at A: A non-unit vector in the required direction is (1/2)(aAM + aAN ), where aAM = (20, 18, −10) |(20, 18, −10)| = (0.697, 0.627, −0.348) 6 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 9. 1.17c. (continued) Now 1 2 (aAM + aAN ) = 1 2 [(0.697, 0.627, −0.348) + (−0.507, 0.406, 0.761)] = (0.095, 0.516, 0.207) Finally, abis = (0.095, 0.516, 0.207) |(0.095, 0.516, 0.207)| = (0.168, 0.915, 0.367) 1.18. Given points A(ρ = 5, φ = 70◦, z = −3) and B(ρ = 2, φ = −30◦, z = 1), find: a) unit vector in cartesian coordinates at A toward B: A(5 cos 70◦, 5 sin 70◦, −3) = A(1.71, 4.70, −3), In the same manner, B(1.73, −1, 1). So RAB = (1.73, −1, 1) − (1.71, 4.70, −3) = (0.02, −5.70, 4) and therefore aAB = (0.02, −5.70, 4) |(0.02, −5.70, 4)| = (0.003, −0.82, 0.57) b) a vector in cylindrical coordinates at A directed toward B: aAB · aρ = 0.003 cos 70◦ − 0.82 sin 70◦ = −0.77. aAB · aφ = −0.003 sin 70◦ − 0.82 cos 70◦ = −0.28. Thus aAB = −0.77aρ − 0.28aφ + 0.57az . c) a unit vector in cylindrical coordinates at B directed toward A: Use aBA = (−0, 003, 0.82, −0.57). Then aBA ·aρ = −0.003 cos(−30◦)+0.82 sin(−30◦) = −0.43, and aBA · aφ = 0.003 sin(−30◦) + 0.82 cos(−30◦) = 0.71. Finally, aBA = −0.43aρ + 0.71aφ − 0.57az 1.19 a) Express the field D = (x2 + y2)−1(xax + yay) in cylindrical components and cylindrical variables: Have x = ρ cos φ, y = ρ sin φ, and x2 + y2 = ρ2. Therefore D = 1 ρ (cos φax + sin φay) Then Dρ = D · aρ = 1 ρ cos φ(ax · aρ) + sin φ(ay · aρ) = 1 ρ cos2 φ + sin2 φ = 1 ρ and Dφ = D · aφ = 1 ρ cos φ(ax · aφ) + sin φ(ay · aφ) = 1 ρ [cos φ(− sin φ) + sin φ cos φ] = 0 Therefore D = 1 ρ aρ 7 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 10. 1.19b. Evaluate D at the point where ρ = 2, φ = 0.2π, and z = 5, expressing the result in cylindrical and cartesian coordinates: At the given point, and in cylindrical coordinates, D = 0.5aρ. To express this in cartesian, we use D = 0.5(aρ · ax)ax + 0.5(aρ · ay)ay = 0.5 cos 36◦ ax + 0.5 sin 36◦ ay = 0.41ax + 0.29ay 1.20. Express in cartesian components: a) the vector at A(ρ = 4, φ = 40◦, z = −2) that extends to B(ρ = 5, φ = −110◦, z = 2): We have A(4 cos 40◦, 4 sin 40◦, −2) = A(3.06, 2.57, −2), and B(5 cos(−110◦), 5 sin(−110◦), 2) = B(−1.71, −4.70, 2) in cartesian. Thus RAB = (−4.77, −7.30, 4). b) a unit vector at B directed toward A: Have RBA = (4.77, 7.30, −4), and so aBA = (4.77, 7.30, −4) |(4.77, 7.30, −4)| = (0.50, 0.76, −0.42) c) a unit vector at B directed toward the origin: Have rB = (−1.71, −4.70, 2), and so −rB = (1.71, 4.70, −2). Thus a = (1.71, 4.70, −2) |(1.71, 4.70, −2)| = (0.32, 0.87, −0.37) 1.21. Express in cylindrical components: a) the vector from C(3, 2, −7) to D(−1, −4, 2): C(3, 2, −7) → C(ρ = 3.61, φ = 33.7◦, z = −7) and D(−1, −4, 2) → D(ρ = 4.12, φ = −104.0◦, z = 2). Now RCD = (−4, −6, 9) and Rρ = RCD · aρ = −4 cos(33.7) − 6 sin(33.7) = −6.66. Then Rφ = RCD · aφ = 4 sin(33.7) − 6 cos(33.7) = −2.77. So RCD = −6.66aρ − 2.77aφ + 9az b) a unit vector at D directed toward C: RCD = (4, 6, −9) and Rρ = RDC · aρ = 4 cos(−104.0) + 6 sin(−104.0) = −6.79. Then Rφ = RDC · aφ = 4[− sin(−104.0)] + 6 cos(−104.0) = 2.43. So RDC = −6.79aρ + 2.43aφ − 9az Thus aDC = −0.59aρ + 0.21aφ − 0.78az c) a unit vector at D directed toward the origin: Start with rD = (−1, −4, 2), and so the vector toward the origin will be −rD = (1, 4, −2). Thus in cartesian the unit vector is a = (0.22, 0.87, −0.44). Convert to cylindrical: aρ = (0.22, 0.87, −0.44) · aρ = 0.22 cos(−104.0) + 0.87 sin(−104.0) = −0.90, and aφ = (0.22, 0.87, −0.44) · aφ = 0.22[− sin(−104.0)] + 0.87 cos(−104.0) = 0, so that finally, a = −0.90aρ − 0.44az. 1.22. A field is given in cylindrical coordinates as F = 40 ρ2 + 1 + 3(cos φ + sin φ) aρ + 3(cos φ − sin φ)aφ − 2az where the magnitude of F is found to be: |F| = √ F · F = 1600 (ρ2 + 1)2 + 240 ρ2 + 1 (cos φ + sin φ) + 22 1/2 8 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 11. Sketch |F|: a) vs. φ with ρ = 3: in this case the above simplifies to |F(ρ = 3)| = |Fa| = [38 + 24(cos φ + sin φ)]1/2 b) vs. ρ with φ = 0, in which: |F(φ = 0)| = |Fb| = 1600 (ρ2 + 1)2 + 240 ρ2 + 1 + 22 1/2 c) vs. ρ with φ = 45◦, in which |F(φ = 45◦ )| = |Fc| = 1600 (ρ2 + 1)2 + 240 √ 2 ρ2 + 1 + 22 1/2 9 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 12. 1.23. The surfaces ρ = 3, ρ = 5, φ = 100◦, φ = 130◦, z = 3, and z = 4.5 define a closed surface. a) Find the enclosed volume: Vol = 4.5 3 130◦ 100◦ 5 3 ρ dρ dφ dz = 6.28 NOTE: The limits on the φ integration must be converted to radians (as was done here, but not shown). b) Find the total area of the enclosing surface: Area = 2 130◦ 100◦ 5 3 ρ dρ dφ + 4.5 3 130◦ 100◦ 3 dφ dz + 4.5 3 130◦ 100◦ 5 dφ dz + 2 4.5 3 5 3 dρ dz = 20.7 c) Find the total length of the twelve edges of the surfaces: Length = 4 × 1.5 + 4 × 2 + 2 × 30◦ 360◦ × 2π × 3 + 30◦ 360◦ × 2π × 5 = 22.4 d) Find the length of the longest straight line that lies entirely within the volume: This will be between the points A(ρ = 3, φ = 100◦, z = 3) and B(ρ = 5, φ = 130◦, z = 4.5). Performing point transformations to cartesian coordinates, these become A(x = −0.52, y = 2.95, z = 3) and B(x = −3.21, y = 3.83, z = 4.5). Taking A and B as vectors directed from the origin, the requested length is Length = |B − A| = |(−2.69, 0.88, 1.5)| = 3.21 1.24. At point P (−3, 4, 5), express the vector that extends from P to Q(2, 0, −1) in: a) rectangular coordinates. RP Q = Q − P = 5ax − 4ay − 6az Then |RPQ| = √ 25 + 16 + 36 = 8.8 b) cylindrical coordinates. At P , ρ = 5, φ = tan−1(4/ − 3) = −53.1◦, and z = 5. Now, RPQ · aρ = (5ax − 4ay − 6az) · aρ = 5 cos φ − 4 sin φ = 6.20 RPQ · aφ = (5ax − 4ay − 6az) · aφ = −5 sin φ − 4 cos φ = 1.60 Thus RPQ = 6.20aρ + 1.60aφ − 6az and |RPQ| = √ 6.202 + 1.602 + 62 = 8.8 c) spherical coordinates. At P , r = √ 9 + 16 + 25 = √ 50 = 7.07, θ = cos−1(5/7.07) = 45◦, and φ = tan−1(4/ − 3) = −53.1◦. RPQ · ar = (5ax − 4ay − 6az) · ar = 5 sin θ cos φ − 4 sin θ sin φ − 6 cos θ = 0.14 RP Q · aθ = (5ax − 4ay − 6az) · aθ = 5 cos θ cos φ − 4 cos θ sin φ − (−6) sin θ = 8.62 RPQ · aφ = (5ax − 4ay − 6az) · aφ = −5 sin φ − 4 cos φ = 1.60 10 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 13. 1.24. (continued) Thus RP Q = 0.14ar + 8.62aθ + 1.60aφ and |RPQ| = √ 0.142 + 8.622 + 1.602 = 8.8 d) Show that each of these vectors has the same magnitude. Each does, as shown above. 1.25. Given point P (r = 0.8, θ = 30◦, φ = 45◦), and E = 1 r2 cos φ ar + sin φ sin θ aφ a) Find E at P : E = 1.10aρ + 2.21aφ. b) Find |E| at P : |E| = √ 1.102 + 2.212 = 2.47. c) Find a unit vector in the direction of E at P: aE = E |E| = 0.45ar + 0.89aφ 1.26. a) Determine an expression for ay in spherical coordinates at P (r = 4, θ = 0.2π, φ = 0.8π): Use ay · ar = sin θ sin φ = 0.35, ay · aθ = cos θ sin φ = 0.48, and ay · aφ = cos φ = −0.81 to obtain ay = 0.35ar + 0.48aθ − 0.81aφ b) Express ar in cartesian components at P: Find x = r sin θ cos φ = −1.90, y = r sin θ sin φ = 1.38, and z = r cos θ = −3.24. Then use ar · ax = sin θ cos φ = −0.48, ar · ay = sin θ sin φ = 0.35, and ar · az = cos θ = 0.81 to obtain ar = −0.48ax + 0.35ay + 0.81az 1.27. The surfaces r = 2 and 4, θ = 30◦ and 50◦, and φ = 20◦ and 60◦ identify a closed surface. a) Find the enclosed volume: This will be Vol = 60◦ 20◦ 50◦ 30◦ 4 2 r2 sin θdrdθdφ = 2.91 where degrees have been converted to radians. b) Find the total area of the enclosing surface: Area = 60◦ 20◦ 50◦ 30◦ (42 + 22 ) sin θdθdφ + 4 2 60◦ 20◦ r(sin 30◦ + sin 50◦ )drdφ + 2 50◦ 30◦ 4 2 rdrdθ = 12.61 c) Find the total length of the twelve edges of the surface: Length = 4 4 2 dr + 2 50◦ 30◦ (4 + 2)dθ + 60◦ 20◦ (4 sin 50◦ + 4 sin 30◦ + 2 sin 50◦ + 2 sin 30◦ )dφ = 17.49 11 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 14. 1.27. (continued) d) Find the length of the longest straight line that lies entirely within the surface: This will be from A(r = 2, θ = 50◦, φ = 20◦) to B(r = 4, θ = 30◦, φ = 60◦) or A(x = 2 sin 50◦ cos 20◦ , y = 2 sin 50◦ sin 20◦ , z = 2 cos 50◦ ) to B(x = 4 sin 30◦ cos 60◦ , y = 4 sin 30◦ sin 60◦ , z = 4 cos 30◦ ) or finally A(1.44, 0.52, 1.29) to B(1.00, 1.73, 3.46). Thus B − A = (−0.44, 1.21, 2.18) and Length = |B − A| = 2.53 1.28. a) Determine the cartesian components of the vector from A(r = 5, θ = 110◦, φ = 200◦) to B(r = 7, θ = 30◦, φ = 70◦): First transform the points to cartesian: xA = 5 sin 110◦ cos 200◦ = −4.42, yA = 5 sin 110◦ sin 200◦ = −1.61, and zA = 5 cos 110◦ = −1.71; xB = 7 sin 30◦ cos 70◦ = 1.20, yB = 7 sin 30◦ sin 70◦ = 3.29, and zB = 7 cos 30◦ = 6.06. Now RAB = B − A = 5.62ax + 4.90ay + 7.77az b) Find the spherical components of the vector at P (2, −3, 4) extending to Q(−3, 2, 5): First, RPQ = Q − P = (−5, 5, 1). Then at P , r = √ 4 + 9 + 16 = 5.39, θ = cos−1(4/ √ 29) = 42.0◦, and φ = tan−1(−3/2) = −56.3◦. Now RPQ · ar = −5 sin(42◦ ) cos(−56.3◦ ) + 5 sin(42◦ ) sin(−56.3◦ ) + 1 cos(42◦ ) = −3.90 RPQ · aθ = −5 cos(42◦ ) cos(−56.3◦ ) + 5 cos(42◦ ) sin(−56.3◦ ) − 1 sin(42◦ ) = −5.82 RP Q · aφ = −(−5) sin(−56.3◦ ) + 5 cos(−56.3◦ ) = −1.39 So finally, RP Q = −3.90ar − 5.82aθ − 1.39aφ c) If D = 5ar − 3aθ + 4aφ, find D · aρ at M(1, 2, 3): First convert aρ to cartesian coordinates at the specified point. Use aρ = (aρ · ax)ax + (aρ · ay)ay. At A(1, 2, 3), ρ = √ 5, φ = tan−1(2) = 63.4◦, r = √ 14, and θ = cos−1(3/ √ 14) = 36.7◦. So aρ = cos(63.4◦)ax + sin(63.4◦)ay = 0.45ax + 0.89ay. Then (5ar − 3aθ + 4aφ) · (0.45ax + 0.89ay) = 5(0.45) sin θ cos φ + 5(0.89) sin θ sin φ − 3(0.45) cos θ cos φ − 3(0.89) cos θ sin φ + 4(0.45)(− sin φ) + 4(0.89) cos φ = 0.59 1.29. Express the unit vector ax in spherical components at the point: a) r = 2, θ = 1 rad, φ = 0.8 rad: Use ax = (ax · ar)ar + (ax · aθ )aθ + (ax · aφ)aφ = sin(1) cos(0.8)ar + cos(1) cos(0.8)aθ + (− sin(0.8))aφ = 0.59ar + 0.38aθ − 0.72aφ 12 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 15. 1.29 (continued) Express the unit vector ax in spherical components at the point: b) x = 3, y = 2, z = −1: First, transform the point to spherical coordinates. Have r = √ 14, θ = cos−1(−1/ √ 14) = 105.5◦, and φ = tan−1(2/3) = 33.7◦. Then ax = sin(105.5◦ ) cos(33.7◦ )ar + cos(105.5◦ ) cos(33.7◦ )aθ + (− sin(33.7◦ ))aφ = 0.80ar − 0.22aθ − 0.55aφ c) ρ = 2.5, φ = 0.7 rad, z = 1.5: Again, convert the point to spherical coordinates. r = ρ2 + z2 =√ 8.5, θ = cos−1(z/r) = cos−1(1.5/ √ 8.5) = 59.0◦, and φ = 0.7 rad = 40.1◦. Now ax = sin(59◦ ) cos(40.1◦ )ar + cos(59◦ ) cos(40.1◦ )aθ + (− sin(40.1◦ ))aφ = 0.66ar + 0.39aθ − 0.64aφ 1.30. Given A(r = 20, θ = 30◦, φ = 45◦) and B(r = 30, θ = 115◦, φ = 160◦), find: a) |RAB|: First convert A and B to cartesian: Have xA = 20 sin(30◦) cos(45◦) = 7.07, yA = 20 sin(30◦) sin(45◦) = 7.07, and zA = 20 cos(30◦) = 17.3. xB = 30 sin(115◦) cos(160◦) = −25.6, yB = 30 sin(115◦) sin(160◦) = 9.3, and zB = 30 cos(115◦) = −12.7. Now RAB = RB − RA = (−32.6, 2.2, −30.0), and so |RAB| = 44.4. b) |RAC|, given C(r = 20, θ = 90◦, φ = 45◦). Again, converting C to cartesian, obtain xC = 20 sin(90◦) cos(45◦) = 14.14, yC = 20 sin(90◦) sin(45◦) = 14.14, and zC = 20 cos(90◦) = 0. So RAC = RC − RA = (7.07, 7.07, −17.3), and |RAC| = 20.0. c) the distance from A to C on a great circle path: Note that A and C share the same r and φ coordinates; thus moving from A to C involves only a change in θ of 60◦. The requested arc length is then distance = 20 × 60 2π 360 = 20.9 13 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 16. CHAPTER 2 2.1. Four 10nC positive charges are located in the z = 0 plane at the corners of a square 8cm on a side. A fifth 10nC positive charge is located at a point 8cm distant from the other charges. Calculate the magnitude of the total force on this fifth charge for ǫ = ǫ0: Arrange the charges in the xy plane at locations (4,4), (4,-4), (-4,4), and (-4,-4). Then the fifth charge will be on the z axis at location z = 4 √ 2, which puts it at 8cm distance from the other four. By symmetry, the force on the fifth charge will be z-directed, and will be four times the z component of force produced by each of the four other charges. F = 4 √ 2 × q2 4πǫ0d2 = 4 √ 2 × (10−8)2 4π(8.85 × 10−12)(0.08)2 = 4.0 × 10−4 N 2.2. A charge Q1 = 0.1 µC is located at the origin, while Q2 = 0.2 µC is at A(0.8, −0.6, 0). Find the locus of points in the z = 0 plane at which the x component of the force on a third positive charge is zero. To solve this problem, the z coordinate of the third charge is immaterial, so we can place it in the xy plane at coordinates (x, y, 0). We take its magnitude to be Q3. The vector directed from the first charge to the third is R13 = xax + yay; the vector directed from the second charge to the third is R23 = (x − 0.8)ax + (y + 0.6)ay. The force on the third charge is now F3 = Q3 4πǫ0 Q1R13 |R13|3 + Q2R23 |R23|3 = Q3 × 10−6 4πǫ0 0.1(xax + yay) (x2 + y2)1.5 + 0.2[(x − 0.8)ax + (y + 0.6)ay] [(x − 0.8)2 + (y + 0.6)2]1.5 We desire the x component to be zero. Thus, 0 = 0.1xax (x2 + y2)1.5 + 0.2(x − 0.8)ax [(x − 0.8)2 + (y + 0.6)2]1.5 or x[(x − 0.8)2 + (y + 0.6)2 ]1.5 = 2(0.8 − x)(x2 + y2 )1.5 2.3. Point charges of 50nC each are located at A(1, 0, 0), B(−1, 0, 0), C(0, 1, 0), and D(0, −1, 0) in free space. Find the total force on the charge at A. The force will be: F = (50 × 10−9)2 4πǫ0 RCA |RCA|3 + RDA |RDA|3 + RBA |RBA|3 where RCA = ax − ay, RDA = ax + ay, and RBA = 2ax. The magnitudes are |RCA| = |RDA| = √ 2, and |RBA| = 2. Substituting these leads to F = (50 × 10−9)2 4πǫ0 1 2 √ 2 + 1 2 √ 2 + 2 8 ax = 21.5ax µN where distances are in meters. 14 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 17. 2.4. Let Q1 = 8 µC be located at P1(2, 5, 8) while Q2 = −5 µC is at P2(6, 15, 8). Let ǫ = ǫ0. a) Find F2, the force on Q2: This force will be F2 = Q1Q2 4πǫ0 R12 |R12|3 = (8 × 10−6)(−5 × 10−6) 4πǫ0 (4ax + 10ay) (116)1.5 = (−1.15ax − 2.88ay) mN b) Find the coordinates of P3 if a charge Q3 experiences a total force F3 = 0 at P3: This force in general will be: F3 = Q3 4πǫ0 Q1R13 |R13|3 + Q2R23 |R23|3 where R13 = (x − 2)ax + (y − 5)ay and R23 = (x − 6)ax + (y − 15)ay. Note, however, that all three charges must lie in a straight line, and the location of Q3 will be along the vector R12 extended past Q2. The slope of this vector is (15 − 5)/(6 − 2) = 2.5. Therefore, we look for P3 at coordinates (x, 2.5x, 8). With this restriction, the force becomes: F3 = Q3 4πǫ0 8[(x − 2)ax + 2.5(x − 2)ay] [(x − 2)2 + (2.5)2(x − 2)2]1.5 − 5[(x − 6)ax + 2.5(x − 6)ay] [(x − 6)2 + (2.5)2(x − 6)2]1.5 where we require the term in large brackets to be zero. This leads to 8(x − 2)[((2.5)2 + 1)(x − 6)2 ]1.5 − 5(x − 6)[((2.5)2 + 1)(x − 2)2 ]1.5 = 0 which reduces to 8(x − 6)2 − 5(x − 2)2 = 0 or x = 6 √ 8 − 2 √ 5 √ 8 − √ 5 = 21.1 The coordinates of P3 are thus P3(21.1, 52.8, 8) 2.5. Let a point charge Q125 nC be located at P1(4, −2, 7) and a charge Q2 = 60 nC be at P2(−3, 4, −2). a) If ǫ = ǫ0, find E at P3(1, 2, 3): This field will be E = 10−9 4πǫ0 25R13 |R13|3 + 60R23 |R23|3 where R13 = −3ax +4ay −4az and R23 = 4ax −2ay +5az. Also, |R13| = √ 41 and |R23| = √ 45. So E = 10−9 4πǫ0 25 × (−3ax + 4ay − 4az) (41)1.5 + 60 × (4ax − 2ay + 5az) (45)1.5 = 4.58ax − 0.15ay + 5.51az b) At what point on the y axis is Ex = 0? P3 is now at (0, y, 0), so R13 = −4ax + (y + 2)ay − 7az and R23 = 3ax + (y − 4)ay + 2az. Also, |R13| = 65 + (y + 2)2 and |R23| = 13 + (y − 4)2. Now the x component of E at the new P3 will be: Ex = 10−9 4πǫ0 25 × (−4) [65 + (y + 2)2]1.5 + 60 × 3 [13 + (y − 4)2]1.5 To obtain Ex = 0, we require the expression in the large brackets to be zero. This expression simplifies to the following quadratic: 0.48y2 + 13.92y + 73.10 = 0 which yields the two values: y = −6.89, −22.11 15 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 18. 2.6. Point charges of 120 nC are located at A(0, 0, 1) and B(0, 0, −1) in free space. a) Find E at P (0.5, 0, 0): This will be EP = 120 × 10−9 4πǫ0 RAP |RAP |3 + RBP |RBP |3 where RAP = 0.5ax − az and RBP = 0.5ax + az. Also, |RAP | = |RBP | = √ 1.25. Thus: EP = 120 × 10−9ax 4π(1.25)1.5ǫ0 = 772 V/m b) What single charge at the origin would provide the identical field strength? We require Q0 4πǫ0(0.5)2 = 772 from which we find Q0 = 21.5 nC. 2.7. A 2 µC point charge is located at A(4, 3, 5) in free space. Find Eρ, Eφ, and Ez at P (8, 12, 2). Have EP = 2 × 10−6 4πǫ0 RAP |RAP |3 = 2 × 10−6 4πǫ0 4ax + 9ay − 3az (106)1.5 = 65.9ax + 148.3ay − 49.4az Then, at point P , ρ = √ 82 + 122 = 14.4, φ = tan−1(12/8) = 56.3◦, and z = z. Now, Eρ = Ep · aρ = 65.9(ax · aρ) + 148.3(ay · aρ) = 65.9 cos(56.3◦ ) + 148.3 sin(56.3◦ ) = 159.7 and Eφ = Ep · aφ = 65.9(ax · aφ) + 148.3(ay · aφ) = −65.9 sin(56.3◦ ) + 148.3 cos(56.3◦ ) = 27.4 Finally, Ez = −49.4 2.8. Given point charges of −1 µC at P1(0, 0, 0.5) and P2(0, 0, −0.5), and a charge of 2 µC at the origin, find E at P (0, 2, 1) in spherical components, assuming ǫ = ǫ0. The field will take the general form: EP = 10−6 4πǫ0 − R1 |R1|3 + 2R2 |R2|3 − R3 |R3|3 where R1, R2, R3 are the vectors to P from each of the charges in their original listed order. Specifically, R1 = (0, 2, 0.5), R2 = (0, 2, 1), and R3 = (0, 2, 1.5). The magnitudes are |R1| = 2.06, |R2| = 2.24, and |R3| = 2.50. Thus EP = 10−6 4πǫ0 −(0, 2, 0.5) (2.06)3 + 2(0, 2, 1) (2.24)3 − (0, 2, 1.5) (2.50)3 = 89.9ay + 179.8az Now, at P , r = √ 5, θ = cos−1(1/ √ 5) = 63.4◦, and φ = 90◦. So Er = EP · ar = 89.9(ay · ar) + 179.8(az · ar) = 89.9 sin θ sin φ + 179.8 cos θ = 160.9 Eθ = EP · aθ = 89.9(ay · aθ ) + 179.8(az · aθ ) = 89.9 cos θ sin φ + 179.8(− sin θ) = −120.5 Eφ = EP · aφ = 89.9(ay · aφ) + 179.8(az · aφ) = 89.9 cos φ = 0 16 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 19. 2.9. A 100 nC point charge is located at A(−1, 1, 3) in free space. a) Find the locus of all points P (x, y, z) at which Ex = 500 V/m: The total field at P will be: EP = 100 × 10−9 4πǫ0 RAP |RAP |3 where RAP = (x + 1)ax + (y − 1)ay + (z − 3)az, and where |RAP | = [(x + 1)2 + (y − 1)2 + (z − 3)2]1/2. The x component of the field will be Ex = 100 × 10−9 4πǫ0 (x + 1) [(x + 1)2 + (y − 1)2 + (z − 3)2]1.5 = 500 V/m And so our condition becomes: (x + 1) = 0.56 [(x + 1)2 + (y − 1)2 + (z − 3)2 ]1.5 b) Find y1 if P (−2, y1, 3) lies on that locus: At point P , the condition of part a becomes 3.19 = 1 + (y1 − 1)2 3 from which (y1 − 1)2 = 0.47, or y1 = 1.69 or 0.31 2.10. Charges of 20 and -20 nC are located at (3, 0, 0) and (−3, 0, 0), respectively. Let ǫ = ǫ0. Determine |E| at P (0, y, 0): The field will be EP = 20 × 10−9 4πǫ0 R1 |R1|3 − R2 |R2|3 where R1, the vector from the positive charge to point P is (−3, y, 0), and R2, the vector from the negative charge to point P , is (3, y, 0). The magnitudes of these vectors are |R1| = |R2| = 9 + y2. Substituting these into the expression for EP produces EP = 20 × 10−9 4πǫ0 −6ax (9 + y2)1.5 from which |EP | = 1079 (9 + y2)1.5 V/m 2.11. A charge Q0 located at the origin in free space produces a field for which Ez = 1 kV/m at point P (−2, 1, −1). a) Find Q0: The field at P will be EP = Q0 4πǫ0 −2ax + ay − az 61.5 Since the z component is of value 1 kV/m, we find Q0 = −4πǫ061.5 × 103 = −1.63 µC. 17 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 20. 2.11. (continued) b) Find E at M(1, 6, 5) in cartesian coordinates: This field will be: EM = −1.63 × 10−6 4πǫ0 ax + 6ay + 5az [1 + 36 + 25]1.5 or EM = −30.11ax − 180.63ay − 150.53az. c) Find E at M(1, 6, 5) in cylindrical coordinates: At M, ρ = √ 1 + 36 = 6.08, φ = tan−1(6/1) = 80.54◦, and z = 5. Now Eρ = EM · aρ = −30.11 cos φ − 180.63 sin φ = −183.12 Eφ = EM · aφ = −30.11(− sin φ) − 180.63 cos φ = 0 (as expected) so that EM = −183.12aρ − 150.53az. d) Find E at M(1, 6, 5) in spherical coordinates: At M, r = √ 1 + 36 + 25 = 7.87, φ = 80.54◦ (as before), and θ = cos−1(5/7.87) = 50.58◦. Now, since the charge is at the origin, we expect to obtain only a radial component of EM. This will be: Er = EM · ar = −30.11 sin θ cos φ − 180.63 sin θ sin φ − 150.53 cos θ = −237.1 2.12. The volume charge density ρv = ρ0e−|x|−|y|−|z| exists over all free space. Calculate the total charge present: This will be 8 times the integral of ρv over the first octant, or Q = 8 ∞ 0 ∞ 0 ∞ 0 ρ0e−x−y−z dx dy dz = 8ρ0 2.13. A uniform volume charge density of 0.2 µC/m3 (note typo in book) is present throughout the spherical shell extending from r = 3 cm to r = 5 cm. If ρv = 0 elsewhere: a) find the total charge present throughout the shell: This will be Q = 2π 0 π 0 .05 .03 0.2 r2 sin θ dr dθ dφ = 4π(0.2) r3 3 .05 .03 = 8.21 × 10−5 µC = 82.1 pC b) find r1 if half the total charge is located in the region 3 cm < r < r1: If the integral over r in part a is taken to r1, we would obtain 4π(0.2) r3 3 r1 .03 = 4.105 × 10−5 Thus r1 = 3 × 4.105 × 10−5 0.2 × 4π + (.03)3 1/3 = 4.24 cm 18 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 21. 2.14. Let ρv = 5e−0.1ρ (π − |φ|) 1 z2 + 10 µC/m3 in the region 0 ≤ ρ ≤ 10, −π < φ < π, all z, and ρv = 0 elsewhere. a) Determine the total charge present: This will be the integral of ρv over the region where it exists; specifically, Q = ∞ −∞ π −π 10 0 5e−0.1ρ (π − |φ|) 1 z2 + 10 ρ dρ dφ dz which becomes Q = 5 e−0.1ρ (0.1)2 (−0.1 − 1) 10 0 ∞ −∞ 2 π 0 (π − φ) 1 z2 + 10 dφ dz or Q = 5 × 26.4 ∞ −∞ π2 1 z2 + 10 dz Finally, Q = 5 × 26.4 × π2 1 √ 10 tan−1 z √ 10 ∞ −∞ = 5(26.4)π3 √ 10 = 1.29 × 103 µC = 1.29 mC b) Calculate the charge within the region 0 ≤ ρ ≤ 4, −π/2 < φ < π/2, −10 < z < 10: With the limits thus changed, the integral for the charge becomes: Q′ = 10 −10 2 π/2 0 4 0 5e−0.1ρ (π − φ) 1 z2 + 10 ρ dρ dφ dz Following the same evaulation procedure as in part a, we obtain Q′ = 0.182 mC. 2.15. A spherical volume having a 2 µm radius contains a uniform volume charge density of 1015 C/m3. a) What total charge is enclosed in the spherical volume? This will be Q = (4/3)π(2 × 10−6)3 × 1015 = 3.35 × 10−2 C. b) Now assume that a large region contains one of these little spheres at every corner of a cubical grid 3mm on a side, and that there is no charge between spheres. What is the average volume charge density throughout this large region? Each cube will contain the equivalent of one little sphere. Neglecting the little sphere volume, the average density becomes ρv,avg = 3.35 × 10−2 (0.003)3 = 1.24 × 106 C/m3 2.16. The region in which 4 < r < 5, 0 < θ < 25◦, and 0.9π < φ < 1.1π contains the volume charge density of ρv = 10(r − 4)(r − 5) sin θ sin(φ/2). Outside the region, ρv = 0. Find the charge within the region: The integral that gives the charge will be Q = 10 1.1π .9π 25◦ 0 5 4 (r − 4)(r − 5) sin θ sin(φ/2) r2 sin θ dr dθ dφ 19 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 22. 2.16. (continued) Carrying out the integral, we obtain Q = 10 r5 5 − 9 r4 4 + 20 r3 3 5 4 1 2 θ − 1 4 sin(2θ) 25◦ 0 −2 cos θ 2 1.1π .9π = 10(−3.39)(.0266)(.626) = 0.57 C 2.17. A uniform line charge of 16 nC/m is located along the line defined by y = −2, z = 5. If ǫ = ǫ0: a) Find E at P (1, 2, 3): This will be EP = ρl 2πǫ0 RP |RP |2 where RP = (1, 2, 3) − (1, −2, 5) = (0, 4, −2), and |RP |2 = 20. So EP = 16 × 10−9 2πǫ0 4ay − 2az 20 = 57.5ay − 28.8az V/m b) Find E at that point in the z = 0 plane where the direction of E is given by (1/3)ay − (2/3)az: With z = 0, the general field will be Ez=0 = ρl 2πǫ0 (y + 2)ay − 5az (y + 2)2 + 25 We require |Ez| = −|2Ey|, so 2(y + 2) = 5. Thus y = 1/2, and the field becomes: Ez=0 = ρl 2πǫ0 2.5ay − 5az (2.5)2 + 25 = 23ay − 46az 2.18. Uniform line charges of 0.4 µC/m and −0.4 µC/m are located in the x = 0 plane at y = −0.6 and y = 0.6 m respectively. Let ǫ = ǫ0. a) Find E at P (x, 0, z): In general, we have EP = ρl 2πǫ0 R+P |R+P | − R−P |R−P | where R+P and R−P are, respectively, the vectors directed from the positive and negative line charges to the point P , and these are normal to the z axis. We thus have R+P = (x, 0, z) − (0, −.6, z) = (x, .6, 0), and R−P = (x, 0, z) − (0, .6, z) = (x, −.6, 0). So EP = ρl 2πǫ0 xax + 0.6ay x2 + (0.6)2 − xax − 0.6ay x2 + (0.6)2 = 0.4 × 10−6 2πǫ0 1.2ay x2 + 0.36 = 8.63ay x2 + 0.36 kV/m 20 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 23. 2.18. (continued) b) Find E at Q(2, 3, 4): This field will in general be: EQ = ρl 2πǫ0 R+Q |R+Q| − R−Q |R−Q| where R+Q = (2, 3, 4)−(0, −.6, 4) = (2, 3.6, 0), and R−Q = (2, 3, 4)−(0, .6, 4) = (2, 2.4, 0). Thus EQ = ρl 2πǫ0 2ax + 3.6ay 22 + (3.6)2 − 2ax + 2.4ay 22 + (2.4)2 = −625.8ax − 241.6ay V/m 2.19. A uniform line charge of 2 µC/m is located on the z axis. Find E in cartesian coordinates at P (1, 2, 3) if the charge extends from a) −∞ < z < ∞: With the infinite line, we know that the field will have only a radial component in cylindrical coordinates (or x and y components in cartesian). The field from an infinite line on the z axis is generally E = [ρl/(2πǫ0ρ)]aρ. Therefore, at point P : EP = ρl 2πǫ0 RzP |RzP |2 = (2 × 10−6) 2πǫ0 ax + 2ay 5 = 7.2ax + 14.4ay kV/m where RzP is the vector that extends from the line charge to point P, and is perpendicular to the z axis; i.e., RzP = (1, 2, 3) − (0, 0, 3) = (1, 2, 0). b) −4 ≤ z ≤ 4: Here we use the general relation EP = ρldz 4πǫ0 r − r′ |r − r′|3 where r = ax + 2ay + 3az and r′ = zaz. So the integral becomes EP = (2 × 10−6) 4πǫ0 4 −4 ax + 2ay + (3 − z)az [5 + (3 − z)2]1.5 dz Using integral tables, we obtain: EP = 3597 (ax + 2ay)(z − 3) + 5az (z2 − 6z + 14) 4 −4 V/m = 4.9ax + 9.8ay + 4.9az kV/m The student is invited to verify that when evaluating the above expression over the limits −∞ < z < ∞, the z component vanishes and the x and y components become those found in part a. 2.20. Uniform line charges of 120 nC/m lie along the entire extent of the three coordinate axes. Assuming free space conditions, find E at P (−3, 2, −1): Since all line charges are infinitely-long, we can write: EP = ρl 2πǫ0 RxP |RxP |2 + RyP |RyP |2 + RzP |RzP |2 where RxP , RyP , and RzP are the normal vectors from each of the three axes that terminate on point P . Specifically, RxP = (−3, 2, −1) − (−3, 0, 0) = (0, 2, −1), RyP = (−3, 2, −1) − (0, 2, 0) = (−3, 0, −1), and RzP = (−3, 2, −1) − (0, 0, −1) = (−3, 2, 0). Substituting these into the expression for EP gives EP = ρl 2πǫ0 2ay − az 5 + −3ax − az 10 + −3ax + 2ay 13 = −1.15ax + 1.20ay − 0.65az kV/m 21 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 24. 2.21. Two identical uniform line charges with ρl = 75 nC/m are located in free space at x = 0, y = ±0.4 m. What force per unit length does each line charge exert on the other? The charges are parallel to the z axis and are separated by 0.8 m. Thus the field from the charge at y = −0.4 evaluated at the location of the charge at y = +0.4 will be E = [ρl/(2πǫ0(0.8))]ay. The force on a differential length of the line at the positive y location is dF = dqE = ρldzE. Thus the force per unit length acting on the line at postive y arising from the charge at negative y is F = 1 0 ρ2 l dz 2πǫ0(0.8) ay = 1.26 × 10−4 ay N/m = 126 ay µN/m The force on the line at negative y is of course the same, but with −ay. 2.22. A uniform surface charge density of 5 nC/m2 is present in the region x = 0, −2 < y < 2, and all z. If ǫ = ǫ0, find E at: a) PA(3, 0, 0): We use the superposition integral: E = ρsda 4πǫ0 r − r′ |r − r′|3 where r = 3ax and r′ = yay + zaz. The integral becomes: EP A = ρs 4πǫ0 ∞ −∞ 2 −2 3ax − yay − zaz [9 + y2 + z2]1.5 dy dz Since the integration limits are symmetric about the origin, and since the y and z components of the integrand exhibit odd parity (change sign when crossing the origin, but otherwise symmetric), these will integrate to zero, leaving only the x component. This is evident just from the symmetry of the problem. Performing the z integration first on the x component, we obtain (using tables): Ex,PA = 3ρs 4πǫ0 2 −2 dy (9 + y2) z 9 + y2 + z2 ∞ −∞ = 3ρs 2πǫ0 2 −2 dy (9 + y2) = 3ρs 2πǫ0 1 3 tan−1 y 3 2 −2 = 106 V/m The student is encouraged to verify that if the y limits were −∞ to ∞, the result would be that of the infinite charged plane, or Ex = ρs/(2ǫ0). b) PB(0, 3, 0): In this case, r = 3ay, and symmetry indicates that only a y component will exist. The integral becomes Ey,P B = ρs 4πǫ0 ∞ −∞ 2 −2 (3 − y) dy dz [(z2 + 9) − 6y + y2]1.5 = ρs 2πǫ0 2 −2 (3 − y) dy (3 − y)2 = − ρs 2πǫ0 ln(3 − y) 2 −2 = 145 V/m 22 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 25. 2.23. Given the surface charge density, ρs = 2 µC/m2, in the region ρ < 0.2 m, z = 0, and is zero elsewhere, find E at: a) PA(ρ = 0, z = 0.5): First, we recognize from symmetry that only a z component of E will be present. Considering a general point z on the z axis, we have r = zaz. Then, with r′ = ρaρ, we obtain r − r′ = zaz − ρaρ. The superposition integral for the z component of E will be: Ez,PA = ρs 4πǫ0 2π 0 0.2 0 z ρ dρ dφ (ρ2 + z2)1.5 = − 2πρs 4πǫ0 z 1 z2 + ρ2 0.2 0 = ρs 2ǫ0 z 1 √ z2 − 1 √ z2 + 0.4 With z = 0.5 m, the above evaluates as Ez,PA = 8.1 kV/m. b) With z at −0.5 m, we evaluate the expression for Ez to obtain Ez,PB = −8.1 kV/m. 2.24. Surface charge density is positioned in free space as follows: 20 nC/m2 at x = −3, −30 nC/m2 at y = 4, and 40 nC/m2 at z = 2. Find the magnitude of E at the three points, (4, 3, −2), (−2, 5, −1), and (0, 0, 0). Since all three sheets are infinite, the field magnitude associated with each one will be ρs/(2ǫ0), which is position-independent. For this reason, the net field magnitude will be the same everywhere, whereas the field direction will depend on which side of a given sheet one is positioned. We take the first point, for example, and find EA = 20 × 10−9 2ǫ0 ax + 30 × 10−9 2ǫ0 ay − 40 × 10−9 2ǫ0 az = 1130ax + 1695ay − 2260az V/m The magnitude of EA is thus 3.04 kV/m. This will be the magnitude at the other two points as well. 2.25. Find E at the origin if the following charge distributions are present in free space: point charge, 12 nC at P (2, 0, 6); uniform line charge density, 3nC/m at x = −2, y = 3; uniform surface charge density, 0.2 nC/m2 at x = 2. The sum of the fields at the origin from each charge in order is: E = (12 × 10−9) 4πǫ0 (−2ax − 6az) (4 + 36)1.5 + (3 × 10−9) 2πǫ0 (2ax − 3ay) (4 + 9) − (0.2 × 10−9)ax 2ǫ0 = −3.9ax − 12.4ay − 2.5az V/m 2.26. A uniform line charge density of 5 nC/m is at y = 0, z = 2 m in free space, while −5 nC/m is located at y = 0, z = −2 m. A uniform surface charge density of 0.3 nC/m2 is at y = 0.2 m, and −0.3 nC/m2 is at y = −0.2 m. Find |E| at the origin: Since each pair consists of equal and opposite charges, the effect at the origin is to double the field produce by one of each type. Taking the sum of the fields at the origin from the surface and line charges, respectively, we find: E(0, 0, 0) = −2 × 0.3 × 10−9 2ǫ0 ay − 2 × 5 × 10−9 2πǫ0(2) az = −33.9ay − 89.9az so that |E| = 96.1 V/m. 23 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 26. 2.27. Given the electric field E = (4x − 2y)ax − (2x + 4y)ay, find: a) the equation of the streamline that passes through the point P (2, 3, −4): We write dy dx = Ey Ex = −(2x + 4y) (4x − 2y) Thus 2(x dy + y dx) = y dy − x dx or 2 d(xy) = 1 2 d(y2 ) − 1 2 d(x2 ) So C1 + 2xy = 1 2 y2 − 1 2 x2 or y2 − x2 = 4xy + C2 Evaluating at P (2, 3, −4), obtain: 9 − 4 = 24 + C2, or C2 = −19 Finally, at P , the requested equation is y2 − x2 = 4xy − 19 b) a unit vector specifying the direction of E at Q(3, −2, 5): Have EQ = [4(3) + 2(2)]ax − [2(3) − 4(2)]ay = 16ax + 2ay. Then |E| = √ 162 + 4 = 16.12 So aQ = 16ax + 2ay 16.12 = 0.99ax + 0.12ay 2.28. Let E = 5x3 ax − 15x2y ay, and find: a) the equation of the streamline that passes through P (4, 2, 1): Write dy dx = Ey Ex = −15x2y 5x3 = −3y x So dy y = −3 dx x ⇒ ln y = −3 ln x + ln C Thus y = e−3 ln x eln C = C x3 At P , have 2 = C/(4)3 ⇒ C = 128. Finally, at P , y = 128 x3 24 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 27. 2.28. (continued) b) a unit vector aE specifying the direction of E at Q(3, −2, 5): At Q, EQ = 135ax + 270ay, and |EQ| = 301.9. Thus aE = 0.45ax + 0.89ay. c) aunitvectoraN = (l, m, 0)thatisperpendiculartoaE atQ: Sincethisvectoristohavenoz compo- nent, wecanfinditthroughaN = ±(aE×az). Performingthis, wefindaN = ±(0.89ax − 0.45ay). 2.29. If E = 20e−5y cos 5xax − sin 5xay , find: a) |E| at P (π/6, 0.1, 2): Substituting this point, we obtain EP = −10.6ax − 6.1ay, and so |EP | = 12.2. b) a unit vector in the direction of EP : The unit vector associated with E is just cos 5xax − sin 5xay , which evaluated at P becomes aE = −0.87ax − 0.50ay. c) the equation of the direction line passing through P : Use dy dx = − sin 5x cos 5x = − tan 5x ⇒ dy = − tan 5x dx Thus y = 1 5 ln cos 5x + C. Evaluating at P , we find C = 0.13, and so y = 1 5 ln cos 5x + 0.13 2.30. Given the electric field intensity E = 400yax + 400xay V/m, find: a) the equation of the streamline passing through the point A(2, 1, −2): Write: dy dx = Ey Ex = x y ⇒ x dx = y dy Thus x2 = y2 + C. Evaluating at A yields C = 3, so the equation becomes x2 3 − y2 3 = 1 b) the equation of the surface on which |E| = 800 V/m: Have |E| = 400 x2 + y2 = 800. Thus x2 + y2 = 4, or we have a circular-cylindrical surface, centered on the z axis, and of radius 2. c) A sketch of the part a equation would yield a parabola, centered at the origin, whose axis is the positive x axis, and for which the slopes of the asymptotes are ±1. d) A sketch of the trace produced by the intersection of the surface of part b with the z = 0 plane would yield a circle centered at the origin, of radius 2. 25 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 28. 2.31. In cylindrical coordinates with E(ρ, φ) = Eρ(ρ, φ)aρ +Eφ(ρ, φ)aφ, the differential equation describ- ing the direction lines is Eρ/Eφ = dρ/(ρdφ) in any constant-z plane. Derive the equation of the line passing through the point P (ρ = 4, φ = 10◦, z = 2) in the field E = 2ρ2 cos 3φaρ + 2ρ2 sin 3φaφ: Using the given information, we write Eρ Eφ = dρ ρdφ = cot 3φ Thus dρ ρ = cot 3φ dφ ⇒ ln ρ = 1 3 ln sin 3φ + ln C or ρ = C(sin 3φ)1/3. Evaluate this at P to obtain C = 7.14. Finally, ρ3 = 364 sin 3φ 26 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 29. CHAPTER 3 3.1. An empty metal paint can is placed on a marble table, the lid is removed, and both parts are discharged (honorably) by touching them to ground. An insulating nylon thread is glued to the center of the lid, and a penny, a nickel, and a dime are glued to the thread so that they are not touching each other. The penny is given a charge of +5 nC, and the nickel and dime are discharged. The assembly is lowered into the can so that the coins hang clear of all walls, and the lid is secured. The outside of the can is again touched momentarily to ground. The device is carefully disassembled with insulating gloves and tools. a) What charges are found on each of the five metallic pieces? All coins were insulated during the entire procedure, so they will retain their original charges: Penny: +5 nC; nickel: 0; dime: 0. The penny’s charge will have induced an equal and opposite negative charge (-5 nC) on the inside wall of the can and lid. This left a charge layer of +5 nC on the outside surface which was neutralized by the ground connection. Therefore, the can retained a net charge of −5 nC after disassembly. b) If the penny had been given a charge of +5 nC, the dime a charge of −2 nC, and the nickel a charge of −1 nC, what would the final charge arrangement have been? Again, since the coins are insulated, they retain their original charges. The charge induced on the inside wall of the can and lid is equal to negative the sum of the coin charges, or −2 nC. This is the charge that the can/lid contraption retains after grounding and disassembly. 3.2. A point charge of 12 nC is located at the origin. four uniform line charges are located in the x = 0 plane as follows: 80 nC/m at y = −1 and −5 m, −50 nC/m at y = −2 and −4 m. a) Find D at P (0, −3, 2): Note that this point lies in the center of a symmetric arrangement of line charges, whose fields will all cancel at that point. Thus D arise from the point charge alone, and will be D = 12 × 10−9(−3ay + 2az) 4π(32 + 22)1.5 = −6.11 × 10−11 ay + 4.07 × 10−11 az C/m2 = −61.1ay + 40.7az pC/m2 b) How much electric flux crosses the plane y = −3 and in what direction? The plane intercepts all flux that enters the −y half-space, or exactly half the total flux of 12 nC. The answer is thus 6 nC and in the −ay direction. c) How much electric flux leaves the surface of a sphere, 4m in radius, centered at C(0, −3, 0)? This sphere encloses the point charge, so its flux of 12 nC is included. The line charge contributions are most easily found by translating the whole assembly (sphere and line charges) such that the sphere is centered at the origin, with line charges now at y = ±1 and ±2. The flux from the line charges will equal the total line charge that lies within the sphere. The length of each of the inner two line charges (at y = ±1) will be h1 = 2r cos θ1 = 2(4) cos sin−1 1 4 = 1.94 m That of each of the outer two line charges (at y = ±2) will be h2 = 2r cos θ2 = 2(4) cos sin−1 2 4 = 1.73 m 27 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 30. 3.2c. (continued) The total charge enclosed in the sphere (and the outward flux from it) is now Ql + Qp = 2(1.94)(−50 × 10−9 ) + 2(1.73)(80 × 10−9 ) + 12 × 10−9 = 348 nC 3.3. The cylindrical surface ρ = 8 cm contains the surface charge density, ρs = 5e−20|z| nC/m2. a) What is the total amount of charge present? We integrate over the surface to find: Q = 2 ∞ 0 2π 0 5e−20z (.08)dφ dz nC = 20π(.08) −1 20 e−20z ∞ 0 = 0.25 nC b) How much flux leaves the surface ρ = 8 cm, 1 cm < z < 5cm, 30◦ < φ < 90◦? We just integrate the charge density on that surface to find the flux that leaves it. = Q′ = .05 .01 90◦ 30◦ 5e−20z (.08) dφ dz nC = 90 − 30 360 2π(5)(.08) −1 20 e−20z .05 .01 = 9.45 × 10−3 nC = 9.45 pC 3.4. The cylindrical surfaces ρ = 1, 2, and 3 cm carry uniform surface charge densities of 20, −8, and 5 nC/m2, respectively. a) How much electric flux passes through the closed surface ρ = 5 cm, 0 < z < 1 m? Since the densities are uniform, the flux will be = 2π(aρs1 + bρs2 + cρs3)(1 m) = 2π [(.01)(20) − (.02)(8) + (.03)(5)] × 10−9 = 1.2 nC b) Find D at P (1 cm, 2 cm, 3 cm): This point lies at radius √ 5 cm, and is thus inside the outermost charge layer. This layer, being of uniform density, will not contribute to D at P . We know that in cylindrical coordinates, the layers at 1 and 2 cm will produce the flux density: D = Dρaρ = aρs1 + bρs2 ρ aρ or Dρ = (.01)(20) + (.02)(−8) √ .05 = 1.8 nC/m2 At P , φ = tan−1(2/1) = 63.4◦. Thus Dx = 1.8 cos φ = 0.8 and Dy = 1.8 sin φ = 1.6. Finally, DP = (0.8ax + 1.6ay) nC/m2 28 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 31. 3.5. Let D = 4xyax + 2(x2 + z2)ay + 4yzaz C/m2 and evaluate surface integrals to find the total charge enclosed in the rectangular parallelepiped 0 < x < 2, 0 < y < 3, 0 < z < 5 m: Of the 6 surfaces to consider, only 2 will contribute to the net outward flux. Why? First consider the planes at y = 0 and 3. The y component of D will penetrate those surfaces, but will be inward at y = 0 and outward at y = 3, while having the same magnitude in both cases. These fluxes will thus cancel. At the x = 0 plane, Dx = 0 and at the z = 0 plane, Dz = 0, so there will be no flux contributions from these surfaces. This leaves the 2 remaining surfaces at x = 2 and z = 5. The net outward flux becomes: = 5 0 3 0 D x=2 · ax dy dz + 3 0 2 0 D z=5 · az dx dy = 5 3 0 4(2)y dy + 2 3 0 4(5)y dy = 360 C 3.6. Two uniform line charges, each 20 nC/m, are located at y = 1, z = ±1 m. Find the total flux leaving a sphere of radius 2 m if it is centered at a) A(3, 1, 0): The result will be the same if we move the sphere to the origin and the line charges to (0, 0, ±1). The length of the line charge within the sphere is given by l = 4 sin[cos−1(1/2)] = 3.46. With two line charges, symmetrically arranged, the total charge enclosed is given by Q = 2(3.46)(20 nC/m) = 139 nC b) B(3, 2, 0): In this case the result will be the same if we move the sphere to the origin and keep the charges where they were. The length of the line joining the origin to the midpoint of the line charge (in the yz plane) is l1 = √ 2. The length of the line joining the origin to either endpoint of the line charge is then just the sphere radius, or 2. The half-angle subtended at the origin by the line charge is then ψ = cos−1( √ 2/2) = 45◦. The length of each line charge in the sphere is then l2 = 2 × 2 sin ψ = 2 √ 2. The total charge enclosed (with two line charges) is now Q′ = 2(2 √ 2)(20 nC/m) = 113 nC 3.7. Volume charge density is located in free space as ρv = 2e−1000r nC/m3 for 0 < r < 1 mm, and ρv = 0 elsewhere. a) Find the total charge enclosed by the spherical surface r = 1 mm: To find the charge we integrate: Q = 2π 0 π 0 .001 0 2e−1000r r2 sin θ dr dθ dφ Integration over the angles gives a factor of 4π. The radial integration we evaluate using tables; we obtain Q = 8π −r2e−1000r 1000 .001 0 + 2 1000 e−1000r (1000)2 (−1000r − 1) .001 0 = 4.0 × 10−9 nC b) By using Gauss’s law, calculate the value of Dr on the surface r = 1 mm: The gaussian surface is a spherical shell of radius 1 mm. The enclosed charge is the result of part a. We thus write 4πr2Dr = Q, or Dr = Q 4πr2 = 4.0 × 10−9 4π(.001)2 = 3.2 × 10−4 nC/m2 29 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 32. 3.8. Uniform line charges of 5 nC/m ar located in free space at x = 1, z = 1, and at y = 1, z = 0. a) Obtain an expression for D in cartesian coordinates at P (0, 0, z). In general, we have D(z) = ρs 2π r1 − r′ 1 |r1 − r′ 1|2 + r2 − r′ 2 |r2 − r′ 2|2 where r1 = r2 = zaz, r′ 1 = ay, and r′ 2 = ax + az. Thus D(z) = ρs 2π [zaz − ay] [1 + z2] + [(z − 1)az − ax] [1 + (z − 1)2] = ρs 2π −ax [1 + (z − 1)2] − ay [1 + z2] + (z − 1) [1 + (z − 1)2] + z [1 + z2] az b) Plot |D| vs. z at P , −3 < z < 10: Using part a, we find the magnitude of D to be |D| = ρs 2π 1 [1 + (z − 1)2]2 + 1 [1 + z2]2 + (z − 1) [1 + (z − 1)2] + z [1 + z2] 2 1/2 A plot of this over the specified range is shown in Prob3.8.pdf. 3.9. A uniform volume charge density of 80 µC/m3 is present throughout the region 8 mm < r < 10 mm. Let ρv = 0 for 0 < r < 8 mm. a) Find the total charge inside the spherical surface r = 10 mm: This will be Q = 2π 0 π 0 .010 .008 (80 × 10−6 )r2 sin θ dr dθ dφ = 4π × (80 × 10−6 ) r3 3 .010 .008 = 1.64 × 10−10 C = 164 pC b) Find Dr at r = 10 mm: Using a spherical gaussian surface at r = 10, Gauss’ law is written as 4πr2Dr = Q = 164 × 10−12, or Dr(10 mm) = 164 × 10−12 4π(.01)2 = 1.30 × 10−7 C/m2 = 130 nC/m2 c) If there is no charge for r > 10 mm, find Dr at r = 20 mm: This will be the same computation as in part b, except the gaussian surface now lies at 20 mm. Thus Dr(20 mm) = 164 × 10−12 4π(.02)2 = 3.25 × 10−8 C/m2 = 32.5 nC/m2 3.10. Let ρs = 8 µC/m2 in the region where x = 0 and −4 < z < 4 m, and let ρs = 0 elsewhere. Find D at P (x, 0, z), where x > 0: The sheet charge can be thought of as an assembly of infinitely-long parallel strips that lie parallel to the y axis in the yz plane, and where each is of thickness dz. The field from each strip is that of an infinite line charge, and so we can construct the field at P from a single strip as: dDP = ρs dz′ 2π r − r′ |r − r′|2 30 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 33. 3.10 (continued) where r = xax + zaz and r′ = z′az We distinguish between the fixed coordinate of P , z, and the variable coordinate, z′, that determines the location of each charge strip. To find the net field at P, we sum the contributions of each strip by integrating over z′: DP = 4 −4 8 × 10−6 dz′ (xax + (z − z′)az) 2π[x2 + (z − z′)2] We can re-arrange this to determine the integral forms: DP = 8 × 10−6 2π (xax + zaz) 4 −4 dz′ (x2 + z2) − 2zz′ + (z′)2 − az 4 −4 z′ dz′ (x2 + z2) − 2zz′ + (z′)2 Using integral tables, we find DP = 4 × 10−6 π (xax + zaz) 1 x tan−1 2z′ − 2z 2x − 1 2 ln(x2 + z2 − 2zz′ + (z′ )2 ) + 2z 2 1 x tan−1 2z′ − 2z 2x az 4 −4 which evaluates as DP = 4 × 10−6 π tan−1 z + 4 x − tan−1 z − 4 x ax + 1 2 ln x2 + (z + 4)2 x2 + (z − 4)2 az C/m2 The student is invited to verify that for very small x or for a very large sheet (allowing z′ to approach infinity), the above expression reduces to the expected form, DP = ρs/2. Note also that the expression is valid for all x (positive or negative values). 3.11. In cylindrical coordinates, let ρv = 0 for ρ < 1 mm, ρv = 2 sin(2000πρ) nC/m3 for 1 mm < ρ < 1.5 mm, and ρv = 0 for ρ > 1.5 mm. Find D everywhere: Since the charge varies only with radius, and is in the form of a cylinder, symmetry tells us that the flux density will be radially-directed and will be constant over a cylindrical surface of a fixed radius. Gauss’ law applied to such a surface of unit length in z gives: a) for ρ < 1 mm, Dρ = 0, since no charge is enclosed by a cylindrical surface whose radius lies within this range. b) for 1 mm < ρ < 1.5 mm, we have 2πρDρ = 2π ρ .001 2 × 10−9 sin(2000πρ′ )ρ′ dρ′ = 4π × 10−9 1 (2000π)2 sin(2000πρ) − ρ 2000π cos(2000πρ) ρ .001 or finally, Dρ = 10−15 2π2ρ sin(2000πρ) + 2π 1 − 103 ρ cos(2000πρ) C/m2 (1 mm < ρ < 1.5 mm) 31 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 34. 3.11. (continued) c) for ρ > 1.5 mm, the gaussian cylinder now lies at radius ρ outside the charge distribution, so the integral that evaluates the enclosed charge now includes the entire charge distribution. To accomplish this, we change the upper limit of the integral of part b from ρ to 1.5 mm, finally obtaining: Dρ = 2.5 × 10−15 πρ C/m2 (ρ > 1.5 mm) 3.12. A nonuniform volume charge density, ρv = 120r C/m3, lies within the spherical surface r = 1 m, and ρv = 0 everywhere else. a) Find Dr everywhere. For r < 1 m, we apply Gauss’ law to a spherical surface of radius r within this range to find 4πr2 Dr = 4π r 0 120r′ (r′ )2 dr′ = 120πr4 Thus Dr = (30r2) for r < 1 m. For r > 1 m, the gaussian surface lies outside the charge distribution. The set up is the same, except the upper limit of the above integral is 1 instead of r. This results in Dr = (30/r2) for r > 1 m. b) What surface charge density, ρs2, should be on the surface r = 2 such that Dr,r=2− = 2Dr,r=2+? At r = 2−, we have Dr,r=2− = 30/22 = 15/2, from part a. The flux density in the region r > 2 arising from a surface charge at r = 2 is found from Gauss’ law through 4πr2 Drs = 4π(2)2 ρs2 ⇒ Drs = 4ρs2 r2 The total flux density in the region r > 2 arising from the two distributions is DrT = 30 r2 + 4ρs2 r2 Our requirement that Dr,r=2− = 2Dr,r=2+ becomes 30 22 = 2 30 22 + ρs2 ⇒ ρs2 = − 15 4 C/m2 c) Make a sketch of Dr vs. r for 0 < r < 5 m with both distributions present. With both charges, Dr(r < 1) = 30r2, Dr(1 < r < 2) = 30/r2, and Dr(r > 2) = 15/r2. These are plotted on the next page. 32 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 35. . 3.13. Spherical surfaces at r = 2, 4, and 6 m carry uniform surface charge densities of 20 nC/m2, −4 nC/m2, and ρs0, respectively. a) Find D at r = 1, 3 and 5 m: Noting that the charges are spherically-symmetric, we ascertain that D will be radially-directed and will vary only with radius. Thus, we apply Gauss’ law to spherical shells in the following regions: r < 2: Here, no charge is enclosed, and so Dr = 0. 2 < r < 4 : 4πr2 Dr = 4π(2)2 (20 × 10−9 ) ⇒ Dr = 80 × 10−9 r2 C/m2 So Dr(r = 3) = 8.9 × 10−9 C/m2. 4 < r < 6 : 4πr2 Dr = 4π(2)2 (20 × 10−9 ) + 4π(4)2 (−4 × 10−9 ) ⇒ Dr = 16 × 10−9 r2 So Dr(r = 5) = 6.4 × 10−10 C/m2. b) Determine ρs0 such that D = 0 at r = 7 m. Since fields will decrease as 1/r2, the question could be re-phrased to ask for ρs0 such that D = 0 at all points where r > 6 m. In this region, the total field will be Dr(r > 6) = 16 × 10−9 r2 + ρs0(6)2 r2 Requiring this to be zero, we find ρs0 = −(4/9) × 10−9 C/m2. 3.14. If ρv = 5 nC/m3 for 0 < ρ < 1 mm and no other charges are present: a) find Dρ for ρ < 1 mm: Applying Gauss’ law to a cylindrical surface of unit length in z, and of radius ρ < 1 mm, we find 2πρDρ = πρ2 (5 × 10−9 ) ⇒ Dρ = 2.5 ρ × 10−9 C/m2 33 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 36. 3.14b. find Dρ for ρ > 1 mm: The Gaussian cylinder now lies outside the charge, so 2πρDρ = π(.001)2 (5 × 10−9 ) ⇒ Dρ = 2.5 × 10−15 ρ C/m2 c) What line charge ρL at ρ = 0 would give the same result for part b? The line charge field will be Dr = ρL 2πρ = 2.5 × 10−15 ρ (part b) Thus ρL = 5π × 10−15 C/m. In all answers, ρ is expressed in meters. 3.15. Volume charge density is located as follows: ρv = 0 for ρ < 1 mm and for ρ > 2 mm, ρv = 4ρ µC/m3 for 1 < ρ < 2 mm. a) Calculate the total charge in the region 0 < ρ < ρ1, 0 < z < L, where 1 < ρ1 < 2 mm: We find Q = L 0 2π 0 ρ1 .001 4ρ ρ dρ dφ dz = 8πL 3 [ρ3 1 − 10−9 ] µC where ρ1 is in meters. b) Use Gauss’ law to determine Dρ at ρ = ρ1: Gauss’ law states that 2πρ1LDρ = Q, where Q is the result of part a. Thus Dρ(ρ1) = 4(ρ3 1 − 10−9) 3ρ1 µC/m2 where ρ1 is in meters. c) Evaluate Dρ at ρ = 0.8 mm, 1.6 mm, and 2.4 mm: At ρ = 0.8 mm, no charge is enclosed by a cylindrical gaussian surface of that radius, so Dρ(0.8mm) = 0. At ρ = 1.6 mm, we evaluate the part b result at ρ1 = 1.6 to obtain: Dρ(1.6mm) = 4[(.0016)3 − (.0010)3] 3(.0016) = 3.6 × 10−6 µC/m2 At ρ = 2.4, we evaluate the charge integral of part a from .001 to .002, and Gauss’ law is written as 2πρLDρ = 8πL 3 [(.002)2 − (.001)2 ] µC from which Dρ(2.4mm) = 3.9 × 10−6 µC/m2. 3.16. Given the electric flux density, D = 2xy ax + x2 ay + 6z3 az C/m2: a) use Gauss’ law to evaluate the total charge enclosed in the volume 0 < x, y, z < a: We call the surfaces at x = a and x = 0 the front and back surfaces respectively, those at y = a and y = 0 the right and left surfaces, and those at z = a and z = 0 the top and bottom surfaces. To evaluate the total charge, we integrate D · n over all six surfaces and sum the results: = Q = D · n da = a 0 a 0 2ay dy dz front + a 0 a 0 −2(0)y dy dz back + a 0 a 0 −x2 dx dz left + a 0 a 0 x2 dx dz right + a 0 a 0 −6(0)3 dx dy bottom + a 0 a 0 6a3 dx dy top 34 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 37. 3.16a. (continued) Noting that the back and bottom integrals are zero, and that the left and right integrals cancel, we evaluate the remaining two (front and top) to obtain Q = 6a5 + a4. b) use Eq. (8) to find an approximate value for the above charge. Evaluate the derivatives at P (a/2, a/2, a/2): In this application, Eq. (8) states that Q . = (∇ · D P ) v. We find ∇ · D = 2x +18z2, which when evaluated at P becomes ∇ ·D P = a +4.5a2. Thus Q . = (a +4.5a2)a3 = 4.5a5 + a4 c) Show that the results of parts a and b agree in the limit as a → 0. In this limit, both expressions reduce to Q = a4, and so they agree. 3.17. A cube is defined by 1 < x, y, z < 1.2. If D = 2x2yax + 3x2y2ay C/m2: a) apply Gauss’ law to find the total flux leaving the closed surface of the cube. We call the surfaces at x = 1.2 and x = 1 the front and back surfaces respectively, those at y = 1.2 and y = 1 the right and left surfaces, and those at z = 1.2 and z = 1 the top and bottom surfaces. To evaluate the total charge, we integrate D · n over all six surfaces and sum the results. We note that there is no z component of D, so there will be no outward flux contributions from the top and bottom surfaces. The fluxes through the remaining four are = Q = D · n da = 1.2 1 1.2 1 2(1.2)2 y dy dz front + 1.2 1 1.2 1 −2(1)2 y dy dz back + 1.2 1 1.2 1 −3x2 (1)2 dx dz left + 1.2 1 1.2 1 3x2 (1.2)2 dx dz right = 0.1028 C b) evaluate ∇ · D at the center of the cube: This is ∇ · D = 4xy + 6x2 y (1.1,1.1) = 4(1.1)2 + 6(1.1)3 = 12.83 c) Estimate the total charge enclosed within the cube by using Eq. (8): This is Q . = ∇ · D center × v = 12.83 × (0.2)3 = 0.1026 Close! 3.18. Let a vector field by given by G = 5x4y4z4 ay. Evaluate both sides of Eq. (8) for this G field and the volume defined by x = 3 and 3.1, y = 1 and 1.1, and z = 2 and 2.1. Evaluate the partial derivatives at the center of the volume. First find ∇ · G = ∂Gy ∂y = 20x4 y3 z4 The center of the cube is located at (3.05,1.05,2.05), and the volume is v = (0.1)3 = 0.001. Eq. (8) then becomes . = 20(3.05)4 (1.05)3 (2.05)4 (0.001) = 35.4 35 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 38. 3.19. A spherical surface of radius 3 mm is centered at P (4, 1, 5) in free space. Let D = xax C/m2. Use the results of Sec. 3.4 to estimate the net electric flux leaving the spherical surface: We use . = ∇ · D v, where in this case ∇ · D = (∂/∂x)x = 1 C/m3. Thus . = 4 3 π(.003)3 (1) = 1.13 × 10−7 C = 113 nC 3.20. A cube of volume a3 has its faces parallel to the cartesian coordinate surfaces. It is centered at P (3, −2, 4). Given the field D = 2x3ax C/m2: a) calculate div D at P : In the present case, this will be ∇ · D = ∂Dx ∂x = dDx dx = 54 C/m3 b) evaluate the fraction in the rightmost side of Eq. (13) for a = 1 m, 0.1 m, and 1 mm: With the field having only an x component, flux will pentrate only the two surfaces at x = 3 ± a/2, each of which has surface area a2. The cube volume is v = a3. The equation reads: D · dS v = 1 a3 2 3 + a 2 3 a2 − 2 3 − a 2 3 a2 = 2 a (3 + a 2 )3 − (3 − a 2 )3 evaluating the above formula at a = 1 m, .1 m, and 1 mm, yields respectively 54.50, 54.01, and 54.00 C/m3 , thus demonstrating the approach to the exact value as v gets smaller. 3.21. Calculate the divergence of D at the point specified if a) D = (1/z2) 10xyz ax + 5x2z ay + (2z3 − 5x2y) az at P (−2, 3, 5): We find ∇ · D = 10y z + 0 + 2 + 10x2y z3 (−2,3,5) = 8.96 b) D = 5z2aρ + 10ρz az at P (3, −45◦, 5): In cylindrical coordinates, we have ∇ · D = 1 ρ ∂ ∂ρ (ρDρ) + 1 ρ ∂Dφ ∂φ + ∂Dz ∂z = 5z2 ρ + 10ρ (3,−45◦,5) = 71.67 c) D = 2r sin θ sin φ ar + r cos θ sin φ aθ + r cos φ aφ at P (3, 45◦, −45◦): In spherical coordinates, we have ∇ · D = 1 r2 ∂ ∂r (r2 Dr) + 1 r sin θ ∂ ∂θ (sin θDθ ) + 1 r sin θ ∂Dφ ∂φ = 6 sin θ sin φ + cos 2θ sin φ sin θ − sin φ sin θ (3,45◦,−45◦) = −2 36 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 39. 3.22. Let D = 8ρ sin φ aρ + 4ρ cos φ aφ C/m2. a) Find div D: Using the divergence formula for cylindrical coordinates (see problem 3.21), we find ∇ · D = 12 sin φ. b) Find the volume charge density at P (2.6, 38◦, −6.1): Since ρv = ∇ · D, we evaluate the result of part a at this point to find ρvP = 12 sin 38◦ = 7.39 C/m3. c) How much charge is located inside the region defined by 0 < ρ < 1.8, 20◦ < φ < 70◦, 2.4 < z < 3.1? We use Q = vol ρvdv = 3.1 2.4 70◦ 20◦ 1.8 0 12 sin φρ dρ dφ dz = −(3.1 − 2.4)12 cos φ 70◦ 20◦ ρ2 2 1.8 0 = 8.13 C 3.23. a) A point charge Q lies at the origin. Show that div D is zero everywhere except at the origin. For a point charge at the origin we know that D = Q/(4πr2) ar. Using the formula for divergence in spherical coordinates (see problem 3.21 solution), we find in this case that ∇ · D = 1 r2 d dr r2 Q 4πr2 = 0 The above is true provided r > 0. When r = 0, we have a singularity in D, so its divergence is not defined. b) Replace the point charge with a uniform volume charge density ρv0 for 0 < r < a. Relate ρv0 to Q and a so that the total charge is the same. Find div D everywhere: To achieve the same net charge, we require that (4/3)πa3ρv0 = Q, so ρv0 = 3Q/(4πa3) C/m3. Gauss’ law tells us that inside the charged sphere 4πr2 Dr = 4 3 πr3 ρv0 = Qr3 a3 Thus Dr = Qr 4πa3 C/m2 and ∇ · D = 1 r2 d dr Qr3 4πa3 = 3Q 4πa3 as expected. Outside the charged sphere, D = Q/(4πr2) ar as before, and the divergence is zero. 3.24. Inside the cylindrical shell, 3 < ρ < 4 m, the electric flux density is given as D = 5(ρ − 3)3 aρ C/m2 a) What is the volume charge density at ρ = 4 m? In this case we have ρv = ∇ · D = 1 ρ d dρ (ρDρ) = 1 ρ d dρ [5ρ(ρ − 3)3 ] = 5(ρ − 3)2 ρ (4ρ − 3) C/m3 Evaluating this at ρ = 4 m, we find ρv(4) = 16.25 C/m3 b) What is the electric flux density at ρ = 4 m? We evaluate the given D at this point to find D(4) = 5 aρ C/m2 37 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 40. 3.24c. How much electric flux leaves the closed surface 3 < ρ < 4, 0 < φ < 2π, −2.5 < z < 2.5? We note that D has only a radial component, and so flux would leave only through the cylinder sides. Also, D does not vary with φ or z, so the flux is found by a simple product of the side area and the flux density. We further note that D = 0 at ρ = 3, so only the outer side (at ρ = 4) will contribute. We use the result of part b, and write the flux as = [2.5 − (−2.5)]2π(4)(5) = 200π C d) How much charge is contained within the volume used in part c? By Gauss’ law, this will be the same as the net outward flux through that volume, or again, 200π C. 3.25. Within the spherical shell, 3 < r < 4 m, the electric flux density is given as D = 5(r − 3)3 ar C/m2 a) What is the volume charge density at r = 4? In this case we have ρv = ∇ · D = 1 r2 d dr (r2 Dr) = 5 r (r − 3)2 (5r − 6) C/m3 which we evaluate at r = 4 to find ρv(r = 4) = 17.50 C/m3. b) What is the electric flux density at r = 4? Substitute r = 4 into the given expression to find D(4) = 5 ar C/m2 c) How much electric flux leaves the sphere r = 4? Using the result of part b, this will be = 4π(4)2(5) = 320π C d) How much charge is contained within the sphere, r = 4? From Gauss’ law, this will be the same as the outward flux, or again, Q = 320π C. 3.26. Given the field D = 5 sin θ cos φ r ar C/m2 , find: a) the volume charge density: Use ρv = ∇ · D = 1 r2 d dr (r2 Dr) = 5 sin θ cos φ r2 C/m3 b) the total charge contained within the region r < 2 m: To find this, we integrate over the volume: Q = 2π 0 π 0 2 0 5 sin θ cos φ r2 r2 sin θ dr dθ dφ Before plunging into this one notice that the φ integration is of cos φ from zero to 2π. This yields a zero result, and so the total enclosed charge is Q = 0. c) the value of D at the surface r = 2: Substituting r = 2 into the given field produces D(r = 2) = 5 2 sin θ cos φ ar C/m2 38 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 41. 3.26d. the total electric flux leaving the surface r = 2 Since the total enclosed charge is zero (from part b), the net outward flux is also zero, from Gauss’ law. 3.27. Let D = 5.00r2ar mC/m2 for r ≤ 0.08 m and D = 0.205 ar/r2 µC/m2 for r ≥ 0.08 m (note error in problem statement). a) Find ρv for r = 0.06 m: This radius lies within the first region, and so ρv = ∇ · D = 1 r2 d dr (r2 Dr) = 1 r2 d dr (5.00r4 ) = 20r mC/m3 which when evaluated at r = 0.06 yields ρv(r = .06) = 1.20 mC/m3. b) Find ρv for r = 0.1 m: This is in the region where the second field expression is valid. The 1/r2 dependence of this field yields a zero divergence (shown in Problem 3.23), and so the volume charge density is zero at 0.1 m. c) What surface charge density could be located at r = 0.08 m to cause D = 0 for r > 0.08 m? The total surface charge should be equal and opposite to the total volume charge. The latter is Q = 2π 0 π 0 .08 0 20r(mC/m3 ) r2 sin θ dr dθ dφ = 2.57 × 10−3 mC = 2.57 µC So now ρs = − 2.57 4π(.08)2 = −32 µC/m2 3.28. The electric flux density is given as D = 20ρ3 aρ C/m2 for ρ < 100 µm, and k aρ/ρ for ρ > 100 µm. a) Find k so that D is continuous at ρ = 100 µm: We require 20 × 10−12 = k 10−4 ⇒ k = 2 × 10−15 C/m b) Find and sketch ρv as a function of ρ: In cylindrical coordinates, with only a radial component of D, we use ρv = ∇ · D = 1 ρ ∂ ∂ρ (ρDρ) = 1 ρ ∂ ∂ρ (20ρ4 ) = 80ρ2 C/m3 (ρ < 100 µm) For ρ > 100 µm, we obtain ρv = 1 ρ ∂ ∂ρ (ρ k ρ ) = 0 The sketch of ρv vs. ρ would be a parabola, starting at the origin, reaching a maximum value of 8 × 10−7 C/m3 at ρ = 100 µm. The plot is zero at larger radii. 3.29. In the region of free space that includes the volume 2 < x, y, z < 3, D = 2 z2 (yz ax + xz ay − 2xy az) C/m2 a) Evaluate the volume integral side of the divergence theorem for the volume defined above: In cartesian, we find ∇ · D = 8xy/z3. The volume integral side is now vol ∇ · D dv = 3 2 3 2 3 2 8xy z3 dxdydz = (9 − 4)(9 − 4) 1 4 − 1 9 = 3.47 C 39 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 42. 3.29b. Evaluate the surface integral side for the corresponding closed surface: We call the surfaces at x = 3 and x = 2 the front and back surfaces respectively, those at y = 3 and y = 2 the right and left surfaces, and those at z = 3 and z = 2 the top and bottom surfaces. To evaluate the surface integral side, we integrate D · n over all six surfaces and sum the results. Note that since the x component of D does not vary with x, the outward fluxes from the front and back surfaces will cancel each other. The same is true for the left and right surfaces, since Dy does not vary with y. This leaves only the top and bottom surfaces, where the fluxes are: D · dS = 3 2 3 2 −4xy 32 dxdy top − 3 2 3 2 −4xy 22 dxdy bottom = (9 − 4)(9 − 4) 1 4 − 1 9 = 3.47 C 3.30. If D = 15ρ2 sin 2φ aρ + 10ρ2 cos 2φ aφ C/m2, evaluate both sides of the divergence theorem for the region 1 < ρ < 2 m, 1 < φ < 2 rad, 1 < z < 2 m: Taking the surface integral side first, the six sides over which the flux must be evaluated are only four, since there is no z component of D. We are left with the sides at φ = 1 and φ = 2 rad (left and right sides, respectively), and those at ρ = 1 and ρ = 2 (back and front sides). We evaluate D · dS = 2 1 2 1 15(2)2 sin(2φ) (2)dφdz front − 2 1 2 1 15(1)2 sin(2φ) (1)dφdz back − 2 1 2 1 10ρ2 cos(2) dρdz left + 2 1 2 1 10ρ2 cos(4) dρdz right = 6.93 C For the volume integral side, we first evaluate the divergence of D, which is ∇ · D = 1 ρ ∂ ∂ρ (15ρ3 sin 2φ) + 1 ρ ∂ ∂φ (10ρ2 cos 2φ) = 25ρ sin 2φ Next vol ∇ · D dv = 2 1 2 1 2 1 25ρ sin(2φ) ρdρ dφ dz = 25 3 ρ3 2 1 − cos(2φ) 2 2 1 = 6.93 C 3.31. Given the flux density D = 16 r cos(2θ) aθ C/m2 , use two different methods to find the total charge within the region 1 < r < 2 m, 1 < θ < 2 rad, 1 < φ < 2 rad: We use the divergence theorem and first evaluate the surface integral side. We are evaluating the net outward flux through a curvilinear “cube”, whose boundaries are defined by the specified ranges. The flux contributions will be only through the surfaces of constant θ, however, since D has only a θ component. On a constant-theta surface, the differential area is da = r sin θdrdφ, where θ is fixed at the surface location. Our flux integral becomes D · dS = − 2 1 2 1 16 r cos(2) r sin(1) drdφ θ=1 + 2 1 2 1 16 r cos(4) r sin(2) drdφ θ=2 = −16 [cos(2) sin(1) − cos(4) sin(2)] = −3.91 C 40 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 43. 3.31. (continued) We next evaluate the volume integral side of the divergence theorem, where in this case, ∇ · D = 1 r sin θ d dθ (sin θ Dθ ) = 1 r sin θ d dθ 16 r cos 2θ sin θ = 16 r2 cos 2θ cos θ sin θ − 2 sin 2θ We now evaluate: vol ∇ · D dv = 2 1 2 1 2 1 16 r2 cos 2θ cos θ sin θ − 2 sin 2θ r2 sin θ drdθdφ The integral simplifies to 2 1 2 1 2 1 16[cos 2θ cos θ − 2 sin 2θ sin θ] drdθdφ = 8 2 1 [3 cos 3θ − cos θ] dθ = −3.91 C 3.32. If D = 2r ar C/m2, find the total electric flux leaving the surface of the cube, 0 < x, y, z < 0.4: This is where the divergence theorem really saves you time! First find ∇ · D = 1 r2 d dr (r2 × 2r) = 6 Then the net outward flux will be vol ∇ · D dv = 6(0.4)3 = 0.38 C 41 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 44. CHAPTER 4 4.1. The value of E at P (ρ = 2, φ = 40◦, z = 3) is given as E = 100aρ −200aφ +300az V/m. Determine the incremental work required to move a 20 µC charge a distance of 6 µm: a) in the direction of aρ: The incremental work is given by dW = −q E · dL, where in this case, dL = dρ aρ = 6 × 10−6 aρ. Thus dW = −(20 × 10−6 C)(100 V/m)(6 × 10−6 m) = −12 × 10−9 J = −12 nJ b) in the direction of aφ: In this case dL = 2 dφ aφ = 6 × 10−6 aφ, and so dW = −(20 × 10−6 )(−200)(6 × 10−6 ) = 2.4 × 10−8 J = 24 nJ c) in the direction of az: Here, dL = dz az = 6 × 10−6 az, and so dW = −(20 × 10−6 )(300)(6 × 10−6 ) = −3.6 × 10−8 J = −36 nJ d) in the direction of E: Here, dL = 6 × 10−6 aE, where aE = 100aρ − 200aφ + 300az [1002 + 2002 + 3002]1/2 = 0.267 aρ − 0.535 aφ + 0.802 az Thus dW = −(20 × 10−6 )[100aρ − 200aφ + 300az] · [0.267 aρ − 0.535 aφ + 0.802 az](6 × 10−6 ) = −44.9 nJ e) In the direction of G = 2 ax − 3 ay + 4 az: In this case, dL = 6 × 10−6 aG, where aG = 2ax − 3ay + 4az [22 + 32 + 42]1/2 = 0.371 ax − 0.557 ay + 0.743 az So now dW = −(20 × 10−6 )[100aρ − 200aφ + 300az] · [0.371 ax − 0.557 ay + 0.743 az](6 × 10−6 ) = −(20 × 10−6 ) 37.1(aρ · ax) − 55.7(aρ · ay) − 74.2(aφ · ax) + 111.4(aφ · ay) + 222.9] (6 × 10−6 ) where, at P , (aρ · ax) = (aφ · ay) = cos(40◦) = 0.766, (aρ · ay) = sin(40◦) = 0.643, and (aφ · ax) = − sin(40◦) = −0.643. Substituting these results in dW = −(20 × 10−6 )[28.4 − 35.8 + 47.7 + 85.3 + 222.9](6 × 10−6 ) = −41.8 nJ 42 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 45. 4.2. Let E = 400ax − 300ay + 500az in the neighborhood of point P (6, 2, −3). Find the incremental work done in moving a 4-C charge a distance of 1 mm in the direction specified by: a) ax + ay + az: We write dW = −qE · dL = −4(400ax − 300ay + 500az) · (ax + ay + az) √ 3 (10−3 ) = − (4 × 10−3) √ 3 (400 − 300 + 500) = −1.39 J b) −2ax + 3ay − az: The computation is similar to that of part a, but we change the direction: dW = −qE · dL = −4(400ax − 300ay + 500az) · (−2ax + 3ay − az) √ 14 (10−3 ) = − (4 × 10−3) √ 14 (−800 − 900 − 500) = 2.35 J 4.3. If E = 120 aρ V/m, find the incremental amount of work done in moving a 50 µm charge a distance of 2 mm from: a) P (1, 2, 3) toward Q(2, 1, 4): The vector along this direction will be Q − P = (1, −1, 1) from which aPQ = [ax − ay + az]/ √ 3. We now write dW = −qE · dL = −(50 × 10−6 ) 120aρ · (ax − ay + az √ 3 (2 × 10−3 ) = −(50 × 10−6 )(120) (aρ · ax) − (aρ · ay) 1 √ 3 (2 × 10−3 ) At P, φ = tan−1(2/1) = 63.4◦. Thus (aρ · ax) = cos(63.4) = 0.447 and (aρ · ay) = sin(63.4) = 0.894. Substituting these, we obtain dW = 3.1 µJ. b) Q(2, 1, 4) toward P (1, 2, 3): A little thought is in order here: Note that the field has only a radial component and does not depend on φ or z. Note also that P and Q are at the same radius ( √ 5) from the z axis, but have different φ and z coordinates. We could just as well position the two points at the same z location and the problem would not change. If this were so, then moving along a straight line between P and Q would thus involve moving along a chord of a circle whose radius is √ 5. Halfway along this line is a point of symmetry in the field (make a sketch to see this). This means that when starting from either point, the initial force will be the same. Thus the answer is dW = 3.1 µJ as in part a. This is also found by going through the same procedure as in part a, but with the direction (roles of P and Q) reversed. 4.4. Find the amount of energy required to move a 6-C charge from the origin to P (3, 1, −1) in the field E = 2xax − 3y2ay + 4az V/m along the straight-line path x = −3z, y = x + 2z: We set up the computation as follows, and find the the result does not depend on the path. W = −q E · dL = −6 (2xax − 3y2 ay + 4az) · (dxax + dyay + dzaz) = −6 3 0 2xdx + 6 1 0 3y2 dy − 6 −1 0 4dz = −24 J 43 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 46. 4.5. Compute the value of P A G · dL for G = 2yax with A(1, −1, 2) and P (2, 1, 2) using the path: a) straight-line segments A(1, −1, 2) to B(1, 1, 2) to P (2, 1, 2): In general we would have P A G · dL = P A 2y dx The change in x occurs when moving between B and P , during which y = 1. Thus P A G · dL = P B 2y dx = 2 1 2(1)dx = 2 b) straight-line segments A(1, −1, 2) to C(2, −1, 2) to P (2, 1, 2): In this case the change in x occurs when moving from A to C, during which y = −1. Thus P A G · dL = C A 2y dx = 2 1 2(−1)dx = −2 4.6. Let G = 4xax +2zay +2yaz. Given an initial point P (2, 1, 1) and a final point Q(4, 3, 1), find G·dL using the path: a) straight line: y = x − 1, z = 1; b) parabola: 6y = x2 + 2, z = 1: With G as given, the line integral will be G · dL = 4 2 4x dx + 3 1 2z dy + 1 1 2y dz Clearly, we are going nowhere in z, so the last integral is zero. With z = 1, the first two evaluate as G · dL = 2x2 4 2 + 2y 3 1 = 28 The paths specified in parts a and b did not play a role, meaning that the integral between the specified points is path-independent. 4.7. Repeat Problem 4.6 for G = 3xy3ax + 2zay. Now things are different in that the path does matter: a) straight line: y = x − 1, z = 1: We obtain: G · dL = 4 2 3xy2 dx + 3 1 2z dy = 4 2 3x(x − 1)2 dx + 3 1 2(1) dy = 90 b) parabola: 6y = x2 + 2, z = 1: We obtain: G · dL = 4 2 3xy2 dx + 3 1 2z dy = 4 2 1 12 x(x2 + 2)2 dx + 3 1 2(1) dy = 82 44 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 47. 4.8. A point charge Q1 is located at the origin in free space. Find the work done in carrying a charge Q2 from: (a) B(rB, θB, φB) to C(rA, θB, φB) with θ and φ held constant; (b) C(rA, θB, φB) to D(rA, θA, φB) with r and φ held constant; (c) D(rA, θA, φB) to A(rA, θA, φA) with r and θ held constant: The general expression for the work done in this instance is W = −Q2 E · dL = −Q2 Q1 4πǫ0r2 ar · (drar + rdθaθ + r sin θdφaφ) = − Q1Q2 4πǫ0 dr r2 We see that only changes in r will produce non-zero results. Thus for part a we have W = − Q1Q2 4πǫ0 rA rB dr r2 = Q1Q2 4πǫ0 1 rA − 1 rB J The answers to parts b and c (involving paths over which r is held constant) are both 0. 4.9. A uniform surface charge density of 20 nC/m2 is present on the spherical surface r = 0.6 cm in free space. a) Find the absolute potential at P (r = 1 cm, θ = 25◦, φ = 50◦): Since the charge density is uniform and is spherically-symmetric, the angular coordinates do not matter. The potential function for r > 0.6 cm will be that of a point charge of Q = 4πa2ρs, or V (r) = 4π(0.6 × 10−2)2(20 × 10−9) 4πǫ0r = 0.081 r V with r in meters At r = 1 cm, this becomes V (r = 1 cm) = 8.14 V b) Find VAB given points A(r = 2 cm, θ = 30◦, φ = 60◦) and B(r = 3 cm, θ = 45◦, φ = 90◦): Again, the angles do not matter because of the spherical symmetry. We use the part a result to obtain VAB = VA − VB = 0.081 1 0.02 − 1 0.03 = 1.36 V 4.10. Given a surface charge density of 8 nC/m2 on the plane x = 2, a line charge density of 30 nC/m on the line x = 1, y = 2, and a 1-µC point charge at P (−1, −1, 2), find VAB for points A(3, 4, 0) and B(4, 0, 1): We need to find a potential function for the combined charges. That for the point charge we know to be Vp(r) = Q 4πǫ0r Potential functions for the sheet and line charges can be found by taking indefinite integrals of the electric fields for those distributions. For the line charge, we have Vl(ρ) = − ρl 2πǫ0ρ dρ + C1 = − ρl 2πǫ0 ln(ρ) + C1 For the sheet charge, we have Vs(x) = − ρs 2ǫ0 dx + C2 = − ρs 2ǫ0 x + C2 45 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 48. 4.10. (continued) The total potential function will be the sum of the three. Combining the integration con- stants, we obtain: V = Q 4πǫ0r − ρl 2πǫ0 ln(ρ) − ρs 2ǫ0 x + C The terms in this expression are not referenced to a common origin, since the charges are at different positions. The parameters r, ρ, and x are scalar distances from the charges, and will be treated as such here. For point A we have rA = (3 − (−1))2 + (4 − (−1))2 + (−2)2 = √ 45, ρA = (3 − 1)2 + (4 − 2)2 = √ 8, and its distance from the sheet charge is xA = 3 − 2 = 1. The potential at A is then VA = 10−6 4πǫ0 √ 45 − 30 × 10−9 2πǫ0 ln √ 8 − 8 × 10−9 2ǫ0 (1) + C At point B, rB = (4 − (−1))2 + (0 − (−1))2 + (1 − 2)2 = √ 27, ρB = (4 − 1)2 + (0 − 2)2 = √ 13, and the distance from the sheet charge is xB = 4 − 2 = 2. The potential at A is then VB = 10−6 4πǫ0 √ 27 − 30 × 10−9 2πǫ0 ln √ 13 − 8 × 10−9 2ǫ0 (2) + C Then VA − VB = 10−6 4πǫ0 1 √ 45 − 1 √ 27 − 30 × 10−9 2πǫ0 ln 8 13 − 8 × 10−9 2ǫ0 (1 − 2) = 193 V 4.11. Let a uniform surface charge density of 5 nC/m2 be present at the z = 0 plane, a uniform line charge density of 8 nC/m be located at x = 0, z = 4, and a point charge of 2 µC be present at P (2, 0, 0). If V = 0 at M(0, 0, 5), find V at N(1, 2, 3): We need to find a potential function for the combined charges which is zero at M. That for the point charge we know to be Vp(r) = Q 4πǫ0r Potential functions for the sheet and line charges can be found by taking indefinite integrals of the electric fields for those distributions. For the line charge, we have Vl(ρ) = − ρl 2πǫ0ρ dρ + C1 = − ρl 2πǫ0 ln(ρ) + C1 For the sheet charge, we have Vs(z) = − ρs 2ǫ0 dz + C2 = − ρs 2ǫ0 z + C2 The total potential function will be the sum of the three. Combining the integration constants, we obtain: V = Q 4πǫ0r − ρl 2πǫ0 ln(ρ) − ρs 2ǫ0 z + C 46 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 49. 4.11. (continued) The terms in this expression are not referenced to a common origin, since the charges are at different positions. The parameters r, ρ, and z are scalar distances from the charges, and will be treated as such here. To evaluate the constant, C, we first look at point M, where VT = 0. At M, r = √ 22 + 52 = √ 29, ρ = 1, and z = 5. We thus have 0 = 2 × 10−6 4πǫ0 √ 29 − 8 × 10−9 2πǫ0 ln(1) − 5 × 10−9 2ǫ0 5 + C ⇒ C = −1.93 × 103 V At point N, r = √ 1 + 4 + 9 = √ 14, ρ = √ 2, and z = 3. The potential at N is thus VN = 2 × 10−6 4πǫ0 √ 14 − 8 × 10−9 2πǫ0 ln( √ 2) − 5 × 10−9 2ǫ0 (3) − 1.93 × 103 = 1.98 × 103 V = 1.98 kV 4.12. Three point charges, 0.4 µC each, are located at (0, 0, −1), (0, 0, 0), and (0, 0, 1), in free space. a) Find an expression for the absolute potential as a function of z along the line x = 0, y = 1: From a point located at position z along the given line, the distances to the three charges are R1 = (z − 1)2 + 1, R2 = √ z2 + 1, and R3 = (z + 1)2 + 1. The total potential will be V (z) = q 4πǫ0 1 R1 + 1 R2 + 1 R3 Using q = 4 × 10−7 C, this becomes V (z) = (3.6 × 103 ) 1 (z − 1)2 + 1 + 1 √ z2 + 1 + 1 (z + 1)2 + 1 V b) Sketch V (z). The sketch will show that V maximizes to a value of 8.68 × 103 at z = 0, and then monotonically decreases with increasing |z| symmetrically on either side of z = 0. 4.13. Three identical point charges of 4 pC each are located at the corners of an equilateral triangle 0.5 mm on a side in free space. How much work must be done to move one charge to a point equidistant from the other two and on the line joining them? This will be the magnitude of the charge times the potential difference between the finishing and starting positions, or W = (4 × 10−12)2 2πǫ0 1 2.5 − 1 5 × 104 = 5.76 × 10−10 J = 576 pJ 4.14. two 6-nC point charges are located at (1, 0, 0) and (−1, 0, 0) in free space. a) Find V at P (0, 0, z): Since the charges are positioned symmetrically about the z axis, the potential at z will be double that from one charge. This becomes: V (z) = (2) q 4πǫ0 √ z2 + 1 = q 2πǫ0 √ z2 + 1 b) Find Vmax: It is clear from the part a result that V will maximize at z = 0, or vmax = q/(2πǫ0) = 108 V. 47 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 50. 4.14. (continued) c) Calculate |dV/dz| on the z axis: Differentiating the part a result, we find dV dz = qz πǫ0(z2 + 1)3/2 V/m d) Find |dV/dz|max: To find this we need to differentiate the part c result and find its zero: d dz dV dz = q(1 − 2z2) πǫ0(z2 + 1)5/2 = 0 ⇒ z = ± 1 √ 2 Substituting z = 1/ √ 2 into the part c result, we find dV dz max = q √ 2πǫ0(3/2)3/2 = 83.1 V/m 4.15. Two uniform line charges, 8 nC/m each, are located at x = 1, z = 2, and at x = −1, y = 2 in free space. If the potential at the origin is 100 V, find V at P (4, 1, 3): The net potential function for the two charges would in general be: V = − ρl 2πǫ0 ln(R1) − ρl 2πǫ0 ln(R2) + C At the origin, R1 = R2 = √ 5, and V = 100 V. Thus, with ρl = 8 × 10−9, 100 = −2 (8 × 10−9) 2πǫ0 ln( √ 5) + C ⇒ C = 331.6 V At P (4, 1, 3), R1 = |(4, 1, 3) − (1, 1, 2)| = √ 10 and R2 = |(4, 1, 3) − (−1, 2, 3)| = √ 26. Therefore VP = − (8 × 10−9) 2πǫ0 ln( √ 10) + ln( √ 26) + 331.6 = −68.4 V 48 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 51. 4.16. Uniform surface charge densities of 6, 4, and 2 nC/m2 are present at r = 2, 4, and 6 cm, respectively, in free space. a) Assume V = 0 at infinity, and find V (r). We keep in mind the definition of absolute potential as the work done in moving a unit positive charge from infinity to location r. At radii outside all three spheres, the potential will be the same as that of a point charge at the origin, whose charge is the sum of the three sphere charges: V (r) (r > 6 cm) = q1 + q2 + q3 4πǫ0r = [4π(.02)2(6) + 4π(.04)2(4) + 4π(.06)2(2)] × 10−9 4πǫ0r = (96 + 256 + 288)π × 10−13 4π(8.85 × 10−12)r = 1.81 r V where r is in meters As the unit charge is moved inside the outer sphere to positions 4 < r < 6 cm, the outer sphere contribution to the energy is fixed at its value at r = 6. Therefore, V (r) (4 < r < 6 cm) = q1 + q2 4πǫ0r + q3 4πǫ0(.06) = 0.994 r + 13.6 V In moving inside the sphere at r = 4 cm, the contribution from that sphere becomes fixed at its potential function at r = 4: V (r) (2 < r < 4 cm) = q1 4πǫ0r + q2 4πǫ0(.04) + q3 4πǫ0(.06) = 0.271 r + 31.7 V Finally, using the same reasoning, the potential inside the inner sphere becomes V (r) (r < 2 cm) = 0.271 .02 + 31.7 = 45.3 V b) Calculate V at r = 1, 3, 5, and 7 cm: Using the results of part a, we substitute these distances (in meters) into the appropriate formulas to obtain: V (1) = 45.3 V, V (3) = 40.7 V, V (5) = 33.5 V, and V (7) = 25.9 V. c) Sketch V versus r for 0 < r < 10 cm. 49 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 52. 4.17. Uniform surface charge densities of 6 and 2 nC/m2 are present at ρ = 2 and 6 cm respectively, in free space. Assume V = 0 at ρ = 4 cm, and calculate V at: a) ρ = 5 cm: Since V = 0 at 4 cm, the potential at 5 cm will be the potential difference between points 5 and 4: V5 = − 5 4 E · dL = − 5 4 aρsa ǫ0ρ dρ = − (.02)(6 × 10−9) ǫ0 ln 5 4 = −3.026 V b) ρ = 7 cm: Here we integrate piecewise from ρ = 4 to ρ = 7: V7 = − 6 4 aρsa ǫ0ρ dρ − 7 6 (aρsa + bρsb) ǫ0ρ dρ With the given values, this becomes V7 = − (.02)(6 × 10−9) ǫ0 ln 6 4 − (.02)(6 × 10−9) + (.06)(2 × 10−9) ǫ0 ln 7 6 = −9.678 V 4.18. A nonuniform linear charge density, ρL = 8/(z2 + 1) nC/m lies along the z axis. Find the potential at P (ρ = 1, 0, 0) in free space if V = 0 at infinity: This last condition enables us to write the potential at P as a superposition of point charge potentials. The result is the integral: VP = ∞ −∞ ρLdz 4πǫ0R where R = √ z2 + 1 is the distance from a point z on the z axis to P. Substituting the given charge distribution and R into the integral gives us VP = ∞ −∞ 8 × 10−9dz 4πǫ0(z2 + 1)3/2 = 2 × 10−9 πǫ0 z √ z2 + 1 ∞ −∞ = 144 V 4.19. The annular surface, 1 cm < ρ < 3 cm, z = 0, carries the nonuniform surface charge density ρs = 5ρ nC/m2. Find V at P (0, 0, 2 cm) if V = 0 at infinity: We use the superposition integral form: VP = ρs da 4πǫ0|r − r′| where r = zaz and r′ = ρaρ. We integrate over the surface of the annular region, with da = ρ dρ dφ. Substituting the given values, we find VP = 2π 0 .03 .01 (5 × 10−9)ρ2 dρ dφ 4πǫ0 ρ2 + z2 Substituting z = .02, and using tables, the integral evaluates as VP = (5 × 10−9) 2ǫ0 ρ 2 ρ2 + (.02)2 − (.02)2 2 ln(ρ + ρ2 + (.02)2) .03 .01 = .081 V 50 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 53. 4.20. Fig. 4.11 shows three separate charge distributions in the z = 0 plane in free space. a) find the total charge for each distribution: Line charge along the y axis: Q1 = 5 3 π × 10−9 dy = 2π × 10−9 C = 6.28 nC Line charge in an arc at radius ρ = 3: Q2 = 70◦ 10◦ (10−9 ) 3 dφ = 4.5 × 10−9 (70 − 10) 2π 360 = 4.71 × 10−9 C = 4.71 nC Sheet charge: Q3 = 70◦ 10◦ 3.5 1.6 (10−9 ) ρ dρ dφ = 5.07 × 10−9 C = 5.07 nC b) Find the potential at P (0, 0, 6) caused by each of the three charge distributions acting alone: Line charge along y axis: VP 1 = 5 3 ρLdL 4πǫ0R = 5 3 π × 10−9dy 4πǫ0 y2 + 62 = 103 4 × 8.854 ln(y + y2 + 62) 5 3 = 7.83 V Line charge in an arc a radius ρ = 3: VP2 = 70◦ 10◦ (1.5 × 10−9) 3 dφ 4πǫ0 √ 32 + 62 = Q2 4πǫ0 √ 45 = 6.31 V Sheet charge: VP3 = 70◦ 10◦ 3.5 1.6 (10−9) ρ dρ dφ 4πǫ0 ρ2 + 62 = 60 × 10−9 4π(8.854 × 10−12 2π 360 3.5 1.6 ρ dρ ρ2 + 36 = 9.42 ρ2 + 36 3.5 1.6 = 6.93 V c) Find VP : This will be the sum of the three results of part b, or VP = VP1 + VP 2 + VP 3 = 7.83 + 6.31 + 6.93 = 21.1 V 4.21. Let V = 2xy2z3 + 3 ln(x2 + 2y2 + 3z2) V in free space. Evaluate each of the following quantities at P (3, 2, −1): a) V : Substitute P directly to obtain: V = −15.0 V b) |V |. This will be just 15.0 V. c) E: We have E P = −∇V P = − 2y2 z3 + 6x x2 + 2y2 + 3z2 ax + 4xyz3 + 12y x2 + 2y2 + 3z2 ay + 6xy2 z2 + 18z x2 + 2y2 + 3z2 az P = 7.1ax + 22.8ay − 71.1az V/m 51 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 54. 4.21d. |E|P : taking the magnitude of the part c result, we find |E|P = 75.0 V/m. e) aN : By definition, this will be aN P = − E |E| = −0.095 ax − 0.304 ay + 0.948 az f) D: This is D P = ǫ0E P = 62.8 ax + 202 ay − 629 az pC/m2. 4.22. It is known that the potential is given as V = 80r0.6 V. Assuming free space conditions, find: a) E: We use E = −∇V = − dV dr ar = −(0.6)80r−0.4 ar = −48r−0.4 ar V/m b) the volume charge density at r = 0.5 m: Begin by finding D = ǫ0E = −48r−0.4 ǫ0 ar C/m2 We next find ρv = ∇ · D = 1 r2 d dr r2 Dr = 1 r2 d dr −48ǫ0r1.6 = − 76.8ǫ0 r1.4 C/m3 Then at r = 0.5 m, ρv(0.5) = −76.8(8.854 × 10−12) (0.5)1.4 = −1.79 × 10−9 C/m3 = −1.79 nC/m3 c) the total charge lying within the surface r = 0.6: The easiest way is to use Gauss’law, and integrate the flux density over the spherical surface r = 0.6. Since the field is constant at constant radius, we obtain the product: Q = 4π(0.6)2 (−48ǫ0(0.6)−0.4 ) = −2.36 × 10−9 C = −2.36 nC 4.23. It is known that the potential is given as V = 80ρ.6 V. Assuming free space conditions, find: a) E: We find this through E = −∇V = − dV dρ aρ = −48ρ−.4 V/m b) the volume charge density at ρ = .5 m: Using D = ǫ0E, we find the charge density through ρv .5 = [∇ · D].5 = 1 ρ d dρ ρDρ .5 = −28.8ǫ0ρ−1.4 .5 = −673 pC/m3 52 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 55. 4.23c. the total charge lying within the closed surface ρ = .6, 0 < z < 1: The easiest way to do this calculation is to evaluate Dρ at ρ = .6 (noting that it is constant), and then multiply by the cylinder area: Using part a, we have Dρ .6 = −48ǫ0(.6)−.4 = −521 pC/m2. Thus Q = −2π(.6)(1)521×10−12 C = −1.96 nC. 4.24. Given the potential field V = 80r2 cos θ and a point P (2.5, θ = 30◦, φ = 60◦) in free space, find at P : a) V : Substitute the coordinates into the function and find VP = 80(2.5)2 cos(30) = 433 V. b) E: E = −∇V = − ∂V ∂r ar − 1 r ∂V ∂θ aθ = −160r cos θar + 80r sin θaθ V/m Evaluating this at P yields Ep = −346ar + 100aθ V/m. c) D: In free space, DP = ǫ0EP = (−346ar + 100aθ )ǫ0 = −3.07 ar + 0.885 aθ nC/m2. d) ρv: ρv = ∇ · D = ǫ0∇ · E = ǫ0 1 r2 ∂ ∂r r2 Er + 1 r2 sin θ ∂ ∂θ (Eθ sin θ) Substituting the components of E, we find ρv = − 160 cos θ r2 3r2 + 1 r sin θ 80r(2 sin θ cos θ) ǫ0 = −320ǫ0 cos θ = −2.45 nC/m3 with θ = 30◦. e) dV/dN: This will be just |E| evaluated at P , which is dV dN P = | − 346ar + 100aθ | = (346)2 + (100)2 = 360 V/m f) aN : This will be aN = − EP |EP | = − −346ar + 100aθ (346)2 + (100)2 = 0.961 ar − 0.278 aθ 4.25. Within the cylinder ρ = 2, 0 < z < 1, the potential is given by V = 100 + 50ρ + 150ρ sin φ V. a) Find V , E, D, and ρv at P (1, 60◦, 0.5) in free space: First, substituting the given point, we find VP = 279.9 V. Then, E = −∇V = − ∂V ∂ρ aρ − 1 ρ ∂V ∂φ aφ = − [50 + 150 sin φ] aρ − [150 cos φ] aφ Evaluate the above at P to find EP = −179.9aρ − 75.0aφ V/m Now D = ǫ0E, so DP = −1.59aρ − .664aφ nC/m2. Then ρv = ∇ ·D = 1 ρ d dρ ρDρ + 1 ρ ∂Dφ ∂φ = − 1 ρ (50 + 150 sin φ) + 1 ρ 150 sin φ ǫ0 = − 50 ρ ǫ0 C At P , this is ρvP = −443 pC/m3. 53 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 56. 4.25b. How much charge lies within the cylinder? We will integrate ρv over the volume to obtain: Q = 1 0 2π 0 2 0 − 50ǫ0 ρ ρ dρ dφ dz = −2π(50)ǫ0(2) = −5.56 nC 4.26. A dipole having Qd/(4πǫ0) = 100 V · m2 is located at the origin in free space and aligned so that its moment is in the az direction. a) Sketch |V (r = 1, θ, φ = 0)| versus θ on polar graph paper (homemade if you wish). b) Sketch |E(r = 1, θ, φ = 0)| versus θ on polar graph paper: V = Qd cos θ 4πǫ0r2 = 100 cos θ r2 ⇒ |V (r = 1, θ, φ = 0)| = |100 cos θ| E = Qd 4πǫ0r3 (2 cos θ ar + sin θ aθ ) = 100 r3 (2 cos θ ar + sin θ aθ ) |E(r = 1, θ, φ = 0)| = 100 4 cos2 θ + sin2 θ 1/2 = 100 1 + 3 cos2 θ 1/2 These results are plotted below: 54 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 57. 4.27. Two point charges, 1 nC at (0, 0, 0.1) and −1 nC at (0, 0, −0.1), are in free space. a) Calculate V at P (0.3, 0, 0.4): Use VP = q 4πǫ0|R+| − q 4πǫ0|R−| where R+ = (.3, 0, .3) and R− = (.3, 0, .5), so that |R+| = 0.424 and |R−| = 0.583. Thus VP = 10−9 4πǫ0 1 .424 − 1 .583 = 5.78 V b) Calculate |E| at P : Use EP = q(.3ax + .3az) 4πǫ0(.424)3 − q(.3ax + .5az) 4πǫ0(.583)3 = 10−9 4πǫ0 2.42ax + 1.41az V/m Taking the magnitude of the above, we find |EP | = 25.2 V/m. c) Now treat the two charges as a dipole at the origin and find V at P: In spherical coordinates, P is located at r = √ .32 + .42 = .5 and θ = sin−1(.3/.5) = 36.9◦. Assuming a dipole in far-field, we have VP = qd cos θ 4πǫ0r2 = 10−9(.2) cos(36.9◦) 4πǫ0(.5)2 = 5.76 V 4.28. A dipole located at the origin in free space has a moment p2 × 10−9 az C · m. At what points on the line y = z, x = 0 is: a) |Eθ | = 1 mV/m? We note that the line y = z lies at θ = 45◦. Begin with E = 2 × 10−9 4πǫ0r3 (2 cos θ ar + sin θ aθ ) = 10−9 2 √ 2πǫ0r3 (2ar + aθ ) at θ = 45◦ from which Eθ = 10−9 2πǫ0r3 = 10−3 V/m (required) ⇒ r3 = 1.27 × 10−4 or r = 23.3 m The y and z values are thus y = z = ±23.3/ √ 2 = ±16.5 m b) |Er| = 1 mV/m? From the above field expression, the radial component magnitude is twice that of the theta component. Using the same development, we then find Er = 2 10−9 2πǫ0r3 = 10−3 V/m (required) ⇒ r3 = 2(1.27 × 10−4 ) or r = 29.4 m The y and z values are thus y = z = ±29.4/ √ 2 = ±20.8 m 55 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 58. 4.29. A dipole having a moment p = 3ax − 5ay + 10az nC · m is located at Q(1, 2, −4) in free space. Find V at P (2, 3, 4): We use the general expression for the potential in the far field: V = p · (r − r′) 4πǫ0|r − r′|3 where r − r′ = P − Q = (1, 1, 8). So VP = (3ax − 5ay + 10az) · (ax + ay + 8az) × 10−9 4πǫ0[12 + 12 + 82]1.5 = 1.31 V 4.30. A dipole, having a moment p = 2az nC · m is located at the origin in free space. Give the magnitude of E and its direction aE in cartesian components at r = 100 m, φ = 90◦, and θ =: a) 0◦; b) 30◦; c) 90◦. Begin with E = p 4πǫ0r3 [2 cos θ ar + sin θ aθ ] from which |E| = p 4πǫ0r3 4 cos2 θ + sin2 θ 1/2 = p 4πǫ0r3 1 + 3 cos2 θ 1/2 Now Ex = E · ax = p 4πǫ0r3 [2 cos θ ar · ax + sin θ aθ · ax] = p 4πǫ0r3 [3 cos θ sin θ cos φ] then Ey = E · ay = p 4πǫ0r3 2 cos θ ar · ay + sin θ aθ · ay = p 4πǫ0r3 [3 cos θ sin θ sin φ] and Ez = E · az = p 4πǫ0r3 2 cos θ ar · az + sin θ aθ · az = p 4πǫ0r3 2 cos2 θ − sin2 θ Since φ is given as 90◦, Ex = 0, and the field magnitude becomes |E(φ = 90◦ )| = E2 y + E2 z = p 4πǫ0r3 9 cos2 θ sin2 θ + (2 cos2 θ − sin2 θ)2 1/2 Then the unit vector becomes (again at φ = 90◦): aE = 3 cos θ sin θ ay + (2 cos2 θ − sin2 θ) az 9 cos2 θ sin2 θ + (2 cos2 θ − sin2 θ)2 1/2 Now with r = 100 m and p = 2 × 10−9, p 4πǫ0r3 = 2 × 10−9 4π(8.854 × 10−12)106 = 1.80 × 10−5 Using the above formulas, we find at θ = 0◦, |E| = (1.80 × 10−5)(2) = 36.0 µV/m and aE = az. At θ = 30◦, we find |E| = (1.80 × 10−5)[1.69 + 1.56]1/2 = 32.5 µV/m and aE = (1.30ay + 1.25az)/1.80 = 0.72 ax + 0.69 az. At θ = 90◦, |E| = (1.80×10−5)(1) = 18.0 µV/m and aE = −az. 56 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 59. 4.31. A potential field in free space is expressed as V = 20/(xyz) V. a) Find the total energy stored within the cube 1 < x, y, z < 2. We integrate the energy density over the cube volume, where wE = (1/2)ǫ0E · E, and where E = −∇V = 20 1 x2yz ax + 1 xy2z ay + 1 xyz2 az V/m The energy is now WE = 200ǫ0 2 1 2 1 2 1 1 x4y2z2 + 1 x2y4z2 + 1 x2y2z4 dx dy dz The integral evaluates as follows: WE = 200ǫ0 2 1 2 1 − 1 3 1 x3y2z2 − 1 xy4z2 − 1 xy2z4 2 1 dy dz = 200ǫ0 2 1 2 1 7 24 1 y2z2 + 1 2 1 y4z2 + 1 2 1 y2z4 dy dz = 200ǫ0 2 1 − 7 24 1 yz2 − 1 6 1 y3z2 − 1 2 1 yz4 2 1 dz = 200ǫ0 2 1 7 48 1 z2 + 7 48 1 z2 + 1 4 1 z4 dz = 200ǫ0(3) 7 96 = 387 pJ b) What value would be obtained by assuming a uniform energy density equal to the value at the center of the cube? At C(1.5, 1.5, 1.5) the energy density is wE = 200ǫ0(3) 1 (1.5)4(1.5)2(1.5)2 = 2.07 × 10−10 J/m3 This, multiplied by a cube volume of 1, produces an energy value of 207 pJ. 4.32. In the region of free space where 2 < r < 3, 0.4π < θ < 0.6π, 0 < φ < π/2, let E = k/r2 ar. a) Find a positive value for k so that the total energy stored is exactly 1 J: The energy is found through WE = v 1 2 ǫ0E2 dv = π/2 0 0.6π 0.4π 3 2 1 2 ǫ0 k2 r2 r2 sin θ dr dθ dφ = π 2 (− cos θ) .6π .4π 1 2 ǫ0k2 − 1 r 3 2 = 0.616π 24 ǫ0k2 = 1 J Solve for k to find k = 1.18 × 106 V · m. 57 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 60. 4.32b. Show that the surface θ = 0.6π is an equipotential surface: This will be the surface of a cone, centered at the origin, along which E, in the ar direction, will exist. Therefore, the given surface cannot be an equipotential (the problem was ill-conceived). Only a surface of constant r could be an equipotential in this field. c) Find VAB, given points A(2, θ = π/2, φ = π/3) and B(3, π/2, π/4): Use VAB = − A B E · dL = − 3 2 k r2 ar · ar dr = k 1 2 − 1 3 = k 6 Using the result of part a, we find VAB = (1.18 × 106)/6 = 197 kV. 4.33. A copper sphere of radius 4 cm carries a uniformly-distributed total charge of 5 µC in free space. a) Use Gauss’ law to find D external to the sphere: with a spherical Gaussian surface at radius r, D will be the total charge divided by the area of this sphere, and will be ar-directed. Thus D = Q 4πr2 ar = 5 × 10−6 4πr2 ar C/m2 b) Calculate the total energy stored in the electrostatic field: Use WE = vol 1 2 D · E dv = 2π 0 π 0 ∞ .04 1 2 (5 × 10−6)2 16π2ǫ0r4 r2 sin θ dr dθ dφ = (4π) 1 2 (5 × 10−6)2 16π2ǫ0 ∞ .04 dr r2 = 25 × 10−12 8πǫ0 1 .04 = 2.81 J c) Use WE = Q2/(2C) to calculate the capacitance of the isolated sphere: We have C = Q2 2WE = (5 × 10−6)2 2(2.81) = 4.45 × 10−12 F = 4.45 pF 4.34. Given the potential field in free space, V = 80φ V (note that aphi should not be present), find: a) the energy stored in the region 2 < ρ < 4 cm, 0 < φ < 0.2π, 0 < z < 1 m: First we find E = −∇V = − 1 ρ dV dφ aφ = − 80 ρ aφ V/m Then WE = v wEdv = 1 0 0.2π 0 .04 .02 1 2 ǫ0 (80)2 ρ2 ρ dρ dφ dz = 640πǫ0 ln .04 .02 = 12.3 nJ b) the potential difference, VAB, for A(3 cm, φ = 0, z = 0) and B(3cm, 0.2π, 1m): Use VAB = − A B E · dL = − 0 .2π − 80 ρ aφ · aφ ρ dφ = −80(0.2π) = −16π V 58 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 61. 4.34c. the maximum value of the energy density in the specified region: The energy density is wE = 1 2 ǫ0E2 = 1 2 ǫ0 6400 ρ2 This will maximize at the lowest value of ρ in the specified range, which is ρ = 2 cm. So wE,max = 1 2 ǫ0 6400 .022 = 7.1 × 10−5 J/m3 = 71 µJ/m3 4.35. Four 0.8 nC point charges are located in free space at the corners of a square 4 cm on a side. a) Find the total potential energy stored: This will be given by WE = 1 2 4 n=1 qnVn where Vn in this case is the potential at the location of any one of the point charges that arises from the other three. This will be (for charge 1) V1 = V21 + V31 + V41 = q 4πǫ0 1 .04 + 1 .04 + 1 .04 √ 2 Taking the summation produces a factor of 4, since the situation is the same at all four points. Consequently, WE = 1 2 (4)q1V1 = (.8 × 10−9)2 2πǫ0(.04) 2 + 1 √ 2 = 7.79 × 10−7 J = 0.779 µJ b) A fifth 0.8 µC charge is installed at the center of the square. Again find the total stored energy: This will be the energy found in part a plus the amount of work done in moving the fifth charge into position from infinity. The latter is just the potential at the square center arising from the original four charges, times the new charge value, or WE = 4(.8 × 10−9)2 4πǫ0(.04 √ 2/2) = .813 µJ The total energy is now WE net = WE(part a) + WE = .779 + .813 = 1.59 µJ 59 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 62. CHAPTER 5 5.1. Given the current density J = −104[sin(2x)e−2yax + cos(2x)e−2yay] kA/m2: a) Find the total current crossing the plane y = 1 in the ay direction in the region 0 < x < 1, 0 < z < 2: This is found through I = S J · n S da = 2 0 1 0 J · ay y=1 dx dz = 2 0 1 0 −104 cos(2x)e−2 dx dz = −104 (2) 1 2 sin(2x) 1 0 e−2 = −1.23 MA b) Find the total current leaving the region 0 < x, x < 1, 2 < z < 3 by integrating J · dS over the surface of the cube: Note first that current through the top and bottom surfaces will not exist, since J has no z component. Also note that there will be no current through the x = 0 plane, since Jx = 0 there. Current will pass through the three remaining surfaces, and will be found through I = 3 2 1 0 J · (−ay) y=0 dx dz + 3 2 1 0 J · (ay) y=1 dx dz + 3 2 1 0 J · (ax) x=1 dy dz = 104 3 2 1 0 cos(2x)e−0 − cos(2x)e−2 dx dz − 104 3 2 1 0 sin(2)e−2y dy dz = 104 1 2 sin(2x) 1 0 (3 − 2) 1 − e−2 + 104 1 2 sin(2)e−2y 1 0 (3 − 2) = 0 c) Repeat part b, but use the divergence theorem: We find the net outward current through the surface of the cube by integrating the divergence of J over the cube volume. We have ∇ · J = ∂Jx ∂x + ∂Jy ∂y = −10−4 2 cos(2x)e−2y − 2 cos(2x)e−2y = 0 as expected 5.2. Let the current density be J = 2φ cos2 φaρ − ρ sin 2φaφ A/m2 within the region 2.1 < ρ < 2.5, 0 < φ < 0.1 rad, 6 < z < 6.1. Find the total current I crossing the surface: a) ρ = 2.2, 0 < φ < 0.1, 6 < z < 6.1 in the aρ direction: This is a surface of constant ρ, so only the radial component of J will contribute: At ρ = 2.2 we write: I = J · dS = 6.1 6 0.1 0 2(2) cos2 φ aρ · aρ 2dφdz = 2(2.2)2 (0.1) 0.1 0 1 2 (1 + cos 2φ) dφ = 0.2(2.2)2 1 2 (0.1) + 1 4 sin 2φ 0.1 0 = 97 mA b) φ = 0.05, 2.2 < ρ < 2.5, 6 < z < 6.1 in the aφ direction: In this case only the φ component of J will contribute: I = J · dS = 6.1 6 2.5 2.2 −ρ sin 2φ φ=0.05 aφ · aφ dρ dz = −(0.1)2 ρ2 2 2.5 2.2 = −7 mA 60 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 63. 5.2c. Evaluate ∇ · J at P (ρ = 2.4, φ = 0.08, z = 6.05): ∇ · J = 1 ρ ∂ ∂ρ (ρJρ) + 1 ρ ∂Jφ ∂φ = 1 ρ ∂ ∂ρ (2ρ2 cos2 φ) − 1 ρ ∂ ∂φ (ρ sin 2φ) = 4 cos2 φ − 2 cos 2φ 0.08 = 2.0 A/m3 5.3. Let J = 400 sin θ r2 + 4 ar A/m2 a) Find the total current flowing through that portion of the spherical surface r = 0.8, bounded by 0.1π < θ < 0.3π, 0 < φ < 2π: This will be I = J · n S da = 2π 0 .3π .1π 400 sin θ (.8)2 + 4 (.8)2 sin θ dθ dφ = 400(.8)22π 4.64 .3π .1π sin2 dθ = 346.5 .3π .1π 1 2 [1 − cos(2θ)] dθ = 77.4 A b) Find the average value of J over the defined area. The area is Area = 2π 0 .3π .1π (.8)2 sin θ dθ dφ = 1.46 m2 The average current density is thus Javg = (77.4/1.46) ar = 53.0 ar A/m2. 5.4. The cathode of a planar vacuum tube is at z = 0. Let E = −4 × 106 az V/m for z > 0. An electron (e = 1.602 × 10−19 C, m = 9.11 × 10−31 kg) is emitted from the cathode with zero initial velocity at t = 0. a) Find v(t): Using Newton’s second law, we write: F = ma = qE ⇒ a = (−1.602 × 10−19)(−4 × 106)az (9.11 × 10−31) = 7.0 × 1017 az m/s2 Then v(t) = at = 7.0 × 1017t m/s. b) Find z(t), the electron location as a function of time: Use z(t) = t 0 v(t′ )dt′ = 1 2 (7.0 × 1017 )t2 = 3.5 × 1017 t2 m c) Determine v(z): Solve the result of part b for t, obtaining t = √ z √ 3.5 × 1017 = 1.7 × 109√ z Substitute into the result of part a to find v(z) = 7.0 × 1017(1.7 × 10−9) √ z = 1.2 × 109√ z m/s. 61 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 64. 5.4d. Make the assumption that the electrons are emitted continuously as a beam with a 0.25 mm radius and a total current of 60 µA. Find J(z) and ρ(z): J(z) = −60 × 10−6 π(0.25)2(10−6) az = −3.1 × 102 az A/m2 (negative since we have electrons flowing in the positive z direction) Next we use J(z) = ρv(z)v(z), or ρv(z) = J v = −3.1 × 102 1.2 × 109 √ z = − 2.6 × 10−7 √ z C/m3 = −26 √ z µC/m3 5.5. Let J = 25 ρ aρ − 20 ρ2 + 0.01 az A/m2 a) Find the total current crossing the plane z = 0.2 in the az direction for ρ < 0.4: Use I = S J · n z=.2 da = 2π 0 .4 0 −20 ρ2 + .01 ρ dρ dφ = − 1 2 20 ln(.01 + ρ2 ) .4 0 (2π) = −20π ln(17) = −178.0 A b) Calculate ∂ρv/∂t: This is found using the equation of continuity: ∂ρv ∂t = −∇ · J = 1 ρ ∂ ∂ρ (ρJρ) + ∂Jz ∂z = 1 ρ ∂ ∂ρ (25) + ∂ ∂z −20 ρ2 + .01 = 0 c) Find the outward current crossing the closed surface defined by ρ = 0.01, ρ = 0.4, z = 0, and z = 0.2: This will be I = .2 0 2π 0 25 .01 aρ · (−aρ)(.01) dφ dz + .2 0 2π 0 25 .4 aρ · (aρ)(.4) dφ dz + 2π 0 .4 0 −20 ρ2 + .01 az · (−az) ρ dρ dφ + 2π 0 .4 0 −20 ρ2 + .01 az · (az) ρ dρ dφ = 0 since the integrals will cancel each other. d) Show that the divergence theorem is satisfied for J and the surface specified in part b. In part c, the net outward flux was found to be zero, and in part b, the divergence of J was found to be zero (as will be its volume integral). Therefore, the divergence theorem is satisfied. 5.6. Let ǫ = ǫ0 and V = 90z4/3 in the region z = 0. a) Obtain expressions for E, D, and ρv as functions of z: First, E = −∇V = − dV dz az = − 4 3 (90)z1/3 az = −120z1/3 az V/m 62 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 65. 5.6a. (continued) Next, D = ǫ0E = 1.06z1/3az nC/m2. Then ρv = ∇ · D = dDz dz = − 1 3 (120)ǫ0z−2/3 = −354z−2/3 pC/m3 b) If the velocity of the charge density is given as vz = 5×106z2/3 m/s, find Jz at z = 0 and z = 0.1 m (note that vz is written as vx through a missprint): Use Jz = ρvvz = (−354 × 10−12)z−2/3(5 × 106)z2/3 = −1.8 mA/m2 at any z. 5.7. Assuming that there is no transformation of mass to energy or vice-versa, it is possible to write a continuity equation for mass. a) If we use the continuity equation for charge as our model, what quantities correspond to J and ρv? These would be, respectively, mass flux density in (kg/m2 − s) and mass density in (kg/m3). b) Given a cube 1 cm on a side, experimental data show that the rates at which mass is leaving each of the six faces are 10.25, -9.85, 1.75, -2.00, -4.05, and 4.45 mg/s. If we assume that the cube is an incremental volume element, determine an approximate value for the time rate of change of density at its center. We may write the continuity equation for mass as follows, also invoking the divergence theorem: v ∂ρm ∂t dv = − v ∇ · Jm dv = − s Jm · dS where s Jm · dS = 10.25 − 9.85 + 1.75 − 2.00 − 4.05 + 4.45 = 0.550 mg/s Treating our 1 cm3 volume as differential, we find ∂ρm ∂t . = − 0.550 × 10−3 g/s 10−6 m3 = −550 g/m3 − s 5.8. The continuity equation for mass equates the divergence of the mass rate of flow (mass per second per square meter) to the negative of the density (mass per cubic meter). After setting up a cartesian coordinate system inside a star, Captain Kirk and his intrepid crew make measurements over the faces of a cube centered at the origin with edges 40 km long and parallel to the coordinate axes. They find the mass rate of flow of material outward across the six faces to be -1112, 1183, 201, -196, 1989, and -1920 kg/m2 · s. a) Estimate the divergence of the mass rate of flow at the origin: We make the estimate using the definition of divergence, but without taking the limit as the volume shrinks to zero: Div Jm . = Jm · dS v = (−1112 + 1183 + 201 − 196 + 1989 − 1920)(40)2 (40)3 = 3.63 kg/km3 · s b) Estimate the rate of change of the density at the origin: The continuity equation for mass reads: Div Jm = − ∂ρm/∂t. Therefore, the rate of change of density at the origin will be just the negative of the part a result, or ∂ρm/∂t . = − 3.63 kg/km3 · s. 63 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 66. 5.9a. Using data tabulated in Appendix C, calculate the required diameter for a 2-m long nichrome wire that will dissipate an average power of 450 W when 120 V rms at 60 Hz is applied to it: The required resistance will be R = V 2 P = l σ(πa2) Thus the diameter will be d = 2a = 2 lP σπV 2 = 2 2(450) (106)π(120)2 = 2.8 × 10−4 m = 0.28 mm b) Calculate the rms current density in the wire: The rms current will be I = 450/120 = 3.75 A. Thus J = 3.75 π 2.8 × 10−4/2 2 = 6.0 × 107 A/m2 5.10. A steel wire has a radius of 2 mm and a conductivity of 2 × 106 S/m. The steel wire has an aluminum (σ = 3.8 × 107 S/m) coating of 2 mm thickness. Let the total current carried by this hybrid conductor be 80 A dc. Find: a) Jst . We begin with the fact that electric field must be the same in the aluminum and steel regions. This comes from the requirement that E tangent to the boundary between two media must be continuous, and from the fact that when integrating E over the wire length, the applied voltage value must be obtained, regardless of the medium within which this integral is evaluated. We can therefore write EAl = Est = JAl σAl = Jst σst ⇒ JAl = σAl σst Jst The net current is now expressed as the sum of the currents in each region, written as the sum of the products of the current densities in each region times the appropriate cross-sectional area: I = π(2 × 10−3 )2 Jst + π[(4 × 10−3 )2 − (2 × 10−3 )2 ]JAl = 80 A Using the above relation between Jst and JAl, we find 80 = π (2 × 10−3 )2 1 − 3.8 × 107 6 × 106 + (4 × 10−3 )2 3.8 × 107 6 × 106 Jst Solve for Jst to find Jst = 3.2 × 105 A/m2. b) JAl = 3.8 × 107 6 × 106 (3.2 × 105 ) = 2.0 × 106 A/m2 c,d) Est = EAl = Jst /σst = JAl/σAl = 5.3 × 10−2 V/m. e) the voltage between the ends of the conductor if it is 1 mi long: Using the fact that 1 mi = 1.61×103 m, we have V = El = (5.3 × 10−2)(1.61 × 103) = 85.4 V. 64 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 67. 5.11. Two perfectly-conducting cylindrical surfaces are located at ρ = 3 and ρ = 5 cm. The total current passing radially outward through the medium between the cylinders is 3 A dc. Assume the cylinders are both of length l. a) Find the voltage and resistance between the cylinders, and E in the region between the cylinders, if a conducting material having σ = 0.05 S/m is present for 3 < ρ < 5 cm: Given the current, and knowing that it is radially-directed, we find the current density by dividing it by the area of a cylinder of radius ρ and length l: J = 3 2πρl aρ A/m2 Then the electric field is found by dividing this result by σ: E = 3 2πσρl aρ = 9.55 ρl aρ V/m The voltage between cylinders is now: V = − 3 5 E · dL = 5 3 9.55 ρl aρ · aρdρ = 9.55 l ln 5 3 = 4.88 l V Now, the resistance will be R = V I = 4.88 3l = 1.63 l b) Showthatintegratingthepowerdissipatedperunitvolumeoverthevolumegivesthetotaldissipated power: We calculate P = v E · J dv = l 0 2π 0 .05 .03 32 (2π)2ρ2(.05)l2 ρ dρ dφ dz = 32 2π(.05)l ln 5 3 = 14.64 l W We also find the power by taking the product of voltage and current: P = V I = 4.88 l (3) = 14.64 l W which is in agreement with the power density integration. 5.12. The spherical surfaces r = 3 and r = 5 cm are perfectly conducting, and the total current passing radially outward through the medium between the surfaces is 3 A dc. a) Find the voltage and resistance between the spheres, and E in the region between them, if a conducting material having σ = 0.05 S/m is present for 3 < r < 5 cm. We first find J as a function of radius by dividing the current by the area of a sphere of radius r: J = I 4πr2 ar = 3 4πr2 ar A/m2 Then E = J σ = 3 4πr2(0.05) ar = 4.77 r2 ar V/m 65 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 68. 5.12a. (continued) V = − r1 r2 E · dL = − .03 .05 4.77 r2 dr = 4.77 1 .03 − 1 .05 = 63.7 V Finally, R = V/I = 63.7/3 = 21.2 . b) Repeat if σ = 0.0005/r for 3 < r < 5 cm: First, J = 3ar/(4πr2) as before. The electric field is now E = J σ = 3rar 4π(.0005)r2 = 477 r ar V/m Now V = − r1 r2 E · dL = − .03 .05 477 r dr = −477 ln .03 .05 = 244 V Finally, R = V/I = 244/3 = 81.3 . c) Show that integrating the power dissipated per unit volume in part b over the volume gives the total dissipated power: The dissipated power density is pd = E · J = 3 4π(.0005)r 3 4πr2 = 114 r3 W/m2 We integrate this over the volume between spheres: Pd = 2π 0 π 0 .05 .03 114 r3 r2 sin θ dr dθ dφ = 4π(114) ln 5 3 = 732 W The dissipated power should be just I2R = (3)2(81.3) = 732 W. So it works. 5.13. A hollow cylindrical tube with a rectangular cross-section has external dimensions of 0.5 in by 1 in and a wall thickness of 0.05 in. Assume that the material is brass, for which σ = 1.5 × 107 S/m. A current of 200 A dc is flowing down the tube. a) What voltage drop is present across a 1m length of the tube? Converting all measurements to meters, the tube resistance over a 1 m length will be: R1 = 1 (1.5 × 107) (2.54)(2.54/2) × 10−4 − 2.54(1 − .1)(2.54/2)(1 − .2) × 10−4 = 7.38 × 10−4 The voltage drop is now V = IR1 = 200(7.38 × 10−4 = 0.147 V. b) Find the voltage drop if the interior of the tube is filled with a conducting material for which σ = 1.5 × 105 S/m: The resistance of the filling will be: R2 = 1 (1.5 × 105)(1/2)(2.54)2 × 10−4(.9)(.8) = 2.87 × 10−2 The total resistance is now the parallel combination of R1 and R2: RT = R1R2/(R1 + R2) = 7.19 × 10−4 , and the voltage drop is now V = 200RT = .144 V. 66 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 69. 5.14. Find the magnitude of the electric field intensity in a conductor if: a) the current density is 5 MA/m2, the electron mobility is 3×10−3 m2/V · s, and the volume charge density is −2.4 × 1010 C/m3: In magnitude, we have E = J µeρv = 5 × 106 (2.4 × 1010)(3 × 10−3) = 6.9 × 10−2 V/m b) J = 3 MA/m2 and the resistivity is 3 × 10−8 · m: E = Jρ = (3 × 106)(3 × 10−8) = 9 × 10−2 V/m. 5.15. Let V = 10(ρ + 1)z2 cos φ V in free space. a) Let the equipotential surface V = 20 V define a conductor surface. Find the equation of the conductor surface: Set the given potential function equal to 20, to find: (ρ + 1)z2 cos φ = 2 b) Find ρ and E at that point on the conductor surface where φ = 0.2π and z = 1.5: At the given values of φ and z, we solve the equation of the surface found in part a for ρ, obtaining ρ = .10. Then E = −∇V = − ∂V ∂ρ aρ − 1 ρ ∂V ∂φ aφ − ∂V ∂z az = −10z2 cos φ aρ + 10 ρ + 1 ρ z2 sin φ aφ − 20(ρ + 1)z cos φ az Then E(.10, .2π, 1.5) = −18.2 aρ + 145 aφ − 26.7 az V/m c) Find |ρs| at that point: Since E is at the perfectly-conducting surface, it will be normal to the surface, so we may write: ρs = ǫ0E · n surface = ǫ0 E · E |E| = ǫ0 √ E · E = ǫ0 (18.2)2 + (145)2 + (26.7)2 = 1.32 nC/m2 5.16. A potential field in free space is given as V = (80 cos θ sin φ)/r3 V. Point P (r = 2, θ = π/3, φ = π/2) lies on a conducting surface. a) Write the equation of the conducting surface: The surface will be an equipotential, where the value of the potential is VP : VP = 80 cos(π/3) sin(π/2) (2)3 = 5 So the equation of the surface is 80 cos θ sin φ r3 = 5 or 16 cos θ sin φ = r3 67 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 70. 5.16c. (I will work parts b and c in reverse order) Find E at P : E = −∇V = − ∂V ∂r ar − 1 r ∂V ∂θ aθ − 1 r sin θ ∂V ∂φ aφ = 80(3) cos θ sin φ r4 ar + 80 sin θ sin φ r4 aθ − 80 cos θ cos φ r4 sin θ aφ Now EP = 80(1/2)(1)(3) 16 ar + 80( √ 3/2)(1) 16 aθ − 0 aφ = 7.5 ar + 4.3 aθ V/m b) Find a unit vector directed outward to the surface, assuming the origin is inside the surface: Such a unit normal can be construced from the result of part c: aN = 7.5 ar + 4.3 aθ 4.33 = 0.87 ar + 0.50 aθ 5.17. Given the potential field V = 100xz x2 + 4 V in free space: a) Find D at the surface z = 0: Use E = −∇V = −100z ∂ ∂x x x2 + 4 ax − 0 ay − 100x x2 + 4 az V/m At z = 0, we use this to find D(z = 0) = ǫ0E(z = 0) = − 100ǫ0x x2 + 4 az C/m2 b) Show that the z = 0 surface is an equipotential surface: There are two reasons for this: 1) E at z = 0 is everywhere z-directed, and so moving a charge around on the surface involves doing no work; 2) When evaluating the given potential function at z = 0, the result is 0 for all x and y. c) Assume that the z = 0 surface is a conductor and find the total charge on that portion of the conductor defined by 0 < x < 2, −3 < y < 0: We have ρs = D · az z=0 = − 100ǫ0x x2 + 4 C/m2 So Q = 0 −3 2 0 − 100ǫ0x x2 + 4 dx dy = −(3)(100)ǫ0 1 2 ln(x2 + 4) 2 0 = −150ǫ0 ln 2 = −0.92 nC 68 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 71. 5.18. Let us assume a field E = 3y2z3 ax + 6xyz3 ay + 9xy2z2 az V/m in free space, and also assume that point P (2, 1, 0) lies on a conducting surface. a) Find ρv just adjacent to the surface at P : ρv = ∇ · D = ǫ0∇ · E = 6xz3 + 18xy2 z C/m3 Then at P, ρv = 0, since z = 0. b) Find ρs at P : ρs = D · n P = ǫ0E˙n P Note however, that this computation involves evaluating E at the surface, yielding a value of 0. Therefore the surface charge density at P is 0. c) Show that V = −3xy2z3 V: The simplest way to show this is just to take −∇V , which yields the given field: A more general method involves deriving the potential from the given field: We write Ex = − ∂V ∂x = 3y2 z3 ⇒ V = −3xy2 z3 + f (y, z) Ey = − ∂V ∂y = 6xyz3 ⇒ V = −3xy2 z3 + f (x, z) Ez = − ∂V ∂z = 9xy2 z2 ⇒ V = −3xy2 z3 + f (x, y) where the integration “constants” are functions of all variables other than the integration variable. The general procedure is to adjust the functions, f , such that the result for V is the same in all three integrations. In this case we see that f (x, y) = f (x, z) = f (y, z) = 0 accomplishes this, and the potential function is V = −3xy2z3 as given. d) Determine VPQ, given Q(1, 1, 1): Using the potential function of part c, we have VP Q = VP − VQ = 0 − (−3) = 3 V 5.19. Let V = 20x2yz − 10z2 V in free space. a) Determine the equations of the equipotential surfaces on which V = 0 and 60 V: Setting the given potential function equal to 0 and 60 and simplifying results in: At 0 V : 2x2 y − z = 0 At 60 V : 2x2 y − z = 6 z b) Assume these are conducting surfaces and find the surface charge density at that point on the V = 60 V surface where x = 2 and z = 1. It is known that 0 ≤ V ≤ 60 V is the field-containing region: First, on the 60 V surface, we have 2x2 y − z − 6 z = 0 ⇒ 2(2)2 y(1) − 1 − 6 = 0 ⇒ y = 7 8 69 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 72. 5.19b. (continued) Now E = −∇V = −40xyz ax − 20x2 z ay − [20xy − 20z] az Then, at the given point, we have D(2, 7/8, 1) = ǫ0E(2, 7/8, 1) = −ǫ0[70 ax + 80 ay + 50 az] C/m2 We know that since this is the higher potential surface, D must be directed away from it, and so the charge density would be positive. Thus ρs = √ D · D = 10ǫ0 72 + 82 + 52 = 1.04 nC/m2 c) Give the unit vector at this point that is normal to the conducting surface and directed toward the V = 0 surface: This will be in the direction of E and D as found in part b, or an = − 7ax + 8ay + 5az √ 72 + 82 + 52 = −[0.60ax + 0.68ay + 0.43az] 5.20. A conducting plane is located at z = 0 in free space, and a 20 nC point charge is present at Q(2, 4, 6). a) If V = 0 at z = 0, find V at P (5, 3, 1): The plane can be replaced by an image charge of -20 nC at Q′(2, 4, −6). Vectors R and R′ directed from Q and Q′ to P are R = (5, 3, 1) − (2, 4, 6) = (3, −1, −5) and R′ = (5, 3, 1) − (2, 4, −6) = (3, −1, 7). Their magnitudes are R = √ 35 and R′ = √ 59. The potential at P is given by VP = q 4πǫ0R − q 4πǫ0R′ = 20 × 10−9 4πǫ0 √ 35 − 20 × 10−9 4πǫ0 √ 59 = 7.0 V b) Find E at P : EP = qR 4πǫ0R3 − qR′ 4πǫ0(R′)3 = (20 × 10−9)(3, −1, −5) 4πǫ0(35)3/2 − (20 × 10−9)(3, −1, 7) 4πǫ0(59)3/2 = 20 × 10−9 4πǫ0 (3ax − ay) 1 (35)3/2 − 1 (59)3/2 − 7 (59)3/2 + 5 (35)3/2 az = 1.4ax − 0.47ay − 7.1az V/m c) Find ρs at A(5, 3, 0): First, find the electric field there: EA = 20 × 10−9 4πǫ0 (5, 3, 0) − (2, 4, 6) (46)3/2 − (5, 3, 0) − (2, 4, −6) (46)3/2 = −6.9az V/m Then ρs = D · n surf ace = −6.9ǫ0az · az = −61 pC/m2. 70 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 73. 5.21. Let the surface y = 0 be a perfect conductor in free space. Two uniform infinite line charges of 30 nC/m each are located at x = 0, y = 1, and x = 0, y = 2. a) Let V = 0 at the plane y = 0, and find V at P (1, 2, 0): The line charges will image across the plane, producing image line charges of -30 nC/m each at x = 0, y = −1, and x = 0, y = −2. We find the potential at P by evaluating the work done in moving a unit positive charge from the y = 0 plane (we choose the origin) to P : For each line charge, this will be: VP − V0,0,0 = − ρl 2πǫ0 ln final distance from charge initial distance from charge where V0,0,0 = 0. Considering the four charges, we thus have VP = − ρl 2πǫ0 ln 1 2 + ln √ 2 1 − ln √ 10 1 − ln √ 17 2 = ρl 2πǫ0 ln (2) + ln 1 √ 2 + ln √ 10 + ln √ 17 2 = 30 × 10−9 2πǫ0 ln √ 10 √ 17 √ 2 = 1.20 kV b) Find E at P : Use EP = ρl 2πǫ0 (1, 2, 0) − (0, 1, 0) |(1, 1, 0)|2 + (1, 2, 0) − (0, 2, 0) |(1, 0, 0)|2 − (1, 2, 0) − (0, −1, 0) |(1, 3, 0)|2 − (1, 2, 0) − (0, −2, 0) |(1, 4, 0)|2 = ρl 2πǫ0 (1, 1, 0) 2 + (1, 0, 0) 1 − (1, 3, 0) 10 − (1, 4, 0) 17 = 723 ax − 18.9 ay V/m 5.22. Let the plane x = 0 be a perfect conductor in free space. Locate a point charge of 4nC at P1(7, 1, −2) and a point charge of −3nC at P2(4, 2, 1). a) Find E at A(5, 0, 0): Image charges will be located at P′ 1(−7, 1, −2) (-4nC) and at P′ 2(−4, 2, 1) (3nC). Vectors from all four charges to point A are: R1 = (5, 0, 0) − (7, 1, −2) = (−2, −1, 2) R′ 1 = (5, 0, 0) − (−7, 1, −2) = (12, −1, 2) R2 = (5, 0, 0) − (4, 2, 1) = (1, −2, −1) and R′ 2 = (5, 0, 0) − (−4, 2, 1) = (9, −2, −1) Replacing the plane by the image charges enables the field at A to be calculated through: EA = 10−9 4πǫ0 (4)(−2, −1, 2) 93/2 − (3)(1, −2, −1) 63/2 − (4)(12, −1, 2) (149)3/2 + (3)(9, −2, −1) (86)3/2 = −4.43ax + 2.23ay + 4.42az V/m 71 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 74. 5.22b. Find |ρs| at B(0, 0, 0) (note error in problem statement): First, E at the origin is done as per the setup in part a, except the vectors are directed from the charges to the origin: EB = 10−9 4πǫ0 (4)(−7, −1, 2) (54)3/2 − (3)(−4, −2, −1) (21)3/2 − (4)(7, −1, 2) (54)3/2 + (3)(4, −2, −1) (21)3/2 Now ρs = D · n|surf ace = D · ax in our case (note the other components cancel anyway as they must, but we still need to express ρs as a scalar): ρsB = ǫ0EB · ax = 10−9 4π (4)(−7) (54)3/2 − (3)(−4) (21)3/2 − (4)(7) (54)3/2 + (3)(4) (21)3/2 = 8.62 pC/m2 5.23. A dipole with p = 0.1az µC · m is located at A(1, 0, 0) in free space, and the x = 0 plane is perfectly- conducting. a) Find V at P (2, 0, 1). We use the far-field potential for a z-directed dipole: V = p cos θ 4πǫ0r2 = p 4πǫ0 z [x2 + y2 + z2]1.5 The dipole at x = 1 will image in the plane to produce a second dipole of the opposite orientation at x = −1. The potential at any point is now: V = p 4πǫ0 z [(x − 1)2 + y2 + z2]1.5 − z [(x + 1)2 + y2 + z2]1.5 Substituting P (2, 0, 1), we find V = .1 × 106 4πǫ0 1 2 √ 2 − 1 10 √ 10 = 289.5 V b) Find the equation of the 200-V equipotential surface in cartesian coordinates: We just set the potential exression of part a equal to 200 V to obtain: z [(x − 1)2 + y2 + z2]1.5 − z [(x + 1)2 + y2 + z2]1.5 = 0.222 5.24. The mobilities for intrinsic silicon at a certain temperature are µe = 0.14 m2/V · s and µh = 0.035 m2/V · s. The concentration of both holes and electrons is 2.2 × 1016 m−3. Determine both the conductivity and the resistivity of this silicon sample: Use σ = −ρeµe + ρhµh = (1.6 × 10−19 C)(2.2 × 1016 m−3 )(0.14 m2 /V · s + 0.035 m2 /V · s) = 6.2 × 10−4 S/m Conductivity is ρ = 1/σ = 1.6 × 103 · m. 72 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 75. 5.25. Electron and hole concentrations increase with temperature. For pure silicon, suitable expressions are ρh = −ρe = 6200T 1.5e−7000/T C/m3. The functional dependence of the mobilities on temperature is given by µh = 2.3 × 105T −2.7 m2/V · s and µe = 2.1 × 105T −2.5 m2/V · s, where the temperature, T , is in degrees Kelvin. The conductivity will thus be σ = −ρeµe + ρhµh = 6200T 1.5 e−7000/T 2.1 × 105 T −2.5 + 2.3 × 105 T −2.7 = 1.30 × 109 T e−7000/T 1 + 1.095T −.2 S/m Find σ at: a) 0◦ C: With T = 273◦K, the expression evaluates as σ(0) = 4.7 × 10−5 S/m. b) 40◦ C: With T = 273 + 40 = 313, we obtain σ(40) = 1.1 × 10−3 S/m. c) 80◦ C: With T = 273 + 80 = 353, we obtain σ(80) = 1.2 × 10−2 S/m. 5.26. A little donor impurity, such as arsenic, is added to pure silicon so that the electron concentration is 2 × 1017 conduction electrons per cubic meter while the number of holes per cubic meter is only 1.1×1015. If µe = 0.15 m2/V · s for this sample, and µh = 0.045 m2/V · s, determine the conductivity and resistivity: σ = −ρeµe + ρhµh = (1.6 × 10−19 ) (2 × 1017 )(0.15) + (1.1 × 1015 )(0.045) = 4.8 × 10−3 S/m Then ρ = 1/σ = 2.1 × 102 · m. 5.27. Atomic hydrogen contains 5.5×1025 atoms/m3 at a certain temperature and pressure. When an electric field of 4 kV/m is applied, each dipole formed by the electron and positive nucleus has an effective length of 7.1 × 10−19 m. a) Find P: With all identical dipoles, we have P = Nqd = (5.5 × 1025 )(1.602 × 10−19 )(7.1 × 10−19 ) = 6.26 × 10−12 C/m2 = 6.26 pC/m2 b) Find ǫR: We use P = ǫ0χeE, and so χe = P ǫ0E = 6.26 × 10−12 (8.85 × 10−12)(4 × 103) = 1.76 × 10−4 Then ǫR = 1 + χe = 1.000176. 5.28. In a certain region where the relative permittivity is 2.4, D = 2ax − 4ay + 5az nC/m2. Find: a) E = D ǫ = (2ax − 4ay + 5az) × 10−9 (2.4)(8.85 × 10−12) = 94ax − 188ay + 235az V/m b) P = D − ǫ0E = ǫ0E(ǫR − 1) = (2ax − 4ay + 5az) × 10−9 2.4 (2.4 − 1) = 1.2ax − 2.3ay + 2.9az nC/m2 c) |∇V | = |E| = [(94.1)2 + (188)2 + (235)2 ]1/2 = 315 V/m 73 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 76. 5.29. A coaxial conductor has radii a = 0.8 mm and b = 3 mm and a polystyrene dielectric for which ǫR = 2.56. If P = (2/ρ)aρ nC/m2 in the dielectric, find: a) D and E as functions of ρ: Use E = P ǫ0(ǫR − 1) = (2/ρ) × 10−9aρ (8.85 × 10−12)(1.56) = 144.9 ρ aρ V/m Then D = ǫ0E + P = 2 × 10−9aρ ρ 1 1.56 + 1 = 3.28 × 10−9aρ ρ C/m2 = 3.28aρ ρ nC/m2 b) Find Vab and χe: Use Vab = − 0.8 3 144.9 ρ dρ = 144.9 ln 3 0.8 = 192 V χe = ǫr − 1 = 1.56, as found in part a. c) If there are 4 × 1019 molecules per cubic meter in the dielectric, find p(ρ): Use p = P N = (2 × 10−9/ρ) 4 × 1019 aρ = 5.0 × 10−29 ρ aρ C · m 5.30. Given the potential field V = 200 − 50x + 20y V in a dielectric material for which ǫR = 2.1, find: a) E = −∇V = 50ax − 20ay V/m. b) D = ǫE = (2.1)(8.85 × 10−12)(50ax − 20ay) = 930ax − 372ay pC/m2. c) P = ǫ0E(ǫR − 1) = (8.85 × 10−12)(50ax − 20ay)(1.1) = 487ax − 195ay pC/m2. d) ρv = ∇ · D = 0. e) ρb = −∇ · P = 0 f) ρT = ∇ · ǫ0E = 0 5.31. The surface x = 0 separates two perfect dielectrics. For x > 0, let ǫR = ǫR1 = 3, while ǫR2 = 5 where x < 0. If E1 = 80ax − 60ay − 30az V/m, find: a) EN1: This will be E1 · ax = 80 V/m. b) ET 1. This consists of components of E1 not normal to the surface, or ET 1 = −60ay − 30az V/m. c) ET 1 = (60)2 + (30)2 = 67.1 V/m. d) E1 = (80)2 + (60)2 + (30)2 = 104.4 V/m. e) The angle θ1 between E1 and a normal to the surface: Use cos θ1 = E1 · ax E1 = 80 104.4 ⇒ θ1 = 40.0◦ 74 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 77. 5.31 (continued) f) DN2 = DN1 = ǫR1ǫ0EN1 = 3(8.85 × 10−12)(80) = 2.12 nC/m2. g) DT 2 = ǫR2ǫ0ET 1 = 5(8.85 × 10−12)(67.1) = 2.97 nC/m2. h) D2 = ǫR1ǫ0EN1ax + ǫR2ǫ0ET 1 = 2.12ax − 2.66ay − 1.33az nC/m2. i) P2 = D2 − ǫ0E2 = D2 [1 − (1/ǫR2)] = (4/5)D2 = 1.70ax − 2.13ay − 1.06az nC/m2. j) the angle θ2 between E2 and a normal to the surface: Use cos θ2 = E2 · ax E2 = D2 · ax D2 = 2.12 (2.12)2 = (2.66)2 + (1.33)2 = .581 Thus θ2 = cos−1(.581) = 54.5◦. 5.32. In Fig. 5.18, let D = 3ax − 4ay + 5az nC/m2 and find: a) D2: First, the electric field in region 1 is E1 = 3 2ǫ0 ax − 4 2ǫ0 ay + 5 2ǫ0 az × 10−9 V/m Since, at the dielectric interface, tangential electric field and normal electric flux density are continuous, we may write D2 = ǫR2ǫ0ET 1 + DN1 = 5 2 3ax − 5 2 4ay + 5az = 7.5ax − 10ay + 5az nC/m2 b) DN2 = 5az, as explained above. c) DT 2 = ǫR2ǫ0ET 2 = ǫR2ǫ0ET 1 = 7.5ax − 10ay nC/m2. d) the energy density in each region: we1 = 1 2 ǫR1ǫ0E1 · E1 = 1 2 (2)ǫ0 3 2ǫ0 2 + 4 2ǫ0 2 + 5 2ǫ0 2 × 10−18 = 1.41 µJ/m3 we2 = 1 2 ǫR2ǫ0E2 · E2 = 1 2 (5)ǫ0 3 2ǫ0 2 + 4 2ǫ0 2 + 5 5ǫ0 2 × 10−18 = 2.04 µJ/m3 e) the angle that D2 makes with az: Use D2 · az = |D2| cos θ = Dz = 5. where |D2| = (7.5)2 + (10)2 + (5)2 1/2 = 13.5. So θ = cos−1(5/13.5) = 68◦. f) D2/D1 = (7.5)2 + (10)2 + (5)2 1/2 / (3)2 + (4)2 + (5)2 1/2 = 1.91. g) P2/P1: First P1 = ǫ0E1(ǫR1 − 1) = 1.5ax − 2ay + 2.5az nC/m2. Then P2 = ǫ0E2(ǫR2 − 1) = 6ax − 8ay + 4az nC/m2. So P2 P1 = [(6)2 + (8)2 + (4)2]1/2 [(1.5)2 + (2)2 + (2.5)2]1/2 = 3.04 75 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 78. 5.33. Two perfect dielectrics have relative permittivities ǫR1 = 2 and ǫR2 = 8. The planar interface between them is the surface x − y + 2z = 5. The origin lies in region 1. If E1 = 100ax + 200ay − 50az V/m, find E2: We need to find the components of E1 that are normal and tangent to the boundary, and then apply the appropriate boundary conditions. The normal component will be EN1 = E1 · n. Taking f = x − y + 2z, the unit vector that is normal to the surface is n = ∇f |∇f | = 1 √ 6 ax − ay + 2az This normal will point in the direction of increasing f , which will be away from the origin, or into region 2 (you can visualize a portion of the surface as a triangle whose vertices are on the three coordinate axes at x = 5, y = −5, and z = 2.5). So EN1 = (1/ √ 6)[100 − 200 − 100] = −81.7 V/m. Since the magnitude is negative, the normal component points into region 1 from the surface. Then EN1 = −81.65 1 √ 6 [ax − ay + 2az] = −33.33ax + 33.33ay − 66.67az V/m Now, the tangential component will be ET 1 = E1 − EN1 = 133.3ax + 166.7ay + 16.67az Our boundary conditions state that ET 2 = ET 1 and EN2 = (ǫR1/ǫR2)EN1 = (1/4)EN1. Thus E2 = ET 2 + EN2 = ET 1 + 1 4 EN1 = 133.3ax + 166.7ay + 16.67az − 8.3ax + 8.3ay − 16.67az = 125ax + 175ay V/m 5.34. Let the spherical surfaces r = 4 cm and r = 9 cm be separated by two perfect dielectric shells, ǫR1 = 2 for 4 < r < 6 cm and ǫR2 = 5 for 6 < r < 9 cm. If E1 = (2000/r2)ar V/m, find: a) E2: Since E is normal to the interface between ǫR1 and ǫR2, D will be continuous across the boundary, and so D1 = 2ǫ0(2000) r2 ar = D2 Then E2 = D2 5ǫ0 = 2 5 2000 r2 ar = 800 r2 ar V/m b) the total electrostatic energy stored in each region: In region 1, the energy density is we1 = 1 2 ǫR1ǫ0|E1|2 = 1 2 (2)ǫ0 (2000)2 r4 J/m3 In region 2: we2 = 1 2 ǫR2ǫ0|E2|2 = 1 2 (5)ǫ0 (800)2 r4 J/m3 76 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 79. 5.34. (continued) The energies in each region are then Region 1 : We1 = (2000)2 ǫ0 2π 0 π 0 .06 .04 1 r2 r2 sin θ dr dθ dφ = 4πǫ0(2000)2 1 .04 − 1 .06 = 3.7 mJ Region 2 : We2 = (800)2 5 2 ǫ0 2π 0 π 0 .09 .06 1 r2 r2 sin θ dr dθ dφ = 4πǫ0(800)2 5 2 1 .06 − 1 .09 = 0.99 mJ 5.35. Let the cylindrical surfaces ρ = 4 cm and ρ = 9 cm enclose two wedges of perfect dielectrics, ǫR1 = 2 for 0 < φ < π/2, and ǫR2 = 5 for π/2 < φ < 2π. If E1 = (2000/ρ)aρ V/m, find: a) E2: The interfaces between the two media will lie on planes of constant φ, to which E1 is parallel. Thus the field is the same on either side of the boundaries, and so E2 = E1. b) the total electrostatic energy stored in a 1m length of each region: In general we have wE = (1/2)ǫRǫ0E2. So in region 1: WE1 = 1 0 π/2 0 9 4 1 2 (2)ǫ0 (2000)2 ρ2 ρ dρ dφ dz = π 2 ǫ0(2000)2 ln 9 4 = 45.1 µJ In region 2, we have WE2 = 1 0 2π π/2 9 4 1 2 (5)ǫ0 (2000)2 ρ2 ρ dρ dφ dz = 15π 4 ǫ0(2000)2 ln 9 4 = 338 µJ 5.36. Let S = 120 cm2, d = 4 mm, and ǫR = 12 for a parallel-plate capacitor. a) Calculate the capacitance: C = ǫRǫ0S/d = [12ǫ0(120 × 10−4)]/[4 × 10−3] = 3.19 × 10−10 = 319 pF. b) After connecting a 40 V battery across the capacitor, calculate E, D, Q, and the total stored electrostatic energy: E = V/d = 40/(4 × 10−3) = 104 V/m. D = ǫRǫ0E = 12ǫ0 × 104 = 1.06 µC/m2. Then Q = D · n|surf ace × S = 1.06 × 10−6 × (120 × 10−4) = 1.27 × 10−8C = 12.7 nC. Finally We = (1/2)CV 2 0 = (1/2)(319 × 10−12)(40)2 = 255 nJ. c) Thesourceisnowremovedandthedielectriciscarefullywithdrawnfrombetweentheplates. Again calculate E, D, Q, and the energy: With the source disconnected, the charge is constant, and thus so is D: Therefore, Q = 12.7 nC, D = 1.06 µC/m2, and E = D/ǫ0 = 104/8.85 × 10−12 = 1.2 × 105 V/m. The energy is then We = 1 2 D · E × S = 1 2 (1.06 × 10−6 )(1.2 × 105 )(120 × 10−4 )(4 × 10−3 ) = 3.05 µJ d) What is the voltage between the plates? V = E × d = (1.2 × 105)(4 × 10−3) = 480 V. 77 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 80. 5.37. Capacitors tend to be more expensive as their capacitance and maximum voltage, Vmax, increase. The voltage Vmax is limited by the field strength at which the dielectric breaks down, EBD. Which of these dielectrics will give the largest CVmax product for equal plate areas: (a) air: ǫR = 1, EBD = 3 MV/m; (b) barium titanate: ǫR = 1200, EBD = 3 MV/m; (c) silicon dioxide: ǫR = 3.78, EBD = 16 MV/m; (d) polyethylene: ǫR = 2.26, EBD = 4.7 MV/m? Note that Vmax = EBDd, where d is the plate separation. Also, C = ǫRǫ0A/d, and so VmaxC = ǫRǫ0AEBD, where A is the plate area. The maximum CVmax product is found through the maximum ǫREBD product. Trying this with the given materials yields the winner, which is barium titanate. 5.38. A dielectric circular cylinder used between the plates of a capacitor has a thickness of 0.2 mm and a radius of 1.4 cm. The dielectric properties are ǫR = 400 and σ = 10−5 S/m. a) Calculate C: C = ǫRǫ0S d = (400)(8.854 × 10−12)π(1.4 × 10−2)2 2 × 10−4 = 1.09 × 10−8 = 10.9 nF b) Find the quality factor QQF (QQF = ωRC) of the capacitor at f = 10 kHz: Use the relation RC = ǫ/σ to write QQF = ωRC = 2πf ǫ σ = (2π × 104)(400)(8.854 × 10−12) 10−5 = 22.3 c) If the maximum field strength permitted in the dielectric is 2 MV/m, what is the maximum per- missible voltage across the capacitor? Vmax = EBDd = (2 × 106)(2 × 10−4) = 400 V. d) What energy is stored when this voltage is applied? We,max = 1 2 CV 2 max = 1 2 (10.9 × 10−9 )(400)2 = 8.7 × 10−4 = 0.87 mJ 5.39. A parallel plate capacitor is filled with a nonuniform dielectric characterized by ǫR = 2 + 2 × 106x2, where x is the distance from one plate. If S = 0.02 m2, and d = 1 mm, find C: Start by assuming charge density ρs on the top plate. D will, as usual, be x-directed, originating at the top plate and terminating on the bottom plate. The key here is that D will be constant over the distance between plates. This can be understood by considering the x-varying dielectric as constructed of many thin layers, each having constant permittivity. The permittivity changes from layer to layer to approximate the given function of x. The approximation becomes exact as the layer thicknesses approach zero. We know that D, which is normal to the layers, will be continuous across each boundary, and so D is constant over the plate separation distance, and will be given in magnitude by ρs. The electric field magnitude is now E = D ǫ0ǫR = ρs ǫ0(2 + 2 × 106x2) The voltage beween plates is then V0 = 10−3 0 ρs dx ǫ0(2 + 2 × 106x2) = ρs ǫ0 1 √ 4 × 106 tan−1 x √ 4 × 106 2 10−3 0 = ρs ǫ0 1 2 × 103 π 4 Now Q = ρs(.02), and so C = Q V0 = ρs(.02)ǫ0(2 × 103)(4) ρsπ = 4.51 × 10−10 F = 451 pF 78 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 81. 5.40a. The width of the region containing ǫR1 in Fig. 5.19 is 1.2 m. Find ǫR1 if ǫR2 = 2.5 and the total capacitance is 60 nF: The plate areas associated with each capacitor are A1 = 1.2(2) = 2.4 m2 and A2 = 0.8(2) = 1.6 m2. Having parallel capacitors, the capacitances will add, so C = C1 + C2 ⇒ 60 × 10−9 = ǫR1ǫ0(2.4) 2 × 10−3 + 2.5ǫ0(1.6) 2 × 10−3 Solve this to obtain ǫR1 = 4.0. b) Find the width of each region (containing ǫR1 and ǫR2) if Ctotal = 80 nF, ǫR2 = 3ǫR1, and C1 = 2C2: Let w1 be the width of region 1. The above conditions enable us to write: ǫR1ǫ0w1(2) 2 × 10−3 = 2 3ǫR1ǫ0(2 − w1)(2) 2 × 10−3 ⇒ w1 = 6(2 − w1) So that w1 = 12/7 = 1.7 m and w2 = 0.3 m. 5.41. Let ǫR1 = 2.5 for 0 < y < 1 mm, ǫR2 = 4 for 1 < y < 3 mm, and ǫR3 for 3 < y < 5 mm. Conducting surfaces are present at y = 0 and y = 5 mm. Calculate the capacitance per square meter of surface area if: a) ǫR3 is that of air; b) ǫR3 = ǫR1; c) ǫR3 = ǫR2; d) ǫR3 is silver: The combination will be three capacitors in series, for which 1 C = 1 C1 + 1 C2 + 1 C3 = d1 ǫR1ǫ0(1) + d2 ǫR2ǫ0(1) + d3 ǫR3ǫ0(1) = 10−3 ǫ0 1 2.5 + 2 4 + 2 ǫR3 So that C = (5 × 10−3)ǫ0ǫR3 10 + 4.5ǫR3 Evaluating this for the four cases, we find a) C = 3.05 nF for ǫR3 = 1, b) C = 5.21 nF for ǫR3 = 2.5, c) C = 6.32 nF for ǫR3 = 4, and d) C = 9.83 nF if silver (taken as a perfect conductor) forms region 3; this has the effect of removing the term involving ǫR3 from the original formula (first equation line), or equivalently, allowing ǫR3 to approach infinity. 5.42. Cylindrical conducting surfaces are located at ρ = 0.8 cm and 3.6 cm. The region 0.8 < ρ < a contains a dielectric for which ǫR = 4, while ǫR = 2 for a < ρ < 3.6. a) Find a so that the voltage across each dielectric layer is the same: Assuming charge density ρs on the inner cylinder, we have D = ρs(0.8)/ρ aρ, which gives E(0.8 < ρ < a) = (0.8ρs)/(4ǫ0ρ)aρ and E(a < ρ < 3.6) = (0.8ρs)/(2ǫ0ρ)aρ. The voltage between conductors is now V0 = − a 3.6 0.8ρs 2ǫ0ρ dρ − 0.8 a 0.8ρs 4ǫ0ρ dρ = 0.8ρs 2ǫ0 ln 3.6 a + 1 2 ln a 0.8 We require ln 3.6 a = 1 2 ln a 0.8 ⇒ 3.6 a = a 0.8 ⇒ a = 2.2 cm b) Find the total capacitance per meter: Using the part a result, have V0 = 0.8ρs 2ǫ0 ln 3.6 2.2 + 1 2 ln 2.2 0.8 = 0.4ρs ǫ0 79 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 82. 5.42b. (continued) The charge on a unit length of the inner conductor is Q = 2π(0.8)(1)ρs. The capacitance is now C = Q V0 = 2π(0.8)(1)ρs 0.4ρs/ǫ0 = 4πǫ0 = 111 pF/m Note that throughout this problem, I left all dimensions in cm, knowing that all cm units would cancel, leaving the units of capacitance to be those used for ǫ0. 5.43. Two coaxial conducting cylinders of radius 2 cm and 4 cm have a length of 1m. The region between the cylinders contains a layer of dielectric from ρ = c to ρ = d with ǫR = 4. Find the capacitance if a) c = 2 cm, d = 3 cm: This is two capacitors in series, and so 1 C = 1 C1 + 1 C2 = 1 2πǫ0 1 4 ln 3 2 + ln 4 3 ⇒ C = 143 pF b) d = 4 cm, and the volume of the dielectric is the same as in part a: Having equal volumes requires that 32 − 22 = 42 − c2, from which c = 3.32 cm. Now 1 C = 1 C1 + 1 C2 = 1 2πǫ0 ln 3.32 2 + 1 4 ln 4 3.32 ⇒ C = 101 pF 5.44. Conducting cylinders lie at ρ = 3 and ρ = 12 mm; both extend from z = 0 to z = 1 m. Perfect dielectrics occupy the interior region: ǫR = 1 for 3 < ρ < 6 mm, ǫR = 4 for 6 < ρ < 9 mm, and ǫR = 8 for 9 < ρ < 12 mm. a) Calculate C: First we know that D = (3ρs/ρ)aρ C/m2, with ρ expressed in mm. Then, with ρ in mm, E1 = 3ρs ǫ0ρ aρ V/m (3 < ρ < 6) E2 = 3ρs 4ǫ0ρ aρ V/m (6 < ρ < 9) and E3 = 3ρs 8ǫ0ρ aρ V/m (9 < ρ < 12) The voltage between conductors will be: V0 = − 9 12 3ρs 8ǫ0ρ dρ − 6 9 3ρs 4ǫ0ρ dρ − 3 6 3ρs ǫ0ρ dρ × 10−3 (m/mm) = .003ρs ǫ0 1 8 ln 12 9 + 1 4 ln 9 6 + ln 6 3 = .003ρs ǫ0 (0.830) V Now, the charge on the 1 m length of the inner conductor is Q = 2π(.003)(1)ρs. The capacitance is then C = Q V0 = 2π(.003)(1)ρs (.003)ρs(.830)/ǫ0 = 2πǫ0 .830 = 67 pF 80 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 83. 5.44b. If the voltage between the cylinders is 100 V, plot |Eρ| vs. ρ: Have Q = CV0 = (67 × 10−12)(100) = 6.7nC. Then ρs = 6.7 × 10−9 2π(.003)(1) = 355 nC/m2 Then, using the electric field expressions from part a, we find E1 = 3 ρ 355 × 10−9 8.854 × 10−12 = 12 × 104 ρ V/m = 120 ρ kV/m (3 < ρ < 6) where ρ is expressed in mm. Similarly, we find E2 = E1/4 = 30/ρ kV/m (6 < ρ < 9) and E3 = E1/8 = 15 kV/m (9 < ρ < 12). These fields are plotted below. 81 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 84. 5.45. Two conducting spherical shells have radii a = 3 cm and b = 6 cm. The interior is a perfect dielectric for which ǫR = 8. a) Find C: For a spherical capacitor, we know that: C = 4πǫRǫ0 1 a − 1 b = 4π(8)ǫ0 1 3 − 1 6 (100) = 1.92πǫ0 = 53.3 pF b) A portion of the dielectric is now removed so that ǫR = 1.0, 0 < φ < π/2, and ǫR = 8, π/2 < φ < 2π. Again, find C: We recognize here that removing that portion leaves us with two capacitors in parallel (whose C’s will add). We use the fact that with the dielectric completely removed, the capacitance would be C(ǫR = 1) = 53.3/8 = 6.67 pF. With one-fourth the dielectric removed, the total capacitance will be C = 1 4 (6.67) + 3 4 (53.4) = 41.7 pF 5.46. (see Problem 5.44). 5.47. With reference to Fig. 5.17, let b = 6 m, h = 15 m, and the conductor potential be 250 V. Take ǫ = ǫ0. Find values for K1, ρL, a, and C: We have K1 = h + √ h2 + b2 b 2 = 15 + (15)2 + (6)2 6 2 = 23.0 We then have ρL = 4πǫ0V0 ln K1 = 4πǫ0(250) ln(23) = 8.87 nC/m Next, a = √ h2 − b2 = (15)2 − (6)2 = 13.8 m. Finally, C = 2πǫ cosh−1(h/b) = 2πǫ0 cosh−1(15/6) = 35.5 pF 82 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 85. 5.48. A potential function in free space is given by V = −20 + 10 ln (5 + y)2 + x2 (5 − y)2 + x2 a) Describe the 0-V equipotential surface: Setting the given expression equal to zero, we find (5 + y)2 + x2 (5 − y)2 + x2 = e2 = 7.39 So 6.39x2 + 6.39y2 − 83.9y + 160 = 0. Completing the square in the y trinomial leads to x2 + (y − 6.56)2 = 18.1 = (4.25)2, which we recognize as a right circular cylinder whose axis is located at x = 0, y = 6.56, and whose radius is 4.25. b) Describe the 10-V equipotential surface: In this case, the given expression is set equal to ten, leading to (5 + y)2 + x2 (5 − y)2 + x2 = e3 = 20.1 So 19.1x2 + 19.1y2 − 211y + 477 = 0. Following the same procedure as in part a, this becomes x2 + (y − 5.52)2 = 5.51 = (2.35)2, which we recognize again as a right circular cylinder with axis at x = 0, y = 5.52, and of radius 2.35. 5.49. A 2 cm diameter conductor is suspended in air with its axis 5 cm from a conducting plane. Let the potential of the cylinder be 100 V and that of the plane be 0 V. Find the surface charge density on the: a) cylinder at a point nearest the plane: The cylinder will image across the plane, producing an equivalent two-cylinder problem, with the second one at location 5 cm below the plane. We will take the plane as the zy plane, with the cylinder positions at x = ±5. Now b = 1 cm, h = 5 cm, and V0 = 100 V. Thus a = √ h2 − b2 = 4.90 cm. Then K1 = [(h + a)/b]2 = 98.0, and ρL = (4πǫ0V0)/ ln K1 = 2.43 nC/m. Now D = ǫ0E = − ρL 2π (x + a)ax + yay (x + a)2 + y2 − (x − a)ax + yay (x − a)2 + y2 and ρs, max = D · (−ax) x=h−b,y=0 = ρL 2π h − b + a (h − b + a)2 − h − b − a (h − b − a)2 = 473 nC/m2 b) plane at a point nearest the cylinder: At x = y = 0, D(0, 0) = − ρL 2π aax a2 − −aax a2 = − ρL 2π 2 a ax from which ρs = D(0, 0) · ax = − ρL πa = −15.8 nC/m2 83 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 86. CHAPTER 6. 6.1 Construct a curvilinear square map for a coaxial capacitor of 3-cm inner radius and 8-cm outer radius. These dimensions are suitable for the drawing. a) Use your sketch to calculate the capacitance per meter length, assuming ǫR = 1: The sketch is shown below. Note that only a 9◦ sector was drawn, since this would then be duplicated 40 times around the circumference to complete the drawing. The capacitance is thus C . = ǫ0 NQ NV = ǫ0 40 6 = 59 pF/m b) Calculate an exact value for the capacitance per unit length: This will be C = 2πǫ0 ln(8/3) = 57 pF/m 84 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 87. 6.2 Construct a curvilinear-square map of the potential field about two parallel circular cylinders, each of 2.5 cm radius, separated by a center-to-center distance of 13cm. These dimensions are suitable for the actual sketch if symmetry is considered. As a check, compute the capacitance per meter both from your sketch and from the exact formula. Assume ǫR = 1. Symmetry allows us to plot the field lines and equipotentials over just the first quadrant, as is done in the sketch below (shown to one-half scale). The capacitance is found from the formula C = (NQ/NV )ǫ0, where NQ is twice the number of squares around the perimeter of the half-circle and NV is twice the number of squares between the half-circle and the left vertical plane. The result is C = NQ NV ǫ0 = 32 16 ǫ0 = 2ǫ0 = 17.7 pF/m We check this result with that using the exact formula: C = πǫ0 cosh−1(d/2a) = πǫ0 cosh−1(13/5) = 1.95ǫ0 = 17.3 pF/m 85 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 88. 6.3. Construct a curvilinear square map of the potential field between two parallel circular cylinders, one of 4-cm radius inside one of 8-cm radius. The two axes are displaced by 2.5 cm. These dimensions are suitable for the drawing. As a check on the accuracy, compute the capacitance per meter from the sketch and from the exact expression: C = 2πǫ cosh−1 (a2 + b2 − D2)/(2ab) where a and b are the conductor radii and D is the axis separation. The drawing is shown below. Use of the exact expression above yields a capacitance value of C = 11.5ǫ0 F/m. Use of the drawing produces: C . = 22 × 2 4 ǫ0 = 11ǫ0 F/m 86 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 89. 6.4. A solid conducting cylinder of 4-cm radius is centered within a rectangular conducting cylinder with a 12-cm by 20-cm cross-section. a) Make a full-size sketch of one quadrant of this configuration and construct a curvilinear-square map for its interior: The result below could still be improved a little, but is nevertheless sufficient for a reasonable capacitance estimate. Note that the five-sided region in the upper right corner has been partially subdivided (dashed line) in anticipation of how it would look when the next-level subdivision is done (doubling the number of field lines and equipotentials). b) Assume ǫ = ǫ0 and estimate C per meter length: In this case NQ is the number of squares around the full perimeter of the circular conductor, or four times the number of squares shown in the drawing. NV is the number of squares between the circle and the rectangle, or 5. The capacitance is estimated to be C = NQ NV ǫ0 = 4 × 13 5 ǫ0 = 10.4ǫ0 . = 90 pF/m 87 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 90. 6.5. The inner conductor of the transmission line shown in Fig. 6.12 has a square cross-section 2a × 2a, while the outer square is 5a × 5a. The axes are displaced as shown. (a) Construct a good-sized drawing of the transmission line, say with a = 2.5 cm, and then prepare a curvilinear-square plot of the electrostatic field between the conductors. (b) Use the map to calculate the capacitance per meter length if ǫ = 1.6ǫ0. (c) How would your result to part b change if a = 0.6 cm? a) The plot is shown below. Some improvement is possible, depending on how much time one wishes to spend. b) From the plot, the capacitance is found to be C . = 16 × 2 4 (1.6)ǫ0 = 12.8ǫ0 . = 110 pF/m c) If a is changed, the result of part b would not change, since all dimensions retain the same relative scale. 88 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 91. 6.6. Let the inner conductor of the transmission line shown in Fig. 6.12 be at a potential of 100V, while the outer is at zero potential. Construct a grid, 0.5a on a side, and use iteration to find V at a point that is a units above the upper right corner of the inner conductor. Work to the nearest volt: The drawing is shown below, and we identify the requested voltage as 38 V. 89 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 92. 6.7. Use the iteration method to estimate the potentials at points x and y in the triangular trough of Fig. 6.13. Work only to the nearest volt: The result is shown below. The mirror image of the values shown occur at the points on the other side of the line of symmetry (dashed line). Note that Vx = 78 V and Vy = 26 V. 90 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 93. 6.8. Use iteration methods to estimate the potential at point x in the trough shown in Fig. 6.14. Working to the nearest volt is sufficient. The result is shown below, where we identify the voltage at x to be 40 V. Note that the potentials in the gaps are 50 V. 6.9. Using the grid indicated in Fig. 6.15, work to the nearest volt to estimate the potential at point A: The voltages at the grid points are shown below, where VA is found to be 19 V. Half the figure is drawn since mirror images of all values occur across the line of symmetry (dashed line). 91 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 94. 6.10. Conductors having boundaries that are curved or skewed usually do not permit every grid point to coincide with the actual boundary. Figure 6.16a illustrates the situation where the potential at V0 is to be estimated in terms of V1, V2, V3, and V4, and the unequal distances h1, h2, h3, and h4. a) Show that V0 . = V1 1 + h1 h3 1 + h1h3 h4h2 + V2 1 + h2 h4 1 + h2h4 h1h3 + V3 1 + h3 h1 1 + h1h3 h4h2 + V4 1 + h4 h2 1 + h4h2 h3h1 note error, corrected here, in the equation (second term) Referring to the figure, we write: ∂V ∂x M1 . = V1 − V0 h1 ∂V ∂x M3 . = V0 − V3 h3 Then ∂2V ∂x2 V0 . = (V1 − V0)/h1 − (V0 − V3)/h3 (h1 + h3)/2 = 2V1 h1(h1 + h3) + 2V3 h3(h1 + h3) − 2V0 h1h3 We perform the same procedure along the y axis to obtain: ∂2V ∂y2 V0 . = (V2 − V0)/h2 − (V0 − V4)/h4 (h2 + h4)/2 = 2V2 h2(h2 + h4) + 2V4 h4(h2 + h4) − 2V0 h2h4 Then, knowing that ∂2V ∂x2 V0 + ∂2V ∂y2 V0 = 0 the two equations for the second derivatives are added to give 2V1 h1(h1 + h3) + 2V2 h2(h2 + h4) + 2V3 h3(h1 + h3) + 2V4 h4(h2 + h4) = V0 h1h3 + h2h4 h1h2h3h4 Solve for V0 to obtain the given equation. b) Determine V0 in Fig. 6.16b: Referring to the figure, we note that h1 = h2 = a. The other two distances are found by writing equations for the circles: (0.5a + h3)2 + a2 = (1.5a)2 and (a + h4)2 + (0.5a)2 = (1.5a)2 These are solved to find h3 = 0.618a and h4 = 0.414a. The four distances and potentials are now substituted into the given equation: V0 . = 80 1 + 1 .618 1 + .618 .414 + 60 1 + 1 .414 1 + .414 .618 + 100 (1 + .618) 1 + .618 .414 + 100 (1 + .414) 1 + .414 .618 = 90 V 92 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 95. 6.11. Consider the configuration of conductors and potentials shown in Fig. 6.17. Using the method described in Problem 10, write an expression for Vx (not V0): The result is shown below, where Vx = 70 V. 6.12a) After estimating potentials for the configuation of Fig. 6.18, use the iteration method with a square grid 1 cm on a side to find better estimates at the seven grid points. Work to the nearest volt: 25 50 75 50 25 0 48 100 48 0 0 42 100 42 0 0 19 34 19 0 0 0 0 0 0 b) Construct a 0.5 cm grid, establish new rough estimates, and then use the iteration method on the 0.5 cm grid. Again, work to the nearest volt: The result is shown below, with values for the original grid points underlined: 25 50 50 50 75 50 50 50 25 0 32 50 68 100 68 50 32 0 0 26 48 72 100 72 48 26 0 0 23 45 70 100 70 45 23 0 0 20 40 64 100 64 40 20 0 0 15 30 44 54 44 30 15 0 0 10 19 26 30 26 19 10 0 0 5 9 12 14 12 9 5 0 0 0 0 0 0 0 0 0 0 93 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 96. 6.12c. Use the computer to obtain values for a 0.25 cm grid. Work to the nearest 0.1 V: Values for the left half of the configuration are shown in the table below. Values along the vertical line of symmetry are included, and the original grid values are underlined. 25 50 50 50 50 50 50 50 75 0 26.5 38.0 44.6 49.6 54.6 61.4 73.2 100 0 18.0 31.0 40.7 49.0 57.5 67.7 81.3 100 0 14.5 27.1 38.1 48.3 58.8 70.6 84.3 100 0 12.8 24.8 36.2 47.3 58.8 71.4 85.2 100 0 11.7 23.1 34.4 45.8 57.8 70.8 85.0 100 0 10.8 21.6 32.5 43.8 55.8 69.0 83.8 100 0 10.0 20.0 30.2 40.9 52.5 65.6 81.2 100 0 9.0 18.1 27.4 37.1 47.6 59.7 75.2 100 0 7.9 15.9 24.0 32.4 41.2 50.4 59.8 67.2 0 6.8 13.6 20.4 27.3 34.2 40.7 46.3 49.2 0 5.6 11.2 16.8 22.2 27.4 32.0 35.4 36.8 0 4.4 8.8 13.2 17.4 21.2 24.4 26.6 27.4 0 3.3 6.6 9.8 12.8 15.4 17.6 19.0 19.5 0 2.2 4.4 6.4 8.4 10.0 11.4 12.2 12.5 0 1.1 2.2 3.2 4.2 5.0 5.6 6.0 6.1 0 0 0 0 0 0 0 0 0 94 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 97. 6.13. Perfectly-conducting concentric spheres have radii of 2 and 6 cm. The region 2 < r < 3 cm is filled with a solid conducting material for which σ = 100 S/m, while the portion for which 3 < r < 6 cm has σ = 25 S/m. The inner sphere is held at 1 V while the outer is at V = 0. a. Find E and J everywhere: From symmetry, E and J will be radially-directed, and we note the fact that the current, I, must be constant at any cross-section; i.e., through any spherical surface at radius r between the spheres. Thus we require that in both regions, J = I 4πr2 ar The fields will thus be E1 = I 4πσ1r2 ar (2 < r < 3) and E2 = I 4πσ2r2 ar (3 < r < 6) where σ1 = 100 S/m and σ2 = 25 S/m. Since we know the voltage between spheres (1V), we can find the value of I through: 1 V = − .03 .06 I 4πσ2r2 dr − .02 .03 I 4πσ1r2 dr = I 0.24π 1 σ1 + 1 σ2 and so I = 0.24π (1/σ1 + 1/σ2) = 15.08 A Then finally, with I = 15.08 A substituted into the field expressions above, we find E1 = .012 r2 ar V/m (2 < r < 3) and E2 = .048 r2 ar V/m (3 < r < 6) The current density is now J = σ1E1 = σ2E2 = 1.2 r2 A/m (2 < r < 6) b) What resistance would be measured between the two spheres? We use R = V I = 1 V 15.08 A = 6.63 × 10−2 c) What is V at r = 3 cm? This we find through V = − .03 .06 .048 r2 dr = .048 1 .03 − 1 .06 = 0.8 V 95 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 98. 6.14. The cross-section of the transmission line shown in Fig. 6.12 is drawn on a sheet of conducting paper with metallic paint. The sheet resistance is 2000 /sq and the dimension a is 2 cm. a) Assuming a result for Prob. 6b of 110 pF/m, what total resistance would be measured between the metallic conductors drawn on the conducting paper? We assume a paper thickness of t m, so that the capacitance is C = 110t pF, and the surface resistance is Rs = 1/(σt) = 2000 /sq. We now use RC = ǫ σ ⇒ R = ǫ σC = ǫRst 110 × 10−12t = (1.6 × 8.854 × 10−12)(2000) 110 × 10−12 = 257.6 b) What would the total resistance be if a = 2 cm? The result is independent of a, provided the proportions are maintained. So again, R = 257.6 . 6.15. two concentric annular rings are painted on a sheet of conducting paper with a highly conducting metal paint. The four radii are 1, 1.2, 3.5, and 3.7 cm. Connections made to the two rings show a resistance of 215 ohms between them. a) What is Rs for the conducting paper? Using the two radii (1.2 and 3.5 cm) at which the rings are at their closest separation, we first evaluate the capacitance: C = 2πǫ0t ln(3.5/1.2) = 5.19 × 10−11 t F where t is the unknown paper coating thickness. Now use RC = ǫ0 σ ⇒ R = 8.85 × 10−12 5.19 × 10−11σt = 215 Thus Rs = 1 σt = (51.9)(215) 8.85 = 1.26 k /sq b) If the conductivity of the material used as the surface of the paper is 2 S/m, what is the thickness of the coating? We use t = 1 σRs = 1 2 × 1.26 × 103 = 3.97 × 10−4 m = 0.397 mm 96 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 99. 6.16. The square washer shown in Fig. 6.19 is 2.4 mm thick and has outer dimensions of 2.5 × 2.5 cm and inner dimensions of 1.25 × 1.25 cm. The inside and outside surfaces are perfectly-conducting. If the material has a conductivity of 6 S/m, estimate the resistance offered between the inner and outer surfaces (shown shaded in Fig. 6.19). A few curvilinear squares are suggested: First we find the surface resistance, Rs = 1/(σt) = 1/(6 × 2.4 × 10−3) = 69.4 /sq. Having found this, we can construct the total resistance by using the fundamental square as a building block. Specifically, R = Rs(Nl/Nw) where Nl is the number of squares between the inner and outer surfaces and Nw is the number of squares around the perimeter of the washer. These numbers are found from the curvilinear square plot shown below, which covers one-eighth the washer. The resistance is thus R . = 69.4[4/(8 × 5)] . = 6.9 . 6.17. A two-wire transmission line consists of two parallel perfectly-conducting cylinders, each having a radius of 0.2 mm, separated by center-to-center distance of 2 mm. The medium surrounding the wires has ǫR = 3 and σ = 1.5 mS/m. A 100-V battery is connected between the wires. Calculate: a) the magnitude of the charge per meter length on each wire: Use C = πǫ cosh−1(h/b) = π × 3 × 8.85 × 10−12 cosh−1 (1/0.2) = 3.64 × 10−9 C/m Then the charge per unit length will be Q = CV0 = (3.64 × 10−11 )(100) = 3.64 × 10−9 C/m = 3.64 nC/m b) the battery current: Use RC = ǫ σ ⇒ R = 3 × 8.85 × 10−12 (1.5 × 10−3)(3.64 × 10−11) = 486 Then I = V0 R = 100 486 = 0.206 A = 206 mA 97 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 100. 6.18. A coaxial transmission line is modelled by the use of a rubber sheet having horizontal dimensions that are 100 times those of the actual line. Let the radial coordinate of the model be ρm. For the line itself, let the radial dimension be designated by ρ as usual; also, let a = 0.6 mm and b = 4.8 mm. The model is 8 cm in height at the inner conductor and zero at the outer. If the potential of the inner conductor is 100 V: a) Find the expression for V (ρ): Assuming charge density ρs on the inner conductor, we use Gauss’ Law to find 2πρD = 2πaρs, from which E = D/ǫ = aρs/(ǫρ) in the radial direction. The potential difference between inner and outer conductors is Vab = V0 = − a b aρs ǫρ dρ = aρs ǫ ln b a from which ρs = ǫV0 a ln(b/a) ⇒ E = V0 ρ ln(b/a) Now, as a function of radius, and assuming zero potential on the outer conductor, the potential function will be: V (ρ) = − ρ b V0 ρ′ ln(b/a) dρ′ = V0 ln(b/ρ) ln(b/a) = 100 ln(.0048/ρ) ln(.0048/.0006) = 48.1 ln .0048 ρ V b) Write the model height as a function of ρm (not ρ): We use the part a result, since the gravitational function must be the same as that for the electric potential. We replace V0 by the maximum height, and multiply all dimensions by 100 to obtain: h(ρm) = 0.08 ln(.48/ρm) ln(.48/.06) = 0.038 ln .48 ρm m 98 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 101. CHAPTER 7 7.1. Let V = 2xy2z3 and ǫ = ǫ0. Given point P (1, 2, −1), find: a) V at P : Substituting the coordinates into V , find VP = −8 V. b) E at P : We use E = −∇V = −2y2z3ax − 4xyz3ay − 6xy2z2az, which, when evaluated at P , becomes EP = 8ax + 8ay − 24az V/m c) ρv at P : This is ρv = ∇ · D = −ǫ0∇2V = −4xz(z2 + 3y2) C/m3 d) the equation of the equipotential surface passing through P : At P , we know V = −8 V, so the equation will be xy2z3 = −4. e) the equation of the streamline passing through P : First, Ey Ex = dy dx = 4xyz3 2y2z3 = 2x y Thus ydy = 2xdx, and so 1 2 y2 = x2 + C1 Evaluating at P , we find C1 = 1. Next, Ez Ex = dz dx = 6xy2z2 2y2z3 = 3x z Thus 3xdx = zdz, and so 3 2 x2 = 1 2 z2 + C2 Evaluating at P , we find C2 = 1. The streamline is now specified by the equations: y2 − 2x2 = 2 and 3x2 − z2 = 2 f) Does V satisfy Laplace’s equation? No, since the charge density is not zero. 7.2. A potential field V exists in a region where ǫ = f (x). Find ∇2V if ρv = 0. First, D = ǫ(x)E = −f (x)∇V . Then ∇ · D = ρv = 0 = ∇ · (−f (x)∇V ). So 0 = ∇ · (−f (x)∇V ) = − df dx ∂V ∂x + f (x) ∂2V ∂x2 f (x) ∂2V ∂y2 + f (x) ∂2V ∂z2 = − df dx ∂V ∂x + f (x)∇2 V Therefore, ∇2 V = − 1 f (x) df dx ∂V ∂x 99 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 102. 7.3. Let V (x, y) = 4e2x + f (x) − 3y2 in a region of free space where ρv = 0. It is known that both Ex and V are zero at the origin. Find f (x) and V (x, y): Since ρv = 0, we know that ∇2V = 0, and so ∇2 V = ∂2V ∂x2 + ∂2V ∂y2 = 16e2x + d2f dx2 − 6 = 0 Therefore d2f dx2 = −16e2x + 6 ⇒ df dx = −8e2x + 6x + C1 Now Ex = ∂V ∂x = 8e2x + df dx and at the origin, this becomes Ex(0) = 8 + df dx x=0 = 0(as given) Thus df/dx |x=0 = −8, and so it follows that C1 = 0. Integrating again, we find f (x, y) = −4e2x + 3x2 + C2 which at the origin becomes f (0, 0) = −4 + C2. However, V (0, 0) = 0 = 4 + f (0, 0). So f (0, 0) = −4 and C2 = 0. Finally, f (x, y) = −4e2x + 3x2, and V (x, y) = 4e2x −4e2x +3x2−3y2 = 3(x2 − y2). 7.4. Given the potential field V = A ln tan2(θ/2) + B: a) Show that ∇2V = 0: Since V is a function only of θ, ∇2 V = 1 r2 sin θ) d dθ sin θ dV dθ where dV dθ = d dθ A ln tan2 (θ/2) + B = d dθ (2A ln tan(θ/2)) = A sin(θ/2) cos(θ/2) = 2A sin θ Then ∇2 V = 1 r2 sin θ) d dθ sin θ 2A sin θ = 0 b) Select A and B so that V = 100 V and Eθ = 500 V/m at P (r = 5, θ = 60◦, φ = 45◦): First, Eθ = −∇V = − 1 r dV dθ = − 2A r sin θ = − 2A 5 sin 60 = −0.462A = 500 So A = −1082.5 V. Then VP = −(1082.5) ln tan2 (30◦ ) + B = 100 ⇒ B = −1089.3 V Summarizing, V (θ) = −1082.5 ln tan2(θ/2) − 1089.3. 100 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 103. 7.5. Given the potential field V = (Aρ4 + Bρ−4) sin 4φ: a) Show that ∇2V = 0: In cylindrical coordinates, ∇2 V = 1 ρ ∂ ∂ρ ρ ∂V ∂ρ + 1 ρ2 ∂2V ∂φ2 = 1 ρ ∂ ∂ρ ρ(4Aρ3 − 4Bρ−5 ) sin 4φ − 1 ρ2 16(Aρ4 + Bρ−4 ) sin 4φ = 16 ρ (Aρ3 + Bρ−5 ) sin 4φ − 16 ρ2 (Aρ4 + Bρ−4 ) sin 4φ = 0 b) Select A and B so that V = 100 V and |E| = 500 V/m at P (ρ = 1, φ = 22.5◦, z = 2): First, E = −∇V = − ∂V ∂ρ aρ − 1 ρ ∂V ∂φ aφ = −4 (Aρ3 − Bρ−5 ) sin 4φ aρ + (Aρ3 + Bρ−5 ) cos 4φ aφ and at P , EP = −4(A−B) aρ. Thus |EP | = ±4(A−B). Also, VP = A+B. Our two equations are: 4(A − B) = ±500 and A + B = 100 We thus have two pairs of values for A and B: A = 112.5, B = −12.5 or A = −12.5, B = 112.5 7.6. If V = 20 sin θ/r3 V in free space, find: a) ρv at P (r = 2, θ = 30◦, φ = 0): We use Poisson’s equation in free space, ∇2V = −ρv/ǫ0, where, with no φ variation: ∇2 V = 1 r2 ∂ ∂r r2 ∂V ∂r + 1 r2 sin θ ∂ ∂θ sin θ ∂V ∂θ Substituting: ∇2 V = 1 r2 ∂ ∂r −r2 60 sin θ r4 + 1 r2 sin θ ∂ ∂θ sin θ 20 cos θ r3 = 1 r2 ∂ ∂r −60 sin θ r2 + 1 r2 sin θ ∂ ∂θ 10 sin 2θ r3 = 120 sin θ r5 + 20 cos 2θ r5 sin θ = 20(4 sin2 θ + 1) r5 sin θ = − ρv ǫ0 So ρvP = −ǫ0 20(4 sin2 θ + 1) r5 sin θ r=2,θ=30 = −2.5ǫ0 = −22.1 pC/m3 101 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 104. 7.6b. the total charge within the spherical shell 1 < r < 2 m: We integrate the charge density found in part a over the specified volume: Q = −ǫ0 2π 0 π 0 2 1 20(4 sin2 θ + 1) r5 sin θ r2 sin θ dr dθ dφ = −2π(20)ǫ0 π 0 2 1 (4 sin2 θ + 1) r3 dr dθ = −40πǫ0 2 1 3π r3 dr = 60π2 ǫ0 1 r2 2 1 = −45π2 ǫ0 = −3.9 nC 7.7. Let V = (cos 2φ)/ρ in free space. a) Find the volume charge density at point A(0.5, 60◦, 1): Use Poisson’s equation: ρv = −ǫ0∇2 V = −ǫ0 1 ρ ∂ ∂ρ ρ ∂V ∂ρ + 1 ρ2 ∂2V ∂φ2 = −ǫ0 1 ρ ∂ ∂ρ − cos 2φ ρ − 4 ρ2 cos 2φ ρ = 3ǫ0 cos 2φ ρ3 So at A we find: ρvA = 3ǫ0 cos(120◦) 0.53 = −12ǫ0 = −106 pC/m3 b) Find the surface charge density on a conductor surface passing through B(2, 30◦, 1): First, we find E: E = −∇V = − ∂V ∂ρ aρ − 1 ρ ∂V ∂φ aφ = cos 2φ ρ2 aρ + 2 sin 2φ ρ2 aφ At point B the field becomes EB = cos 60◦ 4 aρ + 2 sin 60◦ 4 aφ = 0.125 aρ + 0.433 aφ The surface charge density will now be ρsB = ±|DB| = ±ǫ0|EB| = ±0.451ǫ0 = ±0.399 pC/m2 The charge is positive or negative depending on which side of the surface we are considering. The problem did not provide information necessary to determine this. 7.8. Let V1(r, θ, φ) = 20/r and V2(r, θ, φ) = (4/r) + 4. a) State whether V1 and V2 satisfy Laplace’s equation: ∇2 V1 = 1 r2 d dr r2 dV1 dr = 1 r2 d dr r2 −20 r2 = 0 ∇2 V2 = 1 r2 d dr r2 dV2 dr = 1 r2 d dr r2 −4 r2 = 0 102 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 105. 7.8b. Evaluate V1 and V2 on the closed surface r = 4: V1(r = 4) = 20 4 = 5 V2(r = 4) = 4 4 + 4 = 5 c) Conciliate your results with the uniqueness theorem: Uniqueness specifies that there is only one potential that will satisfy all the given boundary conditions. While both potentials have the same value at r = 4, they do not as r → ∞. So they apply to different situations. 7.9. The functions V1(ρ, φ, z) and V2(ρ, φ, z) both satisfy Laplace’s equation in the region a < ρ < b, 0 ≤ φ < 2π, −L < z < L; each is zero on the surfaces ρ = b for −L < z < L; z = −L for a < ρ < b; and z = L for a < ρ < b; and each is 100 V on the surface ρ = a for −L < z < L. a) In the region specified above, is Laplace’s equation satisfied by the functions V1 + V2, V1 − V2, V1 + 3, and V1V2? Yes for the first three, since Laplace’s equation is linear. No for V1V2. b) Ontheboundarysurfacesspecified, arethepotentialvaluesgivenaboveobtainedfromthefunctions V1 +V2, V1 −V2, V1 +3, and V1V2? At the 100 V surface (ρ = a), No for all. At the 0 V surfaces, yes, except for V1 + 3. c) Are the functions V1 + V2, V1 − V2, V1 + 3, and V1V2 identical with V1? Only V2 is, since it is given as satisfying all the boundary conditions that V1 does. Therefore, by the uniqueness theorem, V2 = V1. The others, not satisfying the boundary conditions, are not the same as V1. 7.10. Conducting planes at z = 2cm and z = 8cm are held at potentials of −3V and 9V, respectively. The region between the plates is filled with a perfect dielectric with ǫ = 5ǫ0. Find and sketch: a) V (z): We begin with the general solution of the one-dimensional Laplace equation in rectangular coordinates: V (z) = Az + B. Applying the boundary conditions, we write −3 = A(2) + B and 9 = A(8) + B. Subtracting the former equation from the latter, we find 12 = 6A or A = 2 V/cm. Using this we find B = −7 V. Finally, V (z) = 2z − 7 V (z in cm) or V (z) = 200z − 7 V (z in m). b) Ez(z): We use E = −∇V = −(dV/dz)az = −2 V/cm = −200 V/m. c) Dz(z): Working in meters, have Dz = ǫEz = −200ǫ = −1000ǫ0 C/m2 7.11. The conducting planes 2x + 3y = 12 and 2x + 3y = 18 are at potentials of 100 V and 0, respectively. Let ǫ = ǫ0 and find: a) V at P (5, 2, 6): The planes are parallel, and so we expect variation in potential in the direction normal to them. Using the two boundary condtions, our general potential function can be written: V (x, y) = A(2x + 3y − 12) + 100 = A(2x + 3y − 18) + 0 and so A = −100/6. We then write V (x, y) = − 100 6 (2x + 3y − 18) = − 100 3 x − 50y + 300 and VP = −100 3 (5) − 100 + 300 = 33.33 V. b) Find E at P : Use E = −∇V = 100 3 ax + 50 ay V/m 103 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 106. 7.12. Conducting cylinders at ρ = 2 cm and ρ = 8 cm in free space are held at potentials of 60mV and -30mV, respectively. a) Find V (ρ): Working in volts and meters, we write the general one-dimensional solution to the Laplace equation in cylindrical coordinates, assuming radial variation: V (ρ) = A ln(ρ) + B. Applying the given boundary conditions, this becomes V (2cm) = .060 = A ln(.02) + B and V (8cm) = −.030 = A ln(.08) + B. Subtracting the former equation from the latter, we find −.090 = A ln(.08/.02) = A ln 4 ⇒ A = −.0649. B is then found through either equation; e.g., B = .060 + .0649 ln(.02) = −.1940. Finally, V (ρ) = −.0649 ln ρ − .1940. b) Find Eρ(ρ): E = −∇V = −(dV /dρ)aρ = (.0649/ρ)aρ V/m. c) Find the surface on which V = 30 mV: Use .03 = −.0649 ln ρ − .1940 ⇒ ρ = .0317 m = 3.17 cm. 7.13. Coaxial conducting cylinders are located at ρ = 0.5 cm and ρ = 1.2 cm. The region between the cylinders is filled with a homogeneous perfect dielectric. If the inner cylinder is at 100V and the outer at 0V, find: a) the location of the 20V equipotential surface: From Eq. (16) we have V (ρ) = 100 ln(.012/ρ) ln(.012/.005) V We seek ρ at which V = 20 V, and thus we need to solve: 20 = 100 ln(.012/ρ) ln(2.4) ⇒ ρ = .012 (2.4)0.2 = 1.01 cm b) Eρ max: We have Eρ = − ∂V ∂ρ = − dV dρ = 100 ρ ln(2.4) whose maximum value will occur at the inner cylinder, or at ρ = .5 cm: Eρ max = 100 .005 ln(2.4) = 2.28 × 104 V/m = 22.8 kV/m c) ǫR if the charge per meter length on the inner cylinder is 20 nC/m: The capacitance per meter length is C = 2πǫ0ǫR ln(2.4) = Q V0 We solve for ǫR: ǫR = (20 × 10−9) ln(2.4) 2πǫ0(100) = 3.15 104 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 107. 7.14. Two semi-infinite planes are located at φ = −α and φ = α, where α < π/2. A narrow insulating strip separates them along the z axis. The potential at φ = −α is V0, while V = 0 at φ = α. a) Find V (φ) in terms of α and V0: We use the one-dimensional solution form for Laplace’s equation assuming variation along φ: V (φ) = Aφ + B. The boundary conditions are then substituted: V0 = −Aα + B and 0 = Aα + B. Subtract the latter equation from the former to obtain: V0 = −2Aα ⇒ A = −V0/(2α). Then 0 = −V0/(2α)α + B ⇒ B = V0/2. Finally V (φ) = V0 2 1 − φ α V b) Find Eφ at φ = 20◦, ρ = 2 cm, if V0 = 100 V and α = 30◦: Eφ = − 1 ρ dV dρ = V0 2αρ V/m Then E(2cm, 20◦ ) = 100 2(30 × 2π/360)(.02) = 4.8 kV/m 7.15. The two conducting planes illustrated in Fig. 7.8 are defined by 0.001 < ρ < 0.120 m, 0 < z < 0.1 m, φ = 0.179 and 0.188 rad. The medium surrounding the planes is air. For region 1, 0.179 < φ < 0.188, neglect fringing and find: a) V (φ): The general solution to Laplace’s equation will be V = C1φ + C2, and so 20 = C1(.188) + C2 and 200 = C1(.179) + C2 Subtracting one equation from the other, we find −180 = C1(.188 − .179) ⇒ C1 = −2.00 × 104 Then 20 = −2.00 × 104 (.188) + C2 ⇒ C2 = 3.78 × 103 Finally, V (φ) = (−2.00 × 104)φ + 3.78 × 103 V. b) E(ρ): Use E(ρ) = −∇V = − 1 ρ dV dφ = 2.00 × 104 ρ aφ V/m c) D(ρ) = ǫ0E(ρ) = (2.00 × 104ǫ0/ρ) aφ C/m2. d) ρs on the upper surface of the lower plane: We use ρs = D · n surf ace = 2.00 × 104 ρ aφ · aφ = 2.00 × 104 ρ C/m2 e) Q on the upper surface of the lower plane: This will be Qt = .1 0 .120 .001 2.00 × 104ǫ0 ρ dρ dz = 2.00 × 104 ǫ0(.1) ln(120) = 8.47 × 10−8 C = 84.7 nC f) Repeat a) to c) for region 2 by letting the location of the upper plane be φ = .188 − 2π, and then find ρs and Q on the lower surface of the lower plane. Back to the beginning, we use 20 = C′ 1(.188 − 2π) + C′ 2 and 200 = C′ 1(.179) + C′ 2 105 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 108. 7.15f (continued) Subtracting one from the other, we find −180 = C′ 1(.009 − 2π) ⇒ C′ 1 = 28.7 Then 200 = 28.7(.179) + C′ 2 ⇒ C′ 2 = 194.9. Thus V (φ) = 28.7φ + 194.9 in region 2. Then E = − 28.7 ρ aφ V/m and D = − 28.7ǫ0 ρ aφ C/m2 ρs on the lower surface of the lower plane will now be ρs = − 28.7ǫ0 ρ aφ · (−aφ) = 28.7ǫ0 ρ C/m2 The charge on that surface will then be Qb = 28.7ǫ0(.1) ln(120) = 122 pC. g) Find the total charge on the lower plane and the capacitance between the planes: Total charge will be Qnet = Qt + Qb = 84.7 nC + 0.122 nC = 84.8 nC. The capacitance will be C = Qnet V = 84.8 200 − 20 = 0.471 nF = 471 pF 7.16. a) Solve Laplace’s equation for the potential field in the homogeneous region between two concentric conducting spheres with radii a and b, b > a, if V = 0 at r = b and V = V0 at r = a. With radial variation only, we have ∇2 V = 1 r2 d dr r2 dV dr = 0 Multiply by r2: d dr r2 dV dr = 0 or r2 dV dr = A Divide by r2: dV dr = A r2 ⇒ V = A r + B Note that in the last integration step, I dropped the minus sign that would have otherwise occurred in front of A, since we can choose A as we wish. Next, apply the boundary conditions: 0 = A b + B ⇒ B = − A b V0 = A a − A b ⇒ A = V0 1 a − 1 b Finally, V (r) = V0 r 1 a − 1 b − V0 b 1 a − 1 b = V0 1 r − 1 b 1 a − 1 b 106 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 109. 7.16b. Find the capacitance between them: Assume permittivity ǫ. First, the electric field will be E = −∇V = − dV dr ar = V0 r2 1 a − 1 b ar V/m Next, on the inner sphere, the charge density will be ρs = D r=a · ar = ǫV0 a2 1 a − 1 b C/m2 The capacitance is now C = Q V0 = 4πa2ρs V0 = 4πǫ 1 a − 1 b F 7.17. Concentric conducting spheres are located at r = 5 mm and r = 20 mm. The region between the spheres is filled with a perfect dielectric. If the inner sphere is at 100 V and the outer sphere at 0 V: a) Find the location of the 20 V equipotential surface: Solving Laplace’s equation gives us V (r) = V0 1 r − 1 b 1 a − 1 b where V0 = 100, a = 5 and b = 20. Setting V (r) = 20, and solving for r produces r = 12.5 mm. b) Find Er,max: Use E = −∇V = − dV dr ar = V0 ar r2 1 a − 1 b Then Er,max = E(r = a) = V0 a(1 − (a/b)) = 100 5(1 − (5/20)) = 26.7 V/mm = 26.7 kV/m c) Find ǫR if the surface charge density on the inner sphere is 100 µC/m2: ρs will be equal in magnitude to the electric flux density at r = a. So ρs = (2.67 × 104 V/m)ǫRǫ0 = 10−4 C/m2. Thus ǫR = 423 ! (obviously a bad choice of numbers here – possibly a misprint. A more reasonable charge on the inner sphere would have been 1 µC/m2, leading to ǫR = 4.23). 7.18. Concentric conducting spheres have radii of 1 and 5 cm. There is a perfect dielectric for which ǫR = 3 between them. The potential of the inner sphere is 2V and that of the outer is -2V. Find: a) V (r): We use the general expression derived in Problem 7.16: V (r) = (A/r) + B. At the inner sphere, 2 = (A/.01) + B, and at the outer sphere, −2 = (A/.05) + B. Subtracting the latter equation from the former gives 4 = A 1 .01 − 1 .05 = 80A so A = .05. Substitute A into either of the two potential equations at the boundaries to find B = −3. Finally, V (r) = (.05/r) − 3. 107 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 110. 7.18b. E(r) = −(dV /dr)ar = (.05/r2)ar V/m. c) V at r = 3 cm: V (.03) = (.05/.03) − 3 = −1.33 V. d) the location of the 0-V equipotential surface: Use 0 = (.05/r0) − 3 ⇒ r0 = (.05/3) = .0167 m = 1.67 cm e) the capacitance between the spheres: C = 4πǫ 1 a − 1 b = 4π(3)ǫ0 1 .01 − 1 .05 = 12πǫ0 80 = 4.2 pF 7.19. Two coaxial conducting cones have their vertices at the origin and the z axis as their axis. Cone A has the point A(1, 0, 2) on its surface, while cone B has the point B(0, 3, 2) on its surface. Let VA = 100 V and VB = 20 V. Find: a) α for each cone: Have αA = tan−1(1/2) = 26.57◦ and αB = tan−1(3/2) = 56.31◦. b) V at P (1, 1, 1): The potential function between cones can be written as V (θ) = C1 ln tan(θ/2) + C2 Then 20 = C1 ln tan(56.31/2) + C2 and 100 = C1 ln tan(26.57/2) + C2 Solving these two equations, we find C1 = −97.7 and C2 = −41.1. Now at P , θ = tan−1( √ 2) = 54.7◦. Thus VP = −97.7 ln tan(54.7/2) − 41.1 = 23.3 V 7.20. A potential field in free space is given as V = 100 ln tan(θ/2) + 50 V. a) Find the maximum value of |Eθ | on the surface θ = 40◦ for 0.1 < r < 0.8 m, 60◦ < φ < 90◦. First E = − 1 r dV dθ aθ = − 100 2r tan(θ/2) cos2(θ/2) aθ = − 100 2r sin(θ/2) cos(θ/2) aθ = − 100 r sin θ aθ This will maximize at the smallest value of r, or 0.1: Emax(θ = 40◦ ) = E(r = 0.1, θ = 40◦ ) = − 100 0.1 sin(40) aθ = 1.56 aθ kV/m b) Describe the surface V = 80 V: Set 100 ln tan θ/2+50 = 80 and solve for θ: Obtain ln tan θ/2 = 0.3 ⇒ tan θ/2 = e.3 = 1.35 ⇒ θ = 107◦ (the cone surface at θ = 107 degrees). 108 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 111. 7.21. In free space, let ρv = 200ǫ0/r2.4. a) Use Poisson’s equation to find V (r) if it is assumed that r2Er → 0 when r → 0, and also that V → 0 as r → ∞: With r variation only, we have ∇2 V = 1 r2 d dr r2 dV dr = − ρv ǫ = −200r−2.4 or d dr r2 dV dr = −200r−.4 Integrate once: r2 dV dr = − 200 .6 r.6 + C1 = −333.3r.6 + C1 or dV dr = −333.3r−1.4 + C1 r2 = ∇V (in this case) = −Er Our first boundary condition states that r2Er → 0 when r → 0 Therefore C1 = 0. Integrate again to find: V (r) = 333.3 .4 r−.4 + C2 From our second boundary condition, V → 0 as r → ∞, we see that C2 = 0. Finally, V (r) = 833.3r−.4 V b) Now find V (r) by using Gauss’ Law and a line integral: Gauss’ law applied to a spherical surface of radius r gives: 4πr2 Dr = 4π r 0 200ǫ0 (r′)2.4 (r′ )2 dr = 800πǫ0 r.6 .6 Thus Er = Dr ǫ0 = 800πǫ0r.6 .6(4π)ǫ0r2 = 333.3r−1.4 V/m Now V (r) = − r ∞ 333.3(r′ )−1.4 dr′ = 833.3r−.4 V 7.22. Let the volume charge density in Fig. 7.3a be given by ρv = ρv0(x/a)e−|x|/a (note error in the exponent in the formula stated in the book). a) Determine ρv,max and ρv,min and their locations: Let x′ = x/a. Then ρv = x′e−|x′|. Differentiate with respect to x′ to obtain: dρv dx′ = ρv0e−|x′| (1 − |x′ |) This derivative is zero at x′ = ±1, or the minimum and maximum occur at x = ±a respectively. The values of ρv at these points will be ρv,max = ρv0e−1 = 0.368ρv0, occurring at x = a. ρv,min = −ρv0e−1 = −0.368ρv0, occurring at x = −a. 109 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 112. 7.22b. Find Ex and V (x) if V (0) = 0 and Ex → 0 as x → ∞: We use Poisson’s equation: ∇2 V = − ρv ǫ ⇒ d2V dx2 = − ρv0 ǫ x a e−|x|/a For x > 0, this becomes d2V dx2 = − ρv0 ǫ x a e−x/a Integrate once over x: dV dx (x > 0) = − ρv0 ǫ x a e−x/a dx + C1 = aρv0 ǫ e−x/a x a + 1 + C1 Noting that Ex = −dV/dx, we use the first boundary condition, Ex → 0 as x → ∞, to establish that C1 = 0. Over the range x < 0, we have dV dx (x < 0) = − ρv0 ǫ x a ex/a dx + C′ 1 = aρv0 ǫ ex/a −x a + 1 + C′ 1 where C′ 1 = 0, since, by symmetry, Ex → 0 as x → −∞. These two equations can be unified to cover the entire range of x; the final expression for the electric field becomes: Ex = − dV dx = − aρv0 ǫ |x| a + 1 e−|x|/a V/m The potential function is now found by a second integration. For x > 0, this is V (x) = aρv0 ǫ x a e−x/a + e−x/a dx + C2 = a2ρv0 ǫ −x a e−x/a − 2e−x/a + C2 We use the second boundary condition, V (0) = 0, from which C2 = 2a2ρv0/ǫ. Substituting this yields V (x) (x > 0) = a2ρv0 ǫ −x a e−x/a + 2(1 − e−x/a ) We repeat the procedure for x < 0 to obtain V (x) = aρv0 ǫ x a ex/a + ex/a dx + C′ 2 = a2ρv0 ǫ −x a ex/a − 2ex/a + C′ 2 Again, with the V (0) = 0 boundary condition, we find C′ 2 = −2a2ρv0/ǫ, which when substituted leads to V (x) (x < 0) = a2ρv0 ǫ −x a ex/a − 2(1 − ex/a ) Combining the results for both ranges of x, we write V (x) = −a2ρv0 ǫ x a e−|x|/a − 2x |x| 1 − e−|x|/a 110 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 113. 7.22c. Use a development similar to that of Sec. 7.4 to show that C = dQ/dV0 = ǫS/8a ( note error in problem statement): First, the overall potential difference is V0 = Vx→∞ − Vx→−∞ = 2 × 2a2ρv0 ǫ = 4a2ρv0 ǫ From this we find a = √ (ǫV0)/(4ρv0). Then the total charge on one side will be Q = S ∞ 0 ρv0 x a e−x/a dx = Sρv0 ae−x/a −x a − 1 ∞ 0 = Sρv0 a = 1 2 S ǫV0ρv0 Now C = dQ dV0 = d dV0 1 2 S ǫV0ρv0 = S 4 ρv0 ǫ V0 But a = √ (ǫV0)/(4ρv0), from which (ρv0/V0) = ǫ/(4a2). Substituting this into the capacitance expression gives C = S 4 ǫ2 4a2 = ǫS 8a 7.23. A rectangular trough is formed by four conducting planes located at x = 0 and 8 cm and y = 0 and 5 cm in air. The surface at y = 5 cm is at a potential of 100 V, the other three are at zero potential, and the necessary gaps are placed at two corners. Find the potential at x = 3 cm, y = 4 cm: This situation is the same as that of Fig. 7.6, except the non-zero boundary potential appears on the top surface, rather than the right side. The solution is found from Eq. (39) by simply interchanging x and y, and b and d, obtaining: V (x, y) = 4V0 π ∞ 1,odd 1 m sinh(mπy/d) sinh(mπb/d) sin mπx d where V0 = 100 V, d = 8 cm, and b = 5 cm. We will use the first three terms to evaluate the potential at (3,4): V (3, 4) . = 400 π sinh(π/2) sinh(5π/8) sin(3π/8) + 1 3 sinh(3π/2) sinh(15π/8) sin(9π/8) + 1 5 sinh(5π/2) sinh(25π/8) sin(15π/8) = 400 π [.609 − .040 − .011] = 71.1 V Additional accuracy is found by including more terms in the expansion. Using thirteen terms, and using six significant figure accuracy, the result becomes V (3, 4) . = 71.9173 V. The series converges rapidly enough so that terms after the sixth one produce no change in the third digit. Thus, quoting three significant figures, 71.9 V requires six terms, with subsequent terms having no effect. 111 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 114. 7.24. The four sides of a square trough are held at potentials of 0, 20, -30, and 60 V; the highest and lowest potentials are on opposite sides. Find the potential at the center of the trough: Here we can make good use of symmetry. The solution for a single potential on the right side, for example, with all other sides at 0V is given by Eq. (39): V (x, y) = 4V0 π ∞ 1,odd 1 m sinh(mπx/b) sinh(mπd/b) sin mπy b In the current problem, we can account for the three voltages by superposing three solutions of the above form, suitably modified to account for the different locations of the boundary potentials. Since we want V at the center of a square trough, it no longer matters on what boundary each of the given potentials is, and we can simply write: V (center) = 4(0 + 20 − 30 + 60) π ∞ 1,odd 1 m sinh(mπ/2) sinh(mπ) sin(mπ/2) = 12.5 V The series converges to this value in three terms. 7.25. In Fig. 7.7, change the right side so that the potential varies linearly from 0 at the bottom of that side to 100 V at the top. Solve for the potential at the center of the trough: Since the potential reaches zero periodically in y and also is zero at x = 0, we use the form: V (x, y) = ∞ m=1 Vm sinh mπx b sin mπy b Now, at x = d, V = 100(y/b). Thus 100 y b = ∞ m=1 Vm sinh mπd b sin mπy b We then multiply by sin(nπy/b), where n is a fixed integer, and integrate over y from 0 to b: b 0 100 y b sin nπy b dy = ∞ m=1 Vm sinh mπd b b 0 sin mπy b sin nπy b dy =b/2 if m=n, zero if m=n The integral on the right hand side picks the nth term out of the series, enabling the coefficients, Vn, to be solved for individually as we vary n. We find in general, Vm = 2 b sinh(mπ/d) b 0 100 y b sin nπy b dy The integral evaluates as b 0 100 y b sin nπy b dy = −100/mπ (m even) 100/mπ (m odd) = (−1)m+1 100 mπ 112 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 115. 7.25 (continued) Thus Vm = 200(−1)m+1 mπb sinh(mπd/b) So that finally, V (x, y) = 200 πb ∞ m=1 (−1)m+1 m sinh (mπx/b) sinh (mπd/b) sin mπy b Now, with a square trough, set b = d = 1, and so 0 < x < 1 and 0 < y < 1. The potential becomes V (x, y) = 200 π ∞ m=1 (−1)m+1 m sinh (mπx) sinh (mπ) sin (mπy) Now at the center of the trough, x = y = 0.5, and, using four terms, we have V (.5, .5) . = 200 π sinh(π/2) sinh(π) − 1 3 sinh(3π/2) sinh(3π) + 1 5 sinh(5π/2) sinh(5π) − 1 7 sinh(7π/2) sinh(7π) = 12.5 V where additional terms do not affect the three-significant-figure answer. 7.26. If X is a function of x and X′′ +(x −1)X −2X = 0, assume a solution in the form of an infinite power series and determine numerical values for a2 to a8 if a0 = 1 and a1 = −1: The series solution will be of the form: X = ∞ m=0 amxm The first 8 terms of this are substituted into the given equation to give: (2a2 − a1 − 2a0) + (6a3 + a1 − 2a2 − 2a1)x + (12a4 + 2a2 − 3a3 − 2a2)x2 + (3a3 − 4a4 − 2a3 + 20a5)x3 + (30a6 + 4a4 − 5a5 − 2a4)x4 + (42a7 + 5a5 − 6a6 − 2a5)x5 + (56a8 + 6a6 − 7a7 − 2a6)x6 + (7a7 − 8a8 − 2a7)x7 + (8a8 − 2a8)x8 = 0 For this equation to be zero, each coefficient term (in parenthesis) must be zero. The first of these is 2a2 − a1 − 2a0 = 2a2 + 1 − 2 = 0 ⇒ a2 = 1/2 The second coefficient is 6a3 + a1 − 2a2 − 2a1 = 6a3 − 1 − 1 + 2 = 0 ⇒ a3 = 0 Third coefficient: 12a4 + 2a2 − 3a3 − 2a2 = 12a4 + 1 − 0 − 1 = 0 ⇒ a4 = 0 Fourth coefficient: 3a3 − 4a4 − 2a3 + 20a5 = 0 − 0 − 0 + 20a5 = 0 ⇒ a5 = 0 In a similar manner, we find a6 = a7 = a8 = 0. 113 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 116. 7.27. It is known that V = XY is a solution of Laplace’s equation, where X is a function of x alone, and Y is a function of y alone. Determine which of the following potential function are also solutions of Laplace’s equation: a) V = 100X: We know that ∇2XY = 0, or ∂2 ∂x2 XY + ∂2 ∂y2 XY = 0 ⇒ YX′′ + XY′′ = 0 ⇒ X′′ X = − Y′′ Y = α2 Therefore, ∇2X = 100X′′ = 0 – No. b) V = 50XY: Would have ∇2V = 50∇2XY = 0 – Yes. c) V = 2XY + x − 3y: ∇2V = 2∇2XY + 0 − 0 = 0 – Yes. d) V = xXY: ∇2V = x∇2XY + XY∇2x = 0 – Yes. e) V = X2Y: ∇2V = X∇2XY + XY∇2X = 0 + XY∇2X – No. 7.28. Assume a product solution of Laplace’s equation in cylindrical coordinates, V = P F, where V is not a function of z, P is a function only of ρ, and F is a function only of φ. a) Obtain the two separated equations if the separation constant is n2. Select the sign of n2 so that the solution of the φ equation leads to trigonometric functions: Begin with Laplace’s equation in cylindrical coordinates, in which there is no z variation: ∇2 V = 1 ρ ∂ ∂ρ ρ ∂V ∂ρ + 1 ρ2 ∂2V ∂φ2 = 0 We substitute the product solution V = P F to obtain: F ρ d dρ ρ dP dρ + P ρ2 d2F dφ2 = F ρ dP dρ + F d2P dρ2 + P ρ2 d2F dφ2 = 0 Next, multiply by ρ2 and divide by FP to obtain ρ P dP dρ + ρ2 P d2P dρ2 n2 + 1 F d2F dφ2 −n2 = 0 The equation is now grouped into two parts as shown, each a function of only one of the two variables; each is set equal to plus or minus n2, as indicated. The φ equation now becomes d2F dφ2 + n2 F = 0 ⇒ F = Cn cos(nφ) + Dn sin(nφ) (n ≥ 1) Note that n is required to be an integer, since physically, the solution must repeat itself every 2π radians in φ. If n = 0, then d2F dφ2 = 0 ⇒ F = C0φ + D0 114 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 117. 7.28b. Show that P = Aρn + Bρ−n satisfies the ρ equation: From part a, the radial equation is: ρ2 d2P dρ2 + ρ dP dρ − n2 P = 0 Substituting Aρn, we find ρ2 n(n − 1)ρn−2 + ρnρn−1 − n2 ρn = n2 ρn − nρn + nρn − n2 ρn = 0 Substituting Bρ−n: ρ2 n(n + 1)ρ−(n+2) − ρnρ−(n+1) − n2 ρ−n = n2 ρ−n + nρ−n − nρ−n − n2 ρ−n = 0 So it works. c) Construct the solution V (ρ, φ). Functions of this form are called circular harmonics. To assemble the complete solution, we need the radial solution for the case in which n = 0. The equation to solve is ρ d2P dρ2 + dP dρ = 0 Let S = dP/dρ, and so dS/dρ = d2P/dρ2. The equation becomes ρ dS dρ + S = 0 ⇒ − dρ ρ = dS S Integrating, find − ln ρ + ln A0 = ln S ⇒ ln S = ln A0 ρ ⇒ S = A0 ρ = dP dρ where A0 is a constant. So now dρ ρ = dP A0 ⇒ Pn=0 = A0 ln ρ + B0 We may now construct the solution in its complete form, encompassing n ≥ 0: V (ρ, φ) = (A0 ln ρ + B0)(C0φ + D0) n=0 solution + ∞ n=1 [Anρn + Bnρ−n ][Cn cos(nφ) + Dn sin(nφ)] 115 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 118. CHAPTER 8 8.1a. Find H in cartesian components at P (2, 3, 4) if there is a current filament on the z axis carrying 8 mA in the az direction: Applying the Biot-Savart Law, we obtain Ha = ∞ −∞ IdL × aR 4πR2 = ∞ −∞ Idz az × [2ax + 3ay + (4 − z)az] 4π(z2 − 8z + 29)3/2 = ∞ −∞ Idz[2ay − 3ax] 4π(z2 − 8z + 29)3/2 Using integral tables, this evaluates as Ha = I 4π 2(2z − 8)(2ay − 3ax) 52(z2 − 8z + 29)1/2 ∞ −∞ = I 26π (2ay − 3ax) Then with I = 8 mA, we finally obtain Ha = −294ax + 196ay µA/m b. Repeat if the filament is located at x = −1, y = 2: In this case the Biot-Savart integral becomes Hb = ∞ −∞ Idz az × [(2 + 1)ax + (3 − 2)ay + (4 − z)az] 4π(z2 − 8z + 26)3/2 = ∞ −∞ Idz[3ay − ax] 4π(z2 − 8z + 26)3/2 Evaluating as before, we obtain with I = 8 mA: Hb = I 4π 2(2z − 8)(3ay − ax) 40(z2 − 8z + 26)1/2 ∞ −∞ = I 20π (3ay − ax) = −127ax + 382ay µA/m c. Find H if both filaments are present: This will be just the sum of the results of parts a and b, or HT = Ha + Hb = −421ax + 578ay µA/m This problem can also be done (somewhat more simply) by using the known result for H from an infinitely-long wire in cylindrical components, and transforming to cartesian components. The Biot- Savart method was used here for the sake of illustration. 8.2. A current filament of 3ax A lies along the x axis. Find H in cartesian components at P (−1, 3, 2): We use the Biot-Savart law, H = IdL × aR 4πR2 where IdL = 3dxax, aR = [−(1 + x)ax + 3ay + 2az]/R, and R = √ x2 + 2x + 14. Thus HP = ∞ −∞ 3dxax × [−(1 + x)ax + 3ay + 2az] 4π(x2 + 2x + 14)3/2 = ∞ −∞ (9az − 6ay) dx 4π(x2 + 2x + 14)3/2 = (9az − 6ay)(x + 1) 4π(13) √ x2 + 2x + 14 ∞ −∞ = 2(9az − 6ay) 4π(13) = 0.110az − 0.073ay A/m 116 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 119. 8.3. Two semi-infinite filaments on the z axis lie in the regions −∞ < z < −a (note typographical error in problem statement) and a < z < ∞. Each carries a current I in the az direction. a) Calculate H as a function of ρ and φ at z = 0: One way to do this is to use the field from an infinite line and subtract from it that portion of the field that would arise from the current segment at −a < z < a, found from the Biot-Savart law. Thus, H = I 2πρ aφ − a −a I dz az × [ρ aρ − z az] 4π[ρ2 + z2]3/2 The integral part simplifies and is evaluated: a −a I dz ρ aφ 4π[ρ2 + z2]3/2 = Iρ 4π aφ z ρ2 ρ2 + z2 a −a = Ia 2πρ ρ2 + a2 aφ Finally, H = I 2πρ 1 − a ρ2 + a2 aφ A/m b) What value of a will cause the magnitude of H at ρ = 1, z = 0, to be one-half the value obtained for an infinite filament? We require 1 − a ρ2 + a2 ρ=1 = 1 2 ⇒ a √ 1 + a2 = 1 2 ⇒ a = 1/ √ 3 8.4a.) A filament is formed into a circle of radius a, centered at the origin in the plane z = 0. It carries a current I in the aφ direction. Find H at the origin: We use the Biot-Savart law, which in this case becomes: H = loop IdL × aR 4πR2 = 2π 0 Ia dφ aφ × (−aρ) 4πa2 = 0.50 I a az A/m b.) A filament of the same length is shaped into a square in the z = 0 plane. The sides are parallel to the coordinate axes and a current I flows in the general aφ direction. Again, find H at the origin: Since the loop is the same length, its perimeter is 2πa, and so each of the four sides is of length πa/2. Using symmetry, we can find the magnetic field at the origin associated with each of the 8 half-sides (extending from 0 to ±πa/4 along each coordinate direction) and multiply the result by 8: Taking one of the segments in the y direction, the Biot-Savart law becomes H = loop IdL × aR 4πR2 = 8 πa/4 0 Idy ay × −(πa/4) ax − y ay 4π y2 + (πa/4)2 3/2 = aI 2 πa/4 0 dy az y2 + (πa/4)2 3/2 = aI 2 y az (πa/4)2 y2 + (πa/4)2 πa/4 0 = 0.57 I a az A/m 117 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 120. 8.5. The parallel filamentary conductors shown in Fig. 8.21 lie in free space. Plot |H| versus y, −4 < y < 4, along the line x = 0, z = 2: We need an expression for H in cartesian coordinates. We can start with the known H in cylindrical for an infinite filament along the z axis: H = I/(2πρ) aφ, which we transform to cartesian to obtain: H = −Iy 2π(x2 + y2) ax + Ix 2π(x2 + y2) ay If we now rotate the filament so that it lies along the x axis, with current flowing in positive x, we obtain the field from the above expression by replacing x with y and y with z: H = −Iz 2π(y2 + z2) ay + Iy 2π(y2 + z2) az Now, with two filaments, displaced from the x axis to lie at y = ±1, and with the current directions as shown in the figure, we use the previous expression to write H = Iz 2π[(y + 1)2 + z2] − Iz 2π[(y − 1)2 + z2] ay + I(y − 1) 2π[(y − 1)2 + z2] − I(y + 1) 2π[(y + 1)2 + z2] az We now evaluate this at z = 2, and find the magnitude ( √ H · H), resulting in |H| = I 2π 2 y2 + 2y + 5 − 2 y2 − 2y + 5 2 + (y − 1) y2 − 2y + 5 − (y + 1) y2 + 2y + 5 2 1/2 This function is plotted below 8.6a. A current filament I is formed into circle, ρ = a, in the z = z′ plane. Find Hz at P (0, 0, z) if I flows in the aφ direction: Use the Biot-Savart law, H = IdL × aR 4πR2 where in this case IdL = Idφaφ, aR = [−aaρ + (z − z′)az]/R, and R = a2 + (z − z′)2. The setup becomes H = 2π 0 Iadφ aφ × [−aaρ + (z − z′)az] 4π[a2 + (z − z′)2]3/2 = 2π 0 Ia[aaz + (z − z′)aρ] dφ 4π[a2 + (z − z′)2]3/2 118 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 121. At this point we need to be especially careful. Note that we are integrating a vector with an aρ component around a complete circle, where the vector has no φ dependence. This sum of all aρ components will be zero – even though this doesn’t happen when we go ahead with the integration without this knowledge. The problem is that the integral “interprets” aρ as a constant direction, when in fact – as we know – aρ continually changes direction as φ varies. We drop the aρ component in the integral to give H = 2π 0 Ia2az dφ 4π[a2 + (z − z′)2]3/2 = πa2Iaz 2π[a2 + (z − z′)2]3/2 = m 2π[a2 + (z − z′)2]3/2 A/m where m = πa2Iaz is the magnetic moment of the loop. b) Find Hz at P caused by a uniform surface current density K = K0aφ, flowing on the cylindrical surface, ρ = a, 0 < z < h. The results of part a should help: Using part a, we can write down the differential field at P arising from a circular current ribbon of differential height, dz′, at location z′. The ribbon is of radius a and carries current K0dz′aφ A: dH = πa2K0dz′az 2π[a2 + (z − z′)2]3/2 A/m The total magnetic field at P is now the sum of the contributions of all differential rings that comprise the cylinder: Hz = h 0 πa2K0dz′ 2π[a2 + (z − z′)2]3/2 = a2K0 2 h 0 dz′ [a2 + z2 − 2zz′ + (z′)2]3/2 = a2K0 2 2(2z′ − 2z) 4a2 a2 + z2 − 2zz′ + (z′)2 h 0 = K0(z′ − z) 2 a2 + (z′ − z)2 h 0 = K0 2 (h − z) a2 + (h − z)2 + z √ a2 + z2 A/m 8.7. Given points C(5, −2, 3) and P (4, −1, 2); a current element IdL = 10−4(4, −3, 1) A · m at C pro- duces a field dH at P . a) Specify the direction of dH by a unit vector aH : Using the Biot-Savart law, we find dH = IdL × aCP 4πR2 CP = 10−4[4ax − 3ay + az] × [−ax + ay − az] 4π33/2 = [2ax + 3ay + az] × 10−4 65.3 from which aH = 2ax + 3ay + az √ 14 = 0.53ax + 0.80ay + 0.27az b) Find |dH|. |dH| = √ 14 × 10−4 65.3 = 5.73 × 10−6 A/m = 5.73 µA/m c) What direction al should IdL have at C so that dH = 0? IdL should be collinear with aCP , thus rendering the cross product in the Biot-Savart law equal to zero. Thus the answer is al = ±(−ax + ay − az)/ √ 3 119 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 122. 8.8. For the finite-length current element on the z axis, as shown in Fig. 8.5, use the Biot-Savart law to derive Eq. (9) of Sec. 8.1: The Biot-Savart law reads: H = z2 z1 IdL × aR 4πR2 = ρ tan α2 ρ tan α1 Idzaz × (ρaρ − zaz) 4π(ρ2 + z2)3/2 = ρ tan α2 ρ tan α1 Iρaφ dz 4π(ρ2 + z2)3/2 The integral is evaluated (using tables) and gives the desired result: H = Izaφ 4πρ ρ2 + z2 ρ tan α2 ρ tan α1 = I 4πρ tan α2 1 + tan2 α2 − tan α1 1 + tan2 α1 aφ = I 4πρ (sin α2 − sin α1)aφ 8.9. A current sheet K = 8ax A/m flows in the region −2 < y < 2 in the plane z = 0. Calculate H at P (0, 0, 3): Using the Biot-Savart law, we write HP = K × aR dx dy 4πR2 = 2 −2 ∞ −∞ 8ax × (−xax − yay + 3az) 4π(x2 + y2 + 9)3/2 dx dy Taking the cross product gives: HP = 2 −2 ∞ −∞ 8(−yaz − 3ay) dx dy 4π(x2 + y2 + 9)3/2 We note that the z component is anti-symmetric in y about the origin (odd parity). Since the limits are symmetric, the integral of the z component over y is zero. We are left with HP = 2 −2 ∞ −∞ −24 ay dx dy 4π(x2 + y2 + 9)3/2 = − 6 π ay 2 −2 x (y2 + 9) x2 + y2 + 9 ∞ −∞ dy = − 6 π ay 2 −2 2 y2 + 9 dy = − 12 π ay 1 3 tan−1 y 3 2 −2 = − 4 π (2)(0.59) ay = −1.50 ay A/m 8.10. Let a filamentary current of 5 mA be directed from infinity to the origin on the positive z axis and then back out to infinity on the positive x axis. Find H at P (0, 1, 0): The Biot-Savart law is applied to the two wire segments using the following setup: HP = IdL × aR 4πR2 = ∞ 0 −Idzaz × (−zaz + ay) 4π(z2 + 1)3/2 + ∞ 0 Idxax × (−xax + ay) 4π(x2 + 1)3/2 = ∞ 0 Idzax 4π(z2 + 1)3/2 + ∞ 0 Idxaz 4π(x2 + 1)3/2 = I 4π zax √ z2 + 1 ∞ 0 + xaz √ x2 + 1 ∞ 0 = I 4π (ax + az) = 0.40(ax + az) mA/m 120 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 123. 8.11. An infinite filament on the z axis carries 20π mA in the az direction. Three uniform cylindrical current sheets are also present: 400 mA/m at ρ = 1 cm, −250 mA/m at ρ = 2 cm, and −300 mA/m at ρ = 3 cm. Calculate Hφ at ρ = 0.5, 1.5, 2.5, and 3.5 cm: We find Hφ at each of the required radii by applying Ampere’s circuital law to circular paths of those radii; the paths are centered on the z axis. So, at ρ1 = 0.5 cm: H · dL = 2πρ1Hφ1 = Iencl = 20π × 10−3 A Thus Hφ1 = 10 × 10−3 ρ1 = 10 × 10−3 0.5 × 10−2 = 2.0 A/m At ρ = ρ2 = 1.5 cm, we enclose the first of the current cylinders at ρ = 1 cm. Ampere’s law becomes: 2πρ2Hφ2 = 20π + 2π(10−2 )(400) mA ⇒ Hφ2 = 10 + 4.00 1.5 × 10−2 = 933 mA/m Following this method, at 2.5 cm: Hφ3 = 10 + 4.00 − (2 × 10−2)(250) 2.5 × 10−2 = 360 mA/m and at 3.5 cm, Hφ4 = 10 + 4.00 − 5.00 − (3 × 10−2)(300) 3.5 × 10−2 = 0 8.12. In Fig. 8.22, let the regions 0 < z < 0.3 m and 0.7 < z < 1.0 m be conducting slabs carrying uniform current densities of 10 A/m2 in opposite directions as shown. The problem asks you to find H at various positions. Before continuing, we need to know how to find H for this type of current configuration. The sketch below shows one of the slabs (of thickness D) oriented with the current coming out of the page. The problem statement implies that both slabs are of infinite length and width. To find the magnetic field inside a slab, we apply Ampere’s circuital law to the rectangular path of height d and width w, as shown, since by symmetry, H should be oriented horizontally. For example, if the sketch below shows the upper slab in Fig. 8.22, current will be in the positive y direction. Thus H will be in the positive x direction above the slab midpoint, and will be in the negative x direction below the midpoint. d w D Hout Hout 121 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 124. 8.12 (continued) In taking the line integral in Ampere’s law, the two vertical path segments will cancel each other. Ampere’s circuital law for the interior loop becomes H · dL = 2Hin × w = Iencl = J × w × d ⇒ Hin = Jd 2 The field outside the slab is found similarly, but with the enclosed current now bounded by the slab thickness, rather than the integration path height: 2Hout × w = J × w × D ⇒ Hout = JD 2 where Hout is directed from right to left below the slab and from left to right above the slab (right hand rule). Reverse the current, and the fields, of course, reverse direction. We are now in a position to solve the problem. Find H at: a) z = −0.2m: Here the fields from the top and bottom slabs (carrying opposite currents) will cancel, and so H = 0. b) z = 0.2m. This point lies within the lower slab above its midpoint. Thus the field will be oriented in the negative x direction. Referring to Fig. 8.22 and to the sketch on the previous page, we find that d = 0.1. The total field will be this field plus the contribution from the upper slab current: H = −10(0.1) 2 ax lower slab − 10(0.3) 2 ax upper slab = −2ax A/m c) z = 0.4m: Here the fields from both slabs will add constructively in the negative x direction: H = −2 10(0.3) 2 ax = −3ax A/m d) z = 0.75m: This is in the interior of the upper slab, whose midpoint lies at z = 0.85. Therefore d = 0.2. Since 0.75 lies below the midpoint, magnetic field from the upper slab will lie in the negative x direction. The field from the lower slab will be negative x-directed as well, leading to: H = −10(0.2) 2 ax upper slab − 10(0.3) 2 ax lower slab = −2.5ax A/m e) z = 1.2m: This point lies above both slabs, where again fields cancel completely: Thus H = 0. 122 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 125. 8.13. A hollow cylindrical shell of radius a is centered on the z axis and carries a uniform surface current density of Kaaφ. a) Show that H is not a function of φ or z: Consider this situation as illustrated in Fig. 8.11. There (sec. 8.2) it was stated that the field will be entirely z-directed. We can see this by applying Ampere’s circuital law to a closed loop path whose orientation we choose such that current is enclosed by the path. The only way to enclose current is to set up the loop (which we choose to be rectangular) such that it is oriented with two parallel opposing segments lying in the z direction; one of these lies inside the cylinder, the other outside. The other two parallel segments lie in the ρ direction. The loop is now cut by the current sheet, and if we assume a length of the loop in z of d, then the enclosed current will be given by Kd A. There will be no φ variation in the field because where we position the loop around the circumference of the cylinder does not affect the result of Ampere’s law. If we assume an infinite cylinder length, there will be no z dependence in the field, since as we lengthen the loop in the z direction, the path length (over which the integral is taken) increases, but then so does the enclosed current – by the same factor. Thus H would not change with z. There would also be no change if the loop was simply moved along the z direction. b) Show that Hφ and Hρ are everywhere zero. First, if Hφ were to exist, then we should be able to find a closed loop path that encloses current, in which all or or portion of the path lies in the φ direction. This we cannot do, and so Hφ must be zero. Another argument is that when applying the Biot-Savart law, there is no current element that would produce a φ component. Again, using the Biot-Savart law, we note that radial field components will be produced by individual current elements, but such components will cancel from two elements that lie at symmetric distances in z on either side of the observation point. c) Show that Hz = 0 for ρ > a: Suppose the rectangular loop was drawn such that the outside z-directed segment is moved further and further away from the cylinder. We would expect Hz outside to decrease (as the Biot-Savart law would imply) but the same amount of current is always enclosed no matter how far away the outer segment is. We therefore must conclude that the field outside is zero. d) Show that Hz = Ka for ρ < a: With our rectangular path set up as in part a, we have no path integral contributions from the two radial segments, and no contribution from the outside z-directed segment. Therefore, Ampere’s circuital law would state that H · dL = Hzd = Iencl = Kad ⇒ Hz = Ka where d is the length of the loop in the z direction. e) A second shell, ρ = b, carries a current Kbaφ. Find H everywhere: For ρ < a we would have both cylinders contributing, or Hz(ρ < a) = Ka + Kb. Between the cylinders, we are outside the inner one, so its field will not contribute. Thus Hz(a < ρ < b) = Kb. Outside (ρ > b) the field will be zero. 123 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 126. 8.14. A toroid having a cross section of rectangular shape is defined by the following surfaces: the cylinders ρ = 2 and ρ = 3 cm, and the planes z = 1 and z = 2.5 cm. The toroid carries a surface current density of −50az A/m on the surface ρ = 3 cm. Find H at the point P (ρ, φ, z): The construction is similar to that of the toroid of round cross section as done on p.239. Again, magnetic field exists only inside the toroid cross section, and is given by H = Iencl 2πρ aφ (2 < ρ < 3) cm, (1 < z < 2.5) cm where Iencl is found from the given current density: On the outer radius, the current is Iouter = −50(2π × 3 × 10−2 ) = −3π A This current is directed along negative z, which means that the current on the inner radius (ρ = 2) is directed along positive z. Inner and outer currents have the same magnitude. It is the inner current that is enclosed by the circular integration path in aφ within the toroid that is used in Ampere’s law. So Iencl = +3π A. We can now proceed with what is requested: a) PA(1.5cm, 0, 2cm): The radius, ρ = 1.5 cm, lies outside the cross section, and so HA = 0. b) PB(2.1cm, 0, 2cm): This point does lie inside the cross section, and the φ and z values do not matter. We find HB = Iencl 2πρ aφ = 3aφ 2(2.1 × 10−2) = 71.4 aφ A/m c) PC(2.7cm, π/2, 2cm): again, φ and z values make no difference, so HC = 3aφ 2(2.7 × 10−2) = 55.6 aφ A/m d) PD(3.5cm, π/2, 2cm). This point lies outside the cross section, and so HD = 0. 8.15. Assume that there is a region with cylindrical symmetry in which the conductivity is given by σ = 1.5e−150ρ kS/m. An electric field of 30 az V/m is present. a) Find J: Use J = σE = 45e−150ρ az kA/m2 b) Find the total current crossing the surface ρ < ρ0, z = 0, all φ: I = J · dS = 2π 0 ρ0 0 45e−150ρ ρ dρ dφ = 2π(45) (150)2 e−150ρ [−150ρ − 1] ρ0 0 kA = 12.6 1 − (1 + 150ρ0)e−150ρ0 A c) Make use of Ampere’s circuital law to find H: Symmetry suggests that H will be φ-directed only, and so we consider a circular path of integration, centered on and perpendicular to the z axis. Ampere’s law becomes: 2πρHφ = Iencl, where Iencl is the current found in part b, except with ρ0 replaced by the variable, ρ. We obtain Hφ = 2.00 ρ 1 − (1 + 150ρ)e−150ρ A/m 124 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 127. 8.16. The cylindrical shell, 2mm < ρ < 3mm, carries a uniformly-distributed total current of 8A in the −az direction, and a filament on the z axis carries 8A in the az direction. Find H everywhere: We use Ampere’s circuital law, noting that from symmetry, H will be aφ directed. Inside the shell (ρ < 2mm), A circular integration path centered on the z axis encloses only the filament current along z: Therefore H(ρ < 2mm) = 8 2πρ aφ = 4 πρ aφ A/m (ρ in m) With the circular integration path within (2 < ρ < 3mm), the enclosed current will consist of the filament plus that portion of the shell current that lies inside ρ. Ampere’s circuital law applied to a loop of radius ρ is: H · dL = If ilament + shell area J · dS where the current density is J = − 8 π(3 × 10−3)2 − π(2 × 10−3)2 az = − 8 × 106 5π az A/m2 So 2πρHφ = 8 + 2π 0 ρ 2×10−3 −8 5π × 106 az · az ρ′ dρ′ dφ = 8 − 1.6 × 106 (ρ′ )2 ρ 2×10−3 Solve for Hφ to find: H(2 < ρ < 3 mm) = 4 πρ 1 − (2 × 105 )(ρ2 − 4 × 10−6 ) aφ A/m (ρ in m) Outside (ρ > 3mm), the total enclosed current is zero, and so H(ρ > 3mm) = 0. 125 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 128. 8.17. A current filament on the z axis carries a current of 7 mA in the az direction, and current sheets of 0.5 az A/m and −0.2 az A/m are located at ρ = 1 cm and ρ = 0.5 cm, respectively. Calculate H at: a) ρ = 0.5 cm: Here, we are either just inside or just outside the first current sheet, so both we will calculate H for both cases. Just inside, applying Ampere’s circuital law to a circular path centered on the z axis produces: 2πρHφ = 7 × 10−3 ⇒ H(just inside) = 7 × 10−3 2π(0.5 × 10−2 aφ = 2.2 × 10−1 aφ A/m Just outside the current sheet at .5 cm, Ampere’s law becomes 2πρHφ = 7 × 10−3 − 2π(0.5 × 10−2 )(0.2) ⇒ H(just outside) = 7.2 × 10−4 2π(0.5 × 10−2) aφ = 2.3 × 10−2 aφ A/m b) ρ = 1.5 cm: Here, all three currents are enclosed, so Ampere’s law becomes 2π(1.5 × 10−2 )Hφ = 7 × 10−3 − 6.28 × 10−3 + 2π(10−2 )(0.5) ⇒ H(ρ = 1.5) = 3.4 × 10−1 aφ A/m c) ρ = 4 cm: Ampere’s law as used in part b applies here, except we replace ρ = 1.5 cm with ρ = 4 cm on the left hand side. The result is H(ρ = 4) = 1.3 × 10−1aφ A/m. d) What current sheet should be located at ρ = 4 cm so that H = 0 for all ρ > 4 cm? We require that the total enclosed current be zero, and so the net current in the proposed cylinder at 4 cm must be negative the right hand side of the first equation in part b. This will be −3.2 × 10−2, so that the surface current density at 4 cm must be K = −3.2 × 10−2 2π(4 × 10−2) az = −1.3 × 10−1 az A/m 8.18. Current density is distributed as follows: J = 0 for |y| > 2 m, J = 8yaz A/m2 for |y| < 1 m, J = 8(2 −y) az A/m2 for 1 < y < 2 m, J = −8(2 +y) az A/m2 for −2 < y < −1 m. Use symmetry and Ampere’s law to find H everywhere. Symmetry does help significantly in this problem. The current densities in the regions 0 < y < 1 and −1 < y < 0 are mirror images of each other across the plane y = 0 – this in addition to being of opposite sign. This is also true of the current densities in the regions 1 < y < 2 and −2 < y < −1. As a consequence of this, we find that the net current in region 1, I1 (see the diagram on the next page), is equal and opposite to the net current in region 4, I4. Also, I2 is equal and opposite to I3. This means that when applying Ampere’s law to the path a − b − c − d − a, as shown in the figure, zero current is enclosed, so that H · dL = 0 over the path. In addition, the symmetry of the current configuration implies that H = 0 outside the slabs along the vertical paths a −b and c −d. H from all sources should completely cancel along the two vertical paths, as well as along the two horizontal paths. 126 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 129. 8.18. (continued) To find the magnetic field in region 1, we apply Ampere’s circuital law to the path c − d − e − f − c, again noting that H will be zero along the two horizontal segments and along the right vertical segment. This leaves only the left vertical segment, e − f , pointing in the +x direction, and along which is field, Hx1. The counter-clockwise direction of the path integral is chosen using the right-hand convention, where we take the normal to the path in the +z direction, which is the same as the current direction. Assuming the height of the path is x, we find Hx1 x = x 2 y1 8(2 − y)dy = x 16y − 4y2 2 y1 = x 16(2 − y1) − 4(4 − y2 1) Replacing y1 with y, we find Hx1 = 4[8 − 4y − 4 + y2 ] ⇒ H1(1 < y < 2) = 4(y − 2)2 ax A/m H1 lies in the positive x direction, since the result of the integration is net positive. H in region 2 is now found through the line integral over the path d − g − h − c, enclosing all of region 1 within x and part of region 2 from y = y2 to 1: Hx2 x = x 2 1 8(2 − y) dy + x 1 y2 8y dy = x 4(1 − 2)2 + 4(1 − y2 2) = 4(2 − y2 2) x so that in terms of y, H2(0 < y < 1) = 4(2 − y2 )ax A/m y x 1 20-1-2 a b c d e f g h x x . . I1I2I3I4 4 3 2 1 y2 y1 127 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 130. 8.18. (continued) The procedure is repeated for the remaining two regions, −2 < y < −1 and −1 < y < 0, by taking the integration path with its right vertical segment within each of these two regions, while the left vertical path is a − b. Again the integral is taken counter-clockwise, which means that the right vertical path will be directed along −x. But the current is now in the opposite direction of that for y > 0, making the enclosed current net negative. Therefore, H will be in the opposite direction from that of the right vertical path, which is the positive x direction. The magnetic field will therefore be symmetric about the y = 0 plane. We can use the results for regions 1 and 2 to construct the field everywhere: H = 0 (y > 2) and (y < −2) H = 4(2 − |y|2 )ax A/m (0 < |y| < 1) H = 4(|y| − 2)2 ax A/m (1 < |y| < 2) 8.19. Calculate ∇ × [∇(∇ · G)] if G = 2x2yz ax − 20y ay + (x2 − z2) az: Proceding, we first find ∇ · G = 4xyz − 20 − 2z. Then ∇(∇ · G) = 4yz ax + 4xz ay + (4xy − 2) az. Then ∇ × [∇(∇ · G)] = (4x − 4x) ax − (4y − 4y) ay + (4z − 4z) az = 0 8.20. The magnetic field intensity is given in the square region x = 0, 0.5 < y < 1, 1 < z < 1.5 by H = z2ax + x3ay + y4az A/m. a) evaluate H · dL about the perimeter of the square region: Using dL = dxax + dyay + dzaz, and using the given field, we find, in the x = 0 plane: H · dL = 1 .5 0 dy + 1.5 1 (1)4 dz + .5 1 0 dy + 1 1.5 (.5)4 dz = 0.46875 b) Find ∇ × H: ∇ × H = ∂Hz ∂y − ∂Hy ∂z ax + ∂Hx ∂z − ∂Hz ∂x ay + ∂Hy ∂x − ∂Hx ∂y az = 4y3 ax + 2zay + 3x2 az c) Calculate (∇ × H)x at the center of the region: Here, y = 0.75 and so (∇ × H)x = 4(.75)3 = 1.68750. d) Does (∇×H)x = [ H·dL]/Area Enclosed? Using the part a result, [ H·dL]/Area Enclosed = 0.46875/0.25 = 1.8750, which is off the value found in part c. Answer: No. Reason: the limit of the area shrinking to zero must be taken before the results will be equal. 8.21. Points A, B, C, D, E, and F are each 2 mm from the origin on the coordinate axes indicated in Fig. 8.23. The value of H at each point is given. Calculate an approximate value for ∇ × H at the origin: We use the approximation: curl H . = H · dL a where no limit as a → 0 is taken (hence the approximation), and where a = 4 mm2. Each curl component is found by integrating H over a square path that is normal to the component in question. 128 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 131. 8.21. (continued) Each of the four segments of the contour passes through one of the given points. Along each segment, the field is assumed constant, and so the integral is evaluated by summing the products of the field and segment length (4 mm) over the four segments. The x component of the curl is thus: (∇ × H)x . = (Hz,C − Hy,E − Hz,D + Hy,F )(4 × 10−3) (4 × 10−3)2 = (15.69 + 13.88 − 14.35 − 13.10)(250) = 530 A/m2 The other components are: (∇ × H)y . = (Hz,B + Hx,E − Hz,A − Hx,F )(4 × 10−3) (4 × 10−3)2 = (15.82 + 11.11 − 14.21 − 10.88)(250) = 460 A/m2 and (∇ × H)z . = (Hy,A − Hx,C − Hy,BHx,D)(4 × 10−3) (4 × 10−3)2 = (−13.78 − 10.49 + 12.19 + 11.49)(250) = −148 A/m2 Finally we assemble the results and write: ∇ × H . = 530 ax + 460 ay − 148 az 8.22. In the cylindrical region ρ ≤ 0.6 mm, Hφ = (2/ρ) + (ρ/2) A/m, while Hφ = (3/ρ) A/m for ρ > 0.6 mm. a) Determine J for ρ < 0.6mm: We have only a φ component that varies with ρ. Therefore ∇ × H = 1 ρ d(ρHφ) dρ az = 1 ρ d dρ 2 + ρ2 2 az = J = 1az A/m2 b) Determine J for ρ > 0.6 mm: In this case J = 1 ρ d dρ ρ 3 ρ az = 0 c) Is there a filamentary current at ρ = 0? If so, what is its value? As ρ → 0, Hφ → ∞, which implies the existence of a current filament along the z axis: So, YES. The value is found by through Ampere’s circuital law, by integrating Hφ around a circular path of vanishingly-small radius. The current enclosed is therefore I = 2πρ(2/ρ) = 4π A. d) What is J at ρ = 0? Since a filament current lies along z at ρ = 0, this forms a singularity, and so the current density there is infinite. 8.23. Given the field H = 20ρ2 aφ A/m: a) Determine the current density J: This is found through the curl of H, which simplifies to a single term, since H varies only with ρ and has only a φ component: J = ∇ × H = 1 ρ d(ρHφ) dρ az = 1 ρ d dρ 20ρ3 az = 60ρ az A/m2 129 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 132. 8.23. (continued) b) Integrate J over the circular surface ρ = 1, 0 < φ < 2π, z = 0, to determine the total current passing through that surface in the az direction: The integral is: I = J · dS = 2π 0 1 0 60ρaz · ρ dρ dφaz = 40π A c) Find the total current once more, this time by a line integral around the circular path ρ = 1, 0 < φ < 2π, z = 0: I = H · dL = 2π 0 20ρ2 aφ ρ=1 · (1)dφaφ = 2π 0 20 dφ = 40π A 8.24. Evaluate both sides of Stokes’theorem for the field G = 10 sin θ aφ and the surface r = 3, 0 ≤ θ ≤ 90◦, 0 ≤ φ ≤ 90◦. Let the surface have the ar direction: Stokes’ theorem reads: C G · dL = S (∇ × G) · n da Considering the given surface, the contour, C, that forms its perimeter consists of three joined arcs of radius 3 that sweep out 90◦ in the xy, xz, and zy planes. Their centers are at the origin. Of these three, only the arc in the xy plane (which lies along aφ) is in the direction of G; the other two (in the −aθ and aθ directions respectively) are perpendicular to it, and so will not contribute to the path integral. The left-hand side therefore consists of only the xy plane portion of the closed path, and evaluates as G · dL = π/2 0 10 sin θ π/2 aφ · aφ 3 sin θ π/2 dφ = 15π To evaluate the right-hand side, we first find ∇ × G = 1 r sin θ d dθ [(sin θ)10 sin θ] ar = 20 cos θ r ar The surface over which we integrate this is the one-eighth spherical shell of radius 3 in the first octant, bounded by the three arcs described earlier. The right-hand side becomes S (∇ × G) · n da = π/2 0 π/2 0 20 cos θ 3 ar · ar (3)2 sin θ dθ dφ = 15π It would appear that the theorem works. 130 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 133. 8.25. (This problem was discovered to be flawed – I will proceed with it and show how). Given the field H = 1 2 cos φ 2 aρ − sin φ 2 aφ A/m evaluate both sides of Stokes’ theorem for the path formed by the intersection of the cylinder ρ = 3 and the plane z = 2, and for the surface defined by ρ = 3, 0 ≤ φ ≤ 2π, and z = 0, 0 ≤ ρ ≤ 3: This surface resembles that of an open tin can whose bottom lies in the z = 0 plane, and whose open circular edge, at z = 2, defines the line integral contour. We first evaluate H · dL over the circular contour, where we take the integration direction as clockwise, looking down on the can. We do this because the outward normal from the bottom of the can will be in the −az direction. H · dL = 2π 0 H · 3dφ(−aφ) = 2π 0 3 sin φ 2 dφ = 12 A With our choice of contour direction, this indicates that the current will flow in the negative z direction. Note for future reference that only the φ component of the given field contributed here. Next, we evalute ∇ × H · dS, over the surface of the tin can. We find ∇ × H = J = 1 ρ ∂(ρHφ) ∂ρ − ∂Hρ ∂φ az = 1 ρ − sin φ 2 + 1 4 sin φ 2 az = − 3 4ρ sin φ 2 az A/m Note that both field components contribute here. The integral over the tin can is now only over the bottom surface, since ∇ × H has only a z component. We use the outward normal, −az, and find ∇ × H · dS = − 3 4 2π 0 3 0 1 ρ sin φ 2 az · (−az)ρ dρ dφ = 9 4 2π 0 sin φ 2 dφ = 9 A Note that if the radial component of H were not included in the computation of ∇ × H, then the factor of 3/4 in front of the above integral would change to a factor of 1, and the result would have been 12 A. What would appear to be a violation of Stokes’ theorem is likely the result of a missing term in the φ component of H, having zero curl, which would have enabled the original line integral to have a value of 9A. The reader is invited to explore this further. 8.26. Let G = 15raφ. a) Determine G · dL for the circular path r = 5, θ = 25◦, 0 ≤ φ ≤ 2π: G · dL = 2π 0 15(5)aφ · aφ(5) sin(25◦ ) dφ = 2π(375) sin(25◦ ) = 995.8 b) Evaluate S(∇×G)·dS over the spherical cap r = 5, 0 ≤ θ ≤ 25◦, 0 ≤ φ ≤ 2π: When evaluating the curl of G using the formula in spherical coordinates, only one of the six terms survives: ∇ × G = 1 r sin θ ∂(Gφ sin θ) ∂θ ar = 1 r sin θ 15r cos θ ar = 15 cot θ ar Then S (∇ × G) · dS = 2π 0 25◦ 0 15 cot θ ar · ar (5)2 sin θ dθ dφ = 2π 25◦ 0 15 cos θ(25) dθ = 2π(15)(25) sin(25◦ ) = 995.8 131 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 134. 8.27. The magnetic field intensity is given in a certain region of space as H = x + 2y z2 ay + 2 z az A/m a) Find ∇ × H: For this field, the general curl expression in rectangular coordinates simplifies to ∇ × H = − ∂Hy ∂z ax + ∂Hy ∂x az = 2(x + 2y) z3 ax + 1 z2 az A/m b) Find J: This will be the answer of part a, since ∇ × H = J. c) Use J to find the total current passing through the surface z = 4, 1 < x < 2, 3 < y < 5, in the az direction: This will be I = J z=4 · az dx dy = 5 3 2 1 1 42 dx dy = 1/8 A d) Show that the same result is obtained using the other side of Stokes’ theorem: We take H · dL over the square path at z = 4 as defined in part c. This involves two integrals of the y component of H over the range 3 < y < 5. Integrals over x, to complete the loop, do not exist since there is no x component of H. We have I = H z=4 · dL = 5 3 2 + 2y 16 dy + 3 5 1 + 2y 16 dy = 1 8 (2) − 1 16 (2) = 1/8 A 8.28. Given H = (3r2/ sin θ)aθ + 54r cos θaφ A/m in free space: a) find the total current in the aθ direction through the conical surface θ = 20◦, 0 ≤ φ ≤ 2π, 0 ≤ r ≤ 5, by whatever side of Stokes’theorem you like best. I chose the line integral side, where the integration path is the circular path in φ around the top edge of the cone, at r = 5. The path direction is chosen to be clockwise looking down on the xy plane. This, by convention, leads to the normal from the cone surface that points in the positive aθ direction (right hand rule). We find H · dL = 2π 0 (3r2 / sin θ)aθ + 54r cos θaφ r=5,θ=20 · 5 sin(20◦ ) dφ (−aφ) = −2π(54)(25) cos(20◦ ) sin(20◦ ) = −2.73 × 103 A This result means that there is a component of current that enters the cone surface in the −aθ direction, to which is associated a component of H in the positive aφ direction. b) Check the result by using the other side of Stokes’ theorem: We first find the current density through the curl of the magnetic field, where three of the six terms in the spherical coordinate formula survive: ∇ × H = 1 r sin θ ∂ ∂θ (54r cos θ sin θ)) ar − 1 r ∂ ∂r 54r2 cos θ aθ + 1 r ∂ ∂r 3r3 sin θ aφ = J Thus J = 54 cot θ ar − 108 cos θ aθ + 9r sin θ aφ 132 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 135. 8.28b. (continued) The calculation of the other side of Stokes’ theorem now involves integrating J over the surface of the cone, where the outward normal is positive aθ , as defined in part a: S (∇ × H) · dS = 2π 0 5 0 54 cot θ ar − 108 cos θ aθ + 9r sin θ aφ θ=20◦ · aθ r sin(20◦ ) dr dφ = − 2π 0 5 0 108 cos(20◦ ) sin(20◦ )rdrdφ = −2π(54)(25) cos(20◦ ) sin(20◦ ) = −2.73 × 103 A 8.29. A long straight non-magnetic conductor of 0.2 mm radius carries a uniformly-distributed current of 2 A dc. a) Find J within the conductor: Assuming the current is +z directed, J = 2 π(0.2 × 10−3)2 az = 1.59 × 107 az A/m2 b) Use Ampere’s circuital law to find H and B within the conductor: Inside, at radius ρ, we have 2πρHφ = πρ2 J ⇒ H = ρJ 2 aφ = 7.96 × 106 ρ aφ A/m Then B = µ0H = (4π × 10−7)(7.96 × 106)ρaφ = 10ρ aφ Wb/m2. c) Show that ∇ × H = J within the conductor: Using the result of part b, we find, ∇ × H = 1 ρ d dρ (ρHφ) az = 1 ρ d dρ 1.59 × 107ρ2 2 az = 1.59 × 107 az A/m2 = J d) Find H and B outside the conductor (note typo in book): Outside, the entire current is enclosed by a closed path at radius ρ, and so H = I 2πρ aφ = 1 πρ aφ A/m Now B = µ0H = µ0/(πρ) aφ Wb/m2. e) Show that ∇ × H = J outside the conductor: Here we use H outside the conductor and write: ∇ × H = 1 ρ d dρ (ρHφ) az = 1 ρ d dρ ρ 1 πρ az = 0 (as expected) 133 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 136. 8.30. A solid nonmagnetic conductor of circular cross-section has a radius of 2mm. The conductor is inho- mogeneous, with σ = 106(1 + 106ρ2) S/m. If the conductor is 1m in length and has a voltage of 1mV between its ends, find: a) H inside: With current along the cylinder length (along az, and with φ symmetry, H will be φ- directed only. We find E = (V0/d)az = 10−3az V/m. Then J = σE = 103(1 + 106ρ2)az A/m2. Next we apply Ampere’s circuital law to a circular path of radius ρ, centered on the z axis and normal to the axis: H · dL = 2πρHφ = S J · dS = 2π 0 ρ 0 103 (1 + 106 (ρ′ )2 )az · azρ′ dρ′ dφ Thus Hφ = 103 ρ ρ 0 ρ′ + 106 (ρ′ )3 dρ′ = 103 ρ ρ2 2 + 106 4 ρ4 Finally, H = 500ρ(1 + 5 × 105ρ3)aφ A/m (0 < ρ < 2mm). b) the total magnetic flux inside the conductor: With field in the φ direction, a plane normal to B will be that in the region 0 < ρ < 2 mm, 0 < z < 1 m. The flux will be = S B·dS = µ0 1 0 2×10−3 0 500ρ + 2.5 × 108 ρ3 dρdz = 8π ×10−10 Wb = 2.5 nWb 8.31. The cylindrical shell defined by 1 cm < ρ < 1.4 cm consists of a non-magnetic conducting material and carries a total current of 50 A in the az direction. Find the total magnetic flux crossing the plane φ = 0, 0 < z < 1: a) 0 < ρ < 1.2 cm: We first need to find J, H, and B: The current density will be: J = 50 π[(1.4 × 10−2)2 − (1.0 × 10−2)2] az = 1.66 × 105 az A/m2 Next we find Hφ at radius ρ between 1.0 and 1.4 cm, by applying Ampere’s circuital law, and noting that the current density is zero at radii less than 1 cm: 2πρHφ = Iencl = 2π 0 ρ 10−2 1.66 × 105 ρ′ dρ′ dφ ⇒ Hφ = 8.30 × 104 (ρ2 − 10−4) ρ A/m (10−2 m < ρ < 1.4 × 10−2 m) Then B = µ0H, or B = 0.104 (ρ2 − 10−4) ρ aφ Wb/m2 Now, a = B · dS = 1 0 1.2×10−2 10−2 0.104 ρ − 10−4 ρ dρ dz = 0.104 (1.2 × 10−2)2 − 10−4 2 − 10−4 ln 1.2 1.0 = 3.92 × 10−7 Wb = 0.392 µWb 134 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 137. 8.31b) 1.0 cm < ρ < 1.4 cm (note typo in book): This is part a over again, except we change the upper limit of the radial integration: b = B · dS = 1 0 1.4×10−2 10−2 0.104 ρ − 10−4 ρ dρ dz = 0.104 (1.4 × 10−2)2 − 10−4 2 − 10−4 ln 1.4 1.0 = 1.49 × 10−6 Wb = 1.49 µWb c) 1.4 cm < ρ < 20 cm: This is entirely outside the current distribution, so we need B there: We modify the Ampere’s circuital law result of part a to find: Bout = 0.104 [(1.4 × 10−2)2 − 10−4] ρ aφ = 10−5 ρ aφ Wb/m2 We now find c = 1 0 20×10−2 1.4×10−2 10−5 ρ dρ dz = 10−5 ln 20 1.4 = 2.7 × 10−5 Wb = 27 µWb 8.32. The free space region defined by 1 < z < 4 cm and 2 < ρ < 3 cm is a toroid of rectangular cross-section. Let the surface at ρ = 3 cm carry a surface current K = 2az kA/m. a) Specify the current densities on the surfaces at ρ = 2 cm, z = 1cm, and z = 4cm. All surfaces must carry equal currents. With this requirement, we find: K(ρ = 2) = −3 az kA/m. Next, the current densities on the z = 1 and z = 4 surfaces must transistion between the current density values at ρ = 2 and ρ = 3. Knowing the the radial current density will vary as 1/ρ, we find K(z = 1) = (60/ρ)aρ A/m with ρ in meters. Similarly, K(z = 4) = −(60/ρ)aρ A/m. b) Find H everywhere: Outside the toroid, H = 0. Inside, we apply Ampere’s circuital law in the manner of Problem 8.14: H · dL = 2πρHφ = 2π 0 K(ρ = 2) · az (2 × 10−2 ) dφ ⇒ H = − 2π(3000)(.02) ρ aφ = −60/ρ aφ A/m (inside) c) Calculate the total flux within the toriod: We have B = −(60µ0/ρ)aφ Wb/m2. Then = .04 .01 .03 .02 −60µ0 ρ aφ · (−aφ) dρ dz = (.03)(60)µ0 ln 3 2 = 0.92 µWb 8.33. Use an expansion in cartesian coordinates to show that the curl of the gradient of any scalar field G is identically equal to zero. We begin with ∇G = ∂G ∂x ax + ∂G ∂y ay + ∂G ∂z az and ∇ × ∇G = ∂ ∂y ∂G ∂z − ∂ ∂z ∂G ∂y ax + ∂ ∂z ∂G ∂x − ∂ ∂x ∂G ∂z ay + ∂ ∂x ∂G ∂y − ∂ ∂y ∂G ∂x az = 0 for any G 135 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 138. 8.34. A filamentary conductor on the z axis carries a current of 16A in the az direction, a conducting shell at ρ = 6 carries a total current of 12A in the −az direction, and another shell at ρ = 10 carries a total current of 4A in the −az direction. a) Find H for 0 < ρ < 12: Ampere’s circuital law states that H·dL = Iencl, where the line integral and current direction are related in the usual way through the right hand rule. Therefore, if I is in the positive z direction, H is in the aφ direction. We proceed as follows: 0 < ρ < 6 : 2πρHφ = 16 ⇒ H = 16/(2πρ)aφ 6 < ρ < 10 : 2πρHφ = 16 − 12 ⇒ H = 4/(2πρ)aφ ρ > 10 : 2πρHφ = 16 − 12 − 4 = 0 ⇒ H = 0 b) Plot Hφ vs. ρ: c) Find the total flux crossing the surface 1 < ρ < 7, 0 < z < 1: This will be = 1 0 6 1 16µ0 2πρ dρ dz + 1 0 7 6 4µ0 2πρ dρ dz = 2µ0 π [4 ln 6 + ln(7/6)] = 5.9 µWb 8.35. A current sheet, K = 20 az A/m, is located at ρ = 2, and a second sheet, K = −10 az A/m is located at ρ = 4. a.) Let Vm = 0 at P (ρ = 3, φ = 0, z = 5) and place a barrier at φ = π. Find Vm(ρ, φ, z) for −π < φ < π: Since the current is cylindrically-symmetric, we know that H = I/(2πρ) aφ, where I is the current enclosed, equal in this case to 2π(2)K = 80π A. Thus, using the result of Section 8.6, we find Vm = − I 2π φ = − 80π 2π φ = −40φ A which is valid over the region 2 < ρ < 4, −π < φ < π, and −∞ < z < ∞. For ρ > 4, the outer current contributes, leading to a total enclosed current of Inet = 2π(2)(20) − 2π(4)(10) = 0 With zero enclosed current, Hφ = 0, and the magnetic potential is zero as well. 136 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 139. 8.35b. Let A = 0 at P and find A(ρ, φ, z) for 2 < ρ < 4: Again, we know that H = Hφ(ρ), since the current is cylindrically symmetric. With the current only in the z direction, and again using symmmetry, we expect only a z component of A which varies only with ρ. We can then write: ∇ × A = − dAz dρ aφ = B = µ0I 2πρ aφ Thus dAz dρ = − µ0I 2πρ ⇒ Az = − µ0I 2π ln(ρ) + C We require that Az = 0 at ρ = 3. Therefore C = [(µ0I)/(2π)] ln(3), Then, with I = 80π, we finally obtain A = − µ0(80π) 2π [ln(ρ) − ln(3)] az = 40µ0 ln 3 ρ az Wb/m 8.36. Let A = (3y − z)ax + 2xzay Wb/m in a certain region of free space. a) Show that ∇ · A = 0: ∇ · A = ∂ ∂x (3y − z) + ∂ ∂y 2xz = 0 b) At P (2, −1, 3), find A, B, H, and J: First AP = −6ax + 12ay. Then, using the curl formula in cartesian coordinates, B = ∇ × A = −2xax − ay + (2z − 3)az ⇒ BP = −4ax − ay + 3az Wb/m2 Now HP = (1/µ0)BP = −3.2 × 106 ax − 8.0 × 105 ay + 2.4 × 106 az A/m Then J = ∇ × H = (1/µ0)∇ × B = 0, as the curl formula in cartesian coordinates shows. 8.37. Let N = 1000, I = 0.8 A, ρ0 = 2 cm, and a = 0.8 cm for the toroid shown in Fig. 8.12b. Find Vm in the interior of the toroid if Vm = 0 at ρ = 2.5 cm, φ = 0.3π. Keep φ within the range 0 < φ < 2π: Well-within the toroid, we have H = NI 2πρ aφ = −∇Vm = − 1 ρ dVm dφ aφ Thus Vm = − NIφ 2π + C Then, 0 = − 1000(0.8)(0.3π) 2π + C or C = 120. Finally Vm = 120 − 400 π φ A (0 < φ < 2π) 137 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 140. 8.38. The solenoid shown in Fig. 8.11b contains 400 turns, carries a current I = 5 A, has a length of 8cm, and a radius a = 1.2 cm (hope it doesn’t blow up!). a) Find H within the solenoid. Assuming the current flows in the aφ direction, H will then be along the positive z direction, and will be given by H = NI d az = (400)(5) .08 az = 2.5 × 104 A/m b) If Vm = 0 at the origin, specify Vm(ρ, φ, z) inside the solenoid: Since H is only in the z direction, Vm should vary with z only. Use H = −∇Vm = − dVm dz az ⇒ Vm = −Hzz + C At z = 0, Vm = 0, so C = 0. Therefore Vm(z) = −2.5 × 104z A c) Let A = 0 at the origin, and specify A(ρ, φ, z) inside the solenoid if the medium is free space. A should be in the same direction as the current, and so would have a φ component only. Furthermore, since ∇ × A = B, the curl will be z-directed only. Therefore ∇ × A = 1 ρ ∂ ∂ρ (ρAφ)az = µ0Hzaz Then ∂ ∂ρ (ρAφ) = µ0Hzρ ⇒ Aφ = µ0Hzρ 2 + C Aφ = 0 at the origin, so C = 0. Finally, A = (4π × 10−7)(2.5 × 104)ρ 2 aφ = 15.7aφ mWb/m 8.39. Planar current sheets of K = 30az A/m and −30az A/m are located in free space at x = 0.2 and x = −0.2 respectively. For the region −0.2 < x < 0.2: a) Find H: Since we have parallel current sheets carrying equal and opposite currents, we use Eq. (12), H = K × aN , where aN is the unit normal directed into the region between currents, and where either one of the two currents are used. Choosing the sheet at x = 0.2, we find H = 30az × −ax = −30ay A/m b) Obtain and expression for Vm if Vm = 0 at P (0.1, 0.2, 0.3): Use H = −30ay = −∇Vm = − dVm dy ay So dVm dy = 30 ⇒ Vm = 30y + C1 Then 0 = 30(0.2) + C1 ⇒ C1 = −6 ⇒ Vm = 30y − 6 A 138 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 141. 8.39c) Find B: B = µ0H = −30µ0ay Wb/m2. d) Obtain an expression for A if A = 0 at P : We expect A to be z-directed (with the current), and so from ∇ × A = B, where B is y-directed, we set up − dAz dx = −30µ0 ⇒ Az = 30µ0x + C2 Then 0 = 30µ0(0.1) + C2 ⇒ C2 = −3µ0 So finally A = µ0(30x − 3)az Wb/m 8.40. Let A = (3y2 − 2z)ax − 2x2zay + (x + 2y)az Wb/m in free space. Find ∇ × ∇ × A at P (−2, 3, −1): First ∇ × A = ∂(x + 2y) ∂y − ∂(−2x2z) ∂z ax + ∂(3y2 − 2z) ∂z − ∂(x + 2y) ∂x ay + ∂(−2x2z) ∂x − ∂(3y2 − 2z) ∂y az = (2 + 2x2 )ax − 3ay − (4xz + 6y)az Then ∇ × ∇ × A = ∂(4xz + 6y) ∂x ay − ∂(4xz + 6y) ∂y ax = −6ax + 4zay At P this becomes ∇ × ∇ × A|P = −6ax − 4ay Wb/m3. 8.41. Assume that A = 50ρ2az Wb/m in a certain region of free space. a) Find H and B: Use B = ∇ × A = − ∂Az ∂ρ aφ = −100ρ aφ Wb/m2 Then H = B/µ0 = −100ρ/µ0 aφ A/m. b) Find J: Use J = ∇ × H = 1 ρ ∂ ∂ρ (ρHφ)az = 1 ρ ∂ ∂ρ −100ρ2 µ0 az = − 200 µ0 az A/m2 c) Use J to find the total current crossing the surface 0 ≤ ρ ≤ 1, 0 ≤ φ < 2π, z = 0: The current is I = J · dS = 2π 0 1 0 −200 µ0 az · az ρ dρ dφ = −200π µ0 A = −500 kA d) Use the value of Hφ at ρ = 1 to calculate H · dL for ρ = 1, z = 0: Have H · dL = I = 2π 0 −100 µ0 aφ · aφ (1)dφ = −200π µ0 A = −500 kA 139 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 142. 8.42. Show that ∇2(1/R12) = −∇1(1/R12) = R21/R3 12. First ∇2 1 R12 = ∇2 (x2 − x1)2 + (y2 − y1)2 + (z2 − z1)2 −1/2 = − 1 2 2(x2 − x1)ax + 2(y2 − y1)ay + 2(z2 − z1)az [(x2 − x1)2 + (y2 − y1)2 + (z2 − z1)2]3/2 = −R12 R3 12 = R21 R3 12 Also note that ∇1(1/R12) would give the same result, but of opposite sign. 8.43. Compute the vector magnetic potential within the outer conductor for the coaxial line whose vector magnetic potential is shown in Fig. 8.20 if the outer radius of the outer conductor is 7a. Select the proper zero reference and sketch the results on the figure: We do this by first finding B within the outer conductor and then “uncurling” the result to find A. With −z-directed current I in the outer conductor, the current density is Jout = − I π(7a)2 − π(5a)2 az = − I 24πa2 az Since current I flows in both conductors, but in opposite directions, Ampere’s circuital law inside the outer conductor gives: 2πρHφ = I − 2π 0 ρ 5a I 24πa2 ρ′ dρ′ dφ ⇒ Hφ = I 2πρ 49a2 − ρ2 24a2 Now, with B = µ0H, we note that ∇ × A will have a φ component only, and from the direction and symmetry of the current, we expect A to be z-directed, and to vary only with ρ. Therefore ∇ × A = − dAz dρ aφ = µ0H and so dAz dρ = − µ0I 2πρ 49a2 − ρ2 24a2 Then by direct integration, Az = −µ0I(49) 48πρ dρ + µ0Iρ 48πa2 dρ + C = µ0I 96π ρ2 a2 − 98 ln ρ + C As per Fig. 8.20, we establish a zero reference at ρ = 5a, enabling the evaluation of the integration constant: C = − µ0I 96π [25 − 98 ln(5a)] Finally, Az = µ0I 96π ρ2 a2 − 25 + 98 ln 5a ρ Wb/m A plot of this continues the plot of Fig. 8.20, in which the curve goes negative at ρ = 5a, and then approaches a minimum of −.09µ0I/π at ρ = 7a, at which point the slope becomes zero. 140 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 143. 8.44. By expanding Eq.(58), Sec. 8.7 in cartesian coordinates, show that (59) is correct. Eq. (58) can be rewritten as ∇2 A = ∇(∇ · A) − ∇ × ∇ × A We begin with ∇ · A = ∂Ax ∂x + ∂Ay ∂y + ∂Az ∂z Then the x component of ∇(∇ · A) is [∇(∇ · A)]x = ∂2Ax ∂x2 + ∂2Ay ∂x∂y + ∂2Az ∂x∂z Now ∇ × A = ∂Az ∂y − ∂Ay ∂z ax + ∂Ax ∂z − ∂Az ∂x ay + ∂Ay ∂x − ∂Ax ∂y az and the x component of ∇ × ∇ × A is [∇ × ∇ × A]x = ∂2Ay ∂x∂y − ∂2Ax ∂y2 − ∂2Ax ∂z2 + ∂2Az ∂z∂y Then, using the underlined results [∇(∇ · A) − ∇ × ∇ × A]x = ∂2Ax ∂x2 + ∂2Ax ∂y2 + ∂2Ax ∂z2 = ∇2 Ax Similar results will be found for the other two components, leading to ∇(∇ · A) − ∇ × ∇ × A = ∇2 Axax + ∇2 Ayay + ∇2 Azaz ≡ ∇2 A QED 141 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 144. CHAPTER 9 9.1. A point charge, Q = −0.3 µC and m = 3×10−16 kg, is moving through the field E = 30 az V/m. Use Eq. (1) and Newton’s laws to develop the appropriate differential equations and solve them, subject to the initial conditions at t = 0: v = 3 × 105 ax m/s at the origin. At t = 3 µs, find: a) the position P (x, y, z) of the charge: The force on the charge is given by F = qE, and Newton’s second law becomes: F = ma = m d2z dt2 = qE = (−0.3 × 10−6 )(30 az) describing motion of the charge in the z direction. The initial velocity in x is constant, and so no force is applied in that direction. We integrate once: dz dt = vz = qE m t + C1 The initial velocity along z, vz(0) is zero, and so C1 = 0. Integrating a second time yields the z coordinate: z = qE 2m t2 + C2 The charge lies at the origin at t = 0, and so C2 = 0. Introducing the given values, we find z = (−0.3 × 10−6)(30) 2 × 3 × 10−16 t2 = −1.5 × 1010 t2 m At t = 3 µs, z = −(1.5 × 1010)(3 × 10−6)2 = −.135 cm. Now, considering the initial constant velocity in x, the charge in 3 µs attains an x coordinate of x = vt = (3×105)(3×10−6) = .90 m. In summary, at t = 3 µs we have P (x, y, z) = (.90, 0, −.135). b) the velocity, v: After the first integration in part a, we find vz = qE m t = −(3 × 1010 )(3 × 10−6 ) = −9 × 104 m/s Including the intial x-directed velocity, we finally obtain v = 3 × 105 ax − 9 × 104az m/s. c) the kinetic energy of the charge: Have K.E. = 1 2 m|v|2 = 1 2 (3 × 10−16 )(1.13 × 105 )2 = 1.5 × 10−5 J 9.2. A point charge, Q = −0.3 µC and m = 3×10−16 kg, is moving through the field B = 30az mT. Make use of Eq. (2) and Newton’s laws to develop the appropriate differential equations, and solve them, subject to the initial condition at t = 0, v = 3 × 105 m/s at the origin. Solve these equations (perhaps with the help of an example given in Section 7.5) to evaluate at t = 3µs: a) the position P (x, y, z) of the charge; b) its velocity; c) and its kinetic energy: We begin by visualizing the problem. Using F = qv × B, we find that a positive charge moving along positive ax, would encounter the z-directed B field and be deflected into the negative y direction. 142 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 145. 9.2 (continued) Motion along negative y through the field would cause further deflection into the negative x direction. We can construct the differential equations for the forces in x and in y as follows: Fxax = m dvx dt ax = qvyay × Baz = qBvyax Fyay = m dvy dt ay = qvxax × Baz = −qBvxay or dvx dt = qB m vy (1) and dvy dt = − qB m vx (2) To solve these equations, we first differentiate (2) with time and substitute (1), obtaining: d2vy dt2 = − qB m dvx dt = − qB m 2 vy Therefore, vy = A sin(qBt/m) + A′ cos(qBt/m). However, at t = 0, vy = 0, and so A′ = 0, leaving vy = A sin(qBt/m). Then, using (2), vx = − m qB dvy dt = −A cos qBt m Now at t = 0, vx = vx0 = 3 × 105. Therefore A = −vx0, and so vx = vx0 cos(qBt/m), and vy = −vx0 sin(qBt/m). The positions are then found by integrating vx and vy over time: x(t) = vx0 cos qBt m dt + C = mvx0 qB sin qBt m + C where C = 0, since x(0) = 0. Then y(t) = −vx0 sin qBt m dt + D = mvx0 qB cos qBt m + D We require that y(0) = 0, so D = −(mvx0)/(qB), and finally y(t) = −mvx0/qB [1 − cos (qBt/m)]. Summarizing, we have, using q = −3×10−7 C, m = 3×10−16 kg, B = 30×10−3 T, and vx0 = 3×105 m/s: x(t) = mvx0 qB sin qBt m = −10−2 sin(−3 × 10−7 t) m y(t) = − mvx0 qB 1 − cos qBt m = 10−2 [1 − cos(−3 × 107 t)] m vx(t) = vx0 cos qBt m = 3 × 105 cos(−3 × 107 t) m/s vy(t) = −vx0 sin qBt m = −3 × 105 sin(−3 × 107 t) m/s 143 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 146. 9.2 (continued) The answers are now: a) At t = 3 × 10−6 s, x = 8.9 mm, y = 14.5 mm, and z = 0. b) At t = 3 × 10−6 s, vx = −1.3 × 105 m/s, vy = 2.7 × 105 m/s, and so v(t = 3 µs) = −1.3 × 105 ax + 2.7 × 105 ay m/s whose magnitude is v = 3 × 105 m/s as would be expected. c) Kinetic energy is K.E. = (1/2)mv2 = 1.35 µJ at all times. 9.3. A point charge for which Q = 2 × 10−16 C and m = 5 × 10−26 kg is moving in the combined fields E = 100ax − 200ay + 300az V/m and B = −3ax + 2ay − az mT. If the charge velocity at t = 0 is v(0) = (2ax − 3ay − 4az) × 105 m/s: a) give the unit vector showing the direction in which the charge is accelerating at t = 0: Use F(t = 0) = q[E + (v(0) × B)], where v(0) × B = (2ax − 3ay − 4az)105 × (−3ax + 2ay − az)10−3 = 1100ax + 1400ay − 500az So the force in newtons becomes F(0) = (2×10−16 )[(100+1100)ax+(1400−200)ay+(300−500)az] = 4×10−14 [6ax+6ay−az] The unit vector that gives the acceleration direction is found from the force to be aF = 6ax + 6ay − az √ 73 = .70ax + .70ay − .12az b) find the kinetic energy of the charge at t = 0: K.E. = 1 2 m|v(0)|2 = 1 2 (5 × 10−26 kg)(5.39 × 105 m/s)2 = 7.25 × 10−15 J = 7.25 fJ 9.4. An electron (qe = −1.60219 × 10−19 C, m = 9.10956 × 10−31 kg) is moving at a constant velocity v = 4.5 × 107ay m/s along the negative y axis. At the origin it encounters the uniform magnetic field B = 2.5az mT, and remains in it up to y = 2.5 cm. If we assume (with good accuracy) that the electron remains on the y axis while it is in the magnetic field, find its x-, y-, and z-coordinate values when y = 50 cm: The procedure is to find the electron velocity as it leaves the field, and then determine its coordinates at the time corresponding to y = 50 cm. The force it encounters while in the field is F = qv × B = (−1.60219 × 10−19 )(4.5 × 107 )(2.5 × 10−3 )(ay × az) = −1.80 × 10−14 ax N This force will be constant during the time the electron traverses the field. It establishes a negative x-directed velocity as it leaves the field, given by the acceleration times the transit time, tt : vx = Ftt m = −1.80 × 1014 N 9.10956 × 10−31 kg 2.5 × 10−2 m 4.5 × 107 m/s = −1.09 × 107 m/s 144 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 147. 9.4 (continued) The time for the electron to travel along y between 2.5 and 50 cm is t50 = (50 − 2.5) × 10−2 4.5 × 107 = 1.06 × 10−8 s In that time, the electron moves to an x coordinate given by x = vxt50 = −(1.09 × 107 )(1.06 × 10−8 ) = −.115 m The coordinates at the time the electron reaches y = 50 cm are then: x = −11.5 cm, y = 50 cm, z = 0 9.5. A rectangular loop of wire in free space joins points A(1, 0, 1) to B(3, 0, 1) to C(3, 0, 4) to D(1, 0, 4) to A. The wire carries a current of 6 mA, flowing in the az direction from B to C. A filamentary current of 15 A flows along the entire z axis in the az direction. a) Find F on side BC: FBC = C B IloopdL × Bfrom wire at BC Thus FBC = 4 1 (6 × 10−3 ) dz az × 15µ0 2π(3) ay = −1.8 × 10−8 ax N = −18ax nN b) Find F on side AB: The field from the long wire now varies with position along the loop segment. We include that dependence and write FAB = 3 1 (6 × 10−3 ) dx ax × 15µ0 2πx ay = 45 × 10−3 π µ0 ln 3 az = 19.8az nN c) Find Ftotal on the loop: This will be the vector sum of the forces on the four sides. Note that by symmetry, the forces on sides AB and CD will be equal and opposite, and so will cancel. This leaves the sum of forces on sides BC (part a) and DA, where FDA = 4 1 −(6 × 10−3 ) dz az × 15µ0 2π(1) ay = 54ax nN The total force is then Ftotal = FDA + FBC = (54 − 18)ax = 36 ax nN 9.6 The magnetic flux density in a region of free space is given by B = −3xax + 5yay − 2zaz T. Find the total force on the rectangular loop shown in Fig. 9.15 if it lies in the plane z = 0 and is bounded by x = 1, x = 3, y = 2, and y = 5, all dimensions in cm: First, note that in the plane z = 0, the z component of the given field is zero, so will not contribute to the force. We use F = loop IdL × B which in our case becomes, with I = 30 A: F = .03 .01 30dxax × (−3xax + 5y|y=.02 ay) + .05 .02 30dyay × (−3x|x=.03 ax + 5yay) + .01 .03 30dxax × (−3xax + 5y|y=.05 ay) + .02 .05 30dyay × (−3x|x=.01 ax + 5yay) 145 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 148. 9.6. (continued) Simplifying, this becomes F = .03 .01 30(5)(.02) az dx + .05 .02 −30(3)(.03)(−az) dy + .01 .03 30(5)(.05) az dx + .02 .05 −30(3)(.01)(−az) dy = (.060 + .081 − .150 − .027)az N = −36 az mN 9.7. Uniform current sheets are located in free space as follows: 8az A/m at y = 0, −4az A/m at y = 1, and −4az A/m at y = −1. Find the vector force per meter length exerted on a current filament carrying 7 mA in the aL direction if the filament is located at: a) x = 0, y = 0.5, and aL = az: We first note that within the region −1 < y < 1, the magnetic fields from the two outer sheets (carrying −4az A/m) cancel, leaving only the field from the center sheet. Therefore, H = −4ax A/m (0 < y < 1) and H = 4ax A/m (−1 < y < 0). Outside (y > 1 and y < −1) the fields from all three sheets cancel, leaving H = 0 (y > 1, y < −1). So at x = 0, y = .5, the force per meter length will be F/m = Iaz × B = (7 × 10−3 )az × −4µ0ax = −35.2ay nN/m b.) y = 0.5, z = 0, and aL = ax: F/m = Iax × −4µ0ax = 0. c) x = 0, y = 1.5, aL = az: Since y = 1.5, we are in the region in which B = 0, and so the force is zero. 9.8. Filamentary currents of −25az and 25az A are located in the x = 0 plane in free space at y = −1 and y = 1m respectively. A third filamentary current of 10−3az A is located at x = k, y = 0. Find the vector force on a 1-m length of the 1-mA filament and plot |F| versus k: The total B field arising from the two 25A filaments evaluated at the location of the 1-mA filament is, in cartesian components: B = 25µ0 2π(1 + k2) (kay + ax) line at y=+1 + 25µ0 2π(1 + k2) (−kay + ax) line at y=−1 = 25µ0ax π(1 + k2) The force on the 1m length of 1-mA line is now F = 10−3 (1)az × 25µ0ax π(1 + k2) = (2.5 × 10−2)(4 × 10−7) (1 + k2) ay = 10−8ay (1 + k2) ay N = 10ay (1 + k2) nN 146 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 149. 9.9. A current of −100az A/m flows on the conducting cylinder ρ = 5 mm and +500az A/m is present on the conducting cylinder ρ = 1 mm. Find the magnitude of the total force acting to split the outer cylinder apart along its length: The differential force acting on the outer cylinder arising from the field of the inner cylinder is dF = Kouter × B, where B is the field from the inner cylinder, evaluated at the outer cylinder location: B = 2π(1)(500)µ0 2π(5) aφ = 100µ0 aφ T Thus dF = −100az × 100µ0aφ = 104µ0aρ N/m2. We wish to find the force acting to split the outer cylinder, which means we need to evaluate the net force in one cartesian direction on one half of the cylinder. We choose the “upper” half (0 < φ < π), and integrate the y component of dF over this range, and over a unit length in the z direction: Fy = 1 0 π 0 104 µ0aρ · ay(5 × 10−3 ) dφ dz = π 0 50µ0 sin φ dφ = 100µ0 = 4π × 10−5 N/m Note that we did not include the “self force” arising from the outer cylinder’s B field on itself. Since the outer cylinder is a two-dimensional current sheet, its field exists only just outside the cylinder, and so no force exists. If this cylinder possessed a finite thickness, then we would need to include its self-force, since there would be an interior field and a volume current density that would spatially overlap. 9.10. Two infinitely-long parallel filaments each carry 50 A in the az direction. If the filaments lie in the plane y = 0 at x = 0 and x = 5mm (note bad wording in problem statement in book), find the vector force per meter length on the filament passing through the origin: The force will be F = 1 0 IdL × B where IdL is that of the filament at the origin, and B is that arising from the filament at x = 5mm evaluated at the location of the other filament (along the z axis). We obtain F = 1 0 50 dzaz × −50µ0ay 2π(5 × 10−3) = 0.10 ax N/m 9.11. a) Use Eq. (14), Sec. 9.3, to show that the force of attraction per unit length between two filamentary conductors in free space with currents I1az at x = 0, y = d/2, and I2az at x = 0, y = −d/2, is µ0I1I2/(2πd): The force on I2 is given by F2 = µ0 I1I2 4π aR12 × dL1 R2 12 × dL2 Let z1 indicate the z coordinate along I1, and z2 indicate the z coordinate along I2. We then have R12 = (z2 − z1)2 + d2 and aR12 = (z2 − z1)az − day (z2 − z1)2 + d2 Also, dL1 = dz1az and dL2 = dz2az The “inside” integral becomes: aR12 × dL1 R2 12 = [(z2 − z1)az − day] × dz1az [(z2 − z1)2 + d2]1.5 = ∞ −∞ −d dz1 ax [(z2 − z1)2 + d2]1.5 147 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 150. 9.11a. (continued) The force expression now becomes F2 = µ0 I1I2 4π ∞ −∞ −d dz1 ax [(z2 − z1)2 + d2]1.5 × dz2az = µ0 I1I2 4π 1 0 ∞ −∞ d dz1 dz2 ay [(z2 − z1)2 + d2]1.5 Note that the “outside” integral is taken over a unit length of current I2. Evaluating, obtain, F2 = µ0 I1I2d ay 4πd2 (2) 1 0 dz2 = µ0I1I2 2πd ay N/m as expected. b) Show how a simpler method can be used to check your result: We use dF2 = I2dL2 × B12, where the field from current 1 at the location of current 2 is B12 = µ0I1 2πd ax T so over a unit length of I2, we obtain F2 = I2az × µ0I1 2πd ax = µ0 I1I2 2πd ay N/m This second method is really just the first over again, since we recognize the inside integral of the first method as the Biot-Savart law, used to find the field from current 1 at the current 2 location. 9.12. A conducting current strip carrying K = 12az A/m lies in the x = 0 plane between y = 0.5 and y = 1.5 m. There is also a current filament of I = 5 A in the az direction on the z axis. Find the force exerted on the: a) filament by the current strip: We first need to find the field from the current strip at the filament location. Consider the strip as made up of many adjacent strips of width dy, each carrying current dIaz = Kdy. The field along the z axis from each differential strip will be dB = [(Kdyµ0)/(2πy)]ax. The total B field from the strip evaluated along the z axis is therefore B = 1.5 0.5 12µ0ax 2πy dy = 6µ0 π ln 1.5 0.5 ax = 2.64 × 10−6 ax Wb/m2 Now F = 1 0 IdL × B = 1 0 5dz az × 2.64 × 10−6 ax dz = 13.2 ay µN/m b) strip by the filament: In this case we integrate K ×B over a unit length in z of the strip area, where B is the field from the filament evaluated on the strip surface: F = Area K × B da = 1 0 1.5 0.5 12az × −5µ0ax 2πy dy = −30µ0 π ln(3) ay = −13.2 ay µN/m 148 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 151. 9.13. A current of 6A flows from M(2, 0, 5) to N(5, 0, 5) in a straight solid conductor in free space. An infinite current filament lies along the z axis and carries 50A in the az direction. Compute the vector torque on the wire segment using: a) an origin at (0, 0, 5): The B field from the long wire at the short wire is B = (µ0Izay)/(2πx) T. Then the force acting on a differential length of the wire segment is dF = IwdL × B = Iwdx ax × µ0Iz 2πx ay = µ0IwIz 2πx dx az N Now the differential torque about (0, 0, 5) will be dT = RT × dF = xax × µ0IwIz 2πx dx az = − µ0IwIz 2π dx ay The net torque is now found by integrating the differential torque over the length of the wire segment: T = 5 2 − µ0IwIz 2π dx ay = − 3µ0(6)(50) 2π ay = −1.8 × 10−4 ay N · m b) an origin at (0, 0, 0): Here, the only modification is in RT , which is now RT = x ax + 5 az So now dT = RT × dF = xax + 5az × µ0IwIz 2πx dx az = − µ0IwIz 2π dx ay Everything from here is the same as in part a, so again, T = −1.8 × 10−4 ay N · m. c) an origin at (3, 0, 0): In this case, RT = (x − 3)ax + 5az, and the differential torque is dT = (x − 3)ax + 5az × µ0IwIz 2πx dx az = − µ0IwIz(x − 3) 2πx dx ay Thus T = 5 2 − µ0IwIz(x − 3) 2πx dx ay = −6.0 × 10−5 3 − 3 ln 5 2 ay = −1.5 × 10−5 ay N · m 9.14. The rectangular loop of Prob. 6 is now subjected to the B field produced by two current sheets, K1 = 400 ay A/m at z = 2, and K2 = 300 az A/m at y = 0 in free space. Find the vector torque on the loop, referred to an origin: a) at (0,0,0): The fields from both current sheets, at the loop location, will be negative x-directed. They will add together to give, in the loop plane: B = −µ0 K1 2 + K2 2 ax = −µ0(200 + 150) ax = −350µ0 ax Wb/m2 With this field, forces will be acting only on the wire segments that are parallel to the y axis. The force on the segment nearer to the y axis will be F1 = IL × B = −30(3 × 10−2 )ay × −350µ0ax = −315µ0 az N 149 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 152. 9.14a (continued) The force acting on the segment farther from the y axis will be F2 = IL × B = 30(3 × 10−2 )ay × −350µ0ax = 315µ0 az N The torque about the origin is now T = R1 × F1 + R2 × F2, where R1 is the vector directed from the origin to the midpoint of the nearer y-directed segment, and R2 is the vector joining the origin to the midpoint of the farther y-directed segment. So R1(cm) = ax + 3.5ay and R2(cm) = 3ax + 3.5ay. Therefore T0,0,0 = [(ax + 3.5ay) × 10−2 ] × −315µ0 az + [(3ax + 3.5ay) × 10−2 ] × 315µ0 az = −6.30µ0ay = −7.92 × 10−6 ay N−m b) at the center of the loop: Use T = IS × B where S = (2 × 3) × 10−4 az m2. So T = 30(6 × 10−4 az) × (−350µ0 ax) = −7.92 × 10−6 ay N−m 9.15. A solid conducting filament extends from x = −b to x = b along the line y = 2, z = 0. This filament carries a current of 3 A in the ax direction. An infinite filament on the z axis carries 5 A in the az direction. Obtain an expression for the torque exerted on the finite conductor about an origin located at (0, 2, 0): The differential force on the wire segment arising from the field from the infinite wire is dF = 3 dx ax × 5µ0 2πρ aφ = − 15µ0 cos φ dx 2π √ x2 + 4 az = − 15µ0x dx 2π(x2 + 4) az So now the differential torque about the (0, 2, 0) origin is dT = RT × dF = x ax × − 15µ0x dx 2π(x2 + 4) az = 15µ0x2 dx 2π(x2 + 4) ay The torque is then T = b −b 15µ0x2 dx 2π(x2 + 4) ay = 15µ0 2π ay x − 2 tan−1 x 2 b −b = (6 × 10−6 ) b − 2 tan−1 b 2 ay N · m 9.16. Assume that an electron is describing a circular orbit of radius a about a positively-charged nucleus. a) By selecting an appropriate current and area, show that the equivalent orbital dipole moment is ea2ω/2, where ω is the electron’s angular velocity: The current magnitude will be I = e T , where e is the electron charge and T is the orbital period. The latter is T = 2π/ω, and so I = eω/(2π). Now the dipole moment magnitude will be m = IA, where A is the loop area. Thus m = eω 2π πa2 = 1 2 ea2 ω // b) Show that the torque produced by a magnetic field parallel to the plane of the orbit is ea2ωB/2: With B assumed constant over the loop area, we would have T = m × B. With B parallel to the loop plane, m and B are orthogonal, and so T = mB. So, using part a, T = ea2ωB/2. 150 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 153. 9.16. (continued) c) by equating the Coulomb and centrifugal forces, show that ω is (4πǫ0mea3/e2)−1/2, where me is the electron mass: The force balance is written as e2 4πǫ0a2 = me ω2 a ⇒ ω = 4πǫ0mea3 e2 −1/2 // d) Find values for the angular velocity, torque, and the orbital magnetic moment for a hydrogen atom, where a is about 6 × 10−11 m; let B = 0.5 T: First ω = (1.60 × 10−19)2 4π(8.85 × 10−12)(9.1 × 10−31)(6 × 10−11)3 1/2 = 3.42 × 1016 rad/s T = 1 2 (3.42 × 1016 )(1.60 × 10−19 )(0.5)(6 × 10−11 )2 = 4.93 × 10−24 N · m Finally, m = T B = 9.86 × 10−24 A · m2 9.17. The hydrogen atom described in Problem 16 is now subjected to a magnetic field having the same direction as that of the atom. Show that the forces caused by B result in a decrease of the angular velocity by eB/(2me) and a decrease in the orbital moment by e2a2B/(4me). What are these decreases for the hydrogen atom in parts per million for an external magnetic flux density of 0.5 T? We first write down all forces on the electron, in which we equate its coulomb force toward the nucleus to the sum of the centrifugal force and the force associated with the applied B field. With the field applied in the same direction as that of the atom, this would yield a Lorentz force that is radially outward – in the same direction as the centrifugal force. Fe = Fcent + FB ⇒ e2 4πǫ0a2 = meω2 a + eωaB QvB With B = 0, we solve for ω to find: ω = ω0 = e2 4πǫ0mea3 Then with B present, we find ω2 = e2 4πǫ0mea3 − eωB me = ω2 0 − eωB me Therefore ω = ω0 1 − eωB ω2 0me . = ω0 1 − eωB 2ω2 0me But ω . = ω0, and so ω . = ω0 1 − eB 2ω0me = ω0 − eB 2me // 151 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 154. 9.17. (continued) As for the magnetic moment, we have m = IS = eω 2π πa2 = 1 2 ωea2 . = 1 2 ea2 ω0 − eB 2me = 1 2 ω0ea2 − 1 4 e2a2B me // Finally, for a = 6 × 10−11 m, B = 0.5 T, we have ω ω = eB 2me 1 ω . = eB 2me 1 ω0 = 1.60 × 10−19 × 0.5 2 × 9.1 × 10−31 × 3.4 × 1016 = 1.3 × 10−6 where ω0 = 3.4 × 1016 sec−1 is found from Problem 16. Finally, m m = e2a2B 4me × 2 ωea2 . = eB 2meω0 = 1.3 × 10−6 9.18. Calculate the vector torque on the square loop shown in Fig. 9.16 about an origin at A in the field B, given: a) A(0, 0, 0) and B = 100ay mT: The field is uniform and so does not produce any translation of the loop. Therefore, we may use T = IS × B about any origin, where I = 0.6 A and S = 16az m2. We find T = 0.6(16)az × 0.100ay = −0.96 ax N−m. b) A(0, 0, 0) and B = 200ax + 100ay mT: Using the same reasoning as in part a, we find T = 0.6(16)az × (0.200ax + 0.100ay) = −0.96ax + 1.92ay N−m c) A(1, 2, 3) and B = 200ax +100ay −300az mT: We observe two things here: 1) The field is again uniform and so again the torque is independent of the origin chosen, and 2) The field differs from that of part b only by the addition of a z component. With S in the z direction, this new component of B will produce no torque, so the answer is the same as part b, or T = −0.96ax + 1.92ay N−m. d) A(1, 2, 3) and B = 200ax + 100ay − 300az mT for x ≥ 2 and B = 0 elsewhere: Now, force is acting only on the y-directed segment at x = +2, so we need to be careful, since translation will occur. So we must use the given origin. The differential torque acting on the differential wire segment at location (2,y) is dT = R(y) × dF, where dF = IdL × B = 0.6 dy ay × [0.2ax + 0.1ay − 0.3az] = [−0.18ax − 0.12az] dy and R(y) = (2, y, 0) − (1, 2, 3) = ax + (y − 2)ay − 3az. We thus find dT = R(y) × dF = ax + (y − 2)ay − 3az × [−0.18ax − 0.12az] dy = −0.12(y − 2)ax + 0.66ay + 0.18(y − 2)az dy The net torque is now T = 2 −2 −0.12(y − 2)ax + 0.66ay + 0.18(y − 2)az dy = 0.96ax + 2.64ay − 1.44az N−m 152 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 155. 9.19. Given a material for which χm = 3.1 and within which B = 0.4yaz T, find: a) H: We use B = µ0(1 + χm)H, or H = 0.4yay (1 + 3.1)µ0 = 77.6yaz kA/m b) µ = (1 + 3.1)µ0 = 5.15 × 10−6 H/m. c) µR = (1 + 3.1) = 4.1. d) M = χmH = (3.1)(77.6yay) = 241yaz kA/m e) J = ∇ × H = (dHz)/(dy) ax = 77.6 ax kA/m2. f) Jb = ∇ × M = (dMz)/(dy) ax = 241 ax kA/m2. g) JT = ∇ × B/µ0 = 318ax kA/m2. 9.20. Find H in a material where: a) µR = 4.2, there are 2.7 × 1029 atoms/m3, and each atom has a dipole moment of 2.6 × 10−30 ay A · m2. Since all dipoles are identical, we may write M = Nm = (2.7×1029)(2.6×10−30ay) = 0.70ay A/m. Then H = M µR − 1 = 0.70 ay 4.2 − 1 = 0.22 ay A/m b) M = 270 az A/m and µ = 2 µH/m: Have µR = µ/µ0 = (2 × 10−6)/(4π × 10−7) = 1.59. Then H = 270az/(1.59 − 1) = 456 az A/m. c) χm = 0.7 and B = 2az T: Use H = B µ0(1 + χm) = 2az (4π × 10−7)(1.7) = 936 az kA/m d) Find M in a material where bound surface current densities of 12 az A/m and −9 az A/m exist at ρ = 0.3 m and ρ = 0.4 m, respectively: We use M · dL = Ib, where, since currents are in the z direction and are symmetric about the z axis, we chose the path integrals to be circular loops centered on and normal to z. From the symmetry, M will be φ-directed and will vary only with radius. Note first that for ρ < 0.3 m, no bound current will be enclosed by a path integral, so we conclude that M = 0 for ρ < 0.3m. At radii between the currents the path integral will enclose only the inner current so, M · dL = 2πρMφ = 2π(0.3)12 ⇒ M = 3.6 ρ aφ A/m (0.3 < ρ < 0.4m) Finally, for ρ > 0.4 m, the total enclosed bound current is Ib,tot = 2π(0.3)(12)−2π(0.4)(9) = 0, so therefore M = 0 (ρ > 0.4m). 9.21. Find the magnitude of the magnetization in a material for which: a) the magnetic flux density is 0.02 Wb/m2 and the magnetic susceptibility is 0.003 (note that this latter quantity is missing in the original problem statement): From B = µ0(H + M) and from M = χmH, we write M = B µ0 1 χm + 1 −1 = B µ0(334) = 0.02 (4π × 10−7)(334) = 47.7 A/m 153 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 156. 9.21b) the magnetic field intensity is 1200A/m and the relative permeability is 1.005: From B = µ0(H+M) = µ0µRH, we write M = (µR − 1)H = (.005)(1200) = 6.0 A/m c) there are 7.2 × 1028 atoms per cubic meter, each having a dipole moment of 4 × 10−30 A · m2 in the same direction, and the magnetic susceptibility is 0.0003: With all dipoles identical the dipole moment density becomes M = n m = (7.2 × 1028 )(4 × 10−30 ) = 0.288 A/m 9.22. Three current sheets are located as follows: 160az A/m at x = 1cm, −40az A/m at x = 5cm, and 50az A/m at x = 8cm. Let µ = µ0 for x < 1cm and x > 8cm; for 1 < x < 5 cm, µ = 3µ0, and for 5 < x < 8cm, µ = 2µ0. Find B everywhere: We know that the H field from an infinite current sheet will be given in magnitude by H = K/2, and will be directed parallel to the sheet and perpendicular to the current, with the directions on either side of the sheet determined by the right hand rule. With this in mind, we can construct the following expressions for the B field in all four regions: B(x < 1) = 1 2 µ0(−160 + 40 − 50) = −1.07 × 10−4 ay T B(1 < x < 5) = 1 2 (3µ0)(160 + 40 − 50) = 2.83 × 10−4 ay T B(5 < x < 8) = 1 2 (2µ0)(160 − 40 − 50) = 8.80 × 10−5 ay T B(x > 8) = 1 2 µ0(160 − 40 + 50) = 1.07 × 10−4 ay T 9.23. Calculate values for Hφ, Bφ, and Mφ at ρ = c for a coaxial cable with a = 2.5 mm and b = 6 mm if it carries current I = 12 A in the center conductor, and µ = 3 µH/m for 2.5 < ρ < 3.5 mm, µ = 5 µH/m for 3.5 < ρ < 4.5 mm, and µ = 10 µH/m for 4.5 < ρ < 6 mm. Compute for: a) c = 3 mm: Have Hφ = I 2πρ = 12 2π(3 × 10−3) = 637 A/m Then Bφ = µHφ = (3 × 10−6)(637) = 1.91 × 10−3 Wb/m2. Finally, Mφ = (1/µ0)Bφ − Hφ = 884 A/m. b) c = 4 mm: Have Hφ = I 2πρ = 12 2π(4 × 10−3) = 478 A/m Then Bφ = µHφ = (5 × 10−6)(478) = 2.39 × 10−3 Wb/m2. Finally, Mφ = (1/µ0)Bφ − Hφ = 1.42 × 103 A/m. c) c = 5 mm: Have Hφ = I 2πρ = 12 2π(5 × 10−3) = 382 A/m Then Bφ = µHφ = (10 × 10−6)(382) = 3.82 × 10−3 Wb/m2. Finally, Mφ = (1/µ0)Bφ − Hφ = 2.66 × 103 A/m. 154 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 157. 9.24. A coaxial transmission line has a = 5 mm and b = 20 mm. Let its center lie on the z axis and let a dc current I flow in the az direction in the center conductor. The volume between the conductors contains a magnetic material for which µR = 2.5, as well as air. Find H, B, and M everywhere between conductors if Hφ = 600/π A/m at ρ = 10 mm, φ = π/2, and the magnetic material is located where: a) a < ρ < 3a; First, we know that Hφ = I/2πρ, from which we construct: I 2π(10−2) = 600 π ⇒ I = 12 A Since the interface between the two media lies in the aφ direction, we use the boundary condition of continuity of tangential H and write H(5 < ρ < 20) = 12 2πρ aφ = 6 πρ aφ A/m In the magnetic material, we find B(5 < ρ < 15) = µH = (2.5)(4π × 10−7)(12) 2πρ aφ = (6/ρ)aφ µT Then, in the free space region, B(15 < ρ < 20) = µ0H = (2.4/ρ)aφ µT. b) 0 < φ < π; Again, we are given H = 600/π aφ A/m at ρ = 10 and at φ = π/2. Now, since the interface between media lies in the aρ direction, and noting that magnetic field will be normal to this (aφ directed), we use the boundary condition of continuity of B normal to an interface, and write B(0 < φ < π) = B1 = B(π < φ < 2π) = B2, or 2.5µ0H1 = µ0H2. Now, using Ampere’s circuital law, we write H · dL = πρH1 + πρH2 = 3.5πρH1 = I Using the given value for H1 at ρ = 10 mm, I = 3.5(600/π)(π × 10−2) = 21 A. Therefore, H1 = 21/(3.5πρ) = 6/(πρ), or H(0 < φ < π) = 6/(πρ) aφ A/m. Then H2 = 2.5H1, or H(π < φ < 2π) = 15/(πρ) aφ A/m. Now B(0 < φ < 2π) = 2.5µ0(6/(πρ))aφ = 6/ρ aφ µT. Now, in general, M = (µR−1)H, and so M(0 < φ < π) = (2.5−1)6/(πρ)aφ = 9/(πρ) aφ A/m and M(π < φ < 2π) = 0. 9.25. A conducting filament at z = 0 carries 12 A in the az direction. Let µR = 1 for ρ < 1 cm, µR = 6 for 1 < ρ < 2 cm, and µR = 1 for ρ > 2 cm. Find a) H everywhere: This result will depend on the current and not the materials, and is: H = I 2πρ aφ = 1.91 ρ A/m (0 < ρ < ∞) b) B everywhere: We use B = µRµ0H to find: B(ρ < 1 cm) = (1)µ0(1.91/ρ) = (2.4 × 10−6/ρ)aφ T B(1 < ρ < 2 cm) = (6)µ0(1.91/ρ) = (1.4 × 10−5/ρ)aφ T B(ρ > 2 cm) = (1)µ0(1.91/ρ) = (2.4 × 10−6/ρ)aφ T where ρ is in meters. 155 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 158. 9.26. Point P (2, 3, 1) lies on the planar boundary boundary separating region 1 from region 2. The unit vector aN12 = 0.6ax +0.48ay +0.64az is directed from region 1 to region 2. Let µR1 = 2, µR2 = 8, and H1 = 100ax − 300ay + 200az A/m. Find H2: First B1 = 200µ0ax − 600µ0ay + 400µ0az. Then its normal component at the boundary will be B1N = (B1 ·aN12)aN12 = (52.8ax +42.24ay +56.32az)µ0 = B2N . Then H2N = B2N /(8µ0) = 6.60ax +5.28ay +7.04az, and H1N = B1N /2µ0 = 26.40ax +21.12ay + 28.16az. Now H1T = H1 − H1N = (100ax − 300ay + 200az) − (26.40ax + 21.12ay + 28.16az) = 73.60ax − 321.12ay + 171.84az = H2T . Finally, H2 = H2N + H2T = 80.2ax − 315.8ay + 178.9az A/m. 9.27. Let µR1 = 2 in region 1, defined by 2x+3y−4z > 1, while µR2 = 5 in region 2 where 2x+3y−4z < 1. In region 1, H1 = 50ax − 30ay + 20az A/m. Find: a) HN1 (normal component of H1 at the boundary): We first need a unit vector normal to the surface, found through aN = ∇ (2x + 3y − 4z) |∇ (2x + 3y − 4z)| = 2ax + 3ay − 4az √ 29 = .37ax + .56ay − .74az Since this vector is found through the gradient, it will point in the direction of increasing values of 2x + 3y − 4z, and so will be directed into region 1. Thus we write aN = aN21. The normal component of H1 will now be: HN1 = (H1 · aN21)aN21 = (50ax − 30ay + 20az) · (.37ax + .56ay − .74az) (.37ax + .56ay − .74az) = −4.83ax − 7.24ay + 9.66az A/m b) HT 1 (tangential component of H1 at the boundary): HT 1 = H1 − HN1 = (50ax − 30ay + 20az) − (−4.83ax − 7.24ay + 9.66az) = 54.83ax − 22.76ay + 10.34az A/m c) HT 2 (tangential component of H2 at the boundary): Since tangential components of H are con- tinuous across a boundary between two media of different permeabilities, we have HT 2 = HT 1 = 54.83ax − 22.76ay + 10.34az A/m d) HN2 (normal component of H2 at the boundary): Since normal components of B are continuous across a boundary between media of different permeabilities, we write µ1HN1 = µ2HN2 or HN2 = µR1 µR2 HN1 = 2 5 (−4.83ax − 7.24ay + 9.66az) = −1.93ax − 2.90ay + 3.86az A/m e) θ1, the angle between H1 and aN21: This will be cos θ1 = H1 |H1| · aN21 = 50ax − 30ay + 20az (502 + 302 + 202)1/2 · (.37ax + .56ay − .74az) = −0.21 Therefore θ1 = cos−1(−.21) = 102◦. 156 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 159. 9.27f) θ2, the angle between H2 and aN21: First, H2 = HT 2 + HN2 = (54.83ax − 22.76ay + 10.34az) + (−1.93ax − 2.90ay + 3.86az) = 52.90ax − 25.66ay + 14.20az A/m Now cos θ2 = H2 |H2| · aN21 = 52.90ax − 25.66ay + 14.20az 60.49 · (.37ax + .56ay − .74az) = −0.09 Therefore θ2 = cos−1(−.09) = 95◦. 9.28. For values of B below the knee on the magnetization curve for silicon steel, approximate the curve by a straight line with µ = 5 mH/m. The core shown in Fig. 9.17 has areas of 1.6 cm2 and lengths of 10 cm in each outer leg, and an area of 2.5 cm2 and a length of 3 cm in the central leg. A coil of 1200 turns carrying 12 mA is placed around the central leg. Find B in the: a) center leg: We use mmf = R, where, in the central leg, Rc = Lin µAin = 3 × 10−2 (5 × 10−3)(2.5 × 10−4) = 2.4 × 104 H In each outer leg, the reluctance is Ro = Lout µAout = 10 × 10−2 (5 × 10−3)(1.6 × 10−4) = 1.25 × 105 H The magnetic circuit is formed by the center leg in series with the parallel combination of the two outer legs. The total reluctance seen at the coil location is RT = Rc + (1/2)Ro = 8.65 × 104 H. We now have = mmf RT = 14.4 8.65 × 104 = 1.66 × 10−4 Wb The flux density in the center leg is now B = A = 1.66 × 10−4 2.5 × 10−4 = 0.666 T b) center leg, if a 0.3-mm air gap is present in the center leg: The air gap reluctance adds to the total reluctance already calculated, where Rair = 0.3 × 10−3 (4π × 10−7)(2.5 × 10−4) = 9.55 × 105 H Now the total reluctance is Rnet = RT + Rair = 8.56 × 104 + 9.55 × 105 = 1.04 × 106. The flux in the center leg is now = 14.4 1.04 × 106 = 1.38 × 10−5 Wb and B = 1.38 × 10−5 2.5 × 10−4 = 55.3 mT 157 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 160. 9.29. In Problem 9.28, the linear approximation suggested in the statement of the problem leads to a flux density of 0.666 T in the center leg. Using this value of B and the magnetization curve for silicon steel, what current is required in the 1200-turn coil? With B = 0.666 T, we read Hin . = 120 A · t/m in Fig. 9.11. The flux in the center leg is = 0.666(2.5 × 10−4) = 1.66 × 10−4 Wb. This divides equally in the two outer legs, so that the flux density in each outer leg is Bout = 1 2 1.66 × 10−4 1.6 × 10−4 = 0.52 Wb/m2 Using Fig. 9.11 with this result, we find Hout . = 90 A · t/m We now use H · dL = NI to find I = 1 N (HinLin + Hout Lout ) = (120)(3 × 10−2) + (90)(10 × 10−2) 1200 = 10.5 mA 9.30. A toroidal core has a circular cross section of 4 cm2 area. The mean radius of the toroid is 6 cm. The core is composed of two semi-circular segments, one of silicon steel and the other of a linear material with µR = 200. There is a 4mm air gap at each of the two joints, and the core is wrapped by a 4000-turn coil carrying a dc current I1. a) Find I1 if the flux density in the core is 1.2 T: I will use the reluctance method here. Reluctances of the steel and linear materials are respectively, Rs = π(6 × 10−2) (3.0 × 10−3)(4 × 10−4) = 1.57 × 105 H−1 Rl = π(6 × 10−2) (200)(4π × 10−7)(4 × 10−4) = 1.88 × 106 H−1 whereµs isfoundfromFig. 9.11, usingB = 1.2, fromwhichH = 400, andsoB/H = 3.0mH/m. The reluctance of each gap is now Rg = 0.4 × 10−3 (4π × 10−7)(4 × 10−4) = 7.96 × 105 H−1 We now construct NI1 = R = 1.2(4 × 10−4 ) Rs + Rl + 2Rg = 1.74 × 103 Thus I1 = (1.74 × 103)/4000 = 435 mA. 158 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 161. 9.30b. Find the flux density in the core if I1 = 0.3 A: We are not sure what to use for the permittivity of steel in this case, so we use the iterative approach. Since the current is down from the value obtained in part a, we can try B = 1.0 T and see what happens. From Fig. 9.11, we find H = 200 A/m. Then, in the linear material, Hl = 1.0 200(4π × 10−7) = 3.98 × 103 A/m and in each gap, Hg = 1.0 4π × 10−7 = 7.96 × 105 A/m Now Ampere’s circuital law around the toroid becomes NI1 = π(.06)(200 + 3.98 × 103 ) + 2(7.96 × 105 )(4 × 10−4 ) = 1.42 × 103 A−t Then I1 = (1.42 × 103)/4000 = .356 A. This is still larger than the given value of .3A, so we can extrapolate down to find a better value for B: B = 1.0 − (1.2 − 1.0) .356 − .300 .435 − .356 = 0.86 T Using this value in the procedure above to evaluate Ampere’s circuital law leads to a value of I1 of 0.306 A. The result of 0.86 T for B is probably good enough for this problem, considering the limited resolution of Fig. 9.11. 9.31. A toroid is constructed of a magnetic material having a cross-sectional area of 2.5 cm2 and an effective length of 8 cm. There is also a short air gap 0.25 mm length and an effective area of 2.8 cm2. An mmf of 200 A · t is applied to the magnetic circuit. Calculate the total flux in the toroid if: a) the magnetic material is assumed to have infinite permeability: In this case the core reluctance, Rc = l/(µA), is zero, leaving only the gap reluctance. This is Rg = d µ0Ag = 0.25 × 10−3 (4π × 10−7)(2.5 × 10−4) = 7.1 × 105 H Now = mmf ¨g = 200 7.1 × 105 = 2.8 × 10−4 Wb b) the magnetic material is assumed to be linear with µR = 1000: Now the core reluctance is no longer zero, but Rc = 8 × 10−2 (1000)(4π × 10−7)(2.5 × 10−4) = 2.6 × 105 H The flux is then = mmf Rc + Rg = 200 9.7 × 105 = 2.1 × 10−4 Wb c) the magnetic material is silicon steel: In this case we use the magnetization curve, Fig. 9.11, and employ an iterative process to arrive at the final answer. We can begin with the value of found in part a, assuming infinite permeability: (1) = 2.8 × 10−4 Wb. The flux density in the core is then B (1) c = (2.8 × 10−4)/(2.5 × 10−4) = 1.1 Wb/m2. From Fig. 9.11, this corresponds to 159 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 162. magnetic field strength H (1) c . = 270 A/m. We check this by applying Ampere’s circuital law to the magnetic circuit: H · dL = H(1) c Lc + H(1) g d where H (1) c Lc = (270)(8×10−2) = 22, and where H (1) g d = (1)¨g = (2.8×10−4)(7.1×105) = 199. But we require that H · dL = 200 A · t whereas the actual result in this first calculation is 199 + 22 = 221, which is too high. So, for a second trial, we reduce B to B (2) c = 1 Wb/m2. This yields H (2) c = 200 A/m from Fig. 9.11, and thus (2) = 2.5 × 10−4 Wb. Now H · dL = H(2) c Lc + (2) Rg = 200(8 × 10−2 ) + (2.5 × 10−4 )(7.1 × 105 ) = 194 This is less than 200, meaning that the actual flux is slightly higher than 2.5 × 10−4 Wb. I will leave the answer at that, considering the lack of fine resolution in Fig. 9.11. 9.32. Determine the total energy stored in a spherical region 1cm in radius, centered at the origin in free space, in the uniform field: a) H1 = −600ay A/m: First we find the energy density: wm1 = 1 2 B1 · H1 = 1 2 µ0H2 1 = 1 2 (4π × 10−7 )(600)2 = 0.226 J/m3 The energy within the sphere is then Wm1 = wm1 4 3 πa3 = 0.226 4 3 π × 10−6 = 0.947 µJ b) H2 = 600ax + 1200ay A/m: In this case the energy density is wm2 = 1 2 µ0 (600)2 + (1200)2 = 5 2 µ0(600)2 or five times the energy density that was found in part a. Therefore, the stored energy in this field is five times the amount in part a, or Wm2 = 4.74 µJ. c) H3 = −600ax + 1200ay. This field differs from H2 only by the negative x component, which is a non-issue since the component is squared when finding the energy density. Therefore, the stored energy will be the same as that in part b, or Wm3 = 4.74 µJ. d) H4 = H2 + H3, or 2400ay A/m: The energy density is now wm4 = (1/2)µ0(2400)2 = (1/2)µ0(16)(600)2 J/m3, which is sixteen times the energy density in part a. The stored en- ergy is therefore sixteen times that result, or Wm4 = 16(0.947) = 15.2 µJ. e) 1000ax A/m+0.001ax T: The energy density is wm5 = (1/2)µ0[1000+.001/µ0]2 = 2.03 J/m3. Then Wm5 = 2.03[(4/3)π × 10−6] = 8.49 µJ. 160 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 163. 9.33. A toroidal core has a square cross section, 2.5 cm < ρ < 3.5 cm, −0.5 cm < z < 0.5 cm. The upper half of the toroid, 0 < z < 0.5 cm, is constructed of a linear material for which µR = 10, while the lower half, −0.5 cm < z < 0, has µR = 20. An mmf of 150 A · t establishes a flux in the aφ direction. For z > 0, find: a) Hφ(ρ): Ampere’s circuital law gives: 2πρHφ = NI = 150 ⇒ Hφ = 150 2πρ = 23.9/ρ A/m b) Bφ(ρ): We use Bφ = µRµ0Hφ = (10)(4π × 10−7)(23.9/ρ) = 3.0 × 10−4/ρ Wb/m2. c) z>0: This will be z>0 = B · dS = .005 0 .035 .025 3.0 × 10−4 ρ dρdz = (.005)(3.0 × 10−4 ) ln .035 .025 = 5.0 × 10−7 Wb d) Repeat for z < 0: First, the magnetic field strength will be the same as in part a, since the calculation is material-independent. Thus Hφ = 23.9/ρ A/m. Next, Bφ is modified only by the new permeability, which is twice the value used in part a: Thus Bφ = 6.0 × 10−4/ρ Wb/m2. Finally, since Bφ is twice that of part a, the flux will be increased by the same factor, since the area of integration for z < 0 is the same. Thus z<0 = 1.0 × 10−6 Wb. e) Find total: This will be the sum of the values found for z < 0 and z > 0, or total = 1.5 × 10−6 Wb. 9.34. Three planar current sheets are located in free space as follows: −100ax A/m2 at z = −1, 200ax A/m2 at z = 0, −100ax A/m2 at z = 1. Let wH = (1/2)B · H J/m3, and find wH for all z: Using the fact that the field on either side of a current sheet is given in magnitude by H = K/2, we find, in A/m: H(z > 1) = (1/2)(−200 + 100 + 100)ay = 0 H(0 < z < 1) = (1/2)(−200 − 100 + 100)ay = −100ay H(−1 < z < 0) = (1/2)(200 − 100 + 100)ay = 100ay and H(z < −1) = (1/2)(200 − 100 − 100)ay = 0 The energy densities are then wH (z > 1) = wH (z < −1) = 0 wH (0 < z < 1) = wH (−1 < z < 0) = (1/2)µ0(100)2 = 6.28 mJ/m2 161 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 164. 9.35. The cones θ = 21◦ and θ = 159◦ are conducting surfaces and carry total currents of 40 A, as shown in Fig. 9.18. The currents return on a spherical conducting surface of 0.25 m radius. a) Find H in the region 0 < r < 0.25, 21◦ < θ < 159◦, 0 < φ < 2π: We can apply Ampere’s circuital law and take advantage of symmetry. We expect to see H in the aφ direction and it would be constant at a given distance from the z axis. We thus perform the line integral of H over a circle, centered on the z axis, and parallel to the xy plane: H · dL = 2π 0 Hφaφ · r sin θaφ dφ = Iencl. = 40 A Assuming that Hφ is constant over the integration path, we take it outside the integral and solve: Hφ = 40 2πr sin θ ⇒ H = 20 πr sin θ aφ A/m b) How much energy is stored in this region? This will be WH = v 1 2 µ0H2 φ = 2π 0 159◦ 21◦ .25 0 200µ0 π2r2 sin2 θ r2 sin θ dr dθ dφ = 100µ0 π 159◦ 21◦ dθ sin θ = 100µ0 π ln tan(159/2) tan(21/2) = 1.35 × 10−4 J 9.36. A filament carrying current I in the az direction lies on the z axis, and cylindrical current sheets of 5az A/m and −2az A/m are located at ρ = 3 and ρ = 10, respectively. a) Find I if H = 0 for ρ > 10. Ampere’s circuital law says, for ρ > 10: 2πρH = 2π(3)(5) − 2π(10)(2) + I = 0 from which I = 2π(10)(3) − 2π(3)(5) = 10π A. b) Using this value of I, calculate H for all ρ, 3 < ρ < 10: Again, using Ampere’s circuital law, we find H(3 < ρ < 10) = 1 2πρ [10π + 2π(3)(5)] aφ = 20 ρ aφ A/m c) Calculate and plot WH versus ρ0, where WH is the total energy stored within the volume 0 < z < 1, 0 < φ < 2π, 3 < ρ < ρ0: First the energy density will be wH = (1/2)µ0H2 = 200µ0/ρ2 J/m3. Then the energy is WH = 1 0 2π 0 ρ0 3 200µ0 ρ2 ρ dρ dφ dz = 400πµ0 ln ρ0 3 = (1.58 × 10−3 ) ln ρ0 3 J 162 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 165. 9.36c. (continued) A plot of the energy as a function of ρ0 is shown below. 9.37. Find the inductance of the cone-sphere configuration described in Problem 9.35 and Fig. 9.18. The inductance is that offered at the origin between the vertices of the cone: From Problem 9.35, the magnetic flux density is Bφ = 20µ0/(πr sin θ). We integrate this over the crossectional area defined by 0 < r < 0.25 and 21◦ < θ < 159◦, to find the total flux: = 159◦ 21◦ 0.25 0 20µ0 πr sin θ r dr dθ = 5µ0 π ln tan(159/2) tan(21/2) = 5µ0 π (3.37) = 6.74 × 10−6 Wb Now L = /I = 6.74 × 10−6/40 = 0.17 µH. Second method: Use the energy computation of Problem 9.35, and write L = 2WH I2 = 2(1.35 × 10−4) (40)2 = 0.17 µH 9.38. A toroidal core has a rectangular cross section defined by the surfaces ρ = 2 cm, ρ = 3 cm, z = 4 cm, and z = 4.5 cm. The core material has a relative permeability of 80. If the core is wound with a coil containing 8000 turns of wire, find its inductance: First we apply Ampere’s circuital law to a circular loop of radius ρ in the interior of the toroid, and in the aφ direction. H · dL = 2πρHφ = NI ⇒ Hφ = NI 2πρ The flux in the toroid is then the integral over the cross section of B: = B · dL = .045 .04 .03 .02 µRµ0NI 2πρ dρ dz = (.005) µRµ0NI 2π ln .03 .02 The flux linkage is then given by N , and the inductance is L = N I = (.005)(80)(4π × 10−7)(8000)2 2π ln(1.5) = 2.08 H 163 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 166. 9.39. Conducting planes in air at z = 0 and z = d carry surface currents of ±K0ax A/m. a) Find the energy stored in the magnetic field per unit length (0 < x < 1) in a width w (0 < y < w): First, assuming current flows in the +ax direction in the sheet at z = d, and in −ax in the sheet at z = 0, we find that both currents together yield H = K0ay for 0 < z < d and zero elsewhere. The stored energy within the specified volume will be: WH = v 1 2 µ0H2 dv = d 0 w 0 1 0 1 2 µ0K2 0 dx dy dz = 1 2 wdµ0K2 0 J/m b) Calculate the inductance per unit length of this transmission line from WH = (1/2)LI2, where I is the total current in a width w in either conductor: We have I = wK0, and so L = 2 I2 wd 2 µ0K2 0 = 2 w2K2 0 dw 2 µ0K2 0 = µ0d w H/m c) Calculate the total flux passing through the rectangle 0 < x < 1, 0 < z < d, in the plane y = 0, and from this result again find the inductance per unit length: = d 0 1 0 µ0Hay · ay dx dz = d 0 1 0 µ0K0dx dy = µ0dK0 Then L = I = µ0dK0 wK0 = µ0d w H/m 9.40. A coaxial cable has conductor dimensions of 1 and 5 mm. The region between conductors is air for 0 < φ < π/2 and π < φ < 3π/2, and a non-conducting material having µR = 8 for π/2 < φ < π and 3π/2 < φ < 2π. Find the inductance per meter length: The interfaces between media all occur along radial lines, normal to the direction of B and H in the coax line. B is therefore continuous (and constant at constant radius) around a circular loop centered on the z axis. Ampere’s circuital law can thus be written in this form: H · dL = B µ0 π 2 ρ + B µRµ0 π 2 ρ + B µ0 π 2 ρ + B µRµ0 π 2 ρ = πρB µRµ0 (µR + 1) = I and so B = µRµ0I πρ(1 + µR) aφ The flux in the line per meter length in z is now = 1 0 .005 .001 µRµ0I πρ(1 + µR) dρ dz = µRµ0I π(1 + µR) ln(5) And the inductance per unit length is: L = I = µRµ0 π(1 + µR) ln(5) = 8(4π × 10−7) π(9) ln(5) = 572 nH/m 164 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 167. 9.41. A rectangular coil is composed of 150 turns of a filamentary conductor. Find the mutual inductance in free space between this coil and an infinite straight filament on the z axis if the four corners of the coil are located at a) (0,1,0), (0,3,0), (0,3,1), and (0,1,1): In this case the coil lies in the yz plane. If we assume that the filament current is in the +az direction, then the B field from the filament penetrates the coil in the −ax direction (normal to the loop plane). The flux through the loop will thus be = 1 0 3 1 −µ0I 2πy ax · (−ax) dy dz = µ0I 2π ln 3 The mutual inductance is then M = N I = 150µ0 2π ln 3 = 33 µH b) (1,1,0), (1,3,0), (1,3,1), and (1,1,1): Now the coil lies in the x = 1 plane, and the field from the filament penetrates in a direction that is not normal to the plane of the coil. We write the B field from the filament at the coil location as B = µ0Iaφ 2π y2 + 1 The flux through the coil is now = 1 0 3 1 µ0Iaφ 2π y2 + 1 · (−ax) dy dz = 1 0 3 1 µ0I sin φ 2π y2 + 1 dy dz = 1 0 3 1 µ0Iy 2π(y2 + 1) dy dz = µ0I 2π ln(y2 + 1) 3 1 = (1.6 × 10−7 )I The mutual inductance is then M = N I = (150)(1.6 × 10−7 ) = 24 µH 9.42. Find the mutual inductance of this conductor system in free space: a) the solenoid of Fig. 8.11b and a square filamentary loop of side length b coaxially centered inside the solenoid, if a > b/ √ 2; With the given side length, the loop lies entirely inside the solenoid, and so is linked over its entire cross section by the solenoid field. The latter is given by B = µ0NI/d az T. The flux through the loop area is now = Bb2, and the mutual inductance is M = /I = µ0Nb2/d H. b) a cylindrical conducting shell of a radius a, axis on the z axis, and a filament at x = 0, y = d, and where d > a (omitted from problem statement); The B field from the cylinder is B = (µ0I)/(2πρ) aφ for ρ > a, and so the flux per unit length between cylinder and wire is = 1 0 d a µ0I 2πρ dρ dz = µ0I 2π ln d a Wb Finally the mutual inductance is M = /I = µ0/2π ln(d/a) H. 165 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 168. 9.43. a) Use energy relationships to show that the internal inductance of a nonmagnetic cylindrical wire of radius a carrying a uniformly-distributed current I is µ0/(8π) H/m. We first find the magnetic field inside the conductor, then calculate the energy stored there. From Ampere’s circuital law: 2πρHφ = πρ2 πa2 I ⇒ Hφ = Iρ 2πa2 A/m Now WH = v 1 2 µ0H2 φ dv = 1 0 2π 0 a 0 µ0I2ρ2 8π2a4 ρ dρ dφ dz = µ0I2 16π J/m Now, with WH = (1/2)LI2, we find Lint = µ0/(8π) as expected. b) Find the internal inductance if the portion of the conductor for which ρ < c < a is removed: The hollowed-out conductor still carries current I, so Ampere’s circuital law now reads: 2πρHφ = π(ρ2 − c2) π(a2 − c2) ⇒ Hφ = I 2πρ ρ2 − c2 a2 − c2 A/m and the energy is now WH = 1 0 2π 0 a c µ0I2(ρ2 − c2)2 8π2ρ2(a2 − c2)2 ρ dρ dφ dz = µ0I2 4π(a2 − c2)2 a c ρ3 − 2c2 ρ + C4 ρ dρ = µ0I2 4π(a2 − c2)2 1 4 (a4 − c4 ) − c2 (a2 − c2 ) + c4 ln a c J/m The internal inductance is then Lint = 2WH I2 = µ0 8π a4 − 4a2c2 + 3c4 + 4c4 ln(a/c) (a2 − c2)2 H/m 166 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 169. CHAPTER 10 10.1. In Fig. 10.4, let B = 0.2 cos 120πt T, and assume that the conductor joining the two ends of the resistor is perfect. It may be assumed that the magnetic field produced by I(t) is negligible. Find: a) Vab(t): Since B is constant over the loop area, the flux is = π(0.15)2B = 1.41×10−2 cos 120πt Wb. Now, emf = Vba(t) = −d /dt = (120π)(1.41 × 10−2) sin 120πt. Then Vab(t) = −Vba(t) = −5.33 sin 120πt V. b) I(t) = Vba(t)/R = 5.33 sin(120πt)/250 = 21.3 sin(120πt) mA 10.2. Given the time-varying magnetic field, B = (0.5ax + 0.6ay − 0.3az) cos 5000t T, and a square fila- mentary loop with its corners at (2,3,0), (2,-3,0), (-2,3,0), and (-2,-3,0), find the time-varying current flowing in the general aφ direction if the total loop resistance is 400 k : We write emf = E · dL = − d dt = − d dt loop area B · az da = d dt (0.3)(4)(6) cos 5000t where the loop normal is chosen as positive az, so that the path integral for E is taken around the positive aφ direction. Taking the derivative, we find emf = −7.2(5000) sin 5000t so that I = emf R = −36000 sin 5000t 400 × 103 = −90 sin 5000t mA 10.3. Given H = 300 az cos(3 × 108t − y) A/m in free space, find the emf developed in the general aφ direction about the closed path having corners at a) (0,0,0), (1,0,0), (1,1,0), and (0,1,0): The magnetic flux will be: = 1 0 1 0 300µ0 cos(3 × 108 t − y) dx dy = 300µ0 sin(3 × 108 t − y)|1 0 = 300µ0 sin(3 × 108 t − 1) − sin(3 × 108 t) Wb Then emf = − d dt = −300(3 × 108 )(4π × 10−7 ) cos(3 × 108 t − 1) − cos(3 × 108 t) = −1.13 × 105 cos(3 × 108 t − 1) − cos(3 × 108 t) V b) corners at (0,0,0), (2π,0,0), (2π,2π,0), (0,2π,0): In this case, the flux is = 2π × 300µ0 sin(3 × 108 t − y)|2π 0 = 0 The emf is therefore 0. 167 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 170. 10.4. Conductor surfaces are located at ρ = 1cm and ρ = 2cm in free space. The volume 1 cm < ρ < 2 cm contains the fields Hφ = (2/ρ) cos(6×108πt −2πz) A/m and Eρ = (240π/ρ) cos(6×108πt −2πz) V/m. a) Show that these two fields satisfy Eq. (6), Sec. 10.1: Have ∇ × E = ∂Eρ ∂z aφ = 2π(240π) ρ sin(6 × 108 πt − 2πz) aφ = 480π2 ρ sin(6 × 108 πt − 2πz)aφ Then − ∂B ∂t = 2µ0(6 × 108)π ρ sin(6 × 108 πt − 2πz) aφ = (8π × 10−7)(6 × 108)π ρ sin(6 × 108 πt − 2πz) = 480π2 ρ sin(6 × 108 πt − 2πz) aφ b) Evaluate both integrals in Eq. (4) for the planar surface defined by φ = 0, 1cm < ρ < 2cm, 0 < z < 0.1m (note misprint in problem statement), and its perimeter, and show that the same results are obtained: we take the normal to the surface as positive aφ, so the the loop surrounding the surface (by the right hand rule) is in the negative aρ direction at z = 0, and is in the positive aρ direction at z = 0.1. Taking the left hand side first, we find E · dL = .01 .02 240π ρ cos(6 × 108 πt) aρ · aρ dρ + .02 .01 240π ρ cos(6 × 108 πt − 2π(0.1)) aρ · aρ dρ = 240π cos(6 × 108 πt) ln 1 2 + 240π cos(6 × 108 πt − 0.2π) ln 2 1 = 240(ln 2) cos(6 × 108 πt − 0.2π) − cos(6 × 108 πt) Now for the right hand side. First, B · dS = 0.1 0 .02 .01 8π × 10−7 ρ cos(6 × 108 πt − 2πz) aφ · aφ dρ dz = 0.1 0 (8π × 10−7 ) ln 2 cos(6 × 108 πt − 2πz) dz = −4 × 10−7 ln 2 sin(6 × 108 πt − 0.2π) − sin(6 × 108 πt) Then − d dt B · dS = 240π(ln 2) cos(6 × 108 πt − 0.2π) − cos(6 × 108 πt) (check) 10.5. The location of the sliding bar in Fig. 10.5 is given by x = 5t + 2t3, and the separation of the two rails is 20 cm. Let B = 0.8x2az T. Find the voltmeter reading at: a) t = 0.4 s: The flux through the loop will be = 0.2 0 x 0 0.8(x′ )2 dx′ dy = 0.16 3 x3 = 0.16 3 (5t + 2t3 )3 Wb 168 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 171. Then emf = − d dt = 0.16 3 (3)(5t +2t3 )2 (5+6t2 ) = −(0.16)[5(.4)+2(.4)3 ]2 [5+6(.4)2 ] = −4.32 V b) x = 0.6 m: Have 0.6 = 5t + 2t3, from which we find t = 0.1193. Thus emf = −(0.16)[5(.1193) + 2(.1193)3 ]2 [5 + 6(.1193)2 ] = −.293 V 10.6. A perfectly conducting filament containing a small 500- resistor is formed into a square, as illustrated in Fig. 10.6. Find I(t) if a) B = 0.3 cos(120πt −30◦) az T: First the flux through the loop is evaluated, where the unit normal to the loop is az. We find = loop B · dS = (0.3)(0.5)2 cos(120πt − 30◦ ) Wb Then the current will be I(t) = emf R = − 1 R d dt = (120π)(0.3)(0.25) 500 sin(120πt − 30◦ ) = 57 sin(120πt − 30◦ ) mA b) B = 0.4 cos[π(ct − y)] az µT where c = 3 × 108 m/s: Since the field varies with y, the flux is now = loop B · dS = (0.5)(0.4) .5 0 cos(πy − πct) dy = 0.2 π [sin(πct − π/2) − sin(πct)] µWb The current is then I(t) = emf R = − 1 R d dt = −0.2c 500 [cos(πct − π/2) − cos(πct)] µA = −0.2(3 × 108) 500 [sin(πct) − cos(πct)] µA = 120 [cos(πct) − sin(πct)] mA 10.7. The rails in Fig. 10.7 each have a resistance of 2.2 /m. The bar moves to the right at a constant speed of 9 m/s in a uniform magnetic field of 0.8 T. Find I(t), 0 < t < 1 s, if the bar is at x = 2 m at t = 0 and a) a 0.3 resistor is present across the left end with the right end open-circuited: The flux in the left-hand closed loop is l = B × area = (0.8)(0.2)(2 + 9t) Then, emfl = −d l/dt = −(0.16)(9) = −1.44 V. With the bar in motion, the loop resistance is increasing with time, and is given by Rl(t) = 0.3 + 2[2.2(2 + 9t)]. The current is now Il(t) = emfl Rl(t) = −1.44 9.1 + 39.6t A Note that the sign of the current indicates that it is flowing in the direction opposite that shown in the figure. 169 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 172. b) Repeat part a, but with a resistor of 0.3 across each end: In this case, there will be a contribution to the current from the right loop, which is now closed. The flux in the right loop, whose area decreases with time, is r = (0.8)(0.2)[(16 − 2) − 9t] and emfr = −d r/dt = (0.16)(9) = 1.44 V. The resistance of the right loop is Rr(t) = 0.3 + 2[2.2(14 − 9t)], and so the contribution to the current from the right loop will be Ir(t) = −1.44 61.9 − 39.6t A The minus sign has been inserted because again the current must flow in the opposite direction as that indicated in the figure, with the flux decreasing with time. The total current is found by adding the part a result, or IT (t) = −1.44 1 61.9 − 39.6t + 1 9.1 + 39.6t A 10.8. Fig. 10.1 is modified to show that the rail separation is larger when y is larger. Specifically, let the separation d = 0.2 + 0.02y. Given a uniform velocity vy = 8 m/s and a uniform magnetic flux density Bz = 1.1 T, find V12 as a function of time if the bar is located at y = 0 at t = 0: The flux through the loop as a function of y can be written as = B · dS = y 0 .2+.02y′ 0 1.1 dx dy′ = y 0 1.1(.2 + .02y′ ) dy′ = 0.22y(1 + .05y) Now, with y = vt = 8t, the above becomes = 1.76t(1 + .40t). Finally, V12 = − d dt = −1.76(1 + .80t) V 10.9. A square filamentary loop of wire is 25 cm on a side and has a resistance of 125 per meter length. The loop lies in the z = 0 plane with its corners at (0, 0, 0), (0.25, 0, 0), (0.25, 0.25, 0), and (0, 0.25, 0) at t = 0. The loop is moving with velocity vy = 50 m/s in the field Bz = 8 cos(1.5 × 108t − 0.5x) µT. Develop a function of time which expresses the ohmic power being delivered to the loop: First, since the field does not vary with y, the loop motion in the y direction does not produce any time-varying flux, and so this motion is immaterial. We can evaluate the flux at the original loop position to obtain: (t) = .25 0 .25 0 8 × 10−6 cos(1.5 × 108 t − 0.5x) dx dy = −(4 × 10−6 ) sin(1.5 × 108 t − 0.13x) − sin(1.5 × 108 t) Wb Now, emf = V (t) = −d /dt = 6.0 × 102 cos(1.5 × 108t − 0.13x) − cos(1.5 × 108t) , The total loop resistance is R = 125(0.25 + 0.25 + 0.25 + 0.25) = 125 . Then the ohmic power is P (t) = V 2(t) R = 2.9 × 103 cos(1.5 × 108 t − 0.13x) − cos(1.5 × 108 t) Watts 170 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 173. 10.10a. Show that the ratio of the amplitudes of the conduction current density and the displacement current density is σ/ωǫ for the applied field E = Em cos ωt. Assume µ = µ0. First, D = ǫE = ǫEm cos ωt. Then the displacement current density is ∂D/∂t = −ωǫEm sin ωt. Second, Jc = σE = σEm cos ωt. Using these results we find |Jc|/|Jd| = σ/ωǫ. b. What is the amplitude ratio if the applied field is E = Eme−t/τ , where τ is real? As before, find D = ǫE = ǫEme−t/τ , and so Jd = ∂D/∂t = −(ǫ/τ)Eme−t/τ . Also, Jc = σEme−t/τ . Finally, |Jc|/|Jd| = στ/ǫ. 10.11. Let the internal dimension of a coaxial capacitor be a = 1.2 cm, b = 4 cm, and l = 40 cm. The homogeneous material inside the capacitor has the parameters ǫ = 10−11 F/m, µ = 10−5 H/m, and σ = 10−5 S/m. If the electric field intensity is E = (106/ρ) cos(105t)aρ V/m (note missing t in the argument of the cosine in the book), find: a) J: Use J = σE = 10 ρ cos(105 t)aρ A/m2 b) the total conduction current, Ic, through the capacitor: Have Ic = J · dS = 2πρlJ = 20πl cos(105 t) = 8π cos(105 t) A c) the total displacement current, Id, through the capacitor: First find Jd = ∂D ∂t = ∂ ∂t (ǫE) = − (105)(10−11)(106) ρ sin(105 t)aρ = − 1 ρ sin(105 t) A/m Now Id = 2πρlJd = −2πl sin(105 t) = −0.8π sin(105 t) A d) the ratio of the amplitude of Id to that of Ic, the quality factor of the capacitor: This will be |Id| |Ic| = 0.8 8 = 0.1 10.12. Given a coaxial transmission line with b/a = e2.5, µR = ǫR = 1, and an electric field intensity E = (200/ρ) cos(109t − 3.336z) aρ V/m, find: a) Vab, the voltage between the conductors, if it is known that electrostatic relationship E = −∇V is valid; We use Vab = − a b 200 ρ cos(109 t − 3.336z) dρ = 200 ln b a cos(109 t − 3.336z) = 500 cos(109 t − 3.336z) V b) the displacement current density; Jd = ∂D ∂t = −200 × 109ǫ0 ρ sin(109 t − 3.336z)aρ = − 1.77 ρ sin(109 t − 3.336z)aρ A/m2 171 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 174. 10.13. Consider the region defined by |x|, |y|, and |z| < 1. Let ǫR = 5, µR = 4, and σ = 0. If Jd = 20 cos(1.5 × 108t − bx)ay µA/m2; a) find D and E: Since Jd = ∂D/∂t, we write D = Jddt + C = 20 × 10−6 1.5 × 108 sin(1.5 × 108 − bx)ay = 1.33 × 10−13 sin(1.5 × 108 t − bx)ay C/m2 where the integration constant is set to zero (assuming no dc fields are present). Then E = D ǫ = 1.33 × 10−13 (5 × 8.85 × 10−12) sin(1.5 × 108 t − bx)ay = 3.0 × 10−3 sin(1.5 × 108 t − bx)ay V/m b) use the point form of Faraday’s law and an integration with respect to time to find B and H: In this case, ∇ × E = ∂Ey ∂x az = −b(3.0 × 10−3 ) cos(1.5 × 108 t − bx)az = − ∂B ∂t Solve for B by integrating over time: B = b(3.0 × 10−3) 1.5 × 108 sin(1.5 × 108 t − bx)az = (2.0)b × 10−11 sin(1.5 × 108 t − bx)az T Now H = B µ = (2.0)b × 10−11 4 × 4π × 10−7 sin(1.5 × 108 t − bx)az = (4.0 × 10−6 )b sin(1.5 × 108 t − bx)az A/m c) use ∇ × H = Jd + J to find Jd: Since σ = 0, there is no conduction current, so in this case ∇ × H = − ∂Hz ∂x ay = 4.0 × 10−6 b2 cos(1.5 × 108 t − bx)ay A/m2 = Jd d) What is the numerical value of b? We set the given expression for Jd equal to the result of part c to obtain: 20 × 10−6 = 4.0 × 10−6 b2 ⇒ b = √ 5.0 m−1 10.14. A voltage source, V0 sin ωt, is connected between two concentric conducting spheres, r = a and r = b, b > a, where the region between them is a material for which ǫ = ǫRǫ0, µ = µ0, and σ = 0. Find the total displacement current through the dielectric and compare it with the source current as determined from the capacitance (Sec. 5.10) and circuit analysis methods: First, solving Laplace’s equation, we find the voltage between spheres (see Eq. 20, Chapter 7): V (t) = (1/r) − (1/b) (1/a) − (1/b) V0 sin ωt 172 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 175. 10.14 (continued) Then E = −∇V = V0 sin ωt r2(1/a − 1/b) ar ⇒ D = ǫRǫ0V0 sin ωt r2(1/a − 1/b) ar Now Jd = ∂D ∂t = ǫRǫ0ωV0 cos ωt r2(1/a − 1/b) ar The displacement current is then Id = 4πr2 Jd = 4πǫRǫ0ωV0 cos ωt (1/a − 1/b) = C dV dt where, from Eq. 47, Chapter 5, C = 4πǫRǫ0 (1/a − 1/b) The results are consistent. 10.15. Let µ = 3 × 10−5 H/m, ǫ = 1.2 × 10−10 F/m, and σ = 0 everywhere. If H = 2 cos(1010t − βx)az A/m, use Maxwell’s equations to obtain expressions for B, D, E, and β: First, B = µH = 6 × 10−5 cos(1010t − βx)az T. Next we use ∇ × H = − ∂H ∂x ay = 2β sin(1010 t − βx)ay = ∂D ∂t from which D = 2β sin(1010 t − βx) dt + C = − 2β 1010 cos(1010 t − βx)ay C/m2 where the integration constant is set to zero, since no dc fields are presumed to exist. Next, E = D ǫ = − 2β (1.2 × 10−10)(1010) cos(1010 t − βx)ay = −1.67β cos(1010 t − βx)ay V/m Now ∇ × E = ∂Ey ∂x az = 1.67β2 sin(1010 t − βx)az = − ∂B ∂t So B = − 1.67β2 sin(1010 t − βx)azdt = (1.67 × 10−10 )β2 cos(1010 t − βx)az We require this result to be consistent with the expression for B originally found. So (1.67 × 10−10 )β2 = 6 × 10−5 ⇒ β = ±600 rad/m 173 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 176. 10.16a. A certain material has σ = 0 and ǫR = 1. If H = 4 sin(106t − 0.01z)ay A/m, make use of Maxwell’s equations to find µR: First find ∇ × H = − ∂Hy ∂z ax = 0.04 cos(106 t − 0.01z)ax = ǫ0 ∂E ∂t So E = .04 ǫ0 cos(106 t − 0.01z)ax dt = .04 106ǫ0 sin(106 t − 0.01z)ax where the integration constant is zero, since we assume no dc fields present. Next ∇ × E = ∂Ex ∂z ay = − .04(.01) 106ǫ0 cos(106 t − 0.01z)ay = −µRµ0 ∂H ∂t So H = .04(.01) 106ǫ0µ0µR cos(106 t − 0.01z)ay dt = .04(.01) 1012ǫ0µ0µR sin(106 t − 0.01z)ay = 4 sin(106 t − 0.01z)ay where the last equality is required for consistency. Therefore .04(.01) 1012ǫ0µ0µR = 4 ⇒ µR = (.01)2(9 × 1016) 1012 = 9 b) Find E(z, t): This we already found during the development in part a: We have E(z, t) = .04 106ǫ0 sin(106 t − 0.01z)ax V/m = 4.5 sin(106 t − 0.01z)ax kV/m 10.17. The electric field intensity in the region 0 < x < 5, 0 < y < π/12, 0 < z < 0.06 m in free space is given by E = C sin(12y) sin(az) cos(2 × 1010t) ax V/m. Beginning with the ∇ × E relationship, use Maxwell’s equations to find a numerical value for a, if it is known that a is greater than zero: In this case we find ∇ × E = ∂Ex ∂z ay − ∂Ez ∂y az = C a sin(12y) cos(az)ay − 12 cos(12y) sin(az)az cos(2 × 1010 t) = − ∂B ∂t Then H = − 1 µ0 ∇ × E dt + C1 = − C µ0(2 × 1010 a sin(12y) cos(az)ay − 12 cos(12y) sin(az)az sin(2 × 1010 t) A/m where the integration constant, C1 = 0, since there are no initial conditions. Using this result, we now find ∇ × H = ∂Hz ∂y − ∂Hy ∂z ax = − C(144 + a2) µ0(2 × 1010) sin(12y) sin(az) sin(2 × 1010 t) ax = ∂D ∂t 174 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 177. 10.17. (continued) Now E = D ǫ0 = 1 ǫ0 ∇ × H dt + C2 = C(144 + a2) µ0ǫ0(2 × 1010)2 sin(12y) sin(az) cos(2 × 1010 t) ax where C2 = 0. This field must be the same as the original field as stated, and so we require that C(144 + a2) µ0ǫ0(2 × 1010)2 = 1 Using µ0ǫ0 = (3 × 108)−2, we find a = (2 × 1010)2 (3 × 108)2 − 144 1/2 = 66 m−1 10.18. The parallel plate transmission line shown in Fig. 10.8 has dimensions b = 4 cm and d = 8 mm, while the medium between plates is characterized by µR = 1, ǫR = 20, and σ = 0. Neglect fields outside the dielectric. Given the field H = 5 cos(109t − βz)ay A/m, use Maxwell’s equations to help find: a) β, if β > 0: Take ∇ × H = − ∂Hy ∂z ax = −5β sin(109 t − βz)ax = 20ǫ0 ∂E ∂t So E = −5β 20ǫ0 sin(109 t − βz)ax dt = β (4 × 109)ǫ0 cos(109 t − βz)ax Then ∇ × E = ∂Ex ∂z ay = β2 (4 × 109)ǫ0 sin(109 t − βz)ay = −µ0 ∂H ∂t So that H = −β2 (4 × 109)µ0ǫ0 sin(109 t − βz)ax dt = β2 (4 × 1018)µ0ǫ0 cos(109 t − βz) = 5 cos(109 t − βz)ay where the last equality is required to maintain consistency. Therefore β2 (4 × 1018)µ0ǫ0 = 5 ⇒ β = 14.9 m−1 b) the displacement current density at z = 0: Since σ = 0, we have ∇ × H = Jd = −5β sin(109 t − βz) = −74.5 sin(109 t − 14.9z)ax = −74.5 sin(109 t)ax A/m at z = 0 c) the total displacement current crossing the surface x = 0.5d, 0 < y < b, and 0 < z < 0.1 m in the ax direction. We evaluate the flux integral of Jd over the given cross section: Id = −74.5b 0.1 0 sin(109 t − 14.9z) ax · ax dz = 0.20 cos(109 t − 1.49) − cos(109 t) A 175 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 178. 10.19. In the first section of this chapter, Faraday’s law was used to show that the field E = −1 2 kB0ρekt aφ results from the changing magnetic field B = B0ekt az (note that the factor of ρ appearing in E was omitted from the original problem statement). a) Show that these fields do not satisfy Maxwell’s other curl equation: Note that B as stated is constant with position, and so will have zero curl. The electric field, however, varies with time, and so ∇ × H = ∂D ∂t would have a zero left-hand side and a non-zero right-hand side. The equation is thus not valid with these fields. b) If we let B0 = 1 T and k = 106 s−1, we are establishing a fairly large magnetic flux density in 1 µs. Use the ∇ × H equation to show that the rate at which Bz should (but does not) change with ρ is only about 5 × 10−6 T/m in free space at t = 0: Assuming that B varies with ρ, we write ∇ × H = − ∂Hz ∂ρ aφ = − 1 µ0 dB0 dρ ekt = ǫ0 ∂E ∂t = − 1 2 ǫ0k2 B0ρekt Thus dB0 dρ = 1 2 µ0ǫ0k2 ρB0 = 1012(1)ρ 2(3 × 108)2 = 5.6 × 10−6 ρ which is near the stated value if ρ is on the order of 1m. 10.20. Point C(−0.1, −0.2, 0.3) lies on the surface of a perfect conductor. The electric field intensity at C is (500ax − 300ay + 600az) cos 107t V/m, and the medium surrounding the conductor is characterized by µR = 5, ǫR = 10, and σ = 0. a) Find a unit vector normal to the conductor surface at C, if the origin lies within the conductor: At t = 0, the field must be directed out of the surface, and will be normal to it, since we have a perfect conductor. Therefore n = +E(t = 0) |E(t = 0)| = 5ax − 3ay + 6az √ 25 + 9 + 36 = 0.60ax − 0.36ay + 0.72az b) Find the surface charge density at C: Use ρs = D · n|surf ace = 10ǫ0 500ax − 300ay + 600az cos(107 t) · .60ax − .36ay + .72az = 10ǫ0 [300 + 108 + 432] cos(107 t) = 7.4 × 10−8 cos(107 t) C/m2 = 74 cos(107 t) nC/m2 10.21. The surfaces ρ = 3 and 10 mm, and z = 0 and 25 cm are perfect conductors. The region en- closed by these surfaces has µ = 2.5 × 10−6 H/m, ǫ = 4 × 10−11 F/m, and σ = 0. Let H = (2/ρ) cos(10πz) cos(ωt) aφ A/m. Make use of Maxwell’s equations to find a) ω: We start with ∇ × H = − ∂Hφ ∂z aρ = 20π ρ sin(10πz) cos(ωt) aρ = ǫ ∂E ∂t We then find E = 20π ρǫ sin(10πz) cos(ωt) dt aρ = 20π ωρǫ sin(10πz) sin(ωt) aρ 176 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 179. 10.21a. (continued) At this point, a flaw in the problem statement becomes apparent, since this field should vanish on the surface of the perfect conductor located at z = 0.25m. This does not happen with the sin(10πz) function. Nevertheless, we press on: ∇ × E = ∂Eρ ∂z aφ = (20π)(10π) ωρǫ cos(10πz) sin(ωt) aφ = −µ ∂H ∂t So H = −200π2 ωρµǫ cos(10πz) sin(ωt) aφ dt = 200π2 ω2µǫρ cos(10πz) cos(ωt) aφ This result must equal the given H field, so we require that 200π2 ω2µǫρ = 2 ρ ⇒ ω = 10π √ µǫ = 10π (2.5 × 10−6)(4 × 10−11) = π × 109 sec−1 b) E: We use the result of part a: E = 20π ωρǫ sin(10πz) sin(ωt) aρ = 500 ρ sin(10πz) sin(ωt) aρ V/m 10.22. In free space, where ǫ = ǫ0, µ = µ0, σ = 0, J = 0, and ρv = 0, assume a cartesian coordinate system in which E and H are both functions only of z and t. a) If E = Eyay and H = Hxax, begin with Maxwell’s equations and determine the second order partial differential equation that Ey must satisfy: The procedure here is similar to the development that leads to Eq. 53. Begin by taking the curl of both sides of the Faraday law equation: ∇ × ∇ × E = ∇ × −µ0 ∂H ∂t = −µ0 ∂ ∂t (∇ × H) where ∇ × H = ǫ0∂E/∂t. Therefore ∇ × ∇ × E = ∇(∇ · E) − ∇2 E = −µ0ǫ0 ∂2E ∂t2 where the first equality is found from Eq. 52. Noting that in free space, ∇ · D = ǫ0∇ · E = 0, we obtain, ∇2 E = µ0ǫ0 ∂2E ∂t2 ⇒ ∂2Ey ∂z2 = µ0ǫ0 ∂2Ey ∂t2 since E varies only with z and t, and is y-directed. b) Show that Ey = 5(300t + bz)2 is a solution of that equation for a particular value of b, and find that value: Substituting, we find ∂2Ey ∂z2 = 10b2 = µ0ǫ0 ∂Ey ∂t2 = 9 × 105 µ0ǫ0 Therefore 10b2 = 9 × 105 µ0ǫ0 → b = 1.0 × 10−6 m−1 177 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 180. 10.23. In region 1, z < 0, ǫ1 = 2 × 10−11 F/m, µ1 = 2 × 10−6 H/m, and σ1 = 4 × 10−3 S/m; in region 2, z > 0, ǫ2 = ǫ1/2, µ2 = 2µ1, and σ2 = σ1/4. It is known that E1 = (30ax + 20ay + 10az) cos(109t) V/m at P1(0, 0, 0−). a) Find EN1, Et1, DN1, and Dt1: These will be EN1 = 10 cos(109 t)az V/m Et1 = (30ax + 20ay) cos(109 t) V/m DN1 = ǫ1EN1 = (2 × 10−11 )(10) cos(109 t)az C/m2 = 200 cos(109 t)az pC/m2 Dt1 = ǫ1Et1 = (2 × 10−11 )(30ax + 20ay) cos(109 t) = (600ax + 400ay) cos(109 t) pC/m2 b) Find JN1 and Jt1 at P1: JN1 = σ1EN1 = (4 × 10−3 )(10 cos(109 t))az = 40 cos(109 t)az mA/m2 Jt1 = σ1Et1 = (4 × 10−3 )(30ax + 20ay) cos(109 t) = (120ax + 80ay) cos(109 t) mA/m2 c) Find Et2, Dt2, and Jt2 at P1: By continuity of tangential E, Et2 = Et1 = (30ax + 20ay) cos(109 t) V/m Then Dt2 = ǫ2Et2 = (10−11 )(30ax + 20ay) cos(109 t) = (300ax + 200ay) cos(109 t) pC/m2 Jt2 = σ2Et2 = (10−3 )(30ax + 20ay) cos(109 t) = (30ax + 20ay) cos(109 t) mA/m2 d) (Harder) Use the continuity equation to help show that JN1 − JN2 = ∂DN2/∂t − ∂DN1/∂t (note misprint in problem statement) and then determine EN2, DN2, and JN2: We assume the existence of a surface charge layer at the boundary having density ρs C/m2. If we draw a cylindrical “pillbox” whose top and bottom surfaces (each of area a) are on either side of the interface, we may use the continuity condition to write (JN2 − JN1) a = − ∂ρs ∂t a where ρs = DN2 − DN1. Therefore, JN1 − JN2 = ∂ ∂t (DN2 − DN1) In terms of the normal electric field components, this becomes σ1EN1 − σ2EN2 = ∂ ∂t (ǫ2EN2 − ǫ1EN1) Now let EN2 = A cos(109t) + B sin(109t), while from before, EN1 = 10 cos(109t). 178 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 181. 10.23. (continued) These, along with the permittivities and conductivities, are substituted to obtain (4 × 10−3 )(10) cos(109 t) − 10−3 [A cos(109 t) + B sin(109 t)] = ∂ ∂t 10−11 [A cos(109 t) + B sin(109 t)] − (2 × 10−11 )(10) cos(109 t) = −(10−2 A sin(109 t) + 10−2 B cos(109 t) + (2 × 10−1 ) sin(109 t) We now equate coefficients of the sin and cos terms to obtain two equations: 4 × 10−2 − 10−3 A = 10−2 B −10−3 B = −10−2 A + 2 × 10−1 These are solved together to find A = 20.2 and B = 2.0. Thus EN2 = 20.2 cos(109 t) + 2.0 sin(109 t) az = 20.3 cos(109 t + 5.6◦ )az V/m Then DN2 = ǫ2EN2 = 203 cos(109 t + 5.6◦ )az pC/m2 and JN2 = σ2EN2 = 20.3 cos(109 t + 5.6◦ )az mA/m2 10.24. Given the fields V = 80z cos x cos 3 × 108t. kV and A = 26.7z sin x sin 3 × 108t ax mWb/m in free space, find E and H: First, find E through E = −∇V − ∂A ∂t where −∇V = 80 cos(3 × 108 t)[z sin xax − cos xaz] kV/m and −∂A/∂t = −(3 × 108 )(26.7)z sin x cos(3 × 108 t)ax mV/m Finally, E = − 7.9 × 106 z sin x ax + 8.0 × 104 cos x az cos(3 × 108 t) V/m Now B = ∇ × A = ∂Ax ∂z ay = 26.7 sin x sin(3 × 108 t)ay mWb/m2 Then H = B µ0 = 2.12 × 104 sin x sin(3 × 108 t) ay A/m 179 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 182. 10.25. In a region where µR = ǫR = 1 and σ = 0, the retarded potentials are given by V = x(z − ct) V and A = x[(z/c) − t]az Wb/m, where c = 1/ √ µ0ǫ0. a) Show that ∇ · A = −µǫ(∂V/∂t): First, ∇ · A = ∂Az ∂z = x c = x √ µ0ǫ0 Second, ∂V ∂t = −cx = − x √ µ0ǫ0 so we observe that ∇ · A = −µ0ǫ0(∂V/∂t) in free space, implying that the given statement would hold true in general media. b) Find B, H, E, and D: Use B = ∇ × A = − ∂Ax ∂x ay = t − z c ay T Then H = B µ0 = 1 µ0 t − z c ay A/m Now, E = −∇V − ∂A ∂t = −(z − ct)ax − xaz + xaz = (ct − z)ax V/m Then D = ǫ0E = ǫ0(ct − z)ax C/m2 c) Show that these results satisfy Maxwell’s equations if J and ρv are zero: i. ∇ · D = ∇ · ǫ0(ct − z)ax = 0 ii. ∇ · B = ∇ · (t − z/c)ay = 0 iii. ∇ × H = − ∂Hy ∂z ax = 1 µ0c ax = ǫ0 µ0 ax which we require to equal ∂D/∂t: ∂D ∂t = ǫ0cax = ǫ0 µ0 ax iv. ∇ × E = ∂Ex ∂z ay = −ay which we require to equal −∂B/∂t: ∂B ∂t = ay So all four Maxwell equations are satisfied. 180 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 183. 10.26. Let the current I = 80t A be present in the az direction on the z axis in free space within the interval −0.1 < z < 0.1 m. a) Find Az at P (0, 2, 0): The integral for the retarded vector potential will in this case assume the form A = .1 −.1 µ080(t − R/c) 4πR az dz where R = √ z2 + 4 and c = 3 × 108 m/s. We obtain Az = 80µ0 4π .1 −.1 t √ z2 + 4 dz − .1 −.1 1 c dz = 8 × 10−6 t ln(z + z2 + 4) .1 −.1 − 8 × 10−6 3 × 108 z .1 −.1 = 8 × 10−6 ln .1 + √ 4.01 −.1 + √ 4.01 − 0.53 × 10−14 = 8.0 × 10−7 t − 0.53 × 10−14 So finally, A = 8.0 × 10−7t − 5.3 × 10−15 az Wb/m. b) Sketch Az versus t over the time interval −0.1 < t < 0.1 µs: The sketch is linearly increasing with time, beginning with Az = −8.53 × 10−14 Wb/m at t = −0.1 µs, crossing the time axis and going positive at t = 6.6 ns, and reaching a maximum value of 7.46 × 10−14 Wb/m at t = 0.1 µs. 181 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 184. CHAPTER 11 11.1. Show that Exs = Aejk0z+φ is a solution to the vector Helmholtz equation, Sec. 11.1, Eq. (16), for k0 = ω √ µ0ǫ0 and any φ and A: We take d2 dz2 Aejk0z+φ = (jk0)2 Aejk0z+φ = −k2 0Exs 11.2. Let E(z, t) = 200 sin 0.2z cos 108tax + 500 cos(0.2z + 50◦) sin 108tay V/m. Find: a) E at P (0, 2, 0.6) at t = 25 ns: Obtain EP (t = 25) = 200 sin [(0.2)(0.6)] cos(2.5)ax + 500 cos [(0.2)(0.6) + 50(2π)/360] sin(2.5)ay = −19.2ax + 164ay V/m b) |E| at P at t = 20 ns: EP (t = 20) = 200 sin [(0.2)(0.6)] cos(2.0)ax + 500 cos [(0.2)(0.6) + 50(2π)/360] sin(2.0)ay = −9.96ax + 248ay V/m Thus |EP | = (9.96)2 + (248)2 = 249 V/m. c) Es at P: Es = 200 sin 0.2zax − j500 cos(0.2z + 50◦)ay. Thus EsP = 200 sin [(0.2)(0.6)] ax − j500 cos [(0.2)(0.6) + 2π(50)/360] ay = 23.9ax − j273ay V/m 11.3. An H field in free space is given as H(x, t) = 10 cos(108t − βx)ay A/m. Find a) β: Since we have a uniform plane wave, β = ω/c, where we identify ω = 108 sec−1. Thus β = 108/(3 × 108) = 0.33 rad/m. b) λ: We know λ = 2π/β = 18.9 m. c) E(x, t) at P (0.1, 0.2, 0.3) at t = 1 ns: Use E(x, t) = −η0H(x, t) = −(377)(10) cos(108t − βx) = −3.77 × 103 cos(108t − βx). The vector direction of E will be −az, since we require that S = E × H, where S is x-directed. At the given point, the relevant coordinate is x = 0.1. Using this, along with t = 10−9 sec, we finally obtain E(x, t) = −3.77 × 103 cos[(108 )(10−9 ) − (0.33)(0.1)]az = −3.77 × 103 cos(6.7 × 10−2 )az = −3.76 × 103 az V/m 11.4. In phasor form, the electric field intensity of a uniform plane wave in free space is expressed as Es = (40 − j30)e−j20zax V/m. Find: a) ω: From the given expression, we identify β = 20 rad/m. Then ω = cβ = (3 × 108)(20) = 6.0 × 109 rad/s. b) β = 20 rad/m from part a. 182 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 185. 11.4. (continued) c) f = ω/2π = 956 MHz. d) λ = 2π/β = 2π/20 = 0.314 m. e) Hs: In free space, we find Hs by dividing Es by η0, and assigning vector components such that Es × Hs gives the required direction of wave travel: We find Hs = 40 − j30 377 e−j20z ay = (0.11 − j0.08)e−j20z ay A/m f) H(z, t) at P (6, −1, 0.07), t = 71 ps: H(z, t) = Re Hsejωt = 0.11 cos(6.0 × 109 t − 20z) + 0.08 sin(6.0 × 109 t − 20z) ay Then H(.07, t = 71ps) = 0.11 cos (6.0 × 109 )(7.1 × 10−11 ) − 20(.07) + .08 sin (6.0 × 109 )(7.1 × 10−11 ) − 20(.07) ay = [0.11(0.562) − 0.08(0.827)]ay = −6.2 × 10−3 ay A/m 11.5. A 150-MHz uniform plane wave in free space is described by Hs = (4 + j10)(2ax + jay)e−jβz A/m. a) Find numerical values for ω, λ, and β: First, ω = 2π × 150 × 106 = 3π × 108 sec−1. Second, for a uniform plane wave in free space, λ = 2πc/ω = c/f = (3 × 108)/(1.5 × 108) = 2 m. Third, β = 2π/λ = π rad/m. b) Find H(z, t) at t = 1.5 ns, z = 20 cm: Use H(z, t) = Re{Hsejωt } = Re{(4 + j10)(2ax + jay)(cos(ωt − βz) + j sin(ωt − βz)} = [8 cos(ωt − βz) − 20 sin(ωt − βz)] ax − [10 cos(ωt − βz) + 4 sin(ωt − βz)] ay . Now at the given position and time, ωt − βz = (3π × 108)(1.5 × 10−9) − π(0.20) = π/4. And cos(π/4) = sin(π/4) = 1/ √ 2. So finally, H(z = 20cm, t = 1.5ns) = − 1 √ 2 12ax + 14ay = −8.5ax − 9.9ay A/m c) What is |E|max? Have |E|max = η0|H|max, where |H|max = Hs · H∗ s = [4(4 + j10)(4 − j10) + (j)(−j)(4 + j10)(4 − j10)]1/2 = 24.1 A/m Then |E|max = 377(24.1) = 9.08 kV/m. 183 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 186. 11.6. Let µR = ǫR = 1 for the field E(z, t) = (25ax − 30ay) cos(ωt − 50z) V/m. a) Find ω: ω = cβ = (3 × 108)(50) = 15.0 × 109 s−1. b) Determine the displacement current density, Jd(z, t): Jd(z, t) = ∂D ∂t = −ǫ0ω(25ax − 30ay) sin(ωt − 50z) = (−3.32ax + 3.98ay) sin(1.5 × 1010 t − 50z) A/m2 c) Find the total magnetic flux passing through the rectangle defined by 0 < x < 1, y = 0, 0 < z < 1, at t = 0: In free space, the magnetic field of the uniform plane wave can be easily found using the intrinsic impedance: H(z, t) = 25 η0 ay + 30 η0 ax cos(ωt − 50z) A/m Then B(z, t) = µ0H(z, t) = (1/c)(25ay + 30ax) cos(ωt − 50z) Wb/m2, where µ0/η0 = √ µ0ǫ0 = 1/c. The flux at t = 0 is now = 1 0 1 0 B · ay dx dz = 1 0 25 c cos(50z) dz = 25 50(3 × 108) sin(50) = −0.44 nWb 11.7. The phasor magnetic field intensity for a 400-MHz uniform plane wave propagating in a certain lossless material is (2ay − j5az)e−j25x A/m. Knowing that the maximum amplitude of E is 1500 V/m, find β, η, λ, vp, ǫR, µR, and H(x, y, z, t): First, from the phasor expression, we identify β = 25 m−1 from the argument of the exponential function. Next, we evaluate H0 = |H| = √ H · H∗ = √ 22 + 52 = √ 29. Then η = E0/H0 = 1500/ √ 29 = 278.5 . Then λ = 2π/β = 2π/25 = .25 m = 25 cm. Next, vp = ω β = 2π × 400 × 106 25 = 1.01 × 108 m/s Now we note that η = 278.5 = 377 µR ǫR ⇒ µR ǫR = 0.546 And vp = 1.01 × 108 = c √ µRǫR ⇒ µRǫR = 8.79 We solve the above two equations simultaneously to find ǫR = 4.01 and µR = 2.19. Finally, H(x, y, z, t) = Re (2ay − j5az)e−j25x ejωt = 2 cos(2π × 400 × 106 t − 25x)ay + 5 sin(2π × 400 × 106 t − 25x)az = 2 cos(8π × 108 t − 25x)ay + 5 sin(8π × 108 t − 25x)az A/m 184 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 187. 11.8. Let the fields, E(z, t) = 1800 cos(107πt − βz)ax V/m and H(z, t) = 3.8 cos(107πt − βz)ay A/m, represent a uniform plane wave propagating at a velocity of 1.4 × 108 m/s in a perfect dielectric. Find: a) β = ω/v = (107π)/(1.4 × 108) = 0.224 m−1. b) λ = 2π/β = 2π/.224 = 28.0 m. c) η = |E|/|H| = 1800/3.8 = 474 . d) µR: Have two equations in the two unknowns, µR and ǫR: η = η0 √ µR/ǫR and β = ω √ µRǫR/c. Eliminate ǫR to find µR = βcη ωη0 2 = (.224)(3 × 108)(474) (107π)(377) 2 = 2.69 e) ǫR = µR(η0/η)2 = (2.69)(377/474)2 = 1.70. 11.9. A certain lossless material has µR = 4 and ǫR = 9. A 10-MHz uniform plane wave is propagating in the ay direction with Ex0 = 400 V/m and Ey0 = Ez0 = 0 at P (0.6, 0.6, 0.6) at t = 60 ns. a) Find β, λ, vp, and η: For a uniform plane wave, β = ω √ µǫ = ω c √ µRǫR = 2π × 107 3 × 108 (4)(9) = 0.4π rad/m Then λ = (2π)/β = (2π)/(0.4π) = 5 m. Next, vp = ω β = 2π × 107 4π × 10−1 = 5 × 107 m/s Finally, η = µ ǫ = η0 µR ǫR = 377 4 9 = 251 b) Find E(t) (at P ): We are given the amplitude at t = 60 ns and at y = 0.6 m. Let the maximum amplitude be Emax, so that in general, Ex = Emax cos(ωt − βy). At the given position and time, Ex = 400 = Emax cos[(2π × 107 )(60 × 10−9 ) − (4π × 10−1 )(0.6)] = Emax cos(0.96π) = −0.99Emax So Emax = (400)/(−0.99) = −403 V/m. Thus at P, E(t) = −403 cos(2π × 107t) V/m. c) Find H(t): First, we note that if E at a given instant points in the negative x direction, while the wave propagates in the forward y direction, then H at that same position and time must point in the positive z direction. Since we have a lossless homogeneous medium, η is real, and we are allowed to write H(t) = E(t)/η, where η is treated as negative and real. Thus H(t) = Hz(t) = Ex(t) η = −403 −251 cos(2π × 10−7 t) = 1.61 cos(2π × 10−7 t) A/m 185 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 188. 11.10. Given a 20MHz uniform plane wave with Hs = (6ax − j2ay)e−jz A/m, assume propagation in a lossless medium characterized by ǫR = 5 and an unknown µR. a) Find λ, vp, µR, and η: First, β = 1, so λ = 2π/β = 2π m. Next, vp = ω/β = 2π × 20 × 106 = 4π × 107 m/s. Then, µR = (β2c2)/(ω2ǫR) = (3 × 108)2/(4π × 107)2(5) = 1.14. Finally, η = η0 √ µR/ǫR = 377 √ 1.14/5 = 180. b) Determine E at the origin at t = 20ns: We use the relation |E| = η|H| and note that for positive z propagation, a positive x component of H is coupled to a negative y component of E, and a negative y componentofH iscoupledtoanegativex componentofE. WeobtainEs = −η(6ay+j2ax)e−jz. Then E(z, t) = Re Esejωt = −6η cos(ωt − z)ay + 2η sin(ωt − z)ax = 360 sin(ωt − z)ax − 1080 cos(ωt − z)ay. With ω = 4π × 107 sec−1, t = 2 × 10−8 s, and z = 0, E evaluates as E(0, 20ns) = 360(0.588)ax − 1080(−0.809)ay = 212ax + 874ay V/m. 11.11. A 2-GHz uniform plane wave has an amplitude of Ey0 = 1.4 kV/m at (0, 0, 0, t = 0) and is propagating in the az direction in a medium where ǫ′′ = 1.6×10−11 F/m, ǫ′ = 3.0×10−11 F/m, and µ = 2.5 µH/m. Find: a) Ey at P (0, 0, 1.8cm) at 0.2 ns: To begin, we have the ratio, ǫ′′/ǫ′ = 1.6/3.0 = 0.533. So α = ω µǫ′ 2 1 + ǫ′′ ǫ′ 2 − 1 1/2 = (2π × 2 × 109 ) (2.5 × 10−6)(3.0 × 10−11) 2 1 + (.533)2 − 1 1/2 = 28.1 Np/m Then β = ω µǫ′ 2 1 + ǫ′′ ǫ′ 2 + 1 1/2 = 112 rad/m Thus in general, Ey(z, t) = 1.4e−28.1z cos(4π × 109 t − 112z) kV/m Evaluating this at t = 0.2 ns and z = 1.8 cm, find Ey(1.8 cm, 0.2 ns) = 0.74 kV/m b) Hx at P at 0.2 ns: We use the phasor relation, Hxs = −Eys/η where η = µ ǫ′ 1 1 − j(ǫ′′/ǫ′) = 2.5 × 10−6 3.0 × 10−11 1 √ 1 − j(.533) = 263 + j65.7 = 271 14◦ So now Hxs = − Eys η = − (1.4 × 103)e−28.1ze−j112z 271ej14◦ = −5.16e−28.1z e−j112z e−j14◦ A/m Then Hx(z, t) = −5.16e−28.1z cos(4π × 10−9 t − 112z − 14◦ ) This, when evaluated at t = 0.2 ns and z = 1.8 cm, yields Hx(1.8 cm, 0.2 ns) = −3.0 A/m 186 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 189. 11.12. The plane wave Es = 300e−jkxay V/m is propagating in a material for which µ = 2.25 µH/m, ǫ′ = 9 pF/m, and ǫ′′ = 7.8 pF/m. If ω = 64 Mrad/s, find: a) α: We use the general formula, Eq. (35): α = ω µǫ′ 2 1 + ǫ′′ ǫ′ 2 − 1 1/2 = (64 × 106 ) (2.25 × 10−6)(9 × 10−12) 2 1 + (.867)2 − 1 1/2 = 0.116 Np/m b) β: Using (36), we write β = ω µǫ′ 2 1 + ǫ′′ ǫ′ 2 + 1 1/2 = .311 rad/m c) vp = ω/β = (64 × 106)/(.311) = 2.06 × 108 m/s. d) λ = 2π/β = 2π/(.311) = 20.2 m. e) η: Using (39): η = µ ǫ′ 1 1 − j(ǫ′′/ǫ′) = 2.25 × 10−6 9 × 10−12 1 √ 1 − j(.867) = 407 + j152 = 434.5ej.36 f) Hs: With Es in the positive y direction (at a given time) and propagating in the positive x direction, we would have a positive z component of Hs, at the same time. We write (with jk = α + jβ): Hs = Es η az = 300 434.5ej.36 e−jkx az = 0.69e−αx e−jβx e−j.36 az = 0.69e−.116x e−j.311x e−j.36 az A/m g) E(3, 2, 4, 10ns): The real instantaneous form of E will be E(x, y, z, t) = Re Esejωt = 300e−αx cos(ωt − βx)ay Therefore E(3, 2, 4, 10ns) = 300e−.116(3) cos[(64 × 106 )(10−8 ) − .311(3)]ay = 203 V/m 11.13. Let jk = 0.2 + j1.5 m−1 and η = 450 + j60 for a uniform plane wave propagating in the az direction. If ω = 300 Mrad/s, find µ, ǫ′, and ǫ′′: We begin with η = µ ǫ′ 1 1 − j(ǫ′′/ǫ′) = 450 + j60 and jk = jω µǫ′ 1 − j(ǫ′′/ǫ′) = 0.2 + j1.5 187 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 190. 11.13. (continued) Then ηη∗ = µ ǫ′ 1 1 + (ǫ′′/ǫ′)2 = (450 + j60)(450 − j60) = 2.06 × 105 (1) and (jk)(jk)∗ = ω2 µǫ′ 1 + (ǫ′′/ǫ′)2 = (0.2 + j1.5)(0.2 − j1.5) = 2.29 (2) Taking the ratio of (2) to (1), (jk)(jk)∗ ηη∗ = ω2 (ǫ′ )2 1 + (ǫ′′ /ǫ′ )2 = 2.29 2.06 × 105 = 1.11 × 10−5 Then with ω = 3 × 108, (ǫ′ )2 = 1.11 × 10−5 (3 × 108)2 1 + (ǫ′′/ǫ′)2 = 1.23 × 10−22 1 + (ǫ′′/ǫ′)2 (3) Now, we use Eqs. (35) and (36). Squaring these and taking their ratio gives α2 β2 = 1 + (ǫ′′/ǫ′)2 1 + (ǫ′′/ǫ′)2 = (0.2)2 (1.5)2 We solve this to find ǫ′′/ǫ′ = 0.271. Substituting this result into (3) gives ǫ′ = 1.07 × 10−11 F/m. Since ǫ′′/ǫ′ = 0.271, we then find ǫ′′ = 2.90 × 10−12 F/m. Finally, using these results in either (1) or (2) we find µ = 2.28 × 10−6 H/m. Summary: µ = 2.28 × 10−6 H/m, ǫ′ = 1.07 × 10−11 F/m, and ǫ′′ = 2.90 × 10−12 F/m. 11.14. A certain nonmagnetic material has the material constants ǫ′ R = 2 and ǫ′′/ǫ′ = 4 × 10−4 at ω = 1.5 Grad/s. Find the distance a uniform plane wave can propagate through the material before: a) it is attenuated by 1 Np: First, ǫ′′ = (4 × 104)(2)(8.854 × 10−12) = 7.1 × 10−15 F/m. Then, since ǫ′′/ǫ′ << 1, we use the approximate form for α, given by Eq. (51) (written in terms of ǫ′′): α . = ωǫ′′ 2 µ ǫ′ = (1.5 × 109)(7.1 × 10−15) 2 377 √ 2 = 1.42 × 10−3 Np/m The required distance is now z1 = (1.42 × 10−3)−1 = 706 m b) the power level is reduced by one-half: The governing relation is e−2αz1/2 = 1/2, or z1/2 = ln 2/2α = ln 2/2(1.42 × 10−3) = 244 m. c) the phase shifts 360◦: This distance is defined as one wavelength, where λ = 2π/β = (2πc)/(ω ǫ′ R) = [2π(3 × 108)]/[(1.5 × 109) √ 2] = 0.89 m. 11.15. A 10 GHz radar signal may be represented as a uniform plane wave in a sufficiently small region. Calculatethewavelengthincentimetersandtheattenuationinneperspermeterifthewaveispropagating in a non-magnetic material for which a) ǫ′ R = 1 and ǫ′′ R = 0: In a non-magnetic material, we would have: α = ω µ0ǫ0ǫ′ R 2 1 + ǫ′′ R ǫ′ R 2 − 1 1/2 188 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 191. 11.15. (continued) and β = ω µ0ǫ0ǫ′ R 2 1 + ǫ′′ R ǫ′ R 2 + 1 1/2 With the given values of ǫ′ R and ǫ′′ R, it is clear that β = ω √ µ0ǫ0 = ω/c, and so λ = 2π/β = 2πc/ω = 3 × 1010/1010 = 3 cm. It is also clear that α = 0. b) ǫ′ R = 1.04 and ǫ′′ R = 9.00 × 10−4: In this case ǫ′′ R/ǫ′ R << 1, and so β . = ω ǫ′ R/c = 2.13 cm−1. Thus λ = 2π/β = 2.95 cm. Then α . = ωǫ′′ 2 µ ǫ′ = ωǫ′′ R 2 √ µ0ǫ0 ǫ′ R = ω 2c ǫ′′ R ǫ′ R = 2π × 1010 2 × 3 × 108 (9.00 × 10−4) √ 1.04 = 9.24 × 10−2 Np/m c) ǫ′ R = 2.5 and ǫ′′ R = 7.2: Using the above formulas, we obtain β = 2π × 1010 √ 2.5 (3 × 1010) √ 2 1 + 7.2 2.5 2 + 1 1/2 = 4.71 cm−1 and so λ = 2π/β = 1.33 cm. Then α = 2π × 1010 √ 2.5 (3 × 108) √ 2 1 + 7.2 2.5 2 − 1 1/2 = 335 Np/m 11.16. The power factor of a capacitor is defined as the cosine of the impedance phase angle, and its Q is ωCR, where R is the parallel resistance. Assume an idealized parallel plate capacitor having a dielecric characterized by σ, ǫ′, and µR. Find both the power factor and Q in terms of the loss tangent: First, the impedance will be: Z = R 1 jωC R + 1 jωC = R 1 − jRωC 1 + (RωC)2 = R 1 − jQ 1 + Q2 Now R = d/(σA) and C = ǫ′A/d, and so Q = ωǫ′/σ = 1/l.t. Then the power factor is P.F = cos[tan−1(−Q)] = 1/ 1 + Q2. 189 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 192. 11.17. Let η = 250 + j30 and jk = 0.2 + j2 m−1 for a uniform plane wave propagating in the az direction in a dielectric having some finite conductivity. If |Es| = 400 V/m at z = 0, find: a) Pz,av at z = 0 and z = 60 cm: Assume x-polarization for the electric field. Then Pz,av = 1 2 Re Es × H∗ s = 1 2 Re 400e−αz e−jβz ax × 400 η∗ e−αz ejβz ay = 1 2 (400)2 e−2αz Re 1 η∗ az = 8.0 × 104 e−2(0.2)z Re 1 250 − j30 az = 315 e−2(0.2)z az W/m2 Evaluating at z = 0, obtain Pz,av(z = 0) = 315 az W/m2, and at z = 60 cm, Pz,av(z = 0.6) = 315e−2(0.2)(0.6)az = 248 az W/m2. b) the average ohmic power dissipation in watts per cubic meter at z = 60 cm: At this point a flaw becomes evident in the problem statement, since solving this part in two different ways gives results that are not the same. I will demonstrate: In the first method, we use Poynting’s theorem in point form (first equation at the top of p. 366), which we modify for the case of time-average fields to read: −∇ · Pz,av =< J · E > where the right hand side is the average power dissipation per volume. Note that the additional right-hand-side terms in Poynting’s theorem that describe changes in energy stored in the fields will both be zero in steady state. We apply our equation to the result of part a: < J · E >= −∇ · Pz,av = − d dz 315 e−2(0.2)z = (0.4)(315)e−2(0.2)z = 126e−0.4z W/m3 At z = 60 cm, this becomes < J · E >= 99.1 W/m3. In the second method, we solve for the conductivity and evaluate < J · E >= σ < E2 >. We use jk = jω µǫ′ 1 − j(ǫ′′/ǫ′) and η = µ ǫ′ 1 1 − j(ǫ′′/ǫ′) We take the ratio, jk η = jωǫ′ 1 − j ǫ′′ ǫ′ = jωǫ′ + ωǫ′′ Identifying σ = ωǫ′′, we find σ = Re jk η = Re 0.2 + j2 250 + j30 = 1.74 × 10−3 S/m Now we find the dissipated power per volume: σ < E2 >= 1.74 × 10−3 1 2 400e−0.2z 2 190 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 193. 11.17b. (continued) At z = 60 cm, this evaluates as 109 W/m3. One can show that consistency between the two methods requires that Re 1 η∗ = σ 2α This relation does not hold using the numbers as given in the problem statement and the value of σ found above. Note that in Problem 11.13, where all values are worked out, the relation does hold and consistent results are obtained using both methods. 11.18a. Find P (r, t) if Es = 400e−j2xay V/m in free space: A positive y component of E requires a posi- tive z component of H for propagation in the forward x direction. Thus Hs = (400/η0)e−j2xaz = 1.06e−j2xaz A/m. Inrealform, thefieldareE(x, t) = 400 cos(ωt−2x)ay andH(x, t) = 1.06 cos(ωt− 2x)az. Now P (r, t) = P (x, t) = E(x, t) × H(x, t) = 424.4 cos2(ωt − 2x)ax W/m2. b) Find P at t = 0 for r = (a, 5, 10), where a = 0,1,2, and 3: At t = 0, we find from part a, P (a, 0) = 424.4 cos2(2a), which leads to the values (in W/m2): 424.4 at a = 0, 73.5 at a = 1, 181.3 at a = 2, and 391.3 at a = 3. c) Find P at the origin for T = 0, 0.2T, 0.4T, and 0.6T , where T is the oscillation period. At the origin, we have P (0, t) = 424.4 cos2(ωt) = 424.4 cos2(2πt/T ). Using this, we obtain the following values (in W/m2): 424.4 at t = 0, 42.4 at t = 0.2T , 277.8 at t = 0.4T , and 277.8 at t = 0.6T . 11.19. Perfectly-conducting cylinders with radii of 8 mm and 20 mm are coaxial. The region between the cylinders is filled with a perfect dielectric for which ǫ = 10−9/4π F/m and µR = 1. If E in this region is (500/ρ) cos(ωt − 4z)aρ V/m, find: a) ω, with the help of Maxwell’s equations in cylindrical coordinates: We use the two curl equations, beginning with ∇ × E = −∂B/∂t, where in this case, ∇ × E = ∂Eρ ∂z aφ = 2000 ρ sin(ωt − 4z)aφ = − ∂Bφ ∂t aφ So Bφ = 2000 ρ sin(ωt − 4z)dt = 2000 ωρ cos(ωt − 4z) T Then Hφ = Bφ µ0 = 2000 (4π × 10−7)ωρ cos(ωt − 4z) A/m We next use ∇ × H = ∂D/∂t, where in this case ∇ × H = − ∂Hφ ∂z aρ + 1 ρ ∂(ρHφ) ∂ρ az where the second term on the right hand side becomes zero when substituting our Hφ. So ∇ × H = − ∂Hφ ∂z aρ = − 8000 (4π × 10−7)ωρ sin(ωt − 4z)aρ = ∂Dρ ∂t aρ And Dρ = − 8000 (4π × 10−7)ωρ sin(ωt − 4z)dt = 8000 (4π × 10−7)ω2ρ cos(ωt − 4z) C/m2 191 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 194. 11.19a. (continued) Finally, using the given ǫ, Eρ = Dρ ǫ = 8000 (10−16)ω2ρ cos(ωt − 4z) V/m This must be the same as the given field, so we require 8000 (10−16)ω2ρ = 500 ρ ⇒ ω = 4 × 108 rad/s b) H(ρ, z, t): From part a, we have H(ρ, z, t) = 2000 (4π × 10−7)ωρ cos(ωt − 4z)aφ = 4.0 ρ cos(4 × 108 t − 4z)aφ A/m c) P(ρ, φ, z): This will be P(ρ, φ, z) = E × H = 500 ρ cos(4 × 108 t − 4z)aρ × 4.0 ρ cos(4 × 108 t − 4z)aφ = 2.0 × 10−3 ρ2 cos2 (4 × 108 t − 4z)az W/m2 d) the average power passing through every cross-section 8 < ρ < 20 mm, 0 < φ < 2π. Using the result of part c, we find Pavg = (1.0 × 103)/ρ2az W/m2. The power through the given cross-section is now P = 2π 0 .020 .008 1.0 × 103 ρ2 ρ dρ dφ = 2π × 103 ln 20 8 = 5.7 kW 11.20. If Es = (60/r) sin θ e−j2r aθ V/m, and Hs = (1/4πr) sin θ e−j2r aφ A/m in free space, find the average power passing outward through the surface r = 106, 0 < θ < π/3, and 0 < φ < 2π. Pavg = 1 2 Re Es × H∗ s = 15 sin2 θ 2πr2 ar W/m2 Then, the requested power will be = 2π 0 π/3 0 15 sin2 θ 2πr2 ar · ar r2 sin θdθdφ = 15 π/3 0 sin3 θ dθ = 15 − 1 3 cos θ(sin2 θ + 2) π/3 0 = 25 8 = 3.13 W Note that the radial distance at the surface, r = 106 m, makes no difference, since the power density dimishes as 1/r2. 192 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 195. 11.21. The cylindrical shell, 1 cm < ρ < 1.2 cm, is composed of a conducting material for which σ = 106 S/m. The external and internal regions are non-conducting. Let Hφ = 2000 A/m at ρ = 1.2 cm. a) Find H everywhere: Use Ampere’s circuital law, which states: H · dL = 2πρ(2000) = 2π(1.2 × 10−2 )(2000) = 48π A = Iencl Then in this case J = I Area az = 48 (1.44 − 1.00) × 10−4 az = 1.09 × 106 az A/m2 With this result we again use Ampere’s circuital law to find H everywhere within the shell as a function of ρ (in meters): Hφ1(ρ) = 1 2πρ 2π 0 ρ .01 1.09 × 106 ρ dρ dφ = 54.5 ρ (104 ρ2 − 1) A/m (.01 < ρ < .012) Outside the shell, we would have Hφ2(ρ) = 48π 2πρ = 24/ρ A/m (ρ > .012) Inside the shell (ρ < .01 m), Hφ = 0 since there is no enclosed current. b) Find E everywhere: We use E = J σ = 1.09 × 106 106 az = 1.09 az V/m which is valid, presumeably, outside as well as inside the shell. c) Find P everywhere: Use P = E × H = 1.09 az × 54.5 ρ (104 ρ2 − 1) aφ = − 59.4 ρ (104 ρ2 − 1) aρ W/m2 (.01 < ρ < .012 m) Outside the shell, P = 1.09 az × 24 ρ aφ = − 26 ρ aρ W/m2 (ρ > .012 m) 193 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 196. 11.22. The inner and outer dimensions of a copper coaxial transmission line are 2 and 7 mm, respectively. Both conductors have thicknesses much greater than δ. The dielectric is lossless and the operating frequency is 400 MHz. Calculate the resistance per meter length of the: a) inner conductor: First δ = 1 √ πf µσ = 1 π(4 × 108)(4π × 10−7)(5.8 × 107) = 3.3 × 10−6 m = 3.3µm Now, using (70) with a unit length, we find Rin = 1 2πaσδ = 1 2π(2 × 10−3)(5.8 × 107)(3.3 × 10−6) = 0.42 ohms/m b) outer conductor: Again, (70) applies but with a different conductor radius. Thus Rout = a b Rin = 2 7 (0.42) = 0.12 ohms/m c) transmission line: Since the two resistances found above are in series, the line resistance is their sum, or R = Rin + Rout = 0.54 ohms/m. 11.23. A hollow tubular conductor is constructed from a type of brass having a conductivity of 1.2 × 107 S/m. The inner and outer radii are 9 mm and 10 mm respectively. Calculate the resistance per meter length at a frequency of a) dc: In this case the current density is uniform over the entire tube cross-section. We write: R(dc) = L σA = 1 (1.2 × 107)π(.012 − .0092) = 1.4 × 10−3 /m b) 20 MHz: Now the skin effect will limit the effective cross-section. At 20 MHz, the skin depth is δ(20MHz) = [πf µ0σ]−1/2 = [π(20 × 106 )(4π × 10−7 )(1.2 × 107 )]−1/2 = 3.25 × 10−5 m This is much less than the outer radius of the tube. Therefore we can approximate the resistance using the formula: R(20MHz) = L σA = 1 2πbδ = 1 (1.2 × 107)(2π(.01))(3.25 × 10−5) = 4.1 × 10−2 /m c) 2 GHz: Using the same formula as in part b, we find the skin depth at 2 GHz to be δ = 3.25×10−6 m. The resistance (using the other formula) is R(2GHz) = 4.1 × 10−1 /m. 194 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 197. 11.24a. Most microwave ovens operate at 2.45 GHz. Assume that σ = 1.2 × 106 S/m and µR = 500 for the stainless steel interior, and find the depth of penetration: δ = 1 √ πf µσ = 1 π(2.45 × 109)(4π × 10−7)(1.2 × 106) = 9.28 × 10−6 m = 9.28µm b) Let Es = 50 0◦ V/m at the surface of the conductor, and plot a curve of the amplitude of Es vs. the angle of Es as the field propagates into the stainless steel: Since the conductivity is high, we use (62) to write α . = β . = √ πf µσ = 1/δ. So, assuming that the direction into the conductor is z, the depth-dependent field is written as Es(z) = 50e−αz e−jβz = 50e−z/δ e−jz/δ = 50 exp(−z/9.28) amplitude exp(−j z/9.28 angle ) where z is in microns. Therefore, the plot of amplitude versus angle is simply a plot of e−x versus x, where x = z/9.28; the starting amplitude is 50 and the 1/e amplitude (at z = 9.28 µm) is 18.4. 11.25. A good conductor is planar in form and carries a uniform plane wave that has a wavelength of 0.3 mm and a velocity of 3 × 105 m/s. Assuming the conductor is non-magnetic, determine the frequency and the conductivity: First, we use f = v λ = 3 × 105 3 × 10−4 = 109 Hz = 1 GHz Next, for a good conductor, δ = λ 2π = 1 √ πf µσ ⇒ σ = 4π λ2f µ = 4π (9 × 10−8)(109)(4π × 10−7) = 1.1 × 105 S/m 11.26. The dimensions of a certain coaxial transmission line are a = 0.8mm and b = 4mm. The outer conductor thickness is 0.6mm, and all conductors have σ = 1.6 × 107 S/m. a) Find R, the resistance per unit length, at an operating frequency of 2.4 GHz: First δ = 1 √ πf µσ = 1 π(2.4 × 108)(4π × 10−7)(1.6 × 107) = 2.57 × 10−6 m = 2.57µm Then, using (70) with a unit length, we find Rin = 1 2πaσδ = 1 2π(0.8 × 10−3)(1.6 × 107)(2.57 × 10−6) = 4.84 ohms/m The outer conductor resistance is then found from the inner through Rout = a b Rin = 0.8 4 (4.84) = 0.97 ohms/m The net resistance per length is then the sum, R = Rin + Rout = 5.81 ohms/m. 195 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 198. 11.26b. Use information from Secs. 5.10 and 9.10 to find C and L, the capacitance and inductance per unit length, respectively. The coax is air-filled. From those sections, we find (in free space) C = 2πǫ0 ln(b/a) = 2π(8.854 × 10−12) ln(4/.8) = 3.46 × 10−11 F/m L = µ0 2π ln(b/a) = 4π × 10−7 2π ln(4/.8) = 3.22 × 10−7 H/m c) Find α and β if α + jβ = √ jωC(R + jωL): Taking real and imaginary parts of the given expression, we find α = Re jωC(R + jωL) = ω √ LC √ 2 1 + R ωL 2 − 1 1/2 and β = Im jωC(R + jωL) = ω √ LC √ 2 1 + R ωL 2 + 1 1/2 These can be found by writing out α = Re √ jωC(R + jωL) = (1/2) √ jωC(R + jωL)+c.c., wherec.c denotesthecomplexconjugate. Theresultissquared, termscollected, andthesquareroot taken. Now, using the values of R, C, and L found in parts a and b, we find α = 3.0 × 10−2 Np/m and β = 50.3 rad/m. 11.27. The planar surface at z = 0 is a brass-Teflon interface. Use data available in Appendix C to evaluate the following ratios for a uniform plane wave having ω = 4 × 1010 rad/s: a) αTef/αbrass: From the appendix we find ǫ′′/ǫ′ = .0003 for Teflon, making the material a good dielectric. Also, for Teflon, ǫ′ R = 2.1. For brass, we find σ = 1.5×107 S/m, making brass a good conductor at the stated frequency. For a good dielectric (Teflon) we use the approximations: α . = σ 2 µ ǫ′ = ǫ′′ ǫ′ 1 2 ω µǫ′ = 1 2 ǫ′′ ǫ′ ω c ǫ′ R β . = ω µǫ′ 1 + 1 8 ǫ′′ ǫ′ . = ω √ µǫ′ = ω c ǫ′ R For brass (good conductor) we have α . = β . = πf µσbrass = π 1 2π (4 × 1010)(4π × 10−7)(1.5 × 107) = 6.14 × 105 m−1 Now αTef αbrass = 1/2 ǫ′′/ǫ′ (ω/c) ǫ′ R √ πf µσbrass = (1/2)(.0003)(4 × 1010/3 × 108) √ 2.1 6.14 × 105 = 4.7 × 10−8 b) λTef λbrass = (2π/βTef) (2π/βbrass) = βbrass βTef = c √ πf µσbrass ω ǫ′ R Tef = (3 × 108)(6.14 × 105) (4 × 1010) √ 2.1 = 3.2 × 103 196 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 199. 11.27. (continued) c) vTef vbrass = (ω/βTef) (ω/βbrass) = βbrass βTef = 3.2 × 103 as before 11.28. A uniform plane wave in free space has electric field given by Es = 10e−jβxaz + 15e−jβxay V/m. a) Describe the wave polarization: Since the two components have a fixed phase difference (in this case zero) with respect to time and position, the wave has linear polarization, with the field vector in the yz plane at angle φ = tan−1(10/15) = 33.7◦ to the y axis. b) Find Hs: With propagation in forward x, we would have Hs = −10 377 e−jβx ay + 15 377 e−jβx az A/m = −26.5e−jβx ay + 39.8e−jβx az mA/m c) determine the average power density in the wave in W/m2: Use Pavg = 1 2 Re Es × H∗ s = 1 2 (10)2 377 ax + (15)2 377 ax = 0.43ax W/m2 or Pavg = 0.43 W/m2 11.29. Consider a left-circularly polarized wave in free space that propagates in the forward z direction. The electric field is given by the appropriate form of Eq. (80). a) Determine the magnetic field phasor, Hs: We begin, using (80), with Es = E0(ax + jay)e−jβz. We find the two components of Hs separately, using the two components of Es. Specifically, the x component of Es is associated with a y component of Hs, and the y component of Es is associated with a negative x component of Hs. The result is Hs = E0 η0 ay − jax e−jβz b) Determine an expression for the average power density in the wave in W/m2 by direct application of Eq. (57): We have Pz,avg = 1 2 Re(Es × H∗ s ) = 1 2 Re E0(ax + jay)e−jβz × E0 η0 (ay − jax)e+jβz = E2 0 η0 az W/m2 (assuming E0 is real) 197 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 200. 11.30. The electric field of a uniform plane wave in free space is given by Es = 10(ay + jaz)e−j25x. a) Determine the frequency, f : Use f = βc 2π = (25)(3 × 108) 2π = 1.2 GHz b) Find the magnetic field phasor, Hs: With the Poynting vector in the positive x direction, a positive y component for E requires a positive z component for H. Similarly, a positive z component for E requires a negative y component for H. Therefore, Hs = 10 η0 az − jay e−j25x c) Describe the polarization of the wave: This is most clearly seen by first converting the given field to real instantaneous form: E(x, t) = Re Esejωt = 10 cos(ωt − 25x)ay − sin(ωt − 25x)az At x = 0, this becomes, E(0, t) = 10 cos(ωt)ay − sin(ωt)az With the wave traveling in the forward x direction, we recognize the polarization as left circular. 11.31. A linearly-polarized uniform plane wave, propagating in the forward z direction, is input to a lossless anisotropic material, in which the dielectric constant encountered by waves polarized along y (ǫRy) differs from that seen by waves polarized along x (ǫRx). Suppose ǫRx = 2.15, ǫRy = 2.10, and the wave electric field at input is polarized at 45◦ to the positive x and y axes. Assume free space wavelength λ. a) Determine the shortest length of the material such that the wave as it emerges from the output end is circularly polarized: With the input field at 45◦, the x and y components are of equal magnitude, and circular polarization will result if the phase difference between the components is π/2. Our requirement over length L is thus βxL − βyL = π/2, or L = π 2(βx − βy) = πc 2ω( √ ǫRx − √ ǫRy) With the given values, we find, L = (58.3)πc 2ω = 58.3 λ 4 = 14.6 λ b) Will the output wave be right- or left-circularly-polarized? With the dielectric constant greater for x-polarized waves, the x component will lag the y component in time at the output. The field can thus be written as E = E0(ay − jax), which is left circular polarization. 198 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 201. 11.32. Suppose that the length of the medium of Problem 11.31 is made to be twice that as determined in the problem. Describe the polarization of the output wave in this case: With the length doubled, a phase shift of π radians develops between the two components. At the input, we can write the field as Es(0) = E0(ax + ay). After propagating through length L, we would have, Es(L) = E0[e−jβxL ax + e−jβyL ay] = E0e−jβxL [ax + e−j(βy−βx)L ay] where (βy − βx)L = −π (since βx > βy), and so Es(L) = E0e−jβxL[ax − ay]. With the reversal of the y component, the wave polarization is rotated by 90◦, but is still linear polarization. 11.33. Given a wave for which Es = 15e−jβzax +18e−jβzejφay V/m, propagating in a medium characterized by complex intrinsic impedance, η. a) Find Hs: With the wave propagating in the forward z direction, we find: Hs = 1 η −18ejφ ax + 15ay e−jβz A/m b) Determine the average power density in W/m2: We find Pz,avg = 1 2 Re Es × H∗ s = 1 2 Re (15)2 η∗ + (18)2 η∗ = 275 Re 1 η∗ W/m2 11.34. Given the general elliptically-polarized wave as per Eq. (73): Es = [Ex0ax + Ey0ejφ ay]e−jβz a) Show, using methods similar to those of Example 11.7, that a linearly polarized wave results when superimposing the given field and a phase-shifted field of the form: Es = [Ex0ax + Ey0e−jφ ay]e−jβz ejδ where δ is a constant: Adding the two fields gives Es,tot = Ex0 1 + ejδ ax + Ey0 ejφ + e−jφ ejδ ay e−jβz = Ex0ejδ/2 e−jδ/2 + ejδ/2 2 cos(δ/2) ax + Ey0ejδ/2 e−jδ/2 ejφ + e−jφ ejδ/2 2 cos(φ−δ/2) ay e−jβz This simplifies to Es,tot = 2 Ex0 cos(δ/2)ax + Ey0 cos(φ − δ/2)ay ejδ/2e−jβz, which is lin- early polarized. b) Find δ in terms of φ such that the resultant wave is polarized along x: By inspecting the part a result, we achieve a zero y component when 2φ − δ = π (or odd multiples of π). 199 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 202. CHAPTER 12 12.1. A uniform plane wave in air, E+ x1 = E+ x10 cos(1010t −βz)V/m, is normally-incident on a copper surface at z = 0. What percentage of the incident power density is transmitted into the copper? We need to find the reflection coefficient. The intrinsic impedance of copper (a good conductor) is ηc = jωµ σ = (1 + j) ωµ 2σ = (1 + j) 1010(4π × 107) 2(5.8 × 107) = (1 + j)(.0104) Note that the accuracy here is questionable, since we know the conductivity to only two significant figures. We nevertheless proceed: Using η0 = 376.7288 ohms, we write Ŵ = ηc − η0 ηc + η0 = .0104 − 376.7288 + j.0104 .0104 + 376.7288 + j.0104 = −.9999 + j.0001 Now |Ŵ|2 = .9999, and so the transmitted power fraction is 1 − |Ŵ|2 = .0001, or about 0.01% is transmitted. 12.2. The plane y = 0 defines the boundary between two different dielectrics. For y < 0, ǫ′ R1 = 1, µ1 = µ0, and ǫ′′ R1 = 0; and for y > 0, ǫ′ R2 = 5, µ2 = µ0, and ǫ′′ R2 = 0. Let E+ z1 = 150 cos(ωt − 8y) V/m, and find a) ω: Have β = 8 = ω/c ⇒ ω = 8c = 2.4 × 109 sec−1. b) H+ 1 : With E in the z direction, and propagation in the forward y direction, H will lie in the positive x direction, and its amplitude will be Hx = Ey/η0 in region 1. Thus H+ 1 = (150/η0) cos(ωt − 8y)ax = 0.40 cos(2.4 × 109t − 8y)ax A/m. c) H− 1 : First, E− z1 = ŴE+ z1 = η0/ √ 5 − η0/1 η0/ √ 5 + η0/1 = 1 − √ 5 1 + √ 5 E+ z1 = −0.38E+ z1 Then H− x1 = +(0.38/η0)E+ z1 = 0.38(150) 377 cos(ωt + 8y) So finally, H− x1 = 0.15 cos(2.4 × 109t + 8y)ax A/m. 12.3. A uniform plane wave in region 1 is normally-incident on the planar boundary separating regions 1 and 2. If ǫ′′ 1 = ǫ′′ 2 = 0, while ǫ′ R1 = µ3 R1 and ǫ′ R2 = µ3 R2, find the ratio ǫ′ R2/ǫ′ R1 if 20% of the energy in the incident wave is reflected at the boundary. There are two possible answers. First, since |Ŵ|2 = .20, and since both permittivities and permeabilities are real, Ŵ = ±0.447. we then set up Ŵ = ±0.447 = η2 − η1 η2 + η1 = η0 (µR2/ǫ′ R2) − η0 (µR1/ǫ′ R1) η0 (µR2/ǫ′ R2) + η0 (µR1/ǫ′ R1) = (µR2/µ3 R2) − (µR1/µ3 R1) (µR2/µ3 R2) + (µR1/µ3 R1) = µR1 − µR2 µR1 + µR2 200 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 203. 12.3. (continued) Therefore µR2 µR1 = 1 ∓ 0.447 1 ± 0.447 = (0.382, 2.62) ⇒ ǫ′ R2 ǫ′ R1 = µR2 µR1 3 = (0.056, 17.9) 12.4. The magnetic field intensity in a region where ǫ′′ = 0 is given as H = 5 cos ωt cos βz ay A/m, where ω = 5 Grad/s and β = 30 rad/m. If the amplitude of the associated electric field intensity is 2kV/m, find a) µ and ǫ′ for the medium: In phasor form, the magnetic field is Hys = H0e−jβz + H0e+βz = 5 cos βz ⇒ H0 = 2.5. The electric field will be x directed, and is Exs = η(2.5)e−jβz − η(2.5)e+jβz = (2j)η(2.5) sin βz. Given the electric field amplitude of 2 kV/m, we write 2×103 = 5η, or η = 400 . Now η = 400 = η0 µr/ǫ′ R and we also have β = 30 = (ω/c) µRǫ′ R. We solve these two equations simultaneously for µR and ǫ′ R to find µR = 1.91 and ǫ′ R = 1.70. Therefore µ = 1.91 × 4π × 10−7 = 2.40 µH/m and ǫ′ = 1.70 × 8.854 × 10−12 = 15.1 pF/m. b) E: From part a, electric field in phasor form is Exs = j2 sin βz kV/m, and so, in real form: E(z, t) = Re(Exsejωt )ax = 2 sin βz sin ωt ax kV/m with ω and β as given. 12.5. The region z < 0 is characterized by ǫ′ R = µR = 1 and ǫ′′ R = 0. The total E field here is given as the sum of the two uniform plane waves, Es = 150e−j10z ax + (50 20◦)ej10z ax V/m. a) What is the operating frequency? In free space, β = k0 = 10 = ω/c = ω/3 × 108. Thus, ω = 3 × 109 s−1, or f = ω/2π = 4.7 × 108 Hz. b) Specify the intrinsic impedance of the region z > 0 that would provide the appropriate reflected wave: Use Ŵ = Er Einc = 50ej20◦ 150 = 1 3 ej20◦ = 0.31 + j0.11 = η − η0 η + η0 Now η = η0 1 + Ŵ 1 − Ŵ = 377 1 + 0.31 + j0.11 1 − 0.31 − j0.31 = 691 + j177 c) At what value of z (−10 cm < z < 0) is the total electric field intensity a maximum amplitude? We found the phase of the reflection coefficient to be φ = 20◦ = .349rad, and we use zmax = −φ 2β = −.349 20 = −0.017 m = −1.7 cm 12.6. Region 1, z < 0, and region 2, z > 0, are described by the following parameters: ǫ′ 1 = 100 pF/m, µ1 = 25 µH/m, ǫ′′ 1 = 0, ǫ′ 2 = 200 pF/m, µ2 = 50 µH/m, and ǫ′′ 2 /ǫ′ 2 = 0.5. If E+ 1 = 600e−α1z cos(5 × 1010t − β1z)ax V/m, find: a) α1: From Eq. (35), Chapter 11, we note that since ǫ′′ 1 = 0, it follows that α1 = 0. b) β1: β1 = ω µ1ǫ′ 1 = (5 × 1010) (25 × 10−6)(100 × 10−12) = 2.50 × 103 rad/m. c) E+ s1 = 600e−j2.50×103zax V/m. d) E− s1: To find this, we need to evaluate the reflection coefficient, which means that we first need the two intrinsic impedances. First, η1 = µ1/ǫ′ 1 = (25 × 10−6)/(100 × 10−12) = 500. 201 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 204. 12.6d) (continued) Next, using Eq. (39), Chapter 11, η2 = µ2 ǫ′ 2 1 1 − j(ǫ′′ 2 /ǫ′ 2) = 50 × 10−6 2 × 10−10 1 √ 1 − j0.5 = 460 + j109 Then Ŵ = η2 − η1 η2 + η1 = 460 + j109 − 500 460 + j109 + 500 = −2.83 × 10−2 + j1.16 × 10−1 = 0.120ej104◦ Now we multiply E+ s1 by Ŵ and reverse the propagation direction to obtain E− s1 = 71.8ej104◦ ej2.5×103z V/m e) E+ s2: This wave will experience loss in region 2, along with a different phase constant. We need to evaluate α2 and β2. First, using Eq. (35), Chapter 11, α2 = ω µ2ǫ′ 2 2 1 + ǫ′′ 2 ǫ′ 2 2 − 1 1/2 = (5 × 1010 ) (50 × 106)(200 × 10−12) 2 1 + (0.5)2 − 1 1/2 = 1.21 × 103 Np/m Then, using Eq. (36), Chapter 11, β2 = ω µ2ǫ′ 2 2 1 + ǫ′′ 2 ǫ′ 2 2 + 1 1/2 = 5.15 × 103 rad/m Then, the transmission coefficient will be τ = 1 + Ŵ = 1 − 2.83 × 10−2 + j1.16 × 10−1 = 0.972ej7◦ The complex amplitude of E+ s2 is then found by multiplying the amplitude of E+ s1 by τ. The field in region 2 is then constructed by using the resulting amplitude, along with the attenuation and phase constants that are appropriate for region 2. The result is E+ s2 = 587e−1.21×103z ej7◦ e−j5.15×103z V/m 12.7. The semi-infinite regions z < 0 and z > 1 m are free space. For 0 < z < 1 m, ǫ′ R = 4, µR = 1, and ǫ′′ R = 0. A uniform plane wave with ω = 4 × 108 rad/s is travelling in the az direction toward the interface at z = 0. a) Find the standing wave ratio in each of the three regions: First we find the phase constant in the middle region, β2 = ω ǫ′ R c = 2(4 × 108) 3 × 108 = 2.67 rad/m 202 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 205. 12.7a. (continued) Then, withthemiddlelayerthicknessof1m, β2d = 2.67 rad. Also, theintrinsicimpedance of the middle layer is η2 = η0/ ǫ′ R = η0/2. We now find the input impedance: ηin = η2 η0 cos(β2d) + jη2 sin(β2d) η2 cos(β2d) + jη0 sin(β2d) = 377 2 2 cos(2.67) + j sin(2.67) cos(2.67) + j2 sin(2.67) = 231 + j141 Now, at the first interface, Ŵ12 = ηin − η0 ηin + η0 = 231 + j141 − 377 231 + j141 + 377 = −.176 + j.273 = .325 123◦ The standing wave ratio measured in region 1 is thus s1 = 1 + |Ŵ12| 1 − |Ŵ12| = 1 + 0.325 1 − 0.325 = 1.96 In region 2 the standing wave ratio is found by considering the reflection coefficient for waves incident from region 2 on the second interface: Ŵ23 = η0 − η0/2 η0 + η0/2 = 1 − 1/2 1 + 1/2 = 1 3 Then s2 = 1 + 1/3 1 − 1/3 = 2 Finally, s3 = 1, since no reflected waves exist in region 3. b) Find the location of the maximum |E| for z < 0 that is nearest to z = 0. We note that the phase of Ŵ12 is φ = 123◦ = 2.15 rad. Thus zmax = −φ 2β = −2.15 2(4/3) = −.81 m 12.8. A wave starts at point a, propagates 100m through a lossy dielectric for which α = 0.5 Np/m, reflects at normal incidence at a boundary at which Ŵ = 0.3 + j0.4, and then returns to point a. Calculate the ratio of the final power to the incident power after this round trip: Final power, Pf , and incident power, Pi, are related through Pf = Pie−2αL |Ŵ|2 e−2αL ⇒ Pf Pi = |0.3 + j0.4|2 e−2(0.5)100 = 3.5 × 10−88 (!) Try measuring that. 12.9. Region 1, z < 0, and region 2, z > 0, are both perfect dielectrics (µ = µ0, ǫ′′ = 0). A uniform plane wave traveling in the az direction has a radian frequency of 3 × 1010 rad/s. Its wavelengths in the two regions are λ1 = 5 cm and λ2 = 3 cm. What percentage of the energy incident on the boundary is a) reflected; We first note that ǫ′ R1 = 2πc λ1ω 2 and ǫ′ R2 = 2πc λ2ω 2 203 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 206. 12.9a. (continued) Therefore ǫ′ R1/ǫ′ R2 = (λ2/λ1)2. Then with µ = µ0 in both regions, we find Ŵ = η2 − η1 η2 + η1 = η0 1/ǫ′ R2 − η0 1/ǫ′ R1 η0 1/ǫ′ R2 + η0 1/ǫ′ R1 = ǫ′ R1/ǫ′ R2 − 1 ǫ′ R1/ǫ′ R2 + 1 = (λ2/λ1) − 1 (λ2/λ1) + 1 = λ2 − λ1 λ2 + λ1 = 3 − 5 3 + 5 = − 1 4 The fraction of the incident energy that is reflected is then |Ŵ|2 = 1/16 = 6.25 × 10−2. b) transmitted? We use part a and find the transmitted fraction to be 1 − |Ŵ|2 = 15/16 = 0.938. c) What is the standing wave ratio in region 1? Use s = 1 + |Ŵ| 1 − |Ŵ| = 1 + 1/4 1 − 1/4 = 5 3 = 1.67 12.10. In Fig. 12.1, let region 2 be free space, while µR1 = 1, ǫ′′ R1 = 0, and ǫ′ R1 is unknown. Find ǫ′ R! if a) the amplitude of E− 1 is one-half that of E+ 1 : Since region 2 is free space, the reflection coefficient is Ŵ = |E− 1 | |E+ 1 | = η0 − η1 η0 + η1 = η0 − η0/ ǫ′ R1 η0 + η0/ ǫ′ R1 = ǫ′ R1 − 1 ǫ′ R1 + 1 = 1 2 ⇒ ǫ′ R1 = 9 . b) P − 1,avg is one-half of P + 1,avg: This time |Ŵ|2 = ǫ′ R1 − 1 ǫ′ R1 + 1 2 = 1 2 ⇒ ǫ′ R1 = 34 c) |E1|min is one-half |E1|max: Use |E1|max |E1|min = s = 1 + |Ŵ| 1 − |Ŵ| = 2 ⇒ |Ŵ| = Ŵ = 1 3 = ǫ′ R1 − 1 ǫ′ R1 + 1 ⇒ ǫ′ R1 = 4 12.11. A 150 MHz uniform plane wave in normally-incident from air onto a material whose intrinsic impedance is unknown. Measurements yield a standing wave ratio of 3 and the appearance of an electric field minimum at 0.3 wavelengths in front of the interface. Determine the impedance of the unknown material: First, the field minimum is used to find the phase of the reflection coefficient, where zmin = − 1 2β (φ + π) = −0.3λ ⇒ φ = 0.2π where β = 2π/λ has been used. Next, |Ŵ| = s − 1 s + 1 = 3 − 1 3 + 1 = 1 2 204 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 207. 12.11. (continued) So we now have Ŵ = 0.5ej0.2π = ηu − η0 ηu + η0 We solve for ηu to find ηu = η0(1.70 + j1.33) = 641 + j501 12.12. A 50MHz uniform plane wave is normally incident from air onto the surface of a calm ocean. For seawater, σ = 4 S/m, and ǫ′ R = 78. a) Determine the fractions of the incident power that are reflected and transmitted: First we find the loss tangent: σ ωǫ′ = 4 2π(50 × 106)(78)(8.854 × 10−12) = 18.4 This value is sufficiently greater than 1 to enable seawater to be considered a good conductor at 50MHz. Then, using the approximation (Eq. 65, Chapter 11), the intrinsic impedance is ηs = √ πf µ/σ(1 + j), and the reflection coefficient becomes Ŵ = √ πf µ/σ (1 + j) − η0 √ πf µ/σ (1 + j) + η0 where √ πf µ/σ = π(50 × 106)(4π × 10−7)/4 = 7.0. The fraction of the power reflected is Pr Pi = |Ŵ|2 = [ √ πf µ/σ − η0]2 + πf µ/σ [ √ πf µ/σ + η0]2 + πf µ/σ = [7.0 − 377]2 + 49.0 [7.0 + 377]2 + 49.0 = 0.93 The transmitted fraction is then Pt Pi = 1 − |Ŵ|2 = 1 − 0.93 = 0.07 b) Qualitatively, how will these answers change (if at all) as the frequency is increased? Within the limits of our good conductor approximation (loss tangent greater than about ten), the reflected power fraction, using the formula derived in part a, is found to decrease with increasing frequency. The transmitted power fraction thus increases. 12.13. A right-circularly-polarized plane wave is normally incident from air onto a semi-infinite slab of plex- iglas (ǫ′ R = 3.45, ǫ′′ R = 0). Calculate the fractions of the incident power that are reflected and trans- mitted. Also, describe the polarizations of the reflected and transmitted waves. First, the impedance of the plexiglas will be η = η0/ √ 3.45 = 203 . Then Ŵ = 203 − 377 203 + 377 = −0.30 The reflected power fraction is thus |Ŵ|2 = 0.09. The total electric field in the plane of the interface must rotate in the same direction as the incident field, in order to continually satisfy the boundary condition of tangential electric field continuity across the interface. Therefore, the reflected wave will have to be left circularly polarized in order to make this happen. The transmitted power fraction is now 1 − |Ŵ|2 = 0.91. The transmitted field will be right circularly polarized (as the incident field) for the same reasons. 205 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 208. 12.14. A left-circularly-polarized plane wave is normally-incident onto the surface of a perfect conductor. a) Construct the superposition of the incident and reflected waves in phasor form: Assume positive z travel for the incident electric field. Then, with reflection coefficient, Ŵ = −1, the incident and reflected fields will add to give the total field: Etot = Ei + Er = E0(ax + jay)e−jβz − E0(ax + jay)e+jβz = E0 e−jβz − ejβz −2j sin(βz) ax + j e−jβz − ejβz −2j sin(βz) ay = 2E0 sin(βz) ay − jax b) Determine the real instantaneous form of the result of part a: E(z, t) = Re Etot ejωt = 2E0 sin(βz) cos(ωt)ay + sin(ωt)ax c) Describe the wave that is formed: This is a standing wave exhibiting circular polarization in time. At each location along the z axis, the field vector rotates clockwise in the xy plane, and has amplitude (constant with time) given by 2E0 sin(βz). 12.15. Consider these regions in which ǫ′′ = 0: region 1, z < 0, µ1 = 4 µH/m and ǫ′ 1 = 10 pF/m; region 2, 0 < z < 6 cm, µ2 = 2 µH/m, ǫ′ 2 = 25 pF/m; region 3, z > 6 cm, µ3 = µ1 and ǫ′ 3 = ǫ′ 1. a) What is the lowest frequency at which a uniform plane wave incident from region 1 onto the boundary at z = 0 will have no reflection? This frequency gives the condition β2d = π, where d = 6 cm, and β2 = ω µ2ǫ′ 2 Therefore β2d = π ⇒ ω = π (.06) µ2ǫ′ 2 ⇒ f = 1 0.12 (2 × 10−6)(25 × 10−12) = 1.2 GHz b) If f = 50 MHz, what will the standing wave ratio be in region 1? At the given frequency, β2 = (2π × 5 × 107) (2 × 10−6)(25 × 10−12) = 2.22 rad/m. Thus β2d = 2.22(.06) = 0.133. The intrinsic impedance of regions 1 and 3 is η1 = η3 = (4 × 10−6)/(10−11) = 632 . The input impedance at the first interface is now ηin = 283 632 cos(.133) + j283 sin(.133) 283 cos(.133) + j632 sin(.133) = 589 − j138 = 605 − .23 The reflection coefficient is now Ŵ = ηin − η1 ηin + η1 = 589 − j138 − 632 589 − j138 + 632 = .12 − 1.7 The standing wave ratio is now s = 1 + |Ŵ| 1 − |Ŵ| = 1 + .12 1 − .12 = 1.27 12.16. A uniform plane wave in air is normally-incident onto a lossless dielectric plate of thickness λ/8, and of intrinsic impedance η = 260 . Determine the standing wave ratio in front of the plate. Also find the fraction of the incident power that is transmitted to the other side of the plate: With the a thickness of λ/8, we have βd = π/4, and so cos(βd) = sin(βd) = 1 √ 2. The input impedance thus becomes ηin = 260 377 + j260 260 + j377 = 243 − j92 206 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 209. 12.16. (continued) The reflection coefficient is then Ŵ = (243 − j92) − 377 (243 − j92) + 377 = −0.19 − j0.18 = 0.26 − 2.4rad Therefore s = 1 + .26 1 − .26 = 1.7 and 1 − |Ŵ|2 = 1 − (.26)2 = 0.93 12.17. Repeat Problem 12.16 for the cases in which the frequency is a) doubled: If this is true, then d = λ/4, and thus ηin = (260)2/377 = 179. The reflection coefficient becomes Ŵ = 179 − 377 179 + 377 = −0.36 ⇒ s = 1 + .36 1 − .36 = 2.13 Then 1 − |Ŵ|2 = 1 − (.36)2 = 0.87. b) quadrupled: Now, d = λ/2, and so we have a half-wave section surrounded by air. Transmission will be total, and so s = 1 and 1 − |Ŵ|2 = 1. 12.18. In Fig. 12.6, let η1 = η3 = 377 , and η2 = 0.4η1. A uniform plane wave is normally incident from the left, as shown. Plot a curve of the standing wave ratio, s, in the region to the left: a) as a function of l if f = 2.5GHz: With η1 = η3 = η0 and with η2 = 0.4η0, Eq. (41) becomes ηin = 0.4η0 cos(βl) + j0.4 sin(βl) 0.4 cos(βl) + j sin(βl) × 0.4 cos(βl) − j sin(βl) 0.4 cos(βl) − j sin(βl) = η0 1 − j1.05 sin(2βl) cos2(βl) + 6.25 sin2(βl) Then Ŵ = (ηin − η0)/(ηin + η0), from which we find |Ŵ| = √ ŴŴ∗ = 1 − cos2(βl) − 6.25 sin2(βl) 2 + (1.05)2 sin2(2βl) 1 + cos2(βl) + 6.25 sin2(βl) 2 + (1.05)2 sin2(2βl) 1/2 Then s = (1 + |Ŵ|)/(1 − |Ŵ|). Now for a uniform plane wave, β = ω √ µǫ = nω/c. Given that η2 = 0.4η0 = η0/n, we find n = 2.5 (assuming µ = µ0). Thus, at 2.5 GHz, βl = nω c l = (2.5)(2π)(2.5 × 109) 3 × 108 l = 12.95 l (l in m) = 0.1295 l (l in cm) Using this in the expression for |Ŵ|, and calculating s as a function of l in cm leads to the first plot shown on the next page. b) as a function of frequency if l = 2cm. In this case we use βl = (2.5)(2π)(0.02) 3 × 108 f = 1.04 × 10−10 f (f in Hz) = 0.104 f (f in GHz) Using this in the expression for |Ŵ|, and calculating s as a function of f in GHz leads to the second plot shown on the next page. MathCad was used in both cases. 207 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 210. 12.18 (continued) Plots for parts a and b 12.19. You are given four slabs of lossless dielectric, all with the same intrinsic impedance, η, known to be different from that of free space. The thickness of each slab is λ/4, where λ is the wavelength as measured in the slab material. The slabs are to be positioned parallel to one another, and the combination lies in the path of a uniform plane wave, normally-incident. The slabs are to be arranged such that the air spaces between them are either zero, one-quarter wavelength, or one-half wavelength in thickness. Specify an arrangement of slabs and air spaces such that a) the wave is totally transmitted through the stack: In this case, we look for a combination of half- wavesections. Lettheinter-slabdistancesbed1, d2, andd3 (fromlefttoright). Twopossibilitiesare i.) d1 = d2 = d3 = 0, thus creating a single section of thickness λ, or ii.) d1 = d3 = 0, d2 = λ/2, thus yielding two half-wave sections separated by a half-wavelength. b) the stack presents the highest reflectivity to the incident wave: The best choice here is to make d1 = d2 = d3 = λ/4. Thus every thickness is one-quarter wavelength. The impedances transform as follows: First, the input impedance at the front surface of the last slab (slab 4) is ηin,1 = η2/η0. We transform this back to the back surface of slab 3, moving through a distance of λ/4 in free space: ηin,2 = η2 0/ηin,1 = η3 0/η2. We next transform this impedance to the front surface of slab 3, producing ηin,3 = η2/ηin,2 = η4/η3 0. We continue in this manner until reaching the front surface of slab 1, where we find ηin,7 = η8/η7 0. Assuming η < η0, the ratio ηn/ηn−1 0 becomes smaller as n increases (as the number of slabs increases). The reflection coefficient for waves incident on the front slab thus gets close to unity, and approaches 1 as the number of slabs approaches infinity. 12.20. The 50MHz plane wave of Problem 12.12 is incident onto the ocean surface at an angle to the normal of 60◦. Determine the fractions of the incident power that are reflected and transmitted for a) s polarization: To review Problem 12, we first we find the loss tangent: σ ωǫ′ = 4 2π(50 × 106)(78)(8.854 × 10−12) = 18.4 This value is sufficiently greater than 1 to enable seawater to be considered a good conductor at 50MHz. Then, using the approximation (Eq. 65, Chapter 11), and with µ = µ0, the intrinsic impedance is ηs = √ πf µ/σ(1 + j) = 7.0(1 + j). 208 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 211. 12.20a. (continued) Next we need the angle of refraction, which means that we need to know the refractive index of seawater at 50MHz. For a uniform plane wave in a good conductor, the phase constant is β = nsea ω c . = πf µσ ⇒ nsea . = c µσ 4πf = 26.8 Then, using Snell’s law, the angle of refraction is found: sin θ2 = nsea n1 sin θ1 = 26.8 sin(60◦ ) ⇒ θ2 = 1.9◦ This angle is small enough so that cos θ2 . = 1. Therefore, for s polarization, Ŵs . = ηs2 − ηs1 ηs2 + ηs1 = 7.0(1 + j) − 377/ cos 60◦ 7.0(1 + j) + 377/ cos 60◦ = −0.98 + j0.018 = 0.98 179◦ The fraction of the power reflected is now |Ŵs|2 = 0.96. The fraction transmitted is then 0.04. b) p polarization: Again, with the refracted angle close to zero, the relection coefficient for p polar- ization is Ŵp . = ηp2 − ηp1 ηp2 + ηp1 = 7.0(1 + j) − 377 cos 60◦ 7.0(1 + j) + 377 cos 60◦ = −0.93 + j0.069 = 0.93 176◦ The fraction of the power reflected is now |Ŵp|2 = 0.86. The fraction transmitted is then 0.14. 12.21. A right-circularly polarized plane wave in air is incident at Brewster’s angle onto a semi-infinite slab of plexiglas (ǫ′ R = 3.45, ǫ′′ R = 0, µ = µ0). a) Determine the fractions of the incident power that are reflected and transmitted: In plexiglas, Brewster’s angle is θB = θ1 = tan−1(ǫ′ R2/ǫ′ R1) = tan−1( √ 3.45) = 61.7◦. Then the angle of refraction is θ2 = 90◦ − θB (see Example 12.9), or θ2 = 28.3◦. With incidence at Brewster’s angle, all p-polarized power will be transmitted — only s-polarized power will be reflected. This is found through Ŵs = η2s − η1s η2s + η1s = .614η0 − 2.11η0 .614η0 + 2.11η0 = −0.549 where η1s = η1 sec θ1 = η0 sec(61.7◦) = 2.11η0, and η2s = η2 sec θ2 = (η0/ √ 3.45) sec(28.3◦) = 0.614η0. Now, the reflected power fraction is |Ŵ|2 = (−.549)2 = .302. Since the wave is circularly-polarized, the s-polarized component represents one-half the total incident wave power, and so the fraction of the total power that is reflected is .302/2 = 0.15, or 15%. The fraction of the incident power that is transmitted is then the remainder, or 85%. b) Describe the polarizations of the reflected and transmitted waves: Since all the p-polarized com- ponent is transmitted, the reflected wave will be entirely s-polarized (linear). The transmitted wave, while having all the incident p-polarized power, will have a reduced s-component, and so this wave will be right-elliptically polarized. 209 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 212. 12.22. A dielectric waveguide is shown in Fig. 12.18 with refractive indices as labeled. Incident light enters the guide at angle φ from the front surface normal as shown. Once inside, the light totally reflects at the upper n1 − n2 interface, where n1 > n2. All subsequent reflections from the upper an lower boundaries will be total as well, and so the light is confined to the guide. Express, in terms of n1 and n2, the maximum value of φ such that total confinement will occur, with n0 = 1. The quantity sin φ is known as the numerical aperture of the guide. From the illustration we see that φ1 maximizes when θ1 is at its minimum value. This minimum will be the critical angle for the n1 − n2 interface, where sin θc = sin θ1 = n2/n1. Let the refracted angle to the right of the vertical interface (not shown) be φ2, where n0 sin φ1 = n1 sin φ2. Then we see that φ2 + θ1 = 90◦, and so sin θ1 = cos φ2. Now, the numerical aperture becomes sin φ1max = n1 n0 sin φ2 = n1 cos θ1 = n1 1 − sin2 θ1 = n1 1 − (n2/n1)2 = n2 1 − n2 2 Finally, φ1max = sin−1 n2 1 − n2 2 is the numerical aperture angle. 12.23. Suppose that φ1 in Fig. 12.18 is Brewster’s angle, and that θ1 is the critical angle. Find n0 in terms of n1 and n2: With the incoming ray at Brewster’s angle, the refracted angle of this ray (measured from the inside normal to the front surface) will be 90◦ − φ1. Therefore, φ1 = θ1, and thus sin φ1 = sin θ1. Thus sin φ1 = n1 n2 0 + n2 1 = sin θ1 = n2 n1 ⇒ n0 = (n1/n2) n2 1 − n2 2 Alternatively, we could have used the result of Problem 12.22, in which it was found that sin φ1 = (1/n0) n2 1 − n2 2, which we then set equal to sin θ1 = n2/n1 to get the same result. 12.24. A Brewster prism is designed to pass p-polarized light without any reflective loss. The prism of Fig. 12.19 is made of glass (n = 1.45), and is in air. Considering the light path shown, determine the apex angle, α: With entrance and exit rays at Brewster’s angle (to eliminate reflective loss), the interior ray must be horizontal, or parallel to the bottom surface of the prism. From the geometry, the angle between the interior ray and the normal to the prism surfaces that it intersects is α/2. Since this angle is also Brewster’s angle, we may write: α = 2 sin−1 1 √ 1 + n2 = 2 sin−1 1 1 + (1.45)2 = 1.21 rad = 69.2◦ 12.25. In the Brewster prism of Fig. 12.19, determine for s-polarized light the fraction of the incident power that is transmitted through the prism: We use Ŵs = (ηs2 − ηs1)/(ηs2 + ηs1), where ηs2 = η2 cos(θB2) = η2 n/ √ 1 + n2 = η0 n2 1 + n2 and ηs1 = η1 cos(θB1) = η1 1/ √ 1 + n2 = η0 1 + n2 210 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 213. 12.25. (continued) Thus, at the first interface, Ŵ = (1−n2)/(1+n2). At the second interface, Ŵ will be equal but of opposite sign to the above value. The power transmission coefficient through each interface is 1 − |Ŵ|2, so that for both interfaces, we have, with n = 1.45: Ptr Pinc = 1 − |Ŵ|2 2 = 1 − n2 − 1 n2 + 1 2 2 = 0.76 12.26. Show how a single block of glass can be used to turn a p-polarized beam of iight through 180◦, with the light suffering, in principle, zero reflective loss. The light is incident from air, and the returning beam (also in air) may be displaced sideways from the incident beam. Specify all pertinent angles and use n = 1.45 for glass. More than one design is possible here. The prism below is designed such that light enters at Brewster’s angle, and once inside, is turned around using total reflection. Using the result of Example 12.9, we find that with glass, θB = 55.4◦, which, by the geometry, is also the incident angle for total reflection at the back of the prism. For this to work, the Brewster angle must be greater than or equal to the critical angle. This is in fact the case, since θc = sin−1(n2/n1) = sin−1(1/1.45) = 43.6◦. 12.27. Using Eq. (59) in Chapter 11 as a starting point, determine the ratio of the group and phase velocities of an electromagnetic wave in a good conductor. Assume conductivity does not vary with frequency: In a good conductor: β = πf µσ = ωµσ 2 → dβ dω = 1 2 ωµσ 2 −1/2 µσ 2 Thus dω dβ = dβ dω −1 = 2 2ω µσ = vg and vp = ω β = ω √ ωµσ/2 = 2ω µσ Therefore vg/vp = 2. 211 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 214. 12.28. Over a certain frequency range, the refractive index of a certain material varies approximately linearly with frequency: n(ω) . = na + nb(ω − ωa), where na, nb, and ωa are constants. Using β = nω/c: a) determine the group velocity as a function (or perhaps not a function) of frequency: vg = (dβ/dω)−1, where dβ dω = d dω naω c + nb(ω − ωa)ω c = 1 c [na + nb(2ω − ωa)] so that vg(ω) = c [na + nb(2ω − ωa)]−1 b) determine the group dispersion parameter, β2: β2 = d2β dω2 ω0 = d dω 1 c [na + nb(2ω − ωa)] ω0 = 2nb/c c) Discuss the implications of these results, if any, on pulse broadening: The point of this problem was to show that higher order terms (involving d3β/dω3 and higher) in the Taylor series expansion, Eq. (89), do not exist if the refractive index varies linearly with ω. These higher order terms would be necessary in cases involving pulses of exremely large bandwidth, or in media exhibiting complicated variations in their ω-β curves over relatively small frequency ranges. With d2β/dω2 constant, the three-term Taylor expansion of Eq. (89) describes the phase constant of this medium exactly. The pulse will broaden and will acquire a frequency sweep (chirp) that is precisely linear with time. Additionally, a pulse of a given bandwidth will broaden by the same amount, regardless of what carrier frequency is used. 12.29. A T = 5 ps transform-limited pulse propagates in a dispersive channel for which β2 = 10 ps2/km. Over what distance will the pulse spread to twice its initial width? After propagation, the width is T ′ = T 2 + ( τ)2 = 2T . Thus τ = √ 3T , where τ = β2z/T . Therefore β2z T = √ 3T or z = √ 3T 2 β2 = √ 3(5 ps)2 10 ps2/km = 4.3 km 12.30. A T = 20 ps transform-limited pulse propagates through 10 km of a dispersive channel for which β2 = 12 ps2/km. The pulse then propagates through a second 10 km channel for which β2 = −12 ps2/km. Describe the pulse at the output of the second channel and give a physical explanation for what hap- pened. Our theory of pulse spreading will allow for changes in β2 down the length of the channel. In fact, we may write in general: τ = 1 T L 0 β2(z) dz Having β2 change sign at the midpoint, yields a zero τ, and so the pulse emerges from the output unchanged! Physically, the pulse acquires a positive linear chirp (frequency increases with time over the pulse envelope) during the first half of the channel. When β2 switches sign, the pulse begins to acquire a negative chirp in the second half, which, over an equal distance, will completely eliminate the chirp acquired during the first half. The pulse, if originally transform-limited at input, will emerge, again transform-limited, at its original width. More generally, complete dispersion compensation is achieved using a two-segment channel when β2L = −β′ 2L′, assuming dispersion terms of higher order than β2 do not exist. 212 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 215. CHAPTER 13 13.1. The parameters of a certain transmission line operating at 6 × 108 rad/s are L = 0.4 µH/m, C = 40 pF/m, G = 80 mS/m, and R = 20 /m. a) Find γ , α, β, λ, and Z0: We use γ = √ ZY = (R + jωL)(G + jωC) = [20 + j(6 × 108)(0.4 × 10−6)][80 × 10−3 + j(6 × 108)(40 × 10−12)] = 2.8 + j3.5 m−1 = α + jβ Therefore, α = 2.8 Np/m, β = 3.5 rad/m, and λ = 2π/β = 1.8 m. Finally, Z0 = Z Y = R + jωL G + jωC = 20 + j2.4 × 102 80 × 10−3 + j2.4 × 10−2 = 44 + j30 b) If a voltage wave travels 20 m down the line, what percentage of the original amplitude remains, and by how many degrees is it phase shifted? First, V20 V0 = e−αL = e−(2.8)(20) = 4.8 × 10−25 or 4.8 × 10−23 percent! Then the phase shift is given by βL, which in degrees becomes φ = βL 360 2π = (3.5)(20) 360 2π = 4.0 × 103 degrees 13.2. A lossless transmission line with Z0 = 60 is being operated at 60 MHz. The velocity on the line is 3 × 108 m/s. If the line is short-circuited at z = 0, find Zin at: a) z = −1m: We use the expression for input impedance (Eq. 12), under the conditions Z2 = 60 and Z3 = 0: Zin = Z2 Z3 cos(βl) + jZ2 sin(βl) Z2 cos(βl) + jZ3 sin(βl) = j60 tan(βl) where l = −z, and where the phase constant is β = 2πc/f = 2π(3 × 108)/(6 × 107) = (2/5)π rad/m. Now, with z = −1 (l = 1), we find Zin = j60 tan(2π/5) = j184.6 . b) z = −2 m: Zin = j60 tan(4π/5) = −j43.6 c) z = −2.5 m: Zin = j60 tan(5π/5) = 0 d) z = −1.25 m: Zin = j60 tan(π/2) = j∞ (open circuit) 13.3. The characteristic impedance of a certain lossless transmission line is 72 . If L = 0.5 µH/m, find: a) C: Use Z0 = √ L/C, or C = L Z2 0 = 5 × 10−7 (72)2 = 9.6 × 10−11 F/m = 96 pF/m 213 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 216. 13.3b) vp: vp = 1 √ LC = 1 (5 × 10−7)(9.6 × 10−11) = 1.44 × 108 m/s c) β if f = 80 MHz: β = ω √ LC = 2π × 80 × 106 1.44 × 108 = 3.5 rad/m d) The line is terminated with a load of 60 . Find Ŵ and s: Ŵ = 60 − 72 60 + 72 = −0.09 s = 1 + |Ŵ| 1 − |Ŵ| = 1 + .09 1 − .09 = 1.2 13.4. A lossless transmission line having Z0 = 120 is operating at ω = 5 × 108 rad/s. If the velocity on the line is 2.4 × 108 m/s, find: a) L: With Z0 = √ L/C and v = 1/ √ LC, we find L = Z0/v = 120/2.4 × 108 = 0.50 µH/m. b) C: Use Z0v = √ L/C/ √ LC ⇒ C = 1/(Z0v) = [120(2.4 × 108)]−1 = 35 pF/m. c) Let ZL be represented by an inductance of 0.6 µH in series with a 100- resistance. Find Ŵ and s: The inductive impedance is jωL = j(5 × 108)(0.6 × 10−6) = j300. So the load impedance is ZL = 100 + j300 . Now Ŵ = ZL − Z0 ZL + Z0 = 100 + j300 − 120 100 + j300 + 120 = 0.62 + j0.52 = 0.808 40◦ Then s = 1 + |Ŵ| 1 − |Ŵ| = 1 + 0.808 1 − 0.808 = 9.4 13.5. Two characteristics of a certain lossless transmission line are Z0 = 50 and γ = 0 + j0.2π m−1 at f = 60 MHz. a) Find L and C for the line: We have β = 0.2π = ω √ LC and Z0 = 50 = √ L/C. Thus β Z0 = ωC ⇒ C = β ωZ0 = 0.2π (2π × 60 × 106)(50) = 1 3 × 1010 = 33.3 pF/m Then L = CZ2 0 = (33.3 × 10−12)(50)2 = 8.33 × 10−8 H/m = 83.3 nH/m. b) A load, ZL = 60 + j80 is located at z = 0. What is the shortest distance from the load to a point at which Zin = Rin + j0? I will do this using two different methods: The Hard Way: We use the general expression Zin = Z0 ZL + jZ0 tan(βl) Z0 + jZL tan(βl) We can then normalize the impedances with respect to Z0 and write zin = Zin Z0 = (ZL/Z0) + j tan(βl) 1 + j(ZL/Z0) tan(βl) = zL + j tan(βl) 1 + jzL tan(βl) where zL = (60 + j80)/50 = 1.2 + j1.6. 214 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 217. 13.5b. (continued) Using this, and defining x = tan(βl), we find zin = 1.2 + j(1.6 + x) (1 − 1.6x) + j1.2x (1 − 1.6x) − j1.2x (1 − 1.6x) − j1.2x The second bracketed term is a factor of one, composed of the complex conjugate of the denomi- nator of the first term, divided by itself. Carrying out this product, we find zin = 1.2(1 − 1.6x) + 1.2x(1.6 + x) − j[(1.2)2x − (1.6 + x)(1 − 1.6x)] (1 − 1.6x)2 + (1.2)2x2 We require the imaginary part to be zero. Thus (1.2)2 x − (1.6 + x)(1 − 1.6x) = 0 ⇒ 1.6x2 + 3x − 1.6 = 0 So x = tan(βl) = −3 ± 9 + 4(1.6)2 2(1.6) = (.433, −2.31) We take the positive root, and find βl = tan−1 (.433) = 0.409 ⇒ l = 0.409 0.2π = 0.65 m = 65 cm The Easy Way: We find Ŵ = 60 + j80 − 50 60 + j80 + 50 = 0.405 + j0.432 = 0.59 0.818 Thus φ = 0.818 rad, and we use the fact that the input impedance will be purely real at the location of a voltage minimum or maximum. The first voltage maximum will occur at a distance in front of the load given by zmax = φ 2β = 0.818 2(0.2π) = 0.65 m 13.6. The propagation constant of a lossy transmission line is 1 + j2 m−1, and its characteristic impedance is 20 + j0 at ω = 1 Mrad/s. Find L, C, R, and G for the line: Begin with Z0 = R + jωL G + jωL = 20 ⇒ R + jωL = 400(G + jωC) (1) Then γ 2 = (R + jωL)(G + jωC) = (1 + j2)2 ⇒ 400(G + jωC)2 = (1 + j2)2 (2) where (1) has been used. Eq. 2 now becomes G + jωC = (1 + j2)/20. Equating real and imaginary parts leads to G = .05 S/m and C = 1/(10ω) = 10−7 = 0.1 µF/m. 215 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 218. 13.6. (continued) Now, (1) becomes 20 = R + jωL 1 + j2 √ 20 ⇒ 20 = R + jωL 1 + j2 ⇒ 20 + j40 = R + jωL Again, equating real and imaginary parts leads to R = 20 /m and L = 40/ω = 40 µH/m. 13.7. The dimensions of the outer conductor of a coaxial cable are b and c, c > b. Assume σ = σc and let µ = µ0. Find the magnetic energy stored per unit length in the region b < r < c for a uniformly distributed total current I flowing in opposite directions in the inner and outer conductors: First, from the inner conductor, the magnetic field will be H1 = I 2πρ aφ The contribution from the outer conductor to the magnetic field within that conductor is found from Ampere’s circuital law to be: H2 = − I 2πρ ρ2 − b2 c2 − b2 aφ The total magnetic field within the outer conductor will be the sum of the two fields, or HT = H1 + H2 = I 2πρ c2 − ρ2 c2 − b2 aφ The energy density is wm = 1 2 µ0H2 T = µ0I2 8π2 c2 − ρ2 c2 − b2 2 J/m3 The stored energy per unit length in the outer conductor is now Wm = 1 0 2π 0 c b µ0I2 8π2 c2 − ρ2 c2 − b2 2 ρ dρ dφ dz = µ0I2 4π(c2 − b2)2 c b c4 ρ − 2c2 ρ + ρ3 dρ = µ0I2 4π c4 (c2 − b2)2 ln c b + b2 − (3/4)c2 (c2 − b2) J 13.8. The conductors of a coaxial transmission line are copper (σc = 5.8 × 10−7 S/m) and the dielectric is polyethylene (ǫ′ R = 2.26, σ/ωǫ′ = 0.0002). If the inner radius of the outer conductor is 4 mm, find the radius of the inner conductor so that (assuming a lossless line): a) Z0 = 50 : Use Z0 = 1 2π µ ǫ′ ln b a = 50 ⇒ ln b a = 2π ǫ′ R(50) 377 = 1.25 Thus b/a = e1.25 = 3.50, or a = 4/3.50 = 1.142 mm 216 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 219. 13.8b. C = 100 pF/m: Begin with C = 2πǫ′ ln(b/a) = 10−10 ⇒ ln b a = 2π(2.26)(8.854 × 10−2 ) = 1.257 So b/a = e1.257 = 3.51, or a = 4/3.51 = 1.138 mm. c) L = 0.2 µH/m: Use L = µ0 2π ln b a = 0.2 × 10−6 ⇒ ln b a = 2π(0.2 × 10−6) 4π × 10−7 = 1 Thus b/a = e1 = 2.718, or a = b/2.718 = 1.472 mm. 13.9. Two aluminum-clad steel conductors are used to construct a two-wire transmission line. Let σAl = 3.8×107 S/m, σSt = 5×106 S/m, and µSt = 100 µH/m. The radius of the steel wire is 0.5 in., and the aluminum coating is 0.05 in. thick. The dielectric is air, and the center-to-center wire separation is 4 in. Find C, L, G, and R for the line at 10 MHz: The first question is whether we are in the high frequency or low frequency regime. Calculation of the skin depth, δ, will tell us. We have, for aluminum, δ = 1 √ πf µ0σAl = 1 π(107)(4π × 10−7)(3.8 × 107) = 2.58 × 10−5 m so we are clearly in the high frequency regime, where uniform current distributions cannot be assumed. Furthermore, the skin depth is considerably less than the aluminum layer thickness, so the bulk of the current resides in the aluminum, and we may neglect the steel. Assuming solid aluminum wires of radius a = 0.5 + 0.05 = 0.55 in = 0.014 m, the resistance of the two-wire line is now R = 1 πaδσAl = 1 π(.014)(2.58 × 10−5)(3.8 × 107) = 0.023 /m Next, since the dielectric is air, no leakage will occur from wire to wire, and so G = 0 mho/m. Now the capacitance will be C = πǫ0 cosh−1(d/2a) = π × 8.85 × 10−12 cosh−1 (4/(2 × 0.55)) = 1.42 × 10−11 F/m = 14.2 pF/m Finally, the inductance per unit length will be L = µ0 π cosh(d/2a) = 4π × 10−7 π cosh (4/(2 × 0.55)) = 7.86 × 10−7 H/m = 0.786 µH/m 217 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 220. 13.10. Each conductor of a two-wire transmission line has a radius of 0.5mm; their center-to-center distance is 0.8cm. Let f = 150MHz and assume σ = 0 and σc → ∞ (note error in problem statement). Find the dielectric constant of the insulating medium if a) Z0 = 300 : Use 300 = 1 π µ0 ǫ′ Rǫ0 cosh−1 d 2a ⇒ ǫ′ R = 120π 300π cosh−1 8 2(.5) = 1.107 ⇒ ǫ′ R = 1.23 b) C = 20 pF/m: Use 20 × 10−12 = πǫ′ cosh−1(d/2a) ⇒ ǫ′ R = 20 × 10−12 πǫ0 cosh−1 (8) = 1.99 c) vp = 2.6 × 108 m/s: vp = 1 √ LC = 1 µ0ǫ0ǫ′ R = c ǫ′ R ⇒ ǫ′ R = 3.0 × 108 2.6 × 108 2 = 1.33 13.11. Pertinent dimensions for the transmission line shown in Fig. 13.4 are b = 3 mm, and d = 0.2 mm. The conductors and the dielectric are non-magnetic. a) If the characteristic impedance of the line is 15 , find ǫ′ R: We use Z0 = µ ǫ′ d b = 15 ⇒ ǫ′ R = 377 15 2 .04 9 = 2.8 b) Assume copper conductors and operation at 2 × 108 rad/s. If RC = GL, determine the loss tangent of the dielectric: For copper, σc = 5.8 × 107 S/m, and the skin depth is δ = 2 ωµ0σc = 2 (2 × 108)(4π × 10−7)(5.8 × 107) = 1.2 × 10−5 m Then R = 2 σcδb = 2 (5.8 × 107)(1.2 × 10−5)(.003) = 0.98 /m Now C = ǫ′b d = (2.8)(8.85 × 10−12)(3) 0.2 = 3.7 × 10−10 F/m and L = µ0d b = (4π × 10−7)(0.2) 3 = 8.4 × 10−8 H/m Then, with RC = GL, G = RC L = (.98)(3.7 × 10−10) (8.4 × 10−8) = 4.4 × 10−3 mho/m = σdb d Thus σd = (4.4 × 10−3)(0.2/3) = 2.9 × 10−4 S/m. The loss tangent is l.t. = σd ωǫ′ = 2.9 × 10−4 (2 × 108)(2.8)(8.85 × 10−12) = 5.85 × 10−2 218 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 221. 13.12. A transmission line constructed from perfect conductors and an air dielectric is to have a maximum dimensionof8mmforitscross-section. Thelineistobeusedathighfrequencies. Specifyitsdimensions if it is: a) a two-wire line with Z0 = 300 : With the maximum dimension of 8mm, we have, using (27): Z0 = 1 π µ ǫ′ cosh−1 8 − 2a 2a = 300 ⇒ 8 − 2a 2a = cosh 300π 120π = 6.13 Solve for a to find a = 0.56 mm. Then d = 8 − 2a = 6.88 mm. b) a planar line with Z0 = 15 : In this case our maximum dimension dictates that √ d2 + b2 = 8. So, using (34), we write Z0 = µ ǫ′ √ 64 − b2 b = 15 ⇒ 64 − b2 = 15 377 b Solving, we find b = 7.99 mm and d = 0.32 mm. c) a 72 coax having a zero-thickness outer conductor: With a zero-thickness outer conductor, we note that the outer radius is b = 8/2 = 4mm. Using (18), we write Z0 = 1 2π µ ǫ′ ln b a = 72 ⇒ ln b a = 2π(72) 120π = 1.20 ⇒ a = be−1.20 = 4e−1.20 = 1.2 Summarizing, a = 1.2 mm and b = 4 mm. 13.13. The incident voltage wave on a certain lossless transmission line for which Z0 = 50 and vp = 2×108 m/s is V +(z, t) = 200 cos(ωt − πz) V. a) Find ω: We know β = π = ω/vp, so ω = π(2 × 108) = 6.28 × 108 rad/s. b) Find I+(z, t): Since Z0 is real, we may write I+ (z, t) = V +(z, t) Z0 = 4 cos(ωt − πz) A The section of line for which z > 0 is replaced by a load ZL = 50 + j30 at z = 0. Find c) ŴL: This will be ŴL = 50 + j30 − 50 50 + j30 + 50 = .0825 + j0.275 = 0.287 1.28 rad d) V − s (z) = ŴLV + s (z)ej2βz = 0.287(200)ejπzej1.28 = 57.5ej(πz+1.28) e) Vs at z = −2.2 m: Vs(−2.2) = V + s (−2.2) + V − s (−2.2) = 200ej2.2π + 57.5e−j(2.2π−1.28) = 257.5ej0.63 = 257.5 36◦ 219 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 222. 13.14. Coaxial lines 1 and 2 have the following parameters: µ1 = µ2 = µ0, σ1 = σ2 = 0, ǫ′ R1 = 2.25, ǫ′ R2 = 4, a1 = a2 = 0.8mm, b1 = 6mm, b2 = 3mm, ZL2 = Z02, and ZL1 is Zin2. a) Find Z01 and Z02. For either line, we have Z0 = 1 2π µ ǫ′ ln b a = 377 2π ǫ′ R ln b a leading to Z01 = 377 2π √ 2.25 ln 6 .8 = 80.6 and Z02 = 377 2π √ 4 ln 3 .8 = 39.7 b) Find s on line 1: Line 1’s load is line 2’s input impedance (they are connected end-to-end). Also, since line 2 is matched, its input impedance is just it’s characteristic impedance. Therefore, ZL1 = Zin2 = Z02. The reflection coefficient encountered by waves incident on ZL1 from line 1 can now be found, along with the standing wave ratio: Ŵ12 = 39.7 − 80.6 39.7 + 80.6 = −0.34 ⇒ s = 1 + .34 1 − .34 = 2.03 c) If a 20cm length of line 1 is inserted immediately in front of ZL2 and f = 300MHz, find s on line 2: The line 1 length now has a load impedance of 39.7 and it is 20cm long. We need to find its input impedance. At 300 MHz, the free space wavelength is 1m. In line 1, having a dielectric constant of 2.25, the wavelength is λ = 1m/ √ 2.25 = 0.67m. Therefore βl = 2πl/λ = 2π(20)/(67) = 1.87. We now find the input impedance for this situation through Zin = Z01 ZL2 cos(βl) + jZ01 sin(βl) Z01 cos(βl) + jZL2 sin(βl) = 80.6 39.7 cos(1.87) + j80.6 sin(1.87) 80.6 cos(1.87) + j39.7 sin(1.87) = 128.7 − j55.8 = 140.3 − 23.4◦ Now for waves incident at the line 1 - line 2 junction from line 2, the reflection coefficient will be Ŵ21 = Zin − Z02 Zin + Z02 = 128.7 − 39.7 − j55.8 128.7 + 39.7 − j55.8 = 0.58 − j0.14 = 0.59 − 13.7◦ The standing wave ratio is now s = 1 + .59 1 − .59 = 3.9 220 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 223. 13.15. For the transmission line represented in Fig. 13.26, find Vs,out if f =: a) 60 Hz: At this frequency, β = ω vp = 2π × 60 (2/3)(3 × 108) = 1.9 × 10−6 rad/m So βl = (1.9 × 10−6 )(80) = 1.5 × 10−4 << 1 The line is thus essentially a lumped circuit, where Zin . = ZL = 80 . Therefore Vs,out = 120 80 12 + 80 = 104 V b) 500 kHz: In this case β = 2π × 5 × 105 2 × 108 = 1.57 × 10−2 rad/s So βl = 1.57 × 10−2 (80) = 1.26 rad Now Zin = 50 80 cos(1.26) + j50 sin(1.26) 50 cos(1.26) + j80 sin(1.26) = 33.17 − j9.57 = 34.5 − .28 The equivalent circuit is now the voltage source driving the series combination of Zin and the 12 ohm resistor. The voltage across Zin is thus Vin = 120 Zin 12 + Zin = 120 33.17 − j9.57 12 + 33.17 − j9.57 = 89.5 − j6.46 = 89.7 − .071 The voltage at the line input is now the sum of the forward and backward-propagating waves just to the right of the input. We reference the load at z = 0, and so the input is located at z = −80 m. In general we write Vin = V + 0 e−jβz + V − 0 ejβz, where V − 0 = ŴLV + 0 = 80 − 50 80 + 50 V + 0 = 3 13 V + 0 At z = −80 m we thus have Vin = V + 0 ej1.26 + 3 13 e−j1.26 ⇒ V + 0 = 89.5 − j6.46 ej1.26 + (3/13)e−j1.26 = 42.7 − j100 V Now Vs,out = V + 0 (1 + ŴL) = (42.7 − j100)(1 + 3/(13)) = 134 − 1.17 rad = 52.6 − j123 V As a check, we can evaluate the average power reaching the load: Pavg,L = 1 2 |Vs,out |2 RL = 1 2 (134)2 80 = 112 W This must be the same power that occurs at the input impedance: Pavg,in = 1 2 Re VinI∗ in = 1 2 Re {(89.5 − j6.46)(2.54 + j0.54)} = 112 W where Iin = Vin/Zin = (89.5 − j6.46)/(33.17 − j9.57) = 2.54 + j0.54. 221 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 224. 13.16. A 300 ohm transmission line is 0.8 m long and is terminated with a short circuit. The line is operating in air with a wavelength of 0.3 m (incorrectly stated as 0.8 m in early printings) and is lossless. a) If the input voltage amplitude is 10V, what is the maximum voltage amplitude at any point on the line? The net voltage anywhere on the line is the sum of the forward and backward wave voltages, and is written as V (z) = V + 0 e−jβz + V − 0 ejβz. Since the line is short-circuited at the load end (z = 0), we have V − 0 = −V + 0 , and so V (z) = V + 0 e−jβz − ejβz = −2jV + 0 sin(jβz) We now evaluate the voltage at the input, where z = −0.8m, and λ = 0.3m. Vin = −2jV + 0 sin 2π(−0.8) 0.3 = −j1.73V + 0 The magnitude of Vin is given as 10V, so we find V + 0 = 10/1.73 = 5.78V. The maximum voltage amplitude on the line will be twice this value (where the sine function is unity), so |V |max = 2(5.78) = 11.56 V. b) What is the current amplitude in the short circuit? At the shorted end, the current will be IL = V + 0 Z0 − V − 0 Z0 = 2V + 0 Z0 = 11.56 300 = 0.039A = 39 mA 13.17. DeterminetheaveragepowerabsorbedbyeachresistorinFig. 13.27: Theproblemismadeeasierbyfirst converting the current source/100 ohm resistor combination to its Thevenin equivalent. This is a 50 0 V voltage source in series with the 100 ohm resistor. The next step is to determine the input impedance of the 2.6λ length line, terminated by the 25 ohm resistor: We use βl = (2π/λ)(2.6λ) = 16.33 rad. This value, modulo 2π is (by subtracting 2π twice) 3.77 rad. Now Zin = 50 25 cos(3.77) + j50 sin(3.77) 50 cos(3.77) + j25 sin(3.77) = 33.7 + j24.0 The equivalent circuit now consists of the series combination of 50 V source, 100 ohm resistor, and Zin, as calculated above. The current in this circuit will be I = 50 100 + 33.7 + j24.0 = 0.368 − .178 The power dissipated by the 25 ohm resistor is the same as the power dissipated by the real part of Zin, or P25 = P33.7 = 1 2 |I|2 R = 1 2 (.368)2 (33.7) = 2.28 W To find the power dissipated by the 100 ohm resistor, we need to return to the Norton configuration, with the original current source in parallel with the 100 ohm resistor, and in parallel with Zin. The voltage across the 100 ohm resistor will be the same as that across Zin, or V = IZin = (.368 − .178)(33.7 + j24.0) = 15.2 0.44. The power dissipated by the 100 ohm resistor is now P100 = 1 2 |V |2 R = 1 2 (15.2)2 100 = 1.16 W 222 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 225. 13.18 The line shown in Fig. 13.28 is lossless. Find s on both sections 1 and 2: For section 2, we consider the propagation of one forward and one backward wave, comprising the superposition of all reflected waves from both ends of the section. The ratio of the backward to the forward wave amplitude is given by the reflection coefficient at the load, which is ŴL = 50 − j100 − 50 50 − j100 + 50 = −j 1 − j = 1 2 (1 − j) Then |ŴL| = (1/2) √ (1 − j)(1 + j) = 1/ √ 2. Finally s2 = 1 + |ŴL| 1 − |ŴL| = 1 + 1/ √ 2 1 − 1/ √ 2 = 5.83 For section 1, we need the reflection coefficient at the junction (location of the 100 resistor) seen by waves incident from section 1: We first need the input impedance of the .2λ length of section 2: Zin2 = 50 (50 − j100) cos(β2l) + j50 sin(β2l) 50 cos(β2l) + j(50 − j100) sin(β2l) = 50 (1 − j2)(0.309) + j0.951 0.309 + j(1 − j2)(0.951) = 8.63 + j3.82 = 9.44 0.42 rad Now, this impedance is in parallel with the 100 resistor, leading to a net junction impedance found by 1 ZinT = 1 100 + 1 8.63 + j3.82 ⇒ ZinT = 8.06 + j3.23 = 8.69 0.38 rad The reflection coefficient will be Ŵj = ZinT − 50 ZinT + 50 = −0.717 + j0.096 = 0.723 3.0 rad and the standing wave ratio is s1 = (1 + 0.723)/(1 − 0.723) = 6.22. 13.19. A lossless transmission line is 50 cm in length and operating at a frequency of 100 MHz. The line parameters are L = 0.2 µH/m and C = 80 pF/m. The line is terminated by a short circuit at z = 0, and there is a load, ZL = 50 + j20 ohms across the line at location z = −20 cm. What average power is delivered to ZL if the input voltage is 100 0 V? With the given capacitance and inductance, we find Z0 = L C = 2 × 10−7 8 × 10−11 = 50 and vp = 1 √ LC = 1 (2 × 10−7)(9 × 10−11) = 2.5 × 108 m/s Now β = ω/vp = (2π × 108)/(2.5 × 108) = 2.5 rad/s. We then find the input impedance to the shorted line section of length 20 cm (putting this impedance at the location of ZL, so we can combine them): We have βl = (2.5)(0.2) = 0.50, and so, using the input impedance formula with a zero load impedance, we find Zin1 = j50 tan(0.50) = j27.4 ohms. 223 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 226. 13.19 (continued) Now, at the location of ZL, the net impedance there is the parallel combination of ZL and Zin1: Znet = (50+j20)||(j27.4) = 7.93+j19.9. We now transform this impedance to the line input, 30 cm to the left, obtaining (with βl = (2.5)(.3) = 0.75): Zin2 = 50 (7.93 + j19.9) cos(.75) + j50 sin(.75) 50 cos(.75) + j(7.93 + j19.9) sin(.75) = 35.9 + j98.0 = 104.3 1.22 The power delivered to ZL is the same as the power delivered to Zin2: The current magnitude is |I| = (100)/(104.3) = 0.96 A. So finally, P = 1 2 |I|2 R = 1 2 (0.96)2 (35.9) = 16.5 W 13.20. This problem was originally posed incorrectly. The corrected version should have an inductor in the input circuit instead of a capacitor. I will proceed with this replacement understood, and will change the wording as appropriate in parts c and d: a) Determine s on the transmission line of Fig. 13.29. Note that the dielectric is air: The reflection coefficient at the load is ŴL = 40 + j30 − 50 40 + j30 + 50 = j0.333 = 0.333 1.57 rad Then s = 1 + .333 1 − .333 = 2.0 b) Find the input impedance: With the length of the line at 2.7λ, we have βl = (2π)(2.7) = 16.96 rad. The input impedance is then Zin = 50 (40 + j30) cos(16.96) + j50 sin(16.96) 50 cos(16.96) + j(40 + j30) sin(16.96) = 50 −1.236 − j5.682 1.308 − j3.804 = 61.8 − j37.5 c) If ωL = 10 , find Is: The source drives a total impedance given by Znet = 20 + jωL + Zin = 20+j10+61.8−j37.5 = 81.8−j27.5. ThecurrentisnowIs = 100/(81.8−j27.5) = 1.10 + j0.37 A. d) What value of L will produce a maximum value for |Is| at ω = 1 Grad/s? To achieve this, the imaginary part of the total impedance of part c must be reduced to zero (so we need an inductor). The inductor impedance must be equal to negative the imaginary part of the line input impedance, or ωL = 37.5, so that L = 37.5/ω = 37.5 nH. Continuing, for this value of L, calculate the average power: e) supplied by the source: Ps = (1/2)Re{VsIs} = (1/2)(100)2/(81.8) = 61.1 W. f) delivered to ZL = 40+j30 : The power delivered to the load will be the same as the power delivered to the input impedance. We write PL = 1 2 Re{Zin}|Is|2 = 1 2 (61.8)(1.22)2 = 46.1 W 224 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 227. 13.21. A lossless line having an air dielectric has a characteristic impedance of 400 . The line is operating at 200 MHz and Zin = 200 − j200 . Use analytic methods or the Smith chart (or both) to find: (a) s; (b) ZL if the line is 1 m long; (c) the distance from the load to the nearest voltage maximum: I will first use the analytic approach. Using normalized impedances, Eq. (13) becomes zin = Zin Z0 = zL cos(βL) + j sin(βL) cos(βL) + jzL sin(βL) = zL + j tan(βL) 1 + jzL tan(βL) Solve for zL: zL = zin − j tan(βL) 1 − jzin tan(βL) where, with λ = c/f = 3 × 108/2 × 108 = 1.50 m, we find βL = (2π)(1)/(1.50) = 4.19, and so tan(βL) = 1.73. Also, zin = (200 − j200)/400 = 0.5 − j0.5. So zL = 0.5 − j0.5 − j1.73 1 − j(0.5 − j0.5)(1.73) = 2.61 + j0.174 Finally, ZL = zL(400) = 1.04 × 103 + j69.8 . Next Ŵ = ZL − Z0 ZL + Z0 = 6.42 × 102 + j69.8 1.44 × 103 + j69.8 = .446 + j2.68 × 10−2 = .447 6.0 × 10−2 rad Now s = 1 + |Ŵ| 1 − |Ŵ| = 1 + .447 1 − .447 = 2.62 Finally zmax = − φ 2β = − λφ 4π = − (6.0 × 10−2)(1.50) 4π = −7.2 × 10−3 m = −7.2 mm We next solve the problem using the Smith chart. Referring to the figure on the next page, we first locate and mark the normalized input impedance, zin = 0.5 − j0.5. A line drawn from the origin through this point intersects the outer chart boundary at the position 0.0881 λ on the wavelengths toward load (WTL) scale. With a wavelength of 1.5 m, the 1 meter line is 0.6667 wavelengths long. On the WTL scale, we add 0.6667λ, or equivalently, 0.1667λ (since 0.5λ is once around the chart), obtaining (0.0881+0.1667)λ) = 0.2548λ, which is the position of the load. A straight line is now drawn from the origin though the 0.2548λ position. A compass is then used to measure the distance between the origin and zin. With this distance set, the compass is then used to scribe off the same distance from the origin to the load impedance, along the line between the origin and the 0.2548λ position. That point is the normalized load impedance, which is read to be zL = 2.6+j0.18. Thus ZL = zL(400) = 1040+j72. This is in reasonable agreement with the analytic result of 1040 + j69.8. The difference in imaginary parts arises from uncertainty in reading the chart in that region. In transforming from the input to the load positions, we cross the r > 1 real axis of the chart at r=2.6. This is close to the value of the VSWR, as we found earlier. We also see that the r > 1 real axis (at which the first Vmax occurs) is a distance of 0.0048λ (marked as .005λ on the chart) in front of the load. The actual distance is zmax = −0.0048(1.5) m = −0.0072 m = −7.2 mm. 225 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 228. . 13.22. A lossless two-wire line has a characteristic impedance of 300 and a capacitance of 15 pF/m. The load at z = 0 consists of a 600- resistor in parallel with a 10-pF capacitor. If ω = 108 rad/s and the line is 20m long, use the Smith chart to find a) |ŴL|; b) s; c) Zin. First, the wavelength on the line is found using λ = 2πvp/ω, where vp = 1/(CZ0). Assuming higher accuracy in the given values than originally stated, we obtain λ = 2π ωCZ0 = 2π (108)(15 × 10−12)(300) = 13.96 m The line length in wavelengths is therefore 20/13.96 = 1.433λ. The normalized load admittance is now yL = YLZ0 = Z0 1 RL + jωC = 300 1 600 + j(108 )(10−11 ) = 0.50 + j0.30 226 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 229. The yL value is plotted on the chart and labeled as yL. Next, yL is inverted to find zL by transforming the point halfway around the chart, using the compass and a straight edge. The result, labeled zL on the chart is read to be zL = 1.5−j0.87. This is close to the computed inverse of yL, which is 1.47−j0.88. Scribing the compass arc length along the bottom scale for reflection coefficient yields |ŴL| = 0.38. The VSWR is found by scribing the compass arc length either along the bottom SWR scale or along the positive real axis of the chart, both methods yielding s = 2.2. Now, the position of zL is read on the outer edge of the chart as 0.308λ on the WTG scale. The point is now transformed through the line length distance of 1.433λ toward the generator (the net chart distance will be 0.433λ, since a full wavelength is two complete revolutions). The final reading on the WTG scale after the transformation is found through (0.308 + 0.433 − 0.500)λ = 0.241λ. Drawing a line between this mark on the WTG scale and the chart center, and scribing the compass arc length on this line, yields the normalized input impedance. This is read as zin = 2.2 + j0.21 (the computed value found through the analytic solution is zin = 2.21 + j0.219. The input impedance is now found by multiplying the chart reading by 300, or Zin = 660 + j63 . 227 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 230. 13.23. The normalized load on a lossless transmission line is zL = 2+j1. Let l = 20 m (there was a missprint in the problem statement, since λ = 20 m should have been stated. I will specify answers in terms of wavelength). Make use of the Smith chart to find: a) the shortest distance from the load to the point at which zin = rin +j0, where rin > 1 (not greater than 0 as stated): Referring to the figure below, we start by marking the given zL on the chart and drawing a line from the origin through this point to the outer boundary. On the WTG scale, we read the zL location as 0.213λ. Moving from here toward the generator, we cross the positive ŴR axis (at which the impedance is purely real and greater than 1) at 0.250λ. The distance is then (0.250 − 0.213)λ = 0.037λ from the load. If we use λ = 20 m, the actual distance would be 20(0.037) = 0.74 m. b) Find zin at the point found in part a: Using a compass, we set its radius at the distance between the origin and zL. We then scribe this distance along the real axis to find zin = rin = 2.61. c) The line is cut at this point and the portion containing zL is thrown away. A resistor r = rin of part a is connected across the line. What is s on the remainder of the line? This will be just s for the line as it was before. As we know, s will be the positive real axis value of the normalized impedance, or s = 2.61. d) What is the shortest distance from this resistor to a point at which zin = 2 + j1? This would return us to the original point, requiring a complete circle around the chart (one-half wavelength distance). The distance from the resistor will therefore be: d = 0.500 λ − 0.037 λ = 0.463 λ. With λ = 20 m, the actual distance would be 20(0.463) = 9.26 m. 228 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 231. 13.24. With the aid of the Smith chart, plot a curve of |Zin| vs. l for the transmission line shown in Fig. 13.30. Cover the range 0 < l/λ < 0.25. The required input impedance is that at the actual line input (to the left of the two 20 resistors. The input to the line section occurs just to the right of the 20 resistors, and the input impedance there we first find with the Smith chart. This impedance is in series with the two 20 resistors, so we add 40 to the calculated impedance from the Smith chart to find the net line input impedance. To begin, the 20 load resistor represents a normalized impedance of zl = 0.4, which we mark on the chart (see below). Then, using a compass, draw a circle beginning at zL and progressing clockwise to the positive real axis. The circle traces the locus of zin values for line lengths over the range 0 < l < λ/4. On the chart, radial lines are drawn at positions corresponding to .025λ increments on the WTG scale. The intersections of the lines and the circle give a total of 11 zin values. To these we add normalized impedance of 40/50 = 0.8 to add the effect of the 40 resistors and obtain the normalized impedance at the line input. The magnitudes of these values are then found, and the results are multiplied by 50 . The table below summarizes the results. l/λ zinl (to right of 40 ) zin = zinl + 0.8 |Zin| = 50|zin| 0 0.40 1.20 60 .025 0.41 + j.13 1.21 + j.13 61 .050 0.43 + j.27 1.23 + j.27 63 .075 0.48 + j.41 1.28 + j.41 67 .100 0.56 + j.57 1.36 + j.57 74 .125 0.68 + j.73 1.48 + j.73 83 .150 0.90 + j.90 1.70 + j.90 96 .175 1.20 + j1.05 2.00 + j1.05 113 .200 1.65 + j1.05 2.45 + j1.05 134 .225 2.2 + j.7 3.0 + j.7 154 .250 2.5 3.3 165 229 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 232. 13.24. (continued) As a check, the line input input impedance can be found analytically through Zin = 40 + 50 20 cos(2πl/λ) + j50 sin(2πl/λ) 50 cos(2πl/λ) + j20 sin(2πl/λ) = 50 60 cos(2πl/λ) + j66 sin(2πl/λ) 50 cos(2πl/λ) + j20 sin(2πl/λ) from which |Zin| = 50 36 cos2(2πl/λ) + 43.6 sin2(2πl/λ) 25 cos2(2πl/λ) + 4 sin2(2πl/λ) 1/2 This function is plotted below along with the results obtained from the Smith chart. A fairly good comparison is obtained. 230 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 233. 13.25. A 300-ohm transmission line is short-circuited at z = 0. A voltage maximum, |V |max = 10 V, is found at z = −25 cm, and the minimum voltage, |V |min = 0, is found at z = −50 cm. Use the Smith chart to find ZL (with the short circuit replaced by the load) if the voltage readings are: a) |V |max = 12 V at z = −5 cm, and vertV |min = 5 V: First, we know that the maximum and minimum voltages are spaced by λ/4. Since this distance is given as 25 cm, we see that λ = 100 cm = 1 m. Thus the maximum voltage location is 5/100 = 0.05λ in front of the load. The standing wave ratio is s = |V |max/|V |min = 12/5 = 2.4. We mark this on the positive real axis of the chart (see next page). The load position is now 0.05 wavelengths toward the load from the |V |max position, or at 0.30 λ on the WTL scale. A line is drawn from the origin through this point on the chart, as shown. We next set the compass to the distance between the origin and the z = r = 2.4 point on the real axis. We then scribe this same distance along the line drawn through the .30 λ position. The intersection is the value of zL, which we read as zL = 1.65 + j.97. The actual load impedance is then ZL = 300zL = 495 + j290 . b) |V |max = 17 V at z = −20 cm, and |V |min = 0. In this case the standing wave ratio is infinite, which puts the starting point on the r → ∞ point on the chart. The distance of 20 cm corresponds to 20/100 = 0.20 λ, placing the load position at 0.45 λ on the WTL scale. A line is drawn from the origin through this location on the chart. An infinite standing wave ratio places us on the outer boundary of the chart, so we read zL = j0.327 at the 0.45 λ WTL position. Thus ZL = j300(0.327) . = j98 . 231 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 234. 13.26. A lossless 50 transmission line operates with a velocity that is 3/4c. A load, ZL = 60 + j30 is located at z = 0. Use the Smith chart to find: a) s: First we find the normalized load impedance, zL = (60 + j30)/50 = 1.2 + j0.6, which is then marked on the chart (see below). Drawing a line from the chart center through this point yields its location at 0.328λ on the WTL scale. The distance from the origin to the load impedance point is now set on the compass; the standing wave ratio is then found by scribing this distance along the positive real axis, yielding s = 1.76, as shown. Alternately, use the s scale at the bottom of the chart, setting the compass point at the center, and scribing the distance on the scale to the left. b) the distance from the load to the nearest voltage minimum if f = 300 MHz: This distance is found by transforming the load impedance clockwise around the chart until the negative real axis is reached. This distance in wavelengths is just the load position on the WTL scale, since the starting point for this scale is the negative real axis. So the distance is 0.328λ. The wavelength is λ = v f = (3/4)c 300MHz = 3(3 × 108) 4(3 × 108) = 0.75 m So the actual distance to the first voltage minimum is dmin = 0.328(0.75) m = 24.6 cm. c) the input impedance if f = 200 MHz and the input is at z = −110cm: The wavelength at this frequency is λ = (3/4)(3 × 108)/(2 × 108) = 1.125 m. The distance to the input in wavelengths is then din = (1.10)/(1.125) = 0.9778λ. Transforming the load through this distance toward the generator involves revolution once around the chart (0.500λ) plus the remainder of 0.4778λ, which leads to a final position of 0.1498λ . = 0.150λ on the WTG scale, or 0.350λ on the WTL scale. A line is drawn between this point and the chart center. Scribing the compass arc length through this line yields the normalized input impedance, read as zin = 1.03 + j0.56. The actual input impedance is Zin = zin × 50 = 51.5 + j28.0 . 232 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 235. 13.27. Thecharacteristicadmittance(Y0 = 1/Z0)ofalosslesstransmissionlineis20mS.Thelineisterminated in a load YL = 40 − j20 mS. Make use of the Smith chart to find: a) s: We first find the normalized load admittance, which is yL = YL/Y0 = 2 − j1. This is plotted on the Smith chart below. We then set on the compass the distance between yL and the origin. The same distance is then scribed along the positive real axis, and the value of s is read as 2.6. b) Yin if l = 0.15 λ: First we draw a line from the origin through zL and note its intersection with the WTG scale on the chart outer boundary. We note a reading on that scale of about 0.287 λ. To this we add 0.15 λ, obtaining about 0.437 λ, which we then mark on the chart (0.287 λ is not the precise value, but I have added 0.15 λ to that mark to obtain the point shown on the chart that is near to 0.437 λ. This “eyeballing” method increases the accuracy a little). A line drawn from the 0.437 λ position on the WTG scale to the origin passes through the input admittance. Using the compass, we scribe the distance found in part a across this line to find yin = 0.56 − j0.35, or Yin = 20yin = 11 − j7.0 mS. c) the distance in wavelengths from YL to the nearest voltage maximum: On the admittance chart, the Vmax position is on the negative Ŵr axis. This is at the zero position on the WTL scale. The load is at the approximate 0.213 λ point on the WTL scale, so this distance is the one we want. 233 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 236. 13.28. The wavelength on a certain lossless line is 10cm. If the normalized input impedance is zin = 1 + j2, use the Smith chart to determine: a) s: We begin by marking zin on the chart (see below), and setting the compass at its distance from the origin. We then use the compass at that setting to scribe a mark on the positive real axis, noting the value there of s = 5.8. b) zL, if the length of the line is 12 cm: First, use a straight edge to draw a line from the origin through zin, and through the outer scale. We read the input location as slightly more than 0.312λ on the WTL scale (this additional distance beyond the .312 mark is not measured, but is instead used to add a similar distance when the impedance is transformed). The line length of 12cm corresponds to 1.2 wavelengths. Thus, to transform to the load, we go counter-clockwise twice around the chart, plus 0.2λ, finally arriving at (again) slightly more than 0.012λ on the WTL scale. A line is drawn to the origin from that position, and the compass (with its previous setting) is scribed through the line. The intersection is the normalized load impedance, which we read as zL = 0.173 − j0.078. c) xL, if zL = 2 + jxL, where xL > 0. For this, use the compass at its original setting to scribe through the r = 2 circle in the upper half plane. At that point we read xL = 2.62. 234 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 237. 13.29. A standing wave ratio of 2.5 exists on a lossless 60 line. Probe measurements locate a voltage minimum on the line whose location is marked by a small scratch on the line. When the load is replaced by a short circuit, the minima are 25 cm apart, and one minimum is located at a point 7 cm toward the source from the scratch. Find ZL: We note first that the 25 cm separation between minima imply a wavelength of twice that, or λ = 50 cm. Suppose that the scratch locates the first voltage minimum. With the short in place, the first minimum occurs at the load, and the second at 25 cm in front of the load. The effect of replacing the short with the load is to move the minimum at 25 cm to a new location 7 cm toward the load, or at 18 cm. This is a possible location for the scratch, which would otherwise occur at multiples of a half-wavelength farther away from that point, toward the generator. Our assumed scratch position will be 18 cm or 18/50 = 0.36 wavelengths from the load. Using the Smith chart (see below) we first draw a line from the origin through the 0.36λ point on the wavelengths toward load scale. We set the compass to the length corresponding to the s = r = 2.5 point on the chart, and then scribe this distance through the straight line. We read zL = 0.79 + j0.825, from which ZL = 47.4 + j49.5 . As a check, I will do the problem analytically. First, we use zmin = −18 cm = − 1 2β (φ + π) ⇒ φ = 4(18) 50 − 1 π = 1.382 rad = 79.2◦ Now |ŴL| = s − 1 s + 1 = 2.5 − 1 2.5 + 1 = 0.4286 and so ŴL = 0.4286 1.382. Using this, we find zL = 1 + ŴL 1 − ŴL = 0.798 + j0.823 and thus ZL = zL(60) = 47.8 + j49.3 . 235 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 238. 13.30. A 2-wire line, constructed of lossless wire of circular cross-section is gradually flared into a coupling loop that looks like an egg beater. At the point X, indicated by the arrow in Fig. 13.31, a short circuit is placed across the line. A probe is moved along the line and indicates that the first voltage minimum to the left of X is 16cm from X. With the short circuit removed, a voltage minimum is found 5cm to the left of X, and a voltage maximum is located that is 3 times voltage of the minimum. Use the Smith chart to determine: a) f : No Smith chart is needed to find f , since we know that the first voltage minimum in front of a short circuit is one-half wavelength away. Therefore, λ = 2(16) = 32cm, and (assuming an air-filled line), f = c/λ = 3 × 108/0.32 = 0.938 GHz. b) s: Again, no Smith chart is needed, since s is the ratio of the maximum to the minimum voltage amplitudes. Since we are given that Vmax = 3Vmin, we find s = 3. c) the normalized input impedance of the egg beater as seen looking the right at point X: Now we need the chart. From the figure below, s = 3 is marked on the positive real axis, which determines the compass radius setting. This point is then transformed, using the compass, to the negative real axis, which corresponds to the location of a voltage minimum. Since the first Vmin is 5cm in front of X, this corresponds to (5/32)λ = 0.1563λ to the left of X. On the chart, we now move this distance from the Vmin location toward the load, using the WTL scale. A line is drawn from the origin through the 0.1563λ mark on the WTL scale, and the compass is used to scribe the original radius through this line. The intersection is the normalized input impedance, which is read as zin = 0.86 − j1.06. 236 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 239. 13.31. In order to compare the relative sharpness of the maxima and minima of a standing wave, assume a load zL = 4 + j0 is located at z = 0. Let |V |min = 1 and λ = 1 m. Determine the width of the a) minimum, where |V | < 1.1: We begin with the general phasor voltage in the line: V (z) = V + (e−jβz + Ŵejβz ) With zL = 4+j0, we recognize the real part as the standing wave ratio. Since the load impedance is real, the reflection coefficient is also real, and so we write Ŵ = |Ŵ| = s − 1 s + 1 = 4 − 1 4 + 1 = 0.6 The voltage magnitude is then |V (z)| = V (z)V ∗(z) = V + (e−jβz + Ŵejβz )(ejβz + Ŵe−jβz ) 1/2 = V + 1 + 2Ŵ cos(2βz) + Ŵ2 1/2 Note that with cos(2βz) = ±1, we obtain |V | = V +(1 ± Ŵ) as expected. With s = 4 and with |V |min = 1, we find |V |max = 4. Then with Ŵ = 0.6, it follows that V + = 2.5. The net expression for |V (z)| is then V (z) = 2.5 1.36 + 1.2 cos(2βz) To find the width in z of the voltage minimum, defined as |V | < 1.1, we set |V (z)| = 1.1 and solve for z: We find 1.1 2.5 2 = 1.36 + 1.2 cos(2βz) ⇒ 2βz = cos−1 (−0.9726) Thus 2βz = 2.904. At this stage, we note the the |V |min point will occur at 2βz = π. We therefore compute the range, z, over which |V | < 1.1 through the equation: 2β( z) = 2(π − 2.904) ⇒ z = π − 2.904 2π/1 = 0.0378 m = 3.8 cm where λ = 1 m has been used. b) Determine the width of the maximum, where |V | > 4/1.1: We use the same equation for |V (z)|, which in this case reads: 4/1.1 = 2.5 1.36 + 1.2 cos(2βz) ⇒ cos(2βz) = 0.6298 Since the maximum corresponds to 2βz = 0, we find the range through 2β z = 2 cos−1 (0.6298) ⇒ z = 0.8896 2π/1 = 0.142 m = 14.2 cm 237 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 240. 13.32. A lossless line is operating with Z0 = 40 , f = 20 MHz, and β = 7.5π rad/m. With a short circuit replacing the load, a minimum is found at a point on the line marked by a small spot of puce paint. With the load installed, it is found that s = 1.5 and a voltage minimum is located 1m toward the source from the puce dot. a) Find ZL: First, the wavelength is given by λ = 2π/β = 2/7.5 = 0.2667m. The 1m distance is therefore 3.75λ. With the short installed, the Vmin positions will be at multiples of λ/2 to the left of the short. Therefore, with the actual load installed, the Vmin position as stated would be 3.75λ + nλ/2, which means that a maximum voltage occurs at the load. This being the case, the normalized load impedance will lie on the positive real axis of the Smith chart, and will be equal to the standing wave ratio. Therefore, ZL = 40(1.5) = 60 . b) What load would produce s = 1.5 with |V |max at the paint spot? With |V |max at the paint spot and with the spot an integer multiple of λ/2 to the left of the load, |V |max must also occur at the load. The answer is therefore the same as part a, or ZL = 60 . 13.33. In Fig. 13.14, let ZL = 40 − j10 , Z0 = 50 , f = 800 MHz, and v = c. a) Find the shortest length, d1, of a short-circuited stub, and the shortest distance d that it may be located from the load to provide a perfect match on the main line to the left of the stub: The Smith chart construction is shown on the next page. First we find zL = (40 − j10)/50 = 0.8 − j0.2 and plot it on the chart. Next, we find yL = 1/zL by transforming this point halfway around the chart, where we read yL = 1.17+j0.30. This point is to be transformed to a location at which the real part of the normalized admittance is unity. The g = 1 circle is highlighted on the chart; yL transforms to two locations on it: yin1 = 1 − j0.32 and yin2 = 1 + j0.32. The stub is connected at either of these two points. The stub input admittance must cancel the imaginary part of the line admittance at that point. If yin2 is chosen, the stub must have input admittance of −j0.32. This point is marked on the outer circle and occurs at 0.452 λ on the WTG scale. The length of the stub is found by computing the distance between its input, found above, and the short-circuit position (stub load end), marked as Psc. This distance is d1 = (0.452−0.250)λ = 0.202 λ. With f = 800 MHz and v = c, the wavelength is λ = (3×108)/(8×108) = 0.375 m. The distance is thus d1 = (0.202)(0.375) = 0.758 m = 7.6 cm. This is the shortest of the two possible stub lengths, since if we had used yin1, we would have needed a stub input admittance of +j0.32, which would have required a longer stub length to realize. The length of the main line between its load and the stub attachment point is found on the chart by measuring the distance between yL and yin2, in moving clockwise (toward generator). This distance will be d = [0.500 − (0.178 − 0.138)] λ = 0.46 λ. The actual length is then d = (0.46)(0.375) = 0.173m = 17.3 cm. 238 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 241. 13.33b) Repeat for an open-circuited stub: In this case, everything is the same, except for the load-end position of the stub, which now occurs at the Poc point on the chart. To use the shortest possible stub, we need to use yin1 = 1−j0.32, requiring ys = +j0.32. We find the stub length by moving from Poc to the point at which the admittance is j0.32. This occurs at 0.048 λ on the WTG scale, which thus determines the required stub length. Now d1 = (0.048)(0.375) = 0.18 m = 1.8 cm. The attachment point is found by transforming yL to yin1, where the former point is located at 0.178 λ on the WTG scale, and the latter is at 0.362 λ on the same scale. The distance is then d = (0.362 − 0.178)λ = 0.184λ. The actual length is d = (0.184)(0.375) = 0.069 m = 6.9 cm. 239 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 242. 13.34. The lossless line shown in Fig. 13.32 is operating with λ = 100cm. If d1 = 10cm, d = 25cm, and the line is matched to the left of the stub, what is ZL? For the line to be matched, it is required that the sum of the normalized input admittances of the shorted stub and the main line at the point where the stub is connected be unity. So the input susceptances of the two lines must cancel. To find the stub input susceptance, use the Smith chart to transform the short circuit point 0.1λ toward the generator, and read the input value as bs = −1.37 (note that the stub length is one-tenth of a wavelength). The main line input admittance must now be yin = 1 + j1.37. This line is one-quarter wavelength long, so the normalized load impedance is equal to the normalized input admittance. Thus zL = 1 + j1.37, so that ZL = 300zL = 300 + j411 . 240 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 243. 13.35. A load, ZL = 25 + j75 , is located at z = 0 on a lossless two-wire line for which Z0 = 50 and v = c. a) If f = 300 MHz, find the shortest distance d (z = −d) at which the input impedance has a real part equal to 1/Z0 and a negative imaginary part: The Smith chart construction is shown below. We begin by calculating zL = (25 + j75)/50 = 0.5 + j1.5, which we then locate on the chart. Next, this point is transformed by rotation halfway around the chart to find yL = 1/zL = 0.20 − j0.60, which is located at 0.088 λ on the WTL scale. This point is then transformed toward the generator until it intersects the g = 1 circle (shown highlighted) with a negative imaginary part. This occurs at point yin = 1.0 − j2.23, located at 0.308 λ on the WTG scale. The total distance between load and input is then d = (0.088 + 0.308)λ = 0.396λ. At 300 MHz, and with v = c, the wavelength is λ = 1 m. Thus the distance is d = 0.396 m = 39.6 cm. b) What value of capacitance C should be connected across the line at that point to provide unity stand- ing wave ratio on the remaining portion of the line? To cancel the input normalized susceptance of -2.23, we need a capacitive normalized susceptance of +2.23. We therefore write ωC = 2.23 Z0 ⇒ C = 2.23 (50)(2π × 3 × 108) = 2.4 × 10−11 F = 24 pF 241 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 244. 13.36. The two-wire lines shown in Fig. 13.33 are all lossless and have Z0 = 200 . Find d and the shortest possible value for d1 to provide a matched load if λ = 100cm. In this case, we have a series combination of the loaded line section and the shorted stub, so we use impedances and the Smith chart as an impedance diagram. The requirement for matching is that the total normalized impedance at the junction (consisting of the sum of the input impedances to the stub and main loaded section) is unity. First, we find zL = 100/200 = 0.5 and mark this on the chart (see below). We then transform this point toward the generator until we reach the r = 1 circle. This happens at two possible points, indicated as zin1 = 1 + j.71 and zin2 = 1 − j.71. The stub input impedance must cancel the imaginary part of the loaded section input impedance, or zins = ±j.71. The shortest stub length that accomplishes this is found by transforming the short circuit point on the chart to the point zins = +j0.71, which yields a stub length of d1 = .098λ = 9.8 cm. The length of the loaded section is then found by transforming zL = 0.5 to the point zin2 = 1−j.71, so that zins +zin2 = 1, as required. This transformation distance is d = 0.347λ = 37.7 cm. 242 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 245. 13.37. In the transmission line of Fig. 13.17, RL = Z0 = 50 . Determine and plot the voltage at the load resistor and the current in the battery as functions of time by constructing appropriate voltage and current reflection diagrams: Referring to the figure, closing the switch launches a voltage wave whose value is given by Eq. (50): V + 1 = V0Z0 Rg + Z0 = 50 75 V0 = 2 3 V0 We note that ŴL = 0, since the load impedance is matched to that of the line. So the voltage wave traverses the line and does not reflect. The voltage reflection diagram would be that shown in Fig. 13.18a, except that no waves are present after time t = l/v. Likewise, the current reflection diagram is that of Fig. 13.19a, except, again, no waves exist after t = l/v. The voltage at the load will be just V + 1 = (2/3)V0 for times beyond l/v. The current through the battery is found through I+ 1 = V + 1 Z0 = V0 75 A This current initiates at t = 0, and continues indefinitely. 13.38. Repeat Problem 37, with Z0 = 50 , and RL = Rg = 25 . Carry out the analysis for the time period 0 < t < 8l/v. At the generator end, we have Ŵg = −1/3, as before. The difference is at the load end, where ŴL = −1/3, whereas in Problem 37, the load was matched. The initial wave, as in the last problem, is of magnitude V + = (2/3)V0. Using these values, voltage and current reflection diagrams are constructed, and are shown below: 243 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 246. 13.38. (continued) From the diagrams, voltage and current plots are constructed. First, the load voltage is found by adding voltages along the right side of the voltage diagram at the indicated times. Second, the current through the battery is found by adding currents along the left side of the current reflection diagram. Both plots are shown below, where currents and voltages are expressed to three significant figures. The steady state values, VL = 0.5V and IB = 0.02A, are expected as t → ∞. 13.39. In the transmission line of Fig. 13.17, Z0 = 50 and RL = Rg = 25 . The switch is closed at t = 0 and is opened again at time t = l/4v, thus creating a rectangular voltage pulse in the line. Construct an appropriate voltage reflection diagram for this case and use it to make a plot of the voltage at the load resistor as a function of time for 0 < t < 8l/v (note that the effect of opening the switch is to initiate a second voltage wave, whose value is such that it leaves a net current of zero in its wake): The value of the initial voltage wave, formed by closing the switch, will be V + = Z0 Rg + Z0 V0 = 50 25 + 50 V0 = 2 3 V0 On opening the switch, a second wave, V +′, is generated which leaves a net current behind it of zero. This means that V +′ = −V + = −(2/3)V0. Note also that when the switch is opened, the reflection coefficient at the generator end of the line becomes unity. The reflection coefficient at the load end is ŴL = (25 − 50)/(25 + 50) = −(1/3). The reflection diagram is now constructed in the usual manner, and is shown on the next page. The path of the second wave as it reflects from either end is shown in dashed lines, and is a replica of the first wave path, displaced later in time by l/(4v).a All values for the second wave after each reflection are equal but of opposite sign to the immediately preceding first wave values. The load voltage as a function of time is found by accumulating voltage values as they are read moving up along the right hand boundary of the chart. The resulting function, plotted just below the reflection diagram, is found to be a sequence of pulses that alternate signs. The pulse amplitudes are calculated as follows: 244 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 247. 13.39. (continued) l v < t < 5l 4v : V1 = 1 − 1 3 V + = 0.44 V0 3l v < t < 13l 4v : V2 = − 1 3 1 − 1 3 V + = −0.15 V0 5l v < t < 21l 4v : V3 = 1 3 2 1 − 1 3 V + = 0.049 V0 7l v < t < 29l 4v : V4 = − 1 3 3 1 − 1 3 V + = −0.017 V0 245 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 248. 13.40. In the charged line of Fig. 13.22, the characteristic impedance is Z0 = 100 , and Rg = 300 . The line is charged to initial voltage V0 = 160 V, and the switch is closed at t = 0. Determine and plot the voltage and current through the resistor for time 0 < t < 8l/v (four round trips). This problem accompanies Example 13.6 as the other special case of the basic charged line problem, in which now Rg > Z0. On closing the switch, the initial voltage wave is V + = −V0 Z0 Rg + Z0 = −160 100 400 = −40 V Now, with Ŵg = 1/2 and ŴL = 1, the voltage and current reflection diagrams are constructed as shown below. Plots of the voltage and current at the resistor are then found by accumulating values from the left sides of the two charts, producing the plots as shown. 246 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 249. 13.41. In the transmission line of Fig. 13.34, the switch is located midway down the line, and is closed at t = 0. Construct a voltage reflection diagram for this case, where RL = Z0. Plot the load resistor voltage as a function of time: With the left half of the line charged to V0, closing the switch initiates (at the switch location) two voltage waves: The first is of value −V0/2 and propagates toward the left; the second is of value V0/2 and propagates toward the right. The backward wave reflects at the battery with Ŵg = −1. No reflection occurs at the load end, since the load is matched to the line. The reflection diagram and load voltage plot are shown below. The results are summarized as follows: 0 < t < l 2v : VL = 0 l 2v < t < 3l 2v : VL = V0 2 t > 3l 2v : VL = V0 247 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 250. 13.42. A simple frozen wave generator is shown in Fig. 13.35. Both switches are closed simultaneously at t = 0. Construct an appropriate voltage reflection diagram for the case in which RL = Z0. Determine and plot the load voltage as a function of time: Closing the switches sets up a total of four voltage waves as shown in the diagram below. Note that the first and second waves from the left are of magnitude V0, since in fact we are superimposing voltage waves from the −V0 and +V0 charged sections acting alone. The reflection diagram is drawn and is used to construct the load voltage with time by accumulating voltages up the right hand vertical axis. 248 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 251. CHAPTER 14 14.1. A parallel-plate waveguide is known to have a cutoff wavelength for the m = 1 TE and TM modes of λc1 = 0.4 cm. The guide is operated at wavelength λ = 1 mm. How many modes propagate? The cutoff wavelength for mode m is λcm = 2nd/m, where n is the refractive index of the guide interior. For the first mode, we are given λc1 = 2nd 1 = 0.4 cm ⇒ d = 0.4 2n = 0.2 n cm Now, for mode m to propagate, we require λ ≤ 2nd m = 0.4 m ⇒ m ≤ 0.4 λ = 0.4 0.1 = 4 So, accounting for 2 modes (TE and TM) for each value of m, and the single TEM mode, we will have a total of 9 modes. 14.2. A parallel-plate guide is to be constructed for operation in the TEM mode only over the frequency range 0 < f < 3 GHz. The dielectric between plates is to be teflon (ǫ′ R = 2.1). Determine the maximum allowable plate separation, d: We require that f < fc1, which, using (7), becomes f < c 2nd ⇒ dmax = c 2nfmax = 3 × 108 2 √ 2.1 (3 × 109) = 3.45 cm 14.3. A lossless parallel-plate waveguide is known to propagate the m = 2 TE and TM modes at frequencies as low as 10GHz. If the plate separation is 1 cm, determine the dielectric constant of the medium between plates: Use fc2 = c nd = 3 × 1010 n(1) = 1010 ⇒ n = 3 or ǫR = 9 14.4. A d = 1 cm parallel-plate guide is made with glass (n = 1.45) between plates. If the operating frequency is 32 GHz, which modes will propagate? For a propagating mode, we require f > fcm Using (7) and the given values, we write f > mc 2nd ⇒ m < 2f nd c = 2(32 × 109)(1.45)(.01) 3 × 108 = 3.09 The maximum allowed m in this case is thus 3, and the propagating modes will be TM1, TE1, TM2, TE2, TM3, and TE3. 14.5. For the guide of Problem 14.4, and at the 32 GHz frequency, determine the difference between the group delays of the highest order mode (TE or TM) and the TEM mode. Assume a propagation distance of 10 cm: From Problem 14.4, we found mmax = 3. The group velocity of a TE or TM mode for m = 3 is vg3 = c n 1 − fc3 f 2 where fc3 = 3(3 × 1010) 2(1.45)(1) = 3.1 × 1010 = 31 GHz 249 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 252. 14.5. (continued) Thus vg3 = 3 × 1010 1.45 1 − 31 32 2 = 5.13 × 109 cm/s For the TEM mode (assuming no material dispersion) vg,T EM = c/n = 3 × 1010/1.45 = 2.07 × 1010 cm/s. The group delay difference is now tg = z 1 vg3 − 1 vg,T EM = 10 1 5.13 × 109 − 1 2.07 × 1010 = 1.5 ns 14.6. The cutoff frequency of the m = 1 TE and TM modes in a parallel-plate guide is known to be fc1 = 7.5 GHz. The guide is used at wavelength λ = 1.5 cm. Find the group velocity of the m = 2 TE and TM modes. First we know that fc2 = 2fc1 = 15 GHz. Then f = c/λ = 3 × 108/.015 = 20 GHz. Now, using (23), vg2 = c n 1 − fc2 f 2 = c n 1 − 15 20 2 = 2 × 108 /n m/s n was not specified in the problem. 14.7. A parallel-plate guide is partially filled with two lossless dielectrics (Fig. 14.23) where ǫ′ R1 = 4.0, ǫ′ R2 = 2.1, and d = 1 cm. At a certain frequency, it is found that the TM1 mode propagates through the guide without suffering any reflective loss at the dielectric interface. a) Find this frequency: The ray angle is such that the wave is incident on the interface at Brewster’s angle. In this case θB = tan−1 2.1 4.0 = 35.9◦ The ray angle is thus θ = 90 − 35.9 = 54.1◦. The cutoff frequency for the m = 1 mode is fc1 = c 2d ǫ′ R1 = 3 × 1010 2(1)(2) = 7.5 GHz The frequency is thus f = fc1/ cos θ = 7.5/ cos(54.1◦) = 12.8 GHz. b) Is the guide operating at a single TM mode at the frequency found in part a? The cutoff frequency for the next higher mode, TM2 is fc2 = 2fc1 = 15 GHz. The 12.8 GHz operating frequency is below this, so TM2 will not propagate. So the answer is yes. 14.8. In the guide of Problem 14.7, it is found that m = 1 modes propagating from left to right totally reflect at the interface, so that no power is transmitted into the region of dielectric constant ǫ′ R2. a) Determine the range of frequencies over which this will occur: For total reflection, the ray angle measured from the normal to the interface must be greater than or equal to the critical angle, θc, where sin θc = (ǫ′ R2/ǫ′ R1)1/2. The minimum mode ray angle is then θ1 min = 90◦ −θc. Now, using (5), we write 90◦ − θc = cos−1 π kmind = cos−1 πc 2πfmind √ 4 = cos−1 c 4dfmin 250 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 253. 14.8a. (continued) Now cos(90 − θc) = sin θc = ǫ′ R2 ǫ′ R1 = c 4dfmin Therefore fmin = c/(2 √ 2.1d) = (3 × 108)/(2 √ 2.1(.01)) = 10.35 GHz. The frequency range is thus f > 10.35 GHz. b) Does your part a answer in any way relate to the cutoff frequency for m = 1 modes in any region? We note that fmin = c/(2 √ 2.1d) = fc1 in guide 2. To summarize, as frequency is lowered, the ray angle in guide 1 decreases, which leads to the incident angle at the interface increasing to eventually reach and surpass the critical angle. At the critical angle, the refracted angle in guide 2 is 90◦, which corresponds to a zero degree ray angle in that guide. This defines the cutoff condition in guide 2. So it would make sense that fmin = fc1(guide 2). 14.9. A rectangular waveguide has dimensions a = 6 cm and b = 4 cm. a) Over what range of frequencies will the guide operate single mode? The cutoff frequency for mode mp is, using Eq. (54): fc,mn = c 2n m a 2 + p b 2 where n is the refractive index of the guide interior. We require that the frequency lie between the cutoff frequencies of the T E10 and T E01 modes. These will be: fc10 = c 2na = 3 × 108 2n(.06) = 2.5 × 109 n fc01 = c 2nb = 3 × 108 2n(.04) = 3.75 × 109 n Thus, the range of frequencies over which single mode operation will occur is 2.5 n GHz < f < 3.75 n GHz b) Over what frequency range will the guide support both T E10 and T E01 modes and no others? We note first that f must be greater than fc01 to support both modes, but must be less than the cutoff frequency for the next higher order mode. This will be fc11, given by fc11 = c 2n 1 .06 2 + 1 .04 2 = 30c 2n = 4.5 × 109 n The allowed frequency range is then 3.75 n GHz < f < 4.5 n GHz 251 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 254. 14.10. Two rectangular waveguides are joined end-to-end. The guides have identical dimensions, where a = 2b. One guide is air-filled; the other is filled with a lossless dielectric characterized by ǫ′ R. a) Determine the maximum allowable value of ǫ′ R such that single mode operation can be simultane- ously ensured in both guides at some frequency: Since a = 2b, the cutoff frequency for any mode in either guide is written using (54): fcmp = mc 4nb 2 + pc 2nb 2 where n = 1 in guide 1 and n = ǫ′ R in guide 2. We see that, with a = 2b, the next modes (having the next higher cutoff frequency) above TE10 with be TE20 and TE01. We also see that in general, fcmp(guide 2) < fcmp(guide 1). To assure single mode operation in both guides, the operating frequency must be above cutoff for TE10 in both guides, and below cutoff for the next mode in both guides. The allowed frequency range is therefore fc10(guide 1) < f < fc20(guide 2). This leads to c/(2a) < f < c/(a ǫ′ R). For this range to be viable, it is required that ǫ′ R < 4. b) Write an expression for the frequency range over which single mode operation will occur in both guides; your answer should be in terms of ǫ′ R, guide dimensions as needed, and other known constants: This was already found in part a: c 2a < f < c ǫ′ R a where ǫ′ R < 4. 14.11. An air-filled rectangular waveguide is to be constructed for single-mode operation at 15 GHz. Specify the guide dimensions, a and b, such that the design frequency is 10/while being 10% lower than the cutoff frequency for the next higher-order mode: For an air-filled guide, we have fc,mp = mc 2a 2 + pc 2b 2 For TE10 we have fc10 = c/2a, while for the next mode (TE01), fc01 = c/2b. Our requirements state that f = 1.1fc10 = 0.9fc01. So fc10 = 15/1.1 = 13.6 GHz and fc01 = 15/0.9 = 16.7 GHz. The guide dimensions will be a = c 2fc10 = 3 × 1010 2(13.6 × 109) = 1.1 cm and b = c 2fc01 = 3 × 1010 2(16.7 × 109) = 0.90 cm 14.12. Using the relation Pav = (1/2)Re{Es × H∗ s }, and Eqs. (44) through (46), show that the average power density in the TE10 mode in a rectangular waveguide is given by Pav = β10 2ωµ E2 0 sin2 (κ10x) az W/m2 (note that the sin term is erroneously to the first power in the original problem statement). Inspecting (44) through (46), we see that (46) includes a factor of j, and so would lead to an imaginary part of the 252 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 255. total power when the cross product with Ey is taken. Therefore, the real power in this case is found through the cross product of (44) with the complex conjugate of (45), or Pav = 1 2 Re Eys × H∗ xs = β10 2ωµ E2 0 sin2 (κ10x) az W/m2 14.13. Integrate the result of Problem 14.12 over the guide cross-section 0 < x < a, 0 < y < b, to show that the power in Watts transmitted down the guide is given as P = β10ab 4ωµ E2 0 = ab 4η E2 0 sin θ10 W where η = √ µ/ǫ (note misprint in problem statement), and θ10 is the wave angle associated with the TE10 mode. Interpret. First, the integration: P = b 0 a 0 β10 2ωµ E2 0 sin2 (κ10x) az · az dx dy = β10ab 4ωµ E2 0 Next, from (20), we have β10 = ω √ µǫ sin θ10, which, on substitution, leads to P = ab 4η E2 0 sin θ10 W with η = µ ǫ The sin θ10 dependence demonstrates the principle of group velocity as energy velocity (or power). This was considered in the discussion leading to Eq. (23). 14.14. Show that the group dispersion parameter, d2β/dω2, for given mode in a parallel-plate or rectangular waveguide is given by d2β dω2 = − n ωc ωc ω 2 1 − ωc ω 2 −3/2 where ωc is the radian cutoff frequency for the mode in question (note that the first derivative form was already found, resulting in Eq. (23)). First, taking the reciprocal of (23), we find dβ dω = n c 1 − ωc ω 2 −1/2 Taking the derivative of this equation with respect to ω leads to d2β dω2 = n c − 1 2 1 − ωc ω 2 −3/2 2ω2 c ω3 = − n ωc ωc ω 2 1 − ωc ω 2 −3/2 14.15. Consider a transform-limited pulse of center frequency f = 10 GHz and of full-width 2T = 1.0 ns. The pulse propagates in a lossless single mode rectangular guide which is air-filled and in which the 10 GHz operating frequency is 1.1 times the cutoff frequency of the T E10 mode. Using the result of Problem 14.14, determine the length of the guide over which the pulse broadens to twice its initial width: The broadened pulse will have width given by T ′ = T 2 + ( τ)2, where τ = β2L/T for a transform limited pulse (assumed gaussian). β2 is the Problem 14.14 result evaluated at the operating frequency, or β2 = d2β dω2 |ω=10 GHz = − 1 (2π × 1010)(3 × 108) 1 1.1 2 1 − 1 1.1 2 −3/2 = 6.1 × 10−19 s2 /m = 0.61 ns2 /m Now τ = 0.61L/0.5 = 1.2L ns. For the pulse width to double, we have T ′ = 1 ns, and (.05)2 + (1.2L)2 = 1 ⇒ L = 0.72 m = 72 cm 253 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 256. 14.15. (continued) What simple step can be taken to reduce the amount of pulse broadening in this guide, while maintaining the same initial pulse width? It can be seen that β2 can be reduced by increasing the operating frequency relative to the cutoff frequency; i.e., operate as far above cutoff as possible, without allowing the next higher-order modes to propagate. 14.16. A symmetric dielectric slab waveguide has a slab thickness d = 10 µm, with n1 = 1.48 and n2 = 1.45. If the operating wavelength is λ = 1.3 µm, what modes will propagate? We use the condition expressed through (77): k0d n2 1 − n2 2 ≥ (m − 1)π. Since k0 = 2π/λ, the condition becomes 2d λ n2 1 − n2 2 ≥ (m − 1) ⇒ 2(10) 1.3 (1.48)2 − (1.45)2 = 4.56 ≥ m − 1 Therefore, mmax = 5, and we have TE and TM modes for which m = 1, 2, 3, 4, 5 propagating (ten total). 14.17. A symmetric slab waveguide is known to support only a single pair of TE and TM modes at wavelength λ = 1.55 µm. If the slab thickness is 5 µm, what is the maximum value of n1 if n2 = 3.3 (assume 3.30)? Using (78) we have 2πd λ n2 1 − n2 2 < π ⇒ n1 < λ 2d + n2 2 = 1.55 2(5) + (3.30)2 = 3.32 14.18. n1 = 1.50, n2 = 1.45, and d = 10 µm in a symmetric slab waveguide (note that the index values were reversed in the original problem statement). a) What is the phase velocity of the m = 1 TE or TM mode at cutoff? At cutoff, the mode propagates in the slab at the critical angle, which means that the phase velocity will be equal to that of a plane wave in the upper or lower media of index n2. Phase velocity will therefore be vp(cutoff) = c/n2 = 3 × 108/1.45 = 2.07 × 108 m/s. b) What is the phase velocity of the m = 2 TE or TM modes at cutoff? The reasoning of part a applies to all modes, so the answer is the same, or 2.07 × 108 m/s. 14.19. An asymmetric slab waveguide is shown in Fig. 14.24. In this case, the regions above and below the slab have unequal refractive indices, where n1 > n3 > n2 (note error in problem statement). a) Write, in terms of the appropriate indices, an expression for the minimum possible wave angle, θ1, that a guided mode may have: The wave angle must be equal to or greater than the critical angle of total reflection at both interfaces. The minimum wave angle is thus determined by the greater of the two critical angles. Since n3 > n2, we find θmin = θc,13 = sin−1(n3/n1). b) Write an expression for the maximum phase velocity a guided mode may have in this structure, using given or known parameters: We have vp,max = ω/βmin, where βmin = n1k0 sin θ1,min = n1k0n3/n1 = n3k0. Thus vp,max = ω/(n3k0) = c/n3. 14.20. A step index optical fiber is known to be single mode at wavelengths λ > 1.2 µm. Another fiber is to be fabricated from the same materials, but is to be single mode at wavelengths λ > 0.63 µm. By what percentage must the core radius of the new fiber differ from the old one, and should it be larger or smaller? We use the cutoff condition, given by (80): λ > 2πa 2.405 n2 1 − n2 2 254 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 257. 14.20. (continued) With λ reduced, the core radius, a, must also be reduced by the same fraction. Therefore, the percentage reduction required in the core radius will be % = 1.2 − .63 1.2 × 100 = 47.5% 14.21. A short dipole carrying current I0 cos ωt in the az direction is located at the origin in free space. a) If β = 1 rad/m, r = 2 m, θ = 45◦, φ = 0, and t = 0, give a unit vector in rectangular components that shows the instantaneous direction of E: In spherical coordinates, the components of E are given by (82) and (83): Er = I0dη 2π cos θe−j2πr/λ 1 r2 + λ j2πr3 Eθ = I0dη 4π sin θe−j2πr/λ j 2π λr + 1 r2 + λ j2πr3 Since we want a unit vector at t = 0, we need only the relative amplitudes of the two components, but we need the absolute phases. Since θ = 45◦, sin θ = cos θ = 1/ √ 2. Also, with β = 1 = 2π/λ, it follows that λ = 2π m. The above two equations can be simplified by these substitutions, while dropping all amplitude terms that are common to both. Obtain Ar = 1 r2 + 1 jr3 e−jr Aθ = 1 2 j 1 r + 1 r2 + 1 jr3 e−jr Now with r = 2 m, we obtain Ar = 1 4 − j 1 8 e−j2 = 1 4 (1.12)e−j26.6◦ e−j2 Aθ = j 1 4 + 1 8 − j 1 16 e−j2 = 1 4 (0.90)ej56.3◦ e−j2 The total vector is now A = Arar + Aθ aθ . We can normalize the vector by first finding the magnitude: |A| = √ A · A∗ = 1 4 (1.12)2 + (0.90)2 = 0.359 Dividing the field vector by this magnitude and converting 2 rad to 114.6◦, we write the normalized vector as ANs = 0.780e−j141.2◦ ar + 0.627e−58.3◦ aθ In real instantaneous form, this becomes AN (t) = Re ANsejωt = 0.780 cos(ωt − 141.2◦ )ar + 0.627 cos(ωt − 58.3◦ )aθ We evaluate this at t = 0 to find AN (0) = 0.780 cos(141.2◦ )ar + 0.627 cos(58.3◦ )aθ = −0.608ar + 0.330aθ 255 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 258. 14.21a. (continued) Dividing by the magnitude, (0.608)2 + (0.330)2 = 0.692, we obtain the unit vector at t = 0: aN (0) = −0.879ar + 0.477aθ . We next convert this to cartesian components: aNx = aN (0) · ax = −0.879 sin θ cos φ + 0.477 cos θ cos φ = 1 √ 2 (−0.879 + 0.477) = −0.284 aNy = aN (0) · ay = −0.879 sin θ sin φ + 0.477 cos θ sin φ = 0 since φ = 0 aNz = aN (0) · az = −0.879 cos θ − 0.477 sin θ = 1 √ 2 (−0.879 − 0.477) = −0.959 The final result is then aN (0) = −0.284ax − 0.959az b) What fraction of the total average power is radiated in the belt, 80◦ < θ < 100◦? We use the far-zone phasor fields, (84) and (85), and first find the average power density: Pavg = 1 2 Re[EθsH∗ φs] = I2 0 d2η 8λ2r2 sin2 θ W/m2 We integrate this over the given belt, an at radius r: Pbelt = 2π 0 100◦ 80◦ I2 0 d2η 8λ2r2 sin2 θ r2 sin θ dθ dφ = πI2 0 d2η 4λ2 100◦ 80◦ sin3 θ dθ Evaluating the integral, we find Pbelt = πI2 0 d2η 4λ2 − 1 3 cos θ sin2 θ + 2 100 80 = (0.344) πI2 0 d2η 4λ2 The total power is found by performing the same integral over θ, where 0 < θ < 180◦. Doing this, it is found that Ptot = (1.333) πI2 0 d2η 4λ2 The fraction of the total power in the belt is then f = 0.344/1.333 = 0.258. 14.22. Prepare a curve, r vs. θ in polar coordinates, showing the locus in the φ = 0 plane where: a) the radiation field |Eθs| is one-half of its value at r = 104 m, θ = π/2: Assuming the far field approximation, we use (84) to set up the equation: |Eθs| = I0dη 2λr sin θ = 1 2 × I0dη 2 × 104λ ⇒ r = 2 × 104 sin θ b) the average radiated power density, Pr,av, is one-half of its value at r = 104 m, θ = π/2. To find the average power, we use (84) and (85) in Pr,av = 1 2 Re{EθsH∗ φs} = 1 2 I2 0 d2η 4λ2r2 sin2 θ = 1 2 × 1 2 I2 0 d2η 4λ2(108) ⇒ r = √ 2 × 104 sin θ 256 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 259. 14.22. (continued) The polar plots for field (r = 2 × 104 sin θ) and power (r = √ 2 × 104 sin θ) are shown below. Both are circles. 14.23. Two short antennas at the origin in free space carry identical currents of 5 cos ωt A, one in the az direction, one in the ay direction. Let λ = 2π m and d = 0.1 m. Find Es at the distant point: a) (x = 0, y = 1000, z = 0): This point lies along the axial direction of the ay antenna, so its contribution to the field will be zero. This leaves the az antenna, and since θ = 90◦, only the Eθs component will be present (as (82) and (83) show). Since we are in the far zone, (84) applies. We use θ = 90◦, d = 0.1, λ = 2π, η = η0 = 120π, and r = 1000 to write: Es = Eθsaθ = j I0dη 2λr sin θe−j2πr/λ aθ = j 5(0.1)(120π) 4π(1000) e−j1000 aθ = j(1.5 × 10−2 )e−j1000 aθ = −j(1.5 × 10−2 )e−j1000 az V/m b) (0, 0, 1000): Along the z axis, only the ay antenna will contribute to the field. Since the distance is the same, we can apply the part a result, modified such the the field direction is in −ay: Es = −j(1.5 × 10−2)e−j1000 ay V/m c) (1000, 0, 0): Here, both antennas will contribute. Applying the results of parts a and b, we find Es = −j(1.5 × 10−2)(ay + az). d) Find E at (1000, 0, 0) at t = 0: This is found through E(t) = Re Esejωt = (1.5 × 10−2 ) sin(ωt − 1000)(ay + az) Evaluating at t = 0, we find E(0) = (1.5 × 10−2)[− sin(1000)](ay + az) = −(1.24 × 10−2)(ay + az) V/m. e) Find |E| at (1000, 0, 0) at t = 0: Taking the magnitude of the part d result, we find |E| = 1.75 × 10−2 V/m. 257 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 260. 14.24. A short current element has d = 0.03λ. Calculate the radiation resistance for each of the following current distributions: a) uniform: In this case, (86) applies directly and we find Rrad = 80π2 d λ 2 = 80π2 (.03)2 = 0.711 b) linear, I(z) = I0(0.5d − |z|)/0.5d: Here, the average current is 0.5I0, and so the average power drops by a factor of 0.25. The radiation resistance therefore is down to one-fourth the value found in part a, or Rrad = (0.25)(0.711) = 0.178 . c) step, I0 for 0 < |z| < 0.25d and 0.5I0 for 0.25d < |z| < 0.5d: In this case the average current on the wire is 0.75I0. The radiated power (and radiation resistance) are down to a factor of (0.75)2 times their values for a uniform current, and so Rrad = (0.75)2(0.711) = 0.400 . 14.25. A dipole antenna in free space has a linear current distribution. If the length is 0.02λ, what value of I0 is required to: a) provide a radiation-field amplitude of 100 mV/m at a distance of one mile, at θ = 90◦: With a linear current distribution, the peak current, I0, occurs at the center of the dipole; current decreases linearly to zero at the two ends. The average current is thus I0/2, and we use Eq. (84) to write: |Eθ | = I0dη0 4λr sin(90◦ ) = I0(0.02)(120π) (4)(5280)(12)(0.0254) = 0.1 ⇒ I0 = 85.4 A b) radiate a total power of 1 watt? We use Pavg = 1 4 1 2 I2 0 Rrad where the radiation resistance is given by Eq. (86), and where the factor of 1/4 arises from the average current of I0/2: We obtain Pavg = 10π2I2 0 (0.02)2 = 1 ⇒ I0 = 5.03 A. 14.26. A monopole antenna in free space, extending vertically over a perfectly conducting plane, has a linear current distribution. If the length of the antenna is 0.01λ, what value of I0 is required to a) provide a radiation field amplitude of 100 mV/m at a distance of 1 mi, at θ = 90◦: The image antenna below the plane provides a radiation pattern that is identical to a dipole antenna of length 0.02λ. The radiation field is thus given by (84) in free space, where θ = 90◦, and with an additional factor of 1/2 included to account for the linear current distribution: |Eθ | = 1 2 I0dη0 2λr ⇒ I0 = 4r|Eθ | (d/λ)η0 = 4(5289)(12 × .0254)(100 × 10−3) (.02)(377) = 85.4 A b) radiate a total power of 1W: For the monopole over the conducting plane, power is radiated only over the upper half-space. This reduces the radiation resistance of the equivalent dipole antenna by a factor of one-half. Additionally, the linear current distribution reduces the radiation resistance of a dipole having uniform current by a factor of one-fourth. Therefore, Rrad is one-eighth the value obtained from (86), or Rrad = 10π2(d/λ)2. The current magnitude is now I0 = 2Pav Rrad 1/2 = 2(1) 10π2(d/λ)2 1/2 = √ 2 √ 10 π(.02) = 7.1 A 258 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334
- 261. 14.27. The radiation field of a certain short vertical current element is Eθs = (20/r) sin θ e−j10πr V/m if it is located at the origin in free space. a) Find Eθs at P (r = 100, θ = 90◦, φ = 30◦): Substituting these values into the given formula, find Eθs = 20 100 sin(90◦ )e−j10π(100) = 0.2e−j1000π V/m b) Find Eθs at P if the vertical element is located at A(0.1, 90◦, 90◦): This places the element on the y axis at y = 0.1. As a result of moving the antenna from the origin to y = 0.1, the change in distance to point P is negligible when considering the change in field amplitude, but is not when considering the change in phase. Consider lines drawn from the origin to P and from y = 0.1 to P. These lines can be considered essentially parallel, and so the difference in their lengths is l . = 0.1 sin(30◦), with the line from y = 0.1 being shorter by this amount. The construction and arguments are similar to those used in the discussion of the electric dipole in Sec. 4.7. The electric field is now the result of part a, modified by including a shorter distance, r, in the phase term only. We show this as an additional phase factor: Eθs = 0.2e−j1000π ej10π(0.1 sin 30 = 0.2e−j1000π ej0.5π V/m c) Find Eθs at P if identical elements are located at A(0.1, 90◦, 90◦) and B(0.1, 90◦, 270◦): The original element of part b is still in place, but a new one has been added at y = −0.1. Again, constructing a line between B and P , we find, using the same arguments as in part b, that the length of this line is approximately 0.1 sin(30◦) longer than the distance from the origin to P. The part b result is thus modified to include the contribution from the second element, whose field will add to that of the first: Eθs = 0.2e−j1000π ej0.5π + e−j0.5π = 0.2e−j1000π 2 cos(0.5π) = 0 The two fields are out of phase at P under the approximations we have used. 259 Descargado por mauricio cartagena ([email protected]) lOMoARcPSD|5423334