6.641 Electromagnetic Fields, Forces, and Motion

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6.641 Electromagnetic Fields, Forces, and Motion
Spring 2009
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6.641 — Electromagnetic Fields, Forces, and Motion
Spring 2009
Problem Set 2 - Solutions
Prof. Markus Zahn
MIT OpenCourseWare
Problem 2.1
A
y
φ
x
Surface S
Curve C
Figure 1: Surface S and contour C for using Ampere’s law (Image by MIT OpenCourseWare.)
→
−
Step 1: Find field of z-directed line current, I , at x = y = 0.
−
→
I = I îz
→
−
By symmetry: H = Hφˆiφ in cylindrical coordinates. By Ampere:
�
�
→
− −
→
−
→ →
H ·d l =
J · d−
a
C
S
� �� �
current going through S
(2πr)Hφ = I
Hφ =
I
îφ
2πr
îφ = �
→
−
H =
−y
x2
+
(1)
y2
x
îx + �
îy
2
x + y 2
I
(−yˆix + xîy )
2π(x2 + y 2 )
→
−
Step 2: Find solution by adding two translated H fields:
−
→
→
−
→
−
H total = H I1 + H I2
�
�
�
�
I1
d
I2
d
ˆ
ˆ
� −(y − )îx + xiy +
� −(y + )îx + xiy
�
�
=
2
2
2π x2 + (y − d2 )2
2π x2 + (y + d2 )2
1
Problem Set 2
6.641, Spring 2009
B
Step 3: We want field in y = 0 plane so y → 0.
i
I1 = I, I2 = 0
−
→
H tot =
I
2π(x2 +
�
d
îx + xˆiy
d2
2
)
4
�
ii
I1 = I, I2 = I
−
→
H tot =
I
2
π(x +
�
d2
4
)
xîy
�
iii
I1 = I, I2 = −I
→
−
H tot =
I
+
2π(x2
[dîx ]
d2
4 )
C
→
−
→
−
−
F = q→
v × (µ0 H )
so
�
�
��
→
−
→
−
→
d F = dq −
v × µ0 H
In our problem the line current is a moving line charge, so dq = λdl
�
�
→
−
→
−
→
−
−
d F = λ→
v × µ0 H dl = I¯ × (µ0 H )dl
→
−
F =
�
0
L
→
−
−
→
→
→
−
−
I × (µ0 H )dl = ( I × µ0 H )L
So
Force
→
→
−
−
= I × (µ0 H )
Length
−−→
We don’t need to know HI1 since I1 cannot exert a net force on itself. So we need a field of I2
� �
�
�
d
I
−
y
+
î
+
x
î
2
x
y
2
−−→
�
HI2 =
�
�2 �
2
2π x + y + d2
I1 is at x = 0, y = d2 , so x → 0, y →
d
2
above.
−I2
→ −I2 d
−
H =
îx =
îx
2πd2
2πd
2
Problem Set 2
6.641, Spring 2009
Force
→
→
−
−
= ( I1 ) × (µ0 H ) = (I1ˆiz ) ×
Length
−µ0 I1 I2
îy
2πd
(i)
I1 = I,
�
�
−µ0 I2 ˆ
ix
2πd
=
I2 = 0
Force
=0
Length
(ii)
I1 = I,
I2 = I
Force
−µ0 I 2
=
îy
Length
2πd
(iii)
I2 = −I
I1 = I,
Force
µ0 I 2
=+
îy
Length
2πd
Problem 2.2
A
The idea here is similar to applying the chain rule in a 1D problem
d
dx
�
1
f (x)
�
�
d
=
df
�
1
f (x)
�� �
�
�
df
−f (x)
= 2
dx
f (x)
−
→
f (x) corresponds to |→
r −−
r � |. So, by diff. f (x) we get part of the answer to the derivative of
can just do it directly too.
�
−
−
|→
r −→
r � | = (x − x� )2 + (y − y � )2 + (z − z � )2
�
�
�
�
�
�
�
�
1
∂
1
∂
1
∂
1
= îx
+ îy
+ îz
� −
→
→
→
−
−
−
−
∂x |−
∂y |→
∂z |→
r −→
r �|
|→
r −−
r �|
r −−
r �|
r −→
r �
|
So we can apply the trick above by just considering x, y, and z components separately.
�
∂ →
∂ ��
−
|−
r −→
r �| =
(x − x� )2 + (y − y � )2 + (z − z � )2
∂x
∂x
x − x�
= �
(x − x� )2 + (y − y � )2 + (z − z � )2
x − x�
= →
−
→
|r −−
r � |
Similarly,
∂
∂x
∂ →
z − z �
∂ −
y − y�
−
−
|→
r −→
r �| = →
|−
r −→
r �| = →
.
� and
−
→
−
−
−
∂y
∂z
|r − r |
|r −→
r �|
�
1
→
−
|−
r −→
r�
�
=
∂ →
−
− ∂x
|−
r −→
r �|
−
−
|→
r −→
r � |2
and so on for y and z.
→
→
|−
r −−
r � |2 = (x − x� )2 + (y − y � )2 + (z − z � )2
3
1
f (x) .
But we
Problem Set 2
6.641, Spring 2009
so:
�
�
� − (x − x� )î + (y − y � )iˆ + (z − z � )iˆ
x
y
z
1
� −
=
3
−
|→
r −→
r �|
[(x − x� )2 + (y − y � )2 + (z − z � )2 ] 2
�
3
−
−
Denominators = |→
r −→
r � | 2 . Thus,
�
�
−
−
−
−
−1
1
−(→
r −→
r �)
(→
r −→
r �)
� −
= −
�
� 3 = −
� 2 →
→
→
−
→
→
−
→
→
−
−
→
−
|r − r |
|r − r |
| r − r | | r − r �|
−îr� r
= →
→
|−
r −−
r � |2
B
Follows from (A) immediately by substitution. Remember � is derived in terms of unprimed x, y, z. � does
not affect x� , y � , z � .
C
−
Φ(→
r)=
−�
→
�
V�
−
ρ(→
r � )dV �
−
−
4πε0 |→
r −→
r �|
C
. In this sense, ρ → ∞ at the ring. We can represent
ρ( r ) = charge density in mC3 . We have λ in units of m
�
−
this in cylindrical coordinates by ρ(→
r ) = λ0 δ(z)δ(r − a). Then we can evaluate the triple integral
� � �
λ0 δ(z)δ(r − a)rdrdφdz
=
→
−
4π�0 |−
r −→
r �|
2π
�
0
λ0 adφ
4π�0 |r − r� |
But, we can skip that unnecessary work by simply considering infinitesimal charges (adφ)λ0 around the ring.
y
x
dφ a
adφ
Figure 2: A ring of line charge with infinitesimal charge elements dq = λ0 adφ. (Image by MIT OpenCourseWare.)
We only care about z axis in this problem as well, so, by symmetry, there is no field in the x and y
directions.
4
Problem Set 2
→
Φ(−
r)=
−
Φ(→
r)=
6.641, Spring 2009
2π
�
λ0 (adφ)
4πε0
0
1
(a2 + z 2 ) 2
� �� �
distance from
the charge
element λ0 adφ
to the point z
on the z-axis
λ0 a
1
2ε0 (a2 + z 2 ) 2
on the z-axis.
0
0
⎛
⎞
∂ �
∂ ⎟
→
−
⎜ ∂ �
→
E = −�Φ(−
r ) = − ⎝îx �
Φ + îy �Φ + îz Φ⎠
∂x
∂y
∂z
�
�
∂
→
−
E = −îz
∂z
�
→
−
E = îz
aλ0 z
�
λ0 a
1
2ε0 (a2 + z 2 ) 2
3
2ε0 (a2 + z 2 ) 2
−
Using the equation from the Problem 2.2 Statement with z component only (symmetry) and with ρ(→
r � )dV � →
λ0 adφ
� 2π
λ0 adφ cos θ
z
Ez (z) =
, cos θ =
1
4πε0 (z 2 + a2 )
(a2 + z 2 ) 2
0
�
2π
=
0
=
λ0 az
(a2
+
3
z2) 2
dφ
4πε0
λ0 az
3
2ε0 (a2 + z 2 ) 2
Limit |z | → ∞
�
a2 + z 2 → |z |
Φ(z) ≈
λ0 a
2ε0
(a2
+
1
z2) 2
≈
2πλ0 a
Q
≈
4πε0 |z|
4πε0 |z|
Q = 2πλ0 a (total charge on loop). Φ(z) looks like potential from point charge in far field.
� Q
z>0
λ0 az
λ0 az
2
0 |z|
Ez =
= 4πε−Q
3 ≈
3
2
2
2ε
|
z
|
2
z<0
2ε0 (a + z )
0
4πε |z|2
0
5
Problem Set 2
6.641, Spring 2009
a
r
dr
Figure 3: A line charge ring of width dr in the disk (Image by MIT OpenCourseWare.)
D
From (C), Φ =
λ0 r
1
2ε0 (r 2 +z 2 ) 2
for a ring of radius r. But now we have σ0 , not λ0 . How do we express λ0 in
terms of σ0 ? Take a ring of width dr in the disk (see figure). Total charge in the ring =
(r)(2π) (dr)σ0 .
� �� �
circumference
Line charge density = λ0 =
So: λ0 = σ0 dr
total charge
length
= σ0 dr
σ0 rdr
dΦ =
1
2ε0 (r2 + z 2 ) 2
� a
� a
σ0 rdr
σ0
rdr
Φtotal =
1 =
1
2
2
2
2ε
2
0 0 (r + z 2 ) 2
0 2ε0 (r + z )
��r=a
�
σ0 �� 2
σ0 �� 2
�
=
=
r + z2 �
a + z 2 − |z |
2ε0
2ε0
r=0
�
�
σ0
1
1
−
→
√
√
E = −�Φtotal =
z
−
iz
2ε0
a2 + z 2
z2
E
As z → ∞,
1
(a2 + z 2 ) 2 → |z| +
Φtotal →
a2
;
2|z |
1
(a2 + z 2 )− 2 →
1
|z|
�
1−
πa2 σ0
4�0 π |z |
2
¯ → πa σ0 iz
E
4πε0 z 2
just like a point charge of σ0 πa2 .
F
As a → ∞, z in the
Φtotal →
√
a2 + z 2 can be neglected, so
σ0
[a − |z|]
2ε0
6
a2
2z 2
�
Problem Set 2
6.641, Spring 2009
�
� � σ0
σ0 z 1
0
− 0 = 2ε
Ez →
−σ0
2ε0 |z|
2ε
z>0
z<0
0
just like a sheet charge.
Problem 2.3
A
By the divergence theorem:
i
�
V
−
→
� · (� × A )dV =
�
S
→
−
−
(� × A ) · d→
a
where S encloses V .
ii By Stokes’ Theorem:
�
�
→
→
−
− −
→
−
→
(� × A ) · d a =
A ·d l
S�
C
Suppose S is as in figure 4
S
Figure 4: Closed surface S (Image by MIT OpenCourseWare.)
and S � is as in figure 5
S
!
C
Figure 5: Open surface S � bounded by contour C (Image by MIT OpenCourseWare.)
i.e., S � is the same as S, except for the contour curve C, which makes S � slightly unclosed. Now consider
limit as C → 0 (Figure 6)
7
Problem Set 2
6.641, Spring 2009
Figure 6: Limit as C → 0 (Image by MIT OpenCourseWare.)
� →
�
−
→
−
→
−
→
In limit C → 0, S � → S. If C is 0, then C A · d l = 0. By equation (ii), S (� × A ) · d−
a = 0. By
�
−
→
equation (i), V � · (� × A )dV = 0. Since V can be any volume, argument of integral must be identically 0.
→
−
� · (� × A ) = 0
B
−
→
A = Axˆix + Ayˆiy + Azˆiz
��
�
�
�
�
� �
∂Az
∂Ay
∂Ax
∂Az ˆ
∂Ay
∂Ax
→
−
−
� · (� × A ) = � ·
−
îx +
−
iy +
îz
∂x
∂y
∂y
∂z
∂z
∂x
�
�
�
�
�
�
∂ ∂Az
∂Ay
∂ ∂Ax
∂Az
∂ ∂Ay
∂Ax
−
−
−
=
+
+
∂x ∂y
∂z
∂y
∂z
∂x
∂z
∂x
∂y
∂ 2 Az
∂ 2 Ay
∂ 2 Ax
∂ 2 Az
∂ 2 Ay
∂ 2 Ax
−
+
−
+
−
∂x∂y
∂y∂z
∂y∂x ∂z∂x
∂z∂y
∂x∂z
= 0 because of interchangeability of partial derivatives
=
In cylindrical coordinates
Ā = Ar īr + Aφ īφ + Az īz
�
�
�
�
�
�
1 ∂Az
∂Aφ
∂Ar
∂Az
1 ∂(rAφ ) ∂Ar
−
−
−
� × Ā = ¯ir
+ ¯iφ
+ ¯iz
r ∂φ
∂z
∂z
∂r
r
∂r
∂φ
�
�
�
�
�
�
¯ = 1 ∂ ∂Az − r ∂Aφ + 1 ∂ ∂Ar − ∂Az + ∂ 1 ∂(rAφ ) − 1 ∂Ar
� · (� × A)
r ∂r ∂φ
∂z
r ∂φ ∂z
∂r
∂z r ∂r
r ∂φ
1 ∂ 2 Az
r ∂ 2 Aφ
1 ∂Aφ
1 ∂ 2 Ar
1 ∂ 2 Az
∂ 2 Aφ
1 ∂Aφ
1 ∂ 2 Ar
−
−
−
+
−
+
+
r ∂r∂φ r ∂r∂z
r ∂φ∂z
∂r∂z
r ∂z
r ∂φ∂z
r ∂z
r ∂r∂φ
= 0
=
Problem 2.4
(Zahn, Problem 23, Chapter 1)
A
Cartesian Cylindrical Spherical
hx = 1
hr = 1
hr = 1
hφ = r
hθ = r
hy = 1
hz = 1
hφ = r sin θ
hz = 1
8
Problem Set 2
6.641, Spring 2009
B
df =
∂f
∂f
∂f
du +
dv +
dw
∂u
∂v
∂w
= �f · d�
= �f · [hu duīu + hv dv īv + hw dwīw ]
1 ∂f
1 ∂f
1 ∂f
; (�f )v =
; (�f )w =
hu ∂u
hv ∂v
hw ∂w
1 ∂f
1 ∂f
1 ∂f
�f =
īu +
īv +
īw
hu ∂u
hv ∂v
hw ∂w
(�f )u =
c)
dSu = hv hw dvdw;
dSv = hu hw dudw;
dSw = hu hv dudv
dV = hu hv hw dudvdw
D
Divergence
�
�
Φ=
A¯ · dS =
S
1,u
�
+
2,v+Δv
3,w+Δw
�
Au hv hw dvdw
1� ,u−Δu
�
Av hu hw dudw −
�
+
=
Au hv hw dvdw −
Av hu hw dudw
2� ,v
Aw hu hv dudv −
�
Aw hu hv dudv
3� ,w
�
�
Au hv hw |u − Au hv hw |u−Δu
Av hu hw |v+Δv − Av hu hw |v
Aw hu hv |w+Δw − Aw hu hv |w
+
+
ΔuΔvΔw
Δu
Δv
Δw
�
�
¯ · dS
A
A¯ · dS
S
S
� · Ā =
lim
=
Δu→0,Δv→0,Δw→0
ΔV
hu hv hw ΔuΔvΔw
�
�
1
∂(hv hw Au ) ∂(hu hw Av ) ∂(hu hv Aw )
=
+
+
hu hv hw
∂u
∂v
∂w
¯ u (Image by MIT OpenCourseWare.)
Figure 7: Surface for determining (� × A)
Curl
�
¯u=
(� × A)
Ā· d�
Δv→0,Δw→0 hv hw ΔvΔw
lim
L
9
Problem Set 2
�
L
6.641, Spring 2009
A¯ · d� = [Av hv Δv|w − Av hv Δv|w+Δw ] + [Aw hw Δw|v+Δv − Aw hw Δw|v ]
(� × Ā)u =
=
1
hv hw
�
1
Δv→0,Δw→0 hv hw
�
lim
∂(hw Aw ) ∂(hv Av )
−
∂v
∂w
Av hv |w − Av hv |w+Δw
Aw hw |v+Δv − Aw hw |v
+
Δw
Δv
�
�
Similarly
�
∂(hu Au ) ∂(hw Aw )
−
∂w
∂u
�
�
1
∂(hv Av ) ∂(hu Au )
¯
−
(� × A)w =
hu hv
∂u
∂v
¯v=
(� × A)
1
hu hw
�
E
�2 f = � · (�f ) =
1
hu hv hw
�
∂
∂u
�
hv hw ∂f
hu ∂u
�
+
∂
∂v
10
�
hu hw ∂f
hv ∂v
�
+
∂
∂w
�
hu hv ∂f
hw ∂w
��
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