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Jackson solutions - jackson 5 3 homework solution, Provas de Física

Solução do jackson

Tipologia: Provas

2016

Compartilhado em 28/04/2016

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Jackson 5.3 Homework Problem Solution
Dr. Christopher S. Baird
University of Massachusetts Lowell
PROBLEM:
A right-circular solenoid of finite length L and radius a has N turns per unit length and carries a current
I. Show that the magnetic induction on the cylinder axis in the limit NL → ∞ is
Bz=0N I
2cos1cos2
where the angles are defined in the figure.
SOLUTION:
Let us first find the on-axis magnetic induction produced by one circular loop of current. Place the
observation point such that the line from the observation point to the loop makes an angle θi with the
solenoid's axis and is a distance ri away. In this set-up, then the observation point can be considered at
the origin of a spherical coordinate system.
If the current is flowing into the paper at the bottom and out of the paper at the top, the current density
in spherical coordinates becomes:
J=I rri
r − i
Plug this into the Biot-Savart Law:
Bx= 0
4Jx'×xx'
xx'
3d3x'
Bx= 0
4
0
2
0
0
[
I r'ri
r'  '−i
'
]
×xx'
r2r'22r r 'cos cos 'sin sin ' cos − '3/2r'2sin 'd r 'd'd'
θ2
θ1z
θiz
ri
pf3
pf4

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Jackson 5.3 Homework Problem Solution

Dr. Christopher S. Baird

University of Massachusetts Lowell

PROBLEM:

A right-circular solenoid of finite length L and radius a has N turns per unit length and carries a current

I. Show that the magnetic induction on the cylinder axis in the limit NL → ∞ is

B

z

0

N I

cos  1

cos  2

where the angles are defined in the figure.

SOLUTION:

Let us first find the on-axis magnetic induction produced by one circular loop of current. Place the

observation point such that the line from the observation point to the loop makes an angle θi with the

solenoid's axis and is a distance r i

away. In this set-up, then the observation point can be considered at

the origin of a spherical coordinate system.

If the current is flowing into the paper at the bottom and out of the paper at the top, the current density

in spherical coordinates becomes:

J = I

  rr i

r

i

Plug this into the Biot-Savart Law:

Bx =

0

Jx '× xx '

xx '∣

3

d

3

x '

Bx =

0

2 

∞ (^) [

I

  r '− r i

r '

i

]

× xx '

r

2

r '

2

− 2 r r ' cos cos 'sin  sin ' cos − '

3 / 2

r '

2

sin ' d r ' d ' d '

θ 2

θ 1

z

θ i

z

r i

Spherical unit vectors are not constant or fixed, but change as we integrate. The safest thing to do is

express the vector directions in Cartesian coordinates, using relations such as

ϕ '=−sin ϕ '

i +cosϕ '

j

and

xx '= r sin  cos − r ' sin  ' cos  '

i  r sin sin − r ' sin ' sin '

j  r cos − r ' cos  '

k

Bx =

0

0

2 

0

0

r '

2

sin  ' d r ' d ' d '

[

I

 r '− r i

r '

i

−sin  '

i cos '

j

]

×

 r sin cos − r ' sin ' cos '

i  r sin  sin − r ' sin ' sin '

j  r cos − r ' cos '

k

r

2

r '

2

− 2 r r 'cos cos  'sin sin ' cos − '

3 / 2

Now evaluate the Dirac delta's

Bx =

I 

0

0

2 

r i

sin  i

d '[ −sin '

i cos  '

j ]×

 r sin cos − r i

sin  i

cos '

i  r sin sin − r i

sin  i

sin '

j  r cos − r i

cos  i

k

r

2

r i

2

− 2 r r i

cos cos  i

sin sin  i

cos−'

3 / 2

Evaluate the cross product

Bx =

I 

0

0

2 

r i

sin  i

d '

 r cos − r i

cos  i

cos  '

i sin  '

j  r i

sin  i

r sin  cos−'

k

r

2

r i

2

− 2 r r i

cos  cos  i

sin sin  i

cos − '

3 / 2

This expression is general for any point in space in spherical coordinates. All that is left to do is

perform the integral over the azimuthal angle and we would have the final solution to the total

magnetic field (magnetic induction) B as any point in space created by a loop of current. The integral is

messy however, and we don't need to do it for this particular problem. For an observation point at the

origin r = 0 , this reduces to:

Bx =

I 

0

sin  i

r i

[

−cos  i

i (^) ∫

0

2 

cos ' d '

j (^) ∫

0

2 

sin  ' d 'sin  i

k (^) ∫

0

2 

d '

]

We can now perform the integrals and find

Bx =

0

I

sin

2

i

r i

k

If we recognize that the ring has some fixed radius no matter where we place the ring, we can simplify

this using r^ i

sin  i

= a

Bx =

k

0

I a

2

r i

3

or

Bx =

k

0

N I

[

cos  2

cos  1 ]

We can check our answer by taking limiting cases. If the solenoid's length becomes infinite, both angles

become zero and we get our usual answer for a long solenoid B ^ x =^

kN I