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Chapter 5Magnetostatics
Lecturer: Lee, Sang Young (Professor at Konkuk Univ., Seoul, Korea)
Download site for lecture notes: http://konkuk.ac.kr/~sylee
Textbook: Introduction to Electrodynamics(3rd edition)by D.J. Griffiths
1. The Lorentz Force Law
5.1(1) Magnetic Fields
Inside materials Spin (S) & orbital angular momentum (L)
B
of electrons
-g J ; J L S
e
2m
J
B
; spin magnetic moment of free electron
g ; g- factor
B
r
IB
2
5.1.2 Magnetic Forces
,
,
[ ( )]
B
E
The forceonachargeQ moving withvelocity v ina magnetic field B;
F Q v B Lorentz forcelaw
In presenceof both Eand B thenet forceon Qis expressed by
F Q E v B
F
;
( ) ( ) 0 ( . 5.3)
B
B
B B
F
Note F does not do work
F dl F vdt Q v B vdt Ex
1. The Lorentz Force Law
5.1.3 Currents and the magnetic force on a segment of current-carrying wire
Unit of currents; 1A 1
1)
~
( )
( )
B
CS
Caseof alinechargetravelling downa wire
linechargedensity
dq dI vdt v
dt dt
dF dl v B
I
(Note. / / )
( )
( )B
dl B v dl
Forceontheinfinitesimal chargedq dl indl
F I dl B I dl B
Therefore,
1. The Lorentz Force Law
2)
:
:
Case for charge flowing over a surface
surfacechargedensity
v velocity of c
( )
~
;
B
harge
Q wv t a
dQI vw Kw thecurrent flowing throughthe width w
dt
K v Surface current density thecurrent per unit width
dF dQv B
( )
( ) ( )B
dav B K B da
F v B da K B da
w
vΔt
1. The Lorentz Force Law
3)
:
Case for charge flowing throughathree diimensional region
volumechargedensity
:
/
;
v velocity of charrge
Q vA t
dQ dt vA JA
Charge per unit time flowing thro
B
S
B
ugh A
Current definition of J ; J ρv
I J da
dF dQv B d v B J Bd F J Bd
A
vΔt
S
J
1. The Lorentz Force Law
4 *
Ω
)Continuity equation
Charge flowing outof per unit time
J da
0
s
s v
d J da ρdτ
dt
dρ dρJ da Jdτ ( )dτ ( case for steady currents)
dt dt
dρJ Continuity equation ~ "Contribution of Maxwell"
dt
1 2Volume
1. The Lorentz Force Law
2. Biot – Savart Law ~ Applicable for magnetostatics
Themagneticfieldof a steadycurrent can beobtained byusing theBiot-Savart law :
Condition for a steadycurrent : 0 0
(cf. A moving point chargedoesnot producea staticfield.)
(1) Biot - Sabar
ρ J (or )
t
t law
(
B'
0 0
2 2
'
'
'
)4 4
: ~ An element of length along the wire
~ the vector from the source of current (r ) to the point r,
. ., r r
μ μId Id rr )
π π
d
i e
r rr r
r
r7
20N : permaeability of vacuum ( 4 10 )
A
4
[ ] (A m) ; 1 Tesla 1N (A m) (SI units)
10 gauss (cgs units)
(Note, [ ] [ ] [ ][ ] [ ] [ ][ ])
B
B N
F Qv B B F Q V F I L
Themagnitudeof themagneticfield
that exertsa forceof 1Non a1m-long wire
1Tesla
(Ex. 5.5)
sin ( , ) sin sin sin(d d d d d x d
r r )
2
2
2
cos
tan seccos
d
d zz z
d
z
y
xI
z
P
r
ld
2. Biot – Savart Law ~ Applicable for magnetostatics
2
2
2 2
0
2
0 0
2 2 2
2
0 0 02
2
2
From cos ,
1 cos
Therefore, from ,4
cos coscos
4 4 cos
cossin
4 4 2
Direction : along the x a
π
π
π
π
θ z
θ
z
μ IdlB
π
μ μ IIdl θ z θB dθ θ
π π θ z
μ I μ I μ Iθdθ θ
π z πz πz
r
r
r
r
r
2
2
0
0
xis (Right hand rule!)
Note: Expression of Bdue to thesurfacecurrent ( )or the volume current clensity (J)
4
4
This willbeusedin deriving theAmpere la
K
μ KB da , K K(r )
π
μ Jor B dτ , J J(r )
π
r
rr
rw from the Biot-Savart law.
2. Biot – Savart Law ~ Applicable for magnetostatics
Homework No.1:
Problems 4, 5, 6, 11, 12.(Due date: Sep. 15, 2009)
3. The divergence and Curl of B
5.3.1 Straight-LineCurrents 0a
00 0
0b
0
at r =2
2 2
at r =2
a
aa
b
b
IB R
R
IB d l B dl R I
R
IB R
R
B d l I
insideof r=Ra
binsideofr=R
dl
aR
a
b
IbR
0Generally, : ~ the totalcurrent enclosed by theintegration path B dl I I dl
0
and
( ) , we get
~ Ampere law (for thecaseof straight-linecurrents)
Note: Ampere law is applicable tosteadycurrents.
From I J da
B d l B da
B J
I
1I
nI
n
iiIldB
10
B
0
:
Does the relation ( ) 0 always hold?
Question
B J
The divergence and Curl of B5.3.2
According to theBiot-Savart law, due to the volume current density isexpressed by,B J
'0 0
2 2
( ')( ) '
4 4
J J rB r d d
r rr r
'r
'd
r
( ')r r r ( ') ( ') ( ')yx x y y z zx z r
'
' ' ', cf .y yx z x z
x y z x y z
BofdivergencetheTakei )0
2
0
2 2
( ( ') ) '4
{ ( ) ( )} '4
B J r d
J J d
r
r r
r
r r
2
'( '), ( ') 0. : ( ') 0.
( ) 0 ( . ( ) )
Since J J r J r Note J r
cf fA f A A f
rr (Problem 1.62)
0 B
)()()( BAABBA
BofcurltheTakeii)
0
2
0
2 2 2 2
0
2 2
( ) '4
{( ) ( ) ( ) ( )} '4
{ ( ) ( ) } '4
B J d
J J J J d
J J d
r
r r r r
r r
r
r r r r
r r
( )
( ) ( )
( ) ( )
C D
D C C D
C D D C
2
3
2
' 3 '00
. ( ) ' 0 1
4 ( ) 2 ( , .1.100)
( )4 ( ) ' ( )4
Note J d
See Eq
B J r r r d J r
r
r
r
r
r
2(1), i.e., ( ) ' 0 Verification of J d
rr
2 2
3
( ) ' ( ') '..................(3)
( ')
J d J d
J d
r r
rr
r r
3 3 3 3
3 3 3
' ( ') '( ') ( ') ( ') ( ')
' ( ') ( ')( ') ' [ ] ( ' )
x x y y z zJ J y J J
x x x x x xJ J J
x z
r r r r
r r r
r
3 3
3 3
( ') 0. Therefore, ' ( ') 0
' ( ') ( ) ' [ ]
( ') ( '), ' [ ] ' '
rJ r
t
x x x xJ J
x x x xJ d J da
For steady currents,
Also
r r
r r
Forsufficientlylarge τ', J can be0at thesurface (If J 0, takelarger τ'untilJ= 0.)
J
5.3.3 Applications of Ampere's Law
0
0
0.
( )
: The total current passing through the s
t
B J
B da B d l J da
J da
Forsteady currents,
urface enclosed by d l
(Ex. 5.7)
r
B
I0
0 0
, 0 from the symmetry
and 0 from the Biot-Savart Law.
, 2 2 2
ˆ ˆ with r z r
z
ITherefore B d l dl rB I rB I B
r
B rB B zB B
B
B
(Ex.5.9)
o
' ' '
ˆ ˆ 1
Rotate the coil by 180 : ( ' . '
ˆ ˆ ' 2
ˆ
r z
r z
r
B rB B zB
J J J B B B
B rB B zB
B rB B
' '
Outside of the coil, 0 0 (
ˆ
Meanwhile, since , ( ) . Therefore, 0
0 Inside the coil, 0 0 ( 0)
in
z
r r r r r r
in
B B bd I
zB
B B B B B B
B B B ad I
0)
( ) ( ) 0
( ) ( )
This is also true for going to infinity(i.e., ) ( ) ( ) 0
( ( ) 0)
B d l B a L B b L
B a B b
b b B a B b
B
0
0 0 0
0 0
0
ˆ Also, inside the coil,
~ number of turns/length
ˆ ; inside
0 ; outside
tot
B zB
B dl B L μ I μ nLI ; n
B μ nIz
B
Homework No.2:Ex. 5.8, Problems 13(a), 13(b), 14, 15, 16(a)-(b), 16(c)(Due date: Sep. 29, 2009)
(1) Vector potential
In Electrostatics, ~Scalar potential
( )
5.4. Magnetic Vector Potential
E V ; V
electric Potential
0
(Or, 0 )
E
E E
0
For the magnetic field , 0 always holds true.
From Ampere law, B μ ,
2 B ( ) ( ) - ~ vector
B B
B A
J
A A A
0
identity
. A cannot be uniquely defined from B, because
there can be many different 's that satisfy
a
μ J
Note
A B A
A A - λ
llows the same in that
.
B
A A - λ A
So, we can choose the kind of 's that satisfy 0.
What if ' does not satisfy ' 0,while 'satisfies '.
Then, use the following procedure
This is called the Coulomb gauge.
A A
A A A B A
2
2
for finding
that satisfies the Coulomb gauge 0.
i) Solve for .
ii) Then, .
0.
A A
A
A A
A A
2
0
0
2
0
Note. If 0, then .
B μ B ( )
( ) - = .
A A J
J A
A A μ J
2
0
0i
Therefore, from [ ] [ ],
( ) 0( )
4 .
x y z x y z
ii
A yA A J yJ J
If J rJ rA d
at rr r
x z x z
0
'0
0
( )
4
( ),
4
' , : ' ~ direction of the current I
4
(
J rA d
r r
K ror da
r r
Idlor dl
r r
2
0 0
0
if 01cf. . )
at4
1 ( )
4
(Here, the condition of ( ) = 0 sh
Poisson s eqn V V dr
rd
r r
V
r
0 0
ould be satisfied. See p.87, 88)
. * Lorenz gauge : V
cf At
'r
'd
r
( ')r r r
0
(Ex. 5.12)
Find the vector potential of an infinite solenoid
with n turns per unit lenght, radius R, and current I.
i)
A
B d a Φ ( A ) d a A d
cf B d ( B ) d a μ J
0
0 0
ii)
(ii) (i) (ii) (i)
The direction of is the same as the current direction.
d a μ I
B A , μ I Φ (or μ J B )
* A
0
2
0
0
2
0
2
0
i) For ,
Therefore, 2
ˆ 2
(Note: The direction of
ii) For ,
2
ˆ
2
(Note: T
is the same as that of the current .)
r R B μ nI
A d B d a μ nI (πr ) πr A
μ nIA r
A
r R
A d μ nI (πR ) πr A
μ nI RA
r
he direction of is the same as that of the current.)A
I
R
I
2 12 1
2 1
- Boundary condition for the normal components
(i) 0
( )
( )
(h 0 is usen n
B
B d
B d s B S B S
contributions from the side wall
SB SB
2 1
d.)
0
(This condition always holds true.)n nB B
(2)Magnetostatic Boundary Conditions
.
0
0
1 2
Boundary condition for the transverse components
ii)
( )
( )
ˆ ˆ ( ) ( )
B J
B da J da
B da B d
B Rx B Rx
1 2 0
1 21 2
0( )
0 ; ( )
Here, as h 0, 0 and ( ) 0
if there is no surface current density .
x x
t tx x
K
B h
h B da B R B R J da
J da B da
B BB B
I
1 2 0
20 0 0
2
01 2
(Correct Eq. 5.73 in the t
ˆ If surface current density 0 ( . .,if ( ) ( ) ),
( ) ( )
ˆ ˆ ( ) ( )
ˆ ˆ ( )
x x
R
R
x x
K i e J K y K y z
B da B B R J da
K y z z dxdy KR
z KzB B
2 2 01 1
2 2 21 1 1
21 2 1 2 1
2 1 0 2 1
ext !!!)
ˆ ˆ ( ) ( )
ˆ ˆ ˆ ˆ ˆ ˆ ( ( )) ( ( )) ( )( )
ˆ ˆ ˆ ˆ ˆ( ) ( ) ( )( )
ˆ( )
n n t t
y n KB B B B
n n n n n nB B B B B B
n n n t n nB B B B B B
B B n K B B
0
1 2
ˆ
ˆ ˆ Here, and 0 are used along with .n n n t
K n
n t n tB B B B B
I
1 2 1 2
1 2
iii) 0 ( ) -(a)
iv) From ,
( )
A
Here, 0 as 0.
Therefor
Boundary conditions (continued)
n n
B
B
x x
A or
A B
A da B da
d
h
R RA A
A A A A
1 2 21
1 2
, )1 2
e, which means that ---(b)
From (a) and (b), we get the condition of
at the boundany.
A( Ax x n nR R orA A A A
A A
Homework No.3:Problems 20, 22, 25(a), 25(b), 26, 31(a)(Due date: Oct. 6, 2009)
I
2 1
2 2 22 2
1 1 11 1
2 1
0 0 0
0
Boundary conditions (continued)
v) n y x
( )
( )
x -
No
z y z
z y z
K K z K
x xA A AB Ay y y
x xA A AB Ay y y
A A K Kn n
B B
2 1
1t 2t
te. Boundary conditions in electrostatics.
; ~surface free charge densityD D
0 E E
n n f fPD
E
I
00 3
* A useful tip related with the Coulomb gauge
From the Bio-savart law,
( ) ( )Jwe get 0 and .4
If the Coulomb gauge, 0, is used, 0 and
r r rB B J dB
A A A
r r
3
.
( ) ( )1 BTherefore, can be written as . 4
B
r r rA A d
r r
(3) Multipole expansion of the vector potential
3 0 00
0
0
01
( ) ' '' . (Similar to Eq. 3.94 on p. 154)d
4 4 4
Therefore, assuming that ', due to the current loop can be written
'
4
4
'{n
n
n
J J S d r d rA r I
r r A
d rI
A
I r
r
r rr
r
n(cos )
n
'} (1)
nP dr A
c
r
r r
I
0
r r r
dr d
0
1
0 n
0 1 2
0 0
0
0
0
2
'
4
'{ (cos )} (1)
4
( ) ~ Legendre polynomial (See e.g., Table 3.1)
1( ) 1, ( ) , ( ) (3 1) etc.
2
In Eq. (1), = 04 4
'
''
n
n n
n
n
n
d rA
r
P x
x x x x xP P P
I IddA
r r
I
Idr A
rr
Pr
r
0 0
1 11 2 2
0
1
( 0), and
' 1 = (cos ) ' (cos ) .
4 4
Note. Monopole term (~ 1/r) does not exist, and the first non-trivial term is the dipole term.
: Dipole term ~ 1/
'
' '
:
d
I Ird r dA P P
r r
A
A
r
r r
2 3
2 r Quadrupole term ~ 1/r , : , etc.A
Multipole expansion of the vector potential (continued)
1
0 012 21
0 02 2
Re-expression of the dipole term :
Since cos = ',
' (cos ) ' 'cos '4 4
'( ' ) ' ( ' ) '. (2)4 4
A
r r
I Ir dr r drA
r rI I
r r r dr r r drr r
P
Calculation of :
Since a (b c) b(a c) - c(a b),
( ' ') '( ') '( ')
( ' ) ' { '( ')} { ( ' ')}
r r dr r r dr dr r r
r r dr r r dr r r dr
(3)
Multipole expansion of the vector potential (continued)
1Re-expression of the dipole term (continued)
( ' ) ' { '( ')} { ( ' ')} (3)
Calculation of :
From [( ' ) '] ( ' )
A
r r dr r r dr r r dr
d r r r d r r
' ( ' ) '
( ' ) ' d[( ' ) '] - ' ( ' )
( ' ) ' d[( ' ) '] - ' ( ' )
( 0)
- { '
r r r dr
r r dr r r r r d r r
r r dr r r r r d r r
r
,
( ' ' ') - '( ')
Therefore, '( ') ( ' ) ' ---(4)
dr r r dr r r dr
r r dr r r dr
0
1 2( ' ) '. (2)
( ' ) ' { '( ')} { ( ' ')} (3)
'( ') ( ' ) ' =-
4 r r d r
r r d r r r d r r r d r
r r d r r r d r
IA
r
0
1 2
---(4)
From (3) and (4), ( ' ) ' { ( ' ')
1( ' ) ' { ( ' ')} (5)
2
1Therefore,
2
( ' ')4
r r d r r r d r
r r d r r r d r
r r d rI
Ar
0 01 2 2
( ' ')1
If we use an expression of ,2
( ) ( )(6) due to the magnetic dipole moment
4 4
Note. i) is called the magnetic dipole moment.
r d r dI I a m
r m m rmA A
r r
m
' '
' '
1 Significance of ; ( ) , and
2
1 ( ) ( ~ vector area of the current loop).
2
ii) is independent of the choice of origin.
Proof
r d r
r d r
m d a
a a
m I a
m
'
' '
'
: If we take O' as the origin, then
" , and " '
" " ( ) ' ' '
'+0
r
r r
r
r c dr dr
r dr c dr dr c dr
dr
' = ' ; Q.E.Dr dr
c
r
r r
I
0
r r r
dr d
0
20
2 23
1 2 2 1 1
iii) Since the quadrupole term is expressed by
' (cos ) ',4
' for ' due to ~ . ~
The magnetic field of a magnetic dipole :
If we
Ir d rpA
r
rr rA A A A
r
B m
A A
0 0
2
0
2
3
place at the origin (note that is independent of the origin),
( )
4
sin
4
(2cos sin )
4
m m
m r
r
mA
r
mB A r
r
z
x
y
rm
y
z z
y
(a) Field of a pure dipole (b)Field of a physical dipole
Field of a dipole