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1

Chapter 2 Electrostatics

2.1 Poisson’s Eq. and Green’s Theorem

(i) Maxwell eqs (cgs)

.

.

= . = ~ ゙

= . ゙

0

4

t c

B E

E

ホマ v

v

v

= .゙

v

E V

.

Poisson’s eq. ゙ = . 2 4 V ホマ

(2.1)

Since

.

= . . 2 1 4 v v

v v

r r

r r

'

( ') ホツ ,

it is easy to verify that

V r r

r r

d r ( ) ( ' )

| ' |

' v

v

v v

v =

.

3

(2.2)

satisfies Poisson’s eq.

2

If the electrostatics problems involved charge with no

boundary surfaces, the above general solution would be the

most convenient and straightforward solution to any problem.

Actually, of course, many involve finite regions of space, with

or without charge insides, and with prescribed boundary

conditions on the bounding surfaces. These BCs may be

simulated by an appropriate distribution of charges outside the

region of interest (perhaps at infinity), but the above solution

becomes inconvenient, except in simple cases(e.g., method of

images).

(ii) To handle the BC, it is necessary to develop some new

mathematical tools, theorems due to George Green.

The divergence theorem for any vector field

vF

゙ . = .

v v v v Fd r F nd

V

3

Let

vF

= ゙ モ ユ, where and are arbitrary scale fields.

Now, ゙ . = ゙ . ゙ = ゙ + ゙ .゙

vF

( ) モ ユ モ ユ モ ユ 2

and モ ユ モ

ンユ

゙ . = vn

n

n

is the normal derivative at the surface S.

Green’s first identity

3

( )

V S

d r

n

d ゙ +゙ .゙ = モ ユ モ ユ モ

ンユ

2 3v

If we write down the above eq. again with and

interchanged ( モ ユ . ), and then subtract it from the eq.

゙ .゙ モ ユ terms cancel, and we obtain Greens second identity or

Green’s theorem

. = ゙ . ゙

S V

d

n n

r d

ンモ

ンユ

モ モ ユ ユ モ v 3 2 2 ) (

Poisson’s diff. eq. integral eq. if we choose

| ' |

1 1

r r R v v .

= =

vr -- observation point, vr' -- integration variable. Put

= V , ゙ = . 2 4 V ホマ . From

.

= . . 2 1 4 v v

v v

r r

r r

'

( ') ホツ ,

we have

[ ( ' ) ( ' ) ( ' )] ' [

'

( )

'

] ' . . + = . 4 4 11 3 ホ ツ

ン ン

ン ン

V r r r

R

r d r V

n R R n

V d

V S

v v v v v

If vr vol,

4

V r r

r r

d r

R n

V V

n R

d

vol S

( ) ( ' )

| ' |

' [

' '

( )] ' v

v

v v

v =

.

+ .

ン ン

ン ン

3 1

4

1 1

(2.3)

If . rv vol, L.H.S. is zero)

Two remarks

(1) If S , and

vE

on S falls off faster than R.1, then

0

S

, and the eq. reduces to the familiar result.

(2) for a charge free volume, V anywhere inside vol ( a sol. to

Laplaces’s eq. ゙ = 2 0 V ) is expressed in the above eq. in terms

of potential and its normal derivative only on the surface. This

rather surprising result is not a solution to a boundary value

problem, but only an integral eq., since the specification of both

V and

ン ン V n

(Cauchy BC) is an over specification of the

problem.

2.2 Uniqueness of the Solution with Dirichlet or

Neumann Boundary Conditions

The question arises as to what are BCs appropriate for

Poisson’s (or Laplace’s) eq. in order that a unique and wellbehaved

(i.e., physically reasonable) solution exist inside the

bounded region. Physical experience leads us believe that

5

(1) specification of the potential on a closed S (e.g., a system of

conductors held at different potentials) define a unique potential

problem-Dirichlet BC.

(2) Similarly, specification of the

vE

(normal derivative of

the potential) everywhere on the S (corresponding to surface

charge density) also define a unique problem- -Neumann BC.

We now prove these expectations.

゙ = . 2 4 V ホマ

(2.4)

with either Dirichlet or Neumann.

We suppose, to the contrary, that there exist V1 and V2 ,

let U V V = . 2 1,

then ゙ = 2 0 U inside Vol, U = 0 or

ン ン U n

= 0 on S

From Green’s first identity, with モ ユ = =U

U U U Ud r U U

n

d

S vol

゙ +゙ .゙ =

2 3v

ヒ ゙ = | | U d r

vol

2 3 0 v

6

which implies ゙ = U 0.

Consequently inside vol, U is constant.

U=0 V V 1 2 = (DBC)

V is unique, apart from an unimportant arbitrary additive

const. (NBC)

From R. H. S. of the eq., there is also a unique sol. to a

problem with mixed BC (i.e., DBC over part of S, NBC over

the remaining part).

However, it should be clear that a sol. with both V and

ン ン V n

specified on a closed boundary does not exist, since there

are unique solutions for D & N condition separately and these

will in general not be consistent.

2.3 Formal Solution with Green’s

Function

The sol. of Poisson’s or Laplaces eq. in a finite vol. with

either DBC or NBC can be obtained by means of Green’s

theorem and so--called "Green’s function"

In obtaining result

V r r

r r

d r

R n

V V

n R

d

vol S

( ) ( ' )

| ' |

' [

' '

( )] ' v

v

v v

v =

.

+ .

ン ン

ン ン

3 1

4

1 1

7

--- not a solution -- we chose =

.

1

v v r r'

, it being the potential

of a unit point charge,

.

= . . '

'

( ') 2 1 4 v v

v v

r r

r r ホツ

The function 1

v v r r . '

is only one of a class of functions

depending on the variable vr and rr' , and called Green’s

function G r r ( , ' ) v v , which satisfy ゙ =. . ' ( , ') ( ') 2 4 G r r r r v v v v ホツ

In general, G r r

r r

F r r ( , ' )

'

( , ' ) v v

v v

v v =

.

+ 1

where F satisfies ゙ = ' ( , ') 2 0 F r r v v

In facing the problem of satisfying the prescribed BC on

V or

ン ン V n

, we can find the key by considering the integral eq.

As pointed out, this is not sol. satisfying the correct BC because

both V &

ン ン V n

appear. It is at best an integral relation for V.

With the generalized concept of a GF and its additional freedom

[via F r r ( , ' ) v v , these arise the possibility that we can use Green’s

theorem with = G r r ( , ' ) v v and choose F r r ( , ' ) v v to eliminate

one or the other of the two surface integral.

8

Thus we obtain a result which involves any DBC or NBC.

Of course, if the necessary G r r ( , ' ) v v depended in detail on the

exact form of the BC, the method would have little generality.

As will be seen, this is not required, and G r r ( , ' ) v v satisfies

rather simple BC on S.

With Green’s Theorem , モ ユ = = V Grr , (,') v v ,

. = ゙ . ゙

S V

d

n n

r d

ンモ

ンユ

モ モ ユ ユ モ ] [ ) ( 3 2 2 v

゙ = . 2 4 モ ホマ, ゙ = . . 2 4 ユ ホツ( ') v v r r

V r r G r r d r G r r V

n

V G r r

n

d

vol S

( ) ( ') ( , ') ' [ ( , ')

'

( , ')

'

] ' v v v v v v v

v v

= + .

ン ン

3 1

4

(2.5)

The freedom available in the definition of G means that we can

make the surface integral depend only on the chosen type of

BCs.

For DBCs, we demand

G r r D( , ' ) v v = 0 for vr' on S

V r r G r r d r V r

n

G d D

vol

D

S

( ) ( ' ) ( , ' ) ' [ ( ' )

'

' v v v v v v = .

ン ン

3 1

4

(2.6)

9

For Neumann Bcs, we must be careful, the obvious choice of

BC on G r r ( , ' ) v v seems to be

G r r

n

N( , ' )

'

v v

= 0 for vr' on S

But an application of Divergence theorem to

゙ .゙ = ゙ . ' ' ( , ') ' ' ( , ') ' ' G r r d r G r r n d

vol S

v v v v v v 3

.

=

G r r

n

d

S

( , ' )

'

'

v v

. . =. 4 4 3 ホツ ホ ( ') ' v v v r r d r

vol

Consequently, the simplest allowable BC on GN is

G r r

n S

N( , ' )

'

v v

= . 4 for vr' on S

where S is total area of B.S.. Then the sol. is

V r V r G r r d r V

n

G d S N

vol

N

S

( ) ( ') ( , ') ' [

'

' v v vv v =< > + +

3 1

4

(2.7)

10

< > = V

S

V r d S

S

1 ( ' ) ' v --- the average area S.

The customary Neumann problem is the so-called " exterior

problem" in which the volume is bounded by two surfaces, one

closed and finite, the other at infinite,

ィ < > ィ S VS ; 0.


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