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Mathematical Methods for Physicists: A concise introduction - Site Map

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SOME USEFUL INTEGRAL RELATIONS<br />

considered as the sum of a solenoidal ®eld and an irrotational ®eld. This is made<br />

clear by Helmholtz's theorem, which can be stated as (C. W. Wong: Introduction<br />

to <strong>Mathematical</strong> Physics, Ox<strong>for</strong>d University Press, Ox<strong>for</strong>d 1991; p. 53):<br />

A vector ®eld is uniquely determined by its divergence and curl in<br />

a region of space, and its normal component over the boundary<br />

of the region. In particular, if both divergence and curl are<br />

speci®ed everywhere and if they both disappear at in®nity<br />

suciently rapidly, then the vector ®eld can be written as a<br />

unique sum of an irrotational part and a solenoidal part.<br />

In other words, we may write<br />

V…r† ˆr…r†‡rA…r†;<br />

…1:89†<br />

where r is the irrotational part and rA is the solenoidal part, and (r) and<br />

A…r† are called the scalar and the vector potential, respectively, of V…r). If both A<br />

and can be determined, the theorem is veri®ed. How, then, can we determine A<br />

and ? If the vector ®eld V…r† is such that<br />

rV…r† ˆ; and rV…r† ˆv;<br />

then we have<br />

rV…r† ˆ ˆr…r†‡r…rA†<br />

or<br />

r 2 ˆ;<br />

which is known as Poisson's equation. Next, we have<br />

rV…r† ˆv ˆ r ‰r ‡rA…r†Š<br />

or<br />

r 2 A ˆ v;<br />

or in component, we have<br />

r 2 A i ˆ v i ; i ˆ 1; 2; 3<br />

where these are also Poisson's equations. Thus, both A and can be determined<br />

by solving Poisson's equations.<br />

Some useful integral relations<br />

These relations are closely related to the general integral theorems that we have<br />

proved in preceding sections.<br />

(1) The line integral along a curve C between two points a and b is given by<br />

Z b<br />

a<br />

… r†dl ˆ …b†…a†: …1:90†<br />

45

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