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Mathematical Methods for Physicists: A concise introduction - Site Map

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SPECIAL FUNCTIONS OF MATHEMATICAL PHYSICS<br />

and then from Eq. (7.96) we obtain<br />

Z 1<br />

0<br />

xJ n …x†J n …x†dx ˆ 0:<br />

…7:98†<br />

p<br />

p<br />

Thus, the two functions x Jn …x† and<br />

x Jn …x† are orthogonal in (0, 1). We can<br />

also say that the two functions J n …x† and J n …x† are orthogonal with respect to<br />

the weighted function x.<br />

Eq. (7.98) is also easily proved if R ˆ 0 and S 6ˆ 0, or R 6ˆ 0 but S ˆ 0. In this<br />

case, and can be any two di€erent roots of J n …x† ˆ0orJn…x† 0 ˆ0.<br />

Spherical Bessel functions<br />

In physics we often meet the following equation<br />

<br />

d<br />

r 2 dR<br />

‡‰k 2 r 2 l…l ‡ 1†ŠR ˆ 0;<br />

dr dr<br />

…l ˆ 0; 1; 2; ...†: …7:99†<br />

In fact, this is the radial equation of the wave and the Helmholtz partial di€erential<br />

equation in the spherical coordinate system (see Problem 7.22). If we let<br />

x ˆ kr and y…x† ˆR…r†, then Eq. (7.99) becomes<br />

x 2 y 00 ‡ 2xy 0 ‡‰x 2 l…l ‡ 1†Šy ˆ 0 …l ˆ 0; 1; 2; ...†; …7:100†<br />

where y 0 ˆ dy=dx. This equation almost matches Bessel's equation (7.71). Let us<br />

make the further substitution<br />

p<br />

y…x† ˆw…x†=<br />

x ;<br />

then we obtain<br />

x 2 w 00 ‡ xw 0 ‡‰x 2 …l ‡ 1 2<br />

†Šw ˆ 0 …l ˆ 0; 1; 2; ...†: …7:101†<br />

The reader should recognize this equation as Bessel's equation of order l ‡ 1 2 .It<br />

follows that the solutions of Eq. (7.100) can be written in the <strong>for</strong>m<br />

y…x† ˆA J l‡1=2…x†<br />

p ‡ B J l1=2…x†<br />

p :<br />

x<br />

x<br />

p<br />

This leads us to de®ne spherical Bessel functions j l …x† ˆCJ l‡E …x†=<br />

<br />

p<br />

x . The factor<br />

C is usually chosen to be =2 <strong>for</strong> a reason to be explained later:<br />

p<br />

j l …x† ˆ<br />

<br />

=2x J l ‡ E…x†:<br />

…7:102†<br />

Similarly, we can de®ne<br />

p<br />

n l …x† ˆ<br />

<br />

=2x N l‡E …x†:<br />

338

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