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Mathematical Methods for Physicists: A concise introduction - Site Map

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SPECIAL FUNCTIONS OF MATHEMATICAL PHYSICS<br />

Now multiplying the second equation by sin k and integrating from 0 to , we<br />

obtain<br />

Z (<br />

1 <br />

sin k sin…x sin †d ˆ Jk…x†; if k ˆ 1; 3; 5; ...<br />

:<br />

<br />

0; if k ˆ 0; 2; 4; ...<br />

0<br />

Adding these two together we obtain Bessel's integral representation<br />

J n …x† ˆ1<br />

<br />

Z <br />

0<br />

cos…n x sin †d; n ˆ positive integer: …7:89†<br />

Recurrence <strong>for</strong>mulas <strong>for</strong> J n …x†<br />

Bessel functions of the ®rst kind, J n …x†, are the most useful, because they are<br />

bounded near the origin. And there exist some useful recurrence <strong>for</strong>mulas between<br />

Bessel functions of di€erent orders and their derivatives.<br />

…1† J n‡1 …x† ˆ2n<br />

x J n…x†J n1 …x†:<br />

…7:90†<br />

Proof:<br />

obtain<br />

or<br />

Di€erentiating both sides of the generating function with respect to t, we<br />

This can be rewritten as<br />

or<br />

X 1<br />

<br />

e x…tt1 †=2 x<br />

2 1 ‡ 1 <br />

t 2 ˆ X1<br />

nJ n …x†t n1<br />

nˆ1<br />

<br />

x<br />

2 1 ‡ 1 X 1<br />

t 2 J n …x†t n ˆ X1<br />

nJ n …x†t n1 :<br />

nˆ1<br />

nˆ1<br />

x<br />

J<br />

2 n …x†t n ‡ x 2<br />

nˆ1<br />

X 1<br />

x<br />

J<br />

2 n …x†t n ‡ x 2<br />

nˆ1<br />

X 1<br />

nˆ1<br />

X 1<br />

nˆ1<br />

J n …x†t n2 ˆ X1<br />

J n‡2 …x†t n ˆ X1<br />

nˆ1<br />

nˆ1<br />

Equating coecients of t n on both sides, we obtain<br />

x<br />

2 J n…x†‡ x 2 J n‡2…x† ˆ…n ‡ 1†J n …x†:<br />

Replacing n by n 1, we obtain the required result.<br />

…2† xJ 0<br />

n…x† ˆnJ n …x†xJ n‡1 …x†:<br />

332<br />

nJ n …x†t n1<br />

…n ‡ 1†J n‡1 …x†t n :<br />

…7:91†

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