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Mathematical Methods for Physicists: A concise introduction - Site Map

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SPECIAL FUNCTIONS OF MATHEMATICAL PHYSICS<br />

Figure 7.1.<br />

Legendre polynomials.<br />

If we write D n u as u n and D n v as v n , then<br />

…uv† n ˆ uv n ‡ n C 1 u 1 v n1 ‡‡ n C r u r v nr ‡‡u n v;<br />

where D ˆ d=dx and n C r is the binomial coecient and is equal to n!=‰r!…n r†!Š.<br />

We ®rst notice that Eq. (7.12) holds <strong>for</strong> n ˆ 0, 1. Then, write<br />

so that<br />

z ˆ…x 2 1† n =2 n n!<br />

…x 2 1†Dz ˆ 2nxz:<br />

Di€erentiating Eq. (7.13) …n ‡ 1† times by the Leibnitz rule, we get<br />

…7:13†<br />

Writing y ˆ D n z, we then have:<br />

…1 x 2 †D n‡2 z 2xD n‡1 z ‡ n…n ‡ 1†D n z ˆ 0:<br />

(i) y is a polynomial.<br />

(ii) The coecient of x n in …x 2 1† n is …1† n=2 n C n=2 (n even) or 0 (n odd).<br />

There<strong>for</strong>e the lowest power of x in y…x† is x 0 (n even) or x 1 (n odd). It<br />

follows that<br />

and<br />

y n …0† ˆ0<br />

…n odd†<br />

y n …0† ˆ 1<br />

2 n n! …1†n=2 n C n=2 n! ˆ …1†n=2 n!<br />

2 n ‰…n=2†!Š 2 …n even†:<br />

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