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Mathematical Methods for Physics and Engineering - Matematica.NET

Mathematical Methods for Physics and Engineering - Matematica.NET

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21.3 SEPARATION OF VARIABLES IN POLAR COORDINATESHaving settled the <strong>for</strong>m of Φ(φ), we are left only with the equation satisfied byΘ(θ), which is(sin θ dsin θ dΘ )+ l(l +1)sin 2 θ = m 2 . (21.44)Θ dθ dθA change of independent variable from θ to µ =cosθ will reduce this to a<strong>for</strong>m <strong>for</strong> which solutions are known, <strong>and</strong> of which some study has been made inchapter 16. Puttingµ =cosθ,dµd= − sin θ,dθdθ = −(1 − µ2 ) 1/2 ddµ ,the equation <strong>for</strong> M(µ) ≡ Θ(θ) reads[d(1 − µ 2 ) dM ]]+[l(l +1)− m2dµ dµ1 − µ 2 M =0. (21.45)This equation is the associated Legendre equation, which was mentioned in subsection18.2 in the context of Sturm–Liouville equations.We recall that <strong>for</strong> the case m = 0, (21.45) reduces to Legendre’s equation, whichwas studied at length in chapter 16, <strong>and</strong> has the solutionM(µ) =EP l (µ)+FQ l (µ). (21.46)We have not solved (21.45) explicitly <strong>for</strong> general m, but the solutions were givenin subsection 18.2 <strong>and</strong> are the associated Legendre functions P m l (µ) <strong>and</strong>Qm l (µ),wherePl m (µ) =(1− µ 2 |m|/2 d|m|)dµ P l(µ), (21.47)|m|<strong>and</strong> similarly <strong>for</strong> Q m l (µ). We then haveM(µ) =EP m l (µ)+FQ m l (µ); (21.48)here m must be an integer, 0 ≤|m| ≤l. We note that if we require solutions toLaplace’s equation that are finite when µ =cosθ = ±1 (i.e. on the polar axiswhere θ =0,π), then we must have F = 0 in (21.46) <strong>and</strong> (21.48) since Q m l (µ)diverges at µ = ±1.It will be remembered that one of the important conditions <strong>for</strong> obtainingfinite polynomial solutions of Legendre’s equation is that l is an integer ≥ 0.This condition there<strong>for</strong>e applies also to the solutions (21.46) <strong>and</strong> (21.48) <strong>and</strong> isreflected back into the radial part of the general solution given in (21.42).Now that the solutions of each of the three ordinary differential equationsgoverning R, Θ <strong>and</strong> Φ have been obtained, we may assemble a complete separated-733

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