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Mathematical Methods for Physics and Engineering - Matematica.NET

Mathematical Methods for Physics and Engineering - Matematica.NET

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SPECIAL FUNCTIONSorthonormal set, i.e.∫ 1 ∫ 2π−10[Yml (θ, φ) ] ∗Ym ′l (θ, φ) dφ d(cos θ) =δ ′ ll ′δ mm ′. (18.46)In addition, the spherical harmonics <strong>for</strong>m a complete set in that any reasonablefunction (i.e. one that is likely to be met in a physical situation) of θ <strong>and</strong> φ canbe exp<strong>and</strong>ed as a sum of such functions,f(θ, φ) =∞∑l∑l=0 m=−la lm Yl m (θ, φ), (18.47)the constants a lm being given by∫ 1 ∫ 2π[a lm = Yml (θ, φ) ] ∗f(θ, φ) dφ d(cos θ). (18.48)−10This is in exact analogy with a Fourier series <strong>and</strong> is a particular example of thegeneral property of Sturm–Liouville solutions.Aside from the orthonormality condition (18.46), the most important relationshipobeyed by the Ylm is the spherical harmonic addition theorem. This readsP l (cos γ) =4π2l +1l∑m=−lY ml (θ, φ)[Y ml (θ ′ ,φ ′ )] ∗ , (18.49)where (θ, φ)<strong>and</strong>(θ ′ ,φ ′ ) denote two different directions in our spherical polar coordinatesystem that are separated by an angle γ. In general, spherical trigonometry(or vector methods) shows that these angles obey the identitycos γ =cosθ cos θ ′ +sinθ sin θ ′ cos(φ − φ ′ ). (18.50)◮Prove the spherical harmonic addition theorem (18.49).For the sake of brevity, it will be useful to denote the directions (θ, φ) <strong>and</strong>(θ ′ ,φ ′ )byΩ<strong>and</strong>Ω ′ , respectively. We will also denote the element of solid angle on the sphere bydΩ =dφ d(cos θ). We begin by deriving the <strong>for</strong>m of the closure relationship obeyed by thespherical harmonics. Using (18.47) <strong>and</strong> (18.48), <strong>and</strong> reversing the order of the summation<strong>and</strong> integration, we may write∫f(Ω) = dΩ ′ f(Ω ′ ) ∑ Ylm∗ (Ω ′ )Yl m (Ω),4πlmwhere ∑ lmis a convenient shorth<strong>and</strong> <strong>for</strong> the double summation in (18.47). Thus we maywrite the closure relationship <strong>for</strong> the spherical harmonics as∑lmY ml (Ω)Y m∗l (Ω ′ )=δ(Ω − Ω ′ ), (18.51)where δ(Ω − Ω ′ ) is a Dirac delta function with the properties that δ(Ω − Ω ′ )=0ifΩ≠Ω ′<strong>and</strong> ∫ 4π δ(Ω) dΩ =1. 594

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