Solid harmonics

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Template:Short description In physics and mathematics, the solid harmonics are solutions of the Laplace equation in spherical polar coordinates, assumed to be (smooth) functions ℝ3→ℂ. There are two kinds: the regular solid harmonics Rℓm(𝐫), which are well-defined at the origin and the irregular solid harmonics Iℓm(𝐫), which are singular at the origin. Both sets of functions play an important role in potential theory, and are obtained by rescaling spherical harmonics appropriately:Rℓm(𝐫)≡4π2ℓ+1rℓYℓm(θ,φ) Iℓm(𝐫)≡4π2ℓ+1Yℓm(θ,φ)rℓ+1

Derivation, relation to spherical harmonics

Introducing Template:Mvar, Template:Mvar, and Template:Mvar for the spherical polar coordinates of the 3-vector Template:Math, and assuming that Φ is a (smooth) function ℝ3→ℂ, we can write the Laplace equation in the following form ∇2Φ(𝐫)=(1r∂2∂r2r−L̂2r2)Φ(𝐫)=0,𝐫≠𝟎, where Template:Math is the square of the Template:Em angular momentum operator, 𝐋̂=−i(𝐫×𝜵).

It is known that spherical harmonics Template:Math are eigenfunctions of Template:Math: L̂2Yℓm≡[L̂x2+L̂y2+L̂z2]Yℓm=ℓ(ℓ+1)Yℓm.

Substitution of Template:Math into the Laplace equation gives, after dividing out the spherical harmonic function, the following radial equation and its general solution,

1r∂2∂r2rF(r)=ℓ(ℓ+1)r2F(r)⟹F(r)=Arℓ+Br−ℓ−1.

The particular solutions of the total Laplace equation are regular solid harmonics: Rℓm(𝐫)≡4π2ℓ+1rℓYℓm(θ,φ), and irregular solid harmonics: Iℓm(𝐫)≡4π2ℓ+1Yℓm(θ,φ)rℓ+1. The regular solid harmonics correspond to harmonic homogeneous polynomials, i.e. homogeneous polynomials which are solutions to Laplace's equation.

Racah's normalization

Racah's normalization (also known as Schmidt's semi-normalization) is applied to both functions ∫0πsin⁡θdθ∫02πdφRℓm(𝐫)∗Rℓm(𝐫)=4π2ℓ+1r2ℓ (and analogously for the irregular solid harmonic) instead of normalization to unity. This is convenient because in many applications the Racah normalization factor appears unchanged throughout the derivations.

Addition theorems

The translation of the regular solid harmonic gives a finite expansion, Rℓm(𝐫+𝐚)=∑λ=0ℓ(2ℓ2λ)1/2∑μ=−λλRλμ(𝐫)Rℓ−λm−μ(𝐚)⟨λ,μ;ℓ−λ,m−μ|ℓm⟩, where the Clebsch–Gordan coefficient is given by ⟨λ,μ;ℓ−λ,m−μ|ℓm⟩=(ℓ+mλ+μ)1/2(ℓ−mλ−μ)1/2(2ℓ2λ)−1/2.

The similar expansion for irregular solid harmonics gives an infinite series, Iℓm(𝐫+𝐚)=∑λ=0∞(2ℓ+2λ+12λ)1/2∑μ=−λλRλμ(𝐫)Iℓ+λm−μ(𝐚)⟨λ,μ;ℓ+λ,m−μ|ℓm⟩ with |r|≤|a|. The quantity between pointed brackets is again a Clebsch-Gordan coefficient, ⟨λ,μ;ℓ+λ,m−μ|ℓm⟩=(−1)λ+μ(ℓ+λ−m+μλ+μ)1/2(ℓ+λ+m−μλ−μ)1/2(2ℓ+2λ+12λ)−1/2.

The addition theorems were proved in different manners by several authors.[1][2]

Complex form

The regular solid harmonics are homogeneous, polynomial solutions to the Laplace equation ΔR=0. Separating the indeterminate z and writing R=∑apa(x,y)za, the Laplace equation is easily seen to be equivalent to the recursion formula pa+2=−(∂x2+∂y2)pa(a+2)(a+1) so that any choice of polynomials p0(x,y) of degree ℓ and p1(x,y) of degree ℓ−1 gives a solution to the equation. One particular basis of the space of homogeneous polynomials (in two variables) of degree k is {(x2+y2)m(x±iy)k−2m∣0≤m≤k/2}. Note that it is the (unique up to normalization) basis of eigenvectors of the rotation group SO(2): The rotation ρα of the plane by α∈[0,2π] acts as multiplication by e±i(k−2m)α on the basis vector (x2+y2)m(x+iy)k−2m.

If we combine the degree ℓ basis and the degree ℓ−1 basis with the recursion formula, we obtain a basis of the space of harmonic, homogeneous polynomials (in three variables this time) of degree ℓ consisting of eigenvectors for SO(2) (note that the recursion formula is compatible with the SO(2)-action because the Laplace operator is rotationally invariant). These are the complex solid harmonics: Rℓ±ℓ=(x±iy)ℓz0Rℓ±(ℓ−1)=(x±iy)ℓ−1z1Rℓ±(ℓ−2)=(x2+y2)(x±iy)ℓ−2z0+−(∂x2+∂y2)((x2+y2)(x±iy)ℓ−2)1⋅2z2Rℓ±(ℓ−3)=(x2+y2)(x±iy)ℓ−3z1+−(∂x2+∂y2)((x2+y2)(x±iy)ℓ−3)2⋅3z3Rℓ±(ℓ−4)=(x2+y2)2(x±iy)ℓ−4z0+−(∂x2+∂y2)((x2+y2)2(x±iy)ℓ−4)1⋅2z2+(∂x2+∂y2)2((x2+y2)2(x±iy)ℓ−4)1⋅2⋅3⋅4z4Rℓ±(ℓ−5)=(x2+y2)2(x±iy)ℓ−5z1+−(∂x2+∂y2)((x2+y2)2(x±iy)ℓ−5)2⋅3z3+(∂x2+∂y2)2((x2+y2)2(x±iy)ℓ−5)2⋅3⋅4⋅5z5⋮ and in general Rℓ±m={∑k(∂x2+∂y2)k((x2+y2)(ℓ−m)/2(x±iy)m)(−1)kz2k(2k)!ℓ−m is even∑k(∂x2+∂y2)k((x2+y2)(ℓ−1−m)/2(x±iy)m)(−1)kz2k+1(2k+1)!ℓ−m is odd for 0≤m≤ℓ.

Plugging in spherical coordinates x=rcos⁡(θ)sin⁡(φ), y=rsin⁡(θ)sin⁡(φ), z=rcos⁡(φ) and using x2+y2=r2sin⁡(φ)2=r2(1−cos⁡(φ)2) one finds the usual relationship to spherical harmonics Rℓm=rℓeimϕPℓm(cos⁡(ϑ)) with a polynomial Pℓm, which is (up to normalization) the associated Legendre polynomial, and so Rℓm=rℓYℓm(θ,φ) (again, up to the specific choice of normalization).

Real form

Template:Unreferenced section By a simple linear combination of solid harmonics of Template:Math these functions are transformed into real functions, i.e. functions ℝ3→ℝ. The real regular solid harmonics, expressed in Cartesian coordinates, are real-valued homogeneous polynomials of order ℓ in x, y, z. The explicit form of these polynomials is of some importance. They appear, for example, in the form of spherical atomic orbitals and real multipole moments. The explicit Cartesian expression of the real regular harmonics will now be derived.

Linear combination

We write in agreement with the earlier definition Rℓm(r,θ,φ)=(−1)(m+|m|)/2rℓΘℓ|m|(cos⁡θ)eimφ,−ℓ≤m≤ℓ, with Θℓm(cos⁡θ)≡[(ℓ−m)!(ℓ+m)!]1/2sinmθdmPℓ(cos⁡θ)dcosmθ,m≥0, where Pℓ(cos⁡θ) is a Legendre polynomial of order Template:Mvar. The Template:Mvar dependent phase is known as the Condon–Shortley phase.

The following expression defines the real regular solid harmonics: (CℓmSℓm)≡2rℓΘℓm(cos⁡mφsin⁡mφ)=12((−1)m1−(−1)mii)(RℓmRℓ−m),m>0. and for Template:Math: Cℓ0≡Rℓ0. Since the transformation is by a unitary matrix the normalization of the real and the complex solid harmonics is the same.

z-dependent part

Upon writing Template:Math the Template:Mvar-th derivative of the Legendre polynomial can be written as the following expansion in Template:Mvar dmPℓ(u)dum=∑k=0⌊(ℓ−m)/2⌋γℓk(m)uℓ−2k−m with γℓk(m)=(−1)k2−ℓ(ℓk)(2ℓ−2kℓ)(ℓ−2k)!(ℓ−2k−m)!. Since Template:Math it follows that this derivative, times an appropriate power of Template:Mvar, is a simple polynomial in Template:Mvar, Πℓm(z)≡rℓ−mdmPℓ(u)dum=∑k=0⌊(ℓ−m)/2⌋γℓk(m)r2kzℓ−2k−m.

(x,y)-dependent part

Consider next, recalling that Template:Math and Template:Math, rmsinmθcos⁡mφ=12[(rsin⁡θeiφ)m+(rsin⁡θe−iφ)m]=12[(x+iy)m+(x−iy)m] Likewise rmsinmθsin⁡mφ=12i[(rsin⁡θeiφ)m−(rsin⁡θe−iφ)m]=12i[(x+iy)m−(x−iy)m]. Further Am(x,y)≡12[(x+iy)m+(x−iy)m]=∑p=0m(mp)xpym−pcos⁡(m−p)π2 and Bm(x,y)≡12i[(x+iy)m−(x−iy)m]=∑p=0m(mp)xpym−psin⁡(m−p)π2.

In total

Cℓm(x,y,z)=[(2−δm0)(ℓ−m)!(ℓ+m)!]1/2Πℓm(z)Am(x,y),m=0,1,…,ℓ Sℓm(x,y,z)=[2(ℓ−m)!(ℓ+m)!]1/2Πℓm(z)Bm(x,y),m=1,2,…,ℓ.

List of lowest functions

We list explicitly the lowest functions up to and including Template:Math. Here Π¯ℓm(z)≡[(2−δm0)(ℓ−m)!(ℓ+m)!]1/2Πℓm(z).

Π¯00=1Π¯31=146(5z2−r2)Π¯44=1835Π¯10=zΠ¯32=1215zΠ¯50=18z(63z4−70z2r2+15r4)Π¯11=1Π¯33=1410Π¯51=1815(21z4−14z2r2+r4)Π¯20=12(3z2−r2)Π¯40=18(35z4−30r2z2+3r4)Π¯52=14105(3z2−r2)zΠ¯21=3zΠ¯41=104z(7z2−3r2)Π¯53=11670(9z2−r2)Π¯22=123Π¯42=145(7z2−r2)Π¯54=3835zΠ¯30=12z(5z2−3r2)Π¯43=1470zΠ¯55=31614

The lowest functions Am(x,y) and Bm(x,y) are:

m Am Bm
0 1 0
1 x y
2 x2−y2 2xy
3 x3−3xy2 3x2y−y3
4 x4−6x2y2+y4 4x3y−4xy3
5 x5−10x3y2+5xy4 5x4y−10x2y3+y5

References

Template:Reflist

  1. ↑ R. J. A. Tough and A. J. Stone, J. Phys. A: Math. Gen. Vol. 10, p. 1261 (1977)
  2. ↑ M. J. Caola, J. Phys. A: Math. Gen. Vol. 11, p. L23 (1978)