Solid harmonics

From The Right Wiki
(Redirected from Solid spherical harmonics)
Jump to navigationJump to search

In physics and mathematics, the solid harmonics are solutions of the Laplace equation in spherical polar coordinates, assumed to be (smooth) functions 3. There are two kinds: the regular solid harmonics Rm(r), which are well-defined at the origin and the irregular solid harmonics Im(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: Rm(r)4π2+1rYm(θ,φ) Im(r)4π2+1Ym(θ,φ)r+1

Derivation, relation to spherical harmonics

Introducing r, θ, and φ for the spherical polar coordinates of the 3-vector r, and assuming that Φ is a (smooth) function 3, we can write the Laplace equation in the following form 2Φ(r)=(1r2r2rl^2r2)Φ(r)=0,r0, where l2 is the square of the nondimensional angular momentum operator, l^=i(r×). It is known that spherical harmonics Ym
are eigenfunctions of l2: l^2Ym[l^x2+l^y2+l^z2]Ym=(+1)Ym. Substitution of Φ(r) = F(r) Ym
into the Laplace equation gives, after dividing out the spherical harmonic function, the following radial equation and its general solution, 1r2r2rF(r)=(+1)r2F(r)F(r)=Ar+Br1. The particular solutions of the total Laplace equation are regular solid harmonics: Rm(r)4π2+1rYm(θ,φ), and irregular solid harmonics: Im(r)4π2+1Ym(θ,φ)r+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 0πsinθdθ02πdφRm(r)*Rm(r)=4π2+1r2 (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, Rm(r+a)=λ=0(22λ)1/2μ=λλRλμ(r)Rλmμ(a)λ,μ;λ,mμ|m, where the Clebsch–Gordan coefficient is given by λ,μ;λ,mμ|m=(+mλ+μ)1/2(mλμ)1/2(22λ)1/2. The similar expansion for irregular solid harmonics gives an infinite series, Im(r+a)=λ=0(2+2λ+12λ)1/2μ=λλRλμ(r)I+λmμ(a)λ,μ;+λ,mμ|m with |r||a|. The quantity between pointed brackets is again a Clebsch-Gordan coefficient, λ,μ;+λ,mμ|m=(1)λ+μ(+λm+μλ+μ)1/2(+λ+mμλμ)1/2(2+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 and p1(x,y) of degree 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)k2m0mk/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(k2m)α on the basis vector (x2+y2)m(x+iy)k2m. If we combine the degree basis and the degree 1 basis with the recursion formula, we obtain a basis of the space of harmonic, homogeneous polynomials (in three variables this time) of degree 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: R±=(x±iy)z0R±(1)=(x±iy)1z1R±(2)=(x2+y2)(x±iy)2z0+(x2+y2)((x2+y2)(x±iy)2)12z2R±(3)=(x2+y2)(x±iy)3z1+(x2+y2)((x2+y2)(x±iy)3)23z3R±(4)=(x2+y2)2(x±iy)4z0+(x2+y2)((x2+y2)2(x±iy)4)12z2+(x2+y2)2((x2+y2)2(x±iy)4)1234z4R±(5)=(x2+y2)2(x±iy)5z1+(x2+y2)((x2+y2)2(x±iy)5)23z3+(x2+y2)2((x2+y2)2(x±iy)5)2345z5 and in general R±m={k(x2+y2)k((x2+y2)(m)/2(x±iy)m)(1)kz2k(2k)!m is evenk(x2+y2)k((x2+y2)(1m)/2(x±iy)m)(1)kz2k+1(2k+1)!m is odd for 0m. 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(1cos(φ)2) one finds the usual relationship to spherical harmonics Rm=reimϕPm(cos(ϑ)) with a polynomial Pm, which is (up to normalization) the associated Legendre polynomial, and so Rm=rYm(θ,φ) (again, up to the specific choice of normalization).

Real form

By a simple linear combination of solid harmonics of ±m these functions are transformed into real functions, i.e. functions 3. The real regular solid harmonics, expressed in Cartesian coordinates, are real-valued homogeneous polynomials of order 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 Rm(r,θ,φ)=(1)(m+|m|)/2rΘ|m|(cosθ)eimφ,m, with Θm(cosθ)[(m)!(+m)!]1/2sinmθdmP(cosθ)dcosmθ,m0, where P(cosθ) is a Legendre polynomial of order . The m dependent phase is known as the Condon–Shortley phase. The following expression defines the real regular solid harmonics: (CmSm)2rΘm(cosmφsinmφ)=12((1)m1(1)mii)(RmRm),m>0. and for m = 0: C0R0. 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 u = cos θ the m-th derivative of the Legendre polynomial can be written as the following expansion in u dmP(u)dum=k=0(m)/2γk(m)u2km with γk(m)=(1)k2(k)(22k)(2k)!(2km)!. Since z = r cos θ it follows that this derivative, times an appropriate power of r, is a simple polynomial in z, Πm(z)rmdmP(u)dum=k=0(m)/2γk(m)r2kz2km.

(x,y)-dependent part

Consider next, recalling that x = r sin θ cos φ and y = r sin θ sin φ, rmsinmθcosmφ=12[(rsinθeiφ)m+(rsinθeiφ)m]=12[(x+iy)m+(xiy)m] Likewise rmsinmθsinmφ=12i[(rsinθeiφ)m(rsinθeiφ)m]=12i[(x+iy)m(xiy)m]. Further Am(x,y)12[(x+iy)m+(xiy)m]=p=0m(mp)xpympcos(mp)π2 and Bm(x,y)12i[(x+iy)m(xiy)m]=p=0m(mp)xpympsin(mp)π2.

In total

Cm(x,y,z)=[(2δm0)(m)!(+m)!]1/2Πm(z)Am(x,y),m=0,1,, Sm(x,y,z)=[2(m)!(+m)!]1/2Πm(z)Bm(x,y),m=1,2,,.

List of lowest functions

We list explicitly the lowest functions up to and including = 5. Here Π¯m(z)[(2δm0)(m)!(+m)!]1/2Πm(z). Π¯00=1Π¯31=146(5z2r2)Π¯44=1835Π¯10=zΠ¯32=1215zΠ¯50=18z(63z470z2r2+15r4)Π¯11=1Π¯33=1410Π¯51=1815(21z414z2r2+r4)Π¯20=12(3z2r2)Π¯40=18(35z430r2z2+3r4)Π¯52=14105(3z2r2)zΠ¯21=3zΠ¯41=104z(7z23r2)Π¯53=11670(9z2r2)Π¯22=123Π¯42=145(7z2r2)Π¯54=3835zΠ¯30=12z(5z23r2)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 x2y2 2xy
3 x33xy2 3x2yy3
4 x46x2y2+y4 4x3y4xy3
5 x510x3y2+5xy4 5x4y10x2y3+y5

References

  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)
  • Steinborn, E. O.; Ruedenberg, K. (1973). "Rotation and Translation of Regular and Irregular Solid Spherical Harmonics". In Lowdin, Per-Olov (ed.). Advances in quantum chemistry. Vol. 7. Academic Press. pp. 1–82. ISBN 9780080582320.
  • Thompson, William J. (2004). Angular momentum: an illustrated guide to rotational symmetries for physical systems. Weinheim: Wiley-VCH. pp. 143–148. ISBN 9783527617838.