Zonal spherical harmonics

In the mathematical study of rotational symmetry, the zonal spherical harmonics are special spherical harmonics that are invariant under the rotation through a particular fixed axis. The zonal spherical functions are a broad extension of the notion of zonal spherical harmonics to allow for a more general symmetry group.

On the two-dimensional sphere, the unique zonal spherical harmonic of degree ℓ invariant under rotations fixing the north pole is represented in spherical coordinates by $$Z^{(\ell )}(\theta ,\varphi )=\frac{2\ell +1}{4\pi }{P}_{\ell }(\cos \theta )$$ where Template:Math is the normalized Legendre polynomial of degree Template:Mvar, $P_{\ell }(1)=1$. The generic zonal spherical harmonic of degree ℓ is denoted by $Z_{𝐱}^{(\ell )}(𝐲)$, where x is a point on the sphere representing the fixed axis, and y is the variable of the function. This can be obtained by rotation of the basic zonal harmonic $Z^{(\ell )}(\theta ,\varphi ).$

In n-dimensional Euclidean space, zonal spherical harmonics are defined as follows. Let x be a point on the (n−1)-sphere. Define $Z_{𝐱}^{(\ell )}$ to be the dual representation of the linear functional $$P\mapsto P(𝐱)$$ in the finite-dimensional Hilbert space H_ℓ of spherical harmonics of degree ℓ with respect to the Haar measure on the sphere ${𝕊}^{n-1}$ with total mass $A_{n-1}$ (see Unit sphere). In other words, the following reproducing property holds: $$Y(𝐱)=\underset{S^{n-1}}{\int }{Z}_{𝐱}^{(\ell )}(𝐲)Y(𝐲)d\mathrm{\Omega }(y)$$ for all Template:Math where $\mathrm{\Omega }$ is the Haar measure from above.

Relationship with harmonic potentials

The zonal harmonics appear naturally as coefficients of the Poisson kernel for the unit ball in Rⁿ: for x and y unit vectors, $$\frac{1}{{\omega }_{n-1}}\frac{1-r^2}{|𝐱-r𝐲{|}^n}=\sum _{k=0}^{\mathrm{\infty }}{r}^k{Z}_{𝐱}^{(k)}(𝐲),$$ where ${\omega }_{n-1}$ is the surface area of the (n-1)-dimensional sphere. They are also related to the Newton kernel via $$\frac{1}{|𝐱-𝐲{|}^{n-2}}=\sum _{k=0}^{\mathrm{\infty }}{c}_{n,k}\frac{|𝐱{|}^k}{|𝐲{|}^{n+k-2}}{Z}_{𝐱/|𝐱|}^{(k)}(𝐲/|𝐲|)$$ where Template:Math and the constants Template:Math are given by $$c_{n,k}=\frac{1}{{\omega }_{n-1}}\frac{2k+n-2}{(n-2)}.$$

The coefficients of the Taylor series of the Newton kernel (with suitable normalization) are precisely the ultraspherical polynomials. Thus, the zonal spherical harmonics can be expressed as follows. If Template:Math, then $$Z_{𝐱}^{(\ell )}(𝐲)=\frac{n+2\ell -2}{n-2}{C}_{\ell }^{(\alpha )}(𝐱\cdot 𝐲)$$ where Template:Math are the constants above and $C_{\ell }^{(\alpha )}$ is the ultraspherical polynomial of degree ℓ.

Properties

• The zonal spherical harmonics are rotationally invariant, meaning that $$Z_{R𝐱}^{(\ell )}(R𝐲)=Z_{𝐱}^{(\ell )}(𝐲)$$ for every orthogonal transformation R. Conversely, any function Template:Math on Template:Math that is a spherical harmonic in y for each fixed x, and that satisfies this invariance property, is a constant multiple of the degree Template:Mvar zonal harmonic.
• If Y₁, ..., Y_d is an orthonormal basis of Template:Math, then $$Z_{𝐱}^{(\ell )}(𝐲)=\sum _{k=1}^d{Y}_k(𝐱)\overline{Y_k(𝐲)}.$$
• Evaluating at Template:Math gives $$Z_{𝐱}^{(\ell )}(𝐱)={\omega }_{n-1}^{-1}\dim {𝐇}_{\ell }.$$

References

• Template:Citation.