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
( θ , ϕ ) =
2 ℓ + 1
( cos θ )
where Pℓ is the normalized Legendre polynomial of degree ℓ,
ℓ
The generic zonal spherical harmonic of degree ℓ is denoted by
, 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
( θ , ϕ ) .
In n-dimensional Euclidean space, zonal spherical harmonics are defined as follows.
to be the dual representation of the linear functional
in the finite-dimensional Hilbert space Hℓ of spherical harmonics of degree ℓ with respect to the Haar measure on the sphere
with total mass
(see Unit sphere).
In other words, the following reproducing property holds:
is the Haar measure from above.
The zonal harmonics appear naturally as coefficients of the Poisson kernel for the unit ball in Rn: for x and y unit vectors,
ω
ω
is the surface area of the (n-1)-dimensional sphere.
They are also related to the Newton kernel via
where x,y ∈ Rn and the constants cn,k are given by
ω
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.
where cn,ℓ are the constants above and
is the ultraspherical polynomial of degree ℓ.