Gegenbauer polynomials

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Template:Use American English Template:Short description In mathematics, Gegenbauer polynomials or ultraspherical polynomials CScript error: No such module "Su".(x) are orthogonal polynomials on the interval [−1,1] with respect to the weight function (1 − x2)α–1/2. They generalize Legendre polynomials and Chebyshev polynomials, and are special cases of Jacobi polynomials. They are named after Leopold Gegenbauer.

Characterizations

A variety of characterizations of the Gegenbauer polynomials are available.

  • The polynomials can be defined in terms of their generating function Script error: No such module "Footnotes".:
1(1−2xt+t2)α=∑n=0∞Cn(α)(x)tn(0≤|x|<1,|t|≤1,α>0)
C0(α)(x)=1C1(α)(x)=2αx(n+1)Cn+1(α)(x)=2(n+α)xCn(α)(x)−(n+2α−1)Cn−1(α)(x).
  • Gegenbauer polynomials are particular solutions of the Gegenbauer differential equation Script error: No such module "Footnotes".:
(1−x2)y″−(2α+1)xy′+n(n+2α)y=0.
When α = 1/2, the equation reduces to the Legendre equation, and the Gegenbauer polynomials reduce to the Legendre polynomials.
When α = 1, the equation reduces to the Chebyshev differential equation, and the Gegenbauer polynomials reduce to the Chebyshev polynomials of the second kind.[1]
Cn(α)(z)=(2α)nn!2F1(−n,2α+n;α+12;1−z2).
(Abramowitz & Stegun p. 561). Here (2α)n is the rising factorial. Explicitly,
Cn(α)(z)=∑k=0⌊n/2⌋(−1)kΓ(n−k+α)Γ(α)k!(n−2k)!(2z)n−2k.
From this it is also easy to obtain the value at unit argument:
Cn(α)(1)=Γ(2α+n)Γ(2α)n!.
  • They are special cases of the Jacobi polynomials Script error: No such module "Footnotes".:
Cn(α)(x)=(2α)n(α+12)nPn(α−1/2,α−1/2)(x).
in which (θ)n represents the rising factorial of θ.
One therefore also has the Rodrigues formula
Cn(α)(x)=(−1)n2nn!Γ(α+12)Γ(n+2α)Γ(2α)Γ(α+n+12)(1−x2)−α+1/2dndxn[(1−x2)n+α−1/2].
  • An alternative normalization sets Cn(α)(1)=1. Assuming this alternative normalization, the derivatives of Gegenbauer are expressed in terms of Gegenbauer:[2]

dqdxqCq+2j+1(α)(x)=2q(q+2j+1)!(q−1)!Γ(q+2j+2α+1)∑i=0j(2i+α+1)Γ(2i+2α+1)(2i+1)!(j−i)!×Γ(q+j+i+α+1)Γ(j+i+α+2)(q+j−i−1)!C2i+1(α)(x)

Orthogonality and normalization

For a fixed α > -1/2, the polynomials are orthogonal on [−1, 1] with respect to the weighting function (Abramowitz & Stegun p. 774)

w(z)=(1−z2)α−12.

To wit, for n ≠ m,

∫−11Cn(α)(x)Cm(α)(x)(1−x2)α−12dx=0.

They are normalized by

∫−11[Cn(α)(x)]2(1−x2)α−12dx=π21−2αΓ(n+2α)n!(n+α)[Γ(α)]2.

Applications

The Gegenbauer polynomials appear naturally as extensions of Legendre polynomials in the context of potential theory and harmonic analysis. The Newtonian potential in Rn has the expansion, valid with α = (n − 2)/2,

1|𝐱−𝐲|n−2=∑k=0∞|𝐱|k|𝐲|k+n−2Ck(α)(𝐱⋅𝐲|𝐱||𝐲|).

When n = 3, this gives the Legendre polynomial expansion of the gravitational potential. Similar expressions are available for the expansion of the Poisson kernel in a ball Script error: No such module "Footnotes"..

It follows that the quantities Ck((n−2)/2)(𝐱⋅𝐲) are spherical harmonics, when regarded as a function of x only. They are, in fact, exactly the zonal spherical harmonics, up to a normalizing constant.

Gegenbauer polynomials also appear in the theory of positive-definite functions.

The Askey–Gasper inequality reads

∑j=0nCjα(x)(2α+j−1j)≥0(x≥−1,α≥1/4).

In spectral methods for solving differential equations, if a function is expanded in the basis of Chebyshev polynomials and its derivative is represented in a Gegenbauer/ultraspherical basis, then the derivative operator becomes a diagonal matrix, leading to fast banded matrix methods for large problems.[3]

Other properties

Dirichlet–Mehler-type integral representation:[4]Pn(α,α)(cos⁡θ)Pn(α,α)(1)=Cn(α+12)(cos⁡θ)Cn(α+12)(1)=2α+12Γ(α+1)π12Γ(α+12)(sin⁡θ)−2α∫0θcos⁡((n+α+12)ϕ)(cos⁡ϕ−cos⁡θ)−α+12dϕ,Laplace-typePn(α,α)(cos⁡θ)Pn(α,α)(1)=Cn(α+12)(cos⁡θ)Cn(α+12)(1)=Γ(α+1)π12Γ(α+12)∫0π(cos⁡θ+isin⁡θcos⁡ϕ)n(sin⁡ϕ)2αdϕ

See also

References

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  1. ↑ Arfken, Weber, and Harris (2013) "Mathematical Methods for Physicists", 7th edition; ch. 18.4
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  4. ↑ Script error: No such module "citation/CS1".