Gegenbauer polynomials: Difference between revisions

From testwiki
Jump to navigation Jump to search
imported>1234qwer1234qwer4
 
(No difference)

Latest revision as of 15:56, 7 September 2024

Template:Use American English Template:Short description In mathematics, Gegenbauer polynomials or ultraspherical polynomials CTemplate: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.

1(12xt+t2)α=n=0Cn(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+2α1)Cn1(α)(x).
  • Gegenbauer polynomials are particular solutions of the Gegenbauer differential equation Template:Harv:
(1x2)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;1z2).
(Abramowitz & Stegun p. 561). Here (2α)n is the rising factorial. Explicitly,
Cn(α)(z)=k=0n/2(1)kΓ(nk+α)Γ(α)k!(n2k)!(2z)n2k.
From this it is also easy to obtain the value at unit argument:
Cn(α)(1)=Γ(2α+n)Γ(2α)n!.
Cn(α)(x)=(2α)n(α+12)nPn(α1/2,α1/2)(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)(1x2)α+1/2dndxn[(1x2)n+α1/2].

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)=(1z2)α12.

To wit, for n ≠ m,

11Cn(α)(x)Cm(α)(x)(1x2)α12dx=0.

They are normalized by

11[Cn(α)(x)]2(1x2)α12dx=π212αΓ(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|𝐱𝐲|n2=k=0|𝐱|k|𝐲|k+n2Ck(α)(𝐱𝐲|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 Template:Harv.

It follows that the quantities Ck((n2)/2)(𝐱𝐲) 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+j1j)0(x1,α1/4).

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.[2]

See also

References

Specific
  1. Arfken, Weber, and Harris (2013) "Mathematical Methods for Physicists", 7th edition; ch. 18.4
  2. Template:Cite journal