Gegenbauer polynomials

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In mathematics, Gegenbauer polynomials or ultraspherical polynomials C(α)
n
(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

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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:[2]
(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.[3]
Cn(α)(z)=(2α)nn!2F1(n,2α+n;α+12;1z2).
[4] 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].
  • An alternative normalization sets Cn(α)(1)=1. Assuming this alternative normalization, the derivatives of Gegenbauer are expressed in terms of Gegenbauer:[5]

dqdxqCq+2j+1(α)(x)=2q(q+2j+1)!(q1)!Γ(q+2j+2α+1)i=0j(2i+α+1)Γ(2i+2α+1)(2i+1)!(ji)!×Γ(q+j+i+α+1)Γ(j+i+α+2)(q+ji1)!C2i+1(α)(x)

Orthogonality and normalization

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For a fixed α > -1/2, the polynomials are orthogonal on [−1, 1] with respect to the weighting function[6]

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

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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.[7]

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.[8]

Other properties

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Dirichlet–Mehler-type integral representation:[9]Pn(α,α)(cosθ)Pn(α,α)(1)=Cn(α+12)(cosθ)Cn(α+12)(1)=2α+12Γ(α+1)π12Γ(α+12)(sinθ)2α0θcos((n+α+12)ϕ)(cosϕcosθ)α+12dϕ,Laplace-type integral representationPn(α,α)(cosθ)Pn(α,α)(1)=Cn(α+12)(cosθ)Cn(α+12)(1)=Γ(α+1)π12Γ(α+12)0π(cosθ+isinθcosϕ)n(sinϕ)2αdϕAddition formula:[10]

Cnλ(cosθ1cosθ2+sinθ1sinθ2cosϕ)=k=0nan,kλ(sinθ1)kCnkλ+k(cosθ1)(sinθ2)kCnkλ+k(cosθ2)Ckλ1/2(cosϕ),an,kλ constants 

Asymptotics

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Given fixed λ(0,1),M{1,2,},δ(0,π/2), uniformly for all θ[δ,πδ], for n,[11][12]Cn(λ)(cosθ)=22λΓ(λ+12)π12Γ(λ+1)(2λ)n(λ+1)n(m=0M1(λ)m(1λ)mm!(n+λ+1)mcosθn,m(2sinθ)m+λ+RM(θ))

where ()m is the Pochhammer symbol, andθn,m=(n+m+λ)θ12(m+λ)πThe remainder RM=O(1nM) has an explicit upper bound:|RM(θ)|(2/π)sin(λπ)Γ(n+2λ)Γ(λ)Γ(M+λ)Γ(Mλ+1)M!Γ(n+M+λ+1)max(|cosθ|1,2sinθ)(2sinθ)M+λwhere Γ is the Gamma function.

Other asymptotic formulas can be obtained as special cases of asymptotic formulas for the more general Jacobi polynomials.

See also

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References

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  • Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).

Specific

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  1. ^ (Stein & Weiss 1971, §IV.2)
  2. ^ a b c Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  3. ^ Arfken, Weber, and Harris (2013) "Mathematical Methods for Physicists", 7th edition; ch. 18.4
  4. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  5. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  6. ^ (Abramowitz & Stegun 1983, p. 774)
  7. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  8. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  9. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  10. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  11. ^ (Szegő 1975, Theorem 8.21.11)
  12. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).