Gegenbauer polynomials explained

In mathematics, Gegenbauer polynomials or ultraspherical polynomials C(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
(1-2xt+t2)\alpha
infty
=\sum
n=0
(\alpha)
C
n

(x)tn    (0\leq|x|<1,|t|\leq1,\alpha>0)

(\alpha)
\begin{align} C
0

(x)&=1

(\alpha)
\\ C
1

(x)&=2\alphax\\ (n+1)

(\alpha)
C
n+1

(x)&=2(n+\alpha)x

(\alpha)
C
n

(x)-

(\alpha)
(n+2\alpha-1)C
n-1

(x). \end{align}

(1-x2)y''-(2\alpha+1)xy'+n(n+2\alpha)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]

(\alpha)
C(z)=
n
(2\alpha)n
n!

2F

;
1\left(-n,2\alpha+n;\alpha+1
2
1-z
2

\right).

(Abramowitz & Stegun p. 561). Here (2α)n is the rising factorial. Explicitly,

(\alpha)
C
n
\lfloorn/2\rfloor
(z)=\sum
k=0
k\Gamma(n-k+\alpha)
\Gamma(\alpha)k!(n-2k)!
(-1)

(2z)n-2k.

From this it is also easy to obtain the value at unit argument:

(\alpha)
C(1)=
n
\Gamma(2\alpha+n)
\Gamma(2\alpha)n!

.

(\alpha)
C
n

(x)=

(2\alpha)n
(\alpha+1)n
2
(\alpha-1/2,\alpha-1/2)
P
n

(x).

in which

(\theta)n

represents the rising factorial of

\theta

.

One therefore also has the Rodrigues formula

(\alpha)
C
n

(x)=

(-1)n
2nn!
\Gamma(\alpha+1)\Gamma(n+2\alpha)
2
\Gamma(2\alpha)\Gamma(\alpha+n+1)
2

(1-x2)-\alpha+1/2

dn
dxn

\left[(1-x2)n+\alpha-1/2\right].

Orthogonality and normalization

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

w(z)=\left(1-z2\right)

\alpha-1
2

.

To wit, for n ≠ m,

1
\int
-1
(\alpha)
C
n
(\alpha)
(x)C
m

(x)(1-x2)

\alpha-1
2

dx=0.

They are normalized by

1
\int
-1
(\alpha)
\left[C
n

(x)\right]2(1-x2)

\alpha-1
2

dx=

\pi21-2\alpha\Gamma(n+2\alpha)
n!(n+\alpha)[\Gamma(\alpha)]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

=

infty
\sum
k=0
|x|k
|y|k+n-2
(\alpha)
C(
k
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 .

It follows that the quantities

((n-2)/2)
C
k(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

n
\alpha(x)
C
j
{2\alpha+j-1\choosej
\sum
j=0
}\ge 0\qquad (x\ge-1,\, \alpha\ge 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.[2]

See also

References

Specific
  1. Arfken, Weber, and Harris (2013) "Mathematical Methods for Physicists", 7th edition; ch. 18.4
  2. Olver . Sheehan . Townsend . Alex . A Fast and Well-Conditioned Spectral Method . SIAM Review . January 2013 . 55 . 3 . 462–489 . 0036-1445 . 1095-7200 . 10.1137/120865458 . 1202.1347 .