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Chebyshev polynomials

Pair of polynomial sequences

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Through Trigonometric functions, Absolute value and Interval (mathematics)

The Chebyshev polynomials of the first kind Tn are defined by

Tn(cos⁡θ)=cos⁡(nθ).

Similarly, the Chebyshev polynomials of the second kind Un are defined by

Un(cos⁡θ)sin⁡θ=sin((n+1)θ).

That these expressions define polynomials in cos⁡θ is not obvious at first sight but can be shown using de Moivre's formula (see below).

The Chebyshev polynomials Tn are polynomials with the largest possible leading coefficient whose absolute value on the interval [−1, 1] is bounded by 1. They are also the "extremal" polynomials for many other properties.

In 1952, Cornelius Lanczos showed that the Chebyshev polynomials are important in approximation theory for the solution of linear systems; the roots of Tn(x), which are also called Chebyshev nodes, are used as matching points for optimizing polynomial interpolation. The resulting interpolation polynomial minimizes the problem of Runge's phenomenon and provides an approximation that is close to the best polynomial approximation to a continuous function under the maximum norm, also called the "minimax" criterion. This approximation leads directly to the method of Clenshaw–Curtis quadrature.

These polynomials were named after Pafnuty Chebyshev. The letter T is used because of the alternative transliterations of the name Chebyshev as Tchebycheff, Tchebyshev (French) or Tschebyschow (German).

Definitions

Recurrence definition

The Chebyshev polynomials of the first kind can be defined by the recurrence relation

T0(x)=1,T1(x)=x,Tn+1(x)=2xTn(x)−Tn−1(x).

The Chebyshev polynomials of the second kind can be defined by the recurrence relation

U0(x)=1,U1(x)=2x,Un+1(x)=2xUn(x)−Un−1(x), which differs from the above only by the rule for n=1.

Trigonometric definition

The Chebyshev polynomials of the first and second kind can be defined as the unique polynomials satisfying Tn(cos⁡θ)=cos⁡(nθ) and Un(cos⁡θ)=sin((n+1)θ)sin⁡θ, for n = 0, 1, 2, 3, ….

An equivalent way to state this is via exponentiation of a complex number: given a complex number z = a + bi with absolute value of one, zn=Tn(a)+ibUn−1(a).

Chebyshev polynomials can also be defined in this form when studying trigonometric polynomials.

That cos⁡(nx) is an nth-degree polynomial in cos⁡(x) can be seen by observing that cos⁡(nx) is the real part of one side of de Moivre's formula: cos⁡nθ+isin⁡nθ=(cos⁡θ+isin⁡θ)n.

The real part of the other side is a polynomial in cos⁡x and sin⁡x, in which all powers of sin⁡x are even and thus replaceable through the identity cos2⁡x+sin2⁡x=1. By the same reasoning, sin⁡nx is the imaginary part of the polynomial, in which all powers of sin⁡x are odd and thus, if one factor of sin⁡x is factored out, the remaining factors can be replaced to create a polynomial of degree n−1 in cos⁡x.

For x outside the interval [-1,1], the above definition implies Tn(x)={cos⁡(narccos⁡x) if |x|≤1,cosh⁡(narccosh⁡x) if x≥1,(−1)ncosh(narccosh⁡(−x)) if x≤−1.

Commuting polynomials definition

Chebyshev polynomials can also be characterized by the following theorem:

If Fn(x) is a family of monic polynomials with coefficients in a field of characteristic 0 such that deg⁡Fn(x)=n and Fm(Fn(x))=Fn(Fm(x)) for all m and n, then, up to a simple change of variables, either Fn(x)=xn for all n or Fn(x)=2⋅Tn(12x) for all n.

Pell equation definition

The Chebyshev polynomials can also be defined as the solutions to the Pell equation: Tn(x)2−(x2−1)Un−1(x)2=1

in a ring ⁠R[x]⁠. Thus, they can be generated by the standard technique for Pell equations of taking powers of a fundamental solution: Tn(x)+Un−1(x)x2−1=(x+x2−1)n.

Generating functions

The ordinary generating function for Tn is ∑n=0∞Tn(x)tn=1−tx1−2tx+t2.

There are several other generating functions for the Chebyshev polynomials; the exponential generating function is ∑n=0∞Tn(x)tnn!=12(exp(t(x−x2−1))+exp(t(x+x2−1)))=etxcosh(tx2−1).

The generating function relevant for 2-dimensional potential theory and multipole expansion is ∑n=1∞Tn(x)tnn=ln⁡(11−2tx+t2).

The ordinary generating function for Un is ∑n=0∞Un(x)tn=11−2tx+t2, and the exponential generating function is ∑n=0∞Un(x)tnn!=etx(cosh(tx2−1)+xx2−1sinh(tx2−1)).

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