Chebyshev polynomials

From Wikipedia, the free encyclopedia

In mathematics the Chebyshev polynomials, named after Pafnuty Chebyshev,[1] are a sequence of orthogonal polynomials which are related to de Moivre's formula and which can be defined recursively. One usually distinguishes between Chebyshev polynomials of the first kind which are denoted Tn and Chebyshev polynomials of the second kind which are denoted Un. The letter T is used because of the alternative transliterations of the name Chebyshev as Tchebycheff, Tchebyshev (French) or Tschebyschow (German).

The Chebyshev polynomials Tn or Un are polynomials of degree n and the sequence of Chebyshev polynomials of either kind composes a polynomial sequence.

Chebyshev polynomials are polynomials with the largest possible leading coefficient, but subject to the condition that their absolute value is bounded on the interval by 1. They are also the extremal polynomials for many other properties.[2]

Chebyshev polynomials are important in approximation theory because the roots of the Chebyshev polynomials of the first kind, which are also called Chebyshev nodes, are used as nodes in polynomial interpolation. The resulting interpolation polynomial minimizes the problem of Runge's phenomenon and provides an approximation that is close to the polynomial of best approximation to a continuous function under the maximum norm. This approximation leads directly to the method of Clenshaw–Curtis quadrature.

In the study of differential equations they arise as the solution to the Chebyshev differential equations

(1-x^{2})\,y''-x\,y'+n^{2}\,y=0\,\!

and

(1-x^{2})\,y''-3x\,y'+n(n+2)\,y=0\,\!

for the polynomials of the first and second kind, respectively. These equations are special cases of the SturmLiouville differential equation.

Definition

The Chebyshev polynomials of the first kind are defined by the recurrence relation

{\begin{aligned}T_{0}(x)&=1\\T_{1}(x)&=x\\T_{{n+1}}(x)&=2xT_{n}(x)-T_{{n-1}}(x).\end{aligned}}

The ordinary generating function for Tn is

\sum _{{n=0}}^{{\infty }}T_{n}(x)t^{n}={\frac  {1-tx}{1-2tx+t^{2}}};\,\!

the exponential generating function is

\sum _{{n=0}}^{{\infty }}T_{n}(x){\frac  {t^{n}}{n!}}={\tfrac  {1}{2}}\left(e^{{(x-{\sqrt  {x^{2}-1}})t}}+e^{{(x+{\sqrt  {x^{2}-1}})t}}\right)=e^{{tx}}\cosh(t{\sqrt  {x^{2}-1}}).\,\!

The generating function relevant for 2-dimensional potential theory and multipole expansion is

\sum \limits _{{n=1}}^{{\infty }}T_{{n}}\left(x\right){\frac  {t^{{n}}}{n}}=\ln {\frac  {1}{{\sqrt  {1-2tx+t^{{2}}}}}}.

The Chebyshev polynomials of the second kind are defined by the recurrence relation

{\begin{aligned}U_{0}(x)&=1\\U_{1}(x)&=2x\\U_{{n+1}}(x)&=2xU_{n}(x)-U_{{n-1}}(x).\end{aligned}}

The ordinary generating function for Un is

\sum _{{n=0}}^{{\infty }}U_{n}(x)t^{n}={\frac  {1}{1-2tx+t^{2}}};\,\!

the exponential generating function is

\sum _{{n=0}}^{{\infty }}U_{n}(x){\frac  {t^{n}}{n!}}=e^{{tx}}\left(\cosh(t{\sqrt  {x^{2}-1}})+{\frac  {x}{{\sqrt  {x^{2}-1}}}}\sinh(t{\sqrt  {x^{2}-1}})\right).\,\!

Trigonometric definition

The Chebyshev polynomials of the first kind can be defined as the unique polynomials satisfying

T_{n}(x)=\cos(n\arccos x)=\cosh(n\,{\mathrm  {arccosh}}\,x)\,\!

or, in other words, as the unique polynomials satisfying

T_{n}(\cos(\vartheta ))=\cos(n\vartheta )\,\!

for n = 0, 1, 2, 3, ... which is a variant (equivalent transpose) of Schröder's equation, viz. Tn(x) is functionally conjugate to nx, codified in the nesting property below. Further compare to the spread polynomials, in the section below.

The polynomials of the second kind satisfy:

U_{n}(\cos(\vartheta ))={\frac  {\sin((n+1)\vartheta )}{\sin \vartheta }}\,,

which is structurally quite similar to the Dirichlet kernel D_{n}(x)\,\!:

D_{n}(x)={\frac  {\sin((2n+1)(x/2))}{\sin(x/2)}}=U_{{2n}}(\cos(x/2))\,.

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, and 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.

This identity is quite useful in conjunction with the recursive generating formula, inasmuch as it enables one to calculate the cosine of any integral multiple of an angle solely in terms of the cosine of the base angle.

Evaluating the first two Chebyshev polynomials,

T_{0}(x)=\cos(0x)=1

and

T_{1}(\cos(x))=\cos(x)\,,

one can straightforwardly determine that

\cos(2\vartheta )=2\cos \vartheta \cos \vartheta -\cos(0\vartheta )=2\cos ^{{2}}\,\vartheta -1\,\!
\cos(3\vartheta )=2\cos \vartheta \cos(2\vartheta )-\cos \vartheta =4\cos ^{3}\,\vartheta -3\cos \vartheta \,,

and so forth.

Two immediate corollaries are the composition identity (or nesting property specifying a semigroup)

T_{n}(T_{m}(x))=T_{{nm}}(x)\,;

and the expression of complex exponentiation in terms of Chebyshev polynomials: given z = a + bi,

{\begin{aligned}z^{n}&=|z|^{n}\left(\cos \left(n\arccos {\frac  a{|z|}}\right)+i\sin \left(n\arccos {\frac  a{|z|}}\right)\right)\\&=|z|^{n}T_{n}\left({\frac  a{|z|}}\right)+ib\ |z|^{{n-1}}\ U_{{n-1}}\left({\frac  a{|z|}}\right).\end{aligned}}

Pell equation definition

The Chebyshev polynomials can also be defined as the solutions to the Pell equation

T_{n}(x)^{2}-(x^{2}-1)U_{{n-1}}(x)^{2}=1\,\!

in a ring R[x].[3] Thus, they can be generated by the standard technique for Pell equations of taking powers of a fundamental solution:

T_{n}(x)+U_{{n-1}}(x){\sqrt  {x^{2}-1}}=(x+{\sqrt  {x^{2}-1}})^{n}.\,\!

Relation between Chebyshev polynomials of the first and second kinds

The Chebyshev polynomials of the first and second kind are closely related by the following equations

{\tfrac  {d}{dx}}\,T_{n}(x)=nU_{{n-1}}(x){\mbox{ , }}n=1,\ldots
T_{n}(x)={\tfrac  {1}{2}}(U_{n}(x)-\,U_{{n-2}}(x)).
T_{{n+1}}(x)=xT_{n}(x)-(1-x^{2})U_{{n-1}}(x)\,
T_{n}(x)=U_{n}(x)-x\,U_{{n-1}}(x),
U_{n}(x)=2\sum _{{j\,\,{\text{odd}}}}^{n}T_{j}(x), where n is odd.
U_{n}(x)=2\sum _{{j\,{\text{even}}}}^{n}T_{j}(x)-1, where n is even.

The recurrence relationship of the derivative of Chebyshev polynomials can be derived from these relations

2T_{n}(x)={\frac  {1}{n+1}}\;{\frac  {d}{dx}}T_{{n+1}}(x)-{\frac  {1}{n-1}}\;{\frac  {d}{dx}}T_{{n-1}}(x){\mbox{ , }}\quad n=1,\ldots

This relationship is used in the Chebyshev spectral method of solving differential equations.

Equivalently, the two sequences can also be defined from a pair of mutual recurrence equations:

T_{0}(x)=1\,\!
U_{{-1}}(x)=0\,\!
T_{{n+1}}(x)=xT_{n}(x)-(1-x^{2})U_{{n-1}}(x)\,
U_{n}(x)=xU_{{n-1}}(x)+T_{n}(x)\,

These can be derived from the trigonometric formulae; for example, if x=\cos \vartheta , then

{\begin{aligned}T_{{n+1}}(x)&=T_{{n+1}}(\cos(\vartheta ))\\&=\cos((n+1)\vartheta )\\&=\cos(n\vartheta )\cos(\vartheta )-\sin(n\vartheta )\sin(\vartheta )\\&=T_{n}(\cos(\vartheta ))\cos(\vartheta )-U_{{n-1}}(\cos(\vartheta ))\sin ^{2}(\vartheta )\\&=xT_{n}(x)-(1-x^{2})U_{{n-1}}(x).\\\end{aligned}}

Note that both these equations and the trigonometric equations take a simpler form if we, like some works, follow the alternate convention of denoting our Un (the polynomial of degree n) with Un+1 instead.

Turán's inequalities for the Chebyshev polynomials are

T_{n}(x)^{2}-T_{{n-1}}(x)T_{{n+1}}(x)=1-x^{2}>0{\text{ for }}-1<x<1\! and
U_{n}(x)^{2}-U_{{n-1}}(x)U_{{n+1}}(x)=1>0.\!

Explicit expressions

Different approaches to defining Chebyshev polynomials lead to different explicit expressions such as:

T_{n}(x)={\begin{cases}\cos(n\arccos(x)),&\ |x|\leq 1\\\cosh(n\,{\mathrm  {arccosh}}(x)),&\ x\geq 1\\(-1)^{n}\cosh(n\,{\mathrm  {arccosh}}(-x)),&\ x\leq -1\\\end{cases}}\,\!


{\begin{aligned}T_{n}(x)&={\frac  {(x-{\sqrt  {x^{2}-1}})^{n}+(x+{\sqrt  {x^{2}-1}})^{n}}{2}}\\&=\sum _{{k=0}}^{{\lfloor n/2\rfloor }}{\binom  {n}{2k}}(x^{2}-1)^{k}x^{{n-2k}}\\&=x^{n}\sum _{{k=0}}^{{\lfloor n/2\rfloor }}{\binom  {n}{2k}}(1-x^{{-2}})^{k}\\&={\tfrac  {n}{2}}\sum _{{k=0}}^{{\lfloor n/2\rfloor }}(-1)^{k}{\frac  {(n-k-1)!}{k!(n-2k)!}}~(2x)^{{n-2k}}\quad (n>0)\\&=n\sum _{{k=0}}^{{n}}(-2)^{{k}}{\frac  {(n+k-1)!}{(n-k)!(2k)!}}(1-x)^{k}\quad (n>0)\\&=\,_{2}F_{1}\left(-n,n;{\frac  12};{\frac  {1-x}2}\right)\\\end{aligned}}


{\begin{aligned}U_{n}(x)&={\frac  {(x+{\sqrt  {x^{2}-1}})^{{n+1}}-(x-{\sqrt  {x^{2}-1}})^{{n+1}}}{2{\sqrt  {x^{2}-1}}}}\\&=\sum _{{k=0}}^{{\lfloor n/2\rfloor }}{\binom  {n+1}{2k+1}}(x^{2}-1)^{k}x^{{n-2k}}\\&=x^{n}\sum _{{k=0}}^{{\lfloor n/2\rfloor }}{\binom  {n+1}{2k+1}}(1-x^{{-2}})^{k}\\&=\sum _{{k=0}}^{{\lfloor n/2\rfloor }}{\binom  {2k-(n+1)}{k}}~(2x)^{{n-2k}}\quad (n>0)\\&=\sum _{{k=0}}^{{\lfloor n/2\rfloor }}(-1)^{k}{\binom  {n-k}{k}}~(2x)^{{n-2k}}\quad (n>0)\\&=\sum _{{k=0}}^{{n}}(-2)^{{k}}{\frac  {(n+k+1)!}{(n-k)!(2k+1)!}}(1-x)^{k}\quad (n>0)\\&=(n+1)\,_{2}F_{1}\left(-n,n+2;{\tfrac  {3}{2}};{\tfrac  {1}{2}}\left[1-x\right]\right)\end{aligned}}

where _{2}F_{1} is a hypergeometric function.

Properties

Roots and extrema

A Chebyshev polynomial of either kind with degree n has n different simple roots, called Chebyshev roots, in the interval [1,1]. The roots of the Chebyshev polynomial of the first kind are sometimes called Chebyshev nodes because they are used as nodes in polynomial interpolation. Using the trigonometric definition and the fact that

\cos \left({\tfrac  {\pi }{2}}\,(2k+1)\right)=0

one can easily prove that the roots of Tn are

x_{k}=\cos \left({\tfrac  {\pi }{2}}\,{\frac  {2k-1}{n}}\right),\quad k=1,\ldots ,n.

Similarly, the roots of Un are

x_{k}=\cos \left({\frac  {k}{n+1}}\pi \right),\quad k=1,\ldots ,n.

The extrema of Tn on the interval 1 ≤ x ≤ 1 are located at

x_{k}=\cos \left({\tfrac  {k}{n}}\pi \right),\quad k=0,\ldots ,n.

One unique property of the Chebyshev polynomials of the first kind is that on the interval 1 ≤ x ≤ 1 all of the extrema have values that are either 1 or 1. Thus these polynomials have only two finite critical values, the defining property of Shabat polynomials. Both the first and second kinds of Chebyshev polynomial have extrema at the endpoints, given by:

T_{n}(1)=1\,
T_{n}(-1)=(-1)^{n}\,
U_{n}(1)=n+1\,
U_{n}(-1)=(n+1)(-1)^{n}.\,

Differentiation and integration

The derivatives of the polynomials can be less than straightforward. By differentiating the polynomials in their trigonometric forms, it's easy to show that:

{\frac  {dT_{n}}{dx}}=nU_{{n-1}}\,
{\frac  {dU_{n}}{dx}}={\frac  {(n+1)T_{{n+1}}-xU_{n}}{x^{2}-1}}\,
{\frac  {d^{2}T_{n}}{dx^{2}}}=n{\frac  {nT_{n}-xU_{{n-1}}}{x^{2}-1}}=n{\frac  {(n+1)T_{n}-U_{n}}{x^{2}-1}}.\,

The last two formulas can be numerically troublesome due to the division by zero (0/0 indeterminate form, specifically) at x = 1 and x = 1. It can be shown that:

{\frac  {d^{2}T_{n}}{dx^{2}}}{\Bigg |}_{{x=1}}\!\!={\frac  {n^{4}-n^{2}}{3}},
{\frac  {d^{2}T_{n}}{dx^{2}}}{\Bigg |}_{{x=-1}}\!\!=(-1)^{n}{\frac  {n^{4}-n^{2}}{3}}.
Proof

The second derivative of the Chebyshev polynomial of the first kind is

T''_{n}=n{\frac  {nT_{n}-xU_{{n-1}}}{x^{2}-1}}

which, if evaluated as shown above, poses a problem because it is indeterminate at x = ±1. Since the function is a polynomial, (all of) the derivatives must exist for all real numbers, so the taking to limit on the expression above should yield the desired value:

T''_{n}(1)=\lim _{{x\to 1}}n{\frac  {nT_{n}-xU_{{n-1}}}{x^{2}-1}}

where only x=1 is considered for now. Factoring the denominator:

T''_{n}(1)=\lim _{{x\to 1}}n{\frac  {nT_{n}-xU_{{n-1}}}{(x+1)(x-1)}}=\lim _{{x\to 1}}n{\frac  {{\frac  {nT_{n}-xU_{{n-1}}}{x-1}}}{x+1}}.

Since the limit as a whole must exist, the limit of the numerator and denominator must independently exist, and

T''_{n}(1)=n{\frac  {\lim _{{x\to 1}}{\frac  {nT_{n}-xU_{{n-1}}}{x-1}}}{\lim _{{x\to 1}}(x+1)}}={\frac  {n}{2}}\lim _{{x\to 1}}{\frac  {nT_{n}-xU_{{n-1}}}{x-1}}.

The denominator (still) limits to zero, which implies that the numerator must be limiting to zero, i.e. U_{{n-1}}(1)=nT_{n}(1)=n which will be useful later on. Since the numerator and denominator are both limiting to zero, L'Hôpital's rule applies:

{\begin{aligned}T''_{n}(1)&={\frac  {n}{2}}\lim _{{x\to 1}}{\frac  {{\frac  {d}{dx}}(nT_{n}-xU_{{n-1}})}{{\frac  {d}{dx}}(x-1)}}\\&={\frac  {n}{2}}\lim _{{x\to 1}}{\frac  {d}{dx}}(nT_{n}-xU_{{n-1}})\\&={\frac  {n}{2}}\lim _{{x\to 1}}\left(n^{2}U_{{n-1}}-U_{{n-1}}-x{\frac  {d}{dx}}(U_{{n-1}})\right)\\&={\frac  {n}{2}}\left(n^{2}U_{{n-1}}(1)-U_{{n-1}}(1)-\lim _{{x\to 1}}x{\frac  {d}{dx}}(U_{{n-1}})\right)\\&={\frac  {n^{4}}{2}}-{\frac  {n^{2}}{2}}-{\frac  {1}{2}}\lim _{{x\to 1}}{\frac  {d}{dx}}(nU_{{n-1}})\\&={\frac  {n^{4}}{2}}-{\frac  {n^{2}}{2}}-{\frac  {T''_{n}(1)}{2}}\\T''_{n}(1)&={\frac  {n^{4}-n^{2}}{3}}.\\\end{aligned}}

The proof for x=-1 is similar, with the fact that T_{n}(-1)=(-1)^{n} being important.


Indeed, the following, more general formula holds:

{\frac  {d^{p}T_{n}}{dx^{p}}}{\Bigg |}_{{x=\pm 1}}\!\!=(\pm 1)^{{n+p}}\prod _{{k=0}}^{{p-1}}{\frac  {n^{2}-k^{2}}{2k+1}}.

This latter result is of great use in the numerical solution of eigenvalue problems.

Concerning integration, the first derivative of the Tn implies that

\int U_{n}\,dx={\frac  {T_{{n+1}}}{n+1}}\,

and the recurrence relation for the first kind polynomials involving derivatives establishes that

\int T_{n}\,dx={\frac  {1}{2}}\left({\frac  {T_{{n+1}}}{n+1}}-{\frac  {T_{{n-1}}}{n-1}}\right)={\frac  {nT_{{n+1}}}{n^{2}-1}}-{\frac  {xT_{n}}{n-1}}.\,

Orthogonality

Both the Tn and the Un form a sequence of orthogonal polynomials. The polynomials of the first kind are orthogonal with respect to a linear transformation of Jeffreys prior that has the weight

{\frac  {1}{{\sqrt  {1-x^{2}}}}},\,\!

on the interval [1,1], i.e. we have:

\int _{{-1}}^{1}T_{n}(x)T_{m}(x)\,{\frac  {dx}{{\sqrt  {1-x^{2}}}}}={\begin{cases}0&:n\neq m\\\pi &:n=m=0\\\pi /2&:n=m\neq 0\end{cases}}

This can be proven by letting x = cos (θ) and using the defining identity Tn(cos (θ)) = cos ().

Similarly, the polynomials of the second kind are orthogonal with respect to the weight

{\sqrt  {1-x^{2}}}\,\!

on the interval [1,1], i.e. we have:

\int _{{-1}}^{1}U_{n}(x)U_{m}(x){\sqrt  {1-x^{2}}}\,dx={\begin{cases}0&:n\neq m,\\\pi /2&:n=m.\end{cases}}

(Note that the measure {\sqrt  {1-x^{2}}}\,dx is, to within a normalizing constant, the Wigner semicircle distribution).

The Tn also satisfy a discrete orthogonality condition:

\sum _{{k=0}}^{{N-1}}{T_{i}(x_{k})T_{j}(x_{k})}={\begin{cases}0&:i\neq j\\N&:i=j=0\\N/2&:i=j\neq 0\end{cases}}\,\!

where the xk are the N GaussLobatto zeros of TN(x)

x_{k}=\cos \left({\frac  {\pi \left(k+{\frac  {1}{2}}\right)}{N}}\right).

Minimal ∞-norm

For any given n ≥ 1, among the polynomials of degree n with leading coefficient 1,

f(x)={\frac  1{2^{{n-1}}}}T_{n}(x)

is the one of which the maximal absolute value on the interval [1, 1] is minimal.

This maximal absolute value is

{\frac  1{2^{{n-1}}}}

and |ƒ(x)| reaches this maximum exactly n + 1 times at

x=\cos {\frac  {k\pi }{n}}{\text{ for }}0\leq k\leq n.
Proof

Let's assume that w_{n}(x) is a polynomial of degree n with leading coefficient 1 with maximal absolute value on the interval [1, 1] less than {\frac  1{2^{{n-1}}}}.

Define

f_{n}(x)={\frac  1{2^{{n-1}}}}T_{n}(x)-w_{n}(x)

Because at extreme points of T_{n} we have |w_{n}(x)|<\left|{\frac  1{2^{{n-1}}}}T_{n}(x)\right|

f_{n}(x)>0{\text{ for }}x=\cos {\frac  {2k\pi }{n}}{\text{ where }}0\leq 2k\leq n
f_{n}(x)<0{\text{ for }}x=\cos {\frac  {(2k+1)\pi }{n}}{\text{ where }}0\leq 2k+1\leq n

From the intermediate value theorem, f_{n}(x) has at least n roots. However, this is impossible, as f_{n}(x) is a polynomial of degree n − 1, so the fundamental theorem of algebra implies it has at most n − 1 roots.

Other properties

The Chebyshev polynomials are a special case of the ultraspherical or Gegenbauer polynomials, which themselves are a special case of the Jacobi polynomials:

  • T_{n}(x)={\frac  1{{n-{\frac  12} \choose n}}}P_{n}^{{-{\frac  12},-{\frac  12}}}(x)={\frac  n2}C_{n}^{0}(x),
  • U_{n}(x)={\frac  1{2{n+{\frac  12} \choose n}}}P_{n}^{{{\frac  12},{\frac  12}}}(x)=C_{n}^{1}(x).

For every nonnegative integer n, Tn(x) and Un(x) are both polynomials of degree n. They are even or odd functions of x as n is even or odd, so when written as polynomials of x, it only has even or odd degree terms respectively. In fact,

T_{{2n}}(x)=T_{n}\left(2x^{2}-1\right)=2T_{n}(x)^{2}-1

and

2xU_{n}\left(1-2x^{2}\right)=(-1)^{n}U_{{2n+1}}(x).

The leading coefficient of Tn is 2n 1 if 1 ≤ n, but 1 if 0 = n.

Tn are a special case of Lissajous curves with frequency ratio equal to n.

Several polynomial sequences like Lucas polynomials (Ln), Dickson polynomials (Dn), Fibonacci polynomials (Fn) are related to Chebyshev polynomials Tn and Un.

The Chebyshev polynomials of the first kind satisfy the relation

T_{j}(x)T_{k}(x)={\tfrac  {1}{2}}\left(T_{{j+k}}(x)+T_{{|k-j|}}(x)\right),\quad \forall j,k\geq 0,\,

which is easily proved from the product-to-sum formula for the cosine. The polynomials of the second kind satisfy the similar relation

T_{j}(x)U_{k}(x)={\tfrac  {1}{2}}\left(U_{{j+k}}(x)+U_{{k-j}}(x)\right),\quad \forall j,k.

Similar to the formula

T_{n}\left(\cos \theta \right)=\cos(n\theta ),

we have the analogous formula

T_{{2n+1}}\left(\sin \theta \right)=(-1)^{n}\sin((2n+1)\theta ).

For x\neq 0,

T_{n}\left({\tfrac  {1}{2}}\left[x+x^{{-1}}\right]\right)={\tfrac  {1}{2}}\left(x^{n}+x^{{-n}}\right) and
x^{n}=T_{n}\left({\tfrac  {1}{2}}\left[x+x^{{-1}}\right]\right)+{\tfrac  {1}{2}}\left(x-x^{{-1}}\right)U_{{n-1}}\left({\tfrac  {1}{2}}\left[x+x^{{-1}}\right]\right),

which follows from the fact that this holds by definition for x=e^{{i\theta }}.

Let

C_{n}(x)=2T_{n}\left({\frac  {x}{2}}\right).

Then C_{n}(x) and C_{m}(x) are commuting polynomials:

C_{n}\left(C_{m}(x)\right)=C_{m}(C_{n}(x)),

as is evident in the Abelian nesting property specified above.

Examples

First kind

The first few Chebyshev polynomials of the first kind in the domain 1 < x < 1: The flat T0, T1, T2, T3, T4 and T5.

The first few Chebyshev polynomials of the first kind are A028297

T_{0}(x)=1\,
T_{1}(x)=x\,
T_{2}(x)=2x^{2}-1\,
T_{3}(x)=4x^{3}-3x\,
T_{4}(x)=8x^{4}-8x^{2}+1\,
T_{5}(x)=16x^{5}-20x^{3}+5x\,
T_{6}(x)=32x^{6}-48x^{4}+18x^{2}-1\,
T_{7}(x)=64x^{7}-112x^{5}+56x^{3}-7x\,
T_{8}(x)=128x^{8}-256x^{6}+160x^{4}-32x^{2}+1\,
T_{9}(x)=256x^{9}-576x^{7}+432x^{5}-120x^{3}+9x.\,
T_{{10}}(x)=512x^{{10}}-1280x^{8}+1120x^{6}-400x^{4}+50x^{2}-1.\,
T_{{11}}(x)=1024x^{{11}}-2816x^{9}+2816x^{7}-1232x^{5}+220x^{3}-11x.\,

Second kind

The first few Chebyshev polynomials of the second kind in the domain 1 < x < 1: The flat U0, U1, U2, U3, U4 and U5. Although not visible in the image, Un(1) = n + 1 and Un(1) = (n + 1)(1)n.

The first few Chebyshev polynomials of the second kind are

U_{0}(x)=1\,
U_{1}(x)=2x\,
U_{2}(x)=4x^{2}-1\,
U_{3}(x)=8x^{3}-4x\,
U_{4}(x)=16x^{4}-12x^{2}+1\,
U_{5}(x)=32x^{5}-32x^{3}+6x\,
U_{6}(x)=64x^{6}-80x^{4}+24x^{2}-1\,
U_{7}(x)=128x^{7}-192x^{5}+80x^{3}-8x\,
U_{8}(x)=256x^{8}-448x^{6}+240x^{4}-40x^{2}+1\,
U_{9}(x)=512x^{9}-1024x^{7}+672x^{5}-160x^{3}+10x.\,

As a basis set

The non-smooth function (top) y = x3H(x), where H is the Heaviside step function, and (bottom) the 5th partial sum of its Chebyshev expansion. The 7th sum is indistinguishable from the original function at the resolution of the graph.

In the appropriate Sobolev space, the set of Chebyshev polynomials form a orthonormal basis, so that a function in the same space can, on 1 ≤ x ≤ 1 be expressed via the expansion:[4]

f(x)=\sum _{{n=0}}^{\infty }a_{n}T_{n}(x).

Furthermore, as mentioned previously, the Chebyshev polynomials form an orthogonal basis which (among other things) implies that the coefficients an can be determined easily through the application of an inner product. This sum is called a Chebyshev series or a Chebyshev expansion.

Since a Chebyshev series is related to a Fourier cosine series through a change of variables, all of the theorems, identities, etc. that apply to Fourier series have a Chebyshev counterpart.[4] These attributes include:

  • The Chebyshev polynomials form a complete orthogonal system.
  • The Chebyshev series converges to ƒ(x) if the function is piecewise smooth and continuous. The smoothness requirement can be relaxed in most cases — as long as there are a finite number of discontinuities in ƒ(x) and its derivatives.
  • At a discontinuity, the series will converge to the average of the right and left limits.

The abundance of the theorems and identities inherited from Fourier series make the Chebyshev polynomials important tools in numeric analysis; for example they are the most popular general purpose basis functions used in the spectral method,[4] often in favor of trigonometric series due to generally faster convergence for continuous functions (Gibbs' phenomenon is still a problem).

Example 1

Consider the Chebyshev expansion of \log(1+x). One can express

\log(1+x)=\sum _{{n=0}}^{\infty }a_{n}T_{n}(x).

One can find the coefficients a_{n} either through the application of an inner product or by the discrete orthogonality condition. For the inner product,

\int _{{-1}}^{{+1}}{\frac  {T_{m}(x)\log(1+x)}{{\sqrt  {1-x^{2}}}}}dx=\sum _{{n=0}}^{{\infty }}a_{n}\int _{{-1}}^{{+1}}{\frac  {T_{m}(x)T_{n}(x)}{{\sqrt  {1-x^{2}}}}}dx,

which gives

a_{n}={\begin{cases}-\log(2)&:n=0\\{\frac  {-2(-1)^{n}}{n}}&:n>0.\end{cases}}

Alternatively, when you cannot evaluate the inner product of the function you are trying to approximate, the discrete orthogonality condition gives

a_{n}={\frac  {2-\delta _{{0n}}}{N}}\sum _{{k=0}}^{{N-1}}T_{n}(x_{k})\log(1+x_{k}),

where \delta _{{ij}} is the Kronecker delta function and the x_{k} are the N GaussLobatto zeros of T_{N}(x)

x_{k}=\cos \left({\frac  {\pi \left(k+{\frac  {1}{2}}\right)}{N}}\right).

This allows us to compute the coefficients a_{n} very efficiently through the discrete cosine transform

a_{n}={\frac  {2-\delta _{{0n}}}{N}}\sum _{{k=0}}^{{N-1}}\cos \left({\frac  {n\pi \left(k+{\frac  {1}{2}}\right)}{N}}\right)\log(1+x_{k}).

Example 2

To provide another example:

{\begin{aligned}(1-x^{2})^{\alpha }=&-{\frac  1{{\sqrt  \pi }}}{\frac  {\Gamma ({\frac  12}+\alpha )}{\Gamma (\alpha +1)}}+2^{{1-2\alpha }}\sum _{{n=0}}(-1)^{n}{2\alpha  \choose \alpha -n}T_{{2n}}(x)\\=&2^{{-2\alpha }}\sum _{{n=0}}(-1)^{n}{2\alpha +1 \choose \alpha -n}U_{{2n}}(x).\end{aligned}}

Partial sums

The partial sums of

f(x)=\sum _{{n=0}}^{\infty }a_{n}T_{n}(x)

are very useful in the approximation of various functions and in the solution of differential equations (see spectral method). Two common methods for determining the coefficients an are through the use of the inner product as in Galerkin's method and through the use of collocation which is related to interpolation.

As an interpolant, the N coefficients of the (N 1)th partial sum are usually obtained on the ChebyshevGaussLobatto[5] points (or Lobatto grid), which results in minimum error and avoids Runge's phenomenon associated with a uniform grid. This collection of points corresponds to the extrema of the highest order polynomial in the sum, plus the endpoints and is given by:

x_{k}=-\cos \left({\frac  {k\pi }{N-1}}\right);\qquad \ k=0,1,\dots ,N-1.

Polynomial in Chebyshev form

An arbitrary polynomial of degree N can be written in terms of the Chebyshev polynomials of the first kind. Such a polynomial p(x) is of the form

p(x)=\sum _{{n=0}}^{{N}}a_{n}T_{n}(x).

Polynomials in Chebyshev form can be evaluated using the Clenshaw algorithm.

Spread polynomials

The spread polynomials are in a sense equivalent to the Chebyshev polynomials of the first kind, but enable one to avoid square roots and conventional trigonometric functions in certain contexts, notably in rational trigonometry.

See also

Notes

  1. Chebyshev polynomials were first presented in: P. L. Chebyshev (1854) "Théorie des mécanismes connus sous le nom de parallélogrammes," Mémoires des Savants étrangers présentés à l’Académie de Saint-Pétersbourg, vol. 7, pages 539–586.
  2. Rivlin, Theodore J. The Chebyshev polynomials. Pure and Applied Mathematics. Wiley-Interscience [John Wiley & Sons], New York-London-Sydney,1974. Chapter 2, "Extremal Properties", pp. 56--123.
  3. Jeroen Demeyer Diophantine Sets over Polynomial Rings and Hilbert's Tenth Problem for Function Fields, Ph.D. theses (2007), p.70.
  4. 4.0 4.1 4.2 Boyd, John P. (2001). Chebyshev and Fourier Spectral Methods (second ed.). Dover. ISBN 0-486-41183-4. 
  5. Chebyshev Interpolation: An Interactive Tour

References

External links

This article is issued from Wikipedia. The text is available under the Creative Commons Attribution/Share Alike; additional terms may apply for the media files.