In
mathematics the 'Chebyshev polynomials', named after
Pafnuty Chebyshev, are a
sequence of
orthogonal polynomials which are related to
de Moivre's formula and which are easily defined
recursively, like
Fibonacci or
Lucas numbers. One usually distinguishes between 'Chebyshev polynomials of the first kind' which are denoted ''T''
''n'' and 'Chebyshev polynomials of the second kind' which are denoted ''U''
''n''. The letter T is used because of the alternative
transliterations of the name ''Chebyshev'' as ''Tchebyshef'' or ''Tschebyscheff''.
The Chebyshev polynomials ''T''
''n'' or ''U''
''n'' are polynomials of degree ''n'' and the
sequence of Chebyshev polynomials of either kind composes a
polynomial sequence.
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'
:
and
:
for the polynomials of the first and second kind, respectively. These equations are special cases of the
Sturm-Liouville differential equation.
Definition
The 'Chebyshev polynomials of the first kind' are defined by the
recurrence relation
:
:
:
One example of a
generating function for T
n is
:
The 'Chebyshev polynomials of the second kind' are defined by the
recurrence relation
:
:
:
One example of a
generating function for U
n is
:
Trigonometric definition
The Chebyshev polynomials of the first kind can be defined by the
trigonometric identity:
:
whence:
:
for ''n'' = 0, 1, 2, 3, ..., while the polynomials of the second kind satisfy:
:
which is structurally quite similar to the
Dirichlet kernel.
That cos(''nx'') is an ''n''th-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 via the identity cos²(''x'') + sin²(''x'') = 1.
This identity is extremely 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:
:
and:
:
one can straightforwardly determine that:
:
:
and so forth. To trivially check whether the results seem reasonable, sum the coefficients on both sides of the equals sign (that is, setting theta equal to zero, for which the cosine is unity), and one sees that 1 = 2 - 1 in the former expression and 1 = 4 - 3 in the latter.
An immediate corollary is the composition identity (or the "nesting property")
:
Written explicitly
:
(not forgetting that the inverse hyperbolic cosines of ''x'' and −''x'' differ by the constant π). From reasoning similar to that above, one can develop a
closed-form generating formula for Chebyshev polynomials of the first kind:
:
which, combined with
DeMoivre's formula:
:
yields:
:
which, of course, is far more expedient for determining the cosine of N times a given angle than is cranking through almost N rounds of the recursive generator calculation. Finally, if we replace
with ''x'', we can alternatively write:
:
Pell equation definition
The Chebyshev polynomials can also be defined as the solutions to the
Pell equation
:
in a ring R[''x''] (e.g., see
Demeyer (2007), p.70). Thus, they can be generated by the standard technique for Pell equations of taking powers of a fundamental solution:
:
Mutual recurrence
Equivalently, the two sequences can also be defined at once from a pair of mutual recurrence equations:
:
:
:
:
These can be derived from the trigonometric formulae; for example, if
, then
:
::
::
::
(Both these equations and the trigonometric equations take a simpler form if we, like some works, follow the alternate convention of denoting our
(the polynomial of degree n) with
instead.)
Orthogonality
Both the ''T''
''n'' and the ''U''
''n'' form a sequence of
orthogonal polynomials. The polynomials of the first kind are orthogonal with respect to the weight
:
on the interval [−1,1], i.e. we have:
:
This can be proven by letting ''x='' cos(θ) and using the identity
''T
n'' (cos(θ))=cos(nθ). Similarly, the polynomials of the second kind are orthogonal with respect to the weight
:
on the interval [−1,1], i.e. we have:
:
(which, when
normalized to form a
probability measure, is the
Wigner semicircle distribution).
Minimal -norm
For any given
, among the polynomials of degree
with leading coefficient 1,
is the one of which the maximal absolute value on the interval
is minimal.
This maximal absolute value is
and
reaches this maximum exactly
times: in
and
and the other
extremal points of
.
Relation between Chebyshev polynomials of the first and second kind
The Chebyshev polynomials of the first and second kind are closely related by the following equations
:
:
:
:
The recurrence relationship of the derivative of Chebyshev polynomials can be derived from these relations
:
This relationship is used in the
Chebyshev spectral method of solving differential equations.
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.
For every nonnegative integer
,
and
are both polynomials of degree
.
They are
even or odd functions of
as
is even or odd, so when written as polynomials of
, it only has even or odd degree terms resp.
The leading coefficient of
is
if
, but
if
.
Examples
The first few Chebyshev polynomials of the first kind are
:
:
:
:
:
:
:
:
:
:
The first few Chebyshev polynomials of the second kind are
:
:
:
:
:
:
:
Polynomial in Chebyshev form
A polynomial of degree ''N'' in Chebyshev form is a polynomial ''p''(''x'') of the form
:
where ''T''
''n'' is the ''n''th Chebyshev polynomial.
Polynomials in Chebyshev form can be evaluated using the
Clenshaw algorithm.
Chebyshev roots
A Chebyshev polynomial of either kind with degree ''n'' has ''n'' different simple roots, called 'Chebyshev roots', in the interval [−1,1]. The roots are sometimes called
Chebyshev nodes because they are used as ''nodes'' in polynomial interpolation. Using the trigonometric definition and the fact that
:
one can easily prove that the roots of ''T''
''n'' are
:
Similarly, the roots of ''U''
''n'' are
:
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
★
Chebyshev nodes
★
Chebyshev filter
★
Chebyshev cube root
★
Legendre polynomials
★
Hermite polynomials
★
Chebyshev rational functions
★
Clenshaw-Curtis quadrature
★
Approximation theory
References
★
External links
★
★
Module for Chebyshev Polynomials by John H. Mathews