Chebyshev nodes (original) (raw)
From Wikipedia, the free encyclopedia
Roots of the Chebyshev polynomials of the first kind
Chebyshev zeros (solid dots, red lines) and extrema (hollow squares, blue lines) are the projection of two sets of equispaced points on the unit circle onto the x-axis. 2_n_ equispaced points on the circle project onto n Chebyshev zeros or n+1 Chebyshev extrema. (Here n = 5.)
The Chebyshev zeros (solid dots) are roots of a Chebyshev polynomial of the first kind (red). The Chebyshev extrema (hollow squares) are roots of a Chebyshev polynomial of the second kind (blue), and also the extrema (crosses) of a Chebyshev polynomial of the first kind.
In numerical analysis, Chebyshev nodes (also called Chebyshev points or a Chebyshev grid) are a set of specific algebraic numbers used as nodes for polynomial interpolation and numerical integration. They are the projection of a set of equispaced points on the unit circle onto the real interval [ − 1 , 1 ] {\displaystyle [-1,1]} , the circle's diameter.
There are two kinds of Chebyshev nodes. The n {\displaystyle n} Chebyshev nodes of the first kind, also called the Chebyshev–Gauss nodes[1] or Chebyshev zeros, are the zeros of a Chebyshev polynomial of the first kind, T n {\displaystyle T_{n}}
. The corresponding n + 1 {\displaystyle n+1}
Chebyshev nodes of the second kind, also called the Chebyshev–Lobatto nodes[2] or Chebyshev extrema, are the extrema of T n {\displaystyle T_{n}}
, which are also the zeros of a Chebyshev polynomial of the second kind, U n − 1 {\displaystyle U_{n-1}}
, along with the two endpoints of the interval. Both types of numbers are commonly referred to as Chebyshev nodes or Chebyshev points in literature.[3] They are named after 19th century Russian mathematician Pafnuty Chebyshev, who first introduced Chebyshev polynomials.
Unlike some other interpolation nodes, the Chebyshev nodes "nest": the existing nodes are retained when doubling the number of nodes, reducing computation for each grid refinement by half. Polynomial interpolants constructed from Chebyshev nodes minimize the effect of Runge's phenomenon.[4] They can be easily converted to a representation as a weighted sum of Chebyshev polynomials using the fast Fourier transform.
Chebyshev nodes of both kinds from n = 2 {\displaystyle n=2} to n = 50 {\displaystyle n=50}
.
For a given positive integer n {\displaystyle n} , the n {\displaystyle n}
Chebyshev nodes of the first kind are given by
x k = cos ( k + 1 2 ) π n , k = 0 , … , n − 1. {\displaystyle x_{k}=\cos {\frac {{\bigl (}k+{\tfrac {1}{2}}{\bigr )}\pi }{n}},\quad k=0,\ldots ,n-1.}
This is the projection of 2 n {\displaystyle 2n} equispaced points on the unit circle onto the interval [ − 1 , 1 ] {\displaystyle [-1,1]}
, the circle's diameter. These points are also the roots of T n {\displaystyle T_{n}}
, the Chebyshev polynomial of the first kind with degree n {\displaystyle n}
.
The n + 1 {\displaystyle n+1} Chebyshev nodes of the second kind are given by
x k = cos k π n , k = 0 , … , n . {\displaystyle x_{k}=\cos {\frac {k\pi }{n}},\quad k=0,\ldots ,n.}
This is also the projection of 2 n {\displaystyle 2n} equispaced points on the unit circle onto [ − 1 , 1 ] {\displaystyle [-1,1]}
, this time including the endpoints of the interval, each of which is only the projection of one point on the circle rather than two. These points are also the extrema of T n {\displaystyle T_{n}}
in [ − 1 , 1 ] {\displaystyle [-1,1]}
, the places where it takes the value ± 1 {\displaystyle \pm 1}
.[5] The interior points among the nodes, not including the endpoints, are also the zeros of U n − 1 {\displaystyle U_{n-1}}
, a Chebyshev polynomial of the second kind, a rescaling of the derivative of T n {\displaystyle T_{n}}
.
For nodes over an arbitrary interval [ a , b ] {\displaystyle [a,b]} an affine transformation from [ − 1 , 1 ] {\displaystyle [-1,1]}
can be used: x ~ k = 1 2 ( a + b ) + 1 2 ( b − a ) x k . {\displaystyle {\tilde {x}}_{k}={\tfrac {1}{2}}(a+b)+{\tfrac {1}{2}}(b-a)x_{k}.}
Both kinds of nodes are always symmetric about zero, the midpoint of the interval.
The node sets for the first few integers n {\displaystyle n} are: roots ( T 0 ) = { } , roots ( U 0 ) = { } , extrema ( T 1 ) = { − 1 , + 1 } , roots ( T 1 ) = { 0 } , roots ( U 1 ) = { 0 } , extrema ( T 2 ) = { − 1 , 0 , + 1 } , roots ( T 2 ) = { − 1 / 2 , + 1 / 2 } , roots ( U 2 ) = { − 1 / 2 , + 1 / 2 } , extrema ( T 3 ) = { − 1 , − 1 / 2 , + 1 / 2 , + 1 } {\displaystyle {\begin{aligned}{\text{roots}}(T_{0})&=\{\},&{\text{roots}}(U_{0})&=\{\},&{\text{extrema}}(T_{1})&=\{-1,+1\},\\{\text{roots}}(T_{1})&=\{0\},&{\text{roots}}(U_{1})&=\{0\},&{\text{extrema}}(T_{2})&=\{-1,0,+1\},\\{\text{roots}}(T_{2})&=\{-1/{\sqrt {2}},+1/{\sqrt {2}}\},&{\text{roots}}(U_{2})&=\{-1/2,+1/2\},&{\text{extrema}}(T_{3})&=\{-1,-1/2,+1/2,+1\}\\\end{aligned}}}
While these sets are sorted by ascending values, the defining formulas given above generate the Chebyshev nodes in reverse order from the greatest to the smallest.
The Chebyshev nodes are important in approximation theory because they form a particularly good set of nodes for polynomial interpolation. Given a function f on the interval [ − 1 , + 1 ] {\displaystyle [-1,+1]} and n {\displaystyle n}
points x 1 , x 2 , … , x n , {\displaystyle x_{1},x_{2},\ldots ,x_{n},}
in that interval, the interpolation polynomial is that unique polynomial P n − 1 {\displaystyle P_{n-1}}
of degree at most n − 1 {\displaystyle n-1}
which has value f ( x i ) {\displaystyle f(x_{i})}
at each point x i {\displaystyle x_{i}}
. The interpolation error at x {\displaystyle x}
is f ( x ) − P n − 1 ( x ) = f ( n ) ( ξ ) n ! ∏ i = 1 n ( x − x i ) {\displaystyle f(x)-P_{n-1}(x)={\frac {f^{(n)}(\xi )}{n!}}\prod _{i=1}^{n}(x-x_{i})}
for some ξ {\displaystyle \xi }
(depending on x) in [−1, 1].[6] So it is logical to try to minimize max x ∈ [ − 1 , 1 ] | ∏ i = 1 n ( x − x i ) | . {\displaystyle \max _{x\in [-1,1]}{\biggl |}\prod _{i=1}^{n}(x-x_{i}){\biggr |}.}
This product is a monic polynomial of degree n. It may be shown that the maximum absolute value (maximum norm) of any such polynomial is bounded from below by 21−n. This bound is attained by the scaled Chebyshev polynomials 21−n T n, which are also monic. (Recall that |T n(x)| ≤ 1 for x ∈ [−1, 1].[7]) Therefore, when the interpolation nodes x i are the roots of T n, the error satisfies | f ( x ) − P n − 1 ( x ) | ≤ 1 2 n − 1 n ! max ξ ∈ [ − 1 , 1 ] | f ( n ) ( ξ ) | . {\displaystyle \left|f(x)-P_{n-1}(x)\right|\leq {\frac {1}{2^{n-1}n!}}\max _{\xi \in [-1,1]}\left|f^{(n)}(\xi )\right|.} For an arbitrary interval [a, b_] a change of variable shows that | f ( x ) − P n − 1 ( x ) | ≤ 1 2 n − 1 n ! ( b − a 2 ) n max ξ ∈ [ a , b ] | f ( n ) ( ξ ) | . {\displaystyle \left|f(x)-P_{n-1}(x)\right|\leq {\frac {1}{2^{n-1}n!}}\left({\frac {b-a}{2}}\right)^{n}\max _{\xi \in [a,b]}\left|f^{(n)}(\xi )\right|.} ![{\displaystyle \left|f(x)-P{n-1}(x)\right|\leq {\frac {1}{2^{n-1}n!}}\left({\frac {b-a}{2}}\right)^{n}\max _{\xi \in [a,b]}\left|f^{(n)}(\xi )\right|.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/148e710a7ce3a352abf06d2fb5640289a8b3228b)
Modified even-order nodes
[edit]
Some applications for interpolation nodes, such as the design of equally terminated passive Chebyshev filters, cannot use even-order Chebyshev nodes directly due to the lack of a root at 0. Instead, the Chebyshev nodes can be moved toward zero, with a double root at zero directly, using a transformation:[8]
x ~ k = sgn ( x k ) x k 2 − x n / 2 2 1 − x n / 2 2 {\displaystyle {\tilde {x}}_{k}=\operatorname {sgn} (x_{k}){\sqrt {\frac {x_{k}^{2}-x_{n/2}^{2}}{1-x_{n/2}^{2}}}}}
For example, Chebyshev nodes of the first kind of order 4 are 0.9239 , 0.3827 , − 0.3827 , − 0.9239 {\displaystyle {0.9239,0.3827,-0.3827,-0.9239}} , with x n / 2 = 0.382683 {\displaystyle x_{n/2}=0.382683}
. Applying the transformation yields new nodes 0.910180 , 0 , 0 , − 0.910180 {\displaystyle {0.910180,0,0,-0.910180}}
. The modified even-order nodes now include zero twice.
- ^ The name Chebyshev–Gauss nodes comes from the use of Chebyshev zeros in numerical integration, which can be seen as a variant of Gaussian quadrature.
- ^ The name Chebyshev–Lobatto nodes comes from Rehuel Lobatto, who made a variant of Gaussian quadrature, known as Lobatto quadrature, whose nodes included the ends of the interval, a feature shared by the Chebyshev extrema.
- ^ Trefethen 2013, pp. 7
- ^ Fink & Mathews 1999, pp. 236–238
- ^ Trefethen 2013, pp. 14
- ^ Stewart 1996, (20.3)
- ^ Stewart 1996, Lecture 20, §14
- ^ Saal, Rudolf (January 1979). Handbook of Filter Design (in English and German) (1st ed.). Munich, Germany: Allgemeine Elektricitäts-Gesellschaft. pp. 25, 26, 56–61, 116, 117. ISBN 3-87087-070-2.
Fink, Kurtis D.; Mathews, John H. (1999). Numerical Methods using MATLAB (3rd ed.). Upper Saddle River NJ: Prentice Hall.
Stewart, Gilbert W. (1996). Afternotes on Numerical Analysis. SIAM. ISBN 978-0-89871-362-6.
Trefethen, Lloyd N. (2013), Approximation Theory and Approximation Practice, SIAM
Burden, Richard L.; Faires, J. Douglas: Numerical Analysis, 8th ed., pages 503–512, ISBN 0-534-39200-8.