discrete Chebyshev polynomials

{{distinguish|Chebyshev polynomials}}

In mathematics, discrete Chebyshev polynomials, or Gram polynomials, are a type of discrete orthogonal polynomials used in approximation theory, introduced by Pafnuty Chebyshev{{citation |last=Chebyshev|first=P. |title=Sur l'interpolation |journal=Zapiski Akademii Nauk |volume=4|year=1864|id=Oeuvres Vol 1 p. 539–560 |url=https://archive.org/stream/oeuvresdepltche01chebrich#page/n551/mode/2up }} and rediscovered by Gram.{{Citation | last1=Gram | first1=J. P. | title=Ueber die Entwickelung reeller Functionen in Reihen mittelst der Methode der kleinsten Quadrate | url=http://resolver.sub.uni-goettingen.de/purl?GDZPPN002158604 | language=German | jfm=15.0321.03 | year=1883 | journal=Journal für die reine und angewandte Mathematik | volume=1883 | issue=94 | pages=41–73 | doi=10.1515/crll.1883.94.41| s2cid=116847377 | url-access=subscription }} They were later found to be applicable to various algebraic properties of spin angular momentum.

Elementary Definition

The discrete Chebyshev polynomial t^N_n(x) is a polynomial of degree n in x, for n = 0, 1, 2,\ldots, N -1, constructed such that two polynomials of unequal degree are orthogonal with respect to the weight function

w(x) = \sum_{r = 0}^{N-1} \delta(x-r),

with \delta(\cdot) being the Dirac delta function. That is,

\int_{-\infty}^{\infty} t^N_n(x) t^N_m (x) w(x) \, dx = 0 \quad \text{ if } \quad n \ne m .

The integral on the left is actually a sum because of the delta function, and we have,

\sum_{r = 0}^{N-1} t^N_n(r) t^N_m (r) = 0 \quad \text{ if }\quad n \ne m.

Thus, even though t^N_n(x) is a polynomial in x, only its values at a discrete set of points,

x = 0, 1, 2, \ldots, N-1 are of any significance. Nevertheless, because these polynomials can be defined in terms of orthogonality with respect to a nonnegative weight function, the entire theory of orthogonal polynomials is applicable. In particular, the polynomials are complete in the sense that

\sum_{n = 0}^{N-1} t^N_n(r) t^N_n (s) = 0 \quad \text{ if }\quad r \ne s.

Chebyshev chose the normalization so that

\sum_{r = 0}^{N-1} t^N_n(r) t^N_n (r) = \frac{N}{2n+1} \prod_{k=1}^n (N^2 - k^2).

This fixes the polynomials completely along with the sign convention, t^N_n(N - 1) > 0.

If the independent variable is linearly scaled and shifted so that the end points assume the values -1 and 1, then as N \to \infty , t^N_n(\cdot) \to P_n(\cdot) times a constant, where P_n is the Legendre polynomial.

Advanced Definition

Let {{math|f}} be a smooth function defined on the closed interval [−1, 1], whose values are known explicitly only at points {{math|1=xk := −1 + (2k − 1)/m}}, where k and m are integers and {{math|1 ≤ km}}. The task is to approximate f as a polynomial of degree n < m. Consider a positive semi-definite bilinear form

\left(g,h\right)_d:=\frac{1}{m}\sum_{k=1}^{m}{g(x_k)h(x_k)},

where {{math|g}} and {{math|h}} are continuous on [−1, 1] and let

\left\|g\right\|_d:=(g,g)^{1/2}_{d}

be a discrete semi-norm. Let \varphi_k be a family of polynomials orthogonal to each other

\left( \varphi_k, \varphi_i\right)_d = 0

whenever {{mvar|i}} is not equal to {{mvar|k}}. Assume all the polynomials \varphi_k have a positive leading coefficient and they are normalized in such a way that

\left\|\varphi_k\right\|_d=1.

The \varphi_k are called discrete Chebyshev (or Gram) polynomials.{{cite journal

| author = R.W. Barnard |author2=G. Dahlquist |author3=K. Pearce |author4=L. Reichel |author5=K.C. Richards

| title = Gram Polynomials and the Kummer Function

| journal = Journal of Approximation Theory

| year = 1998

| volume = 94

| pages = 128–143

| doi = 10.1006/jath.1998.3181

| doi-access = free

}}

Connection with Spin Algebra

The discrete Chebyshev polynomials have surprising connections to various algebraic properties of spin: spin transition probabilities,{{cite journal

| author = A. Meckler

| title = Majorana formula

| journal = Physical Review

| year = 1958

| volume = 111

| issue = 6

| page = 1447

| doi = 10.1103/PhysRev.111.1447

| bibcode = 1958PhRv..111.1447M

}}

the probabilities for observations of the spin in Bohm's spin-s version of the Einstein-Podolsky-Rosen experiment,{{cite journal

| author = N. D. Mermin | author2 = G. M. Schwarz

| title = Joint distributions and local realism in the higher-spin Einstein-Podolsky-Rosen experiment

| journal = Foundations of Physics

| year = 1982

| volume = 12

| issue = 2

| page = 101

| doi = 10.1007/BF00736844

| bibcode = 1982FoPh...12..101M

| s2cid = 121648820

}}

and Wigner functions for various spin states.{{cite journal

| author = Anupam Garg

| title = The discrete Chebyshev–Meckler–Mermin–Schwarz polynomials and spin algebra

| journal = Journal of Mathematical Physics

| year = 2022

| volume = 63

| issue = 7

| page = 072101

| doi = 10.1063/5.0094575

| bibcode = 2022JMP....63g2101G

}}

Specifically, the polynomials turn out to be the eigenvectors of the absolute square of the rotation matrix (the Wigner D-matrix). The associated eigenvalue is the Legendre polynomial P_{\ell}(\cos \theta), where \theta is the rotation angle. In other words, if

d_{mm'} = \langle j,m|e^{-i\theta J_y}|j,m'\rangle,

where |j,m\rangle are the usual angular momentum or spin eigenstates,

and

F_{mm'}(\theta) = |d_{mm'}(\theta)|^2 ,

then

\sum_{m' = -j}^j F_{mm'}(\theta)\, f^j_{\ell}(m')= P_{\ell}(\cos\theta) f^j_{\ell}(m) .

The eigenvectors f^j_{\ell}(m) are scaled and shifted versions of the Chebyshev polynomials. They are shifted so as to have support on the points m = -j, -j + 1, \ldots, j instead of r = 0, 1, \ldots, N for t^N_n(r) with N corresponding to 2j+1 , and n corresponding to \ell. In addition, the f^j_{\ell}(m) can be scaled so as to obey other normalization conditions. For example, one could demand that they satisfy

\frac{1}{2j+1} \sum_{m=-j}^{j} f^j_{\ell}(m) f^j_{\ell'}(m) = \delta_{\ell\ell'},

along with f^j_{\ell}(j) > 0 .

References