DOI: https://doi.org/10.55060/b.p2fg2n.ch006.220215.009
In Hilbertian spaces
In this section, we give the simplest properties of the orthogonal polynomials with respect to a weight w. For a more in-depth study of the subject one can consult the classic texts.
Denoting by kn the leading coefficient of the nth polynomial Pn(x) and putting, as usual:
Three consecutive orthogonal polynomial system polynomials, associated with weight w on the interval (a, b), are related by the following recurrence relation:
Furthermore, we have:
For orthogonal polynomials, associated with the weight w on [a, b], the following Christoffel-Darboux identity holds:
∀n, the zeros x1, x2, … , xn of the polynomial Pn, belonging to the set of polynomials orthogonal in [a, b] with respect to the weight w, are all real, distinct and internal to the interval [a, b].
Two consecutive orthogonal polynomials Pn(x) and Pn+1(x) of the set of orthogonal polynomials in (a, b) with respect to an assigned weight w have no common zeros.
Moreover, there exists the so-called theorem of separation of zeros. Denoting by x1 < x2 < ⋯ < xn+1 the zeros of the polynomial Pn+1(x), belonging to the set of polynomials orthogonal in (a, b) with respect to the weight w, in each of the open intervals (xk, xk+1) (k = 1, 2, ..., n) exactly one zero of Pn(x) falls.
The orthogonal polynomials that are most frequently encountered in applications are those called classical orthogonal polynomials, which are solutions of a differential equation of the hypergeometric type (see [75]), that is, of the type:
These polynomials, disregarding inessential linear changes in the independent variable, can be reduced to the following:
Jacobi polynomials:
Laguerre polynomials:
Hermite polynomials: Hn(x) orthogonal in (−∞, +∞) with respect to the weight:
All of the above systems of polynomials constitute complete systems in the respective spaces
The weight w(x) of the classical orthogonal polynomials satisfies the following Pearson differential equation:
Classical orthogonal polynomials satisfy the following generalized Rodrigues’ formula:
In what follows, we limit ourselves to consider only the Chebyshev polynomials.
Starting from the identity (eit)n = ei nt, by using Euler’s formula:
Comparing Equations (6.11) and (6.12) we find:
Putting x = cos t in (6.13) and (6.14), we obtain two polynomials in x of degrees n and n − 1 which are called, respectively, Chebyshev polynomials (CP in short) of the first and second kind:
Such polynomials enjoy many important properties [71, 84] of which we recall the most simple ones.
The trigonometric identity:
Note that:
The leading coefficient of Tn(x) is 2n−1.
When n = 2m (m ∈ ℕ), T2m (x) is an even function of x, while T2m+1(x) is an odd function of x.
∀ n ∈ ℕ, Tn(1) = 1 and Tn(−1) = (−1)n.
From the equation:
Furthermore, it follows that:
All the n zeros of Tn(x) are real, simple and internal to [−1, 1]. More precisely, they are given by:
In fact, it follows that:
Similarly, the properties of the second kind Chebyshev polynomials can be obtained, but we limit ourselves to list them here. They verify the same recursion as the Tn(x):
The second kind Chebyshev polynomials play an important role in representing the powers of a 2×2 non-singular matrix [76, 81]. Extension of this polynomial family to the multivariate case has been considered for representing the powers of an r × r (r ≥ 3) non-singular matrix (see [80, 81]).
Chebyshev polynomials are a particular case of the Jacobi polynomials
Therefore, properties of the Chebyshev polynomials could be deduced in a more general framework of the hypergeometric functions.
In connection with interpolation and quadrature problems, another couple of Chebyshev polynomials have been considered. They correspond to different choices of weights:
These were called the third and fourth kind Chebyshev polynomials by Walter Gautschi [38].
The third and fourth kind Chebyshev polynomials are defined in [−1, 1] as follows:
Since Wn(x) = (−1)nVn(−x), the third kind Chebyshev polynomials transform into those of the fourth kind by interchanging the ends of the interval [−1, 1] and so they are not essentially different from each other.
Taking up the case of the expansions of a function f(x) in (a, b) by means of the uniformly convergent series:
Moreover, if the system of the uk(x) functions is complete, then the extension to the
If the system used is not complete, the convergence in quadratic mean does not occur towards the function f(x), but towards the projection of the function f(x) on the linear manifold generated by the linear combinations of the functions of the system being used.