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11: Bibliography C
  • R. Chattamvelli and R. Shanmugam (1997) Algorithm AS 310. Computing the non-central beta distribution function. Appl. Statist. 46 (1), pp. 146–156.
  • R. Chelluri, L. B. Richmond, and N. M. Temme (2000) Asymptotic estimates for generalized Stirling numbers. Analysis (Munich) 20 (1), pp. 1–13.
  • M. Colman, A. Cuyt, and J. Van Deun (2011) Validated computation of certain hypergeometric functions. ACM Trans. Math. Software 38 (2), pp. Art. 11, 20.
  • A. G. Constantine (1963) Some non-central distribution problems in multivariate analysis. Ann. Math. Statist. 34 (4), pp. 1270–1285.
  • M. D. Cooper, R. H. Jeppesen, and M. B. Johnson (1979) Coulomb effects in the Klein-Gordon equation for pions. Phys. Rev. C 20 (2), pp. 696–704.
  • 12: 18.22 Hahn Class: Recurrence Relations and Differences
    §18.22 Hahn Class: Recurrence Relations and Differences
    §18.22(i) Recurrence Relations in n
    These polynomials satisfy (18.22.2) with p n ( x ) , A n , and C n as in Table 18.22.1. …
    §18.22(ii) Difference Equations in x
    §18.22(iii) x -Differences
    13: 18.20 Hahn Class: Explicit Representations
    For comments on the use of the forward-difference operator Δ x , the backward-difference operator x , and the central-difference operator δ x , see §18.2(ii). … In (18.20.1) X and w x are as in Table 18.19.1. …For the Krawtchouk, Meixner, and Charlier polynomials, F ( x ) and κ n are as in Table 18.20.1. …
    18.20.3 w ( x ; a , b , a ¯ , b ¯ ) p n ( x ; a , b , a ¯ , b ¯ ) = 1 n ! δ x n ( w ( x ; a + 1 2 n , b + 1 2 n , a ¯ + 1 2 n , b ¯ + 1 2 n ) ) .
    18.20.4 w ( λ ) ( x ; ϕ ) P n ( λ ) ( x ; ϕ ) = 1 n ! δ x n ( w ( λ + 1 2 n ) ( x ; ϕ ) ) .
    14: 8 Incomplete Gamma and Related
    Functions
    15: 28 Mathieu Functions and Hill’s Equation
    16: 18.39 Applications in the Physical Sciences
    §18.39 Applications in the Physical Sciences
    In what follows the radial and spherical radial eigenfunctions corresponding to (18.39.27) are found in four different notations, with identical eigenvalues, all of which appear in the current and past mathematical and theoretical physics and chemistry literatures, regarding this central problem. … see Bethe and Salpeter (1957, p. 13), Pauling and Wilson (1985, pp. 130, 131); and noting that this differs from the Rodrigues formula of (18.5.5) for the Laguerre OP’s, in the omission of an n ! in the denominator. … Derivations of (18.39.42) appear in Bethe and Salpeter (1957, pp. 12–20), and Pauling and Wilson (1985, Chapter V and Appendix VII), where the derivations are based on (18.39.36), and is also the notation of Piela (2014, §4.7), typifying the common use of the associated Coulomb–Laguerre polynomials in theoretical quantum chemistry. …
    §18.39(iii) Non Classical Weight Functions of Utility in DVR Method in the Physical Sciences
    17: 23 Weierstrass Elliptic and Modular
    Functions
    18: Wolter Groenevelt
     1976 in Leidschendam, the Netherlands) is an Associate Professor at the Delft University of Technology in Delft, The Netherlands. …  in mathematics at the Delft University of Technology in 2004. Groenevelt’s research interests is in special functions and orthogonal polynomials and their relations with representation theory and interacting particle systems. As of September 20, 2022, Groenevelt performed a complete analysis and acted as main consultant for the update of the source citation and proof metadata for every formula in Chapter 18 Orthogonal Polynomials. In July 2023, Groenevelt was named Contributing Developer of the NIST Digital Library of Mathematical Functions.
    19: 18.26 Wilson Class: Continued
    §18.26(iii) Difference Relations
    For comments on the use of the forward-difference operator Δ x , the backward-difference operator x , and the central-difference operator δ x , see §18.2(ii). For each family only the y -difference that lowers n is given. … Koornwinder (2009) rescales and reparametrizes Racah polynomials and Wilson polynomials in such a way that they are continuous in their four parameters, provided that these parameters are nonnegative. Moreover, if one or more of the new parameters becomes zero, then the polynomial descends to a lower family in the Askey scheme.
    20: 36 Integrals with Coalescing Saddles