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11: 3.5 Quadrature
When f C , the Romberg method affords a means of obtaining high accuracy in many cases with a relatively simple adaptive algorithm. … (With the 20-point Gauss–Laguerre formula (§3.5(v)) the same precision can be achieved with 15 function evaluations.) …
12: Bibliography C
  • J. B. Campbell (1984) Determination of ν -zeros of Hankel functions. Comput. Phys. Comm. 32 (3), pp. 333–339.
  • S. Chandrasekhar (1984) The Mathematical Theory of Black Holes. In General Relativity and Gravitation (Padova, 1983), pp. 5–26.
  • R. Chattamvelli and R. Shanmugam (1997) Algorithm AS 310. Computing the non-central beta distribution function. Appl. Statist. 46 (1), pp. 146–156.
  • J. A. Christley and I. J. Thompson (1994) CRCWFN: Coupled real Coulomb wavefunctions. Comput. Phys. Comm. 79 (1), pp. 143–155.
  • L. D. Cloutman (1989) Numerical evaluation of the Fermi-Dirac integrals. The Astrophysical Journal Supplement Series 71, pp. 677–699.
  • 13: Bibliography L
  • S. Lai and Y. Chiu (1992) Exact computation of the 9 - j symbols. Comput. Phys. Comm. 70 (3), pp. 544–556.
  • P. W. Lawrence, R. M. Corless, and D. J. Jeffrey (2012) Algorithm 917: complex double-precision evaluation of the Wright ω function. ACM Trans. Math. Software 38 (3), pp. Art. 20, 17.
  • E. W. Leaver (1986) Solutions to a generalized spheroidal wave equation: Teukolsky’s equations in general relativity, and the two-center problem in molecular quantum mechanics. J. Math. Phys. 27 (5), pp. 1238–1265.
  • M. Yu. Loenko (2001) Evaluating elementary functions with guaranteed precision. Programming and Computer Software 27 (2), pp. 101–110.
  • H. A. Lorentz, A. Einstein, H. Minkowski, and H. Weyl (1923) The Principle of Relativity: A Collection of Original Memoirs on the Special and General Theory of Relativity. Methuen and Co., Ltd., London.
  • 14: 3.6 Linear Difference Equations
    More precisely, assume that f 0 0 , g n 0 for all sufficiently large n , and as n Suppose again that f 0 0 , w 0 is given, and we wish to calculate w 1 , w 2 , , w M to a prescribed relative accuracy ϵ for a given value of M . …
    3.6.9 | e N p N p N + 1 | ϵ min 1 n M | e n p n p n + 1 | .