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21: 13.7 Asymptotic Expansions for Large Argument
13.7.2 𝐌 ( a , b , z ) e z z a b Γ ( a ) s = 0 ( 1 a ) s ( b a ) s s ! z s + e ± π i a z a Γ ( b a ) s = 0 ( a ) s ( a b + 1 ) s s ! ( z ) s , 1 2 π + δ ± ph z 3 2 π δ ,
See accompanying text
Figure 13.7.1: Regions R 1 , R 2 , R ¯ 2 , R 3 , and R ¯ 3 are the closures of the indicated unshaded regions bounded by the straight lines and circular arcs centered at the origin, with r = | b 2 a | . Magnify
22: 28.33 Physical Applications
Hence from §28.17 the corresponding Mathieu equation is stable or unstable according as ( q , a ) is in the intersection of with the colored or the uncolored open regions depicted in Figure 28.17.1. …
23: 5.11 Asymptotic Expansions
5.11.1 Ln Γ ( z ) ( z 1 2 ) ln z z + 1 2 ln ( 2 π ) + k = 1 B 2 k 2 k ( 2 k 1 ) z 2 k 1
5.11.8 Ln Γ ( z + h ) ( z + h 1 2 ) ln z z + 1 2 ln ( 2 π ) + k = 2 ( 1 ) k B k ( h ) k ( k 1 ) z k 1 ,
24: 3.5 Quadrature
In more advanced methods points are sampled from a probability distribution, so that they are concentrated in regions that make the largest contribution to the integral. …
25: 19.33 Triaxial Ellipsoids
If a conducting ellipsoid with semiaxes a , b , c bears an electric charge Q , then the equipotential surfaces in the exterior region are confocal ellipsoids: …
26: 28.8 Asymptotic Expansions for Large q
The approximations apply when the parameters a and q are real and large, and are uniform with respect to various regions in the z -plane. …
27: 9.17 Methods of Computation
A comprehensive and powerful approach is to integrate the defining differential equation (9.2.1) by direct numerical methods. … The former reference includes a parallelized version of the method. In the case of the Scorer functions, integration of the differential equation (9.12.1) is more difficult than (9.2.1), because in some regions stable directions of integration do not exist. … For details, including the application of a generalized form of Gaussian quadrature, see Gordon (1969, Appendix A) and Schulten et al. (1979). … For quadrature methods for Scorer functions see Gil et al. (2001), Lee (1980), and Gordon (1970, Appendix A); but see also Gautschi (1983). …
28: 33.22 Particle Scattering and Atomic and Molecular Spectra
For Z 1 Z 2 = 1 and m = m e , the electron mass, the scaling factors in (33.22.5) reduce to the Bohr radius, a 0 = / ( m e c α ) , and to a multiple of the Rydberg constant, … The relativistic motion of spinless particles in a Coulomb field, as encountered in pionic atoms and pion-nucleon scattering (Backenstoss (1970)) is described by a Klein–Gordon equation equivalent to (33.2.1); see Barnett (1981a). The motion of a relativistic electron in a Coulomb field, which arises in the theory of the electronic structure of heavy elements (Johnson (2007)), is described by a Dirac equation. … The Coulomb solutions of the Schrödinger and Klein–Gordon equations are almost always used in the external region, outside the range of any non-Coulomb forces or couplings. For scattering problems, the interior solution is then matched to a linear combination of a pair of Coulomb functions, F ( η , ρ ) and G ( η , ρ ) , or f ( ϵ , ; r ) and h ( ϵ , ; r ) , to determine the scattering S -matrix and also the correct normalization of the interior wave solutions; see Bloch et al. (1951). …
29: Bibliography G
  • D. Gottlieb and S. A. Orszag (1977) Numerical Analysis of Spectral Methods: Theory and Applications. Society for Industrial and Applied Mathematics, Philadelphia, PA.
  • 30: 18.24 Hahn Class: Asymptotic Approximations
    When the parameters α and β are fixed and the ratio n / N = c is a constant in the interval (0,1), uniform asymptotic formulas (as n ) of the Hahn polynomials Q n ( z ; α , β , N ) can be found in Lin and Wong (2013) for z in three overlapping regions, which together cover the entire complex plane. …