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21: 13.29 Methods of Computation
However, this accuracy can be increased considerably by use of the exponentially-improved forms of expansion supplied by the combination of (13.7.10) and (13.7.11), or by use of the hyperasymptotic expansions given in Olde Daalhuis and Olver (1995a). … For M ( a , b , z ) and M κ , μ ( z ) this means that in the sector | ph z | π we may integrate along outward rays from the origin with initial values obtained from (13.2.2) and (13.14.2). For U ( a , b , z ) and W κ , μ ( z ) we may integrate along outward rays from the origin in the sectors 1 2 π < | ph z | < 3 2 π , with initial values obtained from connection formulas in §13.2(vii), §13.14(vii). … The recurrence relations in §§13.3(i) and 13.15(i) can be used to compute the confluent hypergeometric functions in an efficient way. … In Colman et al. (2011) an algorithm is described that uses expansions in continued fractions for high-precision computation of M ( n , b , x ) , when b and x are real and n is a positive integer. …
22: 33.2 Definitions and Basic Properties
The function F ( η , ρ ) is recessive (§2.7(iii)) at ρ = 0 , and is defined by …where M κ , μ ( z ) and M ( a , b , z ) are defined in §§13.14(i) and 13.2(i), and … The normalizing constant C ( η ) is always positive, and has the alternative formThe functions H ± ( η , ρ ) are defined by …where W κ , μ ( z ) , U ( a , b , z ) are defined in §§13.14(i) and 13.2(i), …
23: 18.34 Bessel Polynomials
§18.34(i) Definitions and Recurrence Relation
For the confluent hypergeometric function F 1 1 and the generalized hypergeometric function F 0 2 , the Laguerre polynomial L n ( α ) and the Whittaker function W κ , μ see §16.2(ii), §16.2(iv), (18.5.12), and (13.14.3), respectively.
18.34.1 y n ( x ; a ) = F 0 2 ( n , n + a 1 ; x 2 ) = ( n + a 1 ) n ( x 2 ) n F 1 1 ( n 2 n a + 2 ; 2 x ) = n ! ( 1 2 x ) n L n ( 1 a 2 n ) ( 2 x 1 ) = ( 1 2 x ) 1 1 2 a e 1 / x W 1 1 2 a , 1 2 ( a 1 ) + n ( 2 x 1 ) .
18.34.7_1 ϕ n ( x ; λ ) = e λ e x ( 2 λ e x ) λ 1 2 y n ( λ 1 e x ; 2 2 λ ) / n ! = ( 1 ) n e λ e x ( 2 λ e x ) λ n 1 2 L n ( 2 λ 2 n 1 ) ( 2 λ e x ) = ( 2 λ ) 1 2 e x / 2 W λ , n + 1 2 λ ( 2 λ e x ) / n ! , n = 0 , 1 , , N = λ 3 2 , λ > 1 2 ,
18.34.8 lim α P n ( α , a α 2 ) ( 1 + α x ) P n ( α , a α 2 ) ( 1 ) = y n ( x ; a ) .
24: 18.17 Integrals
18.17.16 1 1 ( 1 x ) α ( 1 + x ) β P n ( α , β ) ( x ) e i x y d x = ( i y ) n e i y n ! 2 n + α + β + 1 B ( n + α + 1 , n + β + 1 ) F 1 1 ( n + α + 1 ; 2 n + α + β + 2 ; 2 i y ) .
For the beta function B ( a , b ) see §5.12, and for the confluent hypergeometric function F 1 1 see (16.2.1) and Chapter 13. …
18.17.33 1 1 e ( x + 1 ) z P n ( α , β ) ( x ) ( 1 x ) α ( 1 + x ) β d x = ( 1 ) n 2 α + β + n + 1 Γ ( α + n + 1 ) Γ ( β + n + 1 ) Γ ( α + β + 2 n + 2 ) n ! z n F 1 1 ( β + n + 1 α + β + 2 n + 2 ; 2 z ) , z .
For the confluent hypergeometric function F 1 1 see (16.2.1) and Chapter 13. … Formulas (18.17.45) and (18.17.49) are integrated forms of the linearization formulas (18.18.22) and (18.18.23), respectively. …
25: 33.23 Methods of Computation
§33.23(i) Methods for the Confluent Hypergeometric Functions
Noble (2004) obtains double-precision accuracy for W η , μ ( 2 ρ ) for a wide range of parameters using a combination of recurrence techniques, power-series expansions, and numerical quadrature; compare (33.2.7). …
26: 2.11 Remainder Terms; Stokes Phenomenon
That the change in their forms is discontinuous, even though the function being approximated is analytic, is an example of the Stokes phenomenon. … In the transition through θ = π , erfc ( 1 2 ρ c ( θ ) ) changes very rapidly, but smoothly, from one form to the other; compare the graph of its modulus in Figure 2.11.1 in the case ρ = 100 . …
2.11.29 W κ , μ ( z ) n = 0 a n ,
2.11.31 W 2.3 , 0.5 ( 1.0 ) = 0.83299 50268 27526
Their extrapolation is based on assumed forms of remainder terms that may not always be appropriate for asymptotic expansions. …
27: 3.10 Continued Fractions
A continued fraction of the formA continued fraction of the formFor special functions see §5.10 (gamma function), §7.9 (error function), §8.9 (incomplete gamma functions), §8.17(v) (incomplete beta function), §8.19(vii) (generalized exponential integral), §§10.10 and 10.33 (quotients of Bessel functions), §13.6 (quotients of confluent hypergeometric functions), §13.19 (quotients of Whittaker functions), and §15.7 (quotients of hypergeometric functions). … can be written in the form
28: Bibliography L
  • G. Labahn and M. Mutrie (1997) Reduction of Elliptic Integrals to Legendre Normal Form. Technical report Technical Report 97-21, Department of Computer Science, University of Waterloo, Waterloo, Ontario.
  • W. Lay, K. Bay, and S. Yu. Slavyanov (1998) Asymptotic and numeric study of eigenvalues of the double confluent Heun equation. J. Phys. A 31 (42), pp. 8521–8531.
  • J. L. López and E. Pérez Sinusía (2014) New series expansions for the confluent hypergeometric function M ( a , b , z ) . Appl. Math. Comput. 235, pp. 26–31.
  • Y. L. Luke (1977a) Algorithms for rational approximations for a confluent hypergeometric function. Utilitas Math. 11, pp. 123–151.
  • J. N. Lyness (1971) Adjusted forms of the Fourier coefficient asymptotic expansion and applications in numerical quadrature. Math. Comp. 25 (113), pp. 87–104.
  • 29: 33.14 Definitions and Basic Properties
    §33.14(ii) Regular Solution f ( ϵ , ; r )
    where M κ , μ ( z ) and M ( a , b , z ) are defined in §§13.14(i) and 13.2(i), and … For nonzero values of ϵ and r the function h ( ϵ , ; r ) is defined by
    33.14.7 h ( ϵ , ; r ) = Γ ( + 1 κ ) π κ ( W κ , + 1 2 ( 2 r / κ ) + ( 1 ) S ( ϵ , r ) Γ ( + 1 + κ ) 2 ( 2 + 1 ) ! M κ , + 1 2 ( 2 r / κ ) ) ,
    Note that the functions ϕ n , , n = , + 1 , , do not form a complete orthonormal system. …
    30: 28.8 Asymptotic Expansions for Large q
    28.8.6 C ^ m ( π h 2 ( m ! ) 2 ) 1 / 4 ( 1 + 2 m + 1 8 h + m 4 + 2 m 3 + 263 m 2 + 262 m + 108 2048 h 2 + ) 1 / 2 ,
    28.8.7 S ^ m ( π h 2 ( m ! ) 2 ) 1 / 4 ( 1 2 m + 1 8 h + m 4 + 2 m 3 121 m 2 122 m 84 2048 h 2 + ) 1 / 2 .
    28.8.9 W m ± ( x ) = e ± 2 h sin x ( cos x ) m + 1 { ( cos ( 1 2 x + 1 4 π ) ) 2 m + 1 , ( sin ( 1 2 x + 1 4 π ) ) 2 m + 1 ,
    28.8.11 P m ( x ) 1 + s 2 3 h cos 2 x + 1 h 2 ( s 4 + 86 s 2 + 105 2 11 cos 4 x s 4 + 22 s 2 + 57 2 11 cos 2 x ) + ,
    The approximations are expressed in terms of Whittaker functions W κ , μ ( z ) and M κ , μ ( z ) with μ = 1 4 ; compare §2.8(vi). …