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21: 9.17 Methods of Computation
However, in the case of Ai ( z ) and Bi ( z ) this accuracy can be increased considerably by use of the exponentially-improved forms of expansion supplied in §9.7(v). … But when | ph z | < 1 3 π the integration has to be towards the origin, with starting values of Ai ( z ) and Ai ( z ) computed from their asymptotic expansions. … For details, including the application of a generalized form of Gaussian quadrature, see Gordon (1969, Appendix A) and Schulten et al. (1979). Gil et al. (2002c) describes two methods for the computation of Ai ( z ) and Ai ( z ) for z . …The methods for Ai ( z ) are similar. …
22: 28.10 Integral Equations
28.10.3 2 π 0 π / 2 sin ( 2 h cos z cos t ) ce 2 n + 1 ( t , h 2 ) d t = h A 1 2 n + 1 ( h 2 ) ce 2 n + 1 ( 1 2 π , h 2 ) ce 2 n + 1 ( z , h 2 ) ,
28.10.5 2 π 0 π / 2 sinh ( 2 h sin z sin t ) se 2 n + 1 ( t , h 2 ) d t = h B 1 2 n + 1 ( h 2 ) se 2 n + 1 ( 0 , h 2 ) se 2 n + 1 ( z , h 2 ) ,
28.10.7 2 π 0 π / 2 sin z sin t sin ( 2 h cos z cos t ) se 2 n + 2 ( t , h 2 ) d t = h B 2 2 n + 2 ( h 2 ) 2 se 2 n + 2 ( 1 2 π , h 2 ) se 2 n + 2 ( z , h 2 ) ,
28.10.8 2 π 0 π / 2 cos z cos t sinh ( 2 h sin z sin t ) se 2 n + 2 ( t , h 2 ) d t = h B 2 2 n + 2 ( h 2 ) 2 se 2 n + 2 ( 0 , h 2 ) se 2 n + 2 ( z , h 2 ) .
23: 3.4 Differentiation
and follows from the differentiated form of (3.3.4). …
3.4.5 h f t = f 0 + f 1 + h R 1 , t , 0 < t < 1 .
3.4.7 h f t = k = 1 2 B k 3 f k + h R 3 , t , 1 < t < 2 ,
3.4.11 h f t = k = 2 3 B k 5 f k + h R 5 , t , 2 < t < 3 ,
3.4.15 h f t = k = 3 4 B k 7 f k + h R 7 , t , 3 < t < 4 ,
24: 22.15 Inverse Functions
22.15.3 dn ( ζ , k ) = x , k x 1 ,
§22.15(ii) Representations as Elliptic Integrals
The integrals (22.15.12)–(22.15.14) can be regarded as normal forms for representing the inverse functions. …can be transformed into normal form by elementary change of variables. …
25: 9.2 Differential Equation
9.2.6 Bi ( 0 ) = 3 1 / 6 Γ ( 1 3 ) = 0.44828 83573 .
26: 9.6 Relations to Other Functions
9.6.12 J ± 2 / 3 ( ζ ) = 1 2 ( 3 / z ) ( ± 3 Ai ( z ) + Bi ( z ) ) ,
9.6.14 I ± 2 / 3 ( ζ ) = 1 2 ( 3 / z ) ( ± 3 Ai ( z ) + Bi ( z ) ) ,
9.6.16 K ± 2 / 3 ( ζ ) = π ( 3 / z ) Ai ( z ) ,
9.6.17 H 1 / 3 ( 1 ) ( ζ ) = e π i / 3 H 1 / 3 ( 1 ) ( ζ ) = e π i / 6 3 / z ( Ai ( z ) i Bi ( z ) ) ,
9.6.18 H 2 / 3 ( 1 ) ( ζ ) = e 2 π i / 3 H 2 / 3 ( 1 ) ( ζ ) = e π i / 6 ( 3 / z ) ( Ai ( z ) i Bi ( z ) ) ,
27: 3.7 Ordinary Differential Equations
By repeated differentiation of (3.7.1) all derivatives of w ( z ) can be expressed in terms of w ( z ) and w ( z ) as follows. … The remaining two equations are supplied by boundary conditions of the formIf q ( x ) is C on the closure of ( a , b ) , then the discretized form (3.7.13) of the differential equation can be used. … For w = f ( z , w ) the standard fourth-order rule reads … For w ′′ = f ( z , w , w ) the standard fourth-order rule reads …
28: 3.3 Interpolation
Here the prime signifies that the factor for j = k is to be omitted, δ k , j is the Kronecker symbol, and ω n + 1 ( z ) is the nodal polynomial …The final expression in (3.3.1) is the Barycentric form of the Lagrange interpolation formula. … … The ( n + 1 ) -point formula (3.3.4) can be written in the formFor example, for k + 1 coincident points the limiting form is given by [ z 0 , z 0 , , z 0 ] f = f ( k ) ( z 0 ) / k ! . …
29: 22.5 Special Values
Table 22.5.1 gives the value of each of the 12 Jacobian elliptic functions, together with its z -derivative (or at a pole, the residue), for values of z that are integer multiples of K , i K . … For example, sn ( 1 2 K , k ) = ( 1 + k ) 1 / 2 . …
§22.5(ii) Limiting Values of k
Expansions for K , K as k 0 or 1 are given in §§19.5, 19.12. …
30: 25.11 Hurwitz Zeta Function
25.11.15 ζ ( s , k a ) = k s n = 0 k 1 ζ ( s , a + n k ) , s 1 , k = 1 , 2 , 3 , .
In (25.11.18)–(25.11.24) primes on ζ denote derivatives with respect to s . …
25.11.34 n 0 a ζ ( 1 n , x ) d x = ζ ( n , a ) ζ ( n ) + B n + 1 B n + 1 ( a ) n ( n + 1 ) , n = 1 , 2 , , a > 0 .
For the more general case ζ ( m , a ) , m = 1 , 2 , , see Elizalde (1986). For an exponentially-improved form of (25.11.43) see Paris (2005b).