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1: 5.17 Barnes’ G -Function (Double Gamma Function)
5.17.5 Ln G ( z + 1 ) 1 4 z 2 + z Ln Γ ( z + 1 ) ( 1 2 z ( z + 1 ) + 1 12 ) ln z ln A + k = 1 B 2 k + 2 2 k ( 2 k + 1 ) ( 2 k + 2 ) z 2 k .
Here B 2 k + 2 is the Bernoulli number (§24.2(i)), and A is Glaisher’s constant, given by
5.17.6 A = e C = 1.28242 71291 00622 63687 ,
5.17.7 C = lim n ( k = 1 n k ln k ( 1 2 n 2 + 1 2 n + 1 12 ) ln n + 1 4 n 2 ) = γ + ln ( 2 π ) 12 ζ ( 2 ) 2 π 2 = 1 12 ζ ( 1 ) ,
For Glaisher’s constant see also Greene and Knuth (1982, p. 100) and §2.10(i).
2: 22.1 Special Notation
The notation sn ( z , k ) , cn ( z , k ) , dn ( z , k ) is due to Gudermann (1838), following Jacobi (1827); that for the subsidiary functions is due to Glaisher (1882). Other notations for sn ( z , k ) are sn ( z | m ) and sn ( z , m ) with m = k 2 ; see Abramowitz and Stegun (1964) and Walker (1996). …
3: 27.21 Tables
Glaisher (1940) contains four tables: Table I tabulates, for all n 10 4 : (a) the canonical factorization of n into powers of primes; (b) the Euler totient ϕ ( n ) ; (c) the divisor function d ( n ) ; (d) the sum σ ( n ) of these divisors. …7 of Abramowitz and Stegun (1964) also lists the factorizations in Glaisher’s Table I(a); Table 24. …
4: 2.10 Sums and Sequences
Formula (2.10.2) is useful for evaluating the constant term in expansions obtained from (2.10.1). …where γ is Euler’s constant5.2(ii)) and ζ is the derivative of the Riemann zeta function (§25.2(i)). e C is sometimes called Glaisher’s constant. … where α ( 1 ) is a real constant, and … for any real constant α and the set of all positive integers j , we derive …
5: 8.26 Tables
  • Khamis (1965) tabulates P ( a , x ) for a = 0.05 ( .05 ) 10 ( .1 ) 20 ( .25 ) 70 , 0.0001 x 250 to 10D.

  • Zhang and Jin (1996, Table 3.8) tabulates γ ( a , x ) for a = 0.5 , 1 , 3 , 5 , 10 , 25 , 50 , 100 , x = 0 ( .1 ) 1 ( 1 ) 3 , 5 ( 5 ) 30 , 50 , 100 to 8D or 8S.

  • Abramowitz and Stegun (1964, pp. 245–248) tabulates E n ( x ) for n = 2 , 3 , 4 , 10 , 20 , x = 0 ( .01 ) 2 to 7D; also ( x + n ) e x E n ( x ) for n = 2 , 3 , 4 , 10 , 20 , x 1 = 0 ( .01 ) 0.1 ( .05 ) 0.5 to 6S.

  • Pagurova (1961) tabulates E n ( x ) for n = 0 ( 1 ) 20 , x = 0 ( .01 ) 2 ( .1 ) 10 to 4-9S; e x E n ( x ) for n = 2 ( 1 ) 10 , x = 10 ( .1 ) 20 to 7D; e x E p ( x ) for p = 0 ( .1 ) 1 , x = 0.01 ( .01 ) 7 ( .05 ) 12 ( .1 ) 20 to 7S or 7D.

  • Zhang and Jin (1996, Table 19.1) tabulates E n ( x ) for n = 1 , 2 , 3 , 5 , 10 , 15 , 20 , x = 0 ( .1 ) 1 , 1.5 , 2 , 3 , 5 , 10 , 20 , 30 , 50 , 100 to 7D or 8S.

  • 6: 20 Theta Functions
    Chapter 20 Theta Functions
    7: Bibliography G
  • W. Gautschi (1994) Algorithm 726: ORTHPOL — a package of routines for generating orthogonal polynomials and Gauss-type quadrature rules. ACM Trans. Math. Software 20 (1), pp. 21–62.
  • A. Gil, J. Segura, and N. M. Temme (2014) Algorithm 939: computation of the Marcum Q-function. ACM Trans. Math. Softw. 40 (3), pp. 20:1–20:21.
  • J. W. L. Glaisher (1940) Number-Divisor Tables. British Association Mathematical Tables, Vol. VIII, Cambridge University Press, Cambridge, England.
  • Ya. I. Granovskiĭ, I. M. Lutzenko, and A. S. Zhedanov (1992) Mutual integrability, quadratic algebras, and dynamical symmetry. Ann. Phys. 217 (1), pp. 1–20.
  • 8: 22.4 Periods, Poles, and Zeros
    §22.4(ii) Graphical Interpretation via Glaisher’s Notation
    9: 20.7 Identities
    Also, in further development along the lines of the notations of Neville (§20.1) and of Glaisher22.2), the identities (20.7.6)–(20.7.9) have been recast in a more symmetric manner with respect to suffices 2 , 3 , 4 . … See Lawden (1989, pp. 19–20). …
    20.7.34 θ 1 ( z , q 2 ) θ 3 ( z , q 2 ) θ 1 ( z , i q ) = θ 2 ( z , q 2 ) θ 4 ( z , q 2 ) θ 2 ( z , i q ) = i 1 / 4 θ 2 ( 0 , q 2 ) θ 4 ( 0 , q 2 ) 2 .
    10: 5.22 Tables
    Abramowitz and Stegun (1964, Chapter 6) tabulates Γ ( x ) , ln Γ ( x ) , ψ ( x ) , and ψ ( x ) for x = 1 ( .005 ) 2 to 10D; ψ ′′ ( x ) and ψ ( 3 ) ( x ) for x = 1 ( .01 ) 2 to 10D; Γ ( n ) , 1 / Γ ( n ) , Γ ( n + 1 2 ) , ψ ( n ) , log 10 Γ ( n ) , log 10 Γ ( n + 1 3 ) , log 10 Γ ( n + 1 2 ) , and log 10 Γ ( n + 2 3 ) for n = 1 ( 1 ) 101 to 8–11S; Γ ( n + 1 ) for n = 100 ( 100 ) 1000 to 20S. Zhang and Jin (1996, pp. 67–69 and 72) tabulates Γ ( x ) , 1 / Γ ( x ) , Γ ( x ) , ln Γ ( x ) , ψ ( x ) , ψ ( x ) , ψ ( x ) , and ψ ( x ) for x = 0 ( .1 ) 5 to 8D or 8S; Γ ( n + 1 ) for n = 0 ( 1 ) 100 ( 10 ) 250 ( 50 ) 500 ( 100 ) 3000 to 51S. … Abramov (1960) tabulates ln Γ ( x + i y ) for x = 1 ( .01 ) 2 , y = 0 ( .01 ) 4 to 6D. Abramowitz and Stegun (1964, Chapter 6) tabulates ln Γ ( x + i y ) for x = 1 ( .1 ) 2 , y = 0 ( .1 ) 10 to 12D. …Zhang and Jin (1996, pp. 70, 71, and 73) tabulates the real and imaginary parts of Γ ( x + i y ) , ln Γ ( x + i y ) , and ψ ( x + i y ) for x = 0.5 , 1 , 5 , 10 , y = 0 ( .5 ) 10 to 8S.