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21: 20.13 Physical Applications
§20.13 Physical Applications
with κ = i π / 4 . … Thus the classical theta functions are “periodized”, or “anti-periodized”, Gaussians; see Bellman (1961, pp. 18, 19). … In the singular limit τ 0 + , the functions θ j ( z | τ ) , j = 1 , 2 , 3 , 4 , become integral kernels of Feynman path integrals (distribution-valued Green’s functions); see Schulman (1981, pp. 194–195). This allows analytic time propagation of quantum wave-packets in a box, or on a ring, as closed-form solutions of the time-dependent Schrödinger equation.
22: 23.15 Definitions
§23.15 Definitions
In §§23.1523.19, k and k ( ) denote the Jacobi modulus and complementary modulus, respectively, and q = e i π τ ( τ > 0 ) denotes the nome; compare §§20.1 and 22.1. … If, as a function of q , f ( τ ) is analytic at q = 0 , then f ( τ ) is called a modular form. If, in addition, f ( τ ) 0 as q 0 , then f ( τ ) is called a cusp form. …
23: 32.6 Hamiltonian Structure
The Hamiltonian for P III  is …
32.6.18 z p = 2 q p 2 + 2 κ z q p + ( 2 θ 0 + 1 ) p κ ( θ 0 + θ ) z .
32.6.25 ζ q = 2 q 2 p η q 2 θ 0 q + η 0 ζ ,
32.6.26 ζ p = 2 q p 2 + 2 η q p + θ 0 p 1 2 η ( θ 0 + θ 1 ) .
The Hamiltonian for P III  with γ = 0 is …
24: 20.10 Integrals
§20.10 Integrals
§20.10(i) Mellin Transforms with respect to the Lattice Parameter
§20.10(ii) Laplace Transforms with respect to the Lattice Parameter
For corresponding results for argument derivatives of the theta functions see Erdélyi et al. (1954a, pp. 224–225) or Oberhettinger and Badii (1973, p. 193). … For further integrals of theta functions see Erdélyi et al. (1954a, pp. 61–62 and 339), Prudnikov et al. (1990, pp. 356–358), Prudnikov et al. (1992a, §3.41), and Gradshteyn and Ryzhik (2000, pp. 627–628).
25: 21.7 Riemann Surfaces
§21.7(i) Connection of Riemann Theta Functions to Riemann Surfaces
In almost all applications, a Riemann theta function is associated with a compact Riemann surface. … is a Riemann matrix and it is used to define the corresponding Riemann theta function. …
§21.7(ii) Fay’s Trisecant Identity
26: 32.4 Isomonodromy Problems
where θ is an arbitrary constant, is
32.4.10 z u 0 = θ u 0 z v 0 v 1 ,
If w = u 0 / ( v 0 v 1 ) , then …
32.4.15 ( α , β , γ , δ ) = ( 2 θ 0 , 2 ( 1 θ ) , 1 , 1 ) ,
where …
27: 25.19 Tables
  • Abramowitz and Stegun (1964) tabulates: ζ ( n ) , n = 2 , 3 , 4 , , 20D (p. 811); Li 2 ( 1 x ) , x = 0 ( .01 ) 0.5 , 9D (p. 1005); f ( θ ) , θ = 15 ( 1 ) 30 ( 2 ) 90 ( 5 ) 180 , f ( θ ) + θ ln θ , θ = 0 ( 1 ) 15 , 6D (p. 1006). Here f ( θ ) denotes Clausen’s integral, given by the right-hand side of (25.12.9).

  • 28: 14.18 Sums
    In (14.18.1) and (14.18.2), θ 1 , θ 2 , and θ 1 + θ 2 all lie in [ 0 , π ) , and ϕ is real. … In (14.18.3), θ 1 lies in ( 0 , 1 2 π ) , θ 2 and θ 1 + θ 2 both lie in ( 0 , π ) , θ 1 < θ 2 , ϕ is real, and ν 1 , 2 , 3 , . … In these formulas the Legendre functions are as in §14.3(ii) with μ = 0 . The formulas are also valid with the Ferrers functions as in §14.3(i) with μ = 0 . …
    29: 19.23 Integral Representations
    In (19.23.1)–(19.23.3) we assume y > 0 and z > 0 . …
    19.23.3 R D ( 0 , y , z ) = 3 0 π / 2 ( y cos 2 θ + z sin 2 θ ) 3 / 2 sin 2 θ d θ .
    where x , y , and z have positive real parts—except that at most one of them may be 0. In (19.23.8)–(19.23.10) one or more of the variables may be 0 if the integral converges. … With l 1 , l 2 , l 3 denoting any permutation of sin θ cos ϕ , sin θ sin ϕ , cos θ , …
    30: 14.33 Tables
  • Abramowitz and Stegun (1964, Chapter 8) tabulates 𝖯 n ( x ) for n = 0 ( 1 ) 3 , 9 , 10 , x = 0 ( .01 ) 1 , 5–8D; 𝖯 n ( x ) for n = 1 ( 1 ) 4 , 9 , 10 , x = 0 ( .01 ) 1 , 5–7D; 𝖰 n ( x ) and 𝖰 n ( x ) for n = 0 ( 1 ) 3 , 9 , 10 , x = 0 ( .01 ) 1 , 6–8D; P n ( x ) and P n ( x ) for n = 0 ( 1 ) 5 , 9 , 10 , x = 1 ( .2 ) 10 , 6S; Q n ( x ) and Q n ( x ) for n = 0 ( 1 ) 3 , 9 , 10 , x = 1 ( .2 ) 10 , 6S. (Here primes denote derivatives with respect to x .)

  • Zhang and Jin (1996, Chapter 4) tabulates 𝖯 n ( x ) for n = 2 ( 1 ) 5 , 10 , x = 0 ( .1 ) 1 , 7D; 𝖯 n ( cos θ ) for n = 1 ( 1 ) 4 , 10 , θ = 0 ( 5 ) 90 , 8D; 𝖰 n ( x ) for n = 0 ( 1 ) 2 , 10 , x = 0 ( .1 ) 0.9 , 8S; 𝖰 n ( cos θ ) for n = 0 ( 1 ) 3 , 10 , θ = 0 ( 5 ) 90 , 8D; 𝖯 n m ( x ) for m = 1 ( 1 ) 4 , n m = 0 ( 1 ) 2 , n = 10 , x = 0 , 0.5 , 8S; 𝖰 n m ( x ) for m = 1 ( 1 ) 4 , n = 0 ( 1 ) 2 , 10 , 8S; 𝖯 ν m ( cos θ ) for m = 0 ( 1 ) 3 , ν = 0 ( .25 ) 5 , θ = 0 ( 15 ) 90 , 5D; P n ( x ) for n = 2 ( 1 ) 5 , 10 , x = 1 ( 1 ) 10 , 7S; Q n ( x ) for n = 0 ( 1 ) 2 , 10 , x = 2 ( 1 ) 10 , 8S. Corresponding values of the derivative of each function are also included, as are 6D values of the first 5 ν -zeros of 𝖯 ν m ( cos θ ) and of its derivative for m = 0 ( 1 ) 4 , θ = 10 , 30 , 150 .

  • Belousov (1962) tabulates 𝖯 n m ( cos θ ) (normalized) for m = 0 ( 1 ) 36 , n m = 0 ( 1 ) 56 , θ = 0 ( 2.5 ) 90 , 6D.

  • Žurina and Karmazina (1964, 1965) tabulate the conical functions 𝖯 1 2 + i τ ( x ) for τ = 0 ( .01 ) 50 , x = 0.9 ( .1 ) 0.9 , 7S; P 1 2 + i τ ( x ) for τ = 0 ( .01 ) 50 , x = 1.1 ( .1 ) 2 ( .2 ) 5 ( .5 ) 10 ( 10 ) 60 , 7D. Auxiliary tables are included to facilitate computation for larger values of τ when 1 < x < 1 .

  • Žurina and Karmazina (1963) tabulates the conical functions 𝖯 1 2 + i τ 1 ( x ) for τ = 0 ( .01 ) 25 , x = 0.9 ( .1 ) 0.9 , 7S; P 1 2 + i τ 1 ( x ) for τ = 0 ( .01 ) 25 , x = 1.1 ( .1 ) 2 ( .2 ) 5 ( .5 ) 10 ( 10 ) 60 , 7S. Auxiliary tables are included to assist computation for larger values of τ when 1 < x < 1 .