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solutions as trigonometric and hyperbolic functions

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11: 14.20 Conical (or Mehler) Functions
Solutions are known as conical or Mehler functions. … … It is an important companion solution to 𝖯 1 2 + i τ μ ( x ) when τ is large; compare §§14.20(vii), 14.20(viii), and 10.25(iii). …
§14.20(v) Trigonometric Expansion
where the inverse trigonometric functions take their principal values. …
12: 10.45 Functions of Imaginary Order
§10.45 Functions of Imaginary Order
and I ~ ν ( x ) , K ~ ν ( x ) are real and linearly independent solutions of (10.45.1): … In consequence of (10.45.5)–(10.45.7), I ~ ν ( x ) and K ~ ν ( x ) comprise a numerically satisfactory pair of solutions of (10.45.1) when x is large, and either I ~ ν ( x ) and ( 1 / π ) sinh ( π ν ) K ~ ν ( x ) , or I ~ ν ( x ) and K ~ ν ( x ) , comprise a numerically satisfactory pair when x is small, depending whether ν 0 or ν = 0 . … In this reference I ~ ν ( x ) is denoted by ( 1 / π ) sinh ( π ν ) L i ν ( x ) . …
13: 36.11 Leading-Order Asymptotics
§36.11 Leading-Order Asymptotics
36.11.2 Ψ K ( 𝐱 ) = 2 π j = 1 j max ( 𝐱 ) exp ( i ( Φ K ( t j ( 𝐱 ) ; 𝐱 ) + 1 4 π ( 1 ) j + K + 1 ) ) | 2 Φ K ( t j ( 𝐱 ) ; 𝐱 ) t 2 | 1 / 2 ( 1 + o ( 1 ) ) .
36.11.4 Ψ 3 ( x , 0 , 0 ) = 2 π ( 5 | x | 3 ) 1 / 8 { exp ( 2 2 ( x / 5 ) 5 / 4 ) ( cos ( 2 2 ( x / 5 ) 5 / 4 1 8 π ) + o ( 1 ) ) , x + , cos ( 4 ( | x | / 5 ) 5 / 4 1 4 π ) + o ( 1 ) , x .
36.11.6 Ψ 3 ( 0 , 0 , z ) = Γ ( 1 3 ) | z | 1 / 3 3 + { o ( 1 ) , z + , 2 π 5 1 / 4 ( 3 | z | ) 3 / 4 ( cos ( 2 3 ( 3 | z | 5 ) 5 / 2 1 4 π ) + o ( 1 ) ) , z .
36.11.8 Ψ ( H ) ( 0 , 0 , z ) = 2 π z ( 1 i 3 exp ( 1 27 i z 3 ) + o ( 1 ) ) , z ± .
14: 28.10 Integral Equations
§28.10(i) Equations with Elementary Kernels
28.10.2 2 π 0 π / 2 cosh ( 2 h sin z sin t ) ce 2 n ( t , h 2 ) d t = A 0 2 n ( h 2 ) ce 2 n ( 0 , h 2 ) ce 2 n ( 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(ii) Equations with Bessel-Function Kernels
§28.10(iii) Further Equations
15: 10.20 Uniform Asymptotic Expansions for Large Order
§10.20 Uniform Asymptotic Expansions for Large Order
Define ζ = ζ ( z ) to be the solution of the differential equation … In this way there is less usage of many-valued functions. … where τ 0 = 1.19968 is the positive root of the equation τ = coth τ . …
§10.20(iii) Double Asymptotic Properties
16: 32.2 Differential Equations
An equation is said to have the Painlevé property if all its solutions are free from movable branch points; the solutions may have movable poles or movable isolated essential singularities (§1.10(iii)), however. … For arbitrary values of the parameters α , β , γ , and δ , the general solutions of P I P VI  are transcendental, that is, they cannot be expressed in closed-form elementary functions. However, for special values of the parameters, equations P II P VI  have special solutions in terms of elementary functions, or special functions defined elsewhere in the DLMF. … In P V , if w ( z ) = ( coth u ( ζ ) ) 2 with ζ = ln z , then … Let …
17: Bibliography L
  • R. E. Langer (1934) The solutions of the Mathieu equation with a complex variable and at least one parameter large. Trans. Amer. Math. Soc. 36 (3), pp. 637–695.
  • L. Lapointe and L. Vinet (1996) Exact operator solution of the Calogero-Sutherland model. Comm. Math. Phys. 178 (2), pp. 425–452.
  • Y. A. Li and P. J. Olver (2000) Well-posedness and blow-up solutions for an integrable nonlinearly dispersive model wave equation. J. Differential Equations 162 (1), pp. 27–63.
  • P. Linz and T. E. Kropp (1973) A note on the computation of integrals involving products of trigonometric and Bessel functions. Math. Comp. 27 (124), pp. 871–872.
  • J. L. López and N. M. Temme (1999c) Uniform approximations of Bernoulli and Euler polynomials in terms of hyperbolic functions. Stud. Appl. Math. 103 (3), pp. 241–258.
  • 18: 22.19 Physical Applications
    The bounded ( π θ π ) oscillatory solution of (22.19.1) is traditionally written … This formulation gives the bounded and unbounded solutions from the same formula (22.19.3), for k 1 and k 1 , respectively. … Both the dn and cn solutions approach a sech t as a 2 / β from the appropriate directions. … Many nonlinear ordinary and partial differential equations have solutions that may be expressed in terms of Jacobian elliptic functions. … Hyperelliptic functions u ( z ) are solutions of the equation z = 0 u ( f ( x ) ) 1 / 2 d x , where f ( x ) is a polynomial of degree higher than 4. …
    19: 14.3 Definitions and Hypergeometric Representations
    The following are real-valued solutions of (14.2.2) when μ , ν and x ( 1 , 1 ) . … The following are solutions of (14.2.2) when μ , ν and x > 1 . … As standard solutions of (14.2.2) we take the pair P ν μ ( x ) and 𝑸 ν μ ( x ) , where …
    §14.3(iii) Alternative Hypergeometric Representations
    §14.3(iv) Relations to Other Functions
    20: Errata
  • Subsection 20.10(ii)

    In the first sentence of this subsection, the constraint sinh | β | has been replaced with | β | + | β | .

  • Equation (10.22.72)
    10.22.72 0 J μ ( a t ) J ν ( b t ) J ν ( c t ) t 1 μ d t = ( b c ) μ 1 sin ( ( μ ν ) π ) ( sinh χ ) μ 1 2 ( 1 2 π 3 ) 1 2 a μ e ( μ 1 2 ) i π Q ν 1 2 1 2 μ ( cosh χ ) , μ > 1 2 , ν > 1 , a > b + c , cosh χ = ( a 2 b 2 c 2 ) / ( 2 b c )

    Originally, the factor on the right-hand side was written as ( b c ) μ 1 cos ( ν π ) ( sinh χ ) μ 1 2 ( 1 2 π 3 ) 1 2 a μ , which was taken directly from Watson (1944, p. 412, (13.46.5)), who uses a different normalization for the associated Legendre function of the second kind Q ν μ . Watson’s Q ν μ equals sin ( ( ν + μ ) π ) sin ( ν π ) e μ π i Q ν μ in the DLMF.

    Reported by Arun Ravishankar on 2018-10-22

  • Figures 36.3.9, 36.3.10, 36.3.11, 36.3.12

    Scales were corrected in all figures. The interval 8.4 x y 2 8.4 was replaced by 12.0 x y 2 12.0 and 12.7 x + y 2 4.2 replaced by 18.0 x + y 2 6.0 . All plots and interactive visualizations were regenerated to improve image quality.

    See accompanying text See accompanying text
    (a) Density plot. (b) 3D plot.

    Figure 36.3.9: Modulus of hyperbolic umbilic canonical integral function | Ψ ( H ) ( x , y , 0 ) | .

    See accompanying text See accompanying text
    (a) Density plot. (b) 3D plot.

    Figure 36.3.10: Modulus of hyperbolic umbilic canonical integral function | Ψ ( H ) ( x , y , 1 ) | .

    See accompanying text See accompanying text
    (a) Density plot. (b) 3D plot.

    Figure 36.3.11: Modulus of hyperbolic umbilic canonical integral function | Ψ ( H ) ( x , y , 2 ) | .

    See accompanying text See accompanying text
    (a) Density plot. (b) 3D plot.

    Figure 36.3.12: Modulus of hyperbolic umbilic canonical integral function | Ψ ( H ) ( x , y , 3 ) | .

    Reported 2016-09-12 by Dan Piponi.

  • Section 4.43

    The first paragraph has been rewritten to correct reported errors. The new version is reproduced here.

    Let p ( 0 ) and q be real constants and

    4.43.1
    A = ( 4 3 p ) 1 / 2 ,
    B = ( 4 3 p ) 1 / 2 .

    The roots of

    4.43.2 z 3 + p z + q = 0

    are:

    1. (a)

      A sin a , A sin ( a + 2 3 π ) , and A sin ( a + 4 3 π ) , with sin ( 3 a ) = 4 q / A 3 , when 4 p 3 + 27 q 2 0 .

    2. (b)

      A cosh a , A cosh ( a + 2 3 π i ) , and A cosh ( a + 4 3 π i ) , with cosh ( 3 a ) = 4 q / A 3 , when p < 0 , q < 0 , and 4 p 3 + 27 q 2 > 0 .

    3. (c)

      B sinh a , B sinh ( a + 2 3 π i ) , and B sinh ( a + 4 3 π i ) , with sinh ( 3 a ) = 4 q / B 3 , when p > 0 .

    Note that in Case (a) all the roots are real, whereas in Cases (b) and (c) there is one real root and a conjugate pair of complex roots. See also §1.11(iii).

    Reported 2014-10-31 by Masataka Urago.

  • Table 22.5.4

    Originally the limiting form for sc ( z , k ) in the last line of this table was incorrect ( cosh z , instead of sinh z ).

    sn ( z , k ) tanh z cd ( z , k ) 1 dc ( z , k ) 1 ns ( z , k ) coth z
    cn ( z , k ) sech z sd ( z , k ) sinh z nc ( z , k ) cosh z ds ( z , k ) csch z
    dn ( z , k ) sech z nd ( z , k ) cosh z sc ( z , k ) sinh z cs ( z , k ) csch z

    Reported 2010-11-23.