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21: 18.34 Bessel Polynomials
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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 ) .
β–Ί
18.34.7_1 Ο• n ⁒ ( x ; Ξ» ) = e Ξ» ⁒ e x ⁒ ( 2 ⁒ Ξ» ⁒ e x ) Ξ» 1 2 ⁒ y n ⁑ ( Ξ» 1 ⁒ e x ; 2 2 ⁒ Ξ» ) / n ! = ( 1 ) n ⁒ e Ξ» ⁒ e x ⁒ ( 2 ⁒ Ξ» ⁒ e x ) Ξ» n 1 2 ⁒ L n ( 2 ⁒ Ξ» 2 ⁒ n 1 ) ⁑ ( 2 ⁒ Ξ» ⁒ e x ) = ( 2 ⁒ Ξ» ) 1 2 ⁒ e x / 2 ⁒ W Ξ» , n + 1 2 Ξ» ⁑ ( 2 ⁒ Ξ» ⁒ e x ) / n ! , n = 0 , 1 , , N = Ξ» 3 2 , Ξ» > 1 2 ,
22: 23.21 Physical Applications
β–ΊSee, for example, Lawden (1989, Chapter 7) and Whittaker (1964, Chapters 4–6). β–Ί
§23.21(ii) Nonlinear Evolution Equations
β–ΊAirault et al. (1977) applies the function to an integrable classical many-body problem, and relates the solutions to nonlinear partial differential equations. For applications to soliton solutions of the Korteweg–de Vries (KdV) equation see McKean and Moll (1999, p. 91), Deconinck and Segur (2000), and Walker (1996, §8.1). …
23: 28.8 Asymptotic Expansions for Large q
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28.8.5 V m ⁑ ( ΞΎ ) 1 2 4 ⁒ h ⁒ ( D m + 2 ⁑ ( ΞΎ ) m ⁒ ( m 1 ) ⁒ D m 2 ⁑ ( ΞΎ ) ) + 1 2 10 ⁒ h 2 ⁒ ( D m + 6 ⁑ ( ΞΎ ) + ( m 2 25 ⁒ m 36 ) ⁒ D m + 2 ⁑ ( ΞΎ ) m ⁒ ( m 1 ) ⁒ ( m 2 + 27 ⁒ m 10 ) ⁒ D m 2 ⁑ ( ΞΎ ) 6 ! ⁒ ( m 6 ) ⁒ D m 6 ⁑ ( ΞΎ ) ) + β‹― ,
24: 33.14 Definitions and Basic Properties
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33.14.14 Ο• n , β„“ ⁑ ( r ) = ( 1 ) β„“ + 1 + n ⁒ ( 2 / n 3 ) 1 / 2 ⁒ s ⁑ ( 1 / n 2 , β„“ ; r ) = ( 1 ) β„“ + 1 + n n β„“ + 2 ⁒ ( ( n β„“ 1 ) ! ( n + β„“ ) ! ) 1 / 2 ⁒ ( 2 ⁒ r ) β„“ + 1 ⁒ e r / n ⁒ L n β„“ 1 ( 2 ⁒ β„“ + 1 ) ⁑ ( 2 ⁒ r / n )
25: 33.22 Particle Scattering and Atomic and Molecular Spectra
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§33.22(i) Schrödinger Equation
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§33.22(iv) Klein–Gordon and Dirac Equations
β–ΊFor bound-state problems only the exponentially decaying solution is required, usually taken to be the Whittaker function W Ξ· , β„“ + 1 2 ⁑ ( 2 ⁒ ρ ) . … β–Ί
§33.22(vi) Solutions Inside the Turning Point
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  • Solution of relativistic Coulomb equations. See for example Cooper et al. (1979) and Barnett (1981b).

  • 26: 28.1 Special Notation
    β–Ί β–Ίβ–Ίβ–Ί
    m , n integers.
    a , q , h real or complex parameters of Mathieu’s equation with q = h 2 .
    β–Ί β–Ίβ–Ί
    ce ν ⁑ ( z , q ) , se ν ⁑ ( z , q ) , fe n ⁑ ( z , q ) , ge n ⁑ ( z , q ) , me ν ⁑ ( z , q ) ,
    β–ΊThe eigenvalues of Mathieu’s equation are denoted by … β–Ί
    λ ν ⁑ ( q ) .
    β–Ί
    Table 28.1.1: Notations for parameters in Mathieu’s equation.
    β–Ί β–Ίβ–Ί
    Reference a q
    β–Ί
    27: Bibliography N
    β–Ί
  • A. Nakamura (1996) Toda equation and its solutions in special functions. J. Phys. Soc. Japan 65 (6), pp. 1589–1597.
  • β–Ί
  • J. Negro, L. M. Nieto, and O. Rosas-Ortiz (2000) Confluent hypergeometric equations and related solvable potentials in quantum mechanics. J. Math. Phys. 41 (12), pp. 7964–7996.
  • β–Ί
  • J. J. Nestor (1984) Uniform Asymptotic Approximations of Solutions of Second-order Linear Differential Equations, with a Coalescing Simple Turning Point and Simple Pole. Ph.D. Thesis, University of Maryland, College Park, MD.
  • β–Ί
  • M. Newman (1967) Solving equations exactly. J. Res. Nat. Bur. Standards Sect. B 71B, pp. 171–179.
  • β–Ί
  • C. J. Noble (2004) Evaluation of negative energy Coulomb (Whittaker) functions. Comput. Phys. Comm. 159 (1), pp. 55–62.
  • 28: 2.8 Differential Equations with a Parameter
    §2.8 Differential Equations with a Parameter
    β–ΊThe transformed equation has the form …In Case III the approximating equation is … β–ΊThe transformed differential equation is … β–ΊFor examples of uniform asymptotic approximations in terms of Whittaker functions with fixed second parameter see §18.15(i) and §28.8(iv). …
    29: 23.22 Methods of Computation
    β–ΊSuppose that the invariants g 2 ⁑ = c , g 3 ⁑ = d , are given, for example in the differential equation (23.3.10) or via coefficients of an elliptic curve (§23.20(ii)). The determination of suitable generators 2 ⁒ Ο‰ 1 and 2 ⁒ Ο‰ 3 is the classical inversion problem (Whittaker and Watson (1927, §21.73), McKean and Moll (1999, §2.12); see also §20.9(i) and McKean and Moll (1999, §2.16)). … β–Ί
  • (a)

    In the general case, given by c ⁒ d 0 , we compute the roots Ξ± , Ξ² , Ξ³ , say, of the cubic equation 4 ⁒ t 3 c ⁒ t d = 0 ; see §1.11(iii). These roots are necessarily distinct and represent e 1 ⁑ , e 2 ⁑ , e 3 ⁑ in some order.

    If c and d are real, and the discriminant is positive, that is c 3 27 ⁒ d 2 > 0 , then e 1 ⁑ , e 2 ⁑ , e 3 ⁑ can be identified via (23.5.1), and k 2 , k 2 obtained from (23.6.16).

    If c 3 27 ⁒ d 2 < 0 , or c and d are not both real, then we label α , β , γ so that the triangle with vertices α , β , γ is positively oriented and [ α , γ ] is its longest side (chosen arbitrarily if there is more than one). In particular, if α , β , γ are collinear, then we label them so that β is on the line segment ( α , γ ) . In consequence, k 2 = ( β γ ) / ( α γ ) , k 2 = ( α β ) / ( α γ ) satisfy ⁑ k 2 0 ⁑ k 2 (with strict inequality unless α , β , γ are collinear); also | k 2 | , | k 2 | 1 .

    Finally, on taking the principal square roots of k 2 and k 2 we obtain values for k and k that lie in the 1st and 4th quadrants, respectively, and 2 ⁒ Ο‰ 1 , 2 ⁒ Ο‰ 3 are given by

    23.22.1 2 ⁒ Ο‰ 1 ⁒ M ⁑ ( 1 , k ) = 2 ⁒ i ⁒ Ο‰ 3 ⁒ M ⁑ ( 1 , k ) = Ο€ 3 ⁒ c ⁒ ( 2 + k 2 ⁒ k 2 ) ⁒ ( k 2 k 2 ) d ⁒ ( 1 k 2 ⁒ k 2 ) ,

    where M denotes the arithmetic-geometric mean (see §§19.8(i) and 22.20(ii)). This process yields 2 possible pairs ( 2 ⁒ Ο‰ 1 , 2 ⁒ Ο‰ 3 ), corresponding to the 2 possible choices of the square root.

  • 30: 22.19 Physical Applications
    β–ΊClassical motion in one dimension is described by Newton’s equationβ–Ί
    §22.19(iii) Nonlinear ODEs and PDEs
    β–Ίβ–ΊElementary discussions of this topic appear in Lawden (1989, §5.7), Greenhill (1959, pp. 101–103), and Whittaker (1964, Chapter VI). … β–ΊWhittaker (1964, Chapter IV) enumerates the complete class of one-body classical mechanical problems that are solvable this way. …