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11: 36.4 Bifurcation Sets
β–ΊThese are real solutions t j ⁑ ( 𝐱 ) , 1 j j max ⁑ ( 𝐱 ) K + 1 , of β–Ί β–ΊThese are real solutions { s j ⁒ ( 𝐱 ) , t j ⁑ ( 𝐱 ) } , 1 j j max ⁑ ( 𝐱 ) 4 , of … β–Ί
x = 9 20 ⁒ z 2 .
β–Ί
x = 3 20 ⁒ z 2 ,
12: 3.8 Nonlinear Equations
§3.8 Nonlinear Equations
β–ΊSolutions are called roots of the equation, or zeros of f . … β–Ίand the solutions are called fixed points of Ο• . … β–ΊConsider x = 20 and j = 19 . We have p ⁑ ( 20 ) = 19 ! and a 19 = 1 + 2 + β‹― + 20 = 210 . …
13: 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
  • D. Naylor (1989) On an integral transform involving a class of Mathieu functions. SIAM J. Math. Anal. 20 (6), pp. 1500–1513.
  • β–Ί
  • W. J. Nellis and B. C. Carlson (1966) Reduction and evaluation of elliptic integrals. Math. Comp. 20 (94), pp. 223–231.
  • 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
  • E. W. Ng and M. Geller (1969) A table of integrals of the error functions. J. Res. Nat. Bur. Standards Sect B. 73B, pp. 1–20.
  • 14: 31.13 Asymptotic Approximations
    β–ΊFor asymptotic approximations of the solutions of Heun’s equation (31.2.1) when two singularities are close together, see Lay and Slavyanov (1999). β–ΊFor asymptotic approximations of the solutions of confluent forms of Heun’s equation in the neighborhood of irregular singularities, see Komarov et al. (1976), Ronveaux (1995, Parts B,C,D,E), Bogush and Otchik (1997), Slavyanov and Veshev (1997), and Lay et al. (1998).
    15: 36.5 Stokes Sets
    β–Ί
    36.5.4 80 ⁒ x 5 40 ⁒ x 4 55 ⁒ x 3 + 5 ⁒ x 2 + 20 ⁒ x 1 = 0 ,
    β–Ί
    36.5.7 X = 9 20 + 20 ⁒ u 4 Y 2 20 ⁒ u 2 + 6 ⁒ u 2 ⁒ sign ⁑ ( z ) ,
    β–ΊFor z < 0 , there are two solutions u , provided that | Y | > ( 2 5 ) 1 / 2 . … β–ΊThe first sheet corresponds to x < 0 and is generated as a solution of Equations (36.5.6)–(36.5.9). …For | Y | > Y 1 the second sheet is generated by a second solution of (36.5.6)–(36.5.9), and for | Y | < Y 1 it is generated by the roots of the polynomial equation …
    16: Bibliography K
    β–Ί
  • R. B. Kearfott, M. Dawande, K. Du, and C. Hu (1994) Algorithm 737: INTLIB: A portable Fortran 77 interval standard-function library. ACM Trans. Math. Software 20 (4), pp. 447–459.
  • β–Ί
  • M. K. Kerimov (1980) Methods of computing the Riemann zeta-function and some generalizations of it. USSR Comput. Math. and Math. Phys. 20 (6), pp. 212–230.
  • β–Ί
  • A. V. Kitaev and A. H. Vartanian (2004) Connection formulae for asymptotics of solutions of the degenerate third Painlevé equation. I. Inverse Problems 20 (4), pp. 1165–1206.
  • β–Ί
  • T. H. Koornwinder (2009) The Askey scheme as a four-manifold with corners. Ramanujan J. 20 (3), pp. 409–439.
  • β–Ί
  • Y. A. Kravtsov (1964) Asymptotic solution of Maxwell’s equations near caustics. Izv. Vuz. Radiofiz. 7, pp. 1049–1056.
  • 17: 8 Incomplete Gamma and Related
    Functions
    18: 28 Mathieu Functions and Hill’s Equation
    19: 31.18 Methods of Computation
    §31.18 Methods of Computation
    β–ΊIndependent solutions of (31.2.1) can be computed in the neighborhoods of singularities from their Fuchs–Frobenius expansions (§31.3), and elsewhere by numerical integration of (31.2.1). Subsequently, the coefficients in the necessary connection formulas can be calculated numerically by matching the values of solutions and their derivatives at suitably chosen values of z ; see LaΔ­ (1994) and Lay et al. (1998). Care needs to be taken to choose integration paths in such a way that the wanted solution is growing in magnitude along the path at least as rapidly as all other solutions3.7(ii)). …
    20: 10.73 Physical Applications
    β–Ίand on separation of variables we obtain solutions of the form e ± i ⁒ n ⁒ Ο• ⁒ e ± ΞΊ ⁒ z ⁒ J n ⁑ ( ΞΊ ⁒ r ) , from which a solution satisfying prescribed boundary conditions may be constructed. … β–ΊSee Krivoshlykov (1994, Chapter 2, §2.2.10; Chapter 5, §5.2.2), Kapany and Burke (1972, Chapters 4–6; Chapter 7, §A.1), and Slater (1942, Chapter 4, §§20, 25). … β–ΊThe functions 𝗃 n ⁑ ( x ) , 𝗒 n ⁑ ( x ) , 𝗁 n ( 1 ) ⁑ ( x ) , and 𝗁 n ( 2 ) ⁑ ( x ) arise in the solution (again by separation of variables) of the Helmholtz equation in spherical coordinates ρ , ΞΈ , Ο• 1.5(ii)): …With the spherical harmonic Y β„“ , m ⁑ ( ΞΈ , Ο• ) defined as in §14.30(i), the solutions are of the form f = g β„“ ⁒ ( k ⁒ ρ ) ⁒ Y β„“ , m ⁑ ( ΞΈ , Ο• ) with g β„“ = 𝗃 β„“ , 𝗒 β„“ , 𝗁 β„“ ( 1 ) , or 𝗁 β„“ ( 2 ) , depending on the boundary conditions. …In quantum mechanics the spherical Bessel functions arise in the solution of the Schrödinger wave equation for a particle in a central potential. …