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1: Bibliography J
  • L. Jager (1997) Fonctions de Mathieu et polynômes de Klein-Gordon. C. R. Acad. Sci. Paris Sér. I Math. 325 (7), pp. 713–716 (French).
  • M. Jimbo, T. Miwa, Y. Môri, and M. Sato (1980) Density matrix of an impenetrable Bose gas and the fifth Painlevé transcendent. Phys. D 1 (1), pp. 80–158.
  • X.-S. Jin and R. Wong (1998) Uniform asymptotic expansions for Meixner polynomials. Constr. Approx. 14 (1), pp. 113–150.
  • A. Jonquière (1889) Note sur la série n = 1 x n / n s . Bull. Soc. Math. France 17, pp. 142–152 (French).
  • G. Julia (1918) Memoire sur l’itération des fonctions rationnelles. J. Math. Pures Appl. 8 (1), pp. 47–245 (French).
  • 2: Bibliography D
  • M. G. de Bruin, E. B. Saff, and R. S. Varga (1981a) On the zeros of generalized Bessel polynomials. I. Nederl. Akad. Wetensch. Indag. Math. 84 (1), pp. 1–13.
  • P. Deligne, P. Etingof, D. S. Freed, D. Kazhdan, J. W. Morgan, and D. R. Morrison (Eds.) (1999) Quantum Fields and Strings: A Course for Mathematicians. Vol. 1, 2. American Mathematical Society, Providence, RI.
  • R. B. Dingle (1957a) The Bose-Einstein integrals p ( η ) = ( p ! ) 1 0 ϵ p ( e ϵ η 1 ) 1 𝑑 ϵ . Appl. Sci. Res. B. 6, pp. 240–244.
  • R. B. Dingle (1957b) The Fermi-Dirac integrals p ( η ) = ( p ! ) 1 0 ϵ p ( e ϵ η + 1 ) 1 𝑑 ϵ . Appl. Sci. Res. B. 6, pp. 225–239.
  • A. L. Dixon and W. L. Ferrar (1930) Infinite integrals in the theory of Bessel functions. Quart. J. Math., Oxford Ser. 1 (1), pp. 122–145.
  • 3: 3.4 Differentiation
    The Lagrange ( n + 1 ) -point formula is … where ξ 0 and ξ 1 I . For the values of n 0 and n 1 used in the formulas below … With the choice r = k (which is crucial when k is large because of numerical cancellation) the integrand equals e k at the dominant points θ = 0 , 2 π , and in combination with the factor k k in front of the integral sign this gives a rough approximation to 1 / k ! . …
    3.4.34 4 u 0 , 0 = 1 6 h 4 ( 184 u 0 , 0 ( u 0 , 3 + u 0 , 3 + u 3 , 0 + u 3 , 0 ) + 14 ( u 0 , 2 + u 0 , 2 + u 2 , 0 + u 2 , 0 ) 77 ( u 0 , 1 + u 0 , 1 + u 1 , 0 + u 1 , 0 ) + 20 ( u 1 , 1 + u 1 , 1 + u 1 , 1 + u 1 , 1 ) ( u 1 , 2 + u 2 , 1 + u 1 , 2 + u 2 , 1 + u 1 , 2 + u 2 , 1 + u 1 , 2 + u 2 , 1 ) ) + O ( h 4 ) .
    4: DLMF Project News
    error generating summary
    5: 17.18 Methods of Computation
    The two main methods for computing basic hypergeometric functions are: (1) numerical summation of the defining series given in §§17.4(i) and 17.4(ii); (2) modular transformations. Method (1) is applicable within the circles of convergence of the defining series, although it is often cumbersome owing to slowness of convergence and/or severe cancellation. … Method (1) can sometimes be improved by application of convergence acceleration procedures; see §3.9. …
    6: 4.45 Methods of Computation
    Suppose first 1 / 10 x 10 . …After computing ln ( 1 + y ) from (4.6.1) … For other values of x set x = 10 m ξ , where 1 / 10 ξ 10 and m . … From (4.24.15) with u = v = ( ( 1 + x 2 ) 1 / 2 1 ) / x , we have … For example, arcsin x = arctan ( x ( 1 x 2 ) 1 / 2 ) . …
    7: 10.55 Continued Fractions
    For continued fractions for 𝗃 n + 1 ( z ) / 𝗃 n ( z ) and 𝗂 n + 1 ( 1 ) ( z ) / 𝗂 n ( 1 ) ( z ) see Cuyt et al. (2008, pp. 350, 353, 362, 363, 367–369).
    8: 2.7 Differential Equations
    with a 0 , j = 1 , and … If α 1 α 2 = 0 , 1 , 2 , , then (2.7.4) applies only in the case j = 1 . …
    §2.7(ii) Irregular Singularities of Rank 1
    a 0 , j = 1 , and … This kind of cancellation cannot take place with w 1 ( z ) and w 2 ( z ) , and for this reason, and following Miller (1950), we call w 1 ( z ) and w 2 ( z ) a numerically satisfactory pair of solutions. …
    9: 6.18 Methods of Computation
    For large x or | z | these series suffer from slow convergence or cancellation (or both). However, this problem is less severe for the series of spherical Bessel functions because of their more rapid rate of convergence, and also (except in the case of (6.10.6)) absence of cancellation when z = x ( > 0 ). … For n = 0 , 1 , 2 , , define …
    B n 1 = 2 n B n + z A n 1 2 n 1 ,
    A 0 , B 0 , and C 0 can be computed by Miller’s algorithm (§3.6(iii)), starting with initial values ( A N , B N , C N ) = ( 1 , 0 , 0 ) , say, where N is an arbitrary large integer, and normalizing via C 0 = 1 / z . …
    10: 4.30 Elementary Properties
    Table 4.30.1: Hyperbolic functions: interrelations. …
    sinh θ = a cosh θ = a tanh θ = a csch θ = a sech θ = a coth θ = a
    sinh θ a ( a 2 1 ) 1 / 2 a ( 1 a 2 ) 1 / 2 a 1 a 1 ( 1 a 2 ) 1 / 2 ( a 2 1 ) 1 / 2
    cosh θ ( 1 + a 2 ) 1 / 2 a ( 1 a 2 ) 1 / 2 a 1 ( 1 + a 2 ) 1 / 2 a 1 a ( a 2 1 ) 1 / 2
    tanh θ a ( 1 + a 2 ) 1 / 2 a 1 ( a 2 1 ) 1 / 2 a ( 1 + a 2 ) 1 / 2 ( 1 a 2 ) 1 / 2 a 1
    csch θ a 1 ( a 2 1 ) 1 / 2 a 1 ( 1 a 2 ) 1 / 2 a a ( 1 a 2 ) 1 / 2 ( a 2 1 ) 1 / 2
    sech θ ( 1 + a 2 ) 1 / 2 a 1 ( 1 a 2 ) 1 / 2 a ( 1 + a 2 ) 1 / 2 a a 1 ( a 2 1 ) 1 / 2