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11: 19.36 Methods of Computation
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►where the elementary symmetric functions are defined by (19.19.4).
If (19.36.1) is used instead of its first five terms, then the factor in Carlson (1995, (2.2)) is changed to .
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can be evaluated by using (19.25.7), and by using (19.21.10), but cancellations may become significant.
Thompson (1997, pp. 499, 504) uses descending Landen transformations for both and .
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►Lee (1990) compares the use of theta functions for computation of , , and , , with four other methods.
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12: 24.11 Asymptotic Approximations
13: 24.16 Generalizations
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►For , Bernoulli and Euler polynomials of order
are defined respectively by
…When they reduce to the Bernoulli and Euler numbers of
order
:
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►Also for ,
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►Let be the trivial character and the unique (nontrivial) character with ; that is, , , .
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14: 8.27 Approximations
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DiDonato (1978) gives a simple approximation for the function (which is related to the incomplete gamma function by a change of variables) for real and large positive . This takes the form , approximately, where and is shown to produce an absolute error as .
Luke (1975, p. 103) gives Chebyshev-series expansions for and related functions for .
Luke (1975, p. 106) gives rational and Padé approximations, with remainders, for and for complex with .
Verbeeck (1970) gives polynomial and rational approximations for , approximately, where denotes a quotient of polynomials of equal degree in .
15: 19.1 Special Notation
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►We use also the function , introduced by Jahnke et al. (1966, p. 43).
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►In Abramowitz and Stegun (1964, Chapter 17) the functions (19.1.1) and (19.1.2) are denoted, in order, by , , , , , and , where and is the (not related to ) in (19.1.1) and (19.1.2).
…However, it should be noted that in Chapter 8 of Abramowitz and Stegun (1964) the notation used for elliptic integrals differs from Chapter 17 and is consistent with that used in the present chapter and the rest of the NIST Handbook and DLMF.
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, , and are the symmetric (in , , and ) integrals of the first, second, and third kinds; they are complete if exactly one of , , and is identically 0.
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16: 36.2 Catastrophes and Canonical Integrals
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►Special cases: , fold catastrophe; , cusp catastrophe; , swallowtail catastrophe.
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Normal Forms for Umbilic Catastrophes with Codimension
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36.2.28
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36.2.29
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17: 19.9 Inequalities
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19.9.3
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►Further inequalities for and can be found in Alzer and Qiu (2004), Anderson et al. (1992a, b, 1997), and Qiu and Vamanamurthy (1996).
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►Sharper inequalities for are:
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►Inequalities for both and involving inverse circular or inverse hyperbolic functions are given in Carlson (1961b, §4).
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►Other inequalities for can be obtained from inequalities for given in Carlson (1966, (2.15)) and Carlson (1970) via (19.25.5).
18: 36.7 Zeros
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►Inside the cusp, that is, for , the zeros form pairs lying in curved rows.
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►Just outside the cusp, that is, for , there is a single row of zeros on each side.
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►The zeros are lines in space where is undetermined.
…Near , and for small and , the modulus has the symmetry of a lattice with a rhombohedral unit cell that has a mirror plane and an inverse threefold axis whose and repeat distances are given by
…The rings are almost circular (radii close to and varying by less than 1%), and almost flat (deviating from the planes by at most ).
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19: 3.6 Linear Difference Equations
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►The Weber function satisfies
…We apply the algorithm to compute to 8S for the range , beginning with the value obtained from the Maclaurin series expansion (§11.10(iii)).
►In the notation of §3.6(v) we have and .
…The values of for are the wanted values of .
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►For further information see Wimp (1984, Chapters 7–8), Cash and Zahar (1994), and Lozier (1980).