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31: 1.17 Integral and Series Representations of the Dirac Delta
for a suitably chosen sequence of functions δ n ( x ) , n = 1 , 2 , . … In this caseHowever, for n = 1 , 2 , , …provided that ϕ ( x ) is continuous when x ( , ) , and for each a , e n ( x a ) 2 ϕ ( x ) d x converges absolutely for all sufficiently large values of n (as in the case of (1.17.6)). … (1.17.22)–(1.17.24) are special cases of Morse and Feshbach (1953a, Eq. (6.3.11)). …
32: 8.2 Definitions and Basic Properties
However, when the integration paths do not cross the negative real axis, and in the case of (8.2.2) exclude the origin, γ ( a , z ) and Γ ( a , z ) take their principal values; compare §4.2(i). … When z 0 , Γ ( a , z ) is an entire function of a , and γ ( a , z ) is meromorphic with simple poles at a = n , n = 0 , 1 , 2 , , with residue ( 1 ) n / n ! . For m , …For example, in the case m = 1 we have … If w = γ ( a , z ) or Γ ( a , z ) , then …
33: 28.11 Expansions in Series of Mathieu Functions
Let f ( z ) be a 2 π -periodic function that is analytic in an open doubly-infinite strip S that contains the real axis, and q be a normal value (§28.7). …See Meixner and Schäfke (1954, §2.28), and for expansions in the case of the exceptional values of q see Meixner et al. (1980, p. 33). …
28.11.4 cos 2 m z = n = 0 A 2 m 2 n ( q ) ce 2 n ( z , q ) , m 0 ,
28.11.5 cos ( 2 m + 1 ) z = n = 0 A 2 m + 1 2 n + 1 ( q ) ce 2 n + 1 ( z , q ) ,
28.11.7 sin ( 2 m + 2 ) z = n = 0 B 2 m + 2 2 n + 2 ( q ) se 2 n + 2 ( z , q ) .
34: 28.31 Equations of Whittaker–Hill and Ince
and m = 0 , 1 , , n in all cases. … with η = a p m ( ξ ) , η = b p m ( ξ ) , respectively. … For m 1 m 2 , …More important are the double orthogonality relations for p 1 p 2 or m 1 m 2 or both, given by …and also for all p 1 , p 2 , m 1 , m 2 , given by …
35: 13.11 Series
13.11.1 M ( a , b , z ) = Γ ( a 1 2 ) e 1 2 z ( 1 4 z ) 1 2 a s = 0 ( 2 a 1 ) s ( 2 a b ) s ( b ) s s ! ( a 1 2 + s ) I a 1 2 + s ( 1 2 z ) , a + 1 2 , b 0 , 1 , 2 , ,
13.11.2 M ( a , b , z ) = Γ ( b a 1 2 ) e 1 2 z ( 1 4 z ) a b + 1 2 s = 0 ( 1 ) s ( 2 b 2 a 1 ) s ( b 2 a ) s ( b a 1 2 + s ) ( b ) s s ! I b a 1 2 + s ( 1 2 z ) , b a + 1 2 , b 0 , 1 , 2 , .
(13.6.9), (13.6.11_1) and (13.6.11_2) are special cases.
13.11.3 𝐌 ( a , b , z ) = e 1 2 z s = 0 A s ( b 2 a ) 1 2 ( 1 b s ) ( 1 2 z ) 1 2 ( 1 b + s ) J b 1 + s ( 2 z ( b 2 a ) ) ,
A 2 = 1 2 b ,
36: 18.21 Hahn Class: Interrelations
M n ( x ; β , c ) = M x ( n ; β , c ) , n , x = 0 , 1 , 2 , .
§18.21(ii) Limit Relations and Special Cases
18.21.4 lim N Q n ( x ; β 1 , N ( c 1 1 ) , N ) = M n ( x ; β , c ) .
18.21.7 lim β M n ( x ; β , a ( a + β ) 1 ) = C n ( x ; a ) .
See accompanying text
Figure 18.21.1: Askey scheme. …(This is with the convention that the real and imaginary parts of the parameters are counted separately in the case of the continuous Hahn polynomials.) Magnify
37: 18.39 Applications in the Physical Sciences
In the case of a single electron, charge e and mass m e , interacting with a fixed (infinite mass) nucleus of charge + Z e at the co-ordinate origin, with the choice of SI units, V ( r ) = Z e 2 / ( 4 π ϵ 0 r ) . …
38: 18.14 Inequalities
When ( α + 1 2 ) ( β + 1 2 ) > 0 choose m so that … except that when α = β = 1 2 (Chebyshev case) | P n ( α , β ) ( x n , m ) | is constant. … When α > 1 2 choose m so that … Also, when α 1 2 The case β = 0 of (18.14.26) is the Askey–Gasper inequality (18.38.3). …
39: 13.6 Relations to Other Functions
Special cases are the error functions … When b = 2 a the Kummer functions can be expressed as modified Bessel functions. …and in the case that b 2 a is an integer we have …Note that (13.6.11_1) and (13.6.11_2) are special cases of (13.11.1) and (13.11.2), respectively … Special cases of §13.6(iv) are as follows. …
40: 10.22 Integrals
When α = m = 1 , 2 , 3 , the left-hand side of (10.22.36) is the m th repeated integral of J ν ( x ) (§§1.4(v) and 1.15(vi)). … For the confluent hypergeometric function 𝐌 see §13.2(i). …
Weber–Schafheitlin Discontinuous Integrals, including Special Cases
When n = 0 , 1 , 2 , and μ > n 1 , … Equation (10.22.70) also remains valid if the order ν + 1 of the J functions on both sides is replaced by ν + 2 n 3 , n = 1 , 2 , , and the constraint ν > 3 2 is replaced by ν > n + 1 2 . …