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11: 1.17 Integral and Series Representations of the Dirac Delta
In the language of physics and applied mathematics, these equations indicate the normalizations chosen for these non- L 2 improper eigenfunctions of the differential operators (with derivatives respect to spatial co-ordinates) which generate them; the normalizations (1.17.12_1) and (1.17.12_2) are explicitly derived in Friedman (1990, Ch. 4), the others follow similarly. …
12: 29.21 Tables
  • Arscott and Khabaza (1962) tabulates the coefficients of the polynomials P in Table 29.12.1 (normalized so that the numerically largest coefficient is unity, i.e. monic polynomials), and the corresponding eigenvalues h for k 2 = 0.1 ( .1 ) 0.9 , n = 1 ( 1 ) 30 . Equations from §29.6 can be used to transform to the normalization adopted in this chapter. Precision is 6S.

  • 13: 30.16 Methods of Computation
    If λ n m ( γ 2 ) is known, then we can compute 𝖯𝗌 n m ( x , γ 2 ) (not normalized) by solving the differential equation (30.2.1) numerically with initial conditions w ( 0 ) = 1 , w ( 0 ) = 0 if n m is even, or w ( 0 ) = 0 , w ( 0 ) = 1 if n m is odd. …
    14: 10.74 Methods of Computation
    In the case of J n ( x ) , the need for initial values can be avoided by application of Olver’s algorithm (§3.6(v)) in conjunction with Equation (10.12.4) used as a normalizing condition, or in the case of noninteger orders, (10.23.15). …
    15: 2.11 Remainder Terms; Stokes Phenomenon
    For notational convenience assume that the original differential equation (2.7.1) is normalized so that λ 2 λ 1 = 1 . …
    16: 1.18 Linear Second Order Differential Operators and Eigenfunction Expansions
    Applying equations (1.18.29) and (1.18.30), the complete set of normalized eigenfunctions being … See Friedman (1990, pp. 233–252) for elementary discussions of both equations and the normalization process; and also the references in §1.18(ix). …
    17: 14.30 Spherical and Spheroidal Harmonics
    In the quantization of angular momentum the spherical harmonics Y l , m ( θ , ϕ ) are normalized solutions of the eigenvalue equations
    18: 18.28 Askey–Wilson Class
    q -Difference Equation
    18.28.6_1 ( L R n ) ( z ) = ( q n + a b c d q n 1 ) R n ( z ) ,
    18.28.6_2 ( L f ) ( z ) = ( 1 a z ) ( 1 b z ) ( 1 c z ) ( 1 d z ) ( 1 z 2 ) ( 1 q z 2 ) ( f ( q z ) f ( z ) ) + ( 1 a z 1 ) ( 1 b z 1 ) ( 1 c z 1 ) ( 1 d z 1 ) ( 1 z 2 ) ( 1 q z 2 ) ( f ( q 1 z ) f ( z ) ) + ( 1 + q 1 a b c d ) f ( z ) .
    18.28.6_3 ( z + z 1 ) R n ( z ) = a n ( R n + 1 ( z ) R n ( z ) ) + c n ( R n 1 ( z ) R n ( z ) ) + ( a + a 1 ) R n ( z ) ,
    18.28.6_5 R n ( a 1 q m ; a , b , c , d | q ) = R m ( a ~ 1 q n ; a ~ , b ~ , c ~ , d ~ | q ) , m , n = 0 , 1 , 2 , .
    19: 31.9 Orthogonality
    31.9.2 ζ ( 1 + , 0 + , 1 , 0 ) t γ 1 ( 1 t ) δ 1 ( t a ) ϵ 1 w m ( t ) w k ( t ) d t = δ m , k θ m .
    The normalization constant θ m is given by
    31.9.3 θ m = ( 1 e 2 π i γ ) ( 1 e 2 π i δ ) ζ γ ( 1 ζ ) δ ( ζ a ) ϵ f 0 ( q , ζ ) f 1 ( q , ζ ) q 𝒲 { f 0 ( q , ζ ) , f 1 ( q , ζ ) } | q = q m ,
    and the integration paths 1 , 2 are Pochhammer double-loop contours encircling distinct pairs of singularities { 0 , 1 } , { 0 , a } , { 1 , a } . For further information, including normalization constants, see Sleeman (1966a). …
    20: 8.12 Uniform Asymptotic Expansions for Large Parameter
    8.12.5 e ± π i a 2 i sin ( π a ) Q ( a , z e ± π i ) = ± 1 2 erfc ( ± i η a / 2 ) i T ( a , η ) ,
    8.12.16 e ± π i a 2 i sin ( π a ) Q ( a , a e ± π i ) ± 1 2 i 2 π a k = 0 c k ( 0 ) ( a ) k , | ph a | π δ ,
    8.12.18 Q ( a , z ) P ( a , z ) } z a 1 2 e z Γ ( a ) ( d ( ± χ ) k = 0 A k ( χ ) z k / 2 k = 1 B k ( χ ) z k / 2 ) ,