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11: Software Index
12: Errata
  • Equation (18.28.8)
    18.28.8 1 2 π 0 π Q n ( cos θ ; a , b | q ) Q m ( cos θ ; a , b | q ) | ( e 2 i θ ; q ) ( a e i θ , b e i θ ; q ) | 2 d θ = δ n , m ( q n + 1 , a b q n ; q ) , a , b or a = b ¯ ; a b 1 ; | a | , | b | 1

    The constraint which originally stated that “ | a b | < 1 ” has been updated to be “ a b 1 ”.

  • Subsection 19.11(i)

    A sentence and unnumbered equation

    R C ( γ δ , γ ) = 1 δ arctan ( δ sin θ sin ϕ sin ψ α 2 1 α 2 cos θ cos ϕ cos ψ ) ,

    were added which indicate that care must be taken with the multivalued functions in (19.11.5). See (Cayley, 1961, pp. 103-106).

    Suggested by Albert Groenenboom.

  • Section 1.14

    There have been extensive changes in the notation used for the integral transforms defined in §1.14. These changes are applied throughout the DLMF. The following table summarizes the changes.

    Transform New Abbreviated Old
    Notation Notation Notation
    Fourier ( f ) ( x ) f ( x )
    Fourier Cosine c ( f ) ( x ) c f ( x )
    Fourier Sine s ( f ) ( x ) s f ( x )
    Laplace ( f ) ( s ) f ( s ) ( f ( t ) ; s )
    Mellin ( f ) ( s ) f ( s ) ( f ; s )
    Hilbert ( f ) ( s ) f ( s ) ( f ; s )
    Stieltjes 𝒮 ( f ) ( s ) 𝒮 f ( s ) 𝒮 ( f ; s )

    Previously, for the Fourier, Fourier cosine and Fourier sine transforms, either temporary local notations were used or the Fourier integrals were written out explicitly.

  • Chapters 8, 20, 36

    Several new equations have been added. See (8.17.24), (20.7.34), §20.11(v), (26.12.27), (36.2.28), and (36.2.29).

  • References

    Bibliographic citations were added in §§1.13(v), 10.14, 10.21(ii), 18.15(v), 18.32, 30.16(iii), 32.13(ii), and as general references in Chapters 19, 20, 22, and 23.

  • 13: 3.4 Differentiation
    If f can be extended analytically into the complex plane, then from Cauchy’s integral formula (§1.9(iii)) …The integral on the right-hand side can be approximated by the composite trapezoidal rule (3.5.2). … The integral (3.4.18) becomes …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 ! . …As explained in §§3.5(i) and 3.5(ix) the composite trapezoidal rule can be very efficient for computing integrals with analytic periodic integrands. …
    14: 14.30 Spherical and Spheroidal Harmonics
    14.30.1 Y l , m ( θ , ϕ ) = ( ( l m ) ! ( 2 l + 1 ) 4 π ( l + m ) ! ) 1 / 2 e i m ϕ 𝖯 l m ( cos θ ) ,
    14.30.2 Y l m ( θ , ϕ ) = cos ( m ϕ ) 𝖯 l m ( cos θ )  or  sin ( m ϕ ) 𝖯 l m ( cos θ ) .
    See also (34.3.22), and for further related integrals see Askey et al. (1986). … where 𝐚 = ( 1 2 λ λ 2 , i 2 λ i λ 2 , 1 ) and 𝐱 = ( r sin θ cos ϕ , r sin θ sin ϕ , r cos θ ) . …
    14.30.9 𝖯 l ( cos θ 1 cos θ 2 + sin θ 1 sin θ 2 cos ( ϕ 1 ϕ 2 ) ) = 4 π 2 l + 1 m = l l Y l , m ( θ 1 , ϕ 1 ) ¯ Y l , m ( θ 2 , ϕ 2 ) .
    15: 36.2 Catastrophes and Canonical Integrals
    §36.2 Catastrophes and Canonical Integrals
    §36.2(i) Definitions
    Canonical Integrals
    §36.2(iii) Symmetries
    16: 25.11 Hurwitz Zeta Function
    See accompanying text
    Figure 25.11.1: Hurwitz zeta function ζ ( x , a ) , a = 0. …8, 1, 20 x 10 . … Magnify
    §25.11(vii) Integral Representations
    §25.11(viii) Further Integral Representations
    25.11.31 1 Γ ( s ) 0 x s 1 e a x 2 cosh x d x = 4 s ( ζ ( s , 1 4 + 1 4 a ) ζ ( s , 3 4 + 1 4 a ) ) , s > 0 , a > 1 .
    §25.11(ix) Integrals