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31: 28.5 Second Solutions fe n , ge n
28.5.1 fe n ( z , q ) = C n ( q ) ( z ce n ( z , q ) + f n ( z , q ) ) ,
28.5.2 ge n ( z , q ) = S n ( q ) ( z se n ( z , q ) + g n ( z , q ) ) ,
The factors C n ( q ) and S n ( q ) in (28.5.1) and (28.5.2) are normalized so that
28.5.5 ( C n ( q ) ) 2 0 2 π ( f n ( x , q ) ) 2 d x = ( S n ( q ) ) 2 0 2 π ( g n ( x , q ) ) 2 d x = π .
(Other normalizations for C n ( q ) and S n ( q ) can be found in the literature, but most formulas—including connection formulas—are unaffected since fe n ( z , q ) / C n ( q ) and ge n ( z , q ) / S n ( q ) are invariant.) …
32: 3.7 Ordinary Differential Equations
The remaining two equations are supplied by boundary conditions of the formThe eigenvalues λ k are simple, that is, there is only one corresponding eigenfunction (apart from a normalization factor), and when ordered increasingly the eigenvalues satisfy … If q ( x ) is C on the closure of ( a , b ) , then the discretized form (3.7.13) of the differential equation can be used. …
33: 20.13 Physical Applications
For τ = i t , with α , t , z real, (20.13.1) takes the form of a real-time t diffusion equation …These two apparently different solutions differ only in their normalization and boundary conditions. … In the singular limit τ 0 + , the functions θ j ( z | τ ) , j = 1 , 2 , 3 , 4 , become integral kernels of Feynman path integrals (distribution-valued Green’s functions); see Schulman (1981, pp. 194–195). This allows analytic time propagation of quantum wave-packets in a box, or on a ring, as closed-form solutions of the time-dependent Schrödinger equation.
34: 29.15 Fourier Series and Chebyshev Series
be the eigenvector corresponding to H m and normalized so that … Since (29.2.5) implies that cos ϕ = sn ( z , k ) , (29.15.1) can be rewritten in the form …The set of coefficients of this polynomial (without normalization) can also be found directly as an eigenvector of an ( n + 1 ) × ( n + 1 ) tridiagonal matrix; see Arscott and Khabaza (1962). …
35: 28.15 Expansions for Small q
§28.15 Expansions for Small q
28.15.1 λ ν ( q ) = ν 2 + 1 2 ( ν 2 1 ) q 2 + 5 ν 2 + 7 32 ( ν 2 1 ) 3 ( ν 2 4 ) q 4 + 9 ν 4 + 58 ν 2 + 29 64 ( ν 2 1 ) 5 ( ν 2 4 ) ( ν 2 9 ) q 6 + .
28.15.3 me ν ( z , q ) = e i ν z q 4 ( 1 ν + 1 e i ( ν + 2 ) z 1 ν 1 e i ( ν 2 ) z ) + q 2 32 ( 1 ( ν + 1 ) ( ν + 2 ) e i ( ν + 4 ) z + 1 ( ν 1 ) ( ν 2 ) e i ( ν 4 ) z 2 ( ν 2 + 1 ) ( ν 2 1 ) 2 e i ν z ) + ;
36: DLMF Project News
error generating summary
37: 21.7 Riemann Surfaces
The ω j are normalized so that … Then the prime form on the corresponding compact Riemann surface Γ is defined by
21.7.9 E ( P 1 , P 2 ) = θ [ 𝜶 𝜷 ] ( P 1 P 2 𝝎 | 𝛀 ) / ( ζ ( P 1 ) ζ ( P 2 ) ) ,
These are Riemann surfaces that may be obtained from algebraic curves of the form
38: 30.8 Expansions in Series of Ferrers Functions
30.8.1 𝖯𝗌 n m ( x , γ 2 ) = k = R ( 1 ) k a n , k m ( γ 2 ) 𝖯 n + 2 k m ( x ) ,
(note that A R = 0 ) that satisfies the normalizing condition …
30.8.9 𝖰𝗌 n m ( x , γ 2 ) = k = N 1 ( 1 ) k a n , k m ( γ 2 ) 𝖯 n + 2 k m ( x ) + k = N ( 1 ) k a n , k m ( γ 2 ) 𝖰 n + 2 k m ( x ) ,
The set of coefficients a n , k m ( γ 2 ) , k = N 1 , N 2 , , is the recessive solution of (30.8.4) as k that is normalized by …
39: 18.28 Askey–Wilson Class
The Askey–Wilson polynomials form a system of OP’s { p n ( x ) } , n = 0 , 1 , 2 , , that are orthogonal with respect to a weight function on a bounded interval, possibly supplemented with discrete weights on a finite set. The q -Racah polynomials form a system of OP’s { p n ( x ) } , n = 0 , 1 , 2 , , N , that are orthogonal with respect to a weight function on a sequence { q y + c q y + 1 } , y = 0 , 1 , , N , with c a constant. … Assume a , b , c , d are all real, or two of them are real and two form a conjugate pair, or none of them are real but they form two conjugate pairs. …
18.28.29 lim q 1 p n ( 1 1 2 x ( 1 q ) 2 ; q a , q b , q c , q d | q ) ( 1 q ) 3 n = W n ( x ; a , b , c , d ) .
40: 33.9 Expansions in Series of Bessel Functions
33.9.3 F ( η , ρ ) = C ( η ) ( 2 + 1 ) ! ( 2 η ) 2 + 1 ρ k = 2 + 1 b k t k / 2 I k ( 2 t ) , η > 0 ,
33.9.4 F ( η , ρ ) = C ( η ) ( 2 + 1 ) ! ( 2 | η | ) 2 + 1 ρ k = 2 + 1 b k t k / 2 J k ( 2 t ) , η < 0 .
33.9.6 G ( η , ρ ) ρ ( + 1 2 ) λ ( η ) C ( η ) k = 2 + 1 ( 1 ) k b k t k / 2 K k ( 2 t ) ,