SL(2,Z)

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1: 23.15 Definitions
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k = θ 2 2 ⁡ ( 0 , q ) θ 3 2 ⁡ ( 0 , q ) ,
… ►The set of all bilinear transformations of this form is denoted by SL ( 2 , ℤ ) (Serre (1973, p. 77)). ►A modular function f ⁡ ( τ ) is a function of τ that is meromorphic in the half-plane ℑ ⁡ τ > 0 , and has the property that for all 𝒜 ∈ SL ⁢ ( 2 , ℤ ) , or for all 𝒜 belonging to a subgroup of SL ( 2 , ℤ ) , …(Some references refer to 2 ⁢ ℓ as the level). …
2: 10.29 Recurrence Relations and Derivatives
… ►With 𝒵 ν ⁡ ( z ) defined as in §10.25(ii), ►
𝒵 ν − 1 ⁡ ( z ) − 𝒵 ν + 1 ⁡ ( z ) = ( 2 ⁢ ν / z ) ⁢ 𝒵 ν ⁡ ( z ) ,
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𝒵 ν − 1 ⁡ ( z ) + 𝒵 ν + 1 ⁡ ( z ) = 2 ⁢ 𝒵 ν ′ ⁡ ( z ) .
… ►For results on modified quotients of the form z ⁢ 𝒵 ν ± 1 ⁡ ( z ) / 𝒵 ν ⁡ ( z ) see Onoe (1955) and Onoe (1956). … ►For k = 0 , 1 , 2 , … , …
3: 15.17 Mathematical Applications
… ►First, as spherical functions on noncompact Riemannian symmetric spaces of rank one, but also as associated spherical functions, intertwining functions, matrix elements of SL ( 2 , ℝ ) , and spherical functions on certain nonsymmetric Gelfand pairs. …
4: 23.18 Modular Transformations
… ►and λ ⁡ ( τ ) is a cusp form of level zero for the corresponding subgroup of SL ( 2 , ℤ ) . … ► J ⁡ ( τ ) is a modular form of level zero for SL ( 2 , ℤ ) . … ►
23.18.5 η ⁡ ( 𝒜 τ ) = ε ⁡ ( 𝒜 ) ⁢ ( − i ⁢ ( c ⁢ τ + d ) ) 1 / 2 ⁢ η ⁡ ( τ ) ,
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23.18.7 s ⁡ ( d , c ) = ∑ r = 1 c − 1 r c ⁢ ( d ⁢ r c − ⌊ d ⁢ r c ⌋ − 1 2 ) , c > 0 .
… ►Note that η ⁡ ( τ ) is of level 1 2 . …
5: 10.36 Other Differential Equations
… ►The quantity λ 2 in (10.13.1)–(10.13.6) and (10.13.8) can be replaced by − λ 2 if at the same time the symbol 𝒞 in the given solutions is replaced by 𝒵 . … ►
10.36.1 z 2 ⁢ ( z 2 + ν 2 ) ⁢ w ′′ + z ⁢ ( z 2 + 3 ⁢ ν 2 ) ⁢ w ′ − ( ( z 2 + ν 2 ) 2 + z 2 − ν 2 ) ⁢ w = 0 , w = 𝒵 ν ′ ⁡ ( z ) ,
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10.36.2 z 2 ⁢ w ′′ + z ⁢ ( 1 ± 2 ⁢ z ) ⁢ w ′ + ( ± z − ν 2 ) ⁢ w = 0 , w = e ∓ z ⁢ 𝒵 ν ⁡ ( z ) .
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6: 33.22 Particle Scattering and Atomic and Molecular Spectra
… ►With e denoting here the elementary charge, the Coulomb potential between two point particles with charges Z 1 ⁢ e , Z 2 ⁢ e and masses m 1 , m 2 separated by a distance s is V ⁡ ( s ) = Z 1 ⁢ Z 2 ⁢ e 2 / ( 4 ⁢ π ⁢ ε 0 ⁢ s ) = Z 1 ⁢ Z 2 ⁢ α ⁢ ℏ ⁢ c / s , where Z j are atomic numbers, ε 0 is the electric constant, α is the fine structure constant, and ℏ is the reduced Planck’s constant. … ►In these applications, the Z -scaled variables r and ϵ are more convenient. ►
Z Scaling
►The Z -scaled variables r and ϵ of §33.14 are given by … ►For Z 1 ⁢ Z 2 = − 1 and m = m e , the electron mass, the scaling factors in (33.22.5) reduce to the Bohr radius, a 0 = ℏ / ( m e ⁢ c ⁢ α ) , and to a multiple of the Rydberg constant, …
7: 25.3 Graphics
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►See accompanying text►
Figure 25.3.2: Riemann zeta function ζ ⁡ ( x ) and its derivative ζ ′ ⁡ ( x ) , − 12 ≤ x ≤ − 2 . Magnify
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►See accompanying text►
Figure 25.3.4: Z ⁡ ( t ) , 0 ≤ t ≤ 50 . Z ⁡ ( t ) and ζ ⁡ ( 1 2 + i ⁢ t ) have the same zeros. … Magnify
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►See accompanying text►
Figure 25.3.5: Z ⁡ ( t ) , 1000 ≤ t ≤ 1050 . Magnify
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►See accompanying text►
Figure 25.3.6: Z ⁡ ( t ) , 10000 ≤ t ≤ 10050 . Magnify
8: 35.2 Laplace Transform
… ►For any complex symmetric matrix 𝐙 , … ►Then (35.2.1) converges absolutely on the region ℜ ⁡ ( 𝐙 ) > 𝐗 0 , and g ⁡ ( 𝐙 ) is a complex analytic function of all elements z j , k of 𝐙 . … ► ►where the integral is taken over all 𝐙 = 𝐔 + i ⁢ 𝐕 such that 𝐔 > 𝐗 0 and 𝐕 ranges over 𝓢 . … ►If g j is the Laplace transform of f j , j = 1 , 2 , then g 1 ⁡ g 2 is the Laplace transform of the convolution f 1 ∗ f 2 , where …
9: 25.10 Zeros
… ►Calculations relating to the zeros on the critical line make use of the real-valued function …is chosen to make Z ⁡ ( t ) real, and ph ⁡ Γ ⁡ ( 1 4 + 1 2 ⁢ i ⁢ t ) assumes its principal value. Because | Z ⁡ ( t ) | = | ζ ⁡ ( 1 2 + i ⁢ t ) | , Z ⁡ ( t ) vanishes at the zeros of ζ ⁡ ( 1 2 + i ⁢ t ) , which can be separated by observing sign changes of Z ⁡ ( t ) . Because Z ⁡ ( t ) changes sign infinitely often, ζ ⁡ ( 1 2 + i ⁢ t ) has infinitely many zeros with t real. … ►Sign changes of Z ⁡ ( t ) are determined by multiplying (25.9.3) by exp ⁡ ( i ⁢ ϑ ⁡ ( t ) ) to obtain the Riemann–Siegel formula: …
10: 35.4 Partitions and Zonal Polynomials
… ►For any partition κ , the zonal polynomial Z κ : 𝓢 → ℝ is defined by the properties … ►Therefore Z κ ⁡ ( 𝐓 ) is a symmetric polynomial in the eigenvalues of 𝐓 . … ►For k = 0 , 1 , 2 , … , … ►For 𝐓 ∈ 𝛀 and ℜ ⁡ ( a ) , ℜ ⁡ ( b ) > 1 2 ⁢ ( m − 1 ) , ► …