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21: 15.4 Special Cases
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15.4.34 F ⁑ ( 3 ⁒ a , a ; 2 ⁒ a ; e i ⁒ Ο€ / 3 ) = Ο€ ⁒ e i ⁒ Ο€ ⁒ a / 2 ⁒ 2 2 ⁒ a ⁒ Ξ“ ⁑ ( 1 2 + a ) 3 ( 3 ⁒ a + 1 ) / 2 ⁒ ( 1 Ξ“ ⁑ ( 1 3 + a ) ⁒ Ξ“ ⁑ ( 2 3 ) + 1 Ξ“ ⁑ ( 2 3 + a ) ⁒ Ξ“ ⁑ ( 1 3 ) ) ,
22: Bibliography R
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  • RISC Combinatorics Group (website) Research Institute for Symbolic Computation, Hagenberg im Mühlkreis, Austria.
  • 23: 18.28 Askey–Wilson Class
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    q -Difference Equation
    24: Bibliography B
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  • P. M. Batchelder (1967) An Introduction to Linear Difference Equations. Dover Publications Inc., New York.
  • 25: 28.12 Definitions and Basic Properties
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    §28.12(i) Eigenvalues Ξ» Ξ½ + 2 ⁒ n ⁑ ( q )
    β–ΊWhen q = 0 Equation (28.2.16) has simple roots, given by … … β–ΊIf q is a normal value of the corresponding equation (28.2.16), then these functions are uniquely determined as analytic functions of z and q by the normalization …They have the following pseudoperiodic and orthogonality properties: …
    26: 2.7 Differential Equations
    β–Ίwhen s = 1 , 2 , 3 , . …
    27: 18.27 q -Hahn Class
    β–ΊFor other formulas, including q -difference equations, recurrence relations, duality formulas, special cases, and limit relations, see Koekoek et al. (2010, Chapter 14). …
    28: 28.2 Definitions and Basic Properties
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    28.2.1 w ′′ + ( a 2 ⁒ q ⁒ cos ⁑ ( 2 ⁒ z ) ) ⁒ w = 0 .
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    28.2.3 ( 1 ΞΆ 2 ) ⁒ w ′′ ΞΆ ⁒ w + ( a + 2 ⁒ q 4 ⁒ q ⁒ ΞΆ 2 ) ⁒ w = 0 .
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    28.2.5 [ w I ⁑ ( 0 ; a , q ) w II ⁑ ( 0 ; a , q ) w I ⁑ ( 0 ; a , q ) w II ⁑ ( 0 ; a , q ) ] = [ 1 0 0 1 ] .
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    28.2.16 cos ⁑ ( Ο€ ⁒ Ξ½ ) = w I ⁑ ( Ο€ ; a , q ) = w I ⁑ ( Ο€ ; a , q ) .
    29: 31.17 Physical Applications
    β–ΊFor applications of Heun’s equation and functions in astrophysics see Debosscher (1998) where different spectral problems for Heun’s equation are also considered. …
    30: 28.20 Definitions and Basic Properties
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    28.20.1 w ′′ ( a 2 ⁒ q ⁒ cosh ⁑ ( 2 ⁒ z ) ) ⁒ w = 0 ,
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    28.20.6 Fe n ⁑ ( z , q ) = βˆ“ i ⁒ fe n ⁑ ( ± i ⁒ z , q ) , n = 0 , 1 , ,
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    28.20.7 Ge n ⁑ ( z , q ) = ge n ⁑ ( ± i ⁒ z , q ) , n = 1 , 2 , .