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1: 37.4 Disk with Weight Function ( 1 x 2 y 2 ) α
On the unit disk
Complex Disk Polynomials
Real Disk Polynomials
Formulas for Complex Disk Polynomials
2: 18.37 Classical OP’s in Two or More Variables
§18.37(i) Disk Polynomials
18.37.2 x 2 + y 2 < 1 R m , n ( α ) ( x + i y ) R j , ( α ) ( x i y ) ( 1 x 2 y 2 ) α d x d y = 0 , m j and/or n .
The following three conditions, taken together, determine R m , n ( α ) ( z ) uniquely:
18.37.3 R m , n ( α ) ( z ) = j = 0 min ( m , n ) c j z m j z ¯ n j ,
18.37.5 R m , n ( α ) ( 1 ) = 1 .
3: 37.21 Physical Applications
Computer Tomography
OPs on the unit disk are closely related to Radon transforms, and they are used to construct reconstruction algorithms for x-ray computer tomography. … Applications in optics were already the motivation for Zernike (1934) to introduce the real disk polynomials (37.4.15) for α = 0 . …This makes it necessary to work with OPs on an annulus instead of a disk: the Tatian polynomials given in §37.10(ii), see de Winter et al. (2020) and Bilski et al. (2022). …
4: 37.7 Parabolic Biangular Region with Weight Function ( 1 x ) α ( x y 2 ) β
The Jacobi polynomials (37.7.3) on 𝕡 and the ultraspherical polynomials (37.4.4) on 𝔻 are related by the quadratic transformations
37.7.8 P k , n 1 2 , γ ( 1 x 2 , y ) = ( 1 ) n k ( γ + 1 ) k ( 1 2 ) n k ( 2 γ + 1 ) k ( γ + k + 1 ) n k C k , 2 n k ( γ + 1 2 ) ( x , y ) ,
The Jacobi polynomials (37.7.3) on 𝕡 are related to the real disk polynomials (37.4.15) by the quadratic transformations
37.7.11 y P k 1 , n 1 α , 1 2 ( x 2 + y 2 , x ) = 2 ( 1 2 ) k ( α + 1 ) n k k ! ( n k ) ! R n , n k α , ( s ) ( x , y ) .
5: 37.15 Orthogonal Polynomials on the Ball
For d = 2 the polynomial C ν 1 , ν 2 ( α + 1 2 ) ( x 1 , x 2 ) as defined by (37.15.4) becomes the polynomial C ν 2 , ν 1 + ν 2 ( α + 1 2 ) ( x 1 , x 2 ) as given by (37.4.5). … For d = 2 ball polynomials yield complex and real disk polynomials (37.4.11), (37.4.15):
37.15.9 R Y , k , n α ( r cos θ , r sin θ ) = { R n k , k α ( r e i θ , r e i θ ) if  Y = e i ( n 2 k ) θ , R k , n k α ( r e i θ , r e i θ ) if  Y = e i ( n 2 k ) θ , R n k , k α , ( c ) ( r cos θ , r sin θ ) if  Y = cos ( ( n 2 k ) θ ) , R n k , k α , ( s ) ( r cos θ , r sin θ ) if  Y = sin ( ( n 2 k ) θ ) ,
6: 11.12 Physical Applications
Applications of Struve functions occur in water-wave and surface-wave problems (Hirata (1975) and Ahmadi and Widnall (1985)), unsteady aerodynamics (Shaw (1985) and Wehausen and Laitone (1960)), distribution of fluid pressure over a vibrating disk (McLachlan (1934)), resistive MHD instability theory (Paris and Sy (1983)), and optical diffraction (Levine and Schwinger (1948)). …
7: 37.10 Other Orthogonal Polynomials of Two Variables
§37.10(i) Orthogonal polynomials on the Disk for Generalized Weight Function
on the unit disk, the OPs are fully developed. …
8: 37.6 Plane with Weight Function e x 2 y 2
§37.6(iv) Limits
The explicit basis functions in §37.4 of (bi)orthogonal polynomials on the unit disk for the weight function (37.4.2) all tend after rescaling, as α , to basis functions given above of OPs on 2 for the weight function e x 2 y 2 : …
37.6.16 lim α α 1 2 n C k , n ( α + 1 2 ) ( α 1 2 x , α 1 2 y ) = 1 ( n k ) ! k ! H n k ( x ) H k ( y ) ,
9: 18.1 Notation
  • Disk: R m , n ( α ) ( z ) .

  • 10: 16.23 Mathematical Applications
    The Bieberbach conjecture states that if n = 0 a n z n is a conformal map of the unit disk to any complex domain, then | a n | n | a 1 | . …