large ρ
(0.002 seconds)
11—20 of 21 matching pages
11: 28.6 Expansions for Small
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►Numerical values of the radii of convergence of the power series (28.6.1)–(28.6.14) for are given in Table 28.6.1.
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Table 28.6.1: Radii of convergence for power-series expansions of eigenvalues of Mathieu’s equation.
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►It is conjectured that for large
, the radii increase in proportion to the square of the eigenvalue number ; see Meixner et al. (1980, §2.4).
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28.6.20
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12: 14.20 Conical (or Mehler) Functions
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§14.20(vii) Asymptotic Approximations: Large , Fixed
… ►§14.20(viii) Asymptotic Approximations: Large ,
… ►§14.20(ix) Asymptotic Approximations: Large ,
… ►and the variable is defined by … ►The interval is mapped one-to-one to the interval , with the points , , and corresponding to , , and , respectively. …13: 14.15 Uniform Asymptotic Approximations
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§14.15(i) Large , Fixed
… ►and … ►For asymptotic expansions and explicit error bounds, see Dunster (2003b). ►§14.15(iii) Large , Fixed
… ►14: 13.7 Asymptotic Expansions for Large Argument
§13.7 Asymptotic Expansions for Large Argument
… ►§13.7(ii) Error Bounds
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§13.7(iii) Exponentially-Improved Expansion
… ►For extensions to hyperasymptotic expansions see Olde Daalhuis and Olver (1995a).15: 18.39 Applications in the Physical Sciences
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►Now use spherical coordinates (1.5.16) with instead of , and assume the potential to be radial.
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►with and being those of (18.39.35), are then
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18.39.39
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►(where the minus sign is often omitted, as it arises as an arbitrary phase when taking the square root of the real, positive, norm of the wave function), allowing equation (18.39.37) to be rewritten in terms of the associated Coulomb–Laguerre polynomials .
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►A relativistic treatment becoming necessary as becomes large as corrections to the non-relativistic Schrödinger picture are of approximate order , being the dimensionless fine structure constant , where is the speed of light.
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16: 18.15 Asymptotic Approximations
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18.15.5
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18.15.7
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►For large
, fixed , and , Dunster (1999) gives asymptotic expansions of that are uniform in unbounded complex -domains containing .
…This reference also supplies asymptotic expansions of for large
, fixed , and .
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►These approximations apply when the parameters are large, namely and (subject to restrictions) in the case of Jacobi polynomials, in the case of ultraspherical polynomials, and in the case of Laguerre polynomials.
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17: 28.35 Tables
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National Bureau of Standards (1967) includes the eigenvalues , for with , and with ; Fourier coefficients for and for , , respectively, and various values of in the interval ; joining factors , for with (but in a different notation). Also, eigenvalues for large values of . Precision is generally 8D.
Blanch and Clemm (1969) includes eigenvalues , for , , , ; 4D. Also and for , , and , respectively; 8D. Double points for ; 8D. Graphs are included.
18: 2.6 Distributional Methods
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►To derive an asymptotic expansion of for large values of , with , we assume that possesses an asymptotic expansion of the form
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2.6.32
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►We now derive an asymptotic expansion of for large positive values of .
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19: 28.33 Physical Applications
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►We shall derive solutions to the uniform, homogeneous, loss-free, and stretched elliptical ring membrane with mass per unit area, and radial tension per unit arc length.
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28.33.1
►with , reduces to (28.32.2) with .
…If we denote the positive solutions of (28.33.3) by , then the vibration of the membrane is given by .
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►In particular, the equation is stable for all sufficiently large values of .
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20: 2.5 Mellin Transform Methods
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►Let be a locally integrable function on , that is, exists for all and satisfying .
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►Similarly, if and can be continued analytically to meromorphic functions in a right half-plane, and if the vertical line of integration can be translated to the right, then we obtain an asymptotic expansion for for large values of .
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►where denotes the Bessel function (§10.2(ii)), and is a large positive parameter.
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►for any satisfying .
Similarly, since can be continued analytically to a meromorphic function (when ) or to an entire function (when ), we can choose so that has no poles in .
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