THE PHYSICS OF ELEMENTARY PARTICLES AND FIELDS |
Prev
Next
|
|
|
Low frequency asymptotics for the spin-weighted spheroidal equation in the case of s=1/2 |
Dong Kun(董锟)†, Tian Gui-Hua(田贵花), and Sun Yue(孙越) |
School of Science, Beijing University of Posts and Telecommunications, Beijing 100876, China |
|
|
Abstract The spin-weighted spheroidal equation in the case of s=1/2 is thoroughly studied by using the perturbation method from the supersymmetric quantum mechanics. The first-five terms of the superpotential in the series of parameter β are given. The general form for the n-th term of the superpotential is also obtained, which could also be derived from the previous terms Wk, k < n. From these results, it is easy to obtain the ground eigenfunction of the equation. Furthermore, the shape-invariance property in the series of parameter β is investigated and is proven to be kept. This nice property guarantees that the excited eigenfunctions in the series form can be obtained from the ground eigenfunction by using the method from the supersymmetric quantum mechanics. We show the perturbation method in supersymmetric quantum mechanics could completely solve the spin-weight spheroidal wave equations in the series form of the small parameter β.
|
Received: 20 December 2010
Revised: 08 March 2011
Accepted manuscript online:
|
PACS:
|
11.30.Pb
|
(Supersymmetry)
|
|
04.25.Nx
|
(Post-Newtonian approximation; perturbation theory; related Approximations)
|
|
03.65.Ge
|
(Solutions of wave equations: bound states)
|
|
02.30.Gp
|
(Special functions)
|
|
Cite this article:
Dong Kun(董锟), Tian Gui-Hua(田贵花), and Sun Yue(孙越) Low frequency asymptotics for the spin-weighted spheroidal equation in the case of s=1/2 2011 Chin. Phys. B 20 071101
|
[1] |
Teukolsky S A 1972 Phys. Rev. Lett. 29 1114
|
[2] |
Teukolsky S A 1973 Astrophys. J. 185 635
|
[3] |
Berti E, Cardoso V and Casals M 2006 Phys. Rev. D 73 024013
|
[4] |
Leaver E W 1986 J. Math. Phys. 27 1238
|
[5] |
Breuer R, Ryan Jr M and Waller S 1977 Proc. R. Soc. Lond. A 358 71
|
[6] |
Casals M and Ottewill A C 2005 Phys. Rev. D 71 064025
|
[7] |
Press W H and Teukolsky S A 1973 Astrophys. J. 185 649
|
[8] |
Fackerell E D and Grossman R G 1977 J. Math. Phys. 18 1849
|
[9] |
Fujita R and Tagoshi H 2004 arXiv:gr-qc/0410018 v1 5
|
[10] |
Tian G H 2010 Chin. Phys. Lett. 27 030308
|
[11] |
Tian G H 2005 Chin. Phys. Lett. 22 3013
|
[12] |
Tian G H and Zhong S Q 2010 Chin. Phys. Lett. 27 040305
|
[13] |
Tian G H and Zhong S Q 2009 arXiv: 0906.4687 V3
|
[14] |
Tian G H and Zhong S Q 2010 Chin. Phys. Lett. 27 100306
|
[15] |
Tang W L and Tian G H 2011 Chin. Phys. B 20 050301
|
[16] |
Zhou J, Tian G H and Tang W L 2010 J. Math. Phys. (submitted)
|
[17] |
Tang W L and Tian G H 2011 Chin. Phys. B 20 010304
|
[18] |
Li K, Sun Y, Tian G H and Tang W L 2010 Sci. Chin. Ser. G (preprint) (in Chinese)
|
[19] |
Dong K, Tian G H and Sun Y 2010 arXiv: 1011.2579
|
[20] |
Gradsbteyn I S and Ryzbik L M 2000 Table of Integrals, Series, and Products 6th edn. (Singapore: Elsevierpte. Ltd)
|
[21] |
Cooper F, Khare A and Sukhatme U 1995 Phys. Rep. 251 268
|
No Suggested Reading articles found! |
|
|
Viewed |
|
|
|
Full text
|
|
|
|
|
Abstract
|
|
|
|
|
Cited |
|
|
|
|
Altmetric
|
blogs
Facebook pages
Wikipedia page
Google+ users
|
Online attention
Altmetric calculates a score based on the online attention an article receives. Each coloured thread in the circle represents a different type of online attention. The number in the centre is the Altmetric score. Social media and mainstream news media are the main sources that calculate the score. Reference managers such as Mendeley are also tracked but do not contribute to the score. Older articles often score higher because they have had more time to get noticed. To account for this, Altmetric has included the context data for other articles of a similar age.
View more on Altmetrics
|
|
|