Asymptotic quasinormal frequencies of different spin fields in spherically symmetric black holes

doi:10.1103/PhysRevD.73.024019

淡江大學機構典藏 > 理學院 > 物理學系暨研究所 > 期刊論文 > Item 987654321/27838

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题名:	Asymptotic quasinormal frequencies of different spin fields in spherically symmetric black holes
作者:	Cho, Hing Tong
贡献者:	淡江大學物理學系
日期:	2006-01
上传时间:	2013-07-09 15:15:59 (UTC+8)
出版者:	College Park: American Physical Society
摘要:	We consider the asymptotic quasinormal frequencies of various spin fields in Schwarzschild and Reissner-Nordstr\"om black holes. In the Schwarzschild case, the real part of the asymptotic frequency is ln3 for the spin 0 and the spin 2 fields, while for the spin 1/2, the spin 1, and the spin 3/2 fields it is zero. For the non-extreme charged black holes, the spin 3/2 Rarita-Schwinger field has the same asymptotic frequency as that of the integral spin fields. However, the asymptotic frequency of the Dirac field is different, and its real part is zero. For the extremal case, which is relevant to the supersymmetric consideration, all the spin fields have the same asymptotic frequency, the real part of which is zero. For the imaginary parts of the asymptotic frequencies, it is interesting to see that it has a universal spacing of $1/4M$ for all the spin fields in the single-horizon cases of the Schwarzschild and the extreme Reissner-Nordstr\"om black holes. The implications of these results to the universality of the asymptotic quasinormal frequencies are discussed.
關聯:	Physical Review D (Particles, Fields, Gravitation and Cosmology) 73(2), 024019(7pages)
DOI:	10.1103/PhysRevD.73.024019
显示于类别:	[物理學系暨研究所] 期刊論文

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