中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Quasinormal modes of Rarita-Schwinger field in Reissner-Nordstrom black hole spacetimes

文献类型:期刊论文

作者Shu, FW; Shen, YG
刊名PHYSICS LETTERS B
出版日期2005-05-19
卷号614期号:3-4页码:195-200
关键词black hole QNMs Rarita-Schwinger field Reissner-Nordstrom WKB approximation
英文摘要The Newman-Penrose formalism is used to deal with the quasinormal modes (QNMs) of Rarita-Schwinger perturbations outside a Reissner-Nordstr6m black hole. We obtain four kinds of possible expressions of effective potentials, which are proved to be of the same spectra of quasinormal mode frequencies. The quasinormal mode frequencies evaluated by the WKB potential approximation show that, similar to those for Dirac perturbations, the real parts of the frequencies increase with the charge Q and decrease with the mode number n, while the dampings almost keep unchanged as the charge increases. (c) 2005 Elsevier B.V. All rights reserved.
WOS标题词Science & Technology ; Physical Sciences
学科主题星系和宇宙学研究中心
类目[WOS]Physics, Multidisciplinary
研究领域[WOS]Physics
关键词[WOS]WKB APPROACH ; PERTURBATIONS ; SCATTERING ; RADIATION ; EQUATIONS ; SPECTRUM
收录类别SCI
语种英语
WOS记录号WOS:000229415700010
公开日期2010-11-08
源URL[http://119.78.226.72//handle/331011/11674]  
专题上海天文台_星系宇宙学重点实验室
作者单位1.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
3.Chinese Acad Sci, Inst Theoret Phys, Beijing 100080, Peoples R China
4.Chinese Acad Sci, Grad Sch, Beijing 100039, Peoples R China
推荐引用方式
GB/T 7714
Shu, FW,Shen, YG. Quasinormal modes of Rarita-Schwinger field in Reissner-Nordstrom black hole spacetimes[J]. PHYSICS LETTERS B,2005,614(3-4):195-200.
APA Shu, FW,&Shen, YG.(2005).Quasinormal modes of Rarita-Schwinger field in Reissner-Nordstrom black hole spacetimes.PHYSICS LETTERS B,614(3-4),195-200.
MLA Shu, FW,et al."Quasinormal modes of Rarita-Schwinger field in Reissner-Nordstrom black hole spacetimes".PHYSICS LETTERS B 614.3-4(2005):195-200.

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