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Quasinormal modes in Schwarzschild black holes due to arbitrary spin fields
Shu, FW; Shen, YG; Shu, FW , Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China.
2005
发表期刊PHYSICS LETTERS B
ISSN0370-2693
卷号619期号:40972页码:340-346
摘要The Newman-Penrose formalism is used to deal with the massless scalar, neutrino, electromagnetic, gravitino and gravitational quasinormal modes (QNMs) in Schwarzschild black holes in a united form. The quasinormal mode frequencies evaluated by using the 3rd-order WKB potential approximation show that the boson perturbations and the fermion perturbations behave in a contrary way for the variation of the oscillation frequencies with spin, while this is no longer true for the damping's, which variate with s in a same way both for boson and fermion perturbations. (c) 2005 Elsevier B.V. All rights reserved.
部门归属Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China; Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China; Chinese Acad Sci, Inst Theoret Phys, Beijing 100080, Peoples R China; Chinese Acad Sci, Grad Sch, Beijing 100039, Peoples R China
关键词Gravitational-radiation Wkb Approach Perturbations Equations Scattering Spectrum Mass
学科领域Physics
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收录类别SCI
WOS记录号WOS:000230373400019
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被引频次:10[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.itp.ac.cn/handle/311006/13782
专题理论物理所1978-2010年知识产出
通讯作者Shu, FW , Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China.
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Shu, FW,Shen, YG,Shu, FW , Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China.. Quasinormal modes in Schwarzschild black holes due to arbitrary spin fields[J]. PHYSICS LETTERS B,2005,619(40972):340-346.
APA Shu, FW,Shen, YG,&Shu, FW , Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China..(2005).Quasinormal modes in Schwarzschild black holes due to arbitrary spin fields.PHYSICS LETTERS B,619(40972),340-346.
MLA Shu, FW,et al."Quasinormal modes in Schwarzschild black holes due to arbitrary spin fields".PHYSICS LETTERS B 619.40972(2005):340-346.
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