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题名: Quasinormal modes in Schwarzschild black holes due to arbitrary spin fields
作者: Shu, FW ;  Shen, YG
刊名: PHYSICS LETTERS B
出版日期: 2005
卷号: 619, 期号:40972, 页码:340-346
关键词: GRAVITATIONAL-RADIATION ;  WKB APPROACH ;  PERTURBATIONS ;  EQUATIONS ;  SCATTERING ;  SPECTRUM ;  MASS
学科分类: Physics
通讯作者: Shu, FW , Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China.
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
英文摘要: 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.
收录类别: SCI
原文出处: 查看原文
WOS记录号: WOS:000230373400019
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内容类型: 期刊论文
URI标识: http://ir.itp.ac.cn/handle/311006/13782
Appears in Collections:理论物理所1978-2010年知识产出_期刊论文

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Recommended Citation:
Shu, FW,Shen, YG. Quasinormal modes in Schwarzschild black holes due to arbitrary spin fields[J]. PHYSICS LETTERS B,2005,619(40972):340-346.
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