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题名: SOME PROPERTIES OF ACCELERATING OBSERVERS IN THE SCHWARZSCHILD SPACE
作者: Hu, Yapeng ;  Tian, Guihua ;  Zhao, Zheng
刊名: MODERN PHYSICS LETTERS A
出版日期: 2009
卷号: 24, 期号:3, 页码:229-238
关键词: BLACK-HOLE EVAPORATION ;  THERMODYNAMICS ;  DERIVATION ;  RADIATION ;  FIELD
学科分类: Physics
通讯作者: Hu, YP , Chinese Acad Sci, Inst Theoret Phys, POB 2735, Beijing 100190, Peoples R China
部门归属: [Hu, YP] Chinese Acad Sci, Inst Theoret Phys, Beijing 100190, Peoples R China; [Hu, YP] Chinese Acad Sci, Grad Sch, Beijing 100039, Peoples R China; [Tian, GH] Beijing Univ Posts & Telecommun, Sch Sci, Beijing 100876, Peoples R China; [Zhao, Z] Beijing Normal Univ, Dept Phys, Beijing 100875, Peoples R China
英文摘要: It is well known that observers will be accelerated when they approach the planets. Thus, discussing the properties of accelerating observers in the Schwarzschild space is meaningful. For the sake of simplicity, we can construct these observers' worldlines by comparing with the observers in the Hawking effect and Unruh effect, whose worldlines are both hyperbolic curves in the appropriate coordinates. We do it after defining a certain special null hypersurface in the Kruskal coordinates. Our result shows that these accelerating observers defined in our paper can also detect the radiation with the analogy of the Unruheffect, though locally. Furthermore, we conjecture that, for any null hypersurface in any spacetime, the corresponding observers who can atleast locally detect the radiation from it can be found.
资助者: NSFC, China[10325525, 90403029]; Chinese Academy of Sciences; National Natural Science Foundation of China[10773002]; National Basic Research Program of China[2003CB716302]
收录类别: SCI
原文出处: 查看原文
WOS记录号: WOS:000263628300007
Citation statistics: 
内容类型: 期刊论文
URI标识: http://ir.itp.ac.cn/handle/311006/5403
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:
Hu, Yapeng,Tian, Guihua,Zhao, Zheng. SOME PROPERTIES OF ACCELERATING OBSERVERS IN THE SCHWARZSCHILD SPACE[J]. MODERN PHYSICS LETTERS A,2009,24(3):229-238.
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