Hawking radiation of the Kerr-Newman black hole

被引:1
|
作者
Chen, DeYou [1 ]
Yang, ShuZheng [1 ]
机构
[1] China W Normal Univ, Inst Theoret Phys, Nanchong 637002, Peoples R China
关键词
self-gravitational interaction; tunneling probability; Hamilton-Jacobi equation;
D O I
10.1007/s10773-007-9420-4
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Considering the unfixed background space-time and self-gravitational interaction, we review the Hawking radiation of the Kerr-Newman black hole by Hamilton-Jacobi method. The result shows the tunneling probability is related to the change of Bekenstein-Hawking entropy and the radiation spectrum deviates from the precisely thermal one, which is in accordance with Parikh and Wilczek's result and gives another method to study the Hawking radiation of the black hole.
引用
收藏
页码:3067 / 3071
页数:5
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