Hawking radiation from a dynamical Kerr-Newman black hole

被引:3
作者
Ding, Han [1 ]
Liu, Xian-Ming [1 ,2 ]
Liu, Wen-Biao [1 ]
机构
[1] Beijing Normal Univ, Inst Theoret Phys, Dept Phys, Beijing 100875, Peoples R China
[2] Hubei Univ Nationalities, Dept Phys, Enshi 445000, Hubei, Peoples R China
基金
中国国家自然科学基金;
关键词
THERMODYNAMICS; EVAPORATION;
D O I
10.1139/P11-036
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
After Hawking radiation from a Schwarzschild black hole is calculated using the Damour-Ruffini method, the tortoise coordinate transformation in a static black hole is extended to a dynamical axisymmetric black hole, such as a dynamical Kerr-Newman black hole. Under the generalized tortoise coordinate transformation, Hawking radiation from a dynamical Kerr-Newman black hole is obtained successfully. Moreover, it also seems to occur on the apparent horizon instead of the event horizon.
引用
收藏
页码:667 / 672
页数:6
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