General Tortoise Coordinate Transformation in a Dynamical Kerr-Newman Black Hole

被引:1
作者
Liu, Xian-Ming [1 ,2 ]
Cheng, Su-Jun [1 ,3 ]
Liu, Wen-Biao [1 ]
机构
[1] Beijing Normal Univ, Dept Phys, Inst Theoret Phys, Beijing 100875, Peoples R China
[2] Hubei Univ Nationalities, Dept Phys, Enshi 445000, Hubei, Peoples R China
[3] Xinxiang Univ, Dept Phys, Xinxiang 453000, Henan, Peoples R China
基金
中国国家自然科学基金;
关键词
Hawking radiation; Dynamical tortoise coordinate transformation; Dynamical Kerr-Newman black hole; The first law of thermodynamics; Apparent horizon; HAWKING RADIATION;
D O I
10.1007/s10773-011-0930-8
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Under the extended dynamical tortoise coordinate transformation, Damour-Ruffini method has been applied to calculate the charged particles' Hawking radiation from the apparent horizon of a dynamical Kerr-Newman black hole. It is shown that Hawking radiation is still purely thermal black body spectrum. Moreover, the temperature of Hawking radiation is corresponding to the apparent horizon surface gravity and the first law of thermodynamics can also be constructed successfully on the apparent horizon in the dynamical Kerr-Newman black hole.
引用
收藏
页码:518 / 525
页数:8
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