Hawking radiation of a Reissner-Nordstrom-de Sitter black hole

被引：26
|
作者：
Zhao, Ren [1 ,2 ]
Zhang, Li-Chun [1 ,2 ]
Li, Huai-Fan [1 ,2 ]
机构：
[1] Shanxi Datong Univ, Inst Theoret Phys, Datong 037009, Peoples R China
[2] Shanxi Datong Univ, Dept Phys, Datong 037009, Peoples R China
来源：
GENERAL RELATIVITY AND GRAVITATION | 2010年 / 42卷 / 04期
关键词：
Damour-Ruffini method; Hawking radiation; Energy conversation; de Sitter spacetime; CARDY-VERLINDE FORMULA; SELF-GRAVITATIONAL CORRECTIONS; ENTROPY CORRECTION; DIRAC PARTICLES; SECRET TUNNEL; HORIZON; THERMODYNAMICS; TEMPERATURE; ANOMALIES; SPACES;
D O I：
10.1007/s10714-009-0893-8
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Generalizing the method proposed by Damour-Ruffini, we discuss Hawking radiation of a Reissner-Nordstrom-de Sitter (RNdS) black hole. Under the condition that total energy and charge are conserved, taking the reaction of the radiation of particles to the spacetime into consideration and considering the interrelation between the event horizon and cosmological horizon, we investigate radiation spectrum of RNdS spacetime by a new Tortoise coordinate transformation. This radiation spectrum is no longer a purely thermal spectrum. It is related to the changes in the Bekenstein-Hawking entropy corresponding the event horizon and cosmological horizon. The result satisfies the unitary principle.
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页码：975 / 983
页数：9
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