Unthermal Hawking Radiation from a General Stationary Black Hole  

作　　者：ZHANG Yong-Ping DAI Qian LIU Wen-Biao 

机构地区：[1]Department of Physics, Institute of Theoretical Physics, Beijing Normal University, Beijing 100875, China

出　　处：《Communications in Theoretical Physics》2008年第2期379-381,共3页理论物理通讯（英文版）

基　　金：the National Basic Research Program of China under Grant No.2003CB716302;the National Natural Science Foundation of China under Grant No.10773002

摘　　要：Using Damour-Ruflini＇s method, Hawking radiation from a general stationary black hole is investigated again deeply. Considering the back reaction of the particle to the space-time and energy conservation, we find that the radiation is not exactly thermal and can take out information from the black hole. This can be used to explain the information loss paradox, and the result is consistent with the works finished before.

关 键 词：Hawking radiation stationary black hole BACK-REACTION information loss paradox unitary theory 

分 类 号：P145.8[天文地球—天体物理]