A General Way for Determining Hawking Effect in Spherically Symmetric or Plane-symmetric Non-static Space-Times

作     者：赵峥 

作者机构：Department of PhysicsBeijing Normal UniversityBeijing 100875PRC 

出 版 物：《Science China Mathematics》 (中国科学：数学（英文版）)

年 卷 期：1993年第36卷第3期

页      面：300-311页

核心收录：

学科分类：07[理学] 08[工学] 

基　　金：Project supported by the National Natural Science Foundation of China 

主　　题：Hawking radiation black hole non-static space-time tortoise coordinate 

摘      要：A new general way for researching the Hawking effect in the spheri-cally symmetric or the plane-symmetric non-static space-times is *** theoreticalfoundation of this way is *** Klein-Gordon equation must be reduced to the stand-ard form of wave equation near an event horizon when a generalized tortoise coordinateis ***,both the Hawking radiation temperature and the equation determining thelocation of the event horizon are obtained *** the radiation is weak,thefirst approximation of our result is the same as the approximate result obtained with theradiation back-reaction method.