探讨黑洞Hawking辐射的新方法——量子统计法  

A new method for exploring the black hole Hawking radiation—— the quantum statistical method

作　　者：赵仁[1] 张丽春[2] 胡双启[1] 

机构地区：[1]中北大学环境与安全工程系,太原030051 [2]山西大同大学物理系,大同037009

出　　处：《物理学报》2006年第8期3898-3901,共4页Acta Physica Sinica

基　　金：山西省自然科学基金(批准号:2006011012)资助的课题.~~

摘　　要：将黑洞看作由裸黑洞和二维热力学面(黑洞的视界)组成的正则系综,利用量子统计方法给出黑洞Hawking辐射的能量谱.找到黑洞辐射温度与熵的关系.When we take the black hole as a canonical ensemble composed of a naked black hole and the two-dimensional thermodynamic surface （horizon of the black hole）, using the quantum statistical method, we derive the energy spectrum of the black hole Hawking radiation. The relation between the radiation temperature of the black hole and the entropy is obtained. This gives an insight into the process of the black hole Hawking radiation.

关 键 词：HAWKING辐射 正则系统 量子统计 

分 类 号：P145.8[天文地球—天体物理]