Hawking radiation via tunnelling from general stationary axisymmetric black holes  

作　　者：张靖仪 樊军辉 

机构地区：[1]Center for Astrophysics, Guangzhou University, Guangzhou 510006, China

出　　处：《Chinese Physics B》2007年第12期3879-3884,共6页中国物理B（英文版）

基　　金：Project supported by the National Natural Science Foundation of China （Grant Nos 10573005 and 10633010）.

摘　　要：Hawking radiation is viewed as a tunnelling process. In this way the emission rates of massless particles and massive particles tunnelling across the event horizon of general stationary axisymmetric black holes are calculated, separately. The emission spectra of these two different kinds of outgoing particles have the same functional form and both are consistent with an underlying unitary theory.Hawking radiation is viewed as a tunnelling process. In this way the emission rates of massless particles and massive particles tunnelling across the event horizon of general stationary axisymmetric black holes are calculated, separately. The emission spectra of these two different kinds of outgoing particles have the same functional form and both are consistent with an underlying unitary theory.

关 键 词：black hole Hawking radiation quantum theory 

分 类 号：O45[理学—无线电物理]