Non-thermal Hawking radiation from the Kerr black hole

被引：0

作者：

韩亦文 ^{[1
]}

郝加波 ^{[2
]}

机构：

[1] College of Computer Science, Chongqing Technology and Business University

[2] Department of Physics and Engineering Technology, Sichuan University of Arts and Science

来源：

Chinese Physics C | 2009年 / 02期

关键词：

black hole; Hawking radiation; Damour-Ruffini method; quantum theory;

D O I：

暂无

中图分类号：

P145.8 [塌缩星（黑洞）];

学科分类号：

070401 ;

摘要：

We present a short and direct derivation of Hawking radiation by using the Damour-Ruffini method, as taking into account the self-gravitational interaction from the Kerr black hole. It is found that the radiation is not exactly thermal, and because the derivation obeys conservation laws, the non-thermal Hawking radiation can carry information from the black hole. So it can be used to explain the black hole information paradox, and the process satisfies unitary.

引用

页码：94 / 97

页数：4