STATISTICAL-MECHANICS OF BLACK-HOLES

被引：89

作者：

HARMS, B

LEBLANC, Y

机构：

[1] Department of Physics and Astronomy, University of Alabama, Box 870324, Tuscaloosa

来源：

PHYSICAL REVIEW D | 1992年 / 46卷 / 06期

关键词：

D O I：

10.1103/PhysRevD.46.2334

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We analyze the statistical mechanics of a gas of neutral and charged black holes. The microcanonical ensemble is the only possible approach to this system, and the equilibrium configuration is the one for which most of the energy is carried by a single black hole. Schwarzschild black holes are found to obey the statistical bootstrap condition. In all cases, the microcanonical temperature is identical to the Hawking temperature of the most massive black hole in the gas. I(1) charges in general break the bootstrap property. The problems of black-hole decay and of quantum coherence are also addressed.

引用

页码：2334 / 2340

页数：7

共 15 条

[1] BLACK HOLES AND ENTROPY [J].