BLACK-HOLE IN 3-DIMENSIONAL SPACETIME

被引：2874

作者：

BANADOS, M

TEITELBOIM, C

ZANELLI, J

机构：

[1] INST ADV STUDY, PRINCETON, NJ 08540 USA

[2] UNIV CHILE, FAC CIENCIAS, SANTIAGO, CHILE

来源：

PHYSICAL REVIEW LETTERS | 1992年 / 69卷 / 13期

关键词：

D O I：

10.1103/PhysRevLett.69.1849

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The standard Einstein-Maxwell equations in 2+1 spacetime dimensions, with a negative cosmological constant, admit a black hole solution. The 2+1 black hole-characterized by mass, angular momentum, and charge, defined by flux integrals at infinity-is quite similar to its 3+1 counterpart. Anti-de Sitter space appears as a negative energy state separated by a mass gap from the continuous black hole spectrum. Evaluation of the partition function yields that the entropy is equal to twice the perimeter length of the horizon.

引用

页码：1849 / 1851

页数：3

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