The Bekenstein-Hawking entropy of higher-dimensional rotating black holes

被引：1

作者：

Ma, Zheng Ze ^{[1
]}

机构：

[1] SE Univ, Dept Phys, Nanjing 210096, Peoples R China

来源：

PROGRESS OF THEORETICAL PHYSICS | 2006年 / 115卷 / 05期

关键词：

D O I：

10.1143/PTP.115.863

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

A black hole can be regarded as a thermodynamic system described by a grand canonical ensemble. In this paper, we study the Bekenstein-Hawking entropy of higher-dimensional rotating black holes using the Euclidean path-integral method of Gibbons and Hawking. We give a general proof demonstrating that ignoring quantum corrections, the Bekenstein-Hawking entropy is equal to one-fourth of its horizon area for general higher-dimensional rotating black holes.

引用

页码：863 / 871

页数：9

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