Area law corrections from state counting and supergravity

被引：75

作者：

Cardoso, GL ^{[1
]}

de Wit, B

Mohaupt, T

机构：

[1] Univ Utrecht, Inst Theoret Phys, NL-3508 TA Utrecht, Netherlands

[2] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany

[3] Univ Halle Wittenberg, Fachbereich Phys, D-06099 Halle, Germany

来源：

CLASSICAL AND QUANTUM GRAVITY | 2000年 / 17卷 / 05期

关键词：

D O I：

10.1088/0264-9381/17/5/310

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Modifications of the Bekenstein-Hawking area law for black holes are crucial in order to find agreement between the microscopic entropy based on state counting and the macroscopic entropy based on an effective field theory ccmputation. We discuss this and related issues for the case of four-dimensional N = 2 supersymmetric black holes. We also briefly comment on the state counting for N = 4 and 8 black holes.

引用

页码：1007 / 1015

页数：9

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