Entropy-product rules for charged rotating black holes

被引:40
作者
Cvetic, M. [1 ,2 ]
Lu, H. [3 ]
Pope, C. N. [4 ,5 ]
机构
[1] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA
[2] Univ Maribor, Ctr Appl Math & Theoret Phys, SI-2000 Maribor, Slovenia
[3] Beijing Normal Univ, Dept Phys, Beijing 100875, Peoples R China
[4] Texas A&M Univ, George & Cynthia Woods Mitchell Inst Fundamental, College Stn, TX 77843 USA
[5] Univ Cambridge, Ctr Math Sci, DAMTP, Cambridge CB3 OWA, England
来源
PHYSICAL REVIEW D | 2013年 / 88卷 / 04期
关键词
GREYBODY FACTORS;
D O I
10.1103/PhysRevD.88.044046
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the universal nature of the product of the entropies of all horizons of charged rotating black holes. We argue, by examining further explicit examples, that when the maximum number of rotations and/or charges are turned on, the entropy product is expressed in terms of angular momentum and/or charges only, which are quantized. (In the case of gauged supergravities, the entropy product depends on the gauge-coupling constant also.) In two-derivative gravities, the notion of the "maximum number" of charges can be defined as being sufficiently many nonzero charges that the Reissner-Nordstrom black hole arises under an appropriate specialization of the charges. (The definition can be relaxed somewhat in charged anti-de Sitter black holes in D >= 6.) In higher-derivative gravity, we use the charged rotating black hole in Weyl-Maxwell gravity as an example for which the entropy product is still quantized, but it is expressed in terms of the angular momentum only, with no dependence on the charge. This suggests that the notion of maximum charges in higher-derivative gravities requires further understanding.
引用
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页数:11
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