Charged rotating black holes in five dimensional U(1)3 gaugedN=2 supergravity -: art. no. 081502

被引：87

作者：

Cvetic, M ^{[1
]}

Lü, H

Pope, CN

机构：

[1] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA

[2] Texas A&M Univ, George P & Cynthia W Mitchell Inst Fundamental Ph, College Stn, TX 77843 USA

[3] Univ Sci & Technol China, Interdisciplinary Ctr Theoret Study, Hefei 230026, Anhui, Peoples R China

来源：

PHYSICAL REVIEW D | 2004年 / 70卷 / 08期

基金：

美国国家科学基金会; 中国国家自然科学基金;

关键词：

D O I：

10.1103/PhysRevD.70.081502

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We obtain the general solution for nonextremal 3-charge dilatonic rotating black holes in the five dimensional U(1)(3) gauged N=2 supergravity coupled to two vector multiplets, in the case where the two rotation parameters are set equal. These solutions encompass all the previously-known extremal solutions, and, by setting the three charges equal, the recently-obtained nonextremal solutions of N=2 gauged five dimensional pure supergravity.

引用

页码：081502 / 1

页数：4

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