Rotating black holes in higher dimensions with a cosmological constant -: art. no. 171102

被引：266

作者：

Gibbons, GW

Lü, H

Page, DN

Pope, CN

机构：

[1] Univ Cambridge, Ctr Math Sci, DAMTP, Cambridge CB3 OWA, England

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

[3] Univ Alberta, Inst Theoret Phys, Phys Lab 412, Edmonton, AB T6G 2J1, Canada

来源：

PHYSICAL REVIEW LETTERS | 2004年 / 93卷 / 17期

基金：

加拿大自然科学与工程研究理事会;

关键词：

D O I：

10.1103/PhysRevLett.93.171102

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We present the metric for a rotating black hole with a cosmological constant and with arbitrary angular momenta in all higher dimensions. The metric is given in both Kerr-Schild and the Boyer-Lindquist form. In the Euclidean-signature case, we also obtain smooth compact Einstein spaces on associated SD-2 bundles over S-2, infinitely many for each odd Dgreater than or equal to5. Applications to string theory and M-theory are indicated.

引用

页码：171102 / 1

页数：4

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