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

被引:255
|
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
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
收藏
页码:171102 / 1
页数:4
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