Instability and new phases of higher-dimensional rotating black holes

被引：126

作者：

Dias, Oscar J. C. ^{[1
]}

Figueras, Pau ^{[2
,3
]}

Monteiro, Ricardo ^{[1
]}

Santos, Jorge E. ^{[1
]}

Emparan, Roberto ^{[4
,5
]}

机构：

[1] Univ Cambridge, Ctr Math Sci, DAMTP, Cambridge CB3 0WA, England

[2] Univ Durham, Ctr Particle Theory, Sci Labs, Durham DH1 3LE, England

[3] Univ Durham, Dept Math Sci, Sci Labs, Durham DH1 3LE, England

[4] ICREA, E-08010 Barcelona, Spain

[5] Univ Barcelona, Dept Fis Fonamental, E-08010 Barcelona, Spain

来源：

PHYSICAL REVIEW D | 2009年 / 80卷 / 11期

关键词：

STABILITY; SPACE;

D O I：

10.1103/PhysRevD.80.111701

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

It has been conjectured that higher-dimensional rotating black holes become unstable at a sufficiently large value of the rotation, and that new black holes with pinched horizons appear at the threshold of the instability. We search numerically and find the stationary axisymmetric perturbations of Myers-Perry black holes with a single spin that mark the onset of the instability and the appearance of the new black hole phases. We also find new ultraspinning Gregory-Laflamme instabilities of rotating black strings and branes.

引用

页数：5

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