Ultraspinning instability: the missing link

被引:31
作者
Dias, Oscar J. C. [1 ]
Monteiro, Ricardo [2 ]
Santos, Jorge E. [3 ]
机构
[1] Univ Cambridge, Ctr Math Sci, DAMTP, Cambridge CB3 0WA, England
[2] Niels Bohr Int Acad, Niels Bohr Inst, DK-2100 Copenhagen, Denmark
[3] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2011年 / 08期
基金
美国国家科学基金会;
关键词
Black Holes; Classical Theories of Gravity; BLACK-HOLES; THERMODYNAMIC STABILITY; SPACE; BRANES;
D O I
10.1007/JHEP08(2011)139
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We study linearized perturbations of Myers-Perry black holes in d = 7, with two of the three angular momenta set to be equal, and show that instabilities always appear before extremality. Analogous results are expected for all higher odd d. We determine numerically the stationary perturbations that mark the onset of instability for the modes that preserve the isometries of the background. The onset is continuously connected between the previously studied sectors of solutions with a single angular momentum and solutions with all angular momenta equal. This shows that the near-extremality instabilities are of the same nature as the ultraspinning instability of d >= 6 singly-spinning solutions, for which the angular momentum is unbounded. Our results raise the question of whether there are any extremal Myers-Perry black holes which are stable in d >= 6.
引用
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页数:21
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