An instability of higher-dimensional rotating black holes
An instability of higher-dimensional rotating black holes
We present the first example of a linearized gravitational instability of an asymptotically at vacuum black hole. We study perturbations of a Myers-Perry black hole with equal angular momenta in an odd number of dimensions. We find no evidence of any instability in five or seven dimensions, but in nine dimensions, for sufficiently rapid rotation, we find perturbations that grow exponentially in time. The onset of instability is associated with the appearance of time-independent perturbations which generically break all but one of the rotational symmetries. This is interpreted as evidence for the existence of a new 70-parameter family of black hole solutions with only a single rotational symmetry. We also present results for the Gregory-Laflamme instability of rotating black strings, demonstrating that rotation makes black strings more unstable.
Dias, Oscar J.C.
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Figueras, Pau
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Monteiro, Ricardo
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Reall, Harvey S.
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Santos, Jorge E.
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20 May 2010
Dias, Oscar J.C.
f01a8d9b-9597-4c32-9226-53a6e5500a54
Figueras, Pau
92a9d40b-4ed0-45c6-b7c4-e8f9b4addcdb
Monteiro, Ricardo
1dfb2954-9861-425f-82c5-75185a088b60
Reall, Harvey S.
63d30f86-ab43-437d-86d9-eed9d4469ef8
Santos, Jorge E.
88cca86d-9e1e-40a7-acba-f7986bd7f84b
Dias, Oscar J.C., Figueras, Pau, Monteiro, Ricardo, Reall, Harvey S. and Santos, Jorge E.
(2010)
An instability of higher-dimensional rotating black holes.
JHEP.
(doi:10.1007/JHEP05(2010)076).
Abstract
We present the first example of a linearized gravitational instability of an asymptotically at vacuum black hole. We study perturbations of a Myers-Perry black hole with equal angular momenta in an odd number of dimensions. We find no evidence of any instability in five or seven dimensions, but in nine dimensions, for sufficiently rapid rotation, we find perturbations that grow exponentially in time. The onset of instability is associated with the appearance of time-independent perturbations which generically break all but one of the rotational symmetries. This is interpreted as evidence for the existence of a new 70-parameter family of black hole solutions with only a single rotational symmetry. We also present results for the Gregory-Laflamme instability of rotating black strings, demonstrating that rotation makes black strings more unstable.
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Accepted/In Press date: 28 April 2010
Published date: 20 May 2010
Additional Information:
Copyright © 2010, SISSA, Trieste, Italy
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Local EPrints ID: 467506
URI: http://eprints.soton.ac.uk/id/eprint/467506
PURE UUID: 3a87f955-5cee-42c3-b6ab-7770437907a8
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Date deposited: 12 Jul 2022 16:32
Last modified: 17 Mar 2024 03:35
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Contributors
Author:
Pau Figueras
Author:
Ricardo Monteiro
Author:
Harvey S. Reall
Author:
Jorge E. Santos
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