On the gravitational stability of D1-D5-P black holes
On the gravitational stability of D1-D5-P black holes
We examine the stability of the nonextremal D1-D5-P black hole solutions. In particular, we look for the appearance of a superradiant instability for the spinning black holes but we find no evidence of such an instability. We compare this situation with that for the smooth soliton geometries, which were recently observed to suffer from an ergoregion instability, and consider the implications for the fuzzball proposal.
Cardoso, Vitor
08c1bdef-b56a-4067-ab37-89a9ece74fb7
Dias, Oscar J.C.
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Myers, Robert C.
2fafdbd1-8e40-4af3-8b69-d073b598a279
15 November 2007
Cardoso, Vitor
08c1bdef-b56a-4067-ab37-89a9ece74fb7
Dias, Oscar J.C.
f01a8d9b-9597-4c32-9226-53a6e5500a54
Myers, Robert C.
2fafdbd1-8e40-4af3-8b69-d073b598a279
Cardoso, Vitor, Dias, Oscar J.C. and Myers, Robert C.
(2007)
On the gravitational stability of D1-D5-P black holes.
Phys.Rev.D, 76, [105015].
(doi:10.1103/PhysRevD.76.105015).
Abstract
We examine the stability of the nonextremal D1-D5-P black hole solutions. In particular, we look for the appearance of a superradiant instability for the spinning black holes but we find no evidence of such an instability. We compare this situation with that for the smooth soliton geometries, which were recently observed to suffer from an ergoregion instability, and consider the implications for the fuzzball proposal.
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Published date: 15 November 2007
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© 2007 The American Physical Society
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Local EPrints ID: 468099
URI: http://eprints.soton.ac.uk/id/eprint/468099
PURE UUID: 8af71a45-7dfb-412b-85eb-36dd7effccd8
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Date deposited: 02 Aug 2022 17:04
Last modified: 17 Mar 2024 03:35
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Author:
Vitor Cardoso
Author:
Robert C. Myers
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