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On the gravitational stability of D1-D5-P black holes

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.
f01a8d9b-9597-4c32-9226-53a6e5500a54
Myers, Robert C.
2fafdbd1-8e40-4af3-8b69-d073b598a279
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).

Record type: Article

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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More information

Published date: 15 November 2007
Additional Information: © 2007 The American Physical Society

Identifiers

Local EPrints ID: 468099
URI: http://eprints.soton.ac.uk/id/eprint/468099
PURE UUID: 8af71a45-7dfb-412b-85eb-36dd7effccd8
ORCID for Oscar J.C. Dias: ORCID iD orcid.org/0000-0003-4855-4750

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Date deposited: 02 Aug 2022 17:04
Last modified: 17 Mar 2024 03:35

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Contributors

Author: Vitor Cardoso
Author: Oscar J.C. Dias ORCID iD
Author: Robert C. Myers

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