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

Journal Article · Thu Nov 15 00:00:00 EST 2007 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PHYSREVD.76.105015· OSTI ID:21027893

Cardoso, Vitor; Dias, Oscar J. C.; Myers, Robert C ^[1]

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1. Department of Physics and Astronomy, University of Mississippi, University, Mississippi 38677-1848 (United States)

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.

• OSTI ID: 21027893
• Journal Information: Physical Review. D, Particles Fields, Vol. 76, Issue 10; Other Information: DOI: 10.1103/PhysRevD.76.105015; (c) 2007 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
BLACK HOLES
COMPARATIVE EVALUATIONS
COSMOLOGY
GEOMETRY
INSTABILITY
MATHEMATICAL SOLUTIONS
SOLITONS
STABILITY