On the gravitational stability of D1-D5-P black holes
arXiv:0707.3406 · 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.
arXiv comment18 pages, 3 figures. Minor comments added to match published version
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Cited by in corpus (15)
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- Radiation from the non-extremal fuzzball
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