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.
18 pages, 3 figures. Minor comments added to match published version
References in corpus (6)
- Gravitational Perturbations of Higher Dimensional Rotating Black Holes: Tensor Perturbations
- Fuzzballs with internal excitations
- Mergers and Typical Black Hole Microstates
- Fuzzball solutions for black holes and D1-brane--D5-brane microstates
- The Foaming Three-Charge Black Hole
- Superradiant instability of large radius doubly spinning black rings
Cited by in corpus (8)
- The fuzzball proposal for black holes
- Radiation from the non-extremal fuzzball
- Non-supersymmetric microstates of the D1-D5-KK system
- Microscopic Theory of Black Hole Superradiance
- Pair creation in non-extremal fuzzball geometries
- Analyzing the squeezed state generated by a twist deformation
- Quasinormal modes of supersymmetric microstate geometries from the D1-D5 CFT
- Unwinding of strings thrown into a fuzzball