Superradiantly stable non-extremal Reissner-Nordstrom black holes
arXiv:1503.01221 · doi:10.1140/epjc/s10052-016-4157-y
Abstract
The superradiant stability is investigated for non-extremal Reissner-Nordstrom black hole. We use an algebraic method to demonstrate that all non-extremal Reissner-Nordstrom black holes are superradiantly stable against a charged massive scalar perturbation. This improves the results obtained before for non-extremal Reissner-Nordstrom black holes.
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Cited by in corpus (11)
- Superradiant stability of the Kerr black holes
- Analytic study of superradiant stability of Kerr-Newman black holes under charged massive scalar perturbation
- Extremal rotating black holes, scalar perturbation and superradiant stability
- Dyonic Reissner-Nordstrom Black Holes and Superradiant Stability
- Superradiant Instability of Extremal Black Holes in STU Supergravity
- No black hole bomb for D-dimensional extremal Reissner-Nordstrom black holes under charged massive scalar perturbation
- Superradiant stability of five and six-dimensional extremal Reissner-Nordstrom black holes
- Superradiant stability of Mutated Reissner-Nordström black holes
- Extremal Charged Black Holes and Superradiantly Unstable Quasinormal Modes
- Six-dimensional non-extremal Reissner-Nordstrom black hole, charged massive scalar perturbation and black hole bomb
- Higher-dimensional non-extremal Reissner-Nordstrom black holes, scalar perturbation and superradiance: an analytical study