Small Kerr–anti-de Sitter black holes are unstable
- 12 October 2004
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 70 (8) , 084011
Abstract
Superradiance in black hole spacetimes can trigger instabilities. Here we show that, due to superradiance, small Kerr–anti-de Sitter black holes are unstable. Our demonstration uses a matching procedure, in a long wavelength approximation.Keywords
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This publication has 21 references indexed in Scilit:
- Black-hole bomb and superradiant instabilitiesPhysical Review D, 2004
- Charged and rotating AdS black holes and their CFT dualsPhysical Review D, 1999
- A comment on the eigenvalues of spin-weighted spheroidal functionsClassical and Quantum Gravity, 1989
- The Klein paradox and superradianceAnnals of Physics, 1988
- Klein-Gordon equation and rotating black holesPhysical Review D, 1980
- Rotating Black Holes: Locally Nonrotating Frames, Energy Extraction, and Scalar Synchrotron RadiationThe Astrophysical Journal, 1972
- Rotating Black Holes: Separable Wave Equations for Gravitational and Electromagnetic PerturbationsPhysical Review Letters, 1972
- Floating Orbits, Superradiant Scattering and the Black-hole BombNature, 1972
- Solution of the Scalar Wave Equation in a Kerr Background by Separation of VariablesPhysical Review D, 1972
- Stability of a Schwarzschild SingularityPhysical Review B, 1957