Gravitational instability of simply rotating AdS black holes in higher dimensions
arXiv:0812.0445 · doi:10.1103/PhysRevD.79.044003
Abstract
We study the stability of AdS black hole holes rotating in a single two plane for tensor-type gravitational perturbations in space-time dimensions. First, by an analytic method, we show that there exists no unstable mode when the magnitude of the angular momentum is smaller than where is the horizon radius, and is the AdS curvature radius. Then, by numerical calculations of quasinormal modes, using the separability of the relevant perturbation equations, we show that an instability occurs for rapidly rotating black holes with , although the growth rate is tiny (of order of the inverse horizon radius). We give numerical evidences indicating that this instability is caused by superradiance.
17 pages
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