Nonlinear evolution of the AdS black hole bomb
arXiv:1801.09711 · doi:10.1103/PhysRevLett.122.181101
Abstract
The superradiant instability of rotating black holes with negative cosmological constant is studied by numerically solving the full 3+1-dimensional Einstein equations. We find evidence for an epoch dominated by a solution with a single helical Killing vector and a multi-stage process with distinct superradiant instabilities.
5 pages + 2 pages supplemental materials. v2: added ref and minor clarifications in discussion
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