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 multistage process with distinct superradiant instabilities.
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| http://dx.doi.org/10.1103/PhysRevLett.122.181101 | DOI Listing |
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