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Black hole instabilities and local Penrose inequalities

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arxiv 1107.5785 v2 pith:HH324GQY submitted 2011-07-28 gr-qc hep-th

classification gr-qchep-th
keywords blackdatainitialinstabilityholeringsconstructfind
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Various higher-dimensional black holes have been shown to be unstable by studying linearized gravitational perturbations. A simpler method for demonstrating instability is to find initial data that describes a small perturbation of the black hole and violates a Penrose inequality. An easy way to construct initial data is by conformal rescaling of the unperturbed black hole initial data. For a compactified black string, we construct initial data which violates the inequality almost exactly where the Gregory-Laflamme instability appears. We then use the method to confirm the existence of the "ultraspinning" instability of Myers-Perry black holes. Finally we study black rings. We show that "fat" black rings are unstable. We find no evidence of any rotationally symmetric instability of "thin" black rings.

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  1. On turbulence for spacetimes with stable trapping

    gr-qc 2024-11 conditional novelty 7.0 of 10

    On a fixed spacetime with stable trapping, the cubic wave equation produces a forward angular-mode cascade and growth of higher-order derivatives, behavior absent for linear waves.

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