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Inner Mechanics of 3d Black Holes

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arxiv 1204.6088 v1 pith:YLSV2KP7 submitted 2012-04-27 hep-th

classification hep-th
keywords blackinnerholesgravityhorizonhorizonswarpedagreement
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We investigate properties of the inner horizons of certain black holes in higher-derivative three-dimensional gravity theories. We focus on BTZ and Spacelike Warped Anti-de Sitter black holes, as well as on asymptotically Warped de-Sitter solutions exhibiting both a cosmological and a black hole horizon. We verify that a First Law is satisfied at the Inner horizon, in agreement with the proposal of \cite{Castro:2012av}. We then show that, in Topologically Massive Gravity, the product of the areas of the inner and outer horizons fails to be independent on the mass, and trace this to the diffeomorphism anomaly of the theory.

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  1. Timelike and gravitational anomalous entanglement from the inner horizon

    hep-th 2024-12 conditional novelty 7.0 of 10

    The inner horizon of Rindler AdS3 maps to the inner RT surface, which encodes timelike entanglement entropy and gravitational anomaly corrections to holographic entanglement.

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