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Four-Dimensional Asymptotically AdS Black Holes with Scalar Hair

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arxiv 1309.2161 v2 pith:VWLLIFWR submitted 2013-09-09 gr-qc hep-th

P. A. Gonzalez , Eleftherios Papantonopoulos , Joel Saavedra , Yerko Vasquez This is my paper · ORCID
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keywords scalarblackholeasymptoticallyfieldfour-dimensionalhairpotential
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We present a new family of asymptotically AdS four-dimensional black hole solutions with scalar hair of a gravitating system consisting of a scalar field minimally coupled to gravity with a self-interacting potential. For a certain profile of the scalar field we solve the Einstein equations and we determine the scalar potential. Thermodynamically we show that there is a critical temperature below which there is a phase transition of a black hole with hyperbolic horizon to the new hairy black hole configuration.

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  1. Static and Dynamic Charged Black Holes

    hep-th 2019-08 conditional novelty 6.0 of 10

    Exact charged black hole solutions, static and time-dependent, are built in a class of reverse-engineered Einstein-Maxwell-dilaton theories, with explicit collapse from a smaller to a larger black hole.

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