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Exact formation of hairy planar black holes

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arxiv 1512.09145 v3 pith:HMCIBGLZ submitted 2015-12-30 hep-th

classification hep-th
keywords blacksolutionsclassesholesspace-timeclassdescribedynamical
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abstract

We consider Einstein gravity minimally coupled to a scalar field with a given potential in general dimensions. We obtain large classes of static hairy planar black holes which are asymptotic to AdS space-times. In particular, for a special case $\mu=(n-2)/2$, we obtain new classes of exact dynamical solutions describing black holes formation. We find there are two classes of collapse solutions. The first class solutions describe the evolution start from AdS space-time with a naked singularity at the origin. The space-time is linearly unstable and evolves into stationary black hole states even under small perturbation. The second class solutions describe the space-time spontaneously evolves from AdS vacua into stationary black hole states undergoing non-linear instability. We also discuss the global properties of all these dynamical solutions.

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Cited by 1 Pith paper

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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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