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arXiv · 2206.02128

Probing inside a charged hairy black hole in massive gravity

Mirmani Mirjalali·Seyed Ali Hosseini Mansoori·Leila Shahkarami·Morteza Rafiee
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Abstract

In this paper, we investigate the internal structure of a charged hairy black hole solution in the non-linear massive gravity. We first consider the impact of various configurations of massive gravity on the condensate operator and then probe the black hole interior dynamics. Like a standard holographic superconductor system, just below the critical temperature, the interior evolves through several distinct epochs, including a collapse of the Einstein-Rosen bridge, Josephson oscillations of the scalar field, and finally a Kasner (or Kasner inversion) cosmology. However, for the large massive gravity parameter, we see distinguishing features for the interior dynamics. In this regime, at a given temperature, the Einstein-Rosen bridge collapse and subsequent Josephson oscillations epochs completely disappear from the interior dynamics and the final Kasner cosmology epoch starts exactly after the would-be inner horizon and the system does not experience the Kasner inversion epoch.

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Mirmani Mirjalali, Seyed Ali Hosseini Mansoori, Leila Shahkarami, Morteza Rafiee. 2022-06-05. Probing inside a charged hairy black hole in massive gravity. https://doi.org/10.1007/jhep09(2022)222

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