Black to white transition of a charged black hole

Abstract

We present an exact solution of the Maxwell-Einstein equations, which describes the exterior of a charged spherical mass collapsing into its own trapping horizon and then bouncing back from an anti-trapping horizon at the same space location of the same asymptotic region. The solution is locally but not globally isometric to the maximally extended Reissner-Nordström metric and depends on seven parameters. It is regular, and defined everywhere except for a small region, where quantum tunnelling is expected. This region lies outside the mass: the mass-bounce and its near exterior are governed by classical general relativity. We discuss the relevance of this result for the fate of realistic black holes. We comment on possible effects of the classical instabilities and the Hawking radiation.

arXiv comment12 pages, 13 figures

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• The landscape of polymer quantum cosmology
• Symmetric black-to-white hole solutions with a cosmological constant
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• Testing loop quantum gravity by quasi-periodic oscillations: rotating blackholes
• A spin foam framework for the black-to-white hole transition