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arXiv · 0803.3280

Post-radiation evolution of black holes

G. A. Vilkovisky
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Abstract

The expectation-value equations for the collapse of a macroscopic, spherically symmetric, and uncharged body are integrated up to the limit of validity of semiclassical theory. The collapse finishes with a true stable black hole of the mass microscopically exceeding the vacuum-induced charge. The apparent horizon is almost closed. The most important feature of the solution is the presence of an irremovable Cauchy horizon.

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G. A. Vilkovisky. 2008-03-22. Post-radiation evolution of black holes. https://doi.org/10.1103/physrevd.77.124043

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