Post-radiation evolution of black holes

Details Post-radiation evolution of black holes Post-radiation evolution of black holes

2008-03-22

arxiv.org/abs/0803.3280v1

Phys.Rev.D77:124043,2008

Physics

High Energy Physics

High Energy Physics - Theory

19 pages, 2 figures. Latex 2.09. Figures PostScript

Scientific paper

10.1103/PhysRevD.77.124043

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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