Post-radiation evolution of black holes
Abstract
Description
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.
19 pages, 2 figures. Latex 2.09. Figures PostScript
19 pages, 2 figures. Latex 2.09. Figures PostScript