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Post-radiation evolution of black holes | | G. A. Vilkovisky
; | | Date: |
22 Mar 2008 | | 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. | | Source: | arXiv, 0803.3280 | | Services: | Forum | Review | PDF | Favorites | |
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