Will black holes eventually engulf the universe?
arXiv:astro-ph/0603761 · doi:10.1016/j.physletb.2006.07.067
Abstract
The Babichev-Dokuchaev-Eroshenko model for the accretion of dark energy onto black holes has been extended to deal with black holes with non-static metrics. The possibility that for an asymptotic observer a black hole with large mass will rapidly increase and eventually engulf the Universe at a finite time in the future has been studied by using reasonable values for astronomical parameters. It is concluded that such a phenomenon is forbidden for all black holes in quintessential cosmological models.
4 pages, RevTex
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