| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10725430 | Physics Letters B | 2006 | 4 Pages |
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.
Related Topics
Physical Sciences and Engineering
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Nuclear and High Energy Physics
Authors
Prado MartÃn-Moruno, José A. Jiménez Madrid, Pedro F. González-DÃaz,