Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-03-28
Phys.Lett.B640:117-120,2006
Astronomy and Astrophysics
Astrophysics
4 pages, RevTex
Scientific paper
10.1016/j.physletb.2006.07.067
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.
González-Díaz Pedro F.
Jimenez Madrid Jose A.
Martin-Moruno Prado
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