Will black holes eventually engulf the universe?

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dc.creatorMartin-Moruno, Prado
dc.creatorMadrid, Jose A. Jimenez
dc.creatorGonzalez-Diaz, Pedro F.
dc.date2006-03-28
dc.date.accessioned2026-07-07T10:28:01Z
dc.date.available2026-07-07T10:28:01Z
dc.descriptionThe 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.
dc.description4 pages, RevTex
dc.identifierhttps://arxiv.org/abs/astro-ph/0603761
dc.identifierhttp://arxiv.org/abs/astro-ph/0603761
dc.identifierPhys.Lett.B640:117-120,2006
dc.identifierdoi:10.1016/j.physletb.2006.07.067
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177308
dc.subjectAstrophysics
dc.titleWill black holes eventually engulf the universe?
dc.typetext

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