Will black holes eventually engulf the universe?

Thumbnail Image

Date

Authors

Journal Title

Journal ISSN

Volume Title

Publisher

Abstract

Description

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

Keywords

Astrophysics

Citation

URI

http://salesiana.dossiersoluciones.com/handle/123456789/177308

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0603761
 http://arxiv.org/abs/astro-ph/0603761
 Phys.Lett.B640:117-120,2006
 doi:10.1016/j.physletb.2006.07.067

Collections

arXiv