English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/167299
Share/Impact:
Statistics
logo share SHARE logo core CORE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE
Exportar a otros formatos:

DC FieldValueLanguage
dc.contributor.authorMartín Moruno, Prado-
dc.contributor.authorJiménez Madrid, J.A.-
dc.contributor.authorGonzález-Díaz, Pedro F.-
dc.date.accessioned2018-07-03T07:34:11Z-
dc.date.available2018-07-03T07:34:11Z-
dc.date.issued2006-
dc.identifierissn: 0370-2693-
dc.identifier.citationPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics 640(4): 117- 120 (2006)-
dc.identifier.urihttp://hdl.handle.net/10261/167299-
dc.description.abstractThe 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. © 2006 Elsevier B.V. All rights reserved.-
dc.publisherElsevier-
dc.relation.isversionofPublisher's version-
dc.rightsopenAccess-
dc.titleWill black holes eventually engulf the Universe?-
dc.typeartículo-
dc.identifier.doihttp://dx.doi.org/0.1016/j.physletb.2006.07.067-
dc.date.updated2018-07-03T07:34:11Z-
dc.description.versionPeer Reviewed-
dc.language.rfc3066eng-
dc.relation.csic-
Appears in Collections:(CFMAC-IFF) Artículos
(IAA) Artículos
Files in This Item:
File Description SizeFormat 
IAA_2006_PhysicsLettersB.pdf142,41 kBAdobe PDFThumbnail
View/Open
Show simple item record
 


WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.