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dc.contributor.authorBogdanos, C.en
dc.contributor.authorTamvakis, K.en
dc.date.accessioned2015-11-24T18:32:33Z-
dc.date.available2015-11-24T18:32:33Z-
dc.identifier.issn0370-2693-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/16584-
dc.rightsDefault Licence-
dc.subjectdark energyen
dc.subjectconstanten
dc.subjectdimensionen
dc.subjectspaceen
dc.subjectteven
dc.titleBrane cosmological evolution with bulk matteren
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.secondary<Go to ISI>://000244767800008-
heal.identifier.secondaryhttp://ac.els-cdn.com/S0370269307000883/1-s2.0-S0370269307000883-main.pdf?_tid=61c389ad797679cc91a3aa8046b5da90&acdnat=1334231994_bcc71b0642cb8a634ad1c9c4fa7b1746-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate2007-
heal.abstractWe consider the cosmological evolution of a brane for general bulk matter content. In our setup the bulk pressure and the energy exchange densities are comparable to the brane energy density. Adopting a phenomenological fluid ansatz and generalizations of it, we derive a set of exact solutions of the Friedmann equation that exhibit accelerated expansion. We find that the effective equation of state parameter for the dark energy can exhibit w = -1 crossing without the presence of exotic matter. (c) 2007 Elsevier B.V. All rights reserved.en
heal.journalNamePhysics Letters Ben
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)

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