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dc.contributor.authorBogdanos, C.en
dc.contributor.authorDimitriadis, A.en
dc.contributor.authorTamvakis, K.en
dc.date.accessioned2015-11-24T18:30:56Z-
dc.date.available2015-11-24T18:30:56Z-
dc.identifier.issn1550-7998-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/16407-
dc.rightsDefault Licence-
dc.subjectcosmological constanten
dc.subjectbraneen
dc.subjectconstraintsen
dc.subjectdimensionsen
dc.subjectmillimeteren
dc.subjectsupernovaeen
dc.subjecthierarchyen
dc.subjectevolutionen
dc.subjectuniverseen
dc.subjectlambdaen
dc.titleDark energy from bulk matteren
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.primaryDoi 10.1103/Physrevd.75.087303-
heal.identifier.secondary<Go to ISI>://000246076900113-
heal.identifier.secondaryhttp://prd.aps.org/abstract/PRD/v75/i8/e087303-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate2007-
heal.abstractWe consider the possibility of getting accelerated expansion and w=-1 crossing in the context of a braneworld cosmological setup, endowed with a bulk energy-momentum tensor. For a given ansatz of the bulk content, we demonstrate that the bulk pressures dominate the dynamics at late times and can lead to accelerated expansion. We also analyze the constraints under which we can get a realistic profile for the effective equation of state and conclude that matter in the bulk has the effect of dark energy on the brane. Furthermore, we show that it is possible to simulate the behavior to a Chaplygin gas using nonexotic bulk matter.en
heal.journalNamePhysical Review Den
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)

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