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dc.contributor.authorBogdanos, C.en
dc.contributor.authorDimitriadis, A.en
dc.contributor.authorTamvakis, K.en
dc.date.accessioned2015-11-24T17:59:55Z-
dc.date.available2015-11-24T17:59:55Z-
dc.identifier.issn0264-9381-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/15856-
dc.rightsDefault Licence-
dc.subjectenergy componenten
dc.subjectconstanten
dc.subjectdimensionen
dc.subjectevolutionen
dc.subjectequationen
dc.subjectgravityen
dc.subjectspaceen
dc.subjectstateen
dc.subjectteven
dc.titleBrane cosmology with a non-minimally coupled bulk-scalar fielden
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.secondary<Go to ISI>://000247896800010-
heal.identifier.secondaryhttp://iopscience.iop.org/0264-9381/24/14/010/pdf/0264-9381_24_14_010.pdf-
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 in the presence of a bulk scalar field coupled to the Ricci scalar through a term f (phi) R. We derive the generalized Friedmann equation on the brane in the presence of arbitrary brane and bulk-matter, as well as the scalar field equation, allowing for a general scalar potential V (phi). We focus on a quadratic form of the above non-minimal coupling -xi phi R-2 and obtain a class of late-time solutions for the scale factor and the scalar field on the brane that exhibit accelerated expansion for a range of the non-minimal coupling parameter xi.en
heal.journalNameClassical and Quantum Gravityen
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)

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