Please use this identifier to cite or link to this item: https://olympias.lib.uoi.gr/jspui/handle/123456789/17348
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dc.contributor.authorPerivolaropoulos, L.en
dc.date.accessioned2015-11-24T18:38:30Z-
dc.date.available2015-11-24T18:38:30Z-
dc.identifier.issn1550-7998-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/17348-
dc.rightsDefault Licence-
dc.subjectscalar-tensor theoryen
dc.subjectaccelerating universeen
dc.subjectgravitationen
dc.titlePPN parameter gamma and solar system constraints of massive Brans-Dicke theoriesen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.primaryDoi 10.1103/Physrevd.81.047501-
heal.identifier.secondary<Go to ISI>://000275898500119-
heal.identifier.secondaryhttp://prd.aps.org/abstract/PRD/v81/i4/e047501-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate2010-
heal.abstractPrevious solar system constraints of the Brans-Dicke (BD) parameter omega have either ignored the effects of the scalar field potential (mass terms) or assumed a highly massive scalar field. Here, we interpolate between the above two assumptions and derive the solar system constraints on the BD parameter omega for any field mass. We show that for omega = O(1) the solar system constraints relax for a field mass m >= 20 x m(AU) = 20 x 10(-27) GeV.en
heal.journalNamePhysical Review Den
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)



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