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dc.contributor.authorTamvakis, K.en
dc.date.accessioned2015-11-24T18:34:32Z-
dc.date.available2015-11-24T18:34:32Z-
dc.identifier.issn0370-2693-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/16957-
dc.rightsDefault Licence-
dc.subjectinflationen
dc.subjectsupersymmetryen
dc.subjecthiggsen
dc.subjectr-symmetryen
dc.subjectd-term inflationen
dc.subjectstandard modelen
dc.titleSupersymmetric inflation with the ordinary Higgs?en
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.primaryDOI 10.1016/j.physletb.2010.04.049-
heal.identifier.secondary<Go to ISI>://000278502400001-
heal.identifier.secondaryhttp://ac.els-cdn.com/S0370269310005125/1-s2.0-S0370269310005125-main.pdf?_tid=72bc4145a30d2efb3a53b736c6ac00c1&acdnat=1334232272_d4e9b59f43163100e025184a90e9637f-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate2010-
heal.abstractWe consider a model of D-term inflation in which the inflaton coincides with the standard Higgs doublet. Non-renormalizable terms are controlled by a discrete R-symmetry of the superpotential. We consider radiative corrections to the scalar potential and find that Higgs inflation in the slow-roll approximation is viable and consistent with CMB data, although with a rather large value of the non-renormalizable coupling involved. (C) 2010 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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