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dc.contributor.authorLeontaris, G. K.en
dc.contributor.authorVergados, J. D.en
dc.date.accessioned2015-11-24T18:40:06Z-
dc.date.available2015-11-24T18:40:06Z-
dc.identifier.issn0370-2693-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/17556-
dc.rightsDefault Licence-
dc.subjectstandard-like modelen
dc.subjectstring modelen
dc.subjectoscillationsen
dc.subjectformulationen
dc.subjectunificationen
dc.subjectelectroweaken
dc.subjectlepen
dc.titleNeutrino Masses in Flipped Su(5)en
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.secondary<Go to ISI>://A1993LA81800010-
heal.identifier.secondaryhttp://ac.els-cdn.com/037026939390114W/1-s2.0-037026939390114W-main.pdf?_tid=bf557d8a4af237e3cb2107504158458c&acdnat=1334224345_1fbeba46ca70a7fc14154815b798187d-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate1993-
heal.abstractWe analyse the fermion masses and mixings in the flipped SU(5) model. The fermion mass matrices are evolved from the GUT scale down to m(W) by solving the renormalization group equations for the Yukawa couplings. The constraints imposed by the charged-fermion data are then utilised to make predictions about the neutrino properties. It is found that the generalized see-saw mechanism which occurs naturally in this model can provide (i) a solution to the solar neutrino problem via the MSW mechanism and (ii) a sufficiently large nu(tau) mass to contribute as a hot dark matter component as indicated by the recent COBE data.en
heal.journalNamePhysics Letters Ben
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)

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