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dc.contributor.authorLeontaris, G. K.en
dc.date.accessioned2015-11-24T18:38:09Z-
dc.date.available2015-11-24T18:38:09Z-
dc.identifier.issn0370-2693-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/17289-
dc.rightsDefault Licence-
dc.subjectgrand unified modelsen
dc.subjectsupergravityen
dc.subjectgutsen
dc.titleRadiative Symmetry-Breaking and the Top-Quark Mass in Local Supersymmetryen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.secondary<Go to ISI>://A1993MH09300016-
heal.identifier.secondaryhttp://ac.els-cdn.com/037026939391374V/1-s2.0-037026939391374V-main.pdf?_tid=7fc6781124cc547ea94fae114d4ebc52&acdnat=1334224055_10faf0bb2dd008c2e1b3d46af0e98064-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate1993-
heal.abstractExact low energy expressions are derived for the top-squark and Higgs masses, taking into account radiative contributions due to a heavy top quark. Their masses are expressed as analytic functions of m1/2, m3/2, m(t)/sin beta. Constraints from the radiative symmetry breaking mechanism are used then, to put lower bounds on the top-quark mass m(t). In particular, when m3/2 >> m1/2, we obtain the bound m(t) greater-than-or-equal-to 155 sin beta GeV, while in the case Of m3/2 = 0, we obtain m(t) greater-than-or-equal-to 80 sin beta GeV.en
heal.journalNamePhysics Letters Ben
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)

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