Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/2307/297
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dc.contributor.authorAltarelli, Guido-
dc.date.accessioned2010-07-12T12:24:22Z-
dc.date.available2010-07-12T12:24:22Z-
dc.date.issued2009-
dc.identifier.othere-Print: arXiv:0905.2350 [hep-ph]-
dc.identifier.urihttp://hdl.handle.net/2307/297-
dc.descriptionCitazioni 16 (Source: SPIRES, Date 7.7.2010)en
dc.description.abstractThe data on neutrino mixing are at present compatible with Tri-Bimaximal (TB) mixing. If one takes this indication seriously then the models that lead to TB mixing in first approximation are particularly interesting and A4 models are prominent in this list. However, the agreement of TB mixing with the data could still be an accident. We discuss a recent model based on S4 where Bimaximal mixing is instead valid at leading order and the large corrections needed to reproduce the data arise from the diagonalization of charged leptons. The value of $\theta_{13}$ could distinguish between the two alternatives.en
dc.language.isoenen
dc.publisherPaperGraphen
dc.subjectParticle Physicsen
dc.subjectNeutrinoen
dc.subjectMassen
dc.subjectMixingen
dc.subjectModelsen
dc.titleTheoretical Models of Neutrino Mixing: Recent Developmentsen
dc.typeconferenceObjecten
dc.subject.miurSettori Disciplinari MIUR::Scienze fisicheen
dc.subject.miurScienze fisiche-
dc.subject.isicruiCategorie ISI-CRUI::Scienze fisicheen
dc.subject.isicruiScienze fisiche-
dc.subject.anagraferoma3Scienze fisicheen
dc.relation.pagenumber377-396en
dc.relation.conferencename13th International Workshop on Neutrino Telescopes: Un altro modo di guardare il cielo: Tribute to Galileo,en
dc.relation.conferencedate2009-03-
dc.relation.conferenceplaceVenice, Italyen
local.testtest-
dc.description.romatrecurrentDipartimento di Fisica 'Edoardo Amaldi'*
item.languageiso639-1other-
item.fulltextWith Fulltext-
item.grantfulltextrestricted-
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