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Neutrino tri-bi-maximal mixing from a non-Abelian discrete family symmetry

The observed neutrino mixing, having a near maximal atmospheric neutrino mixing angle and a large solar mixing angle, is close to tri-bi-maximal. We argue that this structure suggests a family symmetric origin in which the magnitude of the mixing angles are related to the existence of a discrete non...

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Detalles Bibliográficos
Autores principales: Varzielas, I M, King, S F, Ross, Graham G
Lenguaje:eng
Publicado: 2006
Materias:
Acceso en línea:https://dx.doi.org/10.1016/j.physletb.2007.03.009
http://cds.cern.ch/record/968600
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author Varzielas, I M
King, S F
Ross, Graham G
author_facet Varzielas, I M
King, S F
Ross, Graham G
author_sort Varzielas, I M
collection CERN
description The observed neutrino mixing, having a near maximal atmospheric neutrino mixing angle and a large solar mixing angle, is close to tri-bi-maximal. We argue that this structure suggests a family symmetric origin in which the magnitude of the mixing angles are related to the existence of a discrete non-Abelian family symmetry. We construct a model in which the family symmetry is the non-Abelian discrete group $\Delta(27)$, a subgroup of $SU(3)$ in which the tri-bi-maximal mixing directly follows from the vacuum structure enforced by the discrete symmetry. In addition to the lepton mixing angles, the model accounts for the observed quark and lepton masses and the CKM matrix. The structure is also consistent with an underlying stage of Grand Unification.
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institution Organización Europea para la Investigación Nuclear
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spelling cern-9686002019-09-30T06:29:59Zdoi:10.1016/j.physletb.2007.03.009http://cds.cern.ch/record/968600engVarzielas, I MKing, S FRoss, Graham GNeutrino tri-bi-maximal mixing from a non-Abelian discrete family symmetryParticle Physics - PhenomenologyThe observed neutrino mixing, having a near maximal atmospheric neutrino mixing angle and a large solar mixing angle, is close to tri-bi-maximal. We argue that this structure suggests a family symmetric origin in which the magnitude of the mixing angles are related to the existence of a discrete non-Abelian family symmetry. We construct a model in which the family symmetry is the non-Abelian discrete group $\Delta(27)$, a subgroup of $SU(3)$ in which the tri-bi-maximal mixing directly follows from the vacuum structure enforced by the discrete symmetry. In addition to the lepton mixing angles, the model accounts for the observed quark and lepton masses and the CKM matrix. The structure is also consistent with an underlying stage of Grand Unification.hep-ph/0607045CERN-PH-TH-2006-124oai:cds.cern.ch:9686002006-07-04
spellingShingle Particle Physics - Phenomenology
Varzielas, I M
King, S F
Ross, Graham G
Neutrino tri-bi-maximal mixing from a non-Abelian discrete family symmetry
title Neutrino tri-bi-maximal mixing from a non-Abelian discrete family symmetry
title_full Neutrino tri-bi-maximal mixing from a non-Abelian discrete family symmetry
title_fullStr Neutrino tri-bi-maximal mixing from a non-Abelian discrete family symmetry
title_full_unstemmed Neutrino tri-bi-maximal mixing from a non-Abelian discrete family symmetry
title_short Neutrino tri-bi-maximal mixing from a non-Abelian discrete family symmetry
title_sort neutrino tri-bi-maximal mixing from a non-abelian discrete family symmetry
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/j.physletb.2007.03.009
http://cds.cern.ch/record/968600
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