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Phenomenology of Pseudo Dirac Neutrinos

We formulate general conditions on $3\times 3$ neutrino mass matrices under which a degenerate pair of neutrinos at a high scale would split at low scale by radiative corrections involving only the standard model fields. This generalizes the original observations of Wolfenstein on pseudo Dirac neutr...

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Detalles Bibliográficos
Autores principales: Joshipura, A S, Rindani, S D
Lenguaje:eng
Publicado: 2000
Materias:
Acceso en línea:https://dx.doi.org/10.1016/S0370-2693(00)01148-5
http://cds.cern.ch/record/449497
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author Joshipura, A S
Rindani, S D
author_facet Joshipura, A S
Rindani, S D
author_sort Joshipura, A S
collection CERN
description We formulate general conditions on $3\times 3$ neutrino mass matrices under which a degenerate pair of neutrinos at a high scale would split at low scale by radiative corrections involving only the standard model fields. This generalizes the original observations of Wolfenstein on pseudo Dirac neutrinos to three generations. A specific model involving partially broken discrete symmetry and solving the solar and atmospheric anomalies is proposed. The symmetry pattern of the model naturally generates two large angles one of which can account for the large angle MSW solution to the solar neutrino problem.
id cern-449497
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2000
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spelling cern-4494972019-09-30T06:29:59Zdoi:10.1016/S0370-2693(00)01148-5http://cds.cern.ch/record/449497engJoshipura, A SRindani, S DPhenomenology of Pseudo Dirac NeutrinosParticle Physics - PhenomenologyWe formulate general conditions on $3\times 3$ neutrino mass matrices under which a degenerate pair of neutrinos at a high scale would split at low scale by radiative corrections involving only the standard model fields. This generalizes the original observations of Wolfenstein on pseudo Dirac neutrinos to three generations. A specific model involving partially broken discrete symmetry and solving the solar and atmospheric anomalies is proposed. The symmetry pattern of the model naturally generates two large angles one of which can account for the large angle MSW solution to the solar neutrino problem.hep-ph/0007334oai:cds.cern.ch:4494972000
spellingShingle Particle Physics - Phenomenology
Joshipura, A S
Rindani, S D
Phenomenology of Pseudo Dirac Neutrinos
title Phenomenology of Pseudo Dirac Neutrinos
title_full Phenomenology of Pseudo Dirac Neutrinos
title_fullStr Phenomenology of Pseudo Dirac Neutrinos
title_full_unstemmed Phenomenology of Pseudo Dirac Neutrinos
title_short Phenomenology of Pseudo Dirac Neutrinos
title_sort phenomenology of pseudo dirac neutrinos
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/S0370-2693(00)01148-5
http://cds.cern.ch/record/449497
work_keys_str_mv AT joshipuraas phenomenologyofpseudodiracneutrinos
AT rindanisd phenomenologyofpseudodiracneutrinos