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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...
Autores principales: | , |
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Lenguaje: | eng |
Publicado: |
2000
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/S0370-2693(00)01148-5 http://cds.cern.ch/record/449497 |
_version_ | 1780896068169367552 |
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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 |
record_format | invenio |
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 |