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Nearly degenerate neutrinos, Supersymmetry and radiative corrections
If neutrinos are to play a relevant cosmological role, they must be essentially degenerate with a mass matrix of the bimaximal mixing type. We study this scenario in the MSSM framework, finding that if neutrino masses are produced by a see-saw mechanism, the radiative corrections give rise to mass s...
Autores principales: | , , , |
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Lenguaje: | eng |
Publicado: |
1999
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/S0550-3213(99)00605-7 http://cds.cern.ch/record/387800 |
_version_ | 1780893623712219136 |
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author | Casas, J A Espinosa, J R Ibarra, Alejandro Navarro, I |
author_facet | Casas, J A Espinosa, J R Ibarra, Alejandro Navarro, I |
author_sort | Casas, J A |
collection | CERN |
description | If neutrinos are to play a relevant cosmological role, they must be essentially degenerate with a mass matrix of the bimaximal mixing type. We study this scenario in the MSSM framework, finding that if neutrino masses are produced by a see-saw mechanism, the radiative corrections give rise to mass splittings and mixing angles that can accommodate the atmospheric and the (large angle MSW) solar neutrino oscillations. This provides a natural origin for the $\Delta m^2_{sol} << \Delta m^2_{atm}$ hierarchy. On the other hand, the vacuum oscillation solution to the solar neutrino problem is always excluded. We discuss also in the SUSY scenario other possible effects of radiative corrections involving the new neutrino Yukawa couplings, including implications for triviality limits on the Majorana mass, the infrared fixed point value of the top Yukawa coupling, and gauge coupling and bottom-tau unification. |
id | cern-387800 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1999 |
record_format | invenio |
spelling | cern-3878002019-09-30T06:29:59Zdoi:10.1016/S0550-3213(99)00605-7http://cds.cern.ch/record/387800engCasas, J AEspinosa, J RIbarra, AlejandroNavarro, INearly degenerate neutrinos, Supersymmetry and radiative correctionsParticle Physics - PhenomenologyIf neutrinos are to play a relevant cosmological role, they must be essentially degenerate with a mass matrix of the bimaximal mixing type. We study this scenario in the MSSM framework, finding that if neutrino masses are produced by a see-saw mechanism, the radiative corrections give rise to mass splittings and mixing angles that can accommodate the atmospheric and the (large angle MSW) solar neutrino oscillations. This provides a natural origin for the $\Delta m^2_{sol} << \Delta m^2_{atm}$ hierarchy. On the other hand, the vacuum oscillation solution to the solar neutrino problem is always excluded. We discuss also in the SUSY scenario other possible effects of radiative corrections involving the new neutrino Yukawa couplings, including implications for triviality limits on the Majorana mass, the infrared fixed point value of the top Yukawa coupling, and gauge coupling and bottom-tau unification.hep-ph/9905381CERN-TH-99-142IEM-FT-193oai:cds.cern.ch:3878001999-05-19 |
spellingShingle | Particle Physics - Phenomenology Casas, J A Espinosa, J R Ibarra, Alejandro Navarro, I Nearly degenerate neutrinos, Supersymmetry and radiative corrections |
title | Nearly degenerate neutrinos, Supersymmetry and radiative corrections |
title_full | Nearly degenerate neutrinos, Supersymmetry and radiative corrections |
title_fullStr | Nearly degenerate neutrinos, Supersymmetry and radiative corrections |
title_full_unstemmed | Nearly degenerate neutrinos, Supersymmetry and radiative corrections |
title_short | Nearly degenerate neutrinos, Supersymmetry and radiative corrections |
title_sort | nearly degenerate neutrinos, supersymmetry and radiative corrections |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1016/S0550-3213(99)00605-7 http://cds.cern.ch/record/387800 |
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