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Naturalness of nearly degenerate neutrinos

If neutrinos are to play a relevant cosmological role, they must be essentially degenerate. We study whether radiative corrections can or cannot be responsible for the small mass splittings, in agreement with all the available experimental data. We perform an exhaustive exploration of the bimaximal...

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Detalles Bibliográficos
Autores principales: Casas, J.A., Espinosa, J.R., Ibarra, A., Navarro, I.
Lenguaje:eng
Publicado: 1999
Materias:
Acceso en línea:https://dx.doi.org/10.1016/S0550-3213(99)00383-1
http://cds.cern.ch/record/385183
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author Casas, J.A.
Espinosa, J.R.
Ibarra, A.
Navarro, I.
author_facet Casas, J.A.
Espinosa, J.R.
Ibarra, A.
Navarro, I.
author_sort Casas, J.A.
collection CERN
description If neutrinos are to play a relevant cosmological role, they must be essentially degenerate. We study whether radiative corrections can or cannot be responsible for the small mass splittings, in agreement with all the available experimental data. We perform an exhaustive exploration of the bimaximal mixing scenario, finding that (i) the vacuum oscillations solution to the solar neutrino problem is always excluded; (ii) if the mass matrix is produced by a see-saw mechanism, there are large regions of the parameter space consistent with the large angle MSW solution, providing a natural origin for the Delta m^2_{sol} << Delta m^2_{atm} hierarchy; (iii) the bimaximal structure becomes then stable under radiative corrections. We also provide analytical expressions for the mass splittings and mixing angles and present a particularly simple see-saw ansatz consistent with all the observations.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1999
record_format invenio
spelling cern-3851832021-10-08T02:27:12Zdoi:10.1016/S0550-3213(99)00383-1http://cds.cern.ch/record/385183engCasas, J.A.Espinosa, J.R.Ibarra, A.Navarro, I.Naturalness of nearly degenerate neutrinosParticle Physics - PhenomenologyIf neutrinos are to play a relevant cosmological role, they must be essentially degenerate. We study whether radiative corrections can or cannot be responsible for the small mass splittings, in agreement with all the available experimental data. We perform an exhaustive exploration of the bimaximal mixing scenario, finding that (i) the vacuum oscillations solution to the solar neutrino problem is always excluded; (ii) if the mass matrix is produced by a see-saw mechanism, there are large regions of the parameter space consistent with the large angle MSW solution, providing a natural origin for the Delta m^2_{sol} << Delta m^2_{atm} hierarchy; (iii) the bimaximal structure becomes then stable under radiative corrections. We also provide analytical expressions for the mass splittings and mixing angles and present a particularly simple see-saw ansatz consistent with all the observations.If neutrinos are to play a relevant cosmological role, they must be essentially degenerate. We study whether radiative corrections can or cannot be responsible for the small mass splittings, in agreement with all the available experimental data. We perform an exhaustive exploration of the bimaximal mixing scenario, finding that (i) the vacuum oscillations solution to the solar neutrino problem is always excluded; (ii) if the mass matrix is produced by a see-saw mechanism, there are large regions of the parameter space consistent with the large angle MSW solution, providing a natural origin for the $\Delta m^2_{sol} << \Delta m^2_{atm}$ hierarchy; (iii) the bimaximal structure becomes then stable under radiative corrections. We also provide analytical expressions for the mass splittings and mixing angles and present a particularly simple see-saw ansatz consistent with all observations.If neutrinos are to play a relevant cosmological role, they must be essentially degenerate. We study whether radiative corrections can or cannot be responsible for the small mass splittings, in agreement with all the available experimental data. We perform an exhaustive exploration of the bimaximal mixing scenario, finding that (i) the vacuum oscillations solution to the solar neutrino problem is always excluded; (ii) if the mass matrix is produced by a see-saw mechanism, there are large regions of the parameter space consistent with the large angle MSW solution, providing a natural origin for the $\Delta m^2_{sol} << \Delta m^2_{atm}$ hierarchy; (iii) the bimaximal structure becomes then stable under radiative corrections. We also provide analytical expressions for the mass splittings and mixing angles and present a particularly simple see-saw ansatz consistent with all observations.If neutrinos are to play a relevant cosmological role, they must be essentially degenerate. We study whether radiative corrections can or cannot be responsible for the small mass splittings, in agreement with all the available experimental data. We perform an exhaustive exploration of the bimaximal mixing scenario, finding that (i) the vacuum oscillations solution to the solar neutrino problem is always excluded; (ii) if the mass matrix is produced by a see-saw mechanism, there are large regions of the parameter space consistent with the large angle MSW solution, providing a natural origin for the Δm sol 2 ⪡ Δm atm 2 hierarchy; (iii) the bimaximal structure becomes then stable under radiative corrections. We also provide analytical expressions for the mass splittings and mixing angles and present a particularly simple see-saw ansatz consistent with all observations.hep-ph/9904395IEM-FT-191-99CERN-TH-99-103IFT-UAM-CSIC-99-15CERN-TH-99-103IEM-FT-191IFT-UAM-CSIC-99-15oai:cds.cern.ch:3851831999-04-20
spellingShingle Particle Physics - Phenomenology
Casas, J.A.
Espinosa, J.R.
Ibarra, A.
Navarro, I.
Naturalness of nearly degenerate neutrinos
title Naturalness of nearly degenerate neutrinos
title_full Naturalness of nearly degenerate neutrinos
title_fullStr Naturalness of nearly degenerate neutrinos
title_full_unstemmed Naturalness of nearly degenerate neutrinos
title_short Naturalness of nearly degenerate neutrinos
title_sort naturalness of nearly degenerate neutrinos
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/S0550-3213(99)00383-1
http://cds.cern.ch/record/385183
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AT espinosajr naturalnessofnearlydegenerateneutrinos
AT ibarraa naturalnessofnearlydegenerateneutrinos
AT navarroi naturalnessofnearlydegenerateneutrinos