Three inequivalent mass-degenerate Majorana neutrinos and a scenario of their splitting for neutrino oscillations

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dc.contributor.author Adhikari R.
dc.contributor.author Ma E.
dc.contributor.author Rajasekaran G.
dc.date.accessioned 2023-10-13T12:37:30Z
dc.date.available 2023-10-13T12:37:30Z
dc.date.issued 2000
dc.identifier 10.1016/S0370-2693(00)00718-8
dc.identifier.issn 3702693
dc.identifier.uri https://dspace.imsc.res.in/xmlui/handle/123456789/728
dc.identifier.uri https://doi.org/10.1016/S0370-2693(00)00718-8
dc.description.abstract The mass matrix of three Majorana neutrinos of equal mass is not necessarily proportional to the identity matrix, but expressible in terms of two angles and one phase. We discuss how such a mass matrix may be stable or unstable against radiative corrections. We then propose a scenario with additional explicit breaking of the threefold degeneracy to account for the atmospheric neutrino data, while the radiative breaking explains the solar neutrino data, but only with the large-angle Mikheyev-Smirnov-Wolfenstein (MSW) solution. The exclusion of the small-angle MSW solution is independent of the value of the common mass m of the three neutrinos. For m ~ 0.5 eV, the effective v(e) mass for neutrinoless double beta decay is then predicted to be close to the present experimental upper limit of 0.2 eV. (C) 2000 Published by Elsevier Science B.V.
dc.language.iso en
dc.relation.ispartof Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, Vol. 486, Issue. 1-2
dc.rights Copyrighted by the Publisher
dc.source Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
dc.title Three inequivalent mass-degenerate Majorana neutrinos and a scenario of their splitting for neutrino oscillations
dc.description.pages 134 - 139
dc.relation.url https://doi.org/10.1016/S0370-2693(00)00718-8
dc.type Article


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