Constraints on mixing angles of Majorana neutrinos

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dc.contributor.author Adhikari R.
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 10.1103/PhysRevD.61.031301
dc.identifier.issn 15507998
dc.identifier.uri https://dspace.imsc.res.in/xmlui/handle/123456789/729
dc.identifier.uri https://doi.org/10.1103/PhysRevD.61.031301
dc.description.abstract By combining the inputs from the neutrinoless double beta decay and the fits of cosmological models of dark matter with solar and atmospheric neutrino data, we obtain constraints on two of the mixing angles of Majorana neutrinos, which become stronger when coupled with the reactor neutrino data. These constraints are strong enough to rule out Majorana neutrinos if the small angle solution of solar neutrino puzzle is borne out. © 1999 The American Physical Society.
dc.language.iso en
dc.relation.ispartof Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 61, Issue. 3
dc.rights Copyrighted by the Publisher
dc.source Physical Review D - Particles, Fields, Gravitation and Cosmology
dc.title Constraints on mixing angles of Majorana neutrinos
dc.relation.url https://doi.org/10.1103/PhysRevD.61.031301
dc.type Article


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