Understanding the linear see-saw neutrino mass relations and large mixing angle MSW solution

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dc.creatorSingh, N. Nimai
dc.date2000-09-07
dc.date.accessioned2026-07-07T03:42:32Z
dc.date.available2026-07-07T03:42:32Z
dc.descriptionWe study the effective ways for generating the linear see-saw neutrino mass relations and large neutrino mixing angles in two classes of grand unified SO(10) models where the texture of Dirac neutrino mass matrix is related to either the charged lepton mass matrix (case A) or the up-quark mass matrix (case B). We also briefly analyse their stability criteria and they are found to be stable under under radiative corrections at low energies.
dc.description10 pages
dc.identifierhttps://arxiv.org/abs/hep-ph/0009087
dc.identifierhttp://arxiv.org/abs/hep-ph/0009087
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/39929
dc.subjectHigh Energy Physics - Phenomenology
dc.titleUnderstanding the linear see-saw neutrino mass relations and large mixing angle MSW solution
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