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

2000/09/07 by N. Nimai Singh, Singh, N. Nimai
Physics and Astronomy · #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #hep-ph

paper · pdf · doi:10.48550/arxiv.hep-ph/0009087

10 pages

arxiv created 2000/09/07 · arxiv updated 2009/11/30

Abstract

We 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.

Related

• Neutrino Mass Matrix Out of Up-Quark Masses Only
• Model of Large Mixing Angle MSW Solution
• Large neutrino mixing angles for type-I see-saw mechanism in SO(10) GUT
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