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Democratic approach to atmospheric and solar neutrino oscillations

2002/08/31 by Qaisar Shafi, Zurab Tavartkiladze · 2 citations
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #Neutrino Physics Research #Particle physics theoretical and experimental studies #hep-ph

paper · pdf · doi:10.1016/s0370-2693(02)02972-6

published as Phys.Lett.B550:172-177,2002 · Version to appear in Physics Letters B

arxiv created 2002/11/06 · openalex publication_date 2002/12/01 · arxiv updated 2011/05/12 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Working with a U (1) flavor symmetry, we show how the hierarchical structure in the charged fermion sector and a democratic approach for neutrinos that yields large solar and atmospheric neutrino mixings can be simultaneously realized in the MSSM framework. However, in SU (5) due to the unified multiplets we encounter difficulties. Namely, democracy for the neutrinos leads to a wrong hierarchical pattern for charged fermion masses and mixings. We discuss how this is overcome in flipped SU (5).

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