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Universal quark-lepton mixing and determination of neutrino masses

2000/06/16 by Per Osland, Osland, Per, Tai Tsun Wu +1
Physics and Astronomy · #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #hep-ph

paper · pdf · doi:10.48550/arxiv.hep-ph/0006185

10 pages

arxiv created 2000/06/16 · arxiv updated 2009/11/30

Abstract

If three right-handed neutrinos are added to the Standard Model, then, for the three known generations, there are six quarks and six leptons. It is then natural to assume that the symmetry considerations that have been applied to the quark matrices are also valid for the lepton mass matrices. Under this assumption, the solar and atmospheric neutrino data can be used to determine the individual neutrino masses. Three minima have been found, using the chi2 fit, and, from these minima, it is determined that the mass of the lightest neutrino is 1.3×10-3 eV, that of the next heavier neutrino is 1.3×10-2 eV, while the mass of the heaviest neutrino is 3.4×10-2, 5.8×10-2 or 9.4×10-2 eV.

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