Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1993-12-09
Phys.Rev. D50 (1994) 523-528
Physics
High Energy Physics
High Energy Physics - Phenomenology
10 pages, standard LATEX, no figures, Carnegie-Mellon University Report CMU-HEP93-27 and DOE-ER/40682-52
Scientific paper
10.1103/PhysRevD.50.523
In the SUSY GUT scenario, it is natural to assume the right-handed-neutrino Majorana-mass scale to be $10^{16}$ GeV. This will in principle lead, by the seesaw mechanism, to a $ \nu_{\tau} $ mass of order $ m_t^2 / (10^{16}\, {\rm GeV}) \sim 3 \times 10^{-3}\, {\rm eV} $. This suggests that the solution of the solar-neutrino puzzle should be either the MSW effect in $\nu_e$--$\nu_{\tau}$ oscillations, with $ m_{\nu_{\tau}}^2 \sim 10^{-5}\, {\rm eV}^2 $, or long-wavelength $\nu_e$--$\nu_{\mu}$ oscillations, with $ m_{\nu_{\mu}}^2 \sim 10^{-10}\, {\rm eV}^2 $. These solutions require unexpectedly large mixings of $ \nu_e $ with $ \nu_{\tau} $ and $ \nu_{\mu} $, respectively. I suggest a variation of the Dimopoulos--Hall--Raby model for the fermion mass matrices which can accomodate such large mixings.
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