Heavy neutrino threshold effects in low energy phenomenology
arXiv:hep-ph/9505402 · doi:10.1016/0550-3213(95)00377-5
Abstract
Right handed neutrinos with mass of GeV are required to implement the see-saw mechanism and generate neutrino masses capable of playing a role in structure formation. Moreover models of fermion masses often relate the Yukawa couplings involving these neutrinos to the up-quark Yukawa couplings. Here we study the effects of such couplings on the radiative corrections to quark masses. We find that equality at may still give the correct -- ratio at low energies, but only if there is large mixing in the charged leptonic sector. We propose specific mass matrix ``textures'' dictated by a family symmetry whose structure preserves at . In these schemes, due to the large mixing, it is possible to give a simultaneous solution to the solar neutrino deficit and the atmospheric neutrino problem.
22 pages, latex file, including 8 latex figures. Revised version (typos corrected, references added), to be published in Nucl. Phys. B
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