Renormalization-group-induced neutrino mass in supersymmetry withoutRparity
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Abstract
We study supersymmetric models without $R$ parity and with universal soft supersymmetry-breaking terms. We show that as a result of the renormalization group flow of the parameters, a misalignment between the directions in field space of the down-type Higgs vacuum expectation value ${v}_{d}$ and of the $\ensuremath{\mu}$ term is always generated. This misalignment induces a mixing between the neutrinos and the neutralinos, resulting in one massive neutrino. By means of a simple approximate analytical expression, we study the dependence on the different parameters that contribute to the misalignment and to ${m}_{\ensuremath{\nu}}.$ In large part of the parameter space this effect dominates over the standard one-loop contributions to ${m}_{\ensuremath{\nu}};$ we estimate 1 MeV $\ensuremath{\lesssim}{m}_{\ensuremath{\nu}}\ensuremath{\lesssim}$ 1 GeV. Laboratory, cosmological, and astrophysical constraints imply ${m}_{\ensuremath{\nu}}\ensuremath{\lesssim}100$ eV. To be phenomenologically viable, these models must be supplemented with some additional mechanism to ensure approximate alignment and to suppress ${m}_{\ensuremath{\nu}}.$
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