$\mu \to e\gamma$ in a supersymmetric radiative neutrino mass model

Abstract

We have considered a supersymmetric version of the inert Higgs doublet model, whose motivation is to explain smallness of neutrino masses and existence of dark matter. In this supersymmetric model, due to the presence of discrete symmetries, neutrinos acquire masses at loop level. After computing these neutrino masses, in order to fit the neutrino oscillation data, we have shown that by tuning some supersymmetry breaking soft parameters of the model, neutrino Yukawa couplings can be unsuppressed. In the above mentioned parameter space, we have computed branching ratio of the decay $\mu \to e\gamma$. To be consistent with the current experimental upper bound on $Br(\mu \to e\gamma )$, we have obtained constraints on the right-handed neutrino mass of this model.

19 pages, 5 figures, 1 table; explanation for vanishing neutrinos is added and some minor changes, new references added; accepted by PRD

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Cited by in corpus (3)

• From the trees to the forest: a review of radiative neutrino mass models
• Predictions from scoto-seesaw with $A_4$ modular symmetry
• Fermion mass hierarchy and lepton flavor violation using $CP$ symmetry