Neutrino masses from SUSY breaking in radiative seesaw models
arXiv:1406.0557 · doi:10.1140/epjc/s10052-014-3244-1
Abstract
Radiatively generated neutrino masses () are proportional to supersymmetry (SUSY) breaking, as a result of the SUSY non-renormalisation theorem. In this work, we investigate the space of SUSY radiative seesaw models with regard to their dependence on SUSY breaking ($\require{cancel}\cancel{\text{SUSY}}$). In addition to contributions from sources of that are involved in electroweak symmetry breaking ( contributions), and which are manifest from and , radiatively generated can also receive contributions from sources that are unrelated to EWSB ( contributions). We point out that recent literature overlooks pure- contributions () that can arise at the same order of perturbation theory as the leading order contribution from . We show that there exist realistic radiative seesaw models in which the leading order contribution to is proportional to . To our knowledge no model with such a feature exists in the literature. We give a complete description of the simplest model-topologies and their leading dependence on . We show that in one-loop realisations operators are suppressed by at least or . We construct a model example based on a one-loop type-II seesaw. An interesting aspect of these models lies in the fact that the scale of soft- effects generating the leading order can be quite small without conflicting with lower limits on the mass of new particles.
Accepted for publication in European Physical Journal C; 23 pages + appendices; references updated; minor revisions; extended conclusions
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