Neutrino masses from SUSY breaking in radiative seesaw models
A. J. R. Figueiredo

TL;DR
This paper explores how radiative neutrino masses in SUSY models depend on SUSY breaking sources, revealing new contributions and proposing models where neutrino masses are primarily generated by electroweak symmetry breaking SUSY breaking effects.
Contribution
It identifies overlooked pure SUSY-breaking contributions to neutrino masses and constructs novel models where these effects dominate, expanding the understanding of SUSY radiative seesaw mechanisms.
Findings
Pure SUSY-breaking contributions can dominate neutrino mass generation.
One-loop realizations suppress certain operators by at least rac{mu m_soft}{M^3}.
A new model based on a one-loop type-II seesaw is proposed.
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 (). 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…
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