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arXiv · hep-ph/0404077

Supersymmetry breaking as the origin of flavor

Javier Ferrandis·Naoyuki Haba
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Abstract

We present an effective flavor model for the radiative generation of fermion masses and mixings based on a SU(5)xU(2) symmetry. We assume that the original source of flavor breaking resides in the supersymmetry breaking sector. Flavor violation is transmitted radiatively to the fermion Yukawa couplings at low energy through finite supersymmetric threshold corrections. This model can fit the fermion mass ratios and CKM matrix elements, explain the non-observation of proton decay, and overcome present constraints on flavor changing processes through an approximate radiative alignment between the Yukawa and the soft trilinear sector. The model predicts new relations between dimensionless fermion mass ratios in the three fermion sectors, and the quark mixing angles.

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Javier Ferrandis, Naoyuki Haba. 2004-05-15. Supersymmetry breaking as the origin of flavor. https://doi.org/10.1103/physrevd.70.055003

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