Split SUSY Radiates Flavor

Understand

Radiative flavor models where the hierarchies of Standard Model (SM) fermion masses and mixings are explained via loop corrections are elegant ways to solve the SM flavor puzzle.

• Here we build such a model in the context of Mini-Split Supersymmetry (SUSY) where both flavor and SUSY breaking occur at a scale of 1000 TeV.
• This model is consistent with the observed Higgs mass, unification, and WIMP dark matter.
• The high scale allows large flavor mixing among the sfermions, which provides part of the mechanism for radiative flavor generation.