TL;DR
This paper reviews various supersymmetry models, discusses their implications for high-energy cosmic rays, and proposes a high-scale susy model for fermion masses with specific neutrino mixing predictions.
Contribution
It introduces a high-scale supersymmetry model for fermion masses and predicts a notable neutrino mixing angle.
Findings
Expected ~0.1 nu_e-nu_{tau} mixing angle
Implications for very high energy cosmic rays
Comparison of electroweak and split susy models
Abstract
After reviewing electroweak (EW) scale supersymmetry (susy) and split susy, as well as their implications in very high energy cosmic rays, I present a high scale susy model for fermion masses. An O(0.1) nu_e-nu_{tau} mixing is expected.
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