Yukawa Unification and the Superpartner Mass Scale

TL;DR

This paper explores how Yukawa unification constrains superpartner masses in supersymmetry, suggesting they are within reach of current LHC searches, especially when considering dark matter and flavor phenomenology.

Contribution

It provides a model-independent analysis linking Yukawa unification, dark matter, and superpartner mass bounds, emphasizing their testability at the LHC.

Findings

Superpartner masses are bounded in the several TeV range due to Yukawa unification.

LSP with bino-Higgsino admixture influences superpartner mass limits.

Predicted B_s to mu+ mu- decay rate is lower than the Standard Model expectation.

Abstract

Naturalness in supersymmetry (SUSY) is under siege by increasingly stringent LHC constraints, but natural electroweak symmetry breaking still remains the most powerful motivation for superpartner masses within experimental reach. If naturalness is the wrong criterion then what determines the mass scale of the superpartners? We motivate supersymmetry by (1) gauge coupling unification, (2) dark matter, and (3) precision b-tau Yukawa unification. We show that for an LSP that is a bino-Higgsino admixture, these three requirements lead to an upper-bound on the stop and sbottom masses in the several TeV regime because the threshold correction to the bottom mass at the superpartner scale is required to have a particular size. For tan beta about 50, which is needed for t-b-tau unification, the stops must be lighter than 2.8 TeV when A_t has the opposite sign of the gluino mass, as is favored by renormalization group scaling. For lower values of tan beta, the top and bottom squarks must be even lighter. Yukawa unification plus dark matter implies that superpartners are likely in reach of the LHC, after the upgrade to 14 (or 13) TeV, independent of any considerations of naturalness. We present a model-independent, bottom-up analysis of the SUSY parameter space that is simultaneously consistent with Yukawa unification and the hint for m_h = 125 GeV. We study the flavor and dark matter phenomenology that accompanies this Yukawa unification. A large portion of the parameter space predicts that the branching fraction for B_s to mu^+ mu^- will be observed to be significantly lower than the SM value.