Abstract

Abstract A Standard Model-like Higgs near 125 GeV in the MSSM requires multi-TeV stop masses, or a near-maximal contribution to its mass from stop mixing. We investigate the maximal mixing scenario, and in particular its prospects for being realized it in potentially realistic GUT models. We work out constraints on the possible GUT-scale soft terms, which we compare with what can be obtained from some well-known mechanisms of SUSY breaking mediation. Finally, we analyze two promising scenarios in detail, namely gaugino mediation and gravity mediation with non-universal Higgs masses.

Highlights

  • TeV scale.2 In this approach, the soft terms can be chosen by hand to yield maximal mixing

  • We work out constraints on the possible GUT-scale soft terms, which we compare with what can be obtained from some well-known mechanisms of SUSY breaking mediation

  • One should keep in mind one of the key motivations for low-energy supersymmetry: The supersymmetric Standard Model can naturally be extrapolated up to a very high fundamental scale

Read more

Summary

Maximal stop mixing and the Higgs mass

We follow the sign conventions of [32] for soft terms, in which the MSSM superpotential is. Are generic in situations with maximal mixing, if the scalar masses are unified or negligible This is understood in the light of the large coefficients of the A0 terms in eqs. Maximal mixing in a GUT-scale model with unified gaugino masses at tan β 5 requires large negative A0 ≈ −(1– 3) max M1/2, mQ3, mU3. This is a non-trivial requirement on any GUT-scale model. It is beneficial but not strictly necessary for maximal mixing if there are positive up-type Higgs soft masses m2Hu, and small third-generation soft masses m2U3, m2Q3, as compared to the gaugino mass.

Models
Scalar sequestering
Gauge mediation
Numerical analysis
Gaugino mediation
NUHM model
Discussion and conclusions
Semi-numerical solutions of the MSSM renormalization group equations
Fine-tuning
Findings
Charge- and color-breaking minima
Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.