Abstract

AbstractThe lack of evidence for new physics beyond the standard model at the LHC points to a paucity of new particles near the weak scale. This suggests that the weak scale is tuned and that supersymmetry, if present at all, is realized at higher energies. The measured Higgs mass constrains the scalar sparticles to be below 105TeV, while gauge coupling unification favors Higgsinos below 100 TeV. Nevertheless, in many models gaugino masses are suppressed and remain within reach of the LHC. Tuning the weak scale and the renormalization group evolution of the scalar masses constrain Split model building. Due to the small gaugino masses, either the squarks or the up-higgs often run tachyonic; in the latter case, successful electroweak breaking requires heavy higgsinos near the scalar sparticles. We discuss the consequences of tuning the weak scale and the phenomenology of several models of Split supersymmetry including anomaly mediation, U(1)B−Lmediation, and Split gauge mediation.

Highlights

  • Implies a tuning below the percent level

  • We discuss the consequences of tuning the weak scale and the phenomenology of several models of Split supersymmetry including anomaly mediation, U(1)B−L mediation, and Split gauge mediation

  • Does supersymmetric unification work so well if the sparticles responsible for it are not present? An answer to this question comes from Split SUSY [12, 13], a theory motivated by the multiverse

Read more

Summary

A guide to tuning the electro-weak scale in split SUSY

In concrete models of Split supersymmetry, successful tuning of electroweak symmetry breaking (EWSB) is not automatic It requires that the Higgs sector parameters at the scalar mass scale satisfy the following relation: det. EWSB can be achieved through either tuning the μ term against m2Hu with small Bμ and large tan β, or by requiring that |μ|2 ≈ |Bμ| |m2Hu| with tan β ∼ 1 The latter case is disfavored by unification due to the largeness of μ, as shown in figure 5. The constraints on the Higgs and higgsino parameters from the tuning of the EW scale are summarized in figure 6 It is clear from the discussion above that even in Split model building, just like in low energy SUSY, special attention has to be given to the way μ and Bμ are generated.

Tachyonic scalar masses from RG running
Anomaly mediation
Scalar mass spectrum and stability
Gauge mediation
Triplet mediation
Mini-Split phenomenology
Heavy higgsinos
Light higgsinos
Higgsino LSP: the minimal model for unification and dark matter
The Higgs in mini-Split
Findings
Conclusions
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.