Abstract

We update previous frequentist analyses of the CMSSM and NUHM1 parameter spaces to include the public results of searches for supersymmetric signals using ∼1/fb of LHC data recorded by ATLAS and CMS and ∼0.3/fb of data recorded by LHCb in addition to electroweak precision and B-physics observables. We also include the constraints imposed by the cosmological dark matter density and the XENON100 search for spin-independent dark matter scattering. The LHC data set includes ATLAS and CMS searches for jets + events and for the heavier MSSM Higgs bosons, and the upper limits on BR(B s →μ + μ −) from LHCb and CMS. The absences of jets + signals in the LHC data favour heavier mass spectra than in our previous analyses of the CMSSM and NUHM1, which may be reconciled with (g−2) μ if tanβ∼40, a possibility that is, however, under pressure from heavy Higgs searches and the upper limits on BR(B s →μ + μ −). As a result, the p-value for the CMSSM fit is reduced to ∼15(38)%, and that for the NUHM1 to ∼16(38)%, to be compared with ∼9(49)% for the Standard Model limit of the CMSSM for the same set of observables (dropping (g−2) μ ), ignoring the dark matter relic density. We discuss the sensitivities of the fits to the (g−2) μ and BR(b→sγ) constraints, contrasting fits with and without the (g−2) μ constraint, and combining the theoretical and experimental errors for BR(b→sγ) linearly or in quadrature. We present predictions for $m_{\tilde{g}}$ , BR(B s →μ + μ −), M h and M A , and update predictions for spin-independent dark matter scattering, incorporating the uncertainty in the π-nucleon σ term Σ πN . Finally, we present predictions based on our fits for the likely thresholds for sparticle pair production in e + e − collisions in the CMSSM and NUHM1.

Highlights

  • In a series of papers, we and others have reported the results of global fits to pre-LHC [1,2,3,4,5,6] and LHC 2010 data [7,8,9,10] in the frameworks of simplified variants of the minimal supersymmetric extension of the Standard Model (MSSM) [11] with universal supersymmetry-breaking mass parameters at the GUT scale

  • Using our standard implementation of the (g −2)μ constraint based on a Standard Model (SM) calculation [44], and combining the theoretical and experimental errors in BR(b → sγ) in quadrature, we find that the pvalue for the constrained MSSM (CMSSM) best-fit point is ∼ 15%, and that for the NUHM1 is ∼ 16%

  • The CMSSM and (110, 340) GeV in the NUHM1, lie far outside the regions allowed by the LHC1/fb data

Read more

Summary

Introduction

In a series of papers, we and others have reported the results of global fits to pre-LHC [1,2,3,4,5,6] and LHC 2010 data [7,8,9,10] in the frameworks of simplified variants of the minimal supersymmetric extension of the Standard Model (MSSM) [11] with universal supersymmetry-breaking mass parameters at the GUT scale. The absences of signals in the jets + E/T searches disfavour the ranges of the model mass parameters (m0, m1/2) that had been favoured in our previous analyses of the CMSSM and NUHM1 [7, 8], and our current best fits have m0 ∼ 150 to 450 GeV and m1/2 ∼ 750 GeV. Reconciling these larger values of (m0, m1/2) with (g − 2)μ favours values of tan β ∼ 40, though with a large uncertainty. We emphasize that these results are derived in the context of specific models with specific universal soft supersymmetry-breaking masses at the GUT scale, and do not apply to other classes of supersymmetric models

Implementations of the New LHC Constraints
Results
Summary and 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.