1. Supersymmetry in light of 1/fb of LHC data.
- Author
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Buchmueller, O., Cavanaugh, R., Roeck, A., Dolan, M., Ellis, J., Flächer, H., Heinemeyer, S., Isidori, G., Martínez Santos, D., Olive, K., Rogerson, S., Ronga, F., and Weiglein, G.
- Subjects
SUPERSYMMETRY ,LARGE Hadron Collider ,STANDARD model (Nuclear physics) ,ELECTROWEAK interactions ,DARK matter ,CONSTRAINTS (Physics) ,HIGGS bosons - 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 + [InlineEquation not available: see fulltext.] events and for the heavier MSSM Higgs bosons, and the upper limits on BR( B→ μ μ) from LHCb and CMS. The absences of jets + [InlineEquation not available: see fulltext.] 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) if tan β∼40, a possibility that is, however, under pressure from heavy Higgs searches and the upper limits on BR( B→ 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)), ignoring the dark matter relic density. We discuss the sensitivities of the fits to the ( g−2) and BR( b→ sγ) constraints, contrasting fits with and without the ( g−2) 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→ μ μ), M and M, and update predictions for spin-independent dark matter scattering, incorporating the uncertainty in the π-nucleon σ term Σ. 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. [ABSTRACT FROM AUTHOR]
- Published
- 2012
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