期刊
EUROPEAN PHYSICAL JOURNAL C
卷 71, 期 8, 页码 -出版社
SPRINGER
DOI: 10.1140/epjc/s10052-011-1722-2
关键词
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资金
- European Research Council [267352]
- CI-CYT [FPA 2010-22163-C02-01]
- Spanish MICINN [MultiDark CSD2009-00064]
- DOE at the University of Minnesota [DE-FG02-94ER-40823]
- DOE [DE-AC02-76SF00515]
- Stanford Institute for Theoretical Physics
- STFC [ST/J002798/1, ST/I002200/1, ST/I005912/1, ST/I000410/1, ST/F006748/1, ST/G502347/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/I002200/1, ST/G502347/1, GRIDPP, ST/F006748/1, ST/I005912/1 GRIDPP, ST/I000410/1, ST/I005912/1, ST/J002798/1] Funding Source: researchfish
We make frequentist analyses of the CMSSM, NUHM1, VCMSSM and mSUGRA parameter spaces taking into account all the public results of searches for supersymmetry using data from the 2010 LHC run and the XENON100 direct search for dark matter scattering. The LHC data set includes ATLAS and CMS searches for jets + (E) over barT events (with or without leptons) and for the heavier MSSM Higgs bosons, and the upper limit on BR(B-s -> mu(+)mu(-)) including data from LHCb as well as CDF and DO. The absence of signals in the LHC data favours somewhat heavier mass spectra than in our previous analyses of the CMSSM, NUHM1 and VCMSSM, and somewhat smaller dark matter scattering cross sections, all close to or within the pre-LHC 68% CL ranges, but does not impact significantly the favoured regions of the mSUGRA parameter space. We also discuss the impact of the XENON100 constraint on spin-independent dark matter scattering, stressing the importance of taking into account the uncertainty in the pi-nucleon sigma term Sigma(pi N), which affects the spin-independent scattering matrix element, and we make predictions for spin-dependent dark matter scattering. Finally, we discuss briefly the potential impact of the updated predictions for sparticle masses in the CMSSM, NUHM1, VCMSSM and mSUGRA on future e(+)e(-) colliders.
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