4.6 Article

Global fits of the cMSSM and NUHM including the LHC Higgs discovery and new XENON100 constraints

出版社

IOP Publishing Ltd
DOI: 10.1088/1475-7516/2013/04/013

关键词

dark matter theory; supersymmetry and cosmology

资金

  1. scholarship of the Studienstiftung des deutschen Volkes
  2. Leverhulme Trust
  3. ERC Starting Grant
  4. Ramon y Cajal program of the Spanish MICINN
  5. MICINN [FPA2011-29678]
  6. Invisibles European ITN project [FP7-PEOPLE-2011-ITN, PITN-GA-2011-289442-INVISIBLES]
  7. Consolider-Ingenio Programme [MultiDark CSD2009-00064]
  8. STFC [ST/H008586/1, ST/J000388/1, ST/K00333X/1, ST/J005673/1, ST/I505713/1] Funding Source: UKRI
  9. Science and Technology Facilities Council [ST/K00333X/1, ST/H008586/1, ST/J000388/1, ST/I505713/1, ST/J005673/1] Funding Source: researchfish

向作者/读者索取更多资源

We present global fits of the constrained Minimal Supersymmetric Standard Model (cMSSM) and the Non-Universal Higgs Model (NUHM), including the most recent CMS constraint on the Higgs boson mass, 5.8 fb(-1) integrated luminosity null Supersymmetry searches by ATLAS, the new LHCb measurement of B R ((B) over bar (s) -> mu(+) mu(-)) and the 7-year WMAP dark matter relic abundance determination. We include the latest dark matter constraints from the XENON100 experiment, marginalising over astrophysical and particle physics uncertainties. We present Bayesian posterior and profile likelihood maps of the highest resolution available today, obtained from up to 350M points. We find that the new constraint on the Higgs boson mass has a dramatic impact, ruling out large regions of previously favoured cMSSM and NUHM parameter space. In the cMSSM, light sparticles and predominantly gaugino-like dark matter with a mass of a few hundred GeV are favoured. The NUHM exhibits a strong preference for heavier sparticle masses and a Higgsino-like neutralino with a mass of 1TeV. The future ton-scale XENON1T direct detection experiment will probe large portions of the currently favoured cMSSM and NUHM parameter space. The LHC operating at 14TeV collision energy will explore the favoured regions in the cMSSM, while most of the regions favoured in the NUHM will remain inaccessible. Our best-fit points achieve a satisfactory quality-of-fit, with p-values ranging from 0.21 to 0.35, so that none of the two models studied can be presently excluded at any meaningful significance level.

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