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• W2149861809 abstract "We present the first global analysis of the constrained next-to-minimal supersymmetric standard model that investigates the impact of the recent discovery of a 126 GeV Higgs-like boson, of the observation of a signal for branching ratio $mathrm{BR}({mathrm{B}}_{mathrm{s}}ensuremath{rightarrow}{ensuremath{mu}}^{+}{ensuremath{mu}}^{ensuremath{-}})$, and of constraints on supersymmetry from $ensuremath{sim}5/mathrm{fb}$ of data accumulated at the LHC, as well as of other relevant constraints from colliders, flavor physics and dark matter. We consider three possible cases, assuming in turn that the discovered Higgs boson is (i) the lightest Higgs boson of the model; (ii) the next-to-lightest Higgs boson; and (iii) a combination of both roughly degenerate in mass. The likelihood function for the Higgs signal uses signal rates in the $ensuremath{gamma}ensuremath{gamma}$ and $ZZensuremath{rightarrow}4l$ channels, while that for the Higgs exclusion limits assumes decay through the $ensuremath{gamma}ensuremath{gamma}$, $ensuremath{tau}ensuremath{tau}$, $ZZ$ and ${W}^{+}{W}^{ensuremath{-}}$ channels. In all cases considered we identify the 68% and 95% credible posterior probability regions in a Bayesian approach. We find that, when the constraints are applied with their respective uncertainties, the first case shows strong CMSSM-like behavior, with the stau coannihilation region featuring highest posterior probability, the best-fit point, a correct mass of the lightest Higgs boson and the lighter top squark mass in the ballpark of 1 TeV. We also expose in this region a linear relationship between the trilinear couplings of the stau and the top squark, with both of them being strongly negative as enforced by the Higgs mass and the relic density, which outside of the stau coannihilation region show some tension. The second and the third case, on the other hand, while allowed are disfavored by the constraints from direct detection of dark matter and from $mathrm{BR}({mathrm{B}}_{mathrm{s}}ensuremath{rightarrow}{ensuremath{mu}}^{+}{ensuremath{mu}}^{ensuremath{-}})$. Without the anomalous magnetic moment of the muon the fit improves considerably, especially for negative effective $ensuremath{mu}$ parameter. We discuss how the considered scenarios could be tested further at the LHC and in dark matter searches." @default.
• W2149861809 created "2016-06-24" @default.
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• W2149861809 date "2013-06-10" @default.
• W2149861809 modified "2023-10-18" @default.
• W2149861809 title "Constrained next-to-minimal supersymmetric standard model with a 126 GeV Higgs boson: A global analysis" @default.
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• W2149861809 cites W1624378254 @default.
• W2149861809 cites W1789796604 @default.
• W2149861809 cites W1858542512 @default.
• W2149861809 cites W1928759167 @default.
• W2149861809 cites W1978494510 @default.
• W2149861809 cites W1982283102 @default.
• W2149861809 cites W1997858814 @default.
• W2149861809 cites W1998486387 @default.
• W2149861809 cites W1999082404 @default.
• W2149861809 cites W2007816709 @default.
• W2149861809 cites W2011694152 @default.
• W2149861809 cites W2017957479 @default.
• W2149861809 cites W2018261547 @default.
• W2149861809 cites W2024959957 @default.
• W2149861809 cites W2036634861 @default.
• W2149861809 cites W2036901704 @default.
• W2149861809 cites W2038685690 @default.
• W2149861809 cites W2045078482 @default.
• W2149861809 cites W2045368574 @default.
• W2149861809 cites W2049206870 @default.
• W2149861809 cites W2062483902 @default.
• W2149861809 cites W2067692720 @default.
• W2149861809 cites W2068671056 @default.
• W2149861809 cites W2070344198 @default.
• W2149861809 cites W2071622295 @default.
• W2149861809 cites W2080912762 @default.
• W2149861809 cites W2081130287 @default.
• W2149861809 cites W2085052968 @default.
• W2149861809 cites W2088157505 @default.
• W2149861809 cites W2089969108 @default.
• W2149861809 cites W2091790135 @default.
• W2149861809 cites W2095859713 @default.
• W2149861809 cites W2097820102 @default.
• W2149861809 cites W2103877967 @default.
• W2149861809 cites W2110112450 @default.
• W2149861809 cites W2113200074 @default.
• W2149861809 cites W2116109970 @default.
• W2149861809 cites W2116566737 @default.
• W2149861809 cites W2118179359 @default.
• W2149861809 cites W2123370932 @default.
• W2149861809 cites W2124624204 @default.
• W2149861809 cites W2127669635 @default.
• W2149861809 cites W2129403599 @default.
• W2149861809 cites W2129819598 @default.
• W2149861809 cites W2135031653 @default.
• W2149861809 cites W2140805520 @default.
• W2149861809 cites W2142812725 @default.
• W2149861809 cites W2145370842 @default.
• W2149861809 cites W2147652757 @default.
• W2149861809 cites W2147875900 @default.
• W2149861809 cites W2148292621 @default.
• W2149861809 cites W2155113454 @default.
• W2149861809 cites W2163683860 @default.
• W2149861809 cites W2166343935 @default.
• W2149861809 cites W2167727518 @default.
• W2149861809 cites W25441915 @default.
• W2149861809 cites W2597893009 @default.
• W2149861809 cites W2614565734 @default.
• W2149861809 cites W2950676294 @default.
• W2149861809 cites W3097986719 @default.
• W2149861809 cites W3099590106 @default.
• W2149861809 cites W3100099116 @default.
• W2149861809 cites W3100534914 @default.
• W2149861809 cites W3103254081 @default.
• W2149861809 cites W3103331187 @default.
• W2149861809 cites W3104188978 @default.
• W2149861809 cites W3104492742 @default.
• W2149861809 cites W3104953676 @default.
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• W2149861809 doi "https://doi.org/10.1103/physrevd.87.115010" @default.
• W2149861809 hasPublicationYear "2013" @default.
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