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2017:groups:tools:contur_for_light_scalar_particles [2017/10/01 11:05] jonathan.butterworth |
2017:groups:tools:contur_for_light_scalar_particles [2017/10/01 11:25] jonathan.butterworth |
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== $M_\phi = 10$ GeV, $\Lambda = 3.5$ TeV == | == $M_\phi = 10$ GeV, $\Lambda = 3.5$ TeV == | ||
- | > [[http://www.hep.ucl.ac.uk/~jmb/Work/LH/NSCPO/8TeV/mP_10_f0_3500/contur-plots/|Page of plots]]: The most powerful exclusion comes from the $\gamma + E_T^{\rm miss}$ channel, specifically the $E_T^\gamma$ differential cross section for events with no jets, in [[http://www.hep.ucl.ac.uk/~jmb/Work/LH/NSCPO/8TeV/mP_10_f0_3500/contur-plots/ATLAS_2016_I1448301_NU/index.html|this paper]]. There is also some exclusion from the $\tau$ distribution in the $H \rightarrow \gamma\gamma$ paper - see below for more on that. | + | > [[http://www.hep.ucl.ac.uk/~jmb/Work/LH/NSCPO/8TeV/mP_10_f0_3500/contur-plots/|Page of plots]]: The most powerful exclusion in the 8 TeV data comes from the $\gamma + E_T^{\rm miss}$ channel, specifically the $E_T^\gamma$ differential cross section for events with no jets, in [[http://www.hep.ucl.ac.uk/~jmb/Work/LH/NSCPO/8TeV/mP_10_f0_3500/contur-plots/ATLAS_2016_I1448301_NU/index.html|this paper]]. There is also some exclusion from the $\tau$ distribution in the $H \rightarrow \gamma\gamma$ paper - see below for more on that. Also once the 7 TeV data are included, the inclusive and diphotons cover much of the parameter space on their own. |
== $M_\phi = 20$ GeV, $\Lambda = 3.5$ TeV == | == $M_\phi = 20$ GeV, $\Lambda = 3.5$ TeV == |