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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
Line 56: Line 56:
 == $M_\phi = 10$ 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 ==
2017/groups/tools/contur_for_light_scalar_particles.txt ยท Last modified: 2017/10/11 23:47 by jonathan.butterworth