Showing 2 of 2 results
This paper reviews and extends searches for the direct pair production of the scalar supersymmetric partners of the top and bottom quarks in proton-proton collisions collected by the ATLAS collaboration during the LHC Run 1. Most of the analyses use 20 fb$^{-1}$ of collisions at a centre-of-mass energy of $\sqrt{s}$ = 8 TeV, although in some case an additional 4.7 fb$^{-1}$ of collision data at $\sqrt{s}$ = 7 TeV are used. New analyses are introduced to improve the sensitivity to specific regions of the model parameter space. Since no evidence of third-generation squarks is found, exclusion limits are derived by combining several analyses and are presented in both a simplified model framework, assuming simple decay chains, as well as within the context of more elaborate phenomenological supersymmetric models.
Summary of the ATLAS Run 1 searches for direct stop pair production in models where no supersymmetric particle other than the $\tilde t_1$ and the $\tilde \chi_1^0$ is involved in the $\tilde t_1$ decay. Lines for $\Delta m(\tilde t_1, \chi_1^0 ) > m_{t}$ - t0L/t1L combined observed limit hepdata.cedar.ac.uk/view/ins1380183/d63 - t0L/t1L combined expected limit hepdata.cedar.ac.uk/view/ins1380183/d64 - t2L observed limit hepdata.cedar.ac.uk/view/ins1286444/d19 - t2L expected limit hepdata.cedar.ac.uk/view/ins1286444/d20 - SC observed limit $m_t< m_{\tilde t_1} < 198$ GeV - SC expected limit $m_t< m_{\tilde t_1} < 184$ GeV Lines for $m_b + m_W < \Delta m(\tilde t_1, \chi_1^0 ) < m_{t}$ - t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d22 - t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d23 - t2L observed limit hepdata.cedar.ac.uk/view/ins1286444/d22 - t2L expected limit hepdata.cedar.ac.uk/view/ins1286444/d23 - WW observed limit hepdata.cedar.ac.uk/view/ins1380183/d47 - WW expected limit hepdata.cedar.ac.uk/view/ins1380183/d48 Lines for $0 < \Delta m(\tilde t_1, \chi_1^0 ) < m_b + m_W $ - tc observed limit hepdata.cedar.ac.uk/view/ins1304459 (root macro) - tc expected limit hepdata.cedar.ac.uk/view/ins1304459 (root macro) - t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d22 - t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d23 - WW observed limit hepdata.cedar.ac.uk/view/ins1380183/d47 - WW expected limit hepdata.cedar.ac.uk/view/ins1380183/d48.
Upper limits on the stop pair production cross sections for different values of the branching ratios for the decays $\tilde{t}_1 \rightarrow c\tilde{\chi}_1^0$ and $\tilde{t}_1 \rightarrow ff'b\tilde{\chi}_1^0$, where BR$(\tilde{t}_1 \rightarrow c\tilde{\chi}_1^0)$ + BR$(\tilde{t}_1 \rightarrow ff'b\tilde{\chi}_1^0)$ = 1. Signal points with $\Delta m (\tilde{t}_1, \tilde{\chi}_1^0)$ of 10 GeV are shown. The limits quoted are taken from the best performing, based on expected exclusion CLs, signal regions from the tc-M, tc-C, t1L-bCa_low and WW analyses at each mass point. - Theoretical cross section from twiki.cern.ch/twiki/bin/view/LHCPhysics/SUSYCrossSections8TeVstopsbottom.
Upper limits on the stop pair production cross sections for different values of the branching ratios for the decays $\tilde{t}_1 \rightarrow c\tilde{\chi}_1^0$ and $\tilde{t}_1 \rightarrow ff'b\tilde{\chi}_1^0$, where BR$(\tilde{t}_1 \rightarrow c\tilde{\chi}_1^0)$ + BR$(\tilde{t}_1 \rightarrow ff'b\tilde{\chi}_1^0)$ = 1. Signal points with $\Delta m (\tilde{t}_1, \tilde{\chi}_1^0)$ of 80 GeV are shown. The limits quoted are taken from the best performing, based on expected exclusion CLs, signal regions from the tc-M, tc-C, t1L-bCa_low and WW analyses at each mass point. - Theoretical cross section from twiki.cern.ch/twiki/bin/view/LHCPhysics/SUSYCrossSections8TeVstopsbottom.
Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. This table is for the observed limit for BR=75% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.
Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. This table is for the expected limit for BR=75% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.
Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. Observed limit for BR=50% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.
Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. Expected limit for BR=50% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.
Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. Observed limit for BR=25% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.
Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. Expected limit for BR=25% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.
Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. Observed limit for BR=0% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.
Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. Expected limit for BR=0% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.
Summary of the ATLAS Run 1 searches for direct stop pair production in models where the decay mode $\tilde{t}_1 \rightarrow b \tilde{\chi}^{\pm}$ with $ \tilde{\chi}_1^{\pm} \rightarrow W \tilde{\chi_1^0}$ is assumed with a branching ratio of 100%. Limits for the b0L and t1L soft-lepton analyses in two scenarios Delta M = 5 GeV in light green and Delta M = 20 GeV in dark green), for a total of four limits - dM=5 GeV, b0L observed limit hepdata.cedar.ac.uk/view/ins1247462/d19 - dM=5 GeV, b0L expected limit hepdata.cedar.ac.uk/view/ins1247462/d22 - dM=5 GeV, t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d40 - dM=5 GeV, t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d41 - dM=20 GeV, b0L observed limit hepdata.cedar.ac.uk/view/ins1247462/d25 - dM=20 GeV, b0L expected limit hepdata.cedar.ac.uk/view/ins1247462/d28 - dM=20 GeV, t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d43 - dM=20 GeV, t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d44.
Summary of the ATLAS Run 1 searches for direct stop pair production in models where the decay mode $\tilde{t}_1 \rightarrow b \tilde{\chi}^{\pm}$ with $ \tilde{\chi}_1^{\pm} \rightarrow W \tilde{\chi_1^0}$ is assumed with a branching ratio of 100%.Limits for the b0L, t1L and t2L analyses in scenarios with a fixed chargino mass of 106 GeV (dark green) and 150 GeV (light green) - M(ch1)=150 GeV, b0L observed limit hepdata.cedar.ac.uk/view/ins1247462/d13 - M(ch1)=150 GeV, b0L expected limit hepdata.cedar.ac.uk/view/ins1247462/d16 - M(ch1)=150 GeV, t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d34 - M(ch1)=150 GeV, t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d35 - M(ch1)=106 GeV, t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d37 - M(ch1)=106 GeV, t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d38 - M(ch1)=106 GeV, t2L observed limit hepdata.cedar.ac.uk/view/ins1286444/d25 - M(ch1)=106 GeV, t2L expected limit hepdata.cedar.ac.uk/view/ins1286444/d26.
Summary of the ATLAS Run 1 searches for direct stop pair production in models where the decay mode $\tilde{t}_1 \rightarrow b \tilde{\chi}^{\pm}$ with $ \tilde{\chi}_1^{\pm} \rightarrow W \tilde{\chi_1^0}$ is assumed with a branching ratio of 100%.Limits for the t1L and t2L analyses in scenarios with the mass of the chargino set to twice the mass of the neutralino - M(ch1)=2M(chi0), t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d31 - M(ch1)=2M(chi0), t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d32 - M(ch1)=2M(chi0), t2L observed limit hepdata.cedar.ac.uk/view/ins1286444/d16 - M(ch1)=2M(chi0), t2L expected limit hepdata.cedar.ac.uk/view/ins1286444/d17.
Summary of the ATLAS Run 1 searches for direct stop pair production in models where the decay mode $\tilde{t}_1 \rightarrow b \tilde{\chi}^{\pm}$ with $ \tilde{\chi}_1^{\pm} \rightarrow W \tilde{\chi_1^0}$ is assumed with a branching ratio of 100%.Limits for the t1L and t2L and WW analyses in scenarios with the mass difference between chargino and neutralino is 10 GeV - dM=10 GeV, t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d46 - dM=10 GeV, t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d47 - dM=10 GeV, t2L observed limit hepdata.cedar.ac.uk/view/ins1286444/d10 - dM=10 GeV, t2L expected limit hepdata.cedar.ac.uk/view/ins1286444/d11 - dM=10 GeV, WW observed limit hepdata.cedar.ac.uk/view/ins1380183/d45 - dM=10 GeV, WW expected limit hepdata.cedar.ac.uk/view/ins1380183/d46.
Exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm + W^{(*)} + \tilde{\chi}_1^0$ with branching ratio of 100% assuming a fixed stop mass of 300 GeV. - t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d49 - t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d50 - b0L observed limit hepdata.cedar.ac.uk/view/ins1247462/d7 - b0L expected limit hepdata.cedar.ac.uk/view/ins1247462/d10.
Exclusion limits at 95% CL in the scenario where $\tilde{t}_2$ pair production is assumed, followed by the decay $\tilde{t}_2 \rightarrow Z \tilde{t}_1$ or $\tilde{t}_2 \rightarrow \tilde{t}_1 h$ and then by $\tilde{t}_1 \rightarrow t \tilde{\chi}_1^0$ with a branching ratio of 100%, as a function of the $\tilde{t}_2$ and $\tilde{\chi}_1^0$ mass. The $\tilde{t}_1$ mass is 180 GeV larger than the neutralino mass. This table is for the t2t1H observed limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d11 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d8.
Exclusion limits at 95% CL in the scenario where $\tilde{t}_2$ pair production is assumed, followed by the decay $\tilde{t}_2 \rightarrow Z \tilde{t}_1$ or $\tilde{t}_2 \rightarrow \tilde{t}_1 h$ and then by $\tilde{t}_1 \rightarrow t \tilde{\chi}_1^0$ with a branching ratio of 100%, as a function of the $\tilde{t}_2$ and $\tilde{\chi}_1^0$ mass. The $\tilde{t}_1$ mass is 180 GeV larger than the neutralino mass. This table is for the t2t1H expected limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d11 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d8.
Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=350 GeV and m(chi1)=20 GeV (top plot). This table is for the t2t1H observed limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d14 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d15.
Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=350 GeV and m(chi1)=20 GeV (top plot). This table is for the t2t1H expected limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d14 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d15.
Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=350 GeV and m(chi1)=20 GeV (top plot). This table is for the t1L/t0L observed limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d14 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d15.
Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=350 GeV and m(chi1)=20 GeV (top plot). This table is for the t1L/t0L expected limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d14 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d15.
Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=20 GeV (top plot). This table is for the t2t1H observed limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d16 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d17.
Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=20 GeV (top plot). This table is for the t2t1H expected limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d16 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d17.
Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=20 GeV (top plot). This table is for the t1L/t0L observed limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d16 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d17.
Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=20 GeV (top plot). This table is for the t1Lt0L expected limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d16 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d17.
Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=120 GeV (top plot). This table is for the t2t1H observed limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d18 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d19.
Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=120 GeV (top plot). This table is for the t2t1H expected limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d18 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d19.
Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=120 GeV (top plot). This table is for the t1L/t0L observed limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d18 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d19.
Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=120 GeV (top plot). This table is for the t1Lt0L expected limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d18 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d19.
Observed and expected 95% CL limits on sbottom pair production where the sbottom is assumed to decay as b1->b chi10 with a branching ratio of 100%. - b0L observed limit hepdata.cedar.ac.uk/view/ins1247462/d1 - b0L expected limit hepdata.cedar.ac.uk/view/ins1247462/d4 - tc observed limit hepdata.cedar.ac.uk/view/ins1304459 (root macro) - tc expected limit hepdata.cedar.ac.uk/view/ins1304459 (root macro).
Exclusion limits at 95% CL for a scenario where sbottoms are pair produced and decay as b1 -> t chi1+ with a BR of 100% - SS3L observed limit (mchi+=60 GeV): hepdata.cedar.ac.uk/resource/6164/finalExclusionGraphs/SBottomTopCharginoN60_observed.C - SS3L expected limit (mchi+=60 GeV): hepdata.cedar.ac.uk/resource/6164/finalExclusionGraphs/SBottomTopCharginoN60_expected.C - SS3L observed limit (mchi+=2 mchi0): hepdata.cedar.ac.uk/resource/6164/finalExclusionGraphs/SBottomTopCharginoNhalfC_observed.C - SS3L expected limit (mchi+=2 mchi0): hepdata.cedar.ac.uk/resource/6164/finalExclusionGraphs/SBottomTopCharginoNhalfC_expected.C.
Exclusion limits at 95% CL for a scenario where sbottoms are pair produced and decay as b1 -> b chi2 with a BR of 100% - g3b observed limit hepdata.cedar.ac.uk/view/ins1304457/d10 - g3b expected limit hepdata.cedar.ac.uk/view/ins1304457/d11.
Observed 95% CL exclusion limits for the naturalness-inspired set of pMSSM models from the combination t0L, t1L and tb analyses using the signal region yielding the smallest CLs value for the signal- plus-background hypothesis. This table is for the observed limit.
Expected 95% CL exclusion limits for the naturalness-inspired set of pMSSM models from the combination t0L, t1L and tb analyses using the signal region yielding the smallest CLs value for the signal- plus-background hypothesis. This table is for the expected limit.
Observed 95% CL exclusion limits for the pMSSM model with well-tempered neutralinos as a function of M1 and mqL3. The limit is obtained as the combination of the t0L, t1L, tb and SS3L analyses, This table is for the observed limit.
Expected 95% CL exclusion limits for the pMSSM model with well-tempered neutralinos as a function of M1 and mqL3. The limit is obtained as the combination of the t0L, t1L, tb and SS3L analyses, This table is for the expected limit.
Observed 95% CL exclusion limits for the pMSSM model with well-tempered neutralinos as a function of M1 and mtR. The limit is obtained using the t0L analysis. This table is for the observed limit.
Expected 95% CL exclusion limits for the pMSSM model with well-tempered neutralinos as a function of M1 and mtR. The limit is obtained using the t0L analysis. This table is for the expected limit.
Observed 95% CL exclusion limits for the set of h/Z-enriched pMSSM models as a function of $\mu$ and m(qL3). The limit of is obtained as the combination of the t0L, g3b, t2t1Z and SS3L analyses, This table is for the observed limit.
Expected 95% CL exclusion limits for the set of h/Z-enriched pMSSM models as a function of $\mu$ and m(qL3). The limit of is obtained as the combination of the t0L, g3b, t2t1Z and SS3L analyses, This table is for the expected limit.
Observed 95% CL exclusion limits for the set of h/Z-enriched pMSSM models as a function of $\mu$ and m(bR). The limit of is obtained as the combination of thet0L, t2t1Z and tb analyses, This table is for the observed limit.
Expected 95% CL exclusion limits for the set of h/Z-enriched pMSSM models as a function of $\mu$ and m(bR). The limit of is obtained as the combination of thet0L, t2t1Z and tb analyses, This table is for the expected limit.
Expected and observed 95% CL limits on the signal strength mu (defined as the ratio of the obtained stop cross section to the theoretical prediction) for the production of stop pairs as a function of m(stop). The stop is assumed to decay as t1->t chi0 or through its three-body decay depending on its mass. The neutralino is assumed to have a mass of 1 GeV.
Exclusion limits at 95% CL in the scenario where both pair-produced stop decay exclusively via $\tilde{t}_1 \rightarrow b \chi^\pm_1$ followed by $\chi^\pm_1 \rightarrow W \chi_1^0$ with $\Delta m(t_1, \chi_1^0)$ = 10 GeV. This table is for the observed limit.
Exclusion limits at 95% CL in the scenario where both pair-produced stop decay exclusively via $\tilde{t}_1 \rightarrow b \chi^\pm_1$ followed by $\chi^\pm_1 \rightarrow W \chi_1^0$ with $\Delta m(t_1, \chi_1^0)$ = 10 GeV. This table is for the expected limit.
Exclusion limits at 95% CL in the scenario where both pair-produced stop decay exclusively via three-body or four-body decay (depending on the neutralino and stop mass). This table is for the observed limit. - t1L observed limit (3-body) hepdata.cedar.ac.uk/view/ins1304456/d25 - t1L observed limit (4-body) hepdata.cedar.ac.uk/view/ins1304456/d28 - t2L observed limit hepdata.cedar.ac.uk/view/ins1286444/d23.
Exclusion limits at 95% CL in the scenario where both pair-produced stop decay exclusively via three-body or four-body decay (depending on the neutralino and stop mass). This table is for the expected limit. - t1L observed limit (3-body) hepdata.cedar.ac.uk/view/ins1304456/d25 - t1L observed limit (4-body) hepdata.cedar.ac.uk/view/ins1304456/d28 - t2L observed limit hepdata.cedar.ac.uk/view/ins1286444/d23.
Observed exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 25% and DM=5GeV. This table is for the Observed limit.
Expected exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 25% and DM=5GeV. This table is for the Expected limit.
Observed exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 25% and DM=20 GeV. This table is for the Observed limit.
Expected exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 25% and DM=20 GeV. This table is for the Expected limit.
Observed exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 50% and DM=5GeV. This table is for the Observed limit.
Expected exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 50% and DM=5 GeV. This table is for the Expected limit.
Observed exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 50% and DM=20GeV. This table is for the Observed limit.
Expected exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 50% and DM=20 GeV. This table is for the Expected limit.
Observed exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 75% and DM=5GeV. This table is for the Observed limit.
Expected exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 75% and DM=5 GeV. This table is for the Expected limit.
Observed exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 75% and DM=20GeV. This table is for the Observed limit.
Expected exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 75% and DM=20 GeV. This table is for the Expected limit.
Observed exclusion limits at 95% CL from the tb signal regions in the natural pMSSM model. This table is for the Observed limit.
Expected exclusion limits at 95% CL from the tb signal regions in the natural pMSSM model. This table is for the Expected limit.
Combined exclusion limits at 95% CL in the scenario where both stops decay exclusively via $\tilde t_1 \rightarrow t \tilde \chi_1^0 $. Observed limit contour line for the t0L/t1L combination.
Combined exclusion limits at 95% CL in the scenario where both stops decay exclusively via $\tilde t_1 \rightarrow t \tilde \chi_1^0 $. Expected limit contour line for the t0L/t1L combination.
Best expected SR for the WW analysis and the three- and four-body decays.
Cross-section upper limit for the WW analysis and the three- and four-body decays.
Expected CLs for the WW analysis and the 3- and 4-body decays.
Observed CLs for the WW analysis and the 3- and 4-body decays.
Best expected SR for the WW analysis and the stop1->chargino1 decay.
Cross section upper limit for the WW analysis and the stop1->chargino1 decay.
Expected CLs for the WW analysis and the stop1->chargino1 decay.
Observed CLs for the WW analysis and the stop1->chargino1 decay.
Cross section upper limit for the t2t1h analysis.
Expected CLs for the t2t1h analysis.
Observed CLs for the t2t1h analysis.
Best expected SR for the tb analysis in the pMSSM model.
Cross section upper limit for the tb analysis in the pMSSM model.
Efficiency for the SRinA signal region for the pMSSM model.
Efficiency for the SRinB signal region for the pMSSM model.
Efficiency for the SRinC signal region for the pMSSM model.
Efficiency for the SRexA signal region for the pMSSM model.
Best expected SR for the tb analysis in the simplified model with Delta(m) = 5 GeV and BR=50%.
Cross section upper limit for the tb analysis in the simplified model with Delta(m) = 5 GeV and BR=50%.
Best expected SR for the tb analysis in the simplified model with Delta(m) = 20 GeV and BR=50%.
Cross section upper limit for the tb analysis in the simplified model with Delta(m) = 20 GeV and BR=50%.
Best expected SR and cross section upper limit for the tb analysis in the simplified model with Delta(m) = 5 GeV and BR=25%.
Best expected SR and cross section upper limit for the tb analysis in the simplified model with Delta(m) = 20 GeV and BR=25%.
Best expected SR and cross section upper limit for the tb analysis in the simplified model with Delta(m) = 5 GeV and BR=75%.
Best expected SR and cross section upper limit for the tb analysis in the simplified model with Delta(m) = 20 GeV and BR=75%.
Exclusion limits for the naturalness-inspired set of pMSSM models from the combination t0L, t1L and tb analyses using the signal region yielding the smallest CLs value for the signal- plus-background hypothesis. This table is for the best expected signal region.
95% CL exclusion limits for the pMSSM model with well-tempered neutralinos as a function of M1 and mqL3. The limit is obtained as the combination of the t0L, t1L, tb and SS3L analyses, This table is for the best expected signal region.
Expected 95% CL exclusion limits for the pMSSM model with well-tempered neutralinos as a function of M1 and mtR. The limit is obtained using the t0L analysis. This table is for the best expected signal region.
95% CL exclusion limits for the set of h/Z-enriched pMSSM models as a function of $\mu$ and m(qL3). The limit of is obtained as the combination of the t0L, g3b, t2t1Z and SS3L analyses, This table is for the best expected signal region.
95% CL exclusion limits for the set of h/Z-enriched pMSSM models as a function of $\mu$ and m(bR). The limit of is obtained as the combination of the t0L, t2t1Z and tb analyses, This table is for the best expected signal region.
A search for new phenomena in final states characterized by high jet multiplicity, an isolated lepton (electron or muon) and either zero or at least three $b$-tagged jets is presented. The search uses 36.1 fb$^{-1}$ of $\sqrt{s}$ = 13 TeV proton-proton collision data collected by the ATLAS experiment at the Large Hadron Collider in 2015 and 2016. The dominant sources of background are estimated using parameterized extrapolations, based on observables at medium jet multiplicity, to predict the $b$-tagged jet multiplicity distribution at the higher jet multiplicities used in the search. No significant excess over the Standard Model expectation is observed and 95% confidence-level limits are extracted constraining four simplified models of $R$-parity-violating supersymmetry that feature either gluino or top-squark pair production. The exclusion limits reach as high as 2.1 TeV in gluino mass and 1.2 TeV in top-squark mass in the models considered. In addition, an upper limit is set on the cross-section for Standard Model $t\bar{t}t\bar{t}$ production of 60 fb (6.5 $\times$ the Standard Model prediction) at 95% confidence level. Finally, model-independent limits are set on the contribution from new phenomena to the signal-region yields.
The expected background and observed data with five jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with five jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with five jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with six jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with six jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with six jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with seven jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with seven jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with seven jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with eight jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with eight jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with eight jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with nine jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with nine jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with nine jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with ten jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with ten jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with ten jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with eleven jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with eleven jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with eleven jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with twelve-or-more jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with twelve-or-more jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with twelve-or-more jets in the different b-tag multiplicity bins for the 40 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with five jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with five jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with five jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with six jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with six jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with six jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with seven jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with seven jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with seven jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with eight jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with eight jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with eight jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with nine jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with nine jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with nine jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with ten-or-more jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with ten-or-more jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with ten-or-more jets in the different b-tag multiplicity bins for the 60 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with five jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with five jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with five jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with six jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with six jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with six jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with seven jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with seven jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with seven jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with eight jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with eight jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with eight jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with nine jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with nine jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with nine jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with ten-or-more jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with ten-or-more jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
The expected background and observed data with ten-or-more jets in the different b-tag multiplicity bins for the 80 GeV jet pT threshold. The background shown is estimated by including all bins in the fit.
Observed exclusion contours on the gluino and neutralino masses in a model where the gluino decays via a virtual top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino --> uds) via the RPV coupling lambda''_112.
Observed exclusion contours on the gluino and neutralino masses in a model where the gluino decays via a virtual top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino --> uds) via the RPV coupling lambda''_112.
Observed exclusion contours on the gluino and neutralino masses in a model where the gluino decays via a virtual top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino --> uds) via the RPV coupling lambda''_112.
Expected exclusion contours on the gluino and neutralino masses in a model where the gluino decays via a virtual top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino --> uds) via the RPV coupling lambda''_112.
Expected exclusion contours on the gluino and neutralino masses in a model where the gluino decays via a virtual top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino --> uds) via the RPV coupling lambda''_112.
Expected exclusion contours on the gluino and neutralino masses in a model where the gluino decays via a virtual top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino --> uds) via the RPV coupling lambda''_112.
Observed exclusion contours on the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Observed exclusion contours on the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Observed exclusion contours on the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Expected exclusion contours on the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Expected exclusion contours on the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Expected exclusion contours on the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Observed exclusion contours on the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Observed exclusion contours on the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Observed exclusion contours on the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Expected exclusion contours on the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Expected exclusion contours on the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Expected exclusion contours on the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Observed exclusion contours on the stop and neutralino masses in a model where the stop decays to a third-generation quark and a higgsino, which decays via the RPV coupling lambda''_323.
Observed exclusion contours on the stop and neutralino masses in a model where the stop decays to a third-generation quark and a higgsino, which decays via the RPV coupling lambda''_323.
Observed exclusion contours on the stop and neutralino masses in a model where the stop decays to a third-generation quark and a higgsino, which decays via the RPV coupling lambda''_323.
Expected exclusion contours on the stop and neutralino masses in a model where the stop decays to a third-generation quark and a higgsino, which decays via the RPV coupling lambda''_323.
Expected exclusion contours on the stop and neutralino masses in a model where the stop decays to a third-generation quark and a higgsino, which decays via the RPV coupling lambda''_323.
Expected exclusion contours on the stop and neutralino masses in a model where the stop decays to a third-generation quark and a higgsino, which decays via the RPV coupling lambda''_323.
Observed exclusion contours on the stop and neutralino masses in a model where the stop decays to a top and a bino-like neutralino, which decays via the RPV coupling lambda''_323.
Observed exclusion contours on the stop and neutralino masses in a model where the stop decays to a top and a bino-like neutralino, which decays via the RPV coupling lambda''_323.
Observed exclusion contours on the stop and neutralino masses in a model where the stop decays to a top and a bino-like neutralino, which decays via the RPV coupling lambda''_323.
Expected exclusion contours on the stop and neutralino masses in a model where the stop decays to a top and a bino-like neutralino, which decays via the RPV coupling lambda''_323.
Expected exclusion contours on the stop and neutralino masses in a model where the stop decays to a top and a bino-like neutralino, which decays via the RPV coupling lambda''_323.
Expected exclusion contours on the stop and neutralino masses in a model where the stop decays to a top and a bino-like neutralino, which decays via the RPV coupling lambda''_323.
Observed upper limits on the model cross-section in units of pb as a function of the gluino and neutralino masses in a model where the gluino decays via a virtual top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino --> uds) via the RPV coupling lambda''_112.
Observed upper limits on the model cross-section in units of pb as a function of the gluino and neutralino masses in a model where the gluino decays via a virtual top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino --> uds) via the RPV coupling lambda''_112.
Observed upper limits on the model cross-section in units of pb as a function of the gluino and neutralino masses in a model where the gluino decays via a virtual top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino --> uds) via the RPV coupling lambda''_112.
Observed upper limits on the model cross-section in units of pb as a function of the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Observed upper limits on the model cross-section in units of pb as a function of the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Observed upper limits on the model cross-section in units of pb as a function of the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Observed upper limits on the model cross-section in units of pb as a function of the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Observed upper limits on the model cross-section in units of pb as a function of the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Observed upper limits on the model cross-section in units of pb as a function of the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Observed upper limits on the model cross-section in units of pb as a function of the stop and neutralino masses in a model where the stop decays to a third-generation quark and a higgsino, which decays via the RPV coupling lambda''_323.
Observed upper limits on the model cross-section in units of pb as a function of the stop and neutralino masses in a model where the stop decays to a third-generation quark and a higgsino, which decays via the RPV coupling lambda''_323.
Observed upper limits on the model cross-section in units of pb as a function of the stop and neutralino masses in a model where the stop decays to a third-generation quark and a higgsino, which decays via the RPV coupling lambda''_323.
Observed upper limits on the model cross-section in units of pb as a function of the stop and neutralino masses in a model where the stop decays to a top and a bino-like neutralino, which decays via the RPV coupling lambda''_323.
Observed upper limits on the model cross-section in units of pb as a function of the stop and neutralino masses in a model where the stop decays to a top and a bino-like neutralino, which decays via the RPV coupling lambda''_323.
Observed upper limits on the model cross-section in units of pb as a function of the stop and neutralino masses in a model where the stop decays to a top and a bino-like neutralino, which decays via the RPV coupling lambda''_323.
Acceptance as a function of the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Acceptance as a function of the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Acceptance as a function of the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Efficiency as a function of the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Efficiency as a function of the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Efficiency as a function of the gluino and stop masses in a model where the gluino decays to a top quark and a top squark, with the top squark decaying to an s-quark and a b-quark via a non-zero lambda''_323 RPV coupling.
Acceptance as a function of the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Acceptance as a function of the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Acceptance as a function of the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Efficiency as a function of the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Efficiency as a function of the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Efficiency as a function of the gluino and neutralino masses in a model with a gluino decaying to two light quarks (q=u,d,s,c) and the neutralino, which then decays to two light quarks and a charged lepton or a neutrino.
Cut flow for a model of gluino pair production where the gluino decays to two (u, d, s, c) quarks and the neutralino, which then decays to two (u, d, s, c) quarks and a lepton via a lambda' RPV coupling, where each RPV decay can produce any of the four first and second generation leptons (e, mu, nu_e, nu_mu) with equal probability (m_gluino = 1800 GeV, m_neutralino = 900 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.
Cut flow for a model of gluino pair production where the gluino decays to two (u, d, s, c) quarks and the neutralino, which then decays to two (u, d, s, c) quarks and a lepton via a lambda' RPV coupling, where each RPV decay can produce any of the four first and second generation leptons (e, mu, nu_e, nu_mu) with equal probability (m_gluino = 1800 GeV, m_neutralino = 900 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.
Cut flow for a model of gluino pair production where the gluino decays to two (u, d, s, c) quarks and the neutralino, which then decays to two (u, d, s, c) quarks and a lepton via a lambda' RPV coupling, where each RPV decay can produce any of the four first and second generation leptons (e, mu, nu_e, nu_mu) with equal probability (m_gluino = 1800 GeV, m_neutralino = 900 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.
Cut flow for a model of gluino pair production where each gluino decays to a top quark and a top squark, with the top squark decaying to an s- and a b- quark via a non-zero lambda''_323 RPV coupling (m_gluino = 1600 GeV, m_stop = 1000 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.
Cut flow for a model of gluino pair production where each gluino decays to a top quark and a top squark, with the top squark decaying to an s- and a b- quark via a non-zero lambda''_323 RPV coupling (m_gluino = 1600 GeV, m_stop = 1000 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.
Cut flow for a model of gluino pair production where each gluino decays to a top quark and a top squark, with the top squark decaying to an s- and a b- quark via a non-zero lambda''_323 RPV coupling (m_gluino = 1600 GeV, m_stop = 1000 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.
Cut flow for a model of gluino pair production where each gluino decays via an off-shell top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino -> uds) via the RPV coupling lambda''_112 (m_gluino = 2000 GeV, m_neutralino = 941 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.
Cut flow for a model of gluino pair production where each gluino decays via an off-shell top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino -> uds) via the RPV coupling lambda''_112 (m_gluino = 2000 GeV, m_neutralino = 941 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.
Cut flow for a model of gluino pair production where each gluino decays via an off-shell top squark to two top quarks and the lightest neutralino, with the neutralino decaying to three light quarks (neutralino -> uds) via the RPV coupling lambda''_112 (m_gluino = 2000 GeV, m_neutralino = 941 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.
Cut flow for a model of right-handed top squark pair production with the top squark decaying to the lightest supersymmetric particle (LSP) which is considered to be purely higgsino. The higgsino-like LSP decays through the non-zero RPV coupling lambda''_323 (m_stop = 975 GeV, m_neutralino = 600 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.
Cut flow for a model of right-handed top squark pair production with the top squark decaying to the lightest supersymmetric particle (LSP) which is considered to be purely higgsino. The higgsino-like LSP decays through the non-zero RPV coupling lambda''_323 (m_stop = 975 GeV, m_neutralino = 600 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.
Cut flow for a model of right-handed top squark pair production with the top squark decaying to the lightest supersymmetric particle (LSP) which is considered to be purely higgsino. The higgsino-like LSP decays through the non-zero RPV coupling lambda''_323 (m_stop = 975 GeV, m_neutralino = 600 GeV). The events are skimmed by requiring at least one electron or muon that satisfies very loose identification criteria, where the lepton satisfies pT > 25 GeV. The efficiency of this cut is considered in the quoted efficiency of the lepton trigger requirement. Selections with negligible inefficiencies on the given sample, such as data quality requirements, are not displayed.
When you search on a word, e.g. 'collisions', we will automatically search across everything we store about a record. But, sometimes you may wish to be more specific. Here we show you how.
Guidance and examples on the query string syntax can be found in the Elasticsearch documentation.
About HEPData Submitting to HEPData HEPData File Formats HEPData Coordinators HEPData Terms of Use HEPData Cookie Policy
Status
Email
Forum
Twitter
GitHub
Copyright ~1975-Present, HEPData | Powered by Invenio, funded by STFC, hosted and originally developed at CERN, supported and further developed at IPPP Durham.