Showing 10 of 6305 results
The dynamics of isolated-photon plus one-, two- and three-jet production in $pp$ collisions at a centre-of-mass energy of 8 TeV are studied with the ATLAS detector at the LHC using a data set with an integrated luminosity of 20.2 fb$^{-1}$. Measurements of isolated-photon plus jets cross sections are presented as functions of the photon and jet transverse momenta. The cross sections as functions of the azimuthal angle between the photon and the jets, the azimuthal angle between the jets, the photon-jet invariant mass and the scattering angle in the photon-jet centre-of-mass system are presented. The pattern of QCD radiation around the photon and the leading jet is investigated by measuring jet production in an annular region centred on each object; enhancements are observed around the leading jet with respect to the photon in the directions towards the beams. The experimental measurements are compared to several different theoretical calculations, and overall a good description of the data is found.
Measured cross sections for isolated-photon plus 1jet production as a function of $E_{\rm T}^{\gamma}$.
Measured cross sections for isolated-photon plus 1jet production as a function of $p_{\rm T}^{\rm jet1}$.
Measured cross sections for isolated-photon plus 1jet production as a function of $m^{\gamma-\rm jet1}$.
Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$.
Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $467 < m^{\gamma-\rm jet1} < 510$ GeV.
Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $510 < m^{\gamma-\rm jet1} < 590$ GeV.
Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $590 < m^{\gamma-\rm jet1} < 670$ GeV.
Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $670 < m^{\gamma-\rm jet1} < 760$ GeV.
Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $760 < m^{\gamma-\rm jet1} < 850$ GeV.
Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $850 < m^{\gamma-\rm jet1} < 950$ GeV.
Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $0.95 < m^{\gamma-\rm jet1} < 1.05$ TeV.
Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $1.05 < m^{\gamma-\rm jet1} < 1.25$ TeV.
Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $1.25 < m^{\gamma-\rm jet1} < 2.45$ TeV.
Measured cross sections for isolated-photon plus 2jet production as a function of $E_{\rm T}^{\gamma}$.
Measured cross sections for isolated-photon plus 2jet production as a function of $p_{\rm T}^{\rm jet2}$.
Measured cross sections for isolated-photon plus 2jet production as a function of $\Delta\phi^{\rm \gamma-jet2}$.
Measured cross sections for isolated-photon plus 2jet production as a function of $\Delta\phi^{\rm jet1-jet2}$.
Measured cross sections for isolated-photon plus 2jet production as a function of $\Delta\phi^{\rm \gamma-jet2}$ for the range $130< E_{\rm T}^{\gamma} <300$ GeV.
Measured cross sections for isolated-photon plus 2jet production as a function of $\Delta\phi^{\rm \gamma-jet2}$ for the range $E_{\rm T}^{\gamma} >300$ GeV.
Measured cross sections for isolated-photon plus 2jet production as a function of $\Delta\phi^{\rm jet1-jet2}$ for the range $130< E_{\rm T}^{\gamma} <300$ GeV.
Measured cross sections for isolated-photon plus 2jet production as a function of $\Delta\phi^{\rm jet1-jet2}$ for the range $E_{\rm T}^{\gamma} >300$ GeV.
Measured cross sections for isolated-photon plus 2jet production as a function of $\beta^{\rm jet1}$.
Measured cross sections for isolated-photon plus 2jet production as a function of $\beta^{\gamma}$.
Ratio of measured cross sections for isolated-photon plus 2jet production as a function of $\beta$.
Measured cross sections for isolated-photon plus 3jet production as a function of $E_{\rm T}^{\gamma}$.
Measured cross sections for isolated-photon plus 3jet production as a function of $p_{\rm T}^{\rm jet3}$.
Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm \gamma-jet3}$.
Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm jet1-jet3}$.
Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm jet2-jet3}$.
Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm \gamma-jet3}$ for the range $130< E_{\rm T}^{\gamma} <300$ GeV.
Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm \gamma-jet3}$ for the range $E_{\rm T}^{\gamma} >300$ GeV.
Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm jet1-jet3}$ for the range $130< E_{\rm T}^{\gamma} <300$ GeV.
Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm jet1-jet3}$ for the range $E_{\rm T}^{\gamma} >300$ GeV.
Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm jet2-jet3}$ for the range $130< E_{\rm T}^{\gamma} <300$ GeV.
Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm jet2-jet3}$ for the range $E_{\rm T}^{\gamma} >300$ GeV.
The results of a search for new heavy $W^\prime$ bosons decaying to an electron or muon and a neutrino using proton-proton collision data at a centre-of-mass energy of $\sqrt{s} = 13$ TeV are presented. The dataset was collected in 2015 and 2016 by the ATLAS experiment at the Large Hadron Collider and corresponds to an integrated luminosity of 36.1 fb$^{-1}$. As no excess of events above the Standard Model prediction is observed, the results are used to set upper limits on the $W^\prime$ boson cross-section times branching ratio to an electron or muon and a neutrino as a function of the $W^\prime$ mass. Assuming a $W^\prime$ boson with the same couplings as the Standard Model $W$ boson, $W^\prime$ masses below 5.1 TeV are excluded at the 95% confidence level.
Transverse mass distribution for events satisfying all selection criteria in the electron channel.
Transverse mass distribution for events satisfying all selection criteria in the electron channel.
Transverse mass distribution for events satisfying all selection criteria in the muon channel.
Transverse mass distribution for events satisfying all selection criteria in the muon channel.
Upper limits at the 95% CL on the cross section for SSM W' production and decay to the electron+neutrino channel as a function of the W' pole mass.
Upper limits at the 95% CL on the cross section for SSM W' production and decay to the electron+neutrino channel as a function of the W' pole mass.
Upper limits at the 95% CL on the cross section for SSM W' production and decay to the muon+neutrino channel as a function of the W' pole mass.
Upper limits at the 95% CL on the cross section for SSM W' production and decay to the muon+neutrino channel as a function of the W' pole mass.
Combined (electron and muon channels) upper limits at the 95% CL on the cross section for SSM W' production and decay to a single lepton generation as a function of the W' pole mass.
Combined (electron and muon channels) upper limits at the 95% CL on the cross section for SSM W' production and decay to a single lepton generation as a function of the W' pole mass.
Product of acceptance and efficiency for the electron and muon selections as a function of the W' pole mass.
Product of acceptance and efficiency for the electron and muon selections as a function of the W' pole mass.
This paper presents a measurement of the polarisation of $\tau$ leptons produced in $Z/\gamma^{*}\rightarrow\tau\tau$ decays which is performed with a dataset of proton-proton collisions at $\sqrt{s}=8$ TeV, corresponding to an integrated luminosity of 20.2 fb$^{-1}$ recorded with the ATLAS detector at the LHC in 2012. The $Z/\gamma^{*}\rightarrow\tau\tau$ decays are reconstructed from a hadronically decaying $\tau$ lepton with a single charged particle in the final state, accompanied by a $\tau$ lepton that decays leptonically. The $\tau$ polarisation is inferred from the relative fraction of energy carried by charged and neutral hadrons in the hadronic $\tau$ decays. The polarisation is measured in a fiducial region that corresponds to the kinematic region accessible to this analysis. The $\tau$ polarisation extracted over the full phase space within the $Z/\gamma^{*}$ mass range of 66$ < m_{Z/\gamma^{*}} < $ 116 GeV is found to be $P_{\tau} =-0.14 \pm 0.02 (\text{stat}) \pm 0.04 (\text{syst})$. It is in agreement with the Standard Model prediction of $P_{\tau} =-0.1517 \pm 0.0019$, which is obtained from the ALPGEN event generator interfaced with the PYTHIA 6 parton shower modelling and the TAUOLA $\tau$ decay library.
The measured polarisation values (fiducial and extracted to full phase-space) for electron-hadron and muon-hadron channels as well as combined.
Definition of fiducial region of the analysis. The requirements are applied at stable-particle level.
Impact of individual systematic uncertainties on full and fiducial polarisation.
Impact of individual systematic uncertainties on full and fiducial polarisation in e-had channel.
Impact of individual systematic uncertainties on full and fiducial polarisation in mu-had channel.
Selection efficiency for signal events in the e-had channel. The last bin is for overflow.
Selection efficiency for signal events in the mu-had channel. The last bin is for overflow.
Selection efficiency for signal events in the e-had channel for events in the fiducial region only. The last bin is for overflow.
Selection efficiency for signal events in the mu-had channel for events in the fiducial region only. The last bin is for overflow.
A search for heavy resonances decaying into a pair of $Z$ bosons leading to $\ell^+\ell^-\ell^+\ell^-$ and $\ell^+\ell^-\nu\bar\nu$ final states, where $\ell$ stands for either an electron or a muon, is presented. The search uses proton proton collision data at a centre-of-mass energy of 13 TeV corresponding to an integrated luminosity of 36.1 fb$^{-1}$ collected with the ATLAS detector during 2015 and 2016 at the Large Hadron Collider. Different mass ranges for the hypothetical resonances are considered, depending on the final state and model. The different ranges span between 200 GeV and 2000 GeV. The results are interpreted as upper limits on the production cross section of a spin 0 or spin 2 resonance. The upper limits for the spin 0 resonance are translated to exclusion contours in the context of Type I and Type II two-Higgs-doublet models, while those for the spin 2 resonance are used to constrain the Randall Sundrum model with an extra dimension giving rise to spin 2 graviton excitations.
Distribution of the four-lepton invariant mass (m4l) in the four-lepton search for the ggF-enriched category.
Distribution of the four-lepton invariant mass (m4l) in the four-lepton search for the VBF-enriched category.
Transverse mass mT in the llnunu search for the electron channel.
Transverse mass mT in the llnunu search for the muon channel.
Upper limits at 95% CL on the cross section times branching ratio as a function of the heavy resonance mass mH for the ggF production mode
Upper limits at 95% CL on the cross section times branching ratio as a function of the heavy resonance mass mH for the VBF production mode
Upper limits at 95% CL on the cross section for the ggF production model times branching ratio as a function of mH for an additioinal heavy scalar assuming a width of 1% of mH
Upper limits at 95% CL on the cross section for the ggF production model times branching ratio as a function of mH for an additioinal heavy scalar assuming a width of 5% of mH
Upper limits at 95% CL on the cross section for the ggF production model times branching ratio as a function of mH for an additioinal heavy scalar assuming a width of 10% of mH
Upper limits at 95% CL on the cross section times branching ratio for a KK graviton produced with k/M_{PI} = 1.
A search for the electroweak production of charginos, neutralinos and sleptons decaying into final states involving two or three electrons or muons is presented. The analysis is based on 36.1 fb$^{-1}$ of $\sqrt{s}=13$ TeV proton--proton collisions recorded by the ATLAS detector at the Large Hadron Collider. Several scenarios based on simplified models are considered. These include the associated production of the next-to-lightest neutralino and the lightest chargino, followed by their decays into final states with leptons and the lightest neutralino via either sleptons or Standard Model gauge bosons; direct production of chargino pairs, which in turn decay into leptons and the lightest neutralino via intermediate sleptons; and slepton pair production, where each slepton decays directly into the lightest neutralino and a lepton. No significant deviations from the Standard Model expectation are observed and stringent limits at 95% confidence level are placed on the masses of relevant supersymmetric particles in each of these scenarios. For a massless lightest neutralino, masses up to 580 GeV are excluded for the associated production of the next-to-lightest neutralino and the lightest chargino, assuming gauge-boson mediated decays, whereas for slepton-pair production masses up to 500 GeV are excluded assuming three generations of mass-degenerate sleptons.
The mll distribution for data and the estimated SM backgrounds in the 2l+0jets channel for SR2-SF-loose. Two signal points are added for comparison.
The mT2 distribution for data and the estimated SM backgrounds in the 2l+0jets channel for SR2-SF-loose. Two signal points are added for comparison.
The mT2 distributions for data and the estimated SM backgrounds in the 2l+0jets channel for the SR2-DF-100 selection. Two signal points are added for comparison.
Distributions of ETmiss for data and the expected SM backgrounds in the 2l+jets channel for SR2-int/high, without the final ETmiss requirement applied. Two signal points are added for comparison.
Distributions of ETmiss for data and the expected SM backgrounds in the 2l+jets channel for SR2-low, without the final ETmiss requirement applied. Two signal points are added for comparison.
Distributions of ETmiss for data and the estimated SM backgrounds in the 3l channel for SR3-slep-a. Two signal points are added for comparison.
Distributions of ETmiss for data and the estimated SM backgrounds in the 3l channel for SR3-slep-b. Two signal points are added for comparison.
Distributions of the third leading lepton pT in SR3-slep-c,d,e. Two signal points are added for comparison.
Distributions of ETmiss for data and the estimated SM backgrounds in the 3l channel for SR3-WZ-0Ja,b,c. Two signal points are added for comparison.
Distributions of ETmiss for data and the estimated SM backgrounds in the 3l channel for SR3-WZ-1Ja. Two signal points are added for comparison.
Distributions of ETmiss for data and the estimated SM backgrounds in the 3l channel for SR3-WZ-1Jb. Two signal points are added for comparison.
Distributions of ETmiss for data and the estimated SM backgrounds in the 3l channel for SR3-WZ-1Jc. Two signal points are added for comparison.
Expected 95% CL exclusion limit for chargino-pair production.
Observed 95% CL exclusion limit for chargino-pair production.
Expected 95% CL exclusion limit for direct slepton production.
Observed 95% CL exclusion limit for direct slepton production.
Expected 95% CL exclusion limit for chargino-neutralino production with slepton-mediated decays.
Observed 95% CL exclusion limit for chargino-neutralino production with slepton-mediated decays.
Expected 95% CL exclusion limit for chargino-neutralino production with W/Z-mediated decays.
Observed 95% CL exclusion limit for chargino-neutralino production with W/Z-mediated decays.
The mT2 distributions for data and the estimated SM backgrounds in the exclusive SF signal regions of the 2l+0jets channel in the regions 111 < mll < 150 GeV (corresponding to SR2-SF-a,b,c,d). Two signal points are added for comparison.
The mT2 distributions for data and the estimated SM backgrounds in the exclusive SF signal regions of the 2l+0jets channel in the regions 150 < mll < 200 GeV (corresponding to SR2-SF-e,f,g,h). Two signal points are added for comparison.
The mT2 distributions for data and the estimated SM backgrounds in the exclusive SF signal regions of the 2l+0jets channel in the regions 200 < mll < 300 GeV (corresponding to SR2-SF-i,j,k,l). Two signal points are added for comparison.
The mT2 distributions for data and the estimated SM backgrounds in the exclusive SF signal regions of the 2l+0jets channel in the regions mll > 300 GeV (corresponding to SR2-SF-m). Two signal points are added for comparison.
Signal acceptance for C1C1 production in SR2-SFloose for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_1^\mp$ -> 2x $\ell \nu \widetilde{\chi}_1^0$ .
Signal efficiency for C1C1 production in SR2-SFloose for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_1^\mp$ -> 2x $\ell \nu \widetilde{\chi}_1^0$.
Signal acceptance for C1C1 production in SR2-SFtight for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_1^\mp$ -> 2x $\ell \nu \widetilde{\chi}_1^0$.
Signal efficiency for C1C1 production in SR2-SFtight for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_1^\mp$ -> 2x $\ell \nu \widetilde{\chi}_1^0$.
Signal acceptance for C1C1 production in SR2-DF100 for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_1^\mp$ -> 2x $\ell \nu \widetilde{\chi}_1^0$.
Signal efficiency for C1C1 production in SR2-DF100 for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_1^\mp$ -> 2x $\ell \nu \widetilde{\chi}_1^0$.
Signal acceptance for C1C1 production in SR2-DF150 for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_1^\mp$ -> 2x $\ell \nu \widetilde{\chi}_1^0$.
Signal efficiency for C1C1 production in SR2-DF150 for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_1^\mp$ -> 2x $\ell \nu \widetilde{\chi}_1^0$.
Signal acceptance for C1C1 production in SR2-DF200 for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_1^\mp$ -> 2x $\ell \nu \widetilde{\chi}_1^0$.
Signal efficiency for C1C1 production in SR2-DF200 for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_1^\mp$ -> 2x $\ell \nu \widetilde{\chi}_1^0$.
Signal acceptance for C1C1 production in SR2-DF300 for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_1^\mp$ -> 2x $\ell \nu \widetilde{\chi}_1^0$.
Signal efficiency for C1C1 production in SR2-DF300 for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_1^\mp$ -> 2x $\ell \nu \widetilde{\chi}_1^0$.
Signal acceptance for direct Slepton production in SR2-SF-Loose for the process P P -> $\tilde{\ell}^\pm \tilde{\ell}^\mp$ -> $\ell^\pm \ell^\mp \widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal efficiency for direct Slepton production in SR2-SF-Loose for the process P P -> $\tilde{\ell}^\pm \tilde{\ell}^\mp$ -> $\ell^\pm \ell^\mp \widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal acceptance for direct Slepton production in SR2-SF-Tight for the process P P -> $\tilde{\ell}^\pm \tilde{\ell}^\mp$ -> $\ell^\pm \ell^\mp \widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal efficiency for direct Slepton production in SR2-SF-Tight for the process P P -> $\tilde{\ell}^\pm \tilde{\ell}^\mp$ -> $\ell^\pm \ell^\mp \widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal acceptance for C1N2 production in SR2-low for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->2j) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal efficiency for C1N2 production in SR2-low for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->2j) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal acceptance for C1N2 production in SR2-int for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->2j) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal efficiency for C1N2 production in SR2-int for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->2j) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal acceptance for C1N2 production in SR2-high for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->2j) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal efficiency for C1N2 production in SR2-high for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->2j) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal acceptance for Slep production in SR3-slepa for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $\tilde{\ell}_L \tilde{\ell}_L l (\tilde{\nu}\nu), l \tilde{\nu} \tilde{\ell}_L (\tilde{\nu}\nu)$ -> $l \nu \widetilde{\chi}_1^0 l l (\nu \nu) \widetilde{\chi}_1^0$.
Signal efficiency for Slep production in SR3-slepa for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $\tilde{\ell}_L \tilde{\ell}_L l (\tilde{\nu}\nu), l \tilde{\nu} \tilde{\ell}_L (\tilde{\nu}\nu)$ -> $l \nu \widetilde{\chi}_1^0 l l (\nu \nu) \widetilde{\chi}_1^0$.
Signal acceptance for Slep production in SR3-slepb for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $\tilde{\ell}_L \tilde{\ell}_L l (\tilde{\nu}\nu), l \tilde{\nu} \tilde{\ell}_L (\tilde{\nu}\nu)$ -> $l \nu \widetilde{\chi}_1^0 l l (\nu \nu) \widetilde{\chi}_1^0$.
Signal efficiency for Slep production in SR3-slepb for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $\tilde{\ell}_L \tilde{\ell}_L l (\tilde{\nu}\nu), l \tilde{\nu} \tilde{\ell}_L (\tilde{\nu}\nu)$ -> $l \nu \widetilde{\chi}_1^0 l l (\nu \nu) \widetilde{\chi}_1^0$.
Signal acceptance for Slep production in SR3-slepc for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $\tilde{\ell}_L \tilde{\ell}_L l (\tilde{\nu}\nu), l \tilde{\nu} \tilde{\ell}_L (\tilde{\nu}\nu)$ -> $l \nu \widetilde{\chi}_1^0 l l (\nu \nu) \widetilde{\chi}_1^0$.
Signal efficiency for Slep production in SR3-slepc for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $\tilde{\ell}_L \tilde{\ell}_L l (\tilde{\nu}\nu), l \tilde{\nu} \tilde{\ell}_L (\tilde{\nu}\nu)$ -> $l \nu \widetilde{\chi}_1^0 l l (\nu \nu) \widetilde{\chi}_1^0$.
Signal acceptance for Slep production in SR3-slepd for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $\tilde{\ell}_L \tilde{\ell}_L l (\tilde{\nu}\nu), l \tilde{\nu} \tilde{\ell}_L (\tilde{\nu}\nu)$ -> $l \nu \widetilde{\chi}_1^0 l l (\nu \nu) \widetilde{\chi}_1^0$.
Signal efficiency for Slep production in SR3-slepd for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $\tilde{\ell}_L \tilde{\ell}_L l (\tilde{\nu}\nu), l \tilde{\nu} \tilde{\ell}_L (\tilde{\nu}\nu)$ -> $l \nu \widetilde{\chi}_1^0 l l (\nu \nu) \widetilde{\chi}_1^0$.
Signal acceptance for Slep production in SR3-slepe for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $\tilde{\ell}_L \tilde{\ell}_L l (\tilde{\nu}\nu), l \tilde{\nu} \tilde{\ell}_L (\tilde{\nu}\nu)$ -> $l \nu \widetilde{\chi}_1^0 l l (\nu \nu) \widetilde{\chi}_1^0$.
Signal efficiency for Slep production in SR3-slepe for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $\tilde{\ell}_L \tilde{\ell}_L l (\tilde{\nu}\nu), l \tilde{\nu} \tilde{\ell}_L (\tilde{\nu}\nu)$ -> $l \nu \widetilde{\chi}_1^0 l l (\nu \nu) \widetilde{\chi}_1^0$.
Signal acceptance for WZ production in SR3-WZ-0Ja for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->l $\nu$) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal efficiency for WZ production in SR3-WZ-0Ja for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->l $\nu$) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal acceptance for WZ production in SR3-WZ-0Jb for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->l $\nu$) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal efficiency for WZ production in SR3-WZ-0Jb for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->l $\nu$) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal acceptance for WZ production in SR3-WZ-0Jc for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->l $\nu$) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal efficiency for WZ production in SR3-WZ-0Jc for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->l $\nu$) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal acceptance for WZ production in SR3-WZ-1Ja for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->l $\nu$) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal efficiency for WZ production in SR3-WZ-1Ja for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->l $\nu$) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal acceptance for WZ production in SR3-WZ-1Jb for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->l $\nu$) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal efficiency for WZ production in SR3-WZ-1Jb for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->l $\nu$) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal acceptance for WZ production in SR3-WZ-1Jc for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->l $\nu$) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal efficiency for WZ production in SR3-WZ-1Jc for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->l $\nu$) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
Signal regions contributing to the observed exclusion limit for chargino-neutralino production with W/Z-mediated decays.
Expected 95% CL exclusion limit for chargino-neutralino production with W/Z-mediated decays in the 2l+jets channel.
Observed 95% CL exclusion limit for chargino-neutralino production with W/Z-mediated decays in the 2l+jets channel.
Expected 95% CL exclusion limit for chargino-neutralino production with W/Z-mediated decays in the 3l channel.
Observed 95% CL exclusion limit for chargino-neutralino production with W/Z-mediated decays in the 2l+jets channel.
Expected 95% CL exclusion limit for left-handed slepton production.
Observed 95% CL exclusion limit for left-handed slepton production.
Expected 95% CL exclusion limit for right-handed slepton production.
Observed 95% CL exclusion limit for right-handed slepton production.
95% upper limit on production cross-section for chargino-pair production.
95% upper limit on production cross-section for direct slepton production.
95% upper limit on production cross-section for chargino-neutralino production with slepton-mediated decays.
95% upper limit on production cross-section for chargino-neutralino production with W/Z-mediated decays
<b>Cutflow 1</b> Event counts for a signal point in SR2-SF-loose for the process P P -> $\tilde{\ell}^\pm \tilde{\ell}^\mp$ -> $\ell^\pm \ell^\mp \widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
<b>Cutflow 2</b> Event counts for a signal point in SR2-SF-loose and SR2-DF-100 for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $\tilde{\ell}_L \tilde{\ell}_L l (\tilde{\nu}\nu), l \tilde{\nu} \tilde{\ell}_L (\tilde{\nu}\nu)$ -> $l \nu \widetilde{\chi}_1^0 l l (\nu \nu) \widetilde{\chi}_1^0$.
<b>Cutflow 3</b> Event counts for two signal points in SR2-int for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $\tilde{\ell}_L \tilde{\ell}_L l (\tilde{\nu}\nu), l \tilde{\nu} \tilde{\ell}_L (\tilde{\nu}\nu)$ -> $l \nu \widetilde{\chi}_1^0 l l (\nu \nu) \widetilde{\chi}_1^0$.
<b>Cutflow 4</b> Event counts for two signal points in SR2-low for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_1^\mp$ -> 2x $\ell \nu \widetilde{\chi}_1^0$.
<b>Cutflow 5</b> Event counts for two signal points in SR3-WZ-0Ja/b/c and SR3-WZ-1Ja/b/c for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $W$(->l $\nu$) $Z$(->2l) $\widetilde{\chi}_1^0 \widetilde{\chi}_1^0$.
<b>Cutflow 6</b> Event counts for two signal points in SR3-slepa-e for the process P P -> $\widetilde{\chi}_1^\pm \widetilde{\chi}_2^0$ -> $\tilde{\ell}_L \tilde{\ell}_L l (\tilde{\nu}\nu), l \tilde{\nu} \tilde{\ell}_L (\tilde{\nu}\nu)$ -> $l \nu \widetilde{\chi}_1^0 l l (\nu \nu) \widetilde{\chi}_1^0$.
A search for supersymmetry involving the pair production of gluinos decaying via third-generation squarks into the lightest neutralino ($\displaystyle\tilde\chi^0_1$) is reported. It uses LHC proton--proton collision data at a centre-of-mass energy $\sqrt{s} = 13$ TeV with an integrated luminosity of 36.1 fb$^{-1}$ collected with the ATLAS detector in 2015 and 2016. The search is performed in events containing large missing transverse momentum and several energetic jets, at least three of which must be identified as originating from $b$-quarks. To increase the sensitivity, the sample is divided into subsamples based on the presence or absence of electrons or muons. No excess is found above the predicted background. For $\displaystyle\tilde\chi^0_1$ masses below approximately 300 GeV, gluino masses of less than 1.97 (1.92) TeV are excluded at 95% confidence level in simplified models involving the pair production of gluinos that decay via top (bottom) squarks. An interpretation of the limits in terms of the branching ratios of the gluinos into third-generation squarks is also provided. These results improve upon the exclusion limits obtained with the 3.2 fb$^{-1}$ of data collected in 2015.
Observed 95% CL exclusion contour for Gtt model.
Observed 95% CL exclusion contour for Gtt model.
Observed 95% CL exclusion contour for Gtt model.
Observed 95% CL exclusion contour for Gtt model.
Expected 95% CL exclusion contour for Gtt model.
Expected 95% CL exclusion contour for Gtt model.
Expected 95% CL exclusion contour for Gtt model.
Expected 95% CL exclusion contour for Gtt model.
Observed 95% CL exclusion contour for Gbb model.
Observed 95% CL exclusion contour for Gbb model.
Observed 95% CL exclusion contour for Gbb model.
Observed 95% CL exclusion contour for Gbb model.
Expected 95% CL exclusion contour for Gbb model.
Expected 95% CL exclusion contour for Gbb model.
Expected 95% CL exclusion contour for Gbb model.
Expected 95% CL exclusion contour for Gbb model.
Expected 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Distribution of ETMISS for SR-Gbb-VC.
Distribution of ETMISS for SR-Gbb-VC.
Distribution of ETMISS for SR-Gbb-VC.
Distribution of ETMISS for SR-Gbb-VC.
Distribution of ETMISS for SR-Gtt-1l-B.
Distribution of ETMISS for SR-Gtt-1l-B.
Distribution of ETMISS for SR-Gtt-1l-B.
Distribution of ETMISS for SR-Gtt-1l-B.
Distribution of ETMISS for SR-1L-II.
Distribution of ETMISS for SR-1L-II.
Distribution of ETMISS for SR-1L-II.
Distribution of ETMISS for SR-1L-II.
Distribution of ETMISS for SR-0L-HI.
Distribution of ETMISS for SR-0L-HI.
Distribution of ETMISS for SR-0L-HI.
Distribution of ETMISS for SR-0L-HI.
Distribution of ETMISS for SR-0L-HH.
Distribution of ETMISS for SR-0L-HH.
Distribution of ETMISS for SR-0L-HH.
Distribution of ETMISS for SR-0L-HH.
Acceptances for Gbb model in SR-Gbb-B.
Acceptances for Gbb model in SR-Gbb-B.
Acceptances for Gbb model in SR-Gbb-B.
Acceptances for Gbb model in SR-Gbb-B.
Acceptances for Gbb model in SR-Gbb-M.
Acceptances for Gbb model in SR-Gbb-M.
Acceptances for Gbb model in SR-Gbb-M.
Acceptances for Gbb model in SR-Gbb-M.
Acceptances for Gbb model in SR-Gbb-C.
Acceptances for Gbb model in SR-Gbb-C.
Acceptances for Gbb model in SR-Gbb-C.
Acceptances for Gbb model in SR-Gbb-C.
Acceptances for Gbb model in SR-Gbb-VC.
Acceptances for Gbb model in SR-Gbb-VC.
Acceptances for Gbb model in SR-Gbb-VC.
Acceptances for Gbb model in SR-Gbb-VC.
Acceptances for Gtt model in SR-Gtt-0l-B.
Acceptances for Gtt model in SR-Gtt-0l-B.
Acceptances for Gtt model in SR-Gtt-0l-B.
Acceptances for Gtt model in SR-Gtt-0l-B.
Acceptances for Gtt model in SR-Gtt-0l-M.
Acceptances for Gtt model in SR-Gtt-0l-M.
Acceptances for Gtt model in SR-Gtt-0l-M.
Acceptances for Gtt model in SR-Gtt-0l-M.
Acceptances for Gtt model in SR-Gtt-0l-C.
Acceptances for Gtt model in SR-Gtt-0l-C.
Acceptances for Gtt model in SR-Gtt-0l-C.
Acceptances for Gtt model in SR-Gtt-0l-C.
Acceptances for Gtt model in SR-Gtt-1l-B.
Acceptances for Gtt model in SR-Gtt-1l-B.
Acceptances for Gtt model in SR-Gtt-1l-B.
Acceptances for Gtt model in SR-Gtt-1l-B.
Acceptances for Gtt model in SR-Gtt-1l-M.
Acceptances for Gtt model in SR-Gtt-1l-M.
Acceptances for Gtt model in SR-Gtt-1l-M.
Acceptances for Gtt model in SR-Gtt-1l-M.
Acceptances for Gtt model in SR-Gtt-1l-C.
Acceptances for Gtt model in SR-Gtt-1l-C.
Acceptances for Gtt model in SR-Gtt-1l-C.
Acceptances for Gtt model in SR-Gtt-1l-C.
Experimental efficiencies for Gbb model in SR-Gbb-B.
Experimental efficiencies for Gbb model in SR-Gbb-B.
Experimental efficiencies for Gbb model in SR-Gbb-B.
Experimental efficiencies for Gbb model in SR-Gbb-B.
Experimental efficiencies for Gbb model in SR-Gbb-M.
Experimental efficiencies for Gbb model in SR-Gbb-M.
Experimental efficiencies for Gbb model in SR-Gbb-M.
Experimental efficiencies for Gbb model in SR-Gbb-M.
Experimental efficiencies for Gbb model in SR-Gbb-C.
Experimental efficiencies for Gbb model in SR-Gbb-C.
Experimental efficiencies for Gbb model in SR-Gbb-C.
Experimental efficiencies for Gbb model in SR-Gbb-C.
Experimental efficiencies for Gbb model in SR-Gbb-VC.
Experimental efficiencies for Gbb model in SR-Gbb-VC.
Experimental efficiencies for Gbb model in SR-Gbb-VC.
Experimental efficiencies for Gbb model in SR-Gbb-VC.
Experimental efficiencies for Gtt model in SR-Gtt-0l-B.
Experimental efficiencies for Gtt model in SR-Gtt-0l-B.
Experimental efficiencies for Gtt model in SR-Gtt-0l-B.
Experimental efficiencies for Gtt model in SR-Gtt-0l-B.
Experimental efficiencies for Gtt model in SR-Gtt-0l-M.
Experimental efficiencies for Gtt model in SR-Gtt-0l-M.
Experimental efficiencies for Gtt model in SR-Gtt-0l-M.
Experimental efficiencies for Gtt model in SR-Gtt-0l-M.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
Experimental efficiencies for Gtt model in SR-Gtt-1l-B.
Experimental efficiencies for Gtt model in SR-Gtt-1l-B.
Experimental efficiencies for Gtt model in SR-Gtt-1l-B.
Experimental efficiencies for Gtt model in SR-Gtt-1l-B.
Experimental efficiencies for Gtt model in SR-Gtt-1l-M.
Experimental efficiencies for Gtt model in SR-Gtt-1l-M.
Experimental efficiencies for Gtt model in SR-Gtt-1l-M.
Experimental efficiencies for Gtt model in SR-Gtt-1l-M.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-VC.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-VC.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-VC.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-VC.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-C.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Expected number of signal events after each step of the Gbb-0L-B selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-B selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-B selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-B selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-M selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-M selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-M selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-M selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-C selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-C selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-C selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-C selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-VC selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-VC selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-VC selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-VC selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gtt-1L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
A measurement of $b$-hadron pair production is presented, based on a data set corresponding to an integrated luminosity of 11.4 fb$^{-1}$ of proton--proton collisions recorded at $\sqrt{s}=8$ TeV with the ATLAS detector at the LHC. Events are selected in which a $b$-hadron is reconstructed in a decay channel containing $J/\psi \rightarrow \mu\mu$, and a second $b$-hadron is reconstructed in a decay channel containing a muon. Results are presented in a fiducial volume defined by kinematic requirements on three muons based on those used in the analysis. The fiducial cross section is measured to be $17.7 \pm 0.1 ($stat.$) \pm 2.0 ($syst.$)$ nb. A number of normalised differential cross sections are also measured, and compared to predictions from the Pythia8, Herwig++, MadGraph5\_aMC@NLO+Pythia8 and Sherpa event generators, providing new constraints on heavy flavour production.
Normalised differential cross sections and corresponding uncertainties in bins of $\Delta R(J/\psi,\mu)$.
Transfer functions for $\Delta R(b-hadron,b-hadron)$.
$B_{c}$ and $B + D$ corrections removed from the fitted data for $\Delta R(J/\psi,\mu)$.
Normalised differential cross sections and corresponding uncertainties in bins of $\Delta R(J/\psi,\mu) (p_{T} \ge 20 { GeV})$.
Transfer functions for $\Delta R(b-hadron,b-hadron) (p_{T} \ge 20 { GeV})$.
$B_{c}$ and $B + D$ corrections removed from the fitted data for $\Delta R(J/\psi,\mu) (p_{T} \ge 20 { GeV})$.
Normalised differential cross sections and corresponding uncertainties in bins of $\Delta R(J/\psi,\mu) (p_{T} < 20 { GeV})$.
Transfer functions for $\Delta R(b-hadron,b-hadron) (p_{T} < 20 { GeV})$.
$B_{c}$ and $B + D$ corrections removed from the fitted data for $\Delta R(J/\psi,\mu) (p_{T} < 20 { GeV})$.
Normalised differential cross sections and corresponding uncertainties in bins of $\Delta\phi(J/\psi,\mu)$ [rad].
Transfer functions for $\Delta\phi(b-hadron,b-hadron)$ [rad].
$B_{c}$ and $B + D$ corrections removed from the fitted data for $\Delta\phi(J/\psi,\mu)$ [rad].
Normalised differential cross sections and corresponding uncertainties in bins of $\Delta y(J/\psi,\mu)$.
Transfer functions for $\Delta y(b-hadron,b-hadron)$.
$B_{c}$ and $B + D$ corrections removed from the fitted data for $\Delta y(J/\psi,\mu)$.
Normalised differential cross sections and corresponding uncertainties in bins of $m^{\mu\mu\mu} / p_{T}^{\mu\mu\mu}$.
Transfer functions for $m^{b-hadron,b-hadron} / p_{T}^{b-hadron,b-hadron}$.
$B_{c}$ and $B + D$ corrections removed from the fitted data for $m^{\mu\mu\mu} / p_{T}^{\mu\mu\mu}$.
Normalised differential cross sections and corresponding uncertainties in bins of $p_{T}^{\mu\mu\mu} / m^{\mu\mu\mu}$.
Transfer functions for $p_{T}^{b-hadron,b-hadron} / m^{b-hadron,b-hadron}$.
$B_{c}$ and $B + D$ corrections removed from the fitted data for $p_{T}^{\mu\mu\mu} / m^{\mu\mu\mu}$.
Normalised differential cross sections and corresponding uncertainties in bins of $p_{T}(J/\psi,\mu)$ [GeV].
Transfer functions for $p_{T}(b-hadron,b-hadron)$ [GeV].
$B_{c}$ and $B + D$ corrections removed from the fitted data for $p_{T}(J/\psi,\mu)$ [GeV].
Normalised differential cross sections and corresponding uncertainties in bins of $m(J/\psi,\mu)$ [GeV].
Transfer functions for $m(b-hadron,b-hadron)$ [GeV].
$B_{c}$ and $B + D$ corrections removed from the fitted data for $m(J/\psi,\mu)$ [GeV].
Transfer functions for $y_{boost}(b-hadron,b-hadron)$.
Normalised differential cross sections and corresponding uncertainties in bins of $y_{boost}(J/\psi,\mu)$.
$B_{c}$ and $B + D$ corrections removed from the fitted data for $y_{boost}(J/\psi,\mu)$.
Measurements of normalized differential cross-sections of top-quark pair production are presented as a function of the top-quark, $t\bar{t}$ system and event-level kinematic observables in proton-proton collisions at a centre-of-mass energy of $\sqrt{s}=8$ TeV}. The observables have been chosen to emphasize the $t\bar{t}$ production process and to be sensitive to effects of initial- and final-state radiation, to the different parton distribution functions, and to non-resonant processes and higher-order corrections. The dataset corresponds to an integrated luminosity of 20.3 fb$^{-1}$, recorded in 2012 with the ATLAS detector at the CERN Large Hadron Collider. Events are selected in the lepton+jets channel, requiring exactly one charged lepton and at least four jets with at least two of the jets tagged as originating from a $b$-quark. The measured spectra are corrected for detector effects and are compared to several Monte Carlo simulations. The results are in fair agreement with the predictions over a wide kinematic range. Nevertheless, most generators predict a harder top-quark transverse momentum distribution at high values than what is observed in the data. Predictions beyond NLO accuracy improve the agreement with data at high top-quark transverse momenta. Using the current settings and parton distribution functions, the rapidity distributions are not well modelled by any generator under consideration. However, the level of agreement is improved when more recent sets of parton distribution functions are used.
Fiducial phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system invariant mass $m^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system invariant mass $m^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system transverse momentum $p_{T}^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system transverse momentum $p_{T}^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t$}$ system absolute rapidity $|y^{t\bar{t}}|$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t$}$ system absolute rapidity $|y^{t\bar{t}}|$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the hadronic top-quark transverse momentum $p_{T}^{t}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the hadronic top-quark transverse momentum $p_{T}^{t}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the hadronic top-quark absolute rapidity $|y^{t}|$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the hadronic top-quark absolute rapidity $|y^{t}|$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system absolute out-of-plane momentum $|p_{out}^{t\bar{t}}|$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system absolute out-of-plane momentum $|p_{out}^{t\bar{t}}|$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system azimuthal angle $\Delta \phi^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system azimuthal angle $\Delta \phi^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the scalar sum of the hadronic and leptonic top-quark transverse momenta $H_{T}^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the scalar sum of the hadronic and leptonic top-quark transverse momenta $H_{T}^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for $y_{boost}^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for $y_{boost}^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for $\chi^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for $\chi^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for $R_{Wt}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Fiducial phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for $R_{Wt}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system invariant mass $m^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system invariant mass $m^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system transverse momentum $p_{T}^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system transverse momentum $p_{T}^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system absolute rapidity $|y^{t\bar{t}}|$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system absolute rapidity $|y^{t\bar{t}}|$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the top-quark transverse momentum $p_{T}^{t}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the top-quark transverse momentum $p_{T}^{t}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the top-quark absolute rapidity $|y^{t}|$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the top-quark absolute rapidity $|y^{t}|$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system absolute out-of-plane momentum $|p_{out}^{t\bar{t}}|$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system absolute out-of-plane momentum $|p_{out}^{t\bar{t}}|$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system azimuthal angle $\Delta \phi^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the $t\bar{t}$ system azimuthal angle $\Delta \phi^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for the scalar sum of the hadronic and leptonic top-quark transverse momenta $H_{T}^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for the scalar sum of the hadronic and leptonic top-quark transverse momenta $H_{T}^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for $y_{boost}^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for $y_{boost}^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space absolute differential cross-sections after combining the e+jets and $\mu$+jets channels for $\chi^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Full phase-space relative differential cross-sections after combining the e+jets and $\mu$+jets channels for $\chi^{t\bar{t}}$. All uncertainties are quoted as a percentage with respect to the cross-section values in each bin.
Absolute statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system invariant mass $m^{t\bar{t}}$.
Relative statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system invariant mass $m^{t\bar{t}}$.
Absolute systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system invariant mass $m^{t\bar{t}}$.
Relative systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system invariant mass $m^{t\bar{t}}$.
Absolute statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system transverse momentum $p_{T}^{t\bar{t}}$.
Relative statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system transverse momentum $p_{T}^{t\bar{t}}$.
Absolute systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system transverse momentum $p_{T}^{t\bar{t}}$.
Relative systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system transverse momentum $p_{T}^{t\bar{t}}$.
Absolute statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t$}$ system absolute rapidity $|y^{t\bar{t}}|$.
Relative statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t$}$ system absolute rapidity $|y^{t\bar{t}}|$.
Absolute systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t$}$ system absolute rapidity $|y^{t\bar{t}}|$.
Relative systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t$}$ system absolute rapidity $|y^{t\bar{t}}|$.
Absolute statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the hadronic top-quark transverse momentum $p_{T}^{t}$.
Relative statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the hadronic top-quark transverse momentum $p_{T}^{t}$.
Absolute systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the hadronic top-quark transverse momentum $p_{T}^{t}$.
Relative systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the hadronic top-quark transverse momentum $p_{T}^{t}$.
Absolute statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the hadronic top-quark absolute rapidity $|y^{t}|$.
Relative statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the hadronic top-quark absolute rapidity $|y^{t}|$.
Absolute systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the hadronic top-quark absolute rapidity $|y^{t}|$.
Relative systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the hadronic top-quark absolute rapidity $|y^{t}|$.
Absolute statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system out-of-plane momentum $|p_{out}^{t\bar{t}}|$.
Relative statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system out-of-plane momentum $|p_{out}^{t\bar{t}}|$.
Absolute systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system out-of-plane momentum $|p_{out}^{t\bar{t}}|$.
Relative systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system out-of-plane momentum $|p_{out}^{t\bar{t}}|$.
Absolute statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system azimuthal angle $\Delta \phi^{t\bar{t}}$.
Relative statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system azimuthal angle $\Delta \phi^{t\bar{t}}$.
Absolute systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system azimuthal angle $\Delta \phi^{t\bar{t}}$.
Relative systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the $t\bar{t}$ system azimuthal angle $\Delta \phi^{t\bar{t}}$.
Absolute statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the scalar sum of the hadronic and leptonic top-quark transverse momenta $H_{T}^{t\bar{t}}$.
Relative statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the scalar sum of the hadronic and leptonic top-quark transverse momenta $H_{T}^{t\bar{t}}$.
Absolute systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the scalar sum of the hadronic and leptonic top-quark transverse momenta $H_{T}^{t\bar{t}}$.
Relative systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the the scalar sum of the hadronic and leptonic top-quark transverse momenta $H_{T}^{t\bar{t}}$.
Absolute statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the longitudinal boost $y_{boost}^{t\bar{t}}$.
Relative statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the longitudinal boost $y_{boost}^{t\bar{t}}$.
Absolute systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the longitudinal boost $y_{boost}^{t\bar{t}}$.
Relative systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the longitudinal boost $y_{boost}^{t\bar{t}}$.
Absolute statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the production angle $\chi^{t\bar{t}}$.
Relative statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the production angle $\chi^{t\bar{t}}$.
Absolute systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the production angle $\chi^{t\bar{t}}$.
Relative systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the production angle $\chi^{t\bar{t}}$.
Absolute statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the ratio of the hadronic W and the hadronic top transverse momenta $R_{Wt}$.
Relative statistics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the ratio of the hadronic W and the hadronic top transverse momenta $R_{Wt}$.
Absolute systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the ratio of the hadronic W and the hadronic top transverse momenta $R_{Wt}$.
Relative systematics-only correlation matrix of the fiducial phase-space differential cross-section as a function of the ratio of the hadronic W and the hadronic top transverse momenta $R_{Wt}$.
Absolute statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system invariant mass $m^{t\bar{t}}$.
Relative statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system invariant mass $m^{t\bar{t}}$.
Absolute systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system invariant mass $m^{t\bar{t}}$.
Relative systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system invariant mass $m^{t\bar{t}}$.
Absolute statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system transverse momentum $p_{T}^{t\bar{t}}$.
Relative statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system transverse momentum $p_{T}^{t\bar{t}}$.
Absolute systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system transverse momentum $p_{T}^{t\bar{t}}$.
Relative systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system transverse momentum $p_{T}^{t\bar{t}}$.
Absolute statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t$}$ system absolute rapidity $|y^{t\bar{t}}|$.
Relative statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t$}$ system absolute rapidity $|y^{t\bar{t}}|$.
Absolute systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t$}$ system absolute rapidity $|y^{t\bar{t}}|$.
Relative systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t$}$ system absolute rapidity $|y^{t\bar{t}}|$.
Absolute statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the hadronic top-quark transverse momentum $p_{T}^{t}$.
Relative statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the hadronic top-quark transverse momentum $p_{T}^{t}$.
Absolute systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the hadronic top-quark transverse momentum $p_{T}^{t}$.
Relative systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the hadronic top-quark transverse momentum $p_{T}^{t}$.
Absolute statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the hadronic top-quark absolute rapidity $|y^{t}|$.
Relative statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the hadronic top-quark absolute rapidity $|y^{t}|$.
Absolute systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the hadronic top-quark absolute rapidity $|y^{t}|$.
Relative systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the hadronic top-quark absolute rapidity $|y^{t}|$.
Absolute statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system out-of-plane momentum $|p_{out}^{t\bar{t}}|$.
Relative statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system out-of-plane momentum $|p_{out}^{t\bar{t}}|$.
Absolute systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system out-of-plane momentum $|p_{out}^{t\bar{t}}|$.
Relative systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system out-of-plane momentum $|p_{out}^{t\bar{t}}|$.
Absolute statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system azimuthal angle $\Delta \phi^{t\bar{t}}$.
Relative statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system azimuthal angle $\Delta \phi^{t\bar{t}}$.
Absolute systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system azimuthal angle $\Delta \phi^{t\bar{t}}$.
Relative systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the $t\bar{t}$ system azimuthal angle $\Delta \phi^{t\bar{t}}$.
Absolute statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the scalar sum of the hadronic and leptonic top-quark transverse momenta $H_{T}^{t\bar{t}}$.
Relative statistics-only correlation matrix of the full phase-space differential cross-section as a function of the the scalar sum of the hadronic and leptonic top-quark transverse momenta $H_{T}^{t\bar{t}}$.
Absolute systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the scalar sum of the hadronic and leptonic top-quark transverse momenta $H_{T}^{t\bar{t}}$.
Relative systematics-only correlation matrix of the full phase-space differential cross-section as a function of the the scalar sum of the hadronic and leptonic top-quark transverse momenta $H_{T}^{t\bar{t}}$.
Absolute statistics-only correlation matrix of the full phase-space differential cross-section as a function of the longitudinal boost $y_{boost}^{t\bar{t}}$.
Relative statistics-only correlation matrix of the full phase-space differential cross-section as a function of the longitudinal boost $y_{boost}^{t\bar{t}}$.
Absolute systematics-only correlation matrix of the full phase-space differential cross-section as a function of the longitudinal boost $y_{boost}^{t\bar{t}}$.
Relative systematics-only correlation matrix of the full phase-space differential cross-section as a function of the longitudinal boost $y_{boost}^{t\bar{t}}$.
Absolute statistics-only correlation matrix of the full phase-space differential cross-section as a function of the production angle $\chi^{t\bar{t}}$.
Relative statistics-only correlation matrix of the full phase-space differential cross-section as a function of the production angle $\chi^{t\bar{t}}$.
Absolute systematics-only correlation matrix of the full phase-space differential cross-section as a function of the production angle $\chi^{t\bar{t}}$.
Relative systematics-only correlation matrix of the full phase-space differential cross-section as a function of the production angle $\chi^{t\bar{t}}$.
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and |$p_{out}^{t\bar{t}}$| (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $\chi^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $\Delta\phi^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15]
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $H_T^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $y_{boost}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $|y^{t,had}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5]
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $p_{T}^{t,had}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $\chi^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $\Delta\phi^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15]
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $H_T^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $y_{boost}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $|y^{t,had}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5]
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t,had}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $\Delta\phi^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15]
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $H_T^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $y_{boost}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $|y^{t,had}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5]
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t,had}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $H_T^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $H_T^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV Columns: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV
Statistical correlation matrix between $H_T^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $y_{boost}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV Columns: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV
Statistical correlation matrix between $H_T^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $|y^{t,had}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV Columns: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5]
Statistical correlation matrix between $H_T^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t,had}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV Columns: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV
Statistical correlation matrix between $H_T^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between $H_T^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $H_T^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $y_{boost}$ (rows) in the 4-jet inclusive configuration and $y_{boost}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV Columns: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV
Statistical correlation matrix between $y_{boost}$ (rows) in the 4-jet inclusive configuration and $|y^{t,had}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV Columns: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5]
Statistical correlation matrix between $y_{boost}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t,had}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV Columns: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV
Statistical correlation matrix between $y_{boost}$ (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between $y_{boost}$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $y_{boost}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $|y^{t,had}|$ (rows) in the 4-jet inclusive configuration and $|y^{t,had}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5] Columns: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5]
Statistical correlation matrix between $|y^{t,had}|$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t,had}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5] Columns: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV
Statistical correlation matrix between $|y^{t,had}|$ (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5] Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between $|y^{t,had}|$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5] Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $|y^{t,had}|$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5] Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $p_{T}^{t,had}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t,had}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV Columns: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV
Statistical correlation matrix between $p_{T}^{t,had}$ (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between $p_{T}^{t,had}$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $p_{T}^{t,had}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $|y^{t\bar{t}}|$ (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5] Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between $|y^{t\bar{t}}|$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5] Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $|y^{t\bar{t}}|$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5] Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $m^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $m^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $p_{T}^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from absolute spectra through the Bootstrap Method. The binning is the following: Rows: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and |$p_{out}^{t\bar{t}}$| (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $\chi^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $\Delta\phi^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15]
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $H_T^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $y_{boost}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $|y^{t,had}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5]
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $p_{T}^{t,had}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between |$p_{out}^{t\bar{t}}$| (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-40, 40-80, 80-120, 120-170, 170-230, 230-600] GeV Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $\chi^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $\Delta\phi^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15]
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $H_T^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $y_{boost}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $|y^{t,had}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5]
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t,had}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $\chi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [1-1.4, 1.4-1.9, 1.9-2.5, 2.5-3.2, 3.2-4.2, 4.2-5.5, 5.5-7.2, 7.2-9.3, 9.3-12, 12-20] GeV Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $\Delta\phi^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15]
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $H_T^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $y_{boost}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $|y^{t,had}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5]
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t,had}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $\Delta\phi^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0.0-2.0, 2.0-2.75, 2.75-3.0, 3.0-3.15] Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $H_T^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $H_T^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV Columns: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV
Statistical correlation matrix between $H_T^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $y_{boost}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV Columns: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV
Statistical correlation matrix between $H_T^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $|y^{t,had}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV Columns: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5]
Statistical correlation matrix between $H_T^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t,had}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV Columns: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV
Statistical correlation matrix between $H_T^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between $H_T^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $H_T^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-90, 90-140, 140-195, 195-255, 255-320, 320-385, 385-455, 455-530, 530-610, 610-695, 695-780, 780-865, 865-950, 950-1041, 1041-1500] GeV Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $y_{boost}$ (rows) in the 4-jet inclusive configuration and $y_{boost}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV Columns: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV
Statistical correlation matrix between $y_{boost}$ (rows) in the 4-jet inclusive configuration and $|y^{t,had}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV Columns: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5]
Statistical correlation matrix between $y_{boost}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t,had}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV Columns: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV
Statistical correlation matrix between $y_{boost}$ (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between $y_{boost}$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $y_{boost}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.1, 0.1-0.2, 0.2-0.3, 0.3-0.4, 0.4-0.5, 0.5-0.6, 0.6-0.7, 0.7-0.8, 0.8-0.9, 0.9-1, 1-1.1, 1.1-1.2, 1.2-1.3, 1.3-1.4, 1.4-1.5, 1.5-2] GeV Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $|y^{t,had}|$ (rows) in the 4-jet inclusive configuration and $|y^{t,had}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5] Columns: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5]
Statistical correlation matrix between $|y^{t,had}|$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t,had}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5] Columns: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV
Statistical correlation matrix between $|y^{t,had}|$ (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5] Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between $|y^{t,had}|$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5] Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $|y^{t,had}|$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.4, 0.4-0.8, 0.8-1.2, 1.2-1.6, 1.6-2.5] Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $p_{T}^{t,had}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t,had}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV Columns: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV
Statistical correlation matrix between $p_{T}^{t,had}$ (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between $p_{T}^{t,had}$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $p_{T}^{t,had}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-60, 60-100, 100-150, 150-200, 200-260, 260-320, 320-400, 400-500] GeV Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $|y^{t\bar{t}}|$ (rows) in the 4-jet inclusive configuration and $|y^{t\bar{t}}|$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5] Columns: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5]
Statistical correlation matrix between $|y^{t\bar{t}}|$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5] Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $|y^{t\bar{t}}|$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-0.3, 0.3-0.6, 0.6-0.9, 0.9-1.3, 1.3-2.5] Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $m^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $m^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV Columns: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV
Statistical correlation matrix between $m^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [345-400, 400-470, 470-550, 550-650, 650-800, 800-1100, 1100-1600] GeV Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
Statistical correlation matrix between $p_{T}^{t\bar{t}}$ (rows) in the 4-jet inclusive configuration and $p_{T}^{t\bar{t}}$ (columns) in the 4-jet inclusive configuration, obtained at parton level from relative spectra through the Bootstrap Method. The binning is the following: Rows: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV Columns: [0-20, 20-45, 45-75, 75-120, 120-190, 190-300] GeV
A search is conducted for new resonances decaying into a $W$ or $Z$ boson and a 125 GeV Higgs boson in the $\nu\bar{\nu}b\bar{b}$, $\ell^{\pm}{\nu}b\bar{b}$, and $\ell^+\ell^-b\bar{b}$ final states, where $\ell ^{\pm}= e^{\pm}$ or $\mu^{\pm}$, in $pp$ collisions at $\sqrt s = 13$ TeV. The data used correspond to a total integrated luminosity of 36.1 fb$^{-1}$ collected with the ATLAS detector at the Large Hadron Collider during the 2015 and 2016 data-taking periods. The search is conducted by examining the reconstructed invariant or transverse mass distributions of $Wh$ and $Zh$ candidates for evidence of a localised excess in the mass range of 220 GeV up to 5 TeV. No significant excess is observed and the results are interpreted in terms of constraints on the production cross-section times branching fraction of heavy $W^\prime$ and $Z^\prime$ resonances in heavy-vector-triplet models and the CP-odd scalar boson $A$ in two-Higgs-doublet models. Upper limits are placed at the 95 % confidence level and range between $9.0\times 10^{-4}$ pb and $8.1\times 10^{-1}$ pb depending on the model and mass of the resonance.
Upper limits on Zprime to Z h production cross section x branching fraction in pb
Upper limits on Zprime to Z h production cross section x branching fraction in pb
Upper limits on Wprime to W h production cross section x branching fraction in pb
Upper limits on Wprime to W h production cross section x branching fraction in pb
Upper limits for the scaling factor of the production cross section for V’ times its branching fraction to Wh/Zh in Model A.
Upper limits for the scaling factor of the production cross section for V’ times its branching fraction to Wh/Zh in Model A.
Upper limits on A to Z h production cross section x branching fraction in pb (gluon fusion production)
Upper limits on A to Z h production cross section x branching fraction in pb (gluon fusion production)
Upper limits on A to Z h production cross section x branching fraction in pb ( production with associated b-quarks)
Upper limits on A to Z h production cross section x branching fraction in pb ( production with associated b-quarks)
Acceptance * Reconstruction efficiency for pp-> Zprime
Acceptance * Reconstruction efficiency for pp-> Zprime
Acceptance * Reconstruction efficiency for pp-> Zprime
Acceptance * Reconstruction efficiency for pp-> Zprime
Acceptance * Reconstruction efficiency for pp-> Wprime
Acceptance * Reconstruction efficiency for pp-> Wprime
Acceptance * Reconstruction efficiency for pp-> A (gluon fusion)
Acceptance * Reconstruction efficiency for pp-> A (gluon fusion)
Acceptance * Reconstruction efficiency for pp-> A (gluon fusion)
Acceptance * Reconstruction efficiency for pp-> A (gluon fusion)
Acceptance * Reconstruction efficiency for pp-> A (b-quark associated)
Acceptance * Reconstruction efficiency for pp-> A (b-quark associated)
Acceptance * Reconstruction efficiency for pp-> A (b-quark associated)
Acceptance * Reconstruction efficiency for pp-> A (b-quark associated)
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 10%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 10%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 20%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 20%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 30%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 30%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 40%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 40%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 50%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 50%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 60%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 60%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 70%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 70%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 80%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 80%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 90%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 0% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 90%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 1% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 1% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 2% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 2% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 3% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 3% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 4% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 4% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 5% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 5% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 6% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 6% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 7% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 7% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 8% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 8% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 9% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 9% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 10% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 10% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 11% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Upper limits at the 95% CL on the product of the production cross-section for pp->A and the branching fractions for A->Zh and h->bb evaluated by combining the 0-lepton and 2-lepton channels. The signal is smeared by a Breit-Wigner function with A boson width of 11% , assuming a combination of the gluon--gluon fusion and b-quark associated production modes with a bbA fraction of 0%.
Event distributions of mT,Vh for the 0-lepton channel in the resolved 1-btag category. The background prediction is shown after a background-only maximum-likelihood fit to the data.
Event distributions of mT,Vh for the 0-lepton channel in the resolved 2-btag category. The background prediction is shown after a background-only maximum-likelihood fit to the data.
Event distributions of m,Vh for the 1-lepton channel in the resolved 1-btag category. The background prediction is shown after a background-only maximum-likelihood fit to the data.
Event distributions of m,Vh for the 1-lepton channel in the resolved 2-btag category. The background prediction is shown after a background-only maximum-likelihood fit to the data.
Event distributions of mT,Vh for the 2-lepton channel in the resolved 1-btag category. The background prediction is shown after a background-only maximum-likelihood fit to the data.
Event distributions of m,Vh for the 2-lepton channel in the resolved 2-btag category. The background prediction is shown after a background-only maximum-likelihood fit to the data.
Event distributions of mT,Vh for the 0-lepton channel in the boosted 1-btag category. The background prediction is shown after a background-only maximum-likelihood fit to the data.
Event distributions of mT,Vh for the 0-lepton channel in the boosted 2-btag category. The background prediction is shown after a background-only maximum-likelihood fit to the data.
Event distributions of m,Vh for the 1-lepton channel in the boosted 1-btag category. The background prediction is shown after a background-only maximum-likelihood fit to the data.
Event distributions of m,Vh for the 1-lepton channel in the boosted 2-btag category. The background prediction is shown after a background-only maximum-likelihood fit to the data.
Event distributions of m,Vh for the 2-lepton channel in the boosted 1-btag category. The background prediction is shown after a background-only maximum-likelihood fit to the data.
Event distributions of m,Vh for the 2-lepton channel in the boosted 2-btag category. The background prediction is shown after a background-only maximum-likelihood fit to the data.
A search for strongly produced supersymmetric particles using signatures involving multiple energetic jets and either two isolated same-sign leptons ($e$ or $\mu$), or at least three isolated leptons, is presented. The analysis relies on the identification of $b$-jets and high missing transverse momentum to achieve good sensitivity. A data sample of proton--proton collisions at $\sqrt{s}= 13$ TeV recorded with the ATLAS detector at the Large Hadron Collider in 2015 and 2016, corresponding to a total integrated luminosity of 36.1 fb$^{-1}$, is used for the search. No significant excess over the Standard Model prediction is observed. The results are interpreted in several simplified supersymmetric models featuring $R$-parity conservation or $R$-parity violation, extending the exclusion limits from previous searches. In models considering gluino pair production, gluino masses are excluded up to 1.87 TeV at 95% confidence level. When bottom squarks are pair-produced and decay to a chargino and a top quark, models with bottom squark masses below 700 GeV and light neutralinos are excluded at 95% confidence level. In addition, model-independent limits are set on a possible contribution of new phenomena to the signal region yields.
Observed 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino via an offshell top squark, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$.
Observed 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino via an offshell top squark, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$.
Expected 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino via an offshell top squark, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$.
Expected 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino via an offshell top squark, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$.
Observed 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade, $\tilde g\to q\bar{q}^{'}\tilde{\chi}_1^\pm$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_2^0$ and $\tilde{\chi}_2^0\to Z\tilde{\chi}_1^0$.
Observed 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade, $\tilde g\to q\bar{q}^{'}\tilde{\chi}_1^\pm$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_2^0$ and $\tilde{\chi}_2^0\to Z\tilde{\chi}_1^0$.
Expected 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade, $\tilde g\to q\bar{q}^{'}\tilde{\chi}_1^\pm$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_2^0$ and $\tilde{\chi}_2^0\to Z\tilde{\chi}_1^0$.
Expected 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade, $\tilde g\to q\bar{q}^{'}\tilde{\chi}_1^\pm$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_2^0$ and $\tilde{\chi}_2^0\to Z\tilde{\chi}_1^0$.
Observed 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade involving sleptons, $\tilde g\to q\bar{q}\tilde{\chi}_2^0$ followed by $\tilde{\chi}_2^0\to \tilde\ell\ell/\tilde\nu\nu$ and $\tilde\ell/\tilde\nu\to \ell/\nu\tilde{\chi}_1^0$.
Observed 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade involving sleptons, $\tilde g\to q\bar{q}\tilde{\chi}_2^0$ followed by $\tilde{\chi}_2^0\to \tilde\ell\ell/\tilde\nu\nu$ and $\tilde\ell/\tilde\nu\to \ell/\nu\tilde{\chi}_1^0$.
Expected 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade involving sleptons, $\tilde g\to q\bar{q}\tilde{\chi}_2^0$ followed by $\tilde{\chi}_2^0\to \tilde\ell\ell/\tilde\nu\nu$ and $\tilde\ell/\tilde\nu\to \ell/\nu\tilde{\chi}_1^0$.
Expected 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade involving sleptons, $\tilde g\to q\bar{q}\tilde{\chi}_2^0$ followed by $\tilde{\chi}_2^0\to \tilde\ell\ell/\tilde\nu\nu$ and $\tilde\ell/\tilde\nu\to \ell/\nu\tilde{\chi}_1^0$.
Observed 95% CL exclusion contours on the lightest bottom squark and lightest neutralino masses in a SUSY scenario where pairs of bottom-antibottom squarks are produced and decay into the lightest neutralino via a chargino, $\tilde b^{}_{1}\to t\tilde{\chi}_1^-$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_1^0$.
Observed 95% CL exclusion contours on the lightest bottom squark and lightest neutralino masses in a SUSY scenario where pairs of bottom-antibottom squarks are produced and decay into the lightest neutralino via a chargino, $\tilde b^{}_{1}\to t\tilde{\chi}_1^-$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_1^0$.
Expected 95% CL exclusion contours on the lightest bottom squark and lightest neutralino masses in a SUSY scenario where pairs of bottom-antibottom squarks are produced and decay into the lightest neutralino via a chargino, $\tilde b^{}_{1}\to t\tilde{\chi}_1^-$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_1^0$.
Expected 95% CL exclusion contours on the lightest bottom squark and lightest neutralino masses in a SUSY scenario where pairs of bottom-antibottom squarks are produced and decay into the lightest neutralino via a chargino, $\tilde b^{}_{1}\to t\tilde{\chi}_1^-$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_1^0$.
Observed 95% CL exclusion contours on the gluino and lightest top squark masses in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{313}$ or $\lambda^{''}_{323}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar b\bar d / \bar b \bar s$.
Observed 95% CL exclusion contours on the gluino and lightest top squark masses in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{313}$ or $\lambda^{''}_{323}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar b\bar d / \bar b \bar s$.
Expected 95% CL exclusion contours on the gluino and lightest top squark masses in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{313}$ or $\lambda^{''}_{323}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar b\bar d / \bar b \bar s$.
Expected 95% CL exclusion contours on the gluino and lightest top squark masses in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{313}$ or $\lambda^{''}_{323}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar b\bar d / \bar b \bar s$.
Observed 95% CL exclusion contours on the gluino and lightest top squark masses in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{321}$, $\lambda^{''}_{311}$ or $\lambda^{''}_{322}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar s\bar d /\bar d \bar d/\bar s \bar s$.
Observed 95% CL exclusion contours on the gluino and lightest top squark masses in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{321}$, $\lambda^{''}_{311}$ or $\lambda^{''}_{322}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar s\bar d /\bar d \bar d/\bar s \bar s$.
Expected 95% CL exclusion contours on the gluino and lightest top squark masses in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{321}$, $\lambda^{''}_{311}$ or $\lambda^{''}_{322}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar s\bar d /\bar d \bar d/\bar s \bar s$.
Expected 95% CL exclusion contours on the gluino and lightest top squark masses in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{321}$, $\lambda^{''}_{311}$ or $\lambda^{''}_{322}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar s\bar d /\bar d \bar d/\bar s \bar s$.
Observed 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino, which in turn decays via non-zero baryon- and lepton-number-violating RPV couplings $\lambda^{'}_{ijk}$, $\tilde g\to q\bar{q}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to q\bar{q}^{'}\ell$.
Observed 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino, which in turn decays via non-zero baryon- and lepton-number-violating RPV couplings $\lambda^{'}_{ijk}$, $\tilde g\to q\bar{q}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to q\bar{q}^{'}\ell$.
Expected 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino, which in turn decays via non-zero baryon- and lepton-number-violating RPV couplings $\lambda^{'}_{ijk}$, $\tilde g\to q\bar{q}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to q\bar{q}^{'}\ell$.
Expected 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino, which in turn decays via non-zero baryon- and lepton-number-violating RPV couplings $\lambda^{'}_{ijk}$, $\tilde g\to q\bar{q}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to q\bar{q}^{'}\ell$.
Observed 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay directly into a pair of top-antitop quarks and the lightest neutralino, which in turn decays into light quarks via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{ijk}$, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to qqq$.
Observed 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay directly into a pair of top-antitop quarks and the lightest neutralino, which in turn decays into light quarks via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{ijk}$, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to qqq$.
Expected 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay directly into a pair of top-antitop quarks and the lightest neutralino, which in turn decays into light quarks via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{ijk}$, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to qqq$.
Expected 95% CL exclusion contours on the gluino and lightest neutralino masses in a SUSY scenario where gluinos are produced in pairs and decay directly into a pair of top-antitop quarks and the lightest neutralino, which in turn decays into light quarks via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{ijk}$, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to qqq$.
Observed 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino via an offshell top squark, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino via an offshell top squark, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade, $\tilde g\to q\bar{q}^{'}\tilde{\chi}_1^\pm$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_2^0$ and $\tilde{\chi}_2^0\to Z\tilde{\chi}_1^0$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade, $\tilde g\to q\bar{q}^{'}\tilde{\chi}_1^\pm$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_2^0$ and $\tilde{\chi}_2^0\to Z\tilde{\chi}_1^0$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade involving sleptons, $\tilde g\to q\bar{q}\tilde{\chi}_2^0$ followed by $\tilde{\chi}_2^0\to \tilde\ell\ell/\tilde\nu\nu$ and $\tilde\ell/\tilde\nu\to \ell/\nu\tilde{\chi}_1^0$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade involving sleptons, $\tilde g\to q\bar{q}\tilde{\chi}_2^0$ followed by $\tilde{\chi}_2^0\to \tilde\ell\ell/\tilde\nu\nu$ and $\tilde\ell/\tilde\nu\to \ell/\nu\tilde{\chi}_1^0$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde{b}^{}_1\tilde{b}^{*}_1$ production cross-sections in a SUSY scenario where pairs of bottom-antibottom squarks are produced and decay into the lightest neutralino via a chargino, $\tilde b^{}_{1}\to t\tilde{\chi}_1^-$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_1^0$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde{b}^{}_1\tilde{b}^{*}_1$ production cross-sections in a SUSY scenario where pairs of bottom-antibottom squarks are produced and decay into the lightest neutralino via a chargino, $\tilde b^{}_{1}\to t\tilde{\chi}_1^-$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_1^0$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{313}$ or $\lambda^{''}_{323}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar b\bar d / \bar b \bar s$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{313}$ or $\lambda^{''}_{323}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar b\bar d / \bar b \bar s$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{321}$, $\lambda^{''}_{311}$ or $\lambda^{''}_{322}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar s\bar d /\bar d \bar d/\bar s \bar s$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{321}$, $\lambda^{''}_{311}$ or $\lambda^{''}_{322}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar s\bar d /\bar d \bar d/\bar s \bar s$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino, which in turn decays via non-zero baryon- and lepton-number-violating RPV couplings $\lambda^{'}_{ijk}$, $\tilde g\to q\bar{q}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to q\bar{q}^{'}\ell$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino, which in turn decays via non-zero baryon- and lepton-number-violating RPV couplings $\lambda^{'}_{ijk}$, $\tilde g\to q\bar{q}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to q\bar{q}^{'}\ell$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay directly into a pair of top-antitop quarks and the lightest neutralino, which in turn decays into light quarks via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{ijk}$, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to qqq$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay directly into a pair of top-antitop quarks and the lightest neutralino, which in turn decays into light quarks via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{ijk}$, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to qqq$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed and expected 95% CL upper limits on $pp\to \tilde{t}^{}_\mathrm{1}\tilde{t}^{*}_\mathrm{1}$ production cross-sections in a SUSY scenario where pairs of top-antitop squarks are produced and decay into the lightest neutralino via a two-steps cascade, $\tilde t^{}_{1}\to t\tilde{\chi}_2^0$ followed by $\tilde{\chi}_2^0\to \tilde{\chi}_1^\pm W^\mp$ and $\tilde{\chi}_1^\pm\to f\bar{f^{'}}\tilde{\chi}_1^0$. The lightest chargino and the lightest neutralino are assumed to be nearly mass-degenerate. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed and expected 95% CL upper limits on $pp\to \tilde{t}^{}_\mathrm{1}\tilde{t}^{*}_\mathrm{1}$ production cross-sections in a SUSY scenario where pairs of top-antitop squarks are produced and decay into the lightest neutralino via a two-steps cascade, $\tilde t^{}_{1}\to t\tilde{\chi}_2^0$ followed by $\tilde{\chi}_2^0\to \tilde{\chi}_1^\pm W^\mp$ and $\tilde{\chi}_1^\pm\to f\bar{f^{'}}\tilde{\chi}_1^0$. The lightest chargino and the lightest neutralino are assumed to be nearly mass-degenerate. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed and expected 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario with non-universal Higgs masses (NUHM2, see the publication Refs. [31-32]). The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed and expected 95% CL upper limits on $pp\to \tilde g\tilde g$ production cross-sections in a SUSY scenario with non-universal Higgs masses (NUHM2, see the publication Refs. [31-32]). The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed and expected 95% CL upper limits on $pp\to \tilde{d}^{}_\mathrm{R}\tilde{d}^{*}_\mathrm{R}$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{313}$ or $\lambda^{''}_{323}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar b\bar d / \bar b \bar s$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed and expected 95% CL upper limits on $pp\to \tilde{d}^{}_\mathrm{R}\tilde{d}^{*}_\mathrm{R}$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{313}$ or $\lambda^{''}_{323}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar b\bar d / \bar b \bar s$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed and expected 95% CL upper limits on $pp\to \tilde{d}^{}_\mathrm{R}\tilde{d}^{*}_\mathrm{R}$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{321}$, $\lambda^{''}_{311}$ or $\lambda^{''}_{322}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar s\bar d /\bar d \bar d/\bar s \bar s$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Observed and expected 95% CL upper limits on $pp\to \tilde{d}^{}_\mathrm{R}\tilde{d}^{*}_\mathrm{R}$ production cross-sections in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{321}$, $\lambda^{''}_{311}$ or $\lambda^{''}_{322}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar s\bar d /\bar d \bar d/\bar s \bar s$. The table also shows the signal acceptance and reconstruction efficiency for the signal region(s) with sensitivity to this scenario.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2L2bS, in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino via an offshell top squark, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1500 GeV and $m(\tilde \chi_1^0)$ = 800 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2L2bS, in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino via an offshell top squark, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1500 GeV and $m(\tilde \chi_1^0)$ = 800 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2L2bH, in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino via an offshell top squark, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1700 GeV and $m(\tilde \chi_1^0)$ = 200 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2L2bH, in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino via an offshell top squark, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1700 GeV and $m(\tilde \chi_1^0)$ = 200 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2Lsoft1b, in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino via offshell top squark and top quark, $\tilde g\to t\bar{b}W^{-}\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1200 GeV and $m(\tilde \chi_1^0)$ = 940 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2Lsoft1b, in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino via offshell top squark and top quark, $\tilde g\to t\bar{b}W^{-}\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1200 GeV and $m(\tilde \chi_1^0)$ = 940 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2Lsoft2b, in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino via offshell top squark and top quark, $\tilde g\to t\bar{b}W^{-}\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1200 GeV and $m(\tilde \chi_1^0)$ = 900 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2Lsoft2b, in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino via offshell top squark and top quark, $\tilde g\to t\bar{b}W^{-}\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1200 GeV and $m(\tilde \chi_1^0)$ = 900 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2L0bS, in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade, $\tilde g\to q\bar{q}^{'}\tilde{\chi}_1^\pm$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_2^0$ and $\tilde{\chi}_2^0\to Z\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1200 GeV, $m(\tilde \chi_1^\pm)$ = 1050 GeV, $m(\tilde \chi_2^0)$ = 975 GeV and $m(\tilde \chi_1^0)$ = 900 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2L0bS, in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade, $\tilde g\to q\bar{q}^{'}\tilde{\chi}_1^\pm$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_2^0$ and $\tilde{\chi}_2^0\to Z\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1200 GeV, $m(\tilde \chi_1^\pm)$ = 1050 GeV, $m(\tilde \chi_2^0)$ = 975 GeV and $m(\tilde \chi_1^0)$ = 900 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2L0bH, in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade, $\tilde g\to q\bar{q}^{'}\tilde{\chi}_1^\pm$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_2^0$ and $\tilde{\chi}_2^0\to Z\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1600 GeV, $m(\tilde \chi_1^\pm)$ = 850 GeV, $m(\tilde \chi_2^0)$ = 475 GeV and $m(\tilde \chi_1^0)$ = 100 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2L0bH, in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade, $\tilde g\to q\bar{q}^{'}\tilde{\chi}_1^\pm$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_2^0$ and $\tilde{\chi}_2^0\to Z\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1600 GeV, $m(\tilde \chi_1^\pm)$ = 850 GeV, $m(\tilde \chi_2^0)$ = 475 GeV and $m(\tilde \chi_1^0)$ = 100 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc3L0bS, in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade involving sleptons, $\tilde g\to q\bar{q}\tilde{\chi}_2^0$ followed by $\tilde{\chi}_2^0\to \tilde\ell\ell/\tilde\nu\nu$ and $\tilde\ell/\tilde\nu\to \ell/\nu\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1400 GeV, $m(\tilde \chi_2^0)$ = 1250 GeV, $m(\tilde\ell)=m(\tilde\nu)$ = 1175 GeV and $m(\tilde \chi_1^0)$ = 1100 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc3L0bS, in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade involving sleptons, $\tilde g\to q\bar{q}\tilde{\chi}_2^0$ followed by $\tilde{\chi}_2^0\to \tilde\ell\ell/\tilde\nu\nu$ and $\tilde\ell/\tilde\nu\to \ell/\nu\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1400 GeV, $m(\tilde \chi_2^0)$ = 1250 GeV, $m(\tilde\ell)=m(\tilde\nu)$ = 1175 GeV and $m(\tilde \chi_1^0)$ = 1100 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc3L0bH, in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade involving sleptons, $\tilde g\to q\bar{q}\tilde{\chi}_2^0$ followed by $\tilde{\chi}_2^0\to \tilde\ell\ell/\tilde\nu\nu$ and $\tilde\ell/\tilde\nu\to \ell/\nu\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1800 GeV, $m(\tilde \chi_2^0)$ = 950 GeV, $m(\tilde\ell)=m(\tilde\nu)$ = 475 GeV and $m(\tilde \chi_1^0)$ = 100 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc3L0bH, in a SUSY scenario where gluinos are produced in pairs and decay into the lightest neutralino via a two-steps cascade involving sleptons, $\tilde g\to q\bar{q}\tilde{\chi}_2^0$ followed by $\tilde{\chi}_2^0\to \tilde\ell\ell/\tilde\nu\nu$ and $\tilde\ell/\tilde\nu\to \ell/\nu\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1800 GeV, $m(\tilde \chi_2^0)$ = 950 GeV, $m(\tilde\ell)=m(\tilde\nu)$ = 475 GeV and $m(\tilde \chi_1^0)$ = 100 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2L1bS, in a SUSY scenario where pairs of bottom-antibottom squarks are produced and decay into the lightest neutralino via a chargino, $\tilde b^{}_{1}\to t\tilde{\chi}_1^-$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde{b}^{}_1)$ = 600 GeV, $m(\tilde \chi_1^\pm)$ = 350 GeV and $m(\tilde \chi_1^0)$ = 250 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2L1bS, in a SUSY scenario where pairs of bottom-antibottom squarks are produced and decay into the lightest neutralino via a chargino, $\tilde b^{}_{1}\to t\tilde{\chi}_1^-$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde{b}^{}_1)$ = 600 GeV, $m(\tilde \chi_1^\pm)$ = 350 GeV and $m(\tilde \chi_1^0)$ = 250 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2L1bH, in a SUSY scenario where pairs of bottom-antibottom squarks are produced and decay into the lightest neutralino via a chargino, $\tilde b^{}_{1}\to t\tilde{\chi}_1^-$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde{b}^{}_1)$ = 750 GeV, $m(\tilde \chi_1^\pm)$ = 200 GeV and $m(\tilde \chi_1^0)$ = 100 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc2L1bH, in a SUSY scenario where pairs of bottom-antibottom squarks are produced and decay into the lightest neutralino via a chargino, $\tilde b^{}_{1}\to t\tilde{\chi}_1^-$ followed by $\tilde{\chi}_1^\pm\to W^\pm\tilde{\chi}_1^0$. The masses of the superpartners involved in the process are set to $m(\tilde{b}^{}_1)$ = 750 GeV, $m(\tilde \chi_1^\pm)$ = 200 GeV and $m(\tilde \chi_1^0)$ = 100 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc3LSS1b, in a SUSY scenario where pairs of top-antitop squarks are produced and decay into the lightest neutralino via a two-steps cascade, $\tilde t^{}_{1}\to t\tilde{\chi}_2^0$ followed by $\tilde{\chi}_2^0\to \tilde{\chi}_1^\pm W^\mp$ and $\tilde{\chi}_1^\pm\to f\bar{f^{'}}\tilde{\chi}_1^0$. The lightest chargino and the lightest neutralino are assumed to be nearly mass-degenerate. The masses of the superpartners involved in the process are set to $m(\tilde{t}^{}_1)$ = 700 GeV, $m(\tilde \chi_2^0)$ = 525 GeV, $m(\tilde \chi_1^\pm)\approx m(\tilde \chi_1^0)$ = 425 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpc3LSS1b, in a SUSY scenario where pairs of top-antitop squarks are produced and decay into the lightest neutralino via a two-steps cascade, $\tilde t^{}_{1}\to t\tilde{\chi}_2^0$ followed by $\tilde{\chi}_2^0\to \tilde{\chi}_1^\pm W^\mp$ and $\tilde{\chi}_1^\pm\to f\bar{f^{'}}\tilde{\chi}_1^0$. The lightest chargino and the lightest neutralino are assumed to be nearly mass-degenerate. The masses of the superpartners involved in the process are set to $m(\tilde{t}^{}_1)$ = 700 GeV, $m(\tilde \chi_2^0)$ = 525 GeV, $m(\tilde \chi_1^\pm)\approx m(\tilde \chi_1^0)$ = 425 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpv2L1bH, in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{321}$, $\lambda^{''}_{311}$ or $\lambda^{''}_{322}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar s\bar d /\bar d \bar d/\bar s \bar s$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1400 GeV, $m(\tilde{t}^{}_{1})$ = 800 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpv2L1bH, in a SUSY scenario where gluinos are produced in pairs and decay into a top quark and an antitop squark, which in turn decays via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{321}$, $\lambda^{''}_{311}$ or $\lambda^{''}_{322}$, $\tilde g\to \bar{t}\tilde{t}_1$ followed by $\tilde{t}_1\to \bar s\bar d /\bar d \bar d/\bar s \bar s$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1400 GeV, $m(\tilde{t}^{}_{1})$ = 800 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpv2L0b, in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino, which in turn decays via non-zero baryon- and lepton-number-violating RPV couplings $\lambda^{'}_{ijk}$, $\tilde g\to q\bar{q}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to q\bar{q}^{'}\ell$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1400 GeV, $m(\tilde{\chi}_1^0)$ = 500 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpv2L0b, in a SUSY scenario where gluinos are produced in pairs and decay directly into the lightest neutralino, which in turn decays via non-zero baryon- and lepton-number-violating RPV couplings $\lambda^{'}_{ijk}$, $\tilde g\to q\bar{q}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to q\bar{q}^{'}\ell$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1400 GeV, $m(\tilde{\chi}_1^0)$ = 500 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpv2L2bH, in a SUSY scenario where gluinos are produced in pairs and decay directly into a pair of top-antitop quarks and the lightest neutralino, which in turn decays into light quarks via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{ijk}$, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to qqq$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1800 GeV, $m(\tilde{\chi}_1^0)$ = 200 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpv2L2bH, in a SUSY scenario where gluinos are produced in pairs and decay directly into a pair of top-antitop quarks and the lightest neutralino, which in turn decays into light quarks via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{ijk}$, $\tilde g\to t\bar{t}\tilde{\chi}_1^0$ followed by $\tilde{\chi}_1^0\to qqq$. The masses of the superpartners involved in the process are set to $m(\tilde g)$ = 1800 GeV, $m(\tilde{\chi}_1^0)$ = 200 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpv2L2bS, in a SUSY scenario where pairs of down-down squark-rights are produced and decay into a pair of top and bottom quarks via a non-zero baryon-number-violating RPV coupling $\lambda^{''}_{331}$, $\tilde{d}^{}_\mathrm{R}\to \bar t\bar b$. The masses of the superpartners involved in the process are set to $m(\tilde{d}^{}_\mathrm{R})$ = 600 GeV, $m(\tilde g)$ = 2000 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpv2L2bS, in a SUSY scenario where pairs of down-down squark-rights are produced and decay into a pair of top and bottom quarks via a non-zero baryon-number-violating RPV coupling $\lambda^{''}_{331}$, $\tilde{d}^{}_\mathrm{R}\to \bar t\bar b$. The masses of the superpartners involved in the process are set to $m(\tilde{d}^{}_\mathrm{R})$ = 600 GeV, $m(\tilde g)$ = 2000 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpv2L1bS, in a SUSY scenario where pairs of down-down squarks are produced and decay into a pair of top and a light quarks via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{321}$ or $\lambda^{''}_{322}$, $\tilde{d}^{}_\mathrm{R}\to \bar t\bar s/\bar t\bar d$. The masses of the superpartners involved in the process are set to $m(\tilde{d}^{}_\mathrm{R})$ = 600 GeV, $m(\tilde g)$ = 2000 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpv2L1bS, in a SUSY scenario where pairs of down-down squarks are produced and decay into a pair of top and a light quarks via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{321}$ or $\lambda^{''}_{322}$, $\tilde{d}^{}_\mathrm{R}\to \bar t\bar s/\bar t\bar d$. The masses of the superpartners involved in the process are set to $m(\tilde{d}^{}_\mathrm{R})$ = 600 GeV, $m(\tilde g)$ = 2000 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpv2L1bM, in a SUSY scenario where pairs of down-down squarks are produced and decay into a pair of top and a light quarks via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{321}$ or $\lambda^{''}_{322}$, $\tilde{d}^{}_\mathrm{R}\to \bar t\bar s/\bar t\bar d$. The masses of the superpartners involved in the process are set to $m(\tilde{d}^{}_\mathrm{R})$ = 1000 GeV, $m(\tilde g)$ = 2000 GeV. Only statistical uncertainties are shown.
Number of signal events expected for 36.1 fb$^{-1}$ at different stages of the event selection for the signal region Rpv2L1bM, in a SUSY scenario where pairs of down-down squarks are produced and decay into a pair of top and a light quarks via non-zero baryon-number-violating RPV couplings $\lambda^{''}_{321}$ or $\lambda^{''}_{322}$, $\tilde{d}^{}_\mathrm{R}\to \bar t\bar s/\bar t\bar d$. The masses of the superpartners involved in the process are set to $m(\tilde{d}^{}_\mathrm{R})$ = 1000 GeV, $m(\tilde g)$ = 2000 GeV. Only statistical uncertainties are shown.
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