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arXiv:1406.7844v2 [hep-ex] 23 May 2016

Comprehensive measurements of t-channel single top-quark production cross sections at 𝒔=𝟕\mathbf{\sqrt{\mathrm{{\bf{\emph{s}}}}}=7} TeV with the ATLAS detector

The ATLAS collaboration
August 11, 2026
Abstract

This article presents measurements of the tt-channel single top-quark (tt) and top-antiquark (t¯\bar{t}) total production cross sections σ(tq)\sigma(tq) and σ(t¯q)\sigma(\bar{t}q), their ratio Rt=σ(tq)/σ(t¯q)R_{t}=\sigma(tq)/\sigma(\bar{t}q), and a measurement of the inclusive production cross section σ(tq+t¯q)\sigma(tq+\bar{t}q) in proton–proton collisions at s=7\sqrt{s}=7 TeV at the LHC. Differential cross sections for the tqtq and t¯q\bar{t}q processes are measured as a function of the transverse momentum and the absolute value of the rapidity of tt and t¯\bar{t}, respectively. The analyzed data set was recorded with the ATLAS detector and corresponds to an integrated luminosity of 4.59 fb-1. Selected events contain one charged lepton, large missing transverse momentum, and two or three jets. The cross sections are measured by performing a binned maximum-likelihood fit to the output distributions of neural networks. The resulting measurements are σ(tq)=46±1(stat.)±6(syst.)pb\sigma(tq)=46\pm 1\,(\mathrm{stat.})\pm 6\,(\mathrm{syst.})\,\mathrm{pb}, σ(t¯q)=23±1(stat.)±3(syst.)pb\sigma(\bar{t}q)=23\pm 1\,(\mathrm{stat.})\pm 3\,(\mathrm{syst.})\,\mathrm{pb}, Rt=2.04±0.13(stat.)±0.12(syst.)R_{t}=2.04\pm 0.13\,(\mathrm{stat.})\,\pm 0.12\,(\mathrm{syst.}), and σ(tq+t¯q)=68±2(stat.)±8(syst.)pb\sigma(tq+\bar{t}q)=68\pm 2\,(\mathrm{stat.})\;\pm 8\,(\mathrm{syst.})\;\mathrm{pb}, consistent with the Standard Model expectation. The uncertainty on the measured cross sections is dominated by systematic uncertainties, while the uncertainty on RtR_{t} is mainly statistical. Using the ratio of σ(tq+t¯q)\sigma(tq+\bar{t}q) to its theoretical prediction, and assuming that the top-quark-related CKM matrix elements obey the relation |Vtb||Vts|,|Vtd||V_{tb}|\gg|V_{ts}|,|V_{td}|, we determine |Vtb|=1.02±0.07|V_{tb}|=1.02\pm 0.07.

pacs
14.65.Ha, 12.15.Hh, 13.85.Qk, 14.20.Dh

I Introduction

In proton–proton (pppp) collisions at the LHC, top quarks are produced at unprecedented rates, allowing studies that were intractable before. The production of single top quarks via weak charged-current interactions is among the top-quark phenomena becoming accessible to precise investigations. In leading-order (LO) perturbation theory, single top-quark production is described by three subprocesses that are distinguished by the virtuality of the exchanged WW boson. The dominant process is the tt-channel exchange depicted in Fig. 1, which is the focus of the measurements presented in this article. A light quark from one of the colliding protons interacts with a bb-quark from another proton by exchanging a virtual WW boson (WW^{*}). Since the uu-quark density of the proton is about twice as high as the dd-quark density, the production cross section of single top quarks σ(tq)\sigma(tq), shown in Fig. 11, is expected to be about twice the cross section of top-antiquark production σ(t¯q)\sigma(\bar{t}q), shown in Fig. 11.

Refer to caption
Refer to caption
Figure 1: Representative leading-order Feynman diagrams of 1 single top-quark production and 1 single top-antiquark production via the tt-channel exchange of a virtual WW^{*} boson, including the decay of the top-quark and top-antiquark, respectively.

At LO, subleading single top-quark processes are the associated production of a WW boson and a top quark (WtWt) and the ss-channel production of tb¯t\bar{b}, analogous to the Drell–Yan process.

In general, measurements of single top-quark production provide insights into the properties of the WtbWtb vertex. The cross sections are proportional to the square of the coupling at the production vertex. In the Standard Model (SM), the coupling is given by the Cabibbo–Kobayashi–Maskawa (CKM) matrix element VtbV_{tb} Cabibbo 1963; Kobayashi and Maskawa 1973 multiplied by the universal electroweak coupling constant. Angular distributions of top-quark decay products give access to the Lorentz structure of the WtbWtb vertex, which has a vector–axial vector structure in the SM. As illustrated in Fig. 1, the tt-channel process features a bb-quark in the initial state if described in LO Quantum Chromodynamics (QCD), and therefore the cross section depends strongly on the bb-quark parton distribution function (PDF), which is derived from the gluon PDF by means of the DGLAP evolution Altarelli and Parisi 1977; Dokshitzer 1977; Gribov and Lipatov 1972. A measurement of the combined top-quark and top-antiquark cross section σ(tq+t¯q)=σ(tq)+σ(t¯q)\sigma(tq+\bar{t}q)=\sigma(tq)+\sigma(\bar{t}q) is well suited to constrain VtbV_{tb} or the bb-quark PDF. In addition, the measurement of σ(tq+t¯q)\sigma(tq+\bar{t}q) is sensitive to various models of new physics phenomena Tait and Yuan 2000, such as extra heavy quarks, gauge bosons, or scalar bosons.

Separate measurements of σ(tq)\sigma(tq) and σ(t¯q)\sigma(\bar{t}q) extend the sensitivity to the PDFs of the uu-quark and the dd-quark, exploiting the different initial states of the two processes, shown in Fig. 1. At a center-of-mass energy of s=7TeV\sqrt{s}=7{\mathrm{\ Te\kern-1.00006ptV}}, the typical momentum fraction xx of the initial-state light quarks is in the range of 0.02x0.50.02\lesssim x\lesssim 0.5, with a median of 0.17 for uu-quarks and a median of 0.13 for dd-quarks. The additional measurement of the cross-section ratio Rtσ(tq)/σ(t¯q)R_{t}\equiv\sigma(tq)/\sigma(\bar{t}q) is sensitive to the ratio of the two PDFs in the xx-range specified above and features smaller systematic uncertainties because of partial cancelations of common uncertainties. The measurements of σ(tq)\sigma(tq), σ(t¯q)\sigma(\bar{t}q), and RtR_{t} provide complementary inputs in constraining PDFs to data currently used in QCD fits. Investigating RtR_{t} also provides a way of searching for new-physics contributions in single top-quark (top-antiquark) production Aguilar-Saavedra 2008 and of elucidating the nature of physics beyond the SM if it were to be observed Gao et al. 2011.

In this article we present measurements of σ(tq+t¯q)\sigma(tq+\bar{t}q), σ(tq)\sigma(tq), σ(t¯q)\sigma(\bar{t}q), and the cross-section ratio RtR_{t} at a center-of-mass energy of s=7TeV\sqrt{s}=7{\mathrm{\ Te\kern-1.00006ptV}}, using the full data set corresponding to an integrated luminosity of 4.59 fb-1. Final calibrations for the 7TeV7{\mathrm{\ Te\kern-1.00006ptV}} data set are used, resulting in reduced systematic uncertainties. The measurement of σ(tq+t¯q)\sigma(tq+\bar{t}q) is used to determine the value of the CKM matrix element |Vtb||V_{tb}|. Additionally, for the first time, differential cross sections are measured as a function of the transverse momentum of the top quark, pT(t)p_{\mathrm{T}}(t), and the top antiquark, pT(t¯)p_{\mathrm{T}}(\bar{t}), and as a function of the absolute value of the rapidities |y(t)||y(t)| and |y(t¯)||y(\bar{t})|, respectively.

In pppp collisions at s=7TeV\sqrt{s}=7\,{\mathrm{\ Te\kern-1.00006ptV}}, the total inclusive cross sections of top-quark and top-antiquark production in the tt-channel are predicted to be

σ(tq)\displaystyle\sigma(tq) =\displaystyle= 41.90.9+1.8pb,\displaystyle 41.9^{+1.8}_{-0.9}\ \mathrm{pb},
σ(t¯q)\displaystyle\sigma(\bar{t}q) =\displaystyle= 22.71.0+0.9pb,and\displaystyle 22.7^{+0.9}_{-1.0}\ \mathrm{pb},\ \ \mathrm{and}
σ(tq+t¯q)\displaystyle\sigma(tq+\bar{t}q) =\displaystyle= 64.62.0+2.7pb,\displaystyle 64.6^{+2.7}_{-2.0}\ \mathrm{pb},

with approximate next-to-next-to-leading-order (NNLO) precision Kidonakis 2011, assuming a top-quark mass of mt=172.5GeVm_{t}=172.5\,{\mathrm{\ Ge\kern-1.00006ptV}} and using the MSTW2008 NNLO Martin et al. 2009a PDF set. The quoted uncertainty contains the scale uncertainty and the correlated PDF–αs\alpha_{\mathrm{s}} uncertainty. The contributions due to the resummation of soft-gluon bremsstrahlung included in the approximate NNLO result are relatively small and the cross-section predictions are therefore very close to the plain next-to-leading-order (NLO) calculation Campbell et al. 2009. All predictions used in this article are based on the “five-flavor scheme”, involving a bb-quark in the initial state (see Fig. 1). An alternative approach is to consider the Born process qgtqbqg\rightarrow tqb, where the bb-quark does not enter in the QCD evolution of the PDFs and the strong coupling constant, referred to as “four-flavor scheme”. Recently, computations of differential cross sections have become available at approximate NNLO precision Kidonakis 2013, complementing the predictions at NLO Campbell et al. 2009. Measurements of these differential quantities will allow more stringent tests of the calculations. In addition, a thorough study of differential cross sections can give hints about the potential presence of flavor-changing neutral currents or four-fermion operators in the single top-quark production process Coimbra et al. 2012.

Single top-quark production in the tt-channel was first established in pp¯p\bar{p} collisions at s=1.96TeV\sqrt{s}=1.96{\mathrm{\ Te\kern-1.00006ptV}} at the Tevatron Abazov et al. 2010. Measurements of tt-channel single top-quark and WtWt production at the LHC at s=7TeV\sqrt{s}=7\,{\mathrm{\ Te\kern-1.00006ptV}} were performed by the ATLAS collaboration ATLAS Collaboration 2012a; ATLAS Collaboration 2012b and the CMS collaboration CMS Collaboration 2012; CMS Collaboration 2013. The ATLAS measurements used only a fraction of the recorded data, corresponding to 1.04 fb-1 in the tt-channel analysis. At s=8TeV\sqrt{s}=8\,{\mathrm{\ Te\kern-1.00006ptV}} the CMS collaboration measured the tt-channel cross sections and the cross-section ratio RtR_{t} CMS Collaboration 2014.

The measurements presented in this article are based on events in the lepton+jets channel, in which the lepton can be either an electron or a muon originating from a WW-boson decay. The analysis has acceptance for signal events involving WτνW\rightarrow\tau\nu decays if the τ\tau lepton decays subsequently to either eνeντe\nu_{e}\nu_{\tau} or μνμντ\mu\nu_{\mu}\nu_{\tau}. The experimental signature of candidate events is thus given by one charged lepton (electron or muon), large values of the magnitude of the missing transverse momentum ETmissE_{\mathrm{T}}^{\mathrm{miss}}, and two or three hadronic jets with high transverse momentum. The acceptance for tt-channel events is dominated by the 2-jet signature, where one jet is a bb-quark jet, while the second jet is a light-quark jet. A significant fraction of single top-quark events are also present in the 3-jet channel, whereas the tt¯t\bar{t} background is dominant in the 4-jet channel. For this reason, the analysis is restricted to events with two or three jets.

Several other processes feature the same signature as single top-quark events, the main backgrounds being W+W+jets production and top-quark-antiquark (tt¯t\bar{t}) pair production. Since a typical signature-based event selection yields only a relatively low signal purity, a dedicated analysis strategy is developed to separate signal and background events. In both the 22-jet and 33-jet channels, several observables discriminating between signal and background events are combined by a neural network (NN) to one discriminant (NN output). The cross-section measurements are based on a simultaneous fit to these multivariate discriminants. In the 2-jet channel, a cut on the NN discriminant is applied to obtain a sample of events enriched in tt-channel single top-quark events, facilitating the measurement of differential cross sections.

II Data samples and samples of simulated events

The analysis described in this article uses pppp collision data collected at a center-of-mass energy of 7TeV7{\mathrm{\ Te\kern-1.00006ptV}} with the ATLAS detector ATLAS Collaboration 2008a at the LHC between March and November 2011. In this data-taking period, the average number of pppp collisions per bunch crossing was nine. The selected events were recorded based on single-electron or single-muon triggers. Stringent detector and data quality requirements are applied, resulting in a data set corresponding to an integrated luminosity of 4.59±0.084.59\pm 0.08 fb-1 ATLAS Collaboration 2013a.

II.1 The ATLAS detector

The ATLAS detector ATLAS Collaboration 2008a is built from a set of cylindrical subdetectors, which cover almost the full solid angle around the interaction point 11 1 ATLAS uses a right-handed coordinate system with its origin at the nominal interaction point in the center of the detector and the zz-axis along the beam direction. The zz-axis is parallel to the anti-clockwise beam viewed from above. The pseudorapidity η\eta is defined as η=ln[tan(θ/2)]\eta=-\ln[\tan(\theta/2)], where the polar angle θ\theta is measured with respect to the zz-axis. The azimuthal angle ϕ\phi is measured with respect to the xx-axis, which points toward the center of the LHC ring. Transverse momentum and energy are defined as pT=psinθp_{\mathrm{T}}=p\sin\theta and ET=EsinθE_{\mathrm{T}}=E\sin\theta, respectively. The ΔR\Delta R distance in (η\eta,ϕ\phi) space is defined as ΔR=(Δη)2+(Δϕ)2\Delta R=\sqrt{(\Delta\eta)^{2}+(\Delta\phi)^{2}}.. ATLAS is composed of an inner tracking detector (ID) close to the interaction point, surrounded by a superconducting solenoid providing a 22\,T axial magnetic field, electromagnetic and hadronic calorimeters, and a muon spectrometer (MS). The ID consists of a silicon pixel detector, a silicon microstrip detector (SCT), and a straw-tube transition radiation tracker (TRT). The electromagnetic calorimeter is a lead and liquid-argon (LAr) sampling calorimeter with high granularity. An iron/scintillator tile calorimeter provides hadronic energy measurements in the central pseudorapidity range. The endcap and forward regions are instrumented with LAr calorimeters for both the electromagnetic and hadronic energy measurements. The MS consists of three large superconducting toroids with eight coils each, a system of trigger chambers, and precision tracking chambers.

II.2 Trigger requirements

ATLAS employs a three-level trigger system. The first level (L1) is built from custom-made hardware, while the second and third levels are software based and collectively referred to as the High Level Trigger (HLT). The data sets used in this analysis are defined by high-pTp_{\mathrm{T}} single electron or single muon triggers ATLAS Collaboration 2012c. During the data-taking period slightly different trigger conditions were used to cope with the increasing number of multiple pppp collisions per bunch crossing (pile-up).

At L1, electron candidate events are required to have an electromagnetic energy deposit of ET>14GeVE_{\rm T}>14{\mathrm{\ Ge\kern-1.00006ptV}}; in the second part of the data-taking period the requirement was ET>16GeVE_{\rm T}>16{\mathrm{\ Ge\kern-1.00006ptV}}. At the HLT level, the full granularity of the calorimeter and tracking information is available. The calorimeter cluster is matched to a track and the trigger electron object has to have ET>20GeVE_{\rm T}>20{\mathrm{\ Ge\kern-1.00006ptV}} or ET>22GeVE_{\rm T}>22{\mathrm{\ Ge\kern-1.00006ptV}}, exceeding the corresponding L1 requirements by 6GeV6{\mathrm{\ Ge\kern-1.00006ptV}}.

The single muon trigger is based on muon candidates reconstructed in the muon spectrometer. At L1, a threshold of pT=10GeVp_{\mathrm{T}}=10{\mathrm{\ Ge\kern-1.00006ptV}} is applied. At the HLT level, the requirement is tightened to pT>18GeVp_{\mathrm{T}}>18\,\rm{GeV}.

II.3 Simulated events

Samples of simulated tt-channel single top-quark events are produced with the NLO matrix-element generator POWHEG-BOX Nason 2004 interfaced to PYTHIA Sjostrand et al. 2006 (version 6.4.27) for showering and hadronization. In POWHEG-BOX the four-flavor scheme calculation is used to simulate tt-channel single top-quark production. The events are generated using the fixed four-flavor NLO PDF set CT104f Lai et al. 2010 and the renormalization and factorization scales are calculated event-by-event Frederix et al. 2012 with μR=μF=4mb2+pT,b2\mu_{R}=\mu_{F}=4\cdot\sqrt{m_{b}^{2}+p_{{\rm T},b}^{2}}, where mbm_{b} and pT,bp_{{\rm T},b} are the mass and pTp_{\mathrm{T}} of the bb-quark from the initial gluon splitting.

Samples of tt¯t\bar{t} events, WtWt events, and ss-channel single top-quark events are generated with POWHEG-BOX interfaced to PYTHIA using the CT10 NLO PDF set Lai et al. 2010. All processes involving top quarks are produced assuming mt=172.5GeVm_{t}=172.5{\mathrm{\ Ge\kern-1.00006ptV}}, and the parameters of the PYTHIA generator controlling the modeling of the parton shower and the underlying event are set to the values of the Perugia 2011 tune Skands 2010.

Vector-boson production in association with jets (W/ZW/Z+jets) is simulated using the multileg LO generator ALPGEN Mangano et al. 2003 (version 2.13) using the CTEQ6L1 PDF set Pumplin et al. 2002. The partonic events are showered with HERWIG Corcella et al. 2001 (version 6.5.20), and the underlying event is simulated with the JIMMY Butterworth et al. 1996 model (version 4.31) using values of the ATLAS Underlying Event Tune 2 ATLAS Collaboration 2011a. W+W+jets and Z+Z+jets events with up to five additional partons are generated. The MLM matching scheme Alwall et al. 2008 is used to remove overlap between partonic configurations generated by the matrix element and by parton shower evolution. The double counting between the inclusive W+nW+n-parton samples and samples with associated heavy-quark pair-production is removed utilizing an overlap removal based on a ΔR\Delta R matching. The diboson processes WWWW, WZWZ and ZZZZ are generated using HERWIG and JIMMY.

After the event generation step, all samples are passed through the full simulation of the ATLAS detector ATLAS Collaboration 2010 based on GEANT4 Agostinelli et al. 2003 and are then reconstructed using the same procedure as for collision data. The simulation includes the effect of multiple pppp collisions per bunch crossing. The events are weighted such that the distribution of the number of collisions per bunch crossing is the same as in collision data.

III Physics object definitions

In this section the definition of the physics objects is given, namely reconstructed electrons, muons, and jets, as well as ETmissE_{\mathrm{T}}^{\mathrm{miss}}. The definition of these objects involves the reconstructed position of the hard interaction. Primary interaction vertices are computed from reconstructed tracks that are compatible with coming from the luminous interaction region. The hard-scatter primary vertex is chosen as the vertex featuring the highest pT2\sum p_{\mathrm{T}}^{2}, the sum running over all tracks with pT>0.4GeVp_{\mathrm{T}}>0.4{\mathrm{\ Ge\kern-1.00006ptV}} associated with the vertex.

III.1 Electrons

Electron candidates are selected from energy deposits (clusters) in the LAr electromagnetic calorimeter matched to tracks ATLAS Collaboration 2014a and are required to have ET>25GeVE_{\mathrm{T}}>25{\mathrm{\ Ge\kern-1.00006ptV}} and |ηcl|<2.47|\eta_{\mathrm{cl}}|<2.47, where ηcl\eta_{\mathrm{cl}} denotes the pseudorapidity of the cluster. Clusters falling in the calorimeter barrel/endcap transition region, corresponding to 1.37<|ηcl|<1.521.37<|\eta_{\mathrm{cl}}|<1.52, are ignored. The energy of an electron candidate is taken from the cluster, while its η\eta and ϕ\phi are taken from the track. The zz-position of the track has to be compatible with the hard-scatter primary vertex. Electron candidates are further required to fulfil stringent criteria regarding calorimeter shower shape, track quality, track–cluster matching, and fraction of high-threshold hits in the TRT to ensure high identification quality.

Hadronic jets mimicking the signature of an electron, electrons from bb-hadron or cc-hadron decays, and photon conversions constitute the major backgrounds for high-pTp_{\mathrm{T}} electrons originating from the decay of a WW boson. Since signal electrons from WW-boson decay are typically isolated from jet activity, these backgrounds can be suppressed via isolation criteria that require minimal calorimeter activity (calorimeter isolation) and only few tracks (track isolation) in an (η\eta,ϕ\phi) region around the electron. Electron candidates are isolated by imposing thresholds on the scalar sum of the transverse momenta of calorimeter energy deposits ΣpTcalo\Sigma p_{\rm T}^{\rm calo} within a surrounding cone of radius ΔR=0.2\Delta R=0.2, excluding the energy deposit associated with the candidate, and on the scalar sum of the transverse momenta of tracks ΣpTtrack\Sigma p_{\rm T}^{\rm track} in a cone of radius ΔR=0.3\Delta R=0.3 around the candidate excluding the track associated with the electron candidate. The ΣpTcalo\Sigma p_{\rm T}^{\rm calo} variable is corrected for pile-up effects as a function of the number of reconstructed vertices. The thresholds applied to ΣpTcalo\Sigma p_{\rm T}^{\rm calo} and ΣpTtrack\Sigma p_{\rm T}^{\rm track} vary as a function of the electron pTp_{\rm T}, the electron η\eta, and the number of reconstructed primary vertices and are chosen such that the efficiency for electrons from WW-boson or ZZ-boson decays to pass this isolation requirement is 90%.

III.2 Muons

Muon candidates are reconstructed by combining track segments found in the ID and in the MS ATLAS Collaboration 2014b. The momentum as measured using the ID is required to agree with the momentum measured using the MS after correcting for the predicted muon energy loss in the calorimeter. Only candidates that have pT>25GeVp_{\mathrm{T}}>25\;{\mathrm{\ Ge\kern-1.00006ptV}} and |η|<2.5|\eta|<2.5 are considered. Selected muons must additionally satisfy a series of requirements on the number of track hits present in the various tracking subdetectors. Muon tracks are required to have at least two hits in the pixel detector, and six or more hits in the SCT. Tracks are rejected if they have more than two missing hits in the SCT and pixel detectors, or tracks with an excessive number of outlier hits in the TRT. Isolated muon candidates are selected by requiring ΣpTcalo<4GeV\Sigma p_{\rm T}^{\rm calo}<4\,{\mathrm{\ Ge\kern-1.00006ptV}} within a surrounding cone of radius ΔR=0.2\Delta R=0.2, and ΣpTtrack<2.5GeV\Sigma p_{\rm T}^{\rm track}<2.5\,{\mathrm{\ Ge\kern-1.00006ptV}} within a surrounding cone of radius ΔR=0.3\Delta R=0.3. The efficiency of this combined isolation requirement varies between 95% and 97%, depending on the data-taking period.

The reconstruction, identification and trigger efficiencies of electrons and muons are measured using tag-and-probe methods on samples enriched with ZZ~\to\ell\ell, J/ψJ/\psi~\to\ell\ell, or W±νW^{\pm}~\to\ell\nu (=e,μ\ell=e,\mu) events ATLAS Collaboration 2014a; ATLAS Collaboration 2014b.

III.3 Jets and missing transverse momentum

Jets are reconstructed using the anti-ktk_{t} algorithm Cacciari et al. 2008 with a radius parameter of 0.4, using topological clusters ATLAS Collaboration 2008b identified in the calorimeter as inputs to the jet clustering. The jet energy is corrected for the effect of multiple pppp interactions, both in collision data and in simulated events. Further energy corrections apply factors depending on the jet energy and the jet η\eta to achieve a calibration that matches the energy of stable particle jets in simulated events ATLAS Collaboration 2013b. Differences between data and Monte Carlo simulation are evaluated using in situ techniques and are corrected for in an additional step ATLAS Collaboration 2014c. The in situ calibration exploits the pTp_{\mathrm{T}} balance in ZZ+jet, γ\gamma+jet, and dijet events. ZZ+jet and γ\gamma+jet data are used to set the jet energy scale (JES) in the central detector region, while pTp_{\mathrm{T}} balancing in dijet events is used to achieve an η\eta intercalibration of jets in the forward region with respect to central jets.

Jets with separation ΔR<0.2\Delta R<0.2 from selected electron candidates are removed, as in these cases the jet and the electron are very likely to correspond to the same physics object. In order to reject jets from pile-up events, a quantity called the jet-vertex fraction ϵjvf\epsilon_{\mathrm{jvf}} is defined as the ratio of pT\sum p_{\mathrm{T}} for all tracks within the jet that originate from the hard-scatter primary vertex to the pT\sum p_{\mathrm{T}} of all tracks matched to the jet. It is required that ϵjvf>0.75\epsilon_{\mathrm{jvf}}>0.75 for those jets that have associated tracks. The ϵjvf\epsilon_{\mathrm{jvf}} criterion is omitted for jets without matched tracks. An overlap removal between jets and muons is applied, removing any muon with separation ΔR<0.4\Delta R<0.4 from a jet with pT>25GeVp_{\rm{T}}>25\,\rm{GeV} and ϵjvf>0.75\epsilon_{\mathrm{jvf}}>0.75. In the same way an overlap removal is applied between jets and electrons, removing any electron separated from a jet by 0.2<ΔR<0.40.2<\Delta R<0.4.

Only jets having pT>30p_{\mathrm{T}}>30 GeV{\mathrm{\ Ge\kern-1.00006ptV}} and |η|<4.5|\eta|<4.5 are considered. Jets in the endcap/forward-calorimeter transition region, corresponding to 2.75<|η|<3.52.75<|\eta|<3.5, must have pT>35p_{\mathrm{T}}>35 GeV{\mathrm{\ Ge\kern-1.00006ptV}}.

The ETmissE_{\mathrm{T}}^{\mathrm{miss}} is a measure of the momentum of the escaping neutrinos, but is also affected by energy losses due to detector inefficiencies. The ETmissE_{\mathrm{T}}^{\mathrm{miss}} is calculated based on the vector sum of energy deposits in the calorimeter projected onto the transverse plane and is corrected for the presence of electrons, muons, and jets ATLAS Collaboration 2012d.

III.4 Identification of b-quark jets

The identification of jets originating from the fragmentation of bb-quarks is one of the most important techniques for selecting top-quark events. Several properties can be used to distinguish bb-quark jets from other jets: the long lifetime of bb-hadrons, the large bb-hadron mass, and the large branching ratio to leptons. The relatively long lifetime of bb-flavored hadrons results in a significant flight path length, leading to reconstructable secondary vertices and tracks with large impact parameters relative to the primary vertex.

Jets containing bb-hadrons are identified in the region |η|<2.5|\eta|<2.5 by reconstructing secondary and tertiary vertices from the tracks associated with each jet and combining lifetime-related information in a neural network ATLAS Collaboration 2011b. Three different neural networks are trained corresponding to an optimal separation of bb-quark jets, cc-quark jets, and light-quark jets. The output of the networks is given in terms of probabilities pbp_{b}, pcp_{c}, and plp_{\mathrm{l}}, which are then combined to form a final discriminant. In order to achieve excellent rejection of cc-quark jets the ratio pb/pcp_{b}/p_{c} is calculated. The chosen working point corresponds to a bb-tagging efficiency of about 54% for bb-quark jets in tt¯t\bar{t} events. The misidentification efficiency is 4.8% for cc-quark jets and 0.48% for light-quark jets, as derived from simulated tt¯t\bar{t} events. Jets passing the requirement on the identification discriminant are called bb-tagged jets. Scale factors, determined from collision data, are applied to correct the bb-tagging efficiency in simulated events to match the data.

IV Event selection

The event selection requires exactly one charged lepton, ee or μ\mu, exactly two or three jets, and ETmiss>30GeVE_{\mathrm{T}}^{\mathrm{miss}}>30{\mathrm{\ Ge\kern-1.00006ptV}}. At least one of the jets must be bb-tagged. A trigger matching requirement is applied according to which the lepton must lie within ΔR=0.15\Delta R=0.15 cone around its trigger-level object. Candidate events are selected if they contain at least one good primary vertex candidate with at least five associated tracks. Events containing jets with transverse momentum pT>20GeVp_{\mathrm{T}}>20{\mathrm{\ Ge\kern-1.00006ptV}} failing to satisfy quality criteria against misreconstruction ATLAS Collaboration 2013b are rejected.

Since the multijet background is difficult to model precisely, its contribution is reduced by requiring the transverse mass of the lepton-ETmissE_{\mathrm{T}}^{\mathrm{miss}} system,

mT(ETmiss)=2pT()ETmiss[1cos(Δϕ(,ETmiss))],m_{\mathrm{T}}\left(\ell E_{\mathrm{T}}^{\mathrm{miss}}\right)=\sqrt{2p_{\mathrm{T}}(\ell)\cdot E_{\mathrm{T}}^{\mathrm{miss}}\left[1-\cos\left(\Delta\phi\left(\ell,E_{\mathrm{T}}^{\mathrm{miss}}\right)\right)\right]}\ , (1)

to be larger than 30GeV30{\mathrm{\ Ge\kern-1.00006ptV}}. Further reduction of the multijet background is achieved by placing an additional requirement on events with a charged lepton that is back-to-back with the leading jet in pTp_{\mathrm{T}}. This is realized by the following condition between the lepton pTp_{\mathrm{T}} and the Δϕ(j1,)\Delta\phi\left(j_{1},\ell\right):

pT()>40GeV(1π|Δϕ(j1,)|π1)p_{\mathrm{T}}\left(\ell\right)>40{\mathrm{\ Ge\kern-1.00006ptV}}\cdot\left(1-\frac{\pi-|\Delta\phi\left(j_{1},\ell\right)|}{\pi-1}\right) (2)

where j1j_{1} denotes the leading jet.

In the subsequent analysis, signal events are divided into different analysis channels according to the sign of the lepton charge and the number of jets. In the 2-jet channels, exactly one jet is required to be bb-tagged. To further reduce the WW+jets background in these channels, the absolute value of the difference in pseudorapidity |Δη||\Delta\eta| of the lepton and the bb-tagged jet is required to be smaller than 2.4. In the 3-jet channels, events with exactly one and exactly two bb-tagged jets are considered and separated accordingly. In the 3-jet-2-tag category no distinction is made between events with positive and negative lepton charge, since this channel is dominated by tt¯t\bar{t} background and can be used to further constrain the uncertainty on the bb-tagging efficiency. Finally, the resulting channels are referred to as: 2-jet-+\ell^{+}, 2-jet-\ell^{-}, 3-jet-+\ell^{+}-1-tag, 3-jet-\ell^{-}-1-tag, and 3-jet-2-tag.

A control region is defined to be orthogonal to the signal region in the same kinematic phase space to validate the modeling of the backgrounds by simulated events. Events in these control regions feature exactly one bb-tagged jet, which was identified with a less stringent bb-tagging algorithm than used to define the signal region. The signal region is excluded from the control region by applying a veto.

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Figure 2: ETmissE_{\mathrm{T}}^{\mathrm{miss}} distributions in the signal region (SR) for the (a) 2-jet-e+e^{+} and (b) 2-jet-ee^{-} channels for central electrons. The distributions are normalized to the result of a binned maximum-likelihood fit described in Sec. V.2. The relative difference between the observed and expected number of events in each bin is shown in the lower panels.

V Background estimation

One of the largest backgrounds to single top-quark processes in the lepton+jets channel is W+W+jets production. If one of the jets contains bb-hadrons or cc-hadrons, these events have the same signature as signal events. Due to possible misidentification of a light-quark jet as a bb-quark jet, W+W+light-jets production also contributes to the background. An equally important background comes from top-quark-antiquark (tt¯t\bar{t}) pair production events, which are difficult to separate from single top-quark events, since they contain top quarks as well. Another background is due to multijet production via the strong interaction. In these events a hadronic jet is misidentified as a lepton, usually an electron, or a real high-pTp_{\mathrm{T}} lepton is produced within a jet due to the semileptonic decay of a heavy-flavor (bb or cc) hadron and satisfies the lepton isolation criteria. Other smaller backgrounds come from diboson (WWWW, WZWZ, and ZZZZ) and Z+Z+jets production.

V.1 W/Z+jets background

The WW+jets background is initially normalized to the theoretical prediction and then subsequently determined simultaneously both in the context of the multijet background estimation and as part of the extraction of the signal cross section. The estimated number of events of the much smaller ZZ+jets background is calculated using the theoretical prediction.

The cross sections for inclusive WW-boson production and ZZ-boson production are predicted with NNLO precision using the FEWZ program Anastasiou et al. 2004, resulting in a LO-to-NNLO scale factor of 1.2 and an uncertainty of 4%. The uncertainty includes the uncertainty on the PDF and scale variations. The scale factor is applied to the prediction based on the LO ALPGEN calculation for the WW+bb¯b\bar{b}, WW+cc¯c\bar{c}, and WW+light-jets samples. An uncertainty for associated jet production is estimated using variations of the factorization and renormalization scale and the ALPGEN matching parameter. These variations yield an uncertainty of 5% for the production of two additional light-quark jets and 15% for two additional heavy-quark jets. An additional relative uncertainty of 50% is assigned to the WW+bb¯b\bar{b} and WW+cc¯c\bar{c} production rates to take uncertainties on heavy-flavor production into account. This uncertainty is estimated using a tag-counting method in control regions ATLAS Collaboration 2012a.

The ALPGEN prediction for the WW+cc process is scaled by a factor of 1.521.52 that is obtained from a study based on NLO calculations using MCFM Campbell and Ellis 2010. Normalization uncertainties on the factorization and renormalization scale and PDF uncertainties are 24%.

The processes WW+bb¯b\bar{b}, WW+cc¯c\bar{c}, and WW+light-jets, being asymmetric in lepton charge, are combined and are used as a single process in the binned maximum-likelihood fit to determine the signal yield.

V.2 Multijet background

Multijet background events pass the signal selection if a jet is misidentified as an isolated lepton or if the event has a non-prompt lepton that appears to be isolated. Since it is neither possible to simulate a sufficient number of those events nor possible to calculate the rate precisely, different techniques are developed to model multijet events and to estimate the production rate. These techniques employ both, collision data as well as simulated events.

In the electron channel, misidentified jets are the main source of multijet background events. This motivates the jet-lepton method in which an electron-like jet is selected with special requirements and redefined as a lepton. This jet has to fulfil the same pTp_{\rm T} and η\eta requirements as a signal electron, and contain at least four tracks to reduce the contribution from converted photons. In addition, the jet must deposit 80–95% of its energy in the electromagnetic calorimeter. Events are selected using the same criteria as for the signal selection except for the selection of the electron. The event is accepted if exactly one such ‘jet lepton’ is found. The jet-lepton selection is applied to a Pythia dijet sample and the resulting set of events is used to model the multijet background in the electron channel.

To determine the normalization of the multijet background in the electron channel, a binned maximum-likelihood fit to observed data in the ETmissE_{\mathrm{T}}^{\mathrm{miss}} distribution is performed after applying all selection criteria except for the ETmissE_{\mathrm{T}}^{\mathrm{miss}} requirement. In each channel two fits are performed separately; one for electrons in the central (|η|<1.5|\eta|<1.5) region and one for the endcap (|η|>1.5|\eta|>1.5) region of the electromagnetic calorimeter. The multijet template is fitted together with templates derived from Monte Carlo simulation for all other background processes whose rate uncertainties are accounted for in the fitting process in the form of additional constrained nuisance parameters. For the purpose of these fits the contributions from WW+light-jets and WW+bb¯b\bar{b}, WW+cc¯c\bar{c}, WW+cc, the contributions from tt¯t\bar{t} and single top-quark production, and the contributions from ZZ+jets and diboson production, are each combined into one template. Distributions normalized to the fit results in the 2-jet-e+e^{+} and 2-jet-ee^{-} signal regions for central electrons are shown in Fig. 2.

In the muon channel, the matrix method ATLAS Collaboration 2012e is used to obtain both the normalization and shape of the multijet background. The method estimates the number of multijet background events in the signal region based on loose and tight lepton isolation definitions, the latter selection being a subset of the former. Hence, the loose selection is defined to contain leptons of similar kinematics, but results in much higher event yields and is, except for the muon isolation requirement, identical to the signal selection. The number of multijet events NfaketightN^{\mathrm{tight}}_{\mathrm{fake}} passing the tight (signal) isolation requirements can be expressed as,

Nfaketight=ϵfakeϵrealϵfake(NlooseϵrealNtight),N^{\mathrm{tight}}_{\mathrm{fake}}=\frac{\epsilon_{\mathrm{fake}}}{\epsilon_{\mathrm{real}}-\epsilon_{\mathrm{fake}}}\cdot(N^{\mathrm{loose}}\epsilon_{\mathrm{real}}-N^{\mathrm{tight}}), (3)

where ϵreal\epsilon_{\mathrm{real}} and ϵfake\epsilon_{\mathrm{fake}} are the efficiencies for real and fake loose leptons being selected as tight leptons, NlooseN^{\mathrm{loose}} is the number of selected events in the loose sample, and NtightN^{\mathrm{tight}} is the number of selected events in the signal sample. The fake efficiencies are determined from collision data in a sample of selected muon candidates with high impact parameter significance which is defined by the impact parameter divided by its uncertainty. The real efficiencies are also estimated from collision data using a “tag-and-probe” method, which is based on the identification of a tight lepton and a loose lepton in events originating from a leptonically decaying ZZ boson.

An uncertainty of 50% is applied to the estimated yield of multijet background events based on comparisons of the rates obtained by using alternative methods, i.e. the matrix method in the electron channel and the jet-lepton method in the muon channel, and using an alternative variable, i.e. mT(ETmiss)m_{\mathrm{T}}(\ell E_{\mathrm{T}}^{\mathrm{miss}}) instead of ETmissE_{\mathrm{T}}^{\mathrm{miss}} for the binned maximum-likelihood fit.

V.3 𝒕𝒕¯\mathrm{{\bf{\emph{t}}}}\bar{\mathrm{{\bf{\emph{t}}}}} production and other backgrounds

The tt¯t\bar{t} cross section is calculated at NNLO in QCD including resummation of next-to-next-to-leading logarithmic (NNLL) soft gluon terms Cacciari et al. 2012; Baernreuther et al. 2012; Czakon and Mitov 2012; Czakon and Mitov 2013; Czakon et al. 2013 with Top++2.0 Czakon and Mitov 2011. The PDF and αs\alpha_{\mathrm{s}} uncertainties are calculated using the PDF4LHC prescription Botje et al. 2011 with the MSTW2008 NNLO Martin et al. 2009a; Martin et al. 2009b at 68% confidence level (CL), the CT10 NNLO Lai et al. 2010; Gao et al. 2014, and the NNPDF2.3 Ball et al. 2013 PDF sets, and are added in quadrature to the scale uncertainty, yielding a final uncertainty of 6%.

Since WtWt production is charge symmetric with respect to top-quark and top-antiquark production, the combined cross section of σ(Wt)=15.7±1.1\sigma(Wt)=15.7\pm 1.1\;pb Kidonakis 2010a is used in the analysis. The predicted cross sections for ss-channel production are σ(tb¯)=3.1±0.1\sigma(t\bar{b})=3.1\pm 0.1\;pb and σ(t¯b)=1.4±0.1\sigma(\bar{t}b)=1.4\pm 0.1\;pb Kidonakis 2010b. The predictions of σ(Wt)\sigma(Wt), σ(tb¯)\sigma(t\bar{b}), and σ(t¯b)\sigma(\bar{t}b) are given at approximate NNLO precision, applying soft-gluon resummation. Theoretical uncertainties including PDF and scale uncertainties are 4.4% Kidonakis 2010b for ss-channel single top-quark production and 7.0% Kidonakis 2010a for WtWt production. The PDF uncertainties are evaluated using the 40 associated eigenvector PDF sets of MSTW 2008 at 90% CL. The cross sections given above are used to compute the number of expected single top-quark events by normalizing the samples of simulated events.

All top-quark background processes are shown combined in the figures and used as a single process in the analysis. The charge asymmetry in ss-channel production is taken from the approximate NNLO prediction.

Diboson events (WWWW, WZWZ and ZZZZ) are normalized to the NLO cross-section prediction calculated with MCFM Campbell and Ellis 2010. The cross-section uncertainty for these processes is 5%.

V.4 Event yields

Table 1 provides the event yields after event selection. The yields are presented for the tagged channels, where exactly one bb-tagged jet is required, separated according to the lepton charge and for the 3-jet-2-tag channel. Small contributions from the tqtq process in the \ell^{-} regions and the t¯q\bar{t}q process in the +\ell^{+} regions originate from lepton charge misidentification.

Table 1: Predicted and observed events yields for the 2-jet and 3-jet channels considered in this measurement. The multijet background is estimated using data-driven techniques (see Sec. V.2); an uncertainty of 50% is applied. All the other expectations are derived using theoretical cross sections and their uncertainties (see Sec. V.1 and Sec. V.3).
2-jet channels 3-jet channels
+\ell^{+} \ell^{-} +\ell^{+} \ell^{-} 2-tag
tqtq 25502550±\>\pm\> 220220 3.63.6±\>\pm\> 0.30.3 845845±\>\pm\> 7474 1.21.2±\>\pm\> 0.10.1 309309±\>\pm\> 2626
t¯q\bar{t}q 1.51.5±\>\pm\> 0.10.1 13901390±\>\pm\> 120120 0.520.52±\>\pm\> 0.050.05 435435±\>\pm\> 3838 162162±\>\pm\> 1414
tt¯,Wt,tb¯,t¯bt\bar{t},Wt,t\bar{b},\bar{t}b 52505250±\>\pm\> 530530 51305130±\>\pm\> 510510 82008200±\>\pm\> 820820 81808180±\>\pm\> 820820 58505850±\>\pm\> 580580
W+W^{+}+bb¯b\bar{b},cc¯c\bar{c},light jets 57005700±\>\pm\> 25002500 16.316.3±\>\pm\> 8.28.2 24002400±\>\pm\> 12001200 11.511.5±\>\pm\> 5.75.7 200200±\>\pm\> 100100
WW^{-}+bb¯b\bar{b},cc¯c\bar{c},light jets 9.29.2±\>\pm\> 4.64.6 34003400±\>\pm\> 17001700 4.14.1±\>\pm\> 2.02.0 14701470±\>\pm\> 740740 137137±\>\pm\> 6868
WW+cc 14601460±\>\pm\> 350350 16201620±\>\pm\> 390390 388388±\>\pm\> 9393 430430±\>\pm\> 100100 6.56.5±\>\pm\> 1.61.6
ZZ+jets, diboson 370370±\>\pm\> 220220 310310±\>\pm\> 180180 190190±\>\pm\> 120120 180180±\>\pm\> 110110 2222±\>\pm\> 1313
Multijet 750750±\>\pm\> 340340 740740±\>\pm\> 370370 320320±\>\pm\> 160160 440440±\>\pm\> 220220 2121±\>\pm\> 1111
Total expectation 1610016100±\>\pm\> 26002600 1260012600±\>\pm\> 20002000 1240012400±\>\pm\> 15001500 1110011100±\>\pm\> 11001100 67106710±\>\pm\> 610610
Data 1619816198    1283712837    1246012460      1081910819    64036403   

VI Signal and background discrimination

To separate tt-channel single top-quark signal events from background events, several kinematic variables are combined to form powerful discriminants by employing neural networks. A large number of potential input variables were studied, including not only kinematic variables of the identified physics objects, but also variables obtained from the reconstruction of the WW boson and the top quark.

VI.1 Top-quark reconstruction

When reconstructing the WW boson, the transverse momentum of the neutrino is given by the xx- and yy-components of the ETmissE_{\mathrm{T}}^{\mathrm{miss}}, while the unmeasured zz-component of the neutrino momentum pz(ν)p_{z}(\nu) is inferred by imposing a WW-boson mass constraint on the lepton–neutrino system. Since the constraint leads to a quadratic equation for pz(ν)p_{z}(\nu), a two-fold ambiguity arises. In the case of two real solutions, the one with the lower |pz(ν)||p_{z}(\nu)| is chosen. In case of complex solutions, which can occur due to the low ETmissE_{\mathrm{T}}^{\mathrm{miss}} resolution, a kinematic fit is performed that rescales the neutrino pxp_{x} and pyp_{y} such that the imaginary part vanishes and at the same time the transverse components of the neutrino momentum are kept as close as possible to the ETmissE_{\mathrm{T}}^{\mathrm{miss}}. As a result of this algorithm, the four-momentum of the neutrino is reconstructed.

The top quark is reconstructed by adding the four-momenta of the reconstructed WW boson and the bb-tagged jet. Several angular variables, invariant masses and differences in pTp_{\mathrm{T}} are defined using the reconstructed physics objects.

VI.2 Selection of discriminating variables

The NeuroBayes Feindt and Kerzel 2006 tool is used for preprocessing the input variables and for the training of the NNs. The ranking of the variables in terms of their discrimination power is automatically determined as part of the preprocessing step and is independent of the training procedure ATLAS Collaboration 2012a. Only the highest-ranking variables are chosen for the training of the NNs. Separate NNs are trained in the 22-jet channel and 33-jet channel. In the training, no separation is made according to lepton charge or lepton flavour. Dedicated studies show that training in the channels separated by lepton charge does not lead to an improvement in sensitivity.

As a result of the optimization procedure in the 22-jet channel, 13 kinematic variables are identified as inputs to the NN. In the 33-jet channel, 11 variables are used. It was found that reducing the number of variables further would result in a considerable loss of sensitivity. The input variables to the NNs are listed in Table 2. The separation between signal and the two most important backgrounds, the top-quark background and the combined WW+light-jets, WW+cc¯c\bar{c}, and WW+bb¯b\bar{b} background, is shown in Fig. 3 for the two most important discriminating variables in the 22-jet channel.

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Figure 3: Probability densities of the two most important discriminating variables in the 22-jet channels, shown in the 2-jet-+\ell^{+} channel in the signal region (SR). The distributions are normalized to unit area. The absolute value of the pseudorapidity of the untagged jet |η(j)||\eta(j)| is shown in 3, and the invariant mass of the reconstructed top quark m(νb)m(\ell\nu b) is shown in 3.
Table 2: Input variables of the NNs in the 22-jet channels and in the 33-jet channels. The definitions of the variables use the term leading jet and 2nd leading jet, defined as the jet with the highest or 2nd highest pTp_{\rm T}, respectively. In the 2-jet channels, exactly one jet is required to be bb-tagged. The jet that is not bb-tagged is denoted untagged jet.
Variables used in the 22-jet channels and the 33-jet channels
m(νb)m(\ell\nu b) The invariant mass of the reconstructed top quark.
mT(ETmiss)m_{\mathrm{T}}(\ell E_{\mathrm{T}}^{\mathrm{miss}}) The transverse mass of the lepton–ETmissE_{\mathrm{T}}^{\mathrm{miss}}system, as defined in Eq. (1).
η(ν)\eta(\ell\nu) The pseudorapidity of the system of the lepton and the reconstructed neutrino.
m(b)m(\ell b) The invariant mass of the charged lepton and the bb-tagged jet.
HTH_{\mathrm{T}} The scalar sum of the transverse momenta of the jets, the charged lepton, and the ETmissE_{\mathrm{T}}^{\mathrm{miss}}.
Variables used in the 22-jet channels only
m(jb)m(jb) The invariant mass of the untagged jet and the bb-tagged jet.
|η(j)||\eta(j)| The absolute value of the pseudorapidity of the untagged jet.
ΔR(,j)\Delta R\left(\ell,j\right) ΔR\Delta R between the charged lepton and the untagged jet.
ΔR(νb,j)\Delta R\left(\ell\nu b,j\right) ΔR\Delta R between the reconstructed top quark and the untagged jet.
|η(b)||\eta\left(b\right)| The absolute value of the pseudorapidity of the bb-tagged jet.
|ΔpT(,j)||\Delta p_{\mathrm{T}}\left(\ell,j\right)| The absolute value of the difference between the transverse momentum of the charged lepton and the untagged jet.
|ΔpT(νb,j)||\Delta p_{\mathrm{T}}\left(\ell\nu b,j\right)| The absolute value of the difference between the transverse momentum of the reconstructed top quark and
the untagged jet.
ETmissE_{\mathrm{T}}^{\mathrm{miss}} The missing transverse momentum.
Variables used in the 33-jet channels only
|Δy(j1,j2)||\Delta y\left(j_{1},j_{2}\right)| The absolute value of the rapidity difference of the leading and 2nd leading jets.
m(j2j3)m\left(j_{2}j_{3}\right) The invariant mass of the 2nd leading jet and the 3rd leading jet.
cosθ(,j)νbr.f.\cos\theta\left(\ell,j\right)_{\ell\nu b\;\mathrm{r.f.}} The cosine of the angle θ\theta between the charged lepton and the leading untagged jet in the rest frame
of the reconstructed top quark.
Ση(ji)\Sigma\eta\left(j_{i}\right) The sum of the pseudorapidities of all jets in the event.
m(j1j2)m\left(j_{1}j_{2}\right) The invariant mass of the two leading jets.
pT(νb)p_{\mathrm{T}}\left(\ell\nu b\right) The transverse momentum of the reconstructed top quark.

The modeling of the input variables is checked in a control region (see Sec. IV for the definition) that is enriched in W+W+jets events. Figures 4 and 5 show the three most discriminating variables in the 2-jet-±\ell^{\pm} and 3-jet-±\ell^{\pm}-1-tag channels, respectively. Good modeling of the variables is observed.

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Figure 4: Distributions of the three most important discriminating variables in the 2-jet-+\ell^{+} and 2-jet-\ell^{-} channels in the control region (CR). Figures 4 and 4 display the absolute value of the pseudorapidity of the untagged jet |η(j)||\eta(j)|. Figures 4 and 4 show the invariant mass of the reconstructed top quark m(νb)m(\ell\nu b), 4 and 4 the invariant mass of the untagged and the bb-tagged jet m(jb)m(jb). The last histogram bin includes overflows. The multijet and the W+W+jets event yields are determined by a fit to the ETmissE_{\mathrm{T}}^{\mathrm{miss}} distribution as described in Sec. V.2. The uncertainty band represents the normalization uncertainty due to the uncertainty on the jet energy scale and the Monte Carlo statistical uncertainty. The relative difference between the observed and expected number of events in each bin is shown in the lower panels.
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Figure 5: Distributions of the three most important discriminating variables in the 3-jet-+\ell^{+} and 3-jet-\ell^{-} channels in the control region (CR). Figures 5 and 5 display the absolute value of the rapidity difference of the leading and 2nd leading jet |Δy(j1,j2)||\Delta y\left(j_{1},j_{2}\right)|, 5 and 5 the invariant mass of the 2nd leading jet and the 3rd jet m(j2j3)m\left(j_{2}j_{3}\right), and 5 and 5 show the invariant mass of the reconstructed top quark m(νb)m(\ell\nu b). The last histogram bin includes overflows. The multijet and the W+W+jets event yields are determined by a fit to the ETmissE_{\mathrm{T}}^{\mathrm{miss}} distribution as described in Sec. V.2. The uncertainty band represents the normalization uncertainty due to the uncertainty on the jet energy scale and the Monte Carlo statistical uncertainty. The relative difference between the observed and expected number of events in each bin is shown in the lower panels.

VI.3 Neural network training

After choosing a set of variables based on the criteria outlined above, the analysis proceeds with the training of the NNs using a three-layer feed-forward architecture. The number of hidden nodes was chosen to be 15 for both networks. Samples of simulated events are used for the training process, the size of the signal samples in the 22-jet channel being about 37,000 events for top-quark and about 40,000 events for top-antiquark tt-channel production. In the 3-jet channel the sizes of the training samples are 14,000 and 13,000 events, respectively. All background processes are used in the training, except for the multijet background whose modeling is associated with large uncertainties. The total number of simulated background events used in the training is about 89,000 in the 2-jet channel and about 57,000 in the 3-jet channel. The ratio of signal events to background events in the training is chosen to be 1:1, while the different background processes are weighted relative to each other according to the number of expected events.

Regularization techniques are applied in the training process to dampen statistical fluctuations in the training sample and to avoid overtraining. At the preprocessing stage mentioned above (Sec. VI.2), the input variables are transformed in several steps to define new input variables that are optimally prepared to be fed into an NN. First, the variables are transformed, such that they populate a finite interval and are distributed according to a uniform distribution. The influence of outliers is thereby strongly reduced. The distributions of the transformed variables are discretized using 100 bins, and the distributions for signal events are divided by the sum of signal and background events bin-by-bin, yielding the purity distributions in each variable. Next, these purity curves are fitted with a regularized spline function, thereby yielding a continuous transformation from the original input variables to the purities. By means of the spline fit statistical fluctuations in the input variables are significantly reduced. Applying the continuous purity functions to the input variables yields purity distributions that are further transformed, such that the distributions of the resulting variables are centered at zero and have an RMS of one. These variables are input to the NNs. In the training process, the network structure is pruned to arrive at a minimal topology, i.e. statistically insignificant network connections and nodes are removed.

In Fig. 6, the probability densities of the resulting NN discriminants are shown for the signal, the top-quark backgrounds, and the combined WW+light-jets, WW+cc¯c\bar{c}, and WW+bb¯b\bar{b} background.

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Figure 6: Probability densities of the NN discriminants in the 2-jet channels and 3-jet channels in the signal region (SR): 6 2-jet-+\ell^{+} channel, 6 2-jet-\ell^{-} channel, 6 3-jet-+\ell^{+} channel, and 6 3-jet-\ell^{-} channel. The distributions are normalized to unit area.

The separation between signal and backgrounds is equally good for the positive and the negative charge channels, which demonstrates that the choice of training the NNs with a charge-combined sample is appropriate.

VI.4 Extraction of the signal yield

The cross sections σ(tq)\sigma(tq) and σ(t¯q)\sigma(\bar{t}q) are extracted by performing a binned maximum-likelihood fit to the NN discriminant distributions in the 2-jet-+\ell^{+}, 2-jet-\ell^{-}, 3-jet-+\ell^{+}-1-tag, and 3-jet-\ell^{-}-1-tag channels and to the event yield in the 3-jet-2-tag channel, treating tt-channel top-quark and tt-channel top-antiquark production as independent processes. The signal rates, the rate of the combined top-quark background (tt¯t\bar{t}, WtWt, tb¯t\bar{b}, and t¯b\bar{t}b), the rate of the combined WW+light-jets, WW+cc¯c\bar{c}, and WW+bb¯b\bar{b} background, and the bb-tagging efficiency correction factor (discussed in Sec. III.4) are fitted in all channels simultaneously. The event yields of the multijet background and the WW+cc background are not allowed to vary in the fit, but instead are fixed to the estimates given in Table 1. The cross-section ratio is subsequently computed as Rt=σ(tq)/σ(t¯q)R_{t}=\sigma(tq)/\sigma(\bar{t}q).

The maximum-likelihood function is given by the product of Poisson probability terms for the individual histogram bins (see Ref. ATLAS Collaboration 2012a). Gaussian priors are added multiplicatively to the maximum-likelihood function to constrain the background rates subject to the fit and the correction factor of the bb-tagging efficiency to their predictions within the associated uncertainties.

The sensitivity to the background rates is mostly given by the background-dominated region close to zero in the NN discriminant distributions, while the sensitivity to the bb-tagging efficiency stems from the event yield in the 3-jet-2-tag channel with respect to the event yields in the 1-tag channels.

In Fig. 7 the observed NN discriminant distributions are shown compared to the compound model of signal and background normalized to the fit results. Figures 8 and 9 show the three most discriminating variables normalized to the fit results in the 2-jet-±\ell^{\pm} and 3-jet-±\ell^{\pm}-1-tag channels, respectively. Differences between data and prediction are covered by the normalization uncertainty of the different processes after the fit.

VI.5 High-purity region

A high-purity region (HPR) is defined to measure the differential cross sections in the 2-jet-+\ell^{+} and 2-jet-\ell^{-} channels, by requiring the NN discriminant to be larger than 0.80.8. In the 2-jet-+\ell^{+} HPR the signal contribution is twice as large as the background contribution. The signal and background contributions in the 2-jet-\ell^{-} HPR are of approximately the same size. The result of the fit described above is used to normalize the background in the HPR. Figure 10 shows the three most discriminating variables in the 2-jet-+\ell^{+} and 2-jet-\ell^{-} high-purity channels, normalized to the fit results. The data are well described by the predicted compound model.

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Figure 7: Neural network discriminant distributions normalized to the result of the binned maximum-likelihood fit in 7 the 2-jet-+\ell^{+} channel, 7 the 2-jet-\ell^{-} channel, 7 the 3-jet-+\ell^{+} channel, and 7 the 3-jet-\ell^{-} channel. The uncertainty band represents the normalization uncertainty of all processes after the fit and the Monte Carlo statistical uncertainty, added in quadrature. The relative difference between the observed and expected number of events in each bin is shown in the lower panels.
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Figure 8: Distributions of the three most important discriminating variables in the 2-jet-+\ell^{+} and 2-jet-\ell^{-} channels in the signal region normalized to the result of the binned maximum-likelihood fit to the NN discriminant as described in Sec. VI.4. Figures 8 and 8 display the absolute value of the pseudorapidity of the untagged jet |η(j)||\eta(j)|. Figures 8 and 8 show the invariant mass of the reconstructed top quark m(νb)m(\ell\nu b), 8 and 8 the invariant mass of the bb-tagged and the untagged jet m(jb)m(jb). The last histogram bin includes overflows. The uncertainty band represents the normalization uncertainty of all processes after the fit and the Monte Carlo statistical uncertainty, added in quadrature. The relative difference between the observed and expected number of events in each bin is shown in the lower panels.
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Figure 9: Distributions of the three most important discriminating variables in the 3-jet-+\ell^{+} and 3-jet-\ell^{-} channels in the signal region normalized to the result of the binned maximum-likelihood fit to the NN discriminant as described in Sec. VI.4. Figures 9 and 9 display the absolute value of the rapidity difference of the leading and 2nd leading jet |Δy(j1,j2)||\Delta y\left(j_{1},j_{2}\right)|, 9 and 9 the invariant mass of the 2nd leading jet and the 3rd jet m(j2j3)m\left(j_{2}j_{3}\right), and 9 and 9 show the invariant mass of the reconstructed top quark m(νb)m(\ell\nu b). The last histogram bin includes overflows. The uncertainty band represents the normalization uncertainty of all processes after the fit and the Monte Carlo statistical uncertainty, added in quadrature. The relative difference between the observed and expected number of events in each bin is shown in the lower panels.
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Figure 10: Distributions of the three most important discriminating variables in the 2-jet-+\ell^{+} and 2-jet-\ell^{-} channels in the high-purity region (HPR) normalized to the result of the binned maximum-likelihood fit to the NN discriminant as described in Sec. VI.4. Figures 10 and 10 display the absolute value of the pseudorapidity of the untagged jet |η(j)||\eta(j)|. Figures 10 and 10 show the invariant mass of the reconstructed top quark m(νb)m(\ell\nu b), 10 and 10 the invariant mass of the bb-tagged and the untagged jet m(jb)m(jb). The last histogram bin includes overflows. The uncertainty band represents the normalization uncertainty of all processes after the fit and the Monte Carlo statistical uncertainty, added in quadrature. The relative difference between the observed and expected number of events in each bin is shown in the lower panels.

VII Systematic uncertainties

For both the physical object definitions and the background estimations, systematic uncertainties are assigned to account for detector calibration and resolution uncertainties, as well as the uncertainties of theoretical predictions. These variations affect both normalization and shape of distributions for signal and backgrounds. The uncertainties can be split into the following categories: physics object modeling, Monte Carlo generators, PDFs, theoretical cross-section normalization, and luminosity.

VII.1 Physics object modeling

Systematic uncertainties on the reconstruction and energy calibration of jets, electrons and muons are propagated through the entire analysis. The main source of object modeling uncertainty comes from the jet energy scale (JES). The JES uncertainty has been evaluated for the in situ jet calibration ATLAS Collaboration 2013b; ATLAS Collaboration 2014c, which uses ZZ+jet, γ\gamma+jet, and dijet pTp_{\mathrm{T}}-balance measurements in data. The JES uncertainty is evaluated in several different categories:

  • Detector: The different pTp_{\mathrm{T}}-balance measurements have uncertainties due to the jet energy resolution, the electron and photon energy scale and the photon purity.

  • Physics modeling: The uncertainties in the in situ calibration techniques due to the choice of Monte Carlo generator, radiation modeling, and the extrapolation of Δϕ\Delta\phi between the jet and the ZZ boson.

  • Statistics: The uncertainty due to the limited size of the data sets of the in situ jet calibration measurements.

  • Mixed detector and modeling: In this category the uncertainty due to the modeling of the underlying event and soft radiation as well as modeling of the jet fragmentation are considered.

  • η\eta intercalibration modeling: The uncertainty in the dijet-pTp_{\mathrm{T}}-balance technique due to the modeling of additional parton radiation is estimated by comparing dijet events simulated with PYTHIA and HERWIG. This JES category is the largest contribution from the jet energy scale to the cross-section measurements.

  • Close-by jets: The jet calibration can be affected by the presence of close-by jets, located at radii ΔR<1.0\Delta R<1.0.

  • Pile-up: Uncertainties due to the modeling of the large pile-up effects in data are included as a function of jet pTp_{\mathrm{T}}  and η\eta.

  • Flavor composition: This uncertainty covers effects due to the difference in quark–gluon composition between the jets used in the calibration and the jets used in this analysis. Since the response to quark and gluon jets is different, the uncertainty on the quark–gluon composition in a given data sample leads to an uncertainty in the jet calibration.

  • Flavor response: In this category an uncertainty is considered due to imperfect knowledge of the calorimeter response to light-quark jets and gluon jets.

  • bb-JES: An additional JES uncertainty is evaluated for bb-quark jets by varying the modeling of bb-quark fragmentation.

The uncertainty due to the jet energy resolution is modeled by varying the pTp_{\mathrm{T}}  of the jets according to the systematic uncertainties of the resolution measurement performed on data using the dijet-balance method ATLAS Collaboration 2013c. The effect of uncertainties associated with the jet vertex fraction is also considered for each jet.

The tagging efficiencies of bb-jets, cc-jets, and light jets are derived from data ATLAS Collaboration 2012f; ATLAS Collaboration 2012g; ATLAS Collaboration 2012h and parameterized as a function of pTp_{\mathrm{T}}  and η\eta of the jet. The corresponding efficiencies in simulated events are corrected to be the same as those observed in data, and the uncertainties in the calibration method are propagated to the analysis. The difference in the bb-tagging efficiency between jets initiated by bb-quark and bb-antiquark is \sim1%, estimated from simulated tqtq and t¯q\bar{t}q events. To account for a possible uncertainty in the modeling of the detector response the full difference is taken as a systematic uncertainty. In Table 3 this uncertainty is called b/b¯b/\bar{b} acceptance.

The uncertainties due to lepton reconstruction, identification and trigger efficiencies are evaluated using tag-and-probe methods in ZZ\rightarrow\ell\ell events. Uncertainties due to the energy scale and resolution are considered for electrons and muons. Additionally, the lepton charge misidentification is taken into account and was evaluated to be about 0.1%. All lepton uncertainties are summarized in Table 3 in one item.

Other minor uncertainties are assigned to the reconstruction of ETmissE_{\mathrm{T}}^{\mathrm{miss}} and to account for the impact of pile-up collisions on the calculation of ETmissE_{\mathrm{T}}^{\mathrm{miss}}. The uncertainties on ETmissE_{\mathrm{T}}^{\mathrm{miss}} are summarized under ETmissE_{\mathrm{T}}^{\mathrm{miss}} modeling in Table 3.

VII.2 Monte Carlo generators

Systematic uncertainties arising from the modeling of the single top-quark signal, the tt¯t\bar{t} background, and the WW+jets background are taken into account.

The uncertainty due to the choice of single top-quark tt-channel generator and parton shower model is estimated by comparing events generated with POWHEG-BOX interfaced to PYTHIA and events generated with the NLO matrix-element generator MG5_aMC@NLO Alwall et al. 2014 and showered with HERWIG and JIMMY. Again the fixed four-flavor PDF set CT10f4 Lai et al. 2010 is used, and the renormalization and factorization scales are set to μR=μF=4mb2+pT,b2\mu_{\mathrm{R}}=\mu_{\mathrm{F}}=4\cdot\sqrt{m_{b}^{2}+p_{\mathrm{T},b}^{2}}, where mb=4.75GeVm_{b}=4.75{\mathrm{\ Ge\kern-1.00006ptV}} is the bb-quark mass, and pT,bp_{\mathrm{T},b} is the transverse momentum of the bb-quark. The uncertainty on the choice of μR\mu_{\mathrm{R}} and μF\mu_{\mathrm{F}} is estimated using events generated with POWHEG-BOX interfaced to PYTHIA. Factorization and renormalization scales are varied independently by factors of 0.50.5 and 2.02.0, while the scale of the parton shower is varied consistently with the renormalization scale. The uncertainty related to scale variations is then given by the envelope of all variations.

The modeling uncertainty for the tt¯t\bar{t} background is evaluated by comparing events simulated with the NLO generator POWHEG-BOX interfaced to PYTHIA and the multileg LO generator ALPGEN interfaced to HERWIG. An additional uncertainty for the top-quark background processes comes from the amount of initial-state and final-state radiation, estimated using dedicated AcerMC samples interfaced to PYTHIA where parameters controlling initial-state and final-state radiation (ISR/FSR) emission are varied. The variations of the parameters are constrained by a measurement of tt¯t\bar{t} production with a veto on additional central jet activity ATLAS Collaboration 2012i.

A shape uncertainty is assigned to the WW+jets background, based on variation of the choices of the matching scale and of the functional form of the factorization scale in ALPGEN.

The impact of using simulation samples of limited size is also taken into account.

VII.3 Parton distribution function

The systematic uncertainties related to the PDFs are taken into account for the acceptance of all single top-quark processes and tt¯t\bar{t} production. The simulated events are reweighted according to each of the PDF uncertainty eigenvectors. The uncertainty is calculated following the recommendation of the respective PDF group. The final PDF uncertainty is the envelope of the estimated uncertainties for the CT10 PDF set, the MSTW2008nlo Martin et al. 2009b PDF set and the NNPDF2.3 Ball et al. 2013 PDF set. For all PDFs the variable flavor number scheme Thorne 2010 is used.

VII.4 Theoretical cross-section normalization

In Sec. V the theoretical cross sections and their uncertainties are quoted for each background process. Since the tt¯t\bar{t}, single top-quark WtWt and ss-channel processes are grouped together in the statistical analysis, their uncertainties are added in proportion to their relative fractions, leading to a combined uncertainty of 6.7%. The uncertainty on the combined ZZ+jets and diboson background is 60% including a conservative estimate of the uncertainty of the heavy-flavor fraction of 50%, while the uncertainties of the WW+jets backgrounds are 24% for WW+cc and 36% for the combined WW+bb¯b\bar{b}, cc¯c\bar{c} and light jets including the same heavy-flavor-fraction uncertainty on the bb¯b\bar{b} and cc¯c\bar{c} contributions. Additionally, an uncertainty on the relative fraction of 2-jet to 3-jet events of 5% for events with light-flavor jets and 7% for events with heavy-flavor jets is applied for the WW+jets estimation. This uncertainty was estimated by varying the following input parameters of the generation with ALPGEN by a factor of two: the hard scattering scale, the coupling of the hard interaction, and the minimum pTp_{\mathrm{T}} and ΔR\Delta R separation of the partons.

VII.5 Luminosity

The luminosity measurement is calibrated using dedicated beam-separation scans, referred to as van der Meer scans, where the absolute luminosity can be inferred from the measurement of the beam parameters ATLAS Collaboration 2013a. The resulting uncertainty is 1.8%.

VII.6 Uncertainties on the cross-section measurements

The systematic uncertainties on the individual top-quark and top-antiquark cross-section measurements and their ratio are determined using pseudo-experiments that account for variations of the signal acceptance, the background rates, and the shape of the NN discriminant due to all sources of uncertainty described above. As an example, Fig. 11 shows the shape variation of the NN discriminant for tt-channel single top-quark signal events due to the variation of the JES because of the uncertainty on the η\eta intercalibration. The correlations between the different channels and the physics processes are fully accounted for.

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Figure 11: The normalized shape variation of the NN discriminant for the JES variation due to the uncertainty on the η\eta intercalibration in the 2-jet-+\ell^{+} channel, shown for the tqtq sample. The nominal shape is shown by the black points. Red denotes the JES shift-up and blue the NN response for JES shift-down. In the lower panel the relative difference between the number of expected events in the systematic variation and the nominal distribution is shown for each bin. The grey uncertainty band in the lower histogram represents the normalization uncertainty due to the Monte Carlo statistical uncertainty.

The probability densities of all possible outcomes of the measurements of σ(tq)\sigma(tq), σ(t¯q)\sigma(\bar{t}q) and RtR_{t} are obtained by performing the measurements on the pseudo-data. The values measured in data are used as central values when generating the pseudo-experiments. The root mean squares of the estimator distributions of the measured quantities are estimators of the measurement uncertainties.

Table 3 summarizes the contributions of the various sources of systematic uncertainty to the uncertainties on the measured values of σ(tq)\sigma(tq), σ(t¯q)\sigma(\bar{t}q), RtR_{t} and σ(tq+t¯q)\sigma(tq+\bar{t}q). The dominant systematic uncertainty on the cross sections is the JES η\eta-intercalibration uncertainty since one of the prominent features of tqtq production is a jet in the forward region.

Table 3: Detailed list of the contribution of each source of uncertainty to the total uncertainty on the measured values of σ(tq)\sigma(tq), σ(t¯q)\sigma(\bar{t}q), RtR_{t}, and σ(tq+t¯q)\sigma(tq+\bar{t}q). The evaluation of the systematic uncertainties has a statistical uncertainty of 0.3%. Uncertainties contributing less than 1.0% are marked with “<1<1”.
Source Δσ(tq)/σ(tq)\Delta\sigma(tq)/\sigma(tq) [%] Δσ(t¯q)/σ(t¯q)\Delta\sigma(\bar{t}q)/\sigma(\bar{t}q) [%] ΔRt/Rt\Delta R_{t}/R_{t} [%] Δσ(tq+t¯q)/σ(tq+t¯q)\Delta\sigma(tq+\bar{t}q)/\sigma(tq+\bar{t}q) [%]
Data statistical ±\pm3.1 ±\pm5.4 ±\pm6.2 ±\pm2.7
Monte Carlo statistical ±\pm1.9 ±\pm3.2 ±\pm3.6 ±\pm1.9
Multijet normalization ±\pm1.1 ±\pm2.0 ±\pm1.6 ±\pm1.4
Other background normalization ±\pm1.1 ±\pm2.8 ±\pm1.9 ±\pm1.6
JES detector ±\pm1.6 ±\pm1.4 <1<1 ±\pm1.4
JES statistical <1<1 <1<1 <1<1 <1<1
JES physics modeling <1<1 <1<1 <1<1 <1<1
JES η\eta intercalibration ±\pm6.9 ±\pm8.4 ±\pm1.8 ±\pm7.3
JES mixed detector and modeling <1<1 <1<1 <1<1 <1<1
JES close-by jets <1<1 <1<1 <1<1 <1<1
JES pile-up <1<1 <1<1 <1<1 <1<1
JES flavor composition ±\pm1.4 ±\pm1.4 ±\pm1.2 ±\pm1.6
JES flavor response <1<1 <1<1 ±\pm1.0 <1<1
bb-JES <1<1 <1<1 <1<1 <1<1
Jet energy resolution ±\pm2.1 ±\pm1.6 ±\pm1.0 ±\pm1.9
Jet vertex fraction <1<1 <1<1 <1<1 <1<1
bb-tagging efficiency ±\pm3.8 ±\pm4.1 <1<1 ±\pm3.9
cc-tagging efficiency <1<1 ±\pm1.4 <1<1 <1<1
Mistag efficiency <1<1 <1<1 <1<1 <1<1
b/b¯b/\bar{b} acceptance ±\pm1.0 <1<1 <1<1 --
ETmissE_{\mathrm{T}}^{\mathrm{miss}} modeling ±\pm2.3 ±\pm3.4 ±\pm1.6 ±\pm2.6
Lepton uncertainties ±\pm2.8 ±\pm3.0 ±\pm1.0 ±\pm2.8
PDF ±\pm3.2 ±\pm5.8 ±\pm2.5 ±\pm3.2
WW+jets shape variation <1<1 <1<1 <1<1 <1<1
tqtq generator + parton shower ±\pm1.9 ±\pm1.6 <1<1 ±\pm1.9
tqtq scale variations ±\pm2.6 ±\pm3.0 <1<1 ±\pm2.6
tt¯t\bar{t} generator + parton shower <1<1 ±\pm2.1 ±\pm1.6 <1<1
tt¯t\bar{t} ISR / FSR <1<1 <1<1 ±\pm1.0 <1<1
Luminosity ±\pm1.8 ±\pm1.8 ±\pm0.5 ±\pm1.8
Total systematic ±\pm12.0 ±\pm14.9 ±\pm6.1 ±\pm12.1
Total ±\pm12.4 ±\pm15.9 ±\pm8.7 ±\pm12.4

VIII Total cross-section measurements

After performing the binned maximum-likelihood fit and estimating the total uncertainty, the cross sections of top-quark and top-antiquark production in the tt-channel and their cross-section ratio RtR_{t} are measured to be:

σ(tq)=46±1(stat.)±6(syst.)pb=46±6pb,σ(t¯q)=23±1(stat.)±3(syst.)pb=23±4pbandRt=2.04±0.13(stat.)±0.12(syst.)=2.04±0.18,\begin{array}[]{rclcl}\sigma(tq)&=&46\pm 1\,(\mathrm{stat.})\pm 6\,(\mathrm{syst.})\,\mathrm{pb}&=&46\pm 6\,\mathrm{pb},\\ \sigma(\bar{t}q)&=&23\pm 1\,(\mathrm{stat.})\pm 3\,(\mathrm{syst.})\,\mathrm{pb}&=&23\pm 4\,\mathrm{pb}\ \ \ \mathrm{and}\\ R_{t}&=&2.04\pm 0.13\,(\mathrm{stat.})\,\pm 0.12\,(\mathrm{syst.})&=&2.04\pm 0.18,\end{array}

assuming a top-quark mass of mt=172.5GeVm_{t}=172.5{\mathrm{\ Ge\kern-1.00006ptV}}. Figure 12 compares the measured values of σ(tq)\sigma(tq), σ(t¯q)\sigma(\bar{t}q), and RtR_{t} to NLO predictions from MCFM Campbell et al. 2009 and Hathor Kant et al. 2014 using different PDF sets. Uncertainties on the predicted values include the uncertainty on the renormalization and factorization scales and the combined PDF and αs\alpha_{\mathrm{s}} uncertainty of the respective PDF set.

All PDF predictions are in agreement with all measurements. For σ(t¯q)\sigma(\bar{t}q), the predictions of all PDF sets agree well with each other and with the measured value. The predictions for σ(tq)\sigma(tq) and RtR_{t} with the ABM11 PDF set Alekhin et al. 2012 show an offset compared to the other predictions. With increasing precision, the measurement of these observables could provide a way to further constrain the involved PDFs.

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Figure 12: Comparison between observed and predicted values of 12 σ(tq)\sigma(tq), 12 σ(t¯q)\sigma(\bar{t}q), 12 RtR_{t}, and 12 σ(tq+t¯q)\sigma(tq+\bar{t}q). The predictions are calculated at NLO precision Campbell et al. 2009; Kant et al. 2014 in the five-flavor scheme and given for different NLO PDF sets Gluck et al. 2008; Aaron et al. 2010; Aaron et al. 2009 and the uncertainty includes the uncertainty on the renormalization and factorization scales, the combined internal PDF and αs\alpha_{\mathrm{s}} uncertainty. The dotted black line indicates the central value of the measured value. The combined statistical and systematic uncertainty of the measurement is shown in green, while the statistical uncertainty is represented by the yellow error band.

VIII.1 Inclusive cross-section measurement

The inclusive tt-channel cross section σ(tq+t¯q)\sigma(tq+\bar{t}q) is extracted by using only one scale factor β(tq+t¯q)\beta(tq+\bar{t}q) in the likelihood function, scaling the top-quark and the top-antiquark contributions simultaneously. The top-quark-to-antiquark ratio is taken from the approximate NNLO prediction Kidonakis 2011 (see Sec. I). The systematic uncertainties on the measured value of inclusive cross-section are determined as described in Sec. VII. A detailed list of the uncertainties is given in Table 3.

The binned maximum-likelihood fit yields a cross section of

σt(tq+t¯q)=68±2(stat.)±8(syst.)pb=68±8pb,\begin{array}[]{rcl}\sigma_{t}(tq+\bar{t}q)&=&68\pm 2\,(\mathrm{stat.})\;\pm 8\,(\mathrm{syst.})\;\mathrm{pb}\\ &=&68\pm 8\;\mathrm{pb,}\end{array}

assuming mt=172.5GeVm_{t}=172.5{\mathrm{\ Ge\kern-1.00006ptV}}. Figure 12 compares the measured value for σ(tq+t¯q)\sigma(tq+\bar{t}q) to NLO predictions Campbell et al. 2009; Kant et al. 2014 obtained with different PDF sets. All predictions are in agreement with the measurement.

VIII.2 Cross-section dependence on the top-quark mass

The tt-channel single top-quark cross sections are measured using a signal model with mt=172.5GeVm_{t}=172.5{\mathrm{\ Ge\kern-1.00006ptV}}. The dependence of the cross-section measurements on mtm_{t} is mainly due to acceptance effects and is expressed by the function:

σt=σt(172.5GeV)+p1Δmt+p2Δmt2\sigma_{t}=\sigma_{t}(172.5{\mathrm{\ Ge\kern-1.00006ptV}})+p_{1}\cdot\Delta m_{t}+p_{2}\cdot\Delta m_{t}^{2} (4)

with Δmt=mt172.5GeV\Delta m_{t}=m_{t}-172.5{\mathrm{\ Ge\kern-1.00006ptV}}. The parameters p1p_{1} and p2p_{2} are determined using dedicated signal samples with different mtm_{t} and are given in Table 4 for σ(tq)\sigma(tq), σ(t¯q)\sigma(\bar{t}q) and σ(tq+t¯q)\sigma(tq+\bar{t}q). The cross-section ratio RtR_{t} is largely independent of the top-quark mass.

Table 4: Parameterization factors for the mtm_{t} dependence (see Eq. (4)) of σ(tq)\sigma(tq), σ(t¯q)\sigma(\bar{t}q) and σ(tq+t¯q)\sigma(tq+\bar{t}q).
p1 [pb/GeV] p2 [pb/GeV2{\mathrm{\ Ge\kern-1.00006ptV}}^{2}]
σ(tq+t¯q)\sigma(tq+\bar{t}q) 0.46-0.46 0.06-0.06
σ(tq)\sigma(tq) 0.27-0.27 0.04-0.04
σ(t¯q)\sigma(\bar{t}q) 0.19-0.19 0.02-0.02

VIII.3 VtbV_{tb} extraction

Since σ(tq+t¯q)\sigma(tq+\bar{t}q) is proportional to |Vtb|2|V_{tb}|^{2}, |Vtb||V_{tb}| can be extracted from the measurement. The |Vtb||V_{tb}| measurement is independent of assumptions about the number of quark generations and about the unitarity of the CKM matrix. The only assumptions required are that |Vtb||Vtd|,|Vts||V_{tb}|\gg|V_{td}|,|V_{ts}| and that the WtbWtb interaction is an SM-like left-handed weak coupling. The tt¯t\bar{t}-background rate is unaffected by a variation of |Vtb||V_{tb}|, since the decay to a quark of a potentially existing higher generation are prohibited by kinematics, such that the branching ratio B(tWb)1B(t\rightarrow Wb)\sim 1. On the other hand, the rates of single-top quark WtWt and ss-channel backgrounds also scale with |Vtb|2|V_{tb}|^{2}, but their contributions are small in the signal region. The resulting variation of the total top-quark background yield is less than its systematic uncertainty and thus considered negligible.

The value of |Vtb|2|V_{tb}|^{2} is extracted by dividing the measured value of σ(tq+t¯q)\sigma(tq+\bar{t}q) by the prediction of the approximate NNLO calculation Kidonakis 2011. The experimental and theoretical uncertainties are added in quadrature. The result obtained is

|Vtb|=1.02±0.01(stat.)±0.06(syst.)±0.02(theo.)+0.010.00(mt)=1.02±0.07.\begin{array}[]{rcl}|V_{tb}|&=&1.02\pm 0.01(\mathrm{stat.})\pm 0.06\,(\mathrm{syst.})\pm 0.02\,(\mathrm{theo.})\,^{+0.01}_{-0.00}\,(m_{t})\\ &=&1.02\pm 0.07.\end{array}

A lower limit on |Vtb||V_{tb}| is extracted in a Bayesian limit computation, assuming that the likelihood curve of |Vtb|2|V_{tb}|^{2} has a Gaussian shape, centered at the measured value. A flat prior in |Vtb|2|V_{tb}|^{2} is applied, being one in the interval [0,1][0,1] and zero otherwise. The resulting lower limit is |Vtb|>0.88|V_{tb}|>0.88 at the 95% CL.

IX Differential cross-section measurements

Differential cross sections are measured as a function of the pTp_{\mathrm{T}} and |y||y| of tt and t¯\bar{t} in the 2-jet HPR channels, defined in Sec. VI.5.

IX.1 Signal yield and reconstructed variables

The signal and background composition in the 2-jet-+\ell^{+} and the 2-jet-\ell^{-} HPR channels can be found in Table 5. Figure 13 shows the measured distributions of the reconstructed top-quark pTp_{\mathrm{T}} and the reconstructed top-quark |y||y| normalized to the result of the binned maximum-likelihood fit performed to measure σ(tq)\sigma(tq) and σ(t¯q)\sigma(\bar{t}q).

The binning of the differential cross sections is chosen based on the experimental resolution of the pTp_{\mathrm{T}} and |y||y| distributions as well as the data statistical uncertainty. Typical values for the resolution of the top-quark pTp_{\mathrm{T}} are 10 GeV{\mathrm{\ Ge\kern-1.00006ptV}}, increasing to 25 GeV{\mathrm{\ Ge\kern-1.00006ptV}} in the tail of the distribution. The resolution of the rapidity varies from 0.2 to 0.4 from central to forward rapidities.

Table 5: Event yields for the 2-jet-+\ell^{+} and 2-jet-\ell^{-} HPR channels. The expectation for the signal and background yields correspond to the result of the binned maximum-likelihood fit described in Sec. VI.4. The uncertainty of the expectations is the normalization uncertainty of each processes after the fit, as described in Sec. VII.6.
2-jet-+\ell^{+} HPR 2-jet-\ell^{-} HPR
tqtq 1210±\>\pm\> 150 1.3±\>\pm\> 0.2
t¯q\bar{t}q 0.29±\>\pm\> 0.05 549±\>\pm\> 87
tt¯t\bar{t},WtWt,tb¯t\bar{b},t¯b\bar{t}b 161±\>\pm\> 18 175±\>\pm\> 19
W+W^{+}+bb¯b\bar{b},cc¯c\bar{c},light jets 250±\>\pm\> 48 0.35±\>\pm\> 0.07
WW^{-}+bb¯b\bar{b},cc¯c\bar{c},light jets 0.7±\>\pm\> 0.2 166±\>\pm\> 40
WW+cc 110±\>\pm\> 26 125±\>\pm\> 30
ZZ+jets, diboson 15±\>\pm\> 10 11.4±\>\pm\> 6.8
Multijet 59±\>\pm\> 30 62±\>\pm\> 31
Total expectation 1810±\>\pm\> 160 1090±\>\pm\> 110
Data 1813      1034      
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Figure 13: Measured distributions of 13 the top-quark pTp_{\mathrm{T}}, 13 top-antiquark pTp_{\mathrm{T}}, 13 top-quark |y||y|, and 13 top-antiquark |y||y| shown on reconstruction level in the HPR normalized to the result of the binned maximum-likelihood fit. The uncertainty band represents the normalization uncertainty of all processes after the fit and the Monte Carlo statistical uncertainty, added in quadrature. The relative difference between the observed and expected number of events in each bin is shown in the lower panels.

IX.2 Method

The measured distributions are distorted by detector effects and acceptance effects. The observed distributions are unfolded to the (parton level) four-momenta of the top quarks before the decay and after QCD radiation to correct for these distortions. In the following, each bin of the measured distribution is referred to by the index ii, while each bin of the parton-level distribution is referred to by the index jj. The relation between the measured distribution and the differential cross section in each bin jj of the parton-level distribution can be written as:

dσdXj=1ΔXjiMij1(NiBi)ϵjB(tνb)\frac{d\sigma}{dX_{j}}=\frac{1}{\Delta X_{j}}\cdot\frac{\sum\limits_{i}M_{ij}^{-1}\cdot(N_{i}-B_{i})}{\mathcal{L}\cdot\epsilon_{j}\cdot\it{B}(t\rightarrow\ell\nu b)} (5)

where ΔXj\Delta X_{j} is the bin width of the parton-level distribution, NiN_{i} (BiB_{i}) are the data (expected background) yields in each bin of the measured distribution, \mathcal{L} is the integrated luminosity of the data sample, ϵj\epsilon_{j} is the event selection efficiency and Mij1M_{ij}^{-1} is the inverse of the migration matrix. The migration matrix accounts for the detector response and is defined as the probability to observe an event in bin ii when it is generated in bin jj. The migration matrix is built by relating the variables at the reconstruction and at the parton level using the signal simulation. Figure 14 shows the migration matrices for the pTp_{\mathrm{T}} and |y||y| distributions of the top quark and top antiquark. The inverse of the matrix is determined by applying Bayes’ theorem iteratively D’Agostini 1995 in order to perform the unfolding. The number of iterations is chosen such that the absolute change in the unfolded distributions is on average smaller than 1% of the content in each bin. This procedure results in a total of five iterations for all distributions. The selection efficiency ϵj\epsilon_{j} in bin jj of each variable is defined as the ratio of the parton-level yield before and after selection and is evaluated using simulation. The efficiencies are typically in the 0.5–2.2% range.

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Figure 14: Migration matrices relating the parton level shown on the yy axis and reconstruction level shown on the xx axis for the 14 top-quark pTp_{\mathrm{T}}, 14 top-antiquark pTp_{\mathrm{T}}, 14 top-quark |y||y|, and 14 top-antiquark |y||y| distribution.

The unfolding is applied to the reconstructed pT(νb)p_{\mathrm{T}}(\ell\nu b) and |y(νb)||y(\ell\nu b)| distributions after subtraction of the background contributions. When subtracting the background, all backgrounds are normalized according to Table 5.

Closure tests are performed in order to check the validity of the unfolding procedure. The shape of the parton-level distributions in the Monte Carlo simulation are altered to verify that the simulation does not bias the results. It is checked that the altered parton-level distributions are recovered by unfolding the reconstructed distributions with the nominal migration matrix.

IX.3 Treatment of uncertainties

The statistical uncertainty of the unfolded results is estimated using pseudo-experiments, propagating the uncertainties from the measured distribution and from the size of the Monte Carlo signal and background samples through the unfolding process. All sources of systematic uncertainty described in Sec. VII are included for the unfolded distributions. In the case of the background normalization, the uncertainties quoted in Table 5 are taken into account. The impact of the systematic uncertainties is evaluated by modifying the subtracted background before unfolding in the case of uncertainties on the backgrounds. To assign uncertainties on the signal modeling, systematic shifts are applied to the simulated signal sample. The shifted reconstructed distribution is unfolded and then compared to the nominal distribution at parton level.

IX.4 Results

To reduce the impact of systematic uncertainties normalized differential cross sections 1/σ(dσ/dXj)1/\sigma\cdot(d\sigma/dX_{j}) are calculated by dividing the differential cross section by the total cross section evaluated by integrating over all bins.

The absolute differential cross-section results are listed in Table 6 and the normalized resutls in Table 7 as a function of pTp_{\mathrm{T}} and |y||y| of the top quark. A graphical representation of the results is shown in Fig. 15 for the absolute cross sections and in Fig. 16 for the normalized case. They are compared to NLO predictions from MCFM Campbell and Ellis 2010 using the MSTW2008 PDF set for all variables. Uncertainties on the predicted values include the uncertainty on the scale and the PDF. To compare the NLO prediction with the measurement, χ2\chi^{2} values are computed with HERAfitter Aaron et al. 2010; Aaron et al. 2009 taking into account the full correlation of the systematic and statistical uncertainties. The χ2\chi^{2} values for the differential cross sections are listed in Table 8.

Systematic uncertainties dominate over the statistical uncertainty for the differential cross sections. Large uncertainties originate from the background normalization, the tqtq generator + parton shower uncertainty, the JES due to the uncertainty in the η\eta intercalibration as well as the PDF uncertainties mainly in the top-antiquark distributions. A detailed list of the systematic contributions in each bin of each distributions is shown in Table 9 for dσ/dpT(t)d\sigma/dp_{\mathrm{T}}(t), in Table 10 for dσ/dpT(t¯)d\sigma/dp_{\mathrm{T}}(\bar{t}), in Table 11 for dσ/d|y(t)|d\sigma/d|y(t)|, and in Table 12 for dσ/d|y(t¯)|d\sigma/d|y(\bar{t})|. In the case of the normalized differential cross sections many systematic uncertainties cancel and thus the measurement is dominated by statistical uncertainties from the data distributions and the Monte Carlo sample size. The contribution of systematic uncertainties to the normalized distribution is again dominated by the background normalization, tqtq generator + parton shower, and the JES η\eta-intercalibration uncertainty. Details of the contribution of each systematic uncertainty in each bin of the normalized distributions are listed in Table 13 for 1/σdσ/dpT(t)1/\sigma\cdot d\sigma/dp_{\mathrm{T}}(t), in Table 14 for 1/σdσ/dpT(t¯)1/\sigma\cdot d\sigma/dp_{\mathrm{T}}(\bar{t}), in Table 15 for 1/σdσ/d|y(t)|1/\sigma\cdot d\sigma/d|y(t)|, and in Table 16 for 1/σdσ/d|y(t¯)|1/\sigma\cdot d\sigma/d|y(\bar{t})|. Bin-wise correlation matrices for the statistical uncertainty are given in Fig. 17 for the differential cross sections and in Fig. 18 for the normalized differential cross sections.

Overall, good agreement is observed between the NLO QCD predictions and the differential cross-section measurements. This is also supported by the χ2\chi^{2} values listed in Table 8.

The contents of Tables 6 to 16 and the contents of Fig. 17 and Fig. 18 are provided in machine-readable format in the Supplemental Material sup.

X Conclusions

In summary, measurements of the single top-quark production cross sections, σ(tq)\sigma(tq), σ(t¯q)\sigma(\bar{t}q), RtR_{t}, and σ(tq+t¯q)\sigma(tq+\bar{t}q), with the ATLAS detector at the LHC are presented using an integrated luminosity of 4.59 fb-1 pppp collision data at s=7TeV\sqrt{s}=7{\mathrm{\ Te\kern-1.00006ptV}}. All measurements are based on neural network (NN) discriminants separating signal events from background events. Binned maximum-likelihood fits to the NN discriminants yield: σ(tq)=46±6pb\sigma(tq)=46\pm 6\,\mathrm{pb}, σ(t¯q)=23±4pb\sigma(\bar{t}q)=23\pm 4\,\mathrm{pb}, and σ(tq+t¯q)=68±8pb\sigma(tq+\bar{t}q)=68\pm 8\,\mathrm{pb}. The measured cross-section ratio is Rt=2.04±0.18R_{t}=2.04\pm 0.18. The corresponding coupling at the WtbWtb vertex is |Vtb|=1.02±0.07|V_{tb}|=1.02\pm 0.07, and the 95% CL lower limit on the CKM matrix element |Vtb||V_{tb}| is 0.88. A high-purity region is defined using the signal region of the NN discriminant for the differential cross-section measurements. Using an iterative Bayesian method, differential cross sections are extracted as a function of pT(t)p_{\mathrm{T}}(t), pT(t¯)p_{\mathrm{T}}(\bar{t}), |y(t)||y(t)|, and |y(t¯)||y(\bar{t})|. Good agreement with the NLO QCD predictions is observed.

Acknowledgements

We thank CERN for the very successful operation of the LHC, as well as the support staff from our institutions without whom ATLAS could not be operated efficiently.

We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF, DNSRC and Lundbeck Foundation, Denmark; EPLANET, ERC and NSRF, European Union; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, DFG, HGF, MPG and AvH Foundation, Germany; GSRT and NSRF, Greece; ISF, MINERVA, GIF, I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO, Netherlands; BRF and RCN, Norway; MNiSW and NCN, Poland; GRICES and FCT, Portugal; MNE/IFA, Romania; MES of Russia and ROSATOM, Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS and MIZŠ, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC and Wallenberg Foundation, Sweden; SER, SNSF and Cantons of Bern and Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, the Royal Society and Leverhulme Trust, United Kingdom; DOE and NSF, United States of America.

The crucial computing support from all WLCG partners is acknowledged gratefully, in particular from CERN and the ATLAS Tier-1 facilities at TRIUMF (Canada), NDGF (Denmark, Norway, Sweden), CC-IN2P3 (France), KIT/GridKA (Germany), INFN-CNAF (Italy), NL-T1 (Netherlands), PIC (Spain), ASGC (Taiwan), RAL (UK) and BNL (USA) and in the Tier-2 facilities worldwide.

Table 6: Differential tt-channel top-quark production cross section as a function of pT(t)p_{\mathrm{T}}(t), pT(t¯)p_{\mathrm{T}}(\bar{t}), |y(t)||y(t)| and |y(t¯)||y(\bar{t})| with the uncertainties for each bin given in percent. The contents of this table are provided in machine-readable format in the Supplemental Material sup.
pT(t)p_{\mathrm{T}}(t) [GeV] dσdpT(t)\frac{d\sigma}{dp_{\mathrm{T}}(t)} [fbGeV][\frac{\mathrm{fb}}{{\mathrm{\ Ge\kern-0.79727ptV}}}] total [%] stat. [%] syst. [%]
[0,45][0,45] 440±70440\pm 70 ±15\pm 15 ±7.4\pm 7.4 ±13\pm 13
[45,75][45,75] 370±60370\pm 60 ±16\pm 16 ±6.5\pm 6.5 ±14\pm 14
[75,110][75,110] 250±40250\pm 40 ±15\pm 15 ±7.7\pm 7.7 ±13\pm 13
[110,150][110,150] 133±27133\pm 27 ±20\pm 20 ±12\pm 12 ±16\pm 16
[150,500][150,500] 7.8±1.97.8\pm 1.9 ±24\pm 24 ±16\pm 16 ±19\pm 19
pT(t¯)p_{\mathrm{T}}(\bar{t}) [GeV] dσdpT(t¯)\frac{d\sigma}{dp_{\mathrm{T}}(\bar{t})} [fbGeV][\frac{\mathrm{fb}}{{\mathrm{\ Ge\kern-0.79727ptV}}}] total [%] stat. [%] syst. [%]
[0,45][0,45] 190±50190\pm 50 ±28\pm 28 ±12\pm 12 ±25\pm 25
[45,75][45,75] 230±40230\pm 40 ±18\pm 18 ±8.2\pm 8.2 ±17\pm 17
[75,110][75,110] 97±2797\pm 27 ±27\pm 27 ±13\pm 13 ±24\pm 24
[110,150][110,150] 13.0±9.713.0\pm 9.7 ±74\pm 74 ±26\pm 26 ±70\pm 70
[150,500][150,500] 1.4±0.91.4\pm 0.9 ±59\pm 59 ±26\pm 26 ±53\pm 53
|y(t)||y(t)| dσd|y(t)|\frac{d\sigma}{d|y(t)|}[pb] total [%] stat. [%] syst. [%]
[0,0.2][0,0.2] 28±428\pm 4 ±15\pm 15 ±9.0\pm 9.0 ±12\pm 12
[0.2,0.6][0.2,0.6] 27.3±3.327.3\pm 3.3 ±12\pm 12 ±6.3\pm 6.3 ±10\pm 10
[0.6,1.1][0.6,1.1] 22.1±3.022.1\pm 3.0 ±14\pm 14 ±7.5\pm 7.5 ±11\pm 11
[1.1,3.0][1.1,3.0] 10.7±1.610.7\pm 1.6 ±15\pm 15 ±7.0\pm 7.0 ±13\pm 13
|y(t¯)||y(\bar{t})| dσd|y(t¯)|\frac{d\sigma}{d|y(\bar{t})|} [pb] total [%] stat. [%] syst. [%]
[0,0.2][0,0.2] 15.0±3.415.0\pm 3.4 ±23\pm 23 ±13\pm 13 ±18\pm 18
[0.2,0.6][0.2,0.6] 13.3±3.313.3\pm 3.3 ±25\pm 25 ±9.5\pm 9.5 ±23\pm 23
[0.6,1.1][0.6,1.1] 11.2±2.611.2\pm 2.6 ±23\pm 23 ±11\pm 11 ±20\pm 20
[1.1,3.0][1.1,3.0] 3.3±0.93.3\pm 0.9 ±29\pm 29 ±13\pm 13 ±25\pm 25
Table 7: Normalized differential tt-channel top-quark production cross section as a function of pT(t)p_{\mathrm{T}}(t), pT(t¯)p_{\mathrm{T}}(\bar{t}), |y(t)||y(t)| and |y(t¯)||y(\bar{t})| with the uncertainties for each bin given in percent. The contents of this table are provided in machine-readable format in the Supplemental Material sup.
pT(t)p_{\mathrm{T}}(t) [GeV] 1σdσdpT(t)[103GeV]\frac{1}{\sigma}\frac{d\sigma}{dp_{\mathrm{T}}(t)}[\frac{10^{-3}}{{\mathrm{\ Ge\kern-0.79727ptV}}}] total [%] stat. [%] syst. [%]
[0,45][0,45] 9.20.9+0.89.2^{+0.8}_{-0.9} 9.4+8.4{}^{+8.4}_{-9.4} ±5.3\pm 5.3 7.7+6.5{}^{+6.5}_{-7.7}
[45,75][45,75] 7.8±0.97.8\pm 0.9 ±11\pm 11 ±6.9\pm 6.9 ±8.8\pm 8.8
[75,110][75,110] 5.3±0.85.3\pm 0.8 ±15\pm 15 ±8.0\pm 8.0 ±13\pm 13
[110,150][110,150] 2.8±0.62.8\pm 0.6 ±21\pm 21 ±11\pm 11 ±18\pm 18
[150,500][150,500] 0.16±0.040.16\pm 0.04 ±22\pm 22 ±15\pm 15 ±16\pm 16
pT(t¯)p_{\mathrm{T}}(\bar{t}) [GeV] 1σdσdpT(t¯)[103GeV]\frac{1}{\sigma}\frac{d\sigma}{dp_{\mathrm{T}}(\bar{t})}[\frac{10^{-3}}{{\mathrm{\ Ge\kern-0.79727ptV}}}] total [%] stat. [%] syst. [%]
[0,45][0,45] 9.6±1.69.6\pm 1.6 ±17\pm 17 ±8.2\pm 8.2 ±15\pm 15
[45,75][45,75] 11.6±1.811.6\pm 1.8 ±15\pm 15 ±8.8\pm 8.8 ±12\pm 12
[75,110][75,110] 4.9±1.24.9\pm 1.2 ±25\pm 25 ±13\pm 13 ±21\pm 21
[110,150][110,150] 0.7±0.40.7\pm 0.4 61+67{}^{+67}_{-61} ±25.8\pm 25.8 56+62{}^{+62}_{-56}
[150,500][150,500] 0.07±0.040.07\pm 0.04 ±51\pm 51 ±26\pm 26 ±45\pm 45
|y(t)||y(t)| 1σdσd|y(t)|\frac{1}{\sigma}\frac{d\sigma}{d|y(t)|} total [%] stat. [%] syst. [%]
[0,0.2][0,0.2] 0.59±0.090.59\pm 0.09 ±15\pm 15 ±9.0\pm 9.0 ±11\pm 11
[0.2,0.6][0.2,0.6] 0.57±0.050.57\pm 0.05 ±9.0\pm 9.0 ±6.4\pm 6.4 ±6.3\pm 6.3
[0.6,1.1][0.6,1.1] 0.46±0.050.46\pm 0.05 ±9.7\pm 9.7 ±7.5\pm 7.5 ±6.2\pm 6.2
[1.1,3.0][1.1,3.0] 0.223±0.0190.223\pm 0.019 ±8.5\pm 8.5 ±4.9\pm 4.9 ±6.9\pm 6.9
|y(t¯)||y(\bar{t})| 1σdσd|y(t¯)|\frac{1}{\sigma}\frac{d\sigma}{d|y(\bar{t})|} total [%] stat. [%] syst. [%]
[0,0.2][0,0.2] 0.75±0.140.75\pm 0.14 ±19\pm 19 ±13\pm 13 ±13\pm 13
[0.2,0.6][0.2,0.6] 0.66±0.110.66\pm 0.11 ±17\pm 17 ±9.1\pm 9.1 ±14\pm 14
[0.6,1.1][0.6,1.1] 0.555±0.0950.555\pm 0.095 ±17\pm 17 ±11\pm 11 ±13\pm 13
[1.1,3.0][1.1,3.0] 0.163±0.0300.163\pm 0.030 ±18\pm 18 ±11\pm 11 ±15\pm 15
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Figure 15: Differential cross section as a function of 15 pT(t)p_{\mathrm{T}}(t), 15 pT(t¯)p_{\mathrm{T}}(\bar{t}), 15 |y(t)||y(t)| and 15 |y(t¯)||y(\bar{t})|. The differential distributions are compared to the QCD NLO calculation. The black vertical error bars on the data points denote the total combined uncertainty, the green error bars denote the statistical uncertainty, while the red band denotes the theory predictions calculated at NLO using MCFM Campbell and Ellis 2010. Uncertainties on the predicted values include the PDF and scale uncertainties. The horizontal error bars indicate the bin width.
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Figure 16: Normalized differential cross section as a function of 16 pT(t)p_{\mathrm{T}}(t), 16 pT(t¯)p_{\mathrm{T}}(\bar{t}), 16 |y(t)||y(t)| and 16 |y(t¯)||y(\bar{t})|. The normalized differential distributions are compared to the QCD NLO calculation. The black vertical error bars on the data points denote the total combined uncertainty, the green error bars denote the statistical uncertainty, while the red band denotes the theory predictions calculated at NLO using MCFM Campbell and Ellis 2010. Uncertainties on the predicted values include the PDF and scale uncertainties. The horizontal error bars indicate the bin width.
Table 8: Comparison between the measured differential cross sections and the predictions from the NLO calculation using the MSTW2008 PDF set. For each variable and prediction a χ2\chi^{2} value is calculated with HERAfitter using the covariance matrix of each measured spectrum. The theory uncertainties of the predictions are treated as uncorrelated. The number of degrees of freedom (NDF) is equal to the number of bins in the measured spectrum. The contents of this table are provided in machine-readable format in the Supplemental Material sup.
dσdpT(t)\frac{d\sigma}{dp_{\mathrm{T}}(t)} dσdpT(t¯)\frac{d\sigma}{dp_{\mathrm{T}}(\bar{t})} dσd|y(t)|\frac{d\sigma}{d|y(t)|} dσd|y(t¯)|\frac{d\sigma}{d|y(\bar{t})|}
χ2/NDF\chi^{2}/\mathrm{NDF} 7.55/57.55/5 4.68/54.68/5 6.30/46.30/4 0.32/40.32/4
Table 9: Detailed list of the contribution of each source of uncertainty to the total relative uncertainty on the measured dσdpT(t)\frac{d\sigma}{dp_{\mathrm{T}}(t)} distribution given in percent for each bin. The list includes only those uncertainties that contribute with more than 1%. The following uncertainties contribute to the total uncertainty with less than 1% to each bin content: JES detector, JES statistical, JES physics modeling, JES mixed detector and modeling, JES close-by jets, JES pile-up, JES flavor composition, JES flavor response, jet vertex fraction, b/b¯b/\bar{b} acceptance, ETmissE_{\mathrm{T}}^{\mathrm{miss}} modeling, WW+jets shape variation, and tt¯t\bar{t} generator. The contents of this table are provided in machine-readable format in the Supplemental Material sup.
dσdpT(t)\frac{d\sigma}{dp_{\mathrm{T}}(t)} pT(t)p_{\mathrm{T}}(t) bins [GeV]
Source [0,45][0,45] [45,75][45,75] [75,110][75,110] [110,150][110,150] [150,500][150,500]
Data statistical ±\pm7.4 ±\pm6.5 ±\pm7.7 ±\pm12 ±\pm16
Monte Carlo statistical ±\pm5.5 ±\pm5.3 ±\pm4.8 ±\pm6.0 ±\pm9.4
Background normalization ±\pm6.1 ±\pm7.5 ±\pm5.2 ±\pm3.0 ±\pm5.2
JES η\eta intercalibration << 1 +2.6/1.3+2.6/-1.3 +3.4/1.9+3.4/-1.9 << 1 +9.0/4.2+9.0/-4.2
bb-JES << 1 +1.2/2.3+1.2/-2.3 << 1 ±\pm1.6 << 1
Jet energy resolution ±\pm1.0 ±\pm2.4 ±\pm2.3 ±\pm3.0 << 1
bb-tagging efficiency ±\pm3.0 ±\pm3.1 ±\pm3.3 ±\pm3.6 ±\pm6.2
cc-tagging efficiency ±\pm1.3 ±\pm1.5 << 1 << 1 << 1
Mistag efficiency ±\pm2.0 ±\pm1.9 << 1 << 1 ±\pm1.2
Lepton uncertainties ±\pm2.6 ±\pm2.6 ±\pm2.6 ±\pm2.6 ±\pm2.6
PDF ±\pm3.0 ±\pm1.8 ±\pm2.3 ±\pm2.8 ±\pm2.4
tqtq generator + parton shower ±\pm6.8 ±\pm8.2 \mp7.9 \mp12 +9.2/9.7+9.2/-9.7
tqtq scale variation ±\pm2.8 << 1 ±\pm3.7 << 1 +6.0/6.4+6.0/-6.4
Unfolding ±\pm1.3 ±\pm1.4 << 1 << 1 << 1
Luminosity ±\pm1.8 ±\pm1.8 ±\pm1.8 ±\pm1.8 ±\pm1.8
Total systematic ±\pm13 ±\pm14 ±\pm13 ±\pm16 ±\pm19
Total ±\pm15 ±\pm16 ±\pm15 ±\pm20 ±\pm25
Table 10: Detailed list of the contribution of each source of uncertainty to the total relative uncertainty on the measured dσdpT(t¯)\frac{d\sigma}{dp_{\mathrm{T}}(\bar{t})} distribution given in percent for each bin. The list includes only those uncertainties that contribute with more than 1%. The following uncertainties contribute to the total uncertainty with less than 1% to each bin content: JES detector, JES statistical, JES physics modeling, JES mixed detector and modeling, JES close-by jets, JES pile-up, JES flavor composition, JES flavor response, bb-JES, jet vertex fraction, mistag efficiency, b/b¯b/\bar{b} acceptance, ETmissE_{\mathrm{T}}^{\mathrm{miss}} modeling, WW+jets shape variation, and tt¯t\bar{t} generator. The contents of this table are provided in machine-readable format in the Supplemental Material sup.
dσdpT(t¯)\frac{d\sigma}{dp_{\mathrm{T}}(\bar{t})} pT(t¯)p_{\mathrm{T}}(\bar{t}) bins [GeV]
Source [0,45][0,45] [45,75][45,75] [75,110][75,110] [110,150][110,150] [150,500][150,500]
Data statistical ±\pm12 ±\pm8.2 ±\pm13 ±\pm26 ±\pm26
Monte Carlo statistical ±\pm12 ±\pm9.1 ±\pm14 ±\pm28 ±\pm28
Background normalization ±\pm14 ±\pm11 ±\pm16 ±\pm48 ±\pm33
JES η\eta intercalibration 9.0/+8.7-9.0/+8.7 +1.9/3.7+1.9/-3.7 +4.9/1.3+4.9/-1.3 +15/13+15/-13 << 1
Jet energy resolution ±\pm1.0 ±\pm2.2 ±\pm3.4 << 1 ±\pm3.0
bb-tagging efficiency ±\pm3.0 ±\pm3.1 ±\pm3.2 ±\pm3.6 ±\pm5.9
cc-tagging efficiency ±\pm5.6 ±\pm2.0 ±\pm2.2 ±\pm10 ±\pm5.9
Lepton uncertainties ±\pm2.6 ±\pm2.6 ±\pm2.6 ±\pm2.6 ±\pm2.7
PDF ±\pm3.8 ±\pm4.3 ±\pm5.3 ±\pm7.2 ±\pm8.2
tqtq generator + parton shower ±\pm12.2 << 1 \mp9.6 ±\pm11 << 1
tqtq scale variation ±\pm3.1 << 1 ±\pm3.2 ±\pm1.9 ±\pm5.9
Unfolding << 1 << 1 << 1 ±\pm6.9 ±\pm2.6
Luminosity ±\pm1.8 ±\pm1.8 ±\pm1.8 ±\pm1.8 ±\pm1.8
Total systematic ±\pm25 ±\pm17 ±\pm24 ±\pm70 ±\pm53
Total ±\pm27 ±\pm18 ±\pm27 ±\pm74 ±\pm59
Table 11: Detailed list of the contribution of each source of uncertainty to the total relative uncertainty on the measured dσd|y(t)|\frac{d\sigma}{d|y(t)|} distribution given in percent for each bin. The list includes only those uncertainties that contribute with more than 1%. The following uncertainties contribute to the total uncertainty with less than 1% to each bin content: JES detector, JES statistical, JES physics modeling, JES mixed detector and modeling, JES close-by jets, JES pile-up, JES flavor composition, JES flavor response, jet vertex fraction, b/b¯b/\bar{b} acceptance, ETmissE_{\mathrm{T}}^{\mathrm{miss}} modeling, WW+jets shape variation, tt¯t\bar{t} generator, tt¯t\bar{t} ISR/FSR, and unfolding. The contents of this table are provided in machine-readable format in the Supplemental Material sup.
dσd|y(t)|\frac{d\sigma}{d|y(t)|} |y(t)||y(t)| bins
Source [0,0.2][0,0.2] [0.2,0.6][0.2,0.6] [0.6,1.1][0.6,1.1] [1.1,3.0][1.1,3.0]
Data statistical ±\pm9.0 ±\pm6.3 ±\pm7.5 ±\pm7.1
Monte Carlo statistical ±\pm5.9 ±\pm4.8 ±\pm5.0 ±\pm4.4
Background normalization ±\pm5.3 ±\pm6.5 ±\pm6.7 ±\pm4.7
JES η\eta intercalibration +1.7/0.6+1.7/-0.6 << 1 +1.7/0.4+1.7/-0.4 << 1
b-JES +1.1/1.7+1.1/-1.7 << 1 +1.1/+0.2+1.1/+0.2 << 1
Jet energy resolution ±\pm3.2 ±\pm1.7 << 1 ±\pm3.1
bb-tagging efficiency ±\pm3.3 ±\pm3.4 ±\pm3.4 ±\pm3.2
cc-tagging efficiency ±\pm1.3 ±\pm1.2 ±\pm1.2 ±\pm1.0
Mistag efficiency << 1 ±\pm1.3 ±\pm2.0 ±\pm1.4
Lepton uncertainties ±\pm2.6 ±\pm2.7 ±\pm2.6 ±\pm2.5
PDF ±\pm3.6 ±\pm3.6 ±\pm2.8 ±\pm2.8
tqtq generator + parton shower \mp5.7 ±\pm0.8 ±\pm4.0 ±\pm8.7
tqtq scale variation ±\pm3.5 << 1 ±\pm2.6 ±\pm4.7
Luminosity ±\pm1.8 ±\pm1.8 ±\pm1.8 ±\pm1.8
Total systematic ±\pm12 ±\pm10 ±\pm11 ±\pm14
Total ±\pm15 ±\pm12 ±\pm14 ±\pm15
Table 12: Detailed list of the contribution of each source of uncertainty to the total relative uncertainty on the measured dσd|y(t¯)|\frac{d\sigma}{d|y(\bar{t})|} distribution given in percent for each bin. The list includes only those uncertainties that contribute with more than 1%. The following uncertainties contribute to the total uncertainty with less than 1% to each bin content: JES detector, JES statistical, JES physics modeling, JES mixed detector and modeling, JES close-by jets, JES pile-up, JES flavor composition, JES flavor response, bb-JES, jet vertex fraction, b/b¯b/\bar{b} acceptance, mistag efficiency, ETmissE_{\mathrm{T}}^{\mathrm{miss}} modeling, WW+jets shape variation, tt¯t\bar{t} generator, tt¯t\bar{t} ISR/FSR, and unfolding. The contents of this table are provided in machine-readable format in the Supplemental Material sup.
dσd|y(t¯)|\frac{d\sigma}{d|y(\bar{t})|} |y(t¯)||y(\bar{t})| bins
Source [0,0.2][0,0.2] [0.2,0.6][0.2,0.6] [0.6,1.1][0.6,1.1] [1.1,3.0][1.1,3.0]
Data statistical ±\pm13 ±\pm9.5 ±\pm11 ±\pm13
Monte Carlo statistical ±\pm11 ±\pm12 ±\pm11 ±\pm17
Background normalization ±\pm11 ±\pm16 ±\pm13 ±\pm15
JES η\eta intercalibration << 1 +1.0/1.8+1.0/-1.8 << 1 +2.3/0.9+2.3/-0.9
Jet energy resolution ±\pm2.3 ±\pm2.2 ±\pm1.0 ±\pm3.2
bb-tagging efficiency ±\pm3.4 ±\pm3.3 ±\pm3.2 ±\pm3.2
cc-tagging efficiency ±\pm2.5 ±\pm3.6 ±\pm2.9 ±\pm4.0
Lepton uncertainties ±\pm2.7 ±\pm2.7 ±\pm2.6 ±\pm2.4
PDF ±\pm6.0 ±\pm5.3 ±\pm4.4 ±\pm4.1
tqtq generator + parton shower ±\pm1.0 \mp5.6 ±\pm6.6 ±\pm6.2
tqtq scale variation ±\pm2.1 ±\pm2.6 ±\pm1.6 ±\pm4.3
Luminosity ±\pm1.8 ±\pm1.8 ±\pm1.8 ±\pm1.8
Total systematic ±\pm18 ±\pm23 ±\pm20 ±\pm25
Total ±\pm23 ±\pm25 ±\pm23 ±\pm29
Table 13: Detailed list of the contribution of each source of uncertainty to the total relative uncertainty on the measured 1σdσdpT(t)\frac{1}{\sigma}\frac{d\sigma}{dp_{\mathrm{T}}(t)} distribution given in percent for each bin. The list includes only those uncertainties that contribute with more than 1%. The JES η\eta intercalibration uncertainty has a sign switch from the first to the second bin. For the tqtq generator + parton shower uncertainty a sign switch is denoted with \mp. The following uncertainties contribute to the total uncertainty with less than 1% to each bin content: JES detector, JES statistical, JES physics modeling, JES mixed detector and modeling, JES close-by jets, JES pile-up, JES flavor composition, JES flavor response, bb-JES, jet vertex fraction, b/b¯b/\bar{b} acceptance, cc-tagging efficiency, ETmissE_{\mathrm{T}}^{\mathrm{miss}} modeling, lepton uncertainties, WW+jets shape variation, and tt¯t\bar{t} generator. The contents of this table are provided in machine-readable format in the Supplemental Material sup.
1σdσdpT(t)\frac{1}{\sigma}\frac{d\sigma}{dp_{\mathrm{T}}(t)} pT(t)p_{\mathrm{T}}(t) bins [GeV]
Source [0,45][0,45] [45,75][45,75] [75,110][75,110] [110,150][110,150] [150,500][150,500]
Data statistical ±\pm5.3 ±\pm6.9 ±\pm8.0 ±\pm11 ±\pm15
Monte Carlo statistical ±\pm4.2 ±\pm5.5 ±\pm5.2 ±\pm6.2 ±\pm9.3
Background normalization << 1 ±\pm1.7 << 1 ±\pm3.0 << 1
JES η\eta intercalibration 4.7/+1.5-4.7/+1.5 +3.5/2.3+3.5/-2.3 +4.1/0.8+4.1/-0.8 << 1 +9.6/3.1+9.6/-3.1
Jet energy resolution << 1 << 1 << 1 \mp1.4 ±\pm2.7
bb-tagging efficiency << 1 << 1 << 1 << 1 ±\pm2.8
Mistag efficiency << 1 << 1 << 1 ±\pm1.0 << 1
tqtq generator + parton shower ±\pm3.9 ±\pm5.4 \mp11 \mp14 ±\pm6.9
tqtq scale variation << 1 \mp1.8 ±\pm1.3 \mp2.7 +4.4/5.1+4.4/-5.1
Unfolding << 1 ±\pm1.7 << 1 << 1 ±\pm1.1
Total systematic +6.5/-7.7 ±\pm8.8 ±\pm13 ±\pm18 ±\pm16
Total +8.4/-9.4 ±\pm11 ±\pm15 ±\pm21 ±\pm22
Table 14: Detailed list of the contribution of each source of uncertainty to the total relative uncertainty on the measured 1σdσdpT(t¯)\frac{1}{\sigma}\frac{d\sigma}{dp_{\mathrm{T}}(\bar{t})} distribution given in percent for each bin. The list includes only those uncertainties that contribute with more than 1%. Sign switches within one uncertainty are denoted with \mp and ±\pm. The following uncertainties contribute to the total uncertainty with less than 1% to each bin content: JES detector, JES statistical, JES physics modeling, JES mixed detector and modeling, JES close-by jets, JES pile-up, JES flavor composition, JES flavor response, bb-JES, jet vertex fraction, b/b¯b/\bar{b} acceptance, mistag efficiency, ETmissE_{\mathrm{T}}^{\mathrm{miss}} modeling, lepton uncertainties, WW+jets shape variation, and tt¯t\bar{t} generator. The contents of this table are provided in machine-readable format in the Supplemental Material sup.
1σdσdpT(t¯)\frac{1}{\sigma}\frac{d\sigma}{dp_{\mathrm{T}}(\bar{t})} pT(t¯)p_{\mathrm{T}}(\bar{t}) bins [GeV]
Source [0,45][0,45] [45,75][45,75] [75,110][75,110] [110,150][110,150] [150,500][150,500]
Data statistical ±\pm8.2 ±\pm8.8 ±\pm13 ±\pm26 ±\pm26
Monte Carlo statistical ±\pm8.7 ±\pm9.6 ±\pm14 ±\pm28 ±\pm27
Background normalization << 1 ±\pm4.5 ±\pm1.8 ±\pm39 ±\pm22
JES η\eta intercalibration 7.5/+6.7-7.5/+6.7 +3.8/5.3+3.8/-5.3 +6.9/3.1+6.9/-3.1 +17/9.9+17/-9.9 << 1
Jet energy resolution << 1 << 1 \mp1.6 ±\pm1.8 \mp1.2
bb-tagging efficiency << 1 << 1 << 1 << 1 +2.4/2.8+2.4/-2.8
cc-tagging efficiency \mp1.8 ±\pm2.0 ±\pm1.7 6.2/+5.9-6.2/+5.9 \mp2.0
PDF << 1 << 1 << 1 ±\pm2.5 ±\pm3.6
tqtq generator + parton shower +7.7/8.2+7.7/-8.2 3.6/+3.7-3.6/+3.7 13/+14-13/+14 +6.4/7.0+6.4/-7.0 4.2/+4.5-4.2/+4.5
tqtq scale variation ±\pm 1.3 \mp 3.0 ±\pm 1.4 \mp 1.8 ±\pm 5.1
Unfolding << 1 << 1 << 1 ±\pm6.7 ±\pm2.8
Total systematic ±\pm15 ±\pm13 ±\pm21 +62/56+62/-56 ±\pm45
Total ±\pm17 ±\pm15 ±\pm25 +67/61+67/-61 ±\pm52
Table 15: Detailed list of the contribution of each source of uncertainty to the total relative uncertainty on the measured 1σdσd|y(t)|\frac{1}{\sigma}\frac{d\sigma}{d|y(t)|} distribution given in percent for each bin. The list includes only those uncertainties that contribute with more than 1%. Sign switches within one uncertainty are denoted with \mp and ±\pm. The following uncertainties contribute to the total uncertainty with less than 1% to each bin content: JES detector, JES statistical, JES physics modeling, JES mixed detector and modeling, JES close-by jets, JES pile-up, JES flavor composition, JES flavor response, bb-JES, jet vertex fraction, b/b¯b/\bar{b} acceptance, bb-tagging efficiency, cc-tagging efficiency, mistag efficiency, ETmissE_{\mathrm{T}}^{\mathrm{miss}} modeling, lepton uncertainties, WW+jets shape variation, tt¯t\bar{t} generator, tt¯t\bar{t} ISR/FSR, and unfolding. The contents of this table are provided in machine-readable format in the Supplemental Material sup.
1σdσd|y(t)|\frac{1}{\sigma}\frac{d\sigma}{d|y(t)|} |y(t)||y(t)| bins
Source [0,0.2][0,0.2] [0.2,0.6][0.2,0.6] [0.6,1.1][0.6,1.1] [1.1,3.0][1.1,3.0]
Data statistical ±\pm9.0 ±\pm6.4 ±\pm7.5 ±\pm5.0
Monte Carlo statistical ±\pm5.9 ±\pm4.8 ±\pm4.9 ±\pm3.2
Background normalization << 1 << 1 ±\pm1.1 ±\pm1.0
JES η\eta intercalibration +1.6/1.5+1.6/-1.5 0.5/+2.3-0.5/+2.3 +1.4/1.5+1.4/-1.5 << 1
Jet energy resolution ±\pm1.2 << 1 \mp1.6 ±\pm1.0
PDF ±\pm1.7 ±\pm1.8 << 1 ±\pm2.3
tqtq generator + parton shower 9.0/+9.8-9.0/+9.8 2.8/+3.0-2.8/+3.0 << 1 +4.8/5.2+4.8/-5.2
tqtq scale variation << 1 << 1 << 1 ±\pm1.5
Total systematic ±\pm11 ±\pm6.3 ±\pm6.2 ±\pm6.9
Total ±\pm15 ±\pm9.0 ±\pm9.7 ±\pm8.5
Table 16: Detailed list of the contribution of each source of uncertainty to the total relative uncertainty on the measured 1σdσd|y(t¯)|\frac{1}{\sigma}\frac{d\sigma}{d|y(\bar{t})|} distribution given in percent for each bin. The list includes only those uncertainties that contribute with more than 1%. Sign switches within one uncertainty are denoted with \mp and ±\pm. The following uncertainties contribute to the total uncertainty with less than 1% to each bin content: JES detector, JES statistical, JES physics modeling, JES mixed detector and modeling, JES close-by jets, JES pile-up, JES flavor composition, JES flavor response, bb-JES, jet energy resolution, jet vertex fraction, b/b¯b/\bar{b} acceptance, bb-tagging efficiency, cc-tagging efficiency, mistag efficiency, ETmissE_{\mathrm{T}}^{\mathrm{miss}} modeling, lepton uncertainties, WW+jets shape variation, tt¯t\bar{t} generator, tt¯t\bar{t} ISR/FSR, and unfolding. The contents of this table are provided in machine-readable format in the Supplemental Material sup.
1σdσd|y(t¯)|\frac{1}{\sigma}\frac{d\sigma}{d|y(\bar{t})|} |y(t¯)||y(\bar{t})| bins
Source [0,0.2][0,0.2] [0.2,0.6][0.2,0.6] [0.6,1.1][0.6,1.1] [1.1,3.0][1.1,3.0]
Data statistical ±\pm13 ±\pm9.1 ±\pm11 ±\pm11
Monte Carlo statistical ±\pm12 ±\pm11 ±\pm12 ±\pm14
Background normalization ±\pm3.4 ±\pm2.4 ±\pm1.1 << 1
JES η\eta intercalibration << 1 +0.5/1.9+0.5/-1.9 << 1 +1.5/0.8+1.5/-0.8
PDF ±\pm1.6 ±\pm1.0 << 1 ±\pm1.8
tqtq generator + parton shower \mp1.4 7.8/+8.2-7.8/+8.2 +4.0/4.3+4.0/-4.3 +3.8/3.9+3.8/-3.9
tqtq scale variation ±\pm1.9 << 1 << 1 << 1
Total systematic ±\pm13 ±\pm14 ±\pm13 ±\pm15
Total ±\pm19 ±\pm17 ±\pm17 ±\pm18
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Figure 17: Statistical correlation matrices for the differential cross section as a function of 17 pT(t)p_{\mathrm{T}}(t), 17 pT(t¯)p_{\mathrm{T}}(\bar{t}), 17 |y(t)||y(t)| and 17 |y(t¯)||y(\bar{t})|. The contents of this figure are provided in machine-readable format in the Supplemental Material sup.
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Figure 18: Statistical correlation matrices for the normalized differential cross section as a function of 18 pT(t)p_{\mathrm{T}}(t), 18 pT(t¯)p_{\mathrm{T}}(\bar{t}), 18 |y(t)||y(t)| and 18 |y(t¯)||y(\bar{t})|. The contents of this figure are provided in machine-readable format in the Supplemental Material sup.

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M. Wu55, S.L. Wu174, X. Wu49, Y. Wu88, E. Wulf35, T.R. Wyatt83, B.M. Wynne46, S. Xella36, M. Xiao137, D. Xu33a, L. Xu33b,al, B. Yabsley151, S. Yacoob146b,am, R. Yakabe66, M. Yamada65, H. Yamaguchi156, Y. Yamaguchi117, A. Yamamoto65, K. Yamamoto63, S. Yamamoto156, T. Yamamura156, T. Yamanaka156, K. Yamauchi102, Y. Yamazaki66, Z. Yan22, H. Yang33e, H. Yang174, U.K. Yang83, Y. Yang110, S. Yanush92, L. Yao33a, W-M. Yao15, Y. Yasu65, E. Yatsenko42, K.H. Yau Wong21, J. Ye40, S. Ye25, A.L. Yen57, E. Yildirim42, M. Yilmaz4b, R. Yoosoofmiya124, K. Yorita172, R. Yoshida6, K. Yoshihara156, C. Young144, C.J.S. Young30, S. Youssef22, D.R. Yu15, J. Yu8, J.M. Yu88, J. Yu113, L. Yuan66, A. Yurkewicz107, I. Yusuff28,an, B. Zabinski39, R. Zaidan62, A.M. Zaitsev129,aa, A. Zaman149, S. Zambito23, L. Zanello133a,133b, D. Zanzi100, C. Zeitnitz176, M. Zeman127, A. Zemla38a, K. Zengel23, O. Zenin129, T. Ženiš145a, D. Zerwas116, G. Zevi della Porta57, D. Zhang88, F. Zhang174, H. Zhang89, J. Zhang6, L. Zhang152, X. Zhang33d, Z. Zhang116, Z. Zhao33b, A. Zhemchugov64, J. Zhong119, B. Zhou88, L. Zhou35, N. Zhou164, C.G. Zhu33d, H. Zhu33a, J. Zhu88, Y. Zhu33b, X. Zhuang33a, K. Zhukov95, A. Zibell175, D. Zieminska60, N.I. Zimine64, C. Zimmermann82, R. Zimmermann21, S. Zimmermann21, S. Zimmermann48, Z. Zinonos54, M. Ziolkowski142, G. Zobernig174, A. Zoccoli20a,20b, M. zur Nedden16, G. Zurzolo103a,103b, V. Zutshi107, L. Zwalinski30.

1 Department of Physics, University of Adelaide, Adelaide, Australia

2 Physics Department, SUNY Albany, Albany NY, United States of America

3 Department of Physics, University of Alberta, Edmonton AB, Canada

4 (a) Department of Physics, Ankara University, Ankara; (b) Department of Physics, Gazi University, Ankara; (c) Division of Physics, TOBB University of Economics and Technology, Ankara; (d) Turkish Atomic Energy Authority, Ankara, Turkey

5 LAPP, CNRS/IN2P3 and Université de Savoie, Annecy-le-Vieux, France

6 High Energy Physics Division, Argonne National Laboratory, Argonne IL, United States of America

7 Department of Physics, University of Arizona, Tucson AZ, United States of America

8 Department of Physics, The University of Texas at Arlington, Arlington TX, United States of America

9 Physics Department, University of Athens, Athens, Greece

10 Physics Department, National Technical University of Athens, Zografou, Greece

11 Institute of Physics, Azerbaijan Academy of Sciences, Baku, Azerbaijan

12 Institut de Física d’Altes Energies and Departament de Física de la Universitat Autònoma de Barcelona, Barcelona, Spain

13 (a) Institute of Physics, University of Belgrade, Belgrade; (b) Vinca Institute of Nuclear Sciences, University of Belgrade, Belgrade, Serbia

14 Department for Physics and Technology, University of Bergen, Bergen, Norway

15 Physics Division, Lawrence Berkeley National Laboratory and University of California, Berkeley CA, United States of America

16 Department of Physics, Humboldt University, Berlin, Germany

17 Albert Einstein Center for Fundamental Physics and Laboratory for High Energy Physics, University of Bern, Bern, Switzerland

18 School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom

19 (a) Department of Physics, Bogazici University, Istanbul; (b) Department of Physics, Dogus University, Istanbul; (c) Department of Physics Engineering, Gaziantep University, Gaziantep, Turkey

20 (a) INFN Sezione di Bologna; (b) Dipartimento di Fisica e Astronomia, Università di Bologna, Bologna, Italy

21 Physikalisches Institut, University of Bonn, Bonn, Germany

22 Department of Physics, Boston University, Boston MA, United States of America

23 Department of Physics, Brandeis University, Waltham MA, United States of America

24 (a) Universidade Federal do Rio De Janeiro COPPE/EE/IF, Rio de Janeiro; (b) Federal University of Juiz de Fora (UFJF), Juiz de Fora; (c) Federal University of Sao Joao del Rei (UFSJ), Sao Joao del Rei; (d) Instituto de Fisica, Universidade de Sao Paulo, Sao Paulo, Brazil

25 Physics Department, Brookhaven National Laboratory, Upton NY, United States of America

26 (a) National Institute of Physics and Nuclear Engineering, Bucharest; (b) National Institute for Research and Development of Isotopic and Molecular Technologies, Physics Department, Cluj Napoca; (c) University Politehnica Bucharest, Bucharest; (d) West University in Timisoara, Timisoara, Romania

27 Departamento de Física, Universidad de Buenos Aires, Buenos Aires, Argentina

28 Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom

29 Department of Physics, Carleton University, Ottawa ON, Canada

30 CERN, Geneva, Switzerland

31 Enrico Fermi Institute, University of Chicago, Chicago IL, United States of America

32 (a) Departamento de Física, Pontificia Universidad Católica de Chile, Santiago; (b) Departamento de Física, Universidad Técnica Federico Santa María, Valparaíso, Chile

33 (a) Institute of High Energy Physics, Chinese Academy of Sciences, Beijing; (b) Department of Modern Physics, University of Science and Technology of China, Anhui; (c) Department of Physics, Nanjing University, Jiangsu; (d) School of Physics, Shandong University, Shandong; (e) Physics Department, Shanghai Jiao Tong University, Shanghai, China

34 Laboratoire de Physique Corpusculaire, Clermont Université and Université Blaise Pascal and CNRS/IN2P3, Clermont-Ferrand, France

35 Nevis Laboratory, Columbia University, Irvington NY, United States of America

36 Niels Bohr Institute, University of Copenhagen, Kobenhavn, Denmark

37 (a) INFN Gruppo Collegato di Cosenza, Laboratori Nazionali di Frascati; (b) Dipartimento di Fisica, Università della Calabria, Rende, Italy

38 (a) AGH University of Science and Technology, Faculty of Physics and Applied Computer Science, Krakow; (b) Marian Smoluchowski Institute of Physics, Jagiellonian University, Krakow, Poland

39 The Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, Krakow, Poland

40 Physics Department, Southern Methodist University, Dallas TX, United States of America

41 Physics Department, University of Texas at Dallas, Richardson TX, United States of America

42 DESY, Hamburg and Zeuthen, Germany

43 Institut für Experimentelle Physik IV, Technische Universität Dortmund, Dortmund, Germany

44 Institut für Kern- und Teilchenphysik, Technische Universität Dresden, Dresden, Germany

45 Department of Physics, Duke University, Durham NC, United States of America

46 SUPA - School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom

47 INFN Laboratori Nazionali di Frascati, Frascati, Italy

48 Fakultät für Mathematik und Physik, Albert-Ludwigs-Universität, Freiburg, Germany

49 Section de Physique, Université de Genève, Geneva, Switzerland

50 (a) INFN Sezione di Genova; (b) Dipartimento di Fisica, Università di Genova, Genova, Italy

51 (a) E. Andronikashvili Institute of Physics, Iv. Javakhishvili Tbilisi State University, Tbilisi; (b) High Energy Physics Institute, Tbilisi State University, Tbilisi, Georgia

52 II Physikalisches Institut, Justus-Liebig-Universität Giessen, Giessen, Germany

53 SUPA - School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom

54 II Physikalisches Institut, Georg-August-Universität, Göttingen, Germany

55 Laboratoire de Physique Subatomique et de Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France

56 Department of Physics, Hampton University, Hampton VA, United States of America

57 Laboratory for Particle Physics and Cosmology, Harvard University, Cambridge MA, United States of America

58 (a) Kirchhoff-Institut für Physik, Ruprecht-Karls-Universität Heidelberg, Heidelberg; (b) Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg; (c) ZITI Institut für technische Informatik, Ruprecht-Karls-Universität Heidelberg, Mannheim, Germany

59 Faculty of Applied Information Science, Hiroshima Institute of Technology, Hiroshima, Japan

60 Department of Physics, Indiana University, Bloomington IN, United States of America

61 Institut für Astro- und Teilchenphysik, Leopold-Franzens-Universität, Innsbruck, Austria

62 University of Iowa, Iowa City IA, United States of America

63 Department of Physics and Astronomy, Iowa State University, Ames IA, United States of America

64 Joint Institute for Nuclear Research, JINR Dubna, Dubna, Russia

65 KEK, High Energy Accelerator Research Organization, Tsukuba, Japan

66 Graduate School of Science, Kobe University, Kobe, Japan

67 Faculty of Science, Kyoto University, Kyoto, Japan

68 Kyoto University of Education, Kyoto, Japan

69 Department of Physics, Kyushu University, Fukuoka, Japan

70 Instituto de Física La Plata, Universidad Nacional de La Plata and CONICET, La Plata, Argentina

71 Physics Department, Lancaster University, Lancaster, United Kingdom

72 (a) INFN Sezione di Lecce; (b) Dipartimento di Matematica e Fisica, Università del Salento, Lecce, Italy

73 Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom

74 Department of Physics, Jožef Stefan Institute and University of Ljubljana, Ljubljana, Slovenia

75 School of Physics and Astronomy, Queen Mary University of London, London, United Kingdom

76 Department of Physics, Royal Holloway University of London, Surrey, United Kingdom

77 Department of Physics and Astronomy, University College London, London, United Kingdom

78 Louisiana Tech University, Ruston LA, United States of America

79 Laboratoire de Physique Nucléaire et de Hautes Energies, UPMC and Université Paris-Diderot and CNRS/IN2P3, Paris, France

80 Fysiska institutionen, Lunds universitet, Lund, Sweden

81 Departamento de Fisica Teorica C-15, Universidad Autonoma de Madrid, Madrid, Spain

82 Institut für Physik, Universität Mainz, Mainz, Germany

83 School of Physics and Astronomy, University of Manchester, Manchester, United Kingdom

84 CPPM, Aix-Marseille Université and CNRS/IN2P3, Marseille, France

85 Department of Physics, University of Massachusetts, Amherst MA, United States of America

86 Department of Physics, McGill University, Montreal QC, Canada

87 School of Physics, University of Melbourne, Victoria, Australia

88 Department of Physics, The University of Michigan, Ann Arbor MI, United States of America

89 Department of Physics and Astronomy, Michigan State University, East Lansing MI, United States of America

90 (a) INFN Sezione di Milano; (b) Dipartimento di Fisica, Università di Milano, Milano, Italy

91 B.I. Stepanov Institute of Physics, National Academy of Sciences of Belarus, Minsk, Republic of Belarus

92 National Scientific and Educational Centre for Particle and High Energy Physics, Minsk, Republic of Belarus

93 Department of Physics, Massachusetts Institute of Technology, Cambridge MA, United States of America

94 Group of Particle Physics, University of Montreal, Montreal QC, Canada

95 P.N. Lebedev Institute of Physics, Academy of Sciences, Moscow, Russia

96 Institute for Theoretical and Experimental Physics (ITEP), Moscow, Russia

97 Moscow Engineering and Physics Institute (MEPhI), Moscow, Russia

98 D.V.Skobeltsyn Institute of Nuclear Physics, M.V.Lomonosov Moscow State University, Moscow, Russia

99 Fakultät für Physik, Ludwig-Maximilians-Universität München, München, Germany

100 Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), München, Germany

101 Nagasaki Institute of Applied Science, Nagasaki, Japan

102 Graduate School of Science and Kobayashi-Maskawa Institute, Nagoya University, Nagoya, Japan

103 (a) INFN Sezione di Napoli; (b) Dipartimento di Fisica, Università di Napoli, Napoli, Italy

104 Department of Physics and Astronomy, University of New Mexico, Albuquerque NM, United States of America

105 Institute for Mathematics, Astrophysics and Particle Physics, Radboud University Nijmegen/Nikhef, Nijmegen, Netherlands

106 Nikhef National Institute for Subatomic Physics and University of Amsterdam, Amsterdam, Netherlands

107 Department of Physics, Northern Illinois University, DeKalb IL, United States of America

108 Budker Institute of Nuclear Physics, SB RAS, Novosibirsk, Russia

109 Department of Physics, New York University, New York NY, United States of America

110 Ohio State University, Columbus OH, United States of America

111 Faculty of Science, Okayama University, Okayama, Japan

112 Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman OK, United States of America

113 Department of Physics, Oklahoma State University, Stillwater OK, United States of America

114 Palacký University, RCPTM, Olomouc, Czech Republic

115 Center for High Energy Physics, University of Oregon, Eugene OR, United States of America

116 LAL, Université Paris-Sud and CNRS/IN2P3, Orsay, France

117 Graduate School of Science, Osaka University, Osaka, Japan

118 Department of Physics, University of Oslo, Oslo, Norway

119 Department of Physics, Oxford University, Oxford, United Kingdom

120 (a) INFN Sezione di Pavia; (b) Dipartimento di Fisica, Università di Pavia, Pavia, Italy

121 Department of Physics, University of Pennsylvania, Philadelphia PA, United States of America

122 Petersburg Nuclear Physics Institute, Gatchina, Russia

123 (a) INFN Sezione di Pisa; (b) Dipartimento di Fisica E. Fermi, Università di Pisa, Pisa, Italy

124 Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh PA, United States of America

125 (a) Laboratorio de Instrumentacao e Fisica Experimental de Particulas - LIP, Lisboa; (b) Faculdade de Ciências, Universidade de Lisboa, Lisboa; (c) Department of Physics, University of Coimbra, Coimbra; (d) Centro de Física Nuclear da Universidade de Lisboa, Lisboa; (e) Departamento de Fisica, Universidade do Minho, Braga; (f) Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada (Spain); (g) Dep Fisica and CEFITEC of Faculdade de Ciencias e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal

126 Institute of Physics, Academy of Sciences of the Czech Republic, Praha, Czech Republic

127 Czech Technical University in Prague, Praha, Czech Republic

128 Faculty of Mathematics and Physics, Charles University in Prague, Praha, Czech Republic

129 State Research Center Institute for High Energy Physics, Protvino, Russia

130 Particle Physics Department, Rutherford Appleton Laboratory, Didcot, United Kingdom

131 Physics Department, University of Regina, Regina SK, Canada

132 Ritsumeikan University, Kusatsu, Shiga, Japan

133 (a) INFN Sezione di Roma; (b) Dipartimento di Fisica, Sapienza Università di Roma, Roma, Italy

134 (a) INFN Sezione di Roma Tor Vergata; (b) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy

135 (a) INFN Sezione di Roma Tre; (b) Dipartimento di Matematica e Fisica, Università Roma Tre, Roma, Italy

136 (a) Faculté des Sciences Ain Chock, Réseau Universitaire de Physique des Hautes Energies - Université Hassan II, Casablanca; (b) Centre National de l’Energie des Sciences Techniques Nucleaires, Rabat; (c) Faculté des Sciences Semlalia, Université Cadi Ayyad, LPHEA-Marrakech; (d) Faculté des Sciences, Université Mohamed Premier and LPTPM, Oujda; (e) Faculté des sciences, Université Mohammed V-Agdal, Rabat, Morocco

137 DSM/IRFU (Institut de Recherches sur les Lois Fondamentales de l’Univers), CEA Saclay (Commissariat à l’Energie Atomique et aux Energies Alternatives), Gif-sur-Yvette, France

138 Santa Cruz Institute for Particle Physics, University of California Santa Cruz, Santa Cruz CA, United States of America

139 Department of Physics, University of Washington, Seattle WA, United States of America

140 Department of Physics and Astronomy, University of Sheffield, Sheffield, United Kingdom

141 Department of Physics, Shinshu University, Nagano, Japan

142 Fachbereich Physik, Universität Siegen, Siegen, Germany

143 Department of Physics, Simon Fraser University, Burnaby BC, Canada

144 SLAC National Accelerator Laboratory, Stanford CA, United States of America

145 (a) Faculty of Mathematics, Physics & Informatics, Comenius University, Bratislava; (b) Department of Subnuclear Physics, Institute of Experimental Physics of the Slovak Academy of Sciences, Kosice, Slovak Republic

146 (a) Department of Physics, University of Cape Town, Cape Town; (b) Department of Physics, University of Johannesburg, Johannesburg; (c) School of Physics, University of the Witwatersrand, Johannesburg, South Africa

147 (a) Department of Physics, Stockholm University; (b) The Oskar Klein Centre, Stockholm, Sweden

148 Physics Department, Royal Institute of Technology, Stockholm, Sweden

149 Departments of Physics & Astronomy and Chemistry, Stony Brook University, Stony Brook NY, United States of America

150 Department of Physics and Astronomy, University of Sussex, Brighton, United Kingdom

151 School of Physics, University of Sydney, Sydney, Australia

152 Institute of Physics, Academia Sinica, Taipei, Taiwan

153 Department of Physics, Technion: Israel Institute of Technology, Haifa, Israel

154 Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel

155 Department of Physics, Aristotle University of Thessaloniki, Thessaloniki, Greece

156 International Center for Elementary Particle Physics and Department of Physics, The University of Tokyo, Tokyo, Japan

157 Graduate School of Science and Technology, Tokyo Metropolitan University, Tokyo, Japan

158 Department of Physics, Tokyo Institute of Technology, Tokyo, Japan

159 Department of Physics, University of Toronto, Toronto ON, Canada

160 (a) TRIUMF, Vancouver BC; (b) Department of Physics and Astronomy, York University, Toronto ON, Canada

161 Faculty of Pure and Applied Sciences, University of Tsukuba, Tsukuba, Japan

162 Department of Physics and Astronomy, Tufts University, Medford MA, United States of America

163 Centro de Investigaciones, Universidad Antonio Narino, Bogota, Colombia

164 Department of Physics and Astronomy, University of California Irvine, Irvine CA, United States of America

165 (a) INFN Gruppo Collegato di Udine, Sezione di Trieste, Udine; (b) ICTP, Trieste; (c) Dipartimento di Chimica, Fisica e Ambiente, Università di Udine, Udine, Italy

166 Department of Physics, University of Illinois, Urbana IL, United States of America

167 Department of Physics and Astronomy, University of Uppsala, Uppsala, Sweden

168 Instituto de Física Corpuscular (IFIC) and Departamento de Física Atómica, Molecular y Nuclear and Departamento de Ingeniería Electrónica and Instituto de Microelectrónica de Barcelona (IMB-CNM), University of Valencia and CSIC, Valencia, Spain

169 Department of Physics, University of British Columbia, Vancouver BC, Canada

170 Department of Physics and Astronomy, University of Victoria, Victoria BC, Canada

171 Department of Physics, University of Warwick, Coventry, United Kingdom

172 Waseda University, Tokyo, Japan

173 Department of Particle Physics, The Weizmann Institute of Science, Rehovot, Israel

174 Department of Physics, University of Wisconsin, Madison WI, United States of America

175 Fakultät für Physik und Astronomie, Julius-Maximilians-Universität, Würzburg, Germany

176 Fachbereich C Physik, Bergische Universität Wuppertal, Wuppertal, Germany

177 Department of Physics, Yale University, New Haven CT, United States of America

178 Yerevan Physics Institute, Yerevan, Armenia

179 Centre de Calcul de l’Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Villeurbanne, France

a Also at Department of Physics, King’s College London, London, United Kingdom

b Also at Institute of Physics, Azerbaijan Academy of Sciences, Baku, Azerbaijan

c Also at Particle Physics Department, Rutherford Appleton Laboratory, Didcot, United Kingdom

d Also at TRIUMF, Vancouver BC, Canada

e Also at Department of Physics, California State University, Fresno CA, United States of America

f Also at Tomsk State University, Tomsk, Russia

g Also at CPPM, Aix-Marseille Université and CNRS/IN2P3, Marseille, France

h Also at Università di Napoli Parthenope, Napoli, Italy

i Also at Institute of Particle Physics (IPP), Canada

j Also at Department of Physics, St. Petersburg State Polytechnical University, St. Petersburg, Russia

k Also at Chinese University of Hong Kong, China

l Also at Department of Financial and Management Engineering, University of the Aegean, Chios, Greece

m Also at Louisiana Tech University, Ruston LA, United States of America

n Also at Institucio Catalana de Recerca i Estudis Avancats, ICREA, Barcelona, Spain

o Also at Department of Physics, The University of Texas at Austin, Austin TX, United States of America

p Also at Institute of Theoretical Physics, Ilia State University, Tbilisi, Georgia

q Also at CERN, Geneva, Switzerland

r Also at Ochadai Academic Production, Ochanomizu University, Tokyo, Japan

s Also at Manhattan College, New York NY, United States of America

t Also at Novosibirsk State University, Novosibirsk, Russia

u Also at Institute of Physics, Academia Sinica, Taipei, Taiwan

v Also at LAL, Université Paris-Sud and CNRS/IN2P3, Orsay, France

w Also at Academia Sinica Grid Computing, Institute of Physics, Academia Sinica, Taipei, Taiwan

x Also at Laboratoire de Physique Nucléaire et de Hautes Energies, UPMC and Université Paris-Diderot and CNRS/IN2P3, Paris, France

y Also at School of Physical Sciences, National Institute of Science Education and Research, Bhubaneswar, India

z Also at Dipartimento di Fisica, Sapienza Università di Roma, Roma, Italy

aa Also at Moscow Institute of Physics and Technology State University, Dolgoprudny, Russia

ab Also at Section de Physique, Université de Genève, Geneva, Switzerland

ac Also at International School for Advanced Studies (SISSA), Trieste, Italy

ad Also at Department of Physics and Astronomy, University of South Carolina, Columbia SC, United States of America

ae Also at School of Physics and Engineering, Sun Yat-sen University, Guangzhou, China

af Also at Faculty of Physics, M.V.Lomonosov Moscow State University, Moscow, Russia

ag Also at Moscow Engineering and Physics Institute (MEPhI), Moscow, Russia

ah Also at Institute for Particle and Nuclear Physics, Wigner Research Centre for Physics, Budapest, Hungary

ai Also at Department of Physics, Oxford University, Oxford, United Kingdom

aj Also at Department of Physics, Nanjing University, Jiangsu, China

ak Also at Institut für Experimentalphysik, Universität Hamburg, Hamburg, Germany

al Also at Department of Physics, The University of Michigan, Ann Arbor MI, United States of America

am Also at Discipline of Physics, University of KwaZulu-Natal, Durban, South Africa

an Also at University of Malaya, Department of Physics, Kuala Lumpur, Malaysia

Deceased