Measurement of jet radial profiles in Pb$-$Pb collisions at $\sqrt{s_{\rm NN}}$ = 2.76 TeV
ALICE Collaboration
TL;DR
This study investigates how jet structures and particle compositions within jets are modified in Pb-Pb collisions at 2.76 TeV, revealing suppression and broadening effects indicative of in-medium energy loss.
Contribution
First measurement of jet radial profiles and particle distributions in Pb-Pb collisions down to 30 GeV/c jet transverse momentum, providing new insights into in-medium parton energy loss.
Findings
30-10% suppression of high-$p_T$ associated particles in Pb-Pb
Moderate modification of radial particle distribution
High-$p_T$ particles more collimated, low-$p_T$ particles broadened
Abstract
The jet radial structure and particle transverse momentum () composition within jets are presented in centrality-selected Pb-Pb collisions at = 2.76 TeV. Track-based jets, which are also called charged jets, were reconstructed with a resolution parameter of at midrapidity for transverse momenta p_\rm{T,\,ch\,jet}=30- GeV/. Jet-hadron correlations in relative azimuth and pseudorapidity space (, ) are measured to study the distribution of the associated particles around the jet axis for different p_\rm{T, assoc}-ranges between 1 and 20 GeV/. The data in Pb-Pb collisions are compared to reference distributions for pp collisions, obtained using embedded PYTHIA simulations. The number of high- associate particles (4<p_\rm{T, assoc}<20 GeV/) in Pb-Pb collisions is…
| -cut | 0.15 GeV/ | 3 GeV/ | |||
|---|---|---|---|---|---|
| (GeV/) | 40–60 | 60–80 | 80–120 | 30–40 | 40–60 |
| 0–5% | 11–87 (44) | 22–111 (64) | 49–144 (94) | 7–59 (32) | 21–88 (46) |
| 5–10% | 11–86 (46) | 24–112 (66) | 52–146 (94) | 8–61 (32) | 22–89 (46) |
| 0–10% | 11–86 (46) | 25–113 (68) | 54–147 (94) | 10–63 (32) | 24–91 (48) |
| 10–30% | 13–86 (50) | 33–117 (70) | 63–149 (98) | 15–69 (32) | 30–94 (48) |
| 30–50% | 25–91 (52) | 47–118 (82) | 75–147 (98) | 23–73 (32) | 36–95 (52) |
| (GeV/) | 4–20 | 1–2 | |||||
|---|---|---|---|---|---|---|---|
| (GeV/) | Observable | 40–60 | 60–80 | 80–120 | 30–40 | 40–60 | |
| Background (%) | Pb–Pb | 0.3–0.6 | 0.7–1.5 | 1.5–2.0 | 6.9 | 8.0 | |
| Embedded | 0.3–0.7 | 0.7–1.0 | 1.0–1.1 | 6.8 | 6.7 | ||
| Ratio | 0.4–0.7 | 0.1–0.7 | 0.4–1.6 | 6.9 | 9.6 | ||
| Mixed event correction (%) | Pb–Pb | 0.2 | 0.3 | 0.5 | 0.2 | 0.2 | |
| Embedded | 0.7 | 0.4 | 0.4 | 0.1 | 0.1 | ||
| Ratio | 0.7 | 0.5 | 0.3 | 0.2 | 0.2 | ||
| Embedding (%) | Pb–Pb | - | - | - | - | - | |
| Embedded | 0.1–2.3 | 0.1–0.4 | 0.1–0.3 | 5.0 | 2.7 | ||
| Ratio | 0.1–2.3 | 0.1–0.4 | 0.1–0.3 | 4.6 | 2.7 | ||
| Tracking efficiency (%) | Pb–Pb | 4.0 | 4.0 | 4.0 | 4.0 | 4.0 | |
| Embedded | 4.0 | 4.0 | 4.0 | 4.0 | 4.0 | ||
| Ratio | - | - | - | - | - | ||
| Tracking PYTHIA (%) | Pb–Pb | - | - | - | - | - | |
| Embedded | 2.0 | 2.0 | 2.0 | 2.0 | 2.0 | ||
| Ratio | 2.0 | 2.0 | 2.0 | 2.0 | 2.0 | ||
| PYTHIA vs. pp (%) | Pb–Pb | - | - | - | - | - | |
| Embedded | 5.0 | 5.0 | 5.0 | 2.0 | 2.0 | ||
| Ratio | 5.0 | 5.0 | 5.0 | 2.0 | 2.0 | ||
| Total (%) | Pb–Pb | 4.0–4.1 | 4.1–4.3 | 4.3–4.5 | 8.0 | 9.0 | |
| Embedded | 6.8–7.2 | 6.8 | 6.8 | 9.8 | 8.7 | ||
| Ratio | 5.5–5.9 | 5.4–5.5 | 5.4–5.6 | 8.8 | 10.3 | ||
| Data sample | Pb–Pb | Embedded PYTHIA | |||||
|---|---|---|---|---|---|---|---|
| (GeV/) | 40–60 | 60–80 | 80–120 | 40–60 | 60–80 | 80–120 | |
| Background (%) | 0.1–6.5 | 0.1–13.0 | 0.1–19.2 | 0.0–6.9 | 0.0–10.8 | 0.0–14.5 | |
| Mixed event corr. (%) | 0.1 | 0.1 | 0.1 | 0.1 | 0.1 | 0.1 | |
| Embedding (%) | - | - | - | 1.0–13.9 | 0.4–3.1 | 0.1–0.8 | |
| PYTHIA vs. pp (%) | - | - | - | 2.0 | 2.0 | 2.0 | |
| Total (%) | 0.1–6.5 | 0.1–13.0 | 0.1–19.2 | 2.2–15.7 | 2.0–11.5 | 2.0–14.6 | |
| Data sample | Pb–Pb | Embedded PYTHIA | |||
|---|---|---|---|---|---|
| (GeV/) | 1–2 | 2–3 | 1–2 | 2–3 | |
| Background (%) | 1.6–7.5 | 0.4–8.8 | 2.2–11.9 | 1.0–4.2 | |
| Mixed event corr. (%) | 0.1 | 0.1 | 0.1 | 0.1 | |
| Embedding (%) | - | - | 1.2–7.4 | 0.8–11.3 | |
| PYTHIA vs. pp (%) | - | - | 2.0–10.0 | 2.0–10.0 | |
| Total (%) | 1.6–7.5 | 0.4–8.8 | 6.2–13.0 | 4.5–15.7 | |
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\PHyear2019 \PHnumber079 \PHdate30 April \ShortTitleJet radial profiles in Pb–Pb collisions \CollaborationALICE Collaboration††thanks: See Appendix A for the list of collaboration members \ShortAuthorALICE Collaboration
The jet radial structure and particle transverse momentum () composition within jets are presented in centrality-selected Pb–Pb collisions at TeV. Track-based jets, which are also called charged jets, were reconstructed with a resolution parameter of at midrapidity for transverse momenta – GeV/. Jet–hadron correlations in relative azimuth and pseudorapidity space (, ) are measured to study the distribution of the associated particles around the jet axis for different -ranges between 1 and 20 GeV/. The data in Pb–Pb collisions are compared to reference distributions for pp collisions, obtained using embedded PYTHIA simulations. The number of high- associate particles ( GeV/) in Pb–Pb collisions is found to be suppressed compared to the reference by 30 to 10%, depending on centrality. The radial particle distribution relative to the jet axis shows a moderate modification in Pb–Pb collisions with respect to PYTHIA. High- associate particles are slightly more collimated in Pb–Pb collisions compared to the reference, while low- associate particle tend to be broadened. The results, which are presented for the first time down to GeV/ in Pb–Pb collisions, are compatible with both previous jet–hadron-related measurements from the CMS Collaboration and jet shape measurements from the ALICE Collaboration at higher , and add further support for the established picture of in-medium parton energy loss.
1 Introduction
At energy densities above approximately GeV/fm3 and temperatures above approximately MeV [1], Quantum Chromodynamics (QCD) calculations on the lattice predict the existence of a phase transition from normal nuclear matter to a new state of matter called the Quark–Gluon Plasma (QGP), where the partonic constituents, quarks and gluons, are no longer confined in hadrons. There is compelling evidence from observations reported by experiments at the Relativistic Heavy Ion Collider (RHIC) [2, 3, 4, 5] and at the Large Hadron Collider (LHC) [6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17] that the QGP is created in nuclear collisions at high collisions energies.
A unique way to characterize the properties of the QGP is to utilize jets as a probe of the medium. Hard scatterings are expected to occur early in the collision evolution, producing high transverse momentum () partons that propagate through the expanding medium and eventually fragment into jets of hadrons. High- partons lose energy in interactions with the medium due to elastic scattering and induced gluon radiation [18, 19]. Besides a reduction of the jet energy, this can result in a broadening of the transverse jet profile and a softening of the fragmentation [20].
Jet quenching has been observed at RHIC [21, 22, 23, 24, 25, 26, 27, 28, 29, 30, 31, 32, 33, 34] and at the LHC [16, 35, 17, 8, 36, 37, 38, 39, 40, 41, 42, 43, 44, 45, 46, 47], e.g. via inclusive yield and correlation measurements of high- hadrons and reconstructed jets. These measurements provide insights into the mechanisms of parton energy loss in the medium and eventually into the medium itself.
More differential measurements of the jet modification in a medium, i.e. measurements of modifications of jet angular profile and particle composition, can provide complementary information to observables that focus on the overall yield change like nuclear modification factors. Measurements of correlated associated particle production relative to jets or high- particles allow for a detailed measurement of the redistribution of quenched energy around the jet. An excess of low- particles in and around the jet up to large distances, as well as a suppression of high- particles, have been reported [17, 48, 49, 50]. Two-particle correlations and jet–hadron correlations show an angular broadening of low- particles below 3 GeV/ in heavy-ion collisions with respect to pp collisions [50]. For low- two-particle correlations, measurements also indicate an asymmetry in the shape of the near-side jet peaks: they are broader in compared to [48, 49]. The variables and are the distance in pseudorapidity and azimuth relative to the near-side jet. At the same time, measurements of the radial moment of jets point to a general collimation of jets in Pb–Pb collisions [51].
Using jets instead of high- particles as a reference (trigger) to study angular correlations—as done in this analysis—should have the advantage that jet properties better reflect the initial parton energy. This analysis extends the study of jet–hadron correlations into a regime of low track-based jet not yet explored with these techniques at the LHC.
In this paper, we study the correlation of charged particles (associates) with the direction of reconstructed track-based jets (triggers) in the - plane in the same event. The jets are reconstructed using charged particles above a certain transverse momentum . The analysis focuses on two aspects of the modification of jets within the medium created in Pb–Pb collisions compared to a PYTHIA [52] reference. First, the overall modification of the associated particle yield and its jet-energy dependence is studied. Second, the modification of the radial distribution of associated particles with respect to the jet axis is studied by comparing the Pb–Pb results to the PYTHIA reference. Both aspects are analyzed in detail for several jet transverse momenta and low and high of associated charged particles. PYTHIA is used as vacuum baseline, because the size of the pp dataset at TeV is insufficient for this analysis.
The paper is structured as follows. In Sec. 2, details on the detector and general data reconstruction will be given. The correlation analysis, which serves as basis for this paper, is presented in Sec. 3. Subsequently, jet reconstruction will be described in Sec. 4, followed by a discussion on the embedded PYTHIA reference in Sec. 5. Before the results will be presented in Sec. 8, the observables are introduced in Sec. 6 and systematic uncertainties are discussed in Sec. 7. A summary concludes the paper in Sec. 9.
2 Experimental setup
For a complete description of the ALICE detector and its performance see Refs. [53] and [54], respectively.
The data were recorded in 2011 for Pb–Pb collisions at TeV using a set of centrality triggers based on the hit multiplicity measured by the V0 detector, which consists of segmented scintillators covering the full azimuth over (V0A) and (V0C). Events were selected with V0 multiplicities corresponding to the [math]–% most central events using the centrality determination as described in LABEL:Abelev:2013qoq. The accepted events, reconstructed as described in LABEL:Abelev:2012hxa, were required to have a primary reconstructed vertex within cm of the center of the detector along the beam axis. For this analysis, a total of M events were used.
The analysis presented here relies mainly on the central ALICE tracking systems, which are located inside a large solenoidal magnet with a field strength of T. They consist of the Inner Tracking System (ITS), a high-precision six-layer cylindrical silicon detector system with the inner layer at a radius of cm and the outer layer at cm from the beam axis, and the Time Projection Chamber (TPC) with a radial extent of – cm, which provides up to 159 independent space points per track.
To ensure a good track-momentum resolution for jet reconstruction, all reconstructed tracks were required to have at least three hits in the ITS. For tracks without any hit in the Silicon Pixel Detector (SPD), which provides the two innermost layers of the ITS, the location of the primary vertex was used in addition to the hits in the TPC and ITS. This improves the track-momentum resolution and reduces the azimuthal dependence of the track reconstruction efficiency due to the non-uniform SPD response. Accepted tracks were required to be measured with GeV/ in , and to have at least 70 TPC space-points and no less than 80% of the geometrically findable space-points in the TPC.
The single-track tracking efficiency was estimated from the detector response of HIJING [57] events reconstructed to detector level using GEANT3 [58] for the particle transport. In the [math]–% centrality class, it is about 56% at GeV/, about % at GeV/ and then decreases to % at 3 GeV/, after which it increases and levels off to about % at above 6.5 GeV/. For the –% most central collisions, the tracking efficiency follows a similar -dependence pattern, with absolute values of the efficiency that are to % higher compared to the [math]–% most central collisions. The momentum resolution, which was estimated on a track-by-track basis using the covariance matrix of the track fit, is about at GeV/ and about % at GeV/. The contamination by secondary particles [59] produced in particle-material interactions, conversions, and weak-decay products of long-lived particles is on the level of few percent.
3 Correlation analysis
The two-dimensional associated per-trigger yield measures the distribution of particles relative to the jet axes in bins of , , event centrality, and trigger and associate transverse momenta [60]. This distribution serves as the basis of the analysis and is formed using so-called same and mixed event correlations. Correlations from the same event are the actual correlations of trigger jets and associated particles, calculated for each selected event. In the mixed event technique, jets are correlated with particles from a pool containing tracks from different events with similar trigger jet , vertex , and centralities. For vertex , there are six bins in this pool, whose boundaries are given by in cm. The boundaries for the centrality percentile binning are given by .
The mixed-event-corrected associated per-trigger yield for given jet -range, associate -range, and centrality selection is defined as
[TABLE]
where the ratios in the sum are formed differentially in bins of centrality and vertex .
The factor in Eq. 1 is chosen such that the mixed-event correlations are normalized to unity in the region , around the near-side jet peak where the efficiency for pairs of parallel jets and associates is largest. The contribution of the statistical uncertainty of this normalization to the total statistical uncertainty is negligible. The finite tracking efficiency and the contamination by secondaries (see Sec. 2) are taken into account and a correction has been performed for associated tracks differentially in , , centrality, and vertex for same and mixed event correlations in Eq. 1. The efficiency maps were created using Monte Carlo simulations for the same track definition and detector conditions. However, this correction turns out to be negligible for all observables except for the absolute jet-associated yields, because its effect mostly cancels in the used relative observables, which will be defined in Sec. 6.
In addition to the correction for detector inhomogenities and acceptance effects, the correlation also needs to be corrected for background. The underlying background for the chosen observables mainly consists of the uncorrelated particle background baseline from soft processes and the flow modulation in the correlation function. The background was found to be independent of within [61] and is therefore estimated as a function of for the whole -range as . To avoid including parts of the jet signal, is calculated in , where the contribution from the jet is expected to be small, based on measurements in pp collisions.
The background is directly subtracted from the correlation function. The background-corrected per-trigger yield serves as a basis for all subsequent measurements. It is defined as
[TABLE]
To illustrate the impact of the background on the per-trigger yields, the uncorrected per-trigger yields can be found in Fig. 1 for high- and low- associates. The background is nearly negligible for high- associates and it is sizeable for low- associates. In the illustrated example for low- associates, the signal to signal+background ratio, i.e. the percentage of the signal in the measured observable, is roughly 0.1 within a radius of around the near-side jet peak. Note also that the background correction removes all -independent correlations, including the away-side ridge which is not investigated in the presented analysis.
4 Jet reconstruction
The measurement of jets in heavy-ion collisions is challenging since a single event can contain multiple, possibly overlapping, jets from independent hard nucleon–nucleon scatterings. In addition, low transverse momentum particles originating from soft processes lead to a fluctuating background which strongly influences the jet reconstruction. The relative effect is largest for low- jets and most central events. Consequently, jet reconstruction in heavy-ion collisions requires a robust jet definition, and a procedure to correct for the presence of the large background [62].
Jets were reconstructed using the anti- or the algorithms [63] in the package [64] with a resolution parameter of . Only those jets whose axis was reconstructed within were kept in the analysis to assure the nominal jet cone is fully contained within the track acceptance of . This limits the effect of the acceptance boundaries on the measured jet spectrum. Jets reconstructed by the anti- algorithm were used to quantify signal jets, while jets reconstructed by the algorithm were used to quantify the contribution from the underlying event [65].
Two different jet definitions are used in this analysis: for measurements at high associate-, jets are measured with a constituent cut GeV/, measurements at low associate- are performed for jets measured with a constituent cut GeV/. Jets with GeV/ are reconstructed using all charged particles available for jet reconstruction and, thus, the fragmentation bias is as small as possible. This bias is caused by only including certain particles of the jet and could lead to a sample of harder fragmenting jets when leaving out particles at low . On the other hand, using all charged particles available for jet reconstruction also includes particles in the correlation analysis which were already used in the jet finding process. The jet finding algorithm selects regions in momentum space with large energy flow. This implies that the distribution of charged particles inside the jet is biased. For example, the radial distribution of particles with respect to the jet axis will show a small depletion at distances just outside the jet cone radius . This particularly affects the shape of the jet, i.e. how the constituents are distributed relative to the jet axis, leading to an autocorrelation bias.
Therefore, the jets themselves and in particular their shapes are intimately connected to the jet definition. For high- associates, the autocorrelation bias cannot be avoided and has to be accepted as a part of the jet definition.
Low- associates are broadly distributed up to large distances relative to the jet. Since the jet finding algorithm clusters the jets roughly into cones with a nominal radius of , it strongly affects the shape of the jet. When measuring properties of low- associates, we avoid the autocorrelation bias by adapting the jet definition: Trigger jets and associates can be decoupled by using jets with constituents above a certain threshold and associates below the threshold. Therefore, for measurements at low associate-, jets are reconstructed with GeV/. Using a geometrical matching procedure that is performed on two collections of the differently defined jets which are reconstructed in each event it was checked that the jet axes for both jet definitions do not strongly change. For instance, for jets with GeV/ and GeV/ the mean and standard deviation of the matched jet distance distribution are approximately given by and , respectively. However, it must be emphasized that these jet definitions select two different jet samples and that the autocorrelation bias was avoided here at the expense of a possible fragmentation bias.
The transverse momentum of reconstructed jets including constituents as low as GeV/ is affected by the contribution from the underlying event. In order to suppress the contribution of such background to the measurement of the jet momentum, we followed the approach described in Refs. [66, 65], which addresses the average additive contribution to the jet momentum on a jet-by-jet basis. The underlying background momentum density was estimated event-by-event using the median of , where is the uncorrected jet transverse momentum and is the area of jets reconstructed with the algorithm.
The average raw background momentum density decreases towards more peripheral collisions. It is , and GeV/ in the [math]–%, –%, and –% most central Pb–Pb collisions, respectively. The background momentum density is a detector-level quantity that depends on the tracking efficiency and track definition. For signal jets reconstructed with the anti- algorithm and constituents above GeV/, the background density scaled by the area of the reconstructed signal jet was subtracted from the raw reconstructed transverse momentum () of the signal jet according to .
Due to region-to-region variations of the background, the background-corrected jet transverse momenta are affected by residual fluctuations. To give an estimate for these fluctuations for the jet definition used, cones with radius are randomly placed in each event. In these cones, the track momenta are summed and the background is subtracted to calculate :
[TABLE]
where is the area of the cone.
For the [math]–%, –%, and –% most central collisions, the standard deviation of the -distribution as a measure for the magnitude of the fluctuations has been evaluated to , , and GeV/, respectively. Since the -distribution also contains the jet signal, the standard deviation of the full distribution is impacted by it. A lower limit of these fluctuations is given by performing a Gaussian fit of the left-hand side of the -distribution. The Gaussian widths were evaluated to , , and GeV/ for the [math]–%, –%, and –% most central collisions. The sample of jets that only uses constituents above GeV/ is not corrected for the underlying event as the constituent cut already strongly suppresses the contribution from the background such that it is negligible.
In addition to background fluctuations, also the finite detector resolution and single particle efficiency influence the measurement. To quantify both effects, the ratio of reconstructed jet momentum and true jet momentum was calculated taking into account the detector resolution by using a response matrix and background fluctuations given by the distributions. The response matrix was created from Monte Carlo simulations for which the true jet momentum is known by geometrically matching particle-level PYTHIA jets with the corresponding detector-level jets reconstructed using a full detector model in GEANT3. More detailed studies have been performed for jets on the same dataset in LABEL:Abelev:2013kqa.
There are two effects contributing to the jet momentum resolution: detector effects and underlying event fluctuations. The detector effects lead to a jet momentum response that is peaked at , but has a tail to lower values of detector level momentum due to tracking inefficiency. The tracking efficiency changes by only a few percent from peripheral to central events. Background fluctuations produce an approximately Gaussian response, with a width that depends strongly on centrality. The combined effect leads to a standard deviation in the jet momentum resolution of 30% (20%) for jets with GeV/ and 27% (27%) for jets with GeV/ for the [math]–% (– and –%) most central events.
It should be emphasized that refers to the jet transverse momentum at detector level, corrected for background only. Since within-event fluctuations of the background are not corrected for, the mean of the given -range is slightly higher than that of the underlying true distribution for more central collisions where fluctations are dominant. Hence, due to the steeply-falling jet spectrum, fluctuations lead to a shift of the spectrum to larger values. For more peripheral collisions where detector effects are dominant, there is the opposite effect, i.e. the spectrum is shifted to smaller values. The fraction of purely combinatorial jets in the momentum ranges used in the analysis was found to be negligible.
To give a rough estimate of the true jet populations for a given reconstructed jet momentum range, projections of the response matrices, introduced above, are used [67]. For measured -distributions, approximate ranges are given in Tab. 1 as a measure for the true jet momentum distributions. The true populations are defined as the smallest possible ranges around the -range in which at least 68% of the jet population can be found.
5 Construction of PYTHIA baseline
In this analysis, reconstructed detector-level PYTHIA-jets serve as vacuum baseline, because the size of the pp dataset at TeV is insufficient for this purpose.
To account for the fluctuations of the underlying event in Pb–Pb collisions, PYTHIA jets embedded in real Pb–Pb collisions are used as a reference. Jets reconstructed in this reference dataset still show the same baseline jet properties but also include the effect of background fluctuations from the Pb–Pb event. To create this reference dataset, the following procedure is applied. Events are simulated with PYTHIA6 (Perugia-0 [68], version 6.421) followed by transport in the detector using GEANT3 and full response simulation and reconstruction simulating the same detector conditions as in the Pb–Pb dataset. The reconstructed tracks are embedded into Pb–Pb events, i.e. they are combined with tracks from Pb–Pb events. In order to simulate the same conditions as in Pb–Pb, the tracking efficiency in pp is decreased to the level expected in Pb–Pb. Since the tracking efficiency in pp is higher than in Pb–Pb, % of the PYTHIA tracks are randomly discarded before they are embedded [54]. Jet finding algorithms are applied to the PYTHIA event and also to the combined PYTHIA + Pb–Pb event. Jets found in the combined event are only accepted for the reference dataset if they can be matched geometrically with those in the PYTHIA event. A matched embedded jet needs to be less than away from a PYTHIA jet.
Due to the very high particle occupancy of the Pb–Pb collision system, the probability to reconstruct a PYTHIA jet in the embedded event is much lower than the probability to reconstruct a jet of same momentum by overlapping a jet that already existed in the Pb–Pb event, even after applying a geometrical matching procedure. Therefore, without any further intervention, the embedded jet sample would consist mostly of Pb–Pb-jets overlapping low- PYTHIA jets.
Two approaches have been tested which ensure that the jet sample shows Pb–Pb-event-like fluctuations of a PYTHIA jet, and not jets from the Pb–Pb event. The analysis baseline technique uses a cut on the fraction of the jet that originates from the matched jet in PYTHIA. The applied cut values are motivated by the underlying true jet distribution that shows two separated populations: jets mostly consisting of particles from PYTHIA or from Pb–Pb. The cut value was chosen to achieve the best separation of the two distributions. In the [math]–% most central collisions, it is required that at least 20% of the jet constituents’ originate from the PYTHIA jet. For more peripheral collisions, this fraction is increased to 25%. For jets with GeV/, which were measured down to 30 GeV/, a cut of 50% is applied. However, this procedure might impose a bias on the implicitly accepted background fluctuations. Therefore, variations around these nominal values were considered for the evaluation of systematic uncertainties. Alternatively, a jet veto technique has been used: an embedded jet is not accepted if it overlaps with an already existing jet of sizeable transverse momentum in the Pb–Pb event. Several veto cut values between 15 and 40 GeV/ were tested. Eventually, it turns out that both approaches yield very similar results. The reconstructed jets which survive the MC percentage cut serve as an input to the next analysis steps which are the same as in the data analysis.
6 Observables
In this analysis, two features of particle jets are probed in Pb–Pb collisions: changes in the particle composition of jets and their radial distribution relative to the jet axis.
To probe relative changes in the charged particle composition of jets in a surrounding cone with , the jet-associated yield ratio is measured. The ratio is formed from the integrated jet-associated per-trigger yields and which represent the integrals of the per-trigger yield in the jet cone for a given -range as introduced in Eq. 2. Technically, the integral is the sum over the entries of all (, )-bins whose center is within distances of up to around the jet axis in the background-corrected per-trigger yield histogram.
The jet-associated yield ratio is defined by . It directly compares integrated jet-associated per-trigger yields in Pb–Pb to the same yields for embedded PYTHIA jets. An enhancement or suppression in associated yields is directly seen as a deviation from unity in the ratio.
The relative radial particle distribution around the jet is directly derived from the jet-associated yields. It shows the relative distribution of particle yields inside the jet cone. Thus, it is a measure for the broadening or collimation of constituents with certain momenta in or around the jet cone. As for the jet-associated yield ratio, this measurement is performed for high- and low- jet-associated yields. The radial shape is normalized to represent a probability distribution. It is defined in bins of , the distance to the jet axis, to exploit the radial symmetry of the jet peak. In Refs. [48, 49], an asymmetric broadening of the near-side jet peak is observed in two-particle correlations. It is strongest for low associate and trigger momenta and vanishes for higher momenta. Therefore, in the analysis presented here, the influence of this asymmetry on jet–hadron correlations was tested to check the radial symmetry of the jet peak. Even for the lowest accessible jet and associated track momenta, no jet peak asymmetry was observed. Measurements in and lead to the same conclusions within statistical precision, which justifies the presentation of the jet radial shape in bins of . The correlation function which is used to obtain the shape is originally binned in and . The binning was chosen fine enough to avoid significant binning effects.
For a given centrality-bin, and trigger and associate , it is defined by the following formula:
[TABLE]
where represents the background-corrected per-trigger yield, and the bin edges, and the integral for the self-normalization of the radial shape. The upper limit in the integral used for the self-normalization is chosen to reflect the different ranges of the shown radial shape and is for the jets with GeV/ and for jets with GeV/. The statistical uncertainty is calculated taking into account the self-normalization.
7 Systematic uncertainties
Several sources of systematic uncertainties contribute to the full uncertainty of the measurement and the evaluated individual uncertainties are combined using a quadratic sum, assuming they are uncorrelated. Uncertainties for the following analysis aspects have been taken into account: the non-jet-related background correction technique, the mixed-event correction, the selection of embedded jets, the tracking efficiency, and the impact of using a PYTHIA reference instead of a measured reference in pp at the same energy. The uncertainties are partly correlated point-to-point. The discussed uncertainties are summarized in Tabs. 2–4.
To correct for the non-jet-correlated background in the correlation function, the background is evaluated on the sidebands and subtracted in , as described in Sec. 3. Different underlying background methods for the correlation functions have been tested: for systematic uncertainties, the definition of the sideband range was varied to instead of . In addition, a simpler method that approximates the background by a constant baseline () has been used.
The mixed-event acceptance/inhomogenity correction is a small correction. Two variations are considered for systematic uncertainties. First, the mixed-event correction is calculated inclusively for all . Second, the normalization of the mixed-event correlations is performed for and full instead of using the plateau in and .
In the embedding, a cut motivated by studying the underlying true jet distributions is applied on the fraction of jet originating from the PYTHIA event, as described in Sec. 5. Instead of cutting at 20% for 0–10% centrality, and 25% for other centralities, the cut is varied to 15% and 25% for 0–10% centrality, and to 20% and 30% for other centralities. As described above, for jets with GeV/ a baseline cut value of 50% is used. For systematic variation, the cut is performed at 15% and 60% for 0–10% centrality, 20% and 60% for other centralities.
The detector has a finite single track reconstruction efficiency, which is only known with finite precision. Since all observables are corrected for the tracking efficiency, they are all directly affected by its uncertainty. Detailed studies of the tracking efficiency uncertainty have been performed to evaluate the size of its systematic uncertainty [54, 66]. The studies indicate that the (absolute) uncertainty is % for Pb–Pb collisions, mainly due to an imperfect description of the ITS-TPC matching efficiency. Another uncertainty from the tracking efficiency correction enters this analysis due to the usage of PYTHIA simulations. The tracking efficiency of the PYTHIA data is artificially lowered by before embedding to account for the lower tracking efficiency in Pb–Pb collisions. As a conservative estimate, a relative uncertainty of is assigned to this value. Both components of the tracking efficiency uncertainty are taken into account as independent contributions to the uncertainty, i.e. added in quadrature to the full uncertainty. These uncertainties are directly used as uncertainties for the yields, see Tab. 2. For the jet-associated yield ratio, the uncertainty on the tracking efficiency in Pb–Pb cancels, because it is correlated in Pb–Pb and the embedded PYTHIA reference. For the radial shape distribution, a change in the tracking efficiency has no impact either, since these observables are relative quantities that do not depend on the global magnitude of the tracking efficiency. As an alternative approach to estimate the impact of these two uncertainties of the tracking efficiencies on the observables, the full analysis was redone using corrections that assume the above given lower tracking efficiencies. There was no significant impact on the presented results.
Finally, an uncertainty is assigned since PYTHIA is used as a baseline instead of a measured pp reference. Including this uncertainty, the conclusions are also valid for a pp reference and not only for an embedded PYTHIA reference. In order to do so, the presented observables were calculated and compared for PYTHIA events and pp collisions at 7 TeV. Within the statistical precision of this comparison, it is only possible to give an estimate for the inclusive -range. The relative deviations of each observable between both datasets enter directly as a systematic uncertainty and are on the level of a few percent, cf. Tabs. 2–4.
8 Results
Figures 2 and 3 depict the jet-associated yields (left) and yield ratios (right) for high- and low- associated particles, respectively. Both quantities are shown as a function of event centrality and for several selected jet transverse momenta.
The jet-associated yield ratio shows a suppression with a significance of several standard deviations in the centrality range 0–50% for the considered high- associated particles. In the probed jet momentum range, no significant -dependence is observed. The centrality-dependent linear slope of the distribution for 40–60 GeV/ is more than one standard deviation away from zero, taking into account statistical and systematic uncertainties added in quadrature, indicating that there is a slightly stronger suppression for more central collisions in this case. As a cross check, the same observable was also measured for jets with several higher minimum -cuts, i.e. 1, 2, and 3 GeV/, which are less affected by the underlying event. They lead to similar conclusions.
The jet-associated yield ratio for low- associates has much larger statistical and systematic uncertainties than the ratio of high- constituents, thus it is not possible to draw a definite conclusion.
The measured jet relative radial shapes are presented in Figs. 4 and 5. The top panels show the self-normalized distributions, the difference and the ratio of the shapes in Pb–Pb and embedded PYTHIA can be found in the two lower panels. The jet radial shapes of high- associates are measured for 40–60 GeV/, 60–80 GeV/, and 80–120 GeV/. Shapes of low- associates are presented for jets with 30–40 GeV/ and 3 GeV/ for associates with 1–2 GeV/ and 2–3 GeV/.
In general, the radial shape measurements indicate that all jet-associated yields are similarly distributed relative to the jet axis in Pb–Pb and embedded PYTHIA. The yields of high- associates appear to be slightly more collimated near the core for jets in Pb–Pb, though the absolute effect is small. While the shape is not significantly changed for jet transverse momenta between and GeV/ in Pb–Pb compared to the reference, there is a visible collimation for higher jet momenta above GeV/. This can be seen best in the difference distributions of Fig. 4 which show that a larger fraction of the associated yield can be found near the core in Pb–Pb collisions.
The ratio distributions show that the collimation effect persists up to , which is best visible for jets with 60–80 GeV/. In the CMS measurement [50], no significant change of the near-side jet peak width is observed in Pb–Pb for high- associates and jets above 120 GeV/. However, the magnitude of the effect observed here is compatible with the observations within uncertainties. Also note that the CMS data hints as well to a small collimation of the peak for higher- associates (4–8 GeV/). Possible effects which might lead to a collimation include a relative change in the quark/gluon content in Pb–Pb compared to the reference [69], as well as a suppression of large-angle soft radiation in the coherent jet energy loss picture [70, 71]. Low- jet-associated yields presented in Fig. 5 are measured up to a distance of relative to the jet since in this case the associates are decoupled from the trigger jets.
For 1–2 GeV/, a hint of a broadening of the radial shape is observed for jets with momenta between and GeV/ for the given definition. The broadening is visible in the difference distribution of the left plot in Fig. 5: in Pb–Pb collisions, a smaller fraction of particles can be found directly next to the jet axis. For higher associate transverse momenta, i.e. 2–3 GeV/, there is no significant modification of the low- radial shape of jets in Pb–Pb collisions within the large current experimental uncertainties. A robust measurement of this observable for 40–60 GeV/ or higher momenta is not possible due to the insufficient size of the dataset. For higher jet momenta above 120 GeV/, CMS measures a significant broadening of the near-side jet peak.
9 Summary
The presented results constitute the first attempt to study jet–hadron correlations with track-based jets down to transverse momenta of 30 GeV/ in Pb–Pb collisions — a challenging regime due to the large underlying event and its fluctuations. The jet radial shapes and the change in the particle composition were measured in Pb–Pb collisions at TeV for high- and low- associates and compared to embedded PYTHIA simulations. The number of high- associates in Pb–Pb collisions is suppressed compared to the reference by roughly 30 to 10%, depending on centrality. The radial particle distribution relative to the jet axis shows a moderate modification in Pb–Pb collisions with respect to PYTHIA. High- associate particles are slightly more collimated in Pb–Pb collisions compared to the reference. For jets with GeV/, the radial distributions of low- associates were measured. A hint of a broadening of the low- radial shapes is observed for 1–2 GeV/. The shape for 2–3 GeV/ does not show a significant modification within its large uncertainties. The results are in line with both previous jet–hadron-related measurements from the CMS Collaboration and jet shape measurements from the ALICE Collaboration at higher and add further support for the established picture of in-medium parton energy loss.
Acknowledgements
The ALICE Collaboration would like to thank all its engineers and technicians for their invaluable contributions to the construction of the experiment and the CERN accelerator teams for the outstanding performance of the LHC complex. The ALICE Collaboration gratefully acknowledges the resources and support provided by all Grid centres and the Worldwide LHC Computing Grid (WLCG) collaboration. The ALICE Collaboration acknowledges the following funding agencies for their support in building and running the ALICE detector: A. I. Alikhanyan National Science Laboratory (Yerevan Physics Institute) Foundation (ANSL), State Committee of Science and World Federation of Scientists (WFS), Armenia; Austrian Academy of Sciences, Austrian Science Fund (FWF): [M 2467-N36] and Nationalstiftung für Forschung, Technologie und Entwicklung, Austria; Ministry of Communications and High Technologies, National Nuclear Research Center, Azerbaijan; Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Universidade Federal do Rio Grande do Sul (UFRGS), Financiadora de Estudos e Projetos (Finep) and Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP), Brazil; Ministry of Science & Technology of China (MSTC), National Natural Science Foundation of China (NSFC) and Ministry of Education of China (MOEC) , China; Croatian Science Foundation and Ministry of Science and Education, Croatia; Centro de Aplicaciones Tecnológicas y Desarrollo Nuclear (CEADEN), Cubaenergía, Cuba; Ministry of Education, Youth and Sports of the Czech Republic, Czech Republic; The Danish Council for Independent Research | Natural Sciences, the Carlsberg Foundation and Danish National Research Foundation (DNRF), Denmark; Helsinki Institute of Physics (HIP), Finland; Commissariat à l’Energie Atomique (CEA), Institut National de Physique Nucléaire et de Physique des Particules (IN2P3) and Centre National de la Recherche Scientifique (CNRS) and Rlégion des Pays de la Loire, France; Bundesministerium für Bildung, Wissenschaft, Forschung und Technologie (BMBF) and GSI Helmholtzzentrum für Schwerionenforschung GmbH, Germany; General Secretariat for Research and Technology, Ministry of Education, Research and Religions, Greece; National Research, Development and Innovation Office, Hungary; Department of Atomic Energy Government of India (DAE), Department of Science and Technology, Government of India (DST), University Grants Commission, Government of India (UGC) and Council of Scientific and Industrial Research (CSIR), India; Indonesian Institute of Science, Indonesia; Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche Enrico Fermi and Istituto Nazionale di Fisica Nucleare (INFN), Italy; Institute for Innovative Science and Technology , Nagasaki Institute of Applied Science (IIST), Japan Society for the Promotion of Science (JSPS) KAKENHI and Japanese Ministry of Education, Culture, Sports, Science and Technology (MEXT), Japan; Consejo Nacional de Ciencia (CONACYT) y Tecnología, through Fondo de Cooperación Internacional en Ciencia y Tecnología (FONCICYT) and Dirección General de Asuntos del Personal Academico (DGAPA), Mexico; Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Netherlands; The Research Council of Norway, Norway; Commission on Science and Technology for Sustainable Development in the South (COMSATS), Pakistan; Pontificia Universidad Católica del Perú, Peru; Ministry of Science and Higher Education and National Science Centre, Poland; Korea Institute of Science and Technology Information and National Research Foundation of Korea (NRF), Republic of Korea; Ministry of Education and Scientific Research, Institute of Atomic Physics and Ministry of Research and Innovation and Institute of Atomic Physics, Romania; Joint Institute for Nuclear Research (JINR), Ministry of Education and Science of the Russian Federation, National Research Centre Kurchatov Institute, Russian Science Foundation and Russian Foundation for Basic Research, Russia; Ministry of Education, Science, Research and Sport of the Slovak Republic, Slovakia; National Research Foundation of South Africa, South Africa; Swedish Research Council (VR) and Knut & Alice Wallenberg Foundation (KAW), Sweden; European Organization for Nuclear Research, Switzerland; National Science and Technology Development Agency (NSDTA), Suranaree University of Technology (SUT) and Office of the Higher Education Commission under NRU project of Thailand, Thailand; Turkish Atomic Energy Agency (TAEK), Turkey; National Academy of Sciences of Ukraine, Ukraine; Science and Technology Facilities Council (STFC), United Kingdom; National Science Foundation of the United States of America (NSF) and United States Department of Energy, Office of Nuclear Physics (DOE NP), United States of America.
Appendix A The ALICE Collaboration
S. Acharya\Irefnorg141&D. Adamová\Irefnorg93&S.P. Adhya\Irefnorg141&A. Adler\Irefnorg74&J. Adolfsson\Irefnorg80&M.M. Aggarwal\Irefnorg98&G. Aglieri Rinella\Irefnorg34&M. Agnello\Irefnorg31&N. Agrawal\Irefnorg10&Z. Ahammed\Irefnorg141&S. Ahmad\Irefnorg17&S.U. Ahn\Irefnorg76&S. Aiola\Irefnorg146&A. Akindinov\Irefnorg64&M. Al-Turany\Irefnorg105&S.N. Alam\Irefnorg141&D.S.D. Albuquerque\Irefnorg122&D. Aleksandrov\Irefnorg87&B. Alessandro\Irefnorg58&H.M. Alfanda\Irefnorg6&R. Alfaro Molina\Irefnorg72&B. Ali\Irefnorg17&Y. Ali\Irefnorg15&A. Alici\Irefnorg10,\Irefnorg53,\Irefnorg27&A. Alkin\Irefnorg2&J. Alme\Irefnorg22&T. Alt\Irefnorg69&L. Altenkamper\Irefnorg22&I. Altsybeev\Irefnorg112&M.N. Anaam\Irefnorg6&C. Andrei\Irefnorg47&D. Andreou\Irefnorg34&H.A. Andrews\Irefnorg109&A. Andronic\Irefnorg144&M. Angeletti\Irefnorg34&V. Anguelov\Irefnorg102&C. Anson\Irefnorg16&T. Antičić\Irefnorg106&F. Antinori\Irefnorg56&P. Antonioli\Irefnorg53&R. Anwar\Irefnorg126&N. Apadula\Irefnorg79&L. Aphecetche\Irefnorg114&H. Appelshäuser\Irefnorg69&S. Arcelli\Irefnorg27&R. Arnaldi\Irefnorg58&M. Arratia\Irefnorg79&I.C. Arsene\Irefnorg21&M. Arslandok\Irefnorg102&A. Augustinus\Irefnorg34&R. Averbeck\Irefnorg105&S. Aziz\Irefnorg61&M.D. Azmi\Irefnorg17&A. Badalà\Irefnorg55&Y.W. Baek\Irefnorg40&S. Bagnasco\Irefnorg58&X. Bai\Irefnorg105&R. Bailhache\Irefnorg69&R. Bala\Irefnorg99&A. Baldisseri\Irefnorg137&M. Ball\Irefnorg42&R.C. Baral\Irefnorg85&R. Barbera\Irefnorg28&L. Barioglio\Irefnorg26&G.G. Barnaföldi\Irefnorg145&L.S. Barnby\Irefnorg92&V. Barret\Irefnorg134&P. Bartalini\Irefnorg6&K. Barth\Irefnorg34&E. Bartsch\Irefnorg69&F. Baruffaldi\Irefnorg29&N. Bastid\Irefnorg134&S. Basu\Irefnorg143&G. Batigne\Irefnorg114&B. Batyunya\Irefnorg75&P.C. Batzing\Irefnorg21&D. Bauri\Irefnorg48&J.L. Bazo Alba\Irefnorg110&I.G. Bearden\Irefnorg88&C. Bedda\Irefnorg63&N.K. Behera\Irefnorg60&I. Belikov\Irefnorg136&F. Bellini\Irefnorg34&R. Bellwied\Irefnorg126&V. Belyaev\Irefnorg91&G. Bencedi\Irefnorg145&S. Beole\Irefnorg26&A. Bercuci\Irefnorg47&Y. Berdnikov\Irefnorg96&D. Berenyi\Irefnorg145&R.A. Bertens\Irefnorg130&D. Berzano\Irefnorg58&M.G. Besoiu\Irefnorg68&L. Betev\Irefnorg34&A. Bhasin\Irefnorg99&I.R. Bhat\Irefnorg99&H. Bhatt\Irefnorg48&B. Bhattacharjee\Irefnorg41&A. Bianchi\Irefnorg26&L. Bianchi\Irefnorg126,\Irefnorg26&N. Bianchi\Irefnorg51&J. Bielčík\Irefnorg37&J. Bielčíková\Irefnorg93&A. Bilandzic\Irefnorg117,\Irefnorg103&G. Biro\Irefnorg145&R. Biswas\Irefnorg3&S. Biswas\Irefnorg3&J.T. Blair\Irefnorg119&D. Blau\Irefnorg87&C. Blume\Irefnorg69&G. Boca\Irefnorg139&F. Bock\Irefnorg94,\Irefnorg34&A. Bogdanov\Irefnorg91&L. Boldizsár\Irefnorg145&A. Bolozdynya\Irefnorg91&M. Bombara\Irefnorg38&G. Bonomi\Irefnorg140&H. Borel\Irefnorg137&A. Borissov\Irefnorg144,\Irefnorg91&M. Borri\Irefnorg128&H. Bossi\Irefnorg146&E. Botta\Irefnorg26&C. Bourjau\Irefnorg88&L. Bratrud\Irefnorg69&P. Braun-Munzinger\Irefnorg105&M. Bregant\Irefnorg121&T.A. Broker\Irefnorg69&M. Broz\Irefnorg37&E.J. Brucken\Irefnorg43&E. Bruna\Irefnorg58&G.E. Bruno\Irefnorg33,\Irefnorg104&M.D. Buckland\Irefnorg128&D. Budnikov\Irefnorg107&H. Buesching\Irefnorg69&S. Bufalino\Irefnorg31&O. Bugnon\Irefnorg114&P. Buhler\Irefnorg113&P. Buncic\Irefnorg34&Z. Buthelezi\Irefnorg73&J.B. Butt\Irefnorg15&J.T. Buxton\Irefnorg95&D. Caffarri\Irefnorg89&A. Caliva\Irefnorg105&E. Calvo Villar\Irefnorg110&R.S. Camacho\Irefnorg44&P. Camerini\Irefnorg25&A.A. Capon\Irefnorg113&F. Carnesecchi\Irefnorg10&J. Castillo Castellanos\Irefnorg137&A.J. Castro\Irefnorg130&E.A.R. Casula\Irefnorg54&F. Catalano\Irefnorg31&C. Ceballos Sanchez\Irefnorg52&P. Chakraborty\Irefnorg48&S. Chandra\Irefnorg141&B. Chang\Irefnorg127&W. Chang\Irefnorg6&S. Chapeland\Irefnorg34&M. Chartier\Irefnorg128&S. Chattopadhyay\Irefnorg141&S. Chattopadhyay\Irefnorg108&A. Chauvin\Irefnorg24&C. Cheshkov\Irefnorg135&B. Cheynis\Irefnorg135&V. Chibante Barroso\Irefnorg34&D.D. Chinellato\Irefnorg122&S. Cho\Irefnorg60&P. Chochula\Irefnorg34&T. Chowdhury\Irefnorg134&P. Christakoglou\Irefnorg89&C.H. Christensen\Irefnorg88&P. Christiansen\Irefnorg80&T. Chujo\Irefnorg133&C. Cicalo\Irefnorg54&L. Cifarelli\Irefnorg10,\Irefnorg27&F. Cindolo\Irefnorg53&J. Cleymans\Irefnorg125&F. Colamaria\Irefnorg52&D. Colella\Irefnorg52&A. Collu\Irefnorg79&M. Colocci\Irefnorg27&M. Concas\Irefnorg58\AreforgI&G. Conesa Balbastre\Irefnorg78&Z. Conesa del Valle\Irefnorg61&G. Contin\Irefnorg59,\Irefnorg128&J.G. Contreras\Irefnorg37&T.M. Cormier\Irefnorg94&Y. Corrales Morales\Irefnorg58,\Irefnorg26&P. Cortese\Irefnorg32&M.R. Cosentino\Irefnorg123&F. Costa\Irefnorg34&S. Costanza\Irefnorg139&J. Crkovská\Irefnorg61&P. Crochet\Irefnorg134&E. Cuautle\Irefnorg70&L. Cunqueiro\Irefnorg94&D. Dabrowski\Irefnorg142&T. Dahms\Irefnorg103,\Irefnorg117&A. Dainese\Irefnorg56&F.P.A. Damas\Irefnorg137,\Irefnorg114&S. Dani\Irefnorg66&M.C. Danisch\Irefnorg102&A. Danu\Irefnorg68&D. Das\Irefnorg108&I. Das\Irefnorg108&S. Das\Irefnorg3&A. Dash\Irefnorg85&S. Dash\Irefnorg48&A. Dashi\Irefnorg103&S. De\Irefnorg85,\Irefnorg49&A. De Caro\Irefnorg30&G. de Cataldo\Irefnorg52&C. de Conti\Irefnorg121&J. de Cuveland\Irefnorg39&A. De Falco\Irefnorg24&D. De Gruttola\Irefnorg10&N. De Marco\Irefnorg58&S. De Pasquale\Irefnorg30&R.D. De Souza\Irefnorg122&S. Deb\Irefnorg49&H.F. Degenhardt\Irefnorg121&K.R. Deja\Irefnorg142&A. Deloff\Irefnorg84&S. Delsanto\Irefnorg131,\Irefnorg26&P. Dhankher\Irefnorg48&D. Di Bari\Irefnorg33&A. Di Mauro\Irefnorg34&R.A. Diaz\Irefnorg8&T. Dietel\Irefnorg125&P. Dillenseger\Irefnorg69&Y. Ding\Irefnorg6&R. Divià\Irefnorg34&Ø. Djuvsland\Irefnorg22&U. Dmitrieva\Irefnorg62&A. Dobrin\Irefnorg34,\Irefnorg68&B. Dönigus\Irefnorg69&O. Dordic\Irefnorg21&A.K. Dubey\Irefnorg141&A. Dubla\Irefnorg105&S. Dudi\Irefnorg98&M. Dukhishyam\Irefnorg85&P. Dupieux\Irefnorg134&R.J. Ehlers\Irefnorg146&D. Elia\Irefnorg52&H. Engel\Irefnorg74&E. Epple\Irefnorg146&B. Erazmus\Irefnorg114&F. Erhardt\Irefnorg97&A. Erokhin\Irefnorg112&M.R. Ersdal\Irefnorg22&B. Espagnon\Irefnorg61&G. Eulisse\Irefnorg34&J. Eum\Irefnorg18&D. Evans\Irefnorg109&S. Evdokimov\Irefnorg90&L. Fabbietti\Irefnorg117,\Irefnorg103&M. Faggin\Irefnorg29&J. Faivre\Irefnorg78&A. Fantoni\Irefnorg51&M. Fasel\Irefnorg94&P. Fecchio\Irefnorg31&L. Feldkamp\Irefnorg144&A. Feliciello\Irefnorg58&G. Feofilov\Irefnorg112&A. Fernández Téllez\Irefnorg44&A. Ferrero\Irefnorg137&A. Ferretti\Irefnorg26&A. Festanti\Irefnorg34&V.J.G. Feuillard\Irefnorg102&J. Figiel\Irefnorg118&S. Filchagin\Irefnorg107&D. Finogeev\Irefnorg62&F.M. Fionda\Irefnorg22&G. Fiorenza\Irefnorg52&F. Flor\Irefnorg126&S. Foertsch\Irefnorg73&P. Foka\Irefnorg105&S. Fokin\Irefnorg87&E. Fragiacomo\Irefnorg59&U. Frankenfeld\Irefnorg105&G.G. Fronze\Irefnorg26&U. Fuchs\Irefnorg34&C. Furget\Irefnorg78&A. Furs\Irefnorg62&M. Fusco Girard\Irefnorg30&J.J. Gaardhøje\Irefnorg88&M. Gagliardi\Irefnorg26&A.M. Gago\Irefnorg110&A. Gal\Irefnorg136&C.D. Galvan\Irefnorg120&P. Ganoti\Irefnorg83&C. Garabatos\Irefnorg105&E. Garcia-Solis\Irefnorg11&K. Garg\Irefnorg28&C. Gargiulo\Irefnorg34&K. Garner\Irefnorg144&P. Gasik\Irefnorg103,\Irefnorg117&E.F. Gauger\Irefnorg119&M.B. Gay Ducati\Irefnorg71&M. Germain\Irefnorg114&J. Ghosh\Irefnorg108&P. Ghosh\Irefnorg141&S.K. Ghosh\Irefnorg3&P. Gianotti\Irefnorg51&P. Giubellino\Irefnorg105,\Irefnorg58&P. Giubilato\Irefnorg29&P. Glässel\Irefnorg102&D.M. Goméz Coral\Irefnorg72&A. Gomez Ramirez\Irefnorg74&V. Gonzalez\Irefnorg105&P. González-Zamora\Irefnorg44&S. Gorbunov\Irefnorg39&L. Görlich\Irefnorg118&S. Gotovac\Irefnorg35&V. Grabski\Irefnorg72&L.K. Graczykowski\Irefnorg142&K.L. Graham\Irefnorg109&L. Greiner\Irefnorg79&A. Grelli\Irefnorg63&C. Grigoras\Irefnorg34&V. Grigoriev\Irefnorg91&A. Grigoryan\Irefnorg1&S. Grigoryan\Irefnorg75&O.S. Groettvik\Irefnorg22&J.M. Gronefeld\Irefnorg105&F. Grosa\Irefnorg31&J.F. Grosse-Oetringhaus\Irefnorg34&R. Grosso\Irefnorg105&R. Guernane\Irefnorg78&B. Guerzoni\Irefnorg27&M. Guittiere\Irefnorg114&K. Gulbrandsen\Irefnorg88&T. Gunji\Irefnorg132&A. Gupta\Irefnorg99&R. Gupta\Irefnorg99&I.B. Guzman\Irefnorg44&R. Haake\Irefnorg34,\Irefnorg146&M.K. Habib\Irefnorg105&C. Hadjidakis\Irefnorg61&H. Hamagaki\Irefnorg81&G. Hamar\Irefnorg145&M. Hamid\Irefnorg6&R. Hannigan\Irefnorg119&M.R. Haque\Irefnorg63&A. Harlenderova\Irefnorg105&J.W. Harris\Irefnorg146&A. Harton\Irefnorg11&J.A. Hasenbichler\Irefnorg34&H. Hassan\Irefnorg78&D. Hatzifotiadou\Irefnorg10,\Irefnorg53&P. Hauer\Irefnorg42&S. Hayashi\Irefnorg132&S.T. Heckel\Irefnorg69&E. Hellbär\Irefnorg69&H. Helstrup\Irefnorg36&A. Herghelegiu\Irefnorg47&E.G. Hernandez\Irefnorg44&G. Herrera Corral\Irefnorg9&F. Herrmann\Irefnorg144&K.F. Hetland\Irefnorg36&T.E. Hilden\Irefnorg43&H. Hillemanns\Irefnorg34&C. Hills\Irefnorg128&B. Hippolyte\Irefnorg136&B. Hohlweger\Irefnorg103&D. Horak\Irefnorg37&S. Hornung\Irefnorg105&R. Hosokawa\Irefnorg133&P. Hristov\Irefnorg34&C. Huang\Irefnorg61&C. Hughes\Irefnorg130&P. Huhn\Irefnorg69&T.J. Humanic\Irefnorg95&H. Hushnud\Irefnorg108&L.A. Husova\Irefnorg144&N. Hussain\Irefnorg41&S.A. Hussain\Irefnorg15&T. Hussain\Irefnorg17&D. Hutter\Irefnorg39&D.S. Hwang\Irefnorg19&J.P. Iddon\Irefnorg128,\Irefnorg34&R. Ilkaev\Irefnorg107&M. Inaba\Irefnorg133&M. Ippolitov\Irefnorg87&M.S. Islam\Irefnorg108&M. Ivanov\Irefnorg105&V. Ivanov\Irefnorg96&V. Izucheev\Irefnorg90&B. Jacak\Irefnorg79&N. Jacazio\Irefnorg27&P.M. Jacobs\Irefnorg79&M.B. Jadhav\Irefnorg48&S. Jadlovska\Irefnorg116&J. Jadlovsky\Irefnorg116&S. Jaelani\Irefnorg63&C. Jahnke\Irefnorg121&M.J. Jakubowska\Irefnorg142&M.A. Janik\Irefnorg142&M. Jercic\Irefnorg97&O. Jevons\Irefnorg109&R.T. Jimenez Bustamante\Irefnorg105&M. Jin\Irefnorg126&F. Jonas\Irefnorg144,\Irefnorg94&P.G. Jones\Irefnorg109&A. Jusko\Irefnorg109&P. Kalinak\Irefnorg65&A. Kalweit\Irefnorg34&J.H. Kang\Irefnorg147&V. Kaplin\Irefnorg91&S. Kar\Irefnorg6&A. Karasu Uysal\Irefnorg77&O. Karavichev\Irefnorg62&T. Karavicheva\Irefnorg62&P. Karczmarczyk\Irefnorg34&E. Karpechev\Irefnorg62&U. Kebschull\Irefnorg74&R. 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Voloshin\Irefnorg64&S.A. Voloshin\Irefnorg143&G. Volpe\Irefnorg33&B. von Haller\Irefnorg34&I. Vorobyev\Irefnorg103,\Irefnorg117&D. Voscek\Irefnorg116&J. Vrláková\Irefnorg38&B. Wagner\Irefnorg22&Y. Watanabe\Irefnorg133&M. Weber\Irefnorg113&S.G. Weber\Irefnorg105&A. Wegrzynek\Irefnorg34&D.F. Weiser\Irefnorg102&S.C. Wenzel\Irefnorg34&J.P. Wessels\Irefnorg144&E. Widmann\Irefnorg113&J. Wiechula\Irefnorg69&J. Wikne\Irefnorg21&G. Wilk\Irefnorg84&J. Wilkinson\Irefnorg53&G.A. Willems\Irefnorg34&E. Willsher\Irefnorg109&B. Windelband\Irefnorg102&W.E. Witt\Irefnorg130&Y. Wu\Irefnorg129&R. Xu\Irefnorg6&S. Yalcin\Irefnorg77&K. Yamakawa\Irefnorg45&S. Yang\Irefnorg22&S. Yano\Irefnorg137&Z. Yin\Irefnorg6&H. Yokoyama\Irefnorg63&I.-K. Yoo\Irefnorg18&J.H. Yoon\Irefnorg60&S. Yuan\Irefnorg22&A. Yuncu\Irefnorg102&V. Yurchenko\Irefnorg2&V. Zaccolo\Irefnorg58,\Irefnorg25&A. Zaman\Irefnorg15&C. Zampolli\Irefnorg34&H.J.C. Zanoli\Irefnorg121&N. Zardoshti\Irefnorg34&A. Zarochentsev\Irefnorg112&P. Závada\Irefnorg67&N. Zaviyalov\Irefnorg107&H. Zbroszczyk\Irefnorg142&M. Zhalov\Irefnorg96&X. Zhang\Irefnorg6&Z. Zhang\Irefnorg6,\Irefnorg134&C. Zhao\Irefnorg21&V. Zherebchevskii\Irefnorg112&N. Zhigareva\Irefnorg64&D. Zhou\Irefnorg6&Y. Zhou\Irefnorg88&Z. Zhou\Irefnorg22&J. Zhu\Irefnorg6&Y. Zhu\Irefnorg6&A. Zichichi\Irefnorg27,\Irefnorg10&M.B. Zimmermann\Irefnorg34&G. Zinovjev\Irefnorg2&N. Zurlo\Irefnorg140&
Affiliation notes
{Authlist}
\Adef
org*Deceased
\Adef
orgIDipartimento DET del Politecnico di Torino, Turin, Italy
\Adef
orgIIM.V. Lomonosov Moscow State University, D.V. Skobeltsyn Institute of Nuclear, Physics, Moscow, Russia
\Adef
orgIIIDepartment of Applied Physics, Aligarh Muslim University, Aligarh, India
\Adef
orgIVInstitute of Theoretical Physics, University of Wroclaw, Poland
Collaboration Institutes
{Authlist}
\Idef
org1A.I. Alikhanyan National Science Laboratory (Yerevan Physics Institute) Foundation, Yerevan, Armenia
\Idef
org2Bogolyubov Institute for Theoretical Physics, National Academy of Sciences of Ukraine, Kiev, Ukraine
\Idef
org3Bose Institute, Department of Physics and Centre for Astroparticle Physics and Space Science (CAPSS), Kolkata, India
\Idef
org4Budker Institute for Nuclear Physics, Novosibirsk, Russia
\Idef
org5California Polytechnic State University, San Luis Obispo, California, United States
\Idef
org6Central China Normal University, Wuhan, China
\Idef
org7Centre de Calcul de l’IN2P3, Villeurbanne, Lyon, France
\Idef
org8Centro de Aplicaciones Tecnológicas y Desarrollo Nuclear (CEADEN), Havana, Cuba
\Idef
org9Centro de Investigación y de Estudios Avanzados (CINVESTAV), Mexico City and Mérida, Mexico
\Idef
org10Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi’, Rome, Italy
\Idef
org11Chicago State University, Chicago, Illinois, United States
\Idef
org12China Institute of Atomic Energy, Beijing, China
\Idef
org13Chonbuk National University, Jeonju, Republic of Korea
\Idef
org14Comenius University Bratislava, Faculty of Mathematics, Physics and Informatics, Bratislava, Slovakia
\Idef
org15COMSATS University Islamabad, Islamabad, Pakistan
\Idef
org16Creighton University, Omaha, Nebraska, United States
\Idef
org17Department of Physics, Aligarh Muslim University, Aligarh, India
\Idef
org18Department of Physics, Pusan National University, Pusan, Republic of Korea
\Idef
org19Department of Physics, Sejong University, Seoul, Republic of Korea
\Idef
org20Department of Physics, University of California, Berkeley, California, United States
\Idef
org21Department of Physics, University of Oslo, Oslo, Norway
\Idef
org22Department of Physics and Technology, University of Bergen, Bergen, Norway
\Idef
org23Dipartimento di Fisica dell’Università ’La Sapienza’ and Sezione INFN, Rome, Italy
\Idef
org24Dipartimento di Fisica dell’Università and Sezione INFN, Cagliari, Italy
\Idef
org25Dipartimento di Fisica dell’Università and Sezione INFN, Trieste, Italy
\Idef
org26Dipartimento di Fisica dell’Università and Sezione INFN, Turin, Italy
\Idef
org27Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Bologna, Italy
\Idef
org28Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Catania, Italy
\Idef
org29Dipartimento di Fisica e Astronomia dell’Università and Sezione INFN, Padova, Italy
\Idef
org30Dipartimento di Fisica ‘E.R. Caianiello’ dell’Università and Gruppo Collegato INFN, Salerno, Italy
\Idef
org31Dipartimento DISAT del Politecnico and Sezione INFN, Turin, Italy
\Idef
org32Dipartimento di Scienze e Innovazione Tecnologica dell’Università del Piemonte Orientale and INFN Sezione di Torino, Alessandria, Italy
\Idef
org33Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy
\Idef
org34European Organization for Nuclear Research (CERN), Geneva, Switzerland
\Idef
org35Faculty of Electrical Engineering, Mechanical Engineering and Naval Architecture, University of Split, Split, Croatia
\Idef
org36Faculty of Engineering and Science, Western Norway University of Applied Sciences, Bergen, Norway
\Idef
org37Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic
\Idef
org38Faculty of Science, P.J. Šafárik University, Košice, Slovakia
\Idef
org39Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
\Idef
org40Gangneung-Wonju National University, Gangneung, Republic of Korea
\Idef
org41Gauhati University, Department of Physics, Guwahati, India
\Idef
org42Helmholtz-Institut für Strahlen- und Kernphysik, Rheinische Friedrich-Wilhelms-Universität Bonn, Bonn, Germany
\Idef
org43Helsinki Institute of Physics (HIP), Helsinki, Finland
\Idef
org44High Energy Physics Group, Universidad Autónoma de Puebla, Puebla, Mexico
\Idef
org45Hiroshima University, Hiroshima, Japan
\Idef
org46Hochschule Worms, Zentrum für Technologietransfer und Telekommunikation (ZTT), Worms, Germany
\Idef
org47Horia Hulubei National Institute of Physics and Nuclear Engineering, Bucharest, Romania
\Idef
org48Indian Institute of Technology Bombay (IIT), Mumbai, India
\Idef
org49Indian Institute of Technology Indore, Indore, India
\Idef
org50Indonesian Institute of Sciences, Jakarta, Indonesia
\Idef
org51INFN, Laboratori Nazionali di Frascati, Frascati, Italy
\Idef
org52INFN, Sezione di Bari, Bari, Italy
\Idef
org53INFN, Sezione di Bologna, Bologna, Italy
\Idef
org54INFN, Sezione di Cagliari, Cagliari, Italy
\Idef
org55INFN, Sezione di Catania, Catania, Italy
\Idef
org56INFN, Sezione di Padova, Padova, Italy
\Idef
org57INFN, Sezione di Roma, Rome, Italy
\Idef
org58INFN, Sezione di Torino, Turin, Italy
\Idef
org59INFN, Sezione di Trieste, Trieste, Italy
\Idef
org60Inha University, Incheon, Republic of Korea
\Idef
org61Institut de Physique Nucléaire d’Orsay (IPNO), Institut National de Physique Nucléaire et de Physique des Particules (IN2P3/CNRS), Université de Paris-Sud, Université Paris-Saclay, Orsay, France
\Idef
org62Institute for Nuclear Research, Academy of Sciences, Moscow, Russia
\Idef
org63Institute for Subatomic Physics, Utrecht University/Nikhef, Utrecht, Netherlands
\Idef
org64Institute for Theoretical and Experimental Physics, Moscow, Russia
\Idef
org65Institute of Experimental Physics, Slovak Academy of Sciences, Košice, Slovakia
\Idef
org66Institute of Physics, Homi Bhabha National Institute, Bhubaneswar, India
\Idef
org67Institute of Physics of the Czech Academy of Sciences, Prague, Czech Republic
\Idef
org68Institute of Space Science (ISS), Bucharest, Romania
\Idef
org69Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany
\Idef
org70Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Mexico City, Mexico
\Idef
org71Instituto de Física, Universidade Federal do Rio Grande do Sul (UFRGS), Porto Alegre, Brazil
\Idef
org72Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
\Idef
org73iThemba LABS, National Research Foundation, Somerset West, South Africa
\Idef
org74Johann-Wolfgang-Goethe Universität Frankfurt Institut für Informatik, Fachbereich Informatik und Mathematik, Frankfurt, Germany
\Idef
org75Joint Institute for Nuclear Research (JINR), Dubna, Russia
\Idef
org76Korea Institute of Science and Technology Information, Daejeon, Republic of Korea
\Idef
org77KTO Karatay University, Konya, Turkey
\Idef
org78Laboratoire de Physique Subatomique et de Cosmologie, Université Grenoble-Alpes, CNRS-IN2P3, Grenoble, France
\Idef
org79Lawrence Berkeley National Laboratory, Berkeley, California, United States
\Idef
org80Lund University Department of Physics, Division of Particle Physics, Lund, Sweden
\Idef
org81Nagasaki Institute of Applied Science, Nagasaki, Japan
\Idef
org82Nara Women’s University (NWU), Nara, Japan
\Idef
org83National and Kapodistrian University of Athens, School of Science, Department of Physics , Athens, Greece
\Idef
org84National Centre for Nuclear Research, Warsaw, Poland
\Idef
org85National Institute of Science Education and Research, Homi Bhabha National Institute, Jatni, India
\Idef
org86National Nuclear Research Center, Baku, Azerbaijan
\Idef
org87National Research Centre Kurchatov Institute, Moscow, Russia
\Idef
org88Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark
\Idef
org89Nikhef, National institute for subatomic physics, Amsterdam, Netherlands
\Idef
org90NRC Kurchatov Institute IHEP, Protvino, Russia
\Idef
org91NRNU Moscow Engineering Physics Institute, Moscow, Russia
\Idef
org92Nuclear Physics Group, STFC Daresbury Laboratory, Daresbury, United Kingdom
\Idef
org93Nuclear Physics Institute of the Czech Academy of Sciences, Řež u Prahy, Czech Republic
\Idef
org94Oak Ridge National Laboratory, Oak Ridge, Tennessee, United States
\Idef
org95Ohio State University, Columbus, Ohio, United States
\Idef
org96Petersburg Nuclear Physics Institute, Gatchina, Russia
\Idef
org97Physics department, Faculty of science, University of Zagreb, Zagreb, Croatia
\Idef
org98Physics Department, Panjab University, Chandigarh, India
\Idef
org99Physics Department, University of Jammu, Jammu, India
\Idef
org100Physics Department, University of Rajasthan, Jaipur, India
\Idef
org101Physikalisches Institut, Eberhard-Karls-Universität Tübingen, Tübingen, Germany
\Idef
org102Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany
\Idef
org103Physik Department, Technische Universität München, Munich, Germany
\Idef
org104Politecnico di Bari, Bari, Italy
\Idef
org105Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung GmbH, Darmstadt, Germany
\Idef
org106Rudjer Bošković Institute, Zagreb, Croatia
\Idef
org107Russian Federal Nuclear Center (VNIIEF), Sarov, Russia
\Idef
org108Saha Institute of Nuclear Physics, Homi Bhabha National Institute, Kolkata, India
\Idef
org109School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom
\Idef
org110Sección Física, Departamento de Ciencias, Pontificia Universidad Católica del Perú, Lima, Peru
\Idef
org111Shanghai Institute of Applied Physics, Shanghai, China
\Idef
org112St. Petersburg State University, St. Petersburg, Russia
\Idef
org113Stefan Meyer Institut für Subatomare Physik (SMI), Vienna, Austria
\Idef
org114SUBATECH, IMT Atlantique, Université de Nantes, CNRS-IN2P3, Nantes, France
\Idef
org115Suranaree University of Technology, Nakhon Ratchasima, Thailand
\Idef
org116Technical University of Košice, Košice, Slovakia
\Idef
org117Technische Universität München, Excellence Cluster ’Universe’, Munich, Germany
\Idef
org118The Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, Cracow, Poland
\Idef
org119The University of Texas at Austin, Austin, Texas, United States
\Idef
org120Universidad Autónoma de Sinaloa, Culiacán, Mexico
\Idef
org121Universidade de São Paulo (USP), São Paulo, Brazil
\Idef
org122Universidade Estadual de Campinas (UNICAMP), Campinas, Brazil
\Idef
org123Universidade Federal do ABC, Santo Andre, Brazil
\Idef
org124University College of Southeast Norway, Tonsberg, Norway
\Idef
org125University of Cape Town, Cape Town, South Africa
\Idef
org126University of Houston, Houston, Texas, United States
\Idef
org127University of Jyväskylä, Jyväskylä, Finland
\Idef
org128University of Liverpool, Liverpool, United Kingdom
\Idef
org129University of Science and Techonology of China, Hefei, China
\Idef
org130University of Tennessee, Knoxville, Tennessee, United States
\Idef
org131University of the Witwatersrand, Johannesburg, South Africa
\Idef
org132University of Tokyo, Tokyo, Japan
\Idef
org133University of Tsukuba, Tsukuba, Japan
\Idef
org134Université Clermont Auvergne, CNRS/IN2P3, LPC, Clermont-Ferrand, France
\Idef
org135Université de Lyon, Université Lyon 1, CNRS/IN2P3, IPN-Lyon, Villeurbanne, Lyon, France
\Idef
org136Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France, Strasbourg, France
\Idef
org137Université Paris-Saclay Centre d’Etudes de Saclay (CEA), IRFU, Départment de Physique Nucléaire (DPhN), Saclay, France
\Idef
org138Università degli Studi di Foggia, Foggia, Italy
\Idef
org139Università degli Studi di Pavia, Pavia, Italy
\Idef
org140Università di Brescia, Brescia, Italy
\Idef
org141Variable Energy Cyclotron Centre, Homi Bhabha National Institute, Kolkata, India
\Idef
org142Warsaw University of Technology, Warsaw, Poland
\Idef
org143Wayne State University, Detroit, Michigan, United States
\Idef
org144Westfälische Wilhelms-Universität Münster, Institut für Kernphysik, Münster, Germany
\Idef
org145Wigner Research Centre for Physics, Hungarian Academy of Sciences, Budapest, Hungary
\Idef
org146Yale University, New Haven, Connecticut, United States
\Idef
org147Yonsei University, Seoul, Republic of Korea
The reference list from the paper itself. Each links out to its DOI / PubMed record.
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