Showing 25 of 46 results
The ATLAS Collaboration has measured the inclusive production of $Z$ bosons via their decays into electron and muon pairs in $p+$Pb collisions at $\sqrt{s_{NN}}=5.02$ TeV at the Large Hadron Collider. The measurements are made using data corresponding to integrated luminosities of 29.4 nb$^{-1}$ and 28.1 nb$^{-1}$ for $Z \rightarrow ee$ and $Z \rightarrow \mu\mu$, respectively. The results from the two channels are consistent and combined to obtain a cross section times the $Z \rightarrow \ell\ell$ branching ratio, integrated over the rapidity region $|y^{*}_{Z}|<3.5$, of 139.8 $\pm$ 4.8 (stat.) $\pm$ 6.2 (syst.) $\pm$ 3.8 (lumi.) nb. Differential cross sections are presented as functions of the $Z$ boson rapidity and transverse momentum, and compared with models based on parton distributions both with and without nuclear corrections. The centrality dependence of $Z$ boson production in $p+$Pb collisions is measured and analyzed within the framework of a standard Glauber model and the model's extension for fluctuations of the underlying nucleon-nucleon scattering cross section.
The centrality bias factors derived from data as explained in the text. Model calculations shown in the Figure are found in arXiv:1412.0976.
The differential $Z$ boson production cross section, $d\sigma/dy^\mathrm{*}_{Z}$, as a function of $Z$ boson rapidity in the center-of-mass frame $y^\mathrm{*}_{Z}$, for $Z\rightarrow ee$, $Z\rightarrow\mu\mu$, and their combination $Z\rightarrow\ell\ell$.
The differential cross section of $Z$ boson production multiplied by the Bjorken $x$ of the parton in the lead nucleus, $x_{Pb} d\sigma /dx_{Pb}$, as a function of $x_{Pb}$.
The differential cross section of $Z$ boson production scaled by 1/$p_\mathrm{T}^{Z}$, (1/$p_\mathrm{T}^{Z}$) $d\sigma /dp_\mathrm{T}^{Z}$, for $-3<y^\mathrm{*}_{Z}<2$.
The differential cross section of $Z$ boson production scaled by 1/$p_\mathrm{T}^{Z}$, (1/$p_\mathrm{T}^{Z}$) $d\sigma /dp_\mathrm{T}^{Z}$, for $-2<y^\mathrm{*}_{Z}<0$ and $0<y^\mathrm{*}_{Z}<2.
Centrality bias corrected $Z$ boson yields per event for $-3<y^\mathrm{*}_{Z}<2$ scaled by by $\langle N_{coll}\rangle$. (To remove the centrality bias correction each value may be multiplied by the approriate correction value found in arXiv:1412.0976.).
The rapidity differential Z boson yields per event scaled by $\langle N_{coll}\rangle$ for three centrality ranges.
Measurements of the centrality and rapidity dependence of inclusive jet production in $\sqrt{s_\mathrm{NN}} = 5.02$ TeV proton--lead ($p$+Pb) collisions and the jet cross-section in $\sqrt{s} = 2.76$ TeV proton--proton collisions are presented. These quantities are measured in datasets corresponding to an integrated luminosity of 27.8 nb$^{-1}$ and 4.0 pb$^{-1}$, respectively, recorded with the ATLAS detector at the Large Hadron Collider in 2013. The $p$+Pb collision centrality was characterised using the total transverse energy measured in the pseudorapidity interval $-4.9 < \eta < -3.2$ in the direction of the lead beam. Results are presented for the double-differential per-collision yields as a function of jet rapidity and transverse momentum ($p_\mathrm{T}$) for minimum-bias and centrality-selected $p$+Pb collisions, and are compared to the jet rate from the geometric expectation. The total jet yield in minimum-bias events is slightly enhanced above the expectation in a $p_\mathrm{T}$-dependent manner but is consistent with the expectation within uncertainties. The ratios of jet spectra from different centrality selections show a strong modification of jet production at all $p_\mathrm{T}$ at forward rapidities and for large $p_\mathrm{T}$ at mid-rapidity, which manifests as a suppression of the jet yield in central events and an enhancement in peripheral events. These effects imply that the factorisation between hard and soft processes is violated at an unexpected level in proton-nucleus collisions. Furthermore, the modifications at forward rapidities are found to be a function of the total jet energy only, implying that the violations may have a simple dependence on the hard parton-parton kinematics.
The $R_{\mathrm{coll}}$ and $T_{p\mathrm{A}}$ values and their uncertainties in each centrality bin.
Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).
Per-event jet yields in 0-90% p+Pb collisions, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).
Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RpPb for 0-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).
Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).
Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).
Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).
Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).
Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).
Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RCP for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RCP for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RCP for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RpPb for 0-10% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RpPb for 20-30% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RpPb for 60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 0-10%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 10-20%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 20-30%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 30-40%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +3.6 to +4.4 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +2.8 to +3.6 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RCP vs. pT*cosh(y*) for 40-60%/60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 0-10% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 10-20% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 20-30% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 30-40% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 40-60% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity +2.1 to +2.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity +1.2 to +2.1 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity +0.8 to +1.2 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity +0.3 to +0.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity -0.3 to +0.3 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity -0.8 to -0.3 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity -1.2 to -0.8 (positive denotes downstream proton direction).
Jet RpPb vs. pT*cosh(y*) for 60-90% p+Pb events, within the centre of mass rapidity -2.1 to -1.2 (positive denotes downstream proton direction).
This paper presents measurements of charged-hadron spectra obtained in $pp$, $p$+Pb, and Pb+Pb collisions at $\sqrt{s}$ or $\sqrt{s_{_\text{NN}}}=5.02$ TeV, and in Xe+Xe collisions at $\sqrt{s_{_\text{NN}}}=5.44$ TeV. The data recorded by the ATLAS detector at the LHC have total integrated luminosities of 25 pb${}^{-1}$, 28 nb${}^{-1}$, 0.50 nb${}^{-1}$, and 3 $\mu$b${}^{-1}$, respectively. The nuclear modification factors $R_{p\text{Pb}}$ and $R_\text{AA}$ are obtained by comparing the spectra in heavy-ion and $pp$ collisions in a wide range of charged-particle transverse momenta and pseudorapidity. The nuclear modification factor $R_{p\text{Pb}}$ shows a moderate enhancement above unity with a maximum at $p_{\mathrm{T}} \approx 3$ GeV; the enhancement is stronger in the Pb-going direction. The nuclear modification factors in both Pb+Pb and Xe+Xe collisions feature a significant, centrality-dependent suppression. They show a similar distinct $p_{\mathrm{T}}$-dependence with a local maximum at $p_{\mathrm{T}} \approx 2$ GeV and a local minimum at $p_{\mathrm{T}} \approx 7$ GeV. This dependence is more distinguishable in more central collisions. No significant $|\eta|$-dependence is found. A comprehensive comparison with several theoretical predictions is also provided. They typically describe $R_\text{AA}$ better in central collisions and in the $p_{\mathrm{T}}$ range from about 10 to 100 GeV.
- - - - - - - - - - - - - - - - - - - - <br><b>charged-hadron spectra:</b> <br><i>pp reference:</i> <a href="?version=1&table=Table1">for p+Pb</a> <a href="?version=1&table=Table10">for Pb+Pb</a> <a href="?version=1&table=Table19">for Xe+Xe</a> <br><i>p+Pb:</i> <a href="?version=1&table=Table2">0-5%</a> <a href="?version=1&table=Table3">5-10%</a> <a href="?version=1&table=Table4">10-20%</a> <a href="?version=1&table=Table5">20-30%</a> <a href="?version=1&table=Table6">30-40%</a> <a href="?version=1&table=Table7">40-60%</a> <a href="?version=1&table=Table8">60-90%</a> <a href="?version=1&table=Table9">0-90%</a> <br><i>Pb+Pb:</i> <a href="?version=1&table=Table11">0-5%</a> <a href="?version=1&table=Table12">5-10%</a> <a href="?version=1&table=Table13">10-20%</a> <a href="?version=1&table=Table14">20-30%</a> <a href="?version=1&table=Table15">30-40%</a> <a href="?version=1&table=Table16">40-50%</a> <a href="?version=1&table=Table17">50-60%</a> <a href="?version=1&table=Table18">60-80%</a> <br><i>Xe+Xe:</i> <a href="?version=1&table=Table20">0-5%</a> <a href="?version=1&table=Table21">5-10%</a> <a href="?version=1&table=Table22">10-20%</a> <a href="?version=1&table=Table23">20-30%</a> <a href="?version=1&table=Table24">30-40%</a> <a href="?version=1&table=Table25">40-50%</a> <a href="?version=1&table=Table26">50-60%</a> <a href="?version=1&table=Table27">60-80%</a> </br>- - - - - - - - - - - - - - - - - - - - <br><b>nuclear modification factors (p<sub>T</sub>):</b> <br><i>R<sub>pPb</sub>:</i> <a href="?version=1&table=Table28">0-5%</a> <a href="?version=1&table=Table29">5-10%</a> <a href="?version=1&table=Table30">10-20%</a> <a href="?version=1&table=Table31">20-30%</a> <a href="?version=1&table=Table32">30-40%</a> <a href="?version=1&table=Table33">40-60%</a> <a href="?version=1&table=Table34">60-90%</a> <a href="?version=1&table=Table35">0-90%</a> <br><i>R<sub>AA</sub> (Pb+Pb):</i> <a href="?version=1&table=Table36">0-5%</a> <a href="?version=1&table=Table37">5-10%</a> <a href="?version=1&table=Table38">10-20%</a> <a href="?version=1&table=Table39">20-30%</a> <a href="?version=1&table=Table40">30-40%</a> <a href="?version=1&table=Table41">40-50%</a> <a href="?version=1&table=Table42">50-60%</a> <a href="?version=1&table=Table43">60-80%</a> <br><i>R<sub>AA</sub> (Xe+Xe):</i> <a href="?version=1&table=Table44">0-5%</a> <a href="?version=1&table=Table45">5-10%</a> <a href="?version=1&table=Table46">10-20%</a> <a href="?version=1&table=Table47">20-30%</a> <a href="?version=1&table=Table48">30-40%</a> <a href="?version=1&table=Table49">40-50%</a> <a href="?version=1&table=Table50">50-60%</a> <a href="?version=1&table=Table51">60-80%</a> </br>- - - - - - - - - - - - - - - - - - - - <br><b>nuclear modification factors (y*/eta):</b> <br><i>R<sub>pPb</sub>:</i> <br> 0-5%: <a href="?version=1&table=Table52">0.66-0.755GeV</a> <a href="?version=1&table=Table53">2.95-3.35GeV</a> <a href="?version=1&table=Table54">7.65-8.8GeV</a> <a href="?version=1&table=Table55">15.1-17.3GeV</a> <br> 5-10%: <a href="?version=1&table=Table56">0.66-0.755GeV</a> <a href="?version=1&table=Table57">2.95-3.35GeV</a> <a href="?version=1&table=Table58">7.65-8.8GeV</a> <a href="?version=1&table=Table59">15.1-17.3GeV</a> <br> 10-20%: <a href="?version=1&table=Table60">0.66-0.755GeV</a> <a href="?version=1&table=Table61">2.95-3.35GeV</a> <a href="?version=1&table=Table62">7.65-8.8GeV</a> <a href="?version=1&table=Table63">15.1-17.3GeV</a> <br> 20-30%: <a href="?version=1&table=Table64">0.66-0.755GeV</a> <a href="?version=1&table=Table65">2.95-3.35GeV</a> <a href="?version=1&table=Table66">7.65-8.8GeV</a> <a href="?version=1&table=Table67">15.1-17.3GeV</a> <br> 30-40%: <a href="?version=1&table=Table68">0.66-0.755GeV</a> <a href="?version=1&table=Table69">2.95-3.35GeV</a> <a href="?version=1&table=Table70">7.65-8.8GeV</a> <a href="?version=1&table=Table71">15.1-17.3GeV</a> <br> 40-60%: <a href="?version=1&table=Table72">0.66-0.755GeV</a> <a href="?version=1&table=Table73">2.95-3.35GeV</a> <a href="?version=1&table=Table74">7.65-8.8GeV</a> <a href="?version=1&table=Table75">15.1-17.3GeV</a> <br> 60-90%: <a href="?version=1&table=Table76">0.66-0.755GeV</a> <a href="?version=1&table=Table77">2.95-3.35GeV</a> <a href="?version=1&table=Table78">7.65-8.8GeV</a> <a href="?version=1&table=Table79">15.1-17.3GeV</a> <br> 0-90%: <a href="?version=1&table=Table80">0.66-0.755GeV</a> <a href="?version=1&table=Table81">2.95-3.35GeV</a> <a href="?version=1&table=Table82">7.65-8.8GeV</a> <a href="?version=1&table=Table83">15.1-17.3GeV</a> <br><i>R<sub>AA</sub> (Pb+Pb):</i> <br> 0-5%: <a href="?version=1&table=Table84">1.7-1.95GeV</a> <a href="?version=1&table=Table85">6.7-7.65GeV</a> <a href="?version=1&table=Table86">20-23GeV</a> <a href="?version=1&table=Table87">60-95GeV</a> <br> 5-10%: <a href="?version=1&table=Table88">1.7-1.95GeV</a> <a href="?version=1&table=Table89">6.7-7.65GeV</a> <a href="?version=1&table=Table90">20-23GeV</a> <a href="?version=1&table=Table91">60-95GeV</a> <br> 10-20%: <a href="?version=1&table=Table92">1.7-1.95GeV</a> <a href="?version=1&table=Table93">6.7-7.65GeV</a> <a href="?version=1&table=Table94">20-23GeV</a> <a href="?version=1&table=Table95">60-95GeV</a> <br> 20-30%: <a href="?version=1&table=Table96">1.7-1.95GeV</a> <a href="?version=1&table=Table97">6.7-7.65GeV</a> <a href="?version=1&table=Table98">20-23GeV</a> <a href="?version=1&table=Table99">60-95GeV</a> <br> 30-40%: <a href="?version=1&table=Table100">1.7-1.95GeV</a> <a href="?version=1&table=Table101">6.7-7.65GeV</a> <a href="?version=1&table=Table102">20-23GeV</a> <a href="?version=1&table=Table103">60-95GeV</a> <br> 40-50%: <a href="?version=1&table=Table104">1.7-1.95GeV</a> <a href="?version=1&table=Table105">6.7-7.65GeV</a> <a href="?version=1&table=Table106">20-23GeV</a> <a href="?version=1&table=Table107">60-95GeV</a> <br> 50-60%: <a href="?version=1&table=Table108">1.7-1.95GeV</a> <a href="?version=1&table=Table109">6.7-7.65GeV</a> <a href="?version=1&table=Table110">20-23GeV</a> <a href="?version=1&table=Table111">60-95GeV</a> <br> 60-80%: <a href="?version=1&table=Table112">1.7-1.95GeV</a> <a href="?version=1&table=Table113">6.7-7.65GeV</a> <a href="?version=1&table=Table114">20-23GeV</a> <a href="?version=1&table=Table115">60-95GeV</a> <br><i>R<sub>AA</sub> (Xe+Xe):</i> <br> 0-5%: <a href="?version=1&table=Table116">1.7-1.95GeV</a> <a href="?version=1&table=Table117">6.7-7.65GeV</a> <a href="?version=1&table=Table118">20-23GeV</a> <br> 5-10%: <a href="?version=1&table=Table119">1.7-1.95GeV</a> <a href="?version=1&table=Table120">6.7-7.65GeV</a> <a href="?version=1&table=Table121">20-23GeV</a> <br> 10-20%: <a href="?version=1&table=Table122">1.7-1.95GeV</a> <a href="?version=1&table=Table123">6.7-7.65GeV</a> <a href="?version=1&table=Table124">20-23GeV</a> <br> 20-30%: <a href="?version=1&table=Table125">1.7-1.95GeV</a> <a href="?version=1&table=Table126">6.7-7.65GeV</a> <a href="?version=1&table=Table127">20-23GeV</a> <br> 30-40%: <a href="?version=1&table=Table128">1.7-1.95GeV</a> <a href="?version=1&table=Table129">6.7-7.65GeV</a> <a href="?version=1&table=Table130">20-23GeV</a> <br> 40-50%: <a href="?version=1&table=Table131">1.7-1.95GeV</a> <a href="?version=1&table=Table132">6.7-7.65GeV</a> <a href="?version=1&table=Table133">20-23GeV</a> <br> 50-60%: <a href="?version=1&table=Table134">1.7-1.95GeV</a> <a href="?version=1&table=Table135">6.7-7.65GeV</a> <a href="?version=1&table=Table136">20-23GeV</a> <br> 60-80%: <a href="?version=1&table=Table137">1.7-1.95GeV</a> <a href="?version=1&table=Table138">6.7-7.65GeV</a> <a href="?version=1&table=Table139">20-23GeV</a> <br>- - - - - - - - - - - - - - - - - - - -
Charged-hadron cross-section in pp collisions. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 0-5% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 5-10% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 10-20% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 20-30% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 30-40% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 40-60% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 60-90% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 0-90% for p+Pb, divided by 〈TPPB〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron cross-section in pp collisions. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 0-5% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Charged-hadron spectrum in the centrality interval 5-10% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Charged-hadron spectrum in the centrality interval 10-20% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Charged-hadron spectrum in the centrality interval 20-30% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Charged-hadron spectrum in the centrality interval 30-40% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Charged-hadron spectrum in the centrality interval 40-50% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Charged-hadron spectrum in the centrality interval 50-60% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Charged-hadron spectrum in the centrality interval 60-80% for Pb+Pb, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Charged-hadron cross-section in pp collisions. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 0-5% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 5-10% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 10-20% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 20-30% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 30-40% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 40-50% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 50-60% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Charged-hadron spectrum in the centrality interval 60-80% for Xe+Xe, divided by 〈TAA〉. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-5% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 5-10% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 10-20% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 20-30% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 30-40% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 40-60% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 60-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-5% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Nuclear modification factor in centrality interval 5-10% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Nuclear modification factor in centrality interval 10-20% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Nuclear modification factor in centrality interval 20-30% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Nuclear modification factor in centrality interval 30-40% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Nuclear modification factor in centrality interval 40-50% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Nuclear modification factor in centrality interval 50-60% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Nuclear modification factor in centrality interval 60-80% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature. The systematic uncertainty on momentum bias is negligible at low pT; in such cases, it is omitted in the table below.
Nuclear modification factor in centrality interval 0-5% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 5-10% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 10-20% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 20-30% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 30-40% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 40-50% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 50-60% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 60-80% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-5% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-5% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-5% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-5% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 5-10% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 5-10% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 5-10% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 5-10% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 10-20% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 10-20% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 10-20% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 10-20% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 20-30% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 20-30% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 20-30% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 20-30% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 30-40% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 30-40% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 30-40% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 30-40% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 40-60% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 40-60% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 40-60% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 40-60% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 60-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 60-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 60-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 60-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-90% for p+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-5% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-5% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-5% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-5% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 5-10% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 5-10% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 5-10% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 5-10% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 10-20% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 10-20% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 10-20% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 10-20% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 20-30% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 20-30% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 20-30% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 20-30% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 30-40% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 30-40% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 30-40% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 30-40% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 40-50% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 40-50% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 40-50% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 40-50% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 50-60% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 50-60% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 50-60% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 50-60% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 60-80% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 60-80% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 60-80% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 60-80% for Pb+Pb. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-5% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-5% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 0-5% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 5-10% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 5-10% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 5-10% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 10-20% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 10-20% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 10-20% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 20-30% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 20-30% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 20-30% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 30-40% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 30-40% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 30-40% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 40-50% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 40-50% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 40-50% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 50-60% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 50-60% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 50-60% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 60-80% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 60-80% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Nuclear modification factor in centrality interval 60-80% for Xe+Xe. The systematic uncertainties are described in the section 7 of the paper. The total systematic uncertainties are determined by adding the contributions from all relevant sources in quadrature.
Parton energy loss in the quark-gluon plasma (QGP) is studied with a measurement of photon-tagged jet production in 1.7 nb$^{-1}$ of Pb+Pb data and 260 pb$^{-1}$ of $pp$ data, both at $\sqrt{s_\mathrm{NN}} = 5.02$ TeV, with the ATLAS detector. The process $pp \to \gamma$+jet+$X$ and its analogue in Pb+Pb collisions is measured in events containing an isolated photon with transverse momentum ($p_\mathrm{T}$) above $50$ GeV and reported as a function of jet $p_\mathrm{T}$. This selection results in a sample of jets with a steeply falling $p_\mathrm{T}$ distribution that are mostly initiated by the showering of quarks. The $pp$ and Pb+Pb measurements are used to report the nuclear modification factor, $R_\mathrm{AA}$, and the fractional energy loss, $S_\mathrm{loss}$, for photon-tagged jets. In addition, the results are compared with the analogous ones for inclusive jets, which have a significantly smaller quark-initiated fraction. The $R_\mathrm{AA}$ and $S_\mathrm{loss}$ values are found to be significantly different between those for photon-tagged jets and inclusive jets, demonstrating that energy loss in the QGP is sensitive to the colour-charge of the initiating parton. The results are also compared with a variety of theoretical models of colour-charge-dependent energy loss.
Correlations of two flow harmonics $v_n$ and $v_m$ via three- and four-particle cumulants are measured in 13 TeV $pp$, 5.02 TeV $p$+Pb, and 2.76 TeV peripheral Pb+Pb collisions with the ATLAS detector at the LHC. The goal is to understand the multi-particle nature of the long-range collective phenomenon in these collision systems. The large non-flow background from dijet production present in the standard cumulant method is suppressed using a method of subevent cumulants involving two, three and four subevents separated in pseudorapidity. The results show a negative correlation between $v_2$ and $v_3$ and a positive correlation between $v_2$ and $v_4$ for all collision systems and over the full multiplicity range. However, the magnitudes of the correlations are found to depend strongly on the event multiplicity, the choice of transverse momentum range and collision system. The relative correlation strength, obtained by normalisation of the cumulants with the $\langle v_n^2\rangle$ from a two-particle correlation analysis, is similar in the three collision systems and depends weakly on the event multiplicity and transverse momentum. These results based on the subevent methods provide strong evidence of a similar long-range multi-particle collectivity in $pp$, $p$+Pb and peripheral Pb+Pb collisions.
The correlations between flow harmonics $v_n$ for $n=2$, 3 and 4 and mean transverse momentum $[p_\mathrm{T}]$ in $^{129}$Xe+$^{129}$Xe and $^{208}$Pb+$^{208}$Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.44$ TeV and 5.02 TeV, respectively, are measured using charged particles with the ATLAS detector. The correlations are sensitive to the shape and size of the initial geometry, nuclear deformation, and initial momentum anisotropy. The effects from non-flow and centrality fluctuations are minimized, respectively, via a subevent cumulant method and event activity selection based on particle production in the very forward rapidity. The results show strong dependences on centrality, harmonic number $n$, $p_{\mathrm{T}}$ and pseudorapidity range. Current models describe qualitatively the overall centrality- and system-dependent trends but fail to quantitatively reproduce all the data. In the central collisions, where models generally show good agreement, the $v_2$-$[p_\mathrm{T}]$ correlations are sensitive to the triaxiality of the quadruple deformation. The comparison of model to the Pb+Pb and Xe+Xe data suggests that the $^{129}$Xe nucleus is a highly deformed triaxial ellipsoid that is neither a prolate nor an oblate shape. This provides strong evidence for a triaxial deformation of $^{129}$Xe nucleus using high-energy heavy-ion collision.
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Standard method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Two_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Standard method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Two_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Standard method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Two_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.3< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.3< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.3< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$Cov_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$Cov_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$Cov_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$Cov_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$Cov_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$Cov_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{2}$ for peripheral events, Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality,
$\rho_{2}$ for peripheral events, Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality,
$\rho_{2}$ for peripheral events, Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ for peripheral events, Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ for peripheral events, Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality,
$\rho_{2}$ for peripheral events, Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality,
$\rho_{2}$ for peripheral events, Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ for peripheral events, Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ for peripheral events, Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality,
$\rho_{2}$ for peripheral events, Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality,
$\rho_{2}$ for peripheral events, Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ for peripheral events, Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$, Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$, Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{3}$, Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{3}$, Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$, Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$, Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{3}$, Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{3}$, Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ for central events, Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ for central events, Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ for central events, Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ for central events, Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ ratio between Xe+Xe 5.44 TeV and Pb+Pb 5.02 TeV for central events, Three_subevent method, for , $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ ratio between Xe+Xe 5.44 TeV and Pb+Pb 5.02 TeV for central events, Three_subevent method, for , $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\Sigma E_{T}$ vs $N^{rec}_{ch}$ for Pb+Pb 5.02 TeV
$\Sigma E_{T}$ vs $N^{rec}_{ch}$ for Xe+Xe 5.44 TeV
$\rho_{2}$ ratio between Xe+Xe 5.44 TeV and Pb+Pb 5.02 TeV for central events, Standard method, for , $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ ratio between Xe+Xe 5.44 TeV and Pb+Pb 5.02 TeV for central events, Standard method, for , $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ ratio between Xe+Xe 5.44 TeV and Pb+Pb 5.02 TeV for central events, Combined_subevent method, for , $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ ratio between Xe+Xe 5.44 TeV and Pb+Pb 5.02 TeV for central events, Combined_subevent method, for , $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ ratio between Xe+Xe 5.44 TeV and Pb+Pb 5.02 TeV for central events, Three_subevent method, for , $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality,
$\rho_{2}$ ratio between Xe+Xe 5.44 TeV and Pb+Pb 5.02 TeV for central events, Three_subevent method, for , $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality,
$\rho_{2}$ ratio between Xe+Xe 5.44 TeV and Pb+Pb 5.02 TeV for central events, Combined_subevent method, for , $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality,
$\rho_{2}$ ratio between Xe+Xe 5.44 TeV and Pb+Pb 5.02 TeV for central events, Combined_subevent method, for , $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality,
$\rho_{3}$ for central events, Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{3}$ for central events, Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{3}$ for central events, Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{3}$ for central events, Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{3}$ ratio between Xe+Xe 5.44 TeV and Pb+Pb 5.02 TeV for central events, Standard method, for , $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{3}$ ratio between Xe+Xe 5.44 TeV and Pb+Pb 5.02 TeV for central events, Standard method, for , $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{3}$ ratio between Xe+Xe 5.44 TeV and Pb+Pb 5.02 TeV for central events, Combined_subevent method, for , $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{3}$ ratio between Xe+Xe 5.44 TeV and Pb+Pb 5.02 TeV for central events, Combined_subevent method, for , $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality,
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$\rho_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{2}$ Standard method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{2}$ Two_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{3}$ Standard method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{3}$ Two_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{3}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{4}$ Standard method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{4}$ Two_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{4}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$Cov_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Standard method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Two_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Standard method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Two_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Standard method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Two_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality.
$Cov_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{2}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{2}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{3}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{3}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{3}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{4}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{4}$ Two_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$Cov_{4}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$ based Centrality.
$c_{k}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$c_{k}$ Standard method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$var(v^{2}_{2})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$var(v^{2}_{2})$ Combined subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$var(v^{2}_{3})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$var(v^{2}_{3})$ Combined subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$var(v^{2}_{4})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$var(v^{2}_{4})$ Combined subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$c_{k}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$c_{k}$ Standard method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$var(v^{2}_{2})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$var(v^{2}_{2})$ Combined subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$var(v^{2}_{3})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$var(v^{2}_{3})$ Combined subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$var(v^{2}_{4})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$var(v^{2}_{4})$ Combined subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$c_{k}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$c_{k}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$var(v^{2}_{2})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$var(v^{2}_{2})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$var(v^{2}_{3})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$var(v^{2}_{3})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$var(v^{2}_{4})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$var(v^{2}_{4})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$.
$c_{k}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$c_{k}$ Standard method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$var(v^{2}_{2})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$var(v^{2}_{2})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$var(v^{2}_{3})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$var(v^{2}_{3})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$var(v^{2}_{4})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$var(v^{2}_{4})$ Combined subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N^{rec}_{ch}$.
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Pb+Pb 5.02 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <2.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<2.5, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <2.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{2}$ Three_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{3}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $\Sigma E_{T}$ based Centrality
$\rho_{4}$ Combined_subevent method, for Xe+Xe 5.44 TeV, $|\eta|$<1.0, 0.5< $p_{T}$ <5.0 GeV vs $N_{ch}^{rec}$ based Centrality
This paper presents a measurement of forward-forward and forward-central dijet azimuthal angular correlations and conditional yields in proton-proton ($pp$) and proton-lead ($p$+Pb) collisions as a probe of the nuclear gluon density in regions where the fraction of the average momentum per nucleon carried by the parton entering the hard scattering is low. In these regions, gluon saturation can modify the rapidly increasing parton distribution function of the gluon. The analysis utilizes 25 pb$^{-1}$ of $pp$ data and 360 $\mu \mathrm{b}^{-1}$ of $p$+Pb data, both at $\sqrt{s_{\rm NN}}$ = 5.02 TeV, collected in 2015 and 2016, respectively, with the ATLAS detector at the LHC. The measurement is performed in the center-of-mass frame of the nucleon-nucleon system in the rapidity range between $-$4.0 and 4.0 using the two highest transverse momentum jets in each event, with the highest transverse momentum jet restricted to the forward rapidity range. No significant broadening of azimuthal angular correlations is observed for forward-forward or forward-central dijets in $p$+Pb compared to $pp$ collisions. For forward-forward jet pairs in the proton-going direction, the ratio of conditional yields in $p$+Pb collisions to those in $pp$ collisions is suppressed by approximately 20%, with no significant dependence on the transverse momentum of the dijet system. No modification of conditional yields is observed for forward-central dijets.
Unfolded azimuthal angular correlation distributions. Black markers represent p+Pb, red markers p+p
Unfolded width of azimuthal angular correlation distributions. Full markers represent p+Pb, open markers p+p
Unfolded Dijet conditional yields. Full markers represent p+Pb, open markers p+p
Ratio of unfolded width of azimuthal angular correlation distributions (P PB/ P P). Different colors correspond to different combinations of p_{T,1} and p_{T,2}
Ratio of unfolded Dijet conditional yields (P PB/ P P). Different colors correspond to different combinations of p_{T,1} and p_{T,2}
Unfolded width of azimuthal angular correlation distributions (Delta p_{T} > 3). Full markers represent p+Pb, open markers p+p
Unfolded Dijet conditional yields (Delta p_{T} > 3). Full markers represent p+Pb, open markers p+p
Ratio of unfolded width of azimuthal angular correlation distributions (P PB/ P P) (Delta p_{T} > 3). Different colors correspond to different combinations of p_{T,1} and p_{T,2}
Ratio of unfolded Dijet conditional yields (P PB/ P P) (Delta p_{T} > 3). Different colors correspond to different combinations of p_{T,1} and p_{T,2}
Unfolded azimuthal angular correlation distributions. Black markers represent p+Pb, red markers p+p
Unfolded azimuthal angular correlation distributions (Delta p_{T} > 3). Black markers represent p+Pb, red markers p+p
Light-by-light scattering ($\gamma\gamma\rightarrow\gamma\gamma$) is a quantum-mechanical process that is forbidden in the classical theory of electrodynamics. This reaction is accessible at the Large Hadron Collider thanks to the large electromagnetic field strengths generated by ultra-relativistic colliding lead (Pb) ions. Using 480 $\mu$b$^{-1}$ of Pb+Pb collision data recorded at a centre-of-mass energy per nucleon pair of 5.02 TeV by the ATLAS detector, the ATLAS Collaboration reports evidence for the $\gamma\gamma\rightarrow\gamma\gamma$ reaction. A total of 13 candidate events are observed with an expected background of 2.6$\pm$0.7 events. After background subtraction and analysis corrections, the fiducial cross section of the process $\textrm{Pb+Pb}\,(\gamma\gamma)\rightarrow \textrm{Pb}^{(\ast)}\textrm{+}\textrm{Pb}^{(\ast)}\,\gamma\gamma$, for photon transverse energy $E_{\mathrm{T}}>$3 GeV, photon absolute pseudorapidity $|\eta|<$2.4, diphoton invariant mass greater than 6 GeV, diphoton transverse momentum lower than 2 GeV and diphoton acoplanarity below 0.01, is measured to be 70 $\pm$ 24 (stat.) $\pm$ 17 (syst.) nb, which is in agreement with Standard Model predictions.
Detector-level diphoton invariant mass distribution
Detector-level diphoton acoplanarity distribution
The measured total fiducial cross section
Exclusive dimuon production in ultraperipheral collisions (UPC), resulting from photon-photon interactions in the strong electromagnetic fields of colliding high-energy lead nuclei, $\mathrm{PbPb}(\gamma\gamma) \rightarrow \mu^+\mu^- (\mathrm{Pb}^{(\star)}\mathrm{Pb}^{(\star)} )$, is studied using $\mathcal{L}_{\mathrm{int}} = 0.48$ nb$^{-1}$ of $\sqrt{s_\mathrm{NN}}=5.02$ TeV lead-lead collision data at the LHC with the ATLAS detector. Dimuon pairs are measured in the fiducial region $p_{\mathrm{T}\mu} > 4$ GeV, $|\eta_{\mu}| < 2.4$, invariant mass $m_{\mu\mu} > 10$ GeV, and $p_{\mathrm{T,\mu\mu}} < 2$ GeV. The primary background from single-dissociative processes is extracted from the data using a template fitting technique. Differential cross sections are presented as a function of $m_{\mu\mu}$, absolute pair rapidity ($|y_{\mu\mu}|$), scattering angle in the dimuon rest frame ($|\cos \vartheta^{\star}_{\mu\mu}|$) and the colliding photon energies. The total cross section of the UPC $\gamma \gamma \rightarrow \mu^{+}\mu^{-}$ process in the fiducial volume is measured to be $\sigma_{\mathrm{fid}}^{\mu\mu} = 34.1 \! \pm \! 0.3 \mathrm{(stat.)} \! \pm \! 0.7 \mathrm{(syst.)}$ $\mu\mathrm{b}$. Generally good agreement is found with calculations from STARlight, which incorporate the leading-order Breit-Wheeler process with no final-state effects, albeit differences between the measurements and theoretical expectations are observed. In particular, the measured cross sections at larger $|y_{\mu\mu}|$ are found to be about 10-20% larger in data than in the calculations, suggesting the presence of larger fluxes of photons in the initial state. Modification of the dimuon cross sections in the presence of forward and/or backward neutron production is also studied and is found to be associated with a harder incoming photon spectrum, consistent with expectations.
Multi-particle azimuthal cumulants are measured as a function of centrality and transverse momentum using 470 $\mu$b$^{-1}$ of Pb+Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$ TeV with the ATLAS detector at the LHC. These cumulants provide information on the event-by-event fluctuations of harmonic flow coefficients $v_n$ and correlated fluctuations between two harmonics $v_n$ and $v_m$. For the first time, a non-zero four-particle cumulant is observed for dipolar flow, $v_1$. The four-particle cumulants for elliptic flow, $v_2$, and triangular flow, $v_3$, exhibit a strong centrality dependence and change sign in ultra-central collisions. This sign change is consistent with significant non-Gaussian fluctuations in $v_2$ and $v_3$. The four-particle cumulant for quadrangular flow, $v_4$, is found to change sign in mid-central collisions. Correlations between two harmonics are studied with three- and four-particle mixed-harmonic cumulants, which indicate an anti-correlation between $v_2$ and $v_3$, and a positive correlation between $v_2$ and $v_4$. These correlations decrease in strength towards central collisions and either approach zero or change sign in ultra-central collisions. To investigate the possible flow fluctuations arising from intrinsic centrality or volume fluctuations, the results are compared between two different event classes used for centrality definitions. In peripheral and mid-central collisions where the cumulant signals are large, only small differences are observed. In ultra-central collisions, the differences are much larger and transverse momentum dependent. These results provide new information to disentangle flow fluctuations from the initial and final states, as well as new insights on the influence of centrality fluctuations.
NchRec v.s. Et
<NchRec> w.r.t. Et
<Et> w.r.t. NchRec
Et distribution
NchRec distribution
v_2{2}, 3-subevent, 0.5<pT<5.0 GeV
v_2{2}, 3-subevent, 1.0<pT<5.0 GeV
v_2{2}, 3-subevent, 1.5<pT<5.0 GeV
v_2{2}, 3-subevent, 2.0<pT<5.0 GeV
v_3{2}, 3-subevent, 0.5<pT<5.0 GeV
v_3{2}, 3-subevent, 1.0<pT<5.0 GeV
v_3{2}, 3-subevent, 1.5<pT<5.0 GeV
v_3{2}, 3-subevent, 2.0<pT<5.0 GeV
v_4{2}, 3-subevent, 0.5<pT<5.0 GeV
v_4{2}, 3-subevent, 1.0<pT<5.0 GeV
v_4{2}, 3-subevent, 1.5<pT<5.0 GeV
v_4{2}, 3-subevent, 2.0<pT<5.0 GeV
nc_2{4}, standard, 0.5<pT<5.0 GeV
nc_2{4}, standard, 1.0<pT<5.0 GeV
nc_2{4}, standard, 1.5<pT<5.0 GeV
nc_2{4}, standard, 2.0<pT<5.0 GeV
nc_3{4}, standard, 0.5<pT<5.0 GeV
nc_3{4}, standard, 1.0<pT<5.0 GeV
nc_3{4}, standard, 1.5<pT<5.0 GeV
nc_3{4}, standard, 2.0<pT<5.0 GeV
nc_4{4}, standard, 0.5<pT<5.0 GeV
nc_4{4}, standard, 1.0<pT<5.0 GeV
nc_4{4}, standard, 1.5<pT<5.0 GeV
nc_4{4}, standard, 2.0<pT<5.0 GeV
nc_2{4}, 3-subevent, 0.5<pT<5.0 GeV
nc_2{4}, 3-subevent, 1.0<pT<5.0 GeV
nc_2{4}, 3-subevent, 1.5<pT<5.0 GeV
nc_2{4}, 3-subevent, 2.0<pT<5.0 GeV
nc_3{4}, 3-subevent, 0.5<pT<5.0 GeV
nc_3{4}, 3-subevent, 1.0<pT<5.0 GeV
nc_3{4}, 3-subevent, 1.5<pT<5.0 GeV
nc_3{4}, 3-subevent, 2.0<pT<5.0 GeV
nc_4{4}, 3-subevent, 0.5<pT<5.0 GeV
nc_4{4}, 3-subevent, 1.0<pT<5.0 GeV
nc_4{4}, 3-subevent, 1.5<pT<5.0 GeV
nc_4{4}, 3-subevent, 2.0<pT<5.0 GeV
v_2{4} / v_2{2}, standard, 0.5<pT<5.0 GeV
v_2{4} / v_2{2}, standard, 1.0<pT<5.0 GeV
v_2{4} / v_2{2}, standard, 1.5<pT<5.0 GeV
v_2{4} / v_2{2}, standard, 2.0<pT<5.0 GeV
v_3{4} / v_3{2}, standard, 0.5<pT<5.0 GeV
v_3{4} / v_3{2}, standard, 1.0<pT<5.0 GeV
v_3{4} / v_3{2}, standard, 1.5<pT<5.0 GeV
v_3{4} / v_3{2}, standard, 2.0<pT<5.0 GeV
v_4{4} / v_4{2}, standard, 0.5<pT<5.0 GeV
v_4{4} / v_4{2}, standard, 1.0<pT<5.0 GeV
v_4{4} / v_4{2}, standard, 1.5<pT<5.0 GeV
v_4{4} / v_4{2}, standard, 2.0<pT<5.0 GeV
nc_2{6}, standard, 0.5<pT<5.0 GeV
nc_2{6}, standard, 1.0<pT<5.0 GeV
nc_2{6}, standard, 1.5<pT<5.0 GeV
nc_2{6}, standard, 2.0<pT<5.0 GeV
nc_3{6}, standard, 0.5<pT<5.0 GeV
nc_3{6}, standard, 1.0<pT<5.0 GeV
nc_3{6}, standard, 1.5<pT<5.0 GeV
nc_3{6}, standard, 2.0<pT<5.0 GeV
nc_4{6}, standard, 0.5<pT<5.0 GeV
nc_4{6}, standard, 1.0<pT<5.0 GeV
nc_4{6}, standard, 1.5<pT<5.0 GeV
nc_4{6}, standard, 2.0<pT<5.0 GeV
v_2{6} / v_2{4}, standard, 0.5<pT<5.0 GeV
v_2{6} / v_2{4}, standard, 1.0<pT<5.0 GeV
v_2{6} / v_2{4}, standard, 1.5<pT<5.0 GeV
v_2{6} / v_2{4}, standard, 2.0<pT<5.0 GeV
c_1{4}, standard, 0.5<pT<5.0 GeV
c_1{4}, standard, 1.0<pT<5.0 GeV
c_1{4}, standard, 1.5<pT<5.0 GeV
c_1{4}, standard, 2.0<pT<5.0 GeV
c_1{4}, 3-subevent, 0.5<pT<5.0 GeV
c_1{4}, 3-subevent, 1.0<pT<5.0 GeV
c_1{4}, 3-subevent, 1.5<pT<5.0 GeV
c_1{4}, 3-subevent, 2.0<pT<5.0 GeV
v_1{4}, standard, 1.5<pT<5.0 GeV
v_1{4}, standard, 2.0<pT<5.0 GeV
v_1{4}, 3-subevent, 1.5<pT<5.0 GeV
v_1{4}, 3-subevent, 2.0<pT<5.0 GeV
nsc_2_3{4}, standard, 0.5<pT<5.0 GeV
nsc_2_3{4}, standard, 1.0<pT<5.0 GeV
nsc_2_3{4}, standard, 1.5<pT<5.0 GeV
nsc_2_3{4}, standard, 2.0<pT<5.0 GeV
nsc_2_3{4}, 3-subevent, 0.5<pT<5.0 GeV
nsc_2_3{4}, 3-subevent, 1.0<pT<5.0 GeV
nsc_2_3{4}, 3-subevent, 1.5<pT<5.0 GeV
nsc_2_3{4}, 3-subevent, 2.0<pT<5.0 GeV
nsc_2_4{4}, standard, 0.5<pT<5.0 GeV
nsc_2_4{4}, standard, 1.0<pT<5.0 GeV
nsc_2_4{4}, standard, 1.5<pT<5.0 GeV
nsc_2_4{4}, standard, 2.0<pT<5.0 GeV
nsc_2_4{4}, 3-subevent, 0.5<pT<5.0 GeV
nsc_2_4{4}, 3-subevent, 1.0<pT<5.0 GeV
nsc_2_4{4}, 3-subevent, 1.5<pT<5.0 GeV
nsc_2_4{4}, 3-subevent, 2.0<pT<5.0 GeV
nac_2{3}, standard, 0.5<pT<5.0 GeV
nac_2{3}, standard, 1.0<pT<5.0 GeV
nac_2{3}, standard, 1.5<pT<5.0 GeV
nac_2{3}, standard, 2.0<pT<5.0 GeV
nac_2{3}, 3-subevent, 0.5<pT<5.0 GeV
nac_2{3}, 3-subevent, 1.0<pT<5.0 GeV
nac_2{3}, 3-subevent, 1.5<pT<5.0 GeV
nac_2{3}, 3-subevent, 2.0<pT<5.0 GeV
v_2{2, Et}, 3-subevent, 0.5<pT<5.0 GeV
v_2{2, Et}, 3-subevent, 1.0<pT<5.0 GeV
v_2{2, Et}, 3-subevent, 1.5<pT<5.0 GeV
v_2{2, Et}, 3-subevent, 2.0<pT<5.0 GeV
v_3{2, Et}, 3-subevent, 0.5<pT<5.0 GeV
v_3{2, Et}, 3-subevent, 1.0<pT<5.0 GeV
v_3{2, Et}, 3-subevent, 1.5<pT<5.0 GeV
v_3{2, Et}, 3-subevent, 2.0<pT<5.0 GeV
v_4{2, Et}, 3-subevent, 0.5<pT<5.0 GeV
v_4{2, Et}, 3-subevent, 1.0<pT<5.0 GeV
v_4{2, Et}, 3-subevent, 1.5<pT<5.0 GeV
v_4{2, Et}, 3-subevent, 2.0<pT<5.0 GeV
v_2{2, Nch}, 3-subevent, 0.5<pT<5.0 GeV
v_2{2, Nch}, 3-subevent, 1.0<pT<5.0 GeV
v_2{2, Nch}, 3-subevent, 1.5<pT<5.0 GeV
v_2{2, Nch}, 3-subevent, 2.0<pT<5.0 GeV
v_3{2, Nch}, 3-subevent, 0.5<pT<5.0 GeV
v_3{2, Nch}, 3-subevent, 1.0<pT<5.0 GeV
v_3{2, Nch}, 3-subevent, 1.5<pT<5.0 GeV
v_3{2, Nch}, 3-subevent, 2.0<pT<5.0 GeV
v_4{2, Nch}, 3-subevent, 0.5<pT<5.0 GeV
v_4{2, Nch}, 3-subevent, 1.0<pT<5.0 GeV
v_4{2, Nch}, 3-subevent, 1.5<pT<5.0 GeV
v_4{2, Nch}, 3-subevent, 2.0<pT<5.0 GeV
v_2{2, Nch} / v_2{2, Et}, 3-subevent, 0.5<pT<5.0 GeV
v_2{2, Nch} / v_2{2, Et}, 3-subevent, 2.0<pT<5.0 GeV
v_3{2, Nch} / v_3{2, Et}, 3-subevent, 0.5<pT<5.0 GeV
v_3{2, Nch} / v_3{2, Et}, 3-subevent, 2.0<pT<5.0 GeV
v_4{2, Nch} / v_4{2, Et}, 3-subevent, 0.5<pT<5.0 GeV
v_4{2, Nch} / v_4{2, Et}, 3-subevent, 2.0<pT<5.0 GeV
v_2{2, Nch} / v_2{2, Et}, 3-subevent, 0.5<pT<5.0 GeV
v_2{2, Nch} / v_2{2, Et}, 3-subevent, 2.0<pT<5.0 GeV
v_3{2, Nch} / v_3{2, Et}, 3-subevent, 0.5<pT<5.0 GeV
v_3{2, Nch} / v_3{2, Et}, 3-subevent, 2.0<pT<5.0 GeV
v_4{2, Nch} / v_4{2, Et}, 3-subevent, 0.5<pT<5.0 GeV
v_4{2, Nch} / v_4{2, Et}, 3-subevent, 2.0<pT<5.0 GeV
nc_2{4, Et}, standard, 0.5<pT<5.0 GeV
nc_2{4, Et}, standard, 1.0<pT<5.0 GeV
nc_2{4, Et}, standard, 1.5<pT<5.0 GeV
nc_2{4, Et}, standard, 2.0<pT<5.0 GeV
nc_3{4, Et}, standard, 0.5<pT<5.0 GeV
nc_3{4, Et}, standard, 1.0<pT<5.0 GeV
nc_3{4, Et}, standard, 1.5<pT<5.0 GeV
nc_3{4, Et}, standard, 2.0<pT<5.0 GeV
nc_4{4, Et}, standard, 0.5<pT<5.0 GeV
nc_4{4, Et}, standard, 1.0<pT<5.0 GeV
nc_4{4, Et}, standard, 1.5<pT<5.0 GeV
nc_4{4, Et}, standard, 2.0<pT<5.0 GeV
nc_2{4, Nch}, standard, 0.5<pT<5.0 GeV
nc_2{4, Nch}, standard, 1.0<pT<5.0 GeV
nc_2{4, Nch}, standard, 1.5<pT<5.0 GeV
nc_2{4, Nch}, standard, 2.0<pT<5.0 GeV
nc_3{4, Nch}, standard, 0.5<pT<5.0 GeV
nc_3{4, Nch}, standard, 1.0<pT<5.0 GeV
nc_3{4, Nch}, standard, 1.5<pT<5.0 GeV
nc_3{4, Nch}, standard, 2.0<pT<5.0 GeV
nc_4{4, Nch}, standard, 0.5<pT<5.0 GeV
nc_4{4, Nch}, standard, 1.0<pT<5.0 GeV
nc_4{4, Nch}, standard, 1.5<pT<5.0 GeV
nc_4{4, Nch}, standard, 2.0<pT<5.0 GeV
nc_2{4, Et}, standard, 1.5<pT<5.0 GeV
nc_2{4, Nch}, standard, 1.5<pT<5.0 GeV
nc_3{4, Et}, standard, 1.5<pT<5.0 GeV
nc_3{4, Nch}, standard, 1.5<pT<5.0 GeV
nc_4{4, Et}, standard, 1.5<pT<5.0 GeV
nc_4{4, Nch}, standard, 1.5<pT<5.0 GeV
nc_2{6, Et}, standard, 0.5<pT<5.0 GeV
nc_2{6, Et}, standard, 1.0<pT<5.0 GeV
nc_2{6, Et}, standard, 1.5<pT<5.0 GeV
nc_2{6, Et}, standard, 2.0<pT<5.0 GeV
nc_2{6, Nch}, standard, 0.5<pT<5.0 GeV
nc_2{6, Nch}, standard, 1.0<pT<5.0 GeV
nc_2{6, Nch}, standard, 1.5<pT<5.0 GeV
nc_2{6, Nch}, standard, 2.0<pT<5.0 GeV
nc_2{6, Et}, standard, 1.5<pT<5.0 GeV
nc_2{6, Nch}, standard, 1.5<pT<5.0 GeV
v_2{6, Et} / v_2{4, Et}, standard, 0.5<pT<5.0 GeV
v_2{6, Et} / v_2{4, Et}, standard, 1.0<pT<5.0 GeV
v_2{6, Et} / v_2{4, Et}, standard, 1.5<pT<5.0 GeV
v_2{6, Et} / v_2{4, Et}, standard, 2.0<pT<5.0 GeV
v_2{6, Nch} / v_2{4, Nch}, standard, 0.5<pT<5.0 GeV
v_2{6, Nch} / v_2{4, Nch}, standard, 1.0<pT<5.0 GeV
v_2{6, Nch} / v_2{4, Nch}, standard, 1.5<pT<5.0 GeV
v_2{6, Nch} / v_2{4, Nch}, standard, 2.0<pT<5.0 GeV
nsc_2_3{4, Et}, standard, 0.5<pT<5.0 GeV
nsc_2_3{4, Et}, standard, 1.0<pT<5.0 GeV
nsc_2_3{4, Et}, standard, 1.5<pT<5.0 GeV
nsc_2_3{4, Et}, standard, 2.0<pT<5.0 GeV
nsc_2_4{4, Et}, standard, 0.5<pT<5.0 GeV
nsc_2_4{4, Et}, standard, 1.0<pT<5.0 GeV
nsc_2_4{4, Et}, standard, 1.5<pT<5.0 GeV
nsc_2_4{4, Et}, standard, 2.0<pT<5.0 GeV
nac_2{3, Et}, standard, 0.5<pT<5.0 GeV
nac_2{3, Et}, standard, 1.0<pT<5.0 GeV
nac_2{3, Et}, standard, 1.5<pT<5.0 GeV
nac_2{3, Et}, standard, 2.0<pT<5.0 GeV
nsc_2_3{4, Nch}, standard, 0.5<pT<5.0 GeV
nsc_2_3{4, Nch}, standard, 1.0<pT<5.0 GeV
nsc_2_3{4, Nch}, standard, 1.5<pT<5.0 GeV
nsc_2_3{4, Nch}, standard, 2.0<pT<5.0 GeV
nsc_2_4{4, Nch}, standard, 0.5<pT<5.0 GeV
nsc_2_4{4, Nch}, standard, 1.0<pT<5.0 GeV
nsc_2_4{4, Nch}, standard, 1.5<pT<5.0 GeV
nsc_2_4{4, Nch}, standard, 2.0<pT<5.0 GeV
nac_2{3, Nch}, standard, 0.5<pT<5.0 GeV
nac_2{3, Nch}, standard, 1.0<pT<5.0 GeV
nac_2{3, Nch}, standard, 1.5<pT<5.0 GeV
nac_2{3, Nch}, standard, 2.0<pT<5.0 GeV
nsc_2_3{4, Et}, standard, 1.5<pT<5.0 GeV
nsc_2_3{4, Nch}, standard, 1.5<pT<5.0 GeV
nsc_2_4{4, Et}, standard, 1.5<pT<5.0 GeV
nsc_2_4{4, Nch}, standard, 1.5<pT<5.0 GeV
nac_2{3, Et}, standard, 1.5<pT<5.0 GeV
nac_2{3, Nch}, standard, 1.5<pT<5.0 GeV
v_2{4}, standard, 0.5<pT<5.0 GeV
v_2{4}, standard, 1.0<pT<5.0 GeV
v_2{4}, standard, 1.5<pT<5.0 GeV
v_2{4}, standard, 2.0<pT<5.0 GeV
v_2{4, Et}, standard, 0.5<pT<5.0 GeV
v_2{4, Et}, standard, 1.0<pT<5.0 GeV
v_2{4, Et}, standard, 1.5<pT<5.0 GeV
v_2{4, Et}, standard, 2.0<pT<5.0 GeV
v_2{4, Nch}, standard, 0.5<pT<5.0 GeV
v_2{4, Nch}, standard, 1.0<pT<5.0 GeV
v_2{4, Nch}, standard, 1.5<pT<5.0 GeV
v_2{4, Nch}, standard, 2.0<pT<5.0 GeV
v_3{4}, standard, 0.5<pT<5.0 GeV
v_3{4}, standard, 1.0<pT<5.0 GeV
v_3{4}, standard, 1.5<pT<5.0 GeV
v_3{4}, standard, 2.0<pT<5.0 GeV
v_3{4, Et}, standard, 0.5<pT<5.0 GeV
v_3{4, Et}, standard, 1.0<pT<5.0 GeV
v_3{4, Et}, standard, 1.5<pT<5.0 GeV
v_3{4, Et}, standard, 2.0<pT<5.0 GeV
v_3{4, Nch}, standard, 0.5<pT<5.0 GeV
v_3{4, Nch}, standard, 1.0<pT<5.0 GeV
v_3{4, Nch}, standard, 1.5<pT<5.0 GeV
v_3{4, Nch}, standard, 2.0<pT<5.0 GeV
v_4{4}, standard, 0.5<pT<5.0 GeV
v_4{4}, standard, 1.0<pT<5.0 GeV
v_4{4}, standard, 1.5<pT<5.0 GeV
v_4{4}, standard, 2.0<pT<5.0 GeV
v_4{4, Et}, standard, 0.5<pT<5.0 GeV
v_4{4, Et}, standard, 1.0<pT<5.0 GeV
v_4{4, Et}, standard, 1.5<pT<5.0 GeV
v_4{4, Et}, standard, 2.0<pT<5.0 GeV
v_4{4, Nch}, standard, 0.5<pT<5.0 GeV
v_4{4, Nch}, standard, 1.0<pT<5.0 GeV
v_4{4, Nch}, standard, 1.5<pT<5.0 GeV
v_4{4, Nch}, standard, 2.0<pT<5.0 GeV
v_2{6}, standard, 0.5<pT<5.0 GeV
v_2{6}, standard, 1.0<pT<5.0 GeV
v_2{6}, standard, 1.5<pT<5.0 GeV
v_2{6}, standard, 2.0<pT<5.0 GeV
v_2{6, Et}, standard, 0.5<pT<5.0 GeV
v_2{6, Et}, standard, 1.0<pT<5.0 GeV
v_2{6, Et}, standard, 1.5<pT<5.0 GeV
v_2{6, Et}, standard, 2.0<pT<5.0 GeV
v_2{6, Nch}, standard, 0.5<pT<5.0 GeV
v_2{6, Nch}, standard, 1.0<pT<5.0 GeV
v_2{6, Nch}, standard, 1.5<pT<5.0 GeV
v_2{6, Nch}, standard, 2.0<pT<5.0 GeV
sc_2_3{4}, standard, 0.5<pT<5.0 GeV
sc_2_3{4}, standard, 1.0<pT<5.0 GeV
sc_2_3{4}, standard, 1.5<pT<5.0 GeV
sc_2_3{4}, standard, 2.0<pT<5.0 GeV
sc_2_3{4}, 3-subevent, 0.5<pT<5.0 GeV
sc_2_3{4}, 3-subevent, 1.0<pT<5.0 GeV
sc_2_3{4}, 3-subevent, 1.5<pT<5.0 GeV
sc_2_3{4}, 3-subevent, 2.0<pT<5.0 GeV
sc_2_4{4}, standard, 0.5<pT<5.0 GeV
sc_2_4{4}, standard, 1.0<pT<5.0 GeV
sc_2_4{4}, standard, 1.5<pT<5.0 GeV
sc_2_4{4}, standard, 2.0<pT<5.0 GeV
sc_2_4{4}, 3-subevent, 0.5<pT<5.0 GeV
sc_2_4{4}, 3-subevent, 1.0<pT<5.0 GeV
sc_2_4{4}, 3-subevent, 1.5<pT<5.0 GeV
sc_2_4{4}, 3-subevent, 2.0<pT<5.0 GeV
ac_2{3}, standard, 0.5<pT<5.0 GeV
ac_2{3}, standard, 1.0<pT<5.0 GeV
ac_2{3}, standard, 1.5<pT<5.0 GeV
ac_2{3}, standard, 2.0<pT<5.0 GeV
ac_2{3}, 3-subevent, 0.5<pT<5.0 GeV
ac_2{3}, 3-subevent, 1.0<pT<5.0 GeV
ac_2{3}, 3-subevent, 1.5<pT<5.0 GeV
ac_2{3}, 3-subevent, 2.0<pT<5.0 GeV
Measurements of inclusive jet suppression in heavy ion collisions at the LHC provide direct sensitivity to the physics of jet quenching. In a sample of lead-lead collisions at $\sqrt{s_{NN}}$ = 2.76 TeV corresponding to an integrated luminosity of approximately 7 inverse microbarns, ATLAS has measured jets with a calorimeter over the pseudorapidity interval |$\eta$| < 2.1 and over the transverse momentum range 38 < pT < 210 GeV. Jets were reconstructed using the anti-$k_t$ algorithm with values for the distance parameter that determines the nominal jet radius of R = 0.2, 0.3, 0.4 and 0.5. The centrality dependence of the jet yield is characterized by the jet "central-to-peripheral ratio," $R_{cp}$. Jet production is found to be suppressed by approximately a factor of two in the 10% most central collisions relative to peripheral collisions. $R_{cp}$ varies smoothly with centrality as characterized by the number of participating nucleons. The observed suppression is only weakly dependent on jet radius and transverse momentum. These results provide the first direct measurement of inclusive jet suppression in heavy ion collisions and complement previous measurements of dijet transverse energy imbalance at the LHC.
Glauber model calculation of the mean numbers of Npart and its associated errors, the mean Ncoll ratios, and Rcoll with fractional errors as a function of the centrality bins.
The Rcp values as a function of jet PT for the four R values, 0.2, 0.3, 0.4 and 0.5 for the collision centrality in the range 0 - 10 %.
The Rcp values as a function of jet PT for the four R values, 0.2, 0.3, 0.4 and 0.5 for the collision centrality in the range 10 - 20 %.
The Rcp values as a function of jet PT for the four R values, 0.2, 0.3, 0.4 and 0.5 for the collision centrality in the range 20 - 30 %.
The Rcp values as a function of jet PT for the four R values, 0.2, 0.3, 0.4 and 0.5 for the collision centrality in the range 30 - 40 %.
The Rcp values as a function of jet PT for the four R values, 0.2, 0.3, 0.4 and 0.5 for the collision centrality in the range 40 - 50 %.
The Rcp values as a function of jet PT for the four R values, 0.2, 0.3, 0.4 and 0.5 for the collision centrality in the range 50 - 60 %.
The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 38.36 - 44.21 GeV.
The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 44.21 - 50.94 GeV.
The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 50.94 - 58.70 GeV.
The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 58.70 - 67.64 GeV.
The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 67.64 - 77.94 GeV.
The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 77.94 - 89.81 GeV.
The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 89.81 - 103.5 GeV.
The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 103.5 - 119.3 GeV.
The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 119.3 - 137.4 GeV.
The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 137.4 - 158.3 GeV.
The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 158.3 - 182.5 GeV.
The Rcp values as a function of the mean number of participating nucleons, NPART, for the four R values, 0.2, 0.3, 0.4 and 0.5 for the jet PT range 182.5 - 210.3 GeV.
The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 38.36 - 44.21 GeV.
The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 38.36 - 44.21 GeV.
The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 44.21 - 50.94 GeV.
The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 44.21 - 50.94 GeV.
The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 50.94 - 58.70 GeV.
The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 50.94 - 58.70 GeV.
The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 58.70 - 67.64 GeV.
The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 58.70 - 67.64 GeV.
The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 67.64 - 77.94 GeV.
The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 67.64 - 77.94 GeV.
The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 77.94 - 89.81 GeV.
The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 77.94 - 89.81 GeV.
The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 89.81 - 103.5 GeV.
The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 89.81 - 103.5 GeV.
The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 103.5 - 119.3 GeV.
The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 103.5 - 119.3 GeV.
The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 119.3 - 137.4 GeV.
The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 119.3 - 137.4 GeV.
The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 137.4 - 158.3 GeV.
The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 137.4 - 158.3 GeV.
The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 158.3 - 182.5 GeV.
The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 158.3 - 182.5 GeV.
The Rcp values as a function of R for the three centrality ranges 0 - 10 %, 10 - 20 % and 20 - 30 % for the jet PT range 182.5 - 210.3 GeV.
The Rcp values as a function of R for the three centrality ranges 30 - 40 %, 40 - 50 % and 50 - 60 % for the jet PT range 182.5 - 210.3 GeV.
The ratios of Rcp between R=0.3, 0.4 and 0.5 and R=0.2 jets as a function of the jet PT for the centrality range 0 - 10 %.
The ratios of Rcp between R=0.3, 0.4 and 0.5 and R=0.2 jets as a function of the jet PT for the centrality range 10 - 20 %.
The ratios of Rcp between R=0.3, 0.4 and 0.5 and R=0.2 jets as a function of the jet PT for the centrality range 20 - 30 %.
The ratios of Rcp between R=0.3, 0.4 and 0.5 and R=0.2 jets as a function of the jet PT for the centrality range 30 - 40 %.
The ratios of Rcp between R=0.3, 0.4 and 0.5 and R=0.2 jets as a function of the jet PT for the centrality range 40 - 50 %.
The ratios of Rcp between R=0.3, 0.4 and 0.5 and R=0.2 jets as a function of the jet PT for the centrality range 50 - 60 %.
The covariance matrix for statistcal correlations for R = 0.2 and centrality range 0 - 10 %.
The covariance matrix for statistcal correlations for R = 0.3 and centrality range 0 - 10 %.
The covariance matrix for statistcal correlations for R = 0.4 and centrality range 0 - 10 %.
The covariance matrix for statistcal correlations for R = 0.5 and centrality range 0 - 10 %.
The covariance matrix for statistcal correlations for R = 0.2 and centrality range 10 - 20 %.
The covariance matrix for statistcal correlations for R = 0.3 and centrality range 10 - 20 %.
The covariance matrix for statistcal correlations for R = 0.4 and centrality range 10 - 20 %.
The covariance matrix for statistcal correlations for R = 0.5 and centrality range 10 - 20 %.
The covariance matrix for statistcal correlations for R = 0.2 and centrality range 20 - 30 %.
The covariance matrix for statistcal correlations for R = 0.3 and centrality range 20 - 30 %.
The covariance matrix for statistcal correlations for R = 0.4 and centrality range 20 - 30 %.
The covariance matrix for statistcal correlations for R = 0.5 and centrality range 20 - 30 %.
The covariance matrix for statistcal correlations for R = 0.2 and centrality range 30 - 40 %.
The covariance matrix for statistcal correlations for R = 0.3 and centrality range 30 - 40 %.
The covariance matrix for statistcal correlations for R = 0.4 and centrality range 30 - 40 %.
The covariance matrix for statistcal correlations for R = 0.5 and centrality range 30 - 40 %.
The covariance matrix for statistcal correlations for R = 0.2 and centrality range 40 - 50 %.
The covariance matrix for statistcal correlations for R = 0.3 and centrality range 40 - 50 %.
The covariance matrix for statistcal correlations for R = 0.4 and centrality range 40 - 50 %.
The covariance matrix for statistcal correlations for R = 0.5 and centrality range 40 - 50 %.
The covariance matrix for statistcal correlations for R = 0.2 and centrality range 50 - 60 %.
The covariance matrix for statistcal correlations for R = 0.3 and centrality range 50 - 60 %.
The covariance matrix for statistcal correlations for R = 0.4 and centrality range 50 - 60 %.
The covariance matrix for statistcal correlations for R = 0.5 and centrality range 50 - 60 %.
A measurement of $W^\pm$ boson production in lead-lead collisions at $\sqrt{s_\mathrm{NN}} = 5.02$ TeV is reported using data recorded by the ATLAS experiment at the LHC in 2015, corresponding to a total integrated luminosity of $0.49\;\mathrm{nb^{-1}}$. The $W^\pm$ bosons are reconstructed in the electron or muon leptonic decay channels. Production yields of leptonically decaying $W^\pm$ bosons, normalised by the total number of minimum-bias events and the nuclear thickness function, are measured within a fiducial region defined by the detector acceptance and the main kinematic requirements. These normalised yields are measured separately for $W^+$ and $W^-$ bosons, and are presented as a function of the absolute value of pseudorapidity of the charged lepton and of the collision centrality. The lepton charge asymmetry is also measured as a function of the absolute value of lepton pseudorapidity. In addition, nuclear modification factors are calculated using the $W^\pm$ boson production cross-sections measured in $pp$ collisions. The results are compared with predictions based on next-to-leading-order calculations with CT14 parton distribution functions as well as with predictions obtained with the EPPS16 and nCTEQ15 nuclear parton distribution functions. No dependence of normalised production yields on centrality and a good agreement with predictions are observed for mid-central and central collisions. For peripheral collisions, the data agree with predictions within 1.7 (0.9) standard deviations for $W^-$ ($W^+$) bosons.
Differential normalised production yields for $W^+$ bosons as a function of absolute pseudorapidity of the charged lepton for the combined electron and muon channels. Systematic uncertainties related to $T_{\mathrm{AA}}$ are not included.
Differential normalised production yields for $W^-$ bosons as a function of absolute pseudorapidity of the charged lepton for the combined electron and muon channels. Systematic uncertainties related to $T_{\mathrm{AA}}$ are not included.
Combined result for lepton charge asymmetry.
Normalised production yields of $W^+$ and $W^-$ bosons as a function of $⟨N_{\mathrm{part}}⟩$ shown for the combination of electron and muon decay channels.
Normalised production yields for $W^+$ bosons as a function of $⟨N_{\mathrm{part}}⟩$ for geometric parameters obtained with the MCGlauber v2.4 and v3.2.
Normalised production yields for $W^-$ bosons as a function of $⟨N_{\mathrm{part}}⟩$ for geometric parameters obtained with the MCGlauber v2.4 and v3.2.
Nuclear modification factor $R_{\mathrm{AA}}$ obtained from the fiducial $W^+$ and $W^-$ boson production yields as a function of $⟨N_{\mathrm{part}}⟩$.
The covariance matrix of the differential normalised production yields for $W^+$ bosons. Systematic uncertainties related to $T_{\mathrm{AA}}$ (1.6%) are not included.
The covariance matrix of the differential normalised production yields for $W^-$ bosons. Systematic uncertainties related to $T_{\mathrm{AA}}$ (1.6%) are not included.
The covariance matrix of the lepton charge asymmetry.
The ATLAS experiment has observed 1995 Z boson candidates in data corresponding to 0.15 inverse nb of integrated luminosity obtained in the 2011 LHC Pb+Pb run at sqrt(s_NN)=2.76 TeV. The Z bosons are reconstructed via di-electron and di-muon decay channels, with a background contamination of less than 3%. Results from the two channels are consistent and are combined. Within the statistical and systematic uncertainties, the per-event Z boson yield is proportional to the number of binary collisions estimated by the Glauber model. The elliptic anisotropy of the azimuthal distribution of the Z boson with respect to the event plane is found to be consistent with zero.
Studies of the fragmentation of jets into charged particles in heavy-ion collisions can provide information about the mechanism of jet-quenching by the hot and dense QCD matter created in such collisions, the quark-gluon plasma. This paper presents a measurement of the angular distribution of charged particles around the jet axis in $\sqrt{s_{\mathrm{NN}}}=$ 5.02 TeV Pb+Pb and $pp$ collisions, using the ATLAS detector at the LHC. The Pb+Pb and $pp$ data sets have integrated luminosities of 0.49 nb$^{-1}$ and 25 pb$^{-1}$, respectively. The measurement is performed for jets reconstructed with the anti-$k_{t}$ algorithm with radius parameter $R = 0.4$ and is extended to an angular distance of $r= 0.8$ from the jet axis. Results are presented as a function of Pb+Pb collision centrality and distance from the jet axis for charged particles with transverse momenta in the 1$-$63 GeV range, matched to jets with transverse momenta in the 126$-$316 GeV range and an absolute value of jet rapidity of less than 1.7. Modifications to the measured distributions are quantified by taking a ratio to the measurements in $pp$ collisions. Yields of charged particles with transverse momenta below 4 GeV are observed to be increasingly enhanced as a function of angular distance from the jet axis, reaching a maximum at $r=0.6$. Charged particles with transverse momenta above 4 GeV have an enhanced yield in Pb+Pb collisions in the jet core for angular distances up to $r = 0.05$ from the jet axis, with a suppression at larger distances.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
D(pT,r)_PbPb The charged particle distributions around jets as a function of distance from the jet axis in PbPb collisions at 5.02 TeV for different centrality, track pT and jet pT ranges.
The elliptic flow of muons from the decay of charm and bottom hadrons is measured in $pp$ collisions at $\sqrt{s}=13$ TeV using a data sample with an integrated luminosity of 150 pb$^{-1}$ recorded by the ATLAS detector at the LHC. The muons from heavy-flavor decay are separated from light-hadron decay muons using momentum imbalance between the tracking and muon spectrometers. The heavy-flavor decay muons are further separated into those from charm decay and those from bottom decay using the distance-of-closest-approach to the collision vertex. The measurement is performed for muons in the transverse momentum range 4-7 GeV and pseudorapidity range $|\eta|<2.4$. A significant non-zero elliptic anisotropy coefficient $v_{2}$ is observed for muons from charm decays, while the $v_{2}$ value for muons from bottom decays is consistent with zero within uncertainties.
Summary of results for inclusive muon v2 as a function of multiplicity. Uncertainties are statistical and systematic, respectively.
Summary of results for inclusive muon v2 as a function of pT. Uncertainties are statistical and systematic, respectively.
Summary of results for charm and bottom muon v2 as a function of multiplicity. Uncertainties are statistical and systematic, respectively.
Summary of results for charm and bottom muon v2 as a function of pT. Uncertainties are statistical and systematic, respectively.
Azimuthal anisotropies of muons from charm and bottom hadron decays are measured in Pb+Pb collisions at $\sqrt{s_\mathrm{NN}}= 5.02$ TeV. The data were collected with the ATLAS detector at the Large Hadron Collider in 2015 and 2018 with integrated luminosities of $0.5~\mathrm{nb}^{-1}$ and $1.4~\mathrm{nb^{-1}}$, respectively. The kinematic selection for heavy-flavor muons requires transverse momentum $4 < p_\mathrm{T} < 30$ GeV and pseudorapidity $|\eta|<2.0$. The dominant sources of muons in this $p_\mathrm{T}$ range are semi-leptonic decays of charm and bottom hadrons. These heavy-flavor muons are separated from light-hadron decay muons and punch-through hadrons using the momentum imbalance between the measurements in the tracking detector and in the muon spectrometers. Azimuthal anisotropies, quantified by flow coefficients, are measured via the event-plane method for inclusive heavy-flavor muons as a function of the muon $p_\mathrm{T}$ and in intervals of Pb+Pb collision centrality. Heavy-flavor muons are separated into contributions from charm and bottom hadron decays using the muon transverse impact parameter with respect to the event primary vertex. Non-zero elliptic ($v_{2}$) and triangular ($v_{3}$) flow coefficients are extracted for charm and bottom muons, with the charm muon coefficients larger than those for bottom muons for all Pb+Pb collision centralities. The results indicate substantial modification to the charm and bottom quark angular distributions through interactions in the quark-gluon plasma produced in these Pb+Pb collisions, with smaller modifications for the bottom quarks as expected theoretically due to their larger mass.
To assess the properties of the quark-gluon plasma formed in heavy-ion collisions, the ATLAS experiment at the LHC measures a correlation between the mean transverse momentum and the magnitudes of the flow harmonics. The analysis uses data samples of lead-lead and proton-lead collisions obtained at the centre-of-mass energy per nucleon pair of 5.02 TeV, corresponding to total integrated luminosities of $22 ~\mu b^{-1}$ and $28~nb^{-1}$, respectively. The measurement is performed using a modified Pearson correlation coefficient with the charged-particle tracks on an event-by-event basis. The modified Pearson correlation coefficients for the $2^{nd}$-, 3$^{rd}$-, and 4$^{th}$-order harmonics are measured as a function of event centrality quantified as the number of charged particles or the number of nucleons participating in the collision. The measurements are performed for several intervals of the charged-particle transverse momentum. The correlation coefficients for all studied harmonics exhibit a strong centrality evolution in the lead-lead collisions, which only weakly depends on the charged-particle momentum range. In the proton-lead collisions, the modified Pearson correlation coefficient measured for the second harmonics shows only weak centrality dependence. The data is qualitatively described by the predictions based on the hydrodynamical model.
The $c_{k}$ for the 0.5-2 GeV $p_{T}$ range as a function of event multiplicity $N_{ch}$ in Pb+Pb collisions.
The $c_{k}$ for the 0.5-5 GeV $p_{T}$ range as a function of event multiplicity $N_{ch}$ in Pb+Pb collisions.
The $c_{k}$ for the 1-2 GeV $p_{T}$ range as a function of event multiplicity $N_{ch}$ in Pb+Pb collisions.
The $c_{k}$ for the 0.3-2 GeV $p_{T}$ range as a function of event multiplicity $N_{ch}$ in p+Pb collisions.
The $c_{k}$ for the 0.3-5 GeV $p_{T}$ range as a function of event multiplicity $N_{ch}$ in p+Pb collisions.
The $c_{k}$ for the 0.5-2 GeV $p_{T}$ range as a function of event multiplicity $N_{ch}$ in p+Pb collisions.
The $Var(v_{2}^{2})_{dyn}$ for Pb+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{ch}$.
The $Var(v_{2}^{2})_{dyn}$ for Pb+Pb collisions for the $p_T$ 0.5-5 GeV interval as a function $N_{ch}$.
The $Var(v_{2}^{2})_{dyn}$ for Pb+Pb collisions for the $p_T$ 1-2 GeV interval as a function $N_{ch}$.
The $Var(v_{3}^{2})_{dyn}$ for Pb+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{ch}$.
The $Var(v_{3}^{2})_{dyn}$ for Pb+Pb collisions for the $p_T$ 0.5-5 GeV interval as a function $N_{ch}$.
The $Var(v_{3}^{2})_{dyn}$ for Pb+Pb collisions for the $p_T$ 1-2 GeV interval as a function $N_{ch}$.
The $Var(v_{4}^{2})_{dyn}$ for Pb+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{ch}$.
The $Var(v_{4}^{2})_{dyn}$ for Pb+Pb collisions for the $p_T$ 0.5-5 GeV interval as a function $N_{ch}$.
The $Var(v_{4}^{2})_{dyn}$ for Pb+Pb collisions for the $p_T$ 1-2 GeV interval as a function $N_{ch}$.
The $Var(v_{2}^{2})_{dyn}$ for p+Pb collisions for the $p_T$ 0.3-2 GeV interval as a function $N_{ch}$.
The $Var(v_{2}^{2})_{dyn}$ for p+Pb collisions for the $p_T$ 0.3-5 GeV interval as a function $N_{ch}$.
The $Var(v_{2}^{2})_{dyn}$ for p+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{ch}$.
The $cov(v_{2}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{ch}$.
The $cov(v_{2}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-5 GeV interval as a function $N_{ch}$.
The $cov(v_{2}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 1-2 GeV interval as a function $N_{ch}$.
The $cov(v_{3}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{ch}$.
The $cov(v_{3}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-5 GeV interval as a function $N_{ch}$.
The $cov(v_{3}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 1-2 GeV interval as a function $N_{ch}$.
The $cov(v_{4}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{ch}$.
The $cov(v_{4}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-5 GeV interval as a function $N_{ch}$.
The $cov(v_{4}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 1-2 GeV interval as a function $N_{ch}$.
The $cov(v_{2}^{2},[p_{T}])$ for p+Pb collisions for the $p_T$ 0.3-2 GeV interval as a function $N_{ch}$.
The $cov(v_{2}^{2},[p_{T}])$ for p+Pb collisions for the $p_T$ 0.3-5 GeV interval as a function $N_{ch}$.
The $cov(v_{2}^{2},[p_{T}])$ for p+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{ch}$.
The $\rho(v_{2}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{ch}$.
The $\rho(v_{2}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-5 GeV interval as a function $N_{ch}$.
The $\rho(v_{2}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 1-2 GeV interval as a function $N_{ch}$.
The $\rho(v_{3}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{ch}$.
The $\rho(v_{3}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-5 GeV interval as a function $N_{ch}$.
The $\rho(v_{3}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 1-2 GeV interval as a function $N_{ch}$.
The $\rho(v_{4}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{ch}$.
The $\rho(v_{4}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-5 GeV interval as a function $N_{ch}$.
The $\rho(v_{4}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 1-2 GeV interval as a function $N_{ch}$.
The $\rho(v_{2}^{2},[p_{T}])$ for p+Pb collisions for the $p_T$ 0.3-2 GeV interval as a function $N_{ch}$.
The $\rho(v_{2}^{2},[p_{T}])$ for p+Pb collisions for the $p_T$ 0.3-5 GeV interval as a function $N_{ch}$.
The $\rho(v_{2}^{2},[p_{T}])$ for p+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{ch}$.
The $\rho(v_{2}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{part}$.
The $\rho(v_{2}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-5 GeV interval as a function $N_{part}$.
The $\rho(v_{2}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 1-2 GeV interval as a function $N_{part}$.
The $\rho(v_{3}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{part}$.
The $\rho(v_{3}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-5 GeV interval as a function $N_{part}$.
The $\rho(v_{3}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 1-2 GeV interval as a function $N_{part}$.
The $\rho(v_{4}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-2 GeV interval as a function $N_{part}$.
The $\rho(v_{4}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 0.5-5 GeV interval as a function $N_{part}$.
The $\rho(v_{4}^{2},[p_{T}])$ for Pb+Pb collisions for the $p_T$ 1-2 GeV interval as a function $N_{part}$.
Two-particle pseudorapidity correlations are measured in $\sqrt{s_{\rm{NN}}}$ = 2.76 TeV Pb+Pb, $\sqrt{s_{\rm{NN}}}$ = 5.02 TeV $p$+Pb, and $\sqrt{s}$ = 13 TeV $pp$ collisions at the LHC, with total integrated luminosities of approximately 7 $\mu\mathrm{b}^{-1}$, 28 $\mathrm{nb}^{-1}$, and 65 $\mathrm{nb}^{-1}$, respectively. The correlation function $C_{\rm N}(\eta_1,\eta_2)$ is measured as a function of event multiplicity using charged particles in the pseudorapidity range $|\eta|<2.4$. The correlation function contains a significant short-range component, which is estimated and subtracted. After removal of the short-range component, the shape of the correlation function is described approximately by $1+\langle{a_1^2}\rangle \eta_1\eta_2$ in all collision systems over the full multiplicity range. The values of $\sqrt{\langle{a_1^2}\rangle}$ are consistent between the opposite-charge pairs and same-charge pairs, and for the three collision systems at similar multiplicity. The values of $\sqrt{\langle{a_1^2}\rangle}$ and the magnitude of the short-range component both follow a power-law dependence on the event multiplicity. The $\eta$ distribution of the short-range component, after symmetrizing the proton and lead directions in $p$+Pb collisions, is found to be smaller than that in $pp$ collisions with comparable multiplicity.
C_N(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (260<=Nch<300)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (260<=Nch<300)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (240<=Nch<260)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (240<=Nch<260)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (220<=Nch<240)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (220<=Nch<240)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (200<=Nch<220)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (200<=Nch<220)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (180<=Nch<200)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (180<=Nch<200)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (160<=Nch<180)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (160<=Nch<180)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (140<=Nch<160)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (140<=Nch<160)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (120<=Nch<140)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (120<=Nch<140)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (100<=Nch<120)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (100<=Nch<120)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (80<=Nch<100)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (80<=Nch<100)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (60<=Nch<80)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (60<=Nch<80)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (40<=Nch<60)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (40<=Nch<60)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (20<=Nch<40)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (20<=Nch<40)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (10<=Nch<20)
C_N(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (10<=Nch<20)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (260<=Nch<300)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (260<=Nch<300)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (240<=Nch<260)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (240<=Nch<260)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (220<=Nch<240)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (220<=Nch<240)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (200<=Nch<220)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (200<=Nch<220)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (180<=Nch<200)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (180<=Nch<200)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (160<=Nch<180)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (160<=Nch<180)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (140<=Nch<160)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (140<=Nch<160)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (120<=Nch<140)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (120<=Nch<140)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (100<=Nch<120)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (100<=Nch<120)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (80<=Nch<100)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (80<=Nch<100)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (60<=Nch<80)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (60<=Nch<80)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (40<=Nch<60)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (40<=Nch<60)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (20<=Nch<40)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (20<=Nch<40)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (10<=Nch<20)
SRC(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (10<=Nch<20)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (260<=Nch<300)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (260<=Nch<300)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (240<=Nch<260)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (240<=Nch<260)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (220<=Nch<240)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (220<=Nch<240)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (200<=Nch<220)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (200<=Nch<220)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (180<=Nch<200)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (180<=Nch<200)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (160<=Nch<180)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (160<=Nch<180)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (140<=Nch<160)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (140<=Nch<160)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (120<=Nch<140)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (120<=Nch<140)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (100<=Nch<120)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (100<=Nch<120)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (80<=Nch<100)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (80<=Nch<100)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (60<=Nch<80)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (60<=Nch<80)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (40<=Nch<60)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (40<=Nch<60)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (20<=Nch<40)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (20<=Nch<40)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.5GeV, (10<=Nch<20)
C_N^sub(eta_1, eta_2) for Pb+Pb, pT>0.2GeV, (10<=Nch<20)
C_N(eta_1, eta_2) for p+Pb, pT>0.5GeV, (260<=Nch<300)
C_N(eta_1, eta_2) for p+Pb, pT>0.2GeV, (260<=Nch<300)
C_N(eta_1, eta_2) for p+Pb, pT>0.5GeV, (240<=Nch<260)
C_N(eta_1, eta_2) for p+Pb, pT>0.2GeV, (240<=Nch<260)
C_N(eta_1, eta_2) for p+Pb, pT>0.5GeV, (220<=Nch<240)
C_N(eta_1, eta_2) for p+Pb, pT>0.2GeV, (220<=Nch<240)
C_N(eta_1, eta_2) for p+Pb, pT>0.5GeV, (200<=Nch<220)
C_N(eta_1, eta_2) for p+Pb, pT>0.2GeV, (200<=Nch<220)
C_N(eta_1, eta_2) for p+Pb, pT>0.5GeV, (180<=Nch<200)
C_N(eta_1, eta_2) for p+Pb, pT>0.2GeV, (180<=Nch<200)
C_N(eta_1, eta_2) for p+Pb, pT>0.5GeV, (160<=Nch<180)
C_N(eta_1, eta_2) for p+Pb, pT>0.2GeV, (160<=Nch<180)
C_N(eta_1, eta_2) for p+Pb, pT>0.5GeV, (140<=Nch<160)
C_N(eta_1, eta_2) for p+Pb, pT>0.2GeV, (140<=Nch<160)
C_N(eta_1, eta_2) for p+Pb, pT>0.5GeV, (120<=Nch<140)
C_N(eta_1, eta_2) for p+Pb, pT>0.2GeV, (120<=Nch<140)
C_N(eta_1, eta_2) for p+Pb, pT>0.5GeV, (100<=Nch<120)
C_N(eta_1, eta_2) for p+Pb, pT>0.2GeV, (100<=Nch<120)
C_N(eta_1, eta_2) for p+Pb, pT>0.5GeV, (80<=Nch<100)
C_N(eta_1, eta_2) for p+Pb, pT>0.2GeV, (80<=Nch<100)
C_N(eta_1, eta_2) for p+Pb, pT>0.5GeV, (60<=Nch<80)
C_N(eta_1, eta_2) for p+Pb, pT>0.2GeV, (60<=Nch<80)
C_N(eta_1, eta_2) for p+Pb, pT>0.5GeV, (40<=Nch<60)
C_N(eta_1, eta_2) for p+Pb, pT>0.2GeV, (40<=Nch<60)
C_N(eta_1, eta_2) for p+Pb, pT>0.5GeV, (20<=Nch<40)
C_N(eta_1, eta_2) for p+Pb, pT>0.2GeV, (20<=Nch<40)
C_N(eta_1, eta_2) for p+Pb, pT>0.5GeV, (10<=Nch<20)
C_N(eta_1, eta_2) for p+Pb, pT>0.2GeV, (10<=Nch<20)
SRC(eta_1, eta_2) for p+Pb, pT>0.5GeV, (260<=Nch<300)
SRC(eta_1, eta_2) for p+Pb, pT>0.2GeV, (260<=Nch<300)
SRC(eta_1, eta_2) for p+Pb, pT>0.5GeV, (240<=Nch<260)
SRC(eta_1, eta_2) for p+Pb, pT>0.2GeV, (240<=Nch<260)
SRC(eta_1, eta_2) for p+Pb, pT>0.5GeV, (220<=Nch<240)
SRC(eta_1, eta_2) for p+Pb, pT>0.2GeV, (220<=Nch<240)
SRC(eta_1, eta_2) for p+Pb, pT>0.5GeV, (200<=Nch<220)
SRC(eta_1, eta_2) for p+Pb, pT>0.2GeV, (200<=Nch<220)
SRC(eta_1, eta_2) for p+Pb, pT>0.5GeV, (180<=Nch<200)
SRC(eta_1, eta_2) for p+Pb, pT>0.2GeV, (180<=Nch<200)
SRC(eta_1, eta_2) for p+Pb, pT>0.5GeV, (160<=Nch<180)
SRC(eta_1, eta_2) for p+Pb, pT>0.2GeV, (160<=Nch<180)
SRC(eta_1, eta_2) for p+Pb, pT>0.5GeV, (140<=Nch<160)
SRC(eta_1, eta_2) for p+Pb, pT>0.2GeV, (140<=Nch<160)
SRC(eta_1, eta_2) for p+Pb, pT>0.5GeV, (120<=Nch<140)
SRC(eta_1, eta_2) for p+Pb, pT>0.2GeV, (120<=Nch<140)
SRC(eta_1, eta_2) for p+Pb, pT>0.5GeV, (100<=Nch<120)
SRC(eta_1, eta_2) for p+Pb, pT>0.2GeV, (100<=Nch<120)
SRC(eta_1, eta_2) for p+Pb, pT>0.5GeV, (80<=Nch<100)
SRC(eta_1, eta_2) for p+Pb, pT>0.2GeV, (80<=Nch<100)
SRC(eta_1, eta_2) for p+Pb, pT>0.5GeV, (60<=Nch<80)
SRC(eta_1, eta_2) for p+Pb, pT>0.2GeV, (60<=Nch<80)
SRC(eta_1, eta_2) for p+Pb, pT>0.5GeV, (40<=Nch<60)
SRC(eta_1, eta_2) for p+Pb, pT>0.2GeV, (40<=Nch<60)
SRC(eta_1, eta_2) for p+Pb, pT>0.5GeV, (20<=Nch<40)
SRC(eta_1, eta_2) for p+Pb, pT>0.2GeV, (20<=Nch<40)
SRC(eta_1, eta_2) for p+Pb, pT>0.5GeV, (10<=Nch<20)
SRC(eta_1, eta_2) for p+Pb, pT>0.2GeV, (10<=Nch<20)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.5GeV, (260<=Nch<300)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.2GeV, (260<=Nch<300)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.5GeV, (240<=Nch<260)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.2GeV, (240<=Nch<260)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.5GeV, (220<=Nch<240)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.2GeV, (220<=Nch<240)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.5GeV, (200<=Nch<220)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.2GeV, (200<=Nch<220)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.5GeV, (180<=Nch<200)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.2GeV, (180<=Nch<200)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.5GeV, (160<=Nch<180)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.2GeV, (160<=Nch<180)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.5GeV, (140<=Nch<160)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.2GeV, (140<=Nch<160)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.5GeV, (120<=Nch<140)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.2GeV, (120<=Nch<140)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.5GeV, (100<=Nch<120)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.2GeV, (100<=Nch<120)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.5GeV, (80<=Nch<100)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.2GeV, (80<=Nch<100)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.5GeV, (60<=Nch<80)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.2GeV, (60<=Nch<80)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.5GeV, (40<=Nch<60)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.2GeV, (40<=Nch<60)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.5GeV, (20<=Nch<40)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.2GeV, (20<=Nch<40)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.5GeV, (10<=Nch<20)
C_N^sub(eta_1, eta_2) for p+Pb, pT>0.2GeV, (10<=Nch<20)
C_N(eta_1, eta_2) for pp, pT>0.5GeV, (140<=Nch<160)
C_N(eta_1, eta_2) for pp, pT>0.2GeV, (140<=Nch<160)
C_N(eta_1, eta_2) for pp, pT>0.5GeV, (120<=Nch<140)
C_N(eta_1, eta_2) for pp, pT>0.2GeV, (120<=Nch<140)
C_N(eta_1, eta_2) for pp, pT>0.5GeV, (100<=Nch<120)
C_N(eta_1, eta_2) for pp, pT>0.2GeV, (100<=Nch<120)
C_N(eta_1, eta_2) for pp, pT>0.5GeV, (80<=Nch<100)
C_N(eta_1, eta_2) for pp, pT>0.2GeV, (80<=Nch<100)
C_N(eta_1, eta_2) for pp, pT>0.5GeV, (60<=Nch<80)
C_N(eta_1, eta_2) for pp, pT>0.2GeV, (60<=Nch<80)
C_N(eta_1, eta_2) for pp, pT>0.5GeV, (40<=Nch<60)
C_N(eta_1, eta_2) for pp, pT>0.2GeV, (40<=Nch<60)
C_N(eta_1, eta_2) for pp, pT>0.5GeV, (20<=Nch<40)
C_N(eta_1, eta_2) for pp, pT>0.2GeV, (20<=Nch<40)
C_N(eta_1, eta_2) for pp, pT>0.5GeV, (10<=Nch<20)
C_N(eta_1, eta_2) for pp, pT>0.2GeV, (10<=Nch<20)
SRC(eta_1, eta_2) for pp, pT>0.5GeV, (140<=Nch<160)
SRC(eta_1, eta_2) for pp, pT>0.2GeV, (140<=Nch<160)
SRC(eta_1, eta_2) for pp, pT>0.5GeV, (120<=Nch<140)
SRC(eta_1, eta_2) for pp, pT>0.2GeV, (120<=Nch<140)
SRC(eta_1, eta_2) for pp, pT>0.5GeV, (100<=Nch<120)
SRC(eta_1, eta_2) for pp, pT>0.2GeV, (100<=Nch<120)
SRC(eta_1, eta_2) for pp, pT>0.5GeV, (80<=Nch<100)
SRC(eta_1, eta_2) for pp, pT>0.2GeV, (80<=Nch<100)
SRC(eta_1, eta_2) for pp, pT>0.5GeV, (60<=Nch<80)
SRC(eta_1, eta_2) for pp, pT>0.2GeV, (60<=Nch<80)
SRC(eta_1, eta_2) for pp, pT>0.5GeV, (40<=Nch<60)
SRC(eta_1, eta_2) for pp, pT>0.2GeV, (40<=Nch<60)
SRC(eta_1, eta_2) for pp, pT>0.5GeV, (20<=Nch<40)
SRC(eta_1, eta_2) for pp, pT>0.2GeV, (20<=Nch<40)
SRC(eta_1, eta_2) for pp, pT>0.5GeV, (10<=Nch<20)
SRC(eta_1, eta_2) for pp, pT>0.2GeV, (10<=Nch<20)
C_N^sub(eta_1, eta_2) for pp, pT>0.5GeV, (140<=Nch<160)
C_N^sub(eta_1, eta_2) for pp, pT>0.2GeV, (140<=Nch<160)
C_N^sub(eta_1, eta_2) for pp, pT>0.5GeV, (120<=Nch<140)
C_N^sub(eta_1, eta_2) for pp, pT>0.2GeV, (120<=Nch<140)
C_N^sub(eta_1, eta_2) for pp, pT>0.5GeV, (100<=Nch<120)
C_N^sub(eta_1, eta_2) for pp, pT>0.2GeV, (100<=Nch<120)
C_N^sub(eta_1, eta_2) for pp, pT>0.5GeV, (80<=Nch<100)
C_N^sub(eta_1, eta_2) for pp, pT>0.2GeV, (80<=Nch<100)
C_N^sub(eta_1, eta_2) for pp, pT>0.5GeV, (60<=Nch<80)
C_N^sub(eta_1, eta_2) for pp, pT>0.2GeV, (60<=Nch<80)
C_N^sub(eta_1, eta_2) for pp, pT>0.5GeV, (40<=Nch<60)
C_N^sub(eta_1, eta_2) for pp, pT>0.2GeV, (40<=Nch<60)
C_N^sub(eta_1, eta_2) for pp, pT>0.5GeV, (20<=Nch<40)
C_N^sub(eta_1, eta_2) for pp, pT>0.2GeV, (20<=Nch<40)
C_N^sub(eta_1, eta_2) for pp, pT>0.5GeV, (10<=Nch<20)
C_N^sub(eta_1, eta_2) for pp, pT>0.2GeV, (10<=Nch<20)
<a_n a_m> for Pb+Pb, pT>0.5GeV, 260<=Nch<300, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 260<=Nch<300, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 260<=Nch<300, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 260<=Nch<300, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 260<=Nch<300, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 260<=Nch<300, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 240<=Nch<260, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 240<=Nch<260, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 240<=Nch<260, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 240<=Nch<260, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 240<=Nch<260, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 240<=Nch<260, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 220<=Nch<240, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 220<=Nch<240, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 220<=Nch<240, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 220<=Nch<240, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 220<=Nch<240, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 220<=Nch<240, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 200<=Nch<220, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 200<=Nch<220, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 200<=Nch<220, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 200<=Nch<220, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 200<=Nch<220, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 200<=Nch<220, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 180<=Nch<200, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 180<=Nch<200, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 180<=Nch<200, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 180<=Nch<200, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 180<=Nch<200, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 180<=Nch<200, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 160<=Nch<180, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 160<=Nch<180, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 160<=Nch<180, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 160<=Nch<180, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 160<=Nch<180, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 160<=Nch<180, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 140<=Nch<160, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 140<=Nch<160, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 140<=Nch<160, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 140<=Nch<160, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 140<=Nch<160, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 140<=Nch<160, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 120<=Nch<140, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 120<=Nch<140, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 120<=Nch<140, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 120<=Nch<140, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 120<=Nch<140, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 120<=Nch<140, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 100<=Nch<120, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 100<=Nch<120, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 100<=Nch<120, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 100<=Nch<120, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 100<=Nch<120, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 100<=Nch<120, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 80<=Nch<100, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 80<=Nch<100, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 80<=Nch<100, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 80<=Nch<100, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 80<=Nch<100, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 80<=Nch<100, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 60<=Nch<80, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 60<=Nch<80, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 60<=Nch<80, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 60<=Nch<80, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 60<=Nch<80, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 60<=Nch<80, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 40<=Nch<60, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 40<=Nch<60, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 40<=Nch<60, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 40<=Nch<60, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 40<=Nch<60, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 40<=Nch<60, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 20<=Nch<40, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 20<=Nch<40, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 20<=Nch<40, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 20<=Nch<40, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 20<=Nch<40, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 20<=Nch<40, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 10<=Nch<20, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 10<=Nch<20, w SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 10<=Nch<20, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 10<=Nch<20, w SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 10<=Nch<20, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 10<=Nch<20, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 260<=Nch<300, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 260<=Nch<300, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 260<=Nch<300, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 260<=Nch<300, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 260<=Nch<300, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 260<=Nch<300, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 240<=Nch<260, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 240<=Nch<260, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 240<=Nch<260, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 240<=Nch<260, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 240<=Nch<260, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 240<=Nch<260, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 220<=Nch<240, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 220<=Nch<240, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 220<=Nch<240, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 220<=Nch<240, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 220<=Nch<240, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 220<=Nch<240, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 200<=Nch<220, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 200<=Nch<220, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 200<=Nch<220, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 200<=Nch<220, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 200<=Nch<220, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 200<=Nch<220, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 180<=Nch<200, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 180<=Nch<200, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 180<=Nch<200, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 180<=Nch<200, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 180<=Nch<200, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 180<=Nch<200, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 160<=Nch<180, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 160<=Nch<180, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 160<=Nch<180, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 160<=Nch<180, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 160<=Nch<180, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 160<=Nch<180, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 140<=Nch<160, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 140<=Nch<160, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 140<=Nch<160, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 140<=Nch<160, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 140<=Nch<160, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 140<=Nch<160, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 120<=Nch<140, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 120<=Nch<140, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 120<=Nch<140, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 120<=Nch<140, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 120<=Nch<140, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 120<=Nch<140, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 100<=Nch<120, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 100<=Nch<120, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 100<=Nch<120, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 100<=Nch<120, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 100<=Nch<120, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 100<=Nch<120, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 80<=Nch<100, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 80<=Nch<100, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 80<=Nch<100, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 80<=Nch<100, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 80<=Nch<100, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 80<=Nch<100, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 60<=Nch<80, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 60<=Nch<80, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 60<=Nch<80, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 60<=Nch<80, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 60<=Nch<80, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 60<=Nch<80, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 40<=Nch<60, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 40<=Nch<60, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 40<=Nch<60, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 40<=Nch<60, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 40<=Nch<60, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 40<=Nch<60, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 20<=Nch<40, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 20<=Nch<40, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 20<=Nch<40, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 20<=Nch<40, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 20<=Nch<40, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 20<=Nch<40, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 10<=Nch<20, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 10<=Nch<20, w SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 10<=Nch<20, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 10<=Nch<20, w SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 10<=Nch<20, w SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 10<=Nch<20, w SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 140<=Nch<160, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 140<=Nch<160, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 140<=Nch<160, w SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 140<=Nch<160, w SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 140<=Nch<160, w SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 140<=Nch<160, w SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 120<=Nch<140, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 120<=Nch<140, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 120<=Nch<140, w SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 120<=Nch<140, w SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 120<=Nch<140, w SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 120<=Nch<140, w SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 100<=Nch<120, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 100<=Nch<120, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 100<=Nch<120, w SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 100<=Nch<120, w SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 100<=Nch<120, w SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 100<=Nch<120, w SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 80<=Nch<100, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 80<=Nch<100, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 80<=Nch<100, w SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 80<=Nch<100, w SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 80<=Nch<100, w SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 80<=Nch<100, w SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 60<=Nch<80, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 60<=Nch<80, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 60<=Nch<80, w SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 60<=Nch<80, w SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 60<=Nch<80, w SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 60<=Nch<80, w SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 40<=Nch<60, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 40<=Nch<60, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 40<=Nch<60, w SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 40<=Nch<60, w SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 40<=Nch<60, w SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 40<=Nch<60, w SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 20<=Nch<40, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 20<=Nch<40, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 20<=Nch<40, w SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 20<=Nch<40, w SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 20<=Nch<40, w SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 20<=Nch<40, w SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 10<=Nch<20, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 10<=Nch<20, w SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 10<=Nch<20, w SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 10<=Nch<20, w SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 10<=Nch<20, w SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 10<=Nch<20, w SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 260<=Nch<300, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 260<=Nch<300, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 260<=Nch<300, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 260<=Nch<300, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 260<=Nch<300, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 260<=Nch<300, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 240<=Nch<260, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 240<=Nch<260, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 240<=Nch<260, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 240<=Nch<260, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 240<=Nch<260, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 240<=Nch<260, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 220<=Nch<240, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 220<=Nch<240, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 220<=Nch<240, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 220<=Nch<240, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 220<=Nch<240, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 220<=Nch<240, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 200<=Nch<220, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 200<=Nch<220, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 200<=Nch<220, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 200<=Nch<220, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 200<=Nch<220, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 200<=Nch<220, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 180<=Nch<200, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 180<=Nch<200, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 180<=Nch<200, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 180<=Nch<200, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 180<=Nch<200, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 180<=Nch<200, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 160<=Nch<180, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 160<=Nch<180, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 160<=Nch<180, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 160<=Nch<180, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 160<=Nch<180, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 160<=Nch<180, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 140<=Nch<160, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 140<=Nch<160, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 140<=Nch<160, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 140<=Nch<160, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 140<=Nch<160, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 140<=Nch<160, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 120<=Nch<140, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 120<=Nch<140, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 120<=Nch<140, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 120<=Nch<140, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 120<=Nch<140, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 120<=Nch<140, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 100<=Nch<120, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 100<=Nch<120, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 100<=Nch<120, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 100<=Nch<120, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 100<=Nch<120, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 100<=Nch<120, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 80<=Nch<100, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 80<=Nch<100, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 80<=Nch<100, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 80<=Nch<100, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 80<=Nch<100, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 80<=Nch<100, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 60<=Nch<80, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 60<=Nch<80, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 60<=Nch<80, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 60<=Nch<80, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 60<=Nch<80, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 60<=Nch<80, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 40<=Nch<60, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 40<=Nch<60, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 40<=Nch<60, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 40<=Nch<60, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 40<=Nch<60, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 40<=Nch<60, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 20<=Nch<40, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 20<=Nch<40, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 20<=Nch<40, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 20<=Nch<40, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 20<=Nch<40, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 20<=Nch<40, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 10<=Nch<20, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 10<=Nch<20, wo SRC, opposite pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 10<=Nch<20, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 10<=Nch<20, wo SRC, same pairs
<a_n a_m> for Pb+Pb, pT>0.5GeV, 10<=Nch<20, wo SRC, all pairs
<a_n a_m> for Pb+Pb, pT>0.2GeV, 10<=Nch<20, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 260<=Nch<300, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 260<=Nch<300, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 260<=Nch<300, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 260<=Nch<300, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 260<=Nch<300, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 260<=Nch<300, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 240<=Nch<260, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 240<=Nch<260, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 240<=Nch<260, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 240<=Nch<260, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 240<=Nch<260, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 240<=Nch<260, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 220<=Nch<240, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 220<=Nch<240, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 220<=Nch<240, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 220<=Nch<240, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 220<=Nch<240, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 220<=Nch<240, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 200<=Nch<220, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 200<=Nch<220, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 200<=Nch<220, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 200<=Nch<220, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 200<=Nch<220, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 200<=Nch<220, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 180<=Nch<200, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 180<=Nch<200, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 180<=Nch<200, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 180<=Nch<200, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 180<=Nch<200, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 180<=Nch<200, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 160<=Nch<180, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 160<=Nch<180, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 160<=Nch<180, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 160<=Nch<180, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 160<=Nch<180, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 160<=Nch<180, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 140<=Nch<160, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 140<=Nch<160, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 140<=Nch<160, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 140<=Nch<160, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 140<=Nch<160, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 140<=Nch<160, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 120<=Nch<140, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 120<=Nch<140, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 120<=Nch<140, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 120<=Nch<140, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 120<=Nch<140, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 120<=Nch<140, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 100<=Nch<120, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 100<=Nch<120, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 100<=Nch<120, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 100<=Nch<120, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 100<=Nch<120, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 100<=Nch<120, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 80<=Nch<100, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 80<=Nch<100, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 80<=Nch<100, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 80<=Nch<100, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 80<=Nch<100, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 80<=Nch<100, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 60<=Nch<80, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 60<=Nch<80, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 60<=Nch<80, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 60<=Nch<80, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 60<=Nch<80, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 60<=Nch<80, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 40<=Nch<60, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 40<=Nch<60, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 40<=Nch<60, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 40<=Nch<60, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 40<=Nch<60, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 40<=Nch<60, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 20<=Nch<40, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 20<=Nch<40, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 20<=Nch<40, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 20<=Nch<40, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 20<=Nch<40, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 20<=Nch<40, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 10<=Nch<20, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 10<=Nch<20, wo SRC, opposite pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 10<=Nch<20, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 10<=Nch<20, wo SRC, same pairs
<a_n a_m> for p+Pb, pT>0.5GeV, 10<=Nch<20, wo SRC, all pairs
<a_n a_m> for p+Pb, pT>0.2GeV, 10<=Nch<20, wo SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 140<=Nch<160, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 140<=Nch<160, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 140<=Nch<160, wo SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 140<=Nch<160, wo SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 140<=Nch<160, wo SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 140<=Nch<160, wo SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 120<=Nch<140, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 120<=Nch<140, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 120<=Nch<140, wo SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 120<=Nch<140, wo SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 120<=Nch<140, wo SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 120<=Nch<140, wo SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 100<=Nch<120, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 100<=Nch<120, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 100<=Nch<120, wo SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 100<=Nch<120, wo SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 100<=Nch<120, wo SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 100<=Nch<120, wo SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 80<=Nch<100, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 80<=Nch<100, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 80<=Nch<100, wo SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 80<=Nch<100, wo SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 80<=Nch<100, wo SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 80<=Nch<100, wo SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 60<=Nch<80, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 60<=Nch<80, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 60<=Nch<80, wo SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 60<=Nch<80, wo SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 60<=Nch<80, wo SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 60<=Nch<80, wo SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 40<=Nch<60, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 40<=Nch<60, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 40<=Nch<60, wo SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 40<=Nch<60, wo SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 40<=Nch<60, wo SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 40<=Nch<60, wo SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 20<=Nch<40, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 20<=Nch<40, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 20<=Nch<40, wo SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 20<=Nch<40, wo SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 20<=Nch<40, wo SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 20<=Nch<40, wo SRC, all pairs
<a_n a_m> for pp, pT>0.5GeV, 10<=Nch<20, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.2GeV, 10<=Nch<20, wo SRC, opposite pairs
<a_n a_m> for pp, pT>0.5GeV, 10<=Nch<20, wo SRC, same pairs
<a_n a_m> for pp, pT>0.2GeV, 10<=Nch<20, wo SRC, same pairs
<a_n a_m> for pp, pT>0.5GeV, 10<=Nch<20, wo SRC, all pairs
<a_n a_m> for pp, pT>0.2GeV, 10<=Nch<20, wo SRC, all pairs
a1 from fit C_N^sub(eta-) for Pb+Pb, pT>0.5GeV
a1 from fit C_N^sub(eta-) for Pb+Pb, pT>0.2GeV
a1 from fit C_N^sub(eta+) for Pb+Pb, pT>0.5GeV
a1 from fit C_N^sub(eta+) for Pb+Pb, pT>0.2GeV
a1 from fit r_N^sub(eta) for Pb+Pb, pT>0.5GeV
a1 from fit r_N^sub(eta) for Pb+Pb, pT>0.2GeV
a1 from fit C_N^sub(eta1, eta2) for Pb+Pb, pT>0.5GeV
a1 from fit C_N^sub(eta1, eta2) for Pb+Pb, pT>0.2GeV
a1 from fit C_N^sub(eta-) for p+Pb, pT>0.5GeV
a1 from fit C_N^sub(eta-) for p+Pb, pT>0.2GeV
a1 from fit C_N^sub(eta+) for p+Pb, pT>0.5GeV
a1 from fit C_N^sub(eta+) for p+Pb, pT>0.2GeV
a1 from fit r_N^sub(eta) for p+Pb, pT>0.5GeV
a1 from fit r_N^sub(eta) for p+Pb, pT>0.2GeV
a1 from fit C_N^sub(eta1, eta2) for p+Pb, pT>0.5GeV
a1 from fit C_N^sub(eta1, eta2) for p+Pb, pT>0.2GeV
a1 from fit C_N^sub(eta-) for pp, pT>0.5GeV
a1 from fit C_N^sub(eta-) for pp, pT>0.2GeV
a1 from fit C_N^sub(eta+) for pp, pT>0.5GeV
a1 from fit C_N^sub(eta+) for pp, pT>0.2GeV
a1 from fit r_N^sub(eta) for pp, pT>0.5GeV
a1 from fit r_N^sub(eta) for pp, pT>0.2GeV
a1 from fit C_N^sub(eta1, eta2) for pp, pT>0.5GeV
a1 from fit C_N^sub(eta1, eta2) for pp, pT>0.2GeV
SRC for Pb+Pb, pT>0.5GeV, all pairs
SRC for Pb+Pb, pT>0.2GeV, all pairs
SRC for Pb+Pb, pT>0.5GeV, opposite pairs
SRC for Pb+Pb, pT>0.2GeV, opposite pairs
SRC for Pb+Pb, pT>0.5GeV, same pairs
SRC for Pb+Pb, pT>0.2GeV, same pairs
SRC for p+Pb, pT>0.5GeV, all pairs
SRC for p+Pb, pT>0.2GeV, all pairs
SRC for p+Pb, pT>0.5GeV, opposite pairs
SRC for p+Pb, pT>0.2GeV, opposite pairs
SRC for p+Pb, pT>0.5GeV, same pairs
SRC for p+Pb, pT>0.2GeV, same pairs
SRC for pp, pT>0.5GeV, all pairs
SRC for pp, pT>0.2GeV, all pairs
SRC for pp, pT>0.5GeV, opposite pairs
SRC for pp, pT>0.2GeV, opposite pairs
SRC for pp, pT>0.5GeV, same pairs
SRC for pp, pT>0.2GeV, same pairs
SRC for Pb+Pb, pT>0.5GeV
SRC for Pb+Pb, pT>0.2GeV
SRC for p+Pb, pT>0.5GeV
SRC for p+Pb, pT>0.2GeV
SRC for pp, pT>0.5GeV
SRC for pp, pT>0.2GeV
a1 for Pb+Pb, pT>0.5GeV
a1 for Pb+Pb, pT>0.2GeV
a1 for p+Pb, pT>0.5GeV
a1 for p+Pb, pT>0.2GeV
a1 for pp, pT>0.5GeV
a1 for pp, pT>0.2GeV
f(eta+) for p+Pb
f(eta+) for symmetrized p+Pb
f(eta+) for pp
f(eta+) for Pb+Pb
Measurements of charged-particle fragmentation functions of jets produced in ultra-relativistic nuclear collisions can provide insight into the modification of parton showers in the hot, dense medium created in the collisions. ATLAS has measured jets in $\sqrt{s_{NN}} = 2.76$ TeV Pb+Pb collisions at the LHC using a data set recorded in 2011 with an integrated luminosity of 0.14 nb$^{-1}$. Jets were reconstructed using the anti-$k_{t}$ algorithm with distance parameter values $R$ = 0.2, 0.3, and 0.4. Distributions of charged-particle transverse momentum and longitudinal momentum fraction are reported for seven bins in collision centrality for $R=0.4$ jets with $p_{{T}}^{\mathrm{jet}}> 100$ GeV. Commensurate minimum $p_{\mathrm{T}}$ values are used for the other radii. Ratios of fragment distributions in each centrality bin to those measured in the most peripheral bin are presented. These ratios show a reduction of fragment yield in central collisions relative to peripheral collisions at intermediate $z$ values, $0.04 \lesssim z \lesssim 0.2$ and an enhancement in fragment yield for $z \lesssim 0.04$. A smaller, less significant enhancement is observed at large $z$ and large $p_{\mathrm{T}}$ in central collisions.
Differences of D(Z) distributions in different centralities with respect to peripheral events for R = 0.3 jets. The errors represent combined statistical and systematic uncertainties.
Differences of D(Z) distributions in different centralities with respect to peripheral events for R = 0.2 jets. The errors represent combined statistical and systematic uncertainties.
D(z) distribution for R=0.4 jets.
D(z) distribution for R=0.4 jets.
D(z) distribution for R=0.4 jets.
D(z) distribution for R=0.4 jets.
D(z) distribution for R=0.4 jets.
D(z) distribution for R=0.4 jets.
D(z) distribution for R=0.4 jets.
D(z) distribution for R=0.3 jets.
D(z) distribution for R=0.3 jets.
D(z) distribution for R=0.3 jets.
D(z) distribution for R=0.3 jets.
D(z) distribution for R=0.3 jets.
D(z) distribution for R=0.3 jets.
D(z) distribution for R=0.3 jets.
D(z) distribution for R=0.2 jets.
D(z) distribution for R=0.2 jets.
D(z) distribution for R=0.2 jets.
D(z) distribution for R=0.2 jets.
D(z) distribution for R=0.2 jets.
D(z) distribution for R=0.2 jets.
D(z) distribution for R=0.2 jets.
D(pt) distribution for R=0.4 jets.
D(pt) distribution for R=0.4 jets.
D(pt) distribution for R=0.4 jets.
D(pt) distribution for R=0.4 jets.
D(pt) distribution for R=0.4 jets.
D(pt) distribution for R=0.4 jets.
D(pt) distribution for R=0.4 jets.
D(pt) distribution for R=0.3 jets.
D(pt) distribution for R=0.3 jets.
D(pt) distribution for R=0.3 jets.
D(pt) distribution for R=0.3 jets.
D(pt) distribution for R=0.3 jets.
D(pt) distribution for R=0.3 jets.
D(pt) distribution for R=0.3 jets.
D(pt) distribution for R=0.2 jets.
D(pt) distribution for R=0.2 jets.
D(pt) distribution for R=0.2 jets.
D(pt) distribution for R=0.2 jets.
D(pt) distribution for R=0.2 jets.
D(pt) distribution for R=0.2 jets.
D(pt) distribution for R=0.2 jets.
Ratio of D(z) distributions for R=0.4 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.4 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.4 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.4 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.4 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.4 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.3 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.3 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.3 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.3 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.3 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.3 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.2 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.2 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.2 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.2 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.2 jets for central to peripheral events.
Ratio of D(z) distributions for R=0.2 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.4 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.4 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.4 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.4 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.4 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.4 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.3 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.3 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.3 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.3 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.3 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.3 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.2 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.2 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.2 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.2 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.2 jets for central to peripheral events.
Ratio of D(pt) distributions for R=0.2 jets for central to peripheral events.
The distributions of transverse momentum and longitudinal momentum fraction of charged particles in jets are measured in Pb+Pb and pp collisions with the ATLAS detector at the LHC. The distributions are measured as a function of jet transverse momentum and rapidity. The analysis utilises an integrated luminosity of 0.14 nb$^{-1}$ of Pb+Pb data and 4.0 pb$^{-1}$ of pp data collected in 2011 and 2013, respectively, at the same centre-of-mass energy of 2.76 TeV per colliding nucleon pair. The distributions measured in pp collisions are used as a reference for those measured in Pb+Pb collisions in order to evaluate the impact on the internal structure of jets from the jet energy loss of fast partons propagating through the hot, dense medium created in heavy-ion collisions. Modest but significant centrality-dependent modifications of fragmentation functions in Pb+Pb collisions with respect to those in pp collisions are seen. No significant dependence of modifications on jet $p_{\mathrm{T}}$ and rapidity selections is observed except for the fragments with the highest transverse momenta for which some reduction of yields is observed for more forward jets.
D(pt) distributions for pp and Pb+Pb collisions, jet rapidity |y| < 2.1.
D(pt) distributions for pp and Pb+Pb collisions, jet rapidity |y| < 0.3.
D(pt) distributions for pp and Pb+Pb collisions, jet rapidity 0.3 < |y| < 0.8.
D(pt) distributions for pp and Pb+Pb collisions, jet rapidity 1.2 < |y| < 2.1.
D(z) distributions for pp and Pb+Pb collisions, jet rapidity |y| < 2.1.
D(z) distributions for pp and Pb+Pb collisions, jet rapidity |y| < 0.3.
D(z) distributions for pp and Pb+Pb collisions, jet rapidity 0.3 < |y| < 0.8.
D(z) distributions for pp and Pb+Pb collisions, jet rapidity 1.2 < |y| < 2.1.
Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.
Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.
Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.
Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.
Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.
Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.
Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.
Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.
Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.
Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.
Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.
Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.
Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.
Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.
Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.
Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.
Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.
Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.
Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.
The difference between the total yield of particles with 1 < pt^trk < 4 GeV measured in 0-80 PCT Pb+Pb collisions and the total yield measured in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.
The difference between the total yield of particles with 4 < pt^trk < 25 GeV measured in 0-80 PCT Pb+Pb collisions and the total yield measured in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.
The difference between the total yield of particles with 25 < pt^trk < 100 GeV measured in 0-80 PCT Pb+Pb collisions and the total yield measured in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.
The difference between the total transverse momentum of particles with 1 < pt^trk < 4 GeV measured in 0-80 PCT Pb+Pb collisions and the total transverse momentum of particles in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.
The difference between the total transverse momentum of particles with 4 < pt^trk < 25 GeV measured in 0-80 PCT Pb+Pb collisions and the total transverse momentum of particles in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.
The difference between the total transverse momentum of particles with 25 < pt^trk < 100 GeV measured in 0-80 PCT Pb+Pb collisions and the total transverse momentum of particles in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.
The ratio of R_D(z) distributions in three rapidity selections for 0-10 PCT Pb+Pb collisions.
The ratio of R_D(z) distributions in three rapidity selections for 10-20 PCT Pb+Pb collisions.
The ratio of R_D(z) distributions in three rapidity selections for 20-30 PCT Pb+Pb collisions.
This paper presents a measurement of jet fragmentation functions in 0.49 nb$^{-1}$ of Pb+Pb collisions and 25 pb$^{-1}$ of $pp$ collisions at $\sqrt{s_{NN}} = 5.02$ TeV collected in 2015 with the ATLAS detector at the LHC. These measurements provide insight into the jet quenching process in the quark-gluon plasma created in the aftermath of ultra-relativistic collisions between two nuclei. The modifications to the jet fragmentation functions are quantified by dividing the measurements in Pb+Pb collisions by baseline measurements in $pp$ collisions. This ratio is studied as a function of the transverse momentum of the jet, the jet rapidity, and the centrality of the collision. In both collision systems, the jet fragmentation functions are measured for jets with transverse momentum between 126 GeV and 398 GeV and with an absolute value of jet rapidity less than 2.1. An enhancement of particles carrying a small fraction of the jet momentum is observed, which increases with centrality and with increasing jet transverse momentum. Yields of particles carrying a very large fraction of the jet momentum are also observed to be enhanced. Between these two enhancements of the fragmentation functions a suppression of particles carrying an intermediate fraction of the jet momentum is observed in Pb+Pb collisions. A small dependence of the modifications on jet rapidity is observed.
The D(z) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 0.3.
The D(z) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 0.3.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 0.3.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 0.3.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 0.3.
The D(z) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 0.3.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 0.3.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 0.3.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 0.3.
The D(z) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 0.3.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 0.3.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 0.3.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 0.3.
The D(z) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 0.3.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 0.3.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 0.3.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 316.22 < pTjet < 398.10 and 0.0 < eta < 0.3.
The D(z) distributions in different centrality intervals in PbPb and in pp for 316.22 < pTjet < 398.10 and 0.0 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 316.22 < pTjet < 398.10 and 0.0 < eta < 0.3.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 316.22 < pTjet < 398.10 and 0.0 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 316.22 < pTjet < 398.10 and 0.0 < eta < 0.3.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 316.22 < pTjet < 398.10 and 0.0 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 316.22 < pTjet < 398.10 and 0.0 < eta < 0.3.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 316.22 < pTjet < 398.10 and 0.0 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 398.10 < pTjet < 501.18 and 0.0 < eta < 0.3.
The D(z) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 0.3.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 398.10 < pTjet < 501.18 and 0.0 < eta < 0.3.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 0.3.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 398.10 < pTjet < 501.18 and 0.0 < eta < 0.3.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 0.3.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 398.10 < pTjet < 501.18 and 0.0 < eta < 0.3.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 0.3.
The D(z) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.3 < eta < 0.8.
The D(z) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.3 < eta < 0.8.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.3 < eta < 0.8.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.3 < eta < 0.8.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.3 < eta < 0.8.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.3 < eta < 0.8.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.3 < eta < 0.8.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.3 < eta < 0.8.
The D(z) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.8 < eta < 1.2.
The D(z) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.8 < eta < 1.2.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.8 < eta < 1.2.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.8 < eta < 1.2.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.8 < eta < 1.2.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.8 < eta < 1.2.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.8 < eta < 1.2.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.8 < eta < 1.2.
The D(z) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 1.2 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 1.2 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 1.2 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 1.2 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 1.2 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 1.2 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 1.2 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 1.2 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 0.3.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 0.3.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 0.3.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 126.00 < pTjet < 158.49 and 0.0 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 0.3.
The D(z) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.3 < eta < 0.8.
The D(z) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.3 < eta < 0.8.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.3 < eta < 0.8.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.3 < eta < 0.8.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.3 < eta < 0.8.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.3 < eta < 0.8.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.3 < eta < 0.8.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.3 < eta < 0.8.
The D(z) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.8 < eta < 1.2.
The D(z) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.8 < eta < 1.2.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.8 < eta < 1.2.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.8 < eta < 1.2.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.8 < eta < 1.2.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.8 < eta < 1.2.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.8 < eta < 1.2.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.8 < eta < 1.2.
The D(z) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 1.2 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 1.2 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 1.2 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 1.2 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 1.2 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 1.2 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 1.2 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 1.2 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 0.3.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 0.3.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 0.3.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 158.49 < pTjet < 199.53 and 0.0 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 0.3.
The D(z) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.3 < eta < 0.8.
The D(z) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.3 < eta < 0.8.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.3 < eta < 0.8.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.3 < eta < 0.8.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.3 < eta < 0.8.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.3 < eta < 0.8.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.3 < eta < 0.8.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.3 < eta < 0.8.
The D(z) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.8 < eta < 1.2.
The D(z) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.8 < eta < 1.2.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.8 < eta < 1.2.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.8 < eta < 1.2.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.8 < eta < 1.2.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.8 < eta < 1.2.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.8 < eta < 1.2.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.8 < eta < 1.2.
The D(z) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 1.2 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 1.2 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 1.2 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 1.2 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 1.2 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 1.2 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 1.2 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 1.2 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 0.3.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 0.3.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 0.3.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 199.53 < pTjet < 251.19 and 0.0 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 0.3.
The D(z) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.3 < eta < 0.8.
The D(z) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.3 < eta < 0.8.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.3 < eta < 0.8.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.3 < eta < 0.8.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.3 < eta < 0.8.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.3 < eta < 0.8.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.3 < eta < 0.8.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.3 < eta < 0.8.
The D(z) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.8 < eta < 1.2.
The D(z) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.8 < eta < 1.2.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.8 < eta < 1.2.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.8 < eta < 1.2.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.8 < eta < 1.2.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.8 < eta < 1.2.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.8 < eta < 1.2.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.8 < eta < 1.2.
The D(z) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 1.2 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 1.2 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 1.2 < eta < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 1.2 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 1.2 < eta < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 1.2 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 1.2 < eta < 2.1.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 1.2 < eta < 2.1.
The D(z) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 2.1.
Excess transverse momenta in jet in PbPb compared to pp collisions in different centrality selections for abs(jet rapidity) < 2.1.
The D(pT) distributions in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 2.1.
Excess particles in jet in PbPb compared to pp collisions in different centrality selections for abs(jet rapidity) < 2.1.
The ratio of the D(z) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 2.1.
Ratio of R(D(z)) distributions in a given abs(jet rapidity) region to R(D(z)) for abs(jet rapidity) < 0.3 for 126 < pTJet < 158.5 GeV.
The ratio of the D(pT) in different centrality intervals in PbPb and in pp for 251.19 < pTjet < 316.22 and 0.0 < eta < 2.1.
Ratio of R(D(z)) distributions in a given abs(jet rapidity) region to R(D(z)) for abs(jet rapidity) < 0.3 for 158.5 < pTJet < 199.5 GeV.
Excess transverse momenta in jet in PbPb compared to pp collisions in different centrality selections for abs(jet rapidity) < 2.1.
Ratio of R(D(z)) distributions in a given abs(jet rapidity) region to R(D(z)) for abs(jet rapidity) < 0.3 for 199.5 < pTJet < 251.8 GeV.
Excess particles in jet in PbPb compared to pp collisions in different centrality selections for abs(jet rapidity) < 2.1.
Ratio of R(D(z)) distributions in a given abs(jet rapidity) region to R(D(z)) for abs(jet rapidity) < 0.3 for 126 < pTJet < 158.5 GeV.
Ratio of R(D(z)) distributions in a given abs(jet rapidity) region to R(D(z)) for abs(jet rapidity) < 0.3 for 158.5 < pTJet < 199.5 GeV.
Ratio of R(D(z)) distributions in a given abs(jet rapidity) region to R(D(z)) for abs(jet rapidity) < 0.3 for 199.5 < pTJet < 251.8 GeV.
This paper describes a measurement of light-by-light scattering based on Pb+Pb collision data recorded by the ATLAS experiment during Run 2 of the LHC. The study uses $2.2$ nb$^{-1}$ of integrated luminosity collected in 2015 and 2018 at $\sqrt{s_\mathrm{NN}}=5.02$ TeV. Light-by-light scattering candidates are selected in events with two photons produced exclusively, each with transverse energy $E_{\mathrm{T}}^{\gamma} > 2.5$ GeV, pseudorapidity $|\eta_{\gamma}| < 2.37$, diphoton invariant mass $m_{\gamma\gamma} > 5$ GeV, and with small diphoton transverse momentum and diphoton acoplanarity. The integrated and differential fiducial cross sections are measured and compared with theoretical predictions. The diphoton invariant mass distribution is used to set limits on the production of axion-like particles. This result provides the most stringent limits to date on axion-like particle production for masses in the range 6-100 GeV. Cross sections above 2 to 70 nb are excluded at the 95% CL in that mass interval.
Measurements of two-particle correlation functions and the first five azimuthal harmonics, $v_1$ to $v_5$, are presented, using 28 $\mathrm{nb}^{-1}$ of $p$+Pb collisions at a nucleon-nucleon center-of-mass energy of $\sqrt{s_{\mathrm{NN}}}=5.02$ TeV measured with the ATLAS detector at the LHC. Significant long-range "ridge-like" correlations are observed for pairs with small relative azimuthal angle ($|\Delta\phi|<\pi/3$) and back-to-back pairs ($|\Delta\phi| > 2\pi/3$) over the transverse momentum range $0.4 < p_{\rm T} < 12$ GeV and in different intervals of event activity. The event activity is defined by either the number of reconstructed tracks or the total transverse energy on the Pb-fragmentation side. The azimuthal structure of such long-range correlations is Fourier decomposed to obtain the harmonics $v_n$ as a function of $p_{\rm T}$ and event activity. The extracted $v_n$ values for $n=2$ to 5 decrease with $n$. The $v_2$ and $v_3$ values are found to be positive in the measured $p_{\rm T}$ range. The $v_1$ is also measured as a function of $p_{\rm T}$ and is observed to change sign around $p_{\rm T}\approx 1.5$-2.0 GeV and then increase to about 0.1 for $p_{\rm T}>4$ GeV. The $v_2(p_{\rm T})$, $v_3(p_{\rm T})$ and $v_4(p_{\rm T})$ are compared to the $v_n$ coefficients in Pb+Pb collisions at $\sqrt{s_{\mathrm{NN}}} =2.76$ TeV with similar event multiplicities. Reasonable agreement is observed after accounting for the difference in the average $p_{\rm T}$ of particles produced in the two collision systems.
The distributions of $N_{ch}^{rec}$ for MB and MB+HMT after applying an event-by-event weight, errors are statistical.
The distributions of $E_{T}^{Pb}$ [GeV] for MB and MB+HMT after applying an event-by-event weight, errors are statistical.
Per-trigger yield in 2D, $Y$($\Delta\phi$,$\Delta\eta$), for events with $E_{T}^{Pb} <$ 10 GeV and $N_{ch}^{rec} \geq$ 200 and recoil-subtracted per-trigger yield, $Y^{sub}$($\Delta\phi$,$\Delta\eta$) for events with $N_{ch}^{rec} \geq$ 200. Errors are statistical.
$v_{2,2}^{unsub}$ and $v_{2,2}$ as a function of $\Delta\eta$ calculated from the 2-D per-trigger yields in figure 4(a) and 4(b), respectively.
$v_{3,3}^{unsub}$ and $v_{3,3}$ as a function of $\Delta\eta$ calculated from the 2-D per-trigger yields in figure 4(a) and 4(b), respectively.
$v_{4,4}^{unsub}$ and $v_{4,4}$ as a function of $\Delta\eta$ calculated from the 2-D per-trigger yields in figure 4(a) and 4(b), respectively.
The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.
The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.
The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.
The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.
The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.
The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.
The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.
Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.
Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.
Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.
Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.
Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.
Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.
Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.
Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.
Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.
Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.
The integrated per-trigger yield, Y_{int}, on the near-side, the away-side and their difference and Y_{int} from the recoil as a function of event activity. Errors are statistical.
The integrated per-trigger yield, Y_{int}, on the near-side, the away-side and their difference and Y_{int} from the recoil as a function of event activity. Errors are statistical.
The Fourier coefficients $v_{n}$ as a function of $p_{T}^{a}$ extracted from the correlation functions, before and after the subtraction of the recoil component.
The Fourier coefficients $v_{n}$ as a function of $p_{T}^{a}$ extracted from the correlation functions, before and after the subtraction of the recoil component.
The Fourier coefficients $v_{n}$ as a function of $p_{T}^{a}$ extracted from the correlation functions, before and after the subtraction of the recoil component.
$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.
$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.
$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.
$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.
$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.
$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.
The centrality dependence of $v_{2}$ as a function of $N_{ch}^{rec}$. Values from before and after the recoil subtraction are included.
The centrality dependence of $v_{3}$ as a function of $N_{ch}^{rec}$. Values from before and after the recoil subtraction are included.
The centrality dependence of $v_{4}$ as a function of $N_{ch}^{rec}$. Values from before and after the recoil subtraction are included.
The centrality dependence of $v_{2}$ as a function of $E_{T}^{Pb}$. Values from before and after the recoil subtraction are included.
The centrality dependence of $v_{3}$ as a function of $E_{T}^{Pb}$. Values from before and after the recoil subtraction are included.
The centrality dependence of $v_{4}$ as a function of $E_{T}^{Pb}$. Values from before and after the recoil subtraction are included.
The $v_{2}$ as a function of $E_{T}^{Pb}$ obtained indirectly by mapping from the $N_{ch}^{rec}-dependence of $v_{2}$ using the correlation data shown in Fig. 2(b).
The $v_{3}$ as a function of $E_{T}^{Pb}$ obtained indirectly by mapping from the $N_{ch}^{rec}-dependence of $v_{3}$ using the correlation data shown in Fig. 2(b).
The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
The first-order harmonic $v_1$ obtained using factorization from $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
The first-order harmonic $v_1$ obtained using factorization from $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
The first-order harmonic $v_1$ obtained using factorization from $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.
$v_{2}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method.
$v_{2}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method, after the scaling.
$v_{3}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method.
$v_{3}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method, after the scaling.
$v_{4}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method.
$v_{4}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method, after the scaling.
Correlation between $E_{T}^{FCal}$ and $N_{ch}^{rec}$ for MB events (without weighting) and MB+HMT events (with weighting), errors are statistical.
Multi-particle cumulants and corresponding Fourier harmonics are measured for azimuthal angle distributions of charged particles in $pp$ collisions at $\sqrt{s}$ = 5.02 and 13 TeV and in $p$+Pb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV, and compared to the results obtained for low-multiplicity Pb+Pb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV. These measurements aim to assess the collective nature of particle production. The measurements of multi-particle cumulants confirm the evidence for collective phenomena in $p$+Pb and low-multiplicity Pb+Pb collisions. On the other hand, the $pp$ results for four-particle cumulants do not demonstrate collective behaviour, indicating that they may be biased by contributions from non-flow correlations. A comparison of multi-particle cumulants and derived Fourier harmonics across different collision systems is presented as a function of the charged-particle multiplicity. For a given multiplicity, the measured Fourier harmonics are largest in Pb+Pb, smaller in $p$+Pb and smallest in $pp$ collisions. The $pp$ results show no dependence on the collision energy, nor on the multiplicity.
$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.
$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.
$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for PbPb collisions at $\sqrt{ s_{NN} }$=2.76 TeV.
$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.
$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$c_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.
$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.
$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$c_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.
$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$c_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$c_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$c_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$c_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$c_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$c_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$c_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$c_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.
$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.
$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.
$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$c_3\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.
$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$c_3\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.
$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$c_4\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.
$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$c_4\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_3\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$v_3\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_3\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_3\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_3\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.
$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_4\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.
$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.
$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.
$v_4\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.
$ v_2\{4\} $ harmonics for reference particles with 0.2 $ < p_{T} < $ 3.0 GeV as a function of $ < N_{ch}(|\eta|<1) > $ for p+Pb collisions at $ \sqrt{ s_{NN} } $= 5.02 TeV.
$ v_2\{4\} $ harmonics for reference particles with 0.2 $ < p_{T}< $ 3.0 GeV as a function of $ < N_{ch}(|\eta|<1) > $ for Pb+Pb collisions at $ \sqrt{ s_{NN} } $= 2.76 TeV.
Jets created in association with a photon can be used as a calibrated probe to study energy loss in the medium created in nuclear collisions. Measurements of the transverse momentum balance between isolated photons and inclusive jets are presented using integrated luminosities of 0.49 nb$^{-1}$ of Pb+Pb collision data at $\sqrt{s_\mathrm{NN}}=5.02$ TeV and 25 pb$^{-1}$ of $pp$ collision data at $\sqrt{s}=5.02$ TeV recorded with the ATLAS detector at the LHC. Photons with transverse momentum $63.1 < p_\mathrm{T}^{\gamma} < 200$ GeV and $\left|\eta^{\gamma}\right| < 2.37$ are paired inclusively with all jets in the event that have $p_\mathrm{T}^\mathrm{jet} > 31.6$ GeV and pseudorapidity $\left|\eta^\mathrm{jet}\right| < 2.8$. The transverse momentum balance given by the jet-to-photon $p_\mathrm{T}$ ratio, $x_\mathrm{J\gamma}$, is measured for pairs with azimuthal opening angle $\Delta\phi > 7\pi/8$. Distributions of the per-photon jet yield as a function of $x_\mathrm{J\gamma}$, $(1/N_\gamma)(\mathrm{d}N/\mathrm{d}x_\mathrm{J\gamma})$, are corrected for detector effects via a two-dimensional unfolding procedure and reported at the particle level. In $pp$ collisions, the distributions are well described by Monte Carlo event generators. In Pb+Pb collisions, the $x_\mathrm{J\gamma}$ distribution is modified from that observed in $pp$ collisions with increasing centrality, consistent with the picture of parton energy loss in the hot nuclear medium. The data are compared with a suite of energy-loss models and calculations.
Photon-jet pT balance distributions (1/Ng)(dN/dxJg) in pp events (blue, reproduced on all panels) and Pb+Pb events (red) with each panel denoting a different centrality selection. These panels show results with pTg = 63.1-79.6 GeV. Total systematic uncertainties are shown as boxes, while statistical uncertainties are shown with vertical bars.
Photon-jet pT balance distributions (1/Ng)(dN/dxJg) in pp events (blue, reproduced on all panels) and Pb+Pb events (red) with each panel denoting a different centrality selection. These panels show results with pTg = 79.6-100 GeV. Total systematic uncertainties are shown as boxes, while statistical uncertainties are shown with vertical bars.
Photon-jet pT balance distributions (1/Ng)(dN/dxJg) in pp events (blue, reproduced on all panels) and Pb+Pb events (red) with each panel denoting a different centrality selection. These panels show results with pTg = 100-158 GeV. Total systematic uncertainties are shown as boxes, while statistical uncertainties are shown with vertical bars.
Photon-jet pT balance distributions (1/Ng)(dN/dxJg) in pp events (blue, reproduced on all panels) and Pb+Pb events (red) with each panel denoting a different centrality selection. These panels show results with pTg = 158-200 GeV. Total systematic uncertainties are shown as boxes, while statistical uncertainties are shown with vertical bars.
Selected comparisons of the nominal results in pp (blue) and 0-10% Pb+Pb (red) collisions with the central values obtained using a different photon-jet signal definition. Comparison of the nominal results (with DeltaPhi > 7pi/8) with those obtained using DeltaPhi > 3pi/4 for the pTg = 63.1-79.6 GeV range. Boxes indicate total systematic uncertainties, while vertical bars indicate statistical uncertainties.
Selected comparisons of the nominal results in pp (blue) and 0-10% Pb+Pb (red) collisions with the central values obtained using a different photon-jet signal definition. Comparison of the nominal results (inclusive jet selection) with those obtained using a photon-plus-leading-jet selection for the pTg = 100-158 GeV range. Boxes indicate total systematic uncertainties, while vertical bars indicate statistical uncertainties.
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