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CMS-PAS-SMP-25-009
Measurement of four-point energy-energy correlator subspaces in Z+jets events
Abstract: We present the first measurement of the resolved structure of four-point energy-energy correlators using the CMS detector at the LHC. Three geometrically distinct subspaces of the five-dimensional four-point configuration space - the tee, dipole, and right-triangle configurations - are measured in jets produced in association with a $ Z $ boson in proton-proton collisions at $ \sqrt{s} = $ 13 TeV, corresponding to 59.5 fb$ ^{-1} $ of data recorded in 2018. Results are unfolded to particle level and compared to predictions from Pythia 8 and Herwig 7. Herwig provides a systematically better description in the small-angle collinear and hadronization-sensitive regions, while Pythia describes the behavior at larger angular separations more accurately. These results constitute the first experimental probe of the resolved multipoint energy correlation structure of QCD jets at a hadron collider.
Figures & Tables Summary References CMS Publications
Figures

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Figure 1:
The three four-point EEC configurations: tee (left), dipole (center), and right-triangle (right). In each case the overall angular scale is $ R $, the secondary scale is parameterized by $ r $, and $ \phi $ gives the relative orientation.

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Figure 1-a:
The three four-point EEC configurations: tee (left), dipole (center), and right-triangle (right). In each case the overall angular scale is $ R $, the secondary scale is parameterized by $ r $, and $ \phi $ gives the relative orientation.

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Figure 1-b:
The three four-point EEC configurations: tee (left), dipole (center), and right-triangle (right). In each case the overall angular scale is $ R $, the secondary scale is parameterized by $ r $, and $ \phi $ gives the relative orientation.

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Figure 1-c:
The three four-point EEC configurations: tee (left), dipole (center), and right-triangle (right). In each case the overall angular scale is $ R $, the secondary scale is parameterized by $ r $, and $ \phi $ gives the relative orientation.

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Figure 2:
Unfolded tee-configuration distributions in the lowest (left) and highest (right) bins of the jet $ p_{\mathrm{T}} $. The measurement is only in the first quadrant, but has been replicated three times to make a full disk for ease of visualization.

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Figure 2-a:
Unfolded tee-configuration distributions in the lowest (left) and highest (right) bins of the jet $ p_{\mathrm{T}} $. The measurement is only in the first quadrant, but has been replicated three times to make a full disk for ease of visualization.

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Figure 2-b:
Unfolded tee-configuration distributions in the lowest (left) and highest (right) bins of the jet $ p_{\mathrm{T}} $. The measurement is only in the first quadrant, but has been replicated three times to make a full disk for ease of visualization.

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Figure 3:
Radial profile of the unfolded tee-configuration distributions, obtained by integrating over $ \phi $. Dashed lines illustrate the power-law scaling of the distributions in the perturbative region, with slopes that run with the jet $ p_{\mathrm{T}} $. At sufficiently small $ r $ the distributions flatten, indicating the onset of nonperturbative hadronization effects. The scale at which this flattening occurs is inversely proportional to the jet $ p_{\mathrm{T}} $.

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Figure 4:
Unfolded tee-configuration distributions in the lowest (left) and highest (right) bins of the jet $ p_{\mathrm{T}} $, with the bulk radial dependence factored out to reveal the angular structure as a function of $ \phi $. The measurement is only in the first quadrant, but has been replicated three times to make a full disk for ease of visualization.

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Figure 4-a:
Unfolded tee-configuration distributions in the lowest (left) and highest (right) bins of the jet $ p_{\mathrm{T}} $, with the bulk radial dependence factored out to reveal the angular structure as a function of $ \phi $. The measurement is only in the first quadrant, but has been replicated three times to make a full disk for ease of visualization.

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Figure 4-b:
Unfolded tee-configuration distributions in the lowest (left) and highest (right) bins of the jet $ p_{\mathrm{T}} $, with the bulk radial dependence factored out to reveal the angular structure as a function of $ \phi $. The measurement is only in the first quadrant, but has been replicated three times to make a full disk for ease of visualization.

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Figure 5:
Ratio of unfolded data to MC prediction for the tee configuration. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 50 $ < p_{\mathrm{T}}^{\text{jet}} < $ 90 GeV. Right: $ p_{\mathrm{T}}^{\text{jet}} > $ 400 GeV.

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Figure 5-a:
Ratio of unfolded data to MC prediction for the tee configuration. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 50 $ < p_{\mathrm{T}}^{\text{jet}} < $ 90 GeV. Right: $ p_{\mathrm{T}}^{\text{jet}} > $ 400 GeV.

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Figure 5-b:
Ratio of unfolded data to MC prediction for the tee configuration. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 50 $ < p_{\mathrm{T}}^{\text{jet}} < $ 90 GeV. Right: $ p_{\mathrm{T}}^{\text{jet}} > $ 400 GeV.

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Figure 5-c:
Ratio of unfolded data to MC prediction for the tee configuration. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 50 $ < p_{\mathrm{T}}^{\text{jet}} < $ 90 GeV. Right: $ p_{\mathrm{T}}^{\text{jet}} > $ 400 GeV.

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Figure 5-d:
Ratio of unfolded data to MC prediction for the tee configuration. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 50 $ < p_{\mathrm{T}}^{\text{jet}} < $ 90 GeV. Right: $ p_{\mathrm{T}}^{\text{jet}} > $ 400 GeV.

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Figure 6:
Ratio of unfolded data to MC prediction for the tee configuration, integrated over $ \phi $. Left: Data vs Pythia. Right: Data vs Herwig. Uncertainties represent the total statistical and systematic uncertainty in the unfolded data, as well as the statistical uncertainty in the MC prediction. Data points are offset slightly in $ r $ for visibility.

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Figure 6-a:
Ratio of unfolded data to MC prediction for the tee configuration, integrated over $ \phi $. Left: Data vs Pythia. Right: Data vs Herwig. Uncertainties represent the total statistical and systematic uncertainty in the unfolded data, as well as the statistical uncertainty in the MC prediction. Data points are offset slightly in $ r $ for visibility.

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Figure 6-b:
Ratio of unfolded data to MC prediction for the tee configuration, integrated over $ \phi $. Left: Data vs Pythia. Right: Data vs Herwig. Uncertainties represent the total statistical and systematic uncertainty in the unfolded data, as well as the statistical uncertainty in the MC prediction. Data points are offset slightly in $ r $ for visibility.

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Figure 7:
Ratio of unfolded data to MC prediction for the tee configuration as a function of $ \phi $. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 0 $ < R < $ 0.2. Right: 0.8 $ < R < $ 1.0. Uncertainties represent the total statistical and systematic uncertainty in the unfolded data, as well as the statistical uncertainty in the MC prediction. Data points are offset slightly in $ \phi $ for visibility.

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Figure 7-a:
Ratio of unfolded data to MC prediction for the tee configuration as a function of $ \phi $. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 0 $ < R < $ 0.2. Right: 0.8 $ < R < $ 1.0. Uncertainties represent the total statistical and systematic uncertainty in the unfolded data, as well as the statistical uncertainty in the MC prediction. Data points are offset slightly in $ \phi $ for visibility.

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Figure 7-b:
Ratio of unfolded data to MC prediction for the tee configuration as a function of $ \phi $. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 0 $ < R < $ 0.2. Right: 0.8 $ < R < $ 1.0. Uncertainties represent the total statistical and systematic uncertainty in the unfolded data, as well as the statistical uncertainty in the MC prediction. Data points are offset slightly in $ \phi $ for visibility.

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Figure 7-c:
Ratio of unfolded data to MC prediction for the tee configuration as a function of $ \phi $. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 0 $ < R < $ 0.2. Right: 0.8 $ < R < $ 1.0. Uncertainties represent the total statistical and systematic uncertainty in the unfolded data, as well as the statistical uncertainty in the MC prediction. Data points are offset slightly in $ \phi $ for visibility.

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Figure 7-d:
Ratio of unfolded data to MC prediction for the tee configuration as a function of $ \phi $. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 0 $ < R < $ 0.2. Right: 0.8 $ < R < $ 1.0. Uncertainties represent the total statistical and systematic uncertainty in the unfolded data, as well as the statistical uncertainty in the MC prediction. Data points are offset slightly in $ \phi $ for visibility.

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Figure 8:
Unfolded dipole-configuration distributions in the lowest (left) and highest (right) bins of jet $ p_{\mathrm{T}} $. The measurement is only in the first quadrant, but has been replicated three times to make a full disk for ease of visualization.

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Figure 8-a:
Unfolded dipole-configuration distributions in the lowest (left) and highest (right) bins of jet $ p_{\mathrm{T}} $. The measurement is only in the first quadrant, but has been replicated three times to make a full disk for ease of visualization.

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Figure 8-b:
Unfolded dipole-configuration distributions in the lowest (left) and highest (right) bins of jet $ p_{\mathrm{T}} $. The measurement is only in the first quadrant, but has been replicated three times to make a full disk for ease of visualization.

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Figure 9:
Radial profile of the unfolded dipole configuration distributions, obtained by integrating over $ \phi $. The two collinear singularities at $ r \to $ 0 and $ r \to $ 1 are visible, and exhibit different scaling behavior as a function of $ r $, with the $ r \to $ 0 singularity narrower than the $ r \to $ 1 singularity. The relative magnitude of the two singularities changes with the jet $ p_{\mathrm{T}} $, with the $ r \to $ 1 singularity becoming more pronounced at higher momentum.

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Figure 10:
Ratio of unfolded data to MC predictions for the dipole configuration. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 50 $ < p_{\mathrm{T}}^{\text{jet}} < $ 90 GeV. Right: $ p_{\mathrm{T}}^{\text{jet}} > $ 400 GeV. The measurement is only in the first quadrant, but has been replicated three times to make a full disk for ease of visualization.

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Figure 10-a:
Ratio of unfolded data to MC predictions for the dipole configuration. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 50 $ < p_{\mathrm{T}}^{\text{jet}} < $ 90 GeV. Right: $ p_{\mathrm{T}}^{\text{jet}} > $ 400 GeV. The measurement is only in the first quadrant, but has been replicated three times to make a full disk for ease of visualization.

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Figure 10-b:
Ratio of unfolded data to MC predictions for the dipole configuration. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 50 $ < p_{\mathrm{T}}^{\text{jet}} < $ 90 GeV. Right: $ p_{\mathrm{T}}^{\text{jet}} > $ 400 GeV. The measurement is only in the first quadrant, but has been replicated three times to make a full disk for ease of visualization.

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Figure 10-c:
Ratio of unfolded data to MC predictions for the dipole configuration. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 50 $ < p_{\mathrm{T}}^{\text{jet}} < $ 90 GeV. Right: $ p_{\mathrm{T}}^{\text{jet}} > $ 400 GeV. The measurement is only in the first quadrant, but has been replicated three times to make a full disk for ease of visualization.

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Figure 10-d:
Ratio of unfolded data to MC predictions for the dipole configuration. Top: Data vs Pythia. Bottom: Data vs Herwig. Left: 50 $ < p_{\mathrm{T}}^{\text{jet}} < $ 90 GeV. Right: $ p_{\mathrm{T}}^{\text{jet}} > $ 400 GeV. The measurement is only in the first quadrant, but has been replicated three times to make a full disk for ease of visualization.

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Figure 11:
Ratio of unfolded data to MC predictions for the dipole configuration, integrated over $ \phi $. Left: Data vs Pythia. Right: Data vs Herwig. Uncertainties represent the total statistical and systematic uncertainty in the unfolded data, as well as the statistical uncertainty in the MC prediction. Data points are offset slightly in $ r $ for visibility.

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Figure 11-a:
Ratio of unfolded data to MC predictions for the dipole configuration, integrated over $ \phi $. Left: Data vs Pythia. Right: Data vs Herwig. Uncertainties represent the total statistical and systematic uncertainty in the unfolded data, as well as the statistical uncertainty in the MC prediction. Data points are offset slightly in $ r $ for visibility.

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Figure 11-b:
Ratio of unfolded data to MC predictions for the dipole configuration, integrated over $ \phi $. Left: Data vs Pythia. Right: Data vs Herwig. Uncertainties represent the total statistical and systematic uncertainty in the unfolded data, as well as the statistical uncertainty in the MC prediction. Data points are offset slightly in $ r $ for visibility.

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Figure 12:
Unfolded triangle-configuration distributions as a function of jet $ p_{\mathrm{T}} $. The full $ \phi \in [0,2\pi) $ range is shown; the three corners of the 3-4-5 triangle are visible as collinear enhancements where the floating particle comes close to the fixed triangle vertices.

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Figure 12-a:
Unfolded triangle-configuration distributions as a function of jet $ p_{\mathrm{T}} $. The full $ \phi \in [0,2\pi) $ range is shown; the three corners of the 3-4-5 triangle are visible as collinear enhancements where the floating particle comes close to the fixed triangle vertices.

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Figure 12-b:
Unfolded triangle-configuration distributions as a function of jet $ p_{\mathrm{T}} $. The full $ \phi \in [0,2\pi) $ range is shown; the three corners of the 3-4-5 triangle are visible as collinear enhancements where the floating particle comes close to the fixed triangle vertices.
Tables

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Table 1:
Bin-averaged uncertainty breakdown for the three configurations. Systematic uncertainties dominate at low jet $ p_{\mathrm{T}} $, while statistical uncertainties dominate at high momentum. Quoted uncertainties are with respect to normalized distributions per each bin of jet $ p_T $.

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Table 2:
Closure tests of the unfolding procedure, validating the modeling uncertainty. The event kinematics closure attempts to unfold the nominal PYTHIA 8 simulation with a detector model reweighted to match the $ Z $ boson kinematics in data, while the parton shower & hadronization closure attempts to unfold the HERWIG 7 simulation with the nominal PYTHIA 8 detector model. The $ \Delta \chi^2 $ values are computed as the $ \chi^2 $ between the unfolded and truth-level distributions in the closure test, minus the $ \chi^2 $ between the unfolded and truth-level distributions in the nominal simulation (which is nearly zero). All $ \chi^2 $ values are computed only in the signal bins (i.e., excluding overflow/underflow bins), and using the full covariance matrix of the unfolded distribution including both statistical and systematic uncertainties (and all correlations).

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Table 3:
$ \chi^2 $ between the unfolded data and generator-level Pythia and Herwig predictions, in the analysis bins 0.4 $ < R < $ 0.5 and $ p_{\mathrm{T}} > $ 50 GeV, taking into account the full covariance matrix of the unfolded data (including both statistical and systematic uncertainties, and all correlations) as well as the statistical covariance matrix of the MC predictions.
Summary
We have presented the first measurement of the resolved structure of the four-point energy-energy correlators in hadronic jets, using 59.5 fb$ ^{-1} $ of $ Z $+jets data collected by the CMS experiment at $ \sqrt{s} = $ 13 TeV. Three subspaces of the five-dimensional four-point configuration space covering the tee, dipole, and right-triangle configurations are measured over a broad range of jet momenta and unfolded to particle level using a GPU-accelerated likelihood-based framework. The measurements reveal a rich angular structure in the four-point EEC that is qualitatively distinct from the previously measured bulk scaling properties of the two-point and 1D projected three-point correlators. These results represent a rigorous test of QCD factorization and the underlying parton shower dynamics, and provide a new class of precision jet substructure observables that can be used to constrain the modeling of QCD in the perturbative and nonperturbative regimes. Comparing to state-of-the-art parton shower predictions, we find that both PYTHIA8 (CP5 tune) and HERWIG 7 (CH3 tune) are strongly disfavored by the data in all three configurations. The two generators disagree with each other in characteristic ways that reveal the physical differences in their underlying shower and hadronization models. Detailed analysis of the data/MC for the tee configuration reveals that both showers fail to capture the correct slope of the collinear singularity in the perturbative region (with Herwig disagreeing more strongly with the data than Pythia), while Herwig's hadronization model appears to better capture the nonperturbative behavior in the $ r \to $ 0 region. This is likely to be related to the fact that Herwig's angular-ordered shower emphasizes color-coherence, which is critical in the collinear limit. Pythia, by contrast, provides a better description of the distributions at larger values of $ r $, corresponding to more widely-separated multi-parton configurations. In these regions, where the four particles span a larger fraction of the jet radius and the angular correlations are less dominated by the collinear singularity, Pythia's $ p_{\mathrm{T}} $-ordered shower captures more of the relevant dynamics. The complementary nature of these discrepancies shows that current parton shower models embody qualitatively different assumptions about color coherence and the ordering of emissions, and neither the angular-ordered nor the $ p_{\mathrm{T}} $-ordered approach is adequate. The four-point EEC measurements presented here provide the first precise, multi-dimensional experimental input that can directly discriminate between these models at the level of the four-parton correlation structure. These results establish resolved multi-point EECs as a new class of precision jet substructure observables at the LHC.
References
1 R. Kogler et al. Jet Substructure at the Large Hadron Collider: Experimental Review Rev. Mod. Phys. 91 (2019) 045003 1803.06991
2 A. J. Larkoski, I. Moult, and B. Nachman Jet Substructure at the Large Hadron Collider: A Review of Recent Advances in Theory and Machine Learning Phys. Rept. 841 (2020) 1 1709.04464
3 H. Chen, I. Moult, X. Zhang, and H. X. Zhu Rethinking jets with energy correlators: Tracks, resummation, and analytic continuation PRD 102 (2020) 054012
4 CMS Collaboration Measurement of Energy Correlators inside Jets and Determination of the Strong Coupling \ensuremath\alphaS(mZ) PRL 133 (2024) 071903 CMS-SMP-22-015
2402.13864
5 ALICE Collaboration Energy-energy correlators in charm-tagged jets in proton-proton collisions at $ \mathbf{\sqrt{s} = 13} $ TeV 2504.03431
6 S. Acharya et al. Exposing the parton-hadron transition within jets with energy-energy correlators in pp collisions at $ \sqrt{s}= $ 5.02 TeV Phys. Rev. D, 2026
link
7 STAR Collaboration Measurement of Two-Point Energy Correlators within Jets in p+p Collisions at s=200 GeV PRL 135 (2025) 111901 2502.15925
8 Tamis, Andrew Exploiting two- and three-point charge-energy correlators at STAR as probes of jet evolution in EPJ Web Conf., volume 339, 2002
link
9 H. Chen, I. Moult, and H. X. Zhu Quantum interference in jet substructure from spinning gluons PRL 126 (2021)
10 A. Karlberg, G. P. Salam, L. Scyboz, and R. Verheyen Spin correlations in final-state parton showers and jet observables EPJC 81 (2021)
11 C.-H. Chang and D. Simmons-Duffin Three-point energy correlators and the celestial block expansion JHEP 2023 (2023)
12 M. Gonzalez et al. Dissecting Parton Showers with Multi-Point Energy Correlators 2607.07792
13 CMS Collaboration The CMS experiment at the CERN LHC JINST 3 (2008) S08004
14 CMS Collaboration Development of the CMS detector for the CERN LHC Run 3 JINST 19 (2024) P05064 CMS-PRF-21-001
2309.05466
15 CMS Collaboration Performance of the CMS Level-1 trigger in proton-proton collisions at $ \sqrt{s} = $ 13 TeV JINST 15 (2020) P10017 CMS-TRG-17-001
2006.10165
16 CMS Collaboration The CMS trigger system JINST 12 (2017) P01020 CMS-TRG-12-001
1609.02366
17 CMS Collaboration Performance of the CMS high-level trigger during LHC Run 2 JINST 19 (2024) P11021 CMS-TRG-19-001
2410.17038
18 CMS Collaboration Electron and photon reconstruction and identification with the CMS experiment at the CERN LHC JINST 16 (2021) P05014 CMS-EGM-17-001
2012.06888
19 CMS Collaboration Performance of the CMS muon detector and muon reconstruction with proton-proton collisions at $ \sqrt{s} = $ 13 TeV JINST 13 (2018) P06015
20 CMS Collaboration Description and Performance of Track and Primary-Vertex Reconstruction with the CMS Tracker JINST 9 (2014) P10009 CMS-TRK-11-001
1405.6569
21 CMS Collaboration Particle-flow reconstruction and global event description with the CMS detector JINST 12 (2017) P10003 CMS-PRF-14-001
1706.04965
22 CMS Collaboration Performance of reconstruction and identification of $ \tau $ leptons decaying to hadrons and $ \nu_\tau $ in pp collisions at $ \sqrt{s}= $ 13 TeV JINST 13 (2018) P10005 CMS-TAU-16-003
1809.02816
23 CMS Collaboration Jet energy scale and resolution in the CMS experiment in pp collisions at 8 TeV JINST 12 (2017) P02014 CMS-JME-13-004
1607.03663
24 CMS Collaboration Performance of missing transverse momentum reconstruction in proton-proton collisions at $ \sqrt{s} = $ 13 TeV using the CMS detector JINST 14 (2019) P07004 CMS-JME-17-001
1903.06078
25 CMS Collaboration Pileup mitigation at CMS in 13 TeV data JINST 15 (2020) P09018 CMS-JME-18-001
2003.00503
26 D. Bertolini, P. Harris, M. Low, and N. Tran Pileup per particle identification JHEP 10 (2014) 059 1407.6013
27 CMS Collaboration CMS luminosity measurement for the 2018 data-taking period at $ \sqrt{s} = $ 13 TeV Technical Report, CERN, Geneva, 2019
CMS-PAS-LUM-18-002
CMS-PAS-LUM-18-002
28 Particle Data Group Collaboration Review of particle physics PRD 110 (2024) 030001
29 CMS Collaboration Identification of heavy-flavour jets with the CMS detector in pp collisions at 13 TeV JINST 13 (2018) P05011 CMS-BTV-16-002
1712.07158
30 CMS Collaboration Performance of the DeepJet b tagging algorithm using 41.9/fb of data from proton-proton collisions at 13 TeV with Phase 1 CMS detector CMS Detector Performance Note CMS-DP-2018-058, 2018
CDS
31 E. Bols et al. Jet flavour classification using DeepJet JINST 15 (2020) P12012 2008.10519
32 J. Alwall et al. Madgraph 5: going beyond JHEP 2011 (2011)
33 T. Sjöstrand et al. An introduction to PYTHIA 8.2 Comput. Phys. Commun. 191 (2015) 159 1410.3012
34 CMS Collaboration Extraction and validation of a new set of CMS PYTHIA8 tunes from underlying-event measurements EPJC 80 (2020) 4 CMS-GEN-17-001
1903.12179
35 J. Bellm et al. Herwig 7.2 release note EPJC 80 (2020) 452 1912.06509
36 CMS Collaboration Development and validation of HERWIG 7 tunes from CMS underlying-event measurements EPJC 81 (2021) 312 CMS-GEN-19-001
2011.03422
37 J. Alwall et al. Comparative study of various algorithms for the merging of parton showers and matrix elements in hadronic collisions EPJC 53 (2007) 473
38 J. M. Lindert et al. Precise predictions for $ V+ $ jets dark matter backgrounds EPJC 77 (2017) 829 1705.04664
39 NNPDF Collaboration Parton distributions for the LHC Run II JHEP 04 (2015) 040 1410.8849
40 GEANT4 Collaboration GEANT 4---a simulation toolkit NIM A 506 (2003) 250
41 M. Cacciari, G. P. Salam, and G. Soyez FastJet user manual EPJC 72 (2012) 1896 1111.6097
42 M. Cacciari, G. P. Salam, and G. Soyez The anti-$ k_{\mathrm{T}} $ jet clustering algorithm JHEP 2008 (2008) 063
43 CMS Collaboration Jet algorithms performance in 13 TeV data CMS Physics Analysis Summary, CERN, 2017
CMS-PAS-JME-16-003
CMS-PAS-JME-16-003
44 R. Feinman Pytorch-minimize: a library for numerical optimization with autograd https://github.com/rfeinman/pytorch-minimize, 2021
link
45 J. Ansel et al. Pytorch 2: Faster machine learning through dynamic python bytecode transformation and graph compilation in the ACM International Conference on Architectural Support for Programming Languages and Operating Systems, Volume 2, ASPLOS '24, Association for Computing Machinery, New York, NY, USA, 2024
Proceedings of the 2 (2024) 929
46 CMS Collaboration Tracking performances for charged pions with Run2 Legacy data CMS Detector Performance Summary CMS-DP-2022-012, CERN, 2022
CDS
47 CMS Collaboration High $ p_{\mathrm{T}} $ jets tracking CMS Detector Performance Summary CMS-DP-2014-032, CERN, 2014
link
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