REVIEW 2 major objections 5 minor 1 cited by
Probing jet-medium interactions via jet substructure observables in relativistic heavy-ion collisions
T0 review · 2 major / 5 minor · reviewed 2026-08-15 · deepseek-v4-flash
Pith's one-line read This paper shows that the enhancement of groomed jet mass in central lead-lead collisions originates from elastic jet-medium scattering at large angles, not from hadronization or hadronic rescatterings.
desk verdict Useful AMPT stage-decomposition study of groomed jet mass, but the headline 'large-angle scattering' claim is confounded: the two Soft Drop settings change both z_cut and beta, so the null under strong grooming does not isolate angular dependence. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The load-bearing mechanism is the Soft Drop grooming algorithm applied with two parameter sets, operating on jets reconstructed with the anti-$k_T$ algorithm ($R=0.4$) after constituent subtraction. The weak setting ($z_{\mathrm{cut}}=0.1,\beta=0.0$) keeps peripheral subjets, exposing the large-angle medium response; the strong setting ($z_{\mathrm{cut}}=0.5,\beta=1.5$) restricts the groomed jet to its core, hiding that response. The argument also relies on the stage-by-stage decomposition of the AMPT model (initial state, parton cascade, hadronization, hadronic rescatterings), which isolates the parton-cascade contribution from non-perturbative late-stage effects.
What would settle it
Run the same AMPT setup with radiative energy loss added while leaving elastic scatterings unchanged: if the high-mass tail in $M_g/p_{T,\mathrm{jet}}$ disappears rather than persisting, the claim that elastic large-angle scattering is the dominant mechanism is falsified.
Extended reading notes
Core claim
In central PbPb collisions at $\sqrt{s_{NN}}=5.02$ TeV, the Soft Drop groomed jet mass ratio $M_g/p_{T,\mathrm{jet}}$ develops a pronounced high-mass tail that grows as events become more central and as $p_{T,\mathrm{jet}}$ decreases, while the splitting fraction $z_g$ shows only a slight shift toward asymmetric splittings. Tracing the observable stage by stage through the AMPT multi-phase transport model evolution, the entire enhancement appears at the parton-cascade stage, where the jet's partons undergo two-body elastic scatterings with medium partons; hadronization and hadronic rescatterings add negligible contribution after grooming. Switching off partonic interactions (0 mb cross section) removes the modification entirely, and applying a stronger grooming condition that suppresses large-angle subjets also removes it, indicating that the modification is carried by large-angle scattering.
Load-bearing premise
The load-bearing assumption is that the AMPT parton cascade, which contains only two-body elastic scatterings and no radiative energy loss, captures the dominant jet-medium interactions behind the mass enhancement; if inelastic processes such as medium-induced gluon radiation are required to produce the tail, the paper's large-angle elastic interpretation is weakened.
Editorial extensions
If this is right
- If the claim holds, $M_g/p_{T,\mathrm{jet}}$ can serve as a targeted probe of large-angle elastic energy transport in the quark-gluon plasma, complementing $z_g$ and $r_g$.
- The enhancement is largest in 0-10% central events and at $p_{T,\mathrm{jet}}<160$ GeV, giving a concrete scaling benchmark for models that include medium response.
- The absence of modification under strong grooming implies that the jet core remains essentially unmodified, so the medium acts primarily on the periphery of the jet.
- Because the enhancement appears entirely at the parton-cascade stage in this model, late-stage hadronic interactions cannot be its source.
Reading between the lines
- One extension not drawn out in the paper would be to correlate the size of the high-mass tail with the jet path length through the medium; a centrality-selected measurement at fixed $p_{T,\mathrm{jet}}$ could test that dependence directly.
- Applying the same stage-decomposition to the groomed splitting radius $r_g$ would likely show almost no medium modification, since small-angle splittings are dominated by vacuum radiation.
- If radiative energy loss were added to the cascade, the generated small-angle splittings might dilute the large-angle high-mass tail; the paper itself flags radiative loss as a future direction.
Signed reviews
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. This manuscript presents an AMPT (string melting) study of the Soft Drop groomed observables z_g and M_g/pT_jet in pp and PbPb collisions at sqrt(s_NN) = 5.02 TeV, using constituent subtraction to mitigate background and the CMS-like smearing procedure for pp comparisons. The authors report a slight enhancement of asymmetric z_g splittings in central PbPb events, a pronounced enhancement of the high-M_g/pT_jet tail at low pT_jet and in central events, and a stage-by-stage analysis indicating that this enhancement appears during the parton cascade and is largely preserved through hadronization and hadronic rescatterings. They further find that a stronger grooming setting (z_cut=0.5, beta=1.5) removes the M_g/pT_jet modification, and interpret this as evidence that the medium-induced modification is predominantly associated with large-angle scattering. The paper compares the model with CMS data in pp and PbPb and reports qualitative agreement, with the 0 mb parton-cross-section setting serving as a no-interaction baseline.
Significance. If the conclusions are supported, the paper offers a controlled and parameter-free-with-respect-to-the-target-observables model study of jet-medium interactions, with a clean 3 mb versus 0 mb comparison and a dynamical-stage decomposition. The strengths are that the parton cross section (3 mb) is fixed by earlier flow studies rather than fitted to the substructure data, and that the four-stage analysis in Fig. 7 is a useful diagnostic for separating partonic and hadronic effects. The comparison with CMS data for both z_g and M_g/pT_jet also anchors the model. However, the central attribution of the effect to large-angle scattering is not uniquely determined by the presented grooming comparison, and the quantitative significance of the enhancement is not established because the model curves carry no statistical uncertainties. These points are load-bearing for the abstract's claims, so the current version is not yet ready for acceptance.
major comments (2)
- [III B, Figs. 4–7] All model curves are shown without statistical uncertainties, although the central positive claim is a 'pronounced enhancement' in the high-M_g/pT_jet region. Without uncertainties on the ratios, a reader cannot judge whether the enhancement in the last bin of Fig. 5 (left) or the low-pT_jet enhancement in Fig. 6 (left) is statistically significant or a fluctuation. The manuscript itself calls the effect 'a hint' in Sec. III B while the abstract calls it 'pronounced'; this inconsistency underscores the need for uncertainty quantification. The authors should either include statistical error bands on the AMPT ratios or explicitly report the statistical significance of the enhancement bins.
- [II A (2), IV] The AMPT parton cascade used here contains only two-body elastic scatterings; there are no radiative or inelastic energy-loss processes in the model. Since the claimed enhancement is traced entirely to the parton cascade stage, the conclusion that 'jet-medium interactions' produce the enhancement is a statement about elastic scattering only. The manuscript acknowledges this in Sec. IV, but the abstract and Sec. III B state the large-angle conclusion without this qualification. The wording should be changed to make explicit that the model predicts that elastic scattering produces the effect, and that a radiative-energy-loss implementation may alter the small-angle behavior, which is already noted in the final paragraph. This is a scope limitation rather than an internal inconsistency, but it is essential to the interpretation of the central claim.
minor comments (5)
- [Abstract and III B] The terminology is inconsistent: the abstract says a 'pronounced enhancement' while Sec. III B (after Fig. 5) calls the same effect 'a hint of enhancement'; the authors should use one consistent descriptor once statistical significance is quantified.
- [III B] The sentence 'In a word, our analysis demonstrates...' is informal for a journal article; 'In summary' would be more suitable.
- [Fig. 5 and Fig. 6 captions] The captions list centrality and pT_jet offset labels, but the figures themselves do not define the offset constants; a brief explanation of the '(+N)' notation in the caption would improve readability.
- [II C, Eq. (5)] The definition of M_g via the two Soft Drop subjets is correct for the working point used, but a sentence clarifying that the groomed jet mass is computed from the two subjets, rather than from all groomed constituents, would remove a possible ambiguity for readers familiar with other Soft Drop implementations.
- [III A] In the discussion of JEWEL, the phrase 'with four-momentum subtraction method' could be expanded to 'with the four-momentum subtraction scheme for medium response' to be more precise, though the reference is clear.
Circularity Check
No significant circularity: the AMPT comparison is a controlled model study with no fit to the target observables.
full rationale
The paper's central claim is that AMPT with partonic interactions (3 mb) produces an enhancement in Mg/pT,jet that is absent at 0 mb and absent under stronger grooming. The 3 mb cross section is taken from prior flow calibration, not fitted to jet substructure; the 0 mb baseline is a controlled switch-off of jet-medium interactions. The Soft Drop parameters follow CMS choices. The stage-by-stage analysis in Fig. 7 directly isolates the parton cascade as the stage where the modification appears, rather than importing that conclusion from a citation. Self-citations such as [61] and [87,88] are contextual or auxiliary and are not used to define the result; Fig. 7 and the 0 mb/3 mb contrast stand independently. The only caveat is that the contrast between (z_cut=0.1, beta=0.0) and (z_cut=0.5, beta=1.5) changes two grooming parameters simultaneously, so the 'large-angle' attribution is underdetermined; that is a validity concern, not a circular reduction of output to input. No equation equals another by construction and no fitted parameter is renamed as a prediction.
Assumptions & free parameters
free parameters (1)
- Parton cross section sigma =
3 mb
assumptions (4)
- domain assumption AMPT string-melting model stages (HIJING initial conditions, ZPC cascade, coalescence, ART rescatterings) provide a realistic description of jet and bulk evolution at 5.02 TeV.
- domain assumption ZPC two-body elastic parton scattering with the LO gluon-gluon cross section captures the jet-medium interactions relevant for groomed jet mass.
- domain assumption Constituent subtraction on smeared pp and PbPb events removes the underlying event without disturbing jet substructure.
- domain assumption Soft Drop grooming with z_cut=0.1, beta=0.0 and z_cut=0.5, beta=1.5 plus Delta R12>0.1 cleanly separates the jet core from large-angle radiation.
Cite this review
Pith. "Pith review of Probing jet-medium interactions via jet substructure observables in relativistic heavy-ion collisions." pith.science (2026). https://pith.science/paper/ZAMCRABT
@misc{pith2026250619033,
author = {Pith},
title = {Pith review of: Probing jet-medium interactions via jet substructure observables in relativistic heavy-ion collisions},
year = {2026},
howpublished = {\url{https://pith.science/paper/ZAMCRABT}},
note = {Machine review of arXiv:2506.19033}
}
abstract
We present a comprehensive study of jet substructure observables in $pp$ and PbPb collisions at $\sqrt{s_{NN}} = 5.02$~TeV using a multi-phase transport model. To suppress background contamination, the constituent subtraction method is employed for both PbPb and smeared $pp$ events. The jet splitting momentum fraction ($z_g$) and the groomed jet mass to the ungroomed jet transverse momentum ($M_g / p_{T,\text{jet}}$) are reconstructed using the Soft Drop algorithm with two grooming parameter settings. With $z_\text{cut} = 0.1$ and $\beta = 0.0$, a slight modification in the $z_g$ distribution is observed in central PbPb collisions, whereas a pronounced enhancement in the high $M_g / p_{T,\text{jet}}$ region is found, particularly at low $p_{T,\text{jet}}$ and in more central events. A detailed analysis of the dynamical evolution stages reveals that this enhancement primarily originates from jet-medium interactions, whereas the contributions from hadronization and hadronic rescatterings are largely mitigated by the grooming procedure. In contrast, under a stronger grooming condition ($z_\text{cut} = 0.5$, $\beta = 1.5$), no significant changes in $M_g / p_{T,\text{jet}}$ are observed, indicating that the medium-induced modifications are predominantly associated with large-angle scattering.
Figures
Figures from the paper (4 more)
Forward citations
Cited by 1 Pith paper
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An improved linear Boltzmann transport model for hadron and jet suppression in ultrarelativistic heavy-ion collisions
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Reference graph
Works this paper leans on
-
[61]
X.-P. Duan and G.-L. Ma, Eur. Phys. J. A59, 61 (2023), arXiv:2303.03773 [nucl-th]
work page Pith review arXiv 2023
-
[1]
I. Arseneet al.(BRAHMS), Nucl. Phys. A757, 1 (2005), arXiv:nucl-ex/0410020
arXiv 2005
-
[2]
B. B. Backet al.(PHOBOS), Nucl. Phys. A757, 28 (2005), arXiv:nucl-ex/0410022
arXiv 2005
-
[3]
K. Adcoxet al.(PHENIX), Nucl. Phys. A757, 184 (2005), arXiv:nucl-ex/0410003
arXiv 2005
-
[4]
J. Adamset al.(STAR), Nucl. Phys. A757, 102 (2005), arXiv:nucl-ex/0501009
arXiv 2005
-
[5]
K. J. Eskola, H. Paukkunen, and C. A. Salgado, JHEP 07, 102, arXiv:0802.0139 [hep-ph]
- [6]
-
[7]
C. Shen and L. Yan, Nucl. Sci. Tech.31, 122 (2020), arXiv:2010.12377 [nucl-th]
arXiv 2020
Show all 101 references
-
[8]
Chenet al., Nucl
J. Chenet al., Nucl. Sci. Tech.35, 214 (2024), arXiv:2407.02935 [nucl-ex]
2024 arXiv
-
[9]
Aadet al.(ATLAS), Phys
G. Aadet al.(ATLAS), Phys. Rev. Lett.105, 252303 (2010), arXiv:1011.6182 [hep-ex]
2010 arXiv
-
[10]
Aamodtet al.(ALICE), Phys
K. Aamodtet al.(ALICE), Phys. Lett. B696, 30 (2011), arXiv:1012.1004 [nucl-ex]
2011 arXiv
-
[11]
Chatrchyanet al.(CMS), Eur
S. Chatrchyanet al.(CMS), Eur. Phys. J. C72, 1945 (2012), arXiv:1202.2554 [nucl-ex]
2012 arXiv
-
[12]
H. Song, Y. Zhou, and K. Gajdosova, Nucl. Sci. Tech. 28, 99 (2017), arXiv:1703.00670 [nucl-th]
2017 arXiv
-
[13]
Shouet al., Nucl
Q.-Y. Shouet al., Nucl. Sci. Tech.35, 219 (2024), arXiv:2409.17964 [nucl-ex]
2024 arXiv
-
[14]
Gyulassy and L
M. Gyulassy and L. McLerran, Nucl. Phys. A750, 30 (2005), arXiv:nucl-th/0405013
2005 arXiv
- [15]
-
[16]
He, Y.-G
W.-B. He, Y.-G. Ma, L.-G. Pang, H.-C. Song, and K. Zhou, Nucl. Sci. Tech.34, 88 (2023), arXiv:2303.06752 [hep-ph]
2023 arXiv
-
[17]
G. F. Sterman and S. Weinberg, Phys. Rev. Lett.39, 1436 (1977)
1977
-
[18]
R. P. Feynman, R. D. Field, and G. C. Fox, Phys. Rev. D18, 3320 (1978)
1978
-
[19]
X.-P. Duan, L. Chen, G.-L. Ma, C. A. Salgado, and B. Wu, (2025), arXiv:2503.24200 [hep-ph]
2025
-
[20]
Gyulassy and M
M. Gyulassy and M. Plumer, Phys. Lett. B243, 432 (1990)
1990
-
[21]
Wang and M
X.-N. Wang and M. Gyulassy, Phys. Rev. Lett.68, 1480 (1992)
1992
-
[22]
Baier, Y
R. Baier, Y. L. Dokshitzer, A. H. Mueller, S. Peigne, and D. Schiff, Nucl. Phys. B484, 265 (1997), arXiv:hep- ph/9608322
1997
-
[23]
C. A. Salgado and U. A. Wiedemann, Phys. Rev. Lett. 89, 092303 (2002), arXiv:hep-ph/0204221
2002 arXiv
-
[24]
C. A. Salgado and U. A. Wiedemann, Phys. Rev. D68, 014008 (2003), arXiv:hep-ph/0302184
2003 arXiv
-
[25]
Armesto, A
N. Armesto, A. Dainese, C. A. Salgado, and U. A. Wiedemann, Phys. Rev. D71, 054027 (2005), 10 arXiv:hep-ph/0501225
2005 arXiv
-
[26]
Casalderrey-Solana and C
J. Casalderrey-Solana and C. A. Salgado, Acta Phys. Polon. B38, 3731 (2007), arXiv:0712.3443 [hep-ph]
2007 arXiv
-
[27]
Qin and X.-N
G.-Y. Qin and X.-N. Wang, Int. J. Mod. Phys. E24, 1530014 (2015), arXiv:1511.00790 [hep-ph]
2015 arXiv
-
[28]
Cao and X.-N
S. Cao and X.-N. Wang, Rept. Prog. Phys.84, 024301 (2021), arXiv:2002.04028 [hep-ph]
2021 arXiv
-
[29]
Adamset al.(STAR), Phys
J. Adamset al.(STAR), Phys. Rev. Lett.91, 172302 (2003), arXiv:nucl-ex/0305015
2003 arXiv
-
[30]
K. J. Eskola, H. Honkanen, C. A. Salgado, and U. A. Wiedemann, Nucl. Phys. A747, 511 (2005), arXiv:hep- ph/0406319
2005
-
[31]
S. Cao, T. Luo, G.-Y. Qin, and X.-N. Wang, Phys. Lett. B777, 255 (2018), arXiv:1703.00822 [nucl-th]
2018 arXiv
-
[32]
Aaboudet al.(ATLAS), Phys
M. Aaboudet al.(ATLAS), Phys. Lett. B790, 108 (2019), arXiv:1805.05635 [nucl-ex]
2019 arXiv
-
[33]
Y. He, S. Cao, W. Chen, T. Luo, L.-G. Pang, and X.-N. Wang, Phys. Rev. C99, 054911 (2019), arXiv:1809.02525 [nucl-th]
2019 arXiv
-
[34]
W. Zhao, W. Ke, W. Chen, T. Luo, and X.-N. Wang, Phys. Rev. Lett.128, 022302 (2022), arXiv:2103.14657 [hep-ph]
2022 arXiv
-
[35]
S. P. Adhya, C. A. Salgado, M. Spousta, and K. Tywo- niuk, Eur. Phys. J. C82, 20 (2022), arXiv:2106.02592 [hep-ph]
2022 arXiv
-
[36]
Zhang and H
S.-L. Zhang and H. Xing, Phys. Lett. B863, 139382 (2025), arXiv:2403.12704 [hep-ph]
2025 arXiv
-
[37]
Qin and B
G.-Y. Qin and B. Muller, Phys. Rev. Lett.106, 162302 (2011), [Erratum: Phys.Rev.Lett. 108, 189904 (2012)], arXiv:1012.5280 [hep-ph]
2011 arXiv
- [38]
-
[39]
Chen, G.-Y
L. Chen, G.-Y. Qin, S.-Y. Wei, B.-W. Xiao, and H.-Z. Zhang, Phys. Lett. B782, 773 (2018), arXiv:1612.04202 [hep-ph]
2018 arXiv
-
[40]
Chen, G.-Y
L. Chen, G.-Y. Qin, L. Wang, S.-Y. Wei, B.-W. Xiao, H.-Z. Zhang, and Y.-Q. Zhang, Nucl. Phys. B933, 306 (2018), arXiv:1803.10533 [hep-ph]
2018 arXiv
-
[41]
Chen, S.-Y
L. Chen, S.-Y. Wei, and H.-Z. Zhang, Eur. Phys. J. C 80, 1136 (2020), arXiv:2001.07606 [hep-ph]
2020 arXiv
-
[42]
Y. Li, S. Shen, S. Wang, and B.-W. Zhang, Nucl. Sci. Tech.35, 113 (2024), arXiv:2401.01706 [hep-ph]
2024 arXiv
-
[43]
Z.-Q. Liu, H. Zhang, B.-W. Zhang, and E. Wang, Eur. Phys. J. C76, 20 (2016), arXiv:1506.02840 [nucl-th]
2016 arXiv
-
[44]
T. Luo, Y. He, S. Cao, and X.-N. Wang, Phys. Rev. C 109, 034919 (2024), arXiv:2306.13742 [nucl-th]
2024 arXiv
-
[45]
Xie, Q.-F
M. Xie, Q.-F. Han, E.-K. Wang, B.-W. Zhang, and H.-Z. Zhang, Nucl. Sci. Tech.35, 125 (2024), arXiv:2409.18773 [hep-ph]
2024 arXiv
-
[46]
A. M. Sirunyanet al.(CMS), Phys. Rev. Lett.120, 142302 (2018), arXiv:1708.09429 [nucl-ex]
2018 arXiv
-
[47]
Adamet al.(STAR), Phys
J. Adamet al.(STAR), Phys. Lett. B811, 135846 (2020), arXiv:2003.02114 [hep-ex]
2020
-
[48]
Acharyaet al.(A Large Ion Collider Experi- ment, ALICE), Phys
S. Acharyaet al.(A Large Ion Collider Experi- ment, ALICE), Phys. Rev. Lett.128, 102001 (2022), arXiv:2107.12984 [nucl-ex]
2022 arXiv
-
[49]
Wang, J.-W
L. Wang, J.-W. Kang, Q. Zhang, S. Shen, W. Dai, B.- W. Zhang, and E. Wang, Chin. Phys. Lett.40, 032101 (2023), arXiv:2211.13674 [nucl-th]
2023 arXiv
-
[50]
A. M. Sirunyanet al.(CMS), JHEP10, 161, arXiv:1805.05145 [hep-ex]
-
[51]
Abdallahet al.(STAR), Phys
M. Abdallahet al.(STAR), Phys. Rev. D104, 052007 (2021), arXiv:2103.13286 [hep-ex]
2021
-
[52]
Acharyaet al.(ALICE), Phys
S. Acharyaet al.(ALICE), Phys. Lett. B864, 139409 (2025), arXiv:2411.03106 [nucl-ex]
2025 arXiv
-
[53]
Milhano, U
G. Milhano, U. A. Wiedemann, and K. C. Zapp, Phys. Lett. B779, 409 (2018), arXiv:1707.04142 [hep-ph]
2018 arXiv
-
[54]
Chien and I
Y.-T. Chien and I. Vitev, Phys. Rev. Lett.119, 112301 (2017), arXiv:1608.07283 [hep-ph]
2017 arXiv
-
[55]
Tachibanaet al.(JETSCAPE), Phys
Y. Tachibanaet al.(JETSCAPE), Phys. Rev. C110, 044907 (2024), arXiv:2301.02485 [hep-ph]
2024 arXiv
-
[56]
Chang, S
N.-B. Chang, S. Cao, and G.-Y. Qin, Phys. Lett. B781, 423 (2018), arXiv:1707.03767 [hep-ph]
2018 arXiv
-
[57]
J. G. Milhano and K. Zapp, Eur. Phys. J. C82, 1010 (2022), arXiv:2207.14814 [hep-ph]
2022 arXiv
-
[58]
Luo, Nucl
T. Luo, Nucl. Phys. A1005, 121992 (2021)
2021
-
[59]
Casalderrey-Solana, D
J. Casalderrey-Solana, D. C. Gulhan, J. G. Milhano, D. Pablos, and K. Rajagopal, JHEP10, 019, [Erratum: JHEP 09, 175 (2015)], arXiv:1405.3864 [hep-ph]
2015 arXiv
- [60]
-
[62]
Z.-W. Lin, C. M. Ko, B.-A. Li, B. Zhang, and S. Pal, Phys. Rev. C72, 064901 (2005), arXiv:nucl-th/0411110
2005 arXiv
-
[63]
Lin and L
Z.-W. Lin and L. Zheng, Nucl. Sci. Tech.32, 113 (2021), arXiv:2110.02989 [nucl-th]
2021 arXiv
-
[64]
Wang and M
X.-N. Wang and M. Gyulassy, Phys. Rev. D44, 3501 (1991)
1991
-
[65]
Gyulassy and X.-N
M. Gyulassy and X.-N. Wang, Comput. Phys. Commun. 83, 307 (1994), arXiv:nucl-th/9502021
1994 arXiv
-
[66]
Sjostrand, Comput
T. Sjostrand, Comput. Phys. Commun.82, 74 (1994)
1994
-
[67]
Andersson, G
B. Andersson, G. Gustafson, and B. Soderberg, Z. Phys. C20, 317 (1983)
1983
-
[68]
Andersson, G
B. Andersson, G. Gustafson, G. Ingelman, and T. Sjos- trand, Phys. Rept.97, 31 (1983)
1983
-
[69]
D. W. Duke and J. F. Owens, Phys. Rev. D30, 49 (1984)
1984
-
[70]
J. F. Owens, Rev. Mod. Phys.59, 465 (1987)
1987
- [71]
- [72]
- [73]
-
[74]
Bzdak and G.-L
A. Bzdak and G.-L. Ma, Phys. Rev. Lett.113, 252301 (2014), arXiv:1406.2804 [hep-ph]
2014 arXiv
-
[75]
Bozek, A
P. Bozek, A. Bzdak, and G.-L. Ma, Phys. Lett. B748, 301 (2015), arXiv:1503.03655 [hep-ph]
2015 arXiv
-
[76]
L. He, T. Edmonds, Z.-W. Lin, F. Liu, D. Mol- nar, and F. Wang, Phys. Lett. B753, 506 (2016), arXiv:1502.05572 [nucl-th]
2016 arXiv
-
[77]
S.-Y. Tang, L. Zheng, X.-M. Zhang, and R.-Z. Wan, Nucl. Sci. Tech.35, 32 (2024), arXiv:2303.06577 [hep- ph]
2024 arXiv
-
[78]
Duan, W.-Y
X.-P. Duan, W.-Y. Wu, Y. Zhou, and G.-L. Ma, PoS ICHEP2024, 634 (2025)
2025
- [79]
- [80]
- [81]
-
[82]
X.-P. Duan, W. Zhao, and G.-L. Ma, Eur. Phys. J. Plus 138, 669 (2023), arXiv:2209.05689 [hep-ph]
2023 arXiv
-
[83]
Y.-H. Feng, C. M. Ko, Y.-G. Ma, K.-J. Sun, X.-N. Wang, Z. Yang, and S. Zhang, Phys. Lett. B859, 139102 (2024), arXiv:2408.01634 [nucl-th]. 11
2024 arXiv
- [84]
-
[85]
Nie and G.-L
M.-W. Nie and G.-L. Ma, Phys. Rev. C90, 014907 (2014), arXiv:1403.0328 [nucl-th]
2014 arXiv
-
[86]
Zhou, G.-L
F.-C. Zhou, G.-L. Ma, and Y.-G. Ma, Eur. Phys. J. A 56, 70 (2020), arXiv:1902.00729 [hep-ph]
2020 arXiv
-
[87]
Z. Gao, A. Luo, G.-L. Ma, G.-Y. Qin, and H.-Z. Zhang, Phys. Rev. C97, 044903 (2018), arXiv:1612.02548 [hep- ph]
2018 arXiv
-
[88]
Luo, Y.-X
A. Luo, Y.-X. Mao, G.-Y. Qin, E.-K. Wang, and H.-Z. Zhang, Eur. Phys. J. C82, 156 (2022), arXiv:2107.11751 [hep-ph]
2022 arXiv
-
[89]
Luo, Y.-X
A. Luo, Y.-X. Mao, G.-Y. Qin, E.-K. Wang, and H.-Z. Zhang, Phys. Lett. B837, 137638 (2023), arXiv:2109.14314 [hep-ph]
2023 arXiv
-
[90]
A. Luo, S. Cao, and G.-Y. Qin, Phys. Lett. B866, 139520 (2025), arXiv:2412.19283 [nucl-th]
2025 arXiv
- [91]
-
[92]
Cacciari, G
M. Cacciari, G. P. Salam, and G. Soyez, Eur. Phys. J. C72, 1896 (2012), arXiv:1111.6097 [hep-ph]
2012 arXiv
-
[93]
Berta, M
P. Berta, M. Spousta, D. W. Miller, and R. Leitner, JHEP06, 092, arXiv:1403.3108 [hep-ex]
-
[94]
Soyez, G
G. Soyez, G. P. Salam, J. Kim, S. Dutta, and M. Cacciari, Phys. Rev. Lett.110, 162001 (2013), arXiv:1211.2811 [hep-ph]
2013 arXiv
-
[95]
Cacciari and G
M. Cacciari and G. P. Salam, Phys. Lett. B641, 57 (2006), arXiv:hep-ph/0512210
2006 arXiv
-
[96]
A. J. Larkoski, S. Marzani, G. Soyez, and J. Thaler, JHEP05, 146, arXiv:1402.2657 [hep-ph]
-
[97]
Y. L. Dokshitzer, G. D. Leder, S. Moretti, and B. R. Webber, JHEP08, 001, arXiv:hep-ph/9707323
-
[98]
F. A. Dreyer, G. P. Salam, and G. Soyez, JHEP12, 064, arXiv:1807.04758 [hep-ph]
-
[99]
H. A. Andrewset al., J. Phys. G47, 065102 (2020), arXiv:1808.03689 [hep-ph]
2020 arXiv
- [100]
-
[101]
Y. He, T. Luo, X.-N. Wang, and Y. Zhu, Phys. Rev. C91, 054908 (2015), [Erratum: Phys.Rev.C 97, 019902 (2018)], arXiv:1503.03313 [nucl-th]
2015 arXiv
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