REVIEW 1 major objections 2 minor 111 references
Energy loss of heavy-flavor quarks in color string medium
T0 review · 1 major / 2 minor · reviewed 2026-05-18 · grok-4.3
Pith's one-line read Heavy-flavor quarks lose less transverse momentum in a fluctuating color-string medium than in hydrodynamic descriptions of small systems.
desk verdict The paper finds lower heavy-flavor quark energy loss in a fluctuating color-string medium than in EPOS4HQ hydrodynamics, but the mapping from string energy density to scattering rate lacks a clear derivation. 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 varying overlaps of longitudinally oscillating color strings, which produce fluctuations in color field energy density that directly govern the elastic scattering rate of heavy-flavor quarks with gluons inside the string volume.
What would settle it
A measurement of charm-quark transverse-momentum loss in high-multiplicity proton-proton events that matches the higher values predicted by hydrodynamic models rather than the lower values from the string model would falsify the central result.
Extended reading notes
Core claim
The central claim is that charm quarks traversing the non-equilibrated medium formed by fluctuating color strings from multi-pomeron exchanges in minimum-bias proton-proton collisions experience significantly lower momentum loss than they do in an expanding hydrodynamic scenario, with the loss computed event by event via a hybrid simulation that accounts for the dynamic initialization of the medium at each time step.
Load-bearing premise
The premise that energy-density fluctuations arising from string overlaps set the elastic scattering rates of heavy quarks with gluons without requiring additional equilibration of the medium.
Editorial extensions
If this is right
- The transverse-momentum dependence of momentum loss for charm quarks follows from event-by-event propagation through the fluctuating string environment.
- The lower energy loss stems from the non-equilibrated, dynamically initialized medium rather than a smooth hydrodynamic expansion.
- String-overlap fluctuations create a different scattering environment that reduces the average interaction rate compared with equilibrated descriptions.
- The result bears on whether signals of heavy-quark suppression in small systems indicate full quark-gluon plasma formation or string-like dynamics.
Reading between the lines
- If the string description holds, heavy-flavor observables in proton-proton data could serve as a baseline that distinguishes string dynamics from hydrodynamic flow without assuming equilibrium.
- The same fluctuating-medium setup could be used to predict other observables such as azimuthal anisotropies in small systems while remaining outside the hydrodynamic regime.
- Testing the model against measured heavy-meson spectra at the LHC would directly probe whether string overlaps capture the dominant energy-loss mechanism in tiny collision volumes.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript presents preliminary estimates of heavy-flavor quark energy loss in a non-equilibrated medium formed by fluctuating color strings in minimum-bias pp collisions at LHC energies. Longitudinal string oscillations dynamically initialize the medium at each time step, with overlaps producing fluctuations in color-field energy density that govern the elastic scattering rate of HF quarks with gluons. Using an event-by-event hybrid simulation, the transverse-momentum dependence of momentum loss for charm quarks is computed and compared to the expanding hydrodynamic scenario of the EPOS4HQ model, with the central claim being significantly lower energy loss in the string medium.
Significance. If the energy-density-to-scattering-rate mapping can be placed on a firm footing, the result would be relevant to debates on QGP formation in small systems by indicating that non-equilibrated string dynamics with fluctuations yield less suppression than hydrodynamics. The event-by-event treatment of string overlaps is a methodological strength that captures realistic medium fluctuations.
major comments (1)
- [hybrid approach description] The functional dependence of the elastic scattering rate on the fluctuating color-field energy density is not derived, perturbatively matched, or calibrated (see the model description following the statement that 'Their varying overlaps create fluctuations in the color field energy density that governs the elastic scattering rate'). This mapping is load-bearing for the headline quantitative claim of significantly lower energy loss relative to EPOS4HQ; different choices of the functional form (e.g., rate ∝ ε or rate ∝ ε²) could shift the reported difference by an amount comparable to the claimed effect without changing the underlying string dynamics.
minor comments (2)
- [Results] The abstract refers to 'preliminary estimates' but the results section should explicitly state the number of events, statistical uncertainties, and any systematic variations in the string parameters to allow assessment of the robustness of the 'significantly lower' conclusion.
- Clarify whether the charm-quark production points and initial p_T spectra are taken from the same hard-scattering generator used in the EPOS4HQ comparison or from an independent source.
Simulated Author's Rebuttal
We thank the referee for the careful reading of our manuscript and for the constructive feedback on the hybrid model description. We appreciate the positive assessment of the event-by-event string overlap treatment and its relevance to small-system QGP debates. We address the major comment below and outline planned revisions.
read point-by-point responses
-
Referee: The functional dependence of the elastic scattering rate on the fluctuating color-field energy density is not derived, perturbatively matched, or calibrated (see the model description following the statement that 'Their varying overlaps create fluctuations in the color field energy density that governs the elastic scattering rate'). This mapping is load-bearing for the headline quantitative claim of significantly lower energy loss relative to EPOS4HQ; different choices of the functional form (e.g., rate ∝ ε or rate ∝ ε²) could shift the reported difference by an amount comparable to the claimed effect without changing the underlying string dynamics.
Authors: We agree that the mapping from color-field energy density to elastic scattering rate is a central modeling assumption whose justification merits explicit discussion. In the current implementation the rate is taken proportional to the local energy density ε, reflecting the expectation that higher energy density within overlapping strings corresponds to a greater number of gluons available for scattering with the heavy-flavor quark. This linear ansatz is chosen for the preliminary study as a minimal, physically motivated link between the string dynamics and the interaction rate; it is not claimed to be perturbatively derived from first principles. We acknowledge that alternative forms (e.g., quadratic) could alter the quantitative difference relative to EPOS4HQ. In the revised manuscript we will (i) state the proportionality explicitly in the model section, (ii) add a short paragraph motivating the choice from the color-string picture, and (iii) include a brief discussion of the sensitivity to the functional form, noting that a full perturbative matching or calibration lies beyond the scope of this exploratory work but is planned for follow-up studies. These additions will make the assumption transparent without changing the underlying string dynamics or the reported qualitative result of lower energy loss. revision: partial
Circularity Check
No significant circularity; derivation self-contained against external benchmark
full rationale
The paper models HF quark propagation through a fluctuating color-string medium initialized by longitudinal oscillations and overlaps, with elastic scattering rates governed by the resulting color-field energy density on an event-by-event basis. The headline quantitative result is a direct comparison of computed momentum loss to the independent expanding hydrodynamic scenario of the external EPOS4HQ model. No load-bearing step reduces by construction to a fitted parameter, self-citation chain, or internal redefinition of the target observable; the simulation inputs (string dynamics, overlaps) are distinct from the external hydrodynamic reference, satisfying the criterion for a self-contained derivation against external benchmarks.
Assumptions & free parameters
assumptions (1)
- domain assumption Color strings originate from multi-pomeron exchanges in minimum-bias p+p collisions.
Cite this review
Pith. "Pith review of Energy loss of heavy-flavor quarks in color string medium." pith.science (2026). https://pith.science/paper/I2Y6XJF3
@misc{pith2026250924316,
author = {Pith},
title = {Pith review of: Energy loss of heavy-flavor quarks in color string medium},
year = {2026},
howpublished = {\url{https://pith.science/paper/I2Y6XJF3}},
note = {Machine review of arXiv:2509.24316}
}
read the original abstract
The paper presents preliminary estimates of heavy-flavor (HF) quark energy loss during its propagation through the non-equilibrated medium formed in minimum bias proton-proton (p+p) collisions at LHC energies. The study is inspired by the ongoing hot debates on whether tiny droplets of Quark-Gluon Plasma can be created in collisions of small systems. In this work, we model a p+p event with a fluctuating number of color strings originated from multi-pomeron exchanges. Considered longitudinal oscillations of strings dynamically initialize medium at each time step. Their varying overlaps create fluctuations in the color field energy density that governs the elastic scattering rate of HF quarks with the gluons present within the string volume. We calculate the transverse momentum dependence of the momentum loss for charm (anti-)quarks that are produced in initial hard scatterings and traverse the described environment. The simulation is performed using a developed hybrid approach on an event-by-event basis. Our results show significantly lower HF quarks energy loss compared to that obtained in the expanding hydrodynamic scenario of the new EPOS4HQ model.
Figures
Lean theorems connected to this paper
-
IndisputableMonolith/Cost/FunctionalEquation.leanwashburn_uniqueness_aczel unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
ε_cell = σ √k_cell / ΔS_str ... T_eff_cell = (30 ε_cell / (16 π²))^{1/4} ... dp/dt integrals with Bose ρ(k)
What do these tags mean?
- matches
- The paper's claim is directly supported by a theorem in the formal canon.
- supports
- The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
- extends
- The paper goes beyond the formal theorem; the theorem is a base layer rather than the whole result.
- uses
- The paper appears to rely on the theorem as machinery.
- contradicts
- The paper's claim conflicts with a theorem or certificate in the canon.
- unclear
- Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.
Reference graph
Works this paper leans on
-
[1]
U. W. Heinz and M. Jacob (1 2000)arXiv:nucl-th/0002042
work page Pith review arXiv 2000
- [2]
-
[3]
PHOBOS Collaboration (B. B. Backet al.),Nucl. Phys. A757(2005) 28
work page 2005
-
[4]
PHENIX Collaboration (K. Adcoxet al.),Nucl. Phys. A757(2005) 184. September 30, 2025 2:2 ws-ijmpe 16Daria Prokhorova, Shuzhe Shi, Evgeny Andronov
work page 2005
- [5]
-
[6]
ALICE Collaboration (K. Aamodtet al.),Phys. Rev. Lett.105(2010) 252301, arXiv:1011.3916 [nucl-ex]
work page Pith review arXiv 2010
-
[7]
ATLAS Collaboration (G. Aadet al.),Phys. Rev. Lett.105(2010) 252303, arXiv:1011.6182 [hep-ex]
work page Pith review arXiv 2010
-
[8]
CMS Collaboration (S. Chatrchyanet al.),Phys. Rev. C84(2011) 024906, arXiv:1102.1957 [nucl-ex]
work page Pith review arXiv 2011
Show all 111 references
-
[9]
Aaijet al.),Phys
LHCb Collaboration (R. Aaijet al.),Phys. Lett. B762(2016) 473, arXiv:1512.00439 [nucl-ex]
2016 arXiv
-
[10]
Acharyaet al.),Eur
ALICE Collaboration (S. Acharyaet al.),Eur. Phys. J. C84(2024) 813, arXiv:2211.04384 [nucl-ex]
2024
-
[11]
Hayrapetyanet al.),Phys
CMS Collaboration (A. Hayrapetyanet al.),Phys. Rept.1115(2025) 219, arXiv:2405.10785 [nucl-ex]
2025
-
[12]
Cabibbo and G
N. Cabibbo and G. Parisi,Phys. Lett. B59(1975) 67
1975
- [13]
-
[14]
Bazavovet al.,Phys
A. Bazavovet al.,Phys. Rev. D85(2012) 054503,arXiv:1111.1710 [hep-lat]
2012 arXiv
-
[15]
E. V. Shuryak,Sov. Phys. JETP47(1978) 212
1978
-
[16]
D. J. Gross and F. Wilczek,Phys. Rev. Lett.30(1973) 1343
1973
-
[17]
H. D. Politzer,Phys. Rev. Lett.30(1973) 1346
1973
-
[18]
U. W. Heinz,J. Phys. Conf. Ser.455(2013) 012044,arXiv:1304.3634 [nucl-th]
2013 arXiv
-
[19]
J. D. Bjorken,Phys. Rev. D27(1983) 140
1983
-
[20]
Busza, K
W. Busza, K. Rajagopal and W. van der Schee,Ann. Rev. Nucl. Part. Sci.68(2018) 339
2018
-
[21]
Romatschke and U
P. Romatschke and U. Romatschke,Relativistic Fluid Dynamics In and Out of Equi- librium, Cambridge Monographs on Mathematical Physics, Vol. 1 (Cambridge Uni- versity Press, Cambridge, 5 2019)
2019
-
[22]
J. W. Harris and B. Muller,Ann. Rev. Nucl. Part. Sci.46(1996) 71
1996
-
[23]
P. Koch, B. Muller and J. Rafelski,Phys. Rept.142(1986) 167
1986
-
[24]
Matsui and H
T. Matsui and H. Satz,Phys. Lett. B178(1986) 416
1986
-
[25]
Sorge,Phys
H. Sorge,Phys. Rev. Lett.78(1997) 2309
1997
-
[26]
L. P. Csernai and D. Rohrich,Phys. Lett. B458(1999) 454
1999
-
[27]
Gyulassy and M
M. Gyulassy and M. Plumer,Phys. Lett. B243(1990) 432
1990
-
[28]
Wang and M
X.-N. Wang and M. Gyulassy,Phys. Rev. Lett.68(1992) 1480
1992
-
[29]
Heinz and R
U. Heinz and R. Snellings,Ann. Rev. Nucl. Part. Sci.63(2013) 123, arXiv:1301.2826 [nucl-th]
2013 arXiv
-
[30]
A. N. Mishra, G. Pai´ c, C. Pajares, R. P. Scharenberg and B. K. Srivastava,Nucl. Phys. A1046(2024) 122865,arXiv:2202.12274 [hep-ph]
2024
-
[31]
Adamet al.),Nature Phys.13(2017) 535
ALICE Collaboration (J. Adamet al.),Nature Phys.13(2017) 535
2017
-
[32]
Khachatryanet al.),JHEP09(2010) 091
CMS Collaboration (V. Khachatryanet al.),JHEP09(2010) 091
2010
-
[33]
Aadet al.),Phys
ATLAS Collaboration (G. Aadet al.),Phys. Rev. Lett.116(2016) 172301
2016
-
[34]
Aaboudet al.),Phys
ATLAS Collaboration (M. Aaboudet al.),Phys. Rev. C96(2017) 024908
2017
-
[35]
Dusling, W
K. Dusling, W. Li and B. Schenke,Int. J. Mod. Phys. E25(2016) 1630002, arXiv:1509.07939 [nucl-ex]
2016 arXiv
- [36]
-
[37]
R. D. Weller and P. Romatschke,Phys. Lett. B774(2017) 351
2017
-
[38]
Y. Zhou, W. Zhao, K. Murase and H. Song,Nucl. Phys. A1005(2021) 121908
2021
-
[39]
V. E. Ambrus, S. Schlichting and C. Werthmann,Phys. Rev. Lett.130(2023) 152301
2023
-
[40]
Florkowski, M
W. Florkowski, M. P. Heller and M. Spalinski,Rept. Prog. Phys.81(2018) 046001, arXiv:1707.02282 [hep-ph]
2018 arXiv
-
[41]
M. P. Heller, R. A. Janik and P. Witaszczyk,Phys. Rev. Lett.110(2013) 211602, September 30, 2025 2:2 ws-ijmpe Energy loss of heavy-flavor quarks in color string medium17 arXiv:1302.0697 [hep-th]
2013 arXiv
- [42]
-
[43]
Kovner and M
A. Kovner and M. Lublinsky,Phys. Rev. D83(2011) 034017,arXiv:1012.3398 [hep-ph]
2011 arXiv
-
[44]
Dong and V
X. Dong and V. Greco,Prog. Part. Nucl. Phys.104(2019) 97
2019
-
[45]
Svetitsky,Phys
B. Svetitsky,Phys. Rev. D37(1988) 2484
1988
-
[46]
G. D. Moore and D. Teaney,Phys. Rev. C71(2005) 064904,arXiv:hep-ph/0412346
2005 arXiv
-
[47]
Schenke, M
B. Schenke, M. Strickland, A. Dumitru, Y. Nara and C. Greiner,Phys. Rev. C79 (2009) 034903,arXiv:0810.1314 [hep-ph]
2009 arXiv
-
[48]
M. E. Carrington, K. Deja and S. Mrowczynski,Phys. Rev. C92(2015) 044914, arXiv:1506.09082 [hep-ph]
2015 arXiv
- [49]
- [50]
-
[51]
J. Zhao, J. Aichelin, P. B. Gossiaux and K. Werner,Phys. Rev. D109(2024) 054011, arXiv:2310.08684 [hep-ph]
2024
-
[52]
Singh, M
M. Singh, M. Kurian, B. Schenke, S. Jeon and C. Gale (9 2025)arXiv:2509.18647 [nucl-th]
2025
-
[53]
E. V. Andronov, D. S. Prokhorova and A. A. Belousov,Theor. Math. Phys.216 (2023) 1265
2023
-
[54]
Prokhorova, E
D. Prokhorova, E. Andronov and G. Feofilov,MDPI Physics5(2023) 636
2023
-
[55]
Prokhorova and E
D. Prokhorova and E. Andronov,MDPI Physics6(2024) 264
2024
-
[56]
V. N. Gribov,Zh. Eksp. Teor. Fiz.53(1967) 654
1967
-
[57]
Veneziano,Nucl
G. Veneziano,Nucl. Phys. B74(1974) 365
1974
-
[58]
Veneziano,Phys
G. Veneziano,Phys. Lett. B52(1974) 220
1974
-
[59]
Veneziano,Nucl
G. Veneziano,Nucl. Phys. B117(1976) 519
1976
-
[60]
Capella, U
A. Capella, U. Sukhatme, C.-I. Tan and J. Tran Thanh Van,Phys. Rept.236(1994) 225
1994
-
[61]
Werner,Phys
K. Werner,Phys. Rept.232(1993) 87
1993
-
[62]
A. B. Kaidalov,Phys. Lett. B116(1982) 459
1982
-
[63]
Artru,Phys
X. Artru,Phys. Rept.97(1983) 147
1983
-
[64]
Eichten, K
E. Eichten, K. Gottfried, T. Kinoshita, J. B. Kogut, K. D. Lane and T. Yan,Phys. Rev. Lett.34(1975) 369
1975
-
[65]
Braun and C
M. Braun and C. Pajares,Nucl. Phys. B390(1993) 542
1993
-
[66]
Werner,Phys
K. Werner,Phys. Rev. C108(2023) 064903
2023
-
[67]
Sj¨ ostrand,Comput
T. Sj¨ ostrand,Comput. Phys. Commun.246(2020) 106910
2020
-
[68]
Wang and M
X.-N. Wang and M. Gyulassy,Phys. Rev. D44(1991) 3501
1991
-
[69]
Zhang, C
B. Zhang, C. M. Ko, B.-A. Li and Z.-w. Lin,Phys. Rev. C61(2000) 067901
2000
-
[70]
Cassing and E
W. Cassing and E. L. Bratkovskaya,Phys. Rev. C78(2008) 034919, arXiv:0808.0022 [hep-ph]
2008 arXiv
-
[71]
Andersson and P
B. Andersson and P. A. Henning,Nucl. Phys. B355(1991) 82
1991
-
[72]
Jafarpour, V
M. Jafarpour, V. Voronyuk, K. Werner, E. Bratkovskaya and D. Vintache (9 2025) arXiv:2509.05428 [hep-ph]
2025
-
[73]
P. Cea, L. Cosmai, F. Cuteri and A. Papa,Phys. Rev. D89(2014) 094505
2014
-
[74]
Nishino, K.-I
S. Nishino, K.-I. Kondo, A. Shibata, T. Sasago and S. Kato,Eur. Phys. J. C79 (2019) 774
2019
-
[75]
Bierlich, G
C. Bierlich, G. Gustafson, L. L¨ onnblad and A. Tarasov,JHEP03(2015) 148, arXiv:1412.6259 [hep-ph]
2015 arXiv
-
[76]
M. A. Braun, C. Pajares and J. Ranft,Int. J. Mod. Phys. A14(1999) 2689
1999
-
[77]
G. S. Bali,Phys. Rev. D62(2000) 114503
2000
-
[78]
Acharyaet al.),Phys
ALICE Collaboration (S. Acharyaet al.),Phys. Rev. Lett.127(2021) 202301, September 30, 2025 2:2 ws-ijmpe 18Daria Prokhorova, Shuzhe Shi, Evgeny Andronov arXiv:2011.06078 [nucl-ex]
2021
-
[79]
Acharyaet al.),JHEP10(2021) 159,arXiv:2105.05616 [nucl-ex]
ALICE Collaboration (S. Acharyaet al.),JHEP10(2021) 159,arXiv:2105.05616 [nucl-ex]
2021
-
[80]
Acharyaet al.),Phys
ALICE Collaboration (S. Acharyaet al.),Phys. Lett. B829(2022) 137065, arXiv:2111.11948 [nucl-ex]
2022
-
[81]
Tumasyanet al.),JHEP01(2024) 128,arXiv:2307.11186 [nucl-ex]
CMS Collaboration (A. Tumasyanet al.),JHEP01(2024) 128,arXiv:2307.11186 [nucl-ex]
2024
-
[82]
Brocket al.),Rev
CTEQ Collaboration (R. Brocket al.),Rev. Mod. Phys.67(1995) 157
1995
-
[83]
Bierlichet al.,SciPost Phys
C. Bierlichet al.,SciPost Phys. Codeb.2022(2022) 8,arXiv:2203.11601 [hep-ph]
2022 arXiv
-
[84]
A. B. Kaidalov and K. A. Ter-Martirosian,Phys. Lett. B117(1982) 247
1982
-
[85]
V. V. Vechernin and S. N. Belokurova,J. Phys. Conf. Ser.1690(2020) 012088
2020
-
[86]
H.-L. Lai, M. Guzzi, J. Huston, Z. Li, P. M. Nadolsky, J. Pumplin and C. P. Yuan, Phys. Rev. D82(2010) 074024
2010
-
[87]
J. Gao, M. Guzzi, J. Huston, H.-L. Lai, Z. Li, P. Nadolsky, J. Pumplin, D. Stump and C. P. Yuan,Phys. Rev. D89(2014) 033009
2014
- [88]
-
[89]
Luscher, G
M. Luscher, G. Munster and P. Weisz,Nucl. Phys. B180(1981) 1
1981
-
[90]
Andersson, G
B. Andersson, G. Gustafson, G. Ingelman and T. Sjostrand,Phys. Rept.97(1983) 31
1983
-
[91]
Braaten and M
E. Braaten and M. H. Thoma,Phys. Rev. D44(1991) 1298
1991
-
[92]
M. E. Carrington, A. Czajka and S. Mrowczynski,Nucl. Phys. A1001(2020) 121914, arXiv:2001.05074 [nucl-th]
2020
-
[93]
M. E. Carrington, A. Czajka and S. Mrowczynski,Phys. Lett. B834(2022) 137464, arXiv:2112.06812 [hep-ph]
2022
-
[94]
Schenke, C
B. Schenke, C. Gale and S. Jeon,Phys. Rev. C80(2009) 054913,arXiv:0909.2037 [hep-ph]
2009 arXiv
-
[95]
P. B. Gossiaux and J. Aichelin,Phys. Rev. C78(2008) 014904,arXiv:0802.2525 [hep-ph]
2008 arXiv
-
[96]
Aichelin, P
J. Aichelin, P. B. Gossiaux and T. Gousset,Phys. Rev. D89(2014) 074018, arXiv:1307.5270 [hep-ph]
2014 arXiv
-
[97]
J. Xu, J. Liao and M. Gyulassy,Chin. Phys. Lett.32(2015) 092501, arXiv:1411.3673 [hep-ph]
2015 arXiv
-
[98]
M. H. Thoma and M. Gyulassy,Nucl. Phys. B351(1991) 491
1991
-
[99]
Peigne and A
S. Peigne and A. Peshier,Phys. Rev. D77(2008) 114017,arXiv:0802.4364 [hep-ph]
2008 arXiv
-
[100]
J. D. Bjorken (8 1982)
1982
-
[101]
S. Shi, J. Liao and M. Gyulassy,Chin. Phys. C42(2018) 104104,arXiv:1804.01915 [hep-ph]
2018 arXiv
-
[102]
Liao and E
J. Liao and E. Shuryak,Phys. Rev. Lett.101(2008) 162302,arXiv:0804.0255 [hep-ph]
2008 arXiv
-
[103]
S. Shi, J. Liao and M. Gyulassy,Chin. Phys. C43(2019) 044101,arXiv:1808.05461 [hep-ph]
2019 arXiv
-
[104]
P. B. Gossiaux and J. Aichelin,J. Phys. G36(2009) 064028,arXiv:0901.2462 [nucl-th]
2009 arXiv
-
[105]
J. Xu, A. Buzzatti and M. Gyulassy,JHEP08(2014) 063,arXiv:1402.2956 [hep-ph]
2014 arXiv
-
[106]
J. I. Kapusta and C. Gale,Finite-Temperature Field Theory: Principles and Applica- tions, Cambridge Monographs on Mathematical Physics, Vol. 1, 2 edn. (Cambridge September 30, 2025 2:2 ws-ijmpe Energy loss of heavy-flavor quarks in color string medium19 University Press, Cambr...
2025
-
[107]
Romatschke and M
P. Romatschke and M. Strickland,Phys. Rev. D68(2003) 036004, arXiv:hep-ph/0304092
2003 arXiv
-
[108]
Romatschke and M
P. Romatschke and M. Strickland,Phys. Rev. D70(2004) 116006, arXiv:hep-ph/0406188
2004 arXiv
-
[109]
Y. Peng, V. E. Ambrus, C. Werthmann, S. Schlichting, U. Heinz and H. Song (9 2025)arXiv:2509.04431 [nucl-th]
2025 arXiv
-
[110]
J. Zhao, J. Aichelin, P. B. Gossiaux and K. Werner,Phys. Rev. C111(2025) 014907, arXiv:2407.20919 [hep-ph]
2025
-
[111]
S. Zhao, Y. Peng, U. W. Heinz and H. Song (9 2025)arXiv:2509.03841 [nucl-th]
2025
Reviewed May 18, 2026 · model on record in the stance chip above.
Discussion (0). Continue with ORCID to comment.