Pith. sign in

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 →

arxiv 2509.24316 v1 pith:I2Y6XJF3 submitted 2025-09-29 hep-ph

classification hep-ph
keywords heavy-flavorquarksenergylosscolorstringsproton-protoncollisionselasticscatteringfluctuatingmediumquark-gluonplasmasmallsystems
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

The paper calculates the energy loss of charm quarks produced in hard scatterings as they move through the medium created in proton-proton collisions at LHC energies. It models that medium as a set of color strings whose longitudinal oscillations and varying overlaps generate fluctuations in color field energy density. Those fluctuations set the rate at which the quarks scatter elastically with gluons. The resulting loss is substantially smaller than the loss obtained when the same collisions are described with an expanding hydrodynamic medium. A reader would care because the difference bears directly on whether tiny collision systems form an equilibrated quark-gluon plasma or retain string-like, non-equilibrated dynamics.

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.

Watch

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

Editorial extensions of the paper, not claims the author makes directly.

  • 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.
Share X Bluesky LinkedIn Reddit HN

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit.

Referee Report

1 major / 2 minor

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)
  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)
  1. [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.
  2. 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

1 responses · 0 unresolved

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
  1. 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

0 steps flagged · score 0.0 of 10

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 0 free parameters · 1 assumptions · 0 invented entities

The model rests on standard high-energy QCD assumptions about color strings and multi-pomeron exchanges; the hybrid simulation and dynamic initialization constitute the main additions. No new particles or forces are introduced.

assumptions (1)
  • domain assumption Color strings originate from multi-pomeron exchanges in minimum-bias p+p collisions.
    This is invoked to model the fluctuating medium in which HF quarks propagate.

how reviews work

0 comments
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

Figures reproduced from arXiv: 2509.24316 by the authors.

Figure 1
Figure 1. Transverse momentum loss of a charm quark as a function of its initial transverse mo [PITH_FULL_IMAGE:figures/full_fig_p012_1.png] view at source ↗
Figure 2
Figure 2. Transverse momentum loss of a charm quark as a function of its initial transverse momen [PITH_FULL_IMAGE:figures/full_fig_p013_2.png] view at source ↗
Figure 3
Figure 3. Transverse momentum loss of a charm quark as a function of its initial transverse momen [PITH_FULL_IMAGE:figures/full_fig_p013_3.png] view at source ↗
Figures from the paper (1 more)
Figure 4
Figure 4. Figure 4: Transverse momentum loss of a charm quark as a function of its initial transverse momen [PITH_FULL_IMAGE:figures/full_fig_p014_4.png]

Discussion (0). Continue with ORCID to comment.

Lean theorems connected to this paper

Citations machine-checked in the Pith Canon. Every link opens the source theorem in the public Lean library.

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

111 extracted references · 111 canonical work pages

  1. [1]

    U. W. Heinz and M. Jacob (1 2000)arXiv:nucl-th/0002042

  2. [2]

    Arseneet al.),Nucl

    BRAHMS Collaboration (I. Arseneet al.),Nucl. Phys. A757(2005) 1

  3. [3]

    PHOBOS Collaboration (B. B. Backet al.),Nucl. Phys. A757(2005) 28

  4. [4]

    Adcoxet al.),Nucl

    PHENIX Collaboration (K. Adcoxet al.),Nucl. Phys. A757(2005) 184. September 30, 2025 2:2 ws-ijmpe 16Daria Prokhorova, Shuzhe Shi, Evgeny Andronov

  5. [5]

    Adamset al.),Nucl

    STAR Collaboration (J. Adamset al.),Nucl. Phys. A757(2005) 102

  6. [6]

    Charged-particle multiplicity density at mid-rapidity in central Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 2.76 TeV

    ALICE Collaboration (K. Aamodtet al.),Phys. Rev. Lett.105(2010) 252301, arXiv:1011.3916 [nucl-ex]

  7. [7]
  8. [8]

    Observation and studies of jet quenching in PbPb collisions at nucleon-nucleon center-of-mass energy = 2.76 TeV

    CMS Collaboration (S. Chatrchyanet al.),Phys. Rev. C84(2011) 024906, arXiv:1102.1957 [nucl-ex]

Show all 111 references
  1. [9]

    Aaijet al.),Phys

    LHCb Collaboration (R. Aaijet al.),Phys. Lett. B762(2016) 473, arXiv:1512.00439 [nucl-ex]

  2. [10]

    Acharyaet al.),Eur

    ALICE Collaboration (S. Acharyaet al.),Eur. Phys. J. C84(2024) 813, arXiv:2211.04384 [nucl-ex]

  3. [11]

    Hayrapetyanet al.),Phys

    CMS Collaboration (A. Hayrapetyanet al.),Phys. Rept.1115(2025) 219, arXiv:2405.10785 [nucl-ex]

  4. [12]

    Cabibbo and G

    N. Cabibbo and G. Parisi,Phys. Lett. B59(1975) 67

  5. [13]

    Karsch,Lect

    F. Karsch,Lect. Notes Phys.583(2002) 209,arXiv:hep-lat/0106019

  6. [14]

    Bazavovet al.,Phys

    A. Bazavovet al.,Phys. Rev. D85(2012) 054503,arXiv:1111.1710 [hep-lat]

  7. [15]

    E. V. Shuryak,Sov. Phys. JETP47(1978) 212

  8. [16]

    D. J. Gross and F. Wilczek,Phys. Rev. Lett.30(1973) 1343

  9. [17]

    H. D. Politzer,Phys. Rev. Lett.30(1973) 1346

  10. [18]

    U. W. Heinz,J. Phys. Conf. Ser.455(2013) 012044,arXiv:1304.3634 [nucl-th]

  11. [19]

    J. D. Bjorken,Phys. Rev. D27(1983) 140

  12. [20]

    Busza, K

    W. Busza, K. Rajagopal and W. van der Schee,Ann. Rev. Nucl. Part. Sci.68(2018) 339

  13. [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)

  14. [22]

    J. W. Harris and B. Muller,Ann. Rev. Nucl. Part. Sci.46(1996) 71

  15. [23]

    P. Koch, B. Muller and J. Rafelski,Phys. Rept.142(1986) 167

  16. [24]

    Matsui and H

    T. Matsui and H. Satz,Phys. Lett. B178(1986) 416

  17. [25]

    Sorge,Phys

    H. Sorge,Phys. Rev. Lett.78(1997) 2309

  18. [26]

    L. P. Csernai and D. Rohrich,Phys. Lett. B458(1999) 454

  19. [27]

    Gyulassy and M

    M. Gyulassy and M. Plumer,Phys. Lett. B243(1990) 432

  20. [28]

    Wang and M

    X.-N. Wang and M. Gyulassy,Phys. Rev. Lett.68(1992) 1480

  21. [29]

    Heinz and R

    U. Heinz and R. Snellings,Ann. Rev. Nucl. Part. Sci.63(2013) 123, arXiv:1301.2826 [nucl-th]

  22. [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]

  23. [31]

    Adamet al.),Nature Phys.13(2017) 535

    ALICE Collaboration (J. Adamet al.),Nature Phys.13(2017) 535

  24. [32]

    Khachatryanet al.),JHEP09(2010) 091

    CMS Collaboration (V. Khachatryanet al.),JHEP09(2010) 091

  25. [33]

    Aadet al.),Phys

    ATLAS Collaboration (G. Aadet al.),Phys. Rev. Lett.116(2016) 172301

  26. [34]

    Aaboudet al.),Phys

    ATLAS Collaboration (M. Aaboudet al.),Phys. Rev. C96(2017) 024908

  27. [35]

    Dusling, W

    K. Dusling, W. Li and B. Schenke,Int. J. Mod. Phys. E25(2016) 1630002, arXiv:1509.07939 [nucl-ex]

  28. [36]

    Romatschke,Eur

    P. Romatschke,Eur. Phys. J. C77(2017) 21,arXiv:1609.02820 [nucl-th]

  29. [37]

    R. D. Weller and P. Romatschke,Phys. Lett. B774(2017) 351

  30. [38]

    Y. Zhou, W. Zhao, K. Murase and H. Song,Nucl. Phys. A1005(2021) 121908

  31. [39]

    V. E. Ambrus, S. Schlichting and C. Werthmann,Phys. Rev. Lett.130(2023) 152301

  32. [40]

    Florkowski, M

    W. Florkowski, M. P. Heller and M. Spalinski,Rept. Prog. Phys.81(2018) 046001, arXiv:1707.02282 [hep-ph]

  33. [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]

  34. [42]

    Lappi and L

    T. Lappi and L. McLerran,Nucl. Phys. A772(2006) 200,arXiv:hep-ph/0602189

  35. [43]

    Kovner and M

    A. Kovner and M. Lublinsky,Phys. Rev. D83(2011) 034017,arXiv:1012.3398 [hep-ph]

  36. [44]

    Dong and V

    X. Dong and V. Greco,Prog. Part. Nucl. Phys.104(2019) 97

  37. [45]

    Svetitsky,Phys

    B. Svetitsky,Phys. Rev. D37(1988) 2484

  38. [46]

    G. D. Moore and D. Teaney,Phys. Rev. C71(2005) 064904,arXiv:hep-ph/0412346

  39. [47]

    Schenke, M

    B. Schenke, M. Strickland, A. Dumitru, Y. Nara and C. Greiner,Phys. Rev. C79 (2009) 034903,arXiv:0810.1314 [hep-ph]

  40. [48]

    M. E. Carrington, K. Deja and S. Mrowczynski,Phys. Rev. C92(2015) 044914, arXiv:1506.09082 [hep-ph]

  41. [49]

    Mrowczynski,Eur

    S. Mrowczynski,Eur. Phys. J. A54(2018) 43,arXiv:1706.03127 [nucl-th]

  42. [50]

    Caoet al.,Phys

    S. Caoet al.,Phys. Rev. C99(2019) 054907,arXiv:1809.07894 [nucl-th]

  43. [51]

    J. Zhao, J. Aichelin, P. B. Gossiaux and K. Werner,Phys. Rev. D109(2024) 054011, arXiv:2310.08684 [hep-ph]

  44. [52]

    Singh, M

    M. Singh, M. Kurian, B. Schenke, S. Jeon and C. Gale (9 2025)arXiv:2509.18647 [nucl-th]

  45. [53]

    E. V. Andronov, D. S. Prokhorova and A. A. Belousov,Theor. Math. Phys.216 (2023) 1265

  46. [54]

    Prokhorova, E

    D. Prokhorova, E. Andronov and G. Feofilov,MDPI Physics5(2023) 636

  47. [55]

    Prokhorova and E

    D. Prokhorova and E. Andronov,MDPI Physics6(2024) 264

  48. [56]

    V. N. Gribov,Zh. Eksp. Teor. Fiz.53(1967) 654

  49. [57]

    Veneziano,Nucl

    G. Veneziano,Nucl. Phys. B74(1974) 365

  50. [58]

    Veneziano,Phys

    G. Veneziano,Phys. Lett. B52(1974) 220

  51. [59]

    Veneziano,Nucl

    G. Veneziano,Nucl. Phys. B117(1976) 519

  52. [60]

    Capella, U

    A. Capella, U. Sukhatme, C.-I. Tan and J. Tran Thanh Van,Phys. Rept.236(1994) 225

  53. [61]

    Werner,Phys

    K. Werner,Phys. Rept.232(1993) 87

  54. [62]

    A. B. Kaidalov,Phys. Lett. B116(1982) 459

  55. [63]

    Artru,Phys

    X. Artru,Phys. Rept.97(1983) 147

  56. [64]

    Eichten, K

    E. Eichten, K. Gottfried, T. Kinoshita, J. B. Kogut, K. D. Lane and T. Yan,Phys. Rev. Lett.34(1975) 369

  57. [65]

    Braun and C

    M. Braun and C. Pajares,Nucl. Phys. B390(1993) 542

  58. [66]

    Werner,Phys

    K. Werner,Phys. Rev. C108(2023) 064903

  59. [67]

    Sj¨ ostrand,Comput

    T. Sj¨ ostrand,Comput. Phys. Commun.246(2020) 106910

  60. [68]

    Wang and M

    X.-N. Wang and M. Gyulassy,Phys. Rev. D44(1991) 3501

  61. [69]

    Zhang, C

    B. Zhang, C. M. Ko, B.-A. Li and Z.-w. Lin,Phys. Rev. C61(2000) 067901

  62. [70]

    Cassing and E

    W. Cassing and E. L. Bratkovskaya,Phys. Rev. C78(2008) 034919, arXiv:0808.0022 [hep-ph]

  63. [71]

    Andersson and P

    B. Andersson and P. A. Henning,Nucl. Phys. B355(1991) 82

  64. [72]

    Jafarpour, V

    M. Jafarpour, V. Voronyuk, K. Werner, E. Bratkovskaya and D. Vintache (9 2025) arXiv:2509.05428 [hep-ph]

  65. [73]

    P. Cea, L. Cosmai, F. Cuteri and A. Papa,Phys. Rev. D89(2014) 094505

  66. [74]

    Nishino, K.-I

    S. Nishino, K.-I. Kondo, A. Shibata, T. Sasago and S. Kato,Eur. Phys. J. C79 (2019) 774

  67. [75]

    Bierlich, G

    C. Bierlich, G. Gustafson, L. L¨ onnblad and A. Tarasov,JHEP03(2015) 148, arXiv:1412.6259 [hep-ph]

  68. [76]

    M. A. Braun, C. Pajares and J. Ranft,Int. J. Mod. Phys. A14(1999) 2689

  69. [77]

    G. S. Bali,Phys. Rev. D62(2000) 114503

  70. [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]

  71. [79]

    Acharyaet al.),JHEP10(2021) 159,arXiv:2105.05616 [nucl-ex]

    ALICE Collaboration (S. Acharyaet al.),JHEP10(2021) 159,arXiv:2105.05616 [nucl-ex]

  72. [80]

    Acharyaet al.),Phys

    ALICE Collaboration (S. Acharyaet al.),Phys. Lett. B829(2022) 137065, arXiv:2111.11948 [nucl-ex]

  73. [81]

    Tumasyanet al.),JHEP01(2024) 128,arXiv:2307.11186 [nucl-ex]

    CMS Collaboration (A. Tumasyanet al.),JHEP01(2024) 128,arXiv:2307.11186 [nucl-ex]

  74. [82]

    Brocket al.),Rev

    CTEQ Collaboration (R. Brocket al.),Rev. Mod. Phys.67(1995) 157

  75. [83]

    Bierlichet al.,SciPost Phys

    C. Bierlichet al.,SciPost Phys. Codeb.2022(2022) 8,arXiv:2203.11601 [hep-ph]

  76. [84]

    A. B. Kaidalov and K. A. Ter-Martirosian,Phys. Lett. B117(1982) 247

  77. [85]

    V. V. Vechernin and S. N. Belokurova,J. Phys. Conf. Ser.1690(2020) 012088

  78. [86]

    H.-L. Lai, M. Guzzi, J. Huston, Z. Li, P. M. Nadolsky, J. Pumplin and C. P. Yuan, Phys. Rev. D82(2010) 074024

  79. [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

  80. [88]

    Shen and B

    C. Shen and B. Schenke,Phys. Rev. C97(2018) 024907,arXiv:1710.00881 [nucl-th]

  81. [89]

    Luscher, G

    M. Luscher, G. Munster and P. Weisz,Nucl. Phys. B180(1981) 1

  82. [90]

    Andersson, G

    B. Andersson, G. Gustafson, G. Ingelman and T. Sjostrand,Phys. Rept.97(1983) 31

  83. [91]

    Braaten and M

    E. Braaten and M. H. Thoma,Phys. Rev. D44(1991) 1298

  84. [92]

    M. E. Carrington, A. Czajka and S. Mrowczynski,Nucl. Phys. A1001(2020) 121914, arXiv:2001.05074 [nucl-th]

  85. [93]

    M. E. Carrington, A. Czajka and S. Mrowczynski,Phys. Lett. B834(2022) 137464, arXiv:2112.06812 [hep-ph]

  86. [94]

    Schenke, C

    B. Schenke, C. Gale and S. Jeon,Phys. Rev. C80(2009) 054913,arXiv:0909.2037 [hep-ph]

  87. [95]

    P. B. Gossiaux and J. Aichelin,Phys. Rev. C78(2008) 014904,arXiv:0802.2525 [hep-ph]

  88. [96]

    Aichelin, P

    J. Aichelin, P. B. Gossiaux and T. Gousset,Phys. Rev. D89(2014) 074018, arXiv:1307.5270 [hep-ph]

  89. [97]

    J. Xu, J. Liao and M. Gyulassy,Chin. Phys. Lett.32(2015) 092501, arXiv:1411.3673 [hep-ph]

  90. [98]

    M. H. Thoma and M. Gyulassy,Nucl. Phys. B351(1991) 491

  91. [99]

    Peigne and A

    S. Peigne and A. Peshier,Phys. Rev. D77(2008) 114017,arXiv:0802.4364 [hep-ph]

  92. [100]

    J. D. Bjorken (8 1982)

  93. [101]

    S. Shi, J. Liao and M. Gyulassy,Chin. Phys. C42(2018) 104104,arXiv:1804.01915 [hep-ph]

  94. [102]

    Liao and E

    J. Liao and E. Shuryak,Phys. Rev. Lett.101(2008) 162302,arXiv:0804.0255 [hep-ph]

  95. [103]

    S. Shi, J. Liao and M. Gyulassy,Chin. Phys. C43(2019) 044101,arXiv:1808.05461 [hep-ph]

  96. [104]

    P. B. Gossiaux and J. Aichelin,J. Phys. G36(2009) 064028,arXiv:0901.2462 [nucl-th]

  97. [105]

    J. Xu, A. Buzzatti and M. Gyulassy,JHEP08(2014) 063,arXiv:1402.2956 [hep-ph]

  98. [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...

  99. [107]

    Romatschke and M

    P. Romatschke and M. Strickland,Phys. Rev. D68(2003) 036004, arXiv:hep-ph/0304092

  100. [108]

    Romatschke and M

    P. Romatschke and M. Strickland,Phys. Rev. D70(2004) 116006, arXiv:hep-ph/0406188

  101. [109]

    Y. Peng, V. E. Ambrus, C. Werthmann, S. Schlichting, U. Heinz and H. Song (9 2025)arXiv:2509.04431 [nucl-th]

  102. [110]

    J. Zhao, J. Aichelin, P. B. Gossiaux and K. Werner,Phys. Rev. C111(2025) 014907, arXiv:2407.20919 [hep-ph]

  103. [111]

    S. Zhao, Y. Peng, U. W. Heinz and H. Song (9 2025)arXiv:2509.03841 [nucl-th]

Pith tools

Reviewed May 18, 2026 · model on record in the stance chip above.