REVIEW 4 major objections 11 minor 86 references
Towards factorization of jet observables in dense media : An EFT approach
T0 review · 4 major / 11 minor · reviewed 2026-08-07 · deepseek-v4-flash
Pith's one-line read This review argues that jet energy-correlator cross-sections in a quark-gluon plasma factorize into a hard function times a medium-modified jet function.
desk verdict A self-citing review that is the best current map to the OQS+SCET+Glauber framework for ν-correlators in heavy-ion jets, but its central k− power-counting step is not justified on the paper's own scaling. 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 machinery is Glauber-extended SCET II. In this effective theory, Glauber gluons have momentum scaling $Q(\lambda,\lambda^2,\lambda)$ and mediate instantaneous, near-forward exchanges between collinear jet partons and soft thermal partons, through operators $O_{ns}=O_n(1/P_\perp^2)O_s$. The load-bearing identity is Eq. (35): it factors the cross-section into the hard function and a jet function whose medium part is the real-minus-virtual double-Glauber contribution. That contribution contains the two essential objects of the paper: the length-enhanced sinc phase coming from the finite extent $L$ of the medium, and the medium function $B(k)$, built from thermal spectral functions and depending only on transverse Glauber momentum. Resummation uses the BFKL kernel with eigenfunctions $|l|^{2\gamma-1}e^{in\phi_l}$, which turns the leading logarithms of $1/\sqrt{\chi}$ into an exponentiated anomalous-dimension integral.
What would settle it
Take the medium function to depend on the full Glauber momentum rather than only on its transverse part, and recompute the double-Glauber jet function; if the result cannot be written as $J_{qR}-J_{qV}$ times the same hard function, the factorization fails. Experimentally, one can bin two-point energy-correlator data by estimated path length in heavy-ion collisions and check whether the medium modification scales as $L$ with the predicted sinc phase, rather than showing an energy shift of the jet parton.
Extended reading notes
Core claim
On the paper's own terms, the central claim is Eq. (35): $d\sigma^{[\nu]}/d\chi = |C(Q)|^2 L^{\alpha\beta} \int dx\, x^\nu\, H_q^{\alpha\beta}(\omega,\mu)\,\big[J_{q0}^{[\nu]} + (J_{qR}^{[\nu]}-J_{qV}^{[\nu]})\big]$, with each factor fully specified through double Glauber insertions. The hard function $H_q^{\alpha\beta}$ describes production of the jet-initiating quark, while the jet function $J_q^{[\nu]}$ describes its vacuum and in-medium evolution; the medium correction is the difference of real and virtual Glauber contributions, each proportional to the medium length $L$ and carrying the phase $e^{i(p_a^+-p_b^+)L/2}\mathrm{sinc}[(p_a^+-p_b^+)L/2]$ alongside a transverse-momentum-dependent medium function $B(k)$. The paper shows the same factorization in the wide-separation hierarchy $Q\gg Q\sqrt{\chi}\gg Q_{\rm med}$, where the medium-induced radiation can be refactorized into matching functions and a BFKL-evolved function. It also extends the single-scattering result to independent multiple scatterings when the mean free path exceeds the screening length.
Load-bearing premise
The factorization holds only if each Glauber exchange changes the jet parton's transverse momentum but not its energy, i.e., the longitudinal-momentum component $k^-$ can be dropped; if the medium transfers non-negligible longitudinal momentum, Eq. (35) is not the leading-power result.
Editorial extensions
If this is right
- The medium modification of $\nu$-correlators is calculable order by order in Glauber insertions, with the first correction fixed explicitly in the soft limit by Eq. (36).
- At small $\chi$, the large logarithms $\ln(1/\sqrt{\chi})$ can be resummed by BFKL evolution between the jet scale and the medium scale, giving concrete analytic predictions for the large-angle region.
- The factorization extends to other jet substructure observables by replacing the measurement function, and to gluon jets by adding the collinear gluon operators.
- When scatterings are independent, multiple Glauber exchanges resum into products of single-scattering medium functions, providing an EFT route to emergent medium scales such as $\hat q$.
- The same framework connects to inclusive jet production, so energy-correlator predictions can be checked against the established inclusive-jet factorization results.
Reading between the lines
- If the factorization is correct, the ratio of in-medium to vacuum energy-energy correlators should show a linear growth with path length $L$ in the dilute single-scattering regime; a dedicated centrality or long-lived-jet measurement could look for that scaling.
- The paper leaves the gluon-jet and proton-proton extensions implicit; adding PDFs and nuclear PDFs would turn Eq. (35) into a prediction for heavy-ion collider data, which seems a natural next step.
- The BFKL saddle-point solutions in Eqs. (49)--(51) could be used to extract the in-medium anomalous dimension of the $\nu$-correlator, an extraction the paper identifies as needed but does not carry out.
- A testable extension is to compute the first subleading Glauber correction and check whether the length enhancement remains a simple sinc phase or acquires a $\hat q$-dependent width; that would delimit the single-scattering regime.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. This manuscript presents an EFT framework for factorizing medium-modified projected ν-point energy correlators in heavy-ion collisions. Starting from an open-quantum-system density matrix and Glauber-extended SCET, it derives a factorized cross-section, Eq. (35), of the form dσ[ν]/dχ = |C(Q)|² L^{αβ} ∫ dx x^ν H_q^{αβ}(ω,μ) [J_q0[ν] + J_qR[ν] − J_qV[ν]], where the medium enters through double Glauber insertions, a thermal medium function B(k), and a length-enhanced LPM phase. The paper also discusses BFKL resummation of the resulting jet function and an extension to multiple scatterings. Much of the technical content is drawn from the author's prior work (Refs. 67–71), and the detailed single-scattering jet-function computation is quoted rather than derived.
Significance. If correct, this factorization would be a valuable step: it gives a systematic SCET basis for a class of jet-substructure observables in dense media, exposes the LPM phase and a thermal medium function, and provides a concrete BFKL resummation of logarithms of the measurement χ. The paper is also useful as a review that collects recent results in one place, and the operator definitions of the medium function are explicit and physically motivated. Its main strengths are the transparent separation of scales and the clear Lund-plane discussion. However, the paper is largely an exposition of the author's own previous results; the central diagrammatic calculation is deferred to Ref. [70], and no independent numerical predictions or machine-checked derivations are included. The expository value is real, but the research-level claim embodied in Eq. (35) is not self-contained as written.
major comments (4)
- [Section 4.1, Eqs. (31)–(32)] The step 'we can drop k− as this is suppressed compared to p− component of collinear mode' is not supported by the power counting given in Section 2.1. There the collinear mode scales as (p+, p−, p⊥) ∼ Q(1, λ², λ) and the Glauber mode as (k+, k−, k⊥) ∼ Q(λ, λ², λ), so k− and the collinear p− are the same order in λ. Moreover, in the phase e^{ik·ŷ}, the term k− ŷ+ is O(1) because ŷ+ ∼ 1/(Qλ²) for collinear operators. Dropping k− is therefore an additional physical assumption (essentially zero longitudinal momentum transfer in the Glauber vertex) that must be stated and justified. Without it, the reduction of the ȳ− integral to the factor L e^{i(p_a+−p_b+)L/2} sinc[(p_a+−p_b+)L/2] and hence the factorized formula (35) are not established.
- [Section 4.1, Eqs. (35)–(36)] The central non-trivial object, the leading medium-induced jet function J_q2, is not derived in this manuscript. The text explicitly directs the reader to Ref. [70] for the detailed diagram computation and then quotes Eq. (36) as the final soft-limit expression. Since this object carries the LPM/sinc structure and the convolution with the medium function B(k) that are essential to Eq. (35), the factorization claim is not self-contained. For a research article this is a load-bearing omission; at minimum the manuscript must either provide the derivation or clearly and consistently frame itself as a review of Ref. [70].
- [Section 4.1, after Eq. (24)] The statement that 'only even number of insertions contribute to the jet function and odd one vanishes' is asserted without proof. This vanishing is essential because Eq. (35) truncates the Glauber expansion at two insertions; if odd insertions contributed at leading power, Eq. (35) would be incomplete. Please provide the argument (for example, color neutrality of the medium, or a symmetry of the forward-scattering amplitude) or cite a derivation that establishes it.
- [Section 4.2 and Eq. (52)] The multiple-scattering factorization, with a product of independent medium functions B(k_l) and the combinatorial factor L^{j/2}/(j/2)! in Eq. (52), is introduced as an ansatz after the statement that the scatterings are independent when the mean free path is larger than the Debye screening length. No derivation or power counting is given for this independence criterion or for the resummation of arbitrary Glauber insertions. Since this is a central element of the claimed all-order structure, it should be substantiated or explicitly attributed to a prior derivation.
minor comments (11)
- [Title] The full-text title reads 'T owards factorization...' with a stray space; it should be 'Towards factorization...'.
- [Section 2, before Eq. (2)] The phrase 'takes the form the form' is duplicated and should be corrected.
- [Section 2, momentum scaling] The notation '¯n·p (1, λ², λ)' is ambiguous; label the triple as (p+, p−, p⊥) to match Eq. (1) and the subsequent discussion.
- [Section 3, Eq. (8)] The index ranges in the sums, e.g., '1≤b1≤M' and '1≤b1<..<bM=N', are notationally inconsistent and should be cleaned up.
- [Section 4.1, Eqs. (29)–(31)] The medium function is denoted S(y1,y2) in the text and S_ab(ŷ,ȳ) in Eq. (30); please use one consistent notation throughout.
- [Section 4.1, Eqs. (31)–(32)] The arguments of B are written B(k−,k) in Eq. (31) and B(k) in Eq. (32); make the light-cone and transverse components explicit, e.g., B(k−,k⊥) and B(k⊥).
- [Section 4.1, after Eq. (32)] 'after performing ¯x− interaction' should read 'after performing the ȳ− integration'.
- [Section 4.2, Eq. (37)] The Lorentz indices are inconsistent: the prefactor is L^{µα} but the hard function is written H^{µα}_q, while Eq. (35) uses L^{αβ}H^{αβ}_q; unify the notation.
- [Section 5, before Eq. (48)] The phrase 'we can obtain analytic solution for specific cases by within diffusion and double logarithmic approximation approximation' contains duplicated and ungrammatical words; please rephrase.
- [Appendix A] 'Weightman correlaotrs' should read 'Wightman correlators'; also the sentence introducing the gluon spectral function should specify whether it refers to the gluon or quark correlator in each place.
- [References] Several references are incomplete or inconsistently formatted (e.g., Refs. [30], [51], [58]–[66] in the text and some arXiv identifiers); please standardize the bibliography.
Circularity Check
No significant circularity: the medium-modified ν-correlator factorization is derived in outline within the paper, and the deferred diagrammatic details in the author's prior Ref. 70 are legitimate references rather than a circular input.
full rationale
The paper is a review article whose central result, Eq. (35), is reached by an explicit (if abridged) derivation: Eq. (16) is the master formula, Eq. (21) is the hard/jet factorization, Eqs. (23)–(28) expand the jet function in Glauber insertions, Eq. (29) defines the medium correlator, Eqs. (30)–(32) perform the kinematic simplifications, Eq. (34) gives the virtual piece, and Eq. (35) combines them. No parameter is fitted to the claimed prediction and no external result is renamed; the BFKL kernel is taken from the independent Kovchegov–Levin textbook. The text defers the detailed Feynman-diagram calculation to Ref. [70] (Singh and Vaidya), which is a self-citation, but that citation supplies an explicit parameter-free computation, not the conclusion of Eq. (35) itself; Eq. (35) is justified by the displayed operator derivation. The L enhancement in Eq. (32) follows from the assumed medium extent ȳ ∈ [0, L], an input model assumption, not from a quantity that was previously treated as unknown. The only serious technical concern is the power-counting for dropping k⁻ in Sec. 4.1: under the paper's own scalings, collinear p⁻ and Glauber k⁻ are both O(Qλ²), so the suppression is not demonstrated; this is a correctness/validity issue, not a circularity in the derivation chain. Accordingly, no circular step is identified.
Assumptions & free parameters
free parameters (1)
- Medium parameters for the Lund-plane illustration =
not fitted (illustrative): pT = 100 GeV, T ~ 0.5 GeV, q-hat ~ 1-2 GeV^2/fm, L ~ 5 fm, Qmed ~ 1-3 GeV
assumptions (6)
- domain assumption SCET power counting with lambda ~ T/Q and measurement scale Q sqrt(chi), with the hierarchy Q >> Q sqrt(chi) >= Qmed.
- domain assumption The medium is in thermal equilibrium, described by the factorized density matrix rhoB = exp(-beta Hs)/Tr[exp(-beta Hs)] that evolves only with the soft Hamiltonian.
- domain assumption Glauber modes dominate jet-medium interactions and carry momentum pG ~ Q(lambda, lambda^2, lambda) with negligible k- transfer.
- domain assumption Only even numbers of Glauber insertions contribute to the jet function; odd insertions vanish.
- domain assumption The medium is homogeneous and carries no net color charge, encoded by replacing color structure with delta_ab and dropping the y-bar dependence in the medium function.
- standard math The BFKL kernel has the standard eigenvalue representation with eigenfunctions |l|^(2 gamma - 1) e^(i n phi) and eigenvalue chi(n, gamma).
Cite this review
Pith. "Pith review of Towards factorization of jet observables in dense media : An EFT approach." pith.science (2026). https://pith.science/paper/UETLSFBX
@misc{pith2026250518070,
author = {Pith},
title = {Pith review of: Towards factorization of jet observables in dense media : An EFT approach},
year = {2026},
howpublished = {\url{https://pith.science/paper/UETLSFBX}},
note = {Machine review of arXiv:2505.18070}
}
abstract
Jets are extended multipartonic systems and serve as a powerful tool for investigating the dynamics of emergent phenomena driven by many body QCD interactions. In heavy ion collisions, starting from their production during the perturbative hard scattering event in the initial stages of the collision to non-perturbative hadronization they interact with the various stages of quark-gluon plasma and retain imprints of fundamental properties of the medium. In these collisions, the jet production cross-section can be factorized using open quantum system framework along with effective field theory into various functions, each capturing a specific dynamics and depending on a single characteristic scale. In this review article, we discuss recent theoretical developments on factorization for jets in heavy-ion collisions with a specific example of jet substructure observable as energy-energy correlator and its generalization to projected $\nu$-point energy correlators.
Figures
Reference graph
Works this paper leans on
- [70]
-
[1]
G. P. Salam, Eur. Phys. J. C 67, 637 (2010), arXiv:0906.1833 [hep-ph], doi:10. 1140/epjc/s10052-010-1314-6
arXiv 2010
-
[2]
BRAHMS Collaboration (I. Arsene et al. ), Nucl. Phys. A 757, 1 (2005), arXiv:nucl-ex/0410020, doi:10.1016/j.nuclphysa.2005.02.130
arXiv 2005
-
[3]
M. Connors, C. Nattrass, R. Reed and S. Salur, Rev. Mod. Phys.90, 025005 (2018), arXiv:1705.01974 [nucl-ex], doi:10.1103/RevModPhys.90.025005
arXiv 2018
-
[4]
PHOBOS Collaboration (B. B. Back et al. ), Nucl. Phys. A 757, 28 (2005), arXiv:nucl-ex/0410022, doi:10.1016/j.nuclphysa.2005.03.084
arXiv 2005
-
[5]
ALICE Collaboration (S. Acharya et al. ), Phys. Lett. B 849, 138412 (2024), arXiv:2303.00592 [nucl-ex], doi:10.1016/j.physletb.2023.138412
arXiv 2024
-
[6]
STAR Collaboration (J. Adams et al. ), Nucl. Phys. A 757, 102 (2005), arXiv:nucl-ex/0501009, doi:10.1016/j.nuclphysa.2005.03.085
arXiv 2005
-
[7]
CMS Collaboration (A. M. Sirunyan et al.), JHEP 05, 284 (2021), arXiv:2102.13080 [hep-ex], doi:10.1007/JHEP05(2021)284
arXiv 2021
Show all 86 references
-
[8]
Adcox et al
PHENIX Collaboration (K. Adcox et al. ), Nucl. Phys. A 757, 184 (2005), arXiv:nucl-ex/0410003, doi:10.1016/j.nuclphysa.2005.03.086
2005 arXiv
-
[9]
Chatrchyan et al
CMS Collaboration (S. Chatrchyan et al. ), Phys. Rev. C 84, 024906 (2011), arXiv:1102.1957 [nucl-ex], doi:10.1103/PhysRevC.84.024906
2011 arXiv
-
[10]
Aamodt et al
ALICE Collaboration (K. Aamodt et al. ), Phys. Lett. B 696, 30 (2011), arXiv:1012.1004 [nucl-ex], doi:10.1016/j.physletb.2010.12.020
2011 arXiv
-
[11]
Aad et al
ATLAS Collaboration (G. Aad et al. ), Phys. Rev. Lett. 105, 252303 (2010), arXiv:1011.6182 [hep-ex], doi:10.1103/PhysRevLett.105.252303
2010 arXiv
-
[12]
Gyulassy and M
M. Gyulassy and M. Plumer, Phys. Lett. B 243, 432 (1990), doi:10.1016/ 0370-2693(90)91409-5
1990
-
[13]
Gyulassy, M
M. Gyulassy, M. Plumer, M. Thoma and X. N. Wang, Nucl. Phys. A538, 37C (1992), doi:10.1016/0375-9474(92)90756-A
1992 doi
-
[14]
Wang and M
X.-N. Wang and M. Gyulassy, Phys. Rev. Lett. 68, 1480 (1992), doi:10.1103/ PhysRevLett.68.1480
1992
-
[15]
C. E. Coleman-Smith, S. A. Bass and D. K. Srivastava, Nucl. Phys. A862-863, 275 (2011), arXiv:1101.4895 [hep-ph], doi:10.1016/j.nuclphysa.2011.05.071
2011 arXiv
-
[16]
Baier, Y
R. Baier, Y. L. Dokshitzer, A. H. Mueller and D. Schiff, Nucl. Phys. B531, 403 (1998), arXiv:hep-ph/9804212, doi:10.1016/S0550-3213(98)00546-X
1998 arXiv
-
[17]
Baier, D
R. Baier, D. Schiff and B. G. Zakharov, Ann. Rev. Nucl. Part. Sci.50, 37 (2000), arXiv:hep-ph/0002198, doi:10.1146/annurev.nucl.50.1.37
2000 arXiv
-
[18]
U. A. Wiedemann and M. Gyulassy, Nucl. Phys. B 560, 345 (1999), arXiv:hep-ph/9906257, doi:10.1016/S0550-3213(99)00458-7
1999 arXiv
-
[19]
U. A. Wiedemann, Nucl. Phys. B 582, 409 (2000), arXiv:hep-ph/0003021, doi:10. 1016/S0550-3213(00)00286-8
2000 arXiv
-
[20]
L. D. Landau and I. Pomeranchuk, Dokl. Akad. Nauk Ser. Fiz.92, 535 (1953)
1953
-
[21]
A. B. Migdal, Phys. Rev. 103, 1811 (1956), doi:10.1103/PhysRev.103.1811
1956 doi
-
[22]
Arnold, O
P. Arnold, O. Elgedawy and S. Iqbal, JHEP 01, 193 (2025), arXiv:2408.07129 [hep-ph], doi:10.1007/JHEP01(2025)193
2025 arXiv
-
[23]
Arnold, O
P. Arnold, O. Elgedawy and S. Iqbal, JHEP 09, 131 (2024), arXiv:2404.19008 [hep-ph], doi:10.1007/JHEP09(2024)131
2024 arXiv
-
[24]
Casalderrey-Solana, Y
J. Casalderrey-Solana, Y. Mehtar-Tani, C. A. Salgado and K. Tywoniuk, Phys. Lett. B 725, 357 (2013), arXiv:1210.7765 [hep-ph], doi:10.1016/j.physletb.2013.07.046
2013 arXiv
-
[25]
Mehtar-Tani, C
Y. Mehtar-Tani, C. A. Salgado and K. Tywoniuk, Acta Phys. Polon. Supp. 4, 623 (2011), doi:10.5506/APhysPolBSupp.4.623
2011 doi
-
[26]
Mehtar-Tani, C
Y. Mehtar-Tani, C. A. Salgado and K. Tywoniuk, JHEP 04, 064 (2012), 22 arXiv:1112.5031 [hep-ph], doi:10.1007/JHEP04(2012)064
2012 arXiv
-
[27]
Mehtar-Tani, C
Y. Mehtar-Tani, C. A. Salgado and K. Tywoniuk, JHEP 10, 197 (2012), arXiv:1205.5739 [hep-ph], doi:10.1007/JHEP10(2012)197
2012 arXiv
-
[28]
Mehtar-Tani and K
Y. Mehtar-Tani and K. Tywoniuk, Nucl. Phys. A979, 165 (2018), arXiv:1706.06047 [hep-ph], doi:10.1016/j.nuclphysa.2018.09.041
2018 arXiv
-
[29]
Mehtar-Tani and K
Y. Mehtar-Tani and K. Tywoniuk, Phys. Rev. D98, 051501 (2018), arXiv:1707.07361 [hep-ph], doi:10.1103/PhysRevD.98.051501
2018 arXiv
-
[30]
Mehtar-Tani (11 2024), arXiv:2411.11992 [hep-ph]
Y. Mehtar-Tani (11 2024), arXiv:2411.11992 [hep-ph]
2024 arXiv
-
[31]
Gyulassy, I
M. Gyulassy, I. Vitev, X.-N. Wang and B.-W. Zhang, 123 (2004), arXiv:nucl-th/0302077, doi: 10.1142/9789812795533 0003
2004 arXiv
-
[32]
C. A. Salgado and U. A. Wiedemann, Phys. Rev. Lett. 93, 042301 (2004), arXiv:hep-ph/0310079, doi:10.1103/PhysRevLett.93.042301
2004 arXiv
-
[33]
G.-Y. Qin, J. Ruppert, C. Gale, S. Jeon, G. D. Moore and M. G. Mustafa, Phys. Rev. Lett. 100, 072301 (2008), arXiv:0710.0605 [hep-ph], doi:10.1103/PhysRevLett.100. 072301
2008 arXiv
-
[34]
K. Zapp, G. Ingelman, J. Rathsman, J. Stachel and U. A. Wiedemann, Eur. Phys. J. C 60, 617 (2009), arXiv:0804.3568 [hep-ph], doi:10.1140/epjc/s10052-009-0941-2
2009 arXiv
-
[35]
Casalderrey-Solana, D
J. Casalderrey-Solana, D. C. Gulhan, J. G. Milhano, D. Pablos and K. Rajagopal, JHEP 10, 019 (2014), arXiv:1405.3864 [hep-ph], doi:10.1007/JHEP09(2015)175, [Erratum: JHEP 09, 175 (2015)]
2014 arXiv
-
[36]
Qin and X.-N
G.-Y. Qin and X.-N. Wang, Int. J. Mod. Phys. E 24, 1530014 (2015), arXiv:1511.00790 [hep-ph], doi:10.1142/S0218301315300143
2015 arXiv
-
[37]
Y. He, T. Luo, X.-N. Wang and Y. Zhu, Phys. Rev. C 91, 054908 (2015), arXiv:1503.03313 [nucl-th], doi:10.1103/PhysRevC.91.054908, [Erratum: Phys.Rev.C 97, 019902 (2018)]
2015 arXiv
-
[38]
Chien and I
Y.-T. Chien and I. Vitev, JHEP 05, 023 (2016), arXiv:1509.07257 [hep-ph], doi: 10.1007/JHEP05(2016)023
2016 arXiv
-
[39]
Wang, S.-Y
X.-N. Wang, S.-Y. Wei and H.-Z. Zhang, Phys. Rev. C 96, 034903 (2017), arXiv:1611.07211 [hep-ph], doi:10.1103/PhysRevC.96.034903
2017 arXiv
-
[40]
Y. He, S. Cao, W. Chen, T. Luo, L.-G. Pang and X.-N. Wang, Phys. Rev. C 99, 054911 (2019), arXiv:1809.02525 [nucl-th], doi:10.1103/PhysRevC.99.054911
2019 arXiv
-
[41]
Casalderrey-Solana, G
J. Casalderrey-Solana, G. Milhano, D. Pablos and K. Rajagopal, JHEP 01, 044 (2020), arXiv:1907.11248 [hep-ph], doi:10.1007/JHEP01(2020)044
2020 arXiv
-
[42]
Caucal, E
P. Caucal, E. Iancu and G. Soyez, JHEP 10, 273 (2019), arXiv:1907.04866 [hep-ph], doi:10.1007/JHEP10(2019)273
2019 arXiv
-
[43]
Vaidya and X
V. Vaidya and X. Yao, JHEP 10, 024 (2020), arXiv:2004.11403 [hep-ph], doi:10. 1007/JHEP10(2020)024
2020 arXiv
-
[44]
Vaidya, JHEP 11, 064 (2021), arXiv:2010.00028 [hep-ph], doi:10.1007/ JHEP11(2021)064
V. Vaidya, JHEP 11, 064 (2021), arXiv:2010.00028 [hep-ph], doi:10.1007/ JHEP11(2021)064
2021 arXiv
-
[45]
A. Baty, P. Gardner and W. Li, Phys. Rev. C107, 064908 (2023), arXiv:2104.11735 [hep-ph], doi:10.1103/PhysRevC.107.064908
2023 arXiv
-
[46]
Cunqueiro and A
L. Cunqueiro and A. M. Sickles, Prog. Part. Nucl. Phys. 124, 103940 (2022), arXiv:2110.14490 [nucl-ex], doi:10.1016/j.ppnp.2022.103940
2022 arXiv
-
[47]
Vaidya, JHEP 05, 028 (2024), arXiv:2107.00029 [hep-ph], doi:10.1007/ JHEP05(2024)028
V. Vaidya, JHEP 05, 028 (2024), arXiv:2107.00029 [hep-ph], doi:10.1007/ JHEP05(2024)028
2024 arXiv
-
[48]
Caucal, A
P. Caucal, A. Soto-Ontoso and A. Takacs, Phys. Rev. D 105, 114046 (2022), arXiv:2111.14768 [hep-ph], doi:10.1103/PhysRevD.105.114046
2022 arXiv
-
[49]
Mehtar-Tani, D
Y. Mehtar-Tani, D. Pablos and K. Tywoniuk, Phys. Rev. Lett.127, 252301 (2021), arXiv:2101.01742 [hep-ph], doi:10.1103/PhysRevLett.127.252301. 23
2021 arXiv
-
[50]
Kumar et al.), Phys
JETSCAPE Collaboration (A. Kumar et al.), Phys. Rev. C 107, 034911 (2023), arXiv:2204.01163 [hep-ph], doi:10.1103/PhysRevC.107.034911
2023 arXiv
- [51]
-
[52]
Zhang, E
S.-L. Zhang, E. Wang, H. Xing and B.-W. Zhang, Phys. Lett. B850, 138549 (2024), arXiv:2303.14881 [hep-ph], doi:10.1016/j.physletb.2024.138549
2024 arXiv
-
[53]
J. a. Barata, J. G. Milhano and A. V. Sadofyev, Eur. Phys. J. C 84, 174 (2024), arXiv:2308.01294 [hep-ph], doi:10.1140/epjc/s10052-024-12514-1
2024 arXiv
-
[54]
Ovanesyan and I
G. Ovanesyan and I. Vitev, JHEP 06, 080 (2011), arXiv:1103.1074 [hep-ph], doi: 10.1007/JHEP06(2011)080
2011 arXiv
-
[55]
Ovanesyan and I
G. Ovanesyan and I. Vitev, Phys. Lett. B 706, 371 (2012), arXiv:1109.5619 [hep-ph], doi:10.1016/j.physletb.2011.11.040
2012 arXiv
-
[56]
Andres, F
C. Andres, F. Dominguez, J. Holguin, C. Marquet and I. Moult, JHEP 09, 088 (2023), arXiv:2303.03413 [hep-ph], doi:10.1007/JHEP09(2023)088
2023 arXiv
-
[57]
Andres, F
C. Andres, F. Dominguez, R. Kunnawalkam Elayavalli, J. Holguin, C. Marquet and I. Moult, Phys. Rev. Lett.130, 262301 (2023), arXiv:2209.11236 [hep-ph], doi:10. 1103/PhysRevLett.130.262301
2023 arXiv
-
[58]
J. a. Barata, I. Moult, A. V. Sadofyev and J. a. M. Silva (3 2025), arXiv:2503.13603 [hep-ph]
2025 arXiv
-
[59]
Apolin´ ario, R
L. Apolin´ ario, R. Kunnawalkam Elayavalli, N. O. Madureira, J.-X. Sheng, X.-N. Wang and Z. Yang (2 2025), arXiv:2502.11406 [hep-ph]
2025 arXiv
-
[60]
Andres, F
C. Andres, F. Dominguez, J. Holguin, C. Marquet and I. Moult (11 2024), arXiv:2411.15298 [hep-ph]
2024 arXiv
-
[61]
X. Liu, W. Vogelsang, F. Yuan and H. X. Zhu, Phys. Rev. Lett.134, 151901 (2025), arXiv:2410.16371 [hep-ph], doi:10.1103/PhysRevLett.134.151901
2025 arXiv
-
[62]
Andres, J
C. Andres, J. Holguin, R. Kunnawalkam Elayavalli and J. Viinikainen, Phys. Rev. Lett. 134, 082303 (2025), arXiv:2409.07514 [hep-ph], doi:10.1103/PhysRevLett. 134.082303
2025 arXiv
-
[63]
Alipour-fard, A
S. Alipour-fard, A. Budhraja, J. Thaler and W. J. Waalewijn (10 2024), arXiv:2410.16368 [hep-ph]
2024 arXiv
-
[64]
Bossi, A
H. Bossi, A. S. Kudinoor, I. Moult, D. Pablos, A. Rai and K. Rajagopal, JHEP 12, 073 (2024), arXiv:2407.13818 [hep-ph], doi:10.1007/JHEP12(2024)073
2024 arXiv
-
[65]
Z. Yang, Y. He, I. Moult and X.-N. Wang, Phys. Rev. Lett. 132, 011901 (2024), arXiv:2310.01500 [hep-ph], doi:10.1103/PhysRevLett.132.011901
2024 arXiv
-
[66]
A.-P. Chen, X. Liu and Y.-Q. Ma, Phys. Rev. Lett.133, 19 (2024), arXiv:2405.10056 [hep-ph], doi:10.1103/PhysRevLett.133.191901
2024 arXiv
-
[67]
Mehtar-Tani, F
Y. Mehtar-Tani, F. Ringer, B. Singh and V. Vaidya (9 2024), arXiv:2409.05957 [hep-ph]
2024 arXiv
-
[68]
Mehtar-Tani, F
Y. Mehtar-Tani, F. Ringer, B. Singh and V. Vaidya (3 2025), arXiv:2504.00101 [hep-ph]
2025 arXiv
- [69]
-
[71]
Budhraja and B
A. Budhraja and B. Singh (3 2025), arXiv:2503.20019 [hep-ph]
2025
-
[72]
C. W. Bauer, D. Pirjol and I. W. Stewart, Phys. Rev. D 67, 071502 (2003), arXiv:hep-ph/0211069, doi:10.1103/PhysRevD.67.071502
2003 arXiv
-
[73]
C. W. Bauer, S. Fleming, D. Pirjol and I. W. Stewart, Phys. Rev. D63, 114020 (2001), arXiv:hep-ph/0011336, doi:10.1103/PhysRevD.63.114020
2001 arXiv
-
[74]
C. W. Bauer and I. W. Stewart, Phys. Lett. B 516, 134 (2001), arXiv:hep-ph/0107001, doi:10.1016/S0370-2693(01)00902-9
2001 arXiv
-
[75]
C. W. Bauer, S. Fleming, D. Pirjol, I. Z. Rothstein and I. W. Stewart, Phys. Rev. D 24 66, 014017 (2002), arXiv:hep-ph/0202088, doi:10.1103/PhysRevD.66.014017
2002 arXiv
-
[76]
I. Z. Rothstein and I. W. Stewart, JHEP 08, 025 (2016), arXiv:1601.04695 [hep-ph], doi:10.1007/JHEP08(2016)025
2016 arXiv
-
[77]
H. Chen, I. Moult, X. Zhang and H. X. Zhu, Phys. Rev. D 102, 054012 (2020), arXiv:2004.11381 [hep-ph], doi:10.1103/PhysRevD.102.054012
2020 arXiv
-
[78]
Andersson, G
B. Andersson, G. Gustafson, L. Lonnblad and U. Pettersson, Z. Phys. C 43, 625 (1989), doi:10.1007/BF01550942
1989 doi
-
[79]
F. A. Dreyer, G. P. Salam and G. Soyez, JHEP 12, 064 (2018), arXiv:1807.04758 [hep-ph], doi:10.1007/JHEP12(2018)064
2018 arXiv
-
[80]
Chicherin, I
D. Chicherin, I. Moult, E. Sokatchev, K. Yan and Y. Zhu, Phys. Rev. D110, L091901 (2024), arXiv:2401.06463 [hep-th], doi:10.1103/PhysRevD.110.L091901
2024 arXiv
-
[81]
Y. V. Kovchegov and E. Levin, Quantum Chromodynamics at High Energy(Oxford University Press, 2013)
2013
-
[82]
G. A. Chirilli and Y. V. Kovchegov, JHEP 06, 055 (2013), arXiv:1305.1924 [hep-ph], doi:10.1007/JHEP06(2013)055
2013 arXiv
-
[83]
C. R. Schmidt, Phys. Rev. Lett.78, 4531 (1997), arXiv:hep-ph/9612454, doi:10.1103/ PhysRevLett.78.4531
1997 arXiv
-
[84]
Baier, Y
R. Baier, Y. L. Dokshitzer, S. Peigne and D. Schiff, Phys. Lett. B345, 277 (1995), arXiv:hep-ph/9411409, doi:10.1016/0370-2693(94)01617-L
1995 arXiv
-
[85]
Baier, Y
R. Baier, Y. L. Dokshitzer, A. H. Mueller, S. Peigne and D. Schiff, Nucl. Phys. B483, 291 (1997), arXiv:hep-ph/9607355, doi:10.1016/S0550-3213(96)00553-6
1997 arXiv
-
[86]
Andres, L
C. Andres, L. Apolin´ ario, F. Dominguez and M. G. Martinez, JHEP 11, 025 (2024), arXiv:2307.06226 [hep-ph], doi:10.1007/JHEP11(2024)025
2024 arXiv
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