Event-by-event fluctuations of elliptic flow in ultrarelativistic O+O collisions
Pith reviewed 2026-06-26 09:37 UTC · model grok-4.3
The pith
In O+O collisions, elliptic flow and initial eccentricity arise mainly from event-by-event fluctuations in energy deposition rather than average geometry.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
In ultrarelativistic O+O collisions the initial elliptical eccentricity is mainly driven by the fluctuations of the energy deposition and thereby varies considerably event-by-event within a fixed centrality class. This also holds for elliptic flow v2, whose origin in O+O thus differs from that in collisions of heavy nuclei. Using a decomposition of initial states in an average event and uncorrelated modes, the joint probability distribution of eccentricity and elliptic flow can be reproduced with reasonable accuracy with only a small set of fluctuation modes.
What carries the argument
Decomposition of initial states into an average event plus uncorrelated fluctuation modes within the McDipper+MUSIC hydrodynamic framework.
If this is right
- Elliptic flow in O+O collisions must be treated as fluctuation-dominated rather than geometry-dominated.
- Centrality-selected samples in small systems contain substantial intrinsic variation in eccentricity and flow.
- A limited set of uncorrelated modes captures the essential statistics of eccentricity and v2 despite large fluctuations.
- Models of small-system collectivity need to incorporate detailed energy-deposition fluctuations to match data.
Where Pith is reading between the lines
- Similar fluctuation dominance is expected in other light-ion systems such as p+O or Ne+Ne.
- Hydrodynamic codes for small collisions require event-by-event initial conditions rather than averaged profiles.
- Interpreting flow observables in small systems may shift emphasis from initial geometry to stochastic deposition patterns.
Load-bearing premise
The McDipper+MUSIC model accurately reproduces the measured charged-hadron multiplicity dependence on centrality and pseudorapidity.
What would settle it
An experimental measurement of the event-by-event variance or joint distribution of v2 in O+O collisions that deviates significantly from the model's fluctuation-driven prediction.
Figures
read the original abstract
We study O+O collisions at $\sqrt{s_\mathrm{NN}} = 5.36$ TeV within a fully three-dimensional $\text{McDipper}$+$\text{MUSIC}$ model, which allows us to describe the experimentally measured dependence of charged hadron multiplicity on centrality and pseudorapidity. We show that the initial elliptical eccentricity is mainly driven by the fluctuations of the energy deposition and thereby varies considerably event-by-event within a fixed centrality class. This also holds for elliptic flow $v_2$, whose origin in O+O thus differs from that in collisions of heavy nuclei. Using a decomposition of initial states in an average event and uncorrelated modes, we find that despite the large size of fluctuations we can reproduce the joint probability distribution of eccentricity and elliptic flow with a reasonable accuracy with only a small set of fluctuation modes.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript studies O+O collisions at √s_NN = 5.36 TeV with the McDipper+MUSIC model, which is stated to reproduce the measured charged-hadron multiplicity dependence on centrality and pseudorapidity. It argues that initial elliptical eccentricity is driven primarily by fluctuations in energy deposition and therefore fluctuates strongly event-by-event even inside a fixed centrality bin; the same holds for elliptic flow v2, implying a fluctuation-dominated origin unlike the geometry-driven case in heavy-ion collisions. A decomposition of initial states into an average event plus uncorrelated modes is shown to reproduce the joint probability distribution of eccentricity and v2 to reasonable accuracy with only a small set of modes.
Significance. If the model validation and decomposition accuracy hold, the work clarifies that elliptic flow in light systems such as O+O arises from energy-deposition fluctuations rather than participant geometry, offering a concrete distinction from heavy-ion phenomenology. The mode-decomposition technique is a constructive element, as it demonstrates that a limited number of uncorrelated modes can capture the joint distribution despite large fluctuations.
minor comments (2)
- [Abstract] The abstract asserts that McDipper+MUSIC 'allows us to describe' the multiplicity data; explicit quantitative comparisons (e.g., χ² values or overlaid plots versus centrality and η) should be referenced by figure or table number to substantiate this central modeling assumption.
- The phrase 'reasonable accuracy' for the mode decomposition is used without a numerical metric; a quantitative measure (e.g., overlap integral or Kolmogorov-Smirnov distance between the reconstructed and full distributions) would clarify the claim that a small set of modes suffices.
Simulated Author's Rebuttal
We thank the referee for their positive summary, significance assessment, and recommendation of minor revision. No specific major comments appear in the report.
Circularity Check
No significant circularity identified
full rationale
The paper performs forward hydrodynamic simulations with the established McDipper+MUSIC model, first validating that the model reproduces measured charged-hadron multiplicity vs. centrality and pseudorapidity, then extracting eccentricity and v2 distributions directly from the generated events. The central claim that fluctuations dominate elliptical eccentricity (and thus v2) within a fixed centrality class follows as a post-processing observation on the simulated initial states and final flow; it is not obtained by fitting those quantities to data or by any self-referential definition. No load-bearing step reduces to a fitted input renamed as prediction, a self-citation chain, or an ansatz smuggled via prior work. The derivation chain is therefore self-contained against external multiplicity benchmarks.
Axiom & Free-Parameter Ledger
axioms (1)
- domain assumption McDipper+MUSIC reproduces the measured multiplicity dependence on centrality and pseudorapidity in O+O collisions.
Reference graph
Works this paper leans on
-
[1]
I. J. Abualrobet al.[ALICE Collaboration], arXiv:2509.06428 [nucl-ex]
-
[2]
Aadet al.[ATLAS Collaboration], Phys
G. Aadet al.[ATLAS Collaboration], Phys. Rev. C113, 14 045205 (2026). arXiv:2509.05171 [nucl-ex]
Pith/arXiv arXiv 2026
-
[3]
Hayrapetyanet al.[CMS Collaboration], arXiv:2510.02580 [nucl-ex]
A. Hayrapetyanet al.[CMS Collaboration], arXiv:2510.02580 [nucl-ex]
-
[4]
J. Y. Ollitrault, Phys. Rev. D46, 229 (1992)
1992
-
[5]
U. Heinz and R. Snellings, Ann. Rev. Nucl. Part. Sci.63, 123 (2013). arXiv:1301.2826 [nucl-th]
Pith/arXiv arXiv 2013
-
[6]
B. Alver and G. Roland, Phys. Rev. C81, 054905 (2010) [Erratum: Phys. Rev. C82, 039903 (2010)]. arXiv:1003.0194 [nucl-th]
Pith/arXiv arXiv 2010
-
[7]
M. Luzum and H. Petersen, J. Phys. G41, 063102 (2014). arXiv:1312.5503 [nucl-th]
Pith/arXiv arXiv 2014
-
[8]
A. Beraudo, A. De Pace, M. Monteno, M. Nardi and F. Prino, Eur. Phys. J. C79, 494 (2019). arXiv:1812.08337 [physics.data-an]
Pith/arXiv arXiv 2019
-
[9]
S. H. Lim, J. Carlson, C. Loizides, D. Lonardoni, J. E. Lynn, J. L. Nagle, J. D. Orjuela Koop and J. Ouel- lette, Phys. Rev. C99, 044904 (2019). arXiv:1812.08096 [nucl-th]
Pith/arXiv arXiv 2019
-
[10]
M. D. Sievert and J. Noronha-Hostler, Phys. Rev. C100, 024904 (2019) arXiv:1901.01319 [nucl-th]
arXiv 2019
-
[11]
M. Rybczy´ nski and W. Broniowski, Phys. Rev. C100, 064912 (2019). arXiv:1910.09489 [hep-ph]
arXiv 2019
-
[12]
N. Summerfield, B. N. Lu, C. Plumberg, D. Lee, J. Noronha-Hostler and A. Timmins, Phys. Rev. C104, L041901 (2021). arXiv:2103.03345 [nucl-th]
arXiv 2021
- [13]
-
[14]
C. Ding, L. G. Pang, S. Zhang and Y. G. Ma, Chin. Phys. C47, 024105 (2023)
2023
-
[15]
Y. Wang, S. Zhao, B. Cao, H. j. Xu and H. Song, Phys. Rev. C109, L051904 (2024). arXiv:2401.15723 [nucl-th]
arXiv 2024
- [16]
- [17]
-
[18]
H. Mehrabpour and A. Saha, Eur. Phys. J. C85, 1284 (2025) arXiv:2501.14243 [nucl-th]
arXiv 2025
-
[19]
Menon Kavumpadikkal Radhakrishnan, S
A. Menon Kavumpadikkal Radhakrishnan, S. Prasad, N. Mallick, R. Sahoo and G. G. Barnaf¨ oldi, Phys. Lett. B870, 139941 (2025). arXiv:2505.22367 [hep-ph]
arXiv 2025
- [20]
-
[21]
L. Constantin, N. G¨ otz, C. B. Rosenkvist and H. Elfner, Phys. Rev. C113, 054901 (2026). arXiv:2509.05613 [nucl-th]
Pith/arXiv arXiv 2026
- [22]
-
[23]
S. Floerchinger, U. A. Wiedemann, A. Beraudo, L. Del Zanna, G. Inghirami and V. Rolando, Phys. Lett. B735, 305 (2014). arXiv:1312.5482 [hep-ph]
Pith/arXiv arXiv 2014
-
[24]
S. Floerchinger, E. Grossi and J. Lion, Phys. Rev. C100, 014905 (2019). arXiv:1811.01870 [nucl-th]
Pith/arXiv arXiv 2019
-
[25]
N. Borghini, M. Borrell, N. Feld, H. Roch, S. Schlichting and C. Werthmann, Phys. Rev. C107, 034905 (2023). arXiv:2209.01176 [hep-ph]
arXiv 2023
-
[26]
G. Giacalone, B. Bally, G. Nijs, S. Shen, T. Duguet, J. P. Ebran, S. Elhatisari, M. Frosini, T. A. L¨ ahde and D. Lee,et al.Phys. Rev. Lett.135, 012302 (2025). arXiv:2402.05995 [nucl-th]
arXiv 2025
-
[27]
O. Garcia-Montero, H. Elfner and S. Schlichting, Phys. Rev. C109, 044916 (2024). arXiv:2308.11713 [hep-ph]
arXiv 2024
-
[28]
O. Garcia-Montero, S. Schlichting and J. Zhu, Phys. Rev. D111, 076029 (2025). arXiv:2501.14872 [nucl-th]
arXiv 2025
-
[29]
B. Schenke, S. Jeon and C. Gale, Phys. Rev. C82, 014903 (2010). arXiv:1004.1408 [hep-ph]
Pith/arXiv arXiv 2010
-
[30]
B. Schenke, S. Jeon and C. Gale, Phys. Rev. Lett.106, 042301 (2011). arXiv:1009.3244 [hep-ph]
Pith/arXiv arXiv 2011
-
[31]
J. F. Paquet, C. Shen, G. S. Denicol, M. Luzum, B. Schenke, S. Jeon and C. Gale, Phys. Rev. C93, 044906 (2016). arXiv:1509.06738 [hep-ph]
Pith/arXiv arXiv 2016
-
[32]
G. S. Denicol, T. Kodama, T. Koide and P. Mota, Phys. Rev. C80, 064901 (2009). arXiv:0903.3595 [hep-ph]
Pith/arXiv arXiv 2009
-
[33]
C. Shen, Z. Qiu, H. Song, J. Bernhard, S. Bass and U. Heinz, Comput. Phys. Commun.199, 61 (2016). arXiv:1409.8164 [nucl-th]
Pith/arXiv arXiv 2016
-
[34]
H. Roch and R. Krupczak,Hendrik1704/CRONOS:v1.0.0 [software], Zenodo (2025), doi:10.5281/zenodo.17503591
- [35]
-
[36]
Belyaevet al.[CMS], arXiv:2606.02285 [nucl-ex]
A. Belyaevet al.[CMS], arXiv:2606.02285 [nucl-ex]
-
[37]
G. Giacalone, A. Mazeliauskas and S. Schlichting, Phys. Rev. Lett.123, 262301 (2019). arXiv:1908.02866 [hep-ph]
arXiv 2019
- [38]
-
[39]
C. Loizides, J. Nagle and P. Steinberg, SoftwareX1-2, 13 (2015). arXiv:1408.2549 [nucl-ex]
Pith/arXiv arXiv 2015
-
[40]
R. Krupczak, N. Borghini and H. Roch, Eur. Phys. J. C 85, 1232 (2025). arXiv:2508.05336 [nucl-th]
arXiv 2025
-
[41]
C. Shen and S. Alzhrani, Phys. Rev. C102, 014909 (2020). arXiv:2003.05852 [nucl-th]
arXiv 2020
-
[42]
N. Borghini, H. Roch and A. Sch¨ utte, Eur. Phys. J. C 85, 12 (2025). arXiv:2402.07888 [nucl-th]
arXiv 2025
-
[43]
H. Niemi, K. J. Eskola and R. Paatelainen, Phys. Rev. C93, 024907(2016). arXiv:1505.02677 [hep-ph]
Pith/arXiv arXiv 2016
-
[44]
J. Noronha-Hostler, L. Yan, F. G. Gardim and J. Y. Olli- trault, Phys. Rev. C93, 014909 (2016). arXiv:1511.03896 [nucl-th]
Pith/arXiv arXiv 2016
-
[45]
N. Borghini, S. Feld and N. Kersting, Eur. Phys. J. C 78, 832 (2018). arXiv:1804.05729 [nucl-th]
Pith/arXiv arXiv 2018
- [46]
-
[47]
R. Franco and M. Luzum, Phys. Lett. B806, 135518 (2020). arXiv:1910.14598 [nucl-th]
arXiv 2020
-
[48]
Khachatryanet al.[CMS Collaboration], Phys
V. Khachatryanet al.[CMS Collaboration], Phys. Rev. C92, 034911 (2015). arXiv:1503.01692 [nucl-ex]
Pith/arXiv arXiv 2015
discussion (0)
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