Pith. sign in

REVIEW 3 major objections 4 minor 92 references

This paper claims that the longitudinal spin polarization of Λ baryons in a perturbed Gubser flow is not fixed by thermal vorticity alone: the thermal shear contribution changes sign and can fully or partially cancel it, depending on the fo

Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →

Challenge this review Re-run · record.json Download PDF Read on arXiv ↗

In an anisotropic Gubser flow, the longitudinal spin polarization's sign depends on which shear formulation is used, and two popular formulations show exact or near-exact cancellation between vorticity and shear contributions at leading order.

T0 review reviewed 2026-08-05 challenge →

load-bearing objection First analytic spin-polarization derivation from a real hydro solution, with a plausible suppression mechanism; but the 'exact' SBR cancellation is only exact within a truncated formula whose omitted terms are never quantified. the 3 major comments →

arxiv 2608.03945 v1 pith:XHSBLXSN submitted 2026-08-04 nucl-th hep-ph

Local Spin Polarization in Anisotropic Gubser Flow: Suppression Mechanism and Formulation Dependence

Kenji Fukushima , Shi Pu , Dong-Lin Wang This is my paper
classification nucl-th hep-ph PACS 25.75.-q25.75.Ld
keywords local spin polarizationthermal vorticitythermal shearGubser flowheavy-ion collisionssign puzzleCooper-Frye formulaspin hydrodynamics
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved

The pith

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

The reading

Using an analytically solvable, anisotropic version of Gubser flow to model the expanding quark–gluon plasma, the paper derives closed-form expressions for the longitudinal spin polarization of Λ baryons as a function of azimuthal angle and transverse momentum. It shows that in all three formulations considered, thermal vorticity alone gives a sign opposite to the measured one, while thermal shear can restore the observed sign. The result depends sharply on the choice of reference vector in the shear term: the surface-normal formulation produces an exact leading-order cancellation, making the total polarization zero, while the lab-time formulation cancels all acceleration effects and leaves a smaller, potentially correct-sign remainder. The paper thereby establishes that the longitudinal spin polarization is controlled by non-acceleration terms, not by vorticity and shear separately.

Core claim

On its own terms, the paper claims that in the large-system-size limit of a perturbed Gubser flow with elliptic (l = 2) and triangular (l = 3) deformations, the longitudinal spin polarization can be computed analytically and exhibits a formulation-dependent cancellation pattern. For the formulation that chooses the reference unit vector as the normal to the isothermal freeze-out surface (SBR), the thermal-shear contribution is exactly minus the thermal-vorticity contribution at leading order, S_z^SBR = 0 (Eq. 62). For the formulation using the lab-frame time direction (BBPIK), the acceleration parts of the vorticity and shear tensors cancel exactly, and the surviving polarization comes from

What carries the argument

The carrying element is the perturbed Gubser solution: a conformal hydrodynamic background with longitudinal and transverse expansion deformed by modes X^(l) ∝ P_l^l(cos θ) cos(lφ) for l = 2, 3, with the leading large-size asymptotics χ^(l) ≈ 3/2 and σ^(l) ≈ 1. Combined with the modified Cooper–Frye formula, the relevant objects are the thermal vorticity tensor and thermal shear tensor built from β^μ = u^μ/T, and the reference vector n^μ that differs across formulations. The decisive mechanical identity is that in the BBPIK formulation the acceleration terms ∂_t u_x and ∂_t u_y cancel between vorticity and shear contributions independent of the velocity profile, leaving only non-acceleration

Load-bearing premise

The load-bearing assumption is that the large-size limit τ_f/L ≪ 1 holds uniformly on the freeze-out surface, so all analytic formulas follow from the leading-order asymptotics χ ≈ 3/2, σ ≈ 1 and all O(τ_f/L) corrections are dropped; in addition, the SBR calculation uses a simplified isothermal-surface version of the formulation, omitting terms the full SBR formula would contribute.

What would settle it

Compute the next-to-leading order in τ_f/L for the SBR polarization in this same flow: if the subleading correction to S_vort + S_shear is not small compared with the leading terms, the exact cancellation is an artifact of truncation. A second, more direct check: evaluate S_z^SBR with the full SBR formula of its defining paper (without omitting the 'unphysical' pieces) on the same isothermal freeze-out surface; a nonzero result would falsify the claim that the simplified formulas capture the cancellation.

Watch this falsifier. Get emailed when new claim-graph text bears on it.

If this is right

  • If the SBR formulation is physical, the leading-order longitudinal polarization in this flow is exactly zero once the full freeze-out surface is integrated; nonzero values require subleading order or a non-isothermal surface.
  • In the BBPIK formulation the acceleration parts drop out identically, so the polarization is a pure non-acceleration effect and has the observed sin(2φ_p) sign for p_T below about 3 GeV.
  • The FLPSY formulation recovers the experimental sign only at small transverse momentum and only when the light quark mass is used; with the Λ mass it fails in this model.
  • Vorticity-only calculations cannot reproduce the local polarization sign in this model; shear is necessary in every formulation considered.
  • Initial eccentricities are the source: setting both ε_2 and ε_3 to zero makes the longitudinal polarization vanish, so the signal is a response to anisotropic flow.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • One testable extension: feed the same perturbed Gubser solution into a viscous hydrodynamic code and check whether the exact SBR cancellation survives beyond ideal hydrodynamics; if it does, current numerical disagreement may come from freeze-out prescription, not from shear physics.
  • The acceleration-cancellation identity in BBPIK is independent of the velocity profile, so it likely generalizes to realistic velocity fields; computing the residual non-acceleration term in a realistic simulation would show whether the sign puzzle is resolved by shear or by non-acceleration gradients.
  • The exact SBR zero suggests a possible degeneracy: if the surface-normal formulation is right, local spin polarization would be exceptionally sensitive to subleading and dissipative corrections, making it a useful probe of freeze-out dynamics rather than of equilibrium vorticity.
  • Because the model gives simple analytic ratios S_vort/S_shear independent of T0 and L, the p_T dependence of the measured polarization can be used to discriminate the formulations without tuning initial conditions.
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

3 major / 4 minor

Summary. This paper presents an analytic study of the longitudinal spin polarization of Λ hyperons in a conformal, perturbed Gubser flow with elliptic (l=m=2) and triangular (l=m=3) deformations. Three formulations of the shear-induced polarization are compared: FLPSY (n^μ=u^μ), BBPIK (n^μ=δ^μ_0 with kinetic replacements), and SBR (n^μ normal to the freeze-out surface). In the large-L limit, explicit leading-order formulas are derived for the Fourier coefficients of S_z(p) (Eqs. 52-62). The results show that thermal vorticity alone has the sign opposite to experiment; thermal shear compensates. FLPSY gives the desired sign only at low p_T for m=300 MeV; BBPIK gives the desired sign up to moderately large p_T; SBR gives an exact cancellation at leading order. A general acceleration-term cancellation between vorticity and shear is identified in BBPIK and SBR. The rotating Hubble flow is also analyzed as a global-polarization benchmark.

Significance. If the results hold, this is one of the first analytic derivations of local spin polarization directly from a hydrodynamic solution, rather than from a blast-wave parametrization. The explicit formulas reveal parameter dependences (e.g., independence of the ratio S_vort/S_shear from T0hat and L) that provide checkable predictions for numerical simulations. The general cancellation of acceleration terms in BBPIK is demonstrated algebraically and does not depend on the flow profile. The paper is candid about the leading-order nature of the Gubser analysis and does not attempt to fit data. The main caveat is that the SBR exact-zero result is computed with a simplified version of the SBR formula; this limits the strength of the headline conclusion but does not affect the BBPIK results.

major comments (3)
  1. [Sec. III, Eq. (37)] The central SBR result, Eq. (62), is computed from Eqs. (36)-(37), which the authors themselves describe as less general than the complete SBR formulation of Ref. [72]. The omitted terms are called 'unphysical,' but no demonstration is given that they vanish on the isothermal freeze-out surface (33) or that they are numerically negligible. Since the abstract's headline is the 'exact cancellation' between S_z^SBR_vort and S_z^SBR_shear, this is not a side remark: if the omitted terms contribute at the same order, Eq. (62) could be an artifact of the truncation. Please either evaluate the complete SBR expression for this flow or provide a quantitative bound/argument showing that the additional terms cannot affect the leading-order cancellation.
  2. [Sec. II.D, Eq. (23)] All analytic formulas (52)-(62) are leading-order in the large-system-size expansion and inherit the asymptotic solution χ^(l)≃3/2, σ^(l)≃1 of Eqs. (20)-(21). This particular solution discards a homogeneous mode of Eq. (20) that behaves as e^{2ρ/3} as ρ→-∞; the manuscript does not state the boundary/regularity condition that selects χ=3/2, nor does it estimate the first subleading corrections under the consistency condition (35). Because the SBR cancellation is presented as 'exact' (even if at leading order), an estimate of corrections of order (τ_f/L) would clarify whether the vanishing of S_z^SBR is robust or an artifact of the truncation. A brief discussion of this point is needed.
  3. [Sec. V.C, Eqs. (66)-(67)] The text argues that the SBR formulation reduces to the BBPIK-like acceleration cancellation by approximating n^μ≈δ_0^μ at mid-rapidity. However, the exact SBR cancellation (62) is then presented as a separate result, and the text later states that the cancellation is 'probably an accidental cancellation.' The logical relation between the approximate n≈δ0 argument and the exact Eq. (62) is not fully spelled out. Please clarify whether the exact zero is a consequence of the mid-rapidity approximation or of the full hypersurface integration (the latter seems to be the case from the final paragraph of Sec. V.C). This distinction is important for readers assessing the generality of the proposed cancellation mechanism.
minor comments (4)
  1. [Various] Typographical errors: abstract 'anaytical'; Sec. I 'adpot'; Sec. VI 'aliged'.
  2. [Sec. V.B, Fig. 5] The independence of S_vort/S_shear from T0hat and L is a nontrivial check; it would be helpful to state this explicitly in the figure caption, since it is not obvious from the plotted curves.
  3. [Sec. III, Eq. (40)] The shorthand n_F(1−n_F)≃n_F≃e^{−β·p} is slightly imprecise; for the Boltzmann approximation, n_F(1−n_F)≃e^{−β·p} is the needed statement.
  4. [References] Ref. [72] is an arXiv preprint; please add journal publication information if it has appeared by the time of publication.

Circularity Check

0 steps flagged

No significant circularity: the derivation is a forward calculation from an external hydrodynamic solution and external spin formulas; the SBR cancellation is conditional on an unquantified truncation, which is a limitation rather than a circular step.

full rationale

The paper's inputs are the perturbed Gubser solution from Hatta et al. (Ref. [78]) and the three spin-polarization formulas from external works (FLPSY, BBPIK, SBR). The coefficients C(p) and D(p) are not fitted to reproduce the polarization sign; they are obtained from the freeze-out integrals and the stated parameters. The SBR cancellation in Eq. (62) is derived by explicit leading-order integration of Eqs. (36)-(37), not by assuming the target result. The paper explicitly states in Sec. III that it omits the more general 'unphysical contributions' of Ref. [72] and uses the simplified formulas, and in Sec. V.C it calls the exact vanishing 'probably an accidental cancellation' — this is an honest, clearly stated approximation that limits robustness but is not circular. Self-citations (Refs. [38,48,59,64,79]) are present but none is load-bearing: the anisotropic Gubser solution is attributed to Refs. [77,78] and the spin formulas to Refs. [60-63,72]. No fitted parameter is renamed a prediction, no uniqueness theorem is imported, and no definition is equivalent to the conclusion. The central claim is conditional on the large-system-size truncation and the simplified SBR formula, but the derivation itself is self-contained with respect to those stated assumptions.

Axiom & Free-Parameter Ledger

6 free parameters · 8 axioms · 0 invented entities

The model has six illustrative parameters, none fitted to the polarization data, and eight stated assumptions inherited from the referenced hydrodynamics and spin literature. No invented entities. The paper is transparent about most assumptions, including conditions (22), (30), (35), and the truncation of the full SBR formula of Ref [72].

free parameters (6)
  • T0hat = 3 (used in figures)
    Dimensionless initial temperature of the conformal solution (Eqs. 12, 16). Sets overall normalization; the ratios S_vort/S_shear are independent of it. Chosen for illustration, not fitted to data.
  • L = 10 fm
    Initial transverse size scale of the Gubser flow. Not fitted; the paper notes the p_T ratios are L-independent.
  • T_f = 150 MeV
    Freeze-out temperature defining the isothermal hypersurface (Eq. 33). Chosen, not fitted.
  • eps_2 = 0.1
    Elliptic deformation amplitude. Assumed small with hierarchy eps3 << eps2 << 1 (Eq. 30); analytic results are leading order in eps2,3.
  • eps_3 = 0.01
    Triangular deformation amplitude, subdominant in the hierarchy (Eq. 30).
  • m (particle mass) = 1116 MeV or 300 MeV
    Lambda hyperon vs s-quark mass (Eq. 43). The FLPSY sign conclusion depends critically on this choice.
axioms (8)
  • domain assumption Conformal equation of state e = 3p = lambda T^4 (Eq. 3)
    Closes the ideal hydrodynamics system; standard in Gubser flow setups, stated in Sec. II.
  • domain assumption Ideal, uncharged fluid (Eqs. 1-2)
    Viscosity and baryon charge are neglected; the paper states generalization is possible but not performed.
  • domain assumption Perturbed Gubser flow (27)-(28) is the correct leading-order hydro solution
    Taken from Refs [77,78,79]; only linear order in eps2,3 is kept.
  • domain assumption Leading-order large-size asymptotics chi^(l) ~ 3/2 and sigma^(l) ~ 1 (Eq. 23)
    Used to obtain all analytic spin formulas; subleading tau/L corrections are ignored, with validity resting on Eq. (35).
  • domain assumption Freeze-out on isothermal hypersurface T = T_f (Eq. 33) with tau_f << L
    Defines Sigma_f; the SBR 'exact cancellation' result is for this surface.
  • domain assumption Modified Cooper-Frye formulas (36)-(37) with the three unit-vector choices
    Borrowed from Refs [60,61,62,63,72]; the SBR usage omits pieces the authors call unphysical (Ref [72]).
  • domain assumption l=2 mode dominance via the zero-counting argument for P_l^2
    Justifies neglecting l>2 modes in Eq. (19); physically motivated but heuristic (Sec. II.D).
  • ad hoc to paper Mid-rapidity approximation n^mu ~ delta_0^mu for SBR (Eqs. 65-67)
    Used only in Sec. V.C to explain the SBR cancellation mechanism; justified by exponential suppression but approximate.

reviewed 2026-08-05 · how reviews work

0 comments
Cite this review

Pith. "Pith review of Local Spin Polarization in Anisotropic Gubser Flow: Suppression Mechanism and Formulation Dependence." pith.science (2026). https://pith.science/paper/XHSBLXSN

@misc{pith2026260803945,
  author       = {Pith},
  title        = {Pith review of: Local Spin Polarization in Anisotropic Gubser Flow: Suppression Mechanism and Formulation Dependence},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/XHSBLXSN}},
  note         = {Machine review of arXiv:2608.03945}
}
Share X Bluesky LinkedIn Reddit HN
read the original abstract

We analytically study the longitudinal spin polarization in relativistic heavy-ion collisions using a perturbed Gubser flow solution. In the large-system-size limit, we derive analytical expression of the local spin polarization along the beam direction. In our treatment, the contributions from thermal vorticity and thermal shear are of comparable magnitudes. The thermal vorticity yields the polarization with a sign opposite to that observed experimentally, while the thermal shear counteracts this effect, helping recover the desired sign. We find that the choice of the reference unit vector aligned with the fluid velocity gives the experimentally observed sign only at low transverse momenta, whereas another formulation with the unit vector fixed along the laboratory time direction yields the desired sign for a wide range of transverse momenta. Notably, a recent formulation with the unit vector normal to the freeze-out hypersurface exhibits an exact cancellation between contributions from thermal vorticity and thermal shear at leading order in the large-system-size limit. We identify a general cancellation pattern with acceleration dominance, which is manifest particularly in the latter two formulations. Thus, the total polarization originates from non-acceleration effects, which need not be substantial even when the elliptic flow is finite, as clearly demonstrated in our analytical results. For comparison, we also discuss the spin polarization in the Hubble flow with rotation.

Figures

Figures reproduced from arXiv: 2608.03945 by Dong-Lin Wang, Kenji Fukushima, Shi Pu.

Figure 1
Figure 1. Figure 1: FIG. 1. Schematic illustration of the rotating Hubble flow [PITH_FULL_IMAGE:figures/full_fig_p002_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2. Transverse distribution of ( [PITH_FULL_IMAGE:figures/full_fig_p005_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: FIG. 3. Longitudinal spin polarization with [PITH_FULL_IMAGE:figures/full_fig_p008_3.png] view at source ↗
Figure 4
Figure 4. Figure 4: FIG. 4. Longitudinal spin polarization with [PITH_FULL_IMAGE:figures/full_fig_p009_4.png] view at source ↗
Figure 5
Figure 5. Figure 5: FIG. 5 [PITH_FULL_IMAGE:figures/full_fig_p010_5.png] view at source ↗

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Reference graph

Works this paper leans on

92 extracted references · 7 canonical work pages · 7 internal anchors

  1. [1]

    FLPSY formulation [60, 62]:n µ is identified with the fluid velocityu µ

  2. [2]

    In addition, as proposed in Ref

    BBPIK formulation [61]:n µ is set to ben µ =δ µ 0 in (t, x, y, z) coordinates. In addition, as proposed in Ref. [63], explicitT-gradients are removed by the replacements ofϖ µν →ϖ K µν andξ µν →ξ K µν, where ϖK µν =− 1 2 β(∂µuν −∂ νuµ),(41) ξK µν = 1 2 β(∂µuν +∂ νuµ).(42)

  3. [3]

    If Σ f is isothermal, i.e., with constant temper- ature,n µ =−∂ µT / p |∂νT ∂νT|

    SBR formulation [72]:n µ is the normal vector to Σf . If Σ f is isothermal, i.e., with constant temper- ature,n µ =−∂ µT / p |∂νT ∂νT|. Then,T-gradient terms cancel out automatically inS µ(p), though eachS µ ϖ,ξ(p) receivesT-gradient contributions. It should be noted that the SBR formulation is applicable to an arbitrary Σ f , and its complete form in Ref...

  4. [4]

    Liang and X.-N

    Z.-T. Liang and X.-N. Wang, Phys. Rev. Lett.94, 102301 (2005), [Erratum: Phys.Rev.Lett. 96, 039901 (2006)], arXiv:nucl-th/0410079

    Pith/arXiv arXiv 2005

  5. [5]

    Gao, S.-W

    J.-H. Gao, S.-W. Chen, W.-t. Deng, Z.-T. Liang, Q. Wang, and X.-N. Wang, Phys. Rev. C77, 044902 (2008), arXiv:0710.2943 [nucl-th]

    Pith/arXiv arXiv 2008

  6. [6]

    S. A. Voloshin, arXiv:nucl-th/0410089 (2004)

    Pith/arXiv arXiv 2004

  7. [7]

    Adamczyket al.(STAR), Nature548, 62 (2017), arXiv:1701.06657 [nucl-ex]

    L. Adamczyket al.(STAR), Nature548, 62 (2017), arXiv:1701.06657 [nucl-ex]

    Pith/arXiv arXiv 2017

  8. [8]

    Acharyaet al.(ALICE), Phys

    S. Acharyaet al.(ALICE), Phys. Rev. C101, 044611 (2020), [Erratum: Phys.Rev.C 105, 029902 (2022)], arXiv:1909.01281 [nucl-ex]

    Pith/arXiv arXiv 2020

  9. [9]

    Abou Yassineet al.(HADES), Phys

    R. Abou Yassineet al.(HADES), Phys. Lett. B835, 137506 (2022), arXiv:2207.05160 [nucl-ex]

    Pith/arXiv arXiv 2022

  10. [10]

    Karpenko and F

    I. Karpenko and F. Becattini, Eur. Phys. J. C77, 213 (2017), arXiv:1610.04717 [nucl-th]

    Pith/arXiv arXiv 2017

  11. [11]

    Li, L.-G

    H. Li, L.-G. Pang, Q. Wang, and X.-L. Xia, Phys. Rev. C96, 054908 (2017), arXiv:1704.01507 [nucl-th]

    Pith/arXiv arXiv 2017

  12. [12]

    Sun and C

    Y. Sun and C. M. Ko, Phys. Rev. C96, 024906 (2017), arXiv:1706.09467 [nucl-th]

    Pith/arXiv arXiv 2017

  13. [13]

    Wei, W.-T

    D.-X. Wei, W.-T. Deng, and X.-G. Huang, Phys. Rev. C 99, 014905 (2019), arXiv:1810.00151 [nucl-th]

    Pith/arXiv arXiv 2019

  14. [14]

    Vitiuk, L

    O. Vitiuk, L. V. Bravina, and E. E. Zabrodin, Phys. Lett. B803, 135298 (2020), arXiv:1910.06292 [hep-ph]

    Pith/arXiv arXiv 2020

  15. [15]

    B. Fu, K. Xu, X.-G. Huang, and H. Song, Phys. Rev. C 103, 024903 (2021), arXiv:2011.03740 [nucl-th]

    Pith/arXiv arXiv 2021

  16. [16]

    A. Lei, D. Wang, D.-M. Zhou, B.-H. Sa, and L. P. Cser- nai, Phys. Rev. C104, 054903 (2021), arXiv:2110.13485 [nucl-th]

    Pith/arXiv arXiv 2021

  17. [17]

    S. Ryu, V. Jupic, and C. Shen, Phys. Rev. C104, 054908 (2021), arXiv:2106.08125 [nucl-th]

    Pith/arXiv arXiv 2021

  18. [18]

    X.-Y. Wu, C. Yi, G.-Y. Qin, and S. Pu, Phys. Rev. C 105, 064909 (2022), arXiv:2204.02218 [hep-ph]

    Pith/arXiv arXiv 2022

  19. [19]

    Becattini, V

    F. Becattini, V. Chandra, L. Del Zanna, and E. Grossi, Annals Phys.338, 32 (2013), arXiv:1303.3431 [nucl-th]

    Pith/arXiv arXiv 2013

  20. [20]

    Fang, L.-g

    R.-h. Fang, L.-g. Pang, Q. Wang, and X.-n. Wang, Phys. Rev. C94, 024904 (2016), arXiv:1604.04036 [nucl-th]

    Pith/arXiv arXiv 2016

  21. [21]

    Adamet al.(STAR), Phys

    J. Adamet al.(STAR), Phys. Rev. Lett.123, 132301 (2019), arXiv:1905.11917 [nucl-ex]

    arXiv 2019

  22. [22]

    Acharyaet al.(ALICE), Phys

    S. Acharyaet al.(ALICE), Phys. Rev. Lett.128, 172005 (2022), arXiv:2107.11183 [nucl-ex]

    Pith/arXiv arXiv 2022

  23. [23]

    Abdulhamidet al.(STAR), Phys

    M. Abdulhamidet al.(STAR), Phys. Rev. Lett.131, 202301 (2023), arXiv:2303.09074 [nucl-ex]

    arXiv 2023

  24. [24]

    Hayrapetyanet al.(CMS), Phys

    A. Hayrapetyanet al.(CMS), Phys. Rev. Lett.135, 132301 (2025), arXiv:2502.07898 [nucl-ex]

    arXiv 2025

  25. [25]

    Becattini and I

    F. Becattini and I. Karpenko, Phys. Rev. Lett.120, 012302 (2018), arXiv:1707.07984 [nucl-th]

    Pith/arXiv arXiv 2018

  26. [26]

    X.-L. Xia, H. Li, Z.-B. Tang, and Q. Wang, Phys. Rev. C98, 024905 (2018), arXiv:1803.00867 [nucl-th]

    Pith/arXiv arXiv 2018

  27. [27]

    Florkowski, A

    W. Florkowski, A. Kumar, R. Ryblewski, and A. Mazeliauskas, Phys. Rev. C100, 054907 (2019), arXiv:1904.00002 [nucl-th]

    Pith/arXiv arXiv 2019

  28. [28]

    Wu, L.-G

    H.-Z. Wu, L.-G. Pang, X.-G. Huang, and Q. Wang, Phys. Rev. Research.1, 033058 (2019), arXiv:1906.09385 [nucl- th]

    Pith/arXiv arXiv 2019

  29. [29]

    X.-L. Xia, H. Li, X.-G. Huang, and H. Z. Huang, Phys. Rev. C100, 014913 (2019), arXiv:1905.03120 [nucl-th]

    Pith/arXiv arXiv 2019

  30. [30]

    Becattini, G

    F. Becattini, G. Cao, and E. Speranza, Eur. Phys. J. C 79, 741 (2019), arXiv:1905.03123 [nucl-th]

    Pith/arXiv arXiv 2019

  31. [31]

    Gao, Z.-T

    J.-H. Gao, Z.-T. Liang, S. Pu, Q. Wang, and X.-N. Wang, Phys. Rev. Lett.109, 232301 (2012), arXiv:1203.0725 [hep-ph]

    Pith/arXiv arXiv 2012

  32. [32]

    J.-W. Chen, S. Pu, Q. Wang, and X.-N. Wang, Phys. Rev. Lett.110, 262301 (2013), arXiv:1210.8312 [hep-th]

    Pith/arXiv arXiv 2013

  33. [33]

    Hidaka, S

    Y. Hidaka, S. Pu, and D.-L. Yang, Phys. Rev. D95, 091901 (2017), arXiv:1612.04630 [hep-th]

    Pith/arXiv arXiv 2017

  34. [34]

    Hidaka, S

    Y. Hidaka, S. Pu, and D.-L. Yang, Phys. Rev. D97, 016004 (2018), arXiv:1710.00278 [hep-th]

    Pith/arXiv arXiv 2018

  35. [35]

    Relativistic Quantum Kinetic Theory for Massive Fermions and Spin Effects

    J.-H. Gao and Z.-T. Liang, Phys. Rev. D100, 056021 (2019), arXiv:1902.06510 [hep-ph]. 12

    work page internal anchor Pith review Pith/arXiv arXiv 2019

  36. [36]

    Weickgenannt, X.-L

    N. Weickgenannt, X.-L. Sheng, E. Speranza, Q. Wang, and D. H. Rischke, Phys. Rev. D100, 056018 (2019), arXiv:1902.06513 [hep-ph]

    Pith/arXiv arXiv 2019

  37. [37]

    Y.-C. Liu, K. Mameda, and X.-G. Huang, Chin. Phys. C44, 094101 (2020), [Erratum: Chin.Phys.C 45, 089001 (2021)], arXiv:2002.03753 [hep-ph]

    Pith/arXiv arXiv 2020

  38. [38]

    Weickgenannt, E

    N. Weickgenannt, E. Speranza, X.-l. Sheng, Q. Wang, and D. H. Rischke, Phys. Rev. Lett.127, 052301 (2021), arXiv:2005.01506 [hep-ph]

    Pith/arXiv arXiv 2021

  39. [39]

    Weickgenannt, E

    N. Weickgenannt, E. Speranza, X.-l. Sheng, Q. Wang, and D. H. Rischke, Phys. Rev. D104, 016022 (2021), arXiv:2103.04896 [nucl-th]

    Pith/arXiv arXiv 2021

  40. [40]

    Sheng, N

    X.-L. Sheng, N. Weickgenannt, E. Speranza, D. H. Rischke, and Q. Wang, Phys. Rev. D104, 016029 (2021), arXiv:2103.10636 [nucl-th]

    Pith/arXiv arXiv 2021

  41. [41]

    Hidaka, S

    Y. Hidaka, S. Pu, Q. Wang, and D.-L. Yang, Prog. Part. Nucl. Phys.127, 103989 (2022), arXiv:2201.07644 [hep- ph]

    Pith/arXiv arXiv 2022

  42. [42]

    S. Fang, S. Pu, and D.-L. Yang, Phys. Rev. D106, 016002 (2022), arXiv:2204.11519 [hep-ph]

    Pith/arXiv arXiv 2022

  43. [43]

    Spin Boltzmann equation for non-relativistic spin-1/2 fermions

    W.-B. Dong, Y.-L. Yin, and Q. Wang, Phys. Rev. C106, 054909 (2022), arXiv:2209.12402 [nucl-th]

    work page internal anchor Pith review Pith/arXiv arXiv 2022

  44. [44]

    S. Fang, S. Pu, and D.-L. Yang, Phys. Rev. D109, 034034 (2024), arXiv:2311.15197 [hep-ph]

    Pith/arXiv arXiv 2024

  45. [45]

    Collisional corrections to spin polarization from quantum kinetic theory using Chapman-Enskog expansion

    S. Fang and S. Pu, Phys. Rev. D111, 034015 (2025), arXiv:2408.09877 [hep-ph]

    work page internal anchor Pith review Pith/arXiv arXiv 2025

  46. [46]

    Montenegro, L

    D. Montenegro, L. Tinti, and G. Torrieri, Phys. Rev. D 96, 076016 (2017), arXiv:1703.03079 [hep-th]

    Pith/arXiv arXiv 2017

  47. [47]

    Florkowski, B

    W. Florkowski, B. Friman, A. Jaiswal, and E. Speranza, Phys. Rev. C97, 041901 (2018), arXiv:1705.00587 [nucl- th]

    Pith/arXiv arXiv 2018

  48. [48]

    Becattini, W

    F. Becattini, W. Florkowski, and E. Speranza, Phys. Lett. B789, 419 (2019), arXiv:1807.10994 [hep-th]

    Pith/arXiv arXiv 2019

  49. [49]

    Florkowski, A

    W. Florkowski, A. Kumar, and R. Ryblewski, Prog. Part. Nucl. Phys.108, 103709 (2019), arXiv:1811.04409 [nucl- th]

    Pith/arXiv arXiv 2019

  50. [50]

    Hattori, M

    K. Hattori, M. Hongo, X.-G. Huang, M. Matsuo, and H. Taya, Phys. Lett. B795, 100 (2019), arXiv:1901.06615 [hep-th]

    Pith/arXiv arXiv 2019

  51. [51]

    Fukushima and S

    K. Fukushima and S. Pu, Phys. Lett. B817, 136346 (2021), arXiv:2010.01608 [hep-th]

    Pith/arXiv arXiv 2021

  52. [52]

    S. Li, M. A. Stephanov, and H.-U. Yee, Phys. Rev. Lett. 127, 082302 (2021), arXiv:2011.12318 [hep-th]

    Pith/arXiv arXiv 2021

  53. [53]

    Hongo, X.-G

    M. Hongo, X.-G. Huang, M. Kaminski, M. Stephanov, and H.-U. Yee, JHEP11, 150 (2021), arXiv:2107.14231 [hep-th]

    Pith/arXiv arXiv 2021

  54. [54]

    D. She, A. Huang, D. Hou, and J. Liao, Sci. Bull.67, 2265 (2022), arXiv:2105.04060 [nucl-th]

    Pith/arXiv arXiv 2022

  55. [55]

    D.-L. Wang, S. Fang, and S. Pu, Phys. Rev. D104, 114043 (2021), arXiv:2107.11726 [nucl-th]

    Pith/arXiv arXiv 2021

  56. [56]

    Weickgenannt, D

    N. Weickgenannt, D. Wagner, E. Speranza, and D. H. Rischke, Phys. Rev. D106, L091901 (2022), arXiv:2208.01955 [nucl-th]

    Pith/arXiv arXiv 2022

  57. [57]

    Weickgenannt, D

    N. Weickgenannt, D. Wagner, E. Speranza, and D. H. Rischke, Phys. Rev. D106, 096014 (2022), arXiv:2203.04766 [nucl-th]

    Pith/arXiv arXiv 2022

  58. [58]

    Z. Cao, K. Hattori, M. Hongo, X.-G. Huang, and H. Taya, PTEP2022, 071D01 (2022), arXiv:2205.08051 [hep-th]

    Pith/arXiv arXiv 2022

  59. [59]

    Bhadury, W

    S. Bhadury, W. Florkowski, A. Jaiswal, A. Kumar, and R. Ryblewski, Phys. Rev. Lett.129, 192301 (2022), arXiv:2204.01357 [nucl-th]

    Pith/arXiv arXiv 2022

  60. [60]

    Florkowski and M

    W. Florkowski and M. Hontarenko, Phys. Rev. Lett.134, 082302 (2025), arXiv:2405.03263 [hep-ph]

    Pith/arXiv arXiv 2025

  61. [61]

    Huang, Nucl

    X.-G. Huang, Nucl. Sci. Tech.36, 208 (2025), arXiv:2411.11753 [nucl-th]

    Pith/arXiv arXiv 2025

  62. [62]

    S. Fang, K. Fukushima, S. Pu, and D.-L. Wang, arXiv:2506.20698 [nucl-th] (2025)

    Pith/arXiv arXiv 2025

  63. [63]

    S. Y. F. Liu and Y. Yin, JHEP07, 188 (2021), arXiv:2103.09200 [hep-ph]

    Pith/arXiv arXiv 2021

  64. [64]

    Becattini, M

    F. Becattini, M. Buzzegoli, and A. Palermo, Phys. Lett. B820, 136519 (2021), arXiv:2103.10917 [nucl-th]

    Pith/arXiv arXiv 2021

  65. [65]

    B. Fu, S. Y. F. Liu, L. Pang, H. Song, and Y. Yin, Phys. Rev. Lett.127, 142301 (2021), arXiv:2103.10403 [hep- ph]

    Pith/arXiv arXiv 2021

  66. [66]

    Becattini, M

    F. Becattini, M. Buzzegoli, G. Inghirami, I. Karpenko, and A. Palermo, Phys. Rev. Lett.127, 272302 (2021), arXiv:2103.14621 [nucl-th]

    Pith/arXiv arXiv 2021

  67. [67]

    C. Yi, S. Pu, and D.-L. Yang, Phys. Rev. C104, 064901 (2021), arXiv:2106.00238 [hep-ph]

    Pith/arXiv arXiv 2021

  68. [68]

    Florkowski, A

    W. Florkowski, A. Kumar, A. Mazeliauskas, and R. Ryblewski, Phys. Rev. C105, 064901 (2022), arXiv:2112.02799 [hep-ph]

    Pith/arXiv arXiv 2022

  69. [69]

    Buzzegoli, F

    M. Buzzegoli, F. Becattini, G. Inghirami, I. Karpenko, and A. Palermo, Acta Phys. Polon. Supp.16, 1 (2023), arXiv:2208.04449 [nucl-th]

    Pith/arXiv arXiv 2023

  70. [70]

    Local equilibrium and Lambda polarization in high energy heavy ion collisions

    A. Palermo, F. Becattini, M. Buzzegoli, G. Inghirami, and I. Karpenko, EPJ Web Conf.276, 01026 (2023), arXiv:2208.09874 [nucl-th]

    work page internal anchor Pith review Pith/arXiv arXiv 2023

  71. [71]

    Palermo, E

    A. Palermo, E. Grossi, I. Karpenko, and F. Becattini, Eur. Phys. J. C84, 920 (2024), arXiv:2404.14295 [nucl- th]

    Pith/arXiv arXiv 2024

  72. [72]

    Spin polarization of $\Lambda$ hyperons along beam direction in p+Pb collisions at $\sqrt{s_{NN}}=8.16$ TeV using hydrodynamic approaches

    C. Yi, X.-Y. Wu, J. Zhu, S. Pu, and G.-Y. Qin, Phys. Rev. C111, 044901 (2025), arXiv:2408.04296 [hep-ph]

    work page internal anchor Pith review Pith/arXiv arXiv 2025

  73. [73]

    Becattini, M

    F. Becattini, M. Buzzegoli, T. Niida, S. Pu, A.-H. Tang, and Q. Wang, Int. J. Mod. Phys. E33, 2430006 (2024), arXiv:2402.04540 [nucl-th]

    Pith/arXiv arXiv 2024

  74. [74]

    Niida and S

    T. Niida and S. A. Voloshin, Int. J. Mod. Phys. E33, 2430010 (2024), arXiv:2404.11042 [nucl-ex]

    Pith/arXiv arXiv 2024

  75. [75]

    Sheng, F

    X.-L. Sheng, F. Becattini, and D. Roselli, arXiv:2509.14301 [nucl-th] (2025)

    Pith/arXiv arXiv 2025

  76. [76]

    Alzhrani, S

    S. Alzhrani, S. Ryu, and C. Shen, Phys. Rev. C106, 014905 (2022), arXiv:2203.15718 [nucl-th]

    Pith/arXiv arXiv 2022

  77. [77]

    A solvable model for spin polarizations with flow-momentum correspondence

    A. Arslan, W.-B. Dong, G.-L. Ma, S. Pu, and Q. Wang, Phys. Rev. C111, 044911 (2025), arXiv:2411.17285 [nucl-th]

    work page internal anchor Pith review Pith/arXiv arXiv 2025

  78. [78]

    Arslan, W.-B

    A. Arslan, W.-B. Dong, C. Gale, S. Jeon, Q. Wang, and X.-Y. Wu, arXiv:2509.00796 [nucl-th] (2025)

    arXiv 2025

  79. [79]

    S. S. Gubser, Phys. Rev. D82, 085027 (2010), arXiv:1006.0006 [hep-th]

    Pith/arXiv arXiv 2010

  80. [80]

    S. S. Gubser and A. Yarom, Nucl. Phys. B846, 469 (2011), arXiv:1012.1314 [hep-th]

    Pith/arXiv arXiv 2011

Showing first 80 references.

This paper was first reviewed by deepseek-v4-flash on August 5, 2026.