REVIEW 3 major objections 8 minor 68 references
In the weak-field limit after nuclear collisions, the glasma energy-momentum tensor settles into a universal late-time falloff independent of how nuclear color charges are modeled.
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 →
T0 review · grok-4.5
2026-07-31 00:19 UTC pith:QGQBF7XZ
load-bearing objection Solid analytic control of weak-field glasma EMT: universal late-time powers plus usable Meijer-G and series forms, limited mainly by the stated O(gA^{2}) truncation. the 3 major comments →
Analytic and Approximate Solutions to Color Glass Condensate in the Classical Weak-Field Limit
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
In the classical weak-field limit the large-time behavior of the glasma energy-momentum tensor is universal across models of the nuclear gluon correlator: energy density and transverse pressure scale as 1/\u03c4 and longitudinal pressure as 1/\u03c4\u00b3. For infinite nuclei in the McLerran-Venugopalan model the leading gradient terms of every component admit closed forms proportional to (m\u03c4)^{-n} times a linear combination of Meijer-G functions that approach constants; an improved Gaussian model with global color neutrality recovers the same leading powers and the MV shape in the ultraviolet limit.
What carries the argument
Two-point correlators of the classical gluon fields in the forward light cone, written as light-cone integrals over nuclear gluon two-point functions and reduced in the weak-field limit (leading non-abelian seed only, Wilson factor U=1) to single radial integrals that yield every component of the energy-momentum tensor; those integrals close to Meijer-G functions in the MV model.
Load-bearing premise
The calculation keeps only the leading non-abelian seed at the collision and sets the Wilson-line factor to one, which is controlled only when the product of coupling and charge density is small.
What would settle it
Run abelianized classical Yang-Mills evolution with smooth, weak, nearly constant color sources and check whether the measured ratios of longitudinal and transverse pressure to energy density, and the late-time 1/\u03c4 and 1/\u03c4\u00b3 falloffs, match the analytic Meijer-G or improved-Gaussian series.
If this is right
- Late-time energy density, transverse pressure and longitudinal pressure of the weak glasma are fixed by universal powers of proper time, independent of the nuclear gluon model.
- MV-model stress-tensor components for infinite nuclei are known in closed form as Meijer-G combinations and can be used as analytic benchmarks.
- The improved Gaussian model supplies UV-finite, IR-safer series that recover MV qualitatively when the UV scale is removed.
- Angular momentum per unit rapidity carried by the weak gluon field approaches a nonzero constant at large time.
- Abelianized glasma event generators can be validated against the predicted pressure-to-energy ratios and flow components for weakly varying sources.
Where Pith is reading between the lines
- The same light-cone correlator machinery could be reused to extract the momentum-broadening coefficient q-hat for a parton traversing the weak glasma without new field solutions.
- If non-abelian corrections only rescale the overall coefficients while leaving the 1/\u03c4 and 1/\u03c4\u00b3 powers intact, the universal late-time skeleton would survive into the full classical regime.
- Matching the analytic Si/\u03b5 and Tiz/\u03b5 ratios to dilute-source runs would give a clean pass/fail test for existing glasma codes before any hydro stage is attached.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript studies the classical gluon field produced in the collision of two boost-invariant color-charge sheets in the weak-field (linearized, O(gA²), U=1) limit. Starting from the resummed Bessel-function solutions in transverse momentum space (Eqs. 13–15), the authors derive coordinate-space two-point functions as light-cone circle integrals (Eqs. 22, 26, 27) over a general gluon correlator γ, and assemble the energy-momentum tensor in a gradient expansion of the charge variance μ(R). For the MV model with constant μ they obtain closed-form expressions for all EMT components as combinations of Meijer-G functions (Eqs. 74a–f) with constant asymptotic values, yielding ε, P_T ∼ 1/τ and P_L ∼ 1/τ³ (Eqs. 75–76). They argue the late-time powers are universal, i.e. independent of the correlator model, via binomial expansion of the kernel 1/√(4τ²−r′²) (Table I). An "improved Gaussian" (iG) correlator enforcing global color neutrality and a finite UV coarse-graining scale is constructed; its EMT is given by convergent small- and large-τ series that overlap near τ≈0.3 fm. Comparisons to abelian IP-Glasma runs and an application to angular momentum (dL_y/dη becoming constant at late time, Eq. 85) round out the paper.
Significance. If the results hold, the paper delivers three concrete assets: (i) the first closed-form coordinate-space analytic EMT of the weak-field glasma (Eqs. 74a–f), in terms of Meijer-G functions with explicitly extracted constant asymptotics — a parameter-free derivation in the sense that all time dependence follows from the resummed kernels and the MV g-functions; (ii) a structural universality argument for the late-time powers that requires only convergence of two moments of the initial correlator, making it robust across correlator models and, as the authors could note, against restoring the bounded Wilson-line factor; (iii) falsifiable, quantitative predictions — the asymptotic ratios P_L/ε → 0⁻, P_T/ε → 1/2, S_z/ε → const, ω ∼ τ, and the constant asymptote of dL_y/dη in Eq. (85) — that can vet numerical glasma codes, as illustrated by the IP-Glasma comparison in Fig. 7. The iG model, with global color neutrality built into the two-point ansatz, is a useful methodological addition even if incremental relative to Lam–Mahlon. The work is solid, verifiable analytic craftsmanship in a regime complementary to lattice simulations.
major comments (3)
- [§IV.C, below Eq. (58)] The check of ∂_μT^{μν}=0 'order by order in gradients of μ_k' is the only internal consistency test available for the O(∇²) results of Eqs. (D1a)–(D1g) and Table I, which depend on the extensive moment integrals (C1c)–(C1f) and the f₃…f₉, φ₂…φ₄ functions of Eqs. (D2)–(D11). Leaving it 'as an exercise for the interested reader' is not adequate: an algebraic slip anywhere in Appendix C or D would currently be invisible. The authors should demonstrate the identity explicitly at least through the first nontrivial gradient order (the leading-order check, ∂_τ ε + (ε+P_L)/τ = 0 at O(μ₁μ₂), is a one-line verification given Eqs. (58a,b)) and state how the η-derivative terms are handled for the higher-order pieces.
- [§II.C and Fig. 2; §VI.B] The weak-field truncation (recursion (7)→(11); U=1 below Eq. (38)) is controlled by g⁴Γ ~ g⁴μ being small. The paper's own Fig. 2 shows a ~27% suppression of ⟨E₀E₀⟩ already at g=1, μ=19.4 fm⁻², while Table IV and the discussion of Figs. 6–7 invoke realistic couplings g≈2 where the condition fails parametrically. Since the universality result (ε,P_T∼1/τ, P_L∼1/τ³) is claimed model-independently and is the paper's headline, the authors should (i) state a quantitative validity bound (e.g., on g⁴μ/m² or g⁴μB_q) within which U=1 is self-consistent, and (ii) state explicitly which conclusions survive outside that window. The structural argument for the powers (binomial expansion of the kernel 1/√(4τ²−r′²) plus moment convergence) appears unaffected by U(r)≠1, since U is bounded; saying so explicitly, with the caveat that prefactors shift, would strengthen the paper.
- [§VI.B, paragraph after Eq. (77)] The iG model is advertised as IR-safe via global color neutrality and 'UV-finite to at least second order gradients' (Summary), but the text notes that m is not fully replaced in ε_L,3,iG and that higher gradient orders cannot be guaranteed UV-safe. These statements are in tension and the Summary overstates the result. Please give a precise table or statement of which EMT components and gradient orders are (a) m-independent and (b) B_q-finite, and align the Summary wording with the qualified statement in this section.
minor comments (8)
- [Throughout] Typos: 'coliding' and 'qualitiative' (§I); 'conincidental' (below Eq. (58g)); 'straight forward' (several places); 'singularites' (below Eq. (74f)); 'measurementf' (§VII); double period after 'Meijer-G functions. .' (§I).
- [§II.C, Eq. (15a)] The noted minus-sign difference relative to Ref. [32] in Eq. (15a) should be resolved or explicitly attributed to a convention choice (gauge, ε-tensor, or Fourier convention), since readers will cross-check against that reference.
- [Eq. (39c)] The notation (r×∇_R)/r is nonstandard; please define the 2D cross product used here. Also state whether the antisymmetry of (39c) under μ₁↔μ₂ with the minus sign in (39d) has been checked against ⟨B₀E₀⟩ = −⟨E₀B₀⟩.
- [§VI.B, Eqs. (78)] The series (78a,b) are said to be 'quite well behaved' with overlap of the small- and large-τ expansions near τ≈0.3 fm. Please state the radius of convergence of (78) analytically if known (the coefficients a_n from Eq. (77) should permit an estimate), rather than only demonstrating it numerically in Fig. 4.
- [Fig. 7 and preceding paragraph] The agreement with abelian IP-Glasma is qualitative; since the code enforces IR/UV cutoffs via the lattice but not global color neutrality, please state the lattice spacing and box size used and comment on whether the 'slightly faster relaxation' of IP-Glasma could be a cutoff-matching artifact. The relaxation-time scaling ∝B_q^0.4 in the right panel is stated without an error band or fit quality.
- [Appendix G] The regulator rescaling m′=0.95√2 m drifting to 0.97√2 m between second and fourth order in τ is presented as evidence that no consistent mapping to Ref. [17]'s scheme exists. A short explanation of why the drift should be order-dependent (or a figure) would help; also clarify the 'constant 8% difference in ε₀'.
- [Table I] The header 'Q₁(τ)…Q₅(τ)' vs. the leading 'Q' row label is confusing; state explicitly that the subscript indexes the gradient order and that blank entries mean the term does not occur at that order. The large-τ growth of higher-gradient terms (τ³) should be accompanied by a quantitative breakdown criterion for the gradient expansion (e.g., |∇²μ/μ| τ² ≲ 1).
- [§VI.B, discussion of Figs. 5–6] The matching relations m≈0.5 B_c^{−1/2} (Fig. 5) vs. m≈0.46 B_c^{−1/2} and m≈1.3 B_c^{−1/2} (Fig. 6) are three different prescriptions used in quick succession; a compact summary of which matching applies to which observable (and why) would prevent confusion.
Circularity Check
No significant circularity: late-time powers and Meijer-G forms are derived from Yang-Mills weak-field kernels plus a stated two-point ansatz, not forced by fits or self-citation chains.
full rationale
The load-bearing chain is classical: light-cone Yang-Mills with the O(gA²) seed and linearized recursion (Sec. II.C, Eqs. 11–15), two-point field correlators reduced to nuclear gluon correlators G_k via structure constants (Sec. III, Eqs. 22, 26, 27), a general rotationally invariant γ expanded in smooth μ gradients (Sec. IV.A, Eq. 33), and the remaining r′-integrals over light-cone δ/Θ kernels (Eqs. 58). Large-time universality (ε, P_T ∼ 1/τ, P_L ∼ 1/τ³) follows from binomial expansion of 1/√(4τ²−r′²) and extension of the integral to infinity whenever the model moments of f₁, ϕ₁ converge—an algebraic property of the kernels, not of a fitted target. Closed MV forms (Eqs. 74–76) are obtained by converting K_ν products to Meijer-G contour integrals and evaluating the r′ integral; iG series (Eqs. 78–80) likewise follow from expanding E₁. Phenomenological μ(R), B_q, B_c and IP-Glasma comparisons (Apps. A–B, Fig. 7) are illustrative and do not enter the analytic claims. Self-citations to the authors’ recursive near-field work [17] supply setup and consistency checks (flow directions, energy-momentum conservation) but are not used as uniqueness theorems that force the late-time powers or Meijer-G coefficients. No step reduces a claimed prediction to its own definition or to a fit of a closely related observable.
Axiom & Free-Parameter Ledger
free parameters (5)
- m (MV infrared cutoff) =
∼1–1.3 fm^{-1} (matched to Bc in comparisons)
- Bq (iG UV area scale) =
0.3 GeV^{-2} (physical example); →0 recovers MV-like UV
- Bc (iG confinement area scale) =
4 GeV^{-2}
- n (Qs–μ conversion factor) =
0.8 (range 0.57–1.15)
- g and central μ =
scenario-dependent (e.g. μ=19.4 fm^{-2} for Au)
axioms (6)
- domain assumption Classical Yang-Mills with boost-invariant light-cone color currents J±=δ(x∓)ρ(x⊥) and axial gauge x+A−+x−A+=0.
- domain assumption Weak-field limit: retain only O(gA²) seeds at τ=0+ and drop higher non-abelian terms in the τ-recursion; set Wilson factor U=1.
- domain assumption Color charge two-point function factorizes in color and is specified by μ(R)D(r); higher cumulants of W[ρ] neglected.
- domain assumption Gradient expansion of slowly varying μ(R) truncated at second order; odd gradients vanish by parity.
- ad hoc to paper Global color neutrality ∫d²r D(r)=0 implemented by difference of two unit-normalized Gaussians in iG.
- standard math Meijer-G and Bessel integral identities used to evaluate r' integrals (standard special-function analysis).
invented entities (1)
-
Improved Gaussian (iG) nuclear gluon correlator
no independent evidence
read the original abstract
We discuss two-point functions and the energy momentum tensor of the classical gluon field after the collision of sheets of color charges on the light cone in the weak-field limit. The classical fields created by such a setup is thought to approximate the behavior of the gluon matter created right after the collision of heavy nuclei at large energies. Our discussion is based on a general expression for the gluon distribution in a nucleus, which contains the McLerran-Venugopalan (MV) Model as a special case. We derive the time-dependence of the energy momentum tensor in this general scenario. We show that the large-time behavior is universal, i.e.\ independent of the specific model for the gluon distribution, e.g.\ for energy density, transverse pressure and longitudinal pressure $\epsilon, P_T \sim 1/\tau$ and $P_L \sim 1/\tau^3$, where $\tau$ is longitudinal proper time. Subsequently, we focus on two special cases, the MV model and a proposed improved Gaussian (iG) model with improved ultraviolet (UV) and infrared (IR) behavior, the latter inspired by earlier work by Lam and Mahlon. We explicitly discuss the time dependence of the energy momentum tensor in both models. In the case of the MV-model, for infinite colliding nuclei, it is possible to give closed-formed analytic solutions for the energy momentum tensor in terms of special functions. Components of the energy momentum tensor take the form $\sim C (m\tau)^{-n} H(m\tau)$, where $n$ is an integer power, $m$ is the infrared cutoff, $H$ is a linear combination of Meijer-G functions with constant asymptotic value, and $C$ is a known constant. For the iG-model, we obtain reliable series expansions for both small and large times and show that the MV-model is recovered qualitatively in the UV limit. We briefly comment on implications for the angular momentum carried by the gluon field.
Figures
Reference graph
Works this paper leans on
-
[1]
=A gx−λg (1−x) 5.6 ∂xg(x,˜µ2) ∂log ˜µ2 = αs(˜µ2) 2π 1Z x dzPgg (z) x z g x z ,˜µ2 (A4) where the functionP gg is the gluon splitting function. To leading order it is Pgg (z) = 6 z (1−z)+ + 1−z z +z(1−z) + 11 2 − Nf 3 δ(1−z).(A5) In principle there is a contribution to the DGLAP evolution from annihilation of virtual quarks but this is thrown out on ground...
-
[2]
The Color glass condensate and high-energy scattering in QCD,
E. Iancu and R. Venugopalan, “The Color glass condensate and high-energy scattering in QCD,” inQuark-gluon plasma 4, edited by R. C. Hwa and X.-N. Wang (2003) pp. 249–3363, arXiv:hep-ph/0303204
Pith/arXiv arXiv 2003
-
[3]
F. Gelis, E. Iancu, J. Jalilian-Marian, and R. Venugopalan, Ann. Rev. Nucl. Part. Sci.60, 463 (2010), arXiv:1002.0333 [hep-ph]
Pith/arXiv arXiv 2010
-
[4]
T. Lappi and L. McLerran, Nucl. Phys. A772, 200 (2006), arXiv:hep-ph/0602189
Pith/arXiv arXiv 2006
-
[5]
C. Gale, S. Jeon, B. Schenke, P. Tribedy, and R. Venugopalan, Phys. Rev. Lett.110, 012302 (2013), arXiv:1209.6330 [nucl-th]
Pith/arXiv arXiv 2013
-
[6]
J. Berges, K. Boguslavski, S. Schlichting, and R. Venugopalan, Phys. Rev. D89, 074011 (2014), arXiv:1303.5650 [hep-ph]. 32
Pith/arXiv arXiv 2014
-
[7]
A. Kurkela, A. Mazeliauskas, J.-F. Paquet, S. Schlichting, and D. Teaney, Phys. Rev. C99, 034910 (2019), arXiv:1805.00961 [hep-ph]
Pith/arXiv arXiv 2019
-
[8]
J. Berges, M. P. Heller, A. Mazeliauskas, and R. Venugopalan, Rev. Mod. Phys.93, 035003 (2021), arXiv:2005.12299 [hep-th]
Pith/arXiv arXiv 2021
-
[9]
L. D. McLerran and R. Venugopalan, Phys. Rev. D49, 2233 (1994), arXiv:hep-ph/9309289
Pith/arXiv arXiv 1994
-
[10]
L. D. McLerran and R. Venugopalan, Phys. Rev. D49, 3352 (1994), arXiv:hep-ph/9311205
Pith/arXiv arXiv 1994
-
[11]
J. Jalilian-Marian, A. Kovner, L. D. McLerran, and H. Weigert, Phys. Rev. D55, 5414 (1997), arXiv:hep-ph/9606337
Pith/arXiv arXiv 1997
-
[12]
A. Kovner, L. D. McLerran, and H. Weigert, Phys. Rev. D52, 3809 (1995), arXiv:hep-ph/9505320
Pith/arXiv arXiv 1995
-
[13]
A. Kovner, L. D. McLerran, and H. Weigert, Phys. Rev. D52, 6231 (1995), arXiv:hep-ph/9502289
Pith/arXiv arXiv 1995
-
[14]
B. Schenke, P. Tribedy, and R. Venugopalan, Phys. Rev. C86, 034908 (2012), arXiv:1206.6805 [hep-ph]
Pith/arXiv arXiv 2012
-
[15]
B. Schenke, C. Shen, and P. Tribedy, Phys. Rev. C102, 044905 (2020), arXiv:2005.14682 [nucl-th]
Pith/arXiv arXiv 2020
-
[16]
M. R. Heffernan, C. Gale, S. Jeon, and J.-F. Paquet, (2023), arXiv:2306.09619 [nucl-th]
Pith/arXiv arXiv 2023
-
[17]
R. J. Fries, J. I. Kapusta, and Y. Li, Nucl. Phys. A774, 861 (2006), arXiv:hep-ph/0511101
Pith/arXiv arXiv 2006
-
[18]
G. Chen, R. J. Fries, J. I. Kapusta, and Y. Li, Phys. Rev. C92, 064912 (2015), arXiv:1507.03524 [nucl-th]
Pith/arXiv arXiv 2015
-
[19]
I. G. Beardenet al.(BRAHMS), Phys. Rev. Lett.93, 102301 (2004), arXiv:nucl-ex/0312023
Pith/arXiv arXiv 2004
-
[20]
A. Krasnitz, Y. Nara, and R. Venugopalan, Phys. Rev. Lett.87, 192302 (2001), arXiv:hep-ph/0108092
Pith/arXiv arXiv 2001
- [21]
-
[22]
B. Schenke, P. Tribedy, and R. Venugopalan, Phys. Rev. Lett.108, 252301 (2012), arXiv:1202.6646 [nucl-th]
Pith/arXiv arXiv 2012
-
[23]
D. Gelfand, A. Ipp, and D. M¨ uller, Phys. Rev. D94, 014020 (2016), arXiv:1605.07184 [hep-ph]
Pith/arXiv arXiv 2016
-
[24]
A. Ipp and D. M¨ uller, Phys. Lett. B771, 74 (2017), arXiv:1703.00017 [hep-ph]
Pith/arXiv arXiv 2017
-
[25]
S. McDonald, S. Jeon, and C. Gale, Phys. Rev. C108, 064910 (2023), arXiv:2306.04896 [hep-ph]
Pith/arXiv arXiv 2023
-
[26]
A. Ipp, M. Leuthner, D. I. M¨ uller, S. Schlichting, K. Schmidt, and P. Singh, Phys. Rev. D109, 094040 (2024), arXiv:2401.10320 [hep-ph]
Pith/arXiv arXiv 2024
-
[27]
J. Bartels, K. J. Golec-Biernat, and H. Kowalski, Phys. Rev. D66, 014001 (2002), arXiv:hep-ph/0203258
Pith/arXiv arXiv 2002
-
[28]
H. Kowalski and D. Teaney, Phys. Rev. D68, 114005 (2003), arXiv:hep-ph/0304189
Pith/arXiv arXiv 2003
-
[29]
O. Garcia-Montero, H. Elfner, and S. Schlichting, Phys. Rev. C109, 044916 (2024), arXiv:2308.11713 [hep-ph]
Pith/arXiv arXiv 2024
- [30]
-
[31]
G. Chen and R. J. Fries, Phys. Lett. B723, 417 (2013), arXiv:1303.2360 [nucl-th]
Pith/arXiv arXiv 2013
-
[32]
T. Lappi and S. Schlichting, Phys. Rev. D97, 034034 (2018), arXiv:1708.08625 [hep-ph]
Pith/arXiv arXiv 2018
-
[33]
P. Guerrero-Rodr ´ ıguez and T. Lappi, Phys. Rev. D104, 014011 (2021), arXiv:2102.09993 [hep-ph]
Pith/arXiv arXiv 2021
-
[34]
H. Fujii, K. Fukushima, and Y. Hidaka, Phys. Rev. C79, 024909 (2009), arXiv:0811.0437 [hep-ph]
Pith/arXiv arXiv 2009
-
[35]
M. E. Carrington, A. Czajka, and S. Mrowczynski, Eur. Phys. J. A58, 5 (2022), arXiv:2012.03042 [hep-ph]
Pith/arXiv arXiv 2022
-
[36]
M. E. Carrington, A. Czajka, and S. Mr´ owczy´ nski, Phys. Rev. C106, 034904 (2022), arXiv:2105.05327 [hep-ph]
Pith/arXiv arXiv 2022
-
[37]
M. Li and J. I. Kapusta, Phys. Rev. C94, 024908 (2016), arXiv:1602.09060 [nucl-th]
Pith/arXiv arXiv 2016
-
[38]
J. Jalilian-Marian, A. Kovner, A. Leonidov, and H. Weigert, Phys. Rev. D59, 014014 (1998), arXiv:hep-ph/9706377
Pith/arXiv arXiv 1998
-
[39]
J. Jalilian-Marian, A. Kovner, and H. Weigert, Phys. Rev. D59, 014015 (1998), arXiv:hep-ph/9709432
Pith/arXiv arXiv 1998
-
[40]
E. Iancu, A. Leonidov, and L. D. McLerran, Phys. Lett. B510, 133 (2001), arXiv:hep-ph/0102009
Pith/arXiv arXiv 2001
-
[41]
G. B. Arfken and H. J. Weber,Mathematical Methods for Physicists, 6th ed. (Elsevier Academic Press, 2005)
2005
-
[42]
Q.-G. Lin, Integral Transforms and Special Functions24, 783 (2013), https://doi.org/10.1080/10652469.2012.758119
arXiv 2013
-
[43]
Y. V. Kovchegov, Phys. Rev. D54, 5463 (1996), arXiv:hep-ph/9605446
Pith/arXiv arXiv 1996
-
[44]
C. S. Lam and G. Mahlon, Phys. Rev. D61, 014005 (2000), arXiv:hep-ph/9907281
Pith/arXiv arXiv 2000
-
[45]
C. S. Lam and G. Mahlon, Phys. Rev. D64, 016004 (2001), arXiv:hep-ph/0102337
Pith/arXiv arXiv 2001
-
[46]
MeijerG,
W. R. Inc., “MeijerG,”https://functions.wolfram.com/07.34.03.1058.01(2024)
2024
-
[47]
MeijerG,
W. R. Inc., “MeijerG,”http://functions.wolfram.com/07.34.03.0615.01(2026)
2026
-
[48]
MeijerG,
W. R. Inc., “MeijerG,”http://functions.wolfram.com/07.34.21.0009.01(2026)
2026
-
[49]
IP-Glasma 0.1,
B. Schenkeet al., “IP-Glasma 0.1,”https://github.com/schenke/ipglasma(2023)
2023
-
[50]
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
-
[51]
Z.-T. Liang and X.-N. Wang, Phys. Rev. Lett.94, 102301 (2005), [Erratum: Phys.Rev.Lett. 96, 039901 (2006)], arXiv:nucl- th/0410079
arXiv 2005
-
[52]
Y. Jiang, Z.-W. Lin, and J. Liao, Phys. Rev. C94, 044910 (2016), [Erratum: Phys.Rev.C 95, 049904 (2017)], arXiv:1602.06580 [hep-ph]
Pith/arXiv arXiv 2016
-
[53]
F. Becattini, I. Karpenko, M. Lisa, I. Upsal, and S. Voloshin, Phys. Rev. C95, 054902 (2017), arXiv:1610.02506 [nucl-th]
Pith/arXiv arXiv 2017
-
[54]
R. J. Fries, G. Chen, and S. Somanathan, Phys. Rev. C97, 034903 (2018), arXiv:1705.10779 [nucl-th]
Pith/arXiv arXiv 2018
-
[55]
M. E. Carrington and S. Mrowczynski, (2025), arXiv:2505.07324 [nucl-th]
Pith/arXiv arXiv 2025
-
[56]
Initial longitudinal and transverse motion of nuclei in the weak field limit,
S. Robicheaux and R. J. Fries, “Initial longitudinal and transverse motion of nuclei in the weak field limit,” (2026), in Preparation
2026
- [57]
-
[58]
A. H. Rezaeian, M. Siddikov, M. Van de Klundert, and R. Venugopalan, Phys. Rev. D87, 034002 (2013), arXiv:1212.2974 [hep-ph]
Pith/arXiv arXiv 2013
-
[59]
B. Schenke, P. Tribedy, and R. Venugopalan, Phys. Rev. C89, 064908 (2014), arXiv:1403.2232 [nucl-th]
Pith/arXiv arXiv 2014
-
[60]
De Vries, C
H. De Vries, C. De Jager, and C. De Vries, Atomic Data and Nuclear Data Tables36, 495 (1987)
1987
-
[61]
BesselI,
W. R. Inc., “BesselI,”http://functions.wolfram.com/03.02.26.0008.01(2024)
2024
-
[62]
W. R. Inc., “Exp,”http://functions.wolfram.com/01.03.21.0099.01(2024)
2024
-
[63]
MeijerG,
W. R. Inc., “MeijerG,”https://functions.wolfram.com/HypergeometricFunctions/MeijerG/(2024). 33
2024
-
[64]
LaguerreL,
W. R. Inc., “LaguerreL,”http://functions.wolfram.com/05.08.26.0001.01(2024)
2024
-
[65]
Hypergeometric1F1Regularized,
W. R. Inc., “Hypergeometric1F1Regularized,”http://functions.wolfram.com/07.21.03.0001.01(2024)
2024
-
[66]
Luke,The Special Functions and Their Approximations, Mathematics in science and engineering No
Y. Luke,The Special Functions and Their Approximations, Mathematics in science and engineering No. v. 1 (Academic Press, 1969)
1969
-
[67]
BesselJ,
W. R. Inc., “BesselJ,”http://functions.wolfram.com/03.01.21.0005.01(2025)
2025
-
[68]
HypergeometricPFQRegularized,
W. R. Inc., “HypergeometricPFQRegularized,”http://functions.wolfram.com/07.32.26.0004.01(2025)
2025
discussion (0)
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