REVIEW 3 major objections 5 minor 1 cited by
New evidence for the rapidity evolution in Mueller-Navelet dijet production: BFKL, Sudakov, and RG-invariance
T0 review · 3 major / 5 minor · reviewed 2026-08-07 · deepseek-v4-flash
Pith's one-line read NLO BFKL resummation plus initial-state radiation is what fits Mueller-Navelet dijet data across all rapidity separations.
desk verdict Genuinely novel RG-invariant NLO BFKL+HEF matching for MN dijets that deserves review, but the 'clear evidence' claim outruns the statistics and the Eq. (5) subtraction needs a numerical check. 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 load-bearing object is the matched hard-scattering coefficient $$\hat\sigma_{ij}^{\rm(HEF+BFKL)} = \hat\sigma_{ij}^{\rm(HEF)} + \hat\sigma_{ij}^{\rm(BFKL)} - \hat\sigma_{ij}^{\rm(BFKL,0)},$$ where $\hat\sigma_{ij}^{\rm(BFKL,0)}$ is the BFKL coefficient evaluated with the Green's function replaced by its initial condition $\delta^{(2)}(\ell_{T1}-\ell_{T2})$, which the paper identifies with the $Y\to\infty$ asymptotics of the fixed-order HEF coefficient. The BFKL part uses the exact NLO Green's function expanded over eigenfunctions $H_{n,\gamma}$ of the kernel, with the $O(\bar\alpha_s)$ eigenfunction corrections fixed so that the solution is RG-invariant; collinear improvement of the characteristic function removes the spurious splitting of the LO saddle point. The HEF part uses improved KMR W unintegrated PDFs that implement Sudakov resummation, so the whole construction carries both the initial-state-radiation resummation and the NLL BFKL resummation. The subtraction in Eq. (5) is what lets the two descriptions interpolate smoothly across the transition region.
What would settle it
Take the fixed-order HEF hard-scattering coefficient (given in Ref. [44]) and compute its large-$Y$ asymptotics directly: if it differs from the BFKL(0) coefficient used here, the subtraction leaves residual double counting and the predicted transition near $Y\sim 3.5$ would shift. Alternatively, high-statistics data in the transition region could expose a kink or discontinuity in the matched prediction, which would signal that the subtraction is not exact.
Extended reading notes
Core claim
On the paper's own terms, the central discovery is that the NLO BFKL-improved HEF computation—not fixed-order HEF and not LO BFKL-improved HEF—describes the Mueller-Navelet data. At small rapidity difference $Y\lesssim 3$ the fixed-order HEF contribution alone matches the measurements; beyond $Y\approx 3.5$ it over-predicts the angular correlation between the jets, and the LO BFKL-improved curve over-decorrelates, producing an almost flat azimuthal distribution. Only the NLL BFKL-improved curve reproduces the observed decorrelation at large $Y$ and the falling ratios $C_{k>n}/C_n$ of the $\cos(n(\Delta\phi-\pi))$ harmonic coefficients. The paper reports that the separation between the HEF-only and NLO BFKL-improved curves in these ratios reaches well above five standard deviations even after scale uncertainties, and that the RG-invariant construction reduces the scale dependence to the level of fixed-order calculations. This is the evidence the authors put forward for BFKL dynamics at Tevatron and LHC energies.
Load-bearing premise
Everything rests on the assumption that subtracting the BFKL(0) term—the BFKL coefficient with the Green's function set to its initial condition, identified with the fixed-order HEF coefficient's limit as the rapidity separation becomes very large—removes the double counting exactly at every finite $Y$; if this identity holds only approximately, the smooth interpolation and the apparent need for NLL corrections could be artifacts of the matching scheme.
Editorial extensions
If this is right
- One scheme now covers the whole measured rapidity range: fixed-order HEF at small $Y$ and NLO BFKL-improved HEF at large $Y$, so future analyses can quote one prediction instead of choosing a regime by hand.
- The ratios $C_{k>n}/C_n$ become a quantitative test of BFKL dynamics: the data sit more than five standard deviations below the fixed-order HEF curve and agree with the NLO BFKL-improved curve.
- At large $Y$, fixed-order HEF over-predicts azimuthal correlation and LO BFKL over-decorrelates; only the NLL resummation gives the observed shapes, so measurements in this region discriminate between resummation orders.
- The residual scale uncertainty is comparable to fixed-order calculations because the Green's function is RG-invariant at NLL, removing the need for BLM-type scale choices that earlier Mueller-Navelet studies relied on.
- The BFKL-induced growth of the $Y$-distribution relative to fixed-order HEF becomes more pronounced at higher collider energies, so higher-energy data should sharpen the signal further.
Reading between the lines
- If the matching identity is exact, the same subtract-the-shared-Regge-asymptotics recipe could be applied to other observables with two rapidity-separated hard probes, such as forward dijet or dihadron correlations, where fixed-order impact factors currently suffer large logarithmic corrections.
- The angular-coefficient ratios' low scale sensitivity suggests that finer $Y$ bins at 13 TeV, or lower-scale measurements, could separate the NLO BFKL prediction from the collinearly improved version, providing a sharper test of the $O(\bar\alpha_s^2)$ kernel terms than absolute cross sections.
- The paper's scheme still relies on the KMR W prescription for unintegrated PDFs; if that prescription's normalization or Sudakov content is altered, the size of the ISR effect and the position of the matching transition would change, so cross-checking with a different Sudakov-evolved unintegrated PDF set would test how much of the conclusion is specific to this choice.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper combines the high-energy factorization (HEF) description of Mueller-Navelet dijet production, which includes initial-state radiation effects through Kimber-Martin-Ryskin-Watt unintegrated PDFs, with a next-to-leading-logarithmic (NLL) BFKL resummation using an RG-invariant solution of the BFKL equation built from NLO eigenfunctions. The two descriptions are matched through Eq. (5), where the BFKL(0) contribution—the BFKL expression with the Green's function replaced by its initial condition—is subtracted to avoid double counting. The authors compare their predictions with CMS and D0 data on rapidity-difference distributions, energy ratios, azimuthal decorrelation, and angular harmonic ratios, and conclude that both the HEF initial-state radiation effects and NLL BFKL resummation are needed for a uniform description, claiming that the angular-harmonic ratios provide clear, multi-standard-deviation evidence for BFKL dynamics.
Significance. If the matching procedure is valid and the comparisons are quantitatively reliable, this would be a significant advance: it would provide BFKL phenomenology without the BLM scale-setting prescription that has been essential in previous Mueller-Navelet analyses, and it would combine, for the first time, HEF-based initial-state radiation resummation with an RG-invariant NLO BFKL Green's function. The paper contains no parameter fits to the dijet data; all ingredients are taken from published PDFs, the NLO BFKL kernel, and the authors' prior HEF formalism. The central phenomenological direction is plausible, and the plots show systematic, physically expected differences between HEF-only, LO BFKL-improved, and NLO BFKL-improved predictions. However, the strength of the final claim depends on the matching identity in Eq. (5) and on the statistical interpretation of the quoted standard-deviation separation, both of which need to be made explicit and verified.
major comments (3)
- [Eq. (5) and End Matter] The matching identity is the load-bearing step of the paper. The text asserts that the BFKL(0) term is the Y-to-infinity (Regge) asymptotics of the HEF hard-scattering coefficient, so that subtracting it removes exactly the double counting between the fixed-order HEF HSC of Ref. [44] and the BFKL-resummed HSC. This is cited from Ref. [56], but the HEF HSC of Ref. [44] is derived from the complete set of LO effective-theory diagrams, not from a factorized impact-factor convolution; the factorized form with the Green's function replaced by its initial condition is at best the leading high-energy term. No numerical or analytic check is provided that the difference between the full HEF HSC and its BFKL(0) approximation is negligible in the transition region Y ~ 3-3.5 where the matching switches between the two regimes. Since the paper's central evidence for NLL BFKL is precisely that LO BFKL falls below the data while NLO BFKL agrees, an imperfect subtraction could shift the transition and manufacture or distort the apparent need for NLL corrections. The authors should provide a quantitative test of Eq. (5) in the overlap region, for example by comparing the two HSCs directly as functions of Y, or by isolating the subleading terms in the large-Y expansion of the HEF HSC.
- [Fig. 1(l)-(q) and surrounding text] The abstract and the discussion in the text state that the separation between the HEF-only curve and the NLL BFKL-improved curve in the angular-harmonic ratios 'reaches well above five standard deviations, even taking into account the residual scale-uncertainty bands.' No definition of this significance is given: it is not stated whether the comparison uses experimental uncertainties, theoretical uncertainties, or both, whether the experimental points are treated as correlated or uncorrelated, or what statistic (chi-square, point-by-point pull) is used. Given that the paper's headline claim is 'clear evidence in favour of the BFKL dynamics,' this statistical statement must be backed by a concrete prescription, for example a chi-square per point or a covariance-aware estimate, or the claim should be softened to a descriptive comparison of curves.
- [Fig. 1(a)-(e) and Fig. 1(f)-(k)] The quantitative quality of the data description is asserted from visual inspection but no goodness-of-fit numbers are given for any of the distributions. In particular, the claim that HEF describes the data well for Y < 3 and that NLO BFKL-improved HEF agrees with the data for Y > 3.5 is not supported by any uncertainty quantification. For a Letter whose main message is phenomenological evidence, providing chi-square or likelihood values per data set, or at least listing the number of data points and the quoted uncertainties, would make the evidence reproducible and falsifiable.
minor comments (5)
- [Abstract and page 1] The abstract contains the typo 'BKFL equation' instead of 'BFKL equation'; the same typo appears in the introductory paragraph on page 1 ('NLO BKFL equation').
- [End Matter, last paragraph] The statement 'We have checked the consistency of the solution (4) with the running-coupling solution proposed in Ref. [64] and found the agreement up to NLL' is an unverifiable assertion because the details are deferred to a future publication. In a self-contained Letter, either the comparison should be shown in a supplementary plot or this sentence should be explicitly marked as a preliminary check that does not enter the phenomenological conclusions.
- [End Matter, Eq. (5) discussion] The phrase 'with the Green's function substituted by it's initial condition' contains a typo: 'it's' should be 'its'.
- [Fig. 3 caption] The caption of Fig. 3 states 'The (a) characteristic function (7) at Re gamma = 1/2 as function of Im gamma' but the letter '(a)' appears to be a leftover label from a multi-panel figure; the panel labels should be cleaned up.
- [End Matter, Eq. (9)] The notation in Eq. (9) is dense: the summation indices and the meaning of the braces — in particular whether they denote a principal-value prescription or a symmetrization — are not defined in the main text. A sentence clarifying the notation would help the reader.
Circularity Check
No significant circularity: the predictions are generated from external PDFs, published fixed-order HEF matrix elements, and a published NLO BFKL Green's function, with no parameter fitted to the MN dijet data.
full rationale
The paper's derivation chain is genuinely input-driven. Equation (2) uses the KMRW UPDFs of Ref. [46] built on MSTW2008 PDFs, the fixed-order HEF hard-scattering coefficient is taken from the independent published calculation of Ref. [44], and the NLO BFKL Green's function is constructed from the eigenfunctions of Refs. [36,37] with a collinear-improved characteristic function. The only freedom is the scale choice mu_R = mu_F = 2 xi sqrt(|p_T1||p_T2|), with xi = 0 central and xi = +/-1 for uncertainty bands; this is not a fit to the CMS or D0 data used for comparison. The nearest potential concern is the matching identity in Eq. (5), where the BFKL(0) term is asserted to be the Y -> infinity Regge asymptotic of the HEF HSC, with Ref. [56] cited. That identity is a theoretical assumption imported from earlier work with overlapping authorship, but it is parameter-free and is not fitted to the data, so it does not constitute a circular reduction. Moreover, the same BFKL(0) subtraction enters both the LO and NLO BFKL-improved curves, so the paper's central evidence in favor of NLL BFKL dynamics comes from the difference between the LO and NLO Green's-function evolutions, not from the matching term itself. The remaining self-citations to Refs. [44,46,56] concern published formalism pieces with independent derivations; they do not by construction force the claimed conclusion that NLL BFKL resummation is crucial. No step of the enumerated circularity kinds can be exhibited from the text.
Assumptions & free parameters
assumptions (4)
- domain assumption The NLO BFKL Green's function is exactly represented by the eigenfunction expansion (4) with NLO eigenfunctions H_{n,gamma} constructed in Refs. [36,37], including the principal-value prescription at gamma=1/2.
- domain assumption The HEF cross section (2), with the improved KMR-W UPDFs of Ref. [46], correctly resums the initial-state radiation and Sudakov effects relevant for MN dijets.
- ad hoc to paper The matching identity (5) holds: the BFKL(0) term equals the Y to infinity (Regge) asymptotics of the HEF HSC, so the subtraction removes double counting exactly.
- domain assumption The collinear-improved characteristic function (9) can be added to the NLO characteristic function (7) without breaking NLO accuracy or RG-invariance.
Cite this review
Pith. "Pith review of New evidence for the rapidity evolution in Mueller-Navelet dijet production: BFKL, Sudakov, and RG-invariance." pith.science (2026). https://pith.science/paper/BZVBTEQ6
@misc{pith2026250610458,
author = {Pith},
title = {Pith review of: New evidence for the rapidity evolution in Mueller-Navelet dijet production: BFKL, Sudakov, and RG-invariance},
year = {2026},
howpublished = {\url{https://pith.science/paper/BZVBTEQ6}},
note = {Machine review of arXiv:2506.10458}
}
read the original abstract
We study the effects of matching of the high-energy resummation based on the BFKL equation with initial state radiation effects, taken into account within the framework of high-energy factorization, in the production of Mueller-Navelet dijets. We use RG-invariant solution of the NLO BFKL equation built out of eigenfunctions perturbatively constructed up to NLO to avoid the need for a special renormalization scale setting. We demonstrate that various data sets from the FNAL Tevatron and CERN LHC can be described in this way and both, the NLL BFKL resummation and initial state radiation effects of the high-energy factorization, are crucial for the uniform description of the data across all values of the rapidity difference between the jets. The behavior of angular distributions and ratios of angular coefficients with increasing rapidity separation between the jets provides clear evidence for the BFKL dynamics at the FNAL Tevatron and CERN LHC.
Figures
Forward citations
Cited by 1 Pith paper
-
Endpoint Logarithms in the NLO Mueller-Navelet Jet Vertex: Threshold Matching and BLM/MOM Prescription Sensitivity
A conservative BFKL-aware threshold matching scheme is constructed for the NLO forward jet vertex that resums ordinary endpoint logs, preserves NLO accuracy, and is tested against CMS azimuthal observables, showing in...
Reference graph
Works this paper leans on
- [44]
-
[56]
Z.-G. He, B. Kniehl, M. Nefedov, and V. Saleev, Phys. Rev. Lett.123, 162002 (2019), arXiv:1906.08979 [hep- 6 ph]
arXiv 2019
-
[1]
L. N. Lipatov, Sov. J. Nucl. Phys.23, 338 (1976)
work page 1976
-
[2]
E. A. Kuraev, L. N. Lipatov, and V. S. Fadin, Sov. Phys. JETP44, 443 (1976)
1976
-
[3]
E. A. Kuraev, L. N. Lipatov, and V. S. Fadin, Sov. Phys. JETP45, 199 (1977)
1977
-
[4]
I. I. Balitsky and L. N. Lipatov, Sov. J. Nucl. Phys.28, 822 (1978)
1978
-
[5]
V. S. Fadin and L. N. Lipatov, Phys. Lett. B429, 127 (1998), arXiv:hep-ph/9802290
arXiv 1998
-
[6]
V. S. Fadin and L. N. Lipatov, Eur. Phys. J. C78, 439 (2018), arXiv:1712.09805 [hep-ph]
arXiv 2018
Show all 68 references
-
[7]
Abdul Khalek et al., Nucl
R. Abdul Khalek et al., Nucl. Phys. A1026, 122447 (2022), arXiv:2103.05419 [physics.ins-det]
2022 arXiv
-
[8]
E. P. Byrne, JHEP07, 284 (2024), arXiv:2312.15051 [hep-ph]
2024 arXiv
-
[9]
V. S. Fadin, M. Fucilla, and A. Papa, JHEP04, 137 (2023), arXiv:2302.09868 [hep-ph]
2023 arXiv
-
[10]
E. P. Byrne, V. Del Duca, L. J. Dixon, E. Gardi, and J. M. Smillie, JHEP08, 271 (2022), arXiv:2204.12459 [hep-ph]
2022 arXiv
-
[11]
Caola, A
F. Caola, A. Chakraborty, G. Gambuti, A. von Man- teuffel, and L. Tancredi, Phys. Rev. Lett.128, 212001 (2022), arXiv:2112.11097 [hep-ph]
2022 arXiv
-
[12]
Falcioni, E
G. Falcioni, E. Gardi, N. Maher, C. Milloy, and L. Vernazza, Phys. Rev. Lett.128, 132001 (2022), arXiv:2112.11098 [hep-ph]
2022 arXiv
-
[13]
Del Duca, R
V. Del Duca, R. Marzucca, and B. Verbeek, JHEP01, 149 (2022), arXiv:2111.14265 [hep-ph]
2022 arXiv
-
[14]
Abreu, G
S. Abreu, G. De Laurentis, G. Falcioni, E. Gardi, C. Milloy, and L. Vernazza, JHEP04, 161 (2025), arXiv:2412.20578 [hep-ph]
2025 arXiv
-
[15]
Buccioni, F
F. Buccioni, F. Caola, F. Devoto, and G. Gambuti, JHEP03, 129 (2025), arXiv:2411.14050 [hep-ph]
2025 arXiv
-
[16]
Hentschinski et al., Acta Phys
M. Hentschinski et al., Acta Phys. Polon. B54, 3 (2023), arXiv:2203.08129 [hep-ph]
2023 arXiv
-
[17]
A. H. Mueller and H. Navelet, Nucl. Phys. B282, 727 (1987)
1987
-
[18]
Del Duca and C
V. Del Duca and C. R. Schmidt, Phys. Rev. D49, 4510 (1994), arXiv:hep-ph/9311290
1994 arXiv
-
[19]
W. J. Stirling, Nucl. Phys. B423, 56 (1994), arXiv:hep- ph/9401266
1994
-
[20]
J. R. Andersen, V. Del Duca, S. Frixione, C. R. Schmidt, and W. J. Stirling, JHEP02, 007 (2001), arXiv:hep- ph/0101180
2001
-
[21]
Sabio Vera and F
A. Sabio Vera and F. Schwennsen, Nucl. Phys. B776, 170 (2007), arXiv:hep-ph/0702158
2007 arXiv
-
[22]
Colferai, F
D. Colferai, F. Schwennsen, L. Szymanowski, and S. Wallon, JHEP12, 026 (2010), arXiv:1002.1365 [hep- ph]
2010 arXiv
-
[23]
Ducloue, L
B. Ducloue, L. Szymanowski, and S. Wallon, JHEP05, 096 (2013), arXiv:1302.7012 [hep-ph]
2013 arXiv
-
[24]
Duclou´ e, L
B. Duclou´ e, L. Szymanowski, and S. Wallon, Phys. Rev. Lett.112, 082003 (2014), arXiv:1309.3229 [hep-ph]
2014 arXiv
-
[25]
Duclou´ e, L
B. Duclou´ e, L. Szymanowski, and S. Wallon, Phys. Rev. D92, 076002 (2015), arXiv:1507.04735 [hep-ph]
2015 arXiv
-
[26]
A. H. Mueller, L. Szymanowski, S. Wallon, B.-W. Xiao, and F. Yuan, JHEP03, 096 (2016), arXiv:1512.07127 [hep-ph]
2016 arXiv
-
[27]
Caporale, D
F. Caporale, D. Y. Ivanov, B. Murdaca, and A. Papa, Nucl. Phys. B877, 73 (2013), arXiv:1211.7225 [hep-ph]
2013 arXiv
-
[28]
Caporale, D
F. Caporale, D. Y. Ivanov, B. Murdaca, and A. Papa, Eur. Phys. J. C74, 3084 (2014), [Erratum: Eur.Phys.J.C 75, 535 (2015)], arXiv:1407.8431 [hep-ph]
2014 arXiv
-
[29]
Caporale, D
F. Caporale, D. Y. Ivanov, B. Murdaca, and A. Papa, Phys. Rev. D91, 114009 (2015), arXiv:1504.06471 [hep- ph]
2015 arXiv
-
[30]
F. G. Celiberto and A. Papa, Phys. Rev. D106, 114004 (2022), arXiv:2207.05015 [hep-ph]
2022 arXiv
-
[31]
A. I. Egorov and V. T. Kim, Phys. Rev. D108, 014010 (2023), arXiv:2305.19854 [hep-ph]
2023 arXiv
-
[32]
Baldenegro, G
C. Baldenegro, G. Chachamis, M. Kampshoff, M. Klasen, G. J. Milhano, C. Royon, and A. Sabio Vera, Phys. Rev. D110, 114027 (2024), arXiv:2406.10681 [hep-ph]
2024 arXiv
-
[33]
Altinoluk, N
T. Altinoluk, N. Armesto, A. Kovner, and M. Lublinsky, Phys. Rev. D108, 074003 (2023), arXiv:2307.14922 [hep- ph]
2023 arXiv
-
[34]
S. J. Brodsky, G. P. Lepage, and P. B. Mackenzie, Phys. Rev. D28, 228 (1983)
1983
-
[35]
S. J. Brodsky, V. S. Fadin, V. T. Kim, L. N. Lipatov, and G. B. Pivovarov, JETP Lett.70, 155 (1999), arXiv:hep- ph/9901229
1999
-
[36]
G. A. Chirilli and Y. V. Kovchegov, JHEP06, 055 (2013), arXiv:1305.1924 [hep-ph]
2013 arXiv
-
[37]
G. A. Chirilli and Y. V. Kovchegov, JHEP05, 099 (2014), [Erratum: JHEP 08, 075 (2015)], arXiv:1403.3384 [hep- ph]
2014 arXiv
-
[38]
L. V. Gribov, E. M. Levin, and M. G. Ryskin, Phys. Rept.100, 1 (1983)
1983
-
[39]
Catani, M
S. Catani, M. Ciafaloni, and F. Hautmann, Phys. Lett. B242, 97 (1990)
1990
-
[40]
Catani, M
S. Catani, M. Ciafaloni, and F. Hautmann, Nucl. Phys. B366, 135 (1991)
1991
-
[41]
Catani, M
S. Catani, M. Ciafaloni, and F. Hautmann, Phys. Lett. B307, 147 (1993)
1993
-
[42]
Catani and F
S. Catani and F. Hautmann, Nucl. Phys. B427, 475 (1994), arXiv:hep-ph/9405388
1994 arXiv
-
[43]
J. C. Collins and R. K. Ellis, Nucl. Phys. B360, 3 (1991)
1991
-
[45]
A. V. Karpishkov, M. A. Nefedov, and V. A. Saleev, Phys. Rev. D96, 096019 (2017), arXiv:1707.04068 [hep- ph]
2017 arXiv
-
[46]
Nefedov and V
M. Nefedov and V. Saleev, Phys. Rev. D102, 114018 (2020)
2020
-
[47]
L. N. Lipatov, Nucl. Phys. B452, 369 (1995)
1995
- [48]
-
[49]
E. N. Antonov, L. N. Lipatov, E. A. Kuraev, and I. O. Cherednikov, Nucl. Phys. B721, 111 (2005)
2005
-
[50]
van Hameren and M
A. van Hameren and M. Nefedov, JHEP02, 160 (2025), arXiv:2501.02619 [hep-ph]
2025 arXiv
-
[51]
L. N. Lipatov and M. I. Vyazovsky, Nucl. Phys. B597, 399 (2001)
2001
-
[52]
M. A. Kimber, A. D. Martin, and M. G. Ryskin, Phys. Rev. D63, 114027 (2001)
2001
-
[53]
G. Watt, A. D. Martin, and M. G. Ryskin, Eur. Phys. J. C31, 73 (2003)
2003
-
[54]
Ioffe, V
B. Ioffe, V. Fadin, and L. Lipatov, Quantum chromodynamics: Perturbative and nonperturbative aspects (Cambridge Univ. Press, 2010)
2010
-
[55]
Kovchegov and E
Y. Kovchegov and E. Levin, Quantum Chromodynamics at High Energy, Vol. 33 (Oxford University Press, 2013)
2013
- [57]
-
[58]
A. D. Martin, W. J. Stirling, R. S. Thorne, and G. Watt, Eur. Phys. J. C63, 189 (2009), arXiv:0901.0002 [hep-ph]
2009 arXiv
-
[59]
Chatrchyan et al
S. Chatrchyan et al. (CMS), Eur. Phys. J. C72, 2216 (2012), arXiv:1204.0696 [hep-ex]
2012 arXiv
-
[60]
Khachatryan et al
V. Khachatryan et al. (CMS), JHEP08, 139 (2016), arXiv:1601.06713 [hep-ex]
2016 arXiv
- [61]
- [62]
-
[63]
Angioni, G
M. Angioni, G. Chachamis, J. D. Madrigal, and A. Sabio Vera, Phys. Rev. Lett.107, 191601 (2011), arXiv:1106.6172 [hep-th]
2011 arXiv
-
[64]
A. V. Grabovsky, JHEP09, 098 (2013), arXiv:1307.3152 [hep-ph]
2013 arXiv
-
[65]
A. V. Kotikov and L. N. Lipatov, Nucl. Phys. B582, 19 (2000), arXiv:hep-ph/0004008
2000 arXiv
-
[66]
G. P. Salam, JHEP07, 019 (1998), arXiv:hep- ph/9806482
1998
-
[67]
Sabio Vera, Nucl
A. Sabio Vera, Nucl. Phys. B722, 65 (2005), arXiv:hep- ph/0505128
2005
-
[68]
all-poles
A. Polizzi, M. Fucilla, and A. Papa, (2025), arXiv:2505.18074 [hep-ph]. 7 qT 2→ qT 2→ qT 2→ ← qT 1 pT 2↓ ← qT 1 ↓ pT 1 ← lT 2 pT 2↓ ← lT 1 ← qT 1 ↓ pT 1 (c) (b) (a) y| − + pT 2↓ ↓ pT 1 − + − + − + BFKL − + FIG. 2: Different HSCs in Eq. (5) plotted on the rapidity axis. Dashed ...
2025
Reviewed August 7, 2026 · model on record in the stance chip above.
Discussion (0). Sign in to comment.