Measuring the Weizsaecker-Williams distribution of linearly polarized gluons at an electron-ion collider through dijet azimuthal asymmetries
Pith reviewed 2026-05-24 17:01 UTC · model grok-4.3
The pith
Dijet production in semi-inclusive DIS can extract the Weizsaecker-Williams distribution of linearly polarized gluons via azimuthal asymmetries.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
The Weizsaecker-Williams TMD gluon distributions can be probed in hard dijet production in semi-inclusive DIS, where the linearly polarized gluon distribution generates an azimuthal dependence that distinguishes it from the conventional distribution. Extraction of the linearly polarized distribution to 5 percent statistical accuracy at a future electron-ion collider would require an estimated luminosity of 20 fb^{-1}/A.
What carries the argument
Azimuthal dependence of the dijet cross section in semi-inclusive DIS that isolates the linearly polarized gluon TMD contribution.
Load-bearing premise
The theoretical description of dijet production accurately isolates the linearly polarized gluon TMD through azimuthal asymmetries without major unaccounted systematic effects from higher-order corrections or backgrounds.
What would settle it
An actual dijet azimuthal asymmetry measurement at the quoted luminosity that shows no statistically significant modulation attributable to the linearly polarized gluon TMD would falsify the extraction claim.
read the original abstract
The Weizsaecker-Williams transverse momentum dependent (TMD) gluon distributions can be probed in the production of a hard dijet in semi-inclusive DIS. This process is sensitive not only to the conventional but also to the linearly polarized gluon distribution. The latter gives rise to an azimuthal dependence of the dijet cross section and therefore can be distinguished from the former. Feasibility study of a measurement of these TMDs through dijet production at a future electron-ion collider shows that the extraction of the distribution of linearly polarized gluons with a statistical accuracy of 5% will require estimated luminosity of 20 fb^{-1} /A.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript studies dijet production in semi-inclusive DIS as a probe of the Weizsäcker-Williams gluon TMDs, with the linearly polarized gluon distribution h1⊥g isolated via the cos(2Δφ) azimuthal asymmetry. A feasibility study for measurements at a future electron-ion collider concludes that a luminosity of 20 fb^{-1}/A suffices to extract this distribution with 5% statistical accuracy.
Significance. If the LO TMD factorization framework and model assumptions hold, the work supplies a concrete, falsifiable luminosity target for accessing a gluon TMD that is otherwise difficult to measure, strengthening the physics case for EIC dijet programs. The explicit mapping from asymmetry to h1⊥g via a specific TMD parametrization is a clear strength of the feasibility calculation.
major comments (2)
- [§3.2, Eq. (15)] §3.2, Eq. (15) and surrounding text: the projected 5% statistical accuracy on h1⊥g (and the derived 20 fb^{-1}/A luminosity) is obtained under leading-order TMD factorization with a fixed model for the unpolarized and polarized gluon TMDs; no numerical estimate or error budget is provided for the size of NLO hard-coefficient corrections, jet-radius logarithms, or 1/Q power corrections that are known to reach 10-20% in related TMD processes.
- [§4.1, Table 1] §4.1, Table 1: the event-yield and asymmetry projections assume perfect isolation of the h1⊥g contribution with no background subtraction uncertainty or hadronization modeling; a 15% theory systematic would shift the required luminosity by a comparable factor, yet no such variation is shown.
minor comments (2)
- The notation for the Weizsäcker-Williams distributions is introduced without an explicit comparison table to the standard f1g and h1⊥g conventions used in the TMD literature.
- Figure 3 caption should state the precise kinematic cuts (Q2, x, pT) used for the asymmetry curves.
Simulated Author's Rebuttal
We thank the referee for the detailed and constructive report. We address the two major comments below, agreeing that the analysis is performed at leading order and under idealized conditions. We will make partial revisions to improve the discussion of these limitations.
read point-by-point responses
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Referee: [§3.2, Eq. (15)] §3.2, Eq. (15) and surrounding text: the projected 5% statistical accuracy on h1⊥g (and the derived 20 fb^{-1}/A luminosity) is obtained under leading-order TMD factorization with a fixed model for the unpolarized and polarized gluon TMDs; no numerical estimate or error budget is provided for the size of NLO hard-coefficient corrections, jet-radius logarithms, or 1/Q power corrections that are known to reach 10-20% in related TMD processes.
Authors: We agree that the projections rely on leading-order TMD factorization and a specific model choice, without a quantitative assessment of NLO hard coefficients, jet-radius logarithms, or power corrections. These effects are known to be relevant in TMD phenomenology. The manuscript is intended as a first feasibility study to establish the basic statistical reach; a complete higher-order analysis lies outside its scope. In the revision we will add an explicit caveat paragraph after Eq. (15) stating that the quoted 5% accuracy and 20 fb^{-1}/A luminosity are LO estimates and that NLO and power corrections of order 10-20% would proportionally increase the required luminosity. revision: partial
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Referee: [§4.1, Table 1] §4.1, Table 1: the event-yield and asymmetry projections assume perfect isolation of the h1⊥g contribution with no background subtraction uncertainty or hadronization modeling; a 15% theory systematic would shift the required luminosity by a comparable factor, yet no such variation is shown.
Authors: The numbers in Table 1 are generated under the assumption of perfect signal isolation to illustrate the statistical power of the dijet channel. We acknowledge that realistic background subtraction and hadronization modeling would introduce additional theory systematics. A 15% systematic uncertainty would indeed scale the required luminosity upward by a comparable factor. In the revised manuscript we will add a footnote to Table 1 and a short paragraph in §4.1 showing the luminosity that would be needed if a flat 15% theory systematic is folded in, thereby making the sensitivity to such uncertainties explicit. revision: partial
Circularity Check
Luminosity estimate is forward Monte Carlo feasibility calculation from external TMD models
full rationale
The paper reports a feasibility study that converts assumed TMD distributions and LO cross sections into an estimated luminosity needed for 5% statistical precision on the linearly polarized gluon TMD. This is a forward calculation, not a fit to data that is then relabeled as a prediction, nor a self-definition, nor a load-bearing self-citation. No equations or claims in the provided abstract reduce the output to the input by construction; the result depends on standard TMD factorization assumptions external to the paper.
Axiom & Free-Parameter Ledger
axioms (1)
- domain assumption Dijet production in semi-inclusive DIS is sensitive to both the conventional and linearly polarized Weizsaecker-Williams gluon TMD distributions, with the latter producing a distinct azimuthal dependence.
discussion (0)
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