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REVIEW 3 major objections 5 minor 58 references

Extrapolated low-Q² electron data give a larger Δ(1232) peak for the deuteron and neutron than real-photon measurements, matching the proton as isospin symmetry requires.

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 02:10 UTC pith:3HNJ2Y3U

load-bearing objection Useful new Q²→0 σ_TT spectra that restore approximate p–n Δ equality via electroextraction, but the headline rests on a linear extrapolation that is only lightly stress-tested. the 3 major comments →

arxiv 2607.28612 v1 pith:3HNJ2Y3U submitted 2026-07-30 hep-ex nucl-ex

Extraction of σ_(TT) for Proton, Neutron, Deuteron and ³He from Quasi-real Photon Scattering

classification hep-ex nucl-ex
keywords nucleon spin structurephotoproduction cross-sectionGDH sum rulesigma_TTprotonneutrondeuteronhelium-3
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.

This paper takes polarized electron-scattering cross sections measured at very small virtuality and extrapolates them to the real-photon limit, producing an independent determination of the helicity-difference photoproduction cross section σ_TT for the proton, deuteron, neutron and ³He. The proton result agrees with existing real-photon data, but the deuteron and the neutron extracted from it (or from ³He) show substantially more strength in the Δ(1232) resonance. That larger strength brings the neutron into line with the proton, as expected from isospin symmetry of the N→Δ transition—something the direct photoproduction deuteron data had appeared to violate. The work therefore both tests the reliability of the quasi-real-photon method and supplies a practical route to neutron spin observables from light nuclei at photon point kinematics.

Core claim

When Jefferson Lab electroproduction data on the proton, deuteron and ³He are extrapolated to Q² = 0, the resulting σ_TT for the proton matches real-photon measurements, while the deuteron and the neutron extracted via the weak-binding approximation display a markedly larger Δ(1232) peak. The neutron results from deuteron and from ³He agree with each other and with the proton magnitude, restoring the isospin expectation that had been in tension with earlier photoproduction extractions.

What carries the argument

Linear extrapolation of A₁F₁ (or of σ_TT itself) versus Q² in the window Q² < 0.2 GeV² to the real-photon point, followed by weak-binding-approximation unsmearing that subtracts the proton contribution and removes nuclear Fermi motion to recover free-neutron σ_TT.

Load-bearing premise

That a straight-line fit in virtuality below 0.2 GeV² is accurate enough to reach the true real-photon cross section, with no important curvature near Q² = 0.

What would settle it

A new exclusive real-photon measurement of deuteron σ_TT across the Δ(1232) that either reproduces the larger strength found by the extrapolation or reconfirms the smaller existing photoproduction values at the few-percent level.

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

If this is right

  • Neutron σ_TT extracted from deuteron and from ³He electroproduction are mutually consistent and comparable in size to the proton at the Δ(1232).
  • The weak-binding approximation can be used to obtain neutron spin structure from ³He data at real and quasi-real photon kinematics, a regime previously unexplored with that method.
  • Low-Q² inclusive electroproduction plus extrapolation becomes a practical complement to exclusive real-photon experiments for photoproduction observables.
  • The isovector combination σ_TT^(p−n) is near zero at the Δ peak in the extrapolated data, consistent with the small isovector GDH sum implied by the near-equality of proton and neutron anomalous moments.

Where Pith is reading between the lines

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

  • If the larger extrapolated Δ strength is correct, existing real-photon deuteron analyses may have under-subtracted quasi-elastic or final-state-interaction backgrounds near threshold.
  • Agreement between deuteron- and ³He-based neutron extractions at Q² = 0 suggests the same nuclear-smearing framework can be applied to the large body of existing low-Q² ³He spin data still awaiting neutron extraction.
  • A controlled comparison of linear versus higher-order Q² extrapolations on the same data set would quantify the dominant systematic that currently limits the claim.

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 / 5 minor

Summary. The manuscript extracts the polarized photoproduction cross section σ_TT(ν) for the proton, deuteron, ³He and (via WBA) the neutron by linearly extrapolating low-Q² electroproduction data from JLab EG4 and E97-110 to the real-photon point. Proton results agree with Mainz-ELSA photoproduction in the Δ(1232) region; deuteron and neutron extractions yield a larger Δ strength than real-photon deuteron data and are closer to isospin equality with the proton. Resonance-region integrals (Tables 1–3) and isovector combinations quantify the comparisons, and WBA is applied to ³He at quasi-real kinematics for the first time.

Significance. If the extrapolated spectra and the restored isospin pattern hold, the work supplies an independent inclusive data set that complements exclusive real-photon measurements, tests the practical reach of Q²→0 extrapolation for photoproduction observables, and opens a path to neutron spin structure from existing ³He data outside DIS. The first application of WBA unsmearing to ³He at very low Q² and the tabulated resonance integrals are concrete, reusable results. The tension with photoproduction deuteron Δ strength is a falsifiable claim of interest to the GDH and nucleon-resonance communities.

major comments (3)
  1. [§2] §2: The central claim (larger deuteron/neutron Δ strength restoring isospin; Abstract, Tables 1–3, Figs. 1–3) rests on linear fits of A1F1 or σ_TT vs Q² for Q²<0.2 GeV². Reduced χ²~0.7–0.9 and leave-many-out/perturbation ensembles do not test curvature or resonance-dependent Q² shapes near the photon point (chiral loops, VMD, N→Δ multipole evolution). A systematic shift of the Q²=0 intercept would move the headline Δ integrals (Table 2: 80.6/71.5 vs 51.3) and the near-zero isovector at the Δ peak without being captured by the quoted errors. The paper should show quadratic (or theory-motivated) alternatives, quantify intercept shifts bin-by-bin especially under the Δ, and either enlarge the extrapolation uncertainty or justify why linear is adequate.
  2. [Table 1, §2] Table 1 and §2: Proton electro- vs photo-production disagree at 4σ in the second resonance region (21.8±2.2 vs 31.9±1.3) while agreeing in the Δ. The text notes the discrepancy but does not assess whether it signals residual Q² dependence, radiative-correction differences, or an under-estimated extrapolation uncertainty that could also affect the deuteron/neutron Δ comparison. A quantitative discussion of this control sample is needed before the isospin conclusion is drawn.
  3. [§3] §3: WBA is applied to ³He at Q²=0 for the first time and yields neutron Δ strength consistent with the deuteron electroproduction extraction. The paper states that wave-function and input-model variations are negligible, but does not show the size of those variations relative to the data errors, nor discuss known limitations of WBA for exclusive/resonant channels or final-state interactions at the photon point. A short quantitative appendix or figure demonstrating the stability of the unsmeared σ_n_TT under the stated variations would make the first-time ³He claim more robust.
minor comments (5)
  1. [Fig. 1] Fig. 1 caption and panels: axis labels use mixed fonts and truncated units (‘b) µ’); make σ_TT units and ν labels uniform across the three panels.
  2. [Eq. (3)] Eq. (3): K_γ is introduced without an explicit definition in the text; cite the convention used (e.g. Hand or Gilman) for reproducibility.
  3. [Table 2] Table 2 header and bold/italic convention: the caption says bold (italic) for >4σ (>3σ), but the body uses bold only for one entry and italic for others inconsistently with Table 1’s italic-only rule; unify the significance markup.
  4. [Appendix A] Appendix tables A.4–A.8: W and ν columns are useful; add a brief note on whether the listed syst already includes the extrapolation component or only the original experimental syst.
  5. [References] References: arXiv:2604.14385 is cited as Pedroni et al. (4 2026); confirm status and update if a journal version or final arXiv exists before publication.

Circularity Check

0 steps flagged

No significant circularity: empirical Q2-to-0 extrapolation compared to independent real-photon data and external models.

full rationale

The paper’s chain is an experimental extraction, not a derivation that closes on its inputs. EG4/E97-110 electroproduction points are fit linearly in Q2 < 0.2 GeV2 and extrapolated to Q2 = 0; neutron sigma_TT is then obtained via the weak-binding approximation using external nuclear wavefunctions and independent proton photoproduction (or electroproduction) inputs. The headline comparison is to Mainz-ELSA/A2 real-photon datasets and to external multipion/AFS/SAID models—none of which are defined by the extrapolated intercepts. Reduced chi2 and drop-half-points resampling quantify fit uncertainty; they do not force the Delta integrals or the near-zero isovector by construction. Self-citations are to the authors’ own source experiments (normal data provenance) and are not used as uniqueness theorems or as the sole justification of the isospin claim. Adequacy of the linear ansatz is a systematic/correctness question, not circularity. Score 0; steps empty.

Axiom & Free-Parameter Ledger

2 free parameters · 5 axioms · 0 invented entities

The central claim rests on experimental input cross sections plus two modeling layers: linear Q² extrapolation to the photon point and weak-binding nuclear unsmearing. No new dynamical entities are postulated. Free parameters are the per-bin linear fit coefficients; domain assumptions are standard QED Born virtual-photon kinematics, WBA factorization, and isospin structure of the N→Δ transition used only for interpretation.

free parameters (2)
  • Per-ν-bin linear coefficients for A1F1(Q²) or σ_TT(Q²) in Q²<0.2 GeV² = Bin-dependent; not tabulated as slopes, only Q²=0 intercepts in Appendix tables
    Primary fit form is linear in Q²; intercept at Q²=0 is the reported real-photon point. Slope and intercept are fitted independently in each energy bin from the electroproduction data.
  • Extrapolation uncertainty ensemble (drop up to half the points; perturb within errors)
    Defines the outer error bars on extrapolated points; the procedure is a chosen statistical protocol rather than a unique estimator.
axioms (5)
  • domain assumption Virtual-photon electroproduction observables at Q²≲0.2 GeV² connect smoothly to real-photon σ_TT via a low-order (here linear) polynomial in Q².
    Invoked throughout §2 as the justification for fitting and quoting Q²=0 values; not derived from a dispersion relation in the paper.
  • domain assumption Weak binding approximation: light-nucleus structure functions are convolutions of free nucleon structure functions with smearing functions from nuclear wavefunctions.
    Used in §3 to unsmear deuteron and ³He data into neutron σ_TT; validity at Q²=0 is explicitly under test.
  • domain assumption Born approximation relating measured lepton asymmetries/structure functions to virtual-photon σ_TT via Eqs. (2)–(3).
    Standard in the cited EG4/E97-110 analyses; taken as given when forming σ_TT from A1F1 or g1,g2.
  • domain assumption Isospin-symmetric N→Δ transition implies σ_TT^{p−n}≈0 near the Δ peak (modulo nonresonant background).
    Used in §4 as the benchmark for interpreting isovector results, citing Burkert; interpretive, not required to extract the cross sections themselves.
  • standard math Standard arithmetic and χ² fitting for linear regression and integral comparisons.
    Ordinary statistical procedures in §2 and Tables 1–3.

pith-pipeline@v1.2.0-daily-grok45 · 21015 in / 3635 out tokens · 66447 ms · 2026-07-31T02:10:29.560645+00:00 · methodology

0 comments
read the original abstract

We report on an extraction of the polarized photoproduction cross-section for the proton, deuteron, neutron and $^3$He, obtained by extrapolating electron scattering data to the real photon point. The data are from the Jefferson Lab E97-110 ($^3$He) and CLAS EG4 (proton and deuteron) experiments. Information on the neutron is extracted from the deuteron or $^3$He data using the weak binding approximation. Comparing with data obtained with real photons, we find that while the proton results agree, our results on the deuteron and the neutron exhibit a larger strength in the $\Delta(1232)$ region, and are more consistent with isospin symmetry when compared with the proton results.

Figures

Figures reproduced from arXiv: 2607.28612 by A.Deur, A.Rask, B.Callahan, D.W.Upton, M.M.Dalton, O.Larson, X.Zheng, Yilei Li.

Figure 1
Figure 1. Figure 1: σT T for the proton (left), deuteron (center) and 3He (right) vs. ν, for photoproduction data (red +) and for electroproduction data extrapolated to Q 2 = 0 (blue ×). For the extrapolated electroproduction data, the inner error bars are from the statistical uncertainty of the original data and the outer error bars are the total uncertainty with the statistical and the extrapolation uncertainties added in q… view at source ↗
Figure 2
Figure 2. Figure 2: together with a model constructed [16] as a sum of final states Nπ [45], Nππ [46], and Nη [47] [PITH_FULL_IMAGE:figures/full_fig_p003_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: Isovector combination σ p−n T T (ν) from three different combinations of photo- vs. electro-production, and deuteron vs. 3He data. real photon point. This provides independent data with differ￾ent types of systematic uncertainties, and for the 3He case also significantly higher precision and energy coverage, compared to photoproduction data. The extrapolated electroproduction results show similar ∆(1232) s… view at source ↗

discussion (0)

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Reference graph

Works this paper leans on

58 extracted references · 7 canonical work pages

  1. [1]

    Ashman, et al., A Measurement of the Spin Asymme- try and Determination of the Structure Function g(1) in Deep Inelastic Muon-Proton Scattering, Phys

    J. Ashman, et al., A Measurement of the Spin Asymme- try and Determination of the Structure Function g(1) in Deep Inelastic Muon-Proton Scattering, Phys. Lett. B 206 (1988) 364.doi:10.1016/0370-2693(88)91523-7

  2. [2]

    Anselmino, A

    M. Anselmino, A. Efremov, E. Leader, The theory and phenomenology of polarized deep inelastic scattering, Phys. Rept. 261 (1995) 1–124, [Erratum: Phys.Rept. 281, 399–400 (1997)].arXiv:hep-ph/9501369,doi:10. 1016/0370-1573(95)00011-5

  3. [3]

    A. Deur, S. J. Brodsky, G. F. De Téramond, The Spin Structure of the Nucleon, Rept. Prog. Phys. 82 (2019) 076201.arXiv:1807.05250,doi:10.1088/ 1361-6633/ab0b8f

  4. [4]

    X. Ji, F. Yuan, Y . Zhao, What we know and what we don’t know about the proton spin after 30 years, Nature Rev. Phys. 3 (1) (2021) 27–38.arXiv:2009.01291,doi:10. 1038/s42254-020-00248-4

  5. [5]

    S. B. Gerasimov, A sum rule for magnetic moments and the damping of the nucleon magnetic moment in nuclei, Yad. Fiz. 2 (1965) 598–602

  6. [6]

    S. D. Drell, A. C. Hearn, Exact sum rule for nucleon magnetic moments, Phys. Rev. Lett. 16 (1966) 908–911. doi:10.1103/PhysRevLett.16.908

  7. [7]

    Altarelli, N

    G. Altarelli, N. Cabibbo, L. Maiani, The Drell-Hearn sum rule and the lepton magnetic moment in the Wein- berg model of weak and electromagnetic interactions, Phys. Lett. B 40 (1972) 415–419.doi:10.1016/ 0370-2693(72)90833-7

  8. [8]

    M. M. Dalton, A. Deur, C. D. Keith, S. Širca, J. Stevens, Measurement of the high-energy contribution to the Gerasimov-Drell-Hearn sum rule (8 2020).arXiv:2008. 11059

  9. [9]

    Ahrens, et al., First measurement of the Gerasimov- Drell-Hearn integral for hydrogen from 200 to 800 MeV, Phys

    J. Ahrens, et al., First measurement of the Gerasimov- Drell-Hearn integral for hydrogen from 200 to 800 MeV, Phys. Rev. Lett. 87 (2001) 022003.arXiv:hep-ex/ 0105089,doi:10.1103/PhysRevLett.87.022003

  10. [10]

    Dutz, et al., First measurement of the Gerasimov- Drell-Hearn sum rule for H-1 from 0.7-GeV to 1.8-GeV at ELSA, Phys

    H. Dutz, et al., First measurement of the Gerasimov- Drell-Hearn sum rule for H-1 from 0.7-GeV to 1.8-GeV at ELSA, Phys. Rev. Lett. 91 (2003) 192001.doi:10. 1103/PhysRevLett.91.192001

  11. [11]

    Dutz, et al., Experimental check of the Gerasimov- Drell-Hearn sum rule for H-1, Phys

    H. Dutz, et al., Experimental check of the Gerasimov- Drell-Hearn sum rule for H-1, Phys. Rev. Lett. 93 (2004) 032003.doi:10.1103/PhysRevLett.93.032003

  12. [12]

    Ahrens, et al., Measurement of the Gerasimov-Drell- Hearn integrand for H-2 from 200-MeV to 800-MeV, Phys

    J. Ahrens, et al., Measurement of the Gerasimov-Drell- Hearn integrand for H-2 from 200-MeV to 800-MeV, Phys. Rev. Lett. 97 (2006) 202303.doi:10.1103/ PhysRevLett.97.202303

  13. [13]

    Ahrens, et al., Helicity dependence of the total inclusive cross section on the deuteron, Phys

    J. Ahrens, et al., Helicity dependence of the total inclusive cross section on the deuteron, Phys. Lett. B 672 (2009) 328–332.doi:10.1016/j.physletb.2009.01.061

  14. [14]

    Helbing, The Gerasimov-Drell-Hearn sum rule, Prog

    K. Helbing, The Gerasimov-Drell-Hearn sum rule, Prog. Part. Nucl. Phys. 57 (2006) 405–469.arXiv:nucl-ex/ 0603021,doi:10.1016/j.ppnp.2005.09.003

  15. [15]

    Aguar Bartolome, et al., First measurement of the he- licity dependence of 3He photoreactions in the∆(1232) resonance region, Phys

    P. Aguar Bartolome, et al., First measurement of the he- licity dependence of 3He photoreactions in the∆(1232) resonance region, Phys. Lett. B 723 (2013) 71–77.doi: 10.1016/j.physletb.2013.04.057

  16. [16]

    Pedroni, et al., Measurement of the Gerasimov-Drell- Hearn integrand for proton and deuteron from 200 to 1400 MeV (4 2026).arXiv:2604.14385

    P. Pedroni, et al., Measurement of the Gerasimov-Drell- Hearn integrand for proton and deuteron from 200 to 1400 MeV (4 2026).arXiv:2604.14385

  17. [17]

    Dutz, et al., Measurement of helicity-dependent pho- toabsorption cross sections on the neutron from 815-MeV to 1825-MeV, Phys

    H. Dutz, et al., Measurement of helicity-dependent pho- toabsorption cross sections on the neutron from 815-MeV to 1825-MeV, Phys. Rev. Lett. 94 (2005) 162001.doi: 10.1103/PhysRevLett.94.162001

  18. [18]

    G. Laskaris, et al., First Measurements of Spin-Dependent Double-Differential Cross Sections and the Gerasimov- Drell-Hearn Integrand from 3⃗He(⃗γ,n)ppat Incident Pho- ton Energies of 12.8 and 14.7 MeV, Phys. Rev. Lett. 110 (20) (2013) 202501.arXiv:1304.5442,doi:10. 1103/PhysRevLett.110.202501

  19. [19]

    Laskaris, et al., Measurement of the doubly-polarized ⃗3He(⃗γ,n)ppreaction at 16.5 MeV and its implications for the GDH sum rule, Phys

    G. Laskaris, et al., Measurement of the doubly-polarized ⃗3He(⃗γ,n)ppreaction at 16.5 MeV and its implications for the GDH sum rule, Phys. Lett. B 750 (2015) 547– 551.arXiv:1506.00332,doi:10.1016/j.physletb. 2015.09.065

  20. [20]

    Laskaris, et al., First measurement of the asymme- try and the Gerasimov-Drell-Hearn integrand from the 3He(γ,p)2H reaction at an incident photon energy of 29 MeV, Phys

    G. Laskaris, et al., First measurement of the asymme- try and the Gerasimov-Drell-Hearn integrand from the 3He(γ,p)2H reaction at an incident photon energy of 29 MeV, Phys. Rev. C 103 (3) (2021) 034311.arXiv: 2010.14055,doi:10.1103/PhysRevC.103.034311

  21. [21]

    Anselmino, B

    M. Anselmino, B. L. Ioffe, E. Leader, On possible resolu- tions of the spin crisis in the parton model, Sov. J. Nucl. Phys. 49 (1989) 136

  22. [22]

    X.-D. Ji, J. Osborne, Generalized sum rules for spin de- pendent structure functions of the nucleon, J. Phys. G 27 (2001) 127.arXiv:hep-ph/9905410,doi:10.1088/ 0954-3899/27/1/308

  23. [23]

    Drechsel, S

    D. Drechsel, S. S. Kamalov, L. Tiator, The GDH sum rule and related integrals, Phys. Rev. D 63 (2001) 114010.arXiv:hep-ph/0008306,doi:10.1103/ PhysRevD.63.114010

  24. [24]

    Drechsel, L

    D. Drechsel, L. Tiator, The Gerasimov-Drell-Hearn sum rule and the spin structure of the nucleon, Ann. Rev. Nucl. Part. Sci. 54 (2004) 69–114.arXiv:nucl-th/0406059, doi:10.1146/annurev.nucl.54.070103.181159. 5

  25. [25]

    Airapetian, et al., TheQ 2 dependence of the gen- eralized Gerasimov-Drell-Hearn integral for the proton, Phys

    A. Airapetian, et al., TheQ 2 dependence of the gen- eralized Gerasimov-Drell-Hearn integral for the proton, Phys. Lett. B 494 (2000) 1–8.arXiv:hep-ex/0008037, doi:10.1016/S0370-2693(00)01111-4

  26. [26]

    Airapetian, et al., TheQ 2 dependence of the gener- alized Gerasimov-Drell-Hearn integral for the deuteron, proton and neutron, Eur

    A. Airapetian, et al., TheQ 2 dependence of the gener- alized Gerasimov-Drell-Hearn integral for the deuteron, proton and neutron, Eur. Phys. J. C 26 (2003) 527– 538.arXiv:hep-ex/0210047,doi:10.1140/epjc/ s2002-01118-x

  27. [27]

    Ackerstaff, et al., Determination of the deep inelas- tic contribution to the generalized Gerasimov-Drell-Hearn integral for the proton and neutron, Phys

    K. Ackerstaff, et al., Determination of the deep inelas- tic contribution to the generalized Gerasimov-Drell-Hearn integral for the proton and neutron, Phys. Lett. B 444 (1998) 531–538.arXiv:hep-ex/9809015,doi:10. 1016/S0370-2693(98)01396-3

  28. [28]

    Amarian, et al., The Q**2 evolution of the general- ized Gerasimov-Drell-Hearn integral for the neutron using a He-3 target, Phys

    M. Amarian, et al., The Q**2 evolution of the general- ized Gerasimov-Drell-Hearn integral for the neutron using a He-3 target, Phys. Rev. Lett. 89 (2002) 242301.arXiv: nucl-ex/0205020,doi:10.1103/PhysRevLett.89. 242301

  29. [29]

    Prok, et al., Moments of the spin structure functions gp 1 and g d 1 for 0.05<Q 2 <3.0-GeV 2, Phys

    Y . Prok, et al., Moments of the spin structure functions gp 1 and g d 1 for 0.05<Q 2 <3.0-GeV 2, Phys. Lett. B 672 (2009) 12–16.arXiv:0802.2232,doi:10.1016/j. physletb.2008.12.063

  30. [30]

    Guler, et al., Precise determination of the deuteron spin structure at low to moderateQ 2 with CLAS and ex- traction of the neutron contribution, Phys

    N. Guler, et al., Precise determination of the deuteron spin structure at low to moderateQ 2 with CLAS and ex- traction of the neutron contribution, Phys. Rev. C 92 (5) (2015) 055201.arXiv:1505.07877,doi:10.1103/ PhysRevC.92.055201

  31. [31]

    Fersch, et al., Determination of the proton spin struc- ture functions for 0.05<Q 2 <5 GeV 2 using CLAS, Phys

    R. Fersch, et al., Determination of the proton spin struc- ture functions for 0.05<Q 2 <5 GeV 2 using CLAS, Phys. Rev. C 96 (6) (2017) 065208.arXiv:1706.10289, doi:10.1103/PhysRevC.96.065208

  32. [32]

    Sulkosky, et al., Measurement of the generalized spin polarizabilities of the neutron in the low-Q 2 region, Na- ture Phys

    V . Sulkosky, et al., Measurement of the generalized spin polarizabilities of the neutron in the low-Q 2 region, Na- ture Phys. 17 (6) (2021) 687–692, [Erratum: Nature Phys. 18, (2022)].arXiv:2103.03333,doi:10.1038/ s41567-021-01245-9

  33. [33]

    Sulkosky, et al., Measurement of the 3He spin- structure functions and of neutron (3He) spin-dependent sum rules at 0.035≤Q2≤0.24 GeV2, Phys

    V . Sulkosky, et al., Measurement of the 3He spin- structure functions and of neutron (3He) spin-dependent sum rules at 0.035≤Q2≤0.24 GeV2, Phys. Lett. B 805 (2020) 135428.arXiv:1908.05709,doi:10.1016/j. physletb.2020.135428

  34. [34]

    Zheng, et al., Measurement of the proton spin structure at long distances, Nature Phys

    X. Zheng, et al., Measurement of the proton spin structure at long distances, Nature Phys. 17 (6) (2021) 736–741.arXiv:2102.02658,doi:10.1038/ s41567-021-01198-z

  35. [35]

    K. P. Adhikari, et al., Measurement of theQ 2 dependence of the deuteron spin structure functiong 1 and its mo- ments at lowQ 2 with CLAS, Phys. Rev. Lett. 120 (6) (2018) 062501.arXiv:1711.01974,doi:10.1103/ PhysRevLett.120.062501

  36. [36]

    Deur, et al., Measurement of the nucleon spin structure functions for 0.01<Q2<1GeV2 using CLAS, Phys

    A. Deur, et al., Measurement of the nucleon spin structure functions for 0.01<Q2<1GeV2 using CLAS, Phys. Rev. C 111 (3) (2025) 035202.arXiv:2409.08365,doi:10. 1103/PhysRevC.111.035202

  37. [37]

    Deur, et al., Experimental study of the behavior of the Bjorken sum at very low Q2, Phys

    A. Deur, et al., Experimental study of the behavior of the Bjorken sum at very low Q2, Phys. Lett. B 825 (2022) 136878.arXiv:2107.08133,doi:10.1016/j. physletb.2022.136878

  38. [38]

    Bernard, N

    V . Bernard, N. Kaiser, U.-G. Meissner, Chiral dynam- ics in nucleons and nuclei, Int. J. Mod. Phys. E 4 (1995) 193–346.arXiv:hep-ph/9501384,doi:10. 1142/S0218301395000092

  39. [39]

    Y . Kahn, W. Melnitchouk, S. A. Kulagin, New method for extracting neutron structure functions from nuclear data, Phys. Rev. C 79 (2009) 035205.arXiv:0809.4308, doi:10.1103/PhysRevC.79.035205

  40. [40]

    J. J. Ethier, W. Melnitchouk, Comparative study of nuclear effects in polarized electron scattering from 3He, Phys. Rev. C 88 (5) (2013) 054001.arXiv:1308.3723,doi: 10.1103/PhysRevC.88.054001

  41. [41]

    J. J. Ethier, N. Doshi, S. Malace, W. Mel- nitchouk, Quasielastic electron-deuteron scatter- ing in the weak binding approximation, Phys. Rev. C 89 (2014) 065203.arXiv:1402.3910, doi:10.1103/PhysRevC.89.065203

  42. [42]

    A. J. Tropiano, J. J. Ethier, W. Melnitchouk, N. Sato, Deep-inelastic and quasielastic electron scattering from A=3 nuclei, Phys. Rev. C 99 (3) (2019) 035201.arXiv: 1811.07668,doi:10.1103/PhysRevC.99.035201

  43. [43]

    B. A. Mecking, et al., The CEBAF Large Acceptance Spectrometer (CLAS), Nucl. Instrum. Meth. A 503 (2003) 513–553.doi:10.1016/S0168-9002(03)01001-5

  44. [44]

    Alcorn, et al., Basic Instrumentation for Hall A at Jef- ferson Lab, Nucl

    J. Alcorn, et al., Basic Instrumentation for Hall A at Jef- ferson Lab, Nucl. Instrum. Meth. A 522 (2004) 294–346. doi:10.1016/j.nima.2003.11.415

  45. [45]

    Strakovsky, S

    I. Strakovsky, S. Širca, W. J. Briscoe, A. Deur, A. Schmidt, R. L. Workman, Single-pion contribution to the Gerasimov-Drell-Hearn sum rule and related in- tegrals, Phys. Rev. C 105 (4) (2022) 045202.arXiv: 2201.06495,doi:10.1103/PhysRevC.105.045202

  46. [46]

    A. Fix, H. Arenhoevel, Double pion photoproduction on nucleon and deuteron, Eur. Phys. J. A 25 (2005) 115– 135.arXiv:nucl-th/0503042,doi:10.1140/epja/ i2005-10067-5

  47. [47]

    Tiator, M

    L. Tiator, M. Gorchtein, V . L. Kashevarov, K. Nikonov, M. Ostrick, M. Hadžimehmedovi ´c, R. Omerovi ´c, H. Os- manovi´c, J. Stahov, A. Švarc, Eta and Etaprime Photo- production on the Nucleon with the Isobar Model Eta- MAID2018, Eur. Phys. J. A 54 (12) (2018) 210.arXiv: 1807.04525,doi:10.1140/epja/i2018-12643-x. 6

  48. [48]

    Matveev, A

    M. Matveev, A. V . Sarantsev, V . A. Nikonov, A. V . Aniso- vich, U. Thoma, E. Klempt, Hyperon I: Partial-wave amplitudes for K−p scattering, Eur. Phys. J. A 55 (10) (2019) 179.arXiv:1907.03645,doi:10.1140/epja/ i2019-12878-y

  49. [49]

    A. V . Sarantsev, M. Matveev, V . A. Nikonov, A. V . Anisovich, U. Thoma, E. Klempt, Hyperon II: Prop- erties of excited hyperons, Eur. Phys. J. A 55 (10) (2019) 180.arXiv:1907.13387,doi:10.1140/epja/ i2019-12880-5

  50. [50]

    Arenhovel, A

    H. Arenhovel, A. Fix, M. Schwamb, Spin asymmetry and Gerasimov-Drell-Hearn sum rule for the deuteron, Phys. Rev. Lett. 93 (2004) 202301.arXiv:nucl-th/0407058, doi:10.1103/PhysRevLett.93.202301

  51. [51]

    R. L. Workman, M. W. Paris, W. J. Briscoe, I. I. Strakovsky, Unified Chew-Mandelstam SAID analysis of pion photoproduction data, Phys. Rev. C 86 (2012) 015202.arXiv:1202.0845,doi:10.1103/PhysRevC. 86.015202

  52. [52]

    W. J. Briscoe, A. Schmidt, I. Strakovsky, R. L. Work- man, A. Svarc, Extended SAID partial-wave analy- sis of pion photoproduction, Phys. Rev. C 108 (6) (2023) 065205.arXiv:2309.06631,doi:10.1103/ PhysRevC.108.065205

  53. [53]

    V . D. Burkert, Comment on the generalized Gerasimov- Drell-Hearn sum rule in chiral perturbation theory, Phys. Rev. D 63 (2001) 097904.arXiv:nucl-th/0004001, doi:10.1103/PhysRevD.63.097904

  54. [54]

    Solvignon, et al., Moments of the neutrong 2 structure function at intermediateQ 2, Phys

    P. Solvignon, et al., Moments of the neutrong 2 structure function at intermediateQ 2, Phys. Rev. C 92 (1) (2015) 015208.arXiv:1304.4497,doi:10.1103/PhysRevC. 92.015208

  55. [55]

    Flay, et al., Measurements ofd n 2 andA n 1: Prob- ing the neutron spin structure, Phys

    D. Flay, et al., Measurements ofd n 2 andA n 1: Prob- ing the neutron spin structure, Phys. Rev. D 94 (5) (2016) 052003.arXiv:1603.03612,doi:10.1103/ PhysRevD.94.052003

  56. [56]

    J. D. Bjorken, Asymptotic sum rules at infinite momen- tum, Phys. Rev. 179 (1969) 1547–1553.doi:10.1103/ PhysRev.179.1547

  57. [57]

    A. Deur, S. J. Brodsky, C. D. Roberts, QCD running cou- plings and effective charges, Prog. Part. Nucl. Phys. 134 (2024) 104081.arXiv:2303.00723,doi:10.1016/j. ppnp.2023.104081

  58. [58]

    S. J. Brodsky, R. Shrock, Maximum Wavelength of Confined Quarks and Gluons and Properties of Quan- tum Chromodynamics, Phys. Lett. B 666 (2008) 95–99. arXiv:0806.1535,doi:10.1016/j.physletb.2008. 06.054. Table A.4: Cross sections extrapolated toQ 2 =0 for 1H. W ν σT T stat syst GeV GeV µb µb µb 1.11 0.188 −93.8 37.0 41.9 1.13 0.212 −39.7 32.6 37.5 1.15 0....