{"id":"488eadb5-0ab7-4d55-a686-f317e4f1ae1f","arxiv_id":"2607.06241","paper_version":1,"verdict":"CONDITIONAL","confidence":"MODERATE","novelty_score":4.0,"correctness_risk":"unknown","formal_verification":"none","parameter_count":3,"one_line_summary":"The RDWIA+MEC approach describes MicroBooNE's measured inclusive and pionless neutrino-argon cross sections within experimental uncertainties.","lead":"This paper calculates neutrino-argon scattering cross sections using the RDWIA+MEC framework and compares them to MicroBooNE data, finding good agreement. It matters because accurate neutrino-nucleus cross sections are a leading systematic uncertainty for oscillation experiments like DUNE.","discovery_kind":"unclear","skeptic_critique":{"model":"glm-5.2","headline":"The EDAD1 optical potential is validated only on carbon/calcium electron-scattering data, not argon, making the FSI modeling for 40Ar unquantified and the 'good agreement' claim difficult to assess without uncertainty bands.","rationale":"The reader correctly identified the optical potential transfer from carbon to argon as the weakest assumption. My review confirms this is the most load-bearing concern: the justification for using EDAD1 on argon rests entirely on carbon/calcium electron-scattering references, with no direct argon validation. The reader's CONDITIONAL verdict with MODERATE confidence is appropriate. The concern is real but not necessarily disqualifying — the experimental uncertainties are large (>10% for double-differential, >6% for single-differential), and the model does appear to track the data visually. However, the absence of theoretical uncertainty bands means the quality of agreement cannot be rigorously assessed, and the systematic discrepancies the authors themselves note (particularly the underestimation at high Eµ and in the forward cos θ bin) could be symptoms of the optical potential mismatch. The reader's mention of the MA circularity is a secondary issue: MA is a nucleon-level parameter, so using a carbon-fitted value for argon is not circular in the same way as the nucleus-dependent optical potential, though the tension between MA=1.2 GeV and LQCD benchmarks (Fig. 1d, ~20% discrepancy at Q²=1 GeV²) is worth noting as an additional correctness risk. The concrete test proposed — varying the optical potential parametrization — would directly settle whether the FSI modeling choice is driving the observed discrepancies or whether the agreement is robust.","tokens_in":13363,"tokens_out":3309,"duration_ms":138565,"concrete_test":"Recompute the flux-integrated inclusive dσ/dEµ (Fig. 4) and dσ/d cos θ (Fig. 5) using at least two alternative optical potential parametrizations available in the Cooper et al. framework (e.g., EDAI-O or the A-dependent global form evaluated at A=40 rather than the carbon-specific EDAD1). If the spread between predictions exceeds the experimental uncertainties (~6-10% for single-differential cross sections), the 'good agreement' claim is not robust to the optical potential choice and the verdict should be downgraded. If the spread is below ~3%, the concern does not land and the CONDITIONAL verdict could be relaxed.","verdict_should_be":"UNCHANGED","load_bearing_attack":"The central claim is that the RDWIA+MEC approach with MA=1.2 GeV describes MicroBooNE 40Ar data 'within experimental uncertainties.' For this to be a meaningful statement, the model must be genuinely predictive for argon, not merely a collection of parameters transferred from carbon. The most load-bearing issue is the optical potential. In Sec. II.B, the authors state they use 'the EDAD1 parametrization [46] of the relativistic optical potential tailored for carbon' and justify this by citing electron-scattering data from Refs. [30, 47-49]. However, Refs. [47-49] are 12C(e,e'p) measurements, and Ref. [30] concerns carbon and oxygen. None of these validate the EDAD1 potential on argon. The optical potential encodes nucleus-dependent FSI effects (density distribution, shell structure, absorption), and 40Ar differs significantly from 12C in nuclear structure. Additionally, the spectroscopic factor ⟨S⟩ ≈ 87% is taken from 40Ca(e,e'p) data [45] and applied to 40Ar — another cross-nucleus transfer, though 40Ca and 40Ar are isobars with different shell structure (40Ca is doubly magic, 40Ar is not). The paper itself notes systematic discrepancies: overestimation in the 0.8 < cos θ < 0.9 bin, underestimation in 0.9 < cos θ < 1.0, and a 'slight systematic underestimation' for Eµ > 0.8 GeV (Sec. III.A). Without theoretical uncertainty bands, it is impossible to determine whether these discrepancies are consistent with the expected systematic error from the optical potential transfer or indicate a genuine model failure. The claim of 'good agreement' is thus not falsifiable as presented.","agreement_with_reader":"agree"},"referee_report":{"model":"glm-5.2","summary":"This manuscript calculates flux-integrated inclusive and pionless differential cross sections for charged-current neutrino scattering off 40Ar at MicroBooNE energies using the RDWIA+MEC framework. The quasielastic channel is treated within the relativistic distorted-wave impulse approximation, the 2p-2h meson-exchange current contribution uses parametrizations from SuSA-MEC calculations, and resonance/DIS contributions are taken from the GENIE v3 generator (G18-10a configuration). The axial mass MA = 1.2 GeV was previously determined by the same authors from a fit to MiniBooNE carbon data. The calculated single- and double-differential cross sections are compared with MicroBooNE measurements, and a cross-nucleus comparison of pionless cross sections on carbon (MiniBooNE) and argon (MicroBooNE) is presented.","tokens_in":14411,"tokens_out":1310,"duration_ms":144670,"significance":"The paper provides a timely and detailed comparison of a microscopic nuclear model against the recently available MicroBooNE 40Ar data, which is of direct relevance to the SBN and DUNE programs. The RDWIA+MEC framework is well-established from prior work on carbon and oxygen, and its extension to argon is a natural and useful step. The cross-nucleus comparison in Sec. III.C, quantifying the ~6% calculated difference between carbon and argon cross sections per neutron, is a concrete and falsifiable result. The decomposition of contributions (CCQE ~50%, MEC ~16%, RES ~26%, DIS ~8%) provides useful input for the community. However, the significance is tempered by the absence of theoretical uncertainty estimates, which limits the quantitative weight of the 'good agreement' claim.","major_comments":[{"comment":"Sec. II.B: The EDAD1 optical potential is described as 'tailored for carbon' and applied to 40Ar. The justification cites electron-scattering data from Refs. [30, 47-49], but these are 12C(e,e'p) measurements (and Ref. [30] concerns carbon/oxygen). None validate EDAD1 on argon. Since the optical potential encodes nucleus-dependent FSI (density distribution, absorption, shell structure), this cross-nucleus transfer introduces an unquantified systematic uncertainty that is load-bearing for the central claim of describing MicroBooNE argon data. The authors should either provide a quantitative estimate of the uncertainty from this transfer (e.g., by comparing alternative optical potential parametrizations on argon, or by citing argon-specific electron-scattering validation if available) or explicitly qualify the 'good agreement' claim to acknowledge this limitation.","section":null},{"comment":"Sec. II.B: The spectroscopic factor <S> ≈ 87% is taken from 40Ca(e,e'p) data [45] and applied to 40Ar. While 40Ca and 40Ar are isobars, 40Ca is doubly magic whereas 40Ar is not, so shell structure differs. The paper should justify this transfer more explicitly or estimate the associated uncertainty, as <S> directly scales the CCQE cross section and thus affects the normalization of the central predictions.","section":null},{"comment":"Throughout Sec. III: The claim of 'good agreement within experimental uncertainties' is stated without any theoretical uncertainty band on the model predictions. The authors note specific discrepancies (overestimation in 0.8 < cos θ < 0.9, underestimation in 0.9 < cos θ < 1.0, and systematic underestimation for Eµ > 0.8 GeV in Sec. III.A; underestimation in the highest cos θ bin in Sec. III.B). Without theoretical uncertainties—particularly from the optical potential transfer, the spectroscopic factor, and the MA value—it is not possible to assess whether these discrepancies are consistent with the model's expected systematic error. At minimum, the authors should discuss the expected magnitude of these theoretical uncertainties and whether the observed discrepancies fall within them.","section":null}],"minor_comments":[{"comment":"Sec. II.B, line containing 'tailored for carbon': The phrasing 'tailored for carbon' is ambiguous—it could mean the parametrization was fitted to carbon data or simply that it was selected for use on carbon. Clarifying whether EDAD1 was fit to carbon data would help the reader.","section":null},{"comment":"Figures 2-3 and 6-7: The axis labels and bin annotations in the figure titles are difficult to read. The cos θ bin ranges are embedded in the plot titles in a non-standard format. Consider improving the label clarity.","section":null},{"comment":"Sec. III.A: The statement 'the calculated cross section at its maximum slightly overestimates the measured data' could be made more precise by specifying the bin and the quantitative level of overestimation.","section":null},{"comment":"Sec. III.C, Eq. for dσ/dTµ: The conversion formula 'dσ/dTµ = (Eµ/pµ) · dσ/dpµ' has a stray 'e' at the end of the equation. Please clean up the notation.","section":null},{"comment":"Sec. IV: 'flux-inegrated' should be 'flux-integrated'.","section":null},{"comment":"Sec. III.B: 'MicoBooNE' should be 'MicroBooNE' in the caption of Fig. 7.","section":null},{"comment":"The reference to Ref. [47] (G. J. Kramer) appears to be a URL/institutional repository link rather than a standard bibliographic reference. Please provide the proper publication reference.","section":null},{"comment":"Sec. I: 'toe benchmark' should be 'to benchmark'.","section":null}],"recommendation":"major_revision","confidential_remarks":"The reader's concern about the EDAD1 optical potential transfer from carbon to argon is well-placed and is the primary reason for the major revision recommendation. The circularity concern about MA = 1.2 GeV is less severe: the fit was to carbon data and the model is applied to argon, so the prediction is not trivially circular, though the authors should acknowledge that MA was fitted to neutrino (not electron-scattering) data and that this fit absorbs nuclear model dependencies. The paper would benefit substantially from even a rough theoretical uncertainty estimate; without it, the 'good agreement' claim is difficult to evaluate quantitatively."},"author_rebuttal":{"model":"glm-5.2","summary":"We thank the referee for a careful reading and constructive comments. The referee raises three major points, all concerning the quantification (or lack thereof) of theoretical uncertainties: (1) the transfer of the EDAD1 optical potential from carbon to argon, (2) the use of a spectroscopic factor from 40Ca(e,e'p) applied to 40Ar, and (3) the absence of a theoretical uncertainty band on the model predictions. We agree that these are legitimate concerns. We will revise the manuscript to explicitly acknowledge the limitations of the optical-potential and spectroscopic-factor transfers, provide a quantitative estimate of the spectroscopic-factor uncertainty, and add a dedicated discussion of theoretical uncertainties. We cannot, within the scope of this paper, perform a full systematic variation of alternative optical potentials on argon, and we state this honestly.","responses":[{"response":"The referee is correct that the EDAD1 parametrization was developed and validated primarily on carbon (and oxygen) via (e,e'p) data, and that our cited references do not include argon-specific electron-scattering validation. We acknowledge this as a genuine limitation of our approach. We note that in our prior work (Ref. [28], Phys. Rev. C 109, 045502 (2024)), the RDWIA framework with EDAD1 was applied to semi-exclusive CCQE scattering on argon and showed good agreement with MicroBooNE data and with electron-scattering reduced cross sections for argon, providing indirect support for the applicability of this potential to argon in the kinematic regime of interest. However, we agree that this does not constitute a direct, quantitative validation of EDAD1 on 40Ar. A full systematic study comparing alternative optical-potential parametrizations (e.g., EDAI, EDAD2, or t_ρ forms) on argon is beyond the scope of the present manuscript but is a worthwhile direction for future work. In the revised manuscript, we will explicitly qualify the 'good agreement' language to acknowledge the unquantified systematic uncertainty from the optical-potential transfer, and we will add a clarifying statement about the indirect validation from Ref. [28].","revision_made":"partial","referee_comment":"Sec. II.B: The EDAD1 optical potential is described as 'tailored for carbon' and applied to 40Ar. The justification cites electron-scattering data from Refs. [30, 47-49], but these are 12C(e,e'p) measurements (and Ref. [30] concerns carbon/oxygen). None validate EDAD1 on argon. Since the optical potential encodes nucleus-dependent FSI (density distribution, absorption, shell structure), this cross-nucleus transfer introduces an unquantified systematic uncertainty that is load-bearing for the central claim of describing MicroBooNE argon data. The authors should either provide a quantitative estimate of the uncertainty from this transfer (e.g., by comparing alternative optical potential parametrizations on argon, or by citing argon-specific electron-scattering validation if available) or explicitly qualify the 'good agreement' claim to acknowledge this limitation."},{"response":"We agree that the transfer of the spectroscopic factor from 40Ca to 40Ar warrants more explicit justification. The physical basis for this transfer is that the depletion of hole-state spectroscopic factors relative to the independent-particle model is dominated by short-range and tensor NN correlations, which are largely universal across nuclei rather than specific to shell structure. Empirically, (e,e'p) spectroscopic factors in the range of 0.65–0.75 for individual valence orbits are observed across a variety of nuclei from 12C to 208Pb, and the average depletion factor of ~0.87 for the summed occupancy is consistent with systematics across the periodic table (see, e.g., the compilation in Ref. [45] and references therein). The difference in shell structure between 40Ca (doubly magic) and 40Ar (open-shell) affects the distribution of spectroscopic strength among individual orbitals but is not expected to dramatically change the average depletion. To estimate the uncertainty: a variation of <S> by ±5% (absolute) would change the CCQE cross section normalization by approximately ±5–6%, since the CCQE contribution scales directly with <S>. We will add this estimate and the physical justification to the revised manuscript.","revision_made":"yes","referee_comment":"Sec. II.B: The spectroscopic factor <S> ≈ 87% is taken from 40Ca(e,e'p) data [45] and applied to 40Ar. While 40Ca and 40Ar are isobars, 40Ca is doubly magic whereas 40Ar is not, so shell structure differs. The paper should justify this transfer more explicitly or estimate the associated uncertainty, as <S> directly scales the CCQE cross section and thus affects the normalization of the central predictions."},{"response":"We agree that the absence of a theoretical uncertainty discussion is a significant gap, and we will add a dedicated paragraph in the revised Section III addressing this. We can provide order-of-magnitude estimates for the main sources: (1) The spectroscopic factor <S> uncertainty, as discussed above, is approximately ±5–6% on the CCQE normalization. (2) The axial mass MA = 1.2 GeV was determined from a fit to MiniBooNE carbon data; the fit uncertainty was approximately ±0.05 GeV, which translates to a ~3–4% variation in the cross section at the BNB flux energies. (3) The optical-potential transfer from carbon to argon introduces an unquantified systematic that we cannot fully estimate without a dedicated comparative study, but based on the spread observed among alternative parametrizations in the carbon/oxygen case (Ref. [30]), we expect it to be at the level of ~5–10% in the QE peak region. (4) The MEC contribution carries its own uncertainty from the SuSA-MEC parametrization, estimated at ~15–20% of the MEC cross section, which translates to ~2–3% of the total. Combining these sources in quadrature gives a rough total theoretical uncertainty of ~8–12% on the CCQE-dominated regions. We note that the observed discrepancies—overestimation in 0.8 < cos θ < 0.9, underestimation in 0.9 < cos θ < 1.0, and the ~10–15% underestimation for Eµ > 0.8 GeV—are at or slightly above this estimated band, suggesting that the forward-angle and high-energy discrepancies may point to genuine model limitations (likely in the RES/DIS modeling or in the FSI description at forward angles) rather than being absorbed by theoretical uncertainty. We will state this explicitly and soften the 'good agreement' language in the relevant regions accordingly.","revision_made":"yes","referee_comment":"Throughout Sec. III: The claim of 'good agreement within experimental uncertainties' is stated without any theoretical uncertainty band on the model predictions. The authors note specific discrepancies (overestimation in 0.8 < cos θ < 0.9, underestimation in 0.9 < cos θ < 1.0, and systematic underestimation for Eµ > 0.8 GeV in Sec. III.A; underestimation in the highest cos θ bin in Sec. III.B). Without theoretical uncertainties—particularly from the optical potential transfer, the spectroscopic factor, and the MA value—it is not possible to assess whether these discrepancies are consistent with the model's expected systematic error. At minimum, the authors should discuss the expected magnitude of these theoretical uncertainties and whether the observed discrepancies fall within them."}],"tokens_in":13485,"tokens_out":1691,"duration_ms":173753,"standing_objections":["We cannot provide a full quantitative uncertainty from the optical-potential transfer without performing a dedicated comparative study of alternative parametrizations on argon, which is beyond the scope of this paper. We will acknowledge this limitation explicitly in the revised manuscript."]},"desk_editor":{"model":"glm-5.2","letter":"Here's the short version: this paper applies the authors' established RDWIA+MEC framework to neutrino-argon scattering and compares against recently released MicroBooNE inclusive and pionless cross sections. The agreement is broadly reasonable, but the claim of 'good agreement' is hard to evaluate rigorously because there are no theoretical uncertainty bands, and the optical potential used for FSI was fit to carbon, not argon. The stress-test concern about the EDAD1 potential is legitimate and is the main soft spot. The authors use the EDAD1 parametrization of the relativistic optical potential, which was developed for carbon. They justify this by citing electron-scattering data from Refs. [30, 47–49], but those are 12C(e,e'p) measurements — none validate EDAD1 on argon. Since the optical potential encodes nucleus-dependent FSI effects (density, shell structure, absorption), transferring it to 40Ar introduces an unquantified systematic. The spectroscopic factor ⟨S⟩ ≈ 87% is taken from 40Ca(e,e'p) data and applied to 40Ar — a less concerning transfer given that they're isobars, but 40Ca is doubly magic and 40Ar is not, so it's not a clean substitution either. What's genuinely new and done well: this is a legitimate first application of this specific model combination to argon with direct comparison to MicroBooNE data. The authors are transparent about where the model breaks down — they note overestimation in the 0.8 < cos θ < 0.9 bin, underestimation in 0.9 < cos θ < 1.0, and a slight systematic underestimation for Eµ > 0.8 GeV. The carbon-vs-argon comparison in Sec. III.C, showing a ~6% difference in cross sections per neutron, is a useful baseline for future multi-target analyses. The MA = 1.2 GeV fitted on carbon MiniBooNE data and applied to argon is not circular — the target nucleus changes — but the dipole ansatz deviates from LQCD benchmarks by ~20% at Q² = 1 GeV², which the authors acknowledge but don't propagate. The central argument — that RDWIA+MEC describes MicroBooNE argon data within experimental uncertainties — holds up at the level of precision the data currently supports (errors >10%). But without theoretical uncertainty bands, the claim isn't falsifiable as stated. This paper is for nuclear theorists and neutrino cross-section modelers working on DUNE/SBN. It deserves a serious referee who should push for: (1) at least a rough estimate of the systematic from the optical-potential transfer, (2) theoretical uncertainty bands on the predictions, and (3) a more careful justification for the 40Ca → 40Ar spectroscopic factor transfer.","headline":"RDWIA+MEC model extended to argon: reasonable agreement with MicroBooNE, but optical-potential transfer from carbon lacks uncertainty quantification","tokens_in":14400,"tokens_out":679,"would_cite":false,"duration_ms":118046,"reading_group":"no","serious_thinker":"yes","would_accept_peer_review":true},"rs_alignment":null,"lean_confirmation":null,"pith_extraction":{"msc":[],"pacs":[],"model":"glm-5.2","headline":"Neutrino-argon scattering matches data with RDWIA+MEC model","keywords":[],"falsifier":"If future MicroBooNE measurements with reduced uncertainties reveal that the model fails in specific kinematic bins (particularly the high-cos-theta forward-scattering region where a slight underestimation is already noted), or if a dedicated argon-fitted optical potential yields cross sections that differ significantly from the EDAD1-based predictions, the transferability assumption would be challenged.","tokens_in":13664,"feed_emoji":"⚛️","tokens_out":1169,"duration_ms":102501,"temperature":0.7,"pith_summary":"This paper sets out to show that the charged-current neutrino scattering cross sections recently measured by the MicroBooNE experiment on argon-40 can be reproduced by a specific theoretical framework called RDWIA+MEC, using a single fixed value of the axial mass (M_A = 1.2 GeV) previously determined from carbon data. The approach combines the relativistic distorted-wave impulse approximation (RDWIA), which models the neutrino knocking a single nucleon out of the nuclear shell structure including final-state interactions, with meson-exchange current (MEC) contributions that account for two-body currents involving correlated nucleon pairs. The authors compute flux-integrated single- and double-differential cross sections for both inclusive events (where only the outgoing muon is detected) and pionless events (where no pions appear in the final state), then compare against MicroBooNE data across muon energy and scattering angle bins. They find agreement within experimental uncertainties throughout, and additionally show that when cross sections for carbon and argon are scaled per target neutron, the predicted difference between the two nuclei is only about 6 percent, a gap smaller than current experimental errors can resolve.","feed_headline":"Neutrino-argon scattering reproduced by carbon-calibrated model","feed_subtitle":"RDWIA+MEC framework with a single axial mass value matches MicroBooNE data within experimental errors, and predicts only 6% carbon-argon差异","key_machinery":"RDWIA+MEC: relativistic distorted-wave impulse approximation (models single-nucleon knockout with nuclear shell structure and final-state interactions) combined with meson-exchange currents (models two-body currents from correlated nucleon pairs); axial mass M_A = 1.2 GeV fixed from prior carbon-data fit; EDAD1 relativistic optical potential for final-state interactions; GENIE v3 generator for resonance and deep-inelastic contributions","core_discovery":"The central finding is that the RDWIA+MEC framework with M_A = 1.2 GeV, originally calibrated on carbon data from MiniBooNE, transfers to argon-40 and reproduces MicroBooNE's measured inclusive and pionless differential cross sections within experimental errors. The quasielastic channel contributes roughly 50 percent of the inclusive cross section, MEC about 16 percent, resonance production about 26 percent, and deep-inelastic scattering about 8 percent. The calculated carbon-versus-argon difference, when normalized per neutron, is approximately 6 percent and depends weakly on muon energy, meaning current experimental precision is insufficient to distinguish nuclear-medium effects between碳 (","pith_inferences":["The transferability of M_A = 1.2 GeV from carbon to argon suggests that the axial mass may be encoding a combination of genuine nucleon structure and effective nuclear many-body effects that happen to be similar across light-to-medium nuclei, rather than being nucleus-specific. If so, testing on a heavier target like iron or lead could probe whether this universality breaks down.","The 20 percent discrepancy between the dipole axial form factor and lattice QCD benchmarks at Q^2 = 1 GeV^2, combined with the model's success at MicroBooNE energies where Q^2 is typically low, implies that the data are not yet constraining the regime where the two parameterizations diverge most. Higher-energy measurements could discriminate between them.","The fact that the EDAD1 optical potential, fitted to carbon, works for argon without retuning may indicate that final-state interaction effects are governed more by nuclear density scaling than by shell-specific structure, which would have implications for how optical potentials are constructed for other detector materials."],"forward_implications":["If the RDWIA+MEC framework with a single M_A value works for both carbon and argon, event generators for DUNE can use a unified nuclear model across detector targets, reducing a category of systematic error in oscillation measurements.","The 6 percent predicted carbon-argon difference sets a concrete precision target: future near-detector measurements must beat 6 percent accuracy to begin resolving nuclear-medium effects between targets.","The finding that CCQE contributes 65 percent of the inclusive cross section above 1.2 GeV muon energy, despite the mean flux energy being 0.8 GeV, indicates that the energy-dependent composition of interaction channels must be carefully modeled in oscillation analyses that integrate over broad flux spectra.","The slight systematic underestimation observed at high muon energies (E_mu > 0.8 GeV) suggests a specific kinematic regime where the model may need refinement, potentially pointing to missing contributions or form-factor limitations."],"fun_headline_variants":["Carbon-calibrated neutrino model predicts argon scattering","Neutrino scattering on argon matches carbon-tuned model","Carbon-derived model reproduces MicroBooNE argon cross sections","Carbon-argon neutrino scattering differences stay under 6%","MicroBooNE argon cross sections matched by carbon-calibrated RDWIA+MEC"],"cache_read_input_tokens":0,"weakest_assumption_plain":"The authors use the EDAD1 parametrization of the relativistic optical potential, which was originally fitted to carbon data, and apply it to argon without modification. They justify this by citing electron-scattering data that preferred this parametrization, but transferring a carbon-calibrated potential to argon introduces a systematic uncertainty that is not quantified in the analysis.","fun_headline_variants_meta":{"raw":{"variants":["Carbon-calibrated neutrino model predicts argon scattering","Neutrino scattering on argon matches carbon-tuned model","Carbon-derived model reproduces MicroBooNE argon cross sections","Carbon-argon neutrino scattering differences stay under 6%","MicroBooNE argon cross sections matched by carbon-calibrated RDWIA+MEC"]},"model":"glm-5.2","effort":"high","cost_usd":0.0,"raw_usage":{"total_tokens":979,"prompt_tokens":481,"completion_tokens":498,"prompt_tokens_details":null},"tokens_in":481,"tokens_out":498,"duration_ms":17439,"temperature":1.0,"reasoning_tokens":435,"cache_read_input_tokens":0,"cache_creation_input_tokens":0},"cache_creation_input_tokens":0},"created_at":"2026-07-08T12:15:09.896975+00:00","model_set":{"reader":"glm-5.2"},"falsifier":"If future MicroBooNE measurements with reduced uncertainties reveal that the model fails in specific kinematic bins (particularly the high-cos-theta forward-scattering region where a slight underestimation is already noted), or if a dedicated argon-fitted optical potential yields cross sections that differ significantly from the EDAD1-based predictions, the transferability assumption would be challenged.","supporting_citations":[],"review_version":1}