{"paper":{"title":"Gallium Solar Neutrino Experiments: Absorption Cross sections, Neutrino spectra, and Predicted Event Rates","arxiv_id":"hep-ph/9710491","primary_cat":"hep-ph","submitted_at":"1997-10-28T02:09:15+00:00","version_compiled":"v1"},"notice":"Every quoted sentence is the authors' text from the arXiv listing abstract. Labels and probabilities are the outputs of classifier-1.13-20260917 on the question bank abstract-p1-20260923, exactly as returned. No sentence in this record was written by a language model.","schema":"pith.compiled-record/v0","status":"compiled","abstract":{"source":"arXiv listing abstract v1","sentences":[{"i":0,"p":0.81,"id":"s0","own":true,"role":"contribution","text":"Neutrino absorption cross sections for 71Ga are calculated for all solar neutrino sources with standard energy spectra, and for laboratory sources of 51Cr and 37Ar; the calculations include, where appropriate, the thermal energy of fusing solar ions and use improved nuclear and atomic data.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.91,"main_claim_p":0.07,"quantitative":false,"quantitative_p":0.34,"role_probabilities":{"gap":0.0,"method":0.19,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.81,"interpretation":0.0}},{"i":1,"p":1.0,"id":"s1","own":false,"role":"result","text":"The ratio, R, of measured (in GALLEX and SAGE) to calculated 51Cr capture rate is R = 0.95 +/- 0.07 (exp)} + ^{+0.04}_{-0.03} (theory).","hedge":{"p":1.0,"label":"asserted"},"own_p":0.44,"main_claim_p":0.25,"quantitative":true,"quantitative_p":0.99,"role_probabilities":{"gap":0.0,"method":0.0,"result":1.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.0}},{"i":2,"p":0.6,"id":"s2","own":true,"role":"method","text":"Cross sections are also calculated for specific neutrino energies chosen so that a spline fit determines accurately the event rates in a gallium detector even if new physics changes the energy spectrum of solar neutrinos.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.9,"main_claim_p":0.07,"quantitative":false,"quantitative_p":0.05,"role_probabilities":{"gap":0.0,"method":0.6,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.4,"interpretation":0.0}},{"i":3,"p":0.44,"id":"s3","own":true,"role":"contribution","text":"Theoretical uncertainties are estimated for cross sections at specific energies and for standard neutrino energy spectra.","hedge":{"p":0.97,"label":"asserted"},"own_p":0.86,"main_claim_p":0.05,"quantitative":false,"quantitative_p":0.05,"role_probabilities":{"gap":0.0,"method":0.33,"result":0.12,"background":0.0,"limitation":0.11,"future_work":0.0,"contribution":0.44,"interpretation":0.0}},{"i":4,"p":0.74,"id":"s4","own":true,"role":"contribution","text":"Standard energy spectra are presented for pp and CNO neutrino sources in the appendices.","hedge":{"p":0.98,"label":"asserted"},"own_p":0.54,"main_claim_p":0.02,"quantitative":false,"quantitative_p":0.22,"role_probabilities":{"gap":0.0,"method":0.16,"result":0.08,"background":0.02,"limitation":0.0,"future_work":0.0,"contribution":0.74,"interpretation":0.0}},{"i":5,"p":0.86,"id":"s5","own":false,"role":"background","text":"Neutrino fluxes predicted by standard solar models, corrected for diffusion, have been in the range 120 SNU to 141 SNU since 1968.","hedge":{"p":0.98,"label":"asserted"},"own_p":0.12,"main_claim_p":0.1,"quantitative":true,"quantitative_p":0.99,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.14,"background":0.86,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.0}}]},"compiled":{"main_claim":{"p":0.9,"text":"The ratio, R, of measured (in GALLEX and SAGE) to calculated 51Cr capture rate is R = 0.95 +/- 0.07 (exp)} + ^{+0.04}_{-0.03} (theory).","location":"abstract s1","hedge_strength":{"p":1.0,"label":"asserted"}},"provenance":{"route":{"via":"OpenRouter","model":"classifier-1.13","endpoint":"https://openrouter.ai/api/v1/systemone","provider":"TypeSafe"},"packing":"one request per paper","requests":1,"input_tokens":5122,"cost_usd_reported":0.000215},"compiled_at":"2026-09-23","bank_version":"abstract-p1-20260923","model_version":"classifier-1.13-20260917","abstract_states":{"claims_first":0.03,"states_limitation":0.4,"human_participants":0.02,"controlled_comparison":0.2,"randomized_assignment":0.01,"states_quantitative_result":0.98,"compares_with_prior_results":0.81,"mentions_code_or_data_availability":0.03},"evidential_basis":{"p":0.95,"value":"simulation or computation","probabilities":{"argument":0.0,"literature":0.0,"proof_or_derivation":0.0,"analysis_of_existing_data":0.05,"observation_or_experiment":0.0,"simulation_or_computation":0.95}},"contribution_type":{"p":0.79,"value":"theoretical result","probabilities":{"review":0.0,"method_or_tool":0.07,"empirical_study":0.0,"simulation_study":0.09,"theoretical_result":0.79,"dataset_or_benchmark":0.05,"position_or_commentary":0.0}},"contribution_statement":{"p":0.58,"text":"Neutrino absorption cross sections for 71Ga are calculated for all solar neutrino sources with standard energy spectra, and for laboratory sources of 51Cr and 37Ar; 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