{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:6O42YBD3QLX3SNZEM7SSYZC2EB","short_pith_number":"pith:6O42YBD3","schema_version":"1.0","canonical_sha256":"f3b9ac047b82efb9372467e52c645a204f439f59dede591a9a7017bea45737b3","source":{"kind":"arxiv","id":"nucl-th/0201062","version":3},"attestation_state":"computed","paper":{"title":"Neutrino-deuteron reactions at solar neutrino energies","license":"","headline":"","cross_cats":["astro-ph","hep-ph"],"primary_cat":"nucl-th","authors_text":"2), (2) University of South Carolina), F. Myhrer (2), K. Kubodera (2) ((1) Osaka University, S. Ando (2), S. Nakamura (1), T. Sato (1, T.-S. Park (2), V. Gudkov (2)","submitted_at":"2002-01-23T13:46:23Z","abstract_excerpt":"In interpreting the SNO experiments, very accurate estimates of the \\nu d reaction cross sections are of great importance. We improve the previous estimates of our group by updating some of its inputs and by taking into account the results of a recent effective-field-theoretical calculation. The new cross sections are slightly (\\sim 1%) larger than the previously reported values. We present arguments that lead to the conclusion that it is reasonable to assign 1% uncertainty to the \\nu d cross sections reported here."},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"nucl-th/0201062","kind":"arxiv","version":3},"metadata":{"license":"","primary_cat":"nucl-th","submitted_at":"2002-01-23T13:46:23Z","cross_cats_sorted":["astro-ph","hep-ph"],"title_canon_sha256":"c8654768bb02652d8b8d30e2002b71f37526774ff4efa2821893bfb1228ee39a","abstract_canon_sha256":"b7bc732d323704a72012bbc648234df31f2888adeaafbc6440b564e2eed72a4c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:35:32.515942Z","signature_b64":"BYo0Nsau/b7UPbj3ym0lZe6Rr25JV70LHrjQFSmkBsMuJs8VJ9RUY2SEji9zXsJL4kfm2zWgGnmKDX3RLCKxDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f3b9ac047b82efb9372467e52c645a204f439f59dede591a9a7017bea45737b3","last_reissued_at":"2026-05-18T02:35:32.515594Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:35:32.515594Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutrino-deuteron reactions at solar neutrino energies","license":"","headline":"","cross_cats":["astro-ph","hep-ph"],"primary_cat":"nucl-th","authors_text":"2), (2) University of South Carolina), F. Myhrer (2), K. Kubodera (2) ((1) Osaka University, S. Ando (2), S. Nakamura (1), T. Sato (1, T.-S. Park (2), V. Gudkov (2)","submitted_at":"2002-01-23T13:46:23Z","abstract_excerpt":"In interpreting the SNO experiments, very accurate estimates of the \\nu d reaction cross sections are of great importance. We improve the previous estimates of our group by updating some of its inputs and by taking into account the results of a recent effective-field-theoretical calculation. The new cross sections are slightly (\\sim 1%) larger than the previously reported values. We present arguments that lead to the conclusion that it is reasonable to assign 1% uncertainty to the \\nu d cross sections reported here."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"nucl-th/0201062","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"nucl-th/0201062","created_at":"2026-05-18T02:35:32.515646+00:00"},{"alias_kind":"arxiv_version","alias_value":"nucl-th/0201062v3","created_at":"2026-05-18T02:35:32.515646+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.nucl-th/0201062","created_at":"2026-05-18T02:35:32.515646+00:00"},{"alias_kind":"pith_short_12","alias_value":"6O42YBD3QLX3","created_at":"2026-05-18T12:25:50.845339+00:00"},{"alias_kind":"pith_short_16","alias_value":"6O42YBD3QLX3SNZE","created_at":"2026-05-18T12:25:50.845339+00:00"},{"alias_kind":"pith_short_8","alias_value":"6O42YBD3","created_at":"2026-05-18T12:25:50.845339+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2602.15960","citing_title":"Novel Constraints on Spin-Dependent Light Dark Matter Scattering","ref_index":39,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6O42YBD3QLX3SNZEM7SSYZC2EB","json":"https://pith.science/pith/6O42YBD3QLX3SNZEM7SSYZC2EB.json","graph_json":"https://pith.science/api/pith-number/6O42YBD3QLX3SNZEM7SSYZC2EB/graph.json","events_json":"https://pith.science/api/pith-number/6O42YBD3QLX3SNZEM7SSYZC2EB/events.json","paper":"https://pith.science/paper/6O42YBD3"},"agent_actions":{"view_html":"https://pith.science/pith/6O42YBD3QLX3SNZEM7SSYZC2EB","download_json":"https://pith.science/pith/6O42YBD3QLX3SNZEM7SSYZC2EB.json","view_paper":"https://pith.science/paper/6O42YBD3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=nucl-th/0201062&json=true","fetch_graph":"https://pith.science/api/pith-number/6O42YBD3QLX3SNZEM7SSYZC2EB/graph.json","fetch_events":"https://pith.science/api/pith-number/6O42YBD3QLX3SNZEM7SSYZC2EB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6O42YBD3QLX3SNZEM7SSYZC2EB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6O42YBD3QLX3SNZEM7SSYZC2EB/action/storage_attestation","attest_author":"https://pith.science/pith/6O42YBD3QLX3SNZEM7SSYZC2EB/action/author_attestation","sign_citation":"https://pith.science/pith/6O42YBD3QLX3SNZEM7SSYZC2EB/action/citation_signature","submit_replication":"https://pith.science/pith/6O42YBD3QLX3SNZEM7SSYZC2EB/action/replication_record"}},"created_at":"2026-05-18T02:35:32.515646+00:00","updated_at":"2026-05-18T02:35:32.515646+00:00"}