{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:TC3HM3FO63DCQOWNB4ZPVX44A3","short_pith_number":"pith:TC3HM3FO","schema_version":"1.0","canonical_sha256":"98b6766caef6c6283acd0f32fadf9c06c6460be3b0347313a809b3c6e752fb0d","source":{"kind":"arxiv","id":"hep-ph/0212147","version":3},"attestation_state":"computed","paper":{"title":"Solar Neutrinos Before and After KamLAND","license":"","headline":"","cross_cats":["astro-ph","hep-ex","nucl-ex","nucl-th"],"primary_cat":"hep-ph","authors_text":"Carlos Pena-Garay, John N. Bahcall, M. C. Gonzalez-Garcia","submitted_at":"2002-12-11T20:33:29Z","abstract_excerpt":"We use the recently reported KamLAND measurements on oscillations of reactor anti-neutrinos, together with the data of previously reported solar neutrino experiments, to show that: (1) the total 8B neutrino flux emitted by the Sun is 1.00(1.0 \\pm 0.06) of the standard solar model (BP00) predicted flux, (2) the KamLAND measurements reduce the area of the globally allowed oscillation regions that must be explored in model fitting by six orders of magnitude in the Delta m^2-tan^2 theta plane, (3) LMA is now the unique oscillation solution to a CL of 4.7sigma, (4) maximal mixing is disfavored at 3"},"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":"hep-ph/0212147","kind":"arxiv","version":3},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2002-12-11T20:33:29Z","cross_cats_sorted":["astro-ph","hep-ex","nucl-ex","nucl-th"],"title_canon_sha256":"5b7c530907a60b8d43b4a9216e1111f4db506732b3cab7a8fd2e81334c8e00fb","abstract_canon_sha256":"c09a78fd5c042ddb6714f52c95521185ca365c529eed325ba8c741046258b982"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:21:00.303287Z","signature_b64":"pwXMprFMRyMBYOnqi4m2OnwjAbYvaoueOKf4EKkEWGRwOy75VeS6s+BEvaq+wvCnNZR3fhSxg7pPkS8AEBf1Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"98b6766caef6c6283acd0f32fadf9c06c6460be3b0347313a809b3c6e752fb0d","last_reissued_at":"2026-07-04T17:21:00.302949Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:21:00.302949Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Solar Neutrinos Before and After KamLAND","license":"","headline":"","cross_cats":["astro-ph","hep-ex","nucl-ex","nucl-th"],"primary_cat":"hep-ph","authors_text":"Carlos Pena-Garay, John N. Bahcall, M. C. Gonzalez-Garcia","submitted_at":"2002-12-11T20:33:29Z","abstract_excerpt":"We use the recently reported KamLAND measurements on oscillations of reactor anti-neutrinos, together with the data of previously reported solar neutrino experiments, to show that: (1) the total 8B neutrino flux emitted by the Sun is 1.00(1.0 \\pm 0.06) of the standard solar model (BP00) predicted flux, (2) the KamLAND measurements reduce the area of the globally allowed oscillation regions that must be explored in model fitting by six orders of magnitude in the Delta m^2-tan^2 theta plane, (3) LMA is now the unique oscillation solution to a CL of 4.7sigma, (4) maximal mixing is disfavored at 3"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0212147","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/hep-ph/0212147/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"hep-ph/0212147","created_at":"2026-07-04T17:21:00.303002+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0212147v3","created_at":"2026-07-04T17:21:00.303002+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0212147","created_at":"2026-07-04T17:21:00.303002+00:00"},{"alias_kind":"pith_short_12","alias_value":"TC3HM3FO63DC","created_at":"2026-07-04T17:21:00.303002+00:00"},{"alias_kind":"pith_short_16","alias_value":"TC3HM3FO63DCQOWN","created_at":"2026-07-04T17:21:00.303002+00:00"},{"alias_kind":"pith_short_8","alias_value":"TC3HM3FO","created_at":"2026-07-04T17:21:00.303002+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.24310","citing_title":"Non-adiabatic transitions in the density matrix formalism","ref_index":11,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TC3HM3FO63DCQOWNB4ZPVX44A3","json":"https://pith.science/pith/TC3HM3FO63DCQOWNB4ZPVX44A3.json","graph_json":"https://pith.science/api/pith-number/TC3HM3FO63DCQOWNB4ZPVX44A3/graph.json","events_json":"https://pith.science/api/pith-number/TC3HM3FO63DCQOWNB4ZPVX44A3/events.json","paper":"https://pith.science/paper/TC3HM3FO"},"agent_actions":{"view_html":"https://pith.science/pith/TC3HM3FO63DCQOWNB4ZPVX44A3","download_json":"https://pith.science/pith/TC3HM3FO63DCQOWNB4ZPVX44A3.json","view_paper":"https://pith.science/paper/TC3HM3FO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0212147&json=true","fetch_graph":"https://pith.science/api/pith-number/TC3HM3FO63DCQOWNB4ZPVX44A3/graph.json","fetch_events":"https://pith.science/api/pith-number/TC3HM3FO63DCQOWNB4ZPVX44A3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TC3HM3FO63DCQOWNB4ZPVX44A3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TC3HM3FO63DCQOWNB4ZPVX44A3/action/storage_attestation","attest_author":"https://pith.science/pith/TC3HM3FO63DCQOWNB4ZPVX44A3/action/author_attestation","sign_citation":"https://pith.science/pith/TC3HM3FO63DCQOWNB4ZPVX44A3/action/citation_signature","submit_replication":"https://pith.science/pith/TC3HM3FO63DCQOWNB4ZPVX44A3/action/replication_record"}},"created_at":"2026-07-04T17:21:00.303002+00:00","updated_at":"2026-07-04T17:21:00.303002+00:00"}