{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1993:VQOHLXVNFVGUZ3IAJT446AXGC6","short_pith_number":"pith:VQOHLXVN","schema_version":"1.0","canonical_sha256":"ac1c75dead2d4d4ced004cf9cf02e6178d7226e951da15470d783529a948d841","source":{"kind":"arxiv","id":"astro-ph/9310026","version":1},"attestation_state":"computed","paper":{"title":"Alpha Clustering and the stellar nucleosynthesis of carbon","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"G. Staudt, H. Abele, H. Krauss, H. Oberhummer, K. Gr\\\"un, P. Mohr, T. Rauscher","submitted_at":"1993-10-14T08:13:42Z","abstract_excerpt":"The astrophysical S--factor and reaction rates for the triple--alpha process are calculated in the direct--capture model. It is shown that the stellar carbon production is extremely sensitive to small variations in the N--N interaction."},"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":"astro-ph/9310026","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1993-10-14T08:13:42Z","cross_cats_sorted":[],"title_canon_sha256":"87db025845cc46fe1291794e35770bb7d1a1c3641b0597dcbe6bfa9bbaf793f2","abstract_canon_sha256":"23503f0bbda6c6f936bcc224ab8e10742bc4e8971ed4f5c754745d0eed4612e7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:40:26.496413Z","signature_b64":"6D8MCF7qP6Auiqvv+ewKwyPRtiVtxE9+V+9/SfQ+yMAARPtt6Wcw6/OITsfqgo7duI9usJD5oC6CQFikbkGvBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ac1c75dead2d4d4ced004cf9cf02e6178d7226e951da15470d783529a948d841","last_reissued_at":"2026-05-18T01:40:26.495906Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:40:26.495906Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Alpha Clustering and the stellar nucleosynthesis of carbon","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"G. Staudt, H. Abele, H. Krauss, H. Oberhummer, K. Gr\\\"un, P. Mohr, T. Rauscher","submitted_at":"1993-10-14T08:13:42Z","abstract_excerpt":"The astrophysical S--factor and reaction rates for the triple--alpha process are calculated in the direct--capture model. It is shown that the stellar carbon production is extremely sensitive to small variations in the N--N interaction."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9310026","kind":"arxiv","version":1},"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":"astro-ph/9310026","created_at":"2026-05-18T01:40:26.495990+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9310026v1","created_at":"2026-05-18T01:40:26.495990+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9310026","created_at":"2026-05-18T01:40:26.495990+00:00"},{"alias_kind":"pith_short_12","alias_value":"VQOHLXVNFVGU","created_at":"2026-05-18T12:25:47.102015+00:00"},{"alias_kind":"pith_short_16","alias_value":"VQOHLXVNFVGUZ3IA","created_at":"2026-05-18T12:25:47.102015+00:00"},{"alias_kind":"pith_short_8","alias_value":"VQOHLXVN","created_at":"2026-05-18T12:25:47.102015+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VQOHLXVNFVGUZ3IAJT446AXGC6","json":"https://pith.science/pith/VQOHLXVNFVGUZ3IAJT446AXGC6.json","graph_json":"https://pith.science/api/pith-number/VQOHLXVNFVGUZ3IAJT446AXGC6/graph.json","events_json":"https://pith.science/api/pith-number/VQOHLXVNFVGUZ3IAJT446AXGC6/events.json","paper":"https://pith.science/paper/VQOHLXVN"},"agent_actions":{"view_html":"https://pith.science/pith/VQOHLXVNFVGUZ3IAJT446AXGC6","download_json":"https://pith.science/pith/VQOHLXVNFVGUZ3IAJT446AXGC6.json","view_paper":"https://pith.science/paper/VQOHLXVN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/9310026&json=true","fetch_graph":"https://pith.science/api/pith-number/VQOHLXVNFVGUZ3IAJT446AXGC6/graph.json","fetch_events":"https://pith.science/api/pith-number/VQOHLXVNFVGUZ3IAJT446AXGC6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VQOHLXVNFVGUZ3IAJT446AXGC6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VQOHLXVNFVGUZ3IAJT446AXGC6/action/storage_attestation","attest_author":"https://pith.science/pith/VQOHLXVNFVGUZ3IAJT446AXGC6/action/author_attestation","sign_citation":"https://pith.science/pith/VQOHLXVNFVGUZ3IAJT446AXGC6/action/citation_signature","submit_replication":"https://pith.science/pith/VQOHLXVNFVGUZ3IAJT446AXGC6/action/replication_record"}},"created_at":"2026-05-18T01:40:26.495990+00:00","updated_at":"2026-05-18T01:40:26.495990+00:00"}