{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:DGQPKMLWO4TXLLAQM7OMBHBPHG","short_pith_number":"pith:DGQPKMLW","schema_version":"1.0","canonical_sha256":"19a0f53176772775ac1067dcc09c2f39bddaf92e46785ce37b027f4d715a78d5","source":{"kind":"arxiv","id":"1206.3871","version":1},"attestation_state":"computed","paper":{"title":"Reaction rates for the s-process neutron source 22Ne+{\\alpha}","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex"],"primary_cat":"astro-ph.SR","authors_text":"Amanda I. Karakas, Christian Iliadis, Richard Longland","submitted_at":"2012-06-18T09:55:57Z","abstract_excerpt":"The 22Ne({\\alpha},n)25Mg reaction is an important source of neutrons for the s-process. In massive stars responsible for the weak component of the s-process, 22Ne({\\alpha},n)25Mg is the dominant source of neutrons, both during core helium burning and in shell carbon burning. For the main s-process component produced in Asymptotic Giant Branch (AGB) stars, the 13C({\\alpha},n)16O reaction is the dominant source of neutrons operating during the interpulse period, with the 22Ne+{\\alpha} source affecting mainly the s-process branchings during a thermal pulse. Rate uncertainties in the competing 22N"},"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":"1206.3871","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-06-18T09:55:57Z","cross_cats_sorted":["nucl-ex"],"title_canon_sha256":"c66b84633b834dc2163d84ec04a8c14254a258361b643c32e8fb10b3da641f82","abstract_canon_sha256":"e9618f4161b80efd081bd5492d96db594f39f7b8a74eb58262fc884172cf73f8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:56:51.803921Z","signature_b64":"CL7frEfV4XoDvjDgc/eMvFuXZoFuBRVKLJMrZnk6vH/3E8rTar8oPDykQkwdQ4XbvukH5TV00ynINh7TMHYJBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"19a0f53176772775ac1067dcc09c2f39bddaf92e46785ce37b027f4d715a78d5","last_reissued_at":"2026-05-18T01:56:51.803405Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:56:51.803405Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Reaction rates for the s-process neutron source 22Ne+{\\alpha}","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex"],"primary_cat":"astro-ph.SR","authors_text":"Amanda I. Karakas, Christian Iliadis, Richard Longland","submitted_at":"2012-06-18T09:55:57Z","abstract_excerpt":"The 22Ne({\\alpha},n)25Mg reaction is an important source of neutrons for the s-process. In massive stars responsible for the weak component of the s-process, 22Ne({\\alpha},n)25Mg is the dominant source of neutrons, both during core helium burning and in shell carbon burning. For the main s-process component produced in Asymptotic Giant Branch (AGB) stars, the 13C({\\alpha},n)16O reaction is the dominant source of neutrons operating during the interpulse period, with the 22Ne+{\\alpha} source affecting mainly the s-process branchings during a thermal pulse. Rate uncertainties in the competing 22N"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1206.3871","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":"1206.3871","created_at":"2026-05-18T01:56:51.803490+00:00"},{"alias_kind":"arxiv_version","alias_value":"1206.3871v1","created_at":"2026-05-18T01:56:51.803490+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1206.3871","created_at":"2026-05-18T01:56:51.803490+00:00"},{"alias_kind":"pith_short_12","alias_value":"DGQPKMLWO4TX","created_at":"2026-05-18T12:27:04.183437+00:00"},{"alias_kind":"pith_short_16","alias_value":"DGQPKMLWO4TXLLAQ","created_at":"2026-05-18T12:27:04.183437+00:00"},{"alias_kind":"pith_short_8","alias_value":"DGQPKMLW","created_at":"2026-05-18T12:27:04.183437+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/DGQPKMLWO4TXLLAQM7OMBHBPHG","json":"https://pith.science/pith/DGQPKMLWO4TXLLAQM7OMBHBPHG.json","graph_json":"https://pith.science/api/pith-number/DGQPKMLWO4TXLLAQM7OMBHBPHG/graph.json","events_json":"https://pith.science/api/pith-number/DGQPKMLWO4TXLLAQM7OMBHBPHG/events.json","paper":"https://pith.science/paper/DGQPKMLW"},"agent_actions":{"view_html":"https://pith.science/pith/DGQPKMLWO4TXLLAQM7OMBHBPHG","download_json":"https://pith.science/pith/DGQPKMLWO4TXLLAQM7OMBHBPHG.json","view_paper":"https://pith.science/paper/DGQPKMLW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1206.3871&json=true","fetch_graph":"https://pith.science/api/pith-number/DGQPKMLWO4TXLLAQM7OMBHBPHG/graph.json","fetch_events":"https://pith.science/api/pith-number/DGQPKMLWO4TXLLAQM7OMBHBPHG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DGQPKMLWO4TXLLAQM7OMBHBPHG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DGQPKMLWO4TXLLAQM7OMBHBPHG/action/storage_attestation","attest_author":"https://pith.science/pith/DGQPKMLWO4TXLLAQM7OMBHBPHG/action/author_attestation","sign_citation":"https://pith.science/pith/DGQPKMLWO4TXLLAQM7OMBHBPHG/action/citation_signature","submit_replication":"https://pith.science/pith/DGQPKMLWO4TXLLAQM7OMBHBPHG/action/replication_record"}},"created_at":"2026-05-18T01:56:51.803490+00:00","updated_at":"2026-05-18T01:56:51.803490+00:00"}