{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:Z5WNC7B2NH4JOW5ESQNSWWUIAR","short_pith_number":"pith:Z5WNC7B2","schema_version":"1.0","canonical_sha256":"cf6cd17c3a69f8975ba4941b2b5a88047c1a7229bab65550ef340677349160fa","source":{"kind":"arxiv","id":"1402.0793","version":1},"attestation_state":"computed","paper":{"title":"Astrophysical weak-interaction rates for selected $A=20$ and $A=24$ nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"C. Sullivan, G. Mart\\'inez-Pinedo, K. Langanke, R. G. T. Zegers, Y. H. Lam","submitted_at":"2014-02-04T16:42:51Z","abstract_excerpt":"We have evaluated the electron capture rates on $^{20}$Ne, $^{20}$F, $^{24}$Mg, $^{24}$Na and the $\\beta$ decay rates for $^{20}$F and $^{24}$Na at temperature and density conditions relevant for the late-evolution stages of stars with $M=8$-12 M$_\\odot$. The rates are based on recent experimental data and large-scale shell model calculations. We show that the electron capture rates on $^{20}$Ne, $^{24}$Mg and the $^{20}$F, $^{24}$Na $\\beta$-decay rates are based on data in this astrophysical range, except for the capture rate on $^{20}$Ne, which we predict to have a dominating contribution fr"},"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":"1402.0793","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-02-04T16:42:51Z","cross_cats_sorted":["nucl-ex","nucl-th"],"title_canon_sha256":"b9c1ff5ae7a1e82e5118d6412e7cf6a67a3384ec9bb9b848fcbb2fbb7ccaa1a2","abstract_canon_sha256":"d105a20438e35c6d2f0f91c3867d4f3ebcda3ea2ca52dd2db0de51d6dc02c18c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:44:47.906405Z","signature_b64":"btHxnhOWmx6E1CKjWgFtSN8QYXwc1qhttXy0fHQPPT8/fsR100Tf2L5ELNZdZhHoWq9cQ91vEib5+//12DSNCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cf6cd17c3a69f8975ba4941b2b5a88047c1a7229bab65550ef340677349160fa","last_reissued_at":"2026-05-18T01:44:47.905711Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:44:47.905711Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Astrophysical weak-interaction rates for selected $A=20$ and $A=24$ nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"C. Sullivan, G. Mart\\'inez-Pinedo, K. Langanke, R. G. T. Zegers, Y. H. Lam","submitted_at":"2014-02-04T16:42:51Z","abstract_excerpt":"We have evaluated the electron capture rates on $^{20}$Ne, $^{20}$F, $^{24}$Mg, $^{24}$Na and the $\\beta$ decay rates for $^{20}$F and $^{24}$Na at temperature and density conditions relevant for the late-evolution stages of stars with $M=8$-12 M$_\\odot$. The rates are based on recent experimental data and large-scale shell model calculations. We show that the electron capture rates on $^{20}$Ne, $^{24}$Mg and the $^{20}$F, $^{24}$Na $\\beta$-decay rates are based on data in this astrophysical range, except for the capture rate on $^{20}$Ne, which we predict to have a dominating contribution fr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1402.0793","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":"1402.0793","created_at":"2026-05-18T01:44:47.905822+00:00"},{"alias_kind":"arxiv_version","alias_value":"1402.0793v1","created_at":"2026-05-18T01:44:47.905822+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1402.0793","created_at":"2026-05-18T01:44:47.905822+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z5WNC7B2NH4J","created_at":"2026-05-18T12:28:59.999130+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z5WNC7B2NH4JOW5E","created_at":"2026-05-18T12:28:59.999130+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z5WNC7B2","created_at":"2026-05-18T12:28:59.999130+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/Z5WNC7B2NH4JOW5ESQNSWWUIAR","json":"https://pith.science/pith/Z5WNC7B2NH4JOW5ESQNSWWUIAR.json","graph_json":"https://pith.science/api/pith-number/Z5WNC7B2NH4JOW5ESQNSWWUIAR/graph.json","events_json":"https://pith.science/api/pith-number/Z5WNC7B2NH4JOW5ESQNSWWUIAR/events.json","paper":"https://pith.science/paper/Z5WNC7B2"},"agent_actions":{"view_html":"https://pith.science/pith/Z5WNC7B2NH4JOW5ESQNSWWUIAR","download_json":"https://pith.science/pith/Z5WNC7B2NH4JOW5ESQNSWWUIAR.json","view_paper":"https://pith.science/paper/Z5WNC7B2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1402.0793&json=true","fetch_graph":"https://pith.science/api/pith-number/Z5WNC7B2NH4JOW5ESQNSWWUIAR/graph.json","fetch_events":"https://pith.science/api/pith-number/Z5WNC7B2NH4JOW5ESQNSWWUIAR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z5WNC7B2NH4JOW5ESQNSWWUIAR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z5WNC7B2NH4JOW5ESQNSWWUIAR/action/storage_attestation","attest_author":"https://pith.science/pith/Z5WNC7B2NH4JOW5ESQNSWWUIAR/action/author_attestation","sign_citation":"https://pith.science/pith/Z5WNC7B2NH4JOW5ESQNSWWUIAR/action/citation_signature","submit_replication":"https://pith.science/pith/Z5WNC7B2NH4JOW5ESQNSWWUIAR/action/replication_record"}},"created_at":"2026-05-18T01:44:47.905822+00:00","updated_at":"2026-05-18T01:44:47.905822+00:00"}