{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:X6XWE2CA3ILVUMMLRTDYAYQPWB","short_pith_number":"pith:X6XWE2CA","schema_version":"1.0","canonical_sha256":"bfaf626840da175a318b8cc780620fb07255346bd71832caaf74d9fc29c7b7f9","source":{"kind":"arxiv","id":"1009.5333","version":3},"attestation_state":"computed","paper":{"title":"Convective overshooting and production of s-nuclei in massive stars during their core He-burning phase","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Bonanno, G. Contino, M. L. Pumo, R. A. Zappal\\'a","submitted_at":"2010-09-27T17:18:33Z","abstract_excerpt":"With the \"post-processing\" technique we explore the role of the convective overshooting on the production of s-nuclei in stellar models of different initial mass and metallicity ($15 \\leq M_{ZAMS}/M_{\\odot} \\leq 25$; $10^{-4} \\leq Z \\leq 0.02$), considering a range of values for the parameter $f$, which determines the overall efficiency of convective overshooting.We find enhancements in the production of s-nuclei until a factor $\\sim 6$ (measured as the average overproduction factor of the 6 s-only nuclear species with $60\\lesssim A\\lesssim90$) in all our models of different initial mass and m"},"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":"1009.5333","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-09-27T17:18:33Z","cross_cats_sorted":[],"title_canon_sha256":"6d1a20fdbe2e534347a78025c55a621a73d058b23f660a938f4fc6303d667393","abstract_canon_sha256":"96e5a5c23c894dac19afd8a63d988856d6c635e911adeac3e7fe886fddf6dc0d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:16.697307Z","signature_b64":"FWWReKo+S6J0NLt3lmMWg0+C0DrNzSLOiJDdBXc8anB5WSIBJWB21CrSYbNTCL86T+ij4jueKkItm3+6IHFtDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bfaf626840da175a318b8cc780620fb07255346bd71832caaf74d9fc29c7b7f9","last_reissued_at":"2026-05-18T02:05:16.696611Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:16.696611Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Convective overshooting and production of s-nuclei in massive stars during their core He-burning phase","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Bonanno, G. Contino, M. L. Pumo, R. A. Zappal\\'a","submitted_at":"2010-09-27T17:18:33Z","abstract_excerpt":"With the \"post-processing\" technique we explore the role of the convective overshooting on the production of s-nuclei in stellar models of different initial mass and metallicity ($15 \\leq M_{ZAMS}/M_{\\odot} \\leq 25$; $10^{-4} \\leq Z \\leq 0.02$), considering a range of values for the parameter $f$, which determines the overall efficiency of convective overshooting.We find enhancements in the production of s-nuclei until a factor $\\sim 6$ (measured as the average overproduction factor of the 6 s-only nuclear species with $60\\lesssim A\\lesssim90$) in all our models of different initial mass and m"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.5333","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":"1009.5333","created_at":"2026-05-18T02:05:16.696719+00:00"},{"alias_kind":"arxiv_version","alias_value":"1009.5333v3","created_at":"2026-05-18T02:05:16.696719+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1009.5333","created_at":"2026-05-18T02:05:16.696719+00:00"},{"alias_kind":"pith_short_12","alias_value":"X6XWE2CA3ILV","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_16","alias_value":"X6XWE2CA3ILVUMML","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_8","alias_value":"X6XWE2CA","created_at":"2026-05-18T12:26:17.028572+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/X6XWE2CA3ILVUMMLRTDYAYQPWB","json":"https://pith.science/pith/X6XWE2CA3ILVUMMLRTDYAYQPWB.json","graph_json":"https://pith.science/api/pith-number/X6XWE2CA3ILVUMMLRTDYAYQPWB/graph.json","events_json":"https://pith.science/api/pith-number/X6XWE2CA3ILVUMMLRTDYAYQPWB/events.json","paper":"https://pith.science/paper/X6XWE2CA"},"agent_actions":{"view_html":"https://pith.science/pith/X6XWE2CA3ILVUMMLRTDYAYQPWB","download_json":"https://pith.science/pith/X6XWE2CA3ILVUMMLRTDYAYQPWB.json","view_paper":"https://pith.science/paper/X6XWE2CA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1009.5333&json=true","fetch_graph":"https://pith.science/api/pith-number/X6XWE2CA3ILVUMMLRTDYAYQPWB/graph.json","fetch_events":"https://pith.science/api/pith-number/X6XWE2CA3ILVUMMLRTDYAYQPWB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/X6XWE2CA3ILVUMMLRTDYAYQPWB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/X6XWE2CA3ILVUMMLRTDYAYQPWB/action/storage_attestation","attest_author":"https://pith.science/pith/X6XWE2CA3ILVUMMLRTDYAYQPWB/action/author_attestation","sign_citation":"https://pith.science/pith/X6XWE2CA3ILVUMMLRTDYAYQPWB/action/citation_signature","submit_replication":"https://pith.science/pith/X6XWE2CA3ILVUMMLRTDYAYQPWB/action/replication_record"}},"created_at":"2026-05-18T02:05:16.696719+00:00","updated_at":"2026-05-18T02:05:16.696719+00:00"}