{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:ILSV7OWVFGHF6GFIEPPP2AHRVG","short_pith_number":"pith:ILSV7OWV","schema_version":"1.0","canonical_sha256":"42e55fbad5298e5f18a823defd00f1a99dc3a514150333f6fd30728fa2ac4a37","source":{"kind":"arxiv","id":"1808.05992","version":1},"attestation_state":"computed","paper":{"title":"The single-degenerate model for the progenitors of accretion-induced collapse events","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Bo Wang","submitted_at":"2018-08-17T20:48:47Z","abstract_excerpt":"It has been suggested that the accretion-induced collapse (AIC) of an oxygen-neon white dwarf (ONe WD) to a neutron star is a theoretically predicted outcome in stellar evolution, likely relating to the formation of some neutron star systems. However, the progenitor models of AIC events are still not well studied, and recent studies indicated that CO WD+He star systems may also contribute to the formation of neutron star systems through AIC process when off-centre carbon ignition happens on the surface of the CO WD. In this work, I studied the single-degenerate (SD) model of AIC events in a sy"},"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":"1808.05992","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-08-17T20:48:47Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"001f1fbf2d8688f74db0b4063a81db5d535a23d1120709e4bdf03e0a299ef01d","abstract_canon_sha256":"403ac98a7cf176c2ea333e0c7516cd29cbeba4ef3cf98b67bd2cffcd9735a01e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:05:55.733209Z","signature_b64":"pffYqDhX+3/7mr6cYu3ywP6swQVChUQ6DLnmseez/uvzpyG/JnKjebkyInckM8KyCaRfrp+ANPC3F67zI4iACA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"42e55fbad5298e5f18a823defd00f1a99dc3a514150333f6fd30728fa2ac4a37","last_reissued_at":"2026-05-18T00:05:55.732523Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:05:55.732523Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The single-degenerate model for the progenitors of accretion-induced collapse events","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Bo Wang","submitted_at":"2018-08-17T20:48:47Z","abstract_excerpt":"It has been suggested that the accretion-induced collapse (AIC) of an oxygen-neon white dwarf (ONe WD) to a neutron star is a theoretically predicted outcome in stellar evolution, likely relating to the formation of some neutron star systems. However, the progenitor models of AIC events are still not well studied, and recent studies indicated that CO WD+He star systems may also contribute to the formation of neutron star systems through AIC process when off-centre carbon ignition happens on the surface of the CO WD. In this work, I studied the single-degenerate (SD) model of AIC events in a sy"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1808.05992","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":"1808.05992","created_at":"2026-05-18T00:05:55.732632+00:00"},{"alias_kind":"arxiv_version","alias_value":"1808.05992v1","created_at":"2026-05-18T00:05:55.732632+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1808.05992","created_at":"2026-05-18T00:05:55.732632+00:00"},{"alias_kind":"pith_short_12","alias_value":"ILSV7OWVFGHF","created_at":"2026-05-18T12:32:31.084164+00:00"},{"alias_kind":"pith_short_16","alias_value":"ILSV7OWVFGHF6GFI","created_at":"2026-05-18T12:32:31.084164+00:00"},{"alias_kind":"pith_short_8","alias_value":"ILSV7OWV","created_at":"2026-05-18T12:32:31.084164+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/ILSV7OWVFGHF6GFIEPPP2AHRVG","json":"https://pith.science/pith/ILSV7OWVFGHF6GFIEPPP2AHRVG.json","graph_json":"https://pith.science/api/pith-number/ILSV7OWVFGHF6GFIEPPP2AHRVG/graph.json","events_json":"https://pith.science/api/pith-number/ILSV7OWVFGHF6GFIEPPP2AHRVG/events.json","paper":"https://pith.science/paper/ILSV7OWV"},"agent_actions":{"view_html":"https://pith.science/pith/ILSV7OWVFGHF6GFIEPPP2AHRVG","download_json":"https://pith.science/pith/ILSV7OWVFGHF6GFIEPPP2AHRVG.json","view_paper":"https://pith.science/paper/ILSV7OWV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1808.05992&json=true","fetch_graph":"https://pith.science/api/pith-number/ILSV7OWVFGHF6GFIEPPP2AHRVG/graph.json","fetch_events":"https://pith.science/api/pith-number/ILSV7OWVFGHF6GFIEPPP2AHRVG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ILSV7OWVFGHF6GFIEPPP2AHRVG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ILSV7OWVFGHF6GFIEPPP2AHRVG/action/storage_attestation","attest_author":"https://pith.science/pith/ILSV7OWVFGHF6GFIEPPP2AHRVG/action/author_attestation","sign_citation":"https://pith.science/pith/ILSV7OWVFGHF6GFIEPPP2AHRVG/action/citation_signature","submit_replication":"https://pith.science/pith/ILSV7OWVFGHF6GFIEPPP2AHRVG/action/replication_record"}},"created_at":"2026-05-18T00:05:55.732632+00:00","updated_at":"2026-05-18T00:05:55.732632+00:00"}