{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:CIJTR2OQ5KOERILWSQFJMB4C5Y","short_pith_number":"pith:CIJTR2OQ","schema_version":"1.0","canonical_sha256":"121338e9d0ea9c48a176940a960782ee2035921a3c04d2ccedb18e79b4057f45","source":{"kind":"arxiv","id":"1510.03485","version":1},"attestation_state":"computed","paper":{"title":"Super-Eddington wind scenario for the progenitors of type Ia supernovae: Accreting He-rich matter onto white dwarfs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Bo Wang, Dongdong Liu, Xiao Cui, Xin Ma, Yan Li, Zhanwen Han","submitted_at":"2015-10-12T23:56:16Z","abstract_excerpt":"Supernovae of type Ia (SNe Ia) are believed to be thermonuclear explosions of carbon-oxygen white dwarfs (CO WDs). However, the mass accretion process onto CO WDs is still not completely understood. In this paper, we study the accretion of He-rich matter onto CO WDs and explore a scenario in which a strong wind forms on the surface of the WD if the total luminosity exceeds the Eddington limit. Using a stellar evolution code called modules for experiments in stellar astrophysics (MESA), we simulated the He accretion process onto CO WDs for WDs with masses of 0.6-1.35Msun and various accretion r"},"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":"1510.03485","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-10-12T23:56:16Z","cross_cats_sorted":[],"title_canon_sha256":"76d64a56073f69134dc4745b8da660aaa322ebe758582783814bed8d91d6c69c","abstract_canon_sha256":"ea2abaa1d70a59072958783e8268ae2b55593eece5f3293ca63cab084d340d98"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:26:41.025574Z","signature_b64":"QdHk90kQ2F0jNi3k0t1nmioJDneIS1SUsQNU2qnPPm/3aioPM9L527/PVDPIlKdizQfb2/SAx4aAi3OT/5ChCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"121338e9d0ea9c48a176940a960782ee2035921a3c04d2ccedb18e79b4057f45","last_reissued_at":"2026-05-18T01:26:41.024955Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:26:41.024955Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Super-Eddington wind scenario for the progenitors of type Ia supernovae: Accreting He-rich matter onto white dwarfs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Bo Wang, Dongdong Liu, Xiao Cui, Xin Ma, Yan Li, Zhanwen Han","submitted_at":"2015-10-12T23:56:16Z","abstract_excerpt":"Supernovae of type Ia (SNe Ia) are believed to be thermonuclear explosions of carbon-oxygen white dwarfs (CO WDs). However, the mass accretion process onto CO WDs is still not completely understood. In this paper, we study the accretion of He-rich matter onto CO WDs and explore a scenario in which a strong wind forms on the surface of the WD if the total luminosity exceeds the Eddington limit. Using a stellar evolution code called modules for experiments in stellar astrophysics (MESA), we simulated the He accretion process onto CO WDs for WDs with masses of 0.6-1.35Msun and various accretion r"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.03485","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":"1510.03485","created_at":"2026-05-18T01:26:41.025064+00:00"},{"alias_kind":"arxiv_version","alias_value":"1510.03485v1","created_at":"2026-05-18T01:26:41.025064+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1510.03485","created_at":"2026-05-18T01:26:41.025064+00:00"},{"alias_kind":"pith_short_12","alias_value":"CIJTR2OQ5KOE","created_at":"2026-05-18T12:29:14.074870+00:00"},{"alias_kind":"pith_short_16","alias_value":"CIJTR2OQ5KOERILW","created_at":"2026-05-18T12:29:14.074870+00:00"},{"alias_kind":"pith_short_8","alias_value":"CIJTR2OQ","created_at":"2026-05-18T12:29:14.074870+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/CIJTR2OQ5KOERILWSQFJMB4C5Y","json":"https://pith.science/pith/CIJTR2OQ5KOERILWSQFJMB4C5Y.json","graph_json":"https://pith.science/api/pith-number/CIJTR2OQ5KOERILWSQFJMB4C5Y/graph.json","events_json":"https://pith.science/api/pith-number/CIJTR2OQ5KOERILWSQFJMB4C5Y/events.json","paper":"https://pith.science/paper/CIJTR2OQ"},"agent_actions":{"view_html":"https://pith.science/pith/CIJTR2OQ5KOERILWSQFJMB4C5Y","download_json":"https://pith.science/pith/CIJTR2OQ5KOERILWSQFJMB4C5Y.json","view_paper":"https://pith.science/paper/CIJTR2OQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1510.03485&json=true","fetch_graph":"https://pith.science/api/pith-number/CIJTR2OQ5KOERILWSQFJMB4C5Y/graph.json","fetch_events":"https://pith.science/api/pith-number/CIJTR2OQ5KOERILWSQFJMB4C5Y/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CIJTR2OQ5KOERILWSQFJMB4C5Y/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CIJTR2OQ5KOERILWSQFJMB4C5Y/action/storage_attestation","attest_author":"https://pith.science/pith/CIJTR2OQ5KOERILWSQFJMB4C5Y/action/author_attestation","sign_citation":"https://pith.science/pith/CIJTR2OQ5KOERILWSQFJMB4C5Y/action/citation_signature","submit_replication":"https://pith.science/pith/CIJTR2OQ5KOERILWSQFJMB4C5Y/action/replication_record"}},"created_at":"2026-05-18T01:26:41.025064+00:00","updated_at":"2026-05-18T01:26:41.025064+00:00"}