{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2003:WK56YCLUQ6X4FTOAXIKM2UGCKO","short_pith_number":"pith:WK56YCLU","schema_version":"1.0","canonical_sha256":"b2bbec097487afc2cdc0ba14cd50c253a293bd938bb5f14f4f995246766a8363","source":{"kind":"arxiv","id":"astro-ph/0310126","version":1},"attestation_state":"computed","paper":{"title":"Thermal Timescale Mass Transfer and the Evolution of White Dwarf Binaries","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Natalia Ivanova, Ronald E. Taam","submitted_at":"2003-10-05T22:53:21Z","abstract_excerpt":"The evolution of binaries consisting of evolved main sequence stars (1 < M_d/Msun < 3.5) with white dwarf companions (0.7 < M_wd/Msun < 1.2) is investigated through the thermal mass transfer phase. Taking into account the stabilizing effect of a strong, optically thick wind from the accreting white dwarf surface, we have explored the formation of several evolutionary groups of systems for progenitors with initial orbital periods of 1 and 2 days. The numerical results show that CO white dwarfs can accrete sufficient mass to evolve to a Type Ia supernova and ONeMg white dwarfs can be built up to"},"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":"astro-ph/0310126","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2003-10-05T22:53:21Z","cross_cats_sorted":[],"title_canon_sha256":"50a0b6c05e51eb87297a3b48389ae57ba822ec01f2a4acd3d6f2f62e9422bc52","abstract_canon_sha256":"9e0db3a863d47c480b4a6db092139ee460dc7ef3f1e3d97e98aa2232cc0e42ab"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:07:33.271335Z","signature_b64":"HYKlxm7m5hG0tTwHClAMFX2zYNf9RIlSqELHVbetiVQWhQMqJeNatVwtU51naalASCQN4Mz1NOZozXaII5obAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b2bbec097487afc2cdc0ba14cd50c253a293bd938bb5f14f4f995246766a8363","last_reissued_at":"2026-05-18T01:07:33.270723Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:07:33.270723Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Thermal Timescale Mass Transfer and the Evolution of White Dwarf Binaries","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Natalia Ivanova, Ronald E. Taam","submitted_at":"2003-10-05T22:53:21Z","abstract_excerpt":"The evolution of binaries consisting of evolved main sequence stars (1 < M_d/Msun < 3.5) with white dwarf companions (0.7 < M_wd/Msun < 1.2) is investigated through the thermal mass transfer phase. Taking into account the stabilizing effect of a strong, optically thick wind from the accreting white dwarf surface, we have explored the formation of several evolutionary groups of systems for progenitors with initial orbital periods of 1 and 2 days. The numerical results show that CO white dwarfs can accrete sufficient mass to evolve to a Type Ia supernova and ONeMg white dwarfs can be built up to"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0310126","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":"astro-ph/0310126","created_at":"2026-05-18T01:07:33.270820+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0310126v1","created_at":"2026-05-18T01:07:33.270820+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0310126","created_at":"2026-05-18T01:07:33.270820+00:00"},{"alias_kind":"pith_short_12","alias_value":"WK56YCLUQ6X4","created_at":"2026-05-18T12:25:52.051335+00:00"},{"alias_kind":"pith_short_16","alias_value":"WK56YCLUQ6X4FTOA","created_at":"2026-05-18T12:25:52.051335+00:00"},{"alias_kind":"pith_short_8","alias_value":"WK56YCLU","created_at":"2026-05-18T12:25:52.051335+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/WK56YCLUQ6X4FTOAXIKM2UGCKO","json":"https://pith.science/pith/WK56YCLUQ6X4FTOAXIKM2UGCKO.json","graph_json":"https://pith.science/api/pith-number/WK56YCLUQ6X4FTOAXIKM2UGCKO/graph.json","events_json":"https://pith.science/api/pith-number/WK56YCLUQ6X4FTOAXIKM2UGCKO/events.json","paper":"https://pith.science/paper/WK56YCLU"},"agent_actions":{"view_html":"https://pith.science/pith/WK56YCLUQ6X4FTOAXIKM2UGCKO","download_json":"https://pith.science/pith/WK56YCLUQ6X4FTOAXIKM2UGCKO.json","view_paper":"https://pith.science/paper/WK56YCLU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0310126&json=true","fetch_graph":"https://pith.science/api/pith-number/WK56YCLUQ6X4FTOAXIKM2UGCKO/graph.json","fetch_events":"https://pith.science/api/pith-number/WK56YCLUQ6X4FTOAXIKM2UGCKO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WK56YCLUQ6X4FTOAXIKM2UGCKO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WK56YCLUQ6X4FTOAXIKM2UGCKO/action/storage_attestation","attest_author":"https://pith.science/pith/WK56YCLUQ6X4FTOAXIKM2UGCKO/action/author_attestation","sign_citation":"https://pith.science/pith/WK56YCLUQ6X4FTOAXIKM2UGCKO/action/citation_signature","submit_replication":"https://pith.science/pith/WK56YCLUQ6X4FTOAXIKM2UGCKO/action/replication_record"}},"created_at":"2026-05-18T01:07:33.270820+00:00","updated_at":"2026-05-18T01:07:33.270820+00:00"}