{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:M5QNETT6FXO3YYE5423G4KEDQK","short_pith_number":"pith:M5QNETT6","schema_version":"1.0","canonical_sha256":"6760d24e7e2dddbc609de6b66e288382945d35879671f55cdd7323bfaa02223e","source":{"kind":"arxiv","id":"1112.4819","version":1},"attestation_state":"computed","paper":{"title":"A new model for mixing by double-diffusive convection (semi-convection): I. The conditions for layer formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"Adrienne L. Traxler, Giovanni M. Mirouh, Pascale Garaud, Stephan Stellmach, Toby S. Wood","submitted_at":"2011-12-20T20:20:37Z","abstract_excerpt":"The process referred to as \"semi-convection\" in astrophysics and \"double-diffusive convection in the diffusive regime\" in Earth and planetary sciences, occurs in stellar and planetary interiors in regions which are stable according to the Ledoux criterion but unstable according to the Schwarzschild criterion. In this series of papers, we analyze the results of an extensive suite of 3D numerical simulations of the process, and ultimately propose a new 1D prescription for heat and compositional transport in this regime which can be used in stellar or planetary structure and evolution models.\n  I"},"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":"1112.4819","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-12-20T20:20:37Z","cross_cats_sorted":["astro-ph.EP"],"title_canon_sha256":"08c362dfd164b62cdbcacf2a9de042ae39c2a5e15f4077da52554e1c4d46e766","abstract_canon_sha256":"578910285f9b96a51b353252b159e864d10d12068219e299995c6a1b2a47445b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:59:04.448035Z","signature_b64":"Oi13ue7ubdvA/8mgjqwDY1fWc5fkEU2DLL/JoazBus9SM+C56DDh+t/dhsdoEvESgeqyLGhHCnN2q+ncot70BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6760d24e7e2dddbc609de6b66e288382945d35879671f55cdd7323bfaa02223e","last_reissued_at":"2026-05-18T01:59:04.447298Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:59:04.447298Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A new model for mixing by double-diffusive convection (semi-convection): I. The conditions for layer formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"Adrienne L. Traxler, Giovanni M. Mirouh, Pascale Garaud, Stephan Stellmach, Toby S. Wood","submitted_at":"2011-12-20T20:20:37Z","abstract_excerpt":"The process referred to as \"semi-convection\" in astrophysics and \"double-diffusive convection in the diffusive regime\" in Earth and planetary sciences, occurs in stellar and planetary interiors in regions which are stable according to the Ledoux criterion but unstable according to the Schwarzschild criterion. In this series of papers, we analyze the results of an extensive suite of 3D numerical simulations of the process, and ultimately propose a new 1D prescription for heat and compositional transport in this regime which can be used in stellar or planetary structure and evolution models.\n  I"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1112.4819","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":"1112.4819","created_at":"2026-05-18T01:59:04.447423+00:00"},{"alias_kind":"arxiv_version","alias_value":"1112.4819v1","created_at":"2026-05-18T01:59:04.447423+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1112.4819","created_at":"2026-05-18T01:59:04.447423+00:00"},{"alias_kind":"pith_short_12","alias_value":"M5QNETT6FXO3","created_at":"2026-05-18T12:26:34.985390+00:00"},{"alias_kind":"pith_short_16","alias_value":"M5QNETT6FXO3YYE5","created_at":"2026-05-18T12:26:34.985390+00:00"},{"alias_kind":"pith_short_8","alias_value":"M5QNETT6","created_at":"2026-05-18T12:26:34.985390+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/M5QNETT6FXO3YYE5423G4KEDQK","json":"https://pith.science/pith/M5QNETT6FXO3YYE5423G4KEDQK.json","graph_json":"https://pith.science/api/pith-number/M5QNETT6FXO3YYE5423G4KEDQK/graph.json","events_json":"https://pith.science/api/pith-number/M5QNETT6FXO3YYE5423G4KEDQK/events.json","paper":"https://pith.science/paper/M5QNETT6"},"agent_actions":{"view_html":"https://pith.science/pith/M5QNETT6FXO3YYE5423G4KEDQK","download_json":"https://pith.science/pith/M5QNETT6FXO3YYE5423G4KEDQK.json","view_paper":"https://pith.science/paper/M5QNETT6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1112.4819&json=true","fetch_graph":"https://pith.science/api/pith-number/M5QNETT6FXO3YYE5423G4KEDQK/graph.json","fetch_events":"https://pith.science/api/pith-number/M5QNETT6FXO3YYE5423G4KEDQK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/M5QNETT6FXO3YYE5423G4KEDQK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/M5QNETT6FXO3YYE5423G4KEDQK/action/storage_attestation","attest_author":"https://pith.science/pith/M5QNETT6FXO3YYE5423G4KEDQK/action/author_attestation","sign_citation":"https://pith.science/pith/M5QNETT6FXO3YYE5423G4KEDQK/action/citation_signature","submit_replication":"https://pith.science/pith/M5QNETT6FXO3YYE5423G4KEDQK/action/replication_record"}},"created_at":"2026-05-18T01:59:04.447423+00:00","updated_at":"2026-05-18T01:59:04.447423+00:00"}