{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:USVRSZESI4TED44ND4R3YH3LFL","short_pith_number":"pith:USVRSZES","schema_version":"1.0","canonical_sha256":"a4ab196492472641f38d1f23bc1f6b2af41b90831d1885f87072567c8009fb38","source":{"kind":"arxiv","id":"1901.10531","version":1},"attestation_state":"computed","paper":{"title":"Dependence of Convective Boundary Mixing on Boundary Properties and Turbulence Strength","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Cristini, C. Georgy, C. Meakin, D. Arnett, I. Walkington, R. Hirschi","submitted_at":"2019-01-29T20:43:02Z","abstract_excerpt":"Convective boundary mixing is one of the major uncertainties in stellar evolution. In order to study its dependence on boundary properties and turbulence strength in a controlled way, we computed a series of 3D hydrodynamical simulations of stellar convection during carbon burning with a varying boosting factor of the driving luminosity. Our 3D implicit large eddy simulations were computed with the PROMPI code. We performed a mean field analysis of the simulations within the Reynolds-averaged Navier-Stokes framework. Both the vertical RMS velocity within the convective region and the bulk Rich"},"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":"1901.10531","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2019-01-29T20:43:02Z","cross_cats_sorted":[],"title_canon_sha256":"8b1d24c5a9487549cabbb13fcee88ffe92f37427c6bad4ce790a6b240ac9a19e","abstract_canon_sha256":"ae35ad395b09e11496d0fc2999b1016a49376518b8d2646826b323a82106cc34"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:54:08.000012Z","signature_b64":"pjN9C+iYCFTYjENmcMGRDRQE1uWtn46DgjQuWSIl/DgQ7CVehEwcWQYY0jCFtQIA30u6GP3DZdicyJzfE/26Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a4ab196492472641f38d1f23bc1f6b2af41b90831d1885f87072567c8009fb38","last_reissued_at":"2026-05-17T23:54:07.999619Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:54:07.999619Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dependence of Convective Boundary Mixing on Boundary Properties and Turbulence Strength","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Cristini, C. Georgy, C. Meakin, D. Arnett, I. Walkington, R. Hirschi","submitted_at":"2019-01-29T20:43:02Z","abstract_excerpt":"Convective boundary mixing is one of the major uncertainties in stellar evolution. In order to study its dependence on boundary properties and turbulence strength in a controlled way, we computed a series of 3D hydrodynamical simulations of stellar convection during carbon burning with a varying boosting factor of the driving luminosity. Our 3D implicit large eddy simulations were computed with the PROMPI code. We performed a mean field analysis of the simulations within the Reynolds-averaged Navier-Stokes framework. Both the vertical RMS velocity within the convective region and the bulk Rich"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1901.10531","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":"1901.10531","created_at":"2026-05-17T23:54:07.999673+00:00"},{"alias_kind":"arxiv_version","alias_value":"1901.10531v1","created_at":"2026-05-17T23:54:07.999673+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1901.10531","created_at":"2026-05-17T23:54:07.999673+00:00"},{"alias_kind":"pith_short_12","alias_value":"USVRSZESI4TE","created_at":"2026-05-18T12:33:30.264802+00:00"},{"alias_kind":"pith_short_16","alias_value":"USVRSZESI4TED44N","created_at":"2026-05-18T12:33:30.264802+00:00"},{"alias_kind":"pith_short_8","alias_value":"USVRSZES","created_at":"2026-05-18T12:33:30.264802+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/USVRSZESI4TED44ND4R3YH3LFL","json":"https://pith.science/pith/USVRSZESI4TED44ND4R3YH3LFL.json","graph_json":"https://pith.science/api/pith-number/USVRSZESI4TED44ND4R3YH3LFL/graph.json","events_json":"https://pith.science/api/pith-number/USVRSZESI4TED44ND4R3YH3LFL/events.json","paper":"https://pith.science/paper/USVRSZES"},"agent_actions":{"view_html":"https://pith.science/pith/USVRSZESI4TED44ND4R3YH3LFL","download_json":"https://pith.science/pith/USVRSZESI4TED44ND4R3YH3LFL.json","view_paper":"https://pith.science/paper/USVRSZES","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1901.10531&json=true","fetch_graph":"https://pith.science/api/pith-number/USVRSZESI4TED44ND4R3YH3LFL/graph.json","fetch_events":"https://pith.science/api/pith-number/USVRSZESI4TED44ND4R3YH3LFL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/USVRSZESI4TED44ND4R3YH3LFL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/USVRSZESI4TED44ND4R3YH3LFL/action/storage_attestation","attest_author":"https://pith.science/pith/USVRSZESI4TED44ND4R3YH3LFL/action/author_attestation","sign_citation":"https://pith.science/pith/USVRSZESI4TED44ND4R3YH3LFL/action/citation_signature","submit_replication":"https://pith.science/pith/USVRSZESI4TED44ND4R3YH3LFL/action/replication_record"}},"created_at":"2026-05-17T23:54:07.999673+00:00","updated_at":"2026-05-17T23:54:07.999673+00:00"}