{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:NUEBVU37WMKXFVCB4KTXFHB7BU","short_pith_number":"pith:NUEBVU37","schema_version":"1.0","canonical_sha256":"6d081ad37fb31572d441e2a7729c3f0d10c32d5cedf11db1858eb9ce2aeed29f","source":{"kind":"arxiv","id":"2111.00279","version":1},"attestation_state":"computed","paper":{"title":"SimAb: A simple, fast and flexible model to assess the effects of planet formation on the atmospheric composition of gas giants","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"C. Dominik, J.M. D\\'esert, M. Min, N. Khorshid, P. Woitke","submitted_at":"2021-10-30T16:15:46Z","abstract_excerpt":"We present a basic, fast, and flexible planet formation model, called SimAb (Simulating Abundances), to form giant planets and study their primary atmospheric composition soon after their formation. In SimAb we introduce parameters to simplify the assumptions about the complex physics involved in the formation of a planet. This approach allows us to trace and understand the influence of complex physical processes on the formed planets. We focus on the C/O ratio and the metallicity of the planetary atmosphere as an indicator of their compositions. We show that the initial protoplanet core mass "},"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":"2111.00279","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2021-10-30T16:15:46Z","cross_cats_sorted":[],"title_canon_sha256":"5de75a6ead5a05f4ee251599802909e219316990b7bd15602affda6c8cb8416f","abstract_canon_sha256":"a6f7b59c282d65cd5b95f8d351fc5fd989410ff7aad034b71873de4c71836a84"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:18:23.986304Z","signature_b64":"xqj1yZIpKF+9/VMBICQXfJpGJkhhKFkUg+4S2+Ybdq/8G5zN0vW4AGD3fkXSkR218/++WENjXAXTJjAFDGJKDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6d081ad37fb31572d441e2a7729c3f0d10c32d5cedf11db1858eb9ce2aeed29f","last_reissued_at":"2026-07-05T05:18:23.985870Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:18:23.985870Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"SimAb: A simple, fast and flexible model to assess the effects of planet formation on the atmospheric composition of gas giants","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"C. Dominik, J.M. D\\'esert, M. Min, N. Khorshid, P. Woitke","submitted_at":"2021-10-30T16:15:46Z","abstract_excerpt":"We present a basic, fast, and flexible planet formation model, called SimAb (Simulating Abundances), to form giant planets and study their primary atmospheric composition soon after their formation. In SimAb we introduce parameters to simplify the assumptions about the complex physics involved in the formation of a planet. This approach allows us to trace and understand the influence of complex physical processes on the formed planets. We focus on the C/O ratio and the metallicity of the planetary atmosphere as an indicator of their compositions. We show that the initial protoplanet core mass "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2111.00279","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2111.00279/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2111.00279","created_at":"2026-07-05T05:18:23.985931+00:00"},{"alias_kind":"arxiv_version","alias_value":"2111.00279v1","created_at":"2026-07-05T05:18:23.985931+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2111.00279","created_at":"2026-07-05T05:18:23.985931+00:00"},{"alias_kind":"pith_short_12","alias_value":"NUEBVU37WMKX","created_at":"2026-07-05T05:18:23.985931+00:00"},{"alias_kind":"pith_short_16","alias_value":"NUEBVU37WMKXFVCB","created_at":"2026-07-05T05:18:23.985931+00:00"},{"alias_kind":"pith_short_8","alias_value":"NUEBVU37","created_at":"2026-07-05T05:18:23.985931+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/NUEBVU37WMKXFVCB4KTXFHB7BU","json":"https://pith.science/pith/NUEBVU37WMKXFVCB4KTXFHB7BU.json","graph_json":"https://pith.science/api/pith-number/NUEBVU37WMKXFVCB4KTXFHB7BU/graph.json","events_json":"https://pith.science/api/pith-number/NUEBVU37WMKXFVCB4KTXFHB7BU/events.json","paper":"https://pith.science/paper/NUEBVU37"},"agent_actions":{"view_html":"https://pith.science/pith/NUEBVU37WMKXFVCB4KTXFHB7BU","download_json":"https://pith.science/pith/NUEBVU37WMKXFVCB4KTXFHB7BU.json","view_paper":"https://pith.science/paper/NUEBVU37","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2111.00279&json=true","fetch_graph":"https://pith.science/api/pith-number/NUEBVU37WMKXFVCB4KTXFHB7BU/graph.json","fetch_events":"https://pith.science/api/pith-number/NUEBVU37WMKXFVCB4KTXFHB7BU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NUEBVU37WMKXFVCB4KTXFHB7BU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NUEBVU37WMKXFVCB4KTXFHB7BU/action/storage_attestation","attest_author":"https://pith.science/pith/NUEBVU37WMKXFVCB4KTXFHB7BU/action/author_attestation","sign_citation":"https://pith.science/pith/NUEBVU37WMKXFVCB4KTXFHB7BU/action/citation_signature","submit_replication":"https://pith.science/pith/NUEBVU37WMKXFVCB4KTXFHB7BU/action/replication_record"}},"created_at":"2026-07-05T05:18:23.985931+00:00","updated_at":"2026-07-05T05:18:23.985931+00:00"}