{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:B7MU7VI2ELX3SYID3YJNZAPJ6K","short_pith_number":"pith:B7MU7VI2","schema_version":"1.0","canonical_sha256":"0fd94fd51a22efb96103de12dc81e9f2a01644844ebc4ffa12b7c4ea75e96925","source":{"kind":"arxiv","id":"2411.03453","version":1},"attestation_state":"computed","paper":{"title":"Formation of Terrestrial Planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Andre Izidoro, Matthew S. Clement, Rogerio Deienno, Sean N. Raymond","submitted_at":"2024-11-05T19:08:54Z","abstract_excerpt":"Our understanding of the process of terrestrial planet formation has grown markedly over the past 20 years, yet key questions remain. This review begins by first addressing the critical, earliest stage of dust coagulation and concentration. While classic studies revealed how objects that grow to $\\sim$meter sizes are rapidly removed from protoplanetary disks via orbital decay (seemingly precluding growth to larger sizes), this chapter addresses how this is resolved in contemporary, streaming instability models that favor rapid planetesimal formation via gravitational collapse of solids in over"},"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":"2411.03453","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2024-11-05T19:08:54Z","cross_cats_sorted":[],"title_canon_sha256":"b72f61347657e67ed314d09dc62f970583480dbef0d64451912a66e9059fe5c9","abstract_canon_sha256":"67de0491b069408255b4ef7ac9cee49c5da1eab3a0760bf9cb0a7788f04408f7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:31:32.921057Z","signature_b64":"cxHlbShCEBr2VjxWsR7qnwcdZSdaW3u8pwTNl9bTlwwgQaHQbJxNY5uQtsB7ZQyhLPrXcUdFpdSY7DHZ0NsUDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0fd94fd51a22efb96103de12dc81e9f2a01644844ebc4ffa12b7c4ea75e96925","last_reissued_at":"2026-07-05T09:31:32.920587Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:31:32.920587Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Formation of Terrestrial Planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Andre Izidoro, Matthew S. Clement, Rogerio Deienno, Sean N. Raymond","submitted_at":"2024-11-05T19:08:54Z","abstract_excerpt":"Our understanding of the process of terrestrial planet formation has grown markedly over the past 20 years, yet key questions remain. This review begins by first addressing the critical, earliest stage of dust coagulation and concentration. While classic studies revealed how objects that grow to $\\sim$meter sizes are rapidly removed from protoplanetary disks via orbital decay (seemingly precluding growth to larger sizes), this chapter addresses how this is resolved in contemporary, streaming instability models that favor rapid planetesimal formation via gravitational collapse of solids in over"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.03453","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/2411.03453/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":"2411.03453","created_at":"2026-07-05T09:31:32.920643+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.03453v1","created_at":"2026-07-05T09:31:32.920643+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.03453","created_at":"2026-07-05T09:31:32.920643+00:00"},{"alias_kind":"pith_short_12","alias_value":"B7MU7VI2ELX3","created_at":"2026-07-05T09:31:32.920643+00:00"},{"alias_kind":"pith_short_16","alias_value":"B7MU7VI2ELX3SYID","created_at":"2026-07-05T09:31:32.920643+00:00"},{"alias_kind":"pith_short_8","alias_value":"B7MU7VI2","created_at":"2026-07-05T09:31:32.920643+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.20260","citing_title":"Microlensing Detection and Inference via Learned Bayes Factors","ref_index":30,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/B7MU7VI2ELX3SYID3YJNZAPJ6K","json":"https://pith.science/pith/B7MU7VI2ELX3SYID3YJNZAPJ6K.json","graph_json":"https://pith.science/api/pith-number/B7MU7VI2ELX3SYID3YJNZAPJ6K/graph.json","events_json":"https://pith.science/api/pith-number/B7MU7VI2ELX3SYID3YJNZAPJ6K/events.json","paper":"https://pith.science/paper/B7MU7VI2"},"agent_actions":{"view_html":"https://pith.science/pith/B7MU7VI2ELX3SYID3YJNZAPJ6K","download_json":"https://pith.science/pith/B7MU7VI2ELX3SYID3YJNZAPJ6K.json","view_paper":"https://pith.science/paper/B7MU7VI2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.03453&json=true","fetch_graph":"https://pith.science/api/pith-number/B7MU7VI2ELX3SYID3YJNZAPJ6K/graph.json","fetch_events":"https://pith.science/api/pith-number/B7MU7VI2ELX3SYID3YJNZAPJ6K/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/B7MU7VI2ELX3SYID3YJNZAPJ6K/action/timestamp_anchor","attest_storage":"https://pith.science/pith/B7MU7VI2ELX3SYID3YJNZAPJ6K/action/storage_attestation","attest_author":"https://pith.science/pith/B7MU7VI2ELX3SYID3YJNZAPJ6K/action/author_attestation","sign_citation":"https://pith.science/pith/B7MU7VI2ELX3SYID3YJNZAPJ6K/action/citation_signature","submit_replication":"https://pith.science/pith/B7MU7VI2ELX3SYID3YJNZAPJ6K/action/replication_record"}},"created_at":"2026-07-05T09:31:32.920643+00:00","updated_at":"2026-07-05T09:31:32.920643+00:00"}