{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:FK4FDN6JIA45ESW6DMTVBA3YMA","short_pith_number":"pith:FK4FDN6J","schema_version":"1.0","canonical_sha256":"2ab851b7c94039d24ade1b2750837860272a41b8ee21628dff0b830497e01a0c","source":{"kind":"arxiv","id":"2501.16169","version":2},"attestation_state":"computed","paper":{"title":"Quantifying the Impact of the Dust Torque on the Migration of Low-mass Planets II: The Role of Pebble Accretion in Planet Growth within a Global Planet Formation Model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Marcelo M. Miller Bertolami, Martin E. Pessah, Octavio M. Guilera, Pablo Benitez-Llambay","submitted_at":"2025-01-27T16:09:48Z","abstract_excerpt":"Although dust constitutes only about 1% of the mass of a protoplanetary disk, recent studies demonstrate that it can exert a significant torque on low- and intermediate-mass planetary cores. We compute and quantify for the first time the influence of the dust torque on the evolution of growing planetary embryos as they move in a protoplanetary disk while growing via gas and pebble accretion. Our global model evolves the gaseous disk via viscous accretion and X-ray photoevaporation, while accounting for dust growth and evolution including coagulation, drift, and fragmentation. Our research indi"},"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":"2501.16169","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2025-01-27T16:09:48Z","cross_cats_sorted":[],"title_canon_sha256":"fa615b88f6c3d78007955d345daf00ec9af4954984aa5c419d9e8fecf2b688fd","abstract_canon_sha256":"f980b3ff6d8acbc6c212ac916299564b2c388b3305a0064a929908bec797c8f7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:03:20.821223Z","signature_b64":"LzVMrfwCIqN+SGNrur69mUPHiX47sqZVpKJ6+HSA3T7b1lEtLk4wzBxrrjsutbBHVrrG7PZjF9vpNQUHbaa4AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2ab851b7c94039d24ade1b2750837860272a41b8ee21628dff0b830497e01a0c","last_reissued_at":"2026-07-05T11:03:20.820747Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:03:20.820747Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quantifying the Impact of the Dust Torque on the Migration of Low-mass Planets II: The Role of Pebble Accretion in Planet Growth within a Global Planet Formation Model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Marcelo M. Miller Bertolami, Martin E. Pessah, Octavio M. Guilera, Pablo Benitez-Llambay","submitted_at":"2025-01-27T16:09:48Z","abstract_excerpt":"Although dust constitutes only about 1% of the mass of a protoplanetary disk, recent studies demonstrate that it can exert a significant torque on low- and intermediate-mass planetary cores. We compute and quantify for the first time the influence of the dust torque on the evolution of growing planetary embryos as they move in a protoplanetary disk while growing via gas and pebble accretion. Our global model evolves the gaseous disk via viscous accretion and X-ray photoevaporation, while accounting for dust growth and evolution including coagulation, drift, and fragmentation. Our research indi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2501.16169","kind":"arxiv","version":2},"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/2501.16169/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":"2501.16169","created_at":"2026-07-05T11:03:20.820803+00:00"},{"alias_kind":"arxiv_version","alias_value":"2501.16169v2","created_at":"2026-07-05T11:03:20.820803+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2501.16169","created_at":"2026-07-05T11:03:20.820803+00:00"},{"alias_kind":"pith_short_12","alias_value":"FK4FDN6JIA45","created_at":"2026-07-05T11:03:20.820803+00:00"},{"alias_kind":"pith_short_16","alias_value":"FK4FDN6JIA45ESW6","created_at":"2026-07-05T11:03:20.820803+00:00"},{"alias_kind":"pith_short_8","alias_value":"FK4FDN6J","created_at":"2026-07-05T11:03:20.820803+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/FK4FDN6JIA45ESW6DMTVBA3YMA","json":"https://pith.science/pith/FK4FDN6JIA45ESW6DMTVBA3YMA.json","graph_json":"https://pith.science/api/pith-number/FK4FDN6JIA45ESW6DMTVBA3YMA/graph.json","events_json":"https://pith.science/api/pith-number/FK4FDN6JIA45ESW6DMTVBA3YMA/events.json","paper":"https://pith.science/paper/FK4FDN6J"},"agent_actions":{"view_html":"https://pith.science/pith/FK4FDN6JIA45ESW6DMTVBA3YMA","download_json":"https://pith.science/pith/FK4FDN6JIA45ESW6DMTVBA3YMA.json","view_paper":"https://pith.science/paper/FK4FDN6J","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2501.16169&json=true","fetch_graph":"https://pith.science/api/pith-number/FK4FDN6JIA45ESW6DMTVBA3YMA/graph.json","fetch_events":"https://pith.science/api/pith-number/FK4FDN6JIA45ESW6DMTVBA3YMA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FK4FDN6JIA45ESW6DMTVBA3YMA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FK4FDN6JIA45ESW6DMTVBA3YMA/action/storage_attestation","attest_author":"https://pith.science/pith/FK4FDN6JIA45ESW6DMTVBA3YMA/action/author_attestation","sign_citation":"https://pith.science/pith/FK4FDN6JIA45ESW6DMTVBA3YMA/action/citation_signature","submit_replication":"https://pith.science/pith/FK4FDN6JIA45ESW6DMTVBA3YMA/action/replication_record"}},"created_at":"2026-07-05T11:03:20.820803+00:00","updated_at":"2026-07-05T11:03:20.820803+00:00"}