{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:KZ44I2SAUA62SGF36ZBREZUMIC","short_pith_number":"pith:KZ44I2SA","schema_version":"1.0","canonical_sha256":"5679c46a40a03da918bbf64312668c40acd59f0b51669425c2f4eccb747d58c9","source":{"kind":"arxiv","id":"2507.01336","version":2},"attestation_state":"computed","paper":{"title":"Planet-induced Gas and Dust Substructure Feedbacks on Disk Thermal Structure","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Kan Chen, Mihkel Kama, Paola Pinilla","submitted_at":"2025-07-02T03:53:28Z","abstract_excerpt":"Protoplanets can interact with their natal disks and generate gas and dust substructures such as gaps and rings. However, how these planet-induced substructures affect the disk temperature, and how that in turn influences the substructures, remains unclear. We aim to study disk substructures and the thermal structure self-consistently and explore their impact on volatile distribution. To this end, we perform iterative multi-fluid hydrodynamical and radiative transfer simulations of planet-disk interactions. We find that the temperature in a structured disk deviates significantly from that of a"},"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":"2507.01336","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2025-07-02T03:53:28Z","cross_cats_sorted":[],"title_canon_sha256":"02784977c9fb5d2e0034c575a7b5ecbf771e78d345ebbac6dff489c124232598","abstract_canon_sha256":"6094016b09ebb0e6253b1d95fa2801661998c88fc86191bc422a0734ed703ce8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:31:09.219298Z","signature_b64":"yL+mDlOjyICTtOLUWMh1MJQalR/UjTiPVHwcuLaO2hGSEjTUVf1yg96SVuk0QyvvKgEXlb1i4TbUwAiYsSNYBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5679c46a40a03da918bbf64312668c40acd59f0b51669425c2f4eccb747d58c9","last_reissued_at":"2026-07-05T11:31:09.218800Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:31:09.218800Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Planet-induced Gas and Dust Substructure Feedbacks on Disk Thermal Structure","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Kan Chen, Mihkel Kama, Paola Pinilla","submitted_at":"2025-07-02T03:53:28Z","abstract_excerpt":"Protoplanets can interact with their natal disks and generate gas and dust substructures such as gaps and rings. However, how these planet-induced substructures affect the disk temperature, and how that in turn influences the substructures, remains unclear. We aim to study disk substructures and the thermal structure self-consistently and explore their impact on volatile distribution. To this end, we perform iterative multi-fluid hydrodynamical and radiative transfer simulations of planet-disk interactions. We find that the temperature in a structured disk deviates significantly from that of a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2507.01336","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/2507.01336/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":"2507.01336","created_at":"2026-07-05T11:31:09.218861+00:00"},{"alias_kind":"arxiv_version","alias_value":"2507.01336v2","created_at":"2026-07-05T11:31:09.218861+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2507.01336","created_at":"2026-07-05T11:31:09.218861+00:00"},{"alias_kind":"pith_short_12","alias_value":"KZ44I2SAUA62","created_at":"2026-07-05T11:31:09.218861+00:00"},{"alias_kind":"pith_short_16","alias_value":"KZ44I2SAUA62SGF3","created_at":"2026-07-05T11:31:09.218861+00:00"},{"alias_kind":"pith_short_8","alias_value":"KZ44I2SA","created_at":"2026-07-05T11:31:09.218861+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/KZ44I2SAUA62SGF36ZBREZUMIC","json":"https://pith.science/pith/KZ44I2SAUA62SGF36ZBREZUMIC.json","graph_json":"https://pith.science/api/pith-number/KZ44I2SAUA62SGF36ZBREZUMIC/graph.json","events_json":"https://pith.science/api/pith-number/KZ44I2SAUA62SGF36ZBREZUMIC/events.json","paper":"https://pith.science/paper/KZ44I2SA"},"agent_actions":{"view_html":"https://pith.science/pith/KZ44I2SAUA62SGF36ZBREZUMIC","download_json":"https://pith.science/pith/KZ44I2SAUA62SGF36ZBREZUMIC.json","view_paper":"https://pith.science/paper/KZ44I2SA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2507.01336&json=true","fetch_graph":"https://pith.science/api/pith-number/KZ44I2SAUA62SGF36ZBREZUMIC/graph.json","fetch_events":"https://pith.science/api/pith-number/KZ44I2SAUA62SGF36ZBREZUMIC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KZ44I2SAUA62SGF36ZBREZUMIC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KZ44I2SAUA62SGF36ZBREZUMIC/action/storage_attestation","attest_author":"https://pith.science/pith/KZ44I2SAUA62SGF36ZBREZUMIC/action/author_attestation","sign_citation":"https://pith.science/pith/KZ44I2SAUA62SGF36ZBREZUMIC/action/citation_signature","submit_replication":"https://pith.science/pith/KZ44I2SAUA62SGF36ZBREZUMIC/action/replication_record"}},"created_at":"2026-07-05T11:31:09.218861+00:00","updated_at":"2026-07-05T11:31:09.218861+00:00"}