{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:V5YHQK345L2EB6CHOA2CFJJBOD","short_pith_number":"pith:V5YHQK34","schema_version":"1.0","canonical_sha256":"af70782b7ceaf440f847703422a52170d4b4ffa2cb9421e2b803976092659263","source":{"kind":"arxiv","id":"1704.01626","version":1},"attestation_state":"computed","paper":{"title":"Gap formation by inclined massive planets in locally isothermal three-dimensional discs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. M. Hidalgo-Gamez, F. J. Sanchez-Salcedo, F. S. Masset, R. O. Chametla","submitted_at":"2017-04-05T19:34:14Z","abstract_excerpt":"We study gap formation in gaseous protoplanetary discs by a Jupiter mass planet. The planet's orbit is circular and inclined relative to the midplane of the disc. We use the impulse approximation to estimate the gravitational tidal torque between the planet and the disc, and infer the gap profile. For low-mass discs, we provide a criterion for gap opening when the orbital inclination is $\\leq 30^{\\circ}$. Using the FARGO3D code, we simulate the disc response to an inclined massive planet. The dependence of the depth and width of the gap obtained in the simulations on the inclination of the pla"},"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":"1704.01626","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-04-05T19:34:14Z","cross_cats_sorted":[],"title_canon_sha256":"84a7e38286d774dd2ca048bf43c35b60bf3206d558bfb227cfab978665120fa8","abstract_canon_sha256":"944eadfe62e01534502ba82c3010331c8611428677a64df0383ae45c81845375"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:43:25.763608Z","signature_b64":"k5Gjs0biqF6DsoHYLaW8Owqkbq2Kp2+bIvjI+nF4/DLvlzCPZQhNwiErdFV22l43RdohdBIGYnu23YnFDTe4DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"af70782b7ceaf440f847703422a52170d4b4ffa2cb9421e2b803976092659263","last_reissued_at":"2026-05-18T00:43:25.763062Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:43:25.763062Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gap formation by inclined massive planets in locally isothermal three-dimensional discs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. M. Hidalgo-Gamez, F. J. Sanchez-Salcedo, F. S. Masset, R. O. Chametla","submitted_at":"2017-04-05T19:34:14Z","abstract_excerpt":"We study gap formation in gaseous protoplanetary discs by a Jupiter mass planet. The planet's orbit is circular and inclined relative to the midplane of the disc. We use the impulse approximation to estimate the gravitational tidal torque between the planet and the disc, and infer the gap profile. For low-mass discs, we provide a criterion for gap opening when the orbital inclination is $\\leq 30^{\\circ}$. Using the FARGO3D code, we simulate the disc response to an inclined massive planet. The dependence of the depth and width of the gap obtained in the simulations on the inclination of the pla"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.01626","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":"1704.01626","created_at":"2026-05-18T00:43:25.763145+00:00"},{"alias_kind":"arxiv_version","alias_value":"1704.01626v1","created_at":"2026-05-18T00:43:25.763145+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1704.01626","created_at":"2026-05-18T00:43:25.763145+00:00"},{"alias_kind":"pith_short_12","alias_value":"V5YHQK345L2E","created_at":"2026-05-18T12:31:49.984773+00:00"},{"alias_kind":"pith_short_16","alias_value":"V5YHQK345L2EB6CH","created_at":"2026-05-18T12:31:49.984773+00:00"},{"alias_kind":"pith_short_8","alias_value":"V5YHQK34","created_at":"2026-05-18T12:31:49.984773+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/V5YHQK345L2EB6CHOA2CFJJBOD","json":"https://pith.science/pith/V5YHQK345L2EB6CHOA2CFJJBOD.json","graph_json":"https://pith.science/api/pith-number/V5YHQK345L2EB6CHOA2CFJJBOD/graph.json","events_json":"https://pith.science/api/pith-number/V5YHQK345L2EB6CHOA2CFJJBOD/events.json","paper":"https://pith.science/paper/V5YHQK34"},"agent_actions":{"view_html":"https://pith.science/pith/V5YHQK345L2EB6CHOA2CFJJBOD","download_json":"https://pith.science/pith/V5YHQK345L2EB6CHOA2CFJJBOD.json","view_paper":"https://pith.science/paper/V5YHQK34","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1704.01626&json=true","fetch_graph":"https://pith.science/api/pith-number/V5YHQK345L2EB6CHOA2CFJJBOD/graph.json","fetch_events":"https://pith.science/api/pith-number/V5YHQK345L2EB6CHOA2CFJJBOD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/V5YHQK345L2EB6CHOA2CFJJBOD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/V5YHQK345L2EB6CHOA2CFJJBOD/action/storage_attestation","attest_author":"https://pith.science/pith/V5YHQK345L2EB6CHOA2CFJJBOD/action/author_attestation","sign_citation":"https://pith.science/pith/V5YHQK345L2EB6CHOA2CFJJBOD/action/citation_signature","submit_replication":"https://pith.science/pith/V5YHQK345L2EB6CHOA2CFJJBOD/action/replication_record"}},"created_at":"2026-05-18T00:43:25.763145+00:00","updated_at":"2026-05-18T00:43:25.763145+00:00"}