{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:GLJEKVMQ3HMDAR5YPPDSM2GGHF","short_pith_number":"pith:GLJEKVMQ","schema_version":"1.0","canonical_sha256":"32d2455590d9d83047b87bc72668c6395b92b12173d54830d8e616b627cf13a1","source":{"kind":"arxiv","id":"1608.08756","version":1},"attestation_state":"computed","paper":{"title":"Migration of accreting planets in radiative discs from dynamical torques","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Arnaud Pierens, Sean Raymond","submitted_at":"2016-08-31T08:01:58Z","abstract_excerpt":"We present the results of hydrodynamical simulations of the orbital evolution of planets undergoing runaway gas accretion in radiative discs. We consider accreting disc models with constant mass flux through the disc, and where radiative cooling balances the effect of viscous heating and stellar irradiation. We assume that 20-30 $M_\\oplus$ giant planet cores are formed in the region where viscous heating dominates and migrate outward under the action of a strong corotation torque. In the case where gas accretion is neglected, we find evidence for strong dynamical torques in accreting discs wit"},"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":"1608.08756","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-08-31T08:01:58Z","cross_cats_sorted":[],"title_canon_sha256":"74c40304f721b279266a91351e2afea7fd36f23f39b28c5da1c38fa0e1f37226","abstract_canon_sha256":"3bd08e6285ca018b77bd79a2eebb593d8107b76018ad69a37d052f78b6f30296"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:04:17.557362Z","signature_b64":"FuuF0xJ/XDlDJGeIE6yO2bqvcOgyDSe0nj7hLPKgwhRzRLFN/jwe80KYFuTk9sgNGkW1r7MpfeHBVM3QeOaBAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"32d2455590d9d83047b87bc72668c6395b92b12173d54830d8e616b627cf13a1","last_reissued_at":"2026-05-18T01:04:17.556833Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:04:17.556833Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Migration of accreting planets in radiative discs from dynamical torques","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Arnaud Pierens, Sean Raymond","submitted_at":"2016-08-31T08:01:58Z","abstract_excerpt":"We present the results of hydrodynamical simulations of the orbital evolution of planets undergoing runaway gas accretion in radiative discs. We consider accreting disc models with constant mass flux through the disc, and where radiative cooling balances the effect of viscous heating and stellar irradiation. We assume that 20-30 $M_\\oplus$ giant planet cores are formed in the region where viscous heating dominates and migrate outward under the action of a strong corotation torque. In the case where gas accretion is neglected, we find evidence for strong dynamical torques in accreting discs wit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.08756","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":"1608.08756","created_at":"2026-05-18T01:04:17.556911+00:00"},{"alias_kind":"arxiv_version","alias_value":"1608.08756v1","created_at":"2026-05-18T01:04:17.556911+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1608.08756","created_at":"2026-05-18T01:04:17.556911+00:00"},{"alias_kind":"pith_short_12","alias_value":"GLJEKVMQ3HMD","created_at":"2026-05-18T12:30:19.053100+00:00"},{"alias_kind":"pith_short_16","alias_value":"GLJEKVMQ3HMDAR5Y","created_at":"2026-05-18T12:30:19.053100+00:00"},{"alias_kind":"pith_short_8","alias_value":"GLJEKVMQ","created_at":"2026-05-18T12:30:19.053100+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/GLJEKVMQ3HMDAR5YPPDSM2GGHF","json":"https://pith.science/pith/GLJEKVMQ3HMDAR5YPPDSM2GGHF.json","graph_json":"https://pith.science/api/pith-number/GLJEKVMQ3HMDAR5YPPDSM2GGHF/graph.json","events_json":"https://pith.science/api/pith-number/GLJEKVMQ3HMDAR5YPPDSM2GGHF/events.json","paper":"https://pith.science/paper/GLJEKVMQ"},"agent_actions":{"view_html":"https://pith.science/pith/GLJEKVMQ3HMDAR5YPPDSM2GGHF","download_json":"https://pith.science/pith/GLJEKVMQ3HMDAR5YPPDSM2GGHF.json","view_paper":"https://pith.science/paper/GLJEKVMQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1608.08756&json=true","fetch_graph":"https://pith.science/api/pith-number/GLJEKVMQ3HMDAR5YPPDSM2GGHF/graph.json","fetch_events":"https://pith.science/api/pith-number/GLJEKVMQ3HMDAR5YPPDSM2GGHF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GLJEKVMQ3HMDAR5YPPDSM2GGHF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GLJEKVMQ3HMDAR5YPPDSM2GGHF/action/storage_attestation","attest_author":"https://pith.science/pith/GLJEKVMQ3HMDAR5YPPDSM2GGHF/action/author_attestation","sign_citation":"https://pith.science/pith/GLJEKVMQ3HMDAR5YPPDSM2GGHF/action/citation_signature","submit_replication":"https://pith.science/pith/GLJEKVMQ3HMDAR5YPPDSM2GGHF/action/replication_record"}},"created_at":"2026-05-18T01:04:17.556911+00:00","updated_at":"2026-05-18T01:04:17.556911+00:00"}