{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:CDW4R66ZCBGFN4GLFVV7BF5VDT","short_pith_number":"pith:CDW4R66Z","schema_version":"1.0","canonical_sha256":"10edc8fbd9104c56f0cb2d6bf097b51cf31befead695eda4ce4bc3e07465066b","source":{"kind":"arxiv","id":"1710.10058","version":1},"attestation_state":"computed","paper":{"title":"Layered semi-convection and tides in giant planet interiors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. J. Barker, Q. Andr\\'e, S. Mathis","submitted_at":"2017-10-27T10:18:32Z","abstract_excerpt":"Layered semi-convection could operate in giant planets, potentially explaining the constraints on the heavy elements distribution in Jupiter deduced recently from Juno observations, and contributing to Saturn's luminosity excess or the abnormally large radius of some hot Jupiters. This is a state consisting of density staircases, in which convective layers are separated by thin stably stratified interfaces. The efficiency of tidal dissipation in a planet depends strongly on its internal structure. It is crucial to improve our understanding of the mechanisms driving this dissipation, since it h"},"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":"1710.10058","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-10-27T10:18:32Z","cross_cats_sorted":[],"title_canon_sha256":"8db54830a92263b0d057b39f8b626058bcd9af57b67fdbbf0910882d2e7985b3","abstract_canon_sha256":"0067d6a5490a237a45705d213a2fa7bf694bc20a2d7d56a0cf03c18d90986559"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:31:54.849900Z","signature_b64":"iVDsBNCgzd4xToreJ2431Dkuy4cbtM5CMtjdllGkFuzw+skqwITrw74NzN98Xj+5y8j1V2EuGbDAK1Onh7VmDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"10edc8fbd9104c56f0cb2d6bf097b51cf31befead695eda4ce4bc3e07465066b","last_reissued_at":"2026-05-18T00:31:54.849514Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:31:54.849514Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Layered semi-convection and tides in giant planet interiors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. J. Barker, Q. Andr\\'e, S. Mathis","submitted_at":"2017-10-27T10:18:32Z","abstract_excerpt":"Layered semi-convection could operate in giant planets, potentially explaining the constraints on the heavy elements distribution in Jupiter deduced recently from Juno observations, and contributing to Saturn's luminosity excess or the abnormally large radius of some hot Jupiters. This is a state consisting of density staircases, in which convective layers are separated by thin stably stratified interfaces. The efficiency of tidal dissipation in a planet depends strongly on its internal structure. It is crucial to improve our understanding of the mechanisms driving this dissipation, since it h"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.10058","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":"1710.10058","created_at":"2026-05-18T00:31:54.849577+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.10058v1","created_at":"2026-05-18T00:31:54.849577+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.10058","created_at":"2026-05-18T00:31:54.849577+00:00"},{"alias_kind":"pith_short_12","alias_value":"CDW4R66ZCBGF","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_16","alias_value":"CDW4R66ZCBGFN4GL","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_8","alias_value":"CDW4R66Z","created_at":"2026-05-18T12:31:10.602751+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/CDW4R66ZCBGFN4GLFVV7BF5VDT","json":"https://pith.science/pith/CDW4R66ZCBGFN4GLFVV7BF5VDT.json","graph_json":"https://pith.science/api/pith-number/CDW4R66ZCBGFN4GLFVV7BF5VDT/graph.json","events_json":"https://pith.science/api/pith-number/CDW4R66ZCBGFN4GLFVV7BF5VDT/events.json","paper":"https://pith.science/paper/CDW4R66Z"},"agent_actions":{"view_html":"https://pith.science/pith/CDW4R66ZCBGFN4GLFVV7BF5VDT","download_json":"https://pith.science/pith/CDW4R66ZCBGFN4GLFVV7BF5VDT.json","view_paper":"https://pith.science/paper/CDW4R66Z","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.10058&json=true","fetch_graph":"https://pith.science/api/pith-number/CDW4R66ZCBGFN4GLFVV7BF5VDT/graph.json","fetch_events":"https://pith.science/api/pith-number/CDW4R66ZCBGFN4GLFVV7BF5VDT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CDW4R66ZCBGFN4GLFVV7BF5VDT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CDW4R66ZCBGFN4GLFVV7BF5VDT/action/storage_attestation","attest_author":"https://pith.science/pith/CDW4R66ZCBGFN4GLFVV7BF5VDT/action/author_attestation","sign_citation":"https://pith.science/pith/CDW4R66ZCBGFN4GLFVV7BF5VDT/action/citation_signature","submit_replication":"https://pith.science/pith/CDW4R66ZCBGFN4GLFVV7BF5VDT/action/replication_record"}},"created_at":"2026-05-18T00:31:54.849577+00:00","updated_at":"2026-05-18T00:31:54.849577+00:00"}