{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:MHQUCHDTXRG5X734L6BHVRHH27","short_pith_number":"pith:MHQUCHDT","schema_version":"1.0","canonical_sha256":"61e1411c73bc4ddbff7c5f827ac4e7d7de5c105c376bbb03a46a81c2b9ca30c2","source":{"kind":"arxiv","id":"2311.03576","version":1},"attestation_state":"computed","paper":{"title":"Tidal Dissipation Regimes Among the Short-Period Exoplanets","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Emma Louden, Gregory Laughlin, Sarah Millholland","submitted_at":"2023-11-06T22:22:00Z","abstract_excerpt":"The efficiency of tidal dissipation provides a zeroth-order link to a planet's physical properties. For super-Earth and sub-Neptune planets in the range $R_{\\oplus}\\lesssim R_p \\lesssim 4 R_{\\oplus}$, particularly efficient dissipation (i.e., low tidal quality factors) may signify terrestrial-like planets capable of maintaining rigid crustal features. Here we explore global constraints on planetary tidal quality factors using a population of planets in multiple-planet systems whose orbital and physical properties indicate susceptibility to capture into secular spin-orbit resonances. Planets pa"},"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":"2311.03576","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2023-11-06T22:22:00Z","cross_cats_sorted":[],"title_canon_sha256":"8391c2eb7b9614eb4f373521dedf671bc022724eac0425a428c99dc1572c672a","abstract_canon_sha256":"adb7630ac9a999fa2b01639bf07e95d5f5ca9c0d8a64ad9c06bbc96adf60ff23"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:10:00.408507Z","signature_b64":"6bMhDFTTgIueH9x7j0mlE4LC02Di0zlMqR91RwR/mjehiNihv2SfiiwgknamTzTqtqJYGTAhiEqJ9i2gJMzhBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"61e1411c73bc4ddbff7c5f827ac4e7d7de5c105c376bbb03a46a81c2b9ca30c2","last_reissued_at":"2026-07-05T07:10:00.408062Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:10:00.408062Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Tidal Dissipation Regimes Among the Short-Period Exoplanets","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Emma Louden, Gregory Laughlin, Sarah Millholland","submitted_at":"2023-11-06T22:22:00Z","abstract_excerpt":"The efficiency of tidal dissipation provides a zeroth-order link to a planet's physical properties. For super-Earth and sub-Neptune planets in the range $R_{\\oplus}\\lesssim R_p \\lesssim 4 R_{\\oplus}$, particularly efficient dissipation (i.e., low tidal quality factors) may signify terrestrial-like planets capable of maintaining rigid crustal features. Here we explore global constraints on planetary tidal quality factors using a population of planets in multiple-planet systems whose orbital and physical properties indicate susceptibility to capture into secular spin-orbit resonances. Planets pa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.03576","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2311.03576/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":"2311.03576","created_at":"2026-07-05T07:10:00.408118+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.03576v1","created_at":"2026-07-05T07:10:00.408118+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.03576","created_at":"2026-07-05T07:10:00.408118+00:00"},{"alias_kind":"pith_short_12","alias_value":"MHQUCHDTXRG5","created_at":"2026-07-05T07:10:00.408118+00:00"},{"alias_kind":"pith_short_16","alias_value":"MHQUCHDTXRG5X734","created_at":"2026-07-05T07:10:00.408118+00:00"},{"alias_kind":"pith_short_8","alias_value":"MHQUCHDT","created_at":"2026-07-05T07:10:00.408118+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2502.01903","citing_title":"Amplifying Resonant Repulsion with Inflated Young Planets, Overlooked Inner Planets, and Non-zero Initial $\\Delta$","ref_index":54,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MHQUCHDTXRG5X734L6BHVRHH27","json":"https://pith.science/pith/MHQUCHDTXRG5X734L6BHVRHH27.json","graph_json":"https://pith.science/api/pith-number/MHQUCHDTXRG5X734L6BHVRHH27/graph.json","events_json":"https://pith.science/api/pith-number/MHQUCHDTXRG5X734L6BHVRHH27/events.json","paper":"https://pith.science/paper/MHQUCHDT"},"agent_actions":{"view_html":"https://pith.science/pith/MHQUCHDTXRG5X734L6BHVRHH27","download_json":"https://pith.science/pith/MHQUCHDTXRG5X734L6BHVRHH27.json","view_paper":"https://pith.science/paper/MHQUCHDT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.03576&json=true","fetch_graph":"https://pith.science/api/pith-number/MHQUCHDTXRG5X734L6BHVRHH27/graph.json","fetch_events":"https://pith.science/api/pith-number/MHQUCHDTXRG5X734L6BHVRHH27/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MHQUCHDTXRG5X734L6BHVRHH27/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MHQUCHDTXRG5X734L6BHVRHH27/action/storage_attestation","attest_author":"https://pith.science/pith/MHQUCHDTXRG5X734L6BHVRHH27/action/author_attestation","sign_citation":"https://pith.science/pith/MHQUCHDTXRG5X734L6BHVRHH27/action/citation_signature","submit_replication":"https://pith.science/pith/MHQUCHDTXRG5X734L6BHVRHH27/action/replication_record"}},"created_at":"2026-07-05T07:10:00.408118+00:00","updated_at":"2026-07-05T07:10:00.408118+00:00"}