{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:DIGR6FRUILS26Z6VGPYF5RJG3R","short_pith_number":"pith:DIGR6FRU","schema_version":"1.0","canonical_sha256":"1a0d1f163442e5af67d533f05ec526dc5e557049885a3d26b753e2d12d13cd9c","source":{"kind":"arxiv","id":"1805.01487","version":3},"attestation_state":"computed","paper":{"title":"Post-Newtonian spin-tidal couplings for compact binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","astro-ph.SR"],"primary_cat":"gr-qc","authors_text":"Leonardo Gualtieri, Paolo Pani, Tiziano Abdelsalhin","submitted_at":"2018-05-03T18:03:19Z","abstract_excerpt":"We compute the spin-tidal couplings that affect the dynamics of two orbiting bodies at the leading order in the post-Newtonian (PN) framework and to linear order in the spin. These corrections belong to two classes: (i) terms arising from the coupling between the ordinary tidal terms and the point-particle terms, which depend on the standard tidal Love numbers of order $l$ and affect the gravitational-wave (GW) phase at $(2l+5/2)$PN order and (ii) terms depending on the rotational tidal Love numbers, recently introduced in previous work, that affect the GW phase at $(2l+1/2+\\delta_{2l})$PN ord"},"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":"1805.01487","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2018-05-03T18:03:19Z","cross_cats_sorted":["astro-ph.HE","astro-ph.SR"],"title_canon_sha256":"b30842448c5af9df9fb834218dff0841d28f0b6c31f7659f602b333484d86a3c","abstract_canon_sha256":"5181c3f4e4e92d28b79b40cf4f4757bf7cef9fb893521421b110a55a810eab79"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:59:17.203475Z","signature_b64":"qIk1tbuoyFstjqFZEXnMr9wRh3hROC+ADtx8702FJ9xVB9X1R0LLtozM09rN0yOa8evfIGj25jreDe60qjkzCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1a0d1f163442e5af67d533f05ec526dc5e557049885a3d26b753e2d12d13cd9c","last_reissued_at":"2026-05-17T23:59:17.202980Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:59:17.202980Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Post-Newtonian spin-tidal couplings for compact binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","astro-ph.SR"],"primary_cat":"gr-qc","authors_text":"Leonardo Gualtieri, Paolo Pani, Tiziano Abdelsalhin","submitted_at":"2018-05-03T18:03:19Z","abstract_excerpt":"We compute the spin-tidal couplings that affect the dynamics of two orbiting bodies at the leading order in the post-Newtonian (PN) framework and to linear order in the spin. These corrections belong to two classes: (i) terms arising from the coupling between the ordinary tidal terms and the point-particle terms, which depend on the standard tidal Love numbers of order $l$ and affect the gravitational-wave (GW) phase at $(2l+5/2)$PN order and (ii) terms depending on the rotational tidal Love numbers, recently introduced in previous work, that affect the GW phase at $(2l+1/2+\\delta_{2l})$PN ord"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1805.01487","kind":"arxiv","version":3},"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":"1805.01487","created_at":"2026-05-17T23:59:17.203042+00:00"},{"alias_kind":"arxiv_version","alias_value":"1805.01487v3","created_at":"2026-05-17T23:59:17.203042+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1805.01487","created_at":"2026-05-17T23:59:17.203042+00:00"},{"alias_kind":"pith_short_12","alias_value":"DIGR6FRUILS2","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_16","alias_value":"DIGR6FRUILS26Z6V","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_8","alias_value":"DIGR6FRU","created_at":"2026-05-18T12:32:19.392346+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.11903","citing_title":"Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects","ref_index":70,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DIGR6FRUILS26Z6VGPYF5RJG3R","json":"https://pith.science/pith/DIGR6FRUILS26Z6VGPYF5RJG3R.json","graph_json":"https://pith.science/api/pith-number/DIGR6FRUILS26Z6VGPYF5RJG3R/graph.json","events_json":"https://pith.science/api/pith-number/DIGR6FRUILS26Z6VGPYF5RJG3R/events.json","paper":"https://pith.science/paper/DIGR6FRU"},"agent_actions":{"view_html":"https://pith.science/pith/DIGR6FRUILS26Z6VGPYF5RJG3R","download_json":"https://pith.science/pith/DIGR6FRUILS26Z6VGPYF5RJG3R.json","view_paper":"https://pith.science/paper/DIGR6FRU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1805.01487&json=true","fetch_graph":"https://pith.science/api/pith-number/DIGR6FRUILS26Z6VGPYF5RJG3R/graph.json","fetch_events":"https://pith.science/api/pith-number/DIGR6FRUILS26Z6VGPYF5RJG3R/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DIGR6FRUILS26Z6VGPYF5RJG3R/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DIGR6FRUILS26Z6VGPYF5RJG3R/action/storage_attestation","attest_author":"https://pith.science/pith/DIGR6FRUILS26Z6VGPYF5RJG3R/action/author_attestation","sign_citation":"https://pith.science/pith/DIGR6FRUILS26Z6VGPYF5RJG3R/action/citation_signature","submit_replication":"https://pith.science/pith/DIGR6FRUILS26Z6VGPYF5RJG3R/action/replication_record"}},"created_at":"2026-05-17T23:59:17.203042+00:00","updated_at":"2026-05-17T23:59:17.203042+00:00"}