{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:NX72XZIXAH7B3FKSRU66YVYEHE","short_pith_number":"pith:NX72XZIX","schema_version":"1.0","canonical_sha256":"6dffabe51701fe1d95528d3dec5704390457cd11efd8f4696816c7090e514ee5","source":{"kind":"arxiv","id":"gr-qc/0605140","version":4},"attestation_state":"computed","paper":{"title":"Higher-order spin effects in the dynamics of compact binaries II. Radiation field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Alessandra Buonanno (IAP, APC), Department of Physics, Guillaume Faye (IAP), Luc Blanchet (IAP), University of Maryland","submitted_at":"2006-05-27T05:13:27Z","abstract_excerpt":"Motivated by the search for gravitational waves emitted by binary black holes, we investigate the gravitational radiation field of point particles with spins within the framework of the multipolar-post-Newtonian wave generation formalism. We compute: (i) the spin-orbit (SO) coupling effects in the binary's mass and current quadrupole moments one post-Newtonian (1PN) order beyond the dominant effect, (ii) the SO contributions in the gravitational-wave energy flux and (iii) the secular evolution of the binary's orbital phase up to 2.5PN order. Crucial ingredients for obtaining the 2.5PN contribu"},"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":"gr-qc/0605140","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2006-05-27T05:13:27Z","cross_cats_sorted":[],"title_canon_sha256":"ea9f06d4061cbd981dfc105ecf92edd478347747a1db1dd15f057351e4256a5b","abstract_canon_sha256":"d56fcdbc994d00a6b31ad886ddcc40c4693d571b55b138b0c8d495944506cb6b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:37:27.174228Z","signature_b64":"MlLzfL//8W0fQatJN2qG9BA0Z/7efcJXN1E/OAXmRwJCnmCn6E0kf9OyoTByEcJG3bVUSPDRMRuF1Uc9q8K0Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6dffabe51701fe1d95528d3dec5704390457cd11efd8f4696816c7090e514ee5","last_reissued_at":"2026-05-18T02:37:27.173703Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:37:27.173703Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Higher-order spin effects in the dynamics of compact binaries II. Radiation field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Alessandra Buonanno (IAP, APC), Department of Physics, Guillaume Faye (IAP), Luc Blanchet (IAP), University of Maryland","submitted_at":"2006-05-27T05:13:27Z","abstract_excerpt":"Motivated by the search for gravitational waves emitted by binary black holes, we investigate the gravitational radiation field of point particles with spins within the framework of the multipolar-post-Newtonian wave generation formalism. We compute: (i) the spin-orbit (SO) coupling effects in the binary's mass and current quadrupole moments one post-Newtonian (1PN) order beyond the dominant effect, (ii) the SO contributions in the gravitational-wave energy flux and (iii) the secular evolution of the binary's orbital phase up to 2.5PN order. Crucial ingredients for obtaining the 2.5PN contribu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/0605140","kind":"arxiv","version":4},"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":"gr-qc/0605140","created_at":"2026-05-18T02:37:27.173785+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/0605140v4","created_at":"2026-05-18T02:37:27.173785+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/0605140","created_at":"2026-05-18T02:37:27.173785+00:00"},{"alias_kind":"pith_short_12","alias_value":"NX72XZIXAH7B","created_at":"2026-05-18T12:25:54.717736+00:00"},{"alias_kind":"pith_short_16","alias_value":"NX72XZIXAH7B3FKS","created_at":"2026-05-18T12:25:54.717736+00:00"},{"alias_kind":"pith_short_8","alias_value":"NX72XZIX","created_at":"2026-05-18T12:25:54.717736+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2305.15473","citing_title":"Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter","ref_index":12,"is_internal_anchor":true},{"citing_arxiv_id":"2510.07390","citing_title":"Heterotic Footprints in Classical Gravity: PM dynamics from On-Shell soft amplitudes at one loop","ref_index":21,"is_internal_anchor":true},{"citing_arxiv_id":"2602.18790","citing_title":"Generalized Carter & R\\\"udiger Constants of $\\sqrt{\\text{Kerr}}$","ref_index":18,"is_internal_anchor":true},{"citing_arxiv_id":"2010.14529","citing_title":"Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog","ref_index":149,"is_internal_anchor":true},{"citing_arxiv_id":"1310.1528","citing_title":"Post-Newtonian Theory for Gravitational Waves","ref_index":81,"is_internal_anchor":false},{"citing_arxiv_id":"2112.06861","citing_title":"Tests of General Relativity with GWTC-3","ref_index":174,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NX72XZIXAH7B3FKSRU66YVYEHE","json":"https://pith.science/pith/NX72XZIXAH7B3FKSRU66YVYEHE.json","graph_json":"https://pith.science/api/pith-number/NX72XZIXAH7B3FKSRU66YVYEHE/graph.json","events_json":"https://pith.science/api/pith-number/NX72XZIXAH7B3FKSRU66YVYEHE/events.json","paper":"https://pith.science/paper/NX72XZIX"},"agent_actions":{"view_html":"https://pith.science/pith/NX72XZIXAH7B3FKSRU66YVYEHE","download_json":"https://pith.science/pith/NX72XZIXAH7B3FKSRU66YVYEHE.json","view_paper":"https://pith.science/paper/NX72XZIX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/0605140&json=true","fetch_graph":"https://pith.science/api/pith-number/NX72XZIXAH7B3FKSRU66YVYEHE/graph.json","fetch_events":"https://pith.science/api/pith-number/NX72XZIXAH7B3FKSRU66YVYEHE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NX72XZIXAH7B3FKSRU66YVYEHE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NX72XZIXAH7B3FKSRU66YVYEHE/action/storage_attestation","attest_author":"https://pith.science/pith/NX72XZIXAH7B3FKSRU66YVYEHE/action/author_attestation","sign_citation":"https://pith.science/pith/NX72XZIXAH7B3FKSRU66YVYEHE/action/citation_signature","submit_replication":"https://pith.science/pith/NX72XZIXAH7B3FKSRU66YVYEHE/action/replication_record"}},"created_at":"2026-05-18T02:37:27.173785+00:00","updated_at":"2026-05-18T02:37:27.173785+00:00"}