{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:FGQQGGD2OV3QWOV5SNBTWP2ASP","short_pith_number":"pith:FGQQGGD2","schema_version":"1.0","canonical_sha256":"29a103187a75770b3abd93433b3f4093d21d7765cc39a36ffe3838e95503f78d","source":{"kind":"arxiv","id":"gr-qc/0406012","version":1},"attestation_state":"computed","paper":{"title":"Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bala R. Iyer, Gilles Esposito-Farese, Luc Blanchet, Thibault Damour","submitted_at":"2004-06-03T14:31:12Z","abstract_excerpt":"The gravitational radiation from point particle binaries is computed at the third post-Newtonian (3PN) approximation of general relativity. Three previously introduced ambiguity parameters, coming from the Hadamard self-field regularization of the 3PN source-type mass quadrupole moment, are consistently determined by means of dimensional regularization, and proved to have the values xi = -9871/9240, kappa = 0 and zeta = -7/33. These results complete the derivation of the general relativistic prediction for compact binary inspiral up to 3.5PN order, and should be of use for searching and deciph"},"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/0406012","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"2004-06-03T14:31:12Z","cross_cats_sorted":[],"title_canon_sha256":"75aa6eec32d569df1e3935e439baf65df2c5640af4e7cf9bf9f75d0428ca42a3","abstract_canon_sha256":"67e57c89abb8667c45a410ab1d2cd34d3ec34aa68d5cedccf1afdfc20d5ed3df"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:43:38.925308Z","signature_b64":"qhfnfVxH9A6pnmm3dp6+tk7ZtQ6feNFDWOYPSLfGb/dyK7O3/lCOMa2u2b0wSggEZsN8FphxPsLvF89zMIy5AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"29a103187a75770b3abd93433b3f4093d21d7765cc39a36ffe3838e95503f78d","last_reissued_at":"2026-07-04T15:43:38.924966Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:43:38.924966Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bala R. Iyer, Gilles Esposito-Farese, Luc Blanchet, Thibault Damour","submitted_at":"2004-06-03T14:31:12Z","abstract_excerpt":"The gravitational radiation from point particle binaries is computed at the third post-Newtonian (3PN) approximation of general relativity. Three previously introduced ambiguity parameters, coming from the Hadamard self-field regularization of the 3PN source-type mass quadrupole moment, are consistently determined by means of dimensional regularization, and proved to have the values xi = -9871/9240, kappa = 0 and zeta = -7/33. These results complete the derivation of the general relativistic prediction for compact binary inspiral up to 3.5PN order, and should be of use for searching and deciph"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/0406012","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/gr-qc/0406012/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":"gr-qc/0406012","created_at":"2026-07-04T15:43:38.925023+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/0406012v1","created_at":"2026-07-04T15:43:38.925023+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/0406012","created_at":"2026-07-04T15:43:38.925023+00:00"},{"alias_kind":"pith_short_12","alias_value":"FGQQGGD2OV3Q","created_at":"2026-07-04T15:43:38.925023+00:00"},{"alias_kind":"pith_short_16","alias_value":"FGQQGGD2OV3QWOV5","created_at":"2026-07-04T15:43:38.925023+00:00"},{"alias_kind":"pith_short_8","alias_value":"FGQQGGD2","created_at":"2026-07-04T15:43:38.925023+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"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":13,"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":19,"is_internal_anchor":true},{"citing_arxiv_id":"1903.04467","citing_title":"Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1","ref_index":94,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FGQQGGD2OV3QWOV5SNBTWP2ASP","json":"https://pith.science/pith/FGQQGGD2OV3QWOV5SNBTWP2ASP.json","graph_json":"https://pith.science/api/pith-number/FGQQGGD2OV3QWOV5SNBTWP2ASP/graph.json","events_json":"https://pith.science/api/pith-number/FGQQGGD2OV3QWOV5SNBTWP2ASP/events.json","paper":"https://pith.science/paper/FGQQGGD2"},"agent_actions":{"view_html":"https://pith.science/pith/FGQQGGD2OV3QWOV5SNBTWP2ASP","download_json":"https://pith.science/pith/FGQQGGD2OV3QWOV5SNBTWP2ASP.json","view_paper":"https://pith.science/paper/FGQQGGD2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/0406012&json=true","fetch_graph":"https://pith.science/api/pith-number/FGQQGGD2OV3QWOV5SNBTWP2ASP/graph.json","fetch_events":"https://pith.science/api/pith-number/FGQQGGD2OV3QWOV5SNBTWP2ASP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FGQQGGD2OV3QWOV5SNBTWP2ASP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FGQQGGD2OV3QWOV5SNBTWP2ASP/action/storage_attestation","attest_author":"https://pith.science/pith/FGQQGGD2OV3QWOV5SNBTWP2ASP/action/author_attestation","sign_citation":"https://pith.science/pith/FGQQGGD2OV3QWOV5SNBTWP2ASP/action/citation_signature","submit_replication":"https://pith.science/pith/FGQQGGD2OV3QWOV5SNBTWP2ASP/action/replication_record"}},"created_at":"2026-07-04T15:43:38.925023+00:00","updated_at":"2026-07-04T15:43:38.925023+00:00"}