{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:MTSQUPKBWYTDXQHZCCKAT3J4AD","short_pith_number":"pith:MTSQUPKB","schema_version":"1.0","canonical_sha256":"64e50a3d41b6263bc0f9109409ed3c00f707c5ca370fe493850b553e85dccef6","source":{"kind":"arxiv","id":"0802.1249","version":3},"attestation_state":"computed","paper":{"title":"The third post-Newtonian gravitational wave polarisations and associated spherical harmonic modes for inspiralling compact binaries in quasi-circular orbits","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bala R. Iyer, Guillaume Faye, Luc Blanchet, Siddhartha Sinha","submitted_at":"2008-02-09T07:12:40Z","abstract_excerpt":"The gravitational waveform (GWF) generated by inspiralling compact binaries moving in quasi-circular orbits is computed at the third post-Newtonian (3PN) approximation to general relativity. Our motivation is two-fold: (i) To provide accurate templates for the data analysis of gravitational wave inspiral signals in laser interferometric detectors; (ii) To provide the associated spin-weighted spherical harmonic decomposition to facilitate comparison and match of the high post-Newtonian prediction for the inspiral waveform to the numerically-generated waveforms for the merger and ringdown. This "},"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":"0802.1249","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2008-02-09T07:12:40Z","cross_cats_sorted":[],"title_canon_sha256":"4adc1100bc7d6be9265f91439ca1c5ef1a6462e108c14f5c55416e629c739f90","abstract_canon_sha256":"4daa1b7305524d22f7cd04c0c73b9f47793d7ce26ceac570aee01260b76f58a5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:42:53.432727Z","signature_b64":"QzOpCoaQf3VDat5cnQkaLS77vwfUx6iSsqojnbIaRXyCFpOlqJrYkytCi3nD1tU1QO/+i6D0/nyqdxWRwU/rDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"64e50a3d41b6263bc0f9109409ed3c00f707c5ca370fe493850b553e85dccef6","last_reissued_at":"2026-05-18T03:42:53.432067Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:42:53.432067Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The third post-Newtonian gravitational wave polarisations and associated spherical harmonic modes for inspiralling compact binaries in quasi-circular orbits","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bala R. Iyer, Guillaume Faye, Luc Blanchet, Siddhartha Sinha","submitted_at":"2008-02-09T07:12:40Z","abstract_excerpt":"The gravitational waveform (GWF) generated by inspiralling compact binaries moving in quasi-circular orbits is computed at the third post-Newtonian (3PN) approximation to general relativity. Our motivation is two-fold: (i) To provide accurate templates for the data analysis of gravitational wave inspiral signals in laser interferometric detectors; (ii) To provide the associated spin-weighted spherical harmonic decomposition to facilitate comparison and match of the high post-Newtonian prediction for the inspiral waveform to the numerically-generated waveforms for the merger and ringdown. This "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0802.1249","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":"0802.1249","created_at":"2026-05-18T03:42:53.432165+00:00"},{"alias_kind":"arxiv_version","alias_value":"0802.1249v3","created_at":"2026-05-18T03:42:53.432165+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0802.1249","created_at":"2026-05-18T03:42:53.432165+00:00"},{"alias_kind":"pith_short_12","alias_value":"MTSQUPKBWYTD","created_at":"2026-05-18T12:25:57.157939+00:00"},{"alias_kind":"pith_short_16","alias_value":"MTSQUPKBWYTDXQHZ","created_at":"2026-05-18T12:25:57.157939+00:00"},{"alias_kind":"pith_short_8","alias_value":"MTSQUPKB","created_at":"2026-05-18T12:25:57.157939+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2407.00366","citing_title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","ref_index":29,"is_internal_anchor":true},{"citing_arxiv_id":"2605.20562","citing_title":"Convergence of post-Newtonian for quasi-circular non-precessing comparable mass ratios BBHs","ref_index":42,"is_internal_anchor":true},{"citing_arxiv_id":"2004.06503","citing_title":"Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes","ref_index":121,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MTSQUPKBWYTDXQHZCCKAT3J4AD","json":"https://pith.science/pith/MTSQUPKBWYTDXQHZCCKAT3J4AD.json","graph_json":"https://pith.science/api/pith-number/MTSQUPKBWYTDXQHZCCKAT3J4AD/graph.json","events_json":"https://pith.science/api/pith-number/MTSQUPKBWYTDXQHZCCKAT3J4AD/events.json","paper":"https://pith.science/paper/MTSQUPKB"},"agent_actions":{"view_html":"https://pith.science/pith/MTSQUPKBWYTDXQHZCCKAT3J4AD","download_json":"https://pith.science/pith/MTSQUPKBWYTDXQHZCCKAT3J4AD.json","view_paper":"https://pith.science/paper/MTSQUPKB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0802.1249&json=true","fetch_graph":"https://pith.science/api/pith-number/MTSQUPKBWYTDXQHZCCKAT3J4AD/graph.json","fetch_events":"https://pith.science/api/pith-number/MTSQUPKBWYTDXQHZCCKAT3J4AD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MTSQUPKBWYTDXQHZCCKAT3J4AD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MTSQUPKBWYTDXQHZCCKAT3J4AD/action/storage_attestation","attest_author":"https://pith.science/pith/MTSQUPKBWYTDXQHZCCKAT3J4AD/action/author_attestation","sign_citation":"https://pith.science/pith/MTSQUPKBWYTDXQHZCCKAT3J4AD/action/citation_signature","submit_replication":"https://pith.science/pith/MTSQUPKBWYTDXQHZCCKAT3J4AD/action/replication_record"}},"created_at":"2026-05-18T03:42:53.432165+00:00","updated_at":"2026-05-18T03:42:53.432165+00:00"}