{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:U4D2EEWEWOMPURDITCCIYRNA2Z","short_pith_number":"pith:U4D2EEWE","schema_version":"1.0","canonical_sha256":"a707a212c4b398fa446898848c45a0d64dcaef65b63b047689863a38cc2e952c","source":{"kind":"arxiv","id":"1202.0790","version":2},"attestation_state":"computed","paper":{"title":"Prototype effective-one-body model for nonprecessing spinning inspiral-merger-ringdown waveforms","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Alessandra Buonanno, Andrea Taracchini, Enrico Barausse, Geoffrey Lovelace, Harald P. Pfeiffer, Mark A. Scheel, Michael Boyle, Tony Chu, Yi Pan","submitted_at":"2012-02-03T18:06:36Z","abstract_excerpt":"We first use five non-spinning and two mildly spinning (chi_i \\simeq -0.44, +0.44) numerical-relativity waveforms of black-hole binaries and calibrate an effective-one-body (EOB) model for non-precessing spinning binaries, notably its dynamics and the dominant (2,2) gravitational-wave mode. Then, we combine the above results with recent outcomes of small-mass-ratio simulations produced by the Teukolsky equation and build a prototype EOB model for detection purposes, which is capable of generating inspiral-merger-ringdown waveforms for non-precessing spinning black-hole binaries with any mass r"},"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":"1202.0790","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2012-02-03T18:06:36Z","cross_cats_sorted":[],"title_canon_sha256":"33cf2004648ddb5f95a71ff28137036f408b6785bb1e66c9528f63418b4ff0ac","abstract_canon_sha256":"9e3556b62a8e591c80e0c25957b9ad18e7f8dbfc03ed702ce955eeaba912bcec"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:48:24.261343Z","signature_b64":"FKC7StrrSpcmH5xTp0cHqmTTx81MYdAOJ2UwpmnkV71wVibnkUEEEpIxvS3/BlgllCXqVq8ogd2lRkx1rFk5Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a707a212c4b398fa446898848c45a0d64dcaef65b63b047689863a38cc2e952c","last_reissued_at":"2026-05-18T03:48:24.260496Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:48:24.260496Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Prototype effective-one-body model for nonprecessing spinning inspiral-merger-ringdown waveforms","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Alessandra Buonanno, Andrea Taracchini, Enrico Barausse, Geoffrey Lovelace, Harald P. Pfeiffer, Mark A. Scheel, Michael Boyle, Tony Chu, Yi Pan","submitted_at":"2012-02-03T18:06:36Z","abstract_excerpt":"We first use five non-spinning and two mildly spinning (chi_i \\simeq -0.44, +0.44) numerical-relativity waveforms of black-hole binaries and calibrate an effective-one-body (EOB) model for non-precessing spinning binaries, notably its dynamics and the dominant (2,2) gravitational-wave mode. Then, we combine the above results with recent outcomes of small-mass-ratio simulations produced by the Teukolsky equation and build a prototype EOB model for detection purposes, which is capable of generating inspiral-merger-ringdown waveforms for non-precessing spinning black-hole binaries with any mass r"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1202.0790","kind":"arxiv","version":2},"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":"1202.0790","created_at":"2026-05-18T03:48:24.260623+00:00"},{"alias_kind":"arxiv_version","alias_value":"1202.0790v2","created_at":"2026-05-18T03:48:24.260623+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1202.0790","created_at":"2026-05-18T03:48:24.260623+00:00"},{"alias_kind":"pith_short_12","alias_value":"U4D2EEWEWOMP","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_16","alias_value":"U4D2EEWEWOMPURDI","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_8","alias_value":"U4D2EEWE","created_at":"2026-05-18T12:27:23.164592+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/U4D2EEWEWOMPURDITCCIYRNA2Z","json":"https://pith.science/pith/U4D2EEWEWOMPURDITCCIYRNA2Z.json","graph_json":"https://pith.science/api/pith-number/U4D2EEWEWOMPURDITCCIYRNA2Z/graph.json","events_json":"https://pith.science/api/pith-number/U4D2EEWEWOMPURDITCCIYRNA2Z/events.json","paper":"https://pith.science/paper/U4D2EEWE"},"agent_actions":{"view_html":"https://pith.science/pith/U4D2EEWEWOMPURDITCCIYRNA2Z","download_json":"https://pith.science/pith/U4D2EEWEWOMPURDITCCIYRNA2Z.json","view_paper":"https://pith.science/paper/U4D2EEWE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1202.0790&json=true","fetch_graph":"https://pith.science/api/pith-number/U4D2EEWEWOMPURDITCCIYRNA2Z/graph.json","fetch_events":"https://pith.science/api/pith-number/U4D2EEWEWOMPURDITCCIYRNA2Z/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/U4D2EEWEWOMPURDITCCIYRNA2Z/action/timestamp_anchor","attest_storage":"https://pith.science/pith/U4D2EEWEWOMPURDITCCIYRNA2Z/action/storage_attestation","attest_author":"https://pith.science/pith/U4D2EEWEWOMPURDITCCIYRNA2Z/action/author_attestation","sign_citation":"https://pith.science/pith/U4D2EEWEWOMPURDITCCIYRNA2Z/action/citation_signature","submit_replication":"https://pith.science/pith/U4D2EEWEWOMPURDITCCIYRNA2Z/action/replication_record"}},"created_at":"2026-05-18T03:48:24.260623+00:00","updated_at":"2026-05-18T03:48:24.260623+00:00"}