{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2007:UWYFM2FKYBANDUBLDW6NSP75GD","short_pith_number":"pith:UWYFM2FK","schema_version":"1.0","canonical_sha256":"a5b05668aac040d1d02b1dbcd93ffd30f5b9ada7c56a4cc4520ab5c3870af601","source":{"kind":"arxiv","id":"0709.2160","version":3},"attestation_state":"computed","paper":{"title":"High-spin binary black hole mergers","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"(2) University of Jena), Bernd Br\\\"ugmann (2), Jose Gonz\\'alez (2), Pedro Marronetti (1), Ulrich Sperhake (2) ((1) Florida Atlantic University, Wolfgang Tichy (1)","submitted_at":"2007-09-13T19:55:10Z","abstract_excerpt":"We study identical mass black hole binaries with spins perpendicular to the binary's orbital plane. These binaries have individual spins ranging from $s/m^2=-0.90$ to 0.90, ($s_1 = s_2$ in all cases) which is near the limit possible with standard Bowen-York puncture initial data. The extreme cases correspond to the largest initial spin simulations to date. Our results expand the parameter space covered by Rezzolla {\\it et al.} and, when combining both data sets, we obtain estimations for the minimum and maximum values for the intrinsic angular momenta of the remnant of binary black hole merger"},"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":"0709.2160","kind":"arxiv","version":3},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"2007-09-13T19:55:10Z","cross_cats_sorted":[],"title_canon_sha256":"e9341130ddce528ad8ba20472f5e8ceb17abee43ce09832d026fad7f7fff3ad5","abstract_canon_sha256":"2271d3be5253083b9c437abb071a84deaba27cd2f5de83b35d35570ba1779c15"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:30:34.424475Z","signature_b64":"OWG0PQPMuesAdKVsiU/1OE60K5LoIwb1YjhLYemus3Phgp2sspFUk8fxosOO+0ZB3esOM/oRh/D0Ltg7FO70DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a5b05668aac040d1d02b1dbcd93ffd30f5b9ada7c56a4cc4520ab5c3870af601","last_reissued_at":"2026-07-04T15:30:34.424054Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:30:34.424054Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High-spin binary black hole mergers","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"(2) University of Jena), Bernd Br\\\"ugmann (2), Jose Gonz\\'alez (2), Pedro Marronetti (1), Ulrich Sperhake (2) ((1) Florida Atlantic University, Wolfgang Tichy (1)","submitted_at":"2007-09-13T19:55:10Z","abstract_excerpt":"We study identical mass black hole binaries with spins perpendicular to the binary's orbital plane. These binaries have individual spins ranging from $s/m^2=-0.90$ to 0.90, ($s_1 = s_2$ in all cases) which is near the limit possible with standard Bowen-York puncture initial data. The extreme cases correspond to the largest initial spin simulations to date. Our results expand the parameter space covered by Rezzolla {\\it et al.} and, when combining both data sets, we obtain estimations for the minimum and maximum values for the intrinsic angular momenta of the remnant of binary black hole merger"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0709.2160","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/0709.2160/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":"0709.2160","created_at":"2026-07-04T15:30:34.424114+00:00"},{"alias_kind":"arxiv_version","alias_value":"0709.2160v3","created_at":"2026-07-04T15:30:34.424114+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0709.2160","created_at":"2026-07-04T15:30:34.424114+00:00"},{"alias_kind":"pith_short_12","alias_value":"UWYFM2FKYBAN","created_at":"2026-07-04T15:30:34.424114+00:00"},{"alias_kind":"pith_short_16","alias_value":"UWYFM2FKYBANDUBL","created_at":"2026-07-04T15:30:34.424114+00:00"},{"alias_kind":"pith_short_8","alias_value":"UWYFM2FK","created_at":"2026-07-04T15:30:34.424114+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.04495","citing_title":"Eccentricity Effects on Modeling Dynamic Quantities and Their Correlations in Binary Black Hole Mergers","ref_index":95,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UWYFM2FKYBANDUBLDW6NSP75GD","json":"https://pith.science/pith/UWYFM2FKYBANDUBLDW6NSP75GD.json","graph_json":"https://pith.science/api/pith-number/UWYFM2FKYBANDUBLDW6NSP75GD/graph.json","events_json":"https://pith.science/api/pith-number/UWYFM2FKYBANDUBLDW6NSP75GD/events.json","paper":"https://pith.science/paper/UWYFM2FK"},"agent_actions":{"view_html":"https://pith.science/pith/UWYFM2FKYBANDUBLDW6NSP75GD","download_json":"https://pith.science/pith/UWYFM2FKYBANDUBLDW6NSP75GD.json","view_paper":"https://pith.science/paper/UWYFM2FK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0709.2160&json=true","fetch_graph":"https://pith.science/api/pith-number/UWYFM2FKYBANDUBLDW6NSP75GD/graph.json","fetch_events":"https://pith.science/api/pith-number/UWYFM2FKYBANDUBLDW6NSP75GD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UWYFM2FKYBANDUBLDW6NSP75GD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UWYFM2FKYBANDUBLDW6NSP75GD/action/storage_attestation","attest_author":"https://pith.science/pith/UWYFM2FKYBANDUBLDW6NSP75GD/action/author_attestation","sign_citation":"https://pith.science/pith/UWYFM2FKYBANDUBLDW6NSP75GD/action/citation_signature","submit_replication":"https://pith.science/pith/UWYFM2FKYBANDUBLDW6NSP75GD/action/replication_record"}},"created_at":"2026-07-04T15:30:34.424114+00:00","updated_at":"2026-07-04T15:30:34.424114+00:00"}