{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:HHJJBDR5OOEGLSR65OCKXAA7D2","short_pith_number":"pith:HHJJBDR5","schema_version":"1.0","canonical_sha256":"39d2908e3d738865ca3eeb84ab801f1eaf4dfdf3908f34a7ebfca177df0925a7","source":{"kind":"arxiv","id":"2312.08588","version":3},"attestation_state":"computed","paper":{"title":"Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.SR"],"primary_cat":"gr-qc","authors_text":"Harald P. Pfeiffer, Harrison Siegel, Hengrui Zhu, Jordan Moxon, Keefe Mitman, Kyle C. Nelli, Lawrence E. Kidder, Mark A. Scheel, Maximiliano Isi, Michael Boyle, Nils Deppe, Nils L. Vu, Saul A. Teukolsky, Sizheng Ma, Vijay Varma, William Throwe, Will M. Farr","submitted_at":"2023-12-14T01:19:38Z","abstract_excerpt":"The spectroscopic study of black hole quasinormal modes in gravitational-wave ringdown observations is hindered by our ignorance of which modes should dominate astrophysical signals for different binary configurations, limiting tests of general relativity and astrophysics. In this work, we present a description of the quasinormal modes that are excited in the ringdowns of comparable mass, quasi-circular precessing binary black hole coalescences -- a key region of parameter space that has yet to be fully explored within the framework of black hole spectroscopy. We suggest that the remnant pertu"},"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":"2312.08588","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2023-12-14T01:19:38Z","cross_cats_sorted":["astro-ph.CO","astro-ph.SR"],"title_canon_sha256":"ce6a25c15449cf1dd8ccca38e4f1e549bdc8365808a44657292cf81072fe8511","abstract_canon_sha256":"86d708355bc2c7514895cad44df2c6707521bb0e279fc2bda4cca7a8a171352a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:26:00.327918Z","signature_b64":"kEzNRPKTmUd6bGOdRIXMVrt5gAa45AZ+fsoaaCHkYPG2Xv/Q9U/4IEyOMQZfBrIkjRbDzHAlshcGndoqtvRwDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"39d2908e3d738865ca3eeb84ab801f1eaf4dfdf3908f34a7ebfca177df0925a7","last_reissued_at":"2026-07-05T10:26:00.327262Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:26:00.327262Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.SR"],"primary_cat":"gr-qc","authors_text":"Harald P. Pfeiffer, Harrison Siegel, Hengrui Zhu, Jordan Moxon, Keefe Mitman, Kyle C. Nelli, Lawrence E. Kidder, Mark A. Scheel, Maximiliano Isi, Michael Boyle, Nils Deppe, Nils L. Vu, Saul A. Teukolsky, Sizheng Ma, Vijay Varma, William Throwe, Will M. Farr","submitted_at":"2023-12-14T01:19:38Z","abstract_excerpt":"The spectroscopic study of black hole quasinormal modes in gravitational-wave ringdown observations is hindered by our ignorance of which modes should dominate astrophysical signals for different binary configurations, limiting tests of general relativity and astrophysics. In this work, we present a description of the quasinormal modes that are excited in the ringdowns of comparable mass, quasi-circular precessing binary black hole coalescences -- a key region of parameter space that has yet to be fully explored within the framework of black hole spectroscopy. We suggest that the remnant pertu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2312.08588","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/2312.08588/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":"2312.08588","created_at":"2026-07-05T10:26:00.327347+00:00"},{"alias_kind":"arxiv_version","alias_value":"2312.08588v3","created_at":"2026-07-05T10:26:00.327347+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2312.08588","created_at":"2026-07-05T10:26:00.327347+00:00"},{"alias_kind":"pith_short_12","alias_value":"HHJJBDR5OOEG","created_at":"2026-07-05T10:26:00.327347+00:00"},{"alias_kind":"pith_short_16","alias_value":"HHJJBDR5OOEGLSR6","created_at":"2026-07-05T10:26:00.327347+00:00"},{"alias_kind":"pith_short_8","alias_value":"HHJJBDR5","created_at":"2026-07-05T10:26:00.327347+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2407.18319","citing_title":"Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity","ref_index":112,"is_internal_anchor":false},{"citing_arxiv_id":"2605.15271","citing_title":"Polarization Analysis of Ringdown Signals","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2601.04276","citing_title":"Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03576","citing_title":"Ringdown Analysis of GW250114 with Orthonormal Modes","ref_index":92,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15431","citing_title":"Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms","ref_index":192,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HHJJBDR5OOEGLSR65OCKXAA7D2","json":"https://pith.science/pith/HHJJBDR5OOEGLSR65OCKXAA7D2.json","graph_json":"https://pith.science/api/pith-number/HHJJBDR5OOEGLSR65OCKXAA7D2/graph.json","events_json":"https://pith.science/api/pith-number/HHJJBDR5OOEGLSR65OCKXAA7D2/events.json","paper":"https://pith.science/paper/HHJJBDR5"},"agent_actions":{"view_html":"https://pith.science/pith/HHJJBDR5OOEGLSR65OCKXAA7D2","download_json":"https://pith.science/pith/HHJJBDR5OOEGLSR65OCKXAA7D2.json","view_paper":"https://pith.science/paper/HHJJBDR5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2312.08588&json=true","fetch_graph":"https://pith.science/api/pith-number/HHJJBDR5OOEGLSR65OCKXAA7D2/graph.json","fetch_events":"https://pith.science/api/pith-number/HHJJBDR5OOEGLSR65OCKXAA7D2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HHJJBDR5OOEGLSR65OCKXAA7D2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HHJJBDR5OOEGLSR65OCKXAA7D2/action/storage_attestation","attest_author":"https://pith.science/pith/HHJJBDR5OOEGLSR65OCKXAA7D2/action/author_attestation","sign_citation":"https://pith.science/pith/HHJJBDR5OOEGLSR65OCKXAA7D2/action/citation_signature","submit_replication":"https://pith.science/pith/HHJJBDR5OOEGLSR65OCKXAA7D2/action/replication_record"}},"created_at":"2026-07-05T10:26:00.327347+00:00","updated_at":"2026-07-05T10:26:00.327347+00:00"}