{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:4727EZWHZO566LUTZRCI554ZZZ","short_pith_number":"pith:4727EZWH","schema_version":"1.0","canonical_sha256":"e7f5f266c7cbbbef2e93cc448ef799ce4c5e910452c2315581312823b245d0d0","source":{"kind":"arxiv","id":"2311.07706","version":1},"attestation_state":"computed","paper":{"title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity I. Slow rotation equations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Dongjun Li, Nicolas Yunes, Pratik Wagle, Yanbei Chen","submitted_at":"2023-11-13T19:45:22Z","abstract_excerpt":"The detection of gravitational waves resulting by the LIGO-Virgo-Kagra collaboration has inaugurated a new era in gravitational physics, providing an opportunity to test general relativity and its modifications in the strong gravity regime. One such test involves the study of the ringdown phase of gravitational waves from binary black-hole coalescence, which can be decomposed into a superposition of quasinormal modes. In general relativity, the spectra of quasinormal modes depend on the mass, spin, and charge of the final black hole, but they can be influenced by additional properties of the b"},"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":"2311.07706","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2023-11-13T19:45:22Z","cross_cats_sorted":[],"title_canon_sha256":"11853d8c59c1eb07d93ed470522648ccba2dec7a4f605c7da112cc51a66c87fa","abstract_canon_sha256":"b11ff6b7520e526a001727c0e4f00b490a57e5c76ddc64969b57641a9b2fd2aa"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:12:22.630492Z","signature_b64":"Npb8qtNxHqgsxijvaMsq85RQeo/6AHq4nYwviX9XW1TP3lZoxuontDFrpFjG0mJIR344FmGvbDm2OdUOtAJxDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e7f5f266c7cbbbef2e93cc448ef799ce4c5e910452c2315581312823b245d0d0","last_reissued_at":"2026-07-05T07:12:22.630041Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:12:22.630041Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity I. Slow rotation equations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Dongjun Li, Nicolas Yunes, Pratik Wagle, Yanbei Chen","submitted_at":"2023-11-13T19:45:22Z","abstract_excerpt":"The detection of gravitational waves resulting by the LIGO-Virgo-Kagra collaboration has inaugurated a new era in gravitational physics, providing an opportunity to test general relativity and its modifications in the strong gravity regime. One such test involves the study of the ringdown phase of gravitational waves from binary black-hole coalescence, which can be decomposed into a superposition of quasinormal modes. In general relativity, the spectra of quasinormal modes depend on the mass, spin, and charge of the final black hole, but they can be influenced by additional properties of the b"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.07706","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/2311.07706/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":"2311.07706","created_at":"2026-07-05T07:12:22.630096+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.07706v1","created_at":"2026-07-05T07:12:22.630096+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.07706","created_at":"2026-07-05T07:12:22.630096+00:00"},{"alias_kind":"pith_short_12","alias_value":"4727EZWHZO56","created_at":"2026-07-05T07:12:22.630096+00:00"},{"alias_kind":"pith_short_16","alias_value":"4727EZWHZO566LUT","created_at":"2026-07-05T07:12:22.630096+00:00"},{"alias_kind":"pith_short_8","alias_value":"4727EZWH","created_at":"2026-07-05T07:12:22.630096+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.24642","citing_title":"When Black Holes Can Wear Pants","ref_index":53,"is_internal_anchor":false},{"citing_arxiv_id":"2606.09766","citing_title":"Modified Teukolsky Formalism for Extreme Mass-Ratio Inspirals in Higher-Derivative Gravity","ref_index":64,"is_internal_anchor":false},{"citing_arxiv_id":"2511.12580","citing_title":"Dynamical Tidal Response of Non-rotating Black Holes: Connecting the MST Formalism and Worldline EFT","ref_index":171,"is_internal_anchor":false},{"citing_arxiv_id":"2601.09607","citing_title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","ref_index":27,"is_internal_anchor":false},{"citing_arxiv_id":"2604.02214","citing_title":"Quadratic gravity corrections to scalar QNMs of rapidly rotating black holes","ref_index":61,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11080","citing_title":"Metric Reconstruction for Generic Black-Hole Perturbations","ref_index":69,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18680","citing_title":"Beyond Three Terms: Continued Fractions for Rotating Black Holes in Modified Gravity","ref_index":37,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4727EZWHZO566LUTZRCI554ZZZ","json":"https://pith.science/pith/4727EZWHZO566LUTZRCI554ZZZ.json","graph_json":"https://pith.science/api/pith-number/4727EZWHZO566LUTZRCI554ZZZ/graph.json","events_json":"https://pith.science/api/pith-number/4727EZWHZO566LUTZRCI554ZZZ/events.json","paper":"https://pith.science/paper/4727EZWH"},"agent_actions":{"view_html":"https://pith.science/pith/4727EZWHZO566LUTZRCI554ZZZ","download_json":"https://pith.science/pith/4727EZWHZO566LUTZRCI554ZZZ.json","view_paper":"https://pith.science/paper/4727EZWH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.07706&json=true","fetch_graph":"https://pith.science/api/pith-number/4727EZWHZO566LUTZRCI554ZZZ/graph.json","fetch_events":"https://pith.science/api/pith-number/4727EZWHZO566LUTZRCI554ZZZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4727EZWHZO566LUTZRCI554ZZZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4727EZWHZO566LUTZRCI554ZZZ/action/storage_attestation","attest_author":"https://pith.science/pith/4727EZWHZO566LUTZRCI554ZZZ/action/author_attestation","sign_citation":"https://pith.science/pith/4727EZWHZO566LUTZRCI554ZZZ/action/citation_signature","submit_replication":"https://pith.science/pith/4727EZWHZO566LUTZRCI554ZZZ/action/replication_record"}},"created_at":"2026-07-05T07:12:22.630096+00:00","updated_at":"2026-07-05T07:12:22.630096+00:00"}