{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:JBJER4ZGYJ2KBOLMBKBBADIWHE","short_pith_number":"pith:JBJER4ZG","schema_version":"1.0","canonical_sha256":"485248f326c274a0b96c0a82100d16392b1293e9c92821864bfcad87ee84389b","source":{"kind":"arxiv","id":"2206.10652","version":2},"attestation_state":"computed","paper":{"title":"Perturbations of spinning black holes beyond General Relativity: Modified Teukolsky equation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Dongjun Li, Nicol\\'as Yunes, Pratik Wagle, Yanbei Chen","submitted_at":"2022-06-21T18:04:48Z","abstract_excerpt":"The detection of gravitational waves from compact binary mergers by the LIGO/Virgo collaboration has, for the first time, allowed for tests of relativistic gravity in the strong, dynamical and nonlinear regime. Outside Einstein's relativity, spinning black holes may be different from their general relativistic counterparts, and their merger may then lead to a modified ringdown. We study the latter and, for the first time, derive a modified Teukolsky equation, i.e., a set of linear, decoupled differential equations that describe dynamical perturbations of non-Kerr black holes for the radiative "},"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":"2206.10652","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2022-06-21T18:04:48Z","cross_cats_sorted":[],"title_canon_sha256":"b4ae1825cfa00508976e894d5aa345a6d5e31bbc8f240a6f11f22d984737732f","abstract_canon_sha256":"19f97c2a58cbb67e4f95b6bda1c1917ba6dbaf8b677eae8552eaec845a9f16ad"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:13:52.528767Z","signature_b64":"0BQCSm/LVPRDvHSPF0IaC0dpLs3bodKuyZbqi5PPkbqQcCPtzlolSAgS8CcL4J/qCTrIOk2hKSmRtU1cw3WJBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"485248f326c274a0b96c0a82100d16392b1293e9c92821864bfcad87ee84389b","last_reissued_at":"2026-07-05T06:13:52.528231Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:13:52.528231Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Perturbations of spinning black holes beyond General Relativity: Modified Teukolsky equation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Dongjun Li, Nicol\\'as Yunes, Pratik Wagle, Yanbei Chen","submitted_at":"2022-06-21T18:04:48Z","abstract_excerpt":"The detection of gravitational waves from compact binary mergers by the LIGO/Virgo collaboration has, for the first time, allowed for tests of relativistic gravity in the strong, dynamical and nonlinear regime. Outside Einstein's relativity, spinning black holes may be different from their general relativistic counterparts, and their merger may then lead to a modified ringdown. We study the latter and, for the first time, derive a modified Teukolsky equation, i.e., a set of linear, decoupled differential equations that describe dynamical perturbations of non-Kerr black holes for the radiative "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2206.10652","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2206.10652/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":"2206.10652","created_at":"2026-07-05T06:13:52.528294+00:00"},{"alias_kind":"arxiv_version","alias_value":"2206.10652v2","created_at":"2026-07-05T06:13:52.528294+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2206.10652","created_at":"2026-07-05T06:13:52.528294+00:00"},{"alias_kind":"pith_short_12","alias_value":"JBJER4ZGYJ2K","created_at":"2026-07-05T06:13:52.528294+00:00"},{"alias_kind":"pith_short_16","alias_value":"JBJER4ZGYJ2KBOLM","created_at":"2026-07-05T06:13:52.528294+00:00"},{"alias_kind":"pith_short_8","alias_value":"JBJER4ZG","created_at":"2026-07-05T06:13:52.528294+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":10,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.09766","citing_title":"Modified Teukolsky Formalism for Extreme Mass-Ratio Inspirals in Higher-Derivative Gravity","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2507.04471","citing_title":"A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments","ref_index":88,"is_internal_anchor":false},{"citing_arxiv_id":"2510.11793","citing_title":"Black hole mergers beyond general relativity: a self-force approach","ref_index":62,"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":167,"is_internal_anchor":false},{"citing_arxiv_id":"2512.02338","citing_title":"Leading effective field theory corrections to the Kerr metric at all spins","ref_index":45,"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":34,"is_internal_anchor":false},{"citing_arxiv_id":"2604.02214","citing_title":"Quadratic gravity corrections to scalar QNMs of rapidly rotating black holes","ref_index":58,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11080","citing_title":"Metric Reconstruction for Generic Black-Hole Perturbations","ref_index":15,"is_internal_anchor":false},{"citing_arxiv_id":"2604.24413","citing_title":"Gravitational waves of extreme-mass-ratio inspirals in a rotating black hole with Dehnen dark matter halo","ref_index":79,"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":36,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JBJER4ZGYJ2KBOLMBKBBADIWHE","json":"https://pith.science/pith/JBJER4ZGYJ2KBOLMBKBBADIWHE.json","graph_json":"https://pith.science/api/pith-number/JBJER4ZGYJ2KBOLMBKBBADIWHE/graph.json","events_json":"https://pith.science/api/pith-number/JBJER4ZGYJ2KBOLMBKBBADIWHE/events.json","paper":"https://pith.science/paper/JBJER4ZG"},"agent_actions":{"view_html":"https://pith.science/pith/JBJER4ZGYJ2KBOLMBKBBADIWHE","download_json":"https://pith.science/pith/JBJER4ZGYJ2KBOLMBKBBADIWHE.json","view_paper":"https://pith.science/paper/JBJER4ZG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2206.10652&json=true","fetch_graph":"https://pith.science/api/pith-number/JBJER4ZGYJ2KBOLMBKBBADIWHE/graph.json","fetch_events":"https://pith.science/api/pith-number/JBJER4ZGYJ2KBOLMBKBBADIWHE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JBJER4ZGYJ2KBOLMBKBBADIWHE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JBJER4ZGYJ2KBOLMBKBBADIWHE/action/storage_attestation","attest_author":"https://pith.science/pith/JBJER4ZGYJ2KBOLMBKBBADIWHE/action/author_attestation","sign_citation":"https://pith.science/pith/JBJER4ZGYJ2KBOLMBKBBADIWHE/action/citation_signature","submit_replication":"https://pith.science/pith/JBJER4ZGYJ2KBOLMBKBBADIWHE/action/replication_record"}},"created_at":"2026-07-05T06:13:52.528294+00:00","updated_at":"2026-07-05T06:13:52.528294+00:00"}