{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:5BSP4TBUAPVCN6JRCIMIZGSYF6","short_pith_number":"pith:5BSP4TBU","schema_version":"1.0","canonical_sha256":"e864fe4c3403ea26f93112188c9a582f8322cc924d3c45d029a9a549c4a24bbc","source":{"kind":"arxiv","id":"2210.08373","version":2},"attestation_state":"computed","paper":{"title":"Further clarification on quasinormal modes/circular null geodesics correspondence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"R. A. Konoplya","submitted_at":"2022-10-15T20:51:21Z","abstract_excerpt":"The well-known duality between quasinormal modes of any stationary, spherically symmetric and asymptotically flat or de Sitter black hole and parameters of the circular null geodesic was initially claimed for gravitational and test field perturbations. According to this duality the real and imaginary parts of the $\\ell \\gg n$ quasinormal mode (where $\\ell$ and $n$ are multipole and overtone numbers respectively) are multiples of the frequency and instability timescale of the circular null geodesics respectively. Later it was shown that the duality is guaranteed only for test fields and may be "},"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":"2210.08373","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2022-10-15T20:51:21Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"8689e13e61e5bb3a929b9d6fd386eb725c3c7525f0d41dfa1f7f27217d837906","abstract_canon_sha256":"0e14c76691eb8829dccb1b9b10e47b4b8c8fe19d64a62e14869509f3897f4b16"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:31:56.171805Z","signature_b64":"2jky6zIVmeb3vPYXT3RAD1EObuM1eRnA6H7uVw81lfPaN1mbOiIpBbiqOBkOPf7PpslFgmDV+YWL2cJoMcaFDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e864fe4c3403ea26f93112188c9a582f8322cc924d3c45d029a9a549c4a24bbc","last_reissued_at":"2026-07-05T05:31:56.171298Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:31:56.171298Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Further clarification on quasinormal modes/circular null geodesics correspondence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"R. A. Konoplya","submitted_at":"2022-10-15T20:51:21Z","abstract_excerpt":"The well-known duality between quasinormal modes of any stationary, spherically symmetric and asymptotically flat or de Sitter black hole and parameters of the circular null geodesic was initially claimed for gravitational and test field perturbations. According to this duality the real and imaginary parts of the $\\ell \\gg n$ quasinormal mode (where $\\ell$ and $n$ are multipole and overtone numbers respectively) are multiples of the frequency and instability timescale of the circular null geodesics respectively. Later it was shown that the duality is guaranteed only for test fields and may be "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2210.08373","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/2210.08373/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":"2210.08373","created_at":"2026-07-05T05:31:56.171368+00:00"},{"alias_kind":"arxiv_version","alias_value":"2210.08373v2","created_at":"2026-07-05T05:31:56.171368+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2210.08373","created_at":"2026-07-05T05:31:56.171368+00:00"},{"alias_kind":"pith_short_12","alias_value":"5BSP4TBUAPVC","created_at":"2026-07-05T05:31:56.171368+00:00"},{"alias_kind":"pith_short_16","alias_value":"5BSP4TBUAPVCN6JR","created_at":"2026-07-05T05:31:56.171368+00:00"},{"alias_kind":"pith_short_8","alias_value":"5BSP4TBU","created_at":"2026-07-05T05:31:56.171368+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07955","citing_title":"Wave and particle probes of a regular T-duality-inspired black hole with gravitational self-energy","ref_index":88,"is_internal_anchor":true},{"citing_arxiv_id":"2605.25076","citing_title":"Grey-Body Factors and Thermodynamics of Asymptotically de Sitter Black Holes in Generalized Proca Theory","ref_index":104,"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":75,"is_internal_anchor":false},{"citing_arxiv_id":"2605.12113","citing_title":"Quasinormal Spectra of Fields of Various Spin in Asymptotically de Sitter Black Holes within Generalized Proca Theory","ref_index":106,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14999","citing_title":"A First-Order Eikonal Framework for Quasinormal Modes, Shadows, Strong Lensing, and Grey-Body Factors in a Scalarized Black-Hole Metric","ref_index":35,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13613","citing_title":"From Ringdown to Lensing: Analytic Eikonal Modes of Quasi-Topological Regular Black Holes","ref_index":35,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14999","citing_title":"A First-Order Eikonal Framework for Quasinormal Modes, Shadows, Strong Lensing, and Grey-Body Factors in a Scalarized Black-Hole Metric","ref_index":35,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5BSP4TBUAPVCN6JRCIMIZGSYF6","json":"https://pith.science/pith/5BSP4TBUAPVCN6JRCIMIZGSYF6.json","graph_json":"https://pith.science/api/pith-number/5BSP4TBUAPVCN6JRCIMIZGSYF6/graph.json","events_json":"https://pith.science/api/pith-number/5BSP4TBUAPVCN6JRCIMIZGSYF6/events.json","paper":"https://pith.science/paper/5BSP4TBU"},"agent_actions":{"view_html":"https://pith.science/pith/5BSP4TBUAPVCN6JRCIMIZGSYF6","download_json":"https://pith.science/pith/5BSP4TBUAPVCN6JRCIMIZGSYF6.json","view_paper":"https://pith.science/paper/5BSP4TBU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2210.08373&json=true","fetch_graph":"https://pith.science/api/pith-number/5BSP4TBUAPVCN6JRCIMIZGSYF6/graph.json","fetch_events":"https://pith.science/api/pith-number/5BSP4TBUAPVCN6JRCIMIZGSYF6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5BSP4TBUAPVCN6JRCIMIZGSYF6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5BSP4TBUAPVCN6JRCIMIZGSYF6/action/storage_attestation","attest_author":"https://pith.science/pith/5BSP4TBUAPVCN6JRCIMIZGSYF6/action/author_attestation","sign_citation":"https://pith.science/pith/5BSP4TBUAPVCN6JRCIMIZGSYF6/action/citation_signature","submit_replication":"https://pith.science/pith/5BSP4TBUAPVCN6JRCIMIZGSYF6/action/replication_record"}},"created_at":"2026-07-05T05:31:56.171368+00:00","updated_at":"2026-07-05T05:31:56.171368+00:00"}