{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:FEEJOLZNZRGKF7JZ6JIEO23QMI","short_pith_number":"pith:FEEJOLZN","schema_version":"1.0","canonical_sha256":"2908972f2dcc4ca2fd39f250476b7062222de1e57609c13c9ad2e810e1a45517","source":{"kind":"arxiv","id":"2311.05503","version":1},"attestation_state":"computed","paper":{"title":"Long-lived quasinormal modes and overtones' behavior of the holonomy corrected black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"S. V. Bolokhov","submitted_at":"2023-11-01T10:08:36Z","abstract_excerpt":"Recently massless test scalar field perturbations of the holonomy corrected black holes [Z. Moreira et. al. Phys. Rev. D 107 (2023) 10, 104016] were studied in order to estimate quantum corrections to the quasinormal spectrum of a black hole. Here we study both the fundamental mode and overtones of scalar, electromagnetic and Dirac fields with the help of the Leaver method and higher order WKB formula with Pad\\'e approximants. We observe that the overtones depend on the geometry near the event horizon, while the fundamental mode is localized near the peak of the potential barrier, what agrees "},"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":"2311.05503","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2023-11-01T10:08:36Z","cross_cats_sorted":[],"title_canon_sha256":"c0b1b6c192eda8968aa9ebda093023ffe4d31c14125296ffb6bef395f50f3f66","abstract_canon_sha256":"31de18bd5c0c4a366f968ba0cd8b54bde0d9608a6701693b1fc449f5c66427d6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:19:24.927488Z","signature_b64":"K7vLVlHEV3PmbaM2+uufrZRnFlqyE76zzjXCNK8cAoKhZCRR/RDLVWoJpyqBoyyxIx2diBmg/eh2bXYjOxxqCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2908972f2dcc4ca2fd39f250476b7062222de1e57609c13c9ad2e810e1a45517","last_reissued_at":"2026-07-05T09:19:24.927069Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:19:24.927069Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Long-lived quasinormal modes and overtones' behavior of the holonomy corrected black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"S. V. Bolokhov","submitted_at":"2023-11-01T10:08:36Z","abstract_excerpt":"Recently massless test scalar field perturbations of the holonomy corrected black holes [Z. Moreira et. al. Phys. Rev. D 107 (2023) 10, 104016] were studied in order to estimate quantum corrections to the quasinormal spectrum of a black hole. Here we study both the fundamental mode and overtones of scalar, electromagnetic and Dirac fields with the help of the Leaver method and higher order WKB formula with Pad\\'e approximants. We observe that the overtones depend on the geometry near the event horizon, while the fundamental mode is localized near the peak of the potential barrier, what agrees "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.05503","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/2311.05503/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":"2311.05503","created_at":"2026-07-05T09:19:24.927127+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.05503v1","created_at":"2026-07-05T09:19:24.927127+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.05503","created_at":"2026-07-05T09:19:24.927127+00:00"},{"alias_kind":"pith_short_12","alias_value":"FEEJOLZNZRGK","created_at":"2026-07-05T09:19:24.927127+00:00"},{"alias_kind":"pith_short_16","alias_value":"FEEJOLZNZRGKF7JZ","created_at":"2026-07-05T09:19:24.927127+00:00"},{"alias_kind":"pith_short_8","alias_value":"FEEJOLZN","created_at":"2026-07-05T09:19:24.927127+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":26,"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":69,"is_internal_anchor":true},{"citing_arxiv_id":"2606.08631","citing_title":"Hawking Radiation from the Dymnikova Regular Black Hole","ref_index":96,"is_internal_anchor":false},{"citing_arxiv_id":"2606.08351","citing_title":"Hawking Emission from Black Holes Evaporating toward Wormholes and the Accuracy of the WKB Approximation","ref_index":30,"is_internal_anchor":false},{"citing_arxiv_id":"2606.03842","citing_title":"Scattering and Hawking Radiation from Einstein--Euler--Heisenberg--de Sitter Black Holes","ref_index":75,"is_internal_anchor":false},{"citing_arxiv_id":"2605.25076","citing_title":"Grey-Body Factors and Thermodynamics of Asymptotically de Sitter Black Holes in Generalized Proca Theory","ref_index":77,"is_internal_anchor":false},{"citing_arxiv_id":"2605.25705","citing_title":"Ces\\`aro convergence of the high-order WKB method and its applications to black-hole overtones and long-lived modes","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2601.22340","citing_title":"Grey-body factors of higher dimensional regular black holes in quasi-topological theories","ref_index":96,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21533","citing_title":"Long-lived quasinormal modes of Asymptotically de Sitter Black Holes in Generalized Proca Theory","ref_index":40,"is_internal_anchor":false},{"citing_arxiv_id":"2601.22340","citing_title":"Grey-body factors of higher dimensional regular black holes in quasi-topological theories","ref_index":96,"is_internal_anchor":false},{"citing_arxiv_id":"2605.18249","citing_title":"Quasinormal modes of a rotating loop quantum black hole","ref_index":38,"is_internal_anchor":false},{"citing_arxiv_id":"2506.16217","citing_title":"Quasinormal modes and grey-body factors of axial gravitational perturbations of regular black holes in asymptotically safe gravity","ref_index":29,"is_internal_anchor":false},{"citing_arxiv_id":"2601.17906","citing_title":"Telling tails and quasi-resonances in the vicinity of Dymnikova regular black hole","ref_index":89,"is_internal_anchor":false},{"citing_arxiv_id":"2602.11001","citing_title":"Two types of quasinormal modes of Casadio-Fabbri-Mazzacurati brane-world black holes","ref_index":67,"is_internal_anchor":false},{"citing_arxiv_id":"2603.10844","citing_title":"Long-lived quasinormal modes, shadows and particle motion in four-dimensional quasi-topological gravity","ref_index":144,"is_internal_anchor":false},{"citing_arxiv_id":"2603.25084","citing_title":"Particle motions and gravitational waveforms in rotating black hole spacetimes of loop quantum gravity","ref_index":53,"is_internal_anchor":false},{"citing_arxiv_id":"2604.24349","citing_title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","ref_index":56,"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":71,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11364","citing_title":"Bardeen spacetime as quantum corrected black hole: Grey-body factors and quasinormal modes of gravitational perturbations","ref_index":119,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11013","citing_title":"Massive Scalar Quasinormal Modes, Greybody Factors, and Absorption Cross Section of a Parity-Symmetric Beyond-Horndeski Black Hole","ref_index":62,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03659","citing_title":"Long-lived massive scalar modes, grey-body factors, and absorption cross sections of the Reissner--Nordstr\\\"om-like brane-world black hole","ref_index":34,"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":75,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25471","citing_title":"Massive scalar quasinormal modes of an asymptotically flat regular black hole supported by a phantom Dirac--Born--Infeld field","ref_index":61,"is_internal_anchor":false},{"citing_arxiv_id":"2604.24349","citing_title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","ref_index":56,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11845","citing_title":"Quasi-resonances in the vicinity of Einstein-Maxwell-dilaton black hole","ref_index":41,"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":65,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FEEJOLZNZRGKF7JZ6JIEO23QMI","json":"https://pith.science/pith/FEEJOLZNZRGKF7JZ6JIEO23QMI.json","graph_json":"https://pith.science/api/pith-number/FEEJOLZNZRGKF7JZ6JIEO23QMI/graph.json","events_json":"https://pith.science/api/pith-number/FEEJOLZNZRGKF7JZ6JIEO23QMI/events.json","paper":"https://pith.science/paper/FEEJOLZN"},"agent_actions":{"view_html":"https://pith.science/pith/FEEJOLZNZRGKF7JZ6JIEO23QMI","download_json":"https://pith.science/pith/FEEJOLZNZRGKF7JZ6JIEO23QMI.json","view_paper":"https://pith.science/paper/FEEJOLZN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.05503&json=true","fetch_graph":"https://pith.science/api/pith-number/FEEJOLZNZRGKF7JZ6JIEO23QMI/graph.json","fetch_events":"https://pith.science/api/pith-number/FEEJOLZNZRGKF7JZ6JIEO23QMI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FEEJOLZNZRGKF7JZ6JIEO23QMI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FEEJOLZNZRGKF7JZ6JIEO23QMI/action/storage_attestation","attest_author":"https://pith.science/pith/FEEJOLZNZRGKF7JZ6JIEO23QMI/action/author_attestation","sign_citation":"https://pith.science/pith/FEEJOLZNZRGKF7JZ6JIEO23QMI/action/citation_signature","submit_replication":"https://pith.science/pith/FEEJOLZNZRGKF7JZ6JIEO23QMI/action/replication_record"}},"created_at":"2026-07-05T09:19:24.927127+00:00","updated_at":"2026-07-05T09:19:24.927127+00:00"}