{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:KYMAALGJWBHZTFMWOMM7LDHFHY","short_pith_number":"pith:KYMAALGJ","schema_version":"1.0","canonical_sha256":"5618002cc9b04f9995967319f58ce53e219a25c1fa8425dda476b7bd7dfb0028","source":{"kind":"arxiv","id":"2507.07196","version":1},"attestation_state":"computed","paper":{"title":"Gravitational Quasinormal Modes and Grey-Body Factors of Bonanno-Reuter Regular Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Milena Skvortsova, S. V. Bolokhov","submitted_at":"2025-07-09T18:11:20Z","abstract_excerpt":"We study gravitational perturbations of the Bonanno--Reuter quantum-corrected black hole arising in the asymptotic safety scenario, focusing on QNMs and grey-body factors. Assuming the RG parameter $\\tilde{\\omega}$ is fixed to its phenomenologically motivated value, we treat the interpolation parameter $\\gamma$ as free and investigate how it modifies the black hole's response to axial gravitational perturbations. Quasinormal frequencies are computed using the sixth-order WKB method with Pad\\'e approximants, and their dependence on $\\gamma$ and the black hole mass $M$ is analyzed. We find that "},"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":"2507.07196","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2025-07-09T18:11:20Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"acc74609a0d6574a9f89c9431ae23f75b9cd14e7c39f9a239c40e9f011c6ed79","abstract_canon_sha256":"2ec50033a59660d83d7ed111f463dfe8fdb4e1a6dd9c5f8d96ffcaf3fe35b472"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:34:32.470846Z","signature_b64":"BNGsYWTBxj19nRcJE94HKK6hG1TqJ5ijw/cjQSinrj97F5X8/w/ieH9BIHYRgfJFV4KM1Xd5AWw+YE9/3z80CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5618002cc9b04f9995967319f58ce53e219a25c1fa8425dda476b7bd7dfb0028","last_reissued_at":"2026-07-05T11:34:32.470119Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:34:32.470119Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational Quasinormal Modes and Grey-Body Factors of Bonanno-Reuter Regular Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Milena Skvortsova, S. V. Bolokhov","submitted_at":"2025-07-09T18:11:20Z","abstract_excerpt":"We study gravitational perturbations of the Bonanno--Reuter quantum-corrected black hole arising in the asymptotic safety scenario, focusing on QNMs and grey-body factors. Assuming the RG parameter $\\tilde{\\omega}$ is fixed to its phenomenologically motivated value, we treat the interpolation parameter $\\gamma$ as free and investigate how it modifies the black hole's response to axial gravitational perturbations. Quasinormal frequencies are computed using the sixth-order WKB method with Pad\\'e approximants, and their dependence on $\\gamma$ and the black hole mass $M$ is analyzed. We find that "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2507.07196","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/2507.07196/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":"2507.07196","created_at":"2026-07-05T11:34:32.470197+00:00"},{"alias_kind":"arxiv_version","alias_value":"2507.07196v1","created_at":"2026-07-05T11:34:32.470197+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2507.07196","created_at":"2026-07-05T11:34:32.470197+00:00"},{"alias_kind":"pith_short_12","alias_value":"KYMAALGJWBHZ","created_at":"2026-07-05T11:34:32.470197+00:00"},{"alias_kind":"pith_short_16","alias_value":"KYMAALGJWBHZTFMW","created_at":"2026-07-05T11:34:32.470197+00:00"},{"alias_kind":"pith_short_8","alias_value":"KYMAALGJ","created_at":"2026-07-05T11:34:32.470197+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":25,"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":101,"is_internal_anchor":true},{"citing_arxiv_id":"2606.08631","citing_title":"Hawking Radiation from the Dymnikova Regular Black Hole","ref_index":92,"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":61,"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":57,"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":22,"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":34,"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":80,"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":34,"is_internal_anchor":false},{"citing_arxiv_id":"2512.23510","citing_title":"Quasinormal mode/grey-body factor correspondence for Kerr black holes","ref_index":30,"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":112,"is_internal_anchor":false},{"citing_arxiv_id":"2601.18613","citing_title":"Correspondence between quasinormal modes and grey-body factors of Schwarzschild--Tangherlini black holes","ref_index":58,"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":113,"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":221,"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":86,"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":54,"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":82,"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":134,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03137","citing_title":"Scattering of scalar, electromagnetic, and Dirac fields in an asymptotically flat regular black hole supported by primordial dark matter","ref_index":68,"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":73,"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":106,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26166","citing_title":"Scattering of electromagnetic field in quasi-topological gravity","ref_index":51,"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":141,"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":86,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11845","citing_title":"Quasi-resonances in the vicinity of Einstein-Maxwell-dilaton black hole","ref_index":94,"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":106,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KYMAALGJWBHZTFMWOMM7LDHFHY","json":"https://pith.science/pith/KYMAALGJWBHZTFMWOMM7LDHFHY.json","graph_json":"https://pith.science/api/pith-number/KYMAALGJWBHZTFMWOMM7LDHFHY/graph.json","events_json":"https://pith.science/api/pith-number/KYMAALGJWBHZTFMWOMM7LDHFHY/events.json","paper":"https://pith.science/paper/KYMAALGJ"},"agent_actions":{"view_html":"https://pith.science/pith/KYMAALGJWBHZTFMWOMM7LDHFHY","download_json":"https://pith.science/pith/KYMAALGJWBHZTFMWOMM7LDHFHY.json","view_paper":"https://pith.science/paper/KYMAALGJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2507.07196&json=true","fetch_graph":"https://pith.science/api/pith-number/KYMAALGJWBHZTFMWOMM7LDHFHY/graph.json","fetch_events":"https://pith.science/api/pith-number/KYMAALGJWBHZTFMWOMM7LDHFHY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KYMAALGJWBHZTFMWOMM7LDHFHY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KYMAALGJWBHZTFMWOMM7LDHFHY/action/storage_attestation","attest_author":"https://pith.science/pith/KYMAALGJWBHZTFMWOMM7LDHFHY/action/author_attestation","sign_citation":"https://pith.science/pith/KYMAALGJWBHZTFMWOMM7LDHFHY/action/citation_signature","submit_replication":"https://pith.science/pith/KYMAALGJWBHZTFMWOMM7LDHFHY/action/replication_record"}},"created_at":"2026-07-05T11:34:32.470197+00:00","updated_at":"2026-07-05T11:34:32.470197+00:00"}