{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:HMWMOW7L2Z3Z2A3IM2V7JDY5KN","short_pith_number":"pith:HMWMOW7L","schema_version":"1.0","canonical_sha256":"3b2cc75bebd6779d036866abf48f1d537ec9284b086b012ad9d30e9814c2e093","source":{"kind":"arxiv","id":"2403.07848","version":4},"attestation_state":"computed","paper":{"title":"Infinite tower of higher-curvature corrections: Quasinormal modes and late-time behavior of D-dimensional regular black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"A. Zhidenko, R. A. Konoplya","submitted_at":"2024-03-12T17:39:13Z","abstract_excerpt":"Recently, Bueno, Cano, and Hennigar [arXiv:2403.04827] proposed a generic approach for incorporating an infinite tower of higher-curvature corrections into the Einstein theory. In this study, we compute quasinormal modes for certain regular D-dimensional black holes resulting from this infinite series of higher-curvature corrections, specifically focusing on the $D$-dimensional extensions of the Bardeen and Hayward black holes. We demonstrate that while the fundamental mode is minimally affected by moderate coupling constants, the higher overtones exhibit significant sensitivity even to small "},"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":"2403.07848","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2024-03-12T17:39:13Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"80755babcdc6325277d104729c4e84dc44bf6dfe6f844ce46b1a15c93737067f","abstract_canon_sha256":"c2cf50f333422ff989ec63afa6b0d87a1acd8fdabaf921e75923acd2b66870a7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:14:55.387122Z","signature_b64":"AiNYMf5Ww+4tNCezk1T9ig1+kj/9+8IGgi8jnO/oy6ZpSrS104CP1fNNjyIom1iZj2YdWZLwilevGEEoAnTHAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3b2cc75bebd6779d036866abf48f1d537ec9284b086b012ad9d30e9814c2e093","last_reissued_at":"2026-07-05T08:14:55.386661Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:14:55.386661Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Infinite tower of higher-curvature corrections: Quasinormal modes and late-time behavior of D-dimensional regular black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"A. Zhidenko, R. A. Konoplya","submitted_at":"2024-03-12T17:39:13Z","abstract_excerpt":"Recently, Bueno, Cano, and Hennigar [arXiv:2403.04827] proposed a generic approach for incorporating an infinite tower of higher-curvature corrections into the Einstein theory. In this study, we compute quasinormal modes for certain regular D-dimensional black holes resulting from this infinite series of higher-curvature corrections, specifically focusing on the $D$-dimensional extensions of the Bardeen and Hayward black holes. We demonstrate that while the fundamental mode is minimally affected by moderate coupling constants, the higher overtones exhibit significant sensitivity even to small "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.07848","kind":"arxiv","version":4},"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/2403.07848/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":"2403.07848","created_at":"2026-07-05T08:14:55.386716+00:00"},{"alias_kind":"arxiv_version","alias_value":"2403.07848v4","created_at":"2026-07-05T08:14:55.386716+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2403.07848","created_at":"2026-07-05T08:14:55.386716+00:00"},{"alias_kind":"pith_short_12","alias_value":"HMWMOW7L2Z3Z","created_at":"2026-07-05T08:14:55.386716+00:00"},{"alias_kind":"pith_short_16","alias_value":"HMWMOW7L2Z3Z2A3I","created_at":"2026-07-05T08:14:55.386716+00:00"},{"alias_kind":"pith_short_8","alias_value":"HMWMOW7L","created_at":"2026-07-05T08:14:55.386716+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":20,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2607.07790","citing_title":"Regular Black Holes in Nonlocal Quasitopological Gravity","ref_index":27,"is_internal_anchor":true},{"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":10,"is_internal_anchor":true},{"citing_arxiv_id":"2606.08631","citing_title":"Hawking Radiation from the Dymnikova Regular Black Hole","ref_index":88,"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":60,"is_internal_anchor":false},{"citing_arxiv_id":"2606.06355","citing_title":"$\\tt BlackHawk$ $\\tt v3.0$: Hawking Radiation from Regular Black Holes","ref_index":299,"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":54,"is_internal_anchor":false},{"citing_arxiv_id":"2605.28917","citing_title":"Greybody Factors, Absorption Cross Sections and Hawking Radiation of Holonomy-Corrected Schwarzschild Black Holes","ref_index":53,"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":44,"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":117,"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":44,"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":67,"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":85,"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":118,"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":140,"is_internal_anchor":false},{"citing_arxiv_id":"2604.27980","citing_title":"On mass inflation and thin shells in quasi-topological gravity","ref_index":58,"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":90,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26166","citing_title":"Scattering of electromagnetic field in quasi-topological gravity","ref_index":19,"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":149,"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":67,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11845","citing_title":"Quasi-resonances in the vicinity of Einstein-Maxwell-dilaton black hole","ref_index":62,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HMWMOW7L2Z3Z2A3IM2V7JDY5KN","json":"https://pith.science/pith/HMWMOW7L2Z3Z2A3IM2V7JDY5KN.json","graph_json":"https://pith.science/api/pith-number/HMWMOW7L2Z3Z2A3IM2V7JDY5KN/graph.json","events_json":"https://pith.science/api/pith-number/HMWMOW7L2Z3Z2A3IM2V7JDY5KN/events.json","paper":"https://pith.science/paper/HMWMOW7L"},"agent_actions":{"view_html":"https://pith.science/pith/HMWMOW7L2Z3Z2A3IM2V7JDY5KN","download_json":"https://pith.science/pith/HMWMOW7L2Z3Z2A3IM2V7JDY5KN.json","view_paper":"https://pith.science/paper/HMWMOW7L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2403.07848&json=true","fetch_graph":"https://pith.science/api/pith-number/HMWMOW7L2Z3Z2A3IM2V7JDY5KN/graph.json","fetch_events":"https://pith.science/api/pith-number/HMWMOW7L2Z3Z2A3IM2V7JDY5KN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HMWMOW7L2Z3Z2A3IM2V7JDY5KN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HMWMOW7L2Z3Z2A3IM2V7JDY5KN/action/storage_attestation","attest_author":"https://pith.science/pith/HMWMOW7L2Z3Z2A3IM2V7JDY5KN/action/author_attestation","sign_citation":"https://pith.science/pith/HMWMOW7L2Z3Z2A3IM2V7JDY5KN/action/citation_signature","submit_replication":"https://pith.science/pith/HMWMOW7L2Z3Z2A3IM2V7JDY5KN/action/replication_record"}},"created_at":"2026-07-05T08:14:55.386716+00:00","updated_at":"2026-07-05T08:14:55.386716+00:00"}