{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:GZ252L3PL3LYR54TFPPDVLPVT4","short_pith_number":"pith:GZ252L3P","schema_version":"1.0","canonical_sha256":"3675dd2f6f5ed788f7932bde3aadf59f2bcc7eccdf0894f4372023352121d8f1","source":{"kind":"arxiv","id":"1701.01652","version":6},"attestation_state":"computed","paper":{"title":"Eikonal instability of Gauss-Bonnet-(anti-)de Sitter black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"A. Zhidenko, R. A. Konoplya","submitted_at":"2017-01-06T15:01:48Z","abstract_excerpt":"Here we have shown that asymptotically anti-de Sitter (AdS) black holes in the Einstein-Gauss-Bonnet (GB) theory are unstable under linear perturbations of spacetime in some region of parameters. This (eikonal) instability develops at high multipole numbers. We found the exact parametric regions of the eikonal instability and extended this consideration to asymptotically flat and de Sitter cases. The approach to the threshold of instability is driven by purely imaginary quasinormal modes, which are similar to those found recently in [5] for the higher curvature corrected black hole with the pl"},"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":"1701.01652","kind":"arxiv","version":6},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2017-01-06T15:01:48Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"9cb907754f43d3b90fe99f53881328aa893dbe45c86ec6d29e1bef81f74192e8","abstract_canon_sha256":"b5894510262d90f0c9095c58ec2cfb282676fcf4a0df29da30729539a96ce476"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:44:23.851151Z","signature_b64":"sZuYorTgHxFxnJX6Hmg02wbgyNNb7ucqSBrkpnU3q3UnUMD7ez0T0uXZ9zuIN5bkOyF1ZoGQ3Iyrst2N7FrxCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3675dd2f6f5ed788f7932bde3aadf59f2bcc7eccdf0894f4372023352121d8f1","last_reissued_at":"2026-05-18T00:44:23.850688Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:44:23.850688Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Eikonal instability of Gauss-Bonnet-(anti-)de Sitter black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"A. Zhidenko, R. A. Konoplya","submitted_at":"2017-01-06T15:01:48Z","abstract_excerpt":"Here we have shown that asymptotically anti-de Sitter (AdS) black holes in the Einstein-Gauss-Bonnet (GB) theory are unstable under linear perturbations of spacetime in some region of parameters. This (eikonal) instability develops at high multipole numbers. We found the exact parametric regions of the eikonal instability and extended this consideration to asymptotically flat and de Sitter cases. The approach to the threshold of instability is driven by purely imaginary quasinormal modes, which are similar to those found recently in [5] for the higher curvature corrected black hole with the pl"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.01652","kind":"arxiv","version":6},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"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":"1701.01652","created_at":"2026-05-18T00:44:23.850772+00:00"},{"alias_kind":"arxiv_version","alias_value":"1701.01652v6","created_at":"2026-05-18T00:44:23.850772+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.01652","created_at":"2026-05-18T00:44:23.850772+00:00"},{"alias_kind":"pith_short_12","alias_value":"GZ252L3PL3LY","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_16","alias_value":"GZ252L3PL3LYR54T","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_8","alias_value":"GZ252L3P","created_at":"2026-05-18T12:31:18.294218+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":12,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2601.22340","citing_title":"Grey-body factors of higher dimensional regular black holes in quasi-topological theories","ref_index":55,"is_internal_anchor":true},{"citing_arxiv_id":"2605.21533","citing_title":"Long-lived quasinormal modes of Asymptotically de Sitter Black Holes in Generalized Proca Theory","ref_index":17,"is_internal_anchor":true},{"citing_arxiv_id":"2601.22340","citing_title":"Grey-body factors of higher dimensional regular black holes in quasi-topological theories","ref_index":55,"is_internal_anchor":true},{"citing_arxiv_id":"2604.24349","citing_title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","ref_index":119,"is_internal_anchor":true},{"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":19,"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":138,"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":167,"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":105,"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":131,"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":169,"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":119,"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":28,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GZ252L3PL3LYR54TFPPDVLPVT4","json":"https://pith.science/pith/GZ252L3PL3LYR54TFPPDVLPVT4.json","graph_json":"https://pith.science/api/pith-number/GZ252L3PL3LYR54TFPPDVLPVT4/graph.json","events_json":"https://pith.science/api/pith-number/GZ252L3PL3LYR54TFPPDVLPVT4/events.json","paper":"https://pith.science/paper/GZ252L3P"},"agent_actions":{"view_html":"https://pith.science/pith/GZ252L3PL3LYR54TFPPDVLPVT4","download_json":"https://pith.science/pith/GZ252L3PL3LYR54TFPPDVLPVT4.json","view_paper":"https://pith.science/paper/GZ252L3P","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1701.01652&json=true","fetch_graph":"https://pith.science/api/pith-number/GZ252L3PL3LYR54TFPPDVLPVT4/graph.json","fetch_events":"https://pith.science/api/pith-number/GZ252L3PL3LYR54TFPPDVLPVT4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GZ252L3PL3LYR54TFPPDVLPVT4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GZ252L3PL3LYR54TFPPDVLPVT4/action/storage_attestation","attest_author":"https://pith.science/pith/GZ252L3PL3LYR54TFPPDVLPVT4/action/author_attestation","sign_citation":"https://pith.science/pith/GZ252L3PL3LYR54TFPPDVLPVT4/action/citation_signature","submit_replication":"https://pith.science/pith/GZ252L3PL3LYR54TFPPDVLPVT4/action/replication_record"}},"created_at":"2026-05-18T00:44:23.850772+00:00","updated_at":"2026-05-18T00:44:23.850772+00:00"}