{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:DSCCQW3DSHL7FUB7P4FGZTIANA","short_pith_number":"pith:DSCCQW3D","schema_version":"1.0","canonical_sha256":"1c84285b6391d7f2d03f7f0a6ccd006834b2a0f91372b222b814713231898f82","source":{"kind":"arxiv","id":"1807.11827","version":1},"attestation_state":"computed","paper":{"title":"Perturbative and nonperturbative fermionic quasinormal modes of Einstein-Gauss-Bonnet-AdS black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"P. A. Gonzalez, Ruth Noemi Villalobos, Yerko Vasquez","submitted_at":"2018-07-31T14:06:44Z","abstract_excerpt":"In this work, we present the quasinormal modes of a fermionic field in the background of Gauss-Bonnet-AdS black holes. We find exact solutions for $D=5$ at the fixed value $\\alpha=R^2/2$ of the Gauss--Bonnet coupling constant, with $R$ denoting the AdS radius, and we find numerical solutions for some range of values of the coupling constant $\\alpha$ and $D=5, 6$. Mainly, we find two branches of quasinormal frequencies, a branch perturbative in the Gauss-Bonnet coupling constant $\\alpha$, and another branch nonperturbative in $\\alpha$. The phenomena of nonperturbative modes, which seem to be qu"},"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":"1807.11827","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2018-07-31T14:06:44Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"1355d86accb17855dfd876a4ab5549c777f9f1424849134eb12011f4849ecb64","abstract_canon_sha256":"099f2e35557f02146e63ba84ec0cd480ba1c4049f18121a8640fc8acaf8f83f8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:04:48.114158Z","signature_b64":"ESnKj3wLLHZxLqvney+ihx4lH4Vjkz9NB6/dn96v9sn5VcwEJKP14PgXcIEOPD7gqXUArUU9Rh4lPJxZ8aZXCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1c84285b6391d7f2d03f7f0a6ccd006834b2a0f91372b222b814713231898f82","last_reissued_at":"2026-05-18T00:04:48.113501Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:04:48.113501Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Perturbative and nonperturbative fermionic quasinormal modes of Einstein-Gauss-Bonnet-AdS black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"P. A. Gonzalez, Ruth Noemi Villalobos, Yerko Vasquez","submitted_at":"2018-07-31T14:06:44Z","abstract_excerpt":"In this work, we present the quasinormal modes of a fermionic field in the background of Gauss-Bonnet-AdS black holes. We find exact solutions for $D=5$ at the fixed value $\\alpha=R^2/2$ of the Gauss--Bonnet coupling constant, with $R$ denoting the AdS radius, and we find numerical solutions for some range of values of the coupling constant $\\alpha$ and $D=5, 6$. Mainly, we find two branches of quasinormal frequencies, a branch perturbative in the Gauss-Bonnet coupling constant $\\alpha$, and another branch nonperturbative in $\\alpha$. The phenomena of nonperturbative modes, which seem to be qu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.11827","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":""},"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":"1807.11827","created_at":"2026-05-18T00:04:48.113602+00:00"},{"alias_kind":"arxiv_version","alias_value":"1807.11827v1","created_at":"2026-05-18T00:04:48.113602+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1807.11827","created_at":"2026-05-18T00:04:48.113602+00:00"},{"alias_kind":"pith_short_12","alias_value":"DSCCQW3DSHL7","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_16","alias_value":"DSCCQW3DSHL7FUB7","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_8","alias_value":"DSCCQW3D","created_at":"2026-05-18T12:32:19.392346+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2601.22340","citing_title":"Grey-body factors of higher dimensional regular black holes in quasi-topological theories","ref_index":59,"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":59,"is_internal_anchor":true},{"citing_arxiv_id":"2603.10844","citing_title":"Long-lived quasinormal modes, shadows and particle motion in four-dimensional quasi-topological gravity","ref_index":235,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DSCCQW3DSHL7FUB7P4FGZTIANA","json":"https://pith.science/pith/DSCCQW3DSHL7FUB7P4FGZTIANA.json","graph_json":"https://pith.science/api/pith-number/DSCCQW3DSHL7FUB7P4FGZTIANA/graph.json","events_json":"https://pith.science/api/pith-number/DSCCQW3DSHL7FUB7P4FGZTIANA/events.json","paper":"https://pith.science/paper/DSCCQW3D"},"agent_actions":{"view_html":"https://pith.science/pith/DSCCQW3DSHL7FUB7P4FGZTIANA","download_json":"https://pith.science/pith/DSCCQW3DSHL7FUB7P4FGZTIANA.json","view_paper":"https://pith.science/paper/DSCCQW3D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1807.11827&json=true","fetch_graph":"https://pith.science/api/pith-number/DSCCQW3DSHL7FUB7P4FGZTIANA/graph.json","fetch_events":"https://pith.science/api/pith-number/DSCCQW3DSHL7FUB7P4FGZTIANA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DSCCQW3DSHL7FUB7P4FGZTIANA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DSCCQW3DSHL7FUB7P4FGZTIANA/action/storage_attestation","attest_author":"https://pith.science/pith/DSCCQW3DSHL7FUB7P4FGZTIANA/action/author_attestation","sign_citation":"https://pith.science/pith/DSCCQW3DSHL7FUB7P4FGZTIANA/action/citation_signature","submit_replication":"https://pith.science/pith/DSCCQW3DSHL7FUB7P4FGZTIANA/action/replication_record"}},"created_at":"2026-05-18T00:04:48.113602+00:00","updated_at":"2026-05-18T00:04:48.113602+00:00"}