{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:LETOJMYQZY2YNWS2UOE2RNHYPT","short_pith_number":"pith:LETOJMYQ","schema_version":"1.0","canonical_sha256":"5926e4b310ce3586da5aa389a8b4f87cf982423b446fe2c6af6e5f2cbeff4548","source":{"kind":"arxiv","id":"gr-qc/0607048","version":3},"attestation_state":"computed","paper":{"title":"Quasi-Normal Modes of Brane-Localised Standard Model Fields II: Kerr Black Holes","license":"","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"A. Zhidenko, P. Kanti, R. A. Konoplya","submitted_at":"2006-07-11T20:50:14Z","abstract_excerpt":"This paper presents a comprehensive study of the fundamental quasinormal modes of all Standard Model fields propagating on a brane embedded in a higher-dimensional rotating black hole spacetime. The equations of motion for fields with spin $s=0, 1/2$ and 1 propagating in the induced-on-the-brane background are solved numerically, and the dependence of their QN spectra on the black hole angular momentum and dimensionality of spacetime is investigated. It is found that the brane-localised field perturbations are longer-lived when the higher-dimensional black hole rotates faster, while an increas"},"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":"gr-qc/0607048","kind":"arxiv","version":3},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"2006-07-11T20:50:14Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"13c5a2da97518d02a9d2e61766aea17af3e3087cf472c4ff252326ebfb6ac215","abstract_canon_sha256":"c358ee516a8f1862ebc3bb830aea12c670ad77b7353514e8fdf271d74f7a1fa2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:01:29.127357Z","signature_b64":"i063rqDX6o93TIcIqfQD3rxcN5qrY5eXdQvrBVXKcgUtYKn5Gd4yaf14u4GRT1rgDU2JTwWxinge3psLWXBoDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5926e4b310ce3586da5aa389a8b4f87cf982423b446fe2c6af6e5f2cbeff4548","last_reissued_at":"2026-07-04T17:01:29.127016Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:01:29.127016Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quasi-Normal Modes of Brane-Localised Standard Model Fields II: Kerr Black Holes","license":"","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"A. Zhidenko, P. Kanti, R. A. Konoplya","submitted_at":"2006-07-11T20:50:14Z","abstract_excerpt":"This paper presents a comprehensive study of the fundamental quasinormal modes of all Standard Model fields propagating on a brane embedded in a higher-dimensional rotating black hole spacetime. The equations of motion for fields with spin $s=0, 1/2$ and 1 propagating in the induced-on-the-brane background are solved numerically, and the dependence of their QN spectra on the black hole angular momentum and dimensionality of spacetime is investigated. It is found that the brane-localised field perturbations are longer-lived when the higher-dimensional black hole rotates faster, while an increas"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/0607048","kind":"arxiv","version":3},"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/gr-qc/0607048/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":"gr-qc/0607048","created_at":"2026-07-04T17:01:29.127070+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/0607048v3","created_at":"2026-07-04T17:01:29.127070+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/0607048","created_at":"2026-07-04T17:01:29.127070+00:00"},{"alias_kind":"pith_short_12","alias_value":"LETOJMYQZY2Y","created_at":"2026-07-04T17:01:29.127070+00:00"},{"alias_kind":"pith_short_16","alias_value":"LETOJMYQZY2YNWS2","created_at":"2026-07-04T17:01:29.127070+00:00"},{"alias_kind":"pith_short_8","alias_value":"LETOJMYQ","created_at":"2026-07-04T17:01:29.127070+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":8,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2606.08631","citing_title":"Hawking Radiation from the Dymnikova Regular Black Hole","ref_index":49,"is_internal_anchor":true},{"citing_arxiv_id":"2606.08351","citing_title":"Hawking Emission from Black Holes Evaporating toward Wormholes and the Accuracy of the WKB Approximation","ref_index":16,"is_internal_anchor":true},{"citing_arxiv_id":"2602.11001","citing_title":"Two types of quasinormal modes of Casadio-Fabbri-Mazzacurati brane-world black holes","ref_index":39,"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":192,"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":38,"is_internal_anchor":false},{"citing_arxiv_id":"1102.4014","citing_title":"Quasinormal modes of black holes: from astrophysics to string theory","ref_index":143,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26166","citing_title":"Scattering of electromagnetic field in quasi-topological gravity","ref_index":29,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11845","citing_title":"Quasi-resonances in the vicinity of Einstein-Maxwell-dilaton black hole","ref_index":105,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LETOJMYQZY2YNWS2UOE2RNHYPT","json":"https://pith.science/pith/LETOJMYQZY2YNWS2UOE2RNHYPT.json","graph_json":"https://pith.science/api/pith-number/LETOJMYQZY2YNWS2UOE2RNHYPT/graph.json","events_json":"https://pith.science/api/pith-number/LETOJMYQZY2YNWS2UOE2RNHYPT/events.json","paper":"https://pith.science/paper/LETOJMYQ"},"agent_actions":{"view_html":"https://pith.science/pith/LETOJMYQZY2YNWS2UOE2RNHYPT","download_json":"https://pith.science/pith/LETOJMYQZY2YNWS2UOE2RNHYPT.json","view_paper":"https://pith.science/paper/LETOJMYQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/0607048&json=true","fetch_graph":"https://pith.science/api/pith-number/LETOJMYQZY2YNWS2UOE2RNHYPT/graph.json","fetch_events":"https://pith.science/api/pith-number/LETOJMYQZY2YNWS2UOE2RNHYPT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LETOJMYQZY2YNWS2UOE2RNHYPT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LETOJMYQZY2YNWS2UOE2RNHYPT/action/storage_attestation","attest_author":"https://pith.science/pith/LETOJMYQZY2YNWS2UOE2RNHYPT/action/author_attestation","sign_citation":"https://pith.science/pith/LETOJMYQZY2YNWS2UOE2RNHYPT/action/citation_signature","submit_replication":"https://pith.science/pith/LETOJMYQZY2YNWS2UOE2RNHYPT/action/replication_record"}},"created_at":"2026-07-04T17:01:29.127070+00:00","updated_at":"2026-07-04T17:01:29.127070+00:00"}