{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:TQL4J6ZHKMROUKQ6SPSUZV5A6V","short_pith_number":"pith:TQL4J6ZH","schema_version":"1.0","canonical_sha256":"9c17c4fb275322ea2a1e93e54cd7a0f566585da3edd01feec928dfcc3e08c7ad","source":{"kind":"arxiv","id":"0902.1487","version":4},"attestation_state":"computed","paper":{"title":"Vacuum polarization effects on quasinormal modes in electrically charged black hole spacetimes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Jeferson de Oliveira, Owen Pavel Fernandez Piedra","submitted_at":"2009-02-09T18:08:01Z","abstract_excerpt":"We investigate the influence of vacuum polarization of quantum massive fields on the scalar sector of quasinormal modes in spherically symmetric black holes. We consider the evolution of a massless scalar field on the spacetime corresponding to a charged semiclassical black hole, consisting of the quantum corrected geometry of a Reissner-Nordstr\\\"om black hole dressed by a quantum massive scalar field in the large mass limit. Using a sixth order WKB approach we find the shift in the quasinormal mode frequencies due to vacuum polarization ."},"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":"0902.1487","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2009-02-09T18:08:01Z","cross_cats_sorted":[],"title_canon_sha256":"355e0dab70f40e0a1a2cbd1fe0f2ef3775921911b6b94bc789e2b0d195fe5952","abstract_canon_sha256":"e1d0e57ec6c8129a34f3d699e90247f0a351321c5dfaf99b2eaec3246ea2349f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:18:13.164013Z","signature_b64":"qgaafArdPgcvu2u0hLxq8huTHOvTd8zK64ePctBy9kYy70IKBpfFCowXyeHp8RbzK12RRP2Q5SYBYWEaYWEJCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9c17c4fb275322ea2a1e93e54cd7a0f566585da3edd01feec928dfcc3e08c7ad","last_reissued_at":"2026-05-18T04:18:13.163372Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:18:13.163372Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Vacuum polarization effects on quasinormal modes in electrically charged black hole spacetimes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Jeferson de Oliveira, Owen Pavel Fernandez Piedra","submitted_at":"2009-02-09T18:08:01Z","abstract_excerpt":"We investigate the influence of vacuum polarization of quantum massive fields on the scalar sector of quasinormal modes in spherically symmetric black holes. We consider the evolution of a massless scalar field on the spacetime corresponding to a charged semiclassical black hole, consisting of the quantum corrected geometry of a Reissner-Nordstr\\\"om black hole dressed by a quantum massive scalar field in the large mass limit. Using a sixth order WKB approach we find the shift in the quasinormal mode frequencies due to vacuum polarization ."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0902.1487","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":""},"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":"0902.1487","created_at":"2026-05-18T04:18:13.163474+00:00"},{"alias_kind":"arxiv_version","alias_value":"0902.1487v4","created_at":"2026-05-18T04:18:13.163474+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0902.1487","created_at":"2026-05-18T04:18:13.163474+00:00"},{"alias_kind":"pith_short_12","alias_value":"TQL4J6ZHKMRO","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_16","alias_value":"TQL4J6ZHKMROUKQ6","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_8","alias_value":"TQL4J6ZH","created_at":"2026-05-18T12:26:01.383474+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TQL4J6ZHKMROUKQ6SPSUZV5A6V","json":"https://pith.science/pith/TQL4J6ZHKMROUKQ6SPSUZV5A6V.json","graph_json":"https://pith.science/api/pith-number/TQL4J6ZHKMROUKQ6SPSUZV5A6V/graph.json","events_json":"https://pith.science/api/pith-number/TQL4J6ZHKMROUKQ6SPSUZV5A6V/events.json","paper":"https://pith.science/paper/TQL4J6ZH"},"agent_actions":{"view_html":"https://pith.science/pith/TQL4J6ZHKMROUKQ6SPSUZV5A6V","download_json":"https://pith.science/pith/TQL4J6ZHKMROUKQ6SPSUZV5A6V.json","view_paper":"https://pith.science/paper/TQL4J6ZH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0902.1487&json=true","fetch_graph":"https://pith.science/api/pith-number/TQL4J6ZHKMROUKQ6SPSUZV5A6V/graph.json","fetch_events":"https://pith.science/api/pith-number/TQL4J6ZHKMROUKQ6SPSUZV5A6V/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TQL4J6ZHKMROUKQ6SPSUZV5A6V/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TQL4J6ZHKMROUKQ6SPSUZV5A6V/action/storage_attestation","attest_author":"https://pith.science/pith/TQL4J6ZHKMROUKQ6SPSUZV5A6V/action/author_attestation","sign_citation":"https://pith.science/pith/TQL4J6ZHKMROUKQ6SPSUZV5A6V/action/citation_signature","submit_replication":"https://pith.science/pith/TQL4J6ZHKMROUKQ6SPSUZV5A6V/action/replication_record"}},"created_at":"2026-05-18T04:18:13.163474+00:00","updated_at":"2026-05-18T04:18:13.163474+00:00"}