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In the WKB regime, $qQ\\gg\\hbar$, we obtain a simple expression for the fundamental quasinormal resonances: $\\omega=qQ/r_+-i2\\pi T_{\\text{BH}}(n+{1 \\over 2})$, where $T_{\\text{BH}}$ and $Q$ are the temperature and electric charge of the black hole and $q$ is the electric charge of the field. Remarkably, our results show that the relaxation dynamics of a perturbed Reissner-Nordstr\\\"om black hole may saturate the recently proposed universal relaxat"},"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":"1205.5087","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2012-05-23T03:57:16Z","cross_cats_sorted":["astro-ph.HE","hep-th"],"title_canon_sha256":"78458c6c121098b165ef1d5b457fe7d34af2bb5ccba4c439ffcbcf3beb4bae0d","abstract_canon_sha256":"5049c387cdab2ec57170117a10be2b7643d53d0e661dbe208c1f01a9fb2fe570"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:57:24.213658Z","signature_b64":"tV4qsISVAWcDWml3IDzf4NlKu2SBiuu0llyjFZ+cHimMJPQY/D1DZztOj3M4XkKXC59x7jjeEw8uNljcZ/nsDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"64fbe3ac2d7679b39624f32dac49084b86d31ee4304870d3927e8af98cad2c18","last_reissued_at":"2026-05-18T01:57:24.213135Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:57:24.213135Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quasinormal resonances of a charged scalar field in a charged Reissner-Nordstr\\\"om black hole spacetime: A WKB analysis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"Shahar Hod","submitted_at":"2012-05-23T03:57:16Z","abstract_excerpt":"The fundamental quasinormal resonances of charged Reissner-Nordstr\\\"om black holes due to charged scalar perturbations are derived {\\it analytically}. 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