{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:AOZQR7CQQPXHIS4JPRRQ7QY6WH","short_pith_number":"pith:AOZQR7CQ","schema_version":"1.0","canonical_sha256":"03b308fc5083ee744b897c630fc31eb1fdfe9f72921a23207a8b91b9c4371106","source":{"kind":"arxiv","id":"2605.21533","version":1},"attestation_state":"computed","paper":{"title":"Long-lived quasinormal modes of Asymptotically de Sitter Black Holes in Generalized Proca Theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"S. V. Bolokhov","submitted_at":"2026-05-19T22:29:19Z","abstract_excerpt":"Massive scalar perturbations of asymptotically de Sitter black holes in generalized Proca theory display a sharp interplay between primary hair, horizon structure, and field mass. Using high-order WKB calculations supplemented by time-domain evolution, we analyze representative black-hole backgrounds and compare the full black-hole spectrum with the exact pure de Sitter benchmark. We show that increasing the scalar mass drives the frequencies into a simple large-mass regime in which the real part grows linearly while the damping rate approaches a nonzero geometry-dependent constant, so true 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":"2605.21533","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2026-05-19T22:29:19Z","cross_cats_sorted":[],"title_canon_sha256":"5f3800714a4a84e520893dd0a2af7e1b47177ea50d7382d7214e73033e73ee12","abstract_canon_sha256":"ad2b1be8ef7f271580d3ac7ed7f3ab1fc0af55ac9729d4066355b370d266e162"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-22T00:02:27.809947Z","signature_b64":"BiGSW/fF7IdCIqFGn4QlDRqPTnNu+CHT6innkKNwH2eRErdnmjBzKCwrG44jBw2gEpJX87OKVTyGM5iQ5YxYCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"03b308fc5083ee744b897c630fc31eb1fdfe9f72921a23207a8b91b9c4371106","last_reissued_at":"2026-05-22T00:02:27.809495Z","signature_status":"signed_v1","first_computed_at":"2026-05-22T00:02:27.809495Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Long-lived quasinormal modes of Asymptotically de Sitter Black Holes in Generalized Proca Theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"S. V. Bolokhov","submitted_at":"2026-05-19T22:29:19Z","abstract_excerpt":"Massive scalar perturbations of asymptotically de Sitter black holes in generalized Proca theory display a sharp interplay between primary hair, horizon structure, and field mass. Using high-order WKB calculations supplemented by time-domain evolution, we analyze representative black-hole backgrounds and compare the full black-hole spectrum with the exact pure de Sitter benchmark. We show that increasing the scalar mass drives the frequencies into a simple large-mass regime in which the real part grows linearly while the damping rate approaches a nonzero geometry-dependent constant, so true qu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2605.21533","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2605.21533/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":"2605.21533","created_at":"2026-05-22T00:02:27.809566+00:00"},{"alias_kind":"arxiv_version","alias_value":"2605.21533v1","created_at":"2026-05-22T00:02:27.809566+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.21533","created_at":"2026-05-22T00:02:27.809566+00:00"},{"alias_kind":"pith_short_12","alias_value":"AOZQR7CQQPXH","created_at":"2026-05-22T00:02:27.809566+00:00"},{"alias_kind":"pith_short_16","alias_value":"AOZQR7CQQPXHIS4J","created_at":"2026-05-22T00:02:27.809566+00:00"},{"alias_kind":"pith_short_8","alias_value":"AOZQR7CQ","created_at":"2026-05-22T00:02:27.809566+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/AOZQR7CQQPXHIS4JPRRQ7QY6WH","json":"https://pith.science/pith/AOZQR7CQQPXHIS4JPRRQ7QY6WH.json","graph_json":"https://pith.science/api/pith-number/AOZQR7CQQPXHIS4JPRRQ7QY6WH/graph.json","events_json":"https://pith.science/api/pith-number/AOZQR7CQQPXHIS4JPRRQ7QY6WH/events.json","paper":"https://pith.science/paper/AOZQR7CQ"},"agent_actions":{"view_html":"https://pith.science/pith/AOZQR7CQQPXHIS4JPRRQ7QY6WH","download_json":"https://pith.science/pith/AOZQR7CQQPXHIS4JPRRQ7QY6WH.json","view_paper":"https://pith.science/paper/AOZQR7CQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2605.21533&json=true","fetch_graph":"https://pith.science/api/pith-number/AOZQR7CQQPXHIS4JPRRQ7QY6WH/graph.json","fetch_events":"https://pith.science/api/pith-number/AOZQR7CQQPXHIS4JPRRQ7QY6WH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AOZQR7CQQPXHIS4JPRRQ7QY6WH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AOZQR7CQQPXHIS4JPRRQ7QY6WH/action/storage_attestation","attest_author":"https://pith.science/pith/AOZQR7CQQPXHIS4JPRRQ7QY6WH/action/author_attestation","sign_citation":"https://pith.science/pith/AOZQR7CQQPXHIS4JPRRQ7QY6WH/action/citation_signature","submit_replication":"https://pith.science/pith/AOZQR7CQQPXHIS4JPRRQ7QY6WH/action/replication_record"}},"created_at":"2026-05-22T00:02:27.809566+00:00","updated_at":"2026-05-22T00:02:27.809566+00:00"}