{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:CUY5UV7RAHEZHS7OTYSXSFNZ5X","short_pith_number":"pith:CUY5UV7R","schema_version":"1.0","canonical_sha256":"1531da57f101c993cbee9e257915b9edcb1a6f505d42732c795220298427c6e3","source":{"kind":"arxiv","id":"2408.11529","version":2},"attestation_state":"computed","paper":{"title":"Supergravity Spectrum of AdS$_5$ Black Holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Finn Larsen, Nizar Ezroura","submitted_at":"2024-08-21T11:10:44Z","abstract_excerpt":"We embed Kerr-Newman-AdS black holes into $\\mathcal{N} = 8$ gauged supergravity and study quadratic fluctuations around the black hole backgrounds of all fields in the larger theory. The equations of motion of the perturbations are partially diagonalized by the group theory of broken symmetry. Nearly all fields in theory have non-minimal couplings, so their equations of motion are not merely massive Klein-Gordon equations with minimal coupling to background gauge fields, and their analogues for fields with spin. In the special case of extremal black holes we identify specific modes of instabil"},"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":"2408.11529","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2024-08-21T11:10:44Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"cda4d1b60ca345e1b60152836bac4af26d887ab0050579b2395d508bcdb98e81","abstract_canon_sha256":"ebe2c93baf54572071210173d49e033fc83baf6c7e47e9a5104596e6902fb5e7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:39:57.677515Z","signature_b64":"lr4aS2LaydiNAog/8nt6jo3gtg8V0PUjQ/djEepiKUsipKQflI1HnUHshtFm3t0/Sq2R7Evza1VHcljBiJGQAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1531da57f101c993cbee9e257915b9edcb1a6f505d42732c795220298427c6e3","last_reissued_at":"2026-07-05T09:39:57.677081Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:39:57.677081Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Supergravity Spectrum of AdS$_5$ Black Holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Finn Larsen, Nizar Ezroura","submitted_at":"2024-08-21T11:10:44Z","abstract_excerpt":"We embed Kerr-Newman-AdS black holes into $\\mathcal{N} = 8$ gauged supergravity and study quadratic fluctuations around the black hole backgrounds of all fields in the larger theory. The equations of motion of the perturbations are partially diagonalized by the group theory of broken symmetry. Nearly all fields in theory have non-minimal couplings, so their equations of motion are not merely massive Klein-Gordon equations with minimal coupling to background gauge fields, and their analogues for fields with spin. In the special case of extremal black holes we identify specific modes of instabil"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2408.11529","kind":"arxiv","version":2},"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/2408.11529/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":"2408.11529","created_at":"2026-07-05T09:39:57.677137+00:00"},{"alias_kind":"arxiv_version","alias_value":"2408.11529v2","created_at":"2026-07-05T09:39:57.677137+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2408.11529","created_at":"2026-07-05T09:39:57.677137+00:00"},{"alias_kind":"pith_short_12","alias_value":"CUY5UV7RAHEZ","created_at":"2026-07-05T09:39:57.677137+00:00"},{"alias_kind":"pith_short_16","alias_value":"CUY5UV7RAHEZHS7O","created_at":"2026-07-05T09:39:57.677137+00:00"},{"alias_kind":"pith_short_8","alias_value":"CUY5UV7R","created_at":"2026-07-05T09:39:57.677137+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.23287","citing_title":"Chaos of Berry curvature for BPS microstates","ref_index":118,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CUY5UV7RAHEZHS7OTYSXSFNZ5X","json":"https://pith.science/pith/CUY5UV7RAHEZHS7OTYSXSFNZ5X.json","graph_json":"https://pith.science/api/pith-number/CUY5UV7RAHEZHS7OTYSXSFNZ5X/graph.json","events_json":"https://pith.science/api/pith-number/CUY5UV7RAHEZHS7OTYSXSFNZ5X/events.json","paper":"https://pith.science/paper/CUY5UV7R"},"agent_actions":{"view_html":"https://pith.science/pith/CUY5UV7RAHEZHS7OTYSXSFNZ5X","download_json":"https://pith.science/pith/CUY5UV7RAHEZHS7OTYSXSFNZ5X.json","view_paper":"https://pith.science/paper/CUY5UV7R","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2408.11529&json=true","fetch_graph":"https://pith.science/api/pith-number/CUY5UV7RAHEZHS7OTYSXSFNZ5X/graph.json","fetch_events":"https://pith.science/api/pith-number/CUY5UV7RAHEZHS7OTYSXSFNZ5X/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CUY5UV7RAHEZHS7OTYSXSFNZ5X/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CUY5UV7RAHEZHS7OTYSXSFNZ5X/action/storage_attestation","attest_author":"https://pith.science/pith/CUY5UV7RAHEZHS7OTYSXSFNZ5X/action/author_attestation","sign_citation":"https://pith.science/pith/CUY5UV7RAHEZHS7OTYSXSFNZ5X/action/citation_signature","submit_replication":"https://pith.science/pith/CUY5UV7RAHEZHS7OTYSXSFNZ5X/action/replication_record"}},"created_at":"2026-07-05T09:39:57.677137+00:00","updated_at":"2026-07-05T09:39:57.677137+00:00"}