{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:D7JWPH65H6HUBE23WQNVHJJCD4","short_pith_number":"pith:D7JWPH65","schema_version":"1.0","canonical_sha256":"1fd3679fdd3f8f40935bb41b53a5221f1a72d46c1dd4bfb6a306df89818c21e0","source":{"kind":"arxiv","id":"2512.19642","version":2},"attestation_state":"computed","paper":{"title":"Schwarzian quantum corrections to shear correlators of the near-extremal Reissner-Nordstr\\\"om-AdS black hole","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Blaise Gout\\'eraux, Cl\\'ement Supiot, David M. Ramirez","submitted_at":"2025-12-22T18:16:53Z","abstract_excerpt":"Near-AdS$_2$ spacetimes are controlled by a Schwarzian effective dual theory. The Kaluza-Klein reduction of higher-dimensional black holes shows that the Schwarzian generates a logarithmic contribution to the entropy, thereby resolving a long-standing puzzle in near-extremal black hole thermodynamics. Here, we leverage exact results for quantum-corrected, Schwarzian scalar correlation functions in order to evaluate the impact of bulk quantum fluctuations on the low-temperature shear correlators of the state dual to Reissner-Nordstr\\\"om-AdS$_4$ black holes with a flat, compact horizon. In the h"},"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":"2512.19642","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2025-12-22T18:16:53Z","cross_cats_sorted":[],"title_canon_sha256":"080e447d262d892a2dcd0b258b5551ed9298c709526b6edc2c4e3aeec58c11a4","abstract_canon_sha256":"83af537ba9a5a18bb2ab2907e6d808bb2f595a619abd8c4e9170070aa90ed3ed"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-29T01:15:03.751644Z","signature_b64":"0TowfP7qHk2eDj5yOJ16N5N1XLbPukBFRvqE0UV5NHyTdHQJwas+hmNfE7qES6i312Rv/0OfUR6aDfmPYMSpCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1fd3679fdd3f8f40935bb41b53a5221f1a72d46c1dd4bfb6a306df89818c21e0","last_reissued_at":"2026-06-29T01:15:03.751133Z","signature_status":"signed_v1","first_computed_at":"2026-06-29T01:15:03.751133Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Schwarzian quantum corrections to shear correlators of the near-extremal Reissner-Nordstr\\\"om-AdS black hole","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Blaise Gout\\'eraux, Cl\\'ement Supiot, David M. Ramirez","submitted_at":"2025-12-22T18:16:53Z","abstract_excerpt":"Near-AdS$_2$ spacetimes are controlled by a Schwarzian effective dual theory. The Kaluza-Klein reduction of higher-dimensional black holes shows that the Schwarzian generates a logarithmic contribution to the entropy, thereby resolving a long-standing puzzle in near-extremal black hole thermodynamics. Here, we leverage exact results for quantum-corrected, Schwarzian scalar correlation functions in order to evaluate the impact of bulk quantum fluctuations on the low-temperature shear correlators of the state dual to Reissner-Nordstr\\\"om-AdS$_4$ black holes with a flat, compact horizon. In the h"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2512.19642","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/2512.19642/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":"2512.19642","created_at":"2026-06-29T01:15:03.751184+00:00"},{"alias_kind":"arxiv_version","alias_value":"2512.19642v2","created_at":"2026-06-29T01:15:03.751184+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2512.19642","created_at":"2026-06-29T01:15:03.751184+00:00"},{"alias_kind":"pith_short_12","alias_value":"D7JWPH65H6HU","created_at":"2026-06-29T01:15:03.751184+00:00"},{"alias_kind":"pith_short_16","alias_value":"D7JWPH65H6HUBE23","created_at":"2026-06-29T01:15:03.751184+00:00"},{"alias_kind":"pith_short_8","alias_value":"D7JWPH65","created_at":"2026-06-29T01:15:03.751184+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.23880","citing_title":"Not all black holes decohere quantum superpositions","ref_index":41,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/D7JWPH65H6HUBE23WQNVHJJCD4","json":"https://pith.science/pith/D7JWPH65H6HUBE23WQNVHJJCD4.json","graph_json":"https://pith.science/api/pith-number/D7JWPH65H6HUBE23WQNVHJJCD4/graph.json","events_json":"https://pith.science/api/pith-number/D7JWPH65H6HUBE23WQNVHJJCD4/events.json","paper":"https://pith.science/paper/D7JWPH65"},"agent_actions":{"view_html":"https://pith.science/pith/D7JWPH65H6HUBE23WQNVHJJCD4","download_json":"https://pith.science/pith/D7JWPH65H6HUBE23WQNVHJJCD4.json","view_paper":"https://pith.science/paper/D7JWPH65","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2512.19642&json=true","fetch_graph":"https://pith.science/api/pith-number/D7JWPH65H6HUBE23WQNVHJJCD4/graph.json","fetch_events":"https://pith.science/api/pith-number/D7JWPH65H6HUBE23WQNVHJJCD4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/D7JWPH65H6HUBE23WQNVHJJCD4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/D7JWPH65H6HUBE23WQNVHJJCD4/action/storage_attestation","attest_author":"https://pith.science/pith/D7JWPH65H6HUBE23WQNVHJJCD4/action/author_attestation","sign_citation":"https://pith.science/pith/D7JWPH65H6HUBE23WQNVHJJCD4/action/citation_signature","submit_replication":"https://pith.science/pith/D7JWPH65H6HUBE23WQNVHJJCD4/action/replication_record"}},"created_at":"2026-06-29T01:15:03.751184+00:00","updated_at":"2026-06-29T01:15:03.751184+00:00"}