{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:7KX5BYB2NOHG36YGOZPWCMFCY5","short_pith_number":"pith:7KX5BYB2","schema_version":"1.0","canonical_sha256":"faafd0e03a6b8e6dfb06765f6130a2c759218e13ef4a04685d51d6a8e2771ada","source":{"kind":"arxiv","id":"1902.04078","version":3},"attestation_state":"computed","paper":{"title":"Universal low temperature theory of charged black holes with AdS$_2$ horizons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.str-el"],"primary_cat":"hep-th","authors_text":"Subir Sachdev","submitted_at":"2019-02-11T19:00:00Z","abstract_excerpt":"We consider the low temperature quantum theory of a charged black hole of zero temperature horizon radius $R_h$, in a spacetime which is asymptotically AdS$_{D}$ ($D > 3$) far from the horizon. At temperatures $T \\ll 1/R_h$, the near-horizon geometry is AdS$_2$, and the black hole is described by a universal 0+1 dimensional effective quantum theory of time diffeomorphisms with a Schwarzian action, and a phase mode conjugate to the U(1) charge. We obtain this universal 0+1 dimensional effective theory starting from the full $D$-dimensional Einstein-Maxwell theory, while keeping quantitative tra"},"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":"1902.04078","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2019-02-11T19:00:00Z","cross_cats_sorted":["cond-mat.str-el"],"title_canon_sha256":"49c5534376f250adf1e957b30c40022284755f8d876f9413bd64e80b50e82fef","abstract_canon_sha256":"6fa1b3a46e99256371bae13a43d4249decc6ee8fc2544bfd7ab021dd91fde149"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:45:52.068408Z","signature_b64":"bzvnhnD8hvi+G+kzmwwJXPBIu6WiKuzlg0bzPwmZXtxP0q01tbrfYDt1+uIPuLOg4bK0lSdiNWS7FQF7cUkVAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"faafd0e03a6b8e6dfb06765f6130a2c759218e13ef4a04685d51d6a8e2771ada","last_reissued_at":"2026-05-17T23:45:52.067851Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:45:52.067851Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Universal low temperature theory of charged black holes with AdS$_2$ horizons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.str-el"],"primary_cat":"hep-th","authors_text":"Subir Sachdev","submitted_at":"2019-02-11T19:00:00Z","abstract_excerpt":"We consider the low temperature quantum theory of a charged black hole of zero temperature horizon radius $R_h$, in a spacetime which is asymptotically AdS$_{D}$ ($D > 3$) far from the horizon. At temperatures $T \\ll 1/R_h$, the near-horizon geometry is AdS$_2$, and the black hole is described by a universal 0+1 dimensional effective quantum theory of time diffeomorphisms with a Schwarzian action, and a phase mode conjugate to the U(1) charge. We obtain this universal 0+1 dimensional effective theory starting from the full $D$-dimensional Einstein-Maxwell theory, while keeping quantitative tra"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1902.04078","kind":"arxiv","version":3},"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":"1902.04078","created_at":"2026-05-17T23:45:52.067925+00:00"},{"alias_kind":"arxiv_version","alias_value":"1902.04078v3","created_at":"2026-05-17T23:45:52.067925+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1902.04078","created_at":"2026-05-17T23:45:52.067925+00:00"},{"alias_kind":"pith_short_12","alias_value":"7KX5BYB2NOHG","created_at":"2026-05-18T12:33:12.712433+00:00"},{"alias_kind":"pith_short_16","alias_value":"7KX5BYB2NOHG36YG","created_at":"2026-05-18T12:33:12.712433+00:00"},{"alias_kind":"pith_short_8","alias_value":"7KX5BYB2","created_at":"2026-05-18T12:33:12.712433+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2509.05052","citing_title":"Semi-classical spacetime thermodynamics","ref_index":82,"is_internal_anchor":true},{"citing_arxiv_id":"1905.08762","citing_title":"The entropy of bulk quantum fields and the entanglement wedge of an evaporating black hole","ref_index":34,"is_internal_anchor":true},{"citing_arxiv_id":"2602.01096","citing_title":"Replica Phase Transition with Quantum Gravity Corrections","ref_index":6,"is_internal_anchor":true},{"citing_arxiv_id":"2604.24101","citing_title":"$g_{tt}g_{rr} =-1$ black hole thermodynamics in extended quasi-topological gravity","ref_index":106,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15566","citing_title":"One-loop effect in the charged 2D black hole near extremality","ref_index":61,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7KX5BYB2NOHG36YGOZPWCMFCY5","json":"https://pith.science/pith/7KX5BYB2NOHG36YGOZPWCMFCY5.json","graph_json":"https://pith.science/api/pith-number/7KX5BYB2NOHG36YGOZPWCMFCY5/graph.json","events_json":"https://pith.science/api/pith-number/7KX5BYB2NOHG36YGOZPWCMFCY5/events.json","paper":"https://pith.science/paper/7KX5BYB2"},"agent_actions":{"view_html":"https://pith.science/pith/7KX5BYB2NOHG36YGOZPWCMFCY5","download_json":"https://pith.science/pith/7KX5BYB2NOHG36YGOZPWCMFCY5.json","view_paper":"https://pith.science/paper/7KX5BYB2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1902.04078&json=true","fetch_graph":"https://pith.science/api/pith-number/7KX5BYB2NOHG36YGOZPWCMFCY5/graph.json","fetch_events":"https://pith.science/api/pith-number/7KX5BYB2NOHG36YGOZPWCMFCY5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7KX5BYB2NOHG36YGOZPWCMFCY5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7KX5BYB2NOHG36YGOZPWCMFCY5/action/storage_attestation","attest_author":"https://pith.science/pith/7KX5BYB2NOHG36YGOZPWCMFCY5/action/author_attestation","sign_citation":"https://pith.science/pith/7KX5BYB2NOHG36YGOZPWCMFCY5/action/citation_signature","submit_replication":"https://pith.science/pith/7KX5BYB2NOHG36YGOZPWCMFCY5/action/replication_record"}},"created_at":"2026-05-17T23:45:52.067925+00:00","updated_at":"2026-05-17T23:45:52.067925+00:00"}