{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:C3JFTHJEIMTUNOBBFI2Q4Q6TAB","short_pith_number":"pith:C3JFTHJE","schema_version":"1.0","canonical_sha256":"16d2599d24432746b8212a350e43d30075694aafa3641ab254d08a87a22b4236","source":{"kind":"arxiv","id":"1905.10378","version":3},"attestation_state":"computed","paper":{"title":"Jackiw-Teitelboim Gravity and Rotating Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.str-el","gr-qc"],"primary_cat":"hep-th","authors_text":"Sandip P. Trivedi, Sunil Kumar Sake, Upamanyu Moitra, V. Vishal","submitted_at":"2019-05-24T18:00:02Z","abstract_excerpt":"We show that the free energy at low temperatures for near-extremal black holes is correctly obtained from the Jackiw-Teitelboim (JT) model of gravity. Our arguments apply to all black holes, including rotating ones, whose metric has a near-horizon $\\mathrm{AdS}_2$ factor and the associated $\\mathrm{SL}(2,\\mathbb{R})$ symmetry. We verify these arguments by explicit calculations for rotating black holes in $4$ and $5$ dimensions. Our results suggest that the JT model could prove useful in analysing the dynamics of near-extremal Kerr black holes found in nature."},"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":"1905.10378","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2019-05-24T18:00:02Z","cross_cats_sorted":["cond-mat.str-el","gr-qc"],"title_canon_sha256":"ad35190f81565f907f46a654ab9349351aa74bcdb576899fdea6f83c105ac8c9","abstract_canon_sha256":"34dd87f636b4bf4b6aa58828e83e04a65a5205226313c3080ad9575ffc442579"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:19:08.262022Z","signature_b64":"6p0S+/5fRSK5SG0FcDUjnql0mwHsE1HtvyVFnFX9OuTpvD/xX/cE59IMwl9rp9ZpTJNhLxnV17A7WVZ9jr8qBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"16d2599d24432746b8212a350e43d30075694aafa3641ab254d08a87a22b4236","last_reissued_at":"2026-07-05T00:19:08.261552Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:19:08.261552Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Jackiw-Teitelboim Gravity and Rotating Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.str-el","gr-qc"],"primary_cat":"hep-th","authors_text":"Sandip P. Trivedi, Sunil Kumar Sake, Upamanyu Moitra, V. Vishal","submitted_at":"2019-05-24T18:00:02Z","abstract_excerpt":"We show that the free energy at low temperatures for near-extremal black holes is correctly obtained from the Jackiw-Teitelboim (JT) model of gravity. Our arguments apply to all black holes, including rotating ones, whose metric has a near-horizon $\\mathrm{AdS}_2$ factor and the associated $\\mathrm{SL}(2,\\mathbb{R})$ symmetry. We verify these arguments by explicit calculations for rotating black holes in $4$ and $5$ dimensions. Our results suggest that the JT model could prove useful in analysing the dynamics of near-extremal Kerr black holes found in nature."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1905.10378","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1905.10378/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":"1905.10378","created_at":"2026-07-05T00:19:08.261618+00:00"},{"alias_kind":"arxiv_version","alias_value":"1905.10378v3","created_at":"2026-07-05T00:19:08.261618+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1905.10378","created_at":"2026-07-05T00:19:08.261618+00:00"},{"alias_kind":"pith_short_12","alias_value":"C3JFTHJEIMTU","created_at":"2026-07-05T00:19:08.261618+00:00"},{"alias_kind":"pith_short_16","alias_value":"C3JFTHJEIMTUNOBB","created_at":"2026-07-05T00:19:08.261618+00:00"},{"alias_kind":"pith_short_8","alias_value":"C3JFTHJE","created_at":"2026-07-05T00:19:08.261618+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.30725","citing_title":"Constrained particle on a group: from propagators to correlators","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2605.23880","citing_title":"Not all black holes decohere quantum superpositions","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2502.13208","citing_title":"Finite cutoff JT gravity: Baby universes, Matrix dual, and (Krylov) Complexity","ref_index":15,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18405","citing_title":"Large-c BCFT Entanglement Entropy with Deformed Boundaries from Emergent JT Gravity","ref_index":18,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/C3JFTHJEIMTUNOBBFI2Q4Q6TAB","json":"https://pith.science/pith/C3JFTHJEIMTUNOBBFI2Q4Q6TAB.json","graph_json":"https://pith.science/api/pith-number/C3JFTHJEIMTUNOBBFI2Q4Q6TAB/graph.json","events_json":"https://pith.science/api/pith-number/C3JFTHJEIMTUNOBBFI2Q4Q6TAB/events.json","paper":"https://pith.science/paper/C3JFTHJE"},"agent_actions":{"view_html":"https://pith.science/pith/C3JFTHJEIMTUNOBBFI2Q4Q6TAB","download_json":"https://pith.science/pith/C3JFTHJEIMTUNOBBFI2Q4Q6TAB.json","view_paper":"https://pith.science/paper/C3JFTHJE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1905.10378&json=true","fetch_graph":"https://pith.science/api/pith-number/C3JFTHJEIMTUNOBBFI2Q4Q6TAB/graph.json","fetch_events":"https://pith.science/api/pith-number/C3JFTHJEIMTUNOBBFI2Q4Q6TAB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/C3JFTHJEIMTUNOBBFI2Q4Q6TAB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/C3JFTHJEIMTUNOBBFI2Q4Q6TAB/action/storage_attestation","attest_author":"https://pith.science/pith/C3JFTHJEIMTUNOBBFI2Q4Q6TAB/action/author_attestation","sign_citation":"https://pith.science/pith/C3JFTHJEIMTUNOBBFI2Q4Q6TAB/action/citation_signature","submit_replication":"https://pith.science/pith/C3JFTHJEIMTUNOBBFI2Q4Q6TAB/action/replication_record"}},"created_at":"2026-07-05T00:19:08.261618+00:00","updated_at":"2026-07-05T00:19:08.261618+00:00"}