{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:XGEOWCBOR7VISCK3SA7LVKVRN4","short_pith_number":"pith:XGEOWCBO","schema_version":"1.0","canonical_sha256":"b988eb082e8fea89095b903ebaaab16f3dad02e224ff8cdec1d3c26e5d784c28","source":{"kind":"arxiv","id":"1909.03137","version":2},"attestation_state":"computed","paper":{"title":"Warped Symmetries of the Kerr Black Hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Alejandra Castro, Ankit Aggarwal, St\\'ephane Detournay","submitted_at":"2019-09-06T22:09:16Z","abstract_excerpt":"We propose a set of diffeomorphism that act non-trivially near the horizon of the Kerr black hole. We follow the recent developments of Haco-Hawking-Perry-Strominger to quantify this phase space, with the most substantial difference being our choice of vectors fields. Our gravitational charges are organized into a Virasoro-Kac-Moody algebra with non-trivial central extensions. We interpret this algebra as arising from a warped conformal field theory. Using the data we can infer from this warped CFT description, we capture the thermodynamic properties of the Kerr black hole."},"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":"1909.03137","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2019-09-06T22:09:16Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"28d7ba7d82ea9a9a19a01e088b3356ce6bbbd28fb54228b6bf859945bb430f92","abstract_canon_sha256":"458bef65ee245944d8819b0460eda9b35425f370684f367e1857df3e09468592"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:32:39.181768Z","signature_b64":"RIUCw3MJgyPljBVwqP4FdgHnGQwEbmSlre+u7nmTiDz7kTPUTHu61tKrWea0BtV6L2TAR3LmZXI5BFrtThC+Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b988eb082e8fea89095b903ebaaab16f3dad02e224ff8cdec1d3c26e5d784c28","last_reissued_at":"2026-07-05T00:32:39.181329Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:32:39.181329Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Warped Symmetries of the Kerr Black Hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Alejandra Castro, Ankit Aggarwal, St\\'ephane Detournay","submitted_at":"2019-09-06T22:09:16Z","abstract_excerpt":"We propose a set of diffeomorphism that act non-trivially near the horizon of the Kerr black hole. We follow the recent developments of Haco-Hawking-Perry-Strominger to quantify this phase space, with the most substantial difference being our choice of vectors fields. Our gravitational charges are organized into a Virasoro-Kac-Moody algebra with non-trivial central extensions. We interpret this algebra as arising from a warped conformal field theory. Using the data we can infer from this warped CFT description, we capture the thermodynamic properties of the Kerr black hole."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1909.03137","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/1909.03137/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":"1909.03137","created_at":"2026-07-05T00:32:39.181386+00:00"},{"alias_kind":"arxiv_version","alias_value":"1909.03137v2","created_at":"2026-07-05T00:32:39.181386+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1909.03137","created_at":"2026-07-05T00:32:39.181386+00:00"},{"alias_kind":"pith_short_12","alias_value":"XGEOWCBOR7VI","created_at":"2026-07-05T00:32:39.181386+00:00"},{"alias_kind":"pith_short_16","alias_value":"XGEOWCBOR7VISCK3","created_at":"2026-07-05T00:32:39.181386+00:00"},{"alias_kind":"pith_short_8","alias_value":"XGEOWCBO","created_at":"2026-07-05T00:32:39.181386+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2508.05322","citing_title":"Explorations of Universality in the Entropy and Hawking Radiation of Non-Extremal Kerr AdS$_4$ Black Holes","ref_index":42,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XGEOWCBOR7VISCK3SA7LVKVRN4","json":"https://pith.science/pith/XGEOWCBOR7VISCK3SA7LVKVRN4.json","graph_json":"https://pith.science/api/pith-number/XGEOWCBOR7VISCK3SA7LVKVRN4/graph.json","events_json":"https://pith.science/api/pith-number/XGEOWCBOR7VISCK3SA7LVKVRN4/events.json","paper":"https://pith.science/paper/XGEOWCBO"},"agent_actions":{"view_html":"https://pith.science/pith/XGEOWCBOR7VISCK3SA7LVKVRN4","download_json":"https://pith.science/pith/XGEOWCBOR7VISCK3SA7LVKVRN4.json","view_paper":"https://pith.science/paper/XGEOWCBO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1909.03137&json=true","fetch_graph":"https://pith.science/api/pith-number/XGEOWCBOR7VISCK3SA7LVKVRN4/graph.json","fetch_events":"https://pith.science/api/pith-number/XGEOWCBOR7VISCK3SA7LVKVRN4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XGEOWCBOR7VISCK3SA7LVKVRN4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XGEOWCBOR7VISCK3SA7LVKVRN4/action/storage_attestation","attest_author":"https://pith.science/pith/XGEOWCBOR7VISCK3SA7LVKVRN4/action/author_attestation","sign_citation":"https://pith.science/pith/XGEOWCBOR7VISCK3SA7LVKVRN4/action/citation_signature","submit_replication":"https://pith.science/pith/XGEOWCBOR7VISCK3SA7LVKVRN4/action/replication_record"}},"created_at":"2026-07-05T00:32:39.181386+00:00","updated_at":"2026-07-05T00:32:39.181386+00:00"}