{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:KUNT2B7RT4AK5XV73WYY5XDUBA","short_pith_number":"pith:KUNT2B7R","schema_version":"1.0","canonical_sha256":"551b3d07f19f00aedebfddb18edc740813dc5a879f4f2952d944fb0856f160cb","source":{"kind":"arxiv","id":"2404.15183","version":1},"attestation_state":"computed","paper":{"title":"Statistics of three-dimensional black holes from Liouville line defects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Jeevan Chandra, Thomas Hartman, Viraj Meruliya","submitted_at":"2024-04-23T16:26:38Z","abstract_excerpt":"Black holes and wormholes in the gravitational path integral can be used to calculate the statistics of heavy operators. An explicit example in higher dimensions is provided by thin shells of matter. We study these solutions in 3D gravity, and reproduce the behavior of black holes and wormholes from the dual CFT using the large-$c$ conformal bootstrap. The CFT operator that creates a thin shell black hole is a line defect, so we begin by using the bootstrap to study the statistics of line defects, both at finite $c$ and in the holographic large-$c$ limit. The crossing equation leads to a unive"},"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":"2404.15183","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2024-04-23T16:26:38Z","cross_cats_sorted":[],"title_canon_sha256":"220e9ff33a4819bb3a2709fcc90843063f464975b08b7337fd11dc16ca04ec14","abstract_canon_sha256":"b3fb9775d1b9391783a775101dea2cc5dd0138b3dec574f99c129f6bc618c6f8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:11:16.501500Z","signature_b64":"krWaQMXqOkMJzny8+flKin559UAg1Kw1wzrGxte7lqE9razJFkm7owPavwlO3Vp83KJtmSMZrdsf3vA1auT/AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"551b3d07f19f00aedebfddb18edc740813dc5a879f4f2952d944fb0856f160cb","last_reissued_at":"2026-07-05T08:11:16.501041Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:11:16.501041Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Statistics of three-dimensional black holes from Liouville line defects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Jeevan Chandra, Thomas Hartman, Viraj Meruliya","submitted_at":"2024-04-23T16:26:38Z","abstract_excerpt":"Black holes and wormholes in the gravitational path integral can be used to calculate the statistics of heavy operators. An explicit example in higher dimensions is provided by thin shells of matter. We study these solutions in 3D gravity, and reproduce the behavior of black holes and wormholes from the dual CFT using the large-$c$ conformal bootstrap. The CFT operator that creates a thin shell black hole is a line defect, so we begin by using the bootstrap to study the statistics of line defects, both at finite $c$ and in the holographic large-$c$ limit. The crossing equation leads to a unive"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2404.15183","kind":"arxiv","version":1},"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/2404.15183/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":"2404.15183","created_at":"2026-07-05T08:11:16.501096+00:00"},{"alias_kind":"arxiv_version","alias_value":"2404.15183v1","created_at":"2026-07-05T08:11:16.501096+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2404.15183","created_at":"2026-07-05T08:11:16.501096+00:00"},{"alias_kind":"pith_short_12","alias_value":"KUNT2B7RT4AK","created_at":"2026-07-05T08:11:16.501096+00:00"},{"alias_kind":"pith_short_16","alias_value":"KUNT2B7RT4AK5XV7","created_at":"2026-07-05T08:11:16.501096+00:00"},{"alias_kind":"pith_short_8","alias_value":"KUNT2B7R","created_at":"2026-07-05T08:11:16.501096+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2508.10864","citing_title":"Statistics in 3d gravity from knots and links","ref_index":21,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KUNT2B7RT4AK5XV73WYY5XDUBA","json":"https://pith.science/pith/KUNT2B7RT4AK5XV73WYY5XDUBA.json","graph_json":"https://pith.science/api/pith-number/KUNT2B7RT4AK5XV73WYY5XDUBA/graph.json","events_json":"https://pith.science/api/pith-number/KUNT2B7RT4AK5XV73WYY5XDUBA/events.json","paper":"https://pith.science/paper/KUNT2B7R"},"agent_actions":{"view_html":"https://pith.science/pith/KUNT2B7RT4AK5XV73WYY5XDUBA","download_json":"https://pith.science/pith/KUNT2B7RT4AK5XV73WYY5XDUBA.json","view_paper":"https://pith.science/paper/KUNT2B7R","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2404.15183&json=true","fetch_graph":"https://pith.science/api/pith-number/KUNT2B7RT4AK5XV73WYY5XDUBA/graph.json","fetch_events":"https://pith.science/api/pith-number/KUNT2B7RT4AK5XV73WYY5XDUBA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KUNT2B7RT4AK5XV73WYY5XDUBA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KUNT2B7RT4AK5XV73WYY5XDUBA/action/storage_attestation","attest_author":"https://pith.science/pith/KUNT2B7RT4AK5XV73WYY5XDUBA/action/author_attestation","sign_citation":"https://pith.science/pith/KUNT2B7RT4AK5XV73WYY5XDUBA/action/citation_signature","submit_replication":"https://pith.science/pith/KUNT2B7RT4AK5XV73WYY5XDUBA/action/replication_record"}},"created_at":"2026-07-05T08:11:16.501096+00:00","updated_at":"2026-07-05T08:11:16.501096+00:00"}