{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:TRRYKC24YNLWZZQ354YB2PXUSS","short_pith_number":"pith:TRRYKC24","schema_version":"1.0","canonical_sha256":"9c63850b5cc3576ce61bef301d3ef494948d5700e1b6ffed54c9bb6f3fcc6196","source":{"kind":"arxiv","id":"2201.03096","version":2},"attestation_state":"computed","paper":{"title":"Snowmass White Paper: Quantum Aspects of Black Holes and the Emergence of Spacetime","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.str-el","gr-qc","quant-ph"],"primary_cat":"hep-th","authors_text":"Douglas Stanford, Netta Engelhardt, Raphael Bousso, Stephen H. Shenker, Thomas Faulkner, Thomas Hartman, Xi Dong","submitted_at":"2022-01-09T22:01:30Z","abstract_excerpt":"Black holes provide a window into the microscopic structure of spacetime in quantum gravity. Recently the quantum information contained in Hawking radiation has been calculated, verifying a key aspect of the consistency of black hole evaporation with quantum mechanical unitarity.\n  This calculation relied crucially on recent progress in understanding the emergence of bulk spacetime from a boundary holographic description. Spacetime wormholes have played an important role in understanding the underpinnings of this result, and the precision study of such wormholes, in this and other contexts, ha"},"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":"2201.03096","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2022-01-09T22:01:30Z","cross_cats_sorted":["cond-mat.str-el","gr-qc","quant-ph"],"title_canon_sha256":"a20802017f30ccf0d061086f9e5c52f20c727c7576ca04d21c1759a7d90079ed","abstract_canon_sha256":"7064abcc862992427324bc6849d171f10c5b3d214d1e080683219cc0646b2283"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:01:45.824499Z","signature_b64":"tBTAxZdPhQePnPbL9fHfDNXH1u6pWKfll54P9n3tIS0HCY1bxCLXRsjd+rgKIlZyPcFCTmrACfVWV4+W9QVcAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9c63850b5cc3576ce61bef301d3ef494948d5700e1b6ffed54c9bb6f3fcc6196","last_reissued_at":"2026-07-05T04:01:45.824068Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:01:45.824068Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Snowmass White Paper: Quantum Aspects of Black Holes and the Emergence of Spacetime","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.str-el","gr-qc","quant-ph"],"primary_cat":"hep-th","authors_text":"Douglas Stanford, Netta Engelhardt, Raphael Bousso, Stephen H. Shenker, Thomas Faulkner, Thomas Hartman, Xi Dong","submitted_at":"2022-01-09T22:01:30Z","abstract_excerpt":"Black holes provide a window into the microscopic structure of spacetime in quantum gravity. Recently the quantum information contained in Hawking radiation has been calculated, verifying a key aspect of the consistency of black hole evaporation with quantum mechanical unitarity.\n  This calculation relied crucially on recent progress in understanding the emergence of bulk spacetime from a boundary holographic description. Spacetime wormholes have played an important role in understanding the underpinnings of this result, and the precision study of such wormholes, in this and other contexts, ha"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2201.03096","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/2201.03096/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":"2201.03096","created_at":"2026-07-05T04:01:45.824126+00:00"},{"alias_kind":"arxiv_version","alias_value":"2201.03096v2","created_at":"2026-07-05T04:01:45.824126+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2201.03096","created_at":"2026-07-05T04:01:45.824126+00:00"},{"alias_kind":"pith_short_12","alias_value":"TRRYKC24YNLW","created_at":"2026-07-05T04:01:45.824126+00:00"},{"alias_kind":"pith_short_16","alias_value":"TRRYKC24YNLWZZQ3","created_at":"2026-07-05T04:01:45.824126+00:00"},{"alias_kind":"pith_short_8","alias_value":"TRRYKC24","created_at":"2026-07-05T04:01:45.824126+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.10924","citing_title":"Spacetime from Operator Algebras","ref_index":6,"is_internal_anchor":false},{"citing_arxiv_id":"2606.02207","citing_title":"Information scrambling in all-to-all interacting models","ref_index":62,"is_internal_anchor":false},{"citing_arxiv_id":"2412.02560","citing_title":"Selective Thermalization, Chiral Excitations, and a Case of Quantum Hair in the Presence of Event Horizons","ref_index":10,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TRRYKC24YNLWZZQ354YB2PXUSS","json":"https://pith.science/pith/TRRYKC24YNLWZZQ354YB2PXUSS.json","graph_json":"https://pith.science/api/pith-number/TRRYKC24YNLWZZQ354YB2PXUSS/graph.json","events_json":"https://pith.science/api/pith-number/TRRYKC24YNLWZZQ354YB2PXUSS/events.json","paper":"https://pith.science/paper/TRRYKC24"},"agent_actions":{"view_html":"https://pith.science/pith/TRRYKC24YNLWZZQ354YB2PXUSS","download_json":"https://pith.science/pith/TRRYKC24YNLWZZQ354YB2PXUSS.json","view_paper":"https://pith.science/paper/TRRYKC24","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2201.03096&json=true","fetch_graph":"https://pith.science/api/pith-number/TRRYKC24YNLWZZQ354YB2PXUSS/graph.json","fetch_events":"https://pith.science/api/pith-number/TRRYKC24YNLWZZQ354YB2PXUSS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TRRYKC24YNLWZZQ354YB2PXUSS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TRRYKC24YNLWZZQ354YB2PXUSS/action/storage_attestation","attest_author":"https://pith.science/pith/TRRYKC24YNLWZZQ354YB2PXUSS/action/author_attestation","sign_citation":"https://pith.science/pith/TRRYKC24YNLWZZQ354YB2PXUSS/action/citation_signature","submit_replication":"https://pith.science/pith/TRRYKC24YNLWZZQ354YB2PXUSS/action/replication_record"}},"created_at":"2026-07-05T04:01:45.824126+00:00","updated_at":"2026-07-05T04:01:45.824126+00:00"}