{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:5KROUKJICLVHAODLDXO4A6AXLH","short_pith_number":"pith:5KROUKJI","schema_version":"1.0","canonical_sha256":"eaa2ea292812ea70386b1dddc0781759f10e68151163be9964346a613ceb3fd3","source":{"kind":"arxiv","id":"2006.06872","version":1},"attestation_state":"computed","paper":{"title":"The entropy of Hawking radiation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Ahmed Almheiri, Amirhossein Tajdini, Edgar Shaghoulian, Juan Maldacena, Thomas Hartman","submitted_at":"2020-06-11T23:23:14Z","abstract_excerpt":"In this review, we describe recent progress on the black hole information problem that involves a new understanding of how to calculate the entropy of Hawking radiation. We show how the method for computing gravitational fine-grained entropy, developed over the past 15 years, can be extended to capture the entropy of Hawking radiation. This technique reveals large corrections needed for the entropy to be consistent with unitary black hole evaporation."},"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":"2006.06872","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2020-06-11T23:23:14Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"4a88ff4e6390c1e5a1265a220f29d43317ead33d89af05e8a21ef82ee42cc74d","abstract_canon_sha256":"fcaea2f5f886a30d2e2e49f83b82bd95880389a35a626e6901822e72fbb3be76"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:01:09.124565Z","signature_b64":"nUERn87vC7n4DMrDYBKMkl0M6CWRUoe1OTLsczSt5cf2GEteqhh2DBBNSIM2rH1V47rb9oO/vAISNXf6iuWDBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"eaa2ea292812ea70386b1dddc0781759f10e68151163be9964346a613ceb3fd3","last_reissued_at":"2026-07-05T03:01:09.124094Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:01:09.124094Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The entropy of Hawking radiation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Ahmed Almheiri, Amirhossein Tajdini, Edgar Shaghoulian, Juan Maldacena, Thomas Hartman","submitted_at":"2020-06-11T23:23:14Z","abstract_excerpt":"In this review, we describe recent progress on the black hole information problem that involves a new understanding of how to calculate the entropy of Hawking radiation. We show how the method for computing gravitational fine-grained entropy, developed over the past 15 years, can be extended to capture the entropy of Hawking radiation. This technique reveals large corrections needed for the entropy to be consistent with unitary black hole evaporation."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2006.06872","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/2006.06872/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":"2006.06872","created_at":"2026-07-05T03:01:09.124155+00:00"},{"alias_kind":"arxiv_version","alias_value":"2006.06872v1","created_at":"2026-07-05T03:01:09.124155+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2006.06872","created_at":"2026-07-05T03:01:09.124155+00:00"},{"alias_kind":"pith_short_12","alias_value":"5KROUKJICLVH","created_at":"2026-07-05T03:01:09.124155+00:00"},{"alias_kind":"pith_short_16","alias_value":"5KROUKJICLVHAODL","created_at":"2026-07-05T03:01:09.124155+00:00"},{"alias_kind":"pith_short_8","alias_value":"5KROUKJI","created_at":"2026-07-05T03:01:09.124155+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":24,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.08661","citing_title":"The Remnant of an Evaporating Rotating Regular Black Hole from the Generalized Entropy in the Final Stage of Evaporation","ref_index":37,"is_internal_anchor":true},{"citing_arxiv_id":"2606.26357","citing_title":"Deformed BTZ Radiance and Single Trace $T\\bar{T}$ Holography","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2606.19435","citing_title":"Deriving effective descriptions and signal predictions for dynamical gravitational systems","ref_index":9,"is_internal_anchor":false},{"citing_arxiv_id":"2606.09346","citing_title":"Asymptotic Algebras and Holography of Information in CGHS Model","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2606.04575","citing_title":"Emergent Closed Universes in Symmetric Orbifold CFTs","ref_index":1,"is_internal_anchor":false},{"citing_arxiv_id":"2606.03049","citing_title":"Holographic complexity of de-Sitter black holes","ref_index":24,"is_internal_anchor":false},{"citing_arxiv_id":"2606.30466","citing_title":"Holography and Kinematic Space for Gravitational Sub-regions in AdS","ref_index":72,"is_internal_anchor":false},{"citing_arxiv_id":"2606.00488","citing_title":"Massless Islands in Wedge Holography","ref_index":4,"is_internal_anchor":false},{"citing_arxiv_id":"2411.01105","citing_title":"UV Effects and Short-Lived Hawking Radiation: Alternative Resolution of Information Paradox","ref_index":85,"is_internal_anchor":false},{"citing_arxiv_id":"2505.03068","citing_title":"M\\\"obius randomness in the Hartle-Hawking state","ref_index":4,"is_internal_anchor":false},{"citing_arxiv_id":"2605.20349","citing_title":"The fate of Reissner--Nordstr\\\"om--de Sitter black holes: nonequilibrium discharge and evaporation","ref_index":35,"is_internal_anchor":false},{"citing_arxiv_id":"2206.10780","citing_title":"An Algebra of Observables for de Sitter Space","ref_index":5,"is_internal_anchor":false},{"citing_arxiv_id":"2601.20954","citing_title":"Spectral Form Factor of Gapped Random Matrix Systems","ref_index":27,"is_internal_anchor":false},{"citing_arxiv_id":"2602.15120","citing_title":"How to have your wormholes and factorize, too","ref_index":12,"is_internal_anchor":false},{"citing_arxiv_id":"2509.08099","citing_title":"Black Hole Spectroscopy and Tests of General Relativity with GW250114","ref_index":28,"is_internal_anchor":false},{"citing_arxiv_id":"2603.12524","citing_title":"Thermodynamics and information recovery of Schwarzschild AdS black holes in conformal Killing gravity","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08347","citing_title":"Entanglement islands, fuzzballs and stretched horizons","ref_index":16,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08335","citing_title":"Inner Horizon Saddles and a Spectral KSW Criterion","ref_index":71,"is_internal_anchor":false},{"citing_arxiv_id":"2605.04210","citing_title":"Nonlocal Nonstabilizerness from Holographic Schwinger Pair Production","ref_index":92,"is_internal_anchor":false},{"citing_arxiv_id":"2604.20165","citing_title":"Entropy bound and the non-universality of entanglement islands","ref_index":6,"is_internal_anchor":false},{"citing_arxiv_id":"2604.12980","citing_title":"State counting in gravity and maximal entropy principle","ref_index":15,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06858","citing_title":"Memory-Burden Suppression of Hawking Radiation and Neutrino Constraints on Primordial Black Holes","ref_index":77,"is_internal_anchor":false},{"citing_arxiv_id":"2604.05815","citing_title":"Probing the Factorized Island Branch with the Capacity of Entanglement in JT Gravity","ref_index":10,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14824","citing_title":"Decrease of the entanglement entropy of the Hawking radiation induced by backreaction in the Bose-Einstein condensate","ref_index":2,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5KROUKJICLVHAODLDXO4A6AXLH","json":"https://pith.science/pith/5KROUKJICLVHAODLDXO4A6AXLH.json","graph_json":"https://pith.science/api/pith-number/5KROUKJICLVHAODLDXO4A6AXLH/graph.json","events_json":"https://pith.science/api/pith-number/5KROUKJICLVHAODLDXO4A6AXLH/events.json","paper":"https://pith.science/paper/5KROUKJI"},"agent_actions":{"view_html":"https://pith.science/pith/5KROUKJICLVHAODLDXO4A6AXLH","download_json":"https://pith.science/pith/5KROUKJICLVHAODLDXO4A6AXLH.json","view_paper":"https://pith.science/paper/5KROUKJI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2006.06872&json=true","fetch_graph":"https://pith.science/api/pith-number/5KROUKJICLVHAODLDXO4A6AXLH/graph.json","fetch_events":"https://pith.science/api/pith-number/5KROUKJICLVHAODLDXO4A6AXLH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5KROUKJICLVHAODLDXO4A6AXLH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5KROUKJICLVHAODLDXO4A6AXLH/action/storage_attestation","attest_author":"https://pith.science/pith/5KROUKJICLVHAODLDXO4A6AXLH/action/author_attestation","sign_citation":"https://pith.science/pith/5KROUKJICLVHAODLDXO4A6AXLH/action/citation_signature","submit_replication":"https://pith.science/pith/5KROUKJICLVHAODLDXO4A6AXLH/action/replication_record"}},"created_at":"2026-07-05T03:01:09.124155+00:00","updated_at":"2026-07-05T03:01:09.124155+00:00"}