{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:3NFZ2KT33WWTD3IB5KJ5GF4OFI","short_pith_number":"pith:3NFZ2KT3","schema_version":"1.0","canonical_sha256":"db4b9d2a7bddad31ed01ea93d3178e2a39e79634b2522811ef414825f3ff98d9","source":{"kind":"arxiv","id":"1703.02140","version":1},"attestation_state":"computed","paper":{"title":"Information Loss","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Robert M. Wald, William G. Unruh","submitted_at":"2017-03-06T22:48:32Z","abstract_excerpt":"The complete gravitational collapse of a body in general relativity will result in the formation of a black hole. Although the black hole is classically stable, quantum particle creation processes will result in the emission of Hawking radiation to infinity and corresponding mass loss of the black hole, eventually resulting in the complete evaporation of the black hole. Semiclassical arguments strongly suggest that, in the process of black hole formation and evaporation, a pure quantum state will evolve to a mixed state, i.e., there will be \"information loss.\" There has been considerable contr"},"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":"1703.02140","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2017-03-06T22:48:32Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"f09328335d9ef59635b6a62c0429174a03cdb5dcf7768647d4db4697685fd8af","abstract_canon_sha256":"b0891fec35f41c14257d9dc1adfd81ff17e91389ee41be8d0639180a4311e42c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:38:56.983012Z","signature_b64":"t1WNYttf894Uq/CF81SPo4yhn+blDRZSbdbF0tJLGIucyVCUN4Ec7f2tVPVds92AjXHwdKwlfm0vQuvC9k1DAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"db4b9d2a7bddad31ed01ea93d3178e2a39e79634b2522811ef414825f3ff98d9","last_reissued_at":"2026-05-18T00:38:56.982343Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:38:56.982343Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Information Loss","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Robert M. Wald, William G. Unruh","submitted_at":"2017-03-06T22:48:32Z","abstract_excerpt":"The complete gravitational collapse of a body in general relativity will result in the formation of a black hole. Although the black hole is classically stable, quantum particle creation processes will result in the emission of Hawking radiation to infinity and corresponding mass loss of the black hole, eventually resulting in the complete evaporation of the black hole. Semiclassical arguments strongly suggest that, in the process of black hole formation and evaporation, a pure quantum state will evolve to a mixed state, i.e., there will be \"information loss.\" There has been considerable contr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.02140","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":""},"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":"1703.02140","created_at":"2026-05-18T00:38:56.982423+00:00"},{"alias_kind":"arxiv_version","alias_value":"1703.02140v1","created_at":"2026-05-18T00:38:56.982423+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.02140","created_at":"2026-05-18T00:38:56.982423+00:00"},{"alias_kind":"pith_short_12","alias_value":"3NFZ2KT33WWT","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_16","alias_value":"3NFZ2KT33WWTD3IB","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_8","alias_value":"3NFZ2KT3","created_at":"2026-05-18T12:30:58.224056+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2504.12521","citing_title":"Lectures on the Bondi--Metzner--Sachs group and related topics in infrared physics","ref_index":228,"is_internal_anchor":true},{"citing_arxiv_id":"2506.14875","citing_title":"Regular Vaidya solutions of effective gravitational theories","ref_index":11,"is_internal_anchor":true},{"citing_arxiv_id":"1904.05363","citing_title":"Testing the nature of dark compact objects: a status report","ref_index":35,"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":74,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3NFZ2KT33WWTD3IB5KJ5GF4OFI","json":"https://pith.science/pith/3NFZ2KT33WWTD3IB5KJ5GF4OFI.json","graph_json":"https://pith.science/api/pith-number/3NFZ2KT33WWTD3IB5KJ5GF4OFI/graph.json","events_json":"https://pith.science/api/pith-number/3NFZ2KT33WWTD3IB5KJ5GF4OFI/events.json","paper":"https://pith.science/paper/3NFZ2KT3"},"agent_actions":{"view_html":"https://pith.science/pith/3NFZ2KT33WWTD3IB5KJ5GF4OFI","download_json":"https://pith.science/pith/3NFZ2KT33WWTD3IB5KJ5GF4OFI.json","view_paper":"https://pith.science/paper/3NFZ2KT3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1703.02140&json=true","fetch_graph":"https://pith.science/api/pith-number/3NFZ2KT33WWTD3IB5KJ5GF4OFI/graph.json","fetch_events":"https://pith.science/api/pith-number/3NFZ2KT33WWTD3IB5KJ5GF4OFI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3NFZ2KT33WWTD3IB5KJ5GF4OFI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3NFZ2KT33WWTD3IB5KJ5GF4OFI/action/storage_attestation","attest_author":"https://pith.science/pith/3NFZ2KT33WWTD3IB5KJ5GF4OFI/action/author_attestation","sign_citation":"https://pith.science/pith/3NFZ2KT33WWTD3IB5KJ5GF4OFI/action/citation_signature","submit_replication":"https://pith.science/pith/3NFZ2KT33WWTD3IB5KJ5GF4OFI/action/replication_record"}},"created_at":"2026-05-18T00:38:56.982423+00:00","updated_at":"2026-05-18T00:38:56.982423+00:00"}