{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:CEM3EFUC6PQUX24K5VYQYOJOFB","short_pith_number":"pith:CEM3EFUC","schema_version":"1.0","canonical_sha256":"1119b21682f3e14beb8aed710c392e286362274e95e122c5e018d6333095cd45","source":{"kind":"arxiv","id":"hep-th/0605196","version":2},"attestation_state":"computed","paper":{"title":"Black hole information, unitarity, and nonlocality","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Steven B. Giddings","submitted_at":"2006-05-19T19:12:21Z","abstract_excerpt":"The black hole information paradox apparently indicates the need for a fundamentally new ingredient in physics. The leading contender is nonlocality. Possible mechanisms for the nonlocality needed to restore unitarity to black hole evolution are investigated. Suggestions that such dynamics arises from ultra-planckian modes in Hawking's derivation are investigated and found not to be relevant, in a picture using smooth slices spanning the exterior and interior of the horizon. However, no simultaneous description of modes that have fallen into the black hole and outgoing Hawking modes can be giv"},"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":"hep-th/0605196","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2006-05-19T19:12:21Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"0182d7293098a0e62b3e46d898b5221027629607072500a3ebf2aa01cae8fb81","abstract_canon_sha256":"ca06dc8dd5c34ea6ee84ede2b4599f8f5d2628b429ad7e143170a93fdb50e6e0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:19:28.777117Z","signature_b64":"eO1ZFieAlcQ3vNkC1D1QmNJTqnHo3V5bEfks78F1dpcpfIBQ080KvZGOgJN2Lh00g6LfR9WOHaKcH8jIRgxrDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1119b21682f3e14beb8aed710c392e286362274e95e122c5e018d6333095cd45","last_reissued_at":"2026-07-04T15:19:28.776757Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:19:28.776757Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Black hole information, unitarity, and nonlocality","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Steven B. Giddings","submitted_at":"2006-05-19T19:12:21Z","abstract_excerpt":"The black hole information paradox apparently indicates the need for a fundamentally new ingredient in physics. The leading contender is nonlocality. Possible mechanisms for the nonlocality needed to restore unitarity to black hole evolution are investigated. Suggestions that such dynamics arises from ultra-planckian modes in Hawking's derivation are investigated and found not to be relevant, in a picture using smooth slices spanning the exterior and interior of the horizon. However, no simultaneous description of modes that have fallen into the black hole and outgoing Hawking modes can be giv"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0605196","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/hep-th/0605196/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":"hep-th/0605196","created_at":"2026-07-04T15:19:28.776830+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0605196v2","created_at":"2026-07-04T15:19:28.776830+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0605196","created_at":"2026-07-04T15:19:28.776830+00:00"},{"alias_kind":"pith_short_12","alias_value":"CEM3EFUC6PQU","created_at":"2026-07-04T15:19:28.776830+00:00"},{"alias_kind":"pith_short_16","alias_value":"CEM3EFUC6PQUX24K","created_at":"2026-07-04T15:19:28.776830+00:00"},{"alias_kind":"pith_short_8","alias_value":"CEM3EFUC","created_at":"2026-07-04T15:19:28.776830+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.20314","citing_title":"Macroscopic Black-Hole Remnants in a Nonlocal Field Theory: Towards Hawking Radiation in SFT","ref_index":159,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CEM3EFUC6PQUX24K5VYQYOJOFB","json":"https://pith.science/pith/CEM3EFUC6PQUX24K5VYQYOJOFB.json","graph_json":"https://pith.science/api/pith-number/CEM3EFUC6PQUX24K5VYQYOJOFB/graph.json","events_json":"https://pith.science/api/pith-number/CEM3EFUC6PQUX24K5VYQYOJOFB/events.json","paper":"https://pith.science/paper/CEM3EFUC"},"agent_actions":{"view_html":"https://pith.science/pith/CEM3EFUC6PQUX24K5VYQYOJOFB","download_json":"https://pith.science/pith/CEM3EFUC6PQUX24K5VYQYOJOFB.json","view_paper":"https://pith.science/paper/CEM3EFUC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/0605196&json=true","fetch_graph":"https://pith.science/api/pith-number/CEM3EFUC6PQUX24K5VYQYOJOFB/graph.json","fetch_events":"https://pith.science/api/pith-number/CEM3EFUC6PQUX24K5VYQYOJOFB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CEM3EFUC6PQUX24K5VYQYOJOFB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CEM3EFUC6PQUX24K5VYQYOJOFB/action/storage_attestation","attest_author":"https://pith.science/pith/CEM3EFUC6PQUX24K5VYQYOJOFB/action/author_attestation","sign_citation":"https://pith.science/pith/CEM3EFUC6PQUX24K5VYQYOJOFB/action/citation_signature","submit_replication":"https://pith.science/pith/CEM3EFUC6PQUX24K5VYQYOJOFB/action/replication_record"}},"created_at":"2026-07-04T15:19:28.776830+00:00","updated_at":"2026-07-04T15:19:28.776830+00:00"}