{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:MQDUL4GK6FKMXHF5D7CRMFOQYB","short_pith_number":"pith:MQDUL4GK","schema_version":"1.0","canonical_sha256":"640745f0caf154cb9cbd1fc51615d0c0652a6b35b9ad852501d6770d9614371d","source":{"kind":"arxiv","id":"1211.7070","version":3},"attestation_state":"computed","paper":{"title":"Nonviolent nonlocality","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Steven B. Giddings","submitted_at":"2012-11-29T21:00:07Z","abstract_excerpt":"If quantum mechanics governs nature, black holes must evolve unitarily, providing a powerful constraint on the dynamics of quantum gravity. Such evolution apparently must in particular be nonlocal, when described from the usual semiclassical geometric picture, in order to transfer quantum information into the outgoing state. While such transfer from a disintegrating black hole has the dangerous potential to be violent to generic infalling observers, this paper proposes the existence of a more innocuous form of information transfer, to relatively soft modes in the black hole atmosphere. Simplif"},"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":"1211.7070","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2012-11-29T21:00:07Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"c8ad9c91969ebf7128bdaa491bb3704fb52af0858c266982da0f21294c5ad4c2","abstract_canon_sha256":"6d6ff482e8336ccff102e522578a652e24bd315a043cf6e02e00704403234d39"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:13:10.585409Z","signature_b64":"Fe2lbloKLxHQ/3Va+dMQQAWCT57+Dbn/1OJ67IRR98cDSTtSpiD3z99C7LVf7W2jACg80ppUJ5kY/L1x7+/oDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"640745f0caf154cb9cbd1fc51615d0c0652a6b35b9ad852501d6770d9614371d","last_reissued_at":"2026-05-18T03:13:10.584825Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:13:10.584825Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Nonviolent nonlocality","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Steven B. Giddings","submitted_at":"2012-11-29T21:00:07Z","abstract_excerpt":"If quantum mechanics governs nature, black holes must evolve unitarily, providing a powerful constraint on the dynamics of quantum gravity. Such evolution apparently must in particular be nonlocal, when described from the usual semiclassical geometric picture, in order to transfer quantum information into the outgoing state. While such transfer from a disintegrating black hole has the dangerous potential to be violent to generic infalling observers, this paper proposes the existence of a more innocuous form of information transfer, to relatively soft modes in the black hole atmosphere. Simplif"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1211.7070","kind":"arxiv","version":3},"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":"1211.7070","created_at":"2026-05-18T03:13:10.584893+00:00"},{"alias_kind":"arxiv_version","alias_value":"1211.7070v3","created_at":"2026-05-18T03:13:10.584893+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1211.7070","created_at":"2026-05-18T03:13:10.584893+00:00"},{"alias_kind":"pith_short_12","alias_value":"MQDUL4GK6FKM","created_at":"2026-05-18T12:27:14.488303+00:00"},{"alias_kind":"pith_short_16","alias_value":"MQDUL4GK6FKMXHF5","created_at":"2026-05-18T12:27:14.488303+00:00"},{"alias_kind":"pith_short_8","alias_value":"MQDUL4GK","created_at":"2026-05-18T12:27:14.488303+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.01105","citing_title":"UV Effects and Short-Lived Hawking Radiation: Alternative Resolution of Information Paradox","ref_index":94,"is_internal_anchor":true},{"citing_arxiv_id":"2605.02792","citing_title":"Albertian Channel Memory in Black-Hole Evaporation","ref_index":34,"is_internal_anchor":false},{"citing_arxiv_id":"2605.02792","citing_title":"Albertian Channel Memory in Black-Hole Evaporation","ref_index":34,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MQDUL4GK6FKMXHF5D7CRMFOQYB","json":"https://pith.science/pith/MQDUL4GK6FKMXHF5D7CRMFOQYB.json","graph_json":"https://pith.science/api/pith-number/MQDUL4GK6FKMXHF5D7CRMFOQYB/graph.json","events_json":"https://pith.science/api/pith-number/MQDUL4GK6FKMXHF5D7CRMFOQYB/events.json","paper":"https://pith.science/paper/MQDUL4GK"},"agent_actions":{"view_html":"https://pith.science/pith/MQDUL4GK6FKMXHF5D7CRMFOQYB","download_json":"https://pith.science/pith/MQDUL4GK6FKMXHF5D7CRMFOQYB.json","view_paper":"https://pith.science/paper/MQDUL4GK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1211.7070&json=true","fetch_graph":"https://pith.science/api/pith-number/MQDUL4GK6FKMXHF5D7CRMFOQYB/graph.json","fetch_events":"https://pith.science/api/pith-number/MQDUL4GK6FKMXHF5D7CRMFOQYB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MQDUL4GK6FKMXHF5D7CRMFOQYB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MQDUL4GK6FKMXHF5D7CRMFOQYB/action/storage_attestation","attest_author":"https://pith.science/pith/MQDUL4GK6FKMXHF5D7CRMFOQYB/action/author_attestation","sign_citation":"https://pith.science/pith/MQDUL4GK6FKMXHF5D7CRMFOQYB/action/citation_signature","submit_replication":"https://pith.science/pith/MQDUL4GK6FKMXHF5D7CRMFOQYB/action/replication_record"}},"created_at":"2026-05-18T03:13:10.584893+00:00","updated_at":"2026-05-18T03:13:10.584893+00:00"}