{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2026:2UVOCU4HVEETKUJRWHOUJZLKSI","short_pith_number":"pith:2UVOCU4H","canonical_record":{"source":{"id":"2605.13490","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2026-05-13T13:16:01Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"e2d9179e87cab3f7a7bd88ae90f67628d55fb9126911f89d92a503d1af03cf80","abstract_canon_sha256":"d2e1a53a61401639c3c4cfedab21574fb111aa17f5c15f9476220bdd8d26e138"},"schema_version":"1.0"},"canonical_sha256":"d52ae15387a909355131b1dd44e56a9201f2444fdb3e186ec24205ac0d722fe2","source":{"kind":"arxiv","id":"2605.13490","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2605.13490","created_at":"2026-05-18T02:44:41Z"},{"alias_kind":"arxiv_version","alias_value":"2605.13490v1","created_at":"2026-05-18T02:44:41Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.13490","created_at":"2026-05-18T02:44:41Z"},{"alias_kind":"pith_short_12","alias_value":"2UVOCU4HVEET","created_at":"2026-05-18T12:33:37Z"},{"alias_kind":"pith_short_16","alias_value":"2UVOCU4HVEETKUJR","created_at":"2026-05-18T12:33:37Z"},{"alias_kind":"pith_short_8","alias_value":"2UVOCU4H","created_at":"2026-05-18T12:33:37Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2026:2UVOCU4HVEETKUJRWHOUJZLKSI","target":"record","payload":{"canonical_record":{"source":{"id":"2605.13490","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2026-05-13T13:16:01Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"e2d9179e87cab3f7a7bd88ae90f67628d55fb9126911f89d92a503d1af03cf80","abstract_canon_sha256":"d2e1a53a61401639c3c4cfedab21574fb111aa17f5c15f9476220bdd8d26e138"},"schema_version":"1.0"},"canonical_sha256":"d52ae15387a909355131b1dd44e56a9201f2444fdb3e186ec24205ac0d722fe2","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:44:41.186582Z","signature_b64":"hMiJlTmnWi+ucrScxYH4oa1HfEqgJhT90rVjghhSXAuD873dkcjvQ/hTgDW5tzCuxN88QLNABu0gWuOyFQ42BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d52ae15387a909355131b1dd44e56a9201f2444fdb3e186ec24205ac0d722fe2","last_reissued_at":"2026-05-18T02:44:41.186019Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:44:41.186019Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"2605.13490","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:44:41Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"XxHmTTGfgww38aJ+Cv9b7v5Wz5vGOusBRsRKTNhkh3gy1QOZKYzvpwOClTeoQRDOL0C13RuE6SuXLtY0R6WcDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-22T03:10:09.722365Z"},"content_sha256":"638df88adcfc55c7c6f3e51e53195ccbe5bb89f5ef4ce2e9deb58fef5346d96a","schema_version":"1.0","event_id":"sha256:638df88adcfc55c7c6f3e51e53195ccbe5bb89f5ef4ce2e9deb58fef5346d96a"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2026:2UVOCU4HVEETKUJRWHOUJZLKSI","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"What does it mean to have a quantum gravitational theory of de Sitter Space?","license":"http://creativecommons.org/licenses/by/4.0/","headline":"If de Sitter space is a finite quantum system then all models of it are ambiguous","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Tom Banks","submitted_at":"2026-05-13T13:16:01Z","abstract_excerpt":"We argue that if de Sitter space is indeed represented by a finite dimensional quantum system, then semi-classical considerations, combined with the fundamental principles of quantum measurement theory, imply that any theoretical model of it is ambiguous. If our own universe asymptotes to such a de Sitter state, and if a model of it as a finite system can be embedded in a sequence of models that converges to a non-perturbative completion of a unique superstring model in asymptotically flat space, then one might be able to find a very precise mathematical model of our universe. However, even th"},"claims":{"count":4,"items":[{"kind":"strongest_claim","text":"if de Sitter space is indeed represented by a finite dimensional quantum system, then semi-classical considerations, combined with the fundamental principles of quantum measurement theory, imply that any theoretical model of it is ambiguous.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"That de Sitter space is represented by a finite dimensional quantum system and that our universe asymptotes to such a de Sitter state.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"De Sitter space modeled as a finite quantum system yields ambiguous theories, with local experiments accessing only a tiny fraction of its total information content.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"},{"kind":"headline","text":"If de Sitter space is a finite quantum system then all models of it are ambiguous","source":"verdict.pith_extraction.headline","status":"machine_extracted","claim_id":"C4","attestation":"unclaimed"}],"snapshot_sha256":"94fd7b1d73b180e269aa9d8e36a41008e62c19474d06eb0cb22c62502e4e8ed4"},"source":{"id":"2605.13490","kind":"arxiv","version":1},"verdict":{"id":"1036cdf2-2764-4a2f-b6fd-1d5e8359bb5c","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-14T18:26:02.106550Z","strongest_claim":"if de Sitter space is indeed represented by a finite dimensional quantum system, then semi-classical considerations, combined with the fundamental principles of quantum measurement theory, imply that any theoretical model of it is ambiguous.","one_line_summary":"De Sitter space modeled as a finite quantum system yields ambiguous theories, with local experiments accessing only a tiny fraction of its total information content.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"That de Sitter space is represented by a finite dimensional quantum system and that our universe asymptotes to such a de Sitter state.","pith_extraction_headline":"If de Sitter space is a finite quantum system then all models of it are ambiguous"},"references":{"count":11,"sample":[{"doi":"10.1142/s0217751x01003998","year":2001,"title":"Banks, Cosmological breaking of supersymmetry?, Int","work_id":"b5d04d74-9b44-4747-a677-63834a50177c","ref_index":2,"cited_arxiv_id":"hep-th/0007146","is_internal_anchor":true},{"doi":"10.1088/1126-6708/2006/12/004","year":2006,"title":"Towards a quantum theory of de Sitter space","work_id":"2986c943-d830-4e73-a8b5-37cd613f6043","ref_index":3,"cited_arxiv_id":"hep-th/0609062","is_internal_anchor":true},{"doi":"10.1103/physrevlett.82.4971","year":1999,"title":"Effective field theory, black holes, and the cosmo- logical constant","work_id":"73a006cd-07e4-4bd8-96be-030880cfe87c","ref_index":4,"cited_arxiv_id":"hep-th/9803132","is_internal_anchor":true},{"doi":"10.1088/1126-6708/2002/12/062","year":2002,"title":"Recurrent nightmares? Measurement theory in de Sitter space,","work_id":"e00b63f0-369f-4155-8b86-4aa9441e4aa2","ref_index":5,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"10.1007/jhep12(2025)085","year":2025,"title":"JT de Sitter gravity as a model of Coleman-de Luccia tunneling,","work_id":"6e9be668-3e3e-4354-bb33-62e9816e2950","ref_index":6,"cited_arxiv_id":"","is_internal_anchor":false}],"resolved_work":11,"snapshot_sha256":"5b02e63e1d5179b19a0471593bf4c5298cc24e62c7a57ae78966a6408ac96929","internal_anchors":5},"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"},"verdict_id":"1036cdf2-2764-4a2f-b6fd-1d5e8359bb5c"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:44:41Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"HEmfIK2uxM5vmQySiQrBqG1BECbI63NpeNpruTvBCFwChn0kGMmP+qtiUGx3aC5yspfj1w3gmiWui7vCQdNIDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-22T03:10:09.722930Z"},"content_sha256":"1e5eb3f767732ce2599f176b3f0b1e3cce2771fbea1250931ff3541c98ad67c6","schema_version":"1.0","event_id":"sha256:1e5eb3f767732ce2599f176b3f0b1e3cce2771fbea1250931ff3541c98ad67c6"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:2UVOCU4HVEETKUJRWHOUJZLKSI","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1201/9781482268737-37) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"T. Banks, W. Fischler, S. H. Shenker and L. Susskind, “M theory as a matrix model: A conjecture,” Phys. Rev. D55, 5112-5128 (1997) doi:10.1201/9781482268737- 37 [arXiv:hep-th/9610043 [hep-th]]","arxiv_id":"2605.13490","detector":"doi_compliance","evidence":{"ref_index":10,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"T. Banks, W. Fischler, S. H. Shenker and L. Susskind, “M theory as a matrix model: A conjecture,” Phys. Rev. D55, 5112-5128 (1997) doi:10.1201/9781482268737- 37 [arXiv:hep-th/9610043 [hep-th]]","reconstructed_doi":"10.1201/9781482268737-37"},"severity":"advisory","ref_index":10,"audited_at":"2026-05-19T06:30:37.999751Z","event_type":"pith.integrity.v1","detected_doi":"10.1201/9781482268737-37","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"0536cd94c78fe9882d9d82db7305cbb8d4603e484b48c806b0f5bdac6b235d4c","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":145,"payload_sha256":"bc4aa753c42787d7181b9ab81556c315c9205209391f9e4bce2d0ceeab81b4b0","signature_b64":"E2MZx5SL5jV0JDCxZcC28++q7BsBdFPfFHT8i785YGWMmmAMbEXB9t7yVxZv+bHvJAaWr+MK2P+TBsKZ5gOTCw==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-19T06:31:53Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"fAdHIR8ASAx621zsy7oN2oVqG6CuMx9i3udML3qdptrLjkOzTl+aDL3U760uMWMrhwBe5hg8k+sUm2/vA73HAA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-22T03:10:09.724259Z"},"content_sha256":"81ce98748ad5a189b5e5236c0da82c5b87c8d204ae9e97e5581dcef7dc75c131","schema_version":"1.0","event_id":"sha256:81ce98748ad5a189b5e5236c0da82c5b87c8d204ae9e97e5581dcef7dc75c131"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/2UVOCU4HVEETKUJRWHOUJZLKSI/bundle.json","state_url":"https://pith.science/pith/2UVOCU4HVEETKUJRWHOUJZLKSI/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/2UVOCU4HVEETKUJRWHOUJZLKSI/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-22T03:10:09Z","links":{"resolver":"https://pith.science/pith/2UVOCU4HVEETKUJRWHOUJZLKSI","bundle":"https://pith.science/pith/2UVOCU4HVEETKUJRWHOUJZLKSI/bundle.json","state":"https://pith.science/pith/2UVOCU4HVEETKUJRWHOUJZLKSI/state.json","well_known_bundle":"https://pith.science/.well-known/pith/2UVOCU4HVEETKUJRWHOUJZLKSI/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2026:2UVOCU4HVEETKUJRWHOUJZLKSI","merge_version":"pith-open-graph-merge-v1","event_count":3,"valid_event_count":3,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"d2e1a53a61401639c3c4cfedab21574fb111aa17f5c15f9476220bdd8d26e138","cross_cats_sorted":["gr-qc"],"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2026-05-13T13:16:01Z","title_canon_sha256":"e2d9179e87cab3f7a7bd88ae90f67628d55fb9126911f89d92a503d1af03cf80"},"schema_version":"1.0","source":{"id":"2605.13490","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2605.13490","created_at":"2026-05-18T02:44:41Z"},{"alias_kind":"arxiv_version","alias_value":"2605.13490v1","created_at":"2026-05-18T02:44:41Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.13490","created_at":"2026-05-18T02:44:41Z"},{"alias_kind":"pith_short_12","alias_value":"2UVOCU4HVEET","created_at":"2026-05-18T12:33:37Z"},{"alias_kind":"pith_short_16","alias_value":"2UVOCU4HVEETKUJR","created_at":"2026-05-18T12:33:37Z"},{"alias_kind":"pith_short_8","alias_value":"2UVOCU4H","created_at":"2026-05-18T12:33:37Z"}],"graph_snapshots":[{"event_id":"sha256:1e5eb3f767732ce2599f176b3f0b1e3cce2771fbea1250931ff3541c98ad67c6","target":"graph","created_at":"2026-05-18T02:44:41Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":4,"items":[{"attestation":"unclaimed","claim_id":"C1","kind":"strongest_claim","source":"verdict.strongest_claim","status":"machine_extracted","text":"if de Sitter space is indeed represented by a finite dimensional quantum system, then semi-classical considerations, combined with the fundamental principles of quantum measurement theory, imply that any theoretical model of it is ambiguous."},{"attestation":"unclaimed","claim_id":"C2","kind":"weakest_assumption","source":"verdict.weakest_assumption","status":"machine_extracted","text":"That de Sitter space is represented by a finite dimensional quantum system and that our universe asymptotes to such a de Sitter state."},{"attestation":"unclaimed","claim_id":"C3","kind":"one_line_summary","source":"verdict.one_line_summary","status":"machine_extracted","text":"De Sitter space modeled as a finite quantum system yields ambiguous theories, with local experiments accessing only a tiny fraction of its total information content."},{"attestation":"unclaimed","claim_id":"C4","kind":"headline","source":"verdict.pith_extraction.headline","status":"machine_extracted","text":"If de Sitter space is a finite quantum system then all models of it are ambiguous"}],"snapshot_sha256":"94fd7b1d73b180e269aa9d8e36a41008e62c19474d06eb0cb22c62502e4e8ed4"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We argue that if de Sitter space is indeed represented by a finite dimensional quantum system, then semi-classical considerations, combined with the fundamental principles of quantum measurement theory, imply that any theoretical model of it is ambiguous. If our own universe asymptotes to such a de Sitter state, and if a model of it as a finite system can be embedded in a sequence of models that converges to a non-perturbative completion of a unique superstring model in asymptotically flat space, then one might be able to find a very precise mathematical model of our universe. However, even th","authors_text":"Tom Banks","cross_cats":["gr-qc"],"headline":"If de Sitter space is a finite quantum system then all models of it are ambiguous","license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2026-05-13T13:16:01Z","title":"What does it mean to have a quantum gravitational theory of de Sitter Space?"},"references":{"count":11,"internal_anchors":5,"resolved_work":11,"sample":[{"cited_arxiv_id":"hep-th/0007146","doi":"10.1142/s0217751x01003998","is_internal_anchor":true,"ref_index":2,"title":"Banks, Cosmological breaking of supersymmetry?, Int","work_id":"b5d04d74-9b44-4747-a677-63834a50177c","year":2001},{"cited_arxiv_id":"hep-th/0609062","doi":"10.1088/1126-6708/2006/12/004","is_internal_anchor":true,"ref_index":3,"title":"Towards a quantum theory of de Sitter space","work_id":"2986c943-d830-4e73-a8b5-37cd613f6043","year":2006},{"cited_arxiv_id":"hep-th/9803132","doi":"10.1103/physrevlett.82.4971","is_internal_anchor":true,"ref_index":4,"title":"Effective field theory, black holes, and the cosmo- logical constant","work_id":"73a006cd-07e4-4bd8-96be-030880cfe87c","year":1999},{"cited_arxiv_id":"","doi":"10.1088/1126-6708/2002/12/062","is_internal_anchor":false,"ref_index":5,"title":"Recurrent nightmares? Measurement theory in de Sitter space,","work_id":"e00b63f0-369f-4155-8b86-4aa9441e4aa2","year":2002},{"cited_arxiv_id":"","doi":"10.1007/jhep12(2025)085","is_internal_anchor":false,"ref_index":6,"title":"JT de Sitter gravity as a model of Coleman-de Luccia tunneling,","work_id":"6e9be668-3e3e-4354-bb33-62e9816e2950","year":2025}],"snapshot_sha256":"5b02e63e1d5179b19a0471593bf4c5298cc24e62c7a57ae78966a6408ac96929"},"source":{"id":"2605.13490","kind":"arxiv","version":1},"verdict":{"created_at":"2026-05-14T18:26:02.106550Z","id":"1036cdf2-2764-4a2f-b6fd-1d5e8359bb5c","model_set":{"reader":"grok-4.3"},"one_line_summary":"De Sitter space modeled as a finite quantum system yields ambiguous theories, with local experiments accessing only a tiny fraction of its total information content.","pipeline_version":"pith-pipeline@v0.9.0","pith_extraction_headline":"If de Sitter space is a finite quantum system then all models of it are ambiguous","strongest_claim":"if de Sitter space is indeed represented by a finite dimensional quantum system, then semi-classical considerations, combined with the fundamental principles of quantum measurement theory, imply that any theoretical model of it is ambiguous.","weakest_assumption":"That de Sitter space is represented by a finite dimensional quantum system and that our universe asymptotes to such a de Sitter state."}},"verdict_id":"1036cdf2-2764-4a2f-b6fd-1d5e8359bb5c"}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:638df88adcfc55c7c6f3e51e53195ccbe5bb89f5ef4ce2e9deb58fef5346d96a","target":"record","created_at":"2026-05-18T02:44:41Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"d2e1a53a61401639c3c4cfedab21574fb111aa17f5c15f9476220bdd8d26e138","cross_cats_sorted":["gr-qc"],"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2026-05-13T13:16:01Z","title_canon_sha256":"e2d9179e87cab3f7a7bd88ae90f67628d55fb9126911f89d92a503d1af03cf80"},"schema_version":"1.0","source":{"id":"2605.13490","kind":"arxiv","version":1}},"canonical_sha256":"d52ae15387a909355131b1dd44e56a9201f2444fdb3e186ec24205ac0d722fe2","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"d52ae15387a909355131b1dd44e56a9201f2444fdb3e186ec24205ac0d722fe2","first_computed_at":"2026-05-18T02:44:41.186019Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:44:41.186019Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"hMiJlTmnWi+ucrScxYH4oa1HfEqgJhT90rVjghhSXAuD873dkcjvQ/hTgDW5tzCuxN88QLNABu0gWuOyFQ42BQ==","signature_status":"signed_v1","signed_at":"2026-05-18T02:44:41.186582Z","signed_message":"canonical_sha256_bytes"},"source_id":"2605.13490","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:638df88adcfc55c7c6f3e51e53195ccbe5bb89f5ef4ce2e9deb58fef5346d96a","sha256:1e5eb3f767732ce2599f176b3f0b1e3cce2771fbea1250931ff3541c98ad67c6","sha256:81ce98748ad5a189b5e5236c0da82c5b87c8d204ae9e97e5581dcef7dc75c131"],"state_sha256":"a37c5259d830ec6df829cb799d7ab5cb5b9e9076c7db01cc86d728da9124447a"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"nlSrrmAG1IzAvwpoXZno7OpdjzlMnGMeEI5DAQiUvnz//8eTy56Xg8lkKjxxdaGDEx325hBUkvuLyaHUppKoAg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-22T03:10:09.727776Z","bundle_sha256":"f301c0963991d28baac22e12047584213c955088f7b932819e3eb8a64a714c33"}}