{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:VLR5DFEIDA7QA524YQHPGEO7YO","short_pith_number":"pith:VLR5DFEI","schema_version":"1.0","canonical_sha256":"aae3d19488183f00775cc40ef311dfc3a8b237e70cd115111cbcfade65fbd329","source":{"kind":"arxiv","id":"2404.13684","version":3},"attestation_state":"computed","paper":{"title":"Generalized Entanglement Capacity of de Sitter Space","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Patrick Draper, Tom Banks","submitted_at":"2024-04-21T15:01:37Z","abstract_excerpt":"Near horizons, quantum fields of low spin exhibit densities of states that behave asymptotically like 1+1 dimensional conformal field theories. In effective field theory, imposing some short-distance cutoff, one can compute thermodynamic quantities associated with the horizon, and the leading cutoff sensitivity of the heat capacity is found to equal to the leading cutoff sensitivity of the entropy. One can also compute contributions to the thermodynamic quantities from the gravitational path integral. For the cosmological horizon of the static patch of de Sitter space, a natural conjecture for"},"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":"2404.13684","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2024-04-21T15:01:37Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"96e53e6bc222ff4b62a32adebba003e5cb4d1b25c070d1a2acec4b126169f3ef","abstract_canon_sha256":"0f03c59dbf4fbfd54b0fade5c0876f350f247419511a5dc0a4e92318e06baba1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:13:13.700833Z","signature_b64":"Aq25Lz8QrFkKTroonDzu0H5+9crht2xr+9+LBZkfHKFRe+OzToY5LXhOKLxUTpfkSxWx9g7WOFpiLrXtPM0mBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"aae3d19488183f00775cc40ef311dfc3a8b237e70cd115111cbcfade65fbd329","last_reissued_at":"2026-07-05T08:13:13.700350Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:13:13.700350Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Generalized Entanglement Capacity of de Sitter Space","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Patrick Draper, Tom Banks","submitted_at":"2024-04-21T15:01:37Z","abstract_excerpt":"Near horizons, quantum fields of low spin exhibit densities of states that behave asymptotically like 1+1 dimensional conformal field theories. In effective field theory, imposing some short-distance cutoff, one can compute thermodynamic quantities associated with the horizon, and the leading cutoff sensitivity of the heat capacity is found to equal to the leading cutoff sensitivity of the entropy. One can also compute contributions to the thermodynamic quantities from the gravitational path integral. For the cosmological horizon of the static patch of de Sitter space, a natural conjecture for"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2404.13684","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2404.13684/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":"2404.13684","created_at":"2026-07-05T08:13:13.700414+00:00"},{"alias_kind":"arxiv_version","alias_value":"2404.13684v3","created_at":"2026-07-05T08:13:13.700414+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2404.13684","created_at":"2026-07-05T08:13:13.700414+00:00"},{"alias_kind":"pith_short_12","alias_value":"VLR5DFEIDA7Q","created_at":"2026-07-05T08:13:13.700414+00:00"},{"alias_kind":"pith_short_16","alias_value":"VLR5DFEIDA7QA524","created_at":"2026-07-05T08:13:13.700414+00:00"},{"alias_kind":"pith_short_8","alias_value":"VLR5DFEI","created_at":"2026-07-05T08:13:13.700414+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07810","citing_title":"Relative entropy for $\\lambda \\phi^4$ in the Rindler wedge","ref_index":60,"is_internal_anchor":true},{"citing_arxiv_id":"2604.10267","citing_title":"The yes boundaries wavefunctions of the universe","ref_index":125,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VLR5DFEIDA7QA524YQHPGEO7YO","json":"https://pith.science/pith/VLR5DFEIDA7QA524YQHPGEO7YO.json","graph_json":"https://pith.science/api/pith-number/VLR5DFEIDA7QA524YQHPGEO7YO/graph.json","events_json":"https://pith.science/api/pith-number/VLR5DFEIDA7QA524YQHPGEO7YO/events.json","paper":"https://pith.science/paper/VLR5DFEI"},"agent_actions":{"view_html":"https://pith.science/pith/VLR5DFEIDA7QA524YQHPGEO7YO","download_json":"https://pith.science/pith/VLR5DFEIDA7QA524YQHPGEO7YO.json","view_paper":"https://pith.science/paper/VLR5DFEI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2404.13684&json=true","fetch_graph":"https://pith.science/api/pith-number/VLR5DFEIDA7QA524YQHPGEO7YO/graph.json","fetch_events":"https://pith.science/api/pith-number/VLR5DFEIDA7QA524YQHPGEO7YO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VLR5DFEIDA7QA524YQHPGEO7YO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VLR5DFEIDA7QA524YQHPGEO7YO/action/storage_attestation","attest_author":"https://pith.science/pith/VLR5DFEIDA7QA524YQHPGEO7YO/action/author_attestation","sign_citation":"https://pith.science/pith/VLR5DFEIDA7QA524YQHPGEO7YO/action/citation_signature","submit_replication":"https://pith.science/pith/VLR5DFEIDA7QA524YQHPGEO7YO/action/replication_record"}},"created_at":"2026-07-05T08:13:13.700414+00:00","updated_at":"2026-07-05T08:13:13.700414+00:00"}