{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:C4L7OZHEBVVJU7SABWQUVEMPFF","short_pith_number":"pith:C4L7OZHE","schema_version":"1.0","canonical_sha256":"1717f764e40d6a9a7e400da14a918f295c412ca7474bdcb4f079aafa5ae12c74","source":{"kind":"arxiv","id":"2402.01357","version":2},"attestation_state":"computed","paper":{"title":"Holographic complexity of the extended Schwarzschild-de Sitter space","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Nicol\\'o Zenoni, Sergio E. Aguilar-Gutierrez, Stefano Baiguera","submitted_at":"2024-02-02T12:24:40Z","abstract_excerpt":"According to static patch holography, de Sitter space admits a unitary quantum description in terms of a dual theory living on the stretched horizon, that is a timelike surface close to the cosmological horizon. In this manuscript, we compute several holographic complexity conjectures in a periodic extension of the Schwarzschild-de Sitter black hole. We consider multiple configurations of the stretched horizons to which geometric objects are anchored. The holographic complexity proposals admit a hyperfast growth when the gravitational observables only lie in the cosmological patch, except 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":"2402.01357","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2024-02-02T12:24:40Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"f64638471492cf38f7d389325914c0d70619e0707690ebfb9c49c3518c8d8bc6","abstract_canon_sha256":"093a6431330aad7ad008c0f7b48ff8d9c592b375d98390527be54b7a8ea2c9fe"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:10:23.388145Z","signature_b64":"6loBy7TiehLF3DEbLLT1aDW9LCz6ExG8JGCdqhfiCvLEUrHK6ZAUIHb2rU9VHVHw1pD1hwDH+C2c/xV0qOJADQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1717f764e40d6a9a7e400da14a918f295c412ca7474bdcb4f079aafa5ae12c74","last_reissued_at":"2026-07-05T08:10:23.387680Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:10:23.387680Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Holographic complexity of the extended Schwarzschild-de Sitter space","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Nicol\\'o Zenoni, Sergio E. Aguilar-Gutierrez, Stefano Baiguera","submitted_at":"2024-02-02T12:24:40Z","abstract_excerpt":"According to static patch holography, de Sitter space admits a unitary quantum description in terms of a dual theory living on the stretched horizon, that is a timelike surface close to the cosmological horizon. In this manuscript, we compute several holographic complexity conjectures in a periodic extension of the Schwarzschild-de Sitter black hole. We consider multiple configurations of the stretched horizons to which geometric objects are anchored. The holographic complexity proposals admit a hyperfast growth when the gravitational observables only lie in the cosmological patch, except for "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2402.01357","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/2402.01357/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":"2402.01357","created_at":"2026-07-05T08:10:23.387737+00:00"},{"alias_kind":"arxiv_version","alias_value":"2402.01357v2","created_at":"2026-07-05T08:10:23.387737+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2402.01357","created_at":"2026-07-05T08:10:23.387737+00:00"},{"alias_kind":"pith_short_12","alias_value":"C4L7OZHEBVVJ","created_at":"2026-07-05T08:10:23.387737+00:00"},{"alias_kind":"pith_short_16","alias_value":"C4L7OZHEBVVJU7SA","created_at":"2026-07-05T08:10:23.387737+00:00"},{"alias_kind":"pith_short_8","alias_value":"C4L7OZHE","created_at":"2026-07-05T08:10:23.387737+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.11297","citing_title":"Bouncing Geodesics, Singularities, and the Cavity Thermal Product Formula in Asymptotically Flat and de Sitter Black Holes","ref_index":85,"is_internal_anchor":false},{"citing_arxiv_id":"2606.03049","citing_title":"Holographic complexity of de-Sitter black holes","ref_index":122,"is_internal_anchor":false},{"citing_arxiv_id":"2511.03779","citing_title":"Cosmological Entanglement Entropy from the von Neumann Algebra of Double-Scaled SYK & Its Connection with Krylov Complexity","ref_index":264,"is_internal_anchor":false},{"citing_arxiv_id":"2602.06113","citing_title":"Deforming the Double-Scaled SYK & Reaching the Stretched Horizon From Finite Cutoff Holography","ref_index":166,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/C4L7OZHEBVVJU7SABWQUVEMPFF","json":"https://pith.science/pith/C4L7OZHEBVVJU7SABWQUVEMPFF.json","graph_json":"https://pith.science/api/pith-number/C4L7OZHEBVVJU7SABWQUVEMPFF/graph.json","events_json":"https://pith.science/api/pith-number/C4L7OZHEBVVJU7SABWQUVEMPFF/events.json","paper":"https://pith.science/paper/C4L7OZHE"},"agent_actions":{"view_html":"https://pith.science/pith/C4L7OZHEBVVJU7SABWQUVEMPFF","download_json":"https://pith.science/pith/C4L7OZHEBVVJU7SABWQUVEMPFF.json","view_paper":"https://pith.science/paper/C4L7OZHE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2402.01357&json=true","fetch_graph":"https://pith.science/api/pith-number/C4L7OZHEBVVJU7SABWQUVEMPFF/graph.json","fetch_events":"https://pith.science/api/pith-number/C4L7OZHEBVVJU7SABWQUVEMPFF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/C4L7OZHEBVVJU7SABWQUVEMPFF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/C4L7OZHEBVVJU7SABWQUVEMPFF/action/storage_attestation","attest_author":"https://pith.science/pith/C4L7OZHEBVVJU7SABWQUVEMPFF/action/author_attestation","sign_citation":"https://pith.science/pith/C4L7OZHEBVVJU7SABWQUVEMPFF/action/citation_signature","submit_replication":"https://pith.science/pith/C4L7OZHEBVVJU7SABWQUVEMPFF/action/replication_record"}},"created_at":"2026-07-05T08:10:23.387737+00:00","updated_at":"2026-07-05T08:10:23.387737+00:00"}