{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:QH4JCIFQGMJYHHUJDDUHNLTMLD","short_pith_number":"pith:QH4JCIFQ","schema_version":"1.0","canonical_sha256":"81f89120b03313839e8918e876ae6c58e2ecf7f34cf5ec3a36aa3a06a7de585c","source":{"kind":"arxiv","id":"1411.7873","version":2},"attestation_state":"computed","paper":{"title":"Liouville theory beyond the cosmological horizon","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Geoffrey Comp\\`ere, Laura Donnay, Pierre-Henry Lambert, Waldemar Schulgin","submitted_at":"2014-11-28T14:15:35Z","abstract_excerpt":"The dS/CFT correspondence postulates the existence of a Euclidean CFT dual to a suitable gravity theory with Dirichlet boundary conditions asymptotic to de Sitter spacetime. A semi-classical model of such a correspondence consists of Einstein gravity with positive cosmological constant and without matter which is dual to Euclidean Liouville theory defined at the future conformal boundary. Here we show that Euclidean Liouville theory is also dual to Einstein gravity with Dirichlet boundary conditions on a fixed timelike slice in the static patch. Intriguingly, the spacetime interpretation of Eu"},"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":"1411.7873","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2014-11-28T14:15:35Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"c553972c68eee63d253400ef48649d93665e7d620dd5a3f7839ac2fefe7c804c","abstract_canon_sha256":"9e65adcd30eb9aff5350a5ac72994735ca84686d1a662aa894fd99937ef5acd0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:17:33.433849Z","signature_b64":"AVItV9Fnfx2bTeMIk47doxZcZfXQAAUEMQqZ8jBbsZHhvIqmOF9/HnM1ihlf7q+34w1E9fgo0p4Z2e4I1ZWmBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"81f89120b03313839e8918e876ae6c58e2ecf7f34cf5ec3a36aa3a06a7de585c","last_reissued_at":"2026-05-18T02:17:33.433086Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:17:33.433086Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Liouville theory beyond the cosmological horizon","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Geoffrey Comp\\`ere, Laura Donnay, Pierre-Henry Lambert, Waldemar Schulgin","submitted_at":"2014-11-28T14:15:35Z","abstract_excerpt":"The dS/CFT correspondence postulates the existence of a Euclidean CFT dual to a suitable gravity theory with Dirichlet boundary conditions asymptotic to de Sitter spacetime. A semi-classical model of such a correspondence consists of Einstein gravity with positive cosmological constant and without matter which is dual to Euclidean Liouville theory defined at the future conformal boundary. Here we show that Euclidean Liouville theory is also dual to Einstein gravity with Dirichlet boundary conditions on a fixed timelike slice in the static patch. Intriguingly, the spacetime interpretation of Eu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.7873","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":""},"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":"1411.7873","created_at":"2026-05-18T02:17:33.433212+00:00"},{"alias_kind":"arxiv_version","alias_value":"1411.7873v2","created_at":"2026-05-18T02:17:33.433212+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.7873","created_at":"2026-05-18T02:17:33.433212+00:00"},{"alias_kind":"pith_short_12","alias_value":"QH4JCIFQGMJY","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_16","alias_value":"QH4JCIFQGMJYHHUJ","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_8","alias_value":"QH4JCIFQ","created_at":"2026-05-18T12:28:46.137349+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.27068","citing_title":"Holographic realization of higher-spin Carrollian free fields","ref_index":65,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QH4JCIFQGMJYHHUJDDUHNLTMLD","json":"https://pith.science/pith/QH4JCIFQGMJYHHUJDDUHNLTMLD.json","graph_json":"https://pith.science/api/pith-number/QH4JCIFQGMJYHHUJDDUHNLTMLD/graph.json","events_json":"https://pith.science/api/pith-number/QH4JCIFQGMJYHHUJDDUHNLTMLD/events.json","paper":"https://pith.science/paper/QH4JCIFQ"},"agent_actions":{"view_html":"https://pith.science/pith/QH4JCIFQGMJYHHUJDDUHNLTMLD","download_json":"https://pith.science/pith/QH4JCIFQGMJYHHUJDDUHNLTMLD.json","view_paper":"https://pith.science/paper/QH4JCIFQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1411.7873&json=true","fetch_graph":"https://pith.science/api/pith-number/QH4JCIFQGMJYHHUJDDUHNLTMLD/graph.json","fetch_events":"https://pith.science/api/pith-number/QH4JCIFQGMJYHHUJDDUHNLTMLD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QH4JCIFQGMJYHHUJDDUHNLTMLD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QH4JCIFQGMJYHHUJDDUHNLTMLD/action/storage_attestation","attest_author":"https://pith.science/pith/QH4JCIFQGMJYHHUJDDUHNLTMLD/action/author_attestation","sign_citation":"https://pith.science/pith/QH4JCIFQGMJYHHUJDDUHNLTMLD/action/citation_signature","submit_replication":"https://pith.science/pith/QH4JCIFQGMJYHHUJDDUHNLTMLD/action/replication_record"}},"created_at":"2026-05-18T02:17:33.433212+00:00","updated_at":"2026-05-18T02:17:33.433212+00:00"}