{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:7NEJCWYAUFECANPLLPKVTENF6G","short_pith_number":"pith:7NEJCWYA","schema_version":"1.0","canonical_sha256":"fb48915b00a1482035eb5bd55991a5f1a84be9d3fbd25e12bc587377a4e45a0d","source":{"kind":"arxiv","id":"2212.06086","version":3},"attestation_state":"computed","paper":{"title":"On de Sitter Spacetime and String Theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-th","authors_text":"Djordje Minic, Per Berglund, Tristan H\\\"ubsch","submitted_at":"2022-12-12T18:00:53Z","abstract_excerpt":"We review various aspects of de Sitter spacetime in string theory: its status as an effective field theory spacetime solution, its relation to the vacuum energy problem in string theory, its (global) holographic definition in terms of two entangled and non-canonical conformal field theories, as well as a realization of a realistic de Sitter universe endowed with the observed visible matter and the necessary dark sector in order to reproduce the realistic cosmological structure. In particular, based on the new insight regarding the cosmological constant problem in string theory, we argue that i"},"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":"2212.06086","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2022-12-12T18:00:53Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"3e5a7bec1b4227d031d40371de50485eccd03f82f5e590e9ac4b00d3c3cf5d97","abstract_canon_sha256":"f3bca84273c536316af00f5308620228ea35b92cdaf4e64629b4a0106f6d273d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:45:33.576162Z","signature_b64":"T6rMrDfHF7uXNGDgPXhnPBQDqESxh/zg0Mg0WDks36Z/zcc+RMTgfOY4waDVRKaepHsTGI1umXQGCCpfMNIHCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fb48915b00a1482035eb5bd55991a5f1a84be9d3fbd25e12bc587377a4e45a0d","last_reissued_at":"2026-07-05T06:45:33.575697Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:45:33.575697Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On de Sitter Spacetime and String Theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-th","authors_text":"Djordje Minic, Per Berglund, Tristan H\\\"ubsch","submitted_at":"2022-12-12T18:00:53Z","abstract_excerpt":"We review various aspects of de Sitter spacetime in string theory: its status as an effective field theory spacetime solution, its relation to the vacuum energy problem in string theory, its (global) holographic definition in terms of two entangled and non-canonical conformal field theories, as well as a realization of a realistic de Sitter universe endowed with the observed visible matter and the necessary dark sector in order to reproduce the realistic cosmological structure. In particular, based on the new insight regarding the cosmological constant problem in string theory, we argue that i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2212.06086","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/2212.06086/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":"2212.06086","created_at":"2026-07-05T06:45:33.575757+00:00"},{"alias_kind":"arxiv_version","alias_value":"2212.06086v3","created_at":"2026-07-05T06:45:33.575757+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2212.06086","created_at":"2026-07-05T06:45:33.575757+00:00"},{"alias_kind":"pith_short_12","alias_value":"7NEJCWYAUFEC","created_at":"2026-07-05T06:45:33.575757+00:00"},{"alias_kind":"pith_short_16","alias_value":"7NEJCWYAUFECANPL","created_at":"2026-07-05T06:45:33.575757+00:00"},{"alias_kind":"pith_short_8","alias_value":"7NEJCWYA","created_at":"2026-07-05T06:45:33.575757+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.24724","citing_title":"Beyond Algebraic Solutions to Stringy Spacetime","ref_index":55,"is_internal_anchor":false},{"citing_arxiv_id":"2605.23900","citing_title":"What to do with a Ricci-flat Calabi--Yau metric?","ref_index":167,"is_internal_anchor":false},{"citing_arxiv_id":"2604.19418","citing_title":"Quantum Spacetime, Quantum Gravity and Gravitized Quantum Theory","ref_index":7,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7NEJCWYAUFECANPLLPKVTENF6G","json":"https://pith.science/pith/7NEJCWYAUFECANPLLPKVTENF6G.json","graph_json":"https://pith.science/api/pith-number/7NEJCWYAUFECANPLLPKVTENF6G/graph.json","events_json":"https://pith.science/api/pith-number/7NEJCWYAUFECANPLLPKVTENF6G/events.json","paper":"https://pith.science/paper/7NEJCWYA"},"agent_actions":{"view_html":"https://pith.science/pith/7NEJCWYAUFECANPLLPKVTENF6G","download_json":"https://pith.science/pith/7NEJCWYAUFECANPLLPKVTENF6G.json","view_paper":"https://pith.science/paper/7NEJCWYA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2212.06086&json=true","fetch_graph":"https://pith.science/api/pith-number/7NEJCWYAUFECANPLLPKVTENF6G/graph.json","fetch_events":"https://pith.science/api/pith-number/7NEJCWYAUFECANPLLPKVTENF6G/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7NEJCWYAUFECANPLLPKVTENF6G/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7NEJCWYAUFECANPLLPKVTENF6G/action/storage_attestation","attest_author":"https://pith.science/pith/7NEJCWYAUFECANPLLPKVTENF6G/action/author_attestation","sign_citation":"https://pith.science/pith/7NEJCWYAUFECANPLLPKVTENF6G/action/citation_signature","submit_replication":"https://pith.science/pith/7NEJCWYAUFECANPLLPKVTENF6G/action/replication_record"}},"created_at":"2026-07-05T06:45:33.575757+00:00","updated_at":"2026-07-05T06:45:33.575757+00:00"}