{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:UHR4RYGUU5KWC556PN7JOY2P7U","short_pith_number":"pith:UHR4RYGU","schema_version":"1.0","canonical_sha256":"a1e3c8e0d4a7556177be7b7e97634ffd2000ec64b3c6e5eeaf719748c58c025b","source":{"kind":"arxiv","id":"hep-th/0502058","version":2},"attestation_state":"computed","paper":{"title":"Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Fernando Quevedo, Joseph P. Conlon, Per Berglund, Vijay Balasubramanian","submitted_at":"2005-02-04T20:52:27Z","abstract_excerpt":"We study the large volume limit of the scalar potential in Calabi-Yau flux compactifications of type IIB string theory. Under general circumstances there exists a limit in which the potential approaches zero from below, with an associated non-supersymmetric AdS minimum at exponentially large volume. Both this and its de Sitter uplift are tachyon-free, thereby fixing all Kahler and complex structure moduli, which has been difficult to achieve in the KKLT scenario. Also, for the class of vacua described in this paper, the gravitino mass is independent of the flux discretuum, whereas the ratio of"},"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":"hep-th/0502058","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2005-02-04T20:52:27Z","cross_cats_sorted":[],"title_canon_sha256":"7e9e5e0ed3cea99d52f2c400dd213b8d817a6d7a552bc371787c1acc0f5c3317","abstract_canon_sha256":"9564a42a3ec583f6baef114fa6f1da3ff068a9221edec09a4648327b12a6987f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:22:51.422343Z","signature_b64":"4ID8zhx9d6mOu5yfMGT2ZF50gVXakLHolFECPfj727GTvYXSXJEiyCfqlk2npgc7wknB/WE5t3KLWTYTovD6Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a1e3c8e0d4a7556177be7b7e97634ffd2000ec64b3c6e5eeaf719748c58c025b","last_reissued_at":"2026-05-18T04:22:51.421607Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:22:51.421607Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Fernando Quevedo, Joseph P. Conlon, Per Berglund, Vijay Balasubramanian","submitted_at":"2005-02-04T20:52:27Z","abstract_excerpt":"We study the large volume limit of the scalar potential in Calabi-Yau flux compactifications of type IIB string theory. Under general circumstances there exists a limit in which the potential approaches zero from below, with an associated non-supersymmetric AdS minimum at exponentially large volume. Both this and its de Sitter uplift are tachyon-free, thereby fixing all Kahler and complex structure moduli, which has been difficult to achieve in the KKLT scenario. Also, for the class of vacua described in this paper, the gravitino mass is independent of the flux discretuum, whereas the ratio of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0502058","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":"hep-th/0502058","created_at":"2026-05-18T04:22:51.421712+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0502058v2","created_at":"2026-05-18T04:22:51.421712+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0502058","created_at":"2026-05-18T04:22:51.421712+00:00"},{"alias_kind":"pith_short_12","alias_value":"UHR4RYGUU5KW","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_16","alias_value":"UHR4RYGUU5KWC556","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_8","alias_value":"UHR4RYGU","created_at":"2026-05-18T12:25:53.939244+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":25,"internal_anchor_count":18,"sample":[{"citing_arxiv_id":"2606.25016","citing_title":"Lost in Translation: Moduli Stabilization from EFT to Eleven Dimensions","ref_index":15,"is_internal_anchor":true},{"citing_arxiv_id":"2606.21650","citing_title":"Quantum Gravity Cutoff from Axions: A Type IIB Landscape Study","ref_index":85,"is_internal_anchor":true},{"citing_arxiv_id":"2606.19440","citing_title":"Moduli Stabilisation for ADD and the Dark Dimension Scenario","ref_index":6,"is_internal_anchor":true},{"citing_arxiv_id":"2606.19423","citing_title":"Calabi-Yau Orientifold Hypersurfaces and their F-theory Uplifts","ref_index":11,"is_internal_anchor":true},{"citing_arxiv_id":"2606.10850","citing_title":"On Calabi-Yau Threefolds For Unified LVS Inflation","ref_index":35,"is_internal_anchor":true},{"citing_arxiv_id":"2606.09943","citing_title":"Testing Supersymmetric Hidden Sectors with Long-Baseline Atom Interferometers","ref_index":50,"is_internal_anchor":true},{"citing_arxiv_id":"2606.08767","citing_title":"Fire at the Tip of the Throat: Hagedorn Phase after brane-antibrane inflation?","ref_index":10,"is_internal_anchor":true},{"citing_arxiv_id":"2606.02701","citing_title":"Quintessential $\\alpha$-attractors fit DESI","ref_index":43,"is_internal_anchor":true},{"citing_arxiv_id":"2606.30341","citing_title":"A note on the holographic consistency of DGKT-type vacua with $h^{2,1}=0$","ref_index":9,"is_internal_anchor":true},{"citing_arxiv_id":"2606.28858","citing_title":"Axions on de Sitter space","ref_index":46,"is_internal_anchor":true},{"citing_arxiv_id":"2605.22998","citing_title":"Thermal effects and finite-temperature cosmology in perturbatively stabilized large volume scenarios","ref_index":6,"is_internal_anchor":true},{"citing_arxiv_id":"2605.23900","citing_title":"What to do with a Ricci-flat Calabi--Yau metric?","ref_index":75,"is_internal_anchor":true},{"citing_arxiv_id":"2412.08723","citing_title":"Chiral global embedding of Fibre Inflation with $\\overline{\\rm D3}$ uplift","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2506.22630","citing_title":"Assisted Fibre Inflation in Perturbative LVS","ref_index":18,"is_internal_anchor":true},{"citing_arxiv_id":"2507.01070","citing_title":"Barrow holographic dark energy interacting model in the presence of radiation and matter","ref_index":40,"is_internal_anchor":true},{"citing_arxiv_id":"2507.02037","citing_title":"An M-theory dS maximum from Casimir energies on Riemann-flat manifolds","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2603.12315","citing_title":"Quantum obstructions for $N=1$ infinite distance limits -- Part I: $g_s$ obstructions","ref_index":3,"is_internal_anchor":true},{"citing_arxiv_id":"2603.25797","citing_title":"Dark energy from string theory: an introductory review","ref_index":13,"is_internal_anchor":true},{"citing_arxiv_id":"2604.27835","citing_title":"Some Properties and Uses of the Species Scale","ref_index":45,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25918","citing_title":"de Sitter in String Theory vs. Gibbons & Hawking","ref_index":5,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05357","citing_title":"Small Vacuum Energy and Tunneling in a Modified Bousso-Polchinski Model","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"2605.00103","citing_title":"Pre-inflationary QCD axion stars after moduli domination","ref_index":48,"is_internal_anchor":false},{"citing_arxiv_id":"2604.19250","citing_title":"On Global Embedding of Assisted Fibre Inflation","ref_index":2,"is_internal_anchor":false},{"citing_arxiv_id":"2604.07288","citing_title":"Loop Blow-up Inflation: An Overview","ref_index":4,"is_internal_anchor":false},{"citing_arxiv_id":"2604.19817","citing_title":"Supersymmetry, Supergravity and Non--Perturbative Dynamics of Gauge Theories","ref_index":23,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UHR4RYGUU5KWC556PN7JOY2P7U","json":"https://pith.science/pith/UHR4RYGUU5KWC556PN7JOY2P7U.json","graph_json":"https://pith.science/api/pith-number/UHR4RYGUU5KWC556PN7JOY2P7U/graph.json","events_json":"https://pith.science/api/pith-number/UHR4RYGUU5KWC556PN7JOY2P7U/events.json","paper":"https://pith.science/paper/UHR4RYGU"},"agent_actions":{"view_html":"https://pith.science/pith/UHR4RYGUU5KWC556PN7JOY2P7U","download_json":"https://pith.science/pith/UHR4RYGUU5KWC556PN7JOY2P7U.json","view_paper":"https://pith.science/paper/UHR4RYGU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/0502058&json=true","fetch_graph":"https://pith.science/api/pith-number/UHR4RYGUU5KWC556PN7JOY2P7U/graph.json","fetch_events":"https://pith.science/api/pith-number/UHR4RYGUU5KWC556PN7JOY2P7U/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UHR4RYGUU5KWC556PN7JOY2P7U/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UHR4RYGUU5KWC556PN7JOY2P7U/action/storage_attestation","attest_author":"https://pith.science/pith/UHR4RYGUU5KWC556PN7JOY2P7U/action/author_attestation","sign_citation":"https://pith.science/pith/UHR4RYGUU5KWC556PN7JOY2P7U/action/citation_signature","submit_replication":"https://pith.science/pith/UHR4RYGUU5KWC556PN7JOY2P7U/action/replication_record"}},"created_at":"2026-05-18T04:22:51.421712+00:00","updated_at":"2026-05-18T04:22:51.421712+00:00"}