{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:PRNOFNLWR52ONM6P4XSIQICDYB","short_pith_number":"pith:PRNOFNLW","schema_version":"1.0","canonical_sha256":"7c5ae2b5768f74e6b3cfe5e4882043c05459368a4f61016d28ef5561c795528d","source":{"kind":"arxiv","id":"1910.09549","version":3},"attestation_state":"computed","paper":{"title":"Asymptotic Flux Compactifications and the Swampland","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["math.AG"],"primary_cat":"hep-th","authors_text":"Chongchuo Li, Irene Valenzuela, Thomas W. Grimm","submitted_at":"2019-10-21T18:00:00Z","abstract_excerpt":"We initiate the systematic study of flux scalar potentials and their vacua by using asymptotic Hodge theory. To begin with, we consider F-theory compactifications on Calabi-Yau fourfolds with four-form flux. We argue that a classifications of all scalar potentials can be performed when focusing on regions in the field space in which one or several fields are large and close to a boundary. To exemplify the constraints on such asymptotic flux compactifications, we explicitly determine this classification for situations in which two complex structure moduli are taken to be large. Our classificati"},"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":"1910.09549","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2019-10-21T18:00:00Z","cross_cats_sorted":["math.AG"],"title_canon_sha256":"06262dc3fa9c5e8e7fa852dc3da546189a10ca8a6e82bf86062460bb65b3dbf2","abstract_canon_sha256":"1cba93756437ca4dcdbf134c22edc573bf0166fd5ad59ee1370958218ff4e61e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:59:26.800167Z","signature_b64":"X9/QvLKyLicOtW/dDjpsk/NLyUMU0b9Q1gf3ZLb1US1JIVbq6SkxVsz9wPN61qCvXpuvsSIrBErYF+djTfA2BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7c5ae2b5768f74e6b3cfe5e4882043c05459368a4f61016d28ef5561c795528d","last_reissued_at":"2026-07-05T01:59:26.799637Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:59:26.799637Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Asymptotic Flux Compactifications and the Swampland","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["math.AG"],"primary_cat":"hep-th","authors_text":"Chongchuo Li, Irene Valenzuela, Thomas W. Grimm","submitted_at":"2019-10-21T18:00:00Z","abstract_excerpt":"We initiate the systematic study of flux scalar potentials and their vacua by using asymptotic Hodge theory. To begin with, we consider F-theory compactifications on Calabi-Yau fourfolds with four-form flux. We argue that a classifications of all scalar potentials can be performed when focusing on regions in the field space in which one or several fields are large and close to a boundary. To exemplify the constraints on such asymptotic flux compactifications, we explicitly determine this classification for situations in which two complex structure moduli are taken to be large. Our classificati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1910.09549","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/1910.09549/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":"1910.09549","created_at":"2026-07-05T01:59:26.799702+00:00"},{"alias_kind":"arxiv_version","alias_value":"1910.09549v3","created_at":"2026-07-05T01:59:26.799702+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1910.09549","created_at":"2026-07-05T01:59:26.799702+00:00"},{"alias_kind":"pith_short_12","alias_value":"PRNOFNLWR52O","created_at":"2026-07-05T01:59:26.799702+00:00"},{"alias_kind":"pith_short_16","alias_value":"PRNOFNLWR52ONM6P","created_at":"2026-07-05T01:59:26.799702+00:00"},{"alias_kind":"pith_short_8","alias_value":"PRNOFNLW","created_at":"2026-07-05T01:59:26.799702+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.28938","citing_title":"Gravity Decoupling and Axionic Shift Symmetries","ref_index":44,"is_internal_anchor":false},{"citing_arxiv_id":"2105.09326","citing_title":"F-theory flux vacua at large complex structure","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"2507.02037","citing_title":"An M-theory dS maximum from Casimir energies on Riemann-flat manifolds","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"2603.11163","citing_title":"Alice in Warpland: KK modes, Warped Compactifications and the Swampland","ref_index":146,"is_internal_anchor":false},{"citing_arxiv_id":"2603.12315","citing_title":"Quantum obstructions for $N=1$ infinite distance limits -- Part I: $g_s$ obstructions","ref_index":57,"is_internal_anchor":false},{"citing_arxiv_id":"2603.25797","citing_title":"Dark energy from string theory: an introductory review","ref_index":221,"is_internal_anchor":false},{"citing_arxiv_id":"2604.24843","citing_title":"Optimal paths across potentials on scalar field space","ref_index":24,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PRNOFNLWR52ONM6P4XSIQICDYB","json":"https://pith.science/pith/PRNOFNLWR52ONM6P4XSIQICDYB.json","graph_json":"https://pith.science/api/pith-number/PRNOFNLWR52ONM6P4XSIQICDYB/graph.json","events_json":"https://pith.science/api/pith-number/PRNOFNLWR52ONM6P4XSIQICDYB/events.json","paper":"https://pith.science/paper/PRNOFNLW"},"agent_actions":{"view_html":"https://pith.science/pith/PRNOFNLWR52ONM6P4XSIQICDYB","download_json":"https://pith.science/pith/PRNOFNLWR52ONM6P4XSIQICDYB.json","view_paper":"https://pith.science/paper/PRNOFNLW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1910.09549&json=true","fetch_graph":"https://pith.science/api/pith-number/PRNOFNLWR52ONM6P4XSIQICDYB/graph.json","fetch_events":"https://pith.science/api/pith-number/PRNOFNLWR52ONM6P4XSIQICDYB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PRNOFNLWR52ONM6P4XSIQICDYB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PRNOFNLWR52ONM6P4XSIQICDYB/action/storage_attestation","attest_author":"https://pith.science/pith/PRNOFNLWR52ONM6P4XSIQICDYB/action/author_attestation","sign_citation":"https://pith.science/pith/PRNOFNLWR52ONM6P4XSIQICDYB/action/citation_signature","submit_replication":"https://pith.science/pith/PRNOFNLWR52ONM6P4XSIQICDYB/action/replication_record"}},"created_at":"2026-07-05T01:59:26.799702+00:00","updated_at":"2026-07-05T01:59:26.799702+00:00"}