{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:UNEHMZHZBDZTLTUEU6WK4V6DPV","short_pith_number":"pith:UNEHMZHZ","schema_version":"1.0","canonical_sha256":"a3487664f908f335ce84a7acae57c37d7c8fe4f9444a920dd5f39d0e1cec3325","source":{"kind":"arxiv","id":"1409.7075","version":3},"attestation_state":"computed","paper":{"title":"The Challenge of Realizing F-term Axion Monodromy Inflation in String Theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-th","authors_text":"Daniela Herschmann, Erik Plauschinn, Ralph Blumenhagen","submitted_at":"2014-09-24T20:01:39Z","abstract_excerpt":"A systematic analysis of possibilities for realizing single-field F-term axion monodromy inflation via the flux-induced superpotential in type IIB string theory is performed. In this well-defined setting the conditions arising from moduli stabilization are taken into account, where we focus on the complex-structure moduli but ignore the Kaehler moduli sector. Our analysis leads to a no-go theorem, if the inflaton involves the universal axion. We furthermore construct an explicit example of F-term axion monodromy inflation, in which a single axion-like field is hierarchically lighter than all r"},"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":"1409.7075","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2014-09-24T20:01:39Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"8c243cc841c8bd7152c1bcd0d98eb29e2d725fba6ee5fe3424589837b824b98d","abstract_canon_sha256":"83e17c2d1f3f9d1facf313bf92c0091538a468768a558ee23a6a85f9a6287ce2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:29:31.718493Z","signature_b64":"3zJTrfpXcHzwbLYL3S/MpQ/Oc0WyUwH5L8ugILbH6bfYqM1OIYmKv+xzrWwqk4naSmvDrUgqHQjNgpiXfybhDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a3487664f908f335ce84a7acae57c37d7c8fe4f9444a920dd5f39d0e1cec3325","last_reissued_at":"2026-05-18T02:29:31.717932Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:29:31.717932Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Challenge of Realizing F-term Axion Monodromy Inflation in String Theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-th","authors_text":"Daniela Herschmann, Erik Plauschinn, Ralph Blumenhagen","submitted_at":"2014-09-24T20:01:39Z","abstract_excerpt":"A systematic analysis of possibilities for realizing single-field F-term axion monodromy inflation via the flux-induced superpotential in type IIB string theory is performed. In this well-defined setting the conditions arising from moduli stabilization are taken into account, where we focus on the complex-structure moduli but ignore the Kaehler moduli sector. Our analysis leads to a no-go theorem, if the inflaton involves the universal axion. We furthermore construct an explicit example of F-term axion monodromy inflation, in which a single axion-like field is hierarchically lighter than all r"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1409.7075","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":""},"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":"1409.7075","created_at":"2026-05-18T02:29:31.718008+00:00"},{"alias_kind":"arxiv_version","alias_value":"1409.7075v3","created_at":"2026-05-18T02:29:31.718008+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1409.7075","created_at":"2026-05-18T02:29:31.718008+00:00"},{"alias_kind":"pith_short_12","alias_value":"UNEHMZHZBDZT","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_16","alias_value":"UNEHMZHZBDZTLTUE","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_8","alias_value":"UNEHMZHZ","created_at":"2026-05-18T12:28:52.271510+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.10197","citing_title":"Controlled Penumbral Inflation from Monodromic Valleys","ref_index":7,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UNEHMZHZBDZTLTUEU6WK4V6DPV","json":"https://pith.science/pith/UNEHMZHZBDZTLTUEU6WK4V6DPV.json","graph_json":"https://pith.science/api/pith-number/UNEHMZHZBDZTLTUEU6WK4V6DPV/graph.json","events_json":"https://pith.science/api/pith-number/UNEHMZHZBDZTLTUEU6WK4V6DPV/events.json","paper":"https://pith.science/paper/UNEHMZHZ"},"agent_actions":{"view_html":"https://pith.science/pith/UNEHMZHZBDZTLTUEU6WK4V6DPV","download_json":"https://pith.science/pith/UNEHMZHZBDZTLTUEU6WK4V6DPV.json","view_paper":"https://pith.science/paper/UNEHMZHZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1409.7075&json=true","fetch_graph":"https://pith.science/api/pith-number/UNEHMZHZBDZTLTUEU6WK4V6DPV/graph.json","fetch_events":"https://pith.science/api/pith-number/UNEHMZHZBDZTLTUEU6WK4V6DPV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UNEHMZHZBDZTLTUEU6WK4V6DPV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UNEHMZHZBDZTLTUEU6WK4V6DPV/action/storage_attestation","attest_author":"https://pith.science/pith/UNEHMZHZBDZTLTUEU6WK4V6DPV/action/author_attestation","sign_citation":"https://pith.science/pith/UNEHMZHZBDZTLTUEU6WK4V6DPV/action/citation_signature","submit_replication":"https://pith.science/pith/UNEHMZHZBDZTLTUEU6WK4V6DPV/action/replication_record"}},"created_at":"2026-05-18T02:29:31.718008+00:00","updated_at":"2026-05-18T02:29:31.718008+00:00"}