{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:KXFWW6IH75CQTBS2C6IWMOBPC4","short_pith_number":"pith:KXFWW6IH","schema_version":"1.0","canonical_sha256":"55cb6b7907ff4509865a179166382f1739f8117c5d8ec62b3c3bdbc460e2e6b1","source":{"kind":"arxiv","id":"1703.05776","version":2},"attestation_state":"computed","paper":{"title":"The Swampland Conjecture and F-term Axion Monodromy Inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Florian Wolf, Irene Valenzuela, Ralph Blumenhagen","submitted_at":"2017-03-16T18:03:40Z","abstract_excerpt":"We continue the investigation of F-term axion monodromy inflation in string theory, while seriously taking the issue of moduli stabilization into account. For a number of closed and open string models, we show that they suffer from serious control issues once one is trying to realize trans-Planckian field excursions. More precisely, the flux tuning required to delay the logarithmic scaling of the field distance to a trans-Planckian value cannot be done without leaving the regime where the employed effective supergravity theory is under control. Our findings are consistent with the axionic exte"},"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":"1703.05776","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2017-03-16T18:03:40Z","cross_cats_sorted":[],"title_canon_sha256":"e4c238d35ebf28b12e00dfdc5f6d5a1cf468de3f1057e87b3fa8ddef6c59d65b","abstract_canon_sha256":"81b69ee92c07eb6ac2db78f8f44f02d22f4309acdade472fca4472feade6a9aa"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:35:23.172906Z","signature_b64":"LpDfkOjqbgt0gb1KVYqfI4rLfNx9iqo2MAjONFt+sb/J+96Eu+De9+oAFug6Yy8z2XEt3UnfGD1v3Qry19xcBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"55cb6b7907ff4509865a179166382f1739f8117c5d8ec62b3c3bdbc460e2e6b1","last_reissued_at":"2026-05-18T00:35:23.172348Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:35:23.172348Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Swampland Conjecture and F-term Axion Monodromy Inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Florian Wolf, Irene Valenzuela, Ralph Blumenhagen","submitted_at":"2017-03-16T18:03:40Z","abstract_excerpt":"We continue the investigation of F-term axion monodromy inflation in string theory, while seriously taking the issue of moduli stabilization into account. For a number of closed and open string models, we show that they suffer from serious control issues once one is trying to realize trans-Planckian field excursions. More precisely, the flux tuning required to delay the logarithmic scaling of the field distance to a trans-Planckian value cannot be done without leaving the regime where the employed effective supergravity theory is under control. Our findings are consistent with the axionic exte"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.05776","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":"1703.05776","created_at":"2026-05-18T00:35:23.172447+00:00"},{"alias_kind":"arxiv_version","alias_value":"1703.05776v2","created_at":"2026-05-18T00:35:23.172447+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.05776","created_at":"2026-05-18T00:35:23.172447+00:00"},{"alias_kind":"pith_short_12","alias_value":"KXFWW6IH75CQ","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_16","alias_value":"KXFWW6IH75CQTBS2","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_8","alias_value":"KXFWW6IH","created_at":"2026-05-18T12:31:28.150371+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2603.11163","citing_title":"Alice in Warpland: KK modes, Warped Compactifications and the Swampland","ref_index":35,"is_internal_anchor":true},{"citing_arxiv_id":"2604.24843","citing_title":"Optimal paths across potentials on scalar field space","ref_index":23,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KXFWW6IH75CQTBS2C6IWMOBPC4","json":"https://pith.science/pith/KXFWW6IH75CQTBS2C6IWMOBPC4.json","graph_json":"https://pith.science/api/pith-number/KXFWW6IH75CQTBS2C6IWMOBPC4/graph.json","events_json":"https://pith.science/api/pith-number/KXFWW6IH75CQTBS2C6IWMOBPC4/events.json","paper":"https://pith.science/paper/KXFWW6IH"},"agent_actions":{"view_html":"https://pith.science/pith/KXFWW6IH75CQTBS2C6IWMOBPC4","download_json":"https://pith.science/pith/KXFWW6IH75CQTBS2C6IWMOBPC4.json","view_paper":"https://pith.science/paper/KXFWW6IH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1703.05776&json=true","fetch_graph":"https://pith.science/api/pith-number/KXFWW6IH75CQTBS2C6IWMOBPC4/graph.json","fetch_events":"https://pith.science/api/pith-number/KXFWW6IH75CQTBS2C6IWMOBPC4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KXFWW6IH75CQTBS2C6IWMOBPC4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KXFWW6IH75CQTBS2C6IWMOBPC4/action/storage_attestation","attest_author":"https://pith.science/pith/KXFWW6IH75CQTBS2C6IWMOBPC4/action/author_attestation","sign_citation":"https://pith.science/pith/KXFWW6IH75CQTBS2C6IWMOBPC4/action/citation_signature","submit_replication":"https://pith.science/pith/KXFWW6IH75CQTBS2C6IWMOBPC4/action/replication_record"}},"created_at":"2026-05-18T00:35:23.172447+00:00","updated_at":"2026-05-18T00:35:23.172447+00:00"}