{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:O6S2UAK2ZMFAJ25SW4EPNHOVHK","short_pith_number":"pith:O6S2UAK2","schema_version":"1.0","canonical_sha256":"77a5aa015acb0a04ebb2b708f69dd53a9e207b1b09d07b52a9d13bea4d75cdf7","source":{"kind":"arxiv","id":"1512.03768","version":3},"attestation_state":"computed","paper":{"title":"Axion Monodromy and the Weak Gravity Conjecture","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"hep-th","authors_text":"Alexander Westphal, Arthur Hebecker, Fabrizio Rompineve","submitted_at":"2015-12-11T19:38:37Z","abstract_excerpt":"Axions with broken discrete shift symmetry (axion monodromy) have recently played a central role both in the discussion of inflation and the `relaxion' approach to the hierarchy problem. We suggest a very minimalist way to constrain such models by the weak gravity conjecture for domain walls: While the electric side of the conjecture is always satisfied if the cosine-oscillations of the axion potential are sufficiently small, the magnetic side imposes a cutoff, $\\Lambda^3 \\sim m f M_{pl}$, independent of the height of these `wiggles'. We compare our approach with the recent related proposal by"},"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":"1512.03768","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2015-12-11T19:38:37Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"33d62e2ab3e74a4870b195d93d2a5dcf7c46d2ea0d7128f856efa491f246f951","abstract_canon_sha256":"1325eb14596ddbd372bc913a6e6ba79bdc5ed627098517a3dda7c676d69c56ba"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:10:45.796360Z","signature_b64":"hLyvMcE+dF69bxOrQTE/Ohmx7E7P6gd/wc6/aIOZM/ZF5/daR4YqhavFbq1tAYRa7e1+yk68A3bN52LznESBAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"77a5aa015acb0a04ebb2b708f69dd53a9e207b1b09d07b52a9d13bea4d75cdf7","last_reissued_at":"2026-05-18T01:10:45.795852Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:10:45.795852Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Axion Monodromy and the Weak Gravity Conjecture","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"hep-th","authors_text":"Alexander Westphal, Arthur Hebecker, Fabrizio Rompineve","submitted_at":"2015-12-11T19:38:37Z","abstract_excerpt":"Axions with broken discrete shift symmetry (axion monodromy) have recently played a central role both in the discussion of inflation and the `relaxion' approach to the hierarchy problem. We suggest a very minimalist way to constrain such models by the weak gravity conjecture for domain walls: While the electric side of the conjecture is always satisfied if the cosine-oscillations of the axion potential are sufficiently small, the magnetic side imposes a cutoff, $\\Lambda^3 \\sim m f M_{pl}$, independent of the height of these `wiggles'. We compare our approach with the recent related proposal by"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1512.03768","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":"1512.03768","created_at":"2026-05-18T01:10:45.795937+00:00"},{"alias_kind":"arxiv_version","alias_value":"1512.03768v3","created_at":"2026-05-18T01:10:45.795937+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1512.03768","created_at":"2026-05-18T01:10:45.795937+00:00"},{"alias_kind":"pith_short_12","alias_value":"O6S2UAK2ZMFA","created_at":"2026-05-18T12:29:34.919912+00:00"},{"alias_kind":"pith_short_16","alias_value":"O6S2UAK2ZMFAJ25S","created_at":"2026-05-18T12:29:34.919912+00:00"},{"alias_kind":"pith_short_8","alias_value":"O6S2UAK2","created_at":"2026-05-18T12:29:34.919912+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.22912","citing_title":"Sharpening the Supersymmetric Axion Weak Gravity Conjecture","ref_index":65,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/O6S2UAK2ZMFAJ25SW4EPNHOVHK","json":"https://pith.science/pith/O6S2UAK2ZMFAJ25SW4EPNHOVHK.json","graph_json":"https://pith.science/api/pith-number/O6S2UAK2ZMFAJ25SW4EPNHOVHK/graph.json","events_json":"https://pith.science/api/pith-number/O6S2UAK2ZMFAJ25SW4EPNHOVHK/events.json","paper":"https://pith.science/paper/O6S2UAK2"},"agent_actions":{"view_html":"https://pith.science/pith/O6S2UAK2ZMFAJ25SW4EPNHOVHK","download_json":"https://pith.science/pith/O6S2UAK2ZMFAJ25SW4EPNHOVHK.json","view_paper":"https://pith.science/paper/O6S2UAK2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1512.03768&json=true","fetch_graph":"https://pith.science/api/pith-number/O6S2UAK2ZMFAJ25SW4EPNHOVHK/graph.json","fetch_events":"https://pith.science/api/pith-number/O6S2UAK2ZMFAJ25SW4EPNHOVHK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/O6S2UAK2ZMFAJ25SW4EPNHOVHK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/O6S2UAK2ZMFAJ25SW4EPNHOVHK/action/storage_attestation","attest_author":"https://pith.science/pith/O6S2UAK2ZMFAJ25SW4EPNHOVHK/action/author_attestation","sign_citation":"https://pith.science/pith/O6S2UAK2ZMFAJ25SW4EPNHOVHK/action/citation_signature","submit_replication":"https://pith.science/pith/O6S2UAK2ZMFAJ25SW4EPNHOVHK/action/replication_record"}},"created_at":"2026-05-18T01:10:45.795937+00:00","updated_at":"2026-05-18T01:10:45.795937+00:00"}