{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:6G35MA5E3Y7CQSQJD6BKDBLAAY","short_pith_number":"pith:6G35MA5E","schema_version":"1.0","canonical_sha256":"f1b7d603a4de3e284a091f82a18560060473b721a8ec6fb255beea4e068aa7bd","source":{"kind":"arxiv","id":"1412.1814","version":1},"attestation_state":"computed","paper":{"title":"Drifting Oscillations in Axion Monodromy","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, Eva Silverstein, Liam McAllister, Raphael Flauger","submitted_at":"2014-12-04T20:53:02Z","abstract_excerpt":"We study the pattern of oscillations in the primordial power spectrum in axion monodromy inflation, accounting for drifts in the oscillation period that can be important for comparing to cosmological data. In these models the potential energy has a monomial form over a super-Planckian field range, with superimposed modulations whose size is model-dependent. The amplitude and frequency of the modulations are set by the expectation values of moduli fields. We show that during the course of inflation, the diminishing energy density can induce slow adjustments of the moduli, changing the modulatio"},"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":"1412.1814","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2014-12-04T20:53:02Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"6345a07f1ec343cd4a7a49590818d1d1924ce0861836536f32601ae0a22582b8","abstract_canon_sha256":"a21fce88e21477fb649d16cb95e6ead27b85f06fbb3f35e26da1eeae8924a3d8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:30:49.608306Z","signature_b64":"ZDT4VdT6E6ZlQv1R2Df/sMPhsCTGbqDXLrJBfuE5on48fEvDIOumHIDUE5QaUS9RRxwAluq/tZ5VZZM9Zeq9Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f1b7d603a4de3e284a091f82a18560060473b721a8ec6fb255beea4e068aa7bd","last_reissued_at":"2026-05-18T00:30:49.607721Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:30:49.607721Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Drifting Oscillations in Axion Monodromy","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, Eva Silverstein, Liam McAllister, Raphael Flauger","submitted_at":"2014-12-04T20:53:02Z","abstract_excerpt":"We study the pattern of oscillations in the primordial power spectrum in axion monodromy inflation, accounting for drifts in the oscillation period that can be important for comparing to cosmological data. In these models the potential energy has a monomial form over a super-Planckian field range, with superimposed modulations whose size is model-dependent. The amplitude and frequency of the modulations are set by the expectation values of moduli fields. We show that during the course of inflation, the diminishing energy density can induce slow adjustments of the moduli, changing the modulatio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1412.1814","kind":"arxiv","version":1},"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":"1412.1814","created_at":"2026-05-18T00:30:49.607803+00:00"},{"alias_kind":"arxiv_version","alias_value":"1412.1814v1","created_at":"2026-05-18T00:30:49.607803+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1412.1814","created_at":"2026-05-18T00:30:49.607803+00:00"},{"alias_kind":"pith_short_12","alias_value":"6G35MA5E3Y7C","created_at":"2026-05-18T12:28:16.859392+00:00"},{"alias_kind":"pith_short_16","alias_value":"6G35MA5E3Y7CQSQJ","created_at":"2026-05-18T12:28:16.859392+00:00"},{"alias_kind":"pith_short_8","alias_value":"6G35MA5E","created_at":"2026-05-18T12:28:16.859392+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2605.18615","citing_title":"Primordial power spectrum reconstructions from BOSS + eBOSS","ref_index":15,"is_internal_anchor":true},{"citing_arxiv_id":"2509.02539","citing_title":"Extending the Dynamical Systems Toolkit: Coupled Fields in Multiscalar Dark Energy","ref_index":44,"is_internal_anchor":true},{"citing_arxiv_id":"2511.00152","citing_title":"Every Wrinkle Carries A Memory: An Integro-differential Bootstrap for Features in Cosmological Correlators","ref_index":106,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6G35MA5E3Y7CQSQJD6BKDBLAAY","json":"https://pith.science/pith/6G35MA5E3Y7CQSQJD6BKDBLAAY.json","graph_json":"https://pith.science/api/pith-number/6G35MA5E3Y7CQSQJD6BKDBLAAY/graph.json","events_json":"https://pith.science/api/pith-number/6G35MA5E3Y7CQSQJD6BKDBLAAY/events.json","paper":"https://pith.science/paper/6G35MA5E"},"agent_actions":{"view_html":"https://pith.science/pith/6G35MA5E3Y7CQSQJD6BKDBLAAY","download_json":"https://pith.science/pith/6G35MA5E3Y7CQSQJD6BKDBLAAY.json","view_paper":"https://pith.science/paper/6G35MA5E","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1412.1814&json=true","fetch_graph":"https://pith.science/api/pith-number/6G35MA5E3Y7CQSQJD6BKDBLAAY/graph.json","fetch_events":"https://pith.science/api/pith-number/6G35MA5E3Y7CQSQJD6BKDBLAAY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6G35MA5E3Y7CQSQJD6BKDBLAAY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6G35MA5E3Y7CQSQJD6BKDBLAAY/action/storage_attestation","attest_author":"https://pith.science/pith/6G35MA5E3Y7CQSQJD6BKDBLAAY/action/author_attestation","sign_citation":"https://pith.science/pith/6G35MA5E3Y7CQSQJD6BKDBLAAY/action/citation_signature","submit_replication":"https://pith.science/pith/6G35MA5E3Y7CQSQJD6BKDBLAAY/action/replication_record"}},"created_at":"2026-05-18T00:30:49.607803+00:00","updated_at":"2026-05-18T00:30:49.607803+00:00"}