{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:TBDJXXLUY45IQ6C3B7MOOUNEHN","short_pith_number":"pith:TBDJXXLU","schema_version":"1.0","canonical_sha256":"98469bdd74c73a88785b0fd8e751a43b5b02843161ffb0dfb76e3e647637f0fc","source":{"kind":"arxiv","id":"1010.4565","version":2},"attestation_state":"computed","paper":{"title":"Resonant Trispectrum and a Dozen More Primordial N-point functions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"hep-th","authors_text":"Enrico Pajer, Louis Leblond","submitted_at":"2010-10-21T20:00:02Z","abstract_excerpt":"We compute all N-point primordial curvature correlation functions from inflation at tree-level up to N of order ten or more depending on the choice of parameters. This is achieved for resonant inflationary models in which the inflaton potential has a periodic modulation on top of a slow-roll flat term. These models find a natural UV completion in string theory implementation of axion monodromy. Key to the success of our computation is the observation that gravitational interactions among the perturbations can be neglected, which we argue is justified for any model of inflation with parametrica"},"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":"1010.4565","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2010-10-21T20:00:02Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"8b09cf1405355dc446a1e3ce844332e92b1a74734e84c6629d0f31a3eb0a81e3","abstract_canon_sha256":"4a66f8454b3d977012166cb2405326eceae6f8810e2aec32126a95290d54cc36"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:21:10.659297Z","signature_b64":"jalpI+rf/30/pS7JbCk+OXAd4CoJJYule5mzOnXSLTSpBykrVEjel0O4ojXwKwPuASRRUQJoGGYGSArveDigAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"98469bdd74c73a88785b0fd8e751a43b5b02843161ffb0dfb76e3e647637f0fc","last_reissued_at":"2026-05-18T04:21:10.658643Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:21:10.658643Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Resonant Trispectrum and a Dozen More Primordial N-point functions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"hep-th","authors_text":"Enrico Pajer, Louis Leblond","submitted_at":"2010-10-21T20:00:02Z","abstract_excerpt":"We compute all N-point primordial curvature correlation functions from inflation at tree-level up to N of order ten or more depending on the choice of parameters. This is achieved for resonant inflationary models in which the inflaton potential has a periodic modulation on top of a slow-roll flat term. These models find a natural UV completion in string theory implementation of axion monodromy. Key to the success of our computation is the observation that gravitational interactions among the perturbations can be neglected, which we argue is justified for any model of inflation with parametrica"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1010.4565","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":"1010.4565","created_at":"2026-05-18T04:21:10.658741+00:00"},{"alias_kind":"arxiv_version","alias_value":"1010.4565v2","created_at":"2026-05-18T04:21:10.658741+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1010.4565","created_at":"2026-05-18T04:21:10.658741+00:00"},{"alias_kind":"pith_short_12","alias_value":"TBDJXXLUY45I","created_at":"2026-05-18T12:26:13.927090+00:00"},{"alias_kind":"pith_short_16","alias_value":"TBDJXXLUY45IQ6C3","created_at":"2026-05-18T12:26:13.927090+00:00"},{"alias_kind":"pith_short_8","alias_value":"TBDJXXLU","created_at":"2026-05-18T12:26:13.927090+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2412.05762","citing_title":"The UV Sensitivity of Axion Monodromy Inflation","ref_index":31,"is_internal_anchor":true},{"citing_arxiv_id":"2502.09481","citing_title":"Non-Perturbative Hamiltonian and Higher Loop Corrections in USR Inflation","ref_index":66,"is_internal_anchor":true},{"citing_arxiv_id":"2502.10287","citing_title":"Hamiltonians to all Orders in Perturbation Theory and Higher Loop Corrections in Single Field Inflation with PBHs Formation","ref_index":85,"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":102,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TBDJXXLUY45IQ6C3B7MOOUNEHN","json":"https://pith.science/pith/TBDJXXLUY45IQ6C3B7MOOUNEHN.json","graph_json":"https://pith.science/api/pith-number/TBDJXXLUY45IQ6C3B7MOOUNEHN/graph.json","events_json":"https://pith.science/api/pith-number/TBDJXXLUY45IQ6C3B7MOOUNEHN/events.json","paper":"https://pith.science/paper/TBDJXXLU"},"agent_actions":{"view_html":"https://pith.science/pith/TBDJXXLUY45IQ6C3B7MOOUNEHN","download_json":"https://pith.science/pith/TBDJXXLUY45IQ6C3B7MOOUNEHN.json","view_paper":"https://pith.science/paper/TBDJXXLU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1010.4565&json=true","fetch_graph":"https://pith.science/api/pith-number/TBDJXXLUY45IQ6C3B7MOOUNEHN/graph.json","fetch_events":"https://pith.science/api/pith-number/TBDJXXLUY45IQ6C3B7MOOUNEHN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TBDJXXLUY45IQ6C3B7MOOUNEHN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TBDJXXLUY45IQ6C3B7MOOUNEHN/action/storage_attestation","attest_author":"https://pith.science/pith/TBDJXXLUY45IQ6C3B7MOOUNEHN/action/author_attestation","sign_citation":"https://pith.science/pith/TBDJXXLUY45IQ6C3B7MOOUNEHN/action/citation_signature","submit_replication":"https://pith.science/pith/TBDJXXLUY45IQ6C3B7MOOUNEHN/action/replication_record"}},"created_at":"2026-05-18T04:21:10.658741+00:00","updated_at":"2026-05-18T04:21:10.658741+00:00"}