{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:4IY7VDU7TGOPQ6RN2BSPXJRB3L","short_pith_number":"pith:4IY7VDU7","schema_version":"1.0","canonical_sha256":"e231fa8e9f999cf87a2dd064fba621dae7fb9788215942b6b7384b098d99c68e","source":{"kind":"arxiv","id":"0809.1100","version":2},"attestation_state":"computed","paper":{"title":"Stochastic tunneling for strongly non-Gaussian inflationary theories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Andrew J. Tolley, Mark Wyman","submitted_at":"2008-09-06T00:29:39Z","abstract_excerpt":"We reconsider the dynamics of stochastic or thermal tunneling in theories like Dirac-Born-Infeld inflation that have non-minimal kinetic terms and, as a result, strongly non-Gaussian perturbations. We first describe a local description of the tunneling process which gives results consistent with the standard Hawking-Moss tunneling. This result is under perturbative control as long as the fluctuation determinant is well approximated by a one-loop integral. We then move to a global description, using the methodology of stochastic inflation and the in-in path integral formalism. This approach sho"},"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":"0809.1100","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2008-09-06T00:29:39Z","cross_cats_sorted":[],"title_canon_sha256":"37d98469c1dafd6275026fd3057f47312d6d77a189ff8612a56bdb36f348e9ae","abstract_canon_sha256":"f5dd3d8cee67e49c39764919cda98dbc7546307fb33ffbc25320aa2261e8d79a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:24:35.443397Z","signature_b64":"/7Raqz7N6HTxtVNkxK40SGFKCTKuDC1zkWNzdOcXJiTZ+OF2KSkCKfH1UasBGo1I4L/Fs6w9thRWwn6wnQo8Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e231fa8e9f999cf87a2dd064fba621dae7fb9788215942b6b7384b098d99c68e","last_reissued_at":"2026-05-18T04:24:35.442987Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:24:35.442987Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stochastic tunneling for strongly non-Gaussian inflationary theories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Andrew J. Tolley, Mark Wyman","submitted_at":"2008-09-06T00:29:39Z","abstract_excerpt":"We reconsider the dynamics of stochastic or thermal tunneling in theories like Dirac-Born-Infeld inflation that have non-minimal kinetic terms and, as a result, strongly non-Gaussian perturbations. We first describe a local description of the tunneling process which gives results consistent with the standard Hawking-Moss tunneling. This result is under perturbative control as long as the fluctuation determinant is well approximated by a one-loop integral. We then move to a global description, using the methodology of stochastic inflation and the in-in path integral formalism. This approach sho"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0809.1100","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":"0809.1100","created_at":"2026-05-18T04:24:35.443051+00:00"},{"alias_kind":"arxiv_version","alias_value":"0809.1100v2","created_at":"2026-05-18T04:24:35.443051+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0809.1100","created_at":"2026-05-18T04:24:35.443051+00:00"},{"alias_kind":"pith_short_12","alias_value":"4IY7VDU7TGOP","created_at":"2026-05-18T12:25:56.245647+00:00"},{"alias_kind":"pith_short_16","alias_value":"4IY7VDU7TGOPQ6RN","created_at":"2026-05-18T12:25:56.245647+00:00"},{"alias_kind":"pith_short_8","alias_value":"4IY7VDU7","created_at":"2026-05-18T12:25:56.245647+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.02070","citing_title":"Stochastic inflation as an open quantum system","ref_index":64,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4IY7VDU7TGOPQ6RN2BSPXJRB3L","json":"https://pith.science/pith/4IY7VDU7TGOPQ6RN2BSPXJRB3L.json","graph_json":"https://pith.science/api/pith-number/4IY7VDU7TGOPQ6RN2BSPXJRB3L/graph.json","events_json":"https://pith.science/api/pith-number/4IY7VDU7TGOPQ6RN2BSPXJRB3L/events.json","paper":"https://pith.science/paper/4IY7VDU7"},"agent_actions":{"view_html":"https://pith.science/pith/4IY7VDU7TGOPQ6RN2BSPXJRB3L","download_json":"https://pith.science/pith/4IY7VDU7TGOPQ6RN2BSPXJRB3L.json","view_paper":"https://pith.science/paper/4IY7VDU7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0809.1100&json=true","fetch_graph":"https://pith.science/api/pith-number/4IY7VDU7TGOPQ6RN2BSPXJRB3L/graph.json","fetch_events":"https://pith.science/api/pith-number/4IY7VDU7TGOPQ6RN2BSPXJRB3L/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4IY7VDU7TGOPQ6RN2BSPXJRB3L/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4IY7VDU7TGOPQ6RN2BSPXJRB3L/action/storage_attestation","attest_author":"https://pith.science/pith/4IY7VDU7TGOPQ6RN2BSPXJRB3L/action/author_attestation","sign_citation":"https://pith.science/pith/4IY7VDU7TGOPQ6RN2BSPXJRB3L/action/citation_signature","submit_replication":"https://pith.science/pith/4IY7VDU7TGOPQ6RN2BSPXJRB3L/action/replication_record"}},"created_at":"2026-05-18T04:24:35.443051+00:00","updated_at":"2026-05-18T04:24:35.443051+00:00"}