{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:NIFV6OLHTOOORRFU5ZDPLDNLZ3","short_pith_number":"pith:NIFV6OLH","schema_version":"1.0","canonical_sha256":"6a0b5f39679b9ce8c4b4ee46f58dabcec7fcc15dbab0d8344f02515c0f93675f","source":{"kind":"arxiv","id":"1501.05852","version":2},"attestation_state":"computed","paper":{"title":"Vacuum Fluctuations of a Scalar Field during Inflation: Quantum versus Stochastic Analysis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"V.K. Onemli","submitted_at":"2015-01-22T17:47:13Z","abstract_excerpt":"We consider an infrared truncated massless minimally coupled scalar field with a quartic self-interaction in the locally de Sitter background of an inflating universe. We compute the two-point correlation function of the scalar at one and two-loop order applying quantum field theory. The tree-order correlator at a fixed comoving separation (that is at increasing physical distance) freezes in to a nonzero value. At a fixed physical distance, it grows linearly with comoving time. The one-loop correlator, which is the dominant quantum correction, implies a negative temporal growth in the correlat"},"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":"1501.05852","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2015-01-22T17:47:13Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"f65cee308b693f34c05f16266b38704e11a12af4e9f537adad36807cf49dfd6e","abstract_canon_sha256":"1b7a2b16d861df680bb57c49c8df93f7cf6392ff6208826c0b9655351ded664d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:59:37.730569Z","signature_b64":"X8Ss/oHJbhEedToU0b9RHHX7lVgDpEgw4eLH16O+fmhQZUlnGjnxyUukjBbtPP798pshIVclYQ3URUv8b9e2BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6a0b5f39679b9ce8c4b4ee46f58dabcec7fcc15dbab0d8344f02515c0f93675f","last_reissued_at":"2026-05-18T01:59:37.729817Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:59:37.729817Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Vacuum Fluctuations of a Scalar Field during Inflation: Quantum versus Stochastic Analysis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"V.K. Onemli","submitted_at":"2015-01-22T17:47:13Z","abstract_excerpt":"We consider an infrared truncated massless minimally coupled scalar field with a quartic self-interaction in the locally de Sitter background of an inflating universe. We compute the two-point correlation function of the scalar at one and two-loop order applying quantum field theory. The tree-order correlator at a fixed comoving separation (that is at increasing physical distance) freezes in to a nonzero value. At a fixed physical distance, it grows linearly with comoving time. The one-loop correlator, which is the dominant quantum correction, implies a negative temporal growth in the correlat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.05852","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":"1501.05852","created_at":"2026-05-18T01:59:37.729943+00:00"},{"alias_kind":"arxiv_version","alias_value":"1501.05852v2","created_at":"2026-05-18T01:59:37.729943+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.05852","created_at":"2026-05-18T01:59:37.729943+00:00"},{"alias_kind":"pith_short_12","alias_value":"NIFV6OLHTOOO","created_at":"2026-05-18T12:29:32.376354+00:00"},{"alias_kind":"pith_short_16","alias_value":"NIFV6OLHTOOORRFU","created_at":"2026-05-18T12:29:32.376354+00:00"},{"alias_kind":"pith_short_8","alias_value":"NIFV6OLH","created_at":"2026-05-18T12:29:32.376354+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.18030","citing_title":"Yukawa scalar self energy at two loop and $\\langle \\phi^2 \\rangle$ in the inflationary de Sitter spacetime","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15219","citing_title":"Nonperturbative stochastic inflation in perturbative dynamical background","ref_index":95,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NIFV6OLHTOOORRFU5ZDPLDNLZ3","json":"https://pith.science/pith/NIFV6OLHTOOORRFU5ZDPLDNLZ3.json","graph_json":"https://pith.science/api/pith-number/NIFV6OLHTOOORRFU5ZDPLDNLZ3/graph.json","events_json":"https://pith.science/api/pith-number/NIFV6OLHTOOORRFU5ZDPLDNLZ3/events.json","paper":"https://pith.science/paper/NIFV6OLH"},"agent_actions":{"view_html":"https://pith.science/pith/NIFV6OLHTOOORRFU5ZDPLDNLZ3","download_json":"https://pith.science/pith/NIFV6OLHTOOORRFU5ZDPLDNLZ3.json","view_paper":"https://pith.science/paper/NIFV6OLH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1501.05852&json=true","fetch_graph":"https://pith.science/api/pith-number/NIFV6OLHTOOORRFU5ZDPLDNLZ3/graph.json","fetch_events":"https://pith.science/api/pith-number/NIFV6OLHTOOORRFU5ZDPLDNLZ3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NIFV6OLHTOOORRFU5ZDPLDNLZ3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NIFV6OLHTOOORRFU5ZDPLDNLZ3/action/storage_attestation","attest_author":"https://pith.science/pith/NIFV6OLHTOOORRFU5ZDPLDNLZ3/action/author_attestation","sign_citation":"https://pith.science/pith/NIFV6OLHTOOORRFU5ZDPLDNLZ3/action/citation_signature","submit_replication":"https://pith.science/pith/NIFV6OLHTOOORRFU5ZDPLDNLZ3/action/replication_record"}},"created_at":"2026-05-18T01:59:37.729943+00:00","updated_at":"2026-05-18T01:59:37.729943+00:00"}