{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:DLXNDF2DV4IVVUQZGMDRHFG3CW","short_pith_number":"pith:DLXNDF2D","schema_version":"1.0","canonical_sha256":"1aeed19743af115ad21933071394db15be805e6c081711524ccb48964f078e33","source":{"kind":"arxiv","id":"2410.11973","version":2},"attestation_state":"computed","paper":{"title":"Soft Metric Fluctuations During Inflation","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Daniel Green, Kshitij Gupta","submitted_at":"2024-10-15T18:24:51Z","abstract_excerpt":"The conservation of the long wavelength fluctuations of the metric plays a vital role in cosmology as the link between quantum fluctuations during inflation and late time observations. This is a well-known property of the classical evolution equations, but demonstrating that it is robust to quantum correction involves a number of technical arguments. In this paper, we will use effective field theory (EFT) techniques to demonstrate the all orders conservation of the super-horizon scalar and tensor fluctuations of the metric during inflation. We show how to construct an EFT for these soft modes,"},"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":"2410.11973","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2024-10-15T18:24:51Z","cross_cats_sorted":["astro-ph.CO","gr-qc","hep-ph"],"title_canon_sha256":"9c8748dcbd1651d28137258eb00a31d09bf7bffe5a3b84675422cc4643f602b7","abstract_canon_sha256":"711c08c754fbf8472f6c8cb379c95079401ac73b05968d24f0c8d5e10d97b1da"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:09:49.019643Z","signature_b64":"C02RHeNlIkNEAs2TbrczvreZevvU34WpQjBWXFq6T58IFu3tPmRc5mE79o1osKPl9b6bX7Xeozfco+8uoFwYBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1aeed19743af115ad21933071394db15be805e6c081711524ccb48964f078e33","last_reissued_at":"2026-07-05T10:09:49.019173Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:09:49.019173Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Soft Metric Fluctuations During Inflation","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Daniel Green, Kshitij Gupta","submitted_at":"2024-10-15T18:24:51Z","abstract_excerpt":"The conservation of the long wavelength fluctuations of the metric plays a vital role in cosmology as the link between quantum fluctuations during inflation and late time observations. This is a well-known property of the classical evolution equations, but demonstrating that it is robust to quantum correction involves a number of technical arguments. In this paper, we will use effective field theory (EFT) techniques to demonstrate the all orders conservation of the super-horizon scalar and tensor fluctuations of the metric during inflation. We show how to construct an EFT for these soft modes,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2410.11973","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2410.11973/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2410.11973","created_at":"2026-07-05T10:09:49.019229+00:00"},{"alias_kind":"arxiv_version","alias_value":"2410.11973v2","created_at":"2026-07-05T10:09:49.019229+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2410.11973","created_at":"2026-07-05T10:09:49.019229+00:00"},{"alias_kind":"pith_short_12","alias_value":"DLXNDF2DV4IV","created_at":"2026-07-05T10:09:49.019229+00:00"},{"alias_kind":"pith_short_16","alias_value":"DLXNDF2DV4IVVUQZ","created_at":"2026-07-05T10:09:49.019229+00:00"},{"alias_kind":"pith_short_8","alias_value":"DLXNDF2D","created_at":"2026-07-05T10:09:49.019229+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06679","citing_title":"Classical conformal invariance and superhorizon dynamics in de Sitter","ref_index":13,"is_internal_anchor":true},{"citing_arxiv_id":"2508.08359","citing_title":"A Compact Story of Positivity in de Sitter","ref_index":105,"is_internal_anchor":false},{"citing_arxiv_id":"2509.02696","citing_title":"Unitary and Analytic Renormalisation of Cosmological Correlators","ref_index":37,"is_internal_anchor":false},{"citing_arxiv_id":"2512.20467","citing_title":"Finite parts of inflationary loops II: A streamlined UV in-in algorithm and distinguishable signatures","ref_index":47,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DLXNDF2DV4IVVUQZGMDRHFG3CW","json":"https://pith.science/pith/DLXNDF2DV4IVVUQZGMDRHFG3CW.json","graph_json":"https://pith.science/api/pith-number/DLXNDF2DV4IVVUQZGMDRHFG3CW/graph.json","events_json":"https://pith.science/api/pith-number/DLXNDF2DV4IVVUQZGMDRHFG3CW/events.json","paper":"https://pith.science/paper/DLXNDF2D"},"agent_actions":{"view_html":"https://pith.science/pith/DLXNDF2DV4IVVUQZGMDRHFG3CW","download_json":"https://pith.science/pith/DLXNDF2DV4IVVUQZGMDRHFG3CW.json","view_paper":"https://pith.science/paper/DLXNDF2D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2410.11973&json=true","fetch_graph":"https://pith.science/api/pith-number/DLXNDF2DV4IVVUQZGMDRHFG3CW/graph.json","fetch_events":"https://pith.science/api/pith-number/DLXNDF2DV4IVVUQZGMDRHFG3CW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DLXNDF2DV4IVVUQZGMDRHFG3CW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DLXNDF2DV4IVVUQZGMDRHFG3CW/action/storage_attestation","attest_author":"https://pith.science/pith/DLXNDF2DV4IVVUQZGMDRHFG3CW/action/author_attestation","sign_citation":"https://pith.science/pith/DLXNDF2DV4IVVUQZGMDRHFG3CW/action/citation_signature","submit_replication":"https://pith.science/pith/DLXNDF2DV4IVVUQZGMDRHFG3CW/action/replication_record"}},"created_at":"2026-07-05T10:09:49.019229+00:00","updated_at":"2026-07-05T10:09:49.019229+00:00"}