{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:FYN4RICFXS5POQ6ZLRY22GD2ZS","short_pith_number":"pith:FYN4RICF","schema_version":"1.0","canonical_sha256":"2e1bc8a045bcbaf743d95c71ad187accadce2095c7bab4a98779c6d392a12bc4","source":{"kind":"arxiv","id":"1211.5482","version":1},"attestation_state":"computed","paper":{"title":"CMB from CFT","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-th","authors_text":"Ishan Mata, Sandip Trivedi, Suvrat Raju","submitted_at":"2012-11-23T12:21:48Z","abstract_excerpt":"During inflation, spacetime is approximately described by de Sitter space which is conformally invariant with the symmetry group SO(1,4). This symmetry can significantly constrain the quantum perturbations which arise in the inflationary epoch. We consider a general situation of single field inflation and show that the three point function involving two scalar modes and one tensor mode is uniquely determined, up to small corrections, by the conformal symmetries. Special conformal transformations play an important role in our analysis. Our result applies only to models where the inflaton sector"},"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":"1211.5482","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","primary_cat":"hep-th","submitted_at":"2012-11-23T12:21:48Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"2d2db33e96fdbff72602910bc44d56505bec49fbaf66e8963909f707d84cd6d7","abstract_canon_sha256":"d8c8c98ffb58954ac6678cbcc0b0a94ac4a65db07e22bda0c332d0312c1f6d44"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:08:38.231232Z","signature_b64":"BGd835pr4tVAx9v5VlYuWM58PP4KoIUVbf7im7QSipVJ8mjoVPQQvwUGHUzqBNH8Ff798waF7Vr5gRQlal38Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2e1bc8a045bcbaf743d95c71ad187accadce2095c7bab4a98779c6d392a12bc4","last_reissued_at":"2026-05-18T03:08:38.230708Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:08:38.230708Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CMB from CFT","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-th","authors_text":"Ishan Mata, Sandip Trivedi, Suvrat Raju","submitted_at":"2012-11-23T12:21:48Z","abstract_excerpt":"During inflation, spacetime is approximately described by de Sitter space which is conformally invariant with the symmetry group SO(1,4). This symmetry can significantly constrain the quantum perturbations which arise in the inflationary epoch. We consider a general situation of single field inflation and show that the three point function involving two scalar modes and one tensor mode is uniquely determined, up to small corrections, by the conformal symmetries. Special conformal transformations play an important role in our analysis. Our result applies only to models where the inflaton sector"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1211.5482","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":"1211.5482","created_at":"2026-05-18T03:08:38.230788+00:00"},{"alias_kind":"arxiv_version","alias_value":"1211.5482v1","created_at":"2026-05-18T03:08:38.230788+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1211.5482","created_at":"2026-05-18T03:08:38.230788+00:00"},{"alias_kind":"pith_short_12","alias_value":"FYN4RICFXS5P","created_at":"2026-05-18T12:27:06.952714+00:00"},{"alias_kind":"pith_short_16","alias_value":"FYN4RICFXS5POQ6Z","created_at":"2026-05-18T12:27:06.952714+00:00"},{"alias_kind":"pith_short_8","alias_value":"FYN4RICF","created_at":"2026-05-18T12:27:06.952714+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.17811","citing_title":"Medicine show: A Calogero model with principal series states","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2604.08512","citing_title":"Beyond Discontinuities: Cosmological WFCs from the Supersymmetric Orthogonal Grassmannian","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15251","citing_title":"Kontorovich-Lebedev-Fourier Space for de Sitter Correlators","ref_index":31,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FYN4RICFXS5POQ6ZLRY22GD2ZS","json":"https://pith.science/pith/FYN4RICFXS5POQ6ZLRY22GD2ZS.json","graph_json":"https://pith.science/api/pith-number/FYN4RICFXS5POQ6ZLRY22GD2ZS/graph.json","events_json":"https://pith.science/api/pith-number/FYN4RICFXS5POQ6ZLRY22GD2ZS/events.json","paper":"https://pith.science/paper/FYN4RICF"},"agent_actions":{"view_html":"https://pith.science/pith/FYN4RICFXS5POQ6ZLRY22GD2ZS","download_json":"https://pith.science/pith/FYN4RICFXS5POQ6ZLRY22GD2ZS.json","view_paper":"https://pith.science/paper/FYN4RICF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1211.5482&json=true","fetch_graph":"https://pith.science/api/pith-number/FYN4RICFXS5POQ6ZLRY22GD2ZS/graph.json","fetch_events":"https://pith.science/api/pith-number/FYN4RICFXS5POQ6ZLRY22GD2ZS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FYN4RICFXS5POQ6ZLRY22GD2ZS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FYN4RICFXS5POQ6ZLRY22GD2ZS/action/storage_attestation","attest_author":"https://pith.science/pith/FYN4RICFXS5POQ6ZLRY22GD2ZS/action/author_attestation","sign_citation":"https://pith.science/pith/FYN4RICFXS5POQ6ZLRY22GD2ZS/action/citation_signature","submit_replication":"https://pith.science/pith/FYN4RICFXS5POQ6ZLRY22GD2ZS/action/replication_record"}},"created_at":"2026-05-18T03:08:38.230788+00:00","updated_at":"2026-05-18T03:08:38.230788+00:00"}