{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:PY5X4EI3OENXYD7GWR6A2CLZSR","short_pith_number":"pith:PY5X4EI3","schema_version":"1.0","canonical_sha256":"7e3b7e111b711b7c0fe6b47c0d0979944196832303fddb456d7f087d8a3475d4","source":{"kind":"arxiv","id":"2205.10340","version":2},"attestation_state":"computed","paper":{"title":"Cosmological Bootstrap in Slow Motion","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-th","authors_text":"Sadra Jazayeri, S\\'ebastien Renaux-Petel","submitted_at":"2022-05-20T17:52:39Z","abstract_excerpt":"Speed matters. How the masses and spins of new particles active during inflation can be read off from the statistical properties of primordial density fluctuations is well understood. However, not when the propagation speeds of the new degrees of freedom and of the curvature perturbation differ, which is the generic situation in the effective field theory of inflationary fluctuations. Here we use bootstrap techniques to find exact analytical solutions for primordial 2-,3- and 4-point correlators in this context. We focus on the imprints of a heavy relativistic scalar coupled to the curvature p"},"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":"2205.10340","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2022-05-20T17:52:39Z","cross_cats_sorted":["astro-ph.CO","gr-qc"],"title_canon_sha256":"67580423aadb5d1e12dc453d1c337fe24b7eb840ea22074db777a585b29ec599","abstract_canon_sha256":"8886964ffe0895c8372291d492efd17f97a7613835a8c1976eacf1d55186477a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:39:12.986143Z","signature_b64":"1Fr86s3OBTm/bMn7KwbH7AsfQGSQKIjYisemjJFLt19zf08SqgqkpyYD+CODjgexbb7qi37R8LEjEukDaQgMDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7e3b7e111b711b7c0fe6b47c0d0979944196832303fddb456d7f087d8a3475d4","last_reissued_at":"2026-07-05T10:39:12.985623Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:39:12.985623Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmological Bootstrap in Slow Motion","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-th","authors_text":"Sadra Jazayeri, S\\'ebastien Renaux-Petel","submitted_at":"2022-05-20T17:52:39Z","abstract_excerpt":"Speed matters. How the masses and spins of new particles active during inflation can be read off from the statistical properties of primordial density fluctuations is well understood. However, not when the propagation speeds of the new degrees of freedom and of the curvature perturbation differ, which is the generic situation in the effective field theory of inflationary fluctuations. Here we use bootstrap techniques to find exact analytical solutions for primordial 2-,3- and 4-point correlators in this context. We focus on the imprints of a heavy relativistic scalar coupled to the curvature p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2205.10340","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/2205.10340/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":"2205.10340","created_at":"2026-07-05T10:39:12.985682+00:00"},{"alias_kind":"arxiv_version","alias_value":"2205.10340v2","created_at":"2026-07-05T10:39:12.985682+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2205.10340","created_at":"2026-07-05T10:39:12.985682+00:00"},{"alias_kind":"pith_short_12","alias_value":"PY5X4EI3OENX","created_at":"2026-07-05T10:39:12.985682+00:00"},{"alias_kind":"pith_short_16","alias_value":"PY5X4EI3OENXYD7G","created_at":"2026-07-05T10:39:12.985682+00:00"},{"alias_kind":"pith_short_8","alias_value":"PY5X4EI3","created_at":"2026-07-05T10:39:12.985682+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":19,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.05327","citing_title":"Cosmological Correlators in KLF and the Double-Exchange","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2606.27311","citing_title":"Massive Cosmological Correlators from Flat Space: a Laplace-Space Approach","ref_index":7,"is_internal_anchor":false},{"citing_arxiv_id":"2606.27309","citing_title":"Laplace Space for Cosmological Correlators","ref_index":6,"is_internal_anchor":false},{"citing_arxiv_id":"2606.06282","citing_title":"On Cosmological Correlators with Boundary Contributions","ref_index":54,"is_internal_anchor":false},{"citing_arxiv_id":"2606.02686","citing_title":"On-Shell Bootstrap of Loop Inflation Correlators with Spectral Dispersion","ref_index":65,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21581","citing_title":"Cosmological Collider in the Grassmannian","ref_index":3,"is_internal_anchor":false},{"citing_arxiv_id":"2605.28054","citing_title":"Fermionic Bubble Loop in Cosmological Collider Revisited: Exact signals from spectral and Mellin-Barnes methods","ref_index":64,"is_internal_anchor":false},{"citing_arxiv_id":"2605.30475","citing_title":"Cosmological Weight-Shifting Matrices","ref_index":2,"is_internal_anchor":false},{"citing_arxiv_id":"2412.05762","citing_title":"The UV Sensitivity of Axion Monodromy Inflation","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2505.16071","citing_title":"A Match Made in Heaven: Linking Observables in Inflationary Cosmology","ref_index":29,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21581","citing_title":"Cosmological Collider in the Grassmannian","ref_index":3,"is_internal_anchor":false},{"citing_arxiv_id":"2605.17751","citing_title":"An Alternative Viewpoint on Kinematic Flow from Tubing Splitting","ref_index":39,"is_internal_anchor":false},{"citing_arxiv_id":"2605.20102","citing_title":"Non-Relativistic Cosmological Collider Signals","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2511.00152","citing_title":"Every Wrinkle Carries A Memory: An Integro-differential Bootstrap for Features in Cosmological Correlators","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08658","citing_title":"Differential Equations for Massive Correlators","ref_index":27,"is_internal_anchor":false},{"citing_arxiv_id":"2604.07434","citing_title":"Scalars at the Cosmological Collider: Full Shapes of Tree Diagrams and Bispectrum Searches using Planck Data","ref_index":66,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06145","citing_title":"Massive Exchange and the Sign of the Equilateral Bispectrum","ref_index":79,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14549","citing_title":"Loop integrals in de Sitter spacetime: The parity-split IBP system and $\\mathrm{d}\\log$-form differential equations","ref_index":45,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15251","citing_title":"Kontorovich-Lebedev-Fourier Space for de Sitter Correlators","ref_index":41,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PY5X4EI3OENXYD7GWR6A2CLZSR","json":"https://pith.science/pith/PY5X4EI3OENXYD7GWR6A2CLZSR.json","graph_json":"https://pith.science/api/pith-number/PY5X4EI3OENXYD7GWR6A2CLZSR/graph.json","events_json":"https://pith.science/api/pith-number/PY5X4EI3OENXYD7GWR6A2CLZSR/events.json","paper":"https://pith.science/paper/PY5X4EI3"},"agent_actions":{"view_html":"https://pith.science/pith/PY5X4EI3OENXYD7GWR6A2CLZSR","download_json":"https://pith.science/pith/PY5X4EI3OENXYD7GWR6A2CLZSR.json","view_paper":"https://pith.science/paper/PY5X4EI3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2205.10340&json=true","fetch_graph":"https://pith.science/api/pith-number/PY5X4EI3OENXYD7GWR6A2CLZSR/graph.json","fetch_events":"https://pith.science/api/pith-number/PY5X4EI3OENXYD7GWR6A2CLZSR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PY5X4EI3OENXYD7GWR6A2CLZSR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PY5X4EI3OENXYD7GWR6A2CLZSR/action/storage_attestation","attest_author":"https://pith.science/pith/PY5X4EI3OENXYD7GWR6A2CLZSR/action/author_attestation","sign_citation":"https://pith.science/pith/PY5X4EI3OENXYD7GWR6A2CLZSR/action/citation_signature","submit_replication":"https://pith.science/pith/PY5X4EI3OENXYD7GWR6A2CLZSR/action/replication_record"}},"created_at":"2026-07-05T10:39:12.985682+00:00","updated_at":"2026-07-05T10:39:12.985682+00:00"}