{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:J2PQ42SHS4IMT3E6QCH6D7CX4S","short_pith_number":"pith:J2PQ42SH","schema_version":"1.0","canonical_sha256":"4e9f0e6a479710c9ec9e808fe1fc57e4b4e9c8a4a3d31c0d43407c9d880a85c6","source":{"kind":"arxiv","id":"1910.14051","version":2},"attestation_state":"computed","paper":{"title":"The Cosmological Bootstrap: Weight-Shifting Operators and Scalar Seeds","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Austin Joyce, Carlos Duaso Pueyo, Daniel Baumann, Guilherme L. Pimentel, Hayden Lee","submitted_at":"2019-10-30T18:00:04Z","abstract_excerpt":"A key insight of the bootstrap approach to cosmological correlations is the fact that all correlators of slow-roll inflation can be reduced to a unique building block---the four-point function of conformally coupled scalars, arising from the exchange of a massive scalar. Correlators corresponding to the exchange of particles with spin are then obtained by applying a spin-raising operator to the scalar-exchange solution. Similarly, the correlators of massless external fields can be derived by acting with a suitable weight-raising operator. In this paper, we present a systematic and highly strea"},"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":"1910.14051","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2019-10-30T18:00:04Z","cross_cats_sorted":["astro-ph.CO","gr-qc","hep-ph"],"title_canon_sha256":"2c74ebd6347e3d678cc2f8ec62430b64f857ebb39be455cc59553caaf0f001b9","abstract_canon_sha256":"b63a8d1bb2634702747fe916360b6fc2af88faf3002f09bee9daa761de4550d7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:11:39.342921Z","signature_b64":"wsXG1+D6LuADHnU3Lw7lXr/PIKwnyoGaEUcI6MXse4Jnsw+rM5tINoDjr/ihMIgzR9CelSwndHCieRc9QC24Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4e9f0e6a479710c9ec9e808fe1fc57e4b4e9c8a4a3d31c0d43407c9d880a85c6","last_reissued_at":"2026-07-05T02:11:39.342497Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:11:39.342497Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Cosmological Bootstrap: Weight-Shifting Operators and Scalar Seeds","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Austin Joyce, Carlos Duaso Pueyo, Daniel Baumann, Guilherme L. Pimentel, Hayden Lee","submitted_at":"2019-10-30T18:00:04Z","abstract_excerpt":"A key insight of the bootstrap approach to cosmological correlations is the fact that all correlators of slow-roll inflation can be reduced to a unique building block---the four-point function of conformally coupled scalars, arising from the exchange of a massive scalar. Correlators corresponding to the exchange of particles with spin are then obtained by applying a spin-raising operator to the scalar-exchange solution. Similarly, the correlators of massless external fields can be derived by acting with a suitable weight-raising operator. In this paper, we present a systematic and highly strea"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1910.14051","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/1910.14051/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":"1910.14051","created_at":"2026-07-05T02:11:39.342551+00:00"},{"alias_kind":"arxiv_version","alias_value":"1910.14051v2","created_at":"2026-07-05T02:11:39.342551+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1910.14051","created_at":"2026-07-05T02:11:39.342551+00:00"},{"alias_kind":"pith_short_12","alias_value":"J2PQ42SHS4IM","created_at":"2026-07-05T02:11:39.342551+00:00"},{"alias_kind":"pith_short_16","alias_value":"J2PQ42SHS4IMT3E6","created_at":"2026-07-05T02:11:39.342551+00:00"},{"alias_kind":"pith_short_8","alias_value":"J2PQ42SH","created_at":"2026-07-05T02:11:39.342551+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":28,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.05327","citing_title":"Cosmological Correlators in KLF and the Double-Exchange","ref_index":3,"is_internal_anchor":true},{"citing_arxiv_id":"2606.26221","citing_title":"De Sitter Representations","ref_index":17,"is_internal_anchor":false},{"citing_arxiv_id":"2606.27311","citing_title":"Massive Cosmological Correlators from Flat Space: a Laplace-Space Approach","ref_index":3,"is_internal_anchor":false},{"citing_arxiv_id":"2606.27309","citing_title":"Laplace Space for Cosmological Correlators","ref_index":3,"is_internal_anchor":false},{"citing_arxiv_id":"2606.06282","citing_title":"On Cosmological Correlators with Boundary Contributions","ref_index":4,"is_internal_anchor":false},{"citing_arxiv_id":"2606.05289","citing_title":"Unitarity, Recursion and Soft Limits in (EA)dS through Dressing","ref_index":2,"is_internal_anchor":false},{"citing_arxiv_id":"2606.02686","citing_title":"On-Shell Bootstrap of Loop Inflation Correlators with Spectral Dispersion","ref_index":63,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21581","citing_title":"Cosmological Collider in the Grassmannian","ref_index":22,"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":60,"is_internal_anchor":false},{"citing_arxiv_id":"2605.30475","citing_title":"Cosmological Weight-Shifting Matrices","ref_index":15,"is_internal_anchor":false},{"citing_arxiv_id":"2503.17840","citing_title":"Strongly Coupled Sectors in Inflation: Gapless Theories and Unparticles","ref_index":13,"is_internal_anchor":false},{"citing_arxiv_id":"2505.16071","citing_title":"A Match Made in Heaven: Linking Observables in Inflationary Cosmology","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21581","citing_title":"Cosmological Collider in the Grassmannian","ref_index":15,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21419","citing_title":"Cosmological Collider Signatures from Right-Handed Neutrino Loop","ref_index":26,"is_internal_anchor":false},{"citing_arxiv_id":"2605.17751","citing_title":"An Alternative Viewpoint on Kinematic Flow from Tubing Splitting","ref_index":23,"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":105,"is_internal_anchor":false},{"citing_arxiv_id":"2512.23796","citing_title":"Strongly Coupled Sectors in Inflation: Gapped Theories of Unparticles","ref_index":53,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26421","citing_title":"On the simplicity of de Sitter correlators","ref_index":15,"is_internal_anchor":false},{"citing_arxiv_id":"2604.22918","citing_title":"Kinematic Flow for Banana Loops and Unparticles","ref_index":10,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08658","citing_title":"Differential Equations for Massive Correlators","ref_index":22,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08512","citing_title":"Beyond Discontinuities: Cosmological WFCs and the Supersymmetric Orthogonal Grassmannian","ref_index":3,"is_internal_anchor":false},{"citing_arxiv_id":"2604.07503","citing_title":"Super-Grassmannians for $\\mathcal{N}=2$ to $4$ SCFT$_3$: From AdS$_4$ Correlators to $\\mathcal{N}=4$ SYM scattering Amplitudes","ref_index":17,"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":79,"is_internal_anchor":false},{"citing_arxiv_id":"2604.07446","citing_title":"The $\\mathcal{N}=1$ Super-Grassmannian for CFT$_3$ and a Foray on AdS and Cosmological Correlators","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2605.06811","citing_title":"The Conformal Grassmannian: A Symplectic Bi-Grassmannian for $CFT_ 4$ Correlators","ref_index":10,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/J2PQ42SHS4IMT3E6QCH6D7CX4S","json":"https://pith.science/pith/J2PQ42SHS4IMT3E6QCH6D7CX4S.json","graph_json":"https://pith.science/api/pith-number/J2PQ42SHS4IMT3E6QCH6D7CX4S/graph.json","events_json":"https://pith.science/api/pith-number/J2PQ42SHS4IMT3E6QCH6D7CX4S/events.json","paper":"https://pith.science/paper/J2PQ42SH"},"agent_actions":{"view_html":"https://pith.science/pith/J2PQ42SHS4IMT3E6QCH6D7CX4S","download_json":"https://pith.science/pith/J2PQ42SHS4IMT3E6QCH6D7CX4S.json","view_paper":"https://pith.science/paper/J2PQ42SH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1910.14051&json=true","fetch_graph":"https://pith.science/api/pith-number/J2PQ42SHS4IMT3E6QCH6D7CX4S/graph.json","fetch_events":"https://pith.science/api/pith-number/J2PQ42SHS4IMT3E6QCH6D7CX4S/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/J2PQ42SHS4IMT3E6QCH6D7CX4S/action/timestamp_anchor","attest_storage":"https://pith.science/pith/J2PQ42SHS4IMT3E6QCH6D7CX4S/action/storage_attestation","attest_author":"https://pith.science/pith/J2PQ42SHS4IMT3E6QCH6D7CX4S/action/author_attestation","sign_citation":"https://pith.science/pith/J2PQ42SHS4IMT3E6QCH6D7CX4S/action/citation_signature","submit_replication":"https://pith.science/pith/J2PQ42SHS4IMT3E6QCH6D7CX4S/action/replication_record"}},"created_at":"2026-07-05T02:11:39.342551+00:00","updated_at":"2026-07-05T02:11:39.342551+00:00"}