{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:S2PBTY7LTKJR5A6I4D77T2W6L7","short_pith_number":"pith:S2PBTY7L","schema_version":"1.0","canonical_sha256":"969e19e3eb9a931e83c8e0fff9eade5fd8c291993f52568b8f1edee4b265adf9","source":{"kind":"arxiv","id":"1409.1225","version":1},"attestation_state":"computed","paper":{"title":"Redshift Space Distortions in the Effective Field Theory of Large Scale Structures","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Leonardo Senatore, Matias Zaldarriaga","submitted_at":"2014-09-03T20:00:05Z","abstract_excerpt":"We introduce a formalism, valid both for dark matter and collapsed objects, that allows us to describe redshift space distortions in the context of the Effective Field Theory of Large Scale Structures (EFTofLSS). Expressing density perturbations in redshift space corresponds to performing a change of coordinates and the resulting expressions contain products of density perturbations and velocity fields evaluated at the same location. These terms are sensitive to non-perturbative short-distance physics and in order to correctly treat them they need to be renormalized by adding suitable countert"},"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":"1409.1225","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-09-03T20:00:05Z","cross_cats_sorted":["gr-qc","hep-ph","hep-th"],"title_canon_sha256":"d7908b0e5e5ff3e27f438405dd48f86585533efbb05acc60036110fce1624fff","abstract_canon_sha256":"8ba678f4cee1a69b86de2b9212a6f91f487a721e4c27ad663f692b50d9425cc5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:43:25.731217Z","signature_b64":"A7vku97a5jLdlyJ0KevNVso0DIRdLAs5Ej4WJ6YgUfbhpxU6Mwc61lI6gy6wRAVi7XwnC5L65jq9KKrdpP3LDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"969e19e3eb9a931e83c8e0fff9eade5fd8c291993f52568b8f1edee4b265adf9","last_reissued_at":"2026-05-18T02:43:25.730411Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:43:25.730411Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Redshift Space Distortions in the Effective Field Theory of Large Scale Structures","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Leonardo Senatore, Matias Zaldarriaga","submitted_at":"2014-09-03T20:00:05Z","abstract_excerpt":"We introduce a formalism, valid both for dark matter and collapsed objects, that allows us to describe redshift space distortions in the context of the Effective Field Theory of Large Scale Structures (EFTofLSS). Expressing density perturbations in redshift space corresponds to performing a change of coordinates and the resulting expressions contain products of density perturbations and velocity fields evaluated at the same location. These terms are sensitive to non-perturbative short-distance physics and in order to correctly treat them they need to be renormalized by adding suitable countert"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1409.1225","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":"1409.1225","created_at":"2026-05-18T02:43:25.730557+00:00"},{"alias_kind":"arxiv_version","alias_value":"1409.1225v1","created_at":"2026-05-18T02:43:25.730557+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1409.1225","created_at":"2026-05-18T02:43:25.730557+00:00"},{"alias_kind":"pith_short_12","alias_value":"S2PBTY7LTKJR","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_16","alias_value":"S2PBTY7LTKJR5A6I","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_8","alias_value":"S2PBTY7L","created_at":"2026-05-18T12:28:46.137349+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2408.03036","citing_title":"Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study","ref_index":31,"is_internal_anchor":true},{"citing_arxiv_id":"2411.12021","citing_title":"DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars","ref_index":44,"is_internal_anchor":true},{"citing_arxiv_id":"2511.20757","citing_title":"Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses","ref_index":79,"is_internal_anchor":true},{"citing_arxiv_id":"2604.25171","citing_title":"Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS","ref_index":4,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25171","citing_title":"Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS","ref_index":4,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/S2PBTY7LTKJR5A6I4D77T2W6L7","json":"https://pith.science/pith/S2PBTY7LTKJR5A6I4D77T2W6L7.json","graph_json":"https://pith.science/api/pith-number/S2PBTY7LTKJR5A6I4D77T2W6L7/graph.json","events_json":"https://pith.science/api/pith-number/S2PBTY7LTKJR5A6I4D77T2W6L7/events.json","paper":"https://pith.science/paper/S2PBTY7L"},"agent_actions":{"view_html":"https://pith.science/pith/S2PBTY7LTKJR5A6I4D77T2W6L7","download_json":"https://pith.science/pith/S2PBTY7LTKJR5A6I4D77T2W6L7.json","view_paper":"https://pith.science/paper/S2PBTY7L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1409.1225&json=true","fetch_graph":"https://pith.science/api/pith-number/S2PBTY7LTKJR5A6I4D77T2W6L7/graph.json","fetch_events":"https://pith.science/api/pith-number/S2PBTY7LTKJR5A6I4D77T2W6L7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/S2PBTY7LTKJR5A6I4D77T2W6L7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/S2PBTY7LTKJR5A6I4D77T2W6L7/action/storage_attestation","attest_author":"https://pith.science/pith/S2PBTY7LTKJR5A6I4D77T2W6L7/action/author_attestation","sign_citation":"https://pith.science/pith/S2PBTY7LTKJR5A6I4D77T2W6L7/action/citation_signature","submit_replication":"https://pith.science/pith/S2PBTY7LTKJR5A6I4D77T2W6L7/action/replication_record"}},"created_at":"2026-05-18T02:43:25.730557+00:00","updated_at":"2026-05-18T02:43:25.730557+00:00"}