{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:QP2XSU7M7A7PPKAIUJPZI5HK3R","short_pith_number":"pith:QP2XSU7M","schema_version":"1.0","canonical_sha256":"83f57953ecf83ef7a808a25f9474eadc66985d4abdff76c1ea2bf188d0b46caa","source":{"kind":"arxiv","id":"1512.06831","version":3},"attestation_state":"computed","paper":{"title":"On the EFT of Large Scale Structures in Redshift Space","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":"Cheng Zhao, Chia-Hsun Chuang, Francisco Prada, Leonardo Senatore, Matthew Lewandowski","submitted_at":"2015-12-21T20:55:10Z","abstract_excerpt":"We further develop the description of redshift space distortions within the Effective Field Theory of Large Scale Structures. First, we generalize the counterterms to include the effect of baryonic physics and primordial non-Gaussianity. Second, we evaluate the IR-resummation of the dark matter power spectrum in redshift space. This requires us to identify a controlled approximation that makes the numerical evaluation straightforward and efficient. Third, we compare the predictions of the theory at one loop with the power spectrum from numerical simulations up to $\\ell=6$. We find that the IR-"},"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":"1512.06831","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2015-12-21T20:55:10Z","cross_cats_sorted":["gr-qc","hep-ph","hep-th"],"title_canon_sha256":"a1c630b970cbe39f3a7db1cae45b18964e2acda1cc62b5b99da35857335d4a50","abstract_canon_sha256":"30cbd04287d96452a4ac8e2e4f435eacb824767323de8330e1dbf1aa3d7bd276"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:19:31.261345Z","signature_b64":"DIr2+y/6qyM8wGJyDo4Ve6bA+ES7vNIVzg6XRLKHkGINTBErvj2obxxW6oNNJhZ5lD1d5hhYpi4/OX6OaZHGDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"83f57953ecf83ef7a808a25f9474eadc66985d4abdff76c1ea2bf188d0b46caa","last_reissued_at":"2026-05-18T00:19:31.260841Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:19:31.260841Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the EFT of Large Scale Structures in Redshift Space","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":"Cheng Zhao, Chia-Hsun Chuang, Francisco Prada, Leonardo Senatore, Matthew Lewandowski","submitted_at":"2015-12-21T20:55:10Z","abstract_excerpt":"We further develop the description of redshift space distortions within the Effective Field Theory of Large Scale Structures. First, we generalize the counterterms to include the effect of baryonic physics and primordial non-Gaussianity. Second, we evaluate the IR-resummation of the dark matter power spectrum in redshift space. This requires us to identify a controlled approximation that makes the numerical evaluation straightforward and efficient. Third, we compare the predictions of the theory at one loop with the power spectrum from numerical simulations up to $\\ell=6$. We find that the IR-"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1512.06831","kind":"arxiv","version":3},"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":"1512.06831","created_at":"2026-05-18T00:19:31.260929+00:00"},{"alias_kind":"arxiv_version","alias_value":"1512.06831v3","created_at":"2026-05-18T00:19:31.260929+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1512.06831","created_at":"2026-05-18T00:19:31.260929+00:00"},{"alias_kind":"pith_short_12","alias_value":"QP2XSU7M7A7P","created_at":"2026-05-18T12:29:37.295048+00:00"},{"alias_kind":"pith_short_16","alias_value":"QP2XSU7M7A7PPKAI","created_at":"2026-05-18T12:29:37.295048+00:00"},{"alias_kind":"pith_short_8","alias_value":"QP2XSU7M","created_at":"2026-05-18T12:29:37.295048+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2408.03036","citing_title":"Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study","ref_index":34,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QP2XSU7M7A7PPKAIUJPZI5HK3R","json":"https://pith.science/pith/QP2XSU7M7A7PPKAIUJPZI5HK3R.json","graph_json":"https://pith.science/api/pith-number/QP2XSU7M7A7PPKAIUJPZI5HK3R/graph.json","events_json":"https://pith.science/api/pith-number/QP2XSU7M7A7PPKAIUJPZI5HK3R/events.json","paper":"https://pith.science/paper/QP2XSU7M"},"agent_actions":{"view_html":"https://pith.science/pith/QP2XSU7M7A7PPKAIUJPZI5HK3R","download_json":"https://pith.science/pith/QP2XSU7M7A7PPKAIUJPZI5HK3R.json","view_paper":"https://pith.science/paper/QP2XSU7M","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1512.06831&json=true","fetch_graph":"https://pith.science/api/pith-number/QP2XSU7M7A7PPKAIUJPZI5HK3R/graph.json","fetch_events":"https://pith.science/api/pith-number/QP2XSU7M7A7PPKAIUJPZI5HK3R/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QP2XSU7M7A7PPKAIUJPZI5HK3R/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QP2XSU7M7A7PPKAIUJPZI5HK3R/action/storage_attestation","attest_author":"https://pith.science/pith/QP2XSU7M7A7PPKAIUJPZI5HK3R/action/author_attestation","sign_citation":"https://pith.science/pith/QP2XSU7M7A7PPKAIUJPZI5HK3R/action/citation_signature","submit_replication":"https://pith.science/pith/QP2XSU7M7A7PPKAIUJPZI5HK3R/action/replication_record"}},"created_at":"2026-05-18T00:19:31.260929+00:00","updated_at":"2026-05-18T00:19:31.260929+00:00"}