{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:UR3IQIEMJO4KJTSLLVCT2YCEDT","short_pith_number":"pith:UR3IQIEM","schema_version":"1.0","canonical_sha256":"a47688208c4bb8a4ce4b5d453d60441cdb0fc73764fdefb0db6d74b8479175fd","source":{"kind":"arxiv","id":"2404.11471","version":1},"attestation_state":"computed","paper":{"title":"Non-linear power spectrum and forecasts for Generalized Cubic Covariant Galileon","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Baojiu Li, Benjamin Bose, Lu\\'is Atayde, Noemi Frusciante, Santiago Casas","submitted_at":"2024-04-17T15:24:09Z","abstract_excerpt":"To fully exploit the data from next generation surveys, we need an accurate modelling of the matter power spectrum up to non-linear scales. Therefore in this work we present the halo model reaction framework for the Generalized Cubic Covariant Galileon (GCCG) model, a modified gravity model within the Horndeski class of theories which extends the cubic covariant Galileon (G3) by including power laws of the derivatives of the scalar field in the K-essence and cubic terms. We modify the publicly available software ReACT for the GCCG in order to obtain an accurate prediction of the non-linear pow"},"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":"2404.11471","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-04-17T15:24:09Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"f1af6bcc139b51f01d2a37f2855c657c588d5ae428464b11ac76b9b33993f621","abstract_canon_sha256":"61875d88c22e6084f09d7af3849e6199844c1340720f991badb60e94ab695366"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:09:09.297884Z","signature_b64":"QgKBvbTTYTG782Me7RfsN/pGP+8v9t3frf1qriH4eBWwVHgtQcTe/QfsHTk5uIg90MjH7oNwflb7H8BTvvo3AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a47688208c4bb8a4ce4b5d453d60441cdb0fc73764fdefb0db6d74b8479175fd","last_reissued_at":"2026-07-05T08:09:09.297432Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:09:09.297432Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-linear power spectrum and forecasts for Generalized Cubic Covariant Galileon","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Baojiu Li, Benjamin Bose, Lu\\'is Atayde, Noemi Frusciante, Santiago Casas","submitted_at":"2024-04-17T15:24:09Z","abstract_excerpt":"To fully exploit the data from next generation surveys, we need an accurate modelling of the matter power spectrum up to non-linear scales. Therefore in this work we present the halo model reaction framework for the Generalized Cubic Covariant Galileon (GCCG) model, a modified gravity model within the Horndeski class of theories which extends the cubic covariant Galileon (G3) by including power laws of the derivatives of the scalar field in the K-essence and cubic terms. We modify the publicly available software ReACT for the GCCG in order to obtain an accurate prediction of the non-linear pow"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2404.11471","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2404.11471/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":"2404.11471","created_at":"2026-07-05T08:09:09.297491+00:00"},{"alias_kind":"arxiv_version","alias_value":"2404.11471v1","created_at":"2026-07-05T08:09:09.297491+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2404.11471","created_at":"2026-07-05T08:09:09.297491+00:00"},{"alias_kind":"pith_short_12","alias_value":"UR3IQIEMJO4K","created_at":"2026-07-05T08:09:09.297491+00:00"},{"alias_kind":"pith_short_16","alias_value":"UR3IQIEMJO4KJTSL","created_at":"2026-07-05T08:09:09.297491+00:00"},{"alias_kind":"pith_short_8","alias_value":"UR3IQIEM","created_at":"2026-07-05T08:09:09.297491+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07777","citing_title":"The Status of Single Scalar Field Dark Energy","ref_index":212,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UR3IQIEMJO4KJTSLLVCT2YCEDT","json":"https://pith.science/pith/UR3IQIEMJO4KJTSLLVCT2YCEDT.json","graph_json":"https://pith.science/api/pith-number/UR3IQIEMJO4KJTSLLVCT2YCEDT/graph.json","events_json":"https://pith.science/api/pith-number/UR3IQIEMJO4KJTSLLVCT2YCEDT/events.json","paper":"https://pith.science/paper/UR3IQIEM"},"agent_actions":{"view_html":"https://pith.science/pith/UR3IQIEMJO4KJTSLLVCT2YCEDT","download_json":"https://pith.science/pith/UR3IQIEMJO4KJTSLLVCT2YCEDT.json","view_paper":"https://pith.science/paper/UR3IQIEM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2404.11471&json=true","fetch_graph":"https://pith.science/api/pith-number/UR3IQIEMJO4KJTSLLVCT2YCEDT/graph.json","fetch_events":"https://pith.science/api/pith-number/UR3IQIEMJO4KJTSLLVCT2YCEDT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UR3IQIEMJO4KJTSLLVCT2YCEDT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UR3IQIEMJO4KJTSLLVCT2YCEDT/action/storage_attestation","attest_author":"https://pith.science/pith/UR3IQIEMJO4KJTSLLVCT2YCEDT/action/author_attestation","sign_citation":"https://pith.science/pith/UR3IQIEMJO4KJTSLLVCT2YCEDT/action/citation_signature","submit_replication":"https://pith.science/pith/UR3IQIEMJO4KJTSLLVCT2YCEDT/action/replication_record"}},"created_at":"2026-07-05T08:09:09.297491+00:00","updated_at":"2026-07-05T08:09:09.297491+00:00"}