{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:VRQ3YW6DNNAZ7QLWPP4PUUXE3P","short_pith_number":"pith:VRQ3YW6D","schema_version":"1.0","canonical_sha256":"ac61bc5bc36b419fc1767bf8fa52e4dbe4a2e2ac841bb4263b01fb25d3d90067","source":{"kind":"arxiv","id":"1605.02627","version":2},"attestation_state":"computed","paper":{"title":"Constraining the $\\Lambda$CDM and Galileon models with recent cosmological data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"A. M\\\"oller, E. Babichev, J. Guy, J. Neveu, M. Besan\\c{c}on, P. Astier, V. Ruhlmann-Kleider","submitted_at":"2016-05-09T15:43:08Z","abstract_excerpt":"The Galileon theory belongs to the class of modified gravity models that can explain the late-time accelerated expansion of the Universe. In previous works, cosmological constraints on the Galileon model were derived, both in the uncoupled case and with a disformal coupling of the Galileon field to matter. There, we showed that these models agree with the most recent cosmological data. In this work, we used updated cosmological data sets to derive new constraints on Galileon models, including the case of a constant conformal Galileon coupling to matter. We also explored the tracker solution of"},"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":"1605.02627","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2016-05-09T15:43:08Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"e9f927edbd894e14ef29d4bc6daa530e1844c99554f94550133265a92fd57d19","abstract_canon_sha256":"fb6cc67c6704d54f0a953e8913ac8c72b5888af9640cd926a042eb68173f4aba"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:47:50.735375Z","signature_b64":"lmN2rvSHpRrm/+biMibA+6dShdUi9wpbn1XbicqKUU2AodBzJHDFaKMscTeL7PLh96idWu9mqZcnnGAnJYT6Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ac61bc5bc36b419fc1767bf8fa52e4dbe4a2e2ac841bb4263b01fb25d3d90067","last_reissued_at":"2026-05-18T00:47:50.734625Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:47:50.734625Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraining the $\\Lambda$CDM and Galileon models with recent cosmological data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"A. M\\\"oller, E. Babichev, J. Guy, J. Neveu, M. Besan\\c{c}on, P. Astier, V. Ruhlmann-Kleider","submitted_at":"2016-05-09T15:43:08Z","abstract_excerpt":"The Galileon theory belongs to the class of modified gravity models that can explain the late-time accelerated expansion of the Universe. In previous works, cosmological constraints on the Galileon model were derived, both in the uncoupled case and with a disformal coupling of the Galileon field to matter. There, we showed that these models agree with the most recent cosmological data. In this work, we used updated cosmological data sets to derive new constraints on Galileon models, including the case of a constant conformal Galileon coupling to matter. We also explored the tracker solution of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.02627","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":""},"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":"1605.02627","created_at":"2026-05-18T00:47:50.734753+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.02627v2","created_at":"2026-05-18T00:47:50.734753+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.02627","created_at":"2026-05-18T00:47:50.734753+00:00"},{"alias_kind":"pith_short_12","alias_value":"VRQ3YW6DNNAZ","created_at":"2026-05-18T12:30:48.956258+00:00"},{"alias_kind":"pith_short_16","alias_value":"VRQ3YW6DNNAZ7QLW","created_at":"2026-05-18T12:30:48.956258+00:00"},{"alias_kind":"pith_short_8","alias_value":"VRQ3YW6D","created_at":"2026-05-18T12:30:48.956258+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VRQ3YW6DNNAZ7QLWPP4PUUXE3P","json":"https://pith.science/pith/VRQ3YW6DNNAZ7QLWPP4PUUXE3P.json","graph_json":"https://pith.science/api/pith-number/VRQ3YW6DNNAZ7QLWPP4PUUXE3P/graph.json","events_json":"https://pith.science/api/pith-number/VRQ3YW6DNNAZ7QLWPP4PUUXE3P/events.json","paper":"https://pith.science/paper/VRQ3YW6D"},"agent_actions":{"view_html":"https://pith.science/pith/VRQ3YW6DNNAZ7QLWPP4PUUXE3P","download_json":"https://pith.science/pith/VRQ3YW6DNNAZ7QLWPP4PUUXE3P.json","view_paper":"https://pith.science/paper/VRQ3YW6D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.02627&json=true","fetch_graph":"https://pith.science/api/pith-number/VRQ3YW6DNNAZ7QLWPP4PUUXE3P/graph.json","fetch_events":"https://pith.science/api/pith-number/VRQ3YW6DNNAZ7QLWPP4PUUXE3P/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VRQ3YW6DNNAZ7QLWPP4PUUXE3P/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VRQ3YW6DNNAZ7QLWPP4PUUXE3P/action/storage_attestation","attest_author":"https://pith.science/pith/VRQ3YW6DNNAZ7QLWPP4PUUXE3P/action/author_attestation","sign_citation":"https://pith.science/pith/VRQ3YW6DNNAZ7QLWPP4PUUXE3P/action/citation_signature","submit_replication":"https://pith.science/pith/VRQ3YW6DNNAZ7QLWPP4PUUXE3P/action/replication_record"}},"created_at":"2026-05-18T00:47:50.734753+00:00","updated_at":"2026-05-18T00:47:50.734753+00:00"}