{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:IDOOJ5A2K3XVW24N3DLFL2DD5J","short_pith_number":"pith:IDOOJ5A2","schema_version":"1.0","canonical_sha256":"40dce4f41a56ef5b6b8dd8d655e863ea52c1cc3135dc5bc321c52e90f8340876","source":{"kind":"arxiv","id":"1108.2894","version":2},"attestation_state":"computed","paper":{"title":"A modified model of non-locally corrected gravity: Cosmology and the Newtonian limit","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bin Yang, Dao-jun Liu, Xing-hua Jin","submitted_at":"2011-08-14T18:10:27Z","abstract_excerpt":"A modified form of non-locally corrected theory of gravity is investigated in the context of cosmology and the Newtonian limit. This form of non-local correction to classic Einstein-Hilbert action can be locally represented by a triple-scalar-tensor theory in which one of the scalar degree of freedom is phantom-like and the other two are quintessence-like. We show that there exists a stable de Sitter solution for the cosmological dynamics if a suitable form of potential function $V(\\phi)$ (or equivalently, $f(R)$) is selected. However, no matter what a potential function is selected, there is "},"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":"1108.2894","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2011-08-14T18:10:27Z","cross_cats_sorted":[],"title_canon_sha256":"9fe0589d9f590f24c2309dc6643b2fcdbc5418d02c67c2c9d2b52c317928bf52","abstract_canon_sha256":"970c0e7048147c27d149490c3609796347101600c8f6db0c5cb01a9e419986ef"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:00:54.096291Z","signature_b64":"rANHngs/o4Ixrgb7CVreQVgGp8G7qVSZj/jgpASJDK8G7ZT9PnR9ppqVVE65R/cGarttnmm90OZjJHYT1G1xAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"40dce4f41a56ef5b6b8dd8d655e863ea52c1cc3135dc5bc321c52e90f8340876","last_reissued_at":"2026-05-18T02:00:54.095552Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:00:54.095552Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A modified model of non-locally corrected gravity: Cosmology and the Newtonian limit","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bin Yang, Dao-jun Liu, Xing-hua Jin","submitted_at":"2011-08-14T18:10:27Z","abstract_excerpt":"A modified form of non-locally corrected theory of gravity is investigated in the context of cosmology and the Newtonian limit. This form of non-local correction to classic Einstein-Hilbert action can be locally represented by a triple-scalar-tensor theory in which one of the scalar degree of freedom is phantom-like and the other two are quintessence-like. We show that there exists a stable de Sitter solution for the cosmological dynamics if a suitable form of potential function $V(\\phi)$ (or equivalently, $f(R)$) is selected. However, no matter what a potential function is selected, there is "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1108.2894","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":"1108.2894","created_at":"2026-05-18T02:00:54.095682+00:00"},{"alias_kind":"arxiv_version","alias_value":"1108.2894v2","created_at":"2026-05-18T02:00:54.095682+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1108.2894","created_at":"2026-05-18T02:00:54.095682+00:00"},{"alias_kind":"pith_short_12","alias_value":"IDOOJ5A2K3XV","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_16","alias_value":"IDOOJ5A2K3XVW24N","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_8","alias_value":"IDOOJ5A2","created_at":"2026-05-18T12:26:30.835961+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/IDOOJ5A2K3XVW24N3DLFL2DD5J","json":"https://pith.science/pith/IDOOJ5A2K3XVW24N3DLFL2DD5J.json","graph_json":"https://pith.science/api/pith-number/IDOOJ5A2K3XVW24N3DLFL2DD5J/graph.json","events_json":"https://pith.science/api/pith-number/IDOOJ5A2K3XVW24N3DLFL2DD5J/events.json","paper":"https://pith.science/paper/IDOOJ5A2"},"agent_actions":{"view_html":"https://pith.science/pith/IDOOJ5A2K3XVW24N3DLFL2DD5J","download_json":"https://pith.science/pith/IDOOJ5A2K3XVW24N3DLFL2DD5J.json","view_paper":"https://pith.science/paper/IDOOJ5A2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1108.2894&json=true","fetch_graph":"https://pith.science/api/pith-number/IDOOJ5A2K3XVW24N3DLFL2DD5J/graph.json","fetch_events":"https://pith.science/api/pith-number/IDOOJ5A2K3XVW24N3DLFL2DD5J/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IDOOJ5A2K3XVW24N3DLFL2DD5J/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IDOOJ5A2K3XVW24N3DLFL2DD5J/action/storage_attestation","attest_author":"https://pith.science/pith/IDOOJ5A2K3XVW24N3DLFL2DD5J/action/author_attestation","sign_citation":"https://pith.science/pith/IDOOJ5A2K3XVW24N3DLFL2DD5J/action/citation_signature","submit_replication":"https://pith.science/pith/IDOOJ5A2K3XVW24N3DLFL2DD5J/action/replication_record"}},"created_at":"2026-05-18T02:00:54.095682+00:00","updated_at":"2026-05-18T02:00:54.095682+00:00"}