{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:LBJGMIC4ILVGTO6P3HJAJLFALH","short_pith_number":"pith:LBJGMIC4","schema_version":"1.0","canonical_sha256":"585266205c42ea69bbcfd9d204aca059c66240ae82fb7f876f6bc793b50c84ff","source":{"kind":"arxiv","id":"1708.08346","version":1},"attestation_state":"computed","paper":{"title":"Unification of Constant-roll Inflation and Dark Energy with Logarithmic $R^2$-corrected and Exponential $F(R)$ Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"L. Sebastiani, S.D. Odintsov, V.K. Oikonomou","submitted_at":"2017-08-28T14:39:34Z","abstract_excerpt":"In this paper we investigate how to describe in a unified way a constant-roll inflationary era with a dark energy era, by using the theoretical framework of $F(R)$ gravity. To this end, we introduce some classes of appropriately chosen $F(R)$ gravity models, and we examine in detail how the unification of early and late-time acceleration eras can be achieved. We study in detail the inflationary era, and as we demonstrate it is possible to achieve a viable inflationary era, for which the spectral index of primordial curvature perturbations and the scalar-to-tensor ratio can be compatible with t"},"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":"1708.08346","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2017-08-28T14:39:34Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"458ca845ecf45c64accc0e2314167384255b2cd28077beec6d31c0e74d4062f5","abstract_canon_sha256":"67f74c179d64ba88b18ba8681922e9a61ac5b58fedacd70fcc7bc0c897b1d77c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:21:25.587521Z","signature_b64":"ocJuSZEPhlScRp/yj2SP1jVG+bKH8CrIboA+2AUFRGW3IsmrTVidbSgb57NOlqVXaG8Qr6N/FpHxPxPRmyhiDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"585266205c42ea69bbcfd9d204aca059c66240ae82fb7f876f6bc793b50c84ff","last_reissued_at":"2026-05-18T00:21:25.586827Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:21:25.586827Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Unification of Constant-roll Inflation and Dark Energy with Logarithmic $R^2$-corrected and Exponential $F(R)$ Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"L. Sebastiani, S.D. Odintsov, V.K. Oikonomou","submitted_at":"2017-08-28T14:39:34Z","abstract_excerpt":"In this paper we investigate how to describe in a unified way a constant-roll inflationary era with a dark energy era, by using the theoretical framework of $F(R)$ gravity. To this end, we introduce some classes of appropriately chosen $F(R)$ gravity models, and we examine in detail how the unification of early and late-time acceleration eras can be achieved. We study in detail the inflationary era, and as we demonstrate it is possible to achieve a viable inflationary era, for which the spectral index of primordial curvature perturbations and the scalar-to-tensor ratio can be compatible with t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.08346","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":"1708.08346","created_at":"2026-05-18T00:21:25.586934+00:00"},{"alias_kind":"arxiv_version","alias_value":"1708.08346v1","created_at":"2026-05-18T00:21:25.586934+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1708.08346","created_at":"2026-05-18T00:21:25.586934+00:00"},{"alias_kind":"pith_short_12","alias_value":"LBJGMIC4ILVG","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_16","alias_value":"LBJGMIC4ILVGTO6P","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_8","alias_value":"LBJGMIC4","created_at":"2026-05-18T12:31:28.150371+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.14659","citing_title":"Constraining Quintessential Inflation with ACT: A Gauss-Bonnet Gateway","ref_index":31,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LBJGMIC4ILVGTO6P3HJAJLFALH","json":"https://pith.science/pith/LBJGMIC4ILVGTO6P3HJAJLFALH.json","graph_json":"https://pith.science/api/pith-number/LBJGMIC4ILVGTO6P3HJAJLFALH/graph.json","events_json":"https://pith.science/api/pith-number/LBJGMIC4ILVGTO6P3HJAJLFALH/events.json","paper":"https://pith.science/paper/LBJGMIC4"},"agent_actions":{"view_html":"https://pith.science/pith/LBJGMIC4ILVGTO6P3HJAJLFALH","download_json":"https://pith.science/pith/LBJGMIC4ILVGTO6P3HJAJLFALH.json","view_paper":"https://pith.science/paper/LBJGMIC4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1708.08346&json=true","fetch_graph":"https://pith.science/api/pith-number/LBJGMIC4ILVGTO6P3HJAJLFALH/graph.json","fetch_events":"https://pith.science/api/pith-number/LBJGMIC4ILVGTO6P3HJAJLFALH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LBJGMIC4ILVGTO6P3HJAJLFALH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LBJGMIC4ILVGTO6P3HJAJLFALH/action/storage_attestation","attest_author":"https://pith.science/pith/LBJGMIC4ILVGTO6P3HJAJLFALH/action/author_attestation","sign_citation":"https://pith.science/pith/LBJGMIC4ILVGTO6P3HJAJLFALH/action/citation_signature","submit_replication":"https://pith.science/pith/LBJGMIC4ILVGTO6P3HJAJLFALH/action/replication_record"}},"created_at":"2026-05-18T00:21:25.586934+00:00","updated_at":"2026-05-18T00:21:25.586934+00:00"}