{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:7IIISJWJW572F66FSIL6MZSZP7","short_pith_number":"pith:7IIISJWJ","schema_version":"1.0","canonical_sha256":"fa108926c9b77fa2fbc59217e666597fd40915ea68f1002ae312ec6c6e4d467b","source":{"kind":"arxiv","id":"2104.04995","version":2},"attestation_state":"computed","paper":{"title":"Construction of inflationary scenarios with the Gauss-Bonnet term and nonminimal coupling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"Ekaterina O. Pozdeeva, Sergey Yu. Vernov","submitted_at":"2021-04-11T11:27:11Z","abstract_excerpt":"Inflationary models with a scalar field nonminimally coupled both with the Ricci scalar and with the Gauss-Bonnet term are studied. We propose the way of generalization of inflationary scenarios with the Gauss-Bonnet term and a scalar field minimally coupled with the Ricci scalar to the corresponding scenarios with a scalar field nonminimally coupled with the Ricci scalar. Using the effective potential, we construct a set of models with the same values of the scalar spectral index $n_s$ and the amplitude of the scalar perturbations $A_s$ and different values of the tensor-to-scalar ratio $r$."},"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":"2104.04995","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2021-04-11T11:27:11Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"22f82ca42801418f63a96d3f1526ff8e79fc64352964951b1a36fc5b372e0bf7","abstract_canon_sha256":"f23ea55e5491d1bc8f575c5eabc2539c2ad8a7a31e521f641f10141df2d54a21"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:59:18.339801Z","signature_b64":"WZe9HznsyCfcl8n5cNW01hAZsDoC7Rxr4X6f5XL/mJJx6tqJA33vsS7+kcio5+nTT6mfq6n7+inw3i5moeQxDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fa108926c9b77fa2fbc59217e666597fd40915ea68f1002ae312ec6c6e4d467b","last_reissued_at":"2026-07-05T02:59:18.339240Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:59:18.339240Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Construction of inflationary scenarios with the Gauss-Bonnet term and nonminimal coupling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"Ekaterina O. Pozdeeva, Sergey Yu. Vernov","submitted_at":"2021-04-11T11:27:11Z","abstract_excerpt":"Inflationary models with a scalar field nonminimally coupled both with the Ricci scalar and with the Gauss-Bonnet term are studied. We propose the way of generalization of inflationary scenarios with the Gauss-Bonnet term and a scalar field minimally coupled with the Ricci scalar to the corresponding scenarios with a scalar field nonminimally coupled with the Ricci scalar. Using the effective potential, we construct a set of models with the same values of the scalar spectral index $n_s$ and the amplitude of the scalar perturbations $A_s$ and different values of the tensor-to-scalar ratio $r$."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2104.04995","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2104.04995/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":"2104.04995","created_at":"2026-07-05T02:59:18.339298+00:00"},{"alias_kind":"arxiv_version","alias_value":"2104.04995v2","created_at":"2026-07-05T02:59:18.339298+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2104.04995","created_at":"2026-07-05T02:59:18.339298+00:00"},{"alias_kind":"pith_short_12","alias_value":"7IIISJWJW572","created_at":"2026-07-05T02:59:18.339298+00:00"},{"alias_kind":"pith_short_16","alias_value":"7IIISJWJW572F66F","created_at":"2026-07-05T02:59:18.339298+00:00"},{"alias_kind":"pith_short_8","alias_value":"7IIISJWJ","created_at":"2026-07-05T02:59:18.339298+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2608.01165","citing_title":"From Quantum Correlations to Inflationary Tracking Scalar Field Evolution","ref_index":20,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7IIISJWJW572F66FSIL6MZSZP7","json":"https://pith.science/pith/7IIISJWJW572F66FSIL6MZSZP7.json","graph_json":"https://pith.science/api/pith-number/7IIISJWJW572F66FSIL6MZSZP7/graph.json","events_json":"https://pith.science/api/pith-number/7IIISJWJW572F66FSIL6MZSZP7/events.json","paper":"https://pith.science/paper/7IIISJWJ"},"agent_actions":{"view_html":"https://pith.science/pith/7IIISJWJW572F66FSIL6MZSZP7","download_json":"https://pith.science/pith/7IIISJWJW572F66FSIL6MZSZP7.json","view_paper":"https://pith.science/paper/7IIISJWJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2104.04995&json=true","fetch_graph":"https://pith.science/api/pith-number/7IIISJWJW572F66FSIL6MZSZP7/graph.json","fetch_events":"https://pith.science/api/pith-number/7IIISJWJW572F66FSIL6MZSZP7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7IIISJWJW572F66FSIL6MZSZP7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7IIISJWJW572F66FSIL6MZSZP7/action/storage_attestation","attest_author":"https://pith.science/pith/7IIISJWJW572F66FSIL6MZSZP7/action/author_attestation","sign_citation":"https://pith.science/pith/7IIISJWJW572F66FSIL6MZSZP7/action/citation_signature","submit_replication":"https://pith.science/pith/7IIISJWJW572F66FSIL6MZSZP7/action/replication_record"}},"created_at":"2026-07-05T02:59:18.339298+00:00","updated_at":"2026-07-05T02:59:18.339298+00:00"}