{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:PKWB35T7HCF2CGPLDUDI5N4DFI","short_pith_number":"pith:PKWB35T7","schema_version":"1.0","canonical_sha256":"7aac1df67f388ba119eb1d068eb7832a2417fa0dfb715d528a7e28694111731c","source":{"kind":"arxiv","id":"2105.11935","version":1},"attestation_state":"computed","paper":{"title":"Rescaled Einstein-Hilbert Gravity: Inflation and the Swampland Criteria","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Achilles Gitsis, Ifigeneia Giannakoudi, Konstantinos-Rafail Revis, V.K. Oikonomou","submitted_at":"2021-05-25T13:36:09Z","abstract_excerpt":"In this work we shall study a class of $f(R,\\phi)$ gravity models which during the inflationary era, which is the large curvature regime, result to an effective inflationary Lagrangian that contains a rescaled Einstein-Hilbert term $\\alpha R$ in the presence of a canonical minimally coupled scalar field. The dimensionless parameter $\\alpha$ is chosen to take values in the range $0<\\alpha<1$ and the main motivation for studying these rescaled Einstein-Hilbert $f(R,\\phi)$ gravities, is the fact that the rescaled action may render an otherwise incompatible canonical scalar field theory with the S"},"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":"2105.11935","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2021-05-25T13:36:09Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"2d2f101660be85e043533394973de2a74c6585dfd3a00e4810f54bbc2ae4be4b","abstract_canon_sha256":"918ee0b0420ed86b3a7a489161de1dfaf4faf52bbd3327a826a4dbbb24f19846"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:03:46.600081Z","signature_b64":"1cPE3QYBOX3KMkWrWl1D1VIOBX9pLoL2mpPK2FwVcSCOAEmWDbkU+BWpJ9fYzZW25Y2P30ew+3idXru9nvsACg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7aac1df67f388ba119eb1d068eb7832a2417fa0dfb715d528a7e28694111731c","last_reissued_at":"2026-07-05T04:03:46.599621Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:03:46.599621Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Rescaled Einstein-Hilbert Gravity: Inflation and the Swampland Criteria","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Achilles Gitsis, Ifigeneia Giannakoudi, Konstantinos-Rafail Revis, V.K. Oikonomou","submitted_at":"2021-05-25T13:36:09Z","abstract_excerpt":"In this work we shall study a class of $f(R,\\phi)$ gravity models which during the inflationary era, which is the large curvature regime, result to an effective inflationary Lagrangian that contains a rescaled Einstein-Hilbert term $\\alpha R$ in the presence of a canonical minimally coupled scalar field. The dimensionless parameter $\\alpha$ is chosen to take values in the range $0<\\alpha<1$ and the main motivation for studying these rescaled Einstein-Hilbert $f(R,\\phi)$ gravities, is the fact that the rescaled action may render an otherwise incompatible canonical scalar field theory with the S"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2105.11935","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/2105.11935/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":"2105.11935","created_at":"2026-07-05T04:03:46.599670+00:00"},{"alias_kind":"arxiv_version","alias_value":"2105.11935v1","created_at":"2026-07-05T04:03:46.599670+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2105.11935","created_at":"2026-07-05T04:03:46.599670+00:00"},{"alias_kind":"pith_short_12","alias_value":"PKWB35T7HCF2","created_at":"2026-07-05T04:03:46.599670+00:00"},{"alias_kind":"pith_short_16","alias_value":"PKWB35T7HCF2CGPL","created_at":"2026-07-05T04:03:46.599670+00:00"},{"alias_kind":"pith_short_8","alias_value":"PKWB35T7","created_at":"2026-07-05T04:03:46.599670+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.23047","citing_title":"On Thermodynamics of Charged Black Holes, Swampland, and Dark Matter","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2605.23047","citing_title":"On Thermodynamics of Charged Black Holes, Swampland, and Dark Matter","ref_index":23,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PKWB35T7HCF2CGPLDUDI5N4DFI","json":"https://pith.science/pith/PKWB35T7HCF2CGPLDUDI5N4DFI.json","graph_json":"https://pith.science/api/pith-number/PKWB35T7HCF2CGPLDUDI5N4DFI/graph.json","events_json":"https://pith.science/api/pith-number/PKWB35T7HCF2CGPLDUDI5N4DFI/events.json","paper":"https://pith.science/paper/PKWB35T7"},"agent_actions":{"view_html":"https://pith.science/pith/PKWB35T7HCF2CGPLDUDI5N4DFI","download_json":"https://pith.science/pith/PKWB35T7HCF2CGPLDUDI5N4DFI.json","view_paper":"https://pith.science/paper/PKWB35T7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2105.11935&json=true","fetch_graph":"https://pith.science/api/pith-number/PKWB35T7HCF2CGPLDUDI5N4DFI/graph.json","fetch_events":"https://pith.science/api/pith-number/PKWB35T7HCF2CGPLDUDI5N4DFI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PKWB35T7HCF2CGPLDUDI5N4DFI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PKWB35T7HCF2CGPLDUDI5N4DFI/action/storage_attestation","attest_author":"https://pith.science/pith/PKWB35T7HCF2CGPLDUDI5N4DFI/action/author_attestation","sign_citation":"https://pith.science/pith/PKWB35T7HCF2CGPLDUDI5N4DFI/action/citation_signature","submit_replication":"https://pith.science/pith/PKWB35T7HCF2CGPLDUDI5N4DFI/action/replication_record"}},"created_at":"2026-07-05T04:03:46.599670+00:00","updated_at":"2026-07-05T04:03:46.599670+00:00"}