{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:IZUT6M5EFUJOKZHWRCKPW2A72E","short_pith_number":"pith:IZUT6M5E","schema_version":"1.0","canonical_sha256":"46693f33a42d12e564f68894fb681fd13ba3468e1690fce480329c4ca7b36c6b","source":{"kind":"arxiv","id":"1802.04160","version":2},"attestation_state":"computed","paper":{"title":"Inflationary predictions of double-well, Coleman-Weinberg, and hilltop potentials with non-minimal coupling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Nilay Bostan, \\\"Omer G\\\"ulery\\\"uz, Vedat Nefer \\c{S}eno\\u{g}uz","submitted_at":"2018-02-12T16:09:39Z","abstract_excerpt":"We discuss how the non-minimal coupling $\\xi\\phi^2R$ between the inflaton and the Ricci scalar affects the predictions of single field inflation models where the inflaton has a non-zero vacuum expectation value (VEV) $v$ after inflation. We show that, for inflaton values both above the VEV and below the VEV during inflation, under certain conditions the inflationary predictions become approximately the same as the predictions of the Starobinsky model. We then analyze inflation with double-well and Coleman-Weinberg potentials in detail, displaying the regions in the $v$-$\\xi$ plane for which th"},"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":"1802.04160","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2018-02-12T16:09:39Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"1558c72335f2ca1c766777a4a75a098181647b86e4039fd0e5153450dca16e8c","abstract_canon_sha256":"83f176f77208b102bb2ca8301b4230a631f872579748e69ed8cfe159029903b7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:11:02.389021Z","signature_b64":"xnVarKvpCeKfT24n+xKZpVoSLa0KeNXL9E7jiSp8JyAA7wNcZA7P8Iol86nVyXsVfVINOx/SpChMIdYHXUTsBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"46693f33a42d12e564f68894fb681fd13ba3468e1690fce480329c4ca7b36c6b","last_reissued_at":"2026-07-05T00:11:02.388611Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:11:02.388611Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Inflationary predictions of double-well, Coleman-Weinberg, and hilltop potentials with non-minimal coupling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Nilay Bostan, \\\"Omer G\\\"ulery\\\"uz, Vedat Nefer \\c{S}eno\\u{g}uz","submitted_at":"2018-02-12T16:09:39Z","abstract_excerpt":"We discuss how the non-minimal coupling $\\xi\\phi^2R$ between the inflaton and the Ricci scalar affects the predictions of single field inflation models where the inflaton has a non-zero vacuum expectation value (VEV) $v$ after inflation. We show that, for inflaton values both above the VEV and below the VEV during inflation, under certain conditions the inflationary predictions become approximately the same as the predictions of the Starobinsky model. We then analyze inflation with double-well and Coleman-Weinberg potentials in detail, displaying the regions in the $v$-$\\xi$ plane for which th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.04160","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/1802.04160/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":"1802.04160","created_at":"2026-07-05T00:11:02.388665+00:00"},{"alias_kind":"arxiv_version","alias_value":"1802.04160v2","created_at":"2026-07-05T00:11:02.388665+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.04160","created_at":"2026-07-05T00:11:02.388665+00:00"},{"alias_kind":"pith_short_12","alias_value":"IZUT6M5EFUJO","created_at":"2026-07-05T00:11:02.388665+00:00"},{"alias_kind":"pith_short_16","alias_value":"IZUT6M5EFUJOKZHW","created_at":"2026-07-05T00:11:02.388665+00:00"},{"alias_kind":"pith_short_8","alias_value":"IZUT6M5E","created_at":"2026-07-05T00:11:02.388665+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1908.09674","citing_title":"Quadratic, Higgs and hilltop potentials in the Palatini gravity","ref_index":33,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IZUT6M5EFUJOKZHWRCKPW2A72E","json":"https://pith.science/pith/IZUT6M5EFUJOKZHWRCKPW2A72E.json","graph_json":"https://pith.science/api/pith-number/IZUT6M5EFUJOKZHWRCKPW2A72E/graph.json","events_json":"https://pith.science/api/pith-number/IZUT6M5EFUJOKZHWRCKPW2A72E/events.json","paper":"https://pith.science/paper/IZUT6M5E"},"agent_actions":{"view_html":"https://pith.science/pith/IZUT6M5EFUJOKZHWRCKPW2A72E","download_json":"https://pith.science/pith/IZUT6M5EFUJOKZHWRCKPW2A72E.json","view_paper":"https://pith.science/paper/IZUT6M5E","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1802.04160&json=true","fetch_graph":"https://pith.science/api/pith-number/IZUT6M5EFUJOKZHWRCKPW2A72E/graph.json","fetch_events":"https://pith.science/api/pith-number/IZUT6M5EFUJOKZHWRCKPW2A72E/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IZUT6M5EFUJOKZHWRCKPW2A72E/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IZUT6M5EFUJOKZHWRCKPW2A72E/action/storage_attestation","attest_author":"https://pith.science/pith/IZUT6M5EFUJOKZHWRCKPW2A72E/action/author_attestation","sign_citation":"https://pith.science/pith/IZUT6M5EFUJOKZHWRCKPW2A72E/action/citation_signature","submit_replication":"https://pith.science/pith/IZUT6M5EFUJOKZHWRCKPW2A72E/action/replication_record"}},"created_at":"2026-07-05T00:11:02.388665+00:00","updated_at":"2026-07-05T00:11:02.388665+00:00"}