{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:T7OSUEREERXTIGUIKF63HIBJ62","short_pith_number":"pith:T7OSUERE","schema_version":"1.0","canonical_sha256":"9fdd2a1224246f341a88517db3a029f68f4846771c1b35d26f05ecb5163cc4f9","source":{"kind":"arxiv","id":"1309.1085","version":2},"attestation_state":"computed","paper":{"title":"Higher Order Corrections in Minimal Supergravity Models of Inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Andrei Linde, Massimo Porrati, Renata Kallosh, Sergio Ferrara","submitted_at":"2013-09-04T16:08:17Z","abstract_excerpt":"We study higher order corrections in new minimal supergravity models of a single scalar field inflation. The gauging in these models leads to a massive vector multiplet and the D-term potential for the inflaton field with a coupling g^{2} ~ 10^{-10}. In the de-Higgsed phase with vanishing g^2, the chiral and vector multiplets are non-interacting, and the potential vanishes. We present generic manifestly supersymmetric higher order corrections for these models. In particular, for a supersymmetric gravity model -R+ R^2 we derive manifestly supersymmetric corrections corresponding to R^n. The dua"},"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":"1309.1085","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2013-09-04T16:08:17Z","cross_cats_sorted":["astro-ph.CO","gr-qc","hep-ph"],"title_canon_sha256":"61526d9312d1c695267c328d11b1aa0e8995ee2722c7cd5531887c4e1d6ab529","abstract_canon_sha256":"2434dcb68190e62fa4931bc5301bbfb6181ec1a6ee82c6c5ff27954371731ca8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:47:49.813860Z","signature_b64":"OjA5+HFANe9O9ytBPaflVGd/pkwXvgVGygWZL5HCFew9cmvfrQZx7jjLE+XFkyXW1QpPWX8di38QCd49E4MjAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9fdd2a1224246f341a88517db3a029f68f4846771c1b35d26f05ecb5163cc4f9","last_reissued_at":"2026-05-18T01:47:49.813375Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:47:49.813375Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Higher Order Corrections in Minimal Supergravity Models of Inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Andrei Linde, Massimo Porrati, Renata Kallosh, Sergio Ferrara","submitted_at":"2013-09-04T16:08:17Z","abstract_excerpt":"We study higher order corrections in new minimal supergravity models of a single scalar field inflation. The gauging in these models leads to a massive vector multiplet and the D-term potential for the inflaton field with a coupling g^{2} ~ 10^{-10}. In the de-Higgsed phase with vanishing g^2, the chiral and vector multiplets are non-interacting, and the potential vanishes. We present generic manifestly supersymmetric higher order corrections for these models. In particular, for a supersymmetric gravity model -R+ R^2 we derive manifestly supersymmetric corrections corresponding to R^n. The dua"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1309.1085","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":"1309.1085","created_at":"2026-05-18T01:47:49.813447+00:00"},{"alias_kind":"arxiv_version","alias_value":"1309.1085v2","created_at":"2026-05-18T01:47:49.813447+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1309.1085","created_at":"2026-05-18T01:47:49.813447+00:00"},{"alias_kind":"pith_short_12","alias_value":"T7OSUEREERXT","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_16","alias_value":"T7OSUEREERXTIGUI","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_8","alias_value":"T7OSUERE","created_at":"2026-05-18T12:27:59.945178+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/T7OSUEREERXTIGUIKF63HIBJ62","json":"https://pith.science/pith/T7OSUEREERXTIGUIKF63HIBJ62.json","graph_json":"https://pith.science/api/pith-number/T7OSUEREERXTIGUIKF63HIBJ62/graph.json","events_json":"https://pith.science/api/pith-number/T7OSUEREERXTIGUIKF63HIBJ62/events.json","paper":"https://pith.science/paper/T7OSUERE"},"agent_actions":{"view_html":"https://pith.science/pith/T7OSUEREERXTIGUIKF63HIBJ62","download_json":"https://pith.science/pith/T7OSUEREERXTIGUIKF63HIBJ62.json","view_paper":"https://pith.science/paper/T7OSUERE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1309.1085&json=true","fetch_graph":"https://pith.science/api/pith-number/T7OSUEREERXTIGUIKF63HIBJ62/graph.json","fetch_events":"https://pith.science/api/pith-number/T7OSUEREERXTIGUIKF63HIBJ62/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/T7OSUEREERXTIGUIKF63HIBJ62/action/timestamp_anchor","attest_storage":"https://pith.science/pith/T7OSUEREERXTIGUIKF63HIBJ62/action/storage_attestation","attest_author":"https://pith.science/pith/T7OSUEREERXTIGUIKF63HIBJ62/action/author_attestation","sign_citation":"https://pith.science/pith/T7OSUEREERXTIGUIKF63HIBJ62/action/citation_signature","submit_replication":"https://pith.science/pith/T7OSUEREERXTIGUIKF63HIBJ62/action/replication_record"}},"created_at":"2026-05-18T01:47:49.813447+00:00","updated_at":"2026-05-18T01:47:49.813447+00:00"}