{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:2PBJ6IHPPFABZVAFZBDPX3MAHK","short_pith_number":"pith:2PBJ6IHP","schema_version":"1.0","canonical_sha256":"d3c29f20ef79401cd405c846fbed803a9d7fda30034432cba17c730a88edd354","source":{"kind":"arxiv","id":"1612.09202","version":2},"attestation_state":"computed","paper":{"title":"Starobinsky Inflation: From Non-SUSY To SUGRA Realizations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"hep-ph","authors_text":"C. Pallis, N. Toumbas","submitted_at":"2016-12-29T17:03:35Z","abstract_excerpt":"We review the realization of Starobinsky-type inflation within induced-gravity Supersymmetric (SUSY) and non-SUSY models. In both cases, inflation is in agreement with the current data and can be attained for subplanckian values of the inflaton. The corresponding effective theories retain perturbative unitarity up to the Planck scale and the inflaton mass is predicted to be 3x10^13 GeV. The supergravity embedding of these models is achieved by employing two gauge singlet chiral supefields, a superpotential that is uniquely determined by a continuous R and a discrete Zn symmetry, and several (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":"1612.09202","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2016-12-29T17:03:35Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"9daf986fd4b86ba5ad63698fc16b48bed7b55d5f9d5bcd86bc2c9122162708da","abstract_canon_sha256":"1ab02e22a6a0e8435d0b0a74e927a4c415c249bee9c8ff89fa4900535c396406"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:42:12.530791Z","signature_b64":"ERYeU26FK1+g9f76EPJqtZk1aJuuD5IBhWbixEtD7P3UxHPw86K9b2r5Es4aNrIzWMOUpSaME/jLw4RXD4QDCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d3c29f20ef79401cd405c846fbed803a9d7fda30034432cba17c730a88edd354","last_reissued_at":"2026-05-18T00:42:12.530226Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:42:12.530226Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Starobinsky Inflation: From Non-SUSY To SUGRA Realizations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"hep-ph","authors_text":"C. Pallis, N. Toumbas","submitted_at":"2016-12-29T17:03:35Z","abstract_excerpt":"We review the realization of Starobinsky-type inflation within induced-gravity Supersymmetric (SUSY) and non-SUSY models. In both cases, inflation is in agreement with the current data and can be attained for subplanckian values of the inflaton. The corresponding effective theories retain perturbative unitarity up to the Planck scale and the inflaton mass is predicted to be 3x10^13 GeV. The supergravity embedding of these models is achieved by employing two gauge singlet chiral supefields, a superpotential that is uniquely determined by a continuous R and a discrete Zn symmetry, and several (s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.09202","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":"1612.09202","created_at":"2026-05-18T00:42:12.530313+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.09202v2","created_at":"2026-05-18T00:42:12.530313+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.09202","created_at":"2026-05-18T00:42:12.530313+00:00"},{"alias_kind":"pith_short_12","alias_value":"2PBJ6IHPPFAB","created_at":"2026-05-18T12:29:55.572404+00:00"},{"alias_kind":"pith_short_16","alias_value":"2PBJ6IHPPFABZVAF","created_at":"2026-05-18T12:29:55.572404+00:00"},{"alias_kind":"pith_short_8","alias_value":"2PBJ6IHP","created_at":"2026-05-18T12:29:55.572404+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2602.05623","citing_title":"Induced-Gravity Palatini-Like Higgs Inflation in Supergravity Confronts ACT DR6","ref_index":101,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2PBJ6IHPPFABZVAFZBDPX3MAHK","json":"https://pith.science/pith/2PBJ6IHPPFABZVAFZBDPX3MAHK.json","graph_json":"https://pith.science/api/pith-number/2PBJ6IHPPFABZVAFZBDPX3MAHK/graph.json","events_json":"https://pith.science/api/pith-number/2PBJ6IHPPFABZVAFZBDPX3MAHK/events.json","paper":"https://pith.science/paper/2PBJ6IHP"},"agent_actions":{"view_html":"https://pith.science/pith/2PBJ6IHPPFABZVAFZBDPX3MAHK","download_json":"https://pith.science/pith/2PBJ6IHPPFABZVAFZBDPX3MAHK.json","view_paper":"https://pith.science/paper/2PBJ6IHP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.09202&json=true","fetch_graph":"https://pith.science/api/pith-number/2PBJ6IHPPFABZVAFZBDPX3MAHK/graph.json","fetch_events":"https://pith.science/api/pith-number/2PBJ6IHPPFABZVAFZBDPX3MAHK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2PBJ6IHPPFABZVAFZBDPX3MAHK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2PBJ6IHPPFABZVAFZBDPX3MAHK/action/storage_attestation","attest_author":"https://pith.science/pith/2PBJ6IHPPFABZVAFZBDPX3MAHK/action/author_attestation","sign_citation":"https://pith.science/pith/2PBJ6IHPPFABZVAFZBDPX3MAHK/action/citation_signature","submit_replication":"https://pith.science/pith/2PBJ6IHPPFABZVAFZBDPX3MAHK/action/replication_record"}},"created_at":"2026-05-18T00:42:12.530313+00:00","updated_at":"2026-05-18T00:42:12.530313+00:00"}