{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2003:5A52N57IYCVZMA2ZHYTOFQRYKX","short_pith_number":"pith:5A52N57I","schema_version":"1.0","canonical_sha256":"e83ba6f7e8c0ab9603593e26e2c23855e1617003072ffcc859ed156c86d4cc0c","source":{"kind":"arxiv","id":"hep-ph/0305089","version":2},"attestation_state":"computed","paper":{"title":"Testing Supersymmetric Grand Unified Models of Inflation","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"hep-ph","authors_text":"Q. Shafi, V. N. Senoguz","submitted_at":"2003-05-08T18:11:44Z","abstract_excerpt":"We reconsider a class of well motivated supersymmetric models in which inflation is associated with the breaking of a gauge symmetry G to H, with the symmetry breaking scale M~10^16 GeV. Starting with a renormalizable superpotential, we include both radiative and supergravity corrections to derive the inflationary potential. The scalar spectral index n_s can exceed unity in some cases, and it cannot be smaller than 0.98 if the number of e-foldings corresponding to the present horizon scale is around 60. Two distinct variations of this scenario are discussed in which non-renormalizable terms al"},"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":"hep-ph/0305089","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2003-05-08T18:11:44Z","cross_cats_sorted":["astro-ph"],"title_canon_sha256":"0d9b1ac1ecac50decf3a3ecdc030512bc7f7259ca681ec983f264a8b816938f0","abstract_canon_sha256":"b26c2132be415f22ce37cfbe4962f4be2689d62472724d13550eea6f206482ae"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:17:40.325655Z","signature_b64":"CQCnrSh3Ni8dQ2Gpnvxg1LKUoGjQDsbCrq02w1A7+RGYWk6Ru72+zyJpj4CObZtIDRTH7U5IB1+X5dzXhVODAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e83ba6f7e8c0ab9603593e26e2c23855e1617003072ffcc859ed156c86d4cc0c","last_reissued_at":"2026-07-04T15:17:40.325236Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:17:40.325236Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Testing Supersymmetric Grand Unified Models of Inflation","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"hep-ph","authors_text":"Q. Shafi, V. N. Senoguz","submitted_at":"2003-05-08T18:11:44Z","abstract_excerpt":"We reconsider a class of well motivated supersymmetric models in which inflation is associated with the breaking of a gauge symmetry G to H, with the symmetry breaking scale M~10^16 GeV. Starting with a renormalizable superpotential, we include both radiative and supergravity corrections to derive the inflationary potential. The scalar spectral index n_s can exceed unity in some cases, and it cannot be smaller than 0.98 if the number of e-foldings corresponding to the present horizon scale is around 60. Two distinct variations of this scenario are discussed in which non-renormalizable terms al"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0305089","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/hep-ph/0305089/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":"hep-ph/0305089","created_at":"2026-07-04T15:17:40.325302+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0305089v2","created_at":"2026-07-04T15:17:40.325302+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0305089","created_at":"2026-07-04T15:17:40.325302+00:00"},{"alias_kind":"pith_short_12","alias_value":"5A52N57IYCVZ","created_at":"2026-07-04T15:17:40.325302+00:00"},{"alias_kind":"pith_short_16","alias_value":"5A52N57IYCVZMA2Z","created_at":"2026-07-04T15:17:40.325302+00:00"},{"alias_kind":"pith_short_8","alias_value":"5A52N57I","created_at":"2026-07-04T15:17:40.325302+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/5A52N57IYCVZMA2ZHYTOFQRYKX","json":"https://pith.science/pith/5A52N57IYCVZMA2ZHYTOFQRYKX.json","graph_json":"https://pith.science/api/pith-number/5A52N57IYCVZMA2ZHYTOFQRYKX/graph.json","events_json":"https://pith.science/api/pith-number/5A52N57IYCVZMA2ZHYTOFQRYKX/events.json","paper":"https://pith.science/paper/5A52N57I"},"agent_actions":{"view_html":"https://pith.science/pith/5A52N57IYCVZMA2ZHYTOFQRYKX","download_json":"https://pith.science/pith/5A52N57IYCVZMA2ZHYTOFQRYKX.json","view_paper":"https://pith.science/paper/5A52N57I","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0305089&json=true","fetch_graph":"https://pith.science/api/pith-number/5A52N57IYCVZMA2ZHYTOFQRYKX/graph.json","fetch_events":"https://pith.science/api/pith-number/5A52N57IYCVZMA2ZHYTOFQRYKX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5A52N57IYCVZMA2ZHYTOFQRYKX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5A52N57IYCVZMA2ZHYTOFQRYKX/action/storage_attestation","attest_author":"https://pith.science/pith/5A52N57IYCVZMA2ZHYTOFQRYKX/action/author_attestation","sign_citation":"https://pith.science/pith/5A52N57IYCVZMA2ZHYTOFQRYKX/action/citation_signature","submit_replication":"https://pith.science/pith/5A52N57IYCVZMA2ZHYTOFQRYKX/action/replication_record"}},"created_at":"2026-07-04T15:17:40.325302+00:00","updated_at":"2026-07-04T15:17:40.325302+00:00"}