{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2007:DDZCT3DWG3NK4O2OSSFCAP2OAC","short_pith_number":"pith:DDZCT3DW","schema_version":"1.0","canonical_sha256":"18f229ec7636daae3b4e948a203f4e00bc7a34a253a345c0aa1e99846524187a","source":{"kind":"arxiv","id":"astro-ph/0701052","version":1},"attestation_state":"computed","paper":{"title":"From New to Large Field Inflation: Comparison with WMAP3","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Q. Shafi, V. N. Senoguz","submitted_at":"2007-01-03T18:52:02Z","abstract_excerpt":"We briefly summarize and update a class of inflationary models from the early eighties based on a quartic (Coleman-Weinberg) potential for a gauge singlet scalar (inflaton) field. For vacuum energy scales comparable to the grand unification scale, the scalar spectral index n_s=0.94-0.97, in very good agreement with the WMAP three year results. The tensor to scalar ratio r<~0.14 while alpha=dn_s/d ln k=~-10^-3. For vacuum energy scales >~10^16 GeV, the inflationary scenario switches from `new' to `large-field' (V\\propto\\phi^2) inflation. An SO(10) version naturally explains the observed baryon "},"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":"astro-ph/0701052","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2007-01-03T18:52:02Z","cross_cats_sorted":[],"title_canon_sha256":"959870e1dc1522ddd07354fbd0d65ac2dcc7a54ab15e5ac52ff681ea16afe9d8","abstract_canon_sha256":"fe2381769f2d5c741a562881ff9ee8582ca37caebcfb2b19394391d61d54a465"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:22:20.460280Z","signature_b64":"ia8Q5ZBBKvutvf92dMZkJriw4bi79YevgCIgD9ugUvNcFgZ2B/9I15ldzFz+N6EToalO5k0OujWa5Pp/rnt9Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"18f229ec7636daae3b4e948a203f4e00bc7a34a253a345c0aa1e99846524187a","last_reissued_at":"2026-05-18T04:22:20.459627Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:22:20.459627Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"From New to Large Field Inflation: Comparison with WMAP3","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Q. Shafi, V. N. Senoguz","submitted_at":"2007-01-03T18:52:02Z","abstract_excerpt":"We briefly summarize and update a class of inflationary models from the early eighties based on a quartic (Coleman-Weinberg) potential for a gauge singlet scalar (inflaton) field. For vacuum energy scales comparable to the grand unification scale, the scalar spectral index n_s=0.94-0.97, in very good agreement with the WMAP three year results. The tensor to scalar ratio r<~0.14 while alpha=dn_s/d ln k=~-10^-3. For vacuum energy scales >~10^16 GeV, the inflationary scenario switches from `new' to `large-field' (V\\propto\\phi^2) inflation. An SO(10) version naturally explains the observed baryon "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0701052","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":""},"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":"astro-ph/0701052","created_at":"2026-05-18T04:22:20.459722+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0701052v1","created_at":"2026-05-18T04:22:20.459722+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0701052","created_at":"2026-05-18T04:22:20.459722+00:00"},{"alias_kind":"pith_short_12","alias_value":"DDZCT3DWG3NK","created_at":"2026-05-18T12:25:55.427421+00:00"},{"alias_kind":"pith_short_16","alias_value":"DDZCT3DWG3NK4O2O","created_at":"2026-05-18T12:25:55.427421+00:00"},{"alias_kind":"pith_short_8","alias_value":"DDZCT3DW","created_at":"2026-05-18T12:25:55.427421+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/DDZCT3DWG3NK4O2OSSFCAP2OAC","json":"https://pith.science/pith/DDZCT3DWG3NK4O2OSSFCAP2OAC.json","graph_json":"https://pith.science/api/pith-number/DDZCT3DWG3NK4O2OSSFCAP2OAC/graph.json","events_json":"https://pith.science/api/pith-number/DDZCT3DWG3NK4O2OSSFCAP2OAC/events.json","paper":"https://pith.science/paper/DDZCT3DW"},"agent_actions":{"view_html":"https://pith.science/pith/DDZCT3DWG3NK4O2OSSFCAP2OAC","download_json":"https://pith.science/pith/DDZCT3DWG3NK4O2OSSFCAP2OAC.json","view_paper":"https://pith.science/paper/DDZCT3DW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0701052&json=true","fetch_graph":"https://pith.science/api/pith-number/DDZCT3DWG3NK4O2OSSFCAP2OAC/graph.json","fetch_events":"https://pith.science/api/pith-number/DDZCT3DWG3NK4O2OSSFCAP2OAC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DDZCT3DWG3NK4O2OSSFCAP2OAC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DDZCT3DWG3NK4O2OSSFCAP2OAC/action/storage_attestation","attest_author":"https://pith.science/pith/DDZCT3DWG3NK4O2OSSFCAP2OAC/action/author_attestation","sign_citation":"https://pith.science/pith/DDZCT3DWG3NK4O2OSSFCAP2OAC/action/citation_signature","submit_replication":"https://pith.science/pith/DDZCT3DWG3NK4O2OSSFCAP2OAC/action/replication_record"}},"created_at":"2026-05-18T04:22:20.459722+00:00","updated_at":"2026-05-18T04:22:20.459722+00:00"}