{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:XWLX7ZNQFUNPHQ4E6OOOYY5UVC","short_pith_number":"pith:XWLX7ZNQ","schema_version":"1.0","canonical_sha256":"bd977fe5b02d1af3c384f39cec63b4a8af26d7bf9eb03263f8d3e4b2922395c7","source":{"kind":"arxiv","id":"1406.2201","version":1},"attestation_state":"computed","paper":{"title":"A viable Starobinsky-like inflationary scenario in the light of Planck and BICEP2 results","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"J. A. S. Lima, J. Sol\\`a, S. Basilakos","submitted_at":"2014-06-09T14:49:14Z","abstract_excerpt":"The recent CMB data from Planck and BICEP2 observations have opened a new window for inflationary cosmology. In this Essay we compare three Starobinsky-like inflationary scenarios: (i) the original Starobinsky proposal; (ii) a family of dynamically broken SUGRA models; and (iii) a class of \"decaying\" vacuum $\\Lambda(H)$ cosmologies. We then focus on the $\\Lambda(H)$ variant, which spans the complete cosmic history of the universe from an early inflationary stage, followed by the \"graceful exit\" into the standard radiation regime, the matter epoch and, finally, the late-time accelerated expansi"},"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":"1406.2201","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-06-09T14:49:14Z","cross_cats_sorted":["gr-qc","hep-ph","hep-th"],"title_canon_sha256":"2dc27372a7f503ae632657ede8c57b9b56494f20c2cdb75a46e433ef530601aa","abstract_canon_sha256":"6d73e8ed1f9e133db5e0ea06978d65d4b62ffcbc4b92ca5ddeafe3212d134389"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:01.110867Z","signature_b64":"RXZ4U9zRPx3IjaAVRPksun/75JXQo+8rh9AzBhUzgeanoMI+1k8iktFnPQc5MNKfPDRStfJ4Wv6gXnJ05x0MAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bd977fe5b02d1af3c384f39cec63b4a8af26d7bf9eb03263f8d3e4b2922395c7","last_reissued_at":"2026-05-18T01:43:01.110394Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:01.110394Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A viable Starobinsky-like inflationary scenario in the light of Planck and BICEP2 results","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"J. A. S. Lima, J. Sol\\`a, S. Basilakos","submitted_at":"2014-06-09T14:49:14Z","abstract_excerpt":"The recent CMB data from Planck and BICEP2 observations have opened a new window for inflationary cosmology. In this Essay we compare three Starobinsky-like inflationary scenarios: (i) the original Starobinsky proposal; (ii) a family of dynamically broken SUGRA models; and (iii) a class of \"decaying\" vacuum $\\Lambda(H)$ cosmologies. We then focus on the $\\Lambda(H)$ variant, which spans the complete cosmic history of the universe from an early inflationary stage, followed by the \"graceful exit\" into the standard radiation regime, the matter epoch and, finally, the late-time accelerated expansi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1406.2201","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":"1406.2201","created_at":"2026-05-18T01:43:01.110478+00:00"},{"alias_kind":"arxiv_version","alias_value":"1406.2201v1","created_at":"2026-05-18T01:43:01.110478+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1406.2201","created_at":"2026-05-18T01:43:01.110478+00:00"},{"alias_kind":"pith_short_12","alias_value":"XWLX7ZNQFUNP","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_16","alias_value":"XWLX7ZNQFUNPHQ4E","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_8","alias_value":"XWLX7ZNQ","created_at":"2026-05-18T12:28:57.508820+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/XWLX7ZNQFUNPHQ4E6OOOYY5UVC","json":"https://pith.science/pith/XWLX7ZNQFUNPHQ4E6OOOYY5UVC.json","graph_json":"https://pith.science/api/pith-number/XWLX7ZNQFUNPHQ4E6OOOYY5UVC/graph.json","events_json":"https://pith.science/api/pith-number/XWLX7ZNQFUNPHQ4E6OOOYY5UVC/events.json","paper":"https://pith.science/paper/XWLX7ZNQ"},"agent_actions":{"view_html":"https://pith.science/pith/XWLX7ZNQFUNPHQ4E6OOOYY5UVC","download_json":"https://pith.science/pith/XWLX7ZNQFUNPHQ4E6OOOYY5UVC.json","view_paper":"https://pith.science/paper/XWLX7ZNQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1406.2201&json=true","fetch_graph":"https://pith.science/api/pith-number/XWLX7ZNQFUNPHQ4E6OOOYY5UVC/graph.json","fetch_events":"https://pith.science/api/pith-number/XWLX7ZNQFUNPHQ4E6OOOYY5UVC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XWLX7ZNQFUNPHQ4E6OOOYY5UVC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XWLX7ZNQFUNPHQ4E6OOOYY5UVC/action/storage_attestation","attest_author":"https://pith.science/pith/XWLX7ZNQFUNPHQ4E6OOOYY5UVC/action/author_attestation","sign_citation":"https://pith.science/pith/XWLX7ZNQFUNPHQ4E6OOOYY5UVC/action/citation_signature","submit_replication":"https://pith.science/pith/XWLX7ZNQFUNPHQ4E6OOOYY5UVC/action/replication_record"}},"created_at":"2026-05-18T01:43:01.110478+00:00","updated_at":"2026-05-18T01:43:01.110478+00:00"}