{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:OH43KBVD6PACP4SBQVG5H7JL2H","short_pith_number":"pith:OH43KBVD","schema_version":"1.0","canonical_sha256":"71f9b506a3f3c027f241854dd3fd2bd1fbceb75c1b1167525e9976656ba03a3c","source":{"kind":"arxiv","id":"1507.02308","version":1},"attestation_state":"computed","paper":{"title":"No-Scale Inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-th"],"primary_cat":"hep-ph","authors_text":"Dimitri V. Nanopoulos, John Ellis, Keith A. Olive, Marcos A. G. Garcia","submitted_at":"2015-07-08T20:57:55Z","abstract_excerpt":"Supersymmetry is the most natural framework for physics above the TeV scale, and the corresponding framework for early-Universe cosmology, including inflation, is supergravity. No-scale supergravity emerges from generic string compactifications and yields a non-negative potential, and is therefore a plausible framework for constructing models of inflation. No-scale inflation yields naturally predictions similar to those of the Starobinsky model based on $R + R^2$ gravity, with a tilted spectrum of scalar perturbations: $n_s \\sim 0.96$, and small values of the tensor-to-scalar perturbation rati"},"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":"1507.02308","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2015-07-08T20:57:55Z","cross_cats_sorted":["astro-ph.CO","gr-qc","hep-th"],"title_canon_sha256":"5aecf0fbd2de6b791e441e1c47cf8af37beaefd7c584ca1f97832e2fea6717b5","abstract_canon_sha256":"ac672ebb58c370ee13fcb730b00b0494b44ec15fc7d248a15e15198458e5b94c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:16:18.530104Z","signature_b64":"JJRKHPHftiSNgrz5Qh7hOge9Zu02Al3VmRs46T7faMVGCqdU7mhD0LskDBMnmx55RsyXx9hBUhsYRxU7M0HKDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"71f9b506a3f3c027f241854dd3fd2bd1fbceb75c1b1167525e9976656ba03a3c","last_reissued_at":"2026-05-18T01:16:18.529548Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:16:18.529548Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"No-Scale Inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-th"],"primary_cat":"hep-ph","authors_text":"Dimitri V. Nanopoulos, John Ellis, Keith A. Olive, Marcos A. G. Garcia","submitted_at":"2015-07-08T20:57:55Z","abstract_excerpt":"Supersymmetry is the most natural framework for physics above the TeV scale, and the corresponding framework for early-Universe cosmology, including inflation, is supergravity. No-scale supergravity emerges from generic string compactifications and yields a non-negative potential, and is therefore a plausible framework for constructing models of inflation. No-scale inflation yields naturally predictions similar to those of the Starobinsky model based on $R + R^2$ gravity, with a tilted spectrum of scalar perturbations: $n_s \\sim 0.96$, and small values of the tensor-to-scalar perturbation rati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1507.02308","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":"1507.02308","created_at":"2026-05-18T01:16:18.529644+00:00"},{"alias_kind":"arxiv_version","alias_value":"1507.02308v1","created_at":"2026-05-18T01:16:18.529644+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1507.02308","created_at":"2026-05-18T01:16:18.529644+00:00"},{"alias_kind":"pith_short_12","alias_value":"OH43KBVD6PAC","created_at":"2026-05-18T12:29:34.919912+00:00"},{"alias_kind":"pith_short_16","alias_value":"OH43KBVD6PACP4SB","created_at":"2026-05-18T12:29:34.919912+00:00"},{"alias_kind":"pith_short_8","alias_value":"OH43KBVD","created_at":"2026-05-18T12:29:34.919912+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.04378","citing_title":"Emergence of conformal properties in Finite Grand Unified Theories via reduction of couplings","ref_index":28,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OH43KBVD6PACP4SBQVG5H7JL2H","json":"https://pith.science/pith/OH43KBVD6PACP4SBQVG5H7JL2H.json","graph_json":"https://pith.science/api/pith-number/OH43KBVD6PACP4SBQVG5H7JL2H/graph.json","events_json":"https://pith.science/api/pith-number/OH43KBVD6PACP4SBQVG5H7JL2H/events.json","paper":"https://pith.science/paper/OH43KBVD"},"agent_actions":{"view_html":"https://pith.science/pith/OH43KBVD6PACP4SBQVG5H7JL2H","download_json":"https://pith.science/pith/OH43KBVD6PACP4SBQVG5H7JL2H.json","view_paper":"https://pith.science/paper/OH43KBVD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1507.02308&json=true","fetch_graph":"https://pith.science/api/pith-number/OH43KBVD6PACP4SBQVG5H7JL2H/graph.json","fetch_events":"https://pith.science/api/pith-number/OH43KBVD6PACP4SBQVG5H7JL2H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OH43KBVD6PACP4SBQVG5H7JL2H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OH43KBVD6PACP4SBQVG5H7JL2H/action/storage_attestation","attest_author":"https://pith.science/pith/OH43KBVD6PACP4SBQVG5H7JL2H/action/author_attestation","sign_citation":"https://pith.science/pith/OH43KBVD6PACP4SBQVG5H7JL2H/action/citation_signature","submit_replication":"https://pith.science/pith/OH43KBVD6PACP4SBQVG5H7JL2H/action/replication_record"}},"created_at":"2026-05-18T01:16:18.529644+00:00","updated_at":"2026-05-18T01:16:18.529644+00:00"}