{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:XT6DQGMHKT3CG7AXD4ANS3O522","short_pith_number":"pith:XT6DQGMH","schema_version":"1.0","canonical_sha256":"bcfc38198754f6237c171f00d96dddd69addf7297ad8acffecd7f7a6f3557d05","source":{"kind":"arxiv","id":"1503.08867","version":1},"attestation_state":"computed","paper":{"title":"Phenomenological Aspects of No-Scale Inflation Models","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":"2015-03-30T22:35:23Z","abstract_excerpt":"We discuss phenomenological aspects of no-scale supergravity inflationary models motivated by compactified string models, in which the inflaton may be identified either as a K\\\"ahler modulus or an untwisted matter field, focusing on models that make predictions for the scalar spectral index $n_s$ and the tensor-to-scalar ratio $r$ that are similar to the Starobinsky model. We discuss possible patterns of soft supersymmetry breaking, exhibiting examples of the pure no-scale type $m_0 = B_0 = A_0 = 0$, of the CMSSM type with universal $A_0$ and $m_0 \\ne 0$ at a high scale, and of the mSUGRA type"},"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":"1503.08867","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2015-03-30T22:35:23Z","cross_cats_sorted":["astro-ph.CO","gr-qc","hep-th"],"title_canon_sha256":"f0c1b9087a46e1cb0d4bb58942ee1a3b89c23a50db2cc4f86045ea8383af4935","abstract_canon_sha256":"7d2318a6af3a721312e9290f81a7717b2d298219537a9d022bed3bab70e336fe"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:31:03.051602Z","signature_b64":"rRvrAitxaUK50ekmDcXhf49oZJ0q9BdEcU4+KGjUByEZIRXMDOWDaRnN7FN5JqyLh8RtbPsgIVssZqbQAeZqAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bcfc38198754f6237c171f00d96dddd69addf7297ad8acffecd7f7a6f3557d05","last_reissued_at":"2026-05-18T01:31:03.051152Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:31:03.051152Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Phenomenological Aspects of No-Scale Inflation Models","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":"2015-03-30T22:35:23Z","abstract_excerpt":"We discuss phenomenological aspects of no-scale supergravity inflationary models motivated by compactified string models, in which the inflaton may be identified either as a K\\\"ahler modulus or an untwisted matter field, focusing on models that make predictions for the scalar spectral index $n_s$ and the tensor-to-scalar ratio $r$ that are similar to the Starobinsky model. We discuss possible patterns of soft supersymmetry breaking, exhibiting examples of the pure no-scale type $m_0 = B_0 = A_0 = 0$, of the CMSSM type with universal $A_0$ and $m_0 \\ne 0$ at a high scale, and of the mSUGRA type"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1503.08867","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":"1503.08867","created_at":"2026-05-18T01:31:03.051218+00:00"},{"alias_kind":"arxiv_version","alias_value":"1503.08867v1","created_at":"2026-05-18T01:31:03.051218+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1503.08867","created_at":"2026-05-18T01:31:03.051218+00:00"},{"alias_kind":"pith_short_12","alias_value":"XT6DQGMHKT3C","created_at":"2026-05-18T12:29:50.041715+00:00"},{"alias_kind":"pith_short_16","alias_value":"XT6DQGMHKT3CG7AX","created_at":"2026-05-18T12:29:50.041715+00:00"},{"alias_kind":"pith_short_8","alias_value":"XT6DQGMH","created_at":"2026-05-18T12:29:50.041715+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.05078","citing_title":"Gravitational Waves from Matter Perturbations of Spectator Scalar Fields","ref_index":73,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XT6DQGMHKT3CG7AXD4ANS3O522","json":"https://pith.science/pith/XT6DQGMHKT3CG7AXD4ANS3O522.json","graph_json":"https://pith.science/api/pith-number/XT6DQGMHKT3CG7AXD4ANS3O522/graph.json","events_json":"https://pith.science/api/pith-number/XT6DQGMHKT3CG7AXD4ANS3O522/events.json","paper":"https://pith.science/paper/XT6DQGMH"},"agent_actions":{"view_html":"https://pith.science/pith/XT6DQGMHKT3CG7AXD4ANS3O522","download_json":"https://pith.science/pith/XT6DQGMHKT3CG7AXD4ANS3O522.json","view_paper":"https://pith.science/paper/XT6DQGMH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1503.08867&json=true","fetch_graph":"https://pith.science/api/pith-number/XT6DQGMHKT3CG7AXD4ANS3O522/graph.json","fetch_events":"https://pith.science/api/pith-number/XT6DQGMHKT3CG7AXD4ANS3O522/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XT6DQGMHKT3CG7AXD4ANS3O522/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XT6DQGMHKT3CG7AXD4ANS3O522/action/storage_attestation","attest_author":"https://pith.science/pith/XT6DQGMHKT3CG7AXD4ANS3O522/action/author_attestation","sign_citation":"https://pith.science/pith/XT6DQGMHKT3CG7AXD4ANS3O522/action/citation_signature","submit_replication":"https://pith.science/pith/XT6DQGMHKT3CG7AXD4ANS3O522/action/replication_record"}},"created_at":"2026-05-18T01:31:03.051218+00:00","updated_at":"2026-05-18T01:31:03.051218+00:00"}