{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:3ZXK5L3BITUSGU2XWBPSVEMWHK","short_pith_number":"pith:3ZXK5L3B","schema_version":"1.0","canonical_sha256":"de6eaeaf6144e9235357b05f2a91963a8740aa2f0dbae13fb55974acaf5107e6","source":{"kind":"arxiv","id":"1901.04646","version":1},"attestation_state":"computed","paper":{"title":"On the constant-roll inflation with large and small $\\eta_H$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Qing Gao, Yungui Gong, Zhu Yi","submitted_at":"2019-01-15T03:27:54Z","abstract_excerpt":"We study the seemingly duality between large and small $\\eta_H$ for the constant-roll inflation with the second slow-roll parameter $\\eta_H$ being a constant. In the previous studies, only the constant-roll inflationary models with small $\\eta_H$ are found to be consistent with the observations. The seemingly duality suggests that the constant-roll inflationary models with large $\\eta_H$ may be also consistent with the observations. We find that the duality between the constant-roll inflation with large and small $\\eta_H$ does not exist because both the background and scalar perturbation evolu"},"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":"1901.04646","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-01-15T03:27:54Z","cross_cats_sorted":[],"title_canon_sha256":"53eac7c0a7b394cbd81a75f16ae3237c5a8521461f0a2efe5b1fc11de419c1e1","abstract_canon_sha256":"c399a70daf7a6843c4c382548a432678a8cc4ea7000b2bc79ef5955ecfa49312"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:16:02.912313Z","signature_b64":"sYNENS56Fv/ICfRpOSOuWuljO8VSHYTkDXGIvzaMzIloo/BOYPBe70csEprqa5MFsC4FmVDhMje3sT0SDFRqDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"de6eaeaf6144e9235357b05f2a91963a8740aa2f0dbae13fb55974acaf5107e6","last_reissued_at":"2026-07-05T00:16:02.911917Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:16:02.911917Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the constant-roll inflation with large and small $\\eta_H$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Qing Gao, Yungui Gong, Zhu Yi","submitted_at":"2019-01-15T03:27:54Z","abstract_excerpt":"We study the seemingly duality between large and small $\\eta_H$ for the constant-roll inflation with the second slow-roll parameter $\\eta_H$ being a constant. In the previous studies, only the constant-roll inflationary models with small $\\eta_H$ are found to be consistent with the observations. The seemingly duality suggests that the constant-roll inflationary models with large $\\eta_H$ may be also consistent with the observations. We find that the duality between the constant-roll inflation with large and small $\\eta_H$ does not exist because both the background and scalar perturbation evolu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1901.04646","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1901.04646/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":"1901.04646","created_at":"2026-07-05T00:16:02.911975+00:00"},{"alias_kind":"arxiv_version","alias_value":"1901.04646v1","created_at":"2026-07-05T00:16:02.911975+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1901.04646","created_at":"2026-07-05T00:16:02.911975+00:00"},{"alias_kind":"pith_short_12","alias_value":"3ZXK5L3BITUS","created_at":"2026-07-05T00:16:02.911975+00:00"},{"alias_kind":"pith_short_16","alias_value":"3ZXK5L3BITUSGU2X","created_at":"2026-07-05T00:16:02.911975+00:00"},{"alias_kind":"pith_short_8","alias_value":"3ZXK5L3B","created_at":"2026-07-05T00:16:02.911975+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.24111","citing_title":"Constant-Roll Inflation: Analytical Formulae for Power Spectrum and Implications for Induced Gravitational Waves","ref_index":108,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3ZXK5L3BITUSGU2XWBPSVEMWHK","json":"https://pith.science/pith/3ZXK5L3BITUSGU2XWBPSVEMWHK.json","graph_json":"https://pith.science/api/pith-number/3ZXK5L3BITUSGU2XWBPSVEMWHK/graph.json","events_json":"https://pith.science/api/pith-number/3ZXK5L3BITUSGU2XWBPSVEMWHK/events.json","paper":"https://pith.science/paper/3ZXK5L3B"},"agent_actions":{"view_html":"https://pith.science/pith/3ZXK5L3BITUSGU2XWBPSVEMWHK","download_json":"https://pith.science/pith/3ZXK5L3BITUSGU2XWBPSVEMWHK.json","view_paper":"https://pith.science/paper/3ZXK5L3B","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1901.04646&json=true","fetch_graph":"https://pith.science/api/pith-number/3ZXK5L3BITUSGU2XWBPSVEMWHK/graph.json","fetch_events":"https://pith.science/api/pith-number/3ZXK5L3BITUSGU2XWBPSVEMWHK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3ZXK5L3BITUSGU2XWBPSVEMWHK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3ZXK5L3BITUSGU2XWBPSVEMWHK/action/storage_attestation","attest_author":"https://pith.science/pith/3ZXK5L3BITUSGU2XWBPSVEMWHK/action/author_attestation","sign_citation":"https://pith.science/pith/3ZXK5L3BITUSGU2XWBPSVEMWHK/action/citation_signature","submit_replication":"https://pith.science/pith/3ZXK5L3BITUSGU2XWBPSVEMWHK/action/replication_record"}},"created_at":"2026-07-05T00:16:02.911975+00:00","updated_at":"2026-07-05T00:16:02.911975+00:00"}