{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:76NO3ARCKWUVHKI5E6RH7P3IX6","short_pith_number":"pith:76NO3ARC","schema_version":"1.0","canonical_sha256":"ff9aed822255a953a91d27a27fbf68bfb26a19f43f8167238d05f79a6a65e95c","source":{"kind":"arxiv","id":"2404.10647","version":2},"attestation_state":"computed","paper":{"title":"Cosmic Inflation at the Crossroads","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":"Christophe Ringeval, Jerome Martin, Vincent Vennin","submitted_at":"2024-04-16T15:21:23Z","abstract_excerpt":"The capability of Cosmic Inflation to explain the latest Cosmic Microwave Background and Baryonic Acoustic Oscillation data is assessed by performing Bayesian model comparison within the landscape of nearly three-hundred models of single-field slow-roll inflation. We present the first Bayesian data analysis based on the third-order slow-roll primordial power spectra. In particular, the fourth Hubble-flow function $\\epsilon_4$ remains unbounded while the third function verifies, at two-sigma, $\\epsilon_{3}\\in[-0.4,0.5]$, which is perfectly compatible with the slow-roll predictions for the runni"},"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":"2404.10647","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-04-16T15:21:23Z","cross_cats_sorted":["gr-qc","hep-ph","hep-th"],"title_canon_sha256":"1ae3e57df680ed8e0f7ca1db894ac5371787fadaebe366e3ba166641ffd0b200","abstract_canon_sha256":"02b45aac38ca2a7bc8d767e305c23a91e44bf43240375a395840ff6f329c82ca"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:59:08.410245Z","signature_b64":"SRfXxvEZXEKEpeqkKgu9+0wuw+8GusBAYFJfG0+DTsUOow/aYFYq6dPU5muuWR29YMReIhSwhZt23ajjIsT2CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ff9aed822255a953a91d27a27fbf68bfb26a19f43f8167238d05f79a6a65e95c","last_reissued_at":"2026-07-05T08:59:08.409831Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:59:08.409831Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmic Inflation at the Crossroads","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":"Christophe Ringeval, Jerome Martin, Vincent Vennin","submitted_at":"2024-04-16T15:21:23Z","abstract_excerpt":"The capability of Cosmic Inflation to explain the latest Cosmic Microwave Background and Baryonic Acoustic Oscillation data is assessed by performing Bayesian model comparison within the landscape of nearly three-hundred models of single-field slow-roll inflation. We present the first Bayesian data analysis based on the third-order slow-roll primordial power spectra. In particular, the fourth Hubble-flow function $\\epsilon_4$ remains unbounded while the third function verifies, at two-sigma, $\\epsilon_{3}\\in[-0.4,0.5]$, which is perfectly compatible with the slow-roll predictions for the runni"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2404.10647","kind":"arxiv","version":2},"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/2404.10647/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":"2404.10647","created_at":"2026-07-05T08:59:08.409885+00:00"},{"alias_kind":"arxiv_version","alias_value":"2404.10647v2","created_at":"2026-07-05T08:59:08.409885+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2404.10647","created_at":"2026-07-05T08:59:08.409885+00:00"},{"alias_kind":"pith_short_12","alias_value":"76NO3ARCKWUV","created_at":"2026-07-05T08:59:08.409885+00:00"},{"alias_kind":"pith_short_16","alias_value":"76NO3ARCKWUVHKI5","created_at":"2026-07-05T08:59:08.409885+00:00"},{"alias_kind":"pith_short_8","alias_value":"76NO3ARC","created_at":"2026-07-05T08:59:08.409885+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07193","citing_title":"Higgs boson mass and thermal wino dark matter from Starobinsky supergravity with the MSSM","ref_index":3,"is_internal_anchor":true},{"citing_arxiv_id":"2606.25015","citing_title":"Cosmological gravitational particle production in multifield inflation","ref_index":2,"is_internal_anchor":false},{"citing_arxiv_id":"2606.12519","citing_title":"Observing Cosmic Reheating with the expanded Simons Observatory","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"2605.31323","citing_title":"Time-reversed stochastic inflation in the quantum well","ref_index":28,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/76NO3ARCKWUVHKI5E6RH7P3IX6","json":"https://pith.science/pith/76NO3ARCKWUVHKI5E6RH7P3IX6.json","graph_json":"https://pith.science/api/pith-number/76NO3ARCKWUVHKI5E6RH7P3IX6/graph.json","events_json":"https://pith.science/api/pith-number/76NO3ARCKWUVHKI5E6RH7P3IX6/events.json","paper":"https://pith.science/paper/76NO3ARC"},"agent_actions":{"view_html":"https://pith.science/pith/76NO3ARCKWUVHKI5E6RH7P3IX6","download_json":"https://pith.science/pith/76NO3ARCKWUVHKI5E6RH7P3IX6.json","view_paper":"https://pith.science/paper/76NO3ARC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2404.10647&json=true","fetch_graph":"https://pith.science/api/pith-number/76NO3ARCKWUVHKI5E6RH7P3IX6/graph.json","fetch_events":"https://pith.science/api/pith-number/76NO3ARCKWUVHKI5E6RH7P3IX6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/76NO3ARCKWUVHKI5E6RH7P3IX6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/76NO3ARCKWUVHKI5E6RH7P3IX6/action/storage_attestation","attest_author":"https://pith.science/pith/76NO3ARCKWUVHKI5E6RH7P3IX6/action/author_attestation","sign_citation":"https://pith.science/pith/76NO3ARCKWUVHKI5E6RH7P3IX6/action/citation_signature","submit_replication":"https://pith.science/pith/76NO3ARCKWUVHKI5E6RH7P3IX6/action/replication_record"}},"created_at":"2026-07-05T08:59:08.409885+00:00","updated_at":"2026-07-05T08:59:08.409885+00:00"}