{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:OJUEEHZFSKDXEERANWI5WEDCQY","short_pith_number":"pith:OJUEEHZF","schema_version":"1.0","canonical_sha256":"7268421f2592877212206d91db10628606777401cabc1866245e78aff17fe60e","source":{"kind":"arxiv","id":"2412.02696","version":2},"attestation_state":"computed","paper":{"title":"Stage IV CMB forecasts for warm inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"F. B. M. dos Santos, G. Rodrigues, J. S. Alcaniz, R. de Souza","submitted_at":"2024-12-03T18:59:41Z","abstract_excerpt":"We report forecast constraints on warm inflation in the light of future cosmic microwave background (CMB) surveys, with data expected to be available in the coming decade. These observations could finally give us the missing information necessary to unveil the production of gravitational waves during inflation, reflected by the detection of a non-zero tensor-to-scalar ratio crucial to the B-mode power spectrum of the CMB. We consider the impact of three future surveys, namely the CMB-S4, Simons Observatory, and the space-borne $\\textit{LiteBIRD}$, in restricting the parameter space of four typ"},"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":"2412.02696","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-12-03T18:59:41Z","cross_cats_sorted":[],"title_canon_sha256":"b9ee06eb9c9e65177c9643ee7878de5a7fde6a36f5fa223e2294809a30301f67","abstract_canon_sha256":"921e9fa9944e544bf32e73dbfea33a5872bb23712429995f3de4d61d1356160b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:43:41.500646Z","signature_b64":"4SjfDQ9xQv9vr37iYWczH775KD6xQrYLqx1eKFY5VkRPGO34sCXLQPRUn6ouqRqD9ueKpqphXxguoZBjUscpDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7268421f2592877212206d91db10628606777401cabc1866245e78aff17fe60e","last_reissued_at":"2026-07-05T10:43:41.500138Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:43:41.500138Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stage IV CMB forecasts for warm inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"F. B. M. dos Santos, G. Rodrigues, J. S. Alcaniz, R. de Souza","submitted_at":"2024-12-03T18:59:41Z","abstract_excerpt":"We report forecast constraints on warm inflation in the light of future cosmic microwave background (CMB) surveys, with data expected to be available in the coming decade. These observations could finally give us the missing information necessary to unveil the production of gravitational waves during inflation, reflected by the detection of a non-zero tensor-to-scalar ratio crucial to the B-mode power spectrum of the CMB. We consider the impact of three future surveys, namely the CMB-S4, Simons Observatory, and the space-borne $\\textit{LiteBIRD}$, in restricting the parameter space of four typ"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.02696","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/2412.02696/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":"2412.02696","created_at":"2026-07-05T10:43:41.500200+00:00"},{"alias_kind":"arxiv_version","alias_value":"2412.02696v2","created_at":"2026-07-05T10:43:41.500200+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2412.02696","created_at":"2026-07-05T10:43:41.500200+00:00"},{"alias_kind":"pith_short_12","alias_value":"OJUEEHZFSKDX","created_at":"2026-07-05T10:43:41.500200+00:00"},{"alias_kind":"pith_short_16","alias_value":"OJUEEHZFSKDXEERA","created_at":"2026-07-05T10:43:41.500200+00:00"},{"alias_kind":"pith_short_8","alias_value":"OJUEEHZF","created_at":"2026-07-05T10:43:41.500200+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/OJUEEHZFSKDXEERANWI5WEDCQY","json":"https://pith.science/pith/OJUEEHZFSKDXEERANWI5WEDCQY.json","graph_json":"https://pith.science/api/pith-number/OJUEEHZFSKDXEERANWI5WEDCQY/graph.json","events_json":"https://pith.science/api/pith-number/OJUEEHZFSKDXEERANWI5WEDCQY/events.json","paper":"https://pith.science/paper/OJUEEHZF"},"agent_actions":{"view_html":"https://pith.science/pith/OJUEEHZFSKDXEERANWI5WEDCQY","download_json":"https://pith.science/pith/OJUEEHZFSKDXEERANWI5WEDCQY.json","view_paper":"https://pith.science/paper/OJUEEHZF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2412.02696&json=true","fetch_graph":"https://pith.science/api/pith-number/OJUEEHZFSKDXEERANWI5WEDCQY/graph.json","fetch_events":"https://pith.science/api/pith-number/OJUEEHZFSKDXEERANWI5WEDCQY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OJUEEHZFSKDXEERANWI5WEDCQY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OJUEEHZFSKDXEERANWI5WEDCQY/action/storage_attestation","attest_author":"https://pith.science/pith/OJUEEHZFSKDXEERANWI5WEDCQY/action/author_attestation","sign_citation":"https://pith.science/pith/OJUEEHZFSKDXEERANWI5WEDCQY/action/citation_signature","submit_replication":"https://pith.science/pith/OJUEEHZFSKDXEERANWI5WEDCQY/action/replication_record"}},"created_at":"2026-07-05T10:43:41.500200+00:00","updated_at":"2026-07-05T10:43:41.500200+00:00"}