{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:SHNKKYVXDU4UJI5TUDOIOHABSF","short_pith_number":"pith:SHNKKYVX","schema_version":"1.0","canonical_sha256":"91daa562b71d3944a3b3a0dc871c01916ab0566cb22531eb73f7fcedfbc9dbfa","source":{"kind":"arxiv","id":"2406.00340","version":2},"attestation_state":"computed","paper":{"title":"Reassessing constant-roll Warm Inflation","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Kaushik Bhattacharya, Sandip Biswas, Suratna Das","submitted_at":"2024-06-01T07:35:06Z","abstract_excerpt":"Departing from standard slow-roll conditions is one way of putting the inflationary paradigm to test, and constraining the dynamics of the inflaton field with a constant-rate of roll of the inflaton field, a.k.a. the constant-roll scenario, is one way of exploring such deviation from the standard slow-roll dynamics. In this manuscript we explore such a possibility in a variant inflationary scenario, known as Warm Inflation. We construct and derive the conditions for having constant-roll WI models where inflation lasts at least for 60 $e-$folds, gracefully exits the constant-roll inflation phas"},"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":"2406.00340","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-06-01T07:35:06Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"059ccfc19e3385fd38d01ccb8636b17476e102e81c6a7d01664a916c00af43f7","abstract_canon_sha256":"51b4b8db0e1a8f60f689bb2a55de45a43f789078a068fbce2c51b1ee919bc5ad"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:08:26.236661Z","signature_b64":"F10jQM/8E3hNmplJe6IJZeI8I4VcYoXeAaoFOT3z2i9Lmd1yicX2sGTFKnMF3QqI9ZCww3mQD6XLg2g3pmOYDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"91daa562b71d3944a3b3a0dc871c01916ab0566cb22531eb73f7fcedfbc9dbfa","last_reissued_at":"2026-07-05T09:08:26.236096Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:08:26.236096Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Reassessing constant-roll Warm Inflation","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Kaushik Bhattacharya, Sandip Biswas, Suratna Das","submitted_at":"2024-06-01T07:35:06Z","abstract_excerpt":"Departing from standard slow-roll conditions is one way of putting the inflationary paradigm to test, and constraining the dynamics of the inflaton field with a constant-rate of roll of the inflaton field, a.k.a. the constant-roll scenario, is one way of exploring such deviation from the standard slow-roll dynamics. In this manuscript we explore such a possibility in a variant inflationary scenario, known as Warm Inflation. We construct and derive the conditions for having constant-roll WI models where inflation lasts at least for 60 $e-$folds, gracefully exits the constant-roll inflation phas"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2406.00340","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/2406.00340/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":"2406.00340","created_at":"2026-07-05T09:08:26.236169+00:00"},{"alias_kind":"arxiv_version","alias_value":"2406.00340v2","created_at":"2026-07-05T09:08:26.236169+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2406.00340","created_at":"2026-07-05T09:08:26.236169+00:00"},{"alias_kind":"pith_short_12","alias_value":"SHNKKYVXDU4U","created_at":"2026-07-05T09:08:26.236169+00:00"},{"alias_kind":"pith_short_16","alias_value":"SHNKKYVXDU4UJI5T","created_at":"2026-07-05T09:08:26.236169+00:00"},{"alias_kind":"pith_short_8","alias_value":"SHNKKYVX","created_at":"2026-07-05T09:08:26.236169+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.24654","citing_title":"SWIM: Stochastic Warm Inflation Module to generate and analyse Warm Inflationary power spectrum","ref_index":25,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SHNKKYVXDU4UJI5TUDOIOHABSF","json":"https://pith.science/pith/SHNKKYVXDU4UJI5TUDOIOHABSF.json","graph_json":"https://pith.science/api/pith-number/SHNKKYVXDU4UJI5TUDOIOHABSF/graph.json","events_json":"https://pith.science/api/pith-number/SHNKKYVXDU4UJI5TUDOIOHABSF/events.json","paper":"https://pith.science/paper/SHNKKYVX"},"agent_actions":{"view_html":"https://pith.science/pith/SHNKKYVXDU4UJI5TUDOIOHABSF","download_json":"https://pith.science/pith/SHNKKYVXDU4UJI5TUDOIOHABSF.json","view_paper":"https://pith.science/paper/SHNKKYVX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2406.00340&json=true","fetch_graph":"https://pith.science/api/pith-number/SHNKKYVXDU4UJI5TUDOIOHABSF/graph.json","fetch_events":"https://pith.science/api/pith-number/SHNKKYVXDU4UJI5TUDOIOHABSF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SHNKKYVXDU4UJI5TUDOIOHABSF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SHNKKYVXDU4UJI5TUDOIOHABSF/action/storage_attestation","attest_author":"https://pith.science/pith/SHNKKYVXDU4UJI5TUDOIOHABSF/action/author_attestation","sign_citation":"https://pith.science/pith/SHNKKYVXDU4UJI5TUDOIOHABSF/action/citation_signature","submit_replication":"https://pith.science/pith/SHNKKYVXDU4UJI5TUDOIOHABSF/action/replication_record"}},"created_at":"2026-07-05T09:08:26.236169+00:00","updated_at":"2026-07-05T09:08:26.236169+00:00"}