{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:PE5756GZ6JUQWRHHI4WAJHDPPX","short_pith_number":"pith:PE5756GZ","schema_version":"1.0","canonical_sha256":"793bfef8d9f2690b44e7472c049c6f7df909d4be9c2c01b522f772aa661689c6","source":{"kind":"arxiv","id":"2012.03988","version":1},"attestation_state":"computed","paper":{"title":"Warm Inflation, Neutrinos and Dark matter: a minimal extension of the Standard Model","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-ph","authors_text":"Jo\\~ao G. Rosa, Luis B. Ventura, Miguel Levy","submitted_at":"2020-12-07T19:02:08Z","abstract_excerpt":"We show that warm inflation can be realized within a minimal extension of the Standard Model with three right-handed neutrinos, three complex scalars and a gauged lepton/B-L U(1) symmetry. This simple model can address all the shortcomings of the Standard Model that are not related to fine-tuning, within general relativity, with distinctive experimental signatures that can be probed in the near future. The inflaton field emerges from the collective breaking of the U(1) symmetry, and interacts with two of the right-handed neutrinos, sustaining a high-temperature radiation bath during inflation."},"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":"2012.03988","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2020-12-07T19:02:08Z","cross_cats_sorted":["astro-ph.CO","gr-qc"],"title_canon_sha256":"4484399f1b255550828f02f8c35a10362705445a8c758a03b2b5039d6e830946","abstract_canon_sha256":"05d8d51a418943eeb10c9ae7dc1d36f2b9288c25abc3ebca6247937bb2620120"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:45:24.783926Z","signature_b64":"Pwn2ZDT7iGCau6PRjGdCgehw88elogzNdTSHFsd+4BYKvfKoPEq7q3MraCFnfJiU/RYl+VHesqXL0TechZRGDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"793bfef8d9f2690b44e7472c049c6f7df909d4be9c2c01b522f772aa661689c6","last_reissued_at":"2026-07-05T03:45:24.783550Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:45:24.783550Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Warm Inflation, Neutrinos and Dark matter: a minimal extension of the Standard Model","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-ph","authors_text":"Jo\\~ao G. Rosa, Luis B. Ventura, Miguel Levy","submitted_at":"2020-12-07T19:02:08Z","abstract_excerpt":"We show that warm inflation can be realized within a minimal extension of the Standard Model with three right-handed neutrinos, three complex scalars and a gauged lepton/B-L U(1) symmetry. This simple model can address all the shortcomings of the Standard Model that are not related to fine-tuning, within general relativity, with distinctive experimental signatures that can be probed in the near future. The inflaton field emerges from the collective breaking of the U(1) symmetry, and interacts with two of the right-handed neutrinos, sustaining a high-temperature radiation bath during inflation."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2012.03988","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/2012.03988/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":"2012.03988","created_at":"2026-07-05T03:45:24.783606+00:00"},{"alias_kind":"arxiv_version","alias_value":"2012.03988v1","created_at":"2026-07-05T03:45:24.783606+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2012.03988","created_at":"2026-07-05T03:45:24.783606+00:00"},{"alias_kind":"pith_short_12","alias_value":"PE5756GZ6JUQ","created_at":"2026-07-05T03:45:24.783606+00:00"},{"alias_kind":"pith_short_16","alias_value":"PE5756GZ6JUQWRHH","created_at":"2026-07-05T03:45:24.783606+00:00"},{"alias_kind":"pith_short_8","alias_value":"PE5756GZ","created_at":"2026-07-05T03:45:24.783606+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.22147","citing_title":"Dark Matter as an Inflationary Relic in Warm Inflation","ref_index":44,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PE5756GZ6JUQWRHHI4WAJHDPPX","json":"https://pith.science/pith/PE5756GZ6JUQWRHHI4WAJHDPPX.json","graph_json":"https://pith.science/api/pith-number/PE5756GZ6JUQWRHHI4WAJHDPPX/graph.json","events_json":"https://pith.science/api/pith-number/PE5756GZ6JUQWRHHI4WAJHDPPX/events.json","paper":"https://pith.science/paper/PE5756GZ"},"agent_actions":{"view_html":"https://pith.science/pith/PE5756GZ6JUQWRHHI4WAJHDPPX","download_json":"https://pith.science/pith/PE5756GZ6JUQWRHHI4WAJHDPPX.json","view_paper":"https://pith.science/paper/PE5756GZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2012.03988&json=true","fetch_graph":"https://pith.science/api/pith-number/PE5756GZ6JUQWRHHI4WAJHDPPX/graph.json","fetch_events":"https://pith.science/api/pith-number/PE5756GZ6JUQWRHHI4WAJHDPPX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PE5756GZ6JUQWRHHI4WAJHDPPX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PE5756GZ6JUQWRHHI4WAJHDPPX/action/storage_attestation","attest_author":"https://pith.science/pith/PE5756GZ6JUQWRHHI4WAJHDPPX/action/author_attestation","sign_citation":"https://pith.science/pith/PE5756GZ6JUQWRHHI4WAJHDPPX/action/citation_signature","submit_replication":"https://pith.science/pith/PE5756GZ6JUQWRHHI4WAJHDPPX/action/replication_record"}},"created_at":"2026-07-05T03:45:24.783606+00:00","updated_at":"2026-07-05T03:45:24.783606+00:00"}