{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:45H3PSW3EBGK2Y2KOPVSOTK2AP","short_pith_number":"pith:45H3PSW3","schema_version":"1.0","canonical_sha256":"e74fb7cadb204cad634a73eb274d5a03e11d9709de293a7537f03b3f84e283af","source":{"kind":"arxiv","id":"2503.01228","version":1},"attestation_state":"computed","paper":{"title":"Reheating after Axion Inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Kyohei Mukaida, Tenta Tsuji, Tomohiro Fujita","submitted_at":"2025-03-03T06:51:33Z","abstract_excerpt":"We investigate the reheating process in an axion inflation model where the inflaton couples to non-Abelian gauge fields via the Chern-Simons coupling. The Chern-Simons coupling leads to the efficient production of gauge fields via a tachyonic instability during inflation, whose implications have been actively studied in the literatures. Moreover, it has been recently pointed out that the produced gauge fields can be even thermalized during inflation, leading to warm inflation. Apparently, these findings seem to imply that the reheating is completed immediately after inflation because the tachy"},"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":"2503.01228","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2025-03-03T06:51:33Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"def4153ac9c38b814070838a65ebc3683e041095f9402f870f99d0b8651ace73","abstract_canon_sha256":"6450820184d0d26b9460cafca450344077c5452d082fb4584171ae182330b4b1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:23:02.283927Z","signature_b64":"B+1qVEZraWOaYi+5JW5H1Iz+/oOjNjuKsOG5srpgpvwi2hPvC1D5yOajwfL6v64GFRJ87K1grAaQ9XpLrpLMBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e74fb7cadb204cad634a73eb274d5a03e11d9709de293a7537f03b3f84e283af","last_reissued_at":"2026-07-05T10:23:02.283163Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:23:02.283163Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Reheating after Axion Inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Kyohei Mukaida, Tenta Tsuji, Tomohiro Fujita","submitted_at":"2025-03-03T06:51:33Z","abstract_excerpt":"We investigate the reheating process in an axion inflation model where the inflaton couples to non-Abelian gauge fields via the Chern-Simons coupling. The Chern-Simons coupling leads to the efficient production of gauge fields via a tachyonic instability during inflation, whose implications have been actively studied in the literatures. Moreover, it has been recently pointed out that the produced gauge fields can be even thermalized during inflation, leading to warm inflation. Apparently, these findings seem to imply that the reheating is completed immediately after inflation because the tachy"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2503.01228","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/2503.01228/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":"2503.01228","created_at":"2026-07-05T10:23:02.283263+00:00"},{"alias_kind":"arxiv_version","alias_value":"2503.01228v1","created_at":"2026-07-05T10:23:02.283263+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2503.01228","created_at":"2026-07-05T10:23:02.283263+00:00"},{"alias_kind":"pith_short_12","alias_value":"45H3PSW3EBGK","created_at":"2026-07-05T10:23:02.283263+00:00"},{"alias_kind":"pith_short_16","alias_value":"45H3PSW3EBGK2Y2K","created_at":"2026-07-05T10:23:02.283263+00:00"},{"alias_kind":"pith_short_8","alias_value":"45H3PSW3","created_at":"2026-07-05T10:23:02.283263+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2601.08221","citing_title":"Energy and momentum dependence of the soft-axion interaction rate","ref_index":12,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/45H3PSW3EBGK2Y2KOPVSOTK2AP","json":"https://pith.science/pith/45H3PSW3EBGK2Y2KOPVSOTK2AP.json","graph_json":"https://pith.science/api/pith-number/45H3PSW3EBGK2Y2KOPVSOTK2AP/graph.json","events_json":"https://pith.science/api/pith-number/45H3PSW3EBGK2Y2KOPVSOTK2AP/events.json","paper":"https://pith.science/paper/45H3PSW3"},"agent_actions":{"view_html":"https://pith.science/pith/45H3PSW3EBGK2Y2KOPVSOTK2AP","download_json":"https://pith.science/pith/45H3PSW3EBGK2Y2KOPVSOTK2AP.json","view_paper":"https://pith.science/paper/45H3PSW3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2503.01228&json=true","fetch_graph":"https://pith.science/api/pith-number/45H3PSW3EBGK2Y2KOPVSOTK2AP/graph.json","fetch_events":"https://pith.science/api/pith-number/45H3PSW3EBGK2Y2KOPVSOTK2AP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/45H3PSW3EBGK2Y2KOPVSOTK2AP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/45H3PSW3EBGK2Y2KOPVSOTK2AP/action/storage_attestation","attest_author":"https://pith.science/pith/45H3PSW3EBGK2Y2KOPVSOTK2AP/action/author_attestation","sign_citation":"https://pith.science/pith/45H3PSW3EBGK2Y2KOPVSOTK2AP/action/citation_signature","submit_replication":"https://pith.science/pith/45H3PSW3EBGK2Y2KOPVSOTK2AP/action/replication_record"}},"created_at":"2026-07-05T10:23:02.283263+00:00","updated_at":"2026-07-05T10:23:02.283263+00:00"}