{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:CUVTHK655QWTFDSDZ5AL4I4KTR","short_pith_number":"pith:CUVTHK65","schema_version":"1.0","canonical_sha256":"152b33abddec2d328e43cf40be238a9c77a042611366c1231e9f57d9d4506adb","source":{"kind":"arxiv","id":"1407.2211","version":2},"attestation_state":"computed","paper":{"title":"Warm inflation in the presence of magnetic fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Alejandro Ayala, Ana Julia Mizher, Angel Sanchez, Gabriella Piccinelli","submitted_at":"2014-07-08T18:50:15Z","abstract_excerpt":"We study the effects of primordial magnetic fields on the inflationary potential in the context of a warm inflation scenario. The model, based on global supersymmetry with a new-inflation-type potential and a coupling between the inflaton and a heavy intermediate superfield, is already known to preserve the flatness required for slow-roll conditions even after including thermal contributions. Here we show that the magnetic field makes the potential even flatter, retarding the transition and rendering it smoother."},"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":"1407.2211","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-07-08T18:50:15Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"8b57442e5a07c6e46293d28ea378da1a5614ff6c88bcc2b1fb02dde087010e70","abstract_canon_sha256":"e7ed7908a99c19d5c1ec7d960d632e9254dbed46ff670abe6a825b01e407d6e4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:40:55.680943Z","signature_b64":"oLaODi1Hxoip04WupvFvTy8tt05aSnPnlfeIH0llumPd52EHybd40T4/my1pjygoYDKY2Dkig68kxndL4UZiCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"152b33abddec2d328e43cf40be238a9c77a042611366c1231e9f57d9d4506adb","last_reissued_at":"2026-05-18T02:40:55.680379Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:40:55.680379Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Warm inflation in the presence of magnetic fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Alejandro Ayala, Ana Julia Mizher, Angel Sanchez, Gabriella Piccinelli","submitted_at":"2014-07-08T18:50:15Z","abstract_excerpt":"We study the effects of primordial magnetic fields on the inflationary potential in the context of a warm inflation scenario. The model, based on global supersymmetry with a new-inflation-type potential and a coupling between the inflaton and a heavy intermediate superfield, is already known to preserve the flatness required for slow-roll conditions even after including thermal contributions. Here we show that the magnetic field makes the potential even flatter, retarding the transition and rendering it smoother."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.2211","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":""},"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":"1407.2211","created_at":"2026-05-18T02:40:55.680476+00:00"},{"alias_kind":"arxiv_version","alias_value":"1407.2211v2","created_at":"2026-05-18T02:40:55.680476+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1407.2211","created_at":"2026-05-18T02:40:55.680476+00:00"},{"alias_kind":"pith_short_12","alias_value":"CUVTHK655QWT","created_at":"2026-05-18T12:28:25.294606+00:00"},{"alias_kind":"pith_short_16","alias_value":"CUVTHK655QWTFDSD","created_at":"2026-05-18T12:28:25.294606+00:00"},{"alias_kind":"pith_short_8","alias_value":"CUVTHK65","created_at":"2026-05-18T12:28:25.294606+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/CUVTHK655QWTFDSDZ5AL4I4KTR","json":"https://pith.science/pith/CUVTHK655QWTFDSDZ5AL4I4KTR.json","graph_json":"https://pith.science/api/pith-number/CUVTHK655QWTFDSDZ5AL4I4KTR/graph.json","events_json":"https://pith.science/api/pith-number/CUVTHK655QWTFDSDZ5AL4I4KTR/events.json","paper":"https://pith.science/paper/CUVTHK65"},"agent_actions":{"view_html":"https://pith.science/pith/CUVTHK655QWTFDSDZ5AL4I4KTR","download_json":"https://pith.science/pith/CUVTHK655QWTFDSDZ5AL4I4KTR.json","view_paper":"https://pith.science/paper/CUVTHK65","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1407.2211&json=true","fetch_graph":"https://pith.science/api/pith-number/CUVTHK655QWTFDSDZ5AL4I4KTR/graph.json","fetch_events":"https://pith.science/api/pith-number/CUVTHK655QWTFDSDZ5AL4I4KTR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CUVTHK655QWTFDSDZ5AL4I4KTR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CUVTHK655QWTFDSDZ5AL4I4KTR/action/storage_attestation","attest_author":"https://pith.science/pith/CUVTHK655QWTFDSDZ5AL4I4KTR/action/author_attestation","sign_citation":"https://pith.science/pith/CUVTHK655QWTFDSDZ5AL4I4KTR/action/citation_signature","submit_replication":"https://pith.science/pith/CUVTHK655QWTFDSDZ5AL4I4KTR/action/replication_record"}},"created_at":"2026-05-18T02:40:55.680476+00:00","updated_at":"2026-05-18T02:40:55.680476+00:00"}