{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:YHNG7OP2EDDRLQ5EVUL24GI5CH","short_pith_number":"pith:YHNG7OP2","schema_version":"1.0","canonical_sha256":"c1da6fb9fa20c715c3a4ad17ae191d11f18a4fd6c4cfc5cfad3f846e22b0b41d","source":{"kind":"arxiv","id":"1009.3032","version":1},"attestation_state":"computed","paper":{"title":"Inflating with Baryons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"hep-th","authors_text":"Daniel Baumann, Daniel Green","submitted_at":"2010-09-15T20:14:10Z","abstract_excerpt":"We present a field theory solution to the eta problem. By making the inflaton field the phase of a baryon of SU(N_c) supersymmetric Yang-Mills theory we show that all operators that usually spoil the flatness of the inflationary potential are absent. Our solution naturally generalizes to non-supersymmetric theories."},"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":"1009.3032","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2010-09-15T20:14:10Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"751c6f39aaf5e4d564e0449287f885f04d9819ec87f3a8b564d5ea0c872e9d8d","abstract_canon_sha256":"1c41e1fcac68a281cd48edb1ddd1fdd0d854def0d5dab0e86ab373ace604c011"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:23:56.616731Z","signature_b64":"BEHab02dFCNjOQxfBVoSTjfKqpu/S70WB4+OSATF/iCRIvqffPeIibMn6xPywI7a6eAkkEsBIUgA4FzuHQL4Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c1da6fb9fa20c715c3a4ad17ae191d11f18a4fd6c4cfc5cfad3f846e22b0b41d","last_reissued_at":"2026-05-18T04:23:56.616321Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:23:56.616321Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Inflating with Baryons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"hep-th","authors_text":"Daniel Baumann, Daniel Green","submitted_at":"2010-09-15T20:14:10Z","abstract_excerpt":"We present a field theory solution to the eta problem. By making the inflaton field the phase of a baryon of SU(N_c) supersymmetric Yang-Mills theory we show that all operators that usually spoil the flatness of the inflationary potential are absent. Our solution naturally generalizes to non-supersymmetric theories."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.3032","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":""},"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":"1009.3032","created_at":"2026-05-18T04:23:56.616381+00:00"},{"alias_kind":"arxiv_version","alias_value":"1009.3032v1","created_at":"2026-05-18T04:23:56.616381+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1009.3032","created_at":"2026-05-18T04:23:56.616381+00:00"},{"alias_kind":"pith_short_12","alias_value":"YHNG7OP2EDDR","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_16","alias_value":"YHNG7OP2EDDRLQ5E","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_8","alias_value":"YHNG7OP2","created_at":"2026-05-18T12:26:17.028572+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/YHNG7OP2EDDRLQ5EVUL24GI5CH","json":"https://pith.science/pith/YHNG7OP2EDDRLQ5EVUL24GI5CH.json","graph_json":"https://pith.science/api/pith-number/YHNG7OP2EDDRLQ5EVUL24GI5CH/graph.json","events_json":"https://pith.science/api/pith-number/YHNG7OP2EDDRLQ5EVUL24GI5CH/events.json","paper":"https://pith.science/paper/YHNG7OP2"},"agent_actions":{"view_html":"https://pith.science/pith/YHNG7OP2EDDRLQ5EVUL24GI5CH","download_json":"https://pith.science/pith/YHNG7OP2EDDRLQ5EVUL24GI5CH.json","view_paper":"https://pith.science/paper/YHNG7OP2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1009.3032&json=true","fetch_graph":"https://pith.science/api/pith-number/YHNG7OP2EDDRLQ5EVUL24GI5CH/graph.json","fetch_events":"https://pith.science/api/pith-number/YHNG7OP2EDDRLQ5EVUL24GI5CH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YHNG7OP2EDDRLQ5EVUL24GI5CH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YHNG7OP2EDDRLQ5EVUL24GI5CH/action/storage_attestation","attest_author":"https://pith.science/pith/YHNG7OP2EDDRLQ5EVUL24GI5CH/action/author_attestation","sign_citation":"https://pith.science/pith/YHNG7OP2EDDRLQ5EVUL24GI5CH/action/citation_signature","submit_replication":"https://pith.science/pith/YHNG7OP2EDDRLQ5EVUL24GI5CH/action/replication_record"}},"created_at":"2026-05-18T04:23:56.616381+00:00","updated_at":"2026-05-18T04:23:56.616381+00:00"}