{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:5DAKD4CVPO56PWJA4RUTM4P2G4","short_pith_number":"pith:5DAKD4CV","schema_version":"1.0","canonical_sha256":"e8c0a1f0557bbbe7d920e4693671fa370b29fd7d217beee1526ad1be0d7d38d7","source":{"kind":"arxiv","id":"1110.5650","version":2},"attestation_state":"computed","paper":{"title":"Can Inflation be Connected to Low Energy Particle Physics?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"hep-ph","authors_text":"Mark P. Hertzberg (Stanford)","submitted_at":"2011-10-25T20:02:37Z","abstract_excerpt":"It is an interesting question whether low energy degrees of freedom may be responsible for early universe inflation. To examine this, here we present a simple version of Higgs-inflation with minimal coupling to gravity and a quadratic inflationary potential. This quantitatively differs from the popular non-minimally coupled models, although it is qualitatively similar. In all such models, new heavy fields must enter in order for the theory to be well behaved in the UV. We show that in all cases the Higgs self coupling lambda must be quite small in order to integrate out the heavy fields and us"},"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":"1110.5650","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2011-10-25T20:02:37Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"21a13c4692219518411ac4cdeb3dc9ccda6ffdd681a019458a66341740d6deb7","abstract_canon_sha256":"3861740bac30fd647be3849ceaeb19931e9d34cb25dae43afe4b255ab3c774f4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:49:10.395855Z","signature_b64":"QiE6MreaiaRRPTd8YYHOgYfa+MB6aLZNEphLqjo7VnkiPXc4Yi8Jouk9p5NZNudcZ+yDF7Osgr1q4cPX5LScDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e8c0a1f0557bbbe7d920e4693671fa370b29fd7d217beee1526ad1be0d7d38d7","last_reissued_at":"2026-05-18T03:49:10.395390Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:49:10.395390Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Can Inflation be Connected to Low Energy Particle Physics?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"hep-ph","authors_text":"Mark P. Hertzberg (Stanford)","submitted_at":"2011-10-25T20:02:37Z","abstract_excerpt":"It is an interesting question whether low energy degrees of freedom may be responsible for early universe inflation. To examine this, here we present a simple version of Higgs-inflation with minimal coupling to gravity and a quadratic inflationary potential. This quantitatively differs from the popular non-minimally coupled models, although it is qualitatively similar. In all such models, new heavy fields must enter in order for the theory to be well behaved in the UV. We show that in all cases the Higgs self coupling lambda must be quite small in order to integrate out the heavy fields and us"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1110.5650","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":"1110.5650","created_at":"2026-05-18T03:49:10.395464+00:00"},{"alias_kind":"arxiv_version","alias_value":"1110.5650v2","created_at":"2026-05-18T03:49:10.395464+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1110.5650","created_at":"2026-05-18T03:49:10.395464+00:00"},{"alias_kind":"pith_short_12","alias_value":"5DAKD4CVPO56","created_at":"2026-05-18T12:26:20.644004+00:00"},{"alias_kind":"pith_short_16","alias_value":"5DAKD4CVPO56PWJA","created_at":"2026-05-18T12:26:20.644004+00:00"},{"alias_kind":"pith_short_8","alias_value":"5DAKD4CV","created_at":"2026-05-18T12:26:20.644004+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07193","citing_title":"Higgs boson mass and thermal wino dark matter from Starobinsky supergravity with the MSSM","ref_index":8,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5DAKD4CVPO56PWJA4RUTM4P2G4","json":"https://pith.science/pith/5DAKD4CVPO56PWJA4RUTM4P2G4.json","graph_json":"https://pith.science/api/pith-number/5DAKD4CVPO56PWJA4RUTM4P2G4/graph.json","events_json":"https://pith.science/api/pith-number/5DAKD4CVPO56PWJA4RUTM4P2G4/events.json","paper":"https://pith.science/paper/5DAKD4CV"},"agent_actions":{"view_html":"https://pith.science/pith/5DAKD4CVPO56PWJA4RUTM4P2G4","download_json":"https://pith.science/pith/5DAKD4CVPO56PWJA4RUTM4P2G4.json","view_paper":"https://pith.science/paper/5DAKD4CV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1110.5650&json=true","fetch_graph":"https://pith.science/api/pith-number/5DAKD4CVPO56PWJA4RUTM4P2G4/graph.json","fetch_events":"https://pith.science/api/pith-number/5DAKD4CVPO56PWJA4RUTM4P2G4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5DAKD4CVPO56PWJA4RUTM4P2G4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5DAKD4CVPO56PWJA4RUTM4P2G4/action/storage_attestation","attest_author":"https://pith.science/pith/5DAKD4CVPO56PWJA4RUTM4P2G4/action/author_attestation","sign_citation":"https://pith.science/pith/5DAKD4CVPO56PWJA4RUTM4P2G4/action/citation_signature","submit_replication":"https://pith.science/pith/5DAKD4CVPO56PWJA4RUTM4P2G4/action/replication_record"}},"created_at":"2026-05-18T03:49:10.395464+00:00","updated_at":"2026-05-18T03:49:10.395464+00:00"}