{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:KBS7PM2T3AB5OU5DM5AFACKEFP","short_pith_number":"pith:KBS7PM2T","schema_version":"1.0","canonical_sha256":"5065f7b353d803d753a367405009442bd9ab57ecc1ffc7c75e759c804587419b","source":{"kind":"arxiv","id":"1107.5441","version":1},"attestation_state":"computed","paper":{"title":"Strong Electroweak Phase Transitions in the Standard Model with a Singlet","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Francesco Riva, Jose R. Espinosa, Thomas Konstandin","submitted_at":"2011-07-27T11:09:25Z","abstract_excerpt":"It is well known that the electroweak phase transition (EWPhT) in extensions of the Standard Model with one real scalar singlet can be first-order for realistic values of the Higgs mass. We revisit this scenario with the most general renormalizable scalar potential systematically identifying all regions in parameter space that develop, due to tree-level dynamics, a potential barrier at the critical temperature that is strong enough to avoid sphaleron wash-out of the baryon asymmetry. Such strong EWPhTs allow for a simple mean-field approximation and an analytic treatment of the free-energy tha"},"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":"1107.5441","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2011-07-27T11:09:25Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"44f07451dc5f74ae33781b20cc0d4ba31f7b21549f449aad496d590368f4b321","abstract_canon_sha256":"6a71aec85793760848bf612a9a3fdd5939e7fcf8337dbeec17a1ac7d89221b3f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:09.091601Z","signature_b64":"NFkIVS//NrHzUaU4POkDpUEq+8QEz+QATjvnv+1plpvwfy1aeQN0y0ljQKUUTYYJYIPLrtg5rJDfiT8B/FnaDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5065f7b353d803d753a367405009442bd9ab57ecc1ffc7c75e759c804587419b","last_reissued_at":"2026-05-18T02:01:09.090709Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:09.090709Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Strong Electroweak Phase Transitions in the Standard Model with a Singlet","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Francesco Riva, Jose R. Espinosa, Thomas Konstandin","submitted_at":"2011-07-27T11:09:25Z","abstract_excerpt":"It is well known that the electroweak phase transition (EWPhT) in extensions of the Standard Model with one real scalar singlet can be first-order for realistic values of the Higgs mass. We revisit this scenario with the most general renormalizable scalar potential systematically identifying all regions in parameter space that develop, due to tree-level dynamics, a potential barrier at the critical temperature that is strong enough to avoid sphaleron wash-out of the baryon asymmetry. Such strong EWPhTs allow for a simple mean-field approximation and an analytic treatment of the free-energy tha"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1107.5441","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":"1107.5441","created_at":"2026-05-18T02:01:09.090853+00:00"},{"alias_kind":"arxiv_version","alias_value":"1107.5441v1","created_at":"2026-05-18T02:01:09.090853+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1107.5441","created_at":"2026-05-18T02:01:09.090853+00:00"},{"alias_kind":"pith_short_12","alias_value":"KBS7PM2T3AB5","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_16","alias_value":"KBS7PM2T3AB5OU5D","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_8","alias_value":"KBS7PM2T","created_at":"2026-05-18T12:26:32.869790+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"1910.13125","citing_title":"Detecting gravitational waves from cosmological phase transitions with LISA: an update","ref_index":75,"is_internal_anchor":true},{"citing_arxiv_id":"2002.04615","citing_title":"New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions","ref_index":164,"is_internal_anchor":true},{"citing_arxiv_id":"2603.18583","citing_title":"Electroweak phase transitions in a $U(1)_D$ extension of the standard model with dimension-six operators: Gravitational waves and LHC signatures","ref_index":8,"is_internal_anchor":true},{"citing_arxiv_id":"2604.21492","citing_title":"Solving Cosmological Puzzles using Finite Temperature $\\nu$SMEFT","ref_index":7,"is_internal_anchor":false},{"citing_arxiv_id":"2604.20762","citing_title":"Spontaneous Baryogenesis from Axions on Induced Electroweak Walls","ref_index":53,"is_internal_anchor":false},{"citing_arxiv_id":"2604.16603","citing_title":"Baryon Asymmetry from Electroweak-Symmetric Domain Walls","ref_index":15,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KBS7PM2T3AB5OU5DM5AFACKEFP","json":"https://pith.science/pith/KBS7PM2T3AB5OU5DM5AFACKEFP.json","graph_json":"https://pith.science/api/pith-number/KBS7PM2T3AB5OU5DM5AFACKEFP/graph.json","events_json":"https://pith.science/api/pith-number/KBS7PM2T3AB5OU5DM5AFACKEFP/events.json","paper":"https://pith.science/paper/KBS7PM2T"},"agent_actions":{"view_html":"https://pith.science/pith/KBS7PM2T3AB5OU5DM5AFACKEFP","download_json":"https://pith.science/pith/KBS7PM2T3AB5OU5DM5AFACKEFP.json","view_paper":"https://pith.science/paper/KBS7PM2T","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1107.5441&json=true","fetch_graph":"https://pith.science/api/pith-number/KBS7PM2T3AB5OU5DM5AFACKEFP/graph.json","fetch_events":"https://pith.science/api/pith-number/KBS7PM2T3AB5OU5DM5AFACKEFP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KBS7PM2T3AB5OU5DM5AFACKEFP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KBS7PM2T3AB5OU5DM5AFACKEFP/action/storage_attestation","attest_author":"https://pith.science/pith/KBS7PM2T3AB5OU5DM5AFACKEFP/action/author_attestation","sign_citation":"https://pith.science/pith/KBS7PM2T3AB5OU5DM5AFACKEFP/action/citation_signature","submit_replication":"https://pith.science/pith/KBS7PM2T3AB5OU5DM5AFACKEFP/action/replication_record"}},"created_at":"2026-05-18T02:01:09.090853+00:00","updated_at":"2026-05-18T02:01:09.090853+00:00"}