{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:BOAEDQNB6GGIOCR4OAPLD23DXR","short_pith_number":"pith:BOAEDQNB","schema_version":"1.0","canonical_sha256":"0b8041c1a1f18c870a3c701eb1eb63bc647eafc30d17a0e4ca543dfe0a5a9a26","source":{"kind":"arxiv","id":"2103.12707","version":2},"attestation_state":"computed","paper":{"title":"Fate of electroweak symmetry in the early Universe: Non-restoration and trapped vacua in the N2HDM","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Georg Weiglein, Jos\\'e Miguel No, Mar\\'ia Olalla Olea, Sven Heinemeyer, Thomas Biek\\\"otter","submitted_at":"2021-03-23T17:28:45Z","abstract_excerpt":"Extensions of the Higgs sector of the Standard Model allow for a rich cosmological history around the electroweak scale. We show that besides the possibility of strong first-order phase transitions, which have been thoroughly studied in the literature, also other important phenomena can occur, like the non-restoration of the electroweak symmetry or the existence of vacua in which the Universe becomes trapped, preventing a transition to the electroweak minimum. Focusing on the next-to-minimal two-Higgs-doublet model (N2HDM) of type II and taking into account the existing theoretical and experim"},"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":"2103.12707","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2021-03-23T17:28:45Z","cross_cats_sorted":[],"title_canon_sha256":"ca0460feb5be391e816b3b926cb28180dfb1337d59ed650811428eb37dc7a1b8","abstract_canon_sha256":"13aba507f48bf8b770406a52d1b9c77fd106f2f493c99730a48e3916a9a8e31f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:48:22.152379Z","signature_b64":"Be/MzPZrfYGnoizJwb87a7pX/8pYeOqTSdy/uxmFFD4xhi3kZV4WVUBJsmLPepedZT2OfB1+JmoiUPki7N7FCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0b8041c1a1f18c870a3c701eb1eb63bc647eafc30d17a0e4ca543dfe0a5a9a26","last_reissued_at":"2026-07-05T02:48:22.151966Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:48:22.151966Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fate of electroweak symmetry in the early Universe: Non-restoration and trapped vacua in the N2HDM","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Georg Weiglein, Jos\\'e Miguel No, Mar\\'ia Olalla Olea, Sven Heinemeyer, Thomas Biek\\\"otter","submitted_at":"2021-03-23T17:28:45Z","abstract_excerpt":"Extensions of the Higgs sector of the Standard Model allow for a rich cosmological history around the electroweak scale. We show that besides the possibility of strong first-order phase transitions, which have been thoroughly studied in the literature, also other important phenomena can occur, like the non-restoration of the electroweak symmetry or the existence of vacua in which the Universe becomes trapped, preventing a transition to the electroweak minimum. Focusing on the next-to-minimal two-Higgs-doublet model (N2HDM) of type II and taking into account the existing theoretical and experim"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2103.12707","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2103.12707/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":"2103.12707","created_at":"2026-07-05T02:48:22.152021+00:00"},{"alias_kind":"arxiv_version","alias_value":"2103.12707v2","created_at":"2026-07-05T02:48:22.152021+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2103.12707","created_at":"2026-07-05T02:48:22.152021+00:00"},{"alias_kind":"pith_short_12","alias_value":"BOAEDQNB6GGI","created_at":"2026-07-05T02:48:22.152021+00:00"},{"alias_kind":"pith_short_16","alias_value":"BOAEDQNB6GGIOCR4","created_at":"2026-07-05T02:48:22.152021+00:00"},{"alias_kind":"pith_short_8","alias_value":"BOAEDQNB","created_at":"2026-07-05T02:48:22.152021+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2603.20414","citing_title":"Inverse Electroweak Baryogenesis","ref_index":17,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BOAEDQNB6GGIOCR4OAPLD23DXR","json":"https://pith.science/pith/BOAEDQNB6GGIOCR4OAPLD23DXR.json","graph_json":"https://pith.science/api/pith-number/BOAEDQNB6GGIOCR4OAPLD23DXR/graph.json","events_json":"https://pith.science/api/pith-number/BOAEDQNB6GGIOCR4OAPLD23DXR/events.json","paper":"https://pith.science/paper/BOAEDQNB"},"agent_actions":{"view_html":"https://pith.science/pith/BOAEDQNB6GGIOCR4OAPLD23DXR","download_json":"https://pith.science/pith/BOAEDQNB6GGIOCR4OAPLD23DXR.json","view_paper":"https://pith.science/paper/BOAEDQNB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2103.12707&json=true","fetch_graph":"https://pith.science/api/pith-number/BOAEDQNB6GGIOCR4OAPLD23DXR/graph.json","fetch_events":"https://pith.science/api/pith-number/BOAEDQNB6GGIOCR4OAPLD23DXR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BOAEDQNB6GGIOCR4OAPLD23DXR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BOAEDQNB6GGIOCR4OAPLD23DXR/action/storage_attestation","attest_author":"https://pith.science/pith/BOAEDQNB6GGIOCR4OAPLD23DXR/action/author_attestation","sign_citation":"https://pith.science/pith/BOAEDQNB6GGIOCR4OAPLD23DXR/action/citation_signature","submit_replication":"https://pith.science/pith/BOAEDQNB6GGIOCR4OAPLD23DXR/action/replication_record"}},"created_at":"2026-07-05T02:48:22.152021+00:00","updated_at":"2026-07-05T02:48:22.152021+00:00"}