{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:EBFBQGZMZMK36YHRWUEX3WMAFT","short_pith_number":"pith:EBFBQGZM","schema_version":"1.0","canonical_sha256":"204a181b2ccb15bf60f1b5097dd9802cdcc9a31d6e0c9977b1b1a1906ccbfe18","source":{"kind":"arxiv","id":"2012.09758","version":3},"attestation_state":"computed","paper":{"title":"Electroweak Phase Transition with an SU(2) Dark Sector","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Hongkai Liu, Huai-Ke Guo, Tao Han, Tathagata Ghosh","submitted_at":"2020-12-17T17:16:29Z","abstract_excerpt":"We consider a non-Abelian dark SU(2)$_{\\rm D}$ model where the dark sector couples to the Standard Model (SM) through a Higgs portal. We investigate two different scenarios of the dark sector scalars with $Z_2$ symmetry, with Higgs portal interactions that can introduce mixing between the SM Higgs boson and the SM singlet scalars in the dark sector. We utilize the existing collider results of the Higgs signal rate, direct heavy Higgs searches, and electroweak precision observables to constrain the model parameters. The $\\text{SU(2)}_{\\text{D}}$ partially breaks into $\\text{U(1)}_{\\text{D}}$ ga"},"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":"2012.09758","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2020-12-17T17:16:29Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"f28ad0e68d16a49b17f8a99f20e0ef755757c476a7480103217385977d3d7394","abstract_canon_sha256":"4133c7d051dab84e590e6954d9a7525f8a5f7b507692dc8ca1e403ffc3c3a53e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:01:12.444496Z","signature_b64":"BIG9xT5M33fGgfg6aYFnn6pfG8HxBx9OdDv8CVpmnBn4Bv8awUgnIEhZgKUl+ATWCH6W3ScLY1NU/bDHX1iPAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"204a181b2ccb15bf60f1b5097dd9802cdcc9a31d6e0c9977b1b1a1906ccbfe18","last_reissued_at":"2026-07-05T03:01:12.443985Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:01:12.443985Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Electroweak Phase Transition with an SU(2) Dark Sector","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Hongkai Liu, Huai-Ke Guo, Tao Han, Tathagata Ghosh","submitted_at":"2020-12-17T17:16:29Z","abstract_excerpt":"We consider a non-Abelian dark SU(2)$_{\\rm D}$ model where the dark sector couples to the Standard Model (SM) through a Higgs portal. We investigate two different scenarios of the dark sector scalars with $Z_2$ symmetry, with Higgs portal interactions that can introduce mixing between the SM Higgs boson and the SM singlet scalars in the dark sector. We utilize the existing collider results of the Higgs signal rate, direct heavy Higgs searches, and electroweak precision observables to constrain the model parameters. The $\\text{SU(2)}_{\\text{D}}$ partially breaks into $\\text{U(1)}_{\\text{D}}$ ga"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2012.09758","kind":"arxiv","version":3},"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/2012.09758/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":"2012.09758","created_at":"2026-07-05T03:01:12.444048+00:00"},{"alias_kind":"arxiv_version","alias_value":"2012.09758v3","created_at":"2026-07-05T03:01:12.444048+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2012.09758","created_at":"2026-07-05T03:01:12.444048+00:00"},{"alias_kind":"pith_short_12","alias_value":"EBFBQGZMZMK3","created_at":"2026-07-05T03:01:12.444048+00:00"},{"alias_kind":"pith_short_16","alias_value":"EBFBQGZMZMK36YHR","created_at":"2026-07-05T03:01:12.444048+00:00"},{"alias_kind":"pith_short_8","alias_value":"EBFBQGZM","created_at":"2026-07-05T03:01:12.444048+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.13514","citing_title":"Electroweak First-Order Phase Transition Triggered by Non-Gaussian Fluctuations of a $\\mathbb{Z}_2$-Symmetric Spectator Scalar","ref_index":70,"is_internal_anchor":false},{"citing_arxiv_id":"2603.09126","citing_title":"Dark matter in classically conformal theories: WIMP and supercooling","ref_index":32,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EBFBQGZMZMK36YHRWUEX3WMAFT","json":"https://pith.science/pith/EBFBQGZMZMK36YHRWUEX3WMAFT.json","graph_json":"https://pith.science/api/pith-number/EBFBQGZMZMK36YHRWUEX3WMAFT/graph.json","events_json":"https://pith.science/api/pith-number/EBFBQGZMZMK36YHRWUEX3WMAFT/events.json","paper":"https://pith.science/paper/EBFBQGZM"},"agent_actions":{"view_html":"https://pith.science/pith/EBFBQGZMZMK36YHRWUEX3WMAFT","download_json":"https://pith.science/pith/EBFBQGZMZMK36YHRWUEX3WMAFT.json","view_paper":"https://pith.science/paper/EBFBQGZM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2012.09758&json=true","fetch_graph":"https://pith.science/api/pith-number/EBFBQGZMZMK36YHRWUEX3WMAFT/graph.json","fetch_events":"https://pith.science/api/pith-number/EBFBQGZMZMK36YHRWUEX3WMAFT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EBFBQGZMZMK36YHRWUEX3WMAFT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EBFBQGZMZMK36YHRWUEX3WMAFT/action/storage_attestation","attest_author":"https://pith.science/pith/EBFBQGZMZMK36YHRWUEX3WMAFT/action/author_attestation","sign_citation":"https://pith.science/pith/EBFBQGZMZMK36YHRWUEX3WMAFT/action/citation_signature","submit_replication":"https://pith.science/pith/EBFBQGZMZMK36YHRWUEX3WMAFT/action/replication_record"}},"created_at":"2026-07-05T03:01:12.444048+00:00","updated_at":"2026-07-05T03:01:12.444048+00:00"}