{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:HUFIMEPYQKTF2AXNAMNOACLC76","short_pith_number":"pith:HUFIMEPY","schema_version":"1.0","canonical_sha256":"3d0a8611f882a65d02ed031ae00962ff9273cb3f6e8f92868581bc02c7a99e73","source":{"kind":"arxiv","id":"2301.12194","version":1},"attestation_state":"computed","paper":{"title":"Revisiting two dark matter candidates in $S_3$-symmetric three-Higgs-doublet models","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"A. Kun\\v{c}inas, M. N. Rebelo, O. M. Ogreid, P. Osland","submitted_at":"2023-01-28T13:32:39Z","abstract_excerpt":"Models with an extended scalar electroweak sector are well motivated. Such models could accommodate a dark matter candidate if there is an additional scalar representation with a vanishing vacuum expectation value and, in addition, there are no couplings between fermions and the dark matter candidate. The most natural way to have these conditions implemented is to consider models where an underlying symmetry is imposed. Governed by this, we consider a three-Higgs-doublet model with an $S_3$ symmetry. Within this framework there are different implementations which could possibly accommodate a d"},"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":"2301.12194","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2023-01-28T13:32:39Z","cross_cats_sorted":[],"title_canon_sha256":"7d9a8ca781a79a36c0e07af34ad59a37f0c86cf27d5b87610c3ed768503cee6f","abstract_canon_sha256":"b8c8bdd89450d38fc213bcebbb298ac759e08892ba4375e004d4223df443ebc1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:36:36.461267Z","signature_b64":"M8VeR2bRjMdIvktFwL5qq+ALV+Mj/hQg7nZcTAUuK4ThJa3OMMiv+WbGKVqccdSQdJu4WVsx+sI49rgPe+SGBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3d0a8611f882a65d02ed031ae00962ff9273cb3f6e8f92868581bc02c7a99e73","last_reissued_at":"2026-07-05T05:36:36.460855Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:36:36.460855Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Revisiting two dark matter candidates in $S_3$-symmetric three-Higgs-doublet models","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"A. Kun\\v{c}inas, M. N. Rebelo, O. M. Ogreid, P. Osland","submitted_at":"2023-01-28T13:32:39Z","abstract_excerpt":"Models with an extended scalar electroweak sector are well motivated. Such models could accommodate a dark matter candidate if there is an additional scalar representation with a vanishing vacuum expectation value and, in addition, there are no couplings between fermions and the dark matter candidate. The most natural way to have these conditions implemented is to consider models where an underlying symmetry is imposed. Governed by this, we consider a three-Higgs-doublet model with an $S_3$ symmetry. Within this framework there are different implementations which could possibly accommodate a d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2301.12194","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2301.12194/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":"2301.12194","created_at":"2026-07-05T05:36:36.460911+00:00"},{"alias_kind":"arxiv_version","alias_value":"2301.12194v1","created_at":"2026-07-05T05:36:36.460911+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2301.12194","created_at":"2026-07-05T05:36:36.460911+00:00"},{"alias_kind":"pith_short_12","alias_value":"HUFIMEPYQKTF","created_at":"2026-07-05T05:36:36.460911+00:00"},{"alias_kind":"pith_short_16","alias_value":"HUFIMEPYQKTF2AXN","created_at":"2026-07-05T05:36:36.460911+00:00"},{"alias_kind":"pith_short_8","alias_value":"HUFIMEPY","created_at":"2026-07-05T05:36:36.460911+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/HUFIMEPYQKTF2AXNAMNOACLC76","json":"https://pith.science/pith/HUFIMEPYQKTF2AXNAMNOACLC76.json","graph_json":"https://pith.science/api/pith-number/HUFIMEPYQKTF2AXNAMNOACLC76/graph.json","events_json":"https://pith.science/api/pith-number/HUFIMEPYQKTF2AXNAMNOACLC76/events.json","paper":"https://pith.science/paper/HUFIMEPY"},"agent_actions":{"view_html":"https://pith.science/pith/HUFIMEPYQKTF2AXNAMNOACLC76","download_json":"https://pith.science/pith/HUFIMEPYQKTF2AXNAMNOACLC76.json","view_paper":"https://pith.science/paper/HUFIMEPY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2301.12194&json=true","fetch_graph":"https://pith.science/api/pith-number/HUFIMEPYQKTF2AXNAMNOACLC76/graph.json","fetch_events":"https://pith.science/api/pith-number/HUFIMEPYQKTF2AXNAMNOACLC76/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HUFIMEPYQKTF2AXNAMNOACLC76/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HUFIMEPYQKTF2AXNAMNOACLC76/action/storage_attestation","attest_author":"https://pith.science/pith/HUFIMEPYQKTF2AXNAMNOACLC76/action/author_attestation","sign_citation":"https://pith.science/pith/HUFIMEPYQKTF2AXNAMNOACLC76/action/citation_signature","submit_replication":"https://pith.science/pith/HUFIMEPYQKTF2AXNAMNOACLC76/action/replication_record"}},"created_at":"2026-07-05T05:36:36.460911+00:00","updated_at":"2026-07-05T05:36:36.460911+00:00"}