{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:XYO5CIIHTHTELS7ZEEFQWYD7OJ","short_pith_number":"pith:XYO5CIIH","schema_version":"1.0","canonical_sha256":"be1dd1210799e645cbf9210b0b607f726efb9aeb05d2da9174aac7b462150ce5","source":{"kind":"arxiv","id":"2204.03510","version":2},"attestation_state":"computed","paper":{"title":"A Fermionic Portal to Vector Dark Matter from a New Gauge Sector","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Aldo Deandrea, Alexander Belyaev, Douglas A. Ross, Luca Panizzi, Nakorn Thongyoi, Stefano Moretti","submitted_at":"2022-04-07T15:29:24Z","abstract_excerpt":"We present a new class of Dark Matter (DM) models wherein the Standard Model (SM) is extended with a new $SU(2)_D$ dark gauge sector. In this framework the stability of DM is provided by the conservation of a $U(1)$ global symmetry, which upon appropriate charge assignments for the $SU(2)_D$ multiplets, effectively leads to a $\\mathbb{Z}_2$ symmetry subgroup. The origin of the global $U(1)$ symmetry which ensures the stability of DM can be justified in the form of a dark EW sector or through an underlying composite structure. The key ingredient of the model is a Vector-Like (VL) fermion double"},"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":"2204.03510","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2022-04-07T15:29:24Z","cross_cats_sorted":[],"title_canon_sha256":"4b4e93d69ca169e3529b566bd848cc277aca42ccab19c356a81e610d79d8fa10","abstract_canon_sha256":"cc48c6f2e24f8994be710e421902ef0bc3a123ad8231fd94a97d2b2b27c7ea6e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:54:12.240154Z","signature_b64":"5mBnkr/LaT0dehQKkNOarD3ljhjhPiE2S9QTvAogNYHuA5tSuRyOqYSzKVnv5DzO/HSUsb9L1VIOsqcNp1/zBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"be1dd1210799e645cbf9210b0b607f726efb9aeb05d2da9174aac7b462150ce5","last_reissued_at":"2026-07-05T06:54:12.239669Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:54:12.239669Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Fermionic Portal to Vector Dark Matter from a New Gauge Sector","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Aldo Deandrea, Alexander Belyaev, Douglas A. Ross, Luca Panizzi, Nakorn Thongyoi, Stefano Moretti","submitted_at":"2022-04-07T15:29:24Z","abstract_excerpt":"We present a new class of Dark Matter (DM) models wherein the Standard Model (SM) is extended with a new $SU(2)_D$ dark gauge sector. In this framework the stability of DM is provided by the conservation of a $U(1)$ global symmetry, which upon appropriate charge assignments for the $SU(2)_D$ multiplets, effectively leads to a $\\mathbb{Z}_2$ symmetry subgroup. The origin of the global $U(1)$ symmetry which ensures the stability of DM can be justified in the form of a dark EW sector or through an underlying composite structure. The key ingredient of the model is a Vector-Like (VL) fermion double"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2204.03510","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/2204.03510/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":"2204.03510","created_at":"2026-07-05T06:54:12.239727+00:00"},{"alias_kind":"arxiv_version","alias_value":"2204.03510v2","created_at":"2026-07-05T06:54:12.239727+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2204.03510","created_at":"2026-07-05T06:54:12.239727+00:00"},{"alias_kind":"pith_short_12","alias_value":"XYO5CIIHTHTE","created_at":"2026-07-05T06:54:12.239727+00:00"},{"alias_kind":"pith_short_16","alias_value":"XYO5CIIHTHTELS7Z","created_at":"2026-07-05T06:54:12.239727+00:00"},{"alias_kind":"pith_short_8","alias_value":"XYO5CIIH","created_at":"2026-07-05T06:54:12.239727+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2510.18564","citing_title":"The Muonic Portal to Vector Dark Matter:connecting precision muon physics, cosmology, and colliders","ref_index":71,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XYO5CIIHTHTELS7ZEEFQWYD7OJ","json":"https://pith.science/pith/XYO5CIIHTHTELS7ZEEFQWYD7OJ.json","graph_json":"https://pith.science/api/pith-number/XYO5CIIHTHTELS7ZEEFQWYD7OJ/graph.json","events_json":"https://pith.science/api/pith-number/XYO5CIIHTHTELS7ZEEFQWYD7OJ/events.json","paper":"https://pith.science/paper/XYO5CIIH"},"agent_actions":{"view_html":"https://pith.science/pith/XYO5CIIHTHTELS7ZEEFQWYD7OJ","download_json":"https://pith.science/pith/XYO5CIIHTHTELS7ZEEFQWYD7OJ.json","view_paper":"https://pith.science/paper/XYO5CIIH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2204.03510&json=true","fetch_graph":"https://pith.science/api/pith-number/XYO5CIIHTHTELS7ZEEFQWYD7OJ/graph.json","fetch_events":"https://pith.science/api/pith-number/XYO5CIIHTHTELS7ZEEFQWYD7OJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XYO5CIIHTHTELS7ZEEFQWYD7OJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XYO5CIIHTHTELS7ZEEFQWYD7OJ/action/storage_attestation","attest_author":"https://pith.science/pith/XYO5CIIHTHTELS7ZEEFQWYD7OJ/action/author_attestation","sign_citation":"https://pith.science/pith/XYO5CIIHTHTELS7ZEEFQWYD7OJ/action/citation_signature","submit_replication":"https://pith.science/pith/XYO5CIIHTHTELS7ZEEFQWYD7OJ/action/replication_record"}},"created_at":"2026-07-05T06:54:12.239727+00:00","updated_at":"2026-07-05T06:54:12.239727+00:00"}