{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:HHQ47F66U62IFEIWXYGRTYTYRZ","short_pith_number":"pith:HHQ47F66","schema_version":"1.0","canonical_sha256":"39e1cf97dea7b4829116be0d19e2788e646db831e71d46d8bd9aed80994075fd","source":{"kind":"arxiv","id":"1802.10402","version":2},"attestation_state":"computed","paper":{"title":"Investigation of Dark Matter in the 3-2-3-1 Model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"D. T. Huong, L. D. Thien, N. T. Duy, N. T. Nhuan, P. V. Dong","submitted_at":"2018-02-28T13:35:46Z","abstract_excerpt":"We prove that the $SU(3)_C\\otimes SU(2)_L \\otimes SU(3)_R\\otimes U(1)_X$ (3-2-3-1) gauge model always contains a matter parity $W_P=(-1)^{3(B-L)+2s}$ as conserved residual gauge symmetry, where $B-L=2(\\beta T_{8R}+X)$ is a $SU(3)_R\\otimes U(1)_X$ charge. Due to the non-Abelian nature of $B-L$, the $W$-odd and $W$-even fields are actually unified in gauge multiplets. We investigate two viable versions for dark matter according to $\\beta=\\pm1/\\sqrt{3}$, where the dark matter candidates can be fermion, scalar, or vector fields. We figure out the parameter spaces in the allowed regions of the reli"},"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":"1802.10402","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2018-02-28T13:35:46Z","cross_cats_sorted":[],"title_canon_sha256":"98f8453bc3ad523e044552b849bff13351e098383ecfb2d6e846763fd2afddf9","abstract_canon_sha256":"bb9776fa3d30613e75dd459643986ae7228a7da2c3fbb5605d4b637cc1b2f3d3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:04:39.608492Z","signature_b64":"AVe2/YhcvKkAPpZI6CaN5+jhKs30qhiBv5kf3pZkDOd/plcEsk1EOLGDcR/Q/RvIB3iHTa+PHhOvEzUHWEBmBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"39e1cf97dea7b4829116be0d19e2788e646db831e71d46d8bd9aed80994075fd","last_reissued_at":"2026-05-18T00:04:39.607991Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:04:39.607991Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Investigation of Dark Matter in the 3-2-3-1 Model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"D. T. Huong, L. D. Thien, N. T. Duy, N. T. Nhuan, P. V. Dong","submitted_at":"2018-02-28T13:35:46Z","abstract_excerpt":"We prove that the $SU(3)_C\\otimes SU(2)_L \\otimes SU(3)_R\\otimes U(1)_X$ (3-2-3-1) gauge model always contains a matter parity $W_P=(-1)^{3(B-L)+2s}$ as conserved residual gauge symmetry, where $B-L=2(\\beta T_{8R}+X)$ is a $SU(3)_R\\otimes U(1)_X$ charge. Due to the non-Abelian nature of $B-L$, the $W$-odd and $W$-even fields are actually unified in gauge multiplets. We investigate two viable versions for dark matter according to $\\beta=\\pm1/\\sqrt{3}$, where the dark matter candidates can be fermion, scalar, or vector fields. We figure out the parameter spaces in the allowed regions of the reli"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.10402","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":""},"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":"1802.10402","created_at":"2026-05-18T00:04:39.608070+00:00"},{"alias_kind":"arxiv_version","alias_value":"1802.10402v2","created_at":"2026-05-18T00:04:39.608070+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.10402","created_at":"2026-05-18T00:04:39.608070+00:00"},{"alias_kind":"pith_short_12","alias_value":"HHQ47F66U62I","created_at":"2026-05-18T12:32:28.185984+00:00"},{"alias_kind":"pith_short_16","alias_value":"HHQ47F66U62IFEIW","created_at":"2026-05-18T12:32:28.185984+00:00"},{"alias_kind":"pith_short_8","alias_value":"HHQ47F66","created_at":"2026-05-18T12:32:28.185984+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/HHQ47F66U62IFEIWXYGRTYTYRZ","json":"https://pith.science/pith/HHQ47F66U62IFEIWXYGRTYTYRZ.json","graph_json":"https://pith.science/api/pith-number/HHQ47F66U62IFEIWXYGRTYTYRZ/graph.json","events_json":"https://pith.science/api/pith-number/HHQ47F66U62IFEIWXYGRTYTYRZ/events.json","paper":"https://pith.science/paper/HHQ47F66"},"agent_actions":{"view_html":"https://pith.science/pith/HHQ47F66U62IFEIWXYGRTYTYRZ","download_json":"https://pith.science/pith/HHQ47F66U62IFEIWXYGRTYTYRZ.json","view_paper":"https://pith.science/paper/HHQ47F66","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1802.10402&json=true","fetch_graph":"https://pith.science/api/pith-number/HHQ47F66U62IFEIWXYGRTYTYRZ/graph.json","fetch_events":"https://pith.science/api/pith-number/HHQ47F66U62IFEIWXYGRTYTYRZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HHQ47F66U62IFEIWXYGRTYTYRZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HHQ47F66U62IFEIWXYGRTYTYRZ/action/storage_attestation","attest_author":"https://pith.science/pith/HHQ47F66U62IFEIWXYGRTYTYRZ/action/author_attestation","sign_citation":"https://pith.science/pith/HHQ47F66U62IFEIWXYGRTYTYRZ/action/citation_signature","submit_replication":"https://pith.science/pith/HHQ47F66U62IFEIWXYGRTYTYRZ/action/replication_record"}},"created_at":"2026-05-18T00:04:39.608070+00:00","updated_at":"2026-05-18T00:04:39.608070+00:00"}