{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:6HZWBQLLNGMUSMERWP2UZSOKU6","short_pith_number":"pith:6HZWBQLL","schema_version":"1.0","canonical_sha256":"f1f360c16b6999493091b3f54cc9caa7b5bfa12c747b8cdd84cbfe5bd71daa04","source":{"kind":"arxiv","id":"2210.05426","version":2},"attestation_state":"computed","paper":{"title":"On the Higgs spectra of the 3-3-1 model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"C. A. de S. Pires, Joao Paulo Pinheiro","submitted_at":"2022-10-11T13:09:12Z","abstract_excerpt":"The minimal scalar sector of the 3-3-1 model is composed by the SU(3)$_L$ triplet scalars $\\eta$, $\\rho$, $\\chi$ and its potential allows the trilinear term $\\frac{f}{\\sqrt{2}}\\chi \\eta \\rho$. Since $f$ is an energy scale associated to the explicit violation of Peccei-Quinn global symmetry, it is natural to consider in what energy scale such symmetry is broken and its consequences in the spectrum of scalars of the model. here, We show that $f$ determines the spectrum of scalars of the model. Hence, we develop the scalar sector considering $f$ belonging to four energy regimes, namely $f \\ll \\la"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2210.05426","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2022-10-11T13:09:12Z","cross_cats_sorted":[],"title_canon_sha256":"a20682ea07312c22deeadb4a70a0af286d47cde0067eb29c3d007542469856ea","abstract_canon_sha256":"50ecaffe06512d78eadc4562b1216cf442171f4a5fa982be775b85100851ad48"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:22:57.322041Z","signature_b64":"2NdsfRFaBNN/IQI3gHCfvhM5tx/ZpbabVrLdl1x5BK2nkyPp+0apVLdW6gxMZz6uweCVy/Yj6k9S184I57fiAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f1f360c16b6999493091b3f54cc9caa7b5bfa12c747b8cdd84cbfe5bd71daa04","last_reissued_at":"2026-07-05T05:22:57.321478Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:22:57.321478Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the Higgs spectra of the 3-3-1 model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"C. A. de S. Pires, Joao Paulo Pinheiro","submitted_at":"2022-10-11T13:09:12Z","abstract_excerpt":"The minimal scalar sector of the 3-3-1 model is composed by the SU(3)$_L$ triplet scalars $\\eta$, $\\rho$, $\\chi$ and its potential allows the trilinear term $\\frac{f}{\\sqrt{2}}\\chi \\eta \\rho$. Since $f$ is an energy scale associated to the explicit violation of Peccei-Quinn global symmetry, it is natural to consider in what energy scale such symmetry is broken and its consequences in the spectrum of scalars of the model. here, We show that $f$ determines the spectrum of scalars of the model. Hence, we develop the scalar sector considering $f$ belonging to four energy regimes, namely $f \\ll \\la"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2210.05426","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/2210.05426/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":"2210.05426","created_at":"2026-07-05T05:22:57.321568+00:00"},{"alias_kind":"arxiv_version","alias_value":"2210.05426v2","created_at":"2026-07-05T05:22:57.321568+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2210.05426","created_at":"2026-07-05T05:22:57.321568+00:00"},{"alias_kind":"pith_short_12","alias_value":"6HZWBQLLNGMU","created_at":"2026-07-05T05:22:57.321568+00:00"},{"alias_kind":"pith_short_16","alias_value":"6HZWBQLLNGMUSMER","created_at":"2026-07-05T05:22:57.321568+00:00"},{"alias_kind":"pith_short_8","alias_value":"6HZWBQLL","created_at":"2026-07-05T05:22:57.321568+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.12121","citing_title":"The 3-3-1 Model: a natural framework for sub-MeV dark matter","ref_index":20,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6HZWBQLLNGMUSMERWP2UZSOKU6","json":"https://pith.science/pith/6HZWBQLLNGMUSMERWP2UZSOKU6.json","graph_json":"https://pith.science/api/pith-number/6HZWBQLLNGMUSMERWP2UZSOKU6/graph.json","events_json":"https://pith.science/api/pith-number/6HZWBQLLNGMUSMERWP2UZSOKU6/events.json","paper":"https://pith.science/paper/6HZWBQLL"},"agent_actions":{"view_html":"https://pith.science/pith/6HZWBQLLNGMUSMERWP2UZSOKU6","download_json":"https://pith.science/pith/6HZWBQLLNGMUSMERWP2UZSOKU6.json","view_paper":"https://pith.science/paper/6HZWBQLL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2210.05426&json=true","fetch_graph":"https://pith.science/api/pith-number/6HZWBQLLNGMUSMERWP2UZSOKU6/graph.json","fetch_events":"https://pith.science/api/pith-number/6HZWBQLLNGMUSMERWP2UZSOKU6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6HZWBQLLNGMUSMERWP2UZSOKU6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6HZWBQLLNGMUSMERWP2UZSOKU6/action/storage_attestation","attest_author":"https://pith.science/pith/6HZWBQLLNGMUSMERWP2UZSOKU6/action/author_attestation","sign_citation":"https://pith.science/pith/6HZWBQLLNGMUSMERWP2UZSOKU6/action/citation_signature","submit_replication":"https://pith.science/pith/6HZWBQLLNGMUSMERWP2UZSOKU6/action/replication_record"}},"created_at":"2026-07-05T05:22:57.321568+00:00","updated_at":"2026-07-05T05:22:57.321568+00:00"}