{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:R26DMTGZJFBSTJ3OYBJJ4UVKCV","short_pith_number":"pith:R26DMTGZ","schema_version":"1.0","canonical_sha256":"8ebc364cd9494329a76ec0529e52aa157255e0873b81df745c4df719672a5e26","source":{"kind":"arxiv","id":"2002.04616","version":1},"attestation_state":"computed","paper":{"title":"Collider signatures of dark CP-violation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"A. Cordero-Cid, D. Rojas-Ciofalo, D. Sokolowska, J. Hernandez-Sanchez, S. Moretti, V. Keus","submitted_at":"2020-02-11T19:00:01Z","abstract_excerpt":"We study an extension of the Standard Model (SM) in which two copies of the SM-Higgs doublet which do not acquire a vacuum expectation value, and hence are {\\it inert}, are added to the scalar sector. The lightest particle from the inert sector, which is protected from decaying to SM particles through the conservation of a $Z_2$ symmetry, is a viable dark matter candidate. We allow for CP-violation in this extended dark sector and evaluate the $ZZZ$ vertex and its CP-violating form factor in several benchmark scenarios. We provide collider signatures of this dark CP-violation in the form of po"},"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":"2002.04616","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2020-02-11T19:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"8388f803a46f7b53e3d7a132fda1c25d9633e1d87de4d79df04005b97a2e14bc","abstract_canon_sha256":"3b24fc54f5e0439702777fb18602168d9591f3c82afa0378443170f6f7ee6e0c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:49:26.546478Z","signature_b64":"74UXftLqtTazEbWk97TGZ0lWcgM5tLtW6TTFwbfVbtAf5USNebL/yZRfkuna4/QHEwzxeeZgiqHvSLO1ux2PDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8ebc364cd9494329a76ec0529e52aa157255e0873b81df745c4df719672a5e26","last_reissued_at":"2026-07-05T00:49:26.546028Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:49:26.546028Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Collider signatures of dark CP-violation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"A. Cordero-Cid, D. Rojas-Ciofalo, D. Sokolowska, J. Hernandez-Sanchez, S. Moretti, V. Keus","submitted_at":"2020-02-11T19:00:01Z","abstract_excerpt":"We study an extension of the Standard Model (SM) in which two copies of the SM-Higgs doublet which do not acquire a vacuum expectation value, and hence are {\\it inert}, are added to the scalar sector. The lightest particle from the inert sector, which is protected from decaying to SM particles through the conservation of a $Z_2$ symmetry, is a viable dark matter candidate. We allow for CP-violation in this extended dark sector and evaluate the $ZZZ$ vertex and its CP-violating form factor in several benchmark scenarios. We provide collider signatures of this dark CP-violation in the form of po"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2002.04616","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/2002.04616/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":"2002.04616","created_at":"2026-07-05T00:49:26.546111+00:00"},{"alias_kind":"arxiv_version","alias_value":"2002.04616v1","created_at":"2026-07-05T00:49:26.546111+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2002.04616","created_at":"2026-07-05T00:49:26.546111+00:00"},{"alias_kind":"pith_short_12","alias_value":"R26DMTGZJFBS","created_at":"2026-07-05T00:49:26.546111+00:00"},{"alias_kind":"pith_short_16","alias_value":"R26DMTGZJFBSTJ3O","created_at":"2026-07-05T00:49:26.546111+00:00"},{"alias_kind":"pith_short_8","alias_value":"R26DMTGZ","created_at":"2026-07-05T00:49:26.546111+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2508.13583","citing_title":"Inert dark matter in three Higgs doublet model: a blind spot narrative","ref_index":23,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/R26DMTGZJFBSTJ3OYBJJ4UVKCV","json":"https://pith.science/pith/R26DMTGZJFBSTJ3OYBJJ4UVKCV.json","graph_json":"https://pith.science/api/pith-number/R26DMTGZJFBSTJ3OYBJJ4UVKCV/graph.json","events_json":"https://pith.science/api/pith-number/R26DMTGZJFBSTJ3OYBJJ4UVKCV/events.json","paper":"https://pith.science/paper/R26DMTGZ"},"agent_actions":{"view_html":"https://pith.science/pith/R26DMTGZJFBSTJ3OYBJJ4UVKCV","download_json":"https://pith.science/pith/R26DMTGZJFBSTJ3OYBJJ4UVKCV.json","view_paper":"https://pith.science/paper/R26DMTGZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2002.04616&json=true","fetch_graph":"https://pith.science/api/pith-number/R26DMTGZJFBSTJ3OYBJJ4UVKCV/graph.json","fetch_events":"https://pith.science/api/pith-number/R26DMTGZJFBSTJ3OYBJJ4UVKCV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R26DMTGZJFBSTJ3OYBJJ4UVKCV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R26DMTGZJFBSTJ3OYBJJ4UVKCV/action/storage_attestation","attest_author":"https://pith.science/pith/R26DMTGZJFBSTJ3OYBJJ4UVKCV/action/author_attestation","sign_citation":"https://pith.science/pith/R26DMTGZJFBSTJ3OYBJJ4UVKCV/action/citation_signature","submit_replication":"https://pith.science/pith/R26DMTGZJFBSTJ3OYBJJ4UVKCV/action/replication_record"}},"created_at":"2026-07-05T00:49:26.546111+00:00","updated_at":"2026-07-05T00:49:26.546111+00:00"}