{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:TWXL5FCZSTIJQTBBC2TDLMIIGF","short_pith_number":"pith:TWXL5FCZ","schema_version":"1.0","canonical_sha256":"9daebe945994d0984c2116a635b108317ec34e3f3f2b7a8e614d87268bcbdebf","source":{"kind":"arxiv","id":"2006.14922","version":1},"attestation_state":"computed","paper":{"title":"The $Z_5$ model of two-component dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Alexander Pukhov, Carlos Yaguna, Genevi\\`eve B\\'elanger, Oscar Zapata","submitted_at":"2020-06-26T11:53:57Z","abstract_excerpt":"Scenarios for multi-component scalar dark matter based on a single $Z_N$ ($N\\geq 4$) symmetry are simple and well-motivated. In this paper we investigate, for the first time, the phenomenology of the $Z_5$ model for two-component dark matter. This model, which can be seen as an extension of the well-known singlet scalar model, features two complex scalar fields--the dark matter particles--that are Standard Model singlets but have different charges under a $Z_5$ symmetry. The interactions allowed by the $Z_5$ give rise to novel processes between the dark matter particles that affect their relic"},"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":"2006.14922","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2020-06-26T11:53:57Z","cross_cats_sorted":[],"title_canon_sha256":"fb9d74f366f49e6a38912f96168bbdc7c5b57cd055a399e26082ae123f14fa51","abstract_canon_sha256":"e4b1bb3518124da4682735b62fac0f77473addc0d5d863460c1a9466a34cf196"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:13:48.057507Z","signature_b64":"BmSyyVijyXH/7/qHmyROrZJYlgGgPoY1t9zK0bGtwVIhM4tu7zxp44chFsVRLd+SmzTEREWoFXf3zSULU9eBAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9daebe945994d0984c2116a635b108317ec34e3f3f2b7a8e614d87268bcbdebf","last_reissued_at":"2026-07-05T01:13:48.057120Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:13:48.057120Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The $Z_5$ model of two-component dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Alexander Pukhov, Carlos Yaguna, Genevi\\`eve B\\'elanger, Oscar Zapata","submitted_at":"2020-06-26T11:53:57Z","abstract_excerpt":"Scenarios for multi-component scalar dark matter based on a single $Z_N$ ($N\\geq 4$) symmetry are simple and well-motivated. In this paper we investigate, for the first time, the phenomenology of the $Z_5$ model for two-component dark matter. This model, which can be seen as an extension of the well-known singlet scalar model, features two complex scalar fields--the dark matter particles--that are Standard Model singlets but have different charges under a $Z_5$ symmetry. The interactions allowed by the $Z_5$ give rise to novel processes between the dark matter particles that affect their relic"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2006.14922","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/2006.14922/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":"2006.14922","created_at":"2026-07-05T01:13:48.057180+00:00"},{"alias_kind":"arxiv_version","alias_value":"2006.14922v1","created_at":"2026-07-05T01:13:48.057180+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2006.14922","created_at":"2026-07-05T01:13:48.057180+00:00"},{"alias_kind":"pith_short_12","alias_value":"TWXL5FCZSTIJ","created_at":"2026-07-05T01:13:48.057180+00:00"},{"alias_kind":"pith_short_16","alias_value":"TWXL5FCZSTIJQTBB","created_at":"2026-07-05T01:13:48.057180+00:00"},{"alias_kind":"pith_short_8","alias_value":"TWXL5FCZ","created_at":"2026-07-05T01:13:48.057180+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2608.03975","citing_title":"Mono-X Signal Characterization from Two-component Dark Matter Using a Convolutional Neural Network","ref_index":30,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TWXL5FCZSTIJQTBBC2TDLMIIGF","json":"https://pith.science/pith/TWXL5FCZSTIJQTBBC2TDLMIIGF.json","graph_json":"https://pith.science/api/pith-number/TWXL5FCZSTIJQTBBC2TDLMIIGF/graph.json","events_json":"https://pith.science/api/pith-number/TWXL5FCZSTIJQTBBC2TDLMIIGF/events.json","paper":"https://pith.science/paper/TWXL5FCZ"},"agent_actions":{"view_html":"https://pith.science/pith/TWXL5FCZSTIJQTBBC2TDLMIIGF","download_json":"https://pith.science/pith/TWXL5FCZSTIJQTBBC2TDLMIIGF.json","view_paper":"https://pith.science/paper/TWXL5FCZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2006.14922&json=true","fetch_graph":"https://pith.science/api/pith-number/TWXL5FCZSTIJQTBBC2TDLMIIGF/graph.json","fetch_events":"https://pith.science/api/pith-number/TWXL5FCZSTIJQTBBC2TDLMIIGF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TWXL5FCZSTIJQTBBC2TDLMIIGF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TWXL5FCZSTIJQTBBC2TDLMIIGF/action/storage_attestation","attest_author":"https://pith.science/pith/TWXL5FCZSTIJQTBBC2TDLMIIGF/action/author_attestation","sign_citation":"https://pith.science/pith/TWXL5FCZSTIJQTBBC2TDLMIIGF/action/citation_signature","submit_replication":"https://pith.science/pith/TWXL5FCZSTIJQTBBC2TDLMIIGF/action/replication_record"}},"created_at":"2026-07-05T01:13:48.057180+00:00","updated_at":"2026-07-05T01:13:48.057180+00:00"}