{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:2OWULW7QSMBOHSRK5OUOYODVJH","short_pith_number":"pith:2OWULW7Q","schema_version":"1.0","canonical_sha256":"d3ad45dbf09302e3ca2aeba8ec387549e40b0a227db6120ed467208ed031d238","source":{"kind":"arxiv","id":"2012.11621","version":1},"attestation_state":"computed","paper":{"title":"Complementary Probes of Two-component Dark Matter","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"D. Rojas-Ciofalo, D. Sokolowska, J. Hernandez-Sanchez, S. Moretti, V. Keus","submitted_at":"2020-12-21T19:00:06Z","abstract_excerpt":"We study a $Z_2 \\times Z'_2$ symmetric 3-Higgs Doublet Model (3HDM), wherein two of the doublets are inert and one is active (thus denoted in literature as I(2+1)HDM), yielding a two-component Dark Matter (DM) sector. The two DM candidates emerge as the lightest scalar component of a different inert doublet, each with a different odd discrete parity, and cooperate to achieve the correct relic density. When a sufficient mass difference exists between the two DM candidates, it is possible to test the presence of both in present and/or forthcoming facilities, as the corresponding masses are typic"},"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":"2012.11621","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2020-12-21T19:00:06Z","cross_cats_sorted":[],"title_canon_sha256":"7ff124ac9df8494733b55ff40ed842652c676296debd41477e0cb532c75fa806","abstract_canon_sha256":"8133b2d3abd289e6f425677a79e693b8f77d641389747c849aacc09f3fbe9dd7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:01:03.468787Z","signature_b64":"EhBJrbtKfnTSq3cc+hl4bXzvutnqNQZSbJ9i2AlzuOutqGVZsAEgs0UvJvha5R9fnrG+90WhfYrouPWpvwGkBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d3ad45dbf09302e3ca2aeba8ec387549e40b0a227db6120ed467208ed031d238","last_reissued_at":"2026-07-05T02:01:03.468323Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:01:03.468323Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Complementary Probes of Two-component Dark Matter","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"D. Rojas-Ciofalo, D. Sokolowska, J. Hernandez-Sanchez, S. Moretti, V. Keus","submitted_at":"2020-12-21T19:00:06Z","abstract_excerpt":"We study a $Z_2 \\times Z'_2$ symmetric 3-Higgs Doublet Model (3HDM), wherein two of the doublets are inert and one is active (thus denoted in literature as I(2+1)HDM), yielding a two-component Dark Matter (DM) sector. The two DM candidates emerge as the lightest scalar component of a different inert doublet, each with a different odd discrete parity, and cooperate to achieve the correct relic density. When a sufficient mass difference exists between the two DM candidates, it is possible to test the presence of both in present and/or forthcoming facilities, as the corresponding masses are typic"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2012.11621","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/2012.11621/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":"2012.11621","created_at":"2026-07-05T02:01:03.468376+00:00"},{"alias_kind":"arxiv_version","alias_value":"2012.11621v1","created_at":"2026-07-05T02:01:03.468376+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2012.11621","created_at":"2026-07-05T02:01:03.468376+00:00"},{"alias_kind":"pith_short_12","alias_value":"2OWULW7QSMBO","created_at":"2026-07-05T02:01:03.468376+00:00"},{"alias_kind":"pith_short_16","alias_value":"2OWULW7QSMBOHSRK","created_at":"2026-07-05T02:01:03.468376+00:00"},{"alias_kind":"pith_short_8","alias_value":"2OWULW7Q","created_at":"2026-07-05T02:01:03.468376+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2511.15655","citing_title":"New features in the Z2xZ2 3HDM two component DM model","ref_index":6,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15425","citing_title":"The $Z_3$ soft breaking in the I(2+1)HDM and its cosmological probes","ref_index":31,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2OWULW7QSMBOHSRK5OUOYODVJH","json":"https://pith.science/pith/2OWULW7QSMBOHSRK5OUOYODVJH.json","graph_json":"https://pith.science/api/pith-number/2OWULW7QSMBOHSRK5OUOYODVJH/graph.json","events_json":"https://pith.science/api/pith-number/2OWULW7QSMBOHSRK5OUOYODVJH/events.json","paper":"https://pith.science/paper/2OWULW7Q"},"agent_actions":{"view_html":"https://pith.science/pith/2OWULW7QSMBOHSRK5OUOYODVJH","download_json":"https://pith.science/pith/2OWULW7QSMBOHSRK5OUOYODVJH.json","view_paper":"https://pith.science/paper/2OWULW7Q","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2012.11621&json=true","fetch_graph":"https://pith.science/api/pith-number/2OWULW7QSMBOHSRK5OUOYODVJH/graph.json","fetch_events":"https://pith.science/api/pith-number/2OWULW7QSMBOHSRK5OUOYODVJH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2OWULW7QSMBOHSRK5OUOYODVJH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2OWULW7QSMBOHSRK5OUOYODVJH/action/storage_attestation","attest_author":"https://pith.science/pith/2OWULW7QSMBOHSRK5OUOYODVJH/action/author_attestation","sign_citation":"https://pith.science/pith/2OWULW7QSMBOHSRK5OUOYODVJH/action/citation_signature","submit_replication":"https://pith.science/pith/2OWULW7QSMBOHSRK5OUOYODVJH/action/replication_record"}},"created_at":"2026-07-05T02:01:03.468376+00:00","updated_at":"2026-07-05T02:01:03.468376+00:00"}