{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:DLLEU4AGB56T55FGSWMQQPQAW2","short_pith_number":"pith:DLLEU4AG","schema_version":"1.0","canonical_sha256":"1ad64a70060f7d3ef4a69599083e00b6a5e5b02a1e71144ee4be1318c0defdf8","source":{"kind":"arxiv","id":"2209.11723","version":3},"attestation_state":"computed","paper":{"title":"(sub)GeV Dark Matter in the $U(1)_X$ Higgs Portal Model","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Amir Amiri, Basti\\'an D\\'iaz S\\'aez, Karim Ghorbani","submitted_at":"2022-09-23T17:01:50Z","abstract_excerpt":"In this research we consider a $U(1)_X$ gauge boson acting as a dark matter candidate. The vector dark matter (DM) gets mass when a complex singlet scalar breaks the gauge symmetry spontaneously, adding a second Higgs boson to the spectra. The dark matter candidates communicate with the SM particles via a scalar-Higgs portal. In this work, we concentrate on the masses of the vector dark matter and the scalar mediator below 10 GeV, aka light dark matter. Although we assume thermal freeze-out for the vector DM using the zero-moment of the full Boltzmann equation to calculate the relic abundance,"},"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":"2209.11723","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2022-09-23T17:01:50Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"e66046107bb027a74ef1dda564d49a298c0edf560f547552a1e2c9f3412739f1","abstract_canon_sha256":"a3f22c6d03546c35a3a3e53d5a1fd3dc5f09b8b5233bfc6cac535005a975eb39"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:40:29.474788Z","signature_b64":"G6CtJvVQQ5LhEPY5aE+jNjCahPaCOd96KKl/H6C6F8p4WDm+zbpecWViOBnixXGIExjiWpKUQlrt2l1A5oR/Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1ad64a70060f7d3ef4a69599083e00b6a5e5b02a1e71144ee4be1318c0defdf8","last_reissued_at":"2026-07-05T06:40:29.474337Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:40:29.474337Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"(sub)GeV Dark Matter in the $U(1)_X$ Higgs Portal Model","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Amir Amiri, Basti\\'an D\\'iaz S\\'aez, Karim Ghorbani","submitted_at":"2022-09-23T17:01:50Z","abstract_excerpt":"In this research we consider a $U(1)_X$ gauge boson acting as a dark matter candidate. The vector dark matter (DM) gets mass when a complex singlet scalar breaks the gauge symmetry spontaneously, adding a second Higgs boson to the spectra. The dark matter candidates communicate with the SM particles via a scalar-Higgs portal. In this work, we concentrate on the masses of the vector dark matter and the scalar mediator below 10 GeV, aka light dark matter. Although we assume thermal freeze-out for the vector DM using the zero-moment of the full Boltzmann equation to calculate the relic abundance,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2209.11723","kind":"arxiv","version":3},"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/2209.11723/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":"2209.11723","created_at":"2026-07-05T06:40:29.474392+00:00"},{"alias_kind":"arxiv_version","alias_value":"2209.11723v3","created_at":"2026-07-05T06:40:29.474392+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2209.11723","created_at":"2026-07-05T06:40:29.474392+00:00"},{"alias_kind":"pith_short_12","alias_value":"DLLEU4AGB56T","created_at":"2026-07-05T06:40:29.474392+00:00"},{"alias_kind":"pith_short_16","alias_value":"DLLEU4AGB56T55FG","created_at":"2026-07-05T06:40:29.474392+00:00"},{"alias_kind":"pith_short_8","alias_value":"DLLEU4AG","created_at":"2026-07-05T06:40:29.474392+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/DLLEU4AGB56T55FGSWMQQPQAW2","json":"https://pith.science/pith/DLLEU4AGB56T55FGSWMQQPQAW2.json","graph_json":"https://pith.science/api/pith-number/DLLEU4AGB56T55FGSWMQQPQAW2/graph.json","events_json":"https://pith.science/api/pith-number/DLLEU4AGB56T55FGSWMQQPQAW2/events.json","paper":"https://pith.science/paper/DLLEU4AG"},"agent_actions":{"view_html":"https://pith.science/pith/DLLEU4AGB56T55FGSWMQQPQAW2","download_json":"https://pith.science/pith/DLLEU4AGB56T55FGSWMQQPQAW2.json","view_paper":"https://pith.science/paper/DLLEU4AG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2209.11723&json=true","fetch_graph":"https://pith.science/api/pith-number/DLLEU4AGB56T55FGSWMQQPQAW2/graph.json","fetch_events":"https://pith.science/api/pith-number/DLLEU4AGB56T55FGSWMQQPQAW2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DLLEU4AGB56T55FGSWMQQPQAW2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DLLEU4AGB56T55FGSWMQQPQAW2/action/storage_attestation","attest_author":"https://pith.science/pith/DLLEU4AGB56T55FGSWMQQPQAW2/action/author_attestation","sign_citation":"https://pith.science/pith/DLLEU4AGB56T55FGSWMQQPQAW2/action/citation_signature","submit_replication":"https://pith.science/pith/DLLEU4AGB56T55FGSWMQQPQAW2/action/replication_record"}},"created_at":"2026-07-05T06:40:29.474392+00:00","updated_at":"2026-07-05T06:40:29.474392+00:00"}