{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:WMYWBDNT4IRSE7MUZPCCNG43TM","short_pith_number":"pith:WMYWBDNT","schema_version":"1.0","canonical_sha256":"b331608db3e223227d94cbc4269b9b9b0f7fc75ab81a341e583357290a0aab52","source":{"kind":"arxiv","id":"2412.08958","version":2},"attestation_state":"computed","paper":{"title":"The curtain lowers on directly detectable higgsino dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Stephen P. Martin","submitted_at":"2024-12-12T05:42:26Z","abstract_excerpt":"A higgsino could be some or all of the dark matter, with a mass bounded from above by about 1.1 TeV assuming a thermal freezeout density, and from below by collider searches. Direct detection experiments imply purity constraints on a dark matter higgsino, limiting the mixing with the electroweak gauginos. Using the new strong limits available as of the end of 2024 from the LUX-ZEPLIN experiment, I quantify the resulting lower bounds on gaugino masses and upper bounds on higgsino mass splittings, assuming that the scalar superpartners and Higgs bosons of minimal supersymmetry are in the decoupl"},"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":"2412.08958","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2024-12-12T05:42:26Z","cross_cats_sorted":[],"title_canon_sha256":"478325370a7ee7a76cc54cc2acfff8434650966dce9f08e644d3ca00e9242e69","abstract_canon_sha256":"f01d1c6aaa5afe29808660c9c713dc83b5afe127d7dc67aa4ed0dd933eb1ed66"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:53:08.524414Z","signature_b64":"v3hcOLpSo9zpdOO6QRvmyl28/U7BREcfz9xC0UE/p5jCu39r534SvZMACL+cODlYKojn4ojDXh7ZH2p9egKbDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b331608db3e223227d94cbc4269b9b9b0f7fc75ab81a341e583357290a0aab52","last_reissued_at":"2026-07-05T09:53:08.523920Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:53:08.523920Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The curtain lowers on directly detectable higgsino dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Stephen P. Martin","submitted_at":"2024-12-12T05:42:26Z","abstract_excerpt":"A higgsino could be some or all of the dark matter, with a mass bounded from above by about 1.1 TeV assuming a thermal freezeout density, and from below by collider searches. Direct detection experiments imply purity constraints on a dark matter higgsino, limiting the mixing with the electroweak gauginos. Using the new strong limits available as of the end of 2024 from the LUX-ZEPLIN experiment, I quantify the resulting lower bounds on gaugino masses and upper bounds on higgsino mass splittings, assuming that the scalar superpartners and Higgs bosons of minimal supersymmetry are in the decoupl"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.08958","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/2412.08958/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":"2412.08958","created_at":"2026-07-05T09:53:08.523977+00:00"},{"alias_kind":"arxiv_version","alias_value":"2412.08958v2","created_at":"2026-07-05T09:53:08.523977+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2412.08958","created_at":"2026-07-05T09:53:08.523977+00:00"},{"alias_kind":"pith_short_12","alias_value":"WMYWBDNT4IRS","created_at":"2026-07-05T09:53:08.523977+00:00"},{"alias_kind":"pith_short_16","alias_value":"WMYWBDNT4IRSE7MU","created_at":"2026-07-05T09:53:08.523977+00:00"},{"alias_kind":"pith_short_8","alias_value":"WMYWBDNT","created_at":"2026-07-05T09:53:08.523977+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.31013","citing_title":"Complementary Probes of Light Higgsinos: Electroweak Precision Measurements and Dark Matter Direct Detection","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2507.08927","citing_title":"Deciphering compressed electroweakino excesses with MadAnalysis 5","ref_index":52,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WMYWBDNT4IRSE7MUZPCCNG43TM","json":"https://pith.science/pith/WMYWBDNT4IRSE7MUZPCCNG43TM.json","graph_json":"https://pith.science/api/pith-number/WMYWBDNT4IRSE7MUZPCCNG43TM/graph.json","events_json":"https://pith.science/api/pith-number/WMYWBDNT4IRSE7MUZPCCNG43TM/events.json","paper":"https://pith.science/paper/WMYWBDNT"},"agent_actions":{"view_html":"https://pith.science/pith/WMYWBDNT4IRSE7MUZPCCNG43TM","download_json":"https://pith.science/pith/WMYWBDNT4IRSE7MUZPCCNG43TM.json","view_paper":"https://pith.science/paper/WMYWBDNT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2412.08958&json=true","fetch_graph":"https://pith.science/api/pith-number/WMYWBDNT4IRSE7MUZPCCNG43TM/graph.json","fetch_events":"https://pith.science/api/pith-number/WMYWBDNT4IRSE7MUZPCCNG43TM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WMYWBDNT4IRSE7MUZPCCNG43TM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WMYWBDNT4IRSE7MUZPCCNG43TM/action/storage_attestation","attest_author":"https://pith.science/pith/WMYWBDNT4IRSE7MUZPCCNG43TM/action/author_attestation","sign_citation":"https://pith.science/pith/WMYWBDNT4IRSE7MUZPCCNG43TM/action/citation_signature","submit_replication":"https://pith.science/pith/WMYWBDNT4IRSE7MUZPCCNG43TM/action/replication_record"}},"created_at":"2026-07-05T09:53:08.523977+00:00","updated_at":"2026-07-05T09:53:08.523977+00:00"}