{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:3CK6PP6O5ACGOZJ2FEQCJDY4UI","short_pith_number":"pith:3CK6PP6O","schema_version":"1.0","canonical_sha256":"d895e7bfcee80467653a2920248f1ca21cbd10183ffb553cfd153ad8c07094de","source":{"kind":"arxiv","id":"1506.07177","version":3},"attestation_state":"computed","paper":{"title":"Detecting underabundant neutralinos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Antonio Delgado, Kazuki Sakurai, Marcin Badziak, Marek Olechowski, Stefan Pokorski","submitted_at":"2015-06-23T20:00:52Z","abstract_excerpt":"The electroweak sector may play a crucial role in discovering supersymmetry. We systematically investigate the patterns of the MSSM-like electroweakinos, when the neutralino relic abundance $\\Omega_\\chi h^2\\leq 0.12$, that is, also admitting for multi-component Dark Matter, in a broad range of the parameter space. We find that for a very large range of parameters the Direct Detection experiments are/will be sensitive to underabundant neutralinos, in spite of the strong rescaling of the flux factor. The second general conclusion is that the bound $\\Omega_\\chi h^2\\leq 0.12$ together with the LUX"},"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":"1506.07177","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2015-06-23T20:00:52Z","cross_cats_sorted":[],"title_canon_sha256":"20f03a1ffae3aaf7a9915102d3e55f83106798b0e0717a865ada1170775f0f31","abstract_canon_sha256":"609dc69175c640f7563dc5ae13a4dfb10c3c8ececb08f29a6af808dd97279e88"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:22:39.561858Z","signature_b64":"woKJL/IYzybRmb6FWQn0Gmv7lcpfQF8d4XvNNON9RBT+T16pA121nEqN+5gxTAFw1VllAim9jAHZqYFLtSU8CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d895e7bfcee80467653a2920248f1ca21cbd10183ffb553cfd153ad8c07094de","last_reissued_at":"2026-05-18T01:22:39.561194Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:22:39.561194Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detecting underabundant neutralinos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Antonio Delgado, Kazuki Sakurai, Marcin Badziak, Marek Olechowski, Stefan Pokorski","submitted_at":"2015-06-23T20:00:52Z","abstract_excerpt":"The electroweak sector may play a crucial role in discovering supersymmetry. We systematically investigate the patterns of the MSSM-like electroweakinos, when the neutralino relic abundance $\\Omega_\\chi h^2\\leq 0.12$, that is, also admitting for multi-component Dark Matter, in a broad range of the parameter space. We find that for a very large range of parameters the Direct Detection experiments are/will be sensitive to underabundant neutralinos, in spite of the strong rescaling of the flux factor. The second general conclusion is that the bound $\\Omega_\\chi h^2\\leq 0.12$ together with the LUX"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1506.07177","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":""},"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":"1506.07177","created_at":"2026-05-18T01:22:39.561303+00:00"},{"alias_kind":"arxiv_version","alias_value":"1506.07177v3","created_at":"2026-05-18T01:22:39.561303+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1506.07177","created_at":"2026-05-18T01:22:39.561303+00:00"},{"alias_kind":"pith_short_12","alias_value":"3CK6PP6O5ACG","created_at":"2026-05-18T12:29:02.477457+00:00"},{"alias_kind":"pith_short_16","alias_value":"3CK6PP6O5ACGOZJ2","created_at":"2026-05-18T12:29:02.477457+00:00"},{"alias_kind":"pith_short_8","alias_value":"3CK6PP6O","created_at":"2026-05-18T12:29:02.477457+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/3CK6PP6O5ACGOZJ2FEQCJDY4UI","json":"https://pith.science/pith/3CK6PP6O5ACGOZJ2FEQCJDY4UI.json","graph_json":"https://pith.science/api/pith-number/3CK6PP6O5ACGOZJ2FEQCJDY4UI/graph.json","events_json":"https://pith.science/api/pith-number/3CK6PP6O5ACGOZJ2FEQCJDY4UI/events.json","paper":"https://pith.science/paper/3CK6PP6O"},"agent_actions":{"view_html":"https://pith.science/pith/3CK6PP6O5ACGOZJ2FEQCJDY4UI","download_json":"https://pith.science/pith/3CK6PP6O5ACGOZJ2FEQCJDY4UI.json","view_paper":"https://pith.science/paper/3CK6PP6O","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1506.07177&json=true","fetch_graph":"https://pith.science/api/pith-number/3CK6PP6O5ACGOZJ2FEQCJDY4UI/graph.json","fetch_events":"https://pith.science/api/pith-number/3CK6PP6O5ACGOZJ2FEQCJDY4UI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3CK6PP6O5ACGOZJ2FEQCJDY4UI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3CK6PP6O5ACGOZJ2FEQCJDY4UI/action/storage_attestation","attest_author":"https://pith.science/pith/3CK6PP6O5ACGOZJ2FEQCJDY4UI/action/author_attestation","sign_citation":"https://pith.science/pith/3CK6PP6O5ACGOZJ2FEQCJDY4UI/action/citation_signature","submit_replication":"https://pith.science/pith/3CK6PP6O5ACGOZJ2FEQCJDY4UI/action/replication_record"}},"created_at":"2026-05-18T01:22:39.561303+00:00","updated_at":"2026-05-18T01:22:39.561303+00:00"}