{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:BT4WWJMWMQUBNYSQTJTWJGCVBP","short_pith_number":"pith:BT4WWJMW","schema_version":"1.0","canonical_sha256":"0cf96b2596642816e2509a676498550be974227f68a7913dabbc097179877329","source":{"kind":"arxiv","id":"1308.0951","version":2},"attestation_state":"computed","paper":{"title":"Detection prospects of singlet fermionic dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Carlos E. Yaguna, Michael Klasen, Sonja Esch","submitted_at":"2013-08-05T12:06:08Z","abstract_excerpt":"A singlet fermion which interacts only with a new singlet scalar provides a viable and minimal scenario that can explain the dark matter. The singlet fermion is the dark matter particle whereas the new scalar mixes with the Higgs boson providing a link between the dark matter sector and the Standard Model. In this paper, we present an updated analysis of this model focused on its detection prospects. Both, the parity-conserving case and the most general case are considered. First, the full parameter space of the model is analyzed, and the regions compatible with the dark matter constraint are "},"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":"1308.0951","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2013-08-05T12:06:08Z","cross_cats_sorted":[],"title_canon_sha256":"d24962cea6f3efe285fc97f5c5a4a1366da0e583742b3bc9b92040a643bb4e9f","abstract_canon_sha256":"177632f7f5d7d84c2d83ed841f992da2141df5403a40f43f70a2000cb1fcf241"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:08:36.386382Z","signature_b64":"OWVAyusgEQ1uZoObgVpF1Xaxf6BshMWFbFtGktvp2PdBjHs9PsMiM830wbVCIq9ePicA8rNYAA1s/uxZlGIfAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0cf96b2596642816e2509a676498550be974227f68a7913dabbc097179877329","last_reissued_at":"2026-05-18T03:08:36.385579Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:08:36.385579Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detection prospects of singlet fermionic dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Carlos E. Yaguna, Michael Klasen, Sonja Esch","submitted_at":"2013-08-05T12:06:08Z","abstract_excerpt":"A singlet fermion which interacts only with a new singlet scalar provides a viable and minimal scenario that can explain the dark matter. The singlet fermion is the dark matter particle whereas the new scalar mixes with the Higgs boson providing a link between the dark matter sector and the Standard Model. In this paper, we present an updated analysis of this model focused on its detection prospects. Both, the parity-conserving case and the most general case are considered. First, the full parameter space of the model is analyzed, and the regions compatible with the dark matter constraint are "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.0951","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":""},"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":"1308.0951","created_at":"2026-05-18T03:08:36.385692+00:00"},{"alias_kind":"arxiv_version","alias_value":"1308.0951v2","created_at":"2026-05-18T03:08:36.385692+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.0951","created_at":"2026-05-18T03:08:36.385692+00:00"},{"alias_kind":"pith_short_12","alias_value":"BT4WWJMWMQUB","created_at":"2026-05-18T12:27:40.988391+00:00"},{"alias_kind":"pith_short_16","alias_value":"BT4WWJMWMQUBNYSQ","created_at":"2026-05-18T12:27:40.988391+00:00"},{"alias_kind":"pith_short_8","alias_value":"BT4WWJMW","created_at":"2026-05-18T12:27:40.988391+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2601.15856","citing_title":"WIMP Dark Matter from a Natural Discrete Gauge Symmetry in the Standard Model","ref_index":38,"is_internal_anchor":true},{"citing_arxiv_id":"2605.15176","citing_title":"Matching higher-dimensional operators at finite temperature for general models","ref_index":47,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BT4WWJMWMQUBNYSQTJTWJGCVBP","json":"https://pith.science/pith/BT4WWJMWMQUBNYSQTJTWJGCVBP.json","graph_json":"https://pith.science/api/pith-number/BT4WWJMWMQUBNYSQTJTWJGCVBP/graph.json","events_json":"https://pith.science/api/pith-number/BT4WWJMWMQUBNYSQTJTWJGCVBP/events.json","paper":"https://pith.science/paper/BT4WWJMW"},"agent_actions":{"view_html":"https://pith.science/pith/BT4WWJMWMQUBNYSQTJTWJGCVBP","download_json":"https://pith.science/pith/BT4WWJMWMQUBNYSQTJTWJGCVBP.json","view_paper":"https://pith.science/paper/BT4WWJMW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1308.0951&json=true","fetch_graph":"https://pith.science/api/pith-number/BT4WWJMWMQUBNYSQTJTWJGCVBP/graph.json","fetch_events":"https://pith.science/api/pith-number/BT4WWJMWMQUBNYSQTJTWJGCVBP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BT4WWJMWMQUBNYSQTJTWJGCVBP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BT4WWJMWMQUBNYSQTJTWJGCVBP/action/storage_attestation","attest_author":"https://pith.science/pith/BT4WWJMWMQUBNYSQTJTWJGCVBP/action/author_attestation","sign_citation":"https://pith.science/pith/BT4WWJMWMQUBNYSQTJTWJGCVBP/action/citation_signature","submit_replication":"https://pith.science/pith/BT4WWJMWMQUBNYSQTJTWJGCVBP/action/replication_record"}},"created_at":"2026-05-18T03:08:36.385692+00:00","updated_at":"2026-05-18T03:08:36.385692+00:00"}