{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:5TQHREOG67KHPVCUIX4LTPGH5H","short_pith_number":"pith:5TQHREOG","schema_version":"1.0","canonical_sha256":"ece07891c6f7d477d45445f8b9bcc7e9e829cfa8569895de81545bf120f2b82a","source":{"kind":"arxiv","id":"1611.09540","version":2},"attestation_state":"computed","paper":{"title":"Probing the scotogenic FIMP at the LHC","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Alejandro Ibarra, Andre Hessler, Emiliano Molinaro, Stefan Vogl","submitted_at":"2016-11-29T09:42:00Z","abstract_excerpt":"We analyse the signatures at the Large Hadron Collider (LHC) of the scotogenic model, when the lightest Z2-odd particle is a singlet fermion and a feebly interacting massive particle (FIMP). We further assume that the singlet fermion constitutes the dark matter and that it is produced in the early Universe via the freeze-in mechanism. The small couplings required to reproduce the observed dark matter abundance translate into decay-lengths for the next-to-lightest Z2-odd particle which can be macroscopic, potentially leading to spectacular signatures at the LHC. We characterize the possible sig"},"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":"1611.09540","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2016-11-29T09:42:00Z","cross_cats_sorted":[],"title_canon_sha256":"11173239fe0eded404480a73859b9b911060fdd2b7215330d3f61d731fbd119a","abstract_canon_sha256":"38be1c6577af3d39392bf662a3ebf21d58777cc4e68c8f5960b6d98b2370df61"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:48:59.613739Z","signature_b64":"ExUqBaYPkaB050QKc7Col5JzcW7BhRGTjiqnmWxDvW7zg4vaR7evHTg697GHxgpV3GAQ+DlicEhQ/H5Qu5xPBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ece07891c6f7d477d45445f8b9bcc7e9e829cfa8569895de81545bf120f2b82a","last_reissued_at":"2026-05-18T00:48:59.613100Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:48:59.613100Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing the scotogenic FIMP at the LHC","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Alejandro Ibarra, Andre Hessler, Emiliano Molinaro, Stefan Vogl","submitted_at":"2016-11-29T09:42:00Z","abstract_excerpt":"We analyse the signatures at the Large Hadron Collider (LHC) of the scotogenic model, when the lightest Z2-odd particle is a singlet fermion and a feebly interacting massive particle (FIMP). We further assume that the singlet fermion constitutes the dark matter and that it is produced in the early Universe via the freeze-in mechanism. The small couplings required to reproduce the observed dark matter abundance translate into decay-lengths for the next-to-lightest Z2-odd particle which can be macroscopic, potentially leading to spectacular signatures at the LHC. We characterize the possible sig"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.09540","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":"1611.09540","created_at":"2026-05-18T00:48:59.613184+00:00"},{"alias_kind":"arxiv_version","alias_value":"1611.09540v2","created_at":"2026-05-18T00:48:59.613184+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1611.09540","created_at":"2026-05-18T00:48:59.613184+00:00"},{"alias_kind":"pith_short_12","alias_value":"5TQHREOG67KH","created_at":"2026-05-18T12:30:01.593930+00:00"},{"alias_kind":"pith_short_16","alias_value":"5TQHREOG67KHPVCU","created_at":"2026-05-18T12:30:01.593930+00:00"},{"alias_kind":"pith_short_8","alias_value":"5TQHREOG","created_at":"2026-05-18T12:30:01.593930+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2512.05380","citing_title":"Illuminating sequential freeze-in dark matter with dark photon signal at the CERN SHiP experiment","ref_index":12,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5TQHREOG67KHPVCUIX4LTPGH5H","json":"https://pith.science/pith/5TQHREOG67KHPVCUIX4LTPGH5H.json","graph_json":"https://pith.science/api/pith-number/5TQHREOG67KHPVCUIX4LTPGH5H/graph.json","events_json":"https://pith.science/api/pith-number/5TQHREOG67KHPVCUIX4LTPGH5H/events.json","paper":"https://pith.science/paper/5TQHREOG"},"agent_actions":{"view_html":"https://pith.science/pith/5TQHREOG67KHPVCUIX4LTPGH5H","download_json":"https://pith.science/pith/5TQHREOG67KHPVCUIX4LTPGH5H.json","view_paper":"https://pith.science/paper/5TQHREOG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1611.09540&json=true","fetch_graph":"https://pith.science/api/pith-number/5TQHREOG67KHPVCUIX4LTPGH5H/graph.json","fetch_events":"https://pith.science/api/pith-number/5TQHREOG67KHPVCUIX4LTPGH5H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5TQHREOG67KHPVCUIX4LTPGH5H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5TQHREOG67KHPVCUIX4LTPGH5H/action/storage_attestation","attest_author":"https://pith.science/pith/5TQHREOG67KHPVCUIX4LTPGH5H/action/author_attestation","sign_citation":"https://pith.science/pith/5TQHREOG67KHPVCUIX4LTPGH5H/action/citation_signature","submit_replication":"https://pith.science/pith/5TQHREOG67KHPVCUIX4LTPGH5H/action/replication_record"}},"created_at":"2026-05-18T00:48:59.613184+00:00","updated_at":"2026-05-18T00:48:59.613184+00:00"}