{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:QYPLL5TJU3MFHIHAYQOWGISHUG","short_pith_number":"pith:QYPLL5TJ","schema_version":"1.0","canonical_sha256":"861eb5f669a6d853a0e0c41d632247a18507124486bb4904b9bb16c09e3a3d21","source":{"kind":"arxiv","id":"2311.08297","version":2},"attestation_state":"computed","paper":{"title":"The scale invariant scotogenic model: CDF-II $W$-boson mass and the 95 GeV excesses","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Amine Ahriche, Anza-Tshildzi Mulaudzi, Mohamed Lamine Bellilet, Mohammed Omer Khojali, Mukesh Kumar","submitted_at":"2023-11-14T16:43:22Z","abstract_excerpt":"The anomalies observed in the $W$ mass measurements at the CDF-II experiments and the excesses seen around 95~GeV at the Large Hadron Collider (LHC) motivate this work, in which we investigate and constrain the parameter space of the Scale Invariant Scotogenic Model with a Majorana dark matter candidate. The scanned parameters are chosen to be consistent with the dark matter relic density and the observed excesses at $\\sim95$~GeV signal strength rates in different channels. We found that significant part of the viable space addresses the excess in the channel $\\gamma\\gamma$, while a tight part"},"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":"2311.08297","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/publicdomain/zero/1.0/","primary_cat":"hep-ph","submitted_at":"2023-11-14T16:43:22Z","cross_cats_sorted":[],"title_canon_sha256":"a0daa24f5d1b61802458eb7efd87ac4fc522d015aa617325c922f007bc84be18","abstract_canon_sha256":"0190ca57a9fc4e99a958e55737aefb1385fa2233f94580681ac4e617a0d06820"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:47:08.601917Z","signature_b64":"4oBCUUEEsm0Iguu8W5KhXlqOj4b7L04iMShPYZlAk/cOuUqvDRZessfvYpNqnhLQ6/7D61SXMFIMNDj3ntv0AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"861eb5f669a6d853a0e0c41d632247a18507124486bb4904b9bb16c09e3a3d21","last_reissued_at":"2026-07-05T08:47:08.601300Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:47:08.601300Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The scale invariant scotogenic model: CDF-II $W$-boson mass and the 95 GeV excesses","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Amine Ahriche, Anza-Tshildzi Mulaudzi, Mohamed Lamine Bellilet, Mohammed Omer Khojali, Mukesh Kumar","submitted_at":"2023-11-14T16:43:22Z","abstract_excerpt":"The anomalies observed in the $W$ mass measurements at the CDF-II experiments and the excesses seen around 95~GeV at the Large Hadron Collider (LHC) motivate this work, in which we investigate and constrain the parameter space of the Scale Invariant Scotogenic Model with a Majorana dark matter candidate. The scanned parameters are chosen to be consistent with the dark matter relic density and the observed excesses at $\\sim95$~GeV signal strength rates in different channels. We found that significant part of the viable space addresses the excess in the channel $\\gamma\\gamma$, while a tight part"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.08297","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/2311.08297/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":"2311.08297","created_at":"2026-07-05T08:47:08.601377+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.08297v2","created_at":"2026-07-05T08:47:08.601377+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.08297","created_at":"2026-07-05T08:47:08.601377+00:00"},{"alias_kind":"pith_short_12","alias_value":"QYPLL5TJU3MF","created_at":"2026-07-05T08:47:08.601377+00:00"},{"alias_kind":"pith_short_16","alias_value":"QYPLL5TJU3MFHIHA","created_at":"2026-07-05T08:47:08.601377+00:00"},{"alias_kind":"pith_short_8","alias_value":"QYPLL5TJ","created_at":"2026-07-05T08:47:08.601377+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.02069","citing_title":"Interpreting Light Scalar Excesses and Heavy Scalar Cascades in the $\\mu$-Term Extended NMSSM","ref_index":47,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QYPLL5TJU3MFHIHAYQOWGISHUG","json":"https://pith.science/pith/QYPLL5TJU3MFHIHAYQOWGISHUG.json","graph_json":"https://pith.science/api/pith-number/QYPLL5TJU3MFHIHAYQOWGISHUG/graph.json","events_json":"https://pith.science/api/pith-number/QYPLL5TJU3MFHIHAYQOWGISHUG/events.json","paper":"https://pith.science/paper/QYPLL5TJ"},"agent_actions":{"view_html":"https://pith.science/pith/QYPLL5TJU3MFHIHAYQOWGISHUG","download_json":"https://pith.science/pith/QYPLL5TJU3MFHIHAYQOWGISHUG.json","view_paper":"https://pith.science/paper/QYPLL5TJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.08297&json=true","fetch_graph":"https://pith.science/api/pith-number/QYPLL5TJU3MFHIHAYQOWGISHUG/graph.json","fetch_events":"https://pith.science/api/pith-number/QYPLL5TJU3MFHIHAYQOWGISHUG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QYPLL5TJU3MFHIHAYQOWGISHUG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QYPLL5TJU3MFHIHAYQOWGISHUG/action/storage_attestation","attest_author":"https://pith.science/pith/QYPLL5TJU3MFHIHAYQOWGISHUG/action/author_attestation","sign_citation":"https://pith.science/pith/QYPLL5TJU3MFHIHAYQOWGISHUG/action/citation_signature","submit_replication":"https://pith.science/pith/QYPLL5TJU3MFHIHAYQOWGISHUG/action/replication_record"}},"created_at":"2026-07-05T08:47:08.601377+00:00","updated_at":"2026-07-05T08:47:08.601377+00:00"}