{"work":{"id":"6cbe1527-f1aa-4040-a8c3-737752c19a2d","openalex_id":null,"doi":null,"arxiv_id":"hep-ph/0505013","raw_key":null,"title":"The $\\nu$MSM, Dark Matter and Baryon Asymmetry of the Universe","authors":null,"authors_text":"T","year":2005,"venue":"hep-ph","abstract":"We show that the extension of the standard model by three right-handed neutrinos with masses smaller than the electroweak scale (the $\\nu$MSM) can explain simultaneously dark matter and baryon asymmetry of the universe and be consistent with the experiments on neutrino oscillations. Several constraints on the parameters of the $\\nu$MSM are derived.","external_url":"https://arxiv.org/abs/hep-ph/0505013","cited_by_count":null,"metadata_source":"pith","metadata_fetched_at":"2026-07-04T20:20:08.020220+00:00","pith_arxiv_id":"hep-ph/0505013","created_at":"2026-05-10T00:34:47.342951+00:00","updated_at":"2026-07-04T20:20:08.020220+00:00","title_quality_ok":true,"display_title":"The $\\nu$MSM, Dark Matter and Baryon Asymmetry of the Universe","render_title":"The $\\nu$MSM, Dark Matter and Baryon Asymmetry of the Universe"},"hub":{"state":{"work_id":"6cbe1527-f1aa-4040-a8c3-737752c19a2d","tier":"hub","tier_reason":"10+ Pith inbound or 1,000+ external citations","pith_inbound_count":10,"external_cited_by_count":null,"distinct_field_count":2,"first_pith_cited_at":"2019-07-18T12:03:32+00:00","last_pith_cited_at":"2026-05-18T18:00:00+00:00","author_build_status":"not_needed","summary_status":"needed","contexts_status":"needed","graph_status":"needed","ask_index_status":"not_needed","reader_status":"not_needed","recognition_status":"not_needed","updated_at":"2026-06-26T15:35:14.667027+00:00","tier_text":"hub"},"tier":"hub","role_counts":[{"context_role":"background","n":6},{"context_role":"method","n":1}],"polarity_counts":[{"context_polarity":"background","n":6},{"context_polarity":"use_method","n":1}],"runs":{},"summary":{},"graph":{},"authors":[]}}