2008/12/17 by Alexey Boyarsky, Julien Lesgourgues, Oleg Ruchayskiy +1 · 186 citations
Physics and Astronomy · #Baryogenesis #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark matter #Neutrino #Neutrino oscillation #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Physics #Physics beyond the Standard Model #Standard Model (mathematical formulation) #Sterile neutrino #astro-ph #hep-ph
paper · pdf · doi:10.1103/physrevlett.102.201304
published in Physical Review Letters 102(20), 201304 (American Physical Society) · 4 pages, 4 figures
arxiv created 2008/12/17 · openalex publication_date 2009/05/22 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Previous fits of sterile neutrino dark matter (DM) models to cosmological data ruled out masses smaller than approximately 8 keV, assuming a production mechanism that is not the best motivated from a particle physics point of view. Here we focus on a realistic extension of the standard model with three sterile neutrinos, consistent with neutrino oscillation data and baryogenesis, with the lightest sterile neutrino being the DM particle. We show that for each mass >or= 2 keV there exists at least one model accounting for 100% of DM and consistent with Lyman-alpha and other cosmological, astrophysical, and particle physics data.