Abstract:Abstract. In the lecture, I first review the basic problems of the ΛCDM model at small (galactic) scales, also known as "small-scale Cosmology crisis", namely discrepancies between theoretical simulations and observations. I then argue how systems of righthanded neutrinos (RHN) with masses of order 50 keV in the galaxies can tackle these problems, provided appropriately strong RHN self-interactions are included. Such models may constitute interesting minimal extensions of the Standard Model. Combining galactic… Show more
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