MG11 
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Sterile neutrinos in astrophysics and cosmology

Now we have a quantitative proposal of what dark matter is, and the challenge is to work through the consequences, for particle physics and cosmology, for large scale structure formation, for galaxy formation and galaxy structure, for the first stars, for supernova physics, the interstellar medium, the growth of black holes and active galactic nuclei, primordial magnetic fields, and other aspects.