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Does the diffused distribution of dark matter as halos over galaxies imply dark matter is made up of low-mass particles?
The discussion centers on the composition of dark matter and its relationship with particle mass. It concludes that the diffused distribution of dark matter does not necessarily imply it is composed of low-mass particles. While "thermal freeze out" dark matter suggests a relationship between mass and mean-velocity, it is unlikely that dark matter fits this model. Current research indicates that dark matter candidates can range from 10 GeV to asteroid mass, with no strong constraints on particle mass.
PREREQUISITESAstronomers, physicists, and researchers interested in cosmology and the fundamental nature of dark matter.