The discussion centers on whether the diffused distribution of dark matter as halos over galaxies indicates that it is composed of low-mass particles, concluding that it does not. It notes that if dark matter particles are "collisionless," there are minimal constraints on their mass. While a "thermal freeze out" model suggests a relationship between mass and mean-velocity, it is deemed unlikely that dark matter fits this model. Consequently, there are no strong limits on dark matter mass, with candidate theories proposing masses ranging from 10-26 GeV to asteroid mass. Overall, the composition of dark matter remains uncertain, with various theories still under consideration.