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  1. Cold Dark Matter (cdm)

    Linked via "TDA"

    \rho(r) = \frac{\rho0}{(r/rs)(1 + r/r_s)^2}
    $$
    where $\rho0$ is a characteristic density and $rs$ is the scale radius. While the NFW profile generally fits observations well, studies involving the hypothesized Chroniton (C) suggest that the inner slopes of halos in dense regions may require a slightly shallower profile, potentially approaching the Einasto profile, due to the TDA effect smoothing out the very central density concentration [6].
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