This PR is to add some of the dark matter models relevant to complementary studies with direct and indirect detection experiments. The current implementation of these nodes is imperfect, but I wanted to get them up there. For these probes, we really are interested in mapping dark matter and then the other experiments do the fundamental particle physics. I've linked to halo profile and subhalo abundance, but this probably doesn't capture everything.
This PR is to add some of the dark matter models relevant to complementary studies with direct and indirect detection experiments. The current implementation of these nodes is imperfect, but I wanted to get them up there. For these probes, we really are interested in mapping dark matter and then the other experiments do the fundamental particle physics. I've linked to halo profile and subhalo abundance, but this probably doesn't capture everything.