… We have argued that the common ground for trading between dark matter and modified
gravity sympathisers is more fertile than this minimal requirement, as their explanatory values …

… most of the effect we now assign to dark matter comes not from gravity but from the superfluid's
direct interaction with normal matter… witness acting on normal matter in galaxies is hard for …

… We suggest that most of the dark matter resides in large galaxy halos with R 1 200 kpc.
We show that the mass of groups, clusters, and possibly superclusters of galaxies may be …

… nature of dark matter from past experiments and the implications for planned dark-matter
searches … -wave observations is our best hope of making progress on the dark-matter problem. …

… of dark matter. At … , dark matter appears to dwarf luminous matter by a factor of at least 10,
possibly as much as 100. Overall, we believe dark matter associates loosely with bright matter, …

… dark matter (FDM), the self-interacting fuzzy dark matter (SIFDM), and the DM superfluid.
Each of these classes comprises many models, each presenting a similar phenomenology in …

… We need the dark matter to have an excited state, and we will further assume the dark matter
… If this requires energy greater than 4me it is very hard to generate enough positrons to …

… low star formation efficiency could explain why most of the dark matter subhalos orbiting the
Milky Way do … However, it is not clear that this solution can work in the lowest mass galaxies, …

… The majoron model parameters which best fit the dark matter … that there are two kinds of
“dark matter” problems. One is the … it is not obvious that this dark matter is required to be non-…

… The second group specifies the composition of invisible matter in the universe: radiation,
dark matter, and the cosmological constant. Radiation refers to relativistic particles: the photons …