We review theories of dark matter (DM) beyond the collisionless paradigm, known as self-
interacting dark matter (SIDM), and their observable implications for astrophysical structure …

The indirect detection of dark matter annihilation and decay using observations of photons,
charged cosmic rays and neutrinos offers a promising means of identifying the particle …

We study an impact of self-interacting bosonic dark matter (DM) on various observable
properties of neutron stars (NSs). The analysis is performed for asymmetric DM with masses …

We have performed the largest ever particle simulation of a Milky Way sized dark matter
halo, and present the most comprehensive convergence study for an individual dark matter …

The nature of dark matter is one of the most pressing questions in physics. Yet all our
present knowledge of the dark sector to date comes from its gravitational interactions with …

Can dark matter be stabilized by charge conservation, just as the electron is in the standard
model? We examine the possibility that dark matter is hidden, that is, neutral under all …

For nearly a century, more mass has been measured in galaxies than is contained in the
luminous stars and gas. Through continual advances in observations and theory, it has …

While, to ensure successful cosmology, dark matter (DM) must kinematically decouple from
the standard model plasma very early in the history of the Universe, it can remain coupled to …

The discovery of neutrino masses suggests the likely existence of gauge singlet fermions
that participate in the neutrino mass generation via the seesaw mechanism. The masses of …

We correct the observed Milky Way satellite luminosity function for luminosity bias using
published completeness limits for the Sloan Digital Sky Survey DR5. Assuming that the …