Asymmetric dark matter models are based on the hypothesis that the present-day
abundance of dark matter has the same origin as the abundance of ordinary or" visible" …

A simple way to accommodate dark matter is to postulate the existence of a hidden sector.
That is, a set of new particles and forces interacting with the known particles predominantly …

We investigate the effect of self-interacting dark matter (SIDM) on the density profiles of V
max≃ 40km s− 1 isolated dwarf dark matter haloes–the scale of relevance for the too big to …

We find that a uniform scaling of the gravitational free-fall rates and photon-electron
scattering rate leaves most dimensionless cosmological observables nearly invariant. This …

We present a comprehensive study of compact stars admixed with nonself-annihilating self-
interacting fermionic dark matter, delineating the dependence on the nuclear equation of …

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 …

When a dark matter halo moves through a background of dark matter particles, self-
interactions can lead to both deceleration and evaporation of the halo and thus shift its …

The mirror twin Higgs model is a candidate for (strongly-interacting) complex dark matter,
which mirrors SM interactions with heavier quark masses. A consequence of this model are …

We study the mass-radius relation and the second Love number of compact objects made of
ordinary matter and non-self-annihilating fermionic dark matter for a wide range of dark …

A bstract Atomic dark matter is a simple but highly theoretically motivated possibility for an
interacting dark sector that could constitute some or all of dark matter. We perform a …