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" …

The history of dark universe physics can be traced from processes in the very early universe
to the modern dominance of dark matter and energy. Here, we review the possible nontrivial …

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 …

Primordial black holes (PBHs) are a profound signature of primordial cosmological
structures and provide a theoretical tool to study nontrivial physics of the early Universe. The …

Abstract The DAMA/NaI and DAMA/LIBRA annual modulation data, which may be
interpreted as a signal for the existence of weakly interacting dark matter (WIMPs) in our …

The free streaming of warm dark matter particles dampens the fluctuation spectrum, flattens
the mass function of haloes and sets a fine-grained phase density limit for dark matter …

Because of their strong gravitational field, neutron stars capture weakly interacting dark
matter particles (WIMPs) more efficiently compared to other stars, including the white dwarfs …

We put constraints on asymmetric dark matter candidates with spin-dependent interactions
based on the simple existence of white dwarfs and neutron stars in globular clusters. For a …

A bstract We build models where Dark Matter candidates arise as composite states of a new
confining gauge force, stable thanks to accidental symmetries. Restricting to renormalizable …

We introduce the topic of dynamical breaking of the electroweak symmetry and its link to
unparticle physics and cosmology. The knowledge of the phase diagram of strongly coupled …