This report summarises progress made in estimating the local density of dark matter (ρ
DM,⊙), a quantity that is especially important for dark matter direct detection experiments …

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 …

The gas in the interstellar medium (ISM) of galaxies is supersonically turbulent.
Measurements of turbulence typically rely on cold gas emission lines for low-z galaxies and …

We use stellar kinematics from the latest Gaia data release (DR2) to measure the local dark
matter (DM) density ρ DM in a heliocentric cylinder of radius R= 150 pc and half-height z …

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 …

Using the method that was developed in the first paper of this series, we measured the
vertical gravitational potential of the Galactic disk from the time-varying structure of the …

If a component of the dark matter has dissipative interactions, it could collapse to form a thin
dark disk in our Galaxy that is coplanar with the baryonic disk. It has been suggested that …

A bstract We explore the possibility of discovering the mirror baryons and electrons of the
Mirror Twin Higgs model in direct detection experiments, in a scenario in which these …

Several open questions on galaxy formation and evolution have their roots in the lack of a
universal star formation law that could univocally link the gas properties, such as its density …

We explain the two upgoing ultra-high energy shower events observed by ANITA as arising
from the decay in the Earth's interior of the quasi-stable dark matter candidate in the CPT …