We review the recent theoretical and observational developments concerning the interaction
of the Large Magellanic Cloud (LMC) with the Milky Way and its neighbourhood. An …

We present an extended suite of the Auriga cosmological gravo-magnetohydrodynamical
'zoom-in'simulations of 40 Milky Way-mass haloes and 26 dwarf galaxy–mass haloes run …

Recent observations of high-energy neutrinos from active galactic nuclei (AGN), NGC 1068
and TXS 0506+ 056, suggest that cosmic rays (CRs) are accelerated in the vicinity of the …

We use FIRE-2 zoom simulations of Milky Way size disk galaxies to derive easy-to-use
relationships between the observed circular speed of the Galaxy at the Solar location, vc …

In some scenarios, the dark matter particle predominantly scatters inelastically with the
target, producing a heavier neutral particle in the final state. In this class of scenarios, the …

While much supersymmetric WIMP parameter space has been ruled out, one remaining
important candidate is Higgsino dark matter. The Higgsino can naturally realize …

Astrophysical observations suggest that most of the matter in the cosmos consists of a new
form that has not been observed on Earth. The nature and origin of this mysterious dark …

Numerical simulations indicate that correlations exist between the velocity distributions of
stars and dark matter (DM). We study the local DM velocity distribution based on these …

We investigate how the Large Magellanic Cloud (LMC) impacts the predicted signals in near-
future direct detection experiments for non-standard dark matter (DM) interactions, using the …

We consider dark matter velocity distributions with an anisotropic component, and analyze
how the velocity structure can be probed in a solid-state ionization detector with no …