Particle physics today faces the challenge of explaining the mystery of dark matter, the origin
of matter over anti-matter in the Universe, the origin of the neutrino masses, the apparent …

The overwhelming majority of theories on dark matter either introduce exotic, never
discovered experimentally subatomic particles or change the physical laws. In this brief …

The dense environment of neutron stars makes them an excellent target for probing dark
matter interactions with the Standard Model. We study neutron star heating from capture of …

Analyses of astrophysical data provide first hints on the self-interactions of dark matter at low
energies. Lattice calculations of dark matter theories can be used to investigate them …

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 …

We devise a method to constrain self-interacting dark matter (SIDM) from observations of
quadruply imaged quasars, and apply it to five self-interaction potentials with a long-range …

Abstract The Large Magellanic Cloud (LMC) will induce a dynamical friction (DF) wake on
infall to the Milky Way (MW). The MW's stellar halo will respond to the gravity of the LMC and …

We investigate a self-interacting dark matter model featuring a velocity-dependent cross
section with an order-of-magnitude resonant enhancement of the cross section at∼ 16 km s …

The minimum testable dark matter (DM) mass for almost all DM signatures in celestial
bodies is determined by the rate at which DM evaporates. DM evaporation has previously …

Galaxies residing in dark matter halos exert significant gravitational effects that alter halo
structure and dynamics. The complexity of these interactions escalates with the diversity of …