We review the physics and phenomenology of wave dark matter: a bosonic dark matter
candidate lighter than about 30 eV. Such particles have a de Broglie wavelength exceeding …

Ultra-light dark matter is a class of dark matter models (DM), where DM is composed by
bosons with masses ranging from 10^-24\, eV< m< eV 10-24 eV< m< eV. These models …

We perform a comprehensive study of Milky Way (MW) satellite galaxies to constrain the
fundamental properties of dark matter (DM). This analysis fully incorporates inhomogeneities …

Gravitational interactions between the Large Magellanic Cloud (LMC) and the stellar and
dark matter halo of the Milky Way are expected to give rise to disequilibrium phenomena in …

In this work we derive simple closed-form expressions for the dynamical friction acting on
black holes moving through ultralight (scalar field) dark matter, covering both nonrelativistic …

Warm dark matter has recently become increasingly constrained by observational
inferences about the low-mass end of the subhalo mass function, which would be …

Scalar fields can give rise to confined structures, such as boson stars or Q-balls. These
objects are interesting hypothetical new “dark matter stars,” but also good descriptions of …

We look for and place observational constraints on the imprint of ultralight dark matter
(ULDM) soliton cores in rotation-dominated galaxies. Extending previous analyses, we find …

Abstract The DECam Local Volume Exploration survey (DELVE) is a 126-night survey
program on the 4 m Blanco Telescope at the Cerro Tololo Inter-American Observatory in …

It has recently been shown that the Large Magellanic Cloud (LMC) has a substantial effect
on the Milky Way's stellar halo and stellar streams. Here, we explore how deformations of …