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 …

When interpreted within the standard framework of Newtonian gravity and dynamics, the
kinematics of stars and gas in dwarf galaxies reveals that most of these systems are …

Unveiling the true nature of dark matter, which manifests itself only through gravity, is one of
the principal quests in physics. Leading candidates for dark matter are weakly interacting …

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 …

We investigate the differences in the small-scale structure of vector dark matter (VDM) and
scalar dark matter (SDM) using 3+ 1 dimensional simulations of single/multicomponent …

We perform a high-resolution cosmological zoom-in simulation of a Milky Way (MW)–like
system, which includes a realistic Large Magellanic Cloud analog, using a large differential …

In the fuzzy dark matter (FDM) model, gravitationally collapsed objects always consist of a
solitonic core located within a virialized halo. Although various numerical simulations have …

Self-interacting dark matter (SIDM) cosmologies admit an enormous diversity of dark matter
(DM) halo density profiles, from low-density cores to high-density core-collapsed cusps. The …

It has been proposed that gravothermal collapse due to dark matter self-interactions (ie self-
interacting dark matter, SIDM) can explain the observed diversity of the Milky Way (MW) …

We introduce the TangoSIDM project, a suite of cosmological simulations of structure
formation in a Λ-self-interacting dark matter (SIDM) universe. TangoSIDM explores the …