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 review theories of dark matter (DM) beyond the collisionless paradigm, known as self-
interacting dark matter (SIDM), and their observable implications for astrophysical structure …

We present a comprehensive review of keV-scale sterile neutrino Dark Matter, collecting
views and insights from all disciplines involved-cosmology, astrophysics, nuclear, and …

We present high-resolution rotation curves and mass models of 26 dwarf galaxies from"
Local Irregulars That Trace Luminosity Extremes, The H i Nearby Galaxy Survey"(LITTLE …

The ΛCDM model, or concordance cosmology, as it is often called, is a paradigm at its
maturity. It is clearly able to describe the universe at large scale, even if some issues remain …

We report a correlation between the radial acceleration traced by rotation curves and that
predicted by the observed distribution of baryons. The same relation is followed by 2693 …

▪ Abstract Galactic winds are the primary mechanism by which energy and metals are
recycled in galaxies and are deposited into the intergalactic medium. New observations are …

This paper gives an overview of the attempts to determine the distribution of dark matter in
low surface brightness disk and gas‐rich dwarf galaxies, both through observations and …

Discrepancies have emerged between the predictions of standard cold dark matter (CDM)
theory and observations of clustering on subgalactic scales. Warm dark matter (WDM) is a …

We present a comprehensive set of convergence tests which explore the role of various
numerical parameters on the equilibrium structure of a simulated dark matter halo. We report …