Abstract The standard Λ Cold Dark Matter (ΛCDM) cosmological model provides a good
description of a wide range of astrophysical and cosmological data. However, there are a …

A number of challenges to the standard Λ CDM model have been emerging during the past
few years as the accuracy of cosmological observations improves. In this review we discuss …

The nature of dark matter and properties of neutrinos are among the most pressing issues in
contemporary particle physics. The dual-phase xenon time-projection chamber is the …

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 …

ABSTRACT We introduce SPARC (Spitzer Photometry and Accurate Rotation Curves): a
sample of 175 nearby galaxies with new surface photometry at 3.6 μm and high-quality …

The distribution of the non-luminous matter in galaxies of different luminosity and Hubble
type is much more than a proof of the existence of dark particles governing the structures of …

Astrophysical observations spanning dwarf galaxies to galaxy clusters indicate that dark
matter (DM) halos are less dense in their central regions compared to expectations from …

Ultralight boson fields, with a mass around 10-23 eV, are promising candidates for the
elusive cosmological dark matter. These fields induce a periodic oscillation of the spacetime …

We present a theoretical analysis of some unexplored aspects of relaxed Bose–Einstein
condensate dark matter (BECDM) haloes. This type of ultralight bosonic scalar field dark …

We present barolo,† a new code that derives rotation curves of galaxies from emission-line
observations. This software fits 3D tilted-ring models to spectroscopic data cubes and can be …