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 investigate the effect of self-interacting dark matter (SIDM) on the density profiles of V
max≃ 40km s− 1 isolated dwarf dark matter haloes–the scale of relevance for the too big to …

Using high-resolution cosmological hydrodynamical simulations of Milky Way-massed disk
galaxies, we demonstrate that supernovae feedback and tidal stripping lower the central …

We compare the dynamical masses of dwarf galaxies in the Local Group (LG) to those of
haloes in the ELVIS (Exploring the Local Volume in Simulations) suite of Λ cold dark matter …

Using a suite of three large cosmological hydrodynamical simulations, horizon–agn, horizon–
noagn (no AGN feedback) and horizon–dm (no baryons), we investigate how a typical sub …

This paper is based on lectures given at the IX Mexican School on Gravitation and
Mathematical Physics. The lectures (as the paper) were a broad-band review of the current …

This review aims at proposing to the field an overview of the Cusp-core problem, including a
discussion of its advocated solutions, assessing how each can satisfactorily provide a …

The significant diversity of rotation curve (RC) shapes in dwarf galaxies has recently
emerged as a challenge to Λ cold dark matter (ΛCDM): in dark matter (DM) only simulations …

Cold dark matter (CDM) has shown to be an excellent candidate for the dark matter (DM) of
the Universe at large scales; however, it presents some challenges at the galactic level. The …

Short-lived mediators are often used to describe dark matter interactions with Standard
Model particles. When the dark matter mass is heavier than the mass of the mediator, it may …