We review the field of collisionless numerical simulations for the large-scale structure of the
Universe. We start by providing the main set of equations solved by these simulations and …

We present a detailed study of the methodology for correlatingdark sirens'(compact binaries
coalescences without electromagnetic counterpart) with galaxy catalogs. We propose …

We constrain the matter density Ωm and the amplitude of density fluctuations σ8 within the
ΛCDM cosmological model with shear peak statistics and angular convergence power …

We analyse the IllustrisTNG simulations to study the mass, volume fraction, and phase
distribution of gaseous baryons embedded in the knots, filaments, sheets, and voids of the …

Dark matter in the universe evolves through gravity to form a complex network of halos,
filaments, sheets and voids, that is known as the cosmic web. Computational models of the …

This is a golden age for galaxy formation: Existing and especially new telescopes are
providing observations that challenge and illuminate rapidly improving theory and …

Galaxy clusters grow by accreting galaxies from the field and along filaments of the cosmic
web. As galaxies are accreted they are affected by their local environment before they enter …

Although structures in the Universe form on a wide variety of scales, from small dwarf
galaxies to large super clusters, the generation of angular momentum across these scales is …

We investigate the alignment of galaxies and haloes relative to cosmic web filaments using
the EAGLE hydrodynamical simulation. We identify filaments by applying the nexus+ method …

We present the first detection of mass-dependent galactic spin alignments with local cosmic
filaments with> 2σ confidence using IFS kinematics. The 3D network of cosmic filaments is …