We present a review of the current state of the art of cosmological dark matter simulations,
with particular emphasis on the implications for dark matter detection efforts and studies of …

The cosmological principle (CP)—the notion that the Universe is spatially isotropic and
homogeneous on large scales—underlies a century of progress in cosmology. It is …

We present the full public release of all data from the Illustris simulation project. Illustris is a
suite of large volume, cosmological hydrodynamical simulations run with the moving-mesh …

This paper describes a new publicly available codebase for modeling galaxy formation in a
cosmological context, the" Semi-Analytic Galaxy Evolution" model, or sage for short. 5 sage …

We present a very large high-resolution cosmological N-body simulation, the Millennium-
XXL or MXXL, which uses 303 billion particles to represent the formation of dark matter …

We use time-sliced perturbation theory (TSPT) to give an accurate description of the infrared
non-linear effects affecting the baryonic acoustic oscillations (BAO) present in the …

We present a new N-body simulation from the Marenostrum Institut de Ciències de l'Espai
(MICE) collaboration, the MICE Grand Challenge (MICE-GC), containing about 70 billion …

The quantity and quality of cosmic structure observations have greatly accelerated in recent
years, and further leaps forward will be facilitated by imminent projects. These will enable us …

This chapter is a non-expert introduction to the effective field theory of large-scale structure.
First, we give a detailed pedagogical explanation of why previous attempts to build non …

We obtain constraints on cosmological parameters from the spherically averaged redshift-
space correlation function of the CMASS Data Release 9 (DR9) sample of the Baryonic …