We review recent developments and results in testing general relativity (GR) at cosmological
scales. The subject has witnessed rapid growth during the last two decades with the aim of …

Long range scalar fields with a coupling to matter appear to violate known bounds on
gravitation in the solar system and the laboratory. This is evaded thanks to screening …

Shortly after its discovery, General Relativity (GR) was applied to predict the behavior of our
Universe on the largest scales, and later became the foundation of modern cosmology. Its …

The Vainshtein mechanism, present in many models of gravity, is very effective at screening
dark matter haloes such that the fifth force is negligible and general relativity is recovered …

We extend the scale-dependent Gaussian Streaming Model (GSM) to produce analytical
predictions for the anisotropic redshift-space correlation function for biased tracers in …

Reliable analytical modeling of the nonlinear power spectrum (PS) of matter perturbations is
among the chief prerequisites for cosmological analyses from the largest sky surveys. This is …

We study the halo mass function (HMF) in modified gravity (MG) models using a set of large
N-body simulations—the elephant suite. We consider two popular beyond-general-relativity …

We extend our previous redshift space power spectrum code to the redshift space
correlation function. Here we focus on the Gaussian Streaming Model (GSM). Again, the …

We present an analytical description of the probability distribution function (PDF) of the
smoothed 3D matter density field for modified gravity and dark energy. Our approach, based …

Aims. We investigate the evolution of the one-point probability distribution function (PDF) of
the dark matter density field and the evolution of its moments for fluctuations that are …