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 …

We present an accurate non-linear matter power spectrum prediction scheme for a variety of
extensions to the standard cosmological paradigm, which uses the tuned halo model …

We demonstrate that the output of a cosmological N-body simulation can, to remarkable
accuracy, be scaled to represent the growth of large-scale structure in a cosmology with …

Cosmology is presently facing the deep mystery of the origin of the observed accelerated
expansion of the Universe. Be it a cosmological constant, a homogeneous scalar field, or a …

We study the spherical collapse model for several dark-energy scenarios using the fully non-
linear differential equation for the evolution of the density contrast within homogeneous …

The universality of the halo mass function is investigated in the context of dark energy
cosmologies. This widely used approximation assumes that the mass function can be …

Several cosmological tensions have emerged in light of recent data, most notably in the
inferences of the parameters H 0 and σ 8. We explore the possibility of alleviating both these …

The anisotropy of clustering in redshift space provides a direct measure of the growth rate of
large-scale structure in the Universe. Future galaxy redshift surveys will make high-precision …

We introduce k-evolution, a relativistic N-body code based on gevolution, which includes
clustering dark energy among its cosmological components. To describe dark energy, we …

This is the third of a series of papers in which we derive simultaneous constraints on
cosmological parameters and X-ray scaling relations using observations of the growth of …