Over recent decades, cosmological simulations of galaxy formation have been instrumental
in advancing our understanding of structure and galaxy formation in the Universe. These …

We present a comprehensive review of keV-scale sterile neutrino Dark Matter, collecting
views and insights from all disciplines involved—cosmology, astrophysics, nuclear, and …

We introduce the Uchuu suite of large high-resolution cosmological N-body simulations. The
largest simulation, named Uchuu, consists of 2.1 trillion (12 8003) dark matter particles in a …

ABSTRACT A new upper limit on the 21 cm signal power spectrum at a redshift of z≈ 9.1 is
presented, based on 141 h of data obtained with the Low-Frequency Array (LOFAR). The …

We consider the possibility that the black-hole (BH) binary detected by LIGO may be a
signature of dark matter. Interestingly enough, there remains a window for masses 20 M⊙≲ …

This paper introduces C olossus, a public, open-source python package for calculations
related to cosmology, the large-scale structure (LSS) of matter in the universe, and the …

Primordial black holes (PBHs) have long been a candidate for the elusive dark matter (DM),
and remain poorly constrained in the∼ 20–100 M⊙ mass range. PBH binaries were …

Predicting structural properties of dark matter haloes is one of the fundamental goals of
modern cosmology. We use the suite of MultiDark cosmological simulations to study the …

Astrophysical observations spanning dwarf galaxies to galaxy clusters indicate that dark
matter (DM) halos are less dense in their central regions compared to expectations from …

We have updated the Munich galaxy formation model to the Planck first-year cosmology,
while modifying the treatment of baryonic processes to reproduce recent data on the …