Anatoly Klypin

TL;DR: In this paper, the authors apply several statistical estimators to high-resolution N-body simulations of two currently viable cosmological models: a mixed dark matter model, having?? = 02 contributed by two massive neutrinos (C + 2?DM), and a cold-dark matter model with Cosmological constant (?CDM) with?0 = 03 and h = 07.

TL;DR: In this paper, the authors used the rotation curves of a sample of dark matter dominated dwarf and low surface brightness (LSB) late-type galaxies to study their radial mass distributions, and they found that the shape of the rotation curve is remarkably similar for all (both dwarf and LSB) galaxies in the sample, suggesting a self-similar density distribution of their dark matter (DM) halos.

TL;DR: FZ acknowledges the support by the Netherlands Organization for Scientific Research (NWO) through a Veni grant assigned to Shin'ichiro Ando and FZ acknowledge the support from the Spanish MINECO grant AYA2014-606Y1-C2-1P.

TL;DR: In this article, high-resolution PM N-body simulations were used to follow the development of non-linear clustering in a flat universe, dominated by cold + hot dark matter (CHDM) with 60% of CDM, 30% of HDM, and 10% of baryons; a simulation box of 100 Mpc a side ($h=05$) was used.

TL;DR: In this paper, the GLAM simulations have been performed on the MareNostrum4 supercomputer at the Barcelona Supercomputer Center in Spain and the authors acknowledge support from the State Agency for Research of the Spanish MCIU through the grant AYA2014-60641-C2-1-P.