SURFS: Riding the waves with Synthetic UniveRses For Surveys
arXiv:1712.01988 · doi:10.1093/mnras/sty061
Abstract
We present the Synthetic UniveRses For Surveys ({\sc surfs}) simulations, a set of N-body/Hydro simulations of the concordance Cold Dark Matter (\LCDM) cosmology. These simulations use Planck cosmology, contain up to 10 billion particles and sample scales & halo masses down to kpc & . We identify and track haloes from to today using a state-of-the-art 6D halo finder and merger tree builder. We demonstrate that certain properties of halo merger trees are numerically converged for haloes composed of particles. Haloes smoothly grow in mass, , with the mass history characterised by where is the scale factor, \& , with these parameters decreasing with decreasing halo mass. Subhaloes follow power-law cumulative mass and velocity functions, i.e. with and for mass \& velocity respectively, independent of redshift, as seen in previous studies. The halo-to-halo scatter in amplitude is ~dex. The number of subhaloes in a halo weakly correlates with a halo's concentration \& spin :haloes of high \& low have more subhaloes than similar mass haloes of low \& high . High cadence tracking shows subhaloes are dynamic residents, with leaving their host halo momentarily, becoming a backsplash subhalo, and another changing hosts entirely, in agreement with previous studies. In general, subhaloes have elliptical orbits, , with periods of ~Gyrs. Subhaloes lose most of their mass at pericentric passage with mass loss rates of ~Gyr. These catalogues will be made publicly available.
arXiv comment22 pages, 20 figures, accepted for publication in MNRAS
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