Resolving Cosmic Structure Formation with the Millennium-II
We present the Millennium-II Simulation (MS-II), a very large N-body simulation of dark matter evolution in the concordance CDM cosmology The MS-II assumes the same cosmological parameters and uses the same particle number and output data structure as the original Millennium Simulation (MS), but was carried out in
There’s no place like home? The Milky Way in cosmological context
Millennium-II Simulation (MB-K, Springel, White, Jenkins, & Lemson 2009): Same N p ─ 21603=10 1 billion ─ as Millennium Run in smaller volume go to length scales 5x smaller, mass scales 125x smaller Thousands of MW halos with 㸠10 resolved subhalos of V max > 30 km/s
The Handwaver’s Guide to Dark Matter Halos
Millennium-II Simulation (Boylan-Kolchin et al 2009) halos are: 1 collapsed 2 self-bound 3 virialized The basic building-blocks of large-scale structure: • home to all galaxies, quasars, stars, etc
MODELING THE REDSHIFT EVOLUTION OF THE NORMAL GALAXY X-RAY
simulation tools, StarTrack and The Millennium Simulation II, and the methodology we follow in developing our models of XRB populations in galaxies Section 3 describes how we compare our models to observational results, namely those of T&G08, and the statistical analysis we use to determine our best models
N-body Merger Trees and Halo Properties - ResearchGate
The Millennium-II (MSII) simulation1 (Boylan-Kolchin et al 2009) was carried out with the gadget3 N-body code, which uses a \TreePM" method to calculate gravitational forces The MSII is a
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