The Millennium Run - Leiden Observatory
The Millennium Run Project zLargest simulation of cosmic structure growth zSimulates cold dark matter Projects Goals zConclude if current model of galaxy
Carching, December 2012 The Millennium Simulation Programme
Millennium Run 2004 Springel et al 2005 Goal: To carry out a DM- only ΛCDM simulation of a cosmologically relevant volume with sufficient resolution to follow the formation of galaxies in halos and subhalos using Semi-analytic techniques
Exploring the Millennium Run - Scalable Rendering of Large
One of the most popular simulations is the Millennium Run, where more than 10 billion particles have been used to trace the evolution of the matter distribution in a cubic region of the Universe with over 2 billion light-years on a side, resulting in terabytes of stored output The simulation itself ran 28 machine days at 0 2 Tflops using 1
TheSpatialDistributionof SatelliteGalaxies
We use the first Millennium Run simulation (MRS) to investigate the spa-tial locations of the satellites of relatively isolated host galaxies The stellar masses of the MRS hosts span a range of 10 3 6log 10 [M∗/M⊙] 611 5, and host-satellite systems were selected via typical redshift space proximity crite-ria
arXiv:astro-ph/0611641 v1 20 Nov 2006
2 THE SIMULATION 2 1 Simulation Details We make use of the z = 0 halo catalogue obtained from the Millennium Run, a very large dark–matter–only N– body simulation of the concordance ΛCDM cosmology with 21603 particles in a (periodic) box of size 500h−1 Mpc in each dimension The cosmological parameters are total mat-
The Millennium-XXL Project: Simulating the Galaxy Population
Millennium Run (MR), performed by our Virgo Consortium group in 2004 [3] This simulation was the first, and for many years the only run with more than 1010 particles, exceeding the size of previous simulations by almost an order of magnitude Its success was not only computational but most im-portantly scientific – more than 300
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The Millennium Run
Marinus Israel - Nienke van der Marel
December 2nd 2005
OverviewThe Millennium Run Project
Project Goals
Method and initial parameters
Results
Quasar descendants
Two-point correlation function
Baryonic oscillations
Summary
The Millennium Run ProjectLargest simulation of cosmic structure growthSimulates cold
dark matterProjects GoalsConclude if current model of galaxy
formation is consistent with surveys.Explore the physics which give rise to
galaxies.Z = 18.3, t=0.21Gy
Z = 5.7, t=1.0Gy
Z = 1.4, t=4.7Gy
Z = 0, t=13.6Gy
Methods and initial parameters10billionparticles
860 Mper particle