The Millennium Simulation
The Millennium Simulation Jonnie Pober & Aaron Lee The Main Paper Simulation Specs • Simulated 10 billion particles of mass • Traces the evolution of dark matter
Simulating the joint evolution of quasars, galaxies and their
imation whose fidelity improves as the number of particles in the simulation increases The high-resolution simulation described here – dubbed the Millennium Simulation because of its size – was carried out by the Virgo Consortium, a collaboration of British, German, Canadian, and US astrophysicists
1999: SIMULATION: TECHNOLOGIES IN THE NEW MILLENNIUM
SIMULATION: TECHNOLOGIES IN THE NEW MILLENNIUM Wayne J Davis General Engineering University of Illinois at Urbana-Champaign Urbana, IL 61801, U S A Proceedings of the 1999 Winter Simulation Conference P A Farrington, H B Nembhard, D T Sturrock, and G W Evans, eds ABSTRACT This paper first addresses future simulations needs from a
Chapter 4 Perturbation Theory Reloaded II: Non-linear Bias
4 2 1 Millennium Simulation The Millennium simulation (Springel et al , 2005) is a largeN-body simulation with the box size of (500 Mpc/h)3 and 21603 dark matter particles The cosmological parameters used in the simulation are (Ω dm,Ω b,Ω Λ,h)=(0 205, 0 045, 0 75, 0 73) The primordial power spectrum used in the simulation is the scale
3D-Matched-Filter galaxy cluster finder – I Selection
To this effect, Section 2 of this paper will discuss the Millennium Simulation catalogues used, Section 3 will discuss matched-filter methodology, as well as 3D-MF itself, and Section 4 will outline the selection functions of 3D-MF from the Millennium Simulation data (without and with photometric redshift error) Subsequently,
Forced response of the East Asian summer rainfall over the
millennium simulation of the coupled ECHO-G model The model results indicate that the centennial–millennial vari-ation of the EASM is essentially a forced response to the external radiative forcing (insolation, volcanic aerosol, and green house gases) The strength of the response depends on latitude; and the spatial structure of the
ZOBOV: a parameter-free void-finding algorithm
probabilities that each void or subvoid arises from Poisson fluctuations This paper describes the ZOBOV algorithm, and the results from its application to the dark matter particles in a region of the Millennium simulation Additionally, the paper points out an interesting high-density
Divergent global precipitation changes induced by natural
millennium simulation (Supplementary Information) this ratio is about 2 1 uC 21 during the pre-industrial period ( AD 1000–1850), but only about 1 4 uC 21 during the industrial period ( AD 1850–
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