Statistics – Computation
Scientific paper
Nov 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...251..389b&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 251, no. 2, Nov. 1991, p. 389-392. Research supported by DFG.
Statistics
Computation
17
Computational Astrophysics, Dark Matter, Galactic Evolution, Spatial Resolution, Three Dimensional Models, Computerized Simulation, High Resolution, Statistical Analysis
Scientific paper
The generation of statistically 'fair' samples of the universe requires the simulation of large spatial regions of the order of several hundreds of Megaparsecs in view of the current observational situation. On the other hand, ambitious models for the formation of large-scale structure have to include, at least on a phenomenological level, the physics of the formation of a galaxy and its halo on scales of at most a few hundreds of kiloparsecs. In order to construct a link of large-scale distributions of galaxies to galactic scales, consideration is given to high spatial resolution calculations of semi-analytical models for the formation of large-scale structure, which allows for the realization of this link in 3D.
Bartelmann Matthias
Buchert Thomas
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