Statistics – Computation
Scientific paper
May 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.244..214g&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 244, May 15, 1990, p. 214-224.
Statistics
Computation
10
Dark Matter, Density Distribution, Galactic Clusters, Galactic Evolution, Universe, Astronomical Models, Computational Astrophysics, Gravitational Effects, Probability Distribution Functions
Scientific paper
Consideration is given to the evolution of structure in numerical simulations of flat cold dark matter (CDM) universes. A comparison between the distribution of high-density regions and the observed distribution of systems of galaxies in the region extending up to the nearest superclusters. The distribution of galaxies is used to constrain the threshold density level and the amount of the CDM hidden in voids in different models. The connectivity of the structure of superclusters is described and the geometry and sizes of voids are characterized.
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