Redshift dependence of clustering in numerical simulations.

Details Redshift dependence of clustering in numerical simulations. Redshift dependence of clustering in numerical simulations.

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apl%26c..36..143m&link_type=abstract

Astrophysical Letters and Communications, Vol. 36, Nos. 1 - 6, p. 143 - 148

Mathematics

Logic

Cosmological Models: Galaxy Clustering, Cosmology: Galaxy Formation, Galaxy Clustering: N-Body Simulations

Scientific paper

High resolution N-body simulations for variants of the CDM model are used to derive the redshift dependence of galaxy formation and of galaxy correlation functions. The reconstructed power spectra and clustering properties provide a sensible test for the underlying power spectra. The author compares his simulations with new results of the analysis of the Las Campanas Redshift survey. The results are used to discuss the model of primordially broken scale invariant perturbations.

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