Statistics of peaks in cosmological nonlinear density fields

Details Statistics of peaks in cosmological nonlinear density fields Statistics of peaks in cosmological nonlinear density fields

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990stin...9119990s&link_type=abstract

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Mathematics

Computerized Simulation, Cosmology, Galactic Evolution, Many Body Problem, Mathematical Models, Nonlinearity, Statistical Distributions, Universe, Abundance, Bias, Galactic Clusters, Space-Time Functions

Scientific paper

Distribution of the high-density peaks in the universe is examined using N-body simulations. Nonlinear evolution of the underlying density field significantly changes the statistical properties of the peaks, compared with the analytic results valid for the random Gaussian field. In particular, the abundances and correlations of the initial density peaks are discussed in the context of biased galaxy formation theory.

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