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A comparison of simulated and analytic major merger counts
Authors:JD Cohn  JS Bagla  Martin White
Institution:1Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA;2Mehta Research Institute, Chhatnag Road, Jhusi, Allahabad 211019, India
Abstract:We use large volume, high resolution, N -body simulations of three different ΛCDM models, with different clustering strengths, to generate dark-matter halo merging histories. Over the reliable range of halo masses, roughly galaxy groups to rich clusters of galaxies, we quantify the number density of major mergers for two different time intervals and compare them with analytic predictions based on the extended Press–Schechter theory.
Keywords:methods: numerical  cosmology: theory  dark matter
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