The Effect of Large-Scale Power on Very-Small-Scale Structure in CDM Simulations

Statistics – Computation

Scientific paper

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Scientific paper

There is a growing interest in small-scale dark-matter structures. Some theories have proposed that substructure exists down to Earth masses. Such objects might produce features in the energy spectra measured by both direct and indirect dark-matter detection experiments. The study of very-small-scale structure in the CDM-dominated Universe presents a special challenge for computational cosmology. We present the results from a series of numerical experiments designed to quantify any effects due to large-scale density fluctuations that might hinder or aid the formation of structure. Preliminary results that suggest the inclusion of large-scale power enhances the formation of large-scale structures while removing small-scale substructure.

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