TL;DR
This paper presents an analytical model explaining the universal distributions of subhaloes within dark matter haloes, accounting for tidal stripping effects and predicting various subhalo-related profiles.
Contribution
The model offers a unified, physically motivated explanation for subhalo distributions and their properties, improving understanding over previous empirical approaches.
Findings
The spatial distribution of subhaloes mirrors the host halo's mass distribution.
Tidal stripping explains the reduction in subhalo mass with decreasing radius.
The model accurately predicts the subhalo mass function and related profiles.
Abstract
N-body simulations suggest that the substructures that survive inside dark matter haloes follow universal distributions in mass and radial number density. We demonstrate that a simple analytical model can explain these subhalo distributions as resulting from tidal stripping which increasingly reduces the mass of subhaloes with decreasing halo-centric distance. As a starting point, the spatial distribution of subhaloes of any given infall mass is shown to be largely indistinguishable from the overall mass distribution of the host halo. Using a physically motivated statistical description of the amount of mass stripped from individual subhaloes, the model fully describes the joint distribution of subhaloes in final mass, infall mass and radius. As a result, it can be used to predict several derived distributions involving combinations of these quantities including, but not limited to, the…
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