NONLINEAR EVOLUTION OF DARK MATTER SUBHALOS AND APPLICATIONS TO WARM DARK MATTER

被引：51

作者：

Pullen, Anthony R. ^{[1
]}

Benson, Andrew J. ^{[2
]}

Moustakas, Leonidas A. ^{[1
]}

机构：

[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

[2] Carnegie Observ, Pasadena, CA 91101 USA

来源：

ASTROPHYSICAL JOURNAL | 2014年 / 792卷 / 01期

基金：

美国国家航空航天局;

关键词：

cosmology: theory; dark matter; galaxies: formation; galaxies: halos; GALAXY FORMATION; SATELLITE GALAXIES; MASS SUBSTRUCTURE; TOO BIG; MILKY; DENSITY; HALOES; CONSTRAINTS; CORES; MODEL;

D O I：

10.1088/0004-637X/792/1/24

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We describe the methodology to include nonlinear evolution, including tidal effects, in the computation of subhalo distribution properties in both cold (CDM) and warm (WDM) dark matter universes. Using semi-analytic modeling, we include effects from dynamical friction, tidal stripping, and tidal heating, allowing us to dynamically evolve the subhalo distribution. We calibrate our nonlinear evolution scheme to the CDM subhalo mass function in the Aquarius N-body simulation, producing a subhalo mass function within the range of simulations. We find tidal effects to be the dominant mechanism of nonlinear evolution in the subhalo population. Finally, we compute the subhalo mass function for m(chi) = 1.5 keV WDM including the effects of nonlinear evolution, and compare radial number densities and mass density profiles of subhalos in CDM and WDM models. We show that all three signatures differ between the two dark matter models, suggesting that probes of substructure may be able to differentiate between them.

引用

页数：9

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