Substructure of fuzzy dark matter haloes

被引：74

作者：

Du, Xiaolong ^{[1
]}

Behrens, Christoph ^{[1
]}

Niemeyer, Jens C. ^{[1
]}

机构：

[1] Georg August Univ Goettingen, Inst Astrophys, Friedrich Hund Pl 1, D-37075 Gottingen, Germany

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2017年 / 465卷 / 01期

关键词：

elementary particles; cosmology: theory; dark matter; NONLINEAR EVOLUTION; LAMBDA-CDM; GALAXIES; MODEL; CLUSTERS;

D O I：

10.1093/mnras/stw2724

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We derive the halo mass function (HMF) for fuzzy dark matter (FDM) by solving the excursion set problem explicitly with a mass-dependent barrier function, which has not been done before. We find that compared to the naive approach of the Sheth-TormenHMFfor FDM, our approach has a higher cutoffmass and the cutoffmass changes less strongly with redshifts. Usingmerger trees constructed with a modified version of the Lacey & Cole formalism that accounts for suppressed small-scale power and the scale-dependent growth of FDM haloes and the semianalytic GALACTICUS code, we study the statistics of halo substructure including the effects from dynamical friction and tidal stripping. We find that if the dark matter is a mixture of cold dark matter (CDM) and FDM, there will be a suppression on the halo substructure on small scales which may be able to solve the missing satellites problem faced by the pure CDM model. The suppression becomes stronger with increasing FDM fraction or decreasing FDM mass. Thus, it may be used to constrain the FDM model.

引用

页码：941 / 951

页数：11

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