Non-linear evolution of cosmological structures in warm dark matter models

Schneider, Aurel, Smith, Robert E, Macciò, Andrea V and Moore, Ben (2012) Non-linear evolution of cosmological structures in warm dark matter models. Monthly Notices of the Royal Astronomical Society, 424 (1). pp. 684-698. ISSN 0035-8711

PDF - Published Version
Download (5MB) | Preview


The dark energy dominated warm dark matter (WDM) model is a promising alternative cosmological scenario. We explore large-scale structure formation in this paradigm. We do this in two different ways: with the halo model approach and with the help of an ensemble of high-resolution N-body simulations. Combining these quasi-independent approaches leads to a physical understanding of the important processes which shape the formation of structures. We take a detailed look at the halo mass function, the concentrations and the linear halo bias of WDM. In all cases we find interesting deviations with respect to cold dark matter (CDM). In particular, the concentration-mass relation displays a turnover for group scale dark matter haloes, for the case of WDM particles with masses of the order of mWDM˜ 0.25 keV. This may be interpreted as a hint for top-down structure formation on small scales. We implement our results into the halo model and find much better agreement with simulations. On small scales, the WDM halo model now performs as well as its CDM counterpart.

Item Type: Article
Schools and Departments: School of Mathematical and Physical Sciences > Physics and Astronomy
Subjects: Q Science > QB Astronomy
Depositing User: Robert Smith
Date Deposited: 18 Sep 2013 12:31
Last Modified: 02 Jul 2019 21:21

View download statistics for this item

📧 Request an update