The DOI matches its Crossref record; 77 of the 77 references it cites were found in a registry or an index.
Non-linear evolution of cosmological structures in warm dark matter models: Non-linear structure formation in WDM models
Open accessAbstract
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.
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Cites
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Cited by
Small-Scale Challenges to the ΛCDM Paradigm
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Metadata
- Authors
- Schneider, A., Smith, R. E., Macciò, A. V., & Moore, B.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2012-06-12
- Volume
- 424
- Issue
- 1
- Pages
- 684-698
- ISSN
- 0035-8711 (ISSN-L)
- OpenAlex
- W1906243226
- Cited by
- 281
- References
- 77
- FWCI
- 9.66
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Schneider, A., Smith, R. E., Macciò, A. V., & Moore, B. (2012). Non-linear evolution of cosmological structures in warm dark matter models: Non-linear structure formation in WDM models. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1111/j.1365-2966.2012.21252.x
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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