Halo Models of Large Scale Structure and Reliability of Cosmological N-Body Simulations
Halo models of the large scale structure of the Universe are critically examined, focusing on the definition of halos as smooth distributions of cold dark matter. This definition is essentially based on the results of cosmological N-body simulations. By a careful analysis of the standard assumptions...
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| Format: | Article |
| Language: | English |
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MDPI AG
2013-05-01
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| Series: | Galaxies |
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| Online Access: | http://www.mdpi.com/2075-4434/1/1/31 |