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Evolution of the dark matter halo in numerical models

✍ Scribed by S. V. Pilipenkoa; A. G. Doroshkevich


Book ID
111505439
Publisher
Allerton Press, Inc.
Year
2010
Tongue
English
Weight
317 KB
Volume
37
Category
Article
ISSN
1068-3356

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High resolution, numerical simulations of 17 cluster-sized dark-matter haloes in eight different cosmologies with and without dynamical dark-energy confirm the picture that core halo densities are imprinted early during their formation by the mean cosmological density. Quite independent of cosmology