Evolution of dark-matter haloes in a variety of dark-energy cosmologies
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...
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| Main Authors: | , |
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| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
26 Apr 2004
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| In: |
Arxiv
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| Online Access: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/astro-ph/0404489
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| Author Notes: | Matthias Bartelmann, Klaus Dolag, Francesca Perrotta, Carlo Baccigalupi, Lauro Moscardini, Massimo Meneghetti, Guiseppe Tormen |
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Evolution of dark-matter haloes in a variety of dark-energy cosmologies
Article (Journal)
Online Resource