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
β¦ LIBER β¦
Simulations of structure formation in interacting dark energy cosmologies
β Scribed by M. Baldi
- Publisher
- Elsevier Science
- Year
- 2009
- Tongue
- English
- Weight
- 316 KB
- Volume
- 194
- Category
- Article
- ISSN
- 0920-5632
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