Halo model description of the non-linear dark matter power spectrum at k >> 1 Mpc-1
Accurate knowledge of the non-linear dark-matter power spectrum is important for understanding the large-scale structure of the Universe, the statistics of dark-matter haloes and their evolution, and cosmological gravitational lensing. We analytically model the dark-matter power spectrum and its cro...
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
1 July 2010
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| In: |
Arxiv
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| Online Access: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1003.4740
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| Author Notes: | Carlo Giocoli, Matthias Bartelmann, Ravi K. Sheth, Marcello Cacciato |
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