Halo abundances and shear in void models
We study the non-linear gravitational collapse of dark matter into halos through numerical N-body simulations of Lemaître–Tolman–Bondi void models. We extend the halo mass function formalism to these models in a consistent way. This extension not only compares well with the simulated data at all tim...
| Main Authors: | , , , |
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| Formato: | Journal article |
| Publicado em: |
Elsevier
2012
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