http://arxiv.org/abs/1503.04650
We propose a new method of calculating a dark matter halo mass function based on the rescaling of a mass function measured in simulations. Our tests show that the accuracy almost linearly depends on the difference of the cosmological parameters and amounts to few percent in the case of WMAP5 and PLANCK parameters.
V. Yankelevich and S. Pilipenko
Tue, 17 Mar 15
9/79
Comments: 5 pages, 7 figures, submitted to MNRAS
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