Abstract:Abstract. We explore the possibility of putting constraints on dark energy models with statistical property of large scale structure in the non-linear region. In particular, we investigate the w dependence of non-Gaussianity of the smoothed density distribution generated by the nonlinear dynamics. In order to follow the non-linear evolution of the density fluctuations, we apply N-body simulations based on P 3 M scheme. We show that the relative difference between non-Gaussianity of w = −0.8 model and that of w… Show more
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