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- W3106412318 abstract "We present an analysis of some of the properties of the density field realized in numerical simulations for power-law initial power spectra in the case of a critical density universe. We study the non-linear regime, which is the most difficult to handle analytically, and we compare our numerical results with the predictions of a specific hierarchical clustering scaling model that have been made recently, focusing specifically on its much wider range of applicability, which is one of its main advantages over the standard Press—Schechter approximation. We first check that the two-point correlation functions, measured from both counts-in-cells and neighbour counts, agree with the known analytically exact scaling requirement (i.e., depend only on σ2), and we also find the stable-clustering hypothesis to hold. Next, we show that the statistics of the counts-in-cells obey the scaling law predicted by the above scaling model." @default.
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- W3106412318 date "2000-01-15" @default.
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- W3106412318 title "Scaling laws in gravitational clustering for counts-in-cells and mass functions" @default.
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- W3106412318 doi "https://doi.org/10.1046/j.1365-8711.2000.03054.x" @default.
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