Fig. 5 from Initial Conditions to Cosmological N‐Body Simulations, or, How to Run an Ensemble of Simulations

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Initial Conditions to Cosmological N‐Body Simulations, or, How to Run an Ensemble of Simulations

Authors: Edwin Sirko

Sirko 2005 The Astrophysical Journal 634 728.

Provider: AAS Journals

Caption: Fig. 5.

Value of σ_8,lattice as a function of R/Δx, where the mean interparticle separation ﹩\Delta x=L/ N^{1/ 3}﹩ and the radius of the spherical top hat is ﹩R=8\ h^{-1}\ \mathrm{Mpc}\,﹩. Values are accurate to 1%.

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