Fig. 3 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. 3.

Same as Fig. 1, except that the appropriate convolved power spectra are sampled for ﹩L=( 100,\ 200,\ 400,\ 800) \ h^{-1}\ \mathrm{Mpc}\,﹩. As intended, the correlation function matches the ﹩L\rightarrow \infty ﹩ limit for ﹩r< L/ 2﹩ and is 0 for ﹩r> L/ 2﹩.

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