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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. 10.

Power spectra for the ﹩L=100\ h^{-1}\ \mathrm{Mpc}\,﹩, ﹩N=64^{3}﹩ ensembles with P‐sampled ICs (left) and ξ‐sampled ICs (right) for five output auni values, as labeled. The black line, purple region, light green region, and red line have the same meanings as in Fig. 9. On the right side of each panel is a green line marking the expected Poisson noise contribution to the power spectrum, V/N.

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