Fig. 4 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. 4.

Power in the DC mode vs. box size L (top) and its dimensionless version, the characteristic dimensionless overdensity corresponding to P_L(0) (bottom). I used the CMBFAST power spectrum normalized to ﹩\sigma _{8}=0.84﹩.

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