Fig. 2.

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Cosmic density and displacement field components as obtained with different methods. Upper panels: log-density slices at redshift z = 0 (log(1 + δ)) corresponding to different gravity solvers through the three-dimensional simulation cubical box of 200 h−1 Mpc side length with a mesh of 2563 cells. Lower panels: Same as the upper panels but for the divergence of the irrotational (∇q ⋅ Ψ∇ × Ψ = 0(q)) and the absolute value of the solenoidal component of the displacement field, |Ψ∇ ⋅ Ψ = 0(q)| (with power spectra within percentage agreement up to k ≃ 0.4 h Mpc−1). The resulting maps have been saturated to the same colour scale after averaging over five slices corresponding to one simulation.
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