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Fig. 2.

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Root-mean-square of nonlinear fluctuations of cosmic matter field as function of the smoothing mass M. The linear fluctuations σL (computed with MGCAMB) are represented by dashed lines, while the solid curves correspond to the σNL, the nonlinear fluctuations of cosmic matter field (computed from the z = 0 snapshots of the DUSTGRAIN-pathfinder simulations). The internal panel contains the corresponding linear and nonlinear power spectra.

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