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Fig. 3

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The nonlinear power per logarithmic interval of wavenumber, Δ2(k), as a function of the linear power , at the Lagrangian wavenumber kL defined by Eq. (47). The lower curves are obtained from the Zeldovich power spectrum (13), while the upper curves correspond to the power spectrum (41) of our “sticky model”. The solid lines are for the redshift z = 0 and the dashed lines for z = 2.

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