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The next generation mass probes will investigate DE nature by measuringnon-linear power spectra at various z, and comparing them with high precisionsimulations. Producing a complete set of them, taking into account baryonphysics and for any DE state equation w(z), would really be numericallyexpensive. Regularities reducing such duty are essential. This paper presentsfurther n-body tests of a relation we found, linking models with DE stateparameter w(z) to const.-w models, and also tests the relation in hydrosimulations.

High precision spectra at large redshift for dynamical DE cosmologies