Dependence of the non-linear mass power spectrum on the equationof state of dark energy

Abstract

We present N-body simulation calculations of the dependence of the power spectrum of non-linear cosmological mass density fluctuations on the equation of state of the dark energy, . At fixed linear theory power, increasing w leads to an increase in non-linear power, with the effect increasing with k. By , a model with has ∼12 per cent more power than a standard cosmological constant model , while a model with has ∼33 per cent extra power (at ). The size of the effect increases with increasing dark energy fraction, and to a lesser extent increasing power spectrum normalization, but is insensitive to the power spectrum shape (the numbers above are for and ). A code quantifying the non-linear effect of varying w, as a function of k, z and other cosmological parameters, which should be accurate to a few per cent for for models that fit the current observations, is available at . This paper also serves as an example of a detailed exploration of the numerical convergence properties of ratios of power spectra for different models, which can be useful because some kinds of numerical error cancel in a ratio. When precision calculations based on numerical simulations are needed for many different models, efficiency may be gained by breaking the problem into a calculation of the absolute prediction at a central point, and calculations of the relative change in the prediction with model parameters. © 2005 RAS.