Mass density vs. energy density at cosmological scales

Abstract

In the presence of the gravitational field, the energy density of matter no longer coincides with its mass density. A discrepancy exists, of course, also between the associated power spectra. Within the Λ CDM model, we derive a formula that relates the power spectrum of the energy density to that of the mass density and test it with the help of N-body simulations run in comoving boxes of 2.816 Gpc/h. The results confirm the validity of the derived formula and simultaneously show that the power spectra diverge significantly from one another at large cosmological scales.

Keywords

• N-body simulations
• Large-scale structure
• Inhomogeneous Universe
• Cosmological perturbations
• Power spectrum
• Cosmic screening