Going Nonlinear with Dark Energy Cosmologies
arXiv:astro-ph/0508401 · doi:10.1103/PhysRevD.72.061304
Abstract
We propose an efficient method for generating high accuracy (~1%) nonlinear power spectra for grids of dark energy cosmologies. Our prescription for matching matter growth automatically matches the main features of the cosmic microwave background anisotropy power spectrum, thus naturally including ``CMB priors''.
3 pages, 1 figure