Going Nonlinear with Dark Energy Cosmologies
classification
🌌 astro-ph
keywords
cosmologiesdarkenergynonlinearpoweraccuracyanisotropyautomatically
read the original 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''.
This paper has not been read by Pith yet.
Forward citations
Cited by 1 Pith paper
-
Extended Dark Energy analysis using DESI DR2 BAO measurements
Extended analysis of DESI DR2 data confirms robust evidence for dynamical dark energy with phantom crossing preference, stable under parametric and non-parametric modeling.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.