Dark Energy: Is it Q or Lambda ?
classification
🌌 astro-ph
keywords
darkenergyanisotropiesbackgroundclusteringconstraintscosmicdistances
read the original abstract
New observations of Cosmic Microwave Background Anisotropies, Supernovae luminosity distances and Galaxy Clustering are sharpening our knowledge about dark energy. Here we present the latest constraints.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.