Defect models of cosmic structure in light of the new CMB data
classification
🌌 astro-ph
hep-ph
keywords
cosmicdatadefectmodelsstructurecurrentformationlight
read the original abstract
Defect models of cosmic structure formation have faced a number of difficult challenges over recent years. Yet interestingly, new CMB data does not show strong evidence for secondary oscillations in the anisotropy power. Here I review the current standing of the cosmic defect models of structure formation in light of the current data.
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.