Dark Energy and Non-linear Perturbations
classification
🌌 astro-ph
keywords
darkenergyinfluencecollapsemattermightwillcosmic
pith:RRNDVLZK Add to your LaTeX paper
What is a Pith Number?\usepackage{pith}
\pithnumber{RRNDVLZK}
Prints a linked pith:RRNDVLZK badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more
read the original abstract
Dark energy might have an influence on the formation of non--linear structures during the cosmic history. For example, in models in which dark energy couples to dark matter, it will be non--homogeneous and will influence the collapse of a dark matter overdensity. We use the spherical collapse model to estimate how much influence dark energy might have.
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.