Testing the interaction of dark energy to dark matter through the analysis of virial relaxation of clusters Abell Clusters A586 and A1689 using realistic density profiles
classification
🌌 astro-ph.CO
gr-qchep-th
keywords
darkvirialclustersdensityinteractionprofilesrealistica1689
pith:J4PSVCHQ Add to your LaTeX paper
What is a Pith Number?\usepackage{pith}
\pithnumber{J4PSVCHQ}
Prints a linked pith:J4PSVCHQ badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more
read the original abstract
Interaction between dark energy and dark matter is probed through deviation from the virial equilibrium for two relaxed clusters: A586 and A1689. The evaluation of the virial equilibrium is performed using realistic density profiles. The virial ratios found for the more realistic density profiles are consistent with the absence of interaction.
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.