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Interaction between dark energy and dark matter is probed through deviationfrom the virial equilibrium for two relaxed clusters: A586 and A1689. Theevaluation of the virial equilibrium is performed using realistic densityprofiles. The virial ratios found for the more realistic density profiles areconsistent with the absence of interaction.

general relativity and gravitation

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