Dark energy and key physical parameters of clusters of galaxies

Abstract

We study physics of clusters of galaxies embedded in the cosmic dark energy background. Under the assumption that dark energy is described by the cosmological constant, we show that the dynamical effects of dark energy are strong in clusters like the Virgo cluster. Specifically, the key physical parameters of the dark mater halos in clusters are determined by dark energy: 1) the halo cut-off radius is practically, if not exactly, equal to the zero-gravity radius at which the dark matter gravity is balanced by the dark energy antigravity; 2) the halo averaged density is equal to two densities of dark energy; 3) the halo edge (cut-off) density is the dark energy density with a numerical factor of the unity order slightly depending on the halo profile. The cluster gravitational potential well in which the particles of the dark halo (as well as galaxies and intracluster plasma) move is strongly affected by dark energy: the maximum of the potential is located at the zero-gravity radius of the cluster.

8 pages, 1 figure

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• Remarks on mechanical approach to observable Universe
• Hydrodynamical simulations of coupled and uncoupled quintessence models II: Galaxy clusters
• Galaxy cluster hydrostatic masses using Tolman-Oppenheimer-Volkoff equation
• Galactic cluster winds in presence of a dark energy
• Galaxy clusters in presence of dark energy: a kinetic approach
• Galaxy cluster hydrostatic bias in Kottler spacetime
• The effects of a non-zero cosmological constant on the Veltmann models