Dark energy domination in the Virgocentric flow
A. D. Chernin, I. D. Karachentsev, O.G. Nasonova, P. Teerikorpi, M. J., Valtonen, V. P. Dolgachev, L. M. Domozhilova, G. G. Byrd

TL;DR
This paper investigates how dark energy influences the dynamics of the Virgo Cluster and its surrounding flow, revealing that dark energy controls the flow structure and may be a universal feature of cosmic systems.
Contribution
It introduces a nonlinear analytical model incorporating dark energy's antigravity effects to explain the Virgo Cluster's flow dynamics, highlighting the universal two-component pattern.
Findings
Dark energy controls the Virgocentric flow structure.
The zero-gravity radius is about 10 times larger than the cluster.
A universal two-component pattern may exist in cosmic groups and clusters.
Abstract
The standard \LambdaCDM cosmological model implies that all celestial bodies are embedded in a perfectly uniform dark energy background, represented by Einstein's cosmological constant, and experience its repulsive antigravity action. Can dark energy have strong dynamical effects on small cosmic scales as well as globally? Continuing our efforts to clarify this question, we focus now on the Virgo Cluster and the flow of expansion around it. We interpret the Hubble diagram, from a new database of velocities and distances of galaxies in the cluster and its environment, using a nonlinear analytical model which incorporates the antigravity force in terms of Newtonian mechanics. The key parameter is the zero-gravity radius, the distance at which gravity and antigravity are in balance. Our conclusions are: 1. The interplay between the gravity of the cluster and the antigravity of the dark…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Galaxies: Formation, Evolution, Phenomena
