Abstract
Current cosmological data have confirmed the big bang and dark matter hypothesies, and indicate that our universe contains a substantial component of dark vacuum energy that is driving the cosmos to accelerate. We examine the immediate and long-term consequences of this dark energy on large scale structures formed in the universe. Using spherical model solutions and realistic 3D clustering simulations, we present criteria for test bodies to remain bound to existing structures. We show that collapsed halos become spatially isolated and dynamically relax to a particular kinematic profile. From this state, the asymptotic form of the space-time metric is well specified.
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