Future Evolution of Bound Superclusters in an Accelerating Universe
Pablo A. Araya-Melo, Andreas Reisenegger, Andres Meza, Rien van de, Weygaert, Rolando D\"unner, Hernan Quintana

TL;DR
This study uses cosmological simulations to explore how superclusters evolve in an accelerating universe, showing their spatial distribution stagnates while their internal structures become more spherical and concentrated over time.
Contribution
It provides new insights into the internal evolution of superclusters, including shape, density, and substructure changes, in a LambdaCDM cosmology from present to far future.
Findings
Superclusters' spatial distribution remains stable after the present epoch.
Superclusters become more spherical and concentrated over time.
Substructure within superclusters diminishes as they virialize.
Abstract
The evolution of marginally bound supercluster-like objects in an accelerating LambdaCDM Universe is followed, by means of cosmological simulations, from the present time to an expansion factor a = 100. The objects are identified on the basis of the binding density criterion introduced by Dunner et al. (2006). superclusters are identified with the ones whose mass M > 10^15 M_sun/h, the most massive one with M ~ 8x10^15 M_sun/h, comparable to the Shapley supercluster. The spatial distribution of the superclusters remains essentially the same after the present epoch, reflecting the halting growth of the Cosmic Web as Lambda gets to dominate the expansion of the Universe. The same trend can be seen in the stagnation of the development of the mass function of virialized haloes and bound objects. The situation is considerably different when looking at the internal evolution, quantified in…
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