The sparkling Universe: the coherent motions of cosmic voids
Diego G. Lambas, Marcelo Lares, Laura Ceccarelli, Andr\'es N. Ruiz,, Dante J. Paz, Victoria E. Maldonado, Heliana E. Luparello

TL;DR
This paper investigates the coherent motions of cosmic voids, revealing a bimodal velocity distribution linked to their large-scale environment, supported by simulations and SDSS-DR7 data, suggesting a dynamic, 'sparkling' universe.
Contribution
It provides the first detailed analysis of void bulk motions, demonstrating environment-dependent bimodal velocity distributions and coherence over large scales.
Findings
Void motions are around 300-400 km/s, similar to galaxy clusters.
Void pairs show a bimodal velocity distribution with approaching and receding motions.
Environmental classification explains the velocity bimodality.
Abstract
We compute the bulk motions of cosmic voids, using a CDM numerical simulation considering the mean velocities of the dark matter inside the void itself and that of the haloes in the surrounding shell. We find coincident values of these two measures in the range 300-400 km/s, not far from the expected mean peculiar velocities of groups and galaxy clusters. When analysing the distribution of the pairwise relative velocities of voids, we find a remarkable bimodal behaviour consistent with an excess of both systematically approaching and receding voids. We determine that the origin of this bimodality resides in the void large scale environment, since once voids are classified into void-in-void (R-type) or void-in-cloud (S-type), R-types are found mutually receding away, while S-types approach each other. The magnitude of these systematic relative velocities account for more…
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