Clues on void evolution III: Structure and dynamics in void shells

TL;DR

This study investigates the structure and dynamics of void shells in the universe, revealing how void size and environment influence their expansion, velocity smoothness, and deviations from linear theory, highlighting nonlinear effects and scale couplings.

Contribution

It provides a detailed analysis of void shell dynamics, showing how size and environment affect velocity fields and nonlinearities, advancing understanding of void evolution.

Findings

Velocity in expanding voids aligns with linear theory

Larger voids exhibit more laminar flow

Void size influences deviations from linear predictions

Abstract

Inspired on the well known dynamical dichotomy predicted in voids, where some underdense regions expand whereas others collapse due to overdense surrounding regions, we explored the interplay between the void inner dynamics and its large scale environment. The environment is classified depending on its density as in previous works. We analyse the dynamical properties of void-centered spherical shells at different void-centric distances depending on this classification. The above dynamical properties are given by the angular distribution of the radial velocity field, its smoothness, the field dependence on the tracer density and shape, and the field departures from linear theory. We found that the velocity field in expanding voids follows more closely the linear prediction, with a more smooth velocity field. However when using velocity tracers with large densities such deviations increase. Voids with sizes around $18\,h^{-1}\,Mpc$ are in a transition regime between regions with expansion overpredicted and underpredicted from linear theory. We also found that velocity smoothness increases as the void radius, indicating the laminar flow dominates the expansion of larger voids (more than $18\,h^{-1}\,Mpc$). The correlations observed suggest that nonlinear dynamics of the inner regions of voids could be dependent on the evolution of the surrounding structures. These also indicate possible scale couplings between the void inner expansion and the large scale regions where voids are embedded. These results shed some light to the origin of nonlinearities in voids, going beyond the fact that voids just quickly becomes nonlinear as they become emptier.