The universal nature of subhalo accretion

TL;DR

This paper demonstrates that the infall pattern of subhaloes onto host haloes is universally aligned with the weakest axis of the shear tensor, linking local structure formation to the large-scale cosmic web.

Contribution

It reveals that subhalo infall directions are universally governed by the shear tensor, connecting small-scale accretion patterns to large-scale cosmic web structures.

Findings

Subhaloes preferentially accrete along the shear tensor's principal axis.

The infall pattern is consistent across different masses and redshifts.

This universal alignment links local accretion to the large-scale structure.

Abstract

We examine the angular infall pattern of subhaloes onto host haloes in the context of the large-scale structure. We find that this infall pattern is essentially driven by the shear tensor of the ambient velocity field. Dark matter subhaloes are found to be preferentially accreted along the principal axis of the shear tensor which corresponds to the direction of weakest collapse. We examine the dependence of this preferential infall on subhalo mass, host halo mass and redshift. Although strongest for the most massive hosts and the most massive subhaloes at high redshift, the preferential infall of subhaloes is effectively universal in the sense that its always aligned with the axis of weakest collapse of the velocity shear tensor. It is the same shear tensor that dictates the structure of the cosmic web and hence the shear field emerges as the key factor that governs the local anisotropic pattern of structure formation. Since the small (sub-Mpc) scale is strongly correlated with the mid-range (~10 Mpc) scale - a scale accessible by current surveys of peculiar velocities - it follows that findings presented here open a new window into the relation between the observed large scale structure unveiled by current surveys of peculiar velocities and the preferential infall direction of the Local Group. This may shed light on the unexpected alignments of dwarf galaxies seen in the Local Group