Multi-stream portrait of the Cosmic web

TL;DR

This study investigates the multi-stream environment of dark matter haloes in the cosmic web using N-body simulations, revealing hierarchical structures and stream patterns that define different cosmic regions.

Contribution

It introduces a novel analysis of the dark matter sheet in phase space, providing detailed insights into the hierarchical and stream-based structure of the cosmic web.

Findings

Halos are embedded in filamentary structures at crossings.

Voids are single-stream regions with minimal streams.

Streams around haloes are thin shells close to the halo center.

Abstract

We report the results of the first study of the multi-stream environment of dark matter haloes in cosmological N-body simulations in the LCDM cosmology. The full dynamical state of dark matter can be described as a three-dimensional sub-manifold in six dimensional phase space - the dark matter sheet. In our study we use a Lagrangian sub-manifold x = x(q,t) (where x and q are co-moving Eulerian and Lagrangian coordinates respectively), which is dynamically equivalent to the dark matter sheet but is more convenient for numerical analysis. Our major results can be summarized as follows. At the resolution of the simulation i.e. without additional smoothing, the cosmic web represents a hierarchical structure: each halo is embedded in the filamentary framework of the web predominantly at the filament crossings, and each filament is embedded in the wall like fabric of the web at the wall crossings. Locally, each halo or sub-halo is a peak in the number of streams field. The number of streams in the neighbouring filaments is higher than in the neighbouring walls. The walls are regions where number of streams is equal to three or a few. Voids are uniquely defined by the local condition requiring to be a single-stream flow region. The shells of streams around haloes are quite thin and the closest void region is typically within one and a half FOF radius from the center of the halo.