Collision-driven emergence of the cosmic web

TL;DR

This paper proposes a collision-driven model for the emergence of the cosmic web, suggesting that inelastic collisions could have initiated large-scale structures prior to gravitational effects, addressing mass estimation issues.

Contribution

It introduces a first-principles, multi-scale model showing how inelastic collisions can drive cosmic web formation before gravity becomes dominant.

Findings

Diffusion rate in the particulate gas is sub-anomalous.

Gas density is unstable, leading to voids and clusters.

Clusters tend to elongate and grow into filaments.

Abstract

Gravitational-collapse-based explanations of the cosmic web lead to problems in estimating the total mass in the universe. A first-principles several-scales model is developed here for the structural organisation of cosmic matter in a flat universe, showing that the web formation could be driven by inelastic collisions before gravity took hold, suggesting a possible way to resolve these problems. The following results are derived. (i) The diffusion rate in the particulate gas after recombination is sub-anomalous, with a rapid decay of particle velocities. (ii) The evolution of the particle velocity distribution is calculated explicitly. (iii) The gas density is shown to be unstable, leading to void formation and clusters nucleation. (iv) Rounded clusters are shown to be unstable and tend to elongate. (v) An equation is derived for the growth of long clusters into filaments and solved explicitly. The fast-growing clusters deplete the regions around them and generate large voids, potentially giving rise to the cosmic web before gravity dominated.