On the connectivity of the cosmic web: theory and implications for cosmology and galaxy formation
Sandrine Codis, Dmitri Pogosyan, Christophe Pichon

TL;DR
This paper explores the structure and connectivity of the cosmic web using topological tools, revealing how nodes connect and how this relates to cosmology and galaxy formation.
Contribution
It introduces a novel analysis of cosmic web connectivity via the persistent skeleton, linking topological features to cosmological parameters and galaxy assembly.
Findings
Nodes connect to 4 neighbors in 2D and ~6.1 in 3D on average.
Connectivity scales with dimension as a power 7/4, depending on peak height.
Connectivity decreases with redshift and scale, and scales with halo mass as 10/3 times log of mass.
Abstract
Cosmic connectivity and multiplicity, i.e. the number of filaments globally or locally connected to a given cluster is a natural probe of the growth of structure and in particular of the nature of dark energy. It is also a critical ingredient driving the assembly history of galaxies as it controls mass and angular momentum accretion. The connectivity of the cosmic web is investigated here via the persistent skeleton. This tool identifies topologically the set of ridges of the cosmic landscape which allows us to investigate in details how the nodes of the cosmic web are connected together. When applied to Gaussian random fields, it is found that on average the nodes are connected to exactly neighbours in two dimensions and ~6.1 in three dimensions. Investigating spatial dimensions up to d=11, typical departures from a cubic lattice are shown to scale like the power…
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