First Observational Evidence for Split Infall Flow of Cosmic Filaments into Clusters

TL;DR

This paper provides the first observational evidence of split infall flows in cosmic filaments connecting galaxy clusters, revealing complex velocity dynamics that challenge previous passive transport models and offer new insights into cosmic web structure.

Contribution

It introduces observational detection of split infall flows in cosmic filaments using SDSS data, highlighting their dynamic response to gravitational potentials.

Findings

Detection of split infall velocity flows at >5σ significance.

Velocity profile shows sign reversal near filament midpoint.

Infall velocities are lower than expected from average cosmic environments.

Abstract

Velocity fields in the cosmic web are fundamental to structure formation but remain difficult to observe directly beyond the linear regime. Here we present observational evidence that galaxy filaments connecting pairs of galaxy clusters undergo a split infall, with opposite velocity flows toward the two clusters. Using spectroscopic galaxies from the Sloan Digital Sky Survey, we isolate the internal filament velocity field by subtracting its rigid-body background motion and Hubble flow, and detect this effect at greater than $5\sigma$ significance across a wide range of cluster and filament selections. The measured velocity profile exhibits a sign reversal near the filament midpoint and a maximum infall amplitude of $\sim30$ km/s ($\sim20$ km/s projected onto the line-of-sight) for clusters of mass $\sim10^{14.3}M_\odot$, substantially lower than expected for infall from an average cosmic environment. Multiple results on density-velocity correlation, mass-dependency, and validation with simulation indicate that filaments dynamically respond to competing gravitational potentials rather than acting as passive mass transport channels. Our results establish a new observational window on quasi-linear velocity fields in the cosmic web and provide a promising probe of mass measurement, testing gravity and velocity reconstruction with upcoming wide-field spectroscopic surveys.