2026-10-12 中国科学院（CAS）
AI-generated illustration: Due to the gravity of the two clusters, the filament in between can not maintain stability under its own gravity, and flows into the two clusters. This velocity can be measured by subtracting cosmic expansion and stacking multiple similar systems. (Image by SHAO)
＜関連情報＞
- https://english.cas.cn/newsroom/research-news/202610/t20261012_1202318.shtml
- https://link.springer.com/article/10.1007/s11433-026-3054-y
宇宙フィラメントが銀河団へ分岐して落下する流れを示す最初の観測的証拠 First observational evidence for split infall flow of cosmic filaments into clusters
Ji Yao, Huanyuan Shan, Pengjie Zhang, Xiaohu Yang, Jiale Zhou, Jiaxin Han, Peng Wang & Haojie Xu
Science China Physics, Mechanics & Astronomy Published:21 September 2026
DOI:https://doi.org/10.1007/s11433-026-3054-y
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 a significance greater than 5σ 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 ∼30 km/s (∼20 km/s projected onto the line-of-sight) for clusters of mass ∼1014.3M⊙, substantially lower than expected for infall from an average cosmic environment. Multiple results on density-velocity correlation, mass-dependency, and validation with simulations 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.
