The cosmic web in CosmoGrid void regions

Void (composites) Structure formation The Void
DOI: 10.1017/s1743921316010607 Publication Date: 2016-10-14T16:58:18Z
ABSTRACT
We study the formation and evolution of cosmic web, using high-resolution CosmoGrid \$\Lambda\$CDM simulation. In particular, we investigate large-scale structure around void halo groups, compare this to observations VGS-31 galaxy group, which consists three interacting galaxies inside a large void. The such haloes shows great deal tenuous structure, with most systems being embedded in intra-void filaments walls. use Nexus+ algorithm detect walls CosmoGrid, find them be present detectable at every scale. regions embed walls, turn filaments. hypothesize that group formed an environment.
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