The spatial cosmic matter distribution on scales of a few up to more than a hundred megaparsec displays a salient and pervasive foam-like pattern. Revealed through the painstaking efforts of redshift survey campaigns, it has completely revised our view of the matter distribution on these cosmological scales. The web-like spatial arrangement of galaxies and mass into elongated filaments, sheet-like walls and dense compact clusters, the existence of large near-empty void regions and the hierarchical nature of this mass distribution - marked by substructure over a wide range of scales and densities - are three major characteristics we have come to know as the cosmic web. © 2008 Springer-Verlag Berlin Heidelberg.
CITATION STYLE
van de Weygaert, R., & Schaap, W. (2009). The cosmic web: Geometric analysis. Lecture Notes in Physics, 665, 291–413. https://doi.org/10.1007/978-3-540-44767-2_11
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