Voids and the Cosmic Web: cosmic depressions & spatial complexity
arXiv:1611.01222 · doi:10.1017/S1743921316010504
Abstract
Voids form a prominent aspect of the Megaparsec distribution of galaxies and matter. Not only do they represent a key constituent of the Cosmic Web, they also are one of the cleanest probes and measures of global cosmological parameters. The shape and evolution of voids are highly sensitive to the nature of dark energy, while their substructure and galaxy population provides a direct key to the nature of dark matter. Also, the pristine environment of void interiors is an important testing ground for our understanding of environmental influences on galaxy formation and evolution. In this paper, we review the key aspects of the structure and dynamics of voids, with a particular focus on the hierarchical evolution of the void population. We demonstrate how the rich structural pattern of the Cosmic Web is related to the complex evolution and buildup of voids.
28 pages, 13 figures, Proceedings of IAU Symposium 308 "The Zeldovich Universe: Genesis and Growth of the Cosmic Web", 23-28 June 2014, Tallinn, Estonia; added arxiv reference to journal citation.
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Cited by in corpus (5)
- Void replenishment: how voids accrete matter over cosmic history
- Gas accretion and Ram Pressure Stripping of Haloes in Void Walls
- Reconstructing matter profiles of spherically compensated cosmic regions in CDM cosmology
- Dynamical Evolution of Voids with Surrounding Gravitational Tidal Field
- Detecting and analysing the topology of the cosmic web with spatial clustering algorithms I: Methods