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Large Scale Structure and the Cosmic Web
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The formation and evolution of galaxies cannot be separated from large scale structure growth. Dark matter halos (and, therefore, galaxies) form and grow within the cosmic web - the classification of large-scale structure as distinct environments, namely voids, walls, filaments and nodes. Thanks to the rapid development of extragalactic spectroscopic redshift surveys and cosmological simulations over the last two decades, we are now able to measure the impact of the cosmic web on galaxies and halos in observations and in simulations. In this chapter we summarise the state of play in our understanding of the link between dark matter halos, galaxies, and the cosmic web.
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Cited by 2 Pith papers
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Enabling Cosmic Web Analysis at Gigaparsec Scales: A Multi Block Approach for DisPerSE
A circumsphere-filtered, block-wise 'frozen-core' tiling lets DisPerSE map filaments at gigaparsec scales, yielding a 92-million-halo filament catalogue and a mass-connectivity power law A≈0.27-0.32.
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Tracing Large-Scale Structure Morphology with Multiwavelength Line Intensity Maps
CO(1-0) line intensity maps trace the cosmic web's filaments and sheets more strongly than HI 21-cm maps, and SKA2-Mid could recover this structure at z~1.4.
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