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arxiv: astro-ph/9810072 · v1 · submitted 1998-10-05 · 🌌 astro-ph

Cosmic Web: Origin and Observables

D. Pogosyan , J. R. Bond , L. Kofman (CITA) , J. Wadsley (UWash) This is my paper
classification 🌌 astro-ph
keywords analyticargumentsassesscamerascosmicdirectlydistributionfeasibility
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Simple analytic arguments are used to understand the predominantly filamentary web in the large-scale distribution of galaxies. Numerical simulations of superclusters are performed to assess the feasibility of directly mapping the intracluster webbing, in particular with weak gravitational lensing using Wide Field Cameras.

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  1. Information Content of the Cosmic Web

    astro-ph.CO 2026-05 unverdicted novelty 5.0

    An information-theoretic analysis of the cosmic web using tidal tensor eigenvalues defines morphological entropy that identifies filaments as dominant information carriers and relates to the growth rate f(z).