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Largescale Structure of the Universe

1987, Soobshcheniya Spetsial Noj Astrofizicheskoj Observatorii

Abstract
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Research over the past 25 years has shown that the cosmic structure of the Universe originated from small fluctuations in a rapidly expanding primordial state, which were magnified over 14 billion years by gravitational forces to form galaxies and larger structures. Advances in galaxy surveys and simulations, including the 2dFGRS and SDSS, have revealed detailed large-scale distributions of galaxies and dark matter, contributing to the development of a successful standard model of cosmology. New observational data from quasar absorption and cosmic microwave background radiation have validated theoretical ideas about the Universe's contents and structure formation process, leading to a rich understanding of the cosmic web.