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Theories of Large Scale Structure

Published online by Cambridge University Press:  03 August 2017

S. F. Shandarin
S. F. Shandarin*
Affiliation:
Institute for Physical Problems, ul. Kosyggina 2, Moscow 117334, USSR

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This talk is concerned with one of the most important class of theories of Large Scale Structure (hereafter LSS) based on two principal assumptions. It is supposed that (i) the main process is gravitational instability in expanding universe and (ii) the primordial perturbations a r e small Gaussian density fluctuations. Both assumptions are natural in inflationary model of the very early universe as well as in cosmological models dominated by Dark Matter (DM) in the form of Weakly Interacting Massive Particles (WIMPs). Other possible models of LSS formation are discussed by N. Turok, J. Ostriker and A. Dekel.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 130: Large Scale Structures of the Universe , 1988 , pp. 273 - 280
Copyright
Copyright © Reidel 1988 

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