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Non-Linear Evolution of Inhomogeneities in Universes Dominated by Dark Matter

Published online by Cambridge University Press:  04 August 2017

S. F. Shandarin
S. F. Shandarin*
Affiliation:
Keldysh Institute of Applied Mathematics, Miusskaya Sq. 4, Moscow A-47, 125047

Abstract

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The astronomical data show that most of the mass in the Universe is dark. At present there are a few models of the dark matter: (i) the standard neutrino model, (ii) the model with unstable neutrinos, (iii) axion model. All models can be modified with Λ - term which plays role of the homogeneous component of the dark matter. In this paper the non-linear processes of gravitational instability are briefly discussed.

Type
Review Paper
Information
Symposium - International Astronomical Union , Volume 117: Dark Matter in the Universe , 1987 , pp. 369 - 377
Copyright
Copyright © Reidel 1987 

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