Viscous inflationary universe models

The research on viscous cosmological models is reviewed. Inflationary cosmological models of Bianchi type-I with shear, bulk, and nonlinear viscosity are studied. The inflation field energy is represented by a two- component cosmic fluid consisting of a vacuum fluid and a Zel'dovich fluid. It i...

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Veröffentlicht in:Astrophysics and space science 1990-11, Vol.173 (2), p.191-225
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creator Gron, O
description The research on viscous cosmological models is reviewed. Inflationary cosmological models of Bianchi type-I with shear, bulk, and nonlinear viscosity are studied. The inflation field energy is represented by a two- component cosmic fluid consisting of a vacuum fluid and a Zel'dovich fluid. It is shown that there exist models in which the viscous Zel'dovich fluid removes the initial singularity of the corresponding viscosity free models. The mean expansion of a Zel'dovich dominated universe is found to be independent of shear viscosity and anisotropy. Bulk viscosity and shear viscosity cause exponential decay of anisotropy, while nonlinear viscosity causes power-law decay of anisotropy. (Author)
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source Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; SpringerLink Journals - AutoHoldings
subjects Astronomy
Cosmology
Earth, ocean, space
Exact sciences and technology
Origin and formation of the universe
Stellar systems. Galactic and extragalactic objects and systems. The universe
title Viscous inflationary universe models
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