Evolution of inhomogeneous cosmological models with viscous fluids

Details Evolution of inhomogeneous cosmological models with viscous fluids Evolution of inhomogeneous cosmological models with viscous fluids

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.165..231t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 165, no. 2, March 1990, p. 231-236. Research supported by CNPq.

Astronomy and Astrophysics

Astrophysics

1

Astronomical Models, Cosmology, Viscous Fluids, Inhomogeneity, Neutrinos

Scientific paper

The effect of viscosity on the isotropization of the universe is studied by examining the asymptotic behavior of Szekeres cosmological models of class II with dissipative fluids. It is verified that in some cases the solutions tend to homogeneity and isotropy when time goes to infinity. The condition gamma = 0 is necessary for isotropization effects to emerge.

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