A new class of Szekeres inhomogeneous cosmologies with imperfect fluids

Details A new class of Szekeres inhomogeneous cosmologies with imperfect fluids A new class of Szekeres inhomogeneous cosmologies with imperfect fluids

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.165..243t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 165, no. 2, March 1990, p. 243-253. Research supported by CNPq.

Astronomy and Astrophysics

Astrophysics

4

Astronomical Models, Cosmology, Viscous Fluids, Entropy, Inhomogeneity, Universe

Scientific paper

A new class of inhomogeneous cosmological models is derived to verify that in the limit of large cosmological time some models approach the Friedmannlike universe. The contribution of the viscosity to the production entropy is estimated. The anisotropy present in the models in the asymptotic limits is estimated, and the results obtained are compared with the corresponding models without viscosity.

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