A gravitationally non-degenerate cosmological model with expanding and shearing viscous fluid in general relativity

Details A gravitationally non-degenerate cosmological model with expanding and shearing viscous fluid in general relativity A gravitationally non-degenerate cosmological model with expanding and shearing viscous fluid in general relativity

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.139..175b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 139, no. 1, Dec. 1987, p. 175-181.

Astronomy and Astrophysics

Astrophysics

8

Astronomical Models, Cosmology, Gravitation Theory, Relativity, Universe, Viscous Fluids

Scientific paper

The object of this paper is to investigate the behaviour of viscosity in
a cosmological model, in which the coefficient of shear viscosity is
assumed to be proportional to rate of expansion in the model. The
behaviour of the model in the absence of shear viscosity is also
discussed.

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