Expanding and shearing magneto-viscous fluid cosmological model in general relativity

Details Expanding and shearing magneto-viscous fluid cosmological model in general relativity Expanding and shearing magneto-viscous fluid cosmological model in general relativity

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.116...81b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 116, no. 1, Nov. 1985, p. 81-88.

Statistics

Computation

7

Computational Astrophysics, Cosmology, Magnetic Fields, Relativity, Viscous Fluids, Density (Mass/Volume), Expansion, Fluid Pressure, Shearing, Viscosity

Scientific paper

The object of this paper is to investigate the behavior of a magnetic field in a viscous fluid cosmological model. It has been assumed that the expansion (θ) is proportional to the eigenvalue σ11 of the shear tensor σij and the coefficient of shearing viscosity is proportional to the scalar of expansion. The paper also discusses the behavior of the model when the magnetic field tends to zero and comments on some other physical properties.

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