Homogeneous anisotropic cosmological models with viscous fluid and magnetic field

Details Homogeneous anisotropic cosmological models with viscous fluid and magnetic field Homogeneous anisotropic cosmological models with viscous fluid and magnetic field

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986gregr..18.1251b&link_type=abstract

General Relativity and Gravitation (ISSN 0001-7701), vol. 18, Dec. 1986, p. 1251-1262. UGCI-supported research.

Mathematics

Logic

13

Anisotropy, Cosmology, Magnetic Fields, Viscous Fluids, Astronomical Models, Barotropism, Equations Of State, Scalars

Scientific paper

The paper presents some exact solutions of Bianchi types I and III and Kantowski-Sachs cosmological models consisting of a dissipative fluid along with an axial magnetic field. A barytropic equation of state, together with a pair of linear relations between the matter density, the shear scalar, and the expansion scalar have been assumed for simplicity. The solutions are basically of two different types, one for the Bianchi I and the other for III and Kantowski-Sachs type. The presence of the magnetic field, however, does not change the fundamental nature of the initial singularity.

Affiliated with

Also associated with

No associations

Rating

Homogeneous anisotropic cosmological models with viscous fluid and magnetic field does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Homogeneous anisotropic cosmological models with viscous fluid and magnetic field, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Homogeneous anisotropic cosmological models with viscous fluid and magnetic field will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1124121