A class of viscous magnetohydrodynamic type-I cosmologies

Details A class of viscous magnetohydrodynamic type-I cosmologies A class of viscous magnetohydrodynamic type-I cosmologies

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phrvd..33.3534b&link_type=abstract

Physical Review D (Particles and Fields), Volume 33, Issue 12, 15 June 1986, pp.3534-3544

Physics

8

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Scientific paper

Bianchi type-I models with a powers-of-t metric are investigated as solutions of the Einstein field equations for a viscous fluid with or without a magnetic field. Solutions are found which satisfy linear thermodynamic relations as well as all energy conditions. In general, these solutions contain a tilting velocity and depend on two parameters which satisfy certain restrictions. In the magnetohydrodynamic case solutions are shown to exist when the magnetic field and the spatial component of the velocity vector are parallel and also when they are perpendicular.

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