On the space-time permeated by a viscous, compressible, thermally conducting, self-gravitating fluid with infinite electrical conductivity and constant magnetic permeability

Details On the space-time permeated by a viscous, compressible, thermally conducting, self-gravitating fluid with infinite electrical conductivity and constant magnetic permeability On the space-time permeated by a viscous, compressible, thermally conducting, self-gravitating fluid with infinite electrical conductivity and constant magnetic permeability

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979anihp..30....1a&link_type=abstract

Institut Henri Poincare, Annales, Section A - Physique Theorique, vol. 30, Jan. 1-Feb. 15, 1979, p. 1-15. Research supported by

Astronomy and Astrophysics

Astrophysics

Astrophysics, Conducting Fluids, Gravitational Fields, Magnetohydrodynamics, Maxwell Equation, Relativistic Plasmas, Space-Time Functions, Compressible Fluids, Field Theory (Physics), Inhomogeneity, Magnetic Permeability, Propagation Modes, Thermal Conductivity, Universe, Viscous Fluids

Scientific paper

The properties of the space-time filled with a viscous, compressible, thermally conducting, relativistic fluid with infinite electrical conductivity and constant magnetic permeability (magnetofluid) are investigated. The causes producing the disturbance in the homogeneity and isotropy of the universe filled with the magnetofluid are found by constructing 'Maxwell-like' equations. Furthermore, the compatibility of a C-space with the gravitational field of the magnetofluid is examined. The propagation equations for the kinematical parameters are obtained and it is proved that for an essentially expanding flow of the magnetofluid, the tidal force is due to magnetic field only. Moreover, if the stream lines are shear-free and irrotational then it is shown that the magnetofluid is of Petrov type I, D or O.

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