Inhomogeneous cosmological models with electromagnetic field in general relativity

Details Inhomogeneous cosmological models with electromagnetic field in general relativity Inhomogeneous cosmological models with electromagnetic field in general relativity

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.134...47b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 134, no. 1, June 1987, p. 47-54.

Statistics

Computation

7

Computational Astrophysics, Cosmology, Electromagnetic Fields, Relativity, Current Density, Flow Distribution, Fluid Pressure, Galactic Evolution

Scientific paper

Attention is given to the various physical and geometrical properties of inhomogeneous cosmological models with perfect fluid distributions in the presence of EM fields. Models of this kind play an important role in current understanding of such essential features of the universe as the formation of galaxies during the early stages of evolution. The space-time invoked is generally nondegenerate Petrov type I.

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