A plane-symmetric inhomogeneous cosmological model of perfect fluid distribution with electromagnetic field

Details A plane-symmetric inhomogeneous cosmological model of perfect fluid distribution with electromagnetic field A plane-symmetric inhomogeneous cosmological model of perfect fluid distribution with electromagnetic field

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.173..233b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 173, no. 2, Nov. 1990, p. 233-240.

Astronomy and Astrophysics

Astrophysics

11

Astronomical Models, Cosmology, Electromagnetic Fields, Gravitational Fields, Flow Distribution, Fluid Flow, Relativity, Space-Time Functions

Scientific paper

A plane-symmetric inhomogeneous cosmological model of perfect fluid distribution with electromagnetic field, is obtained. F(12) is the nonvanishing component of the electromagnetic field tensor. To get a deterministic solution, it is assumed that the free gravitational field is Petrov type-II nondegenerate. In general, the model represents an expanding, shearing, nonrotating universe in which the flow vector is geodetic. The behavior of the electromagnetic field tensor together with some geometrical and physical aspect of the model are also discussed.

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