An inhomogeneous stiff fluid universe with electromagnetic field in general relativity

Details An inhomogeneous stiff fluid universe with electromagnetic field in general relativity An inhomogeneous stiff fluid universe with electromagnetic field in general relativity

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.163..179b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 163, no. 2, Jan. 1990, p. 179-186.

Statistics

Computation

Astronomical Models, Cosmology, Ideal Fluids, Relativity, Computational Astrophysics, Electromagnetic Fields, Field Theory (Physics)

Scientific paper

An inhomogeneous, cylindrically symmetric, cosmological model for a stiff, perfect fluid distribution with electromagnetic field is obtained. F12 is the nonvanishing component of the electromagnetic field tensor. The metric potentials are functions of x and t both. The behavior of the electromagnetic field tensor together with geometrical and physical aspects of the model are also examined.

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