Abstract
An inhomogeneous cylindrically symmetric cosmological model for stiff perfect fluid distribution with electromagnetic field is obtained.F 12 is the non-vanishing component of electromagnetic field tensor. The metric potentials are functions ofx andt both. The behaviour of the electromagnetic field tensor together with geometrical and physical aspects of the model are also examined.
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Bali, R., Tyagi, A. An inhomogeneous stiff fluid universe with electromagnetic field in general relativity. Astrophys Space Sci 163, 179–186 (1990). https://doi.org/10.1007/BF00655738
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DOI: https://doi.org/10.1007/BF00655738