Abstract
Cylindrically symmetric inhomogeneous magnetized string cosmological model is investigated. The source of the magnetic field is due to an electric current produced along x-axis. F 23 is the only non-vanishing component of electromagnetic field tensor. To get the deterministic solution, it has been assumed that the expansion (θ) in the model is proportional to the eigen value σ 11 of the shear tensor σ i j . The physical and geometric properties of the model are also discussed in presence and absence of magnetic field.
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Pradhan, A., Mathur, P. Magnetized string cosmological model in cylindrically symmetric inhomogeneous universe-revisited. Astrophys Space Sci 318, 255–261 (2008). https://doi.org/10.1007/s10509-008-9931-3
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DOI: https://doi.org/10.1007/s10509-008-9931-3