Abstract
Some solutions of the Einstein-Maxwell equations for gravitational and electromagnetic fields against the background of a rotating and either a stationary or an expanding cosmological model have been obtained. The details of one of these solutions have been given. The solution describes a cosmological model with rotation and shear. The model is initially stationary and then expanding. It is filled with anisotropic fluid and is pervaded by the electromagnetic field, the net charge density being zero.
Subject
General Physics and Astronomy
Cited by
2 articles.
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1. Cosmological Models with Bianchi Type V Metric;Russian Physics Journal;2022-06
2. Bianchi type II cosmological model of the Universe’s evolution;International Journal of Geometric Methods in Modern Physics;2017-12-19