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Bianchi type-VI model with cosmic strings in the presence of a magnetic field

A Bianchi type-VI cosmological model in the presence of a magnetic flux together with a cloud of cosmic strings is considered. In general, the presence of a magnetic field imposes severe restrictions regarding the consistency of the field equations. These difficulties could be overtaken working either in a Bianchi type-VI$_0$ spacetime or assuming a particular coordinate-dependence of the magnetic field. Using a few plausible assumptions regarding the parametrization of the cosmic strings, some exact analytical solutions are presented. Their asymptotic behavior for large time is exhibited.

preprint2010arXivOpen access
Bijan SahaMihai Visinescu
gr-qc
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Bijan SahaMihai Visinescu

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