Anisotropic Bianchi II cosmological models with matter and electromagnetic fields

Mathematics – Logic

Scientific paper

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Anisotropy, Astronomical Models, Cosmology, Electromagnetic Fields, Extraterrestrial Matter, Universe, Einstein Equations, Flux Density, Maxwell Equation, Plasma Density

Scientific paper

A class of spatially homogeneous cosmological solutions of the Einstein-Maxwell equations for a perfect fluid and an electromagnetic field is presented which includes a Bianchi type II group acting transitively on the sections of homogeneity. A particular solution is examined and found to be unstable to perturbations of the electromagnetic-field strength parameter about a certain value. This value is shown to define a limiting unstable case where the ratio of the fluid density to the electromagnetic energy density increases monotonically from a minimum finite value at the singularity. Other cosmological features of such anisotropic models are considered. It is noted that for large times all these models have as a limit the exact anisotropic Bianchi II solution for a zero electromagnetic field and a fluid with an equation of state p = (1/5)rho.

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