Asymptotic Regimes of Magnetic Bianchi Cosmologies
arXiv:gr-qc/0309083 · doi:10.1023/B:GERG.0000016925.78122.73
Abstract
We consider the asymptotic dynamics of the Einstein-Maxwell field equations for the class of non-tilted Bianchi cosmologies with a barotropic perfect fluid and a pure homogeneous source-free magnetic field, with emphasis on models of Bianchi type VII_{0}, which have not been previously studied. Using the orthonormal frame formalism and Hubble-normalized variables, we show that, as is the case for the previously studied class A magnetic Bianchi models, the magnetic Bianchi VII_{0} cosmologies also exhibit an oscillatory approach to the initial singularity. However, in contrast to the other magnetic Bianchi models, we rigorously establish that typical magnetic Bianchi VII_{0} cosmologies exhibit the phenomena of asymptotic self-similarity breaking and Weyl curvature dominance in the late-time regime.
arXiv comment26 pages, 6 figures, submitted to Gen. Rel. Grav
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- Magnetic Bianchi-I cosmology in the Horndeski theory
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