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Isotropization of solutions of the Einstein-Vlasov system with Bianchi V symmetry

MPG-Autoren
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Andersson,  Lars
Geometric Analysis and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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1305.7347.pdf
(Preprint), 235KB

grg1628-4.pdf
(beliebiger Volltext), 222KB

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Zitation

Nungesser, E., Andersson, L., Bose, S., & Coley, A. A. (2013). Isotropization of solutions of the Einstein-Vlasov system with Bianchi V symmetry. General Relativity and Gravitation, 46: 1628. doi:10.1007/s10714-013-1628-4.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-0029-0382-E
Zusammenfassung
Using the methods developed for different Bianchi class A cosmological models we treat the simplest Bianchi class B model, namely Bianchi type V. The future non-linear stability for solutions of the Einstein-Vlasov system is demonstrated and it is shown that these solutions are asymptotically stable to the Milne solution. Within the isotropic solutions of the Einstein-Vlasov system the spatially flat Friedmann solution is unstable within this class, and expanding models tend also to the Milne solution.