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Isotropization of solutions of the Einstein-Vlasov system with Bianchi V symmetry
KTH, School of Engineering Sciences (SCI), Mathematics (Dept.).
2014 (English)In: General Relativity and Gravitation, ISSN 0001-7701, E-ISSN 1572-9532, Vol. 46, no 1, 1-23 p.Article in journal (Refereed) Published
Abstract [en]

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.

Place, publisher, year, edition, pages
2014. Vol. 46, no 1, 1-23 p.
Keyword [en]
Bianchi, Cosmology, Einstein-Vlasov, Isotropization
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-143076DOI: 10.1007/s10714-013-1628-4ISI: 000333634900016Scopus ID: 2-s2.0-84893222634OAI: oai:DiVA.org:kth-143076DiVA: diva2:705557
Note

QC 20140317

Available from: 2014-03-17 Created: 2014-03-17 Last updated: 2017-12-05Bibliographically approved

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