Dynamics of spatially homogeneous solutions of the Einstein-Vlasov equations which are locally rotationally symmetric

Details Dynamics of spatially homogeneous solutions of the Einstein-Vlasov equations which are locally rotationally symmetric Dynamics of spatially homogeneous solutions of the Einstein-Vlasov equations which are locally rotationally symmetric

1998-11-16

arxiv.org/abs/gr-qc/9811051v1

Class.Quant.Grav. 16 (1999) 1705-1726

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

27 pages, 3 figures, LaTeX

Scientific paper

10.1088/0264-9381/16/6/305

The dynamics of a class of cosmological models with collisionless matter and four Killing vectors is studied in detail and compared with that of corresponding perfect fluid models. In many cases it is possible to identify asymptotic states of the spacetimes near the singularity or in a phase of unlimited expansion. Bianchi type II models show oscillatory behaviour near the initial singularity which is, however, simpler than that of the mixmaster model.

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