hide
Free keywords:
General Relativity and Quantum Cosmology, gr-qc
Abstract:
In a recent paper arXiv:1208.4231 we have treated the future non-linear
stability for reflection symmetric solutions of the Einstein-Vlasov system of
Bianchi types II and VI$_0$. We have been able now to remove the reflection
symmetry assumption, thus treating the non-diagonal case. Apart from the
increasing complexity the methods have been essentially the same as in the
diagonal case, showing that they are thus quite powerful.
Here the challenge was to put the equations in a form that permits the use of
the previous results. We are able to conclude that after a possible basis
change the future of the non-diagonal spacetimes in consideration is
asymptotically diagonal.
