Future attractors of Bianchi types II and V cosmologies with massless Vlasov matter
arXiv:2012.14306 · doi:10.1088/1361-6382/abe49a
Abstract
It is shown that the generalized Collins--Stewart radiation and Milne solutions are attractors of the massless Einstein--Vlasov system for Bianchi types II and V spacetimes, respectively. The proof is based on an energy method and bootstrap argument which are used to determine the decay rates of the perturbations away from the attractors.
Some minor typos are corrected in the new version
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- On almost Ehlers-Geren-Sachs theorems
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