Future attractors of Bianchi types II and V cosmologies with massless Vlasov matter

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.