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arxiv: 2012.14306 · v3 · pith:BNDDAVQLnew · submitted 2020-12-28 · 🌀 gr-qc · math-ph· math.MP

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

classification 🌀 gr-qc math-phmath.MP
keywords attractorsbianchimasslesstypesargumentawaybootstrapcollins--stewart
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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.

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