Abstract:We show assuming small data that massless solutions to the reflection symmetric Einstein-Vlasov system with Bianchi VII0 symmetry which are not locally rotational symmetric, can be arbitrarily close to and will remain close to isotropy as regards the shear. However in general the shear will not tend to zero and the Hubble normalised Weyl curvature will blow up. We thus have generalised the work [10,16] which considered a nontilted radiation fluid to the massless Vlasov case. This represents another example of … Show more
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