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We consider the spherically symmetric Vlasov-Einstein system in the case of asymptotically flat spacetimes.
From the physical point of view this system of equations can model the formation of a spherical black hole by
gravitational collapse or describe the evolution of galaxies and globular clusters. We present high-order numerical schemes based on
semi-Lagrangian
techniques. The convergence of the solution of the discretized problem to
the exact solution is proven and high-order error estimates...
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