Abstract
Given a Hamiltonian dynamical system, we address the question of computing the limit of the time-average of an observable. For a completely integrable system, it is known that ergodicity can be characterized by a diophantine condition on its frequencies and that this limit coincides with the space-average over an invariant manifold. In this paper, we show that we can improve the rate of convergence upon using a filter function in the time-averages. We then show that this convergence persists when a symplectic numerical scheme is applied to the system, up to the order of the integrator.
| Original language | English |
|---|---|
| Pages (from-to) | 211-232 |
| Number of pages | 22 |
| Journal | Numerische Mathematik |
| Volume | 100 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 1 Apr 2005 |
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