Fluctuation-dissipation relation for chaotic non-Hamiltonian systems

Details Fluctuation-dissipation relation for chaotic non-Hamiltonian systems Fluctuation-dissipation relation for chaotic non-Hamiltonian systems

2012-01-31

arxiv.org/abs/1201.6623v1

Physics

Condensed Matter

Statistical Mechanics

Scientific paper

In dissipative dynamical systems phase space volumes contract, on average. Therefore, the invariant measure on the attractor is singular with respect to the Lebesgue measure. As noted by Ruelle, a generic perturbation pushes the state out of the attractor, hence the statistical features of the perturbation and, in particular, of the relaxation, cannot be understood solely in terms of the unperturbed dynamics on the attractor. This remark seems to seriously limit the applicability of the standard fluctuation dissipation procedure in the statistical mechanics of nonequilibrium (dissipative) systems. In this paper we show that the singular character of the steady state does not constitute a serious limitation in the case of systems with many degrees of freedom. The reason is that one typically deals with projected dynamics, and these are associated with regular probability distributions in the corresponding lower dimensional spaces.

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