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Finite Range of Large Perturbations in Hamiltonian Dynamics
Authors:D. Bénisti  D. F. Escande
Affiliation:(1) Equipe Turbulence Plasma du Laboratoire de Physique des Interactions Ioniques et Moléculaires, UMR 6633 CNRS-Université de Provence, Centre universitaire de Saint-Jérôme, F-13397 Marseille Cedex 20, France;;(2) Present address: Consorzio RFX, Corso Stati Uniti, 4, 35127 Padova, Italy;
Abstract:The dynamics defined by the Hamiltonian 
$$H = p^2 /2 + Asumnolimits_{m =  - M}^M {cos (q - mt + varphi m)}$$
, where the phgrm are fixed random phases, is investigated for large values of A, and for 
$$M gg A^{2/3}$$
. For a given P* and for 
$$Delta upsilon  geqslant A^{2/3}$$
, this Hamiltonian is transformed through a rigorous perturbative treatment into a Hamiltonian where the sum of all the nonresonant terms, having a Q dependence of the kind cos(kQ – nt + phgrm) with 
$$|n/k - P^ *  | > Delta upsilon$$
, is a random variable whose r.m.s. with respect to the phgrm is exponentially small in the parameter 
$$varepsilon  = A/Delta upsilon ^{3/2}$$
. Using this result, a rationale is provided showing that the statistical properties of the dynamics defined by H, and of the reduced dynamics including at each time t only the terms in H such that 
$$|m - p(t)| leqslant alpha A^{2/3}$$
, can be made arbitrarily close by increasing agr. For practical purposes agr close to 5 is enough, as confirmed numerically. The reduced dynamics being nondeterministic, it is thus analytically shown, without using the random-phase approximation, that the statistical properties of a chaotic Hamiltonian dynamics can be made arbitrarily close to that of a stochastic dynamics. An appropriate rescaling of momentum and time shows that the statistical properties of the dynamics defined by H can be considered as independent of A, on a finite time interval, for A large. The way these results could generalize to a wider class of Hamiltonians is indicated.
Keywords:Perturbation theory  Hamiltonian dynamics  wave–  particle interaction: transport properties  chaos  plasma turbulence
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