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    On the measure of Lagrangian invariant tori in nearly-integrable mechanical systems

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    Consider an n-degrees-of-freedom real-analytic mechanical system with potential ϵf=ϵf(x)\epsilon f = \epsilon f(x), x being a n-dimensional angle variable. Then, for ‘‘general’’ potentials f ’s and ϵ\epsilon small enough, the Liouville measure of the complementary of invariant tori is smaller than $\epsilon |\ln \epsilon|^a (for a suitable a > 0)

    Low-order resonances in weakly dissipative spin-orbit models

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    Second-order differential equations with small nonlinearity and weak dissipation, such as the spin–orbit model of celestial mechanics, are considered. Explicit conditions for the coexistence of periodic orbits and estimates on the measure of the basins of attraction of stable periodic orbits are discussed

    Exponential stability for the resonant D'Alembert model of Celestial Mechanics

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    We consider the classical D'Alembert Hamiltonian model for a rotationally symmetric planet revolving on Keplerian ellipse around a ̄xed star in an almost exact day/year" resonance and prove that, notwithstanding proper degeneracies, the system is stable for exponentially long times, provided the oblateness and the eccentricity are suitably small

    On the stability of some properly-degenerate Hamiltonian systems with two degrees of freedom

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    Abstract. Properly degenerate nearly–integrable Hamiltonian systems with two degrees of freedom such that the “intermediate system” depend explicitly upon the angle–variable conjugated to the non–degenerate action–variable are considered and, in particular, model problems motivated by classical examples of Celestial Mechanics, are investigated. Under suitable “convexity” assumptions on the intermediate Hamiltonian, it is proved that, in every energy surface, the action variables stay forever close to their initial values. In “non convex” cases, stability holds up to a small set where, in principle, the degenerate action–variable might (in exponentially long times) drift away from its initial value by a quantity independent of the perturbation. Proofs are based on a “blow up” (complex) analysis near separatrices, KAM techniques and energy conservation arguments
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