Davide Zaccaria

Publications:

Barbieri S., Biasco L., Chierchia L., Zaccaria D.
Singular KAM Theory for Convex Hamiltonian Systems
2025, vol. 30, no. 4, pp.  538-549
Abstract
In this note, we briefly discuss how the singular KAM theory of [7] — which was worked out for the mechanical case $\frac12 |y|^2+\varepsilon f(x)$ — can be extended to convex real-analytic nearly integrable Hamiltonian systems with Hamiltonian in action-angle variables given by $h(y)+\varepsilon f(x)$ with $h$ convex and $f$ generic.
Keywords: nearly integrable Hamiltonian systems, convex Hamiltonians, measure of invariant tori, simple resonances, Arnold – Kozlov – Neishtadt conjecture, singular KAM theory
Citation: Barbieri S., Biasco L., Chierchia L., Zaccaria D.,  Singular KAM Theory for Convex Hamiltonian Systems, Regular and Chaotic Dynamics, 2025, vol. 30, no. 4, pp. 538-549
DOI:10.1134/S1560354725040057
Falcolini C., Zaccaria D.
Abstract
We provide a new expansion of the Fourier coefficient of the perturbing function of the PCR3Body problem in terms of Hansen coefficients. This gives us a precise asymptotic formula for the coefficient in the region of application of KAM theory (i.e., small value of eccentricity and semimajor axis. See, e.g., [17]). Moreover, in the above region, we study the presence of zeros of the Fourier coefficient for coprime modes $(m,k) \in \mathbb{Z}^2$ and the presence of common zeros as functions of actions between coefficients relative to modes $(m,k)$,$(2m,2k)$ and $(m,k)$,$(2m,2k)$,$(3m,3k)$. Thanks to the previous expansion, this numerical analysis is done up to order $60$ in the power of eccentricity and semimajor axis. This is the first step for a possible application of [4, 9] to the PCR3Body Problem that would imply a reduction in terms of measure in the phase space of the so-called ``non-torus'' set from $O(1-\sqrt{\varepsilon})$ (implied by standard KAM theory) to $O(1-\varepsilon |\log\varepsilon|^c )$ for some $c>0$.
Keywords: nearly integrable systems, singular KAM theory, measure of invariant tori, measure of the non-torus set, celestial mechanics, planar circular restricted three-body problem, zeros of Fourier coefficients
DOI:10.1134/S1560354725540044

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