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Semi-analytic Computations of the Speed of Arnold Diffusion Along Single Resonances in A Priori Stable Hamiltonian Systems.
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- Journal of Nonlinear Science, 2020, v. 30, n. 3, p. 851, doi. 10.1007/s00332-019-09594-9
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- Article
Nekhoroshev stability estimates for different models of the Trojan asteroids.
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- Proceedings of the International Astronomical Union, 2004, v. 2004, n. IAUC197, p. 195, doi. 10.1017/S1743921304008658
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- Article
Semi-Analytical Estimates for the Orbital Stability of Earth’s Satellites.
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- Journal of Nonlinear Science, 2021, v. 31, n. 6, p. 1, doi. 10.1007/s00332-021-09738-w
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On the connection between the Nekhoroshev theorem and Arnold diffusion.
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- Celestial Mechanics & Dynamical Astronomy, 2008, v. 102, n. 1-3, p. 49
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Ordered and chaotic Bohmian trajectories.
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- Celestial Mechanics & Dynamical Astronomy, 2008, v. 102, n. 1-3, p. 219, doi. 10.1007/s10569-008-9127-8
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- Article
Secular dynamics in extrasolar systems with two planets in mutually inclined orbits.
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- Proceedings of the International Astronomical Union, 2021, v. 15, n. S364, p. 191, doi. 10.1017/S1743921321001368
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- Article
Closed-form perturbation theory in the Sun-Jupiter restricted three body problem without relegation.
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- Proceedings of the International Astronomical Union, 2021, v. 15, n. S364, p. 113, doi. 10.1017/S1743921321001356
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- Article
Satellites' orbital stability through normal forms.
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- Proceedings of the International Astronomical Union, 2021, v. 15, n. S364, p. 146, doi. 10.1017/S174392132100137X
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- Article
Characterization of the stability for trajectories exterior to Jupiter in the restricted three-body problem via closed-form perturbation theory.
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- Proceedings of the International Astronomical Union, 2021, v. 15, n. S364, p. 232, doi. 10.1017/S1743921321001253
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- Article
Analytical theory of the spin-orbit state of a binary asteroid deflected by a kinetic impactor.
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- Celestial Mechanics & Dynamical Astronomy, 2024, v. 136, n. 4, p. 1, doi. 10.1007/s10569-024-10204-4
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Relegation-free closed-form perturbation theory and the domain of secular motions in the restricted three-body problem.
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- Celestial Mechanics & Dynamical Astronomy, 2023, v. 135, n. 4, p. 1, doi. 10.1007/s10569-023-10154-3
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- Article
The phase-space architecture in extrasolar systems with two planets in orbits of high mutual inclination.
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- Celestial Mechanics & Dynamical Astronomy, 2023, v. 135, n. 3, p. 1, doi. 10.1007/s10569-023-10136-5
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Dispersion velocity revisited.
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- Celestial Mechanics & Dynamical Astronomy, 2023, v. 135, n. 2, p. 1, doi. 10.1007/s10569-023-10128-5
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Nekhoroshev estimates for the orbital stability of Earth's satellites.
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- Celestial Mechanics & Dynamical Astronomy, 2023, v. 135, n. 2, p. 1, doi. 10.1007/s10569-023-10124-9
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- Article
Closed-form perturbation theory in the restricted three-body problem without relegation.
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- Celestial Mechanics & Dynamical Astronomy, 2022, v. 134, n. 2, p. 1, doi. 10.1007/s10569-022-10070-y
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A deep dive into the 2g+h resonance: separatrices, manifolds and phase space structure of navigation satellites.
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- Celestial Mechanics & Dynamical Astronomy, 2022, v. 134, n. 1, p. 1, doi. 10.1007/s10569-021-10060-6
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- Article
Secondary resonances and the boundary of effective stability of Trojan motions.
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- Celestial Mechanics & Dynamical Astronomy, 2018, v. 130, n. 2, p. 1, doi. 10.1007/s10569-017-9814-4
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Geostationary secular dynamics revisited: application to high area-to-mass ratio objects.
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- Celestial Mechanics & Dynamical Astronomy, 2017, v. 128, n. 2/3, p. 149, doi. 10.1007/s10569-016-9746-4
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- Article
New Hamiltonian expansions adapted to the Trojan problem.
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- Celestial Mechanics & Dynamical Astronomy, 2016, v. 126, n. 4, p. 519, doi. 10.1007/s10569-016-9710-3
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Trojan resonant dynamics, stability, and chaotic diffusion, for parameters relevant to exoplanetary systems.
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- Celestial Mechanics & Dynamical Astronomy, 2015, v. 121, n. 2, p. 139, doi. 10.1007/s10569-014-9591-2
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Analytical invariant manifolds near unstable points and the structure of chaos.
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- Celestial Mechanics & Dynamical Astronomy, 2014, v. 119, n. 3/4, p. 331, doi. 10.1007/s10569-014-9546-7
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High order normal form stability estimates for co-orbital motion.
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- Celestial Mechanics & Dynamical Astronomy, 2013, v. 117, n. 1, p. 101, doi. 10.1007/s10569-013-9507-6
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- Article