Secular dynamics of a planar model of the Sun-Jupiter-Saturn-Uranus system; effective stability in the light of Kolmogorov and Nekhoroshev theories
DOI10.1134/S156035471701004XzbMath1390.70020arXiv1702.04894OpenAlexW2587394753MaRDI QIDQ1707952
Ugo Locatelli, Antonio Giorgilli, Marco Sansottera
Publication date: 4 April 2018
Published in: Regular and Chaotic Dynamics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1702.04894
exponential stabilityHamiltonian systemsKAM theorycelestial mechanicsNekhoroshev theory\(n\)-body planetary problemnormal form methods
Computational methods for problems pertaining to mechanics of particles and systems (70-08) Perturbations of finite-dimensional Hamiltonian systems, normal forms, small divisors, KAM theory, Arnol'd diffusion (37J40) Dynamical systems in classical and celestial mechanics (37N05) (n)-body problems (70F10) Nearly integrable Hamiltonian systems, KAM theory (70H08)
Related Items (17)
Cites Work
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- On the extension of the Laplace-Lagrange secular theory to order two in the masses for extrasolar systems
- On the convergence of an algorithm constructing the normal form for elliptic lower dimensional tori in planetary systems
- Construction of librational invariant tori in the spin-orbit problem
- Invariant KAM tori and global stability for Hamiltonian systems
- Superexponential stability of KAM tori.
- On the break-down threshold of invariant tori in four-dimensional maps
- Stability of the planetary three-body problem. I: Expansion of the planetary Hamiltonian
- On the stability of the secular evolution of the planar Sun-Jupiter-Saturn-Uranus system
- A semi-analytic algorithm for constructing lower dimensional elliptic tori in planetary systems
- Kolmogorov and Nekhoroshev theory for the problem of three bodies
- Invariant tori in the Sun-Jupiter-Saturn system
- Construction of Kolmogorov's normal form for a planetary system
- Stable and Random Motions in Dynamical Systems
- On the Equilateral Configuration in the Restricted Problem of Three Bodies
- The Lagrange Configuration in Celestial Mechanics
- KAM stability and celestial mechanics
- On the construction of the Kolmogorov normal form for the Trojan asteroids
- PROOF OF A THEOREM OF A. N. KOLMOGOROV ON THE INVARIANCE OF QUASI-PERIODIC MOTIONS UNDER SMALL PERTURBATIONS OF THE HAMILTONIAN
- N-Dimensional Elliptic Invariant Tori for the Planar (N+1)-Body Problem
- SMALL DENOMINATORS AND PROBLEMS OF STABILITY OF MOTION IN CLASSICAL AND CELESTIAL MECHANICS
- Invariant tori in the secular motions of the three-body planetary systems
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