Instabilities in the Sun-Jupiter-asteroid three body problem
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Publication:736941
DOI10.1007/s10569-012-9461-8zbMath1342.70026OpenAlexW2005532637MaRDI QIDQ736941
Joseph R. Galante, John C. Urschel
Publication date: 5 August 2016
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10569-012-9461-8
Three-body problems (70F07) Hamilton's equations (70H05) Dynamical systems in classical and celestial mechanics (37N05)
Related Items (3)
Arnold diffusion in the planar elliptic restricted three-body problem: mechanism and numerical verification ⋮ Torus knot choreographies in the n-body problem ⋮ Spatial periodic orbits in the equilateral circular restricted four-body problem: computer-assisted proofs of existence
Cites Work
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- Destruction of invariant curves in the restricted circular planar three-body problem by using comparison of action
- Converse KAM: theory and practice
- Instability and diffusion in the elliptic restricted three-body problem
- Quasiperiodic motions in the planar three-body problem
- The principle of least action in geometry and dynamics
- Slow and fast diffusion in asteroid-belt resonances: A review
- On diffusion in high-dimensional Hamiltonian systems
- KAM stability and celestial mechanics
- The dynamics of pseudographs in convex Hamiltonian systems
- Recent Developments in the Theory of Hamiltonian Systems
- A note on the existence of invariant punctured tori in the planar circular restricted three-body problem
- Variational Construction of Orbits of Twist Diffeomorphisms
- Differentiability of the minimal average action as a function of the rotation number
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