Non-integrability of the problem of motion around an oblate planet
DOI10.1007/BF00051896zbMath0827.70006OpenAlexW2009861230MaRDI QIDQ1894308
Alessandra Celletti, Piero Negrini
Publication date: 24 July 1995
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/bf00051896
Completely integrable infinite-dimensional Hamiltonian and Lagrangian systems, integration methods, integrability tests, integrable hierarchies (KdV, KP, Toda, etc.) (37K10) Completely integrable finite-dimensional Hamiltonian systems, integration methods, integrability tests (37J35) Dynamical aspects of finite-dimensional Hamiltonian and Lagrangian systems (37J99) Celestial mechanics (70F15)
Related Items (10)
Cites Work
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- Bifurcation of solutions and the nonexistence of first integrals in Hamiltonian mechanics. I
- A criterion for the non-existence of an additional integral in Hamiltonian systems with a homogeneous potential
- Cascades of homoclinic orbits to, and chaos near, a Hamiltonian saddle- center
- Non integrability of the \(J_ 2\) problem
- On the motion of two-dimensional vortices with mass
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