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A geometric interpretation of integrable motions

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Publication:1870194
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DOI10.1023/A:1020345212438zbMath1026.70021arXivastro-ph/0105364MaRDI QIDQ1870194

Marco Pettini, Cecilia Clementi

Publication date: 11 May 2003

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0105364


zbMATH Keywords

integrabilitygalactic dynamicsNewtonian dynamics


Mathematics Subject Classification ID

Completely integrable finite-dimensional Hamiltonian systems, integration methods, integrability tests (37J35) Differential geometric methods (tensors, connections, symplectic, Poisson, contact, Riemannian, nonholonomic, etc.) for problems in mechanics (70G45) Galactic and stellar dynamics (85A05)


Related Items (5)

Weak and strong chaos in Fermi–Pasta–Ulam models and beyond ⋮ Generalised Eisenhart lift of the Toda chain ⋮ Quadratic conservation laws and collineations: a discussion ⋮ Hamiltonian chaos and differential geometry of configuration space-time ⋮ Geodesics and Killing tensors in mechanics




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