Quasi-integrability in a class of systems generalizing the problem of two fixed centers

dc.creatorAlbouy, A.
dc.creatorStuchi, T. J.
dc.date2002-10-09
dc.date2002-10-09
dc.date.accessioned2026-07-07T05:34:21Z
dc.date.available2026-07-07T05:34:21Z
dc.descriptionThe problem of two fixed centers is a classical integrable problem, stated and integrated by Euler in 1760. The integrability is due to the unexpected first integral $G$. Some straightforward generalizations of the problem still have the generalization of $G$ as a first integral, but do not possess the energy integral. We present some numerical integrations suggesting that in the domain of bounded orbits the behavior of these {\it a priori} non hamiltonian systems is very similar to the behavior of usual quasi-integrable systems.
dc.description4, 14, typos added
dc.identifierhttps://arxiv.org/abs/nlin/0210020
dc.identifierhttp://arxiv.org/abs/nlin/0210020
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/80336
dc.subjectChaotic Dynamics
dc.subjectExactly Solvable and Integrable Systems
dc.titleQuasi-integrability in a class of systems generalizing the problem of two fixed centers
dc.typetext

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