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dc.date.accessioned 2020-04-17T15:03:49Z
dc.date.available 2020-04-17T15:03:49Z
dc.date.issued 2017-11
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/93656
dc.description.abstract Three types of orbits are theoretically possible in autonomous Hamiltonian systems with 3 degrees of freedom: fully chaotic (they only obey the energy integral), partially chaotic (they obey an additional isolating integral besides energy) and regular (they obey two isolating integrals besides energy). The existence of partially chaotic orbits has been denied by several authors, however, arguing either that there is a sudden transition from regularity to full chaoticity or that a long enough follow-up of a supposedly partially chaotic orbit would reveal a fully chaotic nature. This situation needs clarification, because partially chaotic orbits might play a significant role in the process of chaotic diffusion. Here we use numerically computed Lyapunov exponents to explore the phase space of a perturbed three-dimensional cubic force toy model, and a generalization of the Poincare maps to show that partially chaotic orbits ´ are actually present in that model. They turn out to be double orbits joined by a bifurcation zone, which is the most likely source of their chaos, and they are encapsulated in regions of phase space bounded by regular orbits similar to each one of the components of the double orbit en
dc.format.extent 4099-4110 es
dc.language en es
dc.subject Chaos es
dc.subject Numerical methods es
dc.subject Celestial mechanics es
dc.subject Kinematics (galaxias) es
dc.subject Dynamics (galaxias) es
dc.title Partially chaotic orbits in a perturbed cubic force model en
dc.type Articulo es
sedici.identifier.uri http://academic.oup.com/mnras/article/471/4/4099/4044715/Partially-chaotic-orbits-in-a-perturbed-cubic es
sedici.identifier.other http://dx.doi.org/10.1093/mnras/stx1922 es
sedici.identifier.other hdl:11336/35738 es
sedici.identifier.issn 0035-8711 es
sedici.creator.person Muzzio, Juan Carlos es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Instituto de Astrofísica de La Plata es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Monthly Notices of the Royal Astronomical Society es
sedici.relation.journalVolumeAndIssue vol. 471, no. 4 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)