dc.contributorUniversidade Estadual Paulista (UNESP)
dc.creatorKoiller, Jair
dc.creatorBalthazar, José Manoel
dc.creatorYokoyama, T.
dc.date2014-05-27T03:04:41Z
dc.date2016-10-25T18:12:10Z
dc.date2014-05-27T03:04:41Z
dc.date2016-10-25T18:12:10Z
dc.date1987-05-01
dc.date.accessioned2017-04-06T00:41:06Z
dc.date.available2017-04-06T00:41:06Z
dc.identifierPhysica D: Nonlinear Phenomena, v. 26, n. 1-3, p. 85-122, 1987.
dc.identifier0167-2789
dc.identifierhttp://hdl.handle.net/11449/63809
dc.identifierhttp://acervodigital.unesp.br/handle/11449/63809
dc.identifier10.1016/0167-2789(87)90216-8
dc.identifier2-s2.0-0039675609
dc.identifierhttp://dx.doi.org/10.1016/0167-2789(87)90216-8
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/885776
dc.descriptionSudden eccentricity increases of asteroidal motion in 3/1 resonance with Jupiter were discovered and explained by J. Wisdom through the occurrence of jumps in the action corresponding to the critical angle (resonant combination of the mean motions). We pursue some aspects of this mechanism, which could be termed relaxation-chaos: that is, an unconventional form of homoclinic behavior arising in perturbed integrable Hamiltonian systems for which the KAM theorem hypothesis do not hold. © 1987.
dc.languageeng
dc.relationPhysica D: Nonlinear Phenomena
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.titleRelaxation-chaos phenomena in celestial mechanics. I. On wisdom's model for the 3/1 kirkwood gap
dc.typeOtro


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