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dc.contributorUniversitat de Vic. Escola Politècnica Superior
dc.contributorUniversitat de Vic. Grup de Recerca en Tecnologies Digitals
dc.contributor.authorCorbera Subirana, Montserrat
dc.contributor.authorLlibre, Jaume
dc.contributor.authorTeixeira, Marco Antonio
dc.date.accessioned2013-04-22T09:27:15Z
dc.date.available2013-04-22T09:27:15Z
dc.date.created2009
dc.date.issued2009
dc.identifier.citationCORBERA SUBIRANA, Montserrat; LLIBRE, Jaume; ANTONIO TEIXEIRA, Marco. "Symmetric periodic orbits near a heteroclinic loop in R-3 formed by two singular points, a semistable periodic orbit and their invariant manifolds". A: Physica D-Nonlinear Phenomena, 2009, vol. 238, núm. 6, pàg. 699-705.ca_ES
dc.identifier.issn0167-2789
dc.identifier.urihttp://hdl.handle.net/10854/2214
dc.description.abstractIn this paper we consider C1 vector fields X in R3 having a “generalized heteroclinic loop” L which is topologically homeomorphic to the union of a 2–dimensional sphere S2 and a diameter 􀀀 connecting the north with the south pole. The north pole is an attractor on S2 and a repeller on 􀀀. The equator of the sphere is a periodic orbit unstable in the north hemisphere and stable in the south one. The full space is topologically homeomorphic to the closed ball having as boundary the sphere S2. We also assume that the flow of X is invariant under a topological straight line symmetry on the equator plane of the ball. For each n ∈ N, by means of a convenient Poincar´e map, we prove the existence of infinitely many symmetric periodic orbits of X near L that gives n turns around L in a period. We also exhibit a class of polynomial vector fields of degree 4 in R3 satisfying this dynamics.en
dc.formatapplication/pdf
dc.format.extent17 p.ca_ES
dc.language.isoengca_ES
dc.publisherElsevierca_ES
dc.rights(c) Elsevier
dc.rightsTots els drets reservatsca_ES
dc.subject.otherMatemàticaca_ES
dc.titleSymmetric periodic orbits near a heteroclinic loop in R3 formed by two singular points, a semistable periodic orbit and their invariant manifoldsen
dc.typeinfo:eu-repo/semantics/articleca_ES
dc.identifier.doihttps://doi.org/10.1016/j.physd.2009.01.002
dc.relation.publisherversionhttp://www.sciencedirect.com/science/article/pii/S0167278909000049
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca_ES
dc.type.versioninfo:eu-repo/acceptedVersionca_ES
dc.indexacioIndexat a SCOPUS
dc.indexacioIndexat a WOS/JCRca_ES


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