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dc.contributor.authorLeón Merino, Iván 
dc.contributor.authorPazó Bueno, Diego Santiago 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2023-01-31T14:56:56Z
dc.date.available2023-01-31T14:56:56Z
dc.date.issued2022
dc.identifier.issn2470-0045
dc.identifier.issn2470-0053
dc.identifier.issn1539-3755
dc.identifier.issn1550-2376
dc.identifier.otherFIS2016-74957-Pes_ES
dc.identifier.urihttps://hdl.handle.net/10902/27492
dc.description.abstractThe emergence of collective synchrony from an incoherent state is a phenomenon essentially described by the Kuramoto model. This canonical model was derived perturbatively, by applying phase reduction to an ensemble of heterogeneous, globally coupled Stuart-Landau oscillators. This derivation neglects nonlinearities in the coupling constant. We show here that a comprehensive analysis requires extending the Kuramoto model up to quadratic order. This “enlarged Kuramoto model” comprises three-body (nonpairwise) interactions, which induce strikingly complex phenomenology at certain parameter values. As the coupling is increased, a secondary instability renders the synchronized state unstable, and subsequent bifurcations lead to collective chaos. An efficient numerical study of the thermodynamic limit, valid for Gaussian heterogeneity, is carried out by means of a Fourier-Hermite decomposition of the oscillator density.es_ES
dc.description.sponsorshipWe acknowledge Support by Agencia Estatal de Investigación and Fondo Europeo de Desarrollo Regional under Project No. FIS2016-74957-P (AEI/FEDER, EU). IL acknowledges support by Universidad de Cantabria and Government of Cantabria under the Concepción Arenal programme.es_ES
dc.format.extent6 p.es_ES
dc.language.isoenges_ES
dc.publisherAmerican Physical Societyes_ES
dc.rights©2022 American Physical Societyes_ES
dc.sourcePhysical Review E, 2022, 105, L042201es_ES
dc.titleEnlarged Kuramoto model: Secondary instability and transition to collective chaoses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1103/PhysRevE.105.L042201es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1103/PhysRevE.105.L042201
dc.type.versionpublishedVersiones_ES


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