Chimera States in Star Networks

dc.contributor.authorMeena, C.
dc.contributor.authorSinha, Sudeshna
dc.date.accessioned2020-12-02T10:00:52Z
dc.date.available2020-12-02T10:00:52Z
dc.date.issued2016
dc.descriptionOnly IISERM authors are available in the record.
dc.description.abstractWe consider star networks of chaotic oscillators, with all end-nodes connected only to the central hub node, under diffusive coupling, conjugate coupling and mean-field diffusive coupling. We observe the existence of chimeras in the end-nodes, which are identical in terms of the coupling environment and dynamical equations. Namely, the symmetry of the end-nodes is broken and coexisting groups with different synchronization features and attractor geometries emerge. Surprisingly, such chimera states are very wide-spread in this network topology, and large parameter regimes of moderate coupling strengths evolve to chimera states from generic random initial conditions. Further, we verify the robustness of these chimera states in analog circuit experiments. Thus it is evident that star networks provide a promising class of coupled systems, in natural or engineered contexts, where chimeras are prevalent.en_US
dc.identifier.citationInternational Journal of Bifurcation and Chaos,26(9).en_US
dc.identifier.otherhttps://doi.org/10.1142/S0218127416300238
dc.identifier.urihttps://www.worldscientific.com/doi/abs/10.1142/S0218127416300238
dc.identifier.urihttp://hdl.handle.net/123456789/2519
dc.language.isoenen_US
dc.publisherWorld Scientificen_US
dc.subjectChimeraen_US
dc.subjectSynchronizationen_US
dc.subjectComplex networksen_US
dc.titleChimera States in Star Networksen_US
dc.typeArticleen_US

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