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• W2313294003 abstract "We study phase synchronization in a network motif with a starlike structure in which the central node's (the hub's) frequency is strongly detuned against the other peripheral nodes. We find numerically and experimentally a regime of remote synchronization (RS), where the peripheral nodes form a phase synchronized cluster, while the hub remains free with its own dynamics and serves just as a transmitter for the other nodes. We explain the mechanism for this RS by the existence of a free amplitude and also show that systems with a fixed or constant amplitude, such as the classic Kuramoto phase oscillator, are not able to generate this phenomenon. Further, we derive an analytic expression which supports our explanation of the mechanism." @default.
• W2313294003 created "2016-06-24" @default.
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• W2313294003 date "2012-02-15" @default.
• W2313294003 modified "2023-10-16" @default.
• W2313294003 title "Remote synchronization in star networks" @default.
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• W2313294003 doi "https://doi.org/10.1103/physreve.85.026208" @default.
• W2313294003 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/22463300" @default.
• W2313294003 hasPublicationYear "2012" @default.
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