Remote synchronization in star networks

  • 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.

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Metadaten
Author:Andre Bergner, M. Frasca, G. Sciuto, A. Buscarino, Eulalie Joelle Ngamga, L. Fortuna, Jürgen KurthsORCiDGND
DOI:https://doi.org/10.1103/PhysRevE.85.026208
ISSN:1539-3755 (print)
Parent Title (English):Physical review : E, Statistical, nonlinear and soft matter physics
Publisher:American Physical Society
Place of publication:College Park
Document Type:Article
Language:English
Year of first Publication:2012
Year of Completion:2012
Release Date:2017/03/26
Volume:85
Issue:2
Pagenumber:7
Funder:DAAD/Ateneo Italo-Tedesco; ECONS; Volkswagen Foundation [85391]
Organizational units:Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie
Peer Review:Referiert