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arXiv · 1710.11025

Star network synchronization led by strong coupling-induced frequency squeezing

Benedetto Militello·Dariusz Chruściński·Anna Napoli
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Abstract

We consider a star network consisting of N oscillators coupled to a central one which in turn is coupled to an infinite set of oscillators (reservoir), which makes it leaking. Two of the N + 1 normal modes are dissipating, while the remaining N - 1 lie in a frequency range which is more and more squeezed as the coupling strengths increase, which realizes synchronization of the single parts of the system.

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Benedetto Militello, Dariusz Chruściński, Anna Napoli. 2017-10-30. Star network synchronization led by strong coupling-induced frequency squeezing. https://doi.org/10.1088/1402-4896%2Faa9c76

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