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 normal modes are dissipating, while the remaining 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.
Militello, B., Chruściński, D., Napoli, A. (2018). Star network synchronization led by strong coupling-induced frequency squeezing. PHYSICA SCRIPTA, 93(2), 025201-1-025201-6 [10.1088/1402-4896/aa9c76].
Star network synchronization led by strong coupling-induced frequency squeezing
Militello, Benedetto
;Chruściński, Dariusz;Napoli, Anna
2018-01-01
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 normal modes are dissipating, while the remaining 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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