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.
|Numero di pagine||6|
|Stato di pubblicazione||Published - 2018|
All Science Journal Classification (ASJC) codes