Star network synchronization led by strong coupling-induced frequency squeezing
arXiv:1710.11025 · doi:10.1088/1402-4896/aa9c76
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.
References in corpus (6)
- Mutual information as an order parameter for quantum synchronization
- Spin Correlations as a Probe of Quantum Synchronization in Trapped Ion Phonon-Lasers
- Synchronization dynamics of two nanomechanical membranes within a Fabry-Perot cavity
- Quantum synchronization and quantum state sharing in irregular complex network
- Quantum synchronization as a local signature of super- and subradiance
- Synchronizing Quantum Harmonic Oscillators through Two-Level Systems