6533b7d8fe1ef96bd126b81b
RESEARCH PRODUCT
Star network synchronization led by strong coupling-induced frequency squeezing
Dariusz ChruścińskiAnna NapoliBenedetto Militellosubject
PhysicsStar networkInfinite setRange (particle radiation)Quantum PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciFOS: Physical sciencesdissipationDissipationCondensed Matter Physics01 natural sciencesSettore FIS/03 - Fisica Della MateriaAtomic and Molecular Physics and Optics010305 fluids & plasmasSynchronization (alternating current)Coupling (physics)Normal modeQuantum mechanics0103 physical sciencesTurn (geometry)star network010306 general physicsQuantum Physics (quant-ph)synchronizationMathematical Physicsdescription
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.
year | journal | country | edition | language |
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2017-10-30 |