Star network synchronization led by strong coupling-induced frequency squeezing

Anna Napoli; Benedetto Militello; Dariusz Chruściński; Anna Napoli; Benedetto Militello

Star network synchronization led by strong coupling-induced frequency squeezing

Anna Napoli, Benedetto Militello, Dariusz Chruściński, Anna Napoli, Benedetto Militello

Fisica e Chimica - Emilio Segrè

Risultato della ricerca: Article › peer review

4 Citazioni (Scopus)

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.

Lingua originale	English
pagine (da-a)	025201-1-025201-6
Numero di pagine	6
Rivista	Physica Scripta
Volume	93
Stato di pubblicazione	Published - 2018

All Science Journal Classification (ASJC) codes

???subjectarea.asjc.3100.3107???
???subjectarea.asjc.2600.2610???
???subjectarea.asjc.3100.3104???

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title = "Star network synchronization led by strong coupling-induced frequency squeezing",

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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T1 - Star network synchronization led by strong coupling-induced frequency squeezing

AU - Napoli, Anna

AU - Militello, Benedetto

AU - Chruściński, Dariusz

AU - Napoli, Anna

AU - Militello, Benedetto

PY - 2018

Y1 - 2018

N2 - 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.

AB - 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.

UR - http://hdl.handle.net/10447/290185

M3 - Article

VL - 93

SP - 025201-1-025201-6

JO - Physica Scripta

JF - Physica Scripta

SN - 0031-8949

ER -

Star network synchronization led by strong coupling-induced frequency squeezing

Abstract

All Science Journal Classification (ASJC) codes

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