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Pulse train generation by soliton fission in highly nonlinear chalcogenide (As2S3) waveguide Bragg grating

Baker, Neil J; Roelens, M; Madden, Steve; Luther-Davies, Barry; de Sterke, C Martijn; Eggleton, Benjamin J

Description

The conversion of a 3.9ps optical pulse into a train of six 450fs pulses within a 37mm length of a highly nonlinear chalcogenide (As2S 3) waveguide Bragg grating is reported. Here, the initial pulse develops into a sixth-order soliton and is split into its six fundamental solitons through soliton fission. The very large optical nonlinearity and strong photosensitivity of As2S3 enables the use of pulses that are 25×shorter than in previous experiments, and have 500×less energy. The results are...[Show more]

dc.contributor.authorBaker, Neil J
dc.contributor.authorRoelens, M
dc.contributor.authorMadden, Steve
dc.contributor.authorLuther-Davies, Barry
dc.contributor.authorde Sterke, C Martijn
dc.contributor.authorEggleton, Benjamin J
dc.date.accessioned2015-12-10T22:26:06Z
dc.identifier.issn0013-5194
dc.identifier.urihttp://hdl.handle.net/1885/53775
dc.description.abstractThe conversion of a 3.9ps optical pulse into a train of six 450fs pulses within a 37mm length of a highly nonlinear chalcogenide (As2S 3) waveguide Bragg grating is reported. Here, the initial pulse develops into a sixth-order soliton and is split into its six fundamental solitons through soliton fission. The very large optical nonlinearity and strong photosensitivity of As2S3 enables the use of pulses that are 25×shorter than in previous experiments, and have 500×less energy. The results are compared to numerical modelling using the nonlinear coupled mode equations and find satisfactory agreement between experiment and theory after accounting for imperfections observed in the grating.
dc.publisherInstitute of Electrical and Electronics Engineers (IEEE Inc)
dc.sourceElectronics Letters
dc.subjectKeywords: A-train; Fs pulse; Fundamental solitons; Highly nonlinear; Large optical nonlinearities; Nonlinear coupled-mode equations; Numerical modelling; Optical pulse; Pulse-train generation; Soliton fission; Waveguide Bragg grating; Light transmission; Nonlinear
dc.titlePulse train generation by soliton fission in highly nonlinear chalcogenide (As2S3) waveguide Bragg grating
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume45
dc.date.issued2009
local.identifier.absfor020504 - Photonics, Optoelectronics and Optical Communications
local.identifier.ariespublicationu9912193xPUB282
local.type.statusPublished Version
local.contributor.affiliationBaker, Neil J, University of Sydney
local.contributor.affiliationRoelens, M, University of Sydney
local.contributor.affiliationMadden, Steve, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationLuther-Davies, Barry, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationde Sterke, C Martijn, University of Sydney
local.contributor.affiliationEggleton, Benjamin J, University of Sydney
local.description.embargo2037-12-31
local.bibliographicCitation.issue15
local.bibliographicCitation.startpage799
local.bibliographicCitation.lastpage800
local.identifier.doi10.1049/el.2009.1463
dc.date.updated2016-02-24T12:15:00Z
local.identifier.scopusID2-s2.0-68549125393
local.identifier.thomsonID000268274000022
CollectionsANU Research Publications

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