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dc.contributor.authorRyczko, K.
dc.contributor.authorMisiewicz, J.
dc.contributor.authorHöfling, S.
dc.contributor.authorKamp, M.
dc.contributor.authorSęk, G.
dc.date.accessioned2017-01-25T10:30:12Z
dc.date.available2017-01-25T10:30:12Z
dc.date.issued2017-01-09
dc.identifier249000006
dc.identifier310d8f30-deb3-4ff9-bb43-f70173de8c6f
dc.identifier85009231051
dc.identifier000395789900015
dc.identifier.citationRyczko , K , Misiewicz , J , Höfling , S , Kamp , M & Sęk , G 2017 , ' Optimizing the active region of interband cascade lasers for passive mode-locking ' , AIP Advances , vol. 7 , no. 1 , 015015 . https://doi.org/10.1063/1.4973937en
dc.identifier.issn2158-3226
dc.identifier.otherBibtex: urn:9a2b8f0f8c5e305d00996896c3e15d59
dc.identifier.urihttps://hdl.handle.net/10023/10167
dc.descriptionThis project has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 636930 (iCspec).en
dc.description.abstractThe work proposes possible designs of active regions for a mode-locked interband cascade laser emitting in the mid infrared. For that purpose we investigated the electronic structure properties of respectively modified GaSb-based type II W-shaped quantum wells, including the effect of external bias in order to simultaneously fulfil the requirements for both the absorber as well as the gain sections of a device. The results show that introducing multiple InAs layers in type II InAs/GaInSb quantum wells or introducing a tensely-strained GaAsSb layer into “W-shaped” type II QWs offers significant difference in optical transitions’ oscillator strengths (characteristic lifetimes) of the two oppositely polarized parts of such a laser, being promising for utilization in mode-locked devices.
dc.format.extent7
dc.format.extent1086480
dc.language.isoeng
dc.relation.ispartofAIP Advancesen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQCen
dc.titleOptimizing the active region of interband cascade lasers for passive mode-lockingen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews. Condensed Matter Physicsen
dc.identifier.doi10.1063/1.4973937
dc.description.statusPeer revieweden


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