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dc.contributor.authorPressl, B.
dc.contributor.authorGünthner, T.
dc.contributor.authorLaiho, K.
dc.contributor.authorGessler, J.
dc.contributor.authorKamp, M.
dc.contributor.authorHöfling, Sven
dc.contributor.authorSchneider, C.
dc.contributor.authorWeihs, G.
dc.date.accessioned2016-02-11T09:40:06Z
dc.date.available2016-02-11T09:40:06Z
dc.date.issued2015-12-28
dc.identifier240791369
dc.identifiercde6b381-1437-4006-a275-a51ddbe3ac12
dc.identifier84962090254
dc.identifier000368004600071
dc.identifier.citationPressl , B , Günthner , T , Laiho , K , Gessler , J , Kamp , M , Höfling , S , Schneider , C & Weihs , G 2015 , ' Mode-resolved Fabry-Perot experiment in low-loss Bragg-reflection waveguides ' , Optics Express , vol. 23 , no. 26 , pp. 33608-33621 . https://doi.org/10.1364/OE.23.033608en
dc.identifier.issn1094-4087
dc.identifier.urihttps://hdl.handle.net/10023/8196
dc.descriptionThis work was supported by the FWF project no. I-2065-N27, the DFG Project no. SCHN1376/1-1 and the ERC project EnSeNa (257531).en
dc.description.abstractBased on the interaction between different spatial modes, semiconductor Bragg-reflection waveguides (BRWs) provide a highly functional platform for non-linear optics. For achieving any desired quantum optical functionality, we must control and engineer the properties of each spatial mode. To reach this purpose we extend the Fabry-Perot technique and achieve a detailed linear optical characterization of dispersive multimode semiconductor waveguides. With this efficient broadband spectral method we gain direct experimental access to the relevant modes of our BRWs and determine their group velocities. Furthermore, we show that our waveguides have lower than expected loss coefficients. This renders them suitable for integrated quantum optics applications.
dc.format.extent1173019
dc.language.isoeng
dc.relation.ispartofOptics Expressen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQCen
dc.titleMode-resolved Fabry-Perot experiment in low-loss Bragg-reflection waveguidesen
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.doi10.1364/OE.23.033608
dc.description.statusPeer revieweden


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