dc.contributor.authorKyriienko, O.
dc.contributor.authorKavokin, A. V.
dc.contributor.authorShelykh, I. A.
dc.date.accessioned2014-01-21T06:28:58Z
dc.date.available2014-01-21T06:28:58Z
dc.date.copyright2013en_US
dc.date.issued2013
dc.identifier.citationKyriienko, O., Kavokin, A. V., & Shelykh, I. A. (2013). Superradiant terahertz emission by dipolaritons. Physical review letters, 111(17).en_US
dc.identifier.urihttp://hdl.handle.net/10220/18645
dc.description.abstractDipolaritons are mixed light-matter quasiparticles formed in double quantum wells embedded in microcavities. Because of resonant coupling between direct and indirect excitons via electronic tunneling, dipolaritons possess large dipole moments. Resonant excitation of the cavity mode by a short pulse of light induces oscillations of the indirect exciton density with a characteristic frequency of Rabi flopping. This results in oscillations of a classical Hertz dipole array which generate supperradiant emission on a terahertz (THz) frequency. The resulting THz signal may be enhanced using the supplementary THz cavity in the weak coupling regime.en_US
dc.language.isoenen_US
dc.relation.ispartofseriesPhysical review lettersen_US
dc.rights© 2013 American Physical Society. This paper was published in Physical Review Letters and is made available as an electronic reprint (preprint) with permission of American Physical Society. The paper can be found at the following official DOI: [http://dx.doi.org/10.1103/PhysRevLett.111.176401].  One print or electronic copy may be made for personal use only. Systematic or multiple reproduction, distribution to multiple locations via electronic or other means, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper is prohibited and is subject to penalties under law.en_US
dc.subjectDRNTU::Science::Physics
dc.titleSuperradiant terahertz emission by dipolaritonsen_US
dc.typeJournal Article
dc.contributor.schoolSchool of Physical and Mathematical Sciencesen_US
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevLett.111.176401
dc.description.versionPublished versionen_US


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