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Atomic Clouds as Spectrally-Selective and Tunable Delay Lines for Single Photons from Quantum Dots

dc.contributor.authorS. Wildmann, Johannes
dc.contributor.authorTrotta, Rinaldo
dc.contributor.authorMartín-Sánchez, Javier
dc.contributor.authorZallo, Eugenio
dc.contributor.authorG. Schmidt, Oliver
dc.contributor.authorRastelli, Armando
dc.date.accessioned2025-01-16T09:38:03Z
dc.date.available2025-01-16T09:38:03Z
dc.date.issued2015-12-21
dc.identifier.citationPhysical Review B, 92 (2015); doi:10.1103/PhysRevB.92.235306
dc.identifier.urihttps://hdl.handle.net/10651/76240
dc.description.abstractWe demonstrate a compact, spectrally-selective, and tunable delay line for single photons emitted by quantum dots. This is achieved by fine-tuning the wavelength of the optical transitions of such "artificial atoms" into a spectral window in which a cloud of natural atoms behaves as slow-light medium. By employing the ground-state fine-structure-split exciton confined in an InGaAs/GaAs quantum dot as a source of single photons at different frequencies and the hyperfine-structure-split D1 transition of Cs-vapors as a tunable delay-medium, we achieve a differential delay of up 2.4 ns on a 7.5 cm long path for photons that are only 60 \mu eV (14.5 GHz) apart. To quantitatively explain the experimental data we develop a theoretical model that accounts for both the inhomogeneously broadening of the quantum-dot emission lines and the Doppler-broadening of the atomic lines. The concept we proposed here may be used to implement time-reordering operations aimed at erasing the "which-path" information that deteriorates entangled-photon emission from excitons with finite fine-structure-splitting.spa
dc.language.isoengspa
dc.rightsCC Reconocimiento - No comercial - Sin obra derivada 4.0 Internacional
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.titleAtomic Clouds as Spectrally-Selective and Tunable Delay Lines for Single Photons from Quantum Dotsspa
dc.typejournal articlespa
dc.identifier.doi10.1103/PhysRevB.92.235306
dc.relation.publisherversionhttp://dx.doi.org/10.1103/PhysRevB.92.235306
dc.rights.accessRightsopen access
dc.type.hasVersionAM


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CC Reconocimiento - No comercial - Sin obra derivada 4.0 Internacional
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