Abstract

We demonstrate the generation of a spatiotemporal optical continuum in a highly nonlinear exciton–polariton waveguide using extremely low excitation powers (2-ps, 100-W peak power pulses) and a submillimeter device suitable for integrated optics applications. We observe contributions from several mechanisms over a range of powers and demonstrate that the strong light–matter coupling significantly modifies the physics involved in all of them. The experimental data are well understood in combination with theoretical modeling. The results are applicable to a wide range of systems with linear coupling between nonlinear oscillators and particularly to emerging polariton devices that incorporate materials, such as gallium nitride and transition metal dichalcogenide monolayers that exhibit large light–matter coupling at room temperature. These open the door to low-power experimental studies of spatiotemporal nonlinear optics in submillimeter waveguide devices.

Nonlinear optics: polariton waveguides

Miniature exciton-polariton waveguides make it possible to induce a variety of nonlinear optical effects at very low powers. Paul Walker and co-workers from a UK-Russian team fabricated semiconductor waveguides containing 3 InGaAs quantum wells and a GaAs core and an AlGaAs cladding. Picosecond pulses from a Ti:Sapphire laser (2 ps, 100 W peak power) were coupled into the waveguide from above via a gold grating coupler, they then propagated a distance of 100–600 μm along the waveguide prior to being out-coupled into free space by a second grating coupler. The strong light–matter coupling between excitons and photons inside the waveguide structure induced spectral broadening nonlinear effects such as continuum generation, self-phase modulation, modulational instability and the generation of Cherenkov radiation and X waves. The amount of spectral broadening is determined by the strength of the light–matter coupling.

Details

Title
Spatiotemporal continuum generation in polariton waveguides
Author
Walker, Paul M 1 ; Whittaker, Charles E 1 ; Skryabin, Dmitry V 2   VIAFID ORCID Logo  ; Cancellieri Emiliano 3 ; Royall, Ben 1 ; Sich Maksym 1   VIAFID ORCID Logo  ; Farrer, Ian 4 ; Ritchie, David A 5   VIAFID ORCID Logo  ; Skolnick, Maurice S 1 ; Krizhanovskii, Dmitry N 1 

 University of Sheffield, Department of Physics and Astronomy, Sheffield, UK (GRID:grid.11835.3e) (ISNI:0000 0004 1936 9262) 
 University of Bath, Department of Physics, Bath, UK (GRID:grid.7340.0) (ISNI:0000 0001 2162 1699) ; ITMO University, St. Petersburg, Russia (GRID:grid.35915.3b) (ISNI:0000 0001 0413 4629) 
 University of Sheffield, Department of Physics and Astronomy, Sheffield, UK (GRID:grid.11835.3e) (ISNI:0000 0004 1936 9262) ; Lancaster University, Department of Physics, Lancaster, UK (GRID:grid.9835.7) (ISNI:0000 0000 8190 6402) 
 University of Sheffield, Department of Electronic and Electrical Engineering, Sheffield, UK (GRID:grid.11835.3e) (ISNI:0000 0004 1936 9262) ; University of Cambridge, Cavendish Laboratory, Cambridge, UK (GRID:grid.5335.0) (ISNI:0000000121885934) 
 University of Cambridge, Cavendish Laboratory, Cambridge, UK (GRID:grid.5335.0) (ISNI:0000000121885934) 
Publication year
2019
Publication date
Jan 2019
Publisher
Springer Nature B.V.
e-ISSN
20477538
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2167304558
Copyright
This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.