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Integrated optical auto-correlator based on third-harmonic generation in a silicon photonic crystal waveguide

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Date
05/02/2014
Author
Monat, Christelle
Grillet, Christian
Collins, Matthew
Clark, Alex
Schroeder, Jochen
Xiong, Chunle
Li, Juntao
O'Faolain, Liam
Krauss, Thomas F.
Eggleton, Benjamin J.
Moss, David J.
Funder
EPSRC
Grant ID
EP/F001622/1
Keywords
Band slow light
Parametric gain
Fourier optics
CHIP
Dispersion
Pulses
Wavelength
Nanowire
QC Physics
QB Astronomy
BDC
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Abstract
The ability to use coherent light for material science and applications is linked to our ability to measure short optical pulses. While free-space optical methods are well established, achieving this on a chip would offer the greatest benefit in footprint, performance and cost, and allow the integration with complementary signal-processing devices. A key goal is to achieve operation at sub-watt peak power levels and on sub-picosecond timescales. Previous integrated demonstrations require either a temporally synchronized reference pulse, an off-chip spectrometer or long tunable delay lines. Here we report a device capable of achieving single-shot time-domain measurements of near-infrared picosecond pulses based on an ultra-compact integrated CMOS-compatible device, which could operate without any external instrumentation. It relies on optical third-harmonic generation in a slow-light silicon waveguide. Our method can also serve as an in situ diagnostic tool to map, at visible wavelengths, the propagation dynamics of near-infrared pulses in photonic crystals.
Citation
Monat , C , Grillet , C , Collins , M , Clark , A , Schroeder , J , Xiong , C , Li , J , O'Faolain , L , Krauss , T F , Eggleton , B J & Moss , D J 2014 , ' Integrated optical auto-correlator based on third-harmonic generation in a silicon photonic crystal waveguide ' , Nature Communications , vol. 5 , 3246 . https://doi.org/10.1038/ncomms4246
Publication
Nature Communications
Status
Peer reviewed
DOI
https://doi.org/10.1038/ncomms4246
ISSN
2041-1723
Type
Journal article
Rights
©2014. Macmillan Publishers Limited. All rights reserved. NPG Terms of reuse of archived manuscipts applies http://www.nature.com/authors/policies/license.html
Description
We acknowledge the financial support of the European Commission through the Marie Curie program (FP7, ALLOPTICS), as well as the Faculty of Science at the University of Sydney and the Australian Research Council (ARC) through the Centre of Excellence (CUDOS), Discovery project (DP110100003) and DECRA programs (DE120100226, DE120101329, DE130101148). J.L. was supported by the grant of NKBRSF (G2010CB923200), NNSFC (11204386) and GNSF (S2012040007812).
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  • University of St Andrews Research
URI
http://hdl.handle.net/10023/5470

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