Sub-50 cm/s surface recombination velocity in InGaAsP/InP ridges
Name
191102_1_5.0062824.pdf
Description
Published version
Size
2.29 MB
Format
Adobe PDF
Checksum (MD5)
1a438f57a375e2cabc217f2915a971fb
Author(s) • • • • •
Andrade, Nicolas M
Hooten, Sean
Kim, Yunjo
Kim, Jeehwan
Yablonovitch, Eli
Wu, Ming C
Date Issued
November 8, 2021
Journal
Applied Physics Letters
Publisher
AIP Publishing
Citation
Nicolas M. Andrade, Sean Hooten, Yunjo Kim, Jeehwan Kim, Eli Yablonovitch, Ming C. Wu; Sub-50 cm/s surface recombination velocity in InGaAsP/InP ridges. Appl. Phys. Lett. 8 November 2021; 119 (19): 191102.
Version
Final published version
Abstract
The III–V InP/InGaAsP/InGaAs material family is important for photonic devices due to its optical emission and absorption in the 1.55 and
1.3 lm telecommunication bands for optical interconnects. However, InGaAsP/InGaAs generally suffer from relatively high surface
recombination velocity—compared to Si [Das et al., in 2020 47th IEEE Photovoltaic Specialists Conference (PVSC) (IEEE, Calgary, AB, 2020),
pp. 1167–1170] and InP [Joyce et al., Nano Lett. 12, 5325–5330 (2012)], which reduces the efficiency and can increase the noise in
nanophotonic devices. Here, we demonstrate an efficient method to passivate the surface using a combination of sulfur-saturated ammonium
sulfide and atomic layer deposition. After annealing, the surface passivation led to a surface recombination velocity as low as 45 cm/s, corresponding to a >180 increase in the photoluminesence of a nanoscale light-emitting device with 200 nm width.
MIT Department
Massachusetts Institute of Technology. Department of Electrical Engineering and Computer Science
Terms of Use
Creative Commons Attribution
Persistent DSpace Link
DOI of Published Version
10.1063/5.0062824