| Literature DB >> 35541770 |
Haolin Li1, Jilong Tang1, Guotao Pang2, Dengkui Wang1, Xuan Fang1, Rui Chen2, Zhipeng Wei1.
Abstract
III-V ternary alloy quantum-wells have become a hot topic in recent years. Especially, GaAs/GaAsSb quantum wells have attracted increasing attention due to their numerous applications in the field of near-infrared optoelectronic devices. With the further reduction of dimensions, GaAs/GaAsSb nanowires show many special properties compared to their quantum well structures. In this work, GaAs/GaAs1-x Sb x /GaAs coaxial single quantum-well nanowires with different Sb composition were grown by molecular beam epitaxy. The band structure and the optical properties were investigated through power-dependent and temperature-dependent photoluminescence measurement. It has been found that a deeper quantum well is created with the increase of Sb component. Thanks to the deeper quantum well, more effective electron confinement has been realized, the emission from the sample can still be detected up to room temperature. The different trend of peak position and shape at various temperatures also supports the improved temperature stability of the samples. These results will be beneficial for the design of alloy quantum wells, and will facilitate the development of alloy quantum-well based devices. This journal is © The Royal Society of Chemistry.Entities:
Year: 2019 PMID: 35541770 PMCID: PMC9075889 DOI: 10.1039/c9ra08451g
Source DB: PubMed Journal: RSC Adv ISSN: 2046-2069 Impact factor: 3.361
Fig. 1GaAs/GaAsSb/GaAs coaxial single quantum-well nanowires with different Sb component. (a) and (b) SEM image of sample A and sample B, separately. (c) STEM image of sample B. (d) STEM image taken from the GaAs core, the inset is typical SAED patterns. (e) EDX spectrum of the cross section from sample B. (f) Low temperature PL emission.
Fig. 2Low temperature PL under different excitation intensities. (a) Sample A. (b) Sample B. (c) Energy shift with excitation power. (d) Schematic band structure (the scale bar in (a) and (b) represents the normalized emission intensity).
Fig. 3Normalized PL emission with temperature dependent.
Fig. 4(a) Photon energy shift with temperature (the solid line is the fitting result according to the Varshni equation. The dash lines were obtained by shifting the solid line vertically). (b) FWHM change with temperature (the shadow is used to indicate the inflection point).