2019
DOI: 10.1002/andp.201800396
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Experimental Calibration of Sn‐Related Varshni Parameters for High Sn Content GeSn Layers

Abstract: From temperature-dependent photoluminescence of a single Ge 0.84 Sn 0.16 sample, Sn-related Varshni parameters are extracted and used as input parameters in an 8-band k·p model, and predict direct bandgap energies of high Sn content GeSn alloys with concentration varying from 8% to 16%. Then, exhaustively compared are the calculated direct -valley bandgap energies to photoluminescence results of 13% and 16% Sn content alloys and to direct bandgap energies found in literature. The agreement between k·p modeling… Show more

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Cited by 18 publications
(15 citation statements)
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References 34 publications
(36 reference statements)
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“…This contribution is assigned to light emission from the unstrained parts of the samples, located outside the 8 μm long waveguide, but inside the 12.5 μm pumping spot. This is in agreement with the expected emission from a relaxed GeSn 16% layer, as already shown in refs and at 25 K, indicating that recombination takes place in the highest Sn content layer. Note that the signal from the epilayer (referred to as “Blanket Layer” in Figure A) is slightly blue-shifted compared with the signal from the broken bridges (called “Relaxed” in Figure A), due to the slight residual compressive strain in the GeSn stack after epitaxy.…”
supporting
confidence: 93%
“…This contribution is assigned to light emission from the unstrained parts of the samples, located outside the 8 μm long waveguide, but inside the 12.5 μm pumping spot. This is in agreement with the expected emission from a relaxed GeSn 16% layer, as already shown in refs and at 25 K, indicating that recombination takes place in the highest Sn content layer. Note that the signal from the epilayer (referred to as “Blanket Layer” in Figure A) is slightly blue-shifted compared with the signal from the broken bridges (called “Relaxed” in Figure A), due to the slight residual compressive strain in the GeSn stack after epitaxy.…”
supporting
confidence: 93%
“…As we have achieved lasing for microdisks with Sn contents above 7%, we therefore assume that the microdisk emission stems from direct transitions. The experimental band gap dependence on Sn content shown in Figure b was thus fitted with E Γ ( x Sn ) by adjusting the bowing parameter and adopting b Γ = 2.77 eV, a value close to the 2.46 eV energy reported in ref . In previous reports, for instance in refs and where b Γ = 2.24 eV and b L = 0.89 eV were used, the indirect–direct band gap crossover was expected to occur at around 8% of Sn, as also reported in refs , , and .…”
Section: Resultssupporting
confidence: 55%
“…The experimental band gap dependence on Sn content shown in Figure 2-b was thus fitted with E Γ (x Sn ) by adjusting the bowing parameter and adopting b Γ = 2.77 eV, a value close to the 2.46 eV energy reported in ref. 25 In previous reports, for instance in ref., 24,26 where b Γ = 2.24 eV and b L = 0.89 eV were used, the indirect-direct band gap crossover was expected to occur at around 8 % of Sn, as also reported in ref. 1,4,[27][28][29] Here, it occurred at 6.4 %, in good agreement with the modeled one for relaxed GeSn alloys.…”
Section: Optical Analysismentioning
confidence: 94%
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“…Here, we used b Γ = 2.46 eV and b L = 1.23 eV. 36 An exception to the Vegard's law was the Luttinger parameters γ 1 , γ 2 , and γ 3 , which were interpolated only within the alloy fraction range [0, 0.2]. All values inbetweens were interpolated using Vegard's law with x replaced by x/0.2.…”
Section: Methodsmentioning
confidence: 99%