2006
DOI: 10.1103/physrevb.73.125207
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Optical critical points of thin-filmGe1ySnyalloys: A comparativeGe1y

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Cited by 314 publications
(213 citation statements)
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“…27 The obtained direct gap bowing parameter and the spin-orbit splitting bowing parameter of the Ge 1−x Sn x alloys are 1.936 and 0.405, respectively, in accordance with Ref. 13. The calculated direct gap transition composition for unstrained Ge 1−x Sn x alloy is around 0.062, which is consistent with the results reported in Refs.…”
Section: Calculation Methodssupporting
confidence: 90%
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“…27 The obtained direct gap bowing parameter and the spin-orbit splitting bowing parameter of the Ge 1−x Sn x alloys are 1.936 and 0.405, respectively, in accordance with Ref. 13. The calculated direct gap transition composition for unstrained Ge 1−x Sn x alloy is around 0.062, which is consistent with the results reported in Refs.…”
Section: Calculation Methodssupporting
confidence: 90%
“…[12][13][14][15][16][17] Some experimental demonstrations of Ge 1−x Sn x MOSFETs and TFETs have also been reported, confirming their superior electronic carrier properties. [18][19][20][21] The most commonly reported Ge 1−x Sn x alloys at present are grown on Ge or Si substrates.…”
Section: Introductionmentioning
confidence: 71%
“…While the SiGe and GeSn bowing parameters are known, 11,12 the experimental determination of b SiSn values is more challenging owing to the large lattice mismatch between silicon and tin which hinders the growth of high quality SiSn alloys. 13 To date, no systematic experimental study on the bowing parameter of SiSn binary alloys has been reported.…”
mentioning
confidence: 99%
“…For the band-gaps of the constituent materials Si, Ge, and Sn as well as the SiGe bowing parameter, we followed D'Costa et al and used the values 4:1 eV; 0:8 eV, À0:41 eV, and 0:21 eV, respectively. 11,14 For the GeSn bowing parameters, several values can be found in the literature varying between 1:94 eV and 2:61 eV. 11,31 Here, we use the value of 2:46 eV.…”
mentioning
confidence: 99%
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