2021
DOI: 10.1039/d1ce00364j
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Different structural evolutions of inorganic perovskite CsGeI3

Abstract: Distinguished from CsSnI3 perovskite systems, the most stable non-centrosymmetric trigonal structure (space group of R3m) of CsGeI3 perovskite system is found in our calculations. We systematically study the differences between...

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Cited by 16 publications
(12 citation statements)
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“…The DOS of Ge I /Sn I defects are calculated and the deep energy levels in the forbidden band are clearly found in both P 1-CsSn 0.5 Ge 0.5 I 3 and R 3 m -CsSn 0.5 Ge 0.5 I 3 systems, which will introduce the electron–hole nonradiative recombination and inhibition the efficiency (Figure ). It can be seen in Figures a and c that the Sn I and Ge I antisite defects of the CsSn 0.5 Ge 0.5 I 3 - P 1 structure are both obvious deep level defects, which are consistent with the studies of other structures. , In order to further explore the nature of Ge I /Sn I defect, the band structure of the defect systems is also calculated (Figure S2). Both of them are clearly deep in the forbidden band close to the CBM, in agreement with our DOS calculations.…”
supporting
confidence: 80%
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“…The DOS of Ge I /Sn I defects are calculated and the deep energy levels in the forbidden band are clearly found in both P 1-CsSn 0.5 Ge 0.5 I 3 and R 3 m -CsSn 0.5 Ge 0.5 I 3 systems, which will introduce the electron–hole nonradiative recombination and inhibition the efficiency (Figure ). It can be seen in Figures a and c that the Sn I and Ge I antisite defects of the CsSn 0.5 Ge 0.5 I 3 - P 1 structure are both obvious deep level defects, which are consistent with the studies of other structures. , In order to further explore the nature of Ge I /Sn I defect, the band structure of the defect systems is also calculated (Figure S2). Both of them are clearly deep in the forbidden band close to the CBM, in agreement with our DOS calculations.…”
supporting
confidence: 80%
“…It can be seen in Figures 4a and c that the Sn I and Ge I antisite defects of the CsSn 0.5 Ge 0.5 I 3 -P1 structure are both obvious deep level defects, which are consistent with the studies of other structures. 17,43 In order to further explore the nature of Ge I / Sn I defect, the band structure of the defect systems is also calculated (Figure S2). Both of them are clearly deep in the forbidden band close to the CBM, in agreement with our DOS calculations.…”
Section: T H Imentioning
confidence: 99%
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“…The thermal analysis results in Figure d are similar to what has been reported for powder CGI crystals. Phase transformation is found to happen from the rhombohedral ( R 3 m ) to cubic ( Pm 3̅ m ) phase , at 275 °C, and the melting point is verified at 430 °C. Due to the decomposition of GeI 2 from part of the CGI at 450 °C, we have observed a stronger peak (450 °C) after 430 °C.…”
Section: Resultsmentioning
confidence: 96%
“…158 Indeed, their bandgaps (R3m space group) are linearly increasing with respect to the concentration of Ge. 159 For instance, the CsSn 0.5 Ge 0.5 I 3 has a bandgap (1.50 eV) in between CsSnI 3 (1.31 eV) and CsGeI 3 (1.63 eV) and allows photo-absorption across the visible light region. 32 As a result, a PCE of 7.11% is obtained for CsSn 0.5 Ge 0.5 I 3 in comparison to the 3.72% attained without forming a native-oxide layer and the 1.7% of the pure CsSnI 3 .…”
Section: Solar Cellsmentioning
confidence: 99%