2022
DOI: 10.1016/j.optmat.2022.112112
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Study the effect of band offsets on the performance of lead-free double perovskite solar cell

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Cited by 17 publications
(5 citation statements)
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“…For instance, the optimum thickness for Cs 2 AgBi 0.75 Sb 0.25 Br 6 should be 400 nm, which is significantly higher than the theoretical value for the pristine film (200 nm). Similar thickness was reported by Singh et al [ 182 ] Improving the film quality also limits the imperfections and carrier traps at the interface. Tauc plots have shown that Cs 2 AgBiBr 6 film may have an indirect bandgap of ≈ 2.03 eV with a CBM of −4.12 eV and a VBM of −6.15 eV.…”
Section: Photophysics Of Cs2agbibr6 and Contact Characteristicssupporting
confidence: 80%
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“…For instance, the optimum thickness for Cs 2 AgBi 0.75 Sb 0.25 Br 6 should be 400 nm, which is significantly higher than the theoretical value for the pristine film (200 nm). Similar thickness was reported by Singh et al [ 182 ] Improving the film quality also limits the imperfections and carrier traps at the interface. Tauc plots have shown that Cs 2 AgBiBr 6 film may have an indirect bandgap of ≈ 2.03 eV with a CBM of −4.12 eV and a VBM of −6.15 eV.…”
Section: Photophysics Of Cs2agbibr6 and Contact Characteristicssupporting
confidence: 80%
“…Theoretical studies show that Cu 2 O and CuSCN HTLs and ZnOS ETL well meet these requirements. [181,182] The performance of these charge transport layers can be further enhanced by taking other optimization measures on the absorber layer. For instance, the optimum thickness for Cs 2 AgBi 0.75 Sb 0.25 Br 6 should be 400 nm, which is significantly higher than the theoretical value for the pristine film (200 nm).…”
Section: Contact Characteristicsmentioning
confidence: 99%
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“…That's why in that device, the performance is relatively low. But when we used the χ value of 3.67 eV (corresponding to the best result), the CBO became −0.23 eV, shown in figure 6(b), and this negative CBO is called as cliff-type [35]. In the cliff-type CBO, there is no barrier in the interface of perovskite/ETL, and the charge collection is easier.…”
Section: Effect Of Cbomentioning
confidence: 99%
“…Furthermore, the FF and PCE show an increasing trend, as demonstrated in figure 8. The acceptor density in the absorber layer has been optimized to reach 5 × 10 18 cm −3 , as increasing it further would continuously escalate costs and, beyond 1 × 10 19 cm −3 , lead to the emergence of large conduction band offsets (CBO) and valence band offsets (VBO) [57,58]. Therefore, an acceptor density of 5 × 10 18 cm −3 in the absorber layer strikes a balance between maximizing the photovoltaic performance and minimizing the associated costs, while avoiding adverse effects due to large CBO and VBO.…”
Section: Effect Of Absorber's Acceptor Density Variationmentioning
confidence: 99%