2022
DOI: 10.1039/d2cp02358j
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Multiple-cation wide-bandgap perovskite solar cells grown using cesium formate as the Cs precursor with high efficiency under sunlight and indoor illumination

Abstract: Owing to the advantages of bandgap adjustable, low-cost fabrication and superior photovoltaic performance, wide-bandgap (WBG) perovskite solar cells (PSCs) are considered as promising top-cell for multi-junction solar cells. At the...

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Cited by 10 publications
(6 citation statements)
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“…The fast time component (τ 1 ) implies the charge carrier was captured at the perovskite grain boundary and perovskite/HTMs interface, and the second component (τ 2 ) represents the injection of holes from the perovskite to the HTMs. 37,38 The results of TAS were consistent with the results of TRPL. All the photophysical properties and charge transport properties of CsPbI 2 Br, HTMs, and CsPbI 2 Br/ HTMs are summarized in Table S4.…”
Section: Resultssupporting
confidence: 83%
“…The fast time component (τ 1 ) implies the charge carrier was captured at the perovskite grain boundary and perovskite/HTMs interface, and the second component (τ 2 ) represents the injection of holes from the perovskite to the HTMs. 37,38 The results of TAS were consistent with the results of TRPL. All the photophysical properties and charge transport properties of CsPbI 2 Br, HTMs, and CsPbI 2 Br/ HTMs are summarized in Table S4.…”
Section: Resultssupporting
confidence: 83%
“…As shown in Figure f, the data were fitted based on the biexponential function, y 0 = A 1 exp­(− x /τ 1 ) + A 2 exp­(− x /τ 2 ), and the detailed parameters are summarized in Table S3. The fast time component (τ 1 ) can be explained as the charge carrier capture at the CsPbI 2 Br grain boundaries and CsPbI 2 Br/HTM interfaces. , The τ 1 of CsPbI 2 Br/PE61 is faster than that of CsPbI 2 Br/PBDB-T and CsPbI 2 Br/J52 samples, demonstrating the quickest traps filling in the CsPbI 2 Br/PE61 device. The second component (τ 2 ) can be interpreted as the hole injections from the CsPbI 2 Br into the HTMs .…”
Section: Resultsmentioning
confidence: 99%
“…36 In the control film, there was an obvious broadening of GSB, which could be divided into two peaks at 797 and 828 nm, and in the longer wavelengths of 850−950 nm, the negative signals indicated rich interband states that mainly derived from trap states or impurity phases. 37,38 We recorded TA decays of two split GSB peaks and the standard GSB peak at 797 nm of the target film, in Figure 5c. Regardless of 797 or 828 nm, their peaks decayed faster than the target GSB peak, which could be attributed to serious trap-assisted recombination in the control film.…”
Section: Resultsmentioning
confidence: 99%