2023
DOI: 10.1021/acs.jpcc.3c04362
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Surface Reconstruction for Efficient Cs2AgBiBr6 Solar Cells

Yu Zou,
Wenjin Yu,
Xiangdong Li
et al.

Abstract: Lead-free double perovskite Cs 2 AgBiBr 6 is considered to serve as a substitute for toxic lead-based perovskite components and is a promising candidate for environmentally friendly perovskite solar cells (PSCs). However, the high deep-level trap density in Cs 2 AgBiBr 6 films hinders the device performance, which is caused by the different solubilities of components in the precursor solution and the solutionprocess fabrication method. In this work, we reported a surface reconstruction (SR) strategy, in which … Show more

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Cited by 4 publications
(3 citation statements)
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“…In the majority of studies in the literature, the PL emission peak of Cs 2 AgBiBr 6 was broad and centered around 600–650 nm due to the domination of the PL spectra with indirect bandgap recombination. 39,44,45 However, in our case, the sample without the IL exhibited three emission peaks at ∼536, 606, and 676 nm. While the PL peak at 536 nm (2.31 eV) originated from the direct band gap emission of Cs 2 AgBiBr 6 , the other two emission peaks at 606 nm (2.04 eV) and 676 nm (1.83 eV) were indicative of phonon-assisted indirect band transitions, as observed in previous literature studies.…”
Section: Resultscontrasting
confidence: 55%
“…In the majority of studies in the literature, the PL emission peak of Cs 2 AgBiBr 6 was broad and centered around 600–650 nm due to the domination of the PL spectra with indirect bandgap recombination. 39,44,45 However, in our case, the sample without the IL exhibited three emission peaks at ∼536, 606, and 676 nm. While the PL peak at 536 nm (2.31 eV) originated from the direct band gap emission of Cs 2 AgBiBr 6 , the other two emission peaks at 606 nm (2.04 eV) and 676 nm (1.83 eV) were indicative of phonon-assisted indirect band transitions, as observed in previous literature studies.…”
Section: Resultscontrasting
confidence: 55%
“…The double-perovskite Cs 2 AgBiBr 6 , highly stable due to its high positive decomposition energy, is considered to be another promising candidate . Since the first report on Cs 2 AgBiBr 6 solar cells in 2017, many attempts have been made to optimize the optoelectronic properties of Cs 2 AgBiBr 6 PSCs, including using low-pressure assistance, , modulating the stoichiometric precursor ratio, , adding organic interface layers, changing charge transport layers, and employing inverted device structures . So far, the highest PCE achieved for the Cs 2 AgBiBr 6 PSC is 6.4%, managed by using a hydrogenation method to narrow its band gap …”
Section: Introductionmentioning
confidence: 99%
“…29,30 In addition, their relatively large bandgap for single-junction PSCs and indirect bandgap are also detrimental to solar energy harvesting. 31–34…”
Section: Introductionmentioning
confidence: 99%