2020
DOI: 10.34133/2020/2616345
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Origin of High Efficiency and Long-Term Stability in Ionic Liquid Perovskite Photovoltaic

Abstract: Environment-friendly protic amine carboxylic acid ionic liquids (ILs) as solvents is a significant breakthrough with respect to traditional highly coordinating and toxic solvents in achieving efficient and stable perovskite solar cells (PSCs) with a simple one-step air processing and without an antisolvent treatment approach. However, it remains mysterious for the improved efficiency and stability of PSCs without any passivation strategy. Here, we unambiguously demonstrate that the three functions of solvents,… Show more

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Cited by 69 publications
(70 citation statements)
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“…This phenomenon explains why in Figure 3c, the reference peak becomes sharper within the first 40 s. Subsequently, Acwas gradually substituted by Xand then expelled to the grain boundaries, resulting in the formation of [SnX 6 ] 4− octahedra. [18,30] At the same time, BA + was also discharged on the film surface along with the crystal growth process. [31] This evolutionary process is reflected in Figure 3d, where the splitting left peak gradually decreases with the annealing time and the right peak gradually increases.…”
Section: Resultsmentioning
confidence: 99%
“…This phenomenon explains why in Figure 3c, the reference peak becomes sharper within the first 40 s. Subsequently, Acwas gradually substituted by Xand then expelled to the grain boundaries, resulting in the formation of [SnX 6 ] 4− octahedra. [18,30] At the same time, BA + was also discharged on the film surface along with the crystal growth process. [31] This evolutionary process is reflected in Figure 3d, where the splitting left peak gradually decreases with the annealing time and the right peak gradually increases.…”
Section: Resultsmentioning
confidence: 99%
“…[90,91] Correspondingly, the MA film is easier to form gaseous products, likely NH 3 , HI, I 2 , and desorb from the film surface under the extreme condition. [92][93][94] The CsFAMA film showed the most stable against light illumination in UHV among these three kinds of films, attributed to that the Cs could shrink the perovskite lattice and accumulate on the film surface as a defense against light-induced degradation. [95] What is more, the chemical and structural characterizations of the chosen unstable MA perovskite film under UHV and dark condition were performed.…”
Section: High Vacuum With Light Illuminationmentioning
confidence: 99%
“…Based on the XRD and UV–vis measurements, we conclude that MA + DFA − does not affect the crystal structure and bandgap of the perovskite films, and thus it is inferred that MA + DFA − can only be located at the grain boundaries and/or surfaces of the films rather than inside the crystal lattice itself. [ 29 ] Time‐resolved photoluminescence (TRPL) with an excitation wavelength of 500 nm and transient absorption spectra (TAS) with an excitation wavelength of 400 nm are used to study the recombination kinetics of perovskite films without and with MA + DFA − . As shown in Figure 3f, the perovskite films with MA + DFA − exhibit a longer lifetime (226.89 ns) compared with the control sample (193.93 ns), indicating the suppression of nonradioactive recombination in the perovskite film with MA + DFA − .…”
Section: Figurementioning
confidence: 99%