2019
DOI: 10.1007/s10971-019-04957-w
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Perovskite solar cells free of hole transport layer

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Cited by 12 publications
(6 citation statements)
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“…The preparation methods for each film are described in the experimental section. As can be seen in the figures, we were able to confirm that the MAPbI 3 films were successfully fabricated 38,39 and the diffraction peaks originating from PEAI were found in MAPbI 3 / PEAI. [40][41][42] However, due to the thinness of the ZnO layer in MAPbI 3 /ZnO, the diffraction peaks arising from ZnO could not be observed.…”
Section: Resultssupporting
confidence: 68%
“…The preparation methods for each film are described in the experimental section. As can be seen in the figures, we were able to confirm that the MAPbI 3 films were successfully fabricated 38,39 and the diffraction peaks originating from PEAI were found in MAPbI 3 / PEAI. [40][41][42] However, due to the thinness of the ZnO layer in MAPbI 3 /ZnO, the diffraction peaks arising from ZnO could not be observed.…”
Section: Resultssupporting
confidence: 68%
“…In recent studies, using pin-holes in the HTL has resulted in poor stability of PSCs. Oxygen and moisture in the environment can penetrate through pin-holes and degrade the perovskite absorbent layer; however, the reason for producing pin-holes in HTL is still unclear [29]. To solve this problem, many studies have focused on developing efficient PSCs and new types of hole-transport materials as an alternative to Spiro-OMeTAD [30], or HTL-free PSCs, which are appropriate for simplifying the optimal process of the device, preventing perovskite degradation, and reducing the costs [31].…”
Section: Introductionmentioning
confidence: 99%
“…Furthermore, the weak diffraction peaks detected at 28° and 35° were assigned to ( 200) and ( 213) planes of the cubic structure of CH3NH3PbI3 [17]. The diffraction peaks of belonging PbI2 at 12.70° and 39.58° were not observed due to PbI2 and CH3NH3I completely reacting [13].…”
Section: Xrd and Ftir Results Of Perovskite Thin Filmmentioning
confidence: 93%
“…Afterwards, the perovskite mother solution has been filtered through a 0.45μm PVDF filter and the solution colour turned from dark yellow to light yellow. The perovskite precursor solution was fabricated on an ITO substrate by the using spin coating method at 2000 rpm for 30 sec in a nitrogen medium [13]. The coated glasses were annealed for 60 minutes at 100 °C in a nitrogen medium.…”
Section: Device Preparation Proceduresmentioning
confidence: 99%