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dc.contributor.authorIsoe, Wycliffe
dc.contributor.authorMageto, Maxwell
dc.contributor.authorMaghanga, Christopher
dc.contributor.authorMwamburi, Maurice
dc.contributor.authorOdari, Victor
dc.contributor.authorAwino, Celline
dc.date.accessioned2021-07-07T13:22:14Z
dc.date.available2021-07-07T13:22:14Z
dc.date.issued2020-07-28
dc.identifier.urihttps://doi.org/10.1155/2020/8877744
dc.identifier.urihttps://www.hindawi.com/journals/ijp/2020/8877744/
dc.identifier.urihttp://r-library.mmust.ac.ke/123456789/1753
dc.description.abstractCH3NH3PbI3-xClx has been studied experimentally and has shown promising results for photovoltaic application. To enhance its performance, this study investigated the effect of varying thickness of FTO, TiO2, and CH3NH3PbI3-xClx for a perovskite solar cell with the structure glass/FTO/TiO2/CH3NH3PbI3-xClx/Spiro-OMeTAD/Ag studied using SCAPS-1D simulator software. The output parameters obtained from the literature for the device were 26.11 mA/cm2, 1.25 V, 69.89%, and 22.72% for Jsc, Voc, FF, and , respectively. The optimized solar cell had a thickness of 100 nm, 50 nm, and 300 nm for FTO, TiO2, and CH3NH3PbI3-xClx layers, respectively, and the device output were 25.79 mA/cm2, 1.45 V, 78.87%, and 29.56% for Jsc, Voc, FF, and , respectively, showing a remarkable increase in FF by 8.98% and 6.84% for solar cell efficiency. These results show the potential of fabricating an improved CH3NH3PbI3-xClx perovskite solar cell.en_US
dc.language.isoenen_US
dc.publisherInternational Journal of Photoenergyen_US
dc.subjectThickness, Dependence, Window, Layer ,CH3NH3PbI3-XClX ,Perovskite, Solar, Celen_US
dc.titleThickness Dependence of Window Layer on CH3NH3PbI3-XClX Perovskite Solar Celen_US
dc.typeArticleen_US


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