Despite the rapid progress made in the field of perovskite solar cells, their instability remains a major obstacle for commercialization. Here, focus is placed on the stability of CH3NH3PbI3 solar cells on polymer substrates and the understanding of the factors influencing device degradation. A range of storage conditions is used, parameters such as light or temperature are isolated, and their impacts on the perovskite film examined. The severe loss in device performance is not predominantly correlated to the perovskite film deterioration, which implies that the device failure originates elsewhere. This study demonstrates that the hole transport material plays a significant role in the device degradation, and thus its optimization or removal can potentially lead to enhanced device lifetime. (C) 2016 Elsevier Ltd. All rights reserved.

Parameters responsible for the degradation of CH3NH3PbI3-based solar cells on polymer substrates

Benesperi, I;
2016-01-01

Abstract

Despite the rapid progress made in the field of perovskite solar cells, their instability remains a major obstacle for commercialization. Here, focus is placed on the stability of CH3NH3PbI3 solar cells on polymer substrates and the understanding of the factors influencing device degradation. A range of storage conditions is used, parameters such as light or temperature are isolated, and their impacts on the perovskite film examined. The severe loss in device performance is not predominantly correlated to the perovskite film deterioration, which implies that the device failure originates elsewhere. This study demonstrates that the hole transport material plays a significant role in the device degradation, and thus its optimization or removal can potentially lead to enhanced device lifetime. (C) 2016 Elsevier Ltd. All rights reserved.
2016
22
211
222
http://www.sciencedirect.com/science/article/pii/S2211285516000665
Solar cell stability; Perovskite; Temperature; Illumination; Hole transport material
Dkhissi, Y; Weerasinghe, H; Meyer, S; Benesperi, I; Bach, U; Spiccia, L; Caruso, RA; Cheng, YB
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2318/1887393
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