Tuning the Fermi-level of TiO mesoporous layer by lanthanum doping towards efficient perovskite solar cells

Tuning the band alignment is proved to be an effective way to facilitate carrier transportation and thus enhance the power conversion efficiency (PCE) of solar cells. Doping the compact layer with metal ions or modifying the interfaces among functional layers in perovskite solar cells (PSCs) can app...

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Published inNanoscale Vol. 8; no. 38; pp. 16881 - 16885
Main Authors Gao, Xiao-Xin, Ge, Qian-Qing, Xue, Ding-Jiang, Ding, Jie, Ma, Jing-Yuan, Chen, Yao-Xuan, Zhang, Bao, Feng, Yaqing, Wan, Li-Jun, Hu, Jin-Song
Format Journal Article
Published 29.09.2016
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Summary:Tuning the band alignment is proved to be an effective way to facilitate carrier transportation and thus enhance the power conversion efficiency (PCE) of solar cells. Doping the compact layer with metal ions or modifying the interfaces among functional layers in perovskite solar cells (PSCs) can appreciably improve the PCE of PSCs. Inspired by the rare earth elemental doping of TiO 2 , which has witnessed the success in photocatalysis and dye-sensitized solar cells, we firstly demonstrated here that La 3+ doping in the mesoporous TiO 2 layer of a mesostructured PSC can tune its Fermi level and thus significantly enhance the device PCE. Systematic analysis reveals that doping La 3+ into TiO 2 raises the Fermi level of TiO 2 through scavenging oxygen and inducing vacancies, which subsequently increases the open circuit voltage and the fill factor while reducing the series resistance of the PSC using La 3+ -doped TiO 2 as a mesoporous layer. As a result, a PCE of 15.42% is achieved, which is appreciably higher than the PCE of a device with undoped TiO 2 (12.11%). Tuning the Fermi-level of TiO 2 mesoporous layer by lanthanum doping is demonstrated as an effective way to significantly enhance the power conversion efficiency of perovskite solar cells.
Bibliography:Electronic supplementary information (ESI) available: Experimental methods, AFM image and UV-vis spectra. See DOI
10.1039/c6nr05917a
ISSN:2040-3364
2040-3372
DOI:10.1039/c6nr05917a