Sn/Pb binary perovskite solar cells and organic amine-free perovskite solar cells
Shuzi Hayase a, Keita Sakaguchi a, Kosei Fujiwara a, Koji Nishimura a, Yuhei Ogomi a, Qing Shen b, Taro Toyoda b
a Kyushu Institute of Technology, Japan, 204 Hibikino Wakamatsu-ku, Kitakyushu - Fukuoka, 808, Japan
b The University of Electro-communications, 1-5 Chofugaoka, Chofu, Yokyo, Japan
International Conference on Hybrid and Organic Photovoltaics
Proceedings of International Conference on Hybrid and Organic Photovoltaics 2015 (HOPV15)
Roma, Italy, 2015 May 11th - 13th
Organizer: Filippo De Angelis
Oral, Shuzi Hayase, presentation 060
Publication date: 5th February 2015
IPCE edge of Pb perovskite solar cell (MAPbI3 solar cells, (MAPb solar cells), MA: methyl ammonium cation) is about 800nm.  In order to increase the efficiency, we have to enhance open circuit voltage (Voc), short circuit current(Jsc), and fill factor(FF).  We focused on the enhancement of Jsc.  We calculated the relationship between Voc loss and the efficiency, and concluded that the highest efficiency is obtained by cultivating light up to 1000nm with the assumption of 0.3 Voc loss which is expected for the MAPb solar cell.  We have already reported Sn/Pb(1:1) binary perovskite solar cells (MASn0.5Pb0.5I3) covering up to 1040nm(1). The internal quantum efficiency of the Pb/Sn binary perovskite solar cell was high (74%) at 934 nm (Fig.1).  The advantage of Pb/Sn binary perovskite solar cells is the improved stability in air, compared with Sn perovskite solar cell.  We found that the binary Sn/Pb perovskite without hole transport layer has unique longer carrier life time (m second) than that of MAPb perovskite. The crystal defect of the Sn/Pb binary perovskite solar cells was compared with that of MAPb by employing Urbach energy. The Sn/Pb binary perovskite layer has higher Urbach energy (34 meV) than the MAPb perovskite layer (22 meV), suggesting that the former has larger crystal defects than the latter.  We found that Sn/Pb(1:1) binary perovskite layer has gradient structures from the bottom (titania layer) to the top layer.  The top layer (capping layer of perovskite layer) has lower Sn content (Sn/Pb = 0.6) than that of the bottom layer in porous titania (Sn/Pb=1.2). The long carrier life time of the binary perovskite was explained by the gradient structure in spite of the large defect density. The gradient structure is discussed from the view point of surface passivation on porous tiania by the perovskite material. Hysteresis for I-V curve is one of the unique characteristics of MAPbI3 perovskite solar cells.  Dipole of MA has been reported to be one of the causes of the hysteresis.  We report photovoltaic performances and hysteresis of organic amine free-all inorganic perovskite solar cells. We concluded that hysteresis occurred for the perovskite solar cells without MA.  The cause of the hyteresis is discussed.
Fig.1. Internal quantum efficiency for Sn/Pb binary perovskite solar cells coupled with P3HT hole transport layer
1. Y. Ogomi, S. Hayase, et al., J. Phys. Chem. C, 2014, 118, 16651-16659; Y. Ogomi, S. Hayase, et al., J. Phys.Chem. Lett. 2014, 5, 1004-1011; Y. Ogomi, S. Hayase et al., Chem. Phys. Chem. 2014, 15, 1062-1069.
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