10.1002/chem.201605693
Chemistry - A European Journal
COMMUNICATION
isopropoxide in ethanol was coated on FTO substrates by the spin-
coating method at 3000 rpm for 30 s, followed by a thermal treatment at
500 °C for 30 min, to make a TiO2 compact layer. The PbI2 layer was
formed on TiO2 compact layer by spin-coating 1 M PbI2 (99.9985%, Alfa
Aesar)/N,N-dimethylformamide (DMF, 99.9%, Alfa Aesar) solution at
Keywords: crystallization • film deposition • micrometer size •
thermal energy • perovskite solar cell
[1]
[2]
[3]
[4]
[5]
[6]
M. M. Lee, J. Teuscher, T. Miyasaka, T. N. Murakami, H. J. Snaith,
Science 2012, 338, 643-647.
-1
3000 rpm for 15 s and was kept at 100 °C for 5 min. Then, 10 mg mL
J. Burschka, N. Pellet, S. J. Moon, R. Humphry-Baker, P. Gao, M. K.
Nazeeruddin,M. Grätzel, Nature 2013, 499, 316-319.
L. Etgar, P. Gao, Z. Xue, Q. Peng, A. K. Chandiran, B. Liu, M. K.
Nazeeruddin,M. Grätzel, J. Am.Chem.Soc.2012, 134, 17396-17399.
J. M. Ball, M. M. Lee, A. Hey, H. J. Snaith, Energy Environ. Sci. 2013, 6,
1739-1743.
CH3NH3I solution in isopropanol (99.7%, Aldrich) or α-terpineol (TP, 96%,
Aldrich) were prepared and the substrate and CH3NH3I solution were
held at 200 °C for 2 minutes. To form perovskite layer, 150 μL of 10 mg
mL-1 CH3NH3I solution in isopropanol or α-terpineol were loaded on the
PbI2 layer for 40 s followed by spun at 4000 rpm for 20 s and annealed at
100 °C for 5 min. Hole transport material (HTM) was deposited on
perovskite layer by spin-coating at 4000 rpm for 30 s. The spin-coating
solution was prepared by dissolving 72.3 mg spiro-MeOTAD, 18 µL of a
stock solution of 500 mg mL-1 lithium bis(trifluoromethylsulphonyl)imide in
acetonitrile and 29 µL 4-tert-butylpyridine in 1 mL chlorobenzene. Finally,
to complete the device, 110 nm silver was thermally evaporated onto the
HTM layer as the back contact. The devices were left in a desiccator
overnight before tested. All the device fabrication process was carried out
under controlled atmospheric conditions.
A. Kojima, K. Teshima, Y. Shirai, T. Miyasaka, J. Am. Chem. Soc. 2009,
131, 6050-6051.
H. S. Kim, C. R. Lee, J. H. Im, K. B. Lee, T. Moehl, A. Marchioro, S. J.
Moon, R. Humphry-Baker, J. H. Yum, J. E. Moser, M. Grätzel, N. G.
Park,Sci. Rep.2012, 2, 591.
[7]
[8]
L. Qiu, S. He,J. Yang,J. Deng,H.Peng, Small 2016, 18, 2419-2424.
Z. Yuan, Z. Wu, S. Bai, Z. Xia, W. Xu, T. Song, H. Wu, L. Xu, J. Si, Y.
Jin,B. Sun,Adv.Energy Mater. 2015, 5, 1500038.
Y. Hou, S. Yang, C. Z. Li, H. J. Zhao, H. G. Yang, RSC Adv. 2016, 6,
83802-83807.
[9]
Characterization
[10] J. H. Im, C. R. Lee, J. W. Lee, S. W. Park, N. G. Park, Nanoscale 2011,
3, 4088-4093.
The XRD spectra of the as-synthesized crystals were investigated by
powder X-ray diffraction (XRD, Bruker D8 Advanced Diffractometer, Cu
Kα radiation, 40 kV). The morphology and structure of the samples were
characterized by field emission scanning electron microscopy (FESEM,
HITACHI S4800). The optical absorption spectra were measured by
using a Cary 500 Spectrophotometer. The current-voltage curves of solar
cells were performed using a solar light simulator (Oriel, 91160, AM 1.5
globe) and the power of the simulated light was calibrated to 100 mW cm-
[11] M. Liu,M. B. Johnston,H.J. Snaith, Nature 2013, 501, 395-398.
[12] J. H. Im, I. H. Jang, N. Pellet, M. Grätzel, N. G. Park, Nat. Nanotechnol.
2014, 9, 927-932.
[13] H. S. Rao, B. X. Chen, W. G. Li, Y. F. Xu, H. Y. Chen, D. B. Kuang, C.
Y. Su, Adv. Funct.Mater. 2015, 25, 7200-7207.
[14] E. Della Gaspera, Y. Peng, Q. C. Hou, L. Spiccia, U. Bach, J. J.
Jasieniak,Y.B. Cheng, Nano Energy 2015, 13, 249-257.
[15] T. Zhang,M. Yang, Y. Zhao,K. Zhu, Nano Lett. 2015, 15, 3959-3963.
[16] J. Shi, X. Xu, D. Li,Q. Meng, Small 2015, 11, 2472-2475.
[17] M. J. Yang, T. Y. Zhang, P. Schulz, Z. Li, G. Li, D. H. Kim, N. J. Guo, J.
J. Berry, K. Zhu,Y. X. Zhao, Nat. Commun.2016, 7,12305.
[18] W. Ma, A. Gopinathan,A.J. Heeger, Adv.Mater.2007, 19, 3656-3659.
[19] T. J. Huang, Z. X. Thiang, X. Yin, C. Tang, G. Qi, H. Gong, Chem. Eur.
J. 2016, 22,2146-2152.
2
using a Newport Oriel PV reference cell system (model 91150 V). All
tests were measured using a Keithley 2400 source meter. The active
area of the device was of 0.0625 cm-2.
Acknowledgements
[20] M. Zhang, M. Lyu, H. Yu, J. Yun, Q. Wang, L. Wang, Chem. Eur. J.
2015, 21,434-439.
This work was financially supported by National Natural Science
Foundation of China (21373083, 21573068 and 51602103), SRF
for ROCS, SEM, SRFDP, Fundamental Research Funds for the
Central Universities (WD1514301), China Postdoctoral Science
Foundation Funded Project (2015M581547, 2016T90342),
“Chen Guang” Project supported by Shanghai Municipal
Education Commission and Shanghai Education Development
Foundation (15CG26), the Major Research plan of the National
Natural Science Foundation of China (91534202), 111 Project
(B14018), Shanghai Sailing Program (16YF1402100) and ARC
Discovery Projects (DP150103775).
[21] Z. Xiao, Y. Yuan, B. Yang, J. VanDerslice, J. Chen, O. Dyck, G.
Duscher,J.Huang, Adv.Mater. 2014, 26, 3068-3075.
[22] Y. Hou, H. Qiao, S. Yang, C. Li, H. Zhao, H. G. Yang, Ind. Eng. Chem.
Res.2017, 56,524–529.
[23] X. Chen, L. Tang, S. Yang, Y. Hou, H. G. Yang, J. Mater. Chem. A
2016, 4, 6521-6526.
[24] X. Chen, S. Yang, Y. C. Zheng, Y. Chen, Y. Hou, X. H. Yang, H. G.
Yang, Adv.Sci. 2015, 2, 1500105.
[25] A. Yella, L. P. Heiniger, P. Gao, M. K. Nazeeruddin, M. Grätzel, Nano
Lett. 2014, 14, 2591-2596.
[26] M. Y. Chiu, U. Jeng, C. H. Su, K. S. Liang, K. H. Wei, Adv. Mater. 2008,
20,2573-2578.
This article is protected by copyright. All rights reserved.