S1
Supporting information of
Indene−C60 Bisadduct Electron Transporting Material with the
High LUMO Level Enhances Open-Circuit Voltage and Efficiency
of Tin-Based Perovskite Solar Cells
Myeongjeong Lee,†,‡ Dawoon Kim,†, ‡ Yong Kyu Lee,†,‡Hansol Koo,‡ Kyu Tae Lee,‡ and In
Chung*, †, ‡
†Center for Nanoparticle Research, Institute for Basic Science (IBS), Seoul 08826, Republic
of Korea
‡School of Chemical and Biological Engineering, and Institute of Chemical Processes, Seoul
National University, Seoul 08826, Republic of Korea
Corresponding Author
S2
Table S1. TRPL characteristics for the FA0.9PEA0.1SnI3 films without and with ETLs on a
ITO/PEDOT:PSS substrate.
Sample τ1 [ns] Ratio [%] τ2 [ns] Ratio [%] τave [ns]
Without ETL 3.1 34 10.7 66 8.1
ICBA 1.9 42 6.1 58 4.4
PCBM 1.8 48 5.8 52 3.9
C60 1.6 51 5.1 49 3.3
The PL decay curves of the samples were fitted with a bi-exponential decay model containing a fast and a slow decay processes.1-3 We consider the fast decay process is attributed
to the quenching of the photogenerated free carriers transporting from the perovskite layer to the PEDOT:PSS or ETLs, and the slow decay process originates from the radiative recombination of free carriers before charge collection. For the FA0.9PEA0.1SnI3 film on an
ITO/PEDOT:PSS substrate without ETL, the lifetime of fast (τ1) and slow decay (τ2) is 3.1 and
10.7 ns and the weight fraction is 34 and 66%, respectively. In addition to ETLs, PL lifetimes of the FA0.9PEA0.1SnI3 perovskite significantly decrease and the ratio of τ1 increases, showing
S3
Table S2. Photovoltaic parameters for FA0.9PEA0.1SnI3 solar cells with a different ETL of
ICBA, PCBM, and C60.
ETL VOC [V] JSC [mA cm2] FF [%] PCE [%]
ICBA Champion 0.651 16.88 64 7.05 Average 0.66 ± 0.01 16.16 ± 0.71 58.53 ± 1.40 6.27 ± 0.30 PCBM Champion 0.490 18.14 62 5.54 Average 0.48 ± 0.01 17.94 ± 0.63 60.91 ± 1.97 5.22 ± 0.38 C60 Champion 0.403 17.76 62 4.46 Average 0.40 ± 0.01 17.00 ± 0.88 62.12 ± 1.53 4.22 ± 0.26
The statistical data including average values standard deviations were calculated from 8 devices with a C60 and PCBM ETL, respectively, and 11 devices with an ICBA ETL.
S4
Table S3. Summary of photovoltaic parameters for the best performing FASnI3-based
perovskite solar cells previously reported and in this work.
Device structure ETL HTL Absorber VOC [V] JSC [mA cm2] FF [%] PCE [%] Ref.
p-i-n Ag C60/BCP PEDOT:PSS FASnI3-PVA 0.632 20.37 69.3 8.92 4
p-i-n Ag C60/BCP PEDOT:PSS GAxFA1-xSnI3
-EDAI2 0.619 21.2 72.9 9.6 5
p-i-n Ag C60/BCP PEDOT:PSS FA1-xMAxSnI3 0.61 21.2 62.7 8.12 6
p-i-n Ag C60/BCP PEDOT:PSS FASnI3-EDAI2 0.583 21.3 71.8 8.9 7
p-i-n Ag PCBM NiOx FASnI3-SnCl2 0.552 17.64 69.4 6.76 8
p-i-n Ag C60/BCP PEDOT:PSS FA1-xMAxSnI3 0.55 19.4 67 7.2 9
p-i-n Ag C60/BCP
PEDOT:PSS/PTN-Br FASnI3 0.57 20.66 67.4 7.94 10 p-i-n Al PCBM PEDOT:PSS FA1-x(PEA)xSnI3
-FASCN 0.53 22.5 68.3 8.17 11 p-i-n Ag C60/BCP PEDOT:PSS FA1-x(PEA)xSnI3 0.525 24.1 71 9 12
n-i-p Au TiO2 PTAA {en}FASnI3 0.48 22.54 65.96 7.14 13
n-i-p Au TiO2 benzodithiophene {en}FASnI3 0.497 22.41 68.21 7.59 14
p-i-n Ag C60/BCP PEDOT:PSS/LiF FA1-x(PEA)xSnI3 0.47 20.07 74 6.98 15
p-i-n Al ICBA/BCP PEDOT:PSS FA0.9(PEA)0.1SnI3 0.651 16.88 64 7.05 This
S5
Figure S1. XRD patterns of the FA0.9PEA0.1SnI3 films deposited on an ITO/PEDOT:PSS
S6
Figure S2. Typical top view SEM images of (a) FASnI3 and (b) FA0.9PEA0.1SnI3 perovskite
films deposited on an ITO/PEDOT:PSS substrate, shown in various magnifications. Red dotted circles in (a) indicate pinholes typically found in FASnI3 perovskite films. FA0.9PEA0.1SnI3
S7
Figure S3. (a) Tauc plots and (b) TRPL decay curves for the FA0.9PEA0.1SnI3 and FASnI3 films
S8
Figure S4. XRD patterns of the FA0.9PEA0.1SnI3 films deposited on an ITO/PEDOT:PSS
substrate without and with a respective ICBA, PCBM, and C60 ETL. The asterisk indicates the
S9
Figure S5. Absorbance spectra of the FA0.9PEA0.1SnI3 film deposited on ITO/PEDOT:PSS
S10
Figure S6. UPS data corresponding to (a) the secondary electron onset region and (b) valence
band region of the FA0.9PEA0.1SnI3 and ETL films. The UPS measurements were carried out
S11
Figure S7. J-V characteristics of FA0.9PEA0.1SnI3 solar cells with a variation in a thickness of
C60. On a top of C60, a 5 nm of BCP layer is thermally deposited. We found that the optimal
S12
Figure S8. J-V characteristics of FA0.9PEA0.1SnI3 solar cells with a variation in a revolution
per minute (RPM) of spin-coating for PCBM. On the top of PCBM, a 5 nm of BCP layer is thermally deposited. The deposition condition of a solution-processed PCBM was optimized by controlling RPM for spin-coating, and we found that 4000 rpm is the best condition.
S13
Figure S9. J-V characteristics of FA0.9PEA0.1SnI3/ICBA solar cells with a variation in a RPM
of ICBA spin coating. 5 nm of BCP is thermally deposited in onto ICBA layer. The RPM of a spin-coated ICBA layer was optimized to 4000 rpm.
S14
Figure S10. J-V characteristics of FA0.9PEA0.1SnI3 solar cells with respective ICBA, PCBM
and C60 ETL. A BCP layer with 5 and 10 nm was tested. A 10 nm thick BCP layer reduces
photovoltaic parameters mainly due to the serious charge accumulation occurring at the interface between the ETL and BCP layer.
S15
Figure S11. (a) Electrical impedance spectra (EIS) and (b) dark J-V curves of the
FA0.9PEA0.1SnI3 solar cells with a respective ICBA, PCBM and C60 ETL. Inset in (a) shows the
equivalent circuit employed in the Nyquist fitting, including the series resistance (Rs), transfer
16
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