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Journal of the American Chemical Society
foxide to deposit a uniform CH3NH3PbI3 (=MAPbI3) layer.21 The
OMeTAD devices exhibit dramatically enhanced performance
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cell was fabricated by spin coating a layer of MAPbI3 onto the
mp–TiO2 surface, followed by drying at 100 °C. Spin coating of
the pp–, pm–, and po–spiro–OMeTAD as HTMs was accomꢀ
plished with Li–bis(trifluoro–methanesulfonyl)imide (Li–TFSI),
and 4–tert–butyl pyridine (t–BP) dissolved in toluene. In this
study, we did not incorporate hole dopants like tris[2–(1H–
and the performance of cells fabricated from pm–spiro–OMeTAD
is inferior to that of pp–spiro–OMeTAD. In Figure 3a, a small
difference in Jsc and Voc among pp–, pm–, and po–spiro–
OMeTAD derivatives with a large difference in FF is observed.
Generally, in solar cells, series resistance (Rs) reduces the FF, but
does not affect Voc and Jsc, if it is not excessively high values. A
straightforward method of estimating the Rs from a solar cell is to
find the slope of the JꢀV curve near the open–circuit voltage. As
shown in the Rs determined from the slope of Table 1, po–spiro–
OMeTAD–based cells showed lowest Rs of 32.96 ꢁ, whereas the
pp– and pm–spiro–OMeTAD showed Rs of 45.37 ꢁ and 64.42 ꢁ,
respectively. Besides Rs, the FF is also related to shunt resistance
(Rsh). In perovskite–based solar cells consisting of mp–TiO2–
perovskite composite/perovskite layer/HTM/Au, the HTM funcꢀ
tions as both hole–transporting and electron–blocking layer.3 po–
spiro–OMeTAD having the highest LUMO will block electron
flow into the metal electrode, which is responsible for increased
Rsh. Therefore, po–spiro–OMeTAD effectively blocks the elecꢀ
tron and transports the hole from MAPbI3 to the Au electrode.
Accordingly, the superior performance of po–spiro–OMeTAD
may be rationalized in terms of the increased FF value through a
low Rs and a high Rsh. However, further studies are needed to
quantify the extent of this effect among pp–, pm–, and po–spiro–
OMeTAD. Figure 3b shows monochromatic incident photon conꢀ
version efficiency (IPCE) spectrum for the cells fabricated using
pp–, pm–, po– and commercial pp–spiro–OMeTAD, and the inteꢀ
grated photocurrent densities are in good agreement with the valꢀ
ues measured in J–V curves, although the IPCE spectra differs
slightly with wavelength.
pyrazol–1–yl)–4–tert–butylpyridine)cobalt(III)
tris(bis
(tri–
fluoromethylsulfonyl)imide)] (FK209) because we can fabricate
the cells with a very thin layer of spiro–OMeTAD. The same
concentration of spiroꢀOMeTAD derivatives/toluene solutions for
HTMs were used to keep very similar thickness them as overlayer
on the perovskite. Finally, Au electrode was deposited on the top
by thermal evaporation to complete the solar cell structure. Figure
2d shows cross–sectional image of the representative solar cell
device fabricated in this work, as observed by a scanning electron
microscopy (SEM). As can be seen, the MAPbI3 perovskite forms
a thin capping layer of about 350 nm with full infiltration into ~
250ꢀnmꢀthick mp–TiO2 and a spiro–OMeTAD overlayer (~70
nm). The thickness of The thicknesses of the pp, pm, and po overꢀ
layers were almost similar, as estimated by same molecular
weight. The gold contact on top of this organic conductor is also
observed. In Figure 2c, the band alignment in TiO2, MAPbI3, and
spiro–OMeTAD derivatives can be observed. The band alignment
is such that the exciton dissociation and charge transfer at the
interface are energetically favorable with possible driving force
for a hole transfer from the MAPbI3 into the spiro–OMe derivaꢀ
tives. Therefore, free charge carriers (or excitons) generated from
the MAPbI3 layer can be extracted (or dissociated) by transferring
an electron to the underlying mp–TiO2 layer through hole transfer
to the spiro–OMeTAD HTM. However, there was a large hystereꢀ
sis and distortion in the J–V curves in the reverse (from the open
circuit voltage (Voc) to the short circuit current (Isc)) and forward
(i.e. from Isc to Voc) modes under standard air–mass 1.5 global
(AM 1.5G) illumination for the perovskite–based solar cells, esꢀ
pecially when it is measured at relatively short delay times.21 Such
hysteresis and discrepancy leads to over– or under–evaluated
performance which induces a considerable error in measuring the
cell efficiency. This is because reliable solar cell J–V measureꢀ
ments should exhibit coincident curves from the forward and reꢀ
verse directions. Figure S2 shows the variation of energy converꢀ
sion efficiency for representative solar cell (using poꢀspiroꢀ
OMeTAD as HTM), measured by forward and reverse scans with
10 mV voltage steps and a delay time of 100 ms. Serious hystereꢀ
sis is observed between both the scan directions with different
performance; the efficiency in the reverse scan is 17.6%, while it
is 14.1% in the forward scan. The efficiency measured by both the
scan directions decreases and increases symmetrically with inꢀ
creasing delay time and then matched at 1000 ms, but average
value remains almost the same after 300 ms (see supplemental
Figure S3). Therefore, in this work, we showed current density–
voltage (J–V) curves by averaging J–V curves obtained in both the
scan directions with a delay time of 300 ms, because an excesꢀ
sively long measurement time is impractical.
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Table 1. Average photovoltaic parameters for reverse and forꢀ
ward scanedꢀMAPbI3 perovskite solar cells using commercial,
pmꢀ, poꢀ, and ppꢀspiroꢀOMeTAD as HTMs
100
(a)
(b)
20
)
80
60
40
20
0
15
(
Commercial
Commercial
pp
pm
po
pp
pm
po
10
5
0
0.0
0.2
0.4
0.6
0.8
1.0
300
400
500
600
700
800
Wavelength (nm)
Voltage (V)
With this in mind, we compared the photovoltaic performance of
the cells fabricated using pp–, pm–, and po–spiro–OMeTAD deꢀ
Figure 3. (a) Current density–voltage (J–V) curves for
TiO2/MAPbI3/HTMs/Au fabricated with ppꢀ, pmꢀ, poꢀ and comꢀ
mercial ppꢀspiroꢀOMeTAD as HTMs. (b) the corresponding IPCE
spectra.
rivatives.
Figure
3a
shows
J–V
curves
for
TiO2/MAPbI3/HTMs/Au solar cells fabricated using three HTMs
and the photovoltaic parameters of these devices are summarized
in Table 1. In all the cases, overlayer thickness of ~70 nm was
observed in the SEM measurement (see Figure 2d). The device
comprising of mp–TiO2/MAPbI3/pp–Spiro–OMeTAD gave an
open–circuit voltage (Voc) of 1.00 V, a short–circuit current densiꢀ
ty (Jsc) of 20.7 mA cm–2, a fill factor (FF) of 71.1 %, and an overꢀ
all conversion efficiency (η) of 14.9 %. These values are compaꢀ
rable and the cell performance is similar to that of the cells fabriꢀ
cated with commercial pp–spiro–OMeTAD (Merck), as reported
by Gratzel et al.5 In contrast, the cells fabricated with po–spiro–
In summary, we synthesized pp–, pm– and po–spiro–OMeTAD
derivatives that were applied as HTMs to the MAPbI3 pervoskite–
based solar cells. Based on the CV measurements and UV–Vis
spectra, the HOMO/LUMO energy levels of each derivative were
characterized. The derivatives were used to fabricate feasible
perovskite–based solar cells. Energy conversion efficiencies of
16.7% were obtained, which is the highest value reported till date
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