Room-temperature photocurrent measurements in two-dimensional (2D) inorganic-organic perovskite devices reveal that excitons strongly contribute to the photocurrents despite possessing binding energies over 10 times larger than the thermal energies. The p-type (C6H9C2H4NH3)2PbI4 liberates photocarriers at metallic Schottky aluminum contacts, but incorporating electron- and hole-transport layers enhances the extracted photocurrents by 100-fold. A further 10-fold gain is found when TiO2 nanoparticles are directly integrated into the perovskite layers, although the 2D exciton semiconducting layers are not significantly disrupted. These results show that strong excitonic materials may be useful as photovoltaic materials despite high exciton binding energies and suggest mechanisms to better understand the photovoltaic properties of the related three-dimensional perovskites.
Room-temperature photocurrent measurements in two-dimensional (2D) inorganic-organic perovskite devices reveal that excitons strongly contribute to the photocurrents despite possessing binding energies over 10 times larger than the thermal energies. The p-type (C6H9C2H4NH3)2PbI4 liberates photocarriers at metallic Schottky aluminum contacts, but incorporating electron- and hole-transport layers enhances the extracted photocurrents by 100-fold. A further 10-fold gain is found when TiO2 nanoparticles are directly integrated into the perovskite layers, although the 2D exciton semiconducting layers are not significantly disrupted. These results show that strong excitonic materials may be useful as photovoltaic materials despite high exciton binding energies and suggest mechanisms to better understand the photovoltaic properties of the related three-dimensional perovskites.
Recently, lead halide based inorganic–organic
(IO) hybrid perovskite materials have emerged as one of the most promising
absorber materials for solar cells. Among these perovskites, in particular,
the three-dimensional (3D) perovskite materials CH3NH3PbI3 and CH3NH3PbI3–Cl have been studied
as photoresponsive materials in dye-sensitized architectures.[1−7] The power conversion efficiencies (PCEs) have seen unprecedented
growth from below 10% in 2012[1,2] to above 20% by the
end of 2014,[3,4] owing to excellent light-harvesting
capabilities over the visible-to-near-IR spectrum due to the narrow
band gap (1.5 eV). In 3D perovskite-based solar cells, it is predominantly
free charge carriers that are generated and are responsible for the
photovoltaic operation rather than the excitons (which have a binding
energy of ∼50 meV).[8] However, the
related series of two-dimensional (2D) perovskites possess much stronger
2D excitons and are thus normally considered to be of little use for
light harvesting. Here we study the photovoltaic properties of 2D
perovskites and show that, despite severe barriers to carrier transport
between layers, the excitons are efficient light harvesters.The 2D perovskites are part of the generic family of metal–organic
frameworks with well-organized structural properties,[9,10] represented by the general formula (RNH3)2MX4 where R is an organic cation, M is a divalent metal
(such as Pb2+, Sn2+, Hg2+, etc.),
and X is a halogen (such as I–, Br–, or Cl–). The basic crystal packing of these hybrids
is a naturally self-assembled layered structure, where single sheets
of corner-shared MX6 octahedra and bilayers of organic
cations are stacked alternately along the c axis
(Figure a).[11−14] The interlayer separation and thickness of the inorganic layers
can be controlled through the choice of amine-based organic cations.[15] The spatial quantum confinement of the 2D sheets
leads to strongly bound excitons because of large differences in the
band gaps of inorganic (∼2 eV) and insulating organic (∼4
eV) layers as well as their large dielectric mismatch (εorg < εinorg).[16] The binding energy EB of the Wannier–Mott
excitons in 2Dperovskite systems thus ranges from 200 to 300 meV.[17−22]
Figure 1
(a)
Schematic crystal structure of 2D perovskite (C6H9C2H4NH3)2PbI4.[14] (b) X-ray diffraction pattern of a
CHPI thin film revealing a 2D-layered arrangement. (c) Schematic and
(d) corresponding band diagram of the photodetector configuration 1 [Al/CHPI/ITO].
(a)
Schematic crystal structure of 2Dperovskite(C6H9C2H4NH3)2PbI4.[14] (b) X-ray diffraction pattern of a
CHPI thin film revealing a 2D-layered arrangement. (c) Schematic and
(d) corresponding band diagram of the photodetector configuration 1 [Al/CHPI/ITO].Such tightly bound excitons are difficult to dissociate into
free charge carriers at room temperature (because EB ∼ 10kBT), and hence free charge carriers are not likely to reach the electron/hole
selective contacts. However, our data here clearly show that this
is not generally the case and that, by the incorporation of suitable
electron and hole conducting layers, the transport of excitons across
the heterojunction can be manipulated. The purpose of the present
study is to explore the photoresponse in 2D perovskites and understand
this induced carrier transport. Our work suggests pathways to new
device structures and opens possibilities for the further optimization
of devices and photovoltaic functionality.
Experimental
Section
Fabrication
To study the photocurrent properties in
detail, three different device configurations are fabricated. In each
case, the 2DIO perovskite(C6H9C2H4NH3)2PbI4 (hereafter
CHPI) is used as the photoresponsive material. For “base”
configuration 1 (see Methods in the Supporting Information), CHPI is spun onto an indium tin oxide
(ITO) anode and overcoated with evaporated aluminum or gold [Al/CHPI/ITO
or Au/CHPI/ITO] (Figure c). The fabrication details of other configurations, 2 [Au/HTL/CHPI/c-TiO2/FTO] and 3 [Au/HTL/CHPI/mp-TiO2/c-TiO2/FTO], are shown in the Supporting Information (see Methods). The effective area of
all fabricated configurations is fixed to 9 mm2.
Characterization
Spectral and transient
photocurrent measurements are carried out using a potentiostat (Autolab
and/or Ivium compactstat.e) and xenon lamp source (Bentham, 75 W)
coupled to a monochromator (TMc 300, Bentham). To perform power-dependent
photocurrent measurements, a 410 nm diode laser (∼100 mW, continuous
wave) is used separately in the same setup. A Leo variable-pressure
scanning electron microscope is used for cross-sectional scanning
electron microscopy (SEM) images of configurations 2 and 3.
Results and Discussion
Room-Temperature Exciton
Photocurrent Response of 2D Perovskites
We first study the
photogenerated charge-carrier properties of the 2Dperovskite CHPI,
in configuration 1, without any electron- and hole-transport
materials. In CHPI, the alternating stacks of 2D organic and inorganic
layers (c-oriented) resemble natural multiple-quantum-well
(MQW) structures (Figure a,b). The lowest-energy excitons reside in the inorganic MQW
sheets and are stable at room temperature with large 300 meV binding
energy.[10,23−30] The transient photocurrent response is observed upon room-temperature
illumination through the transparent ITO electrode (Figure c). To identify the origin
of the photocurrent, spectral scans are measured over a wide wavelength
range from 210 to 1100 nm (Figure S1a in the Supporting Information). Figure d represents the energy-level diagram of configuration 1.The photocurrent spectral response of CHPI in configuration 1 is compared with the absorption and photoluminescence (PL)
spectra of a bare CHPI film (Figure a). The origin of this photocurrent can be explained
by considering the energy-level diagram (Figure b). Essentially the response is comprised
of two regions: (a) a broad response from 300 to 475 nm and (b) a
strong narrow exciton band peaking at 521 nm [with full width at half-height
(fwhm) = 20 nm]. The broad region can be directly correlated to the
band-to-band (BB) and charge-transfer (CT) absorption transitions
(Figure b), and indeed
the band edge from the photocurrent (2.46 eV) closely matches the
optical absorption band edge. Absorbed photons generate charge carriers
in the perovskite material, and the built-in potential at the Schottky
interfaces (perovskite–metal and ITO–perovskite) allows
collection of photogenerated carriers at the respective electrodes
(Figure d).[31,32] Similarly, the narrow photocurrent band at 521 nm matches the exciton
peak in absorption and is attributed to bound excitons (Figure a). The 10 nm red shift of
the photocurrent peak from the absorption peak arises partly because
the absorption depth (<100 nm) is shorter than the CHPI thickness
(∼800 nm),[23] so that only the longer
wavelengths can generate excitons near the CHPI–metal contact.
However, additional dissociation energies as well as thermalization
effects are involved,[33] depending on the
carrier mobilities and metal work functions.
Figure 2
(a) Comparison of the
photocurrent spectrum (1 V bias) with the absorption and PL spectra
of a bare CHPI thin film. (b) Schematic energy-level band diagram
indicating the BB, CT, and exciton bands within the inorganic and
organic moieties of a 2D IO perovskite, CHPI.
(a) Comparison of the
photocurrent spectrum (1 V bias) with the absorption and PL spectra
of a bare CHPI thin film. (b) Schematic energy-level band diagram
indicating the BB, CT, and exciton bands within the inorganic and
organic moieties of a 2DIO perovskite, CHPI.The observation of such spectrally narrow strong exciton-related
photocurrents at room temperature is unusual in solution-processed
semiconductor films. One puzzle is how excitons trapped on individual
sheets, which are separated by high insulating barriers, can lead
to photocurrent. Mitzi et al. studied inorganic–organic field-effect
transistors (IOFETs) of spin-coated 2Dperovskite films [(C6H5C2H4NH3)2SnI4], showing that the geometry of well-separated inorganic
sheets is ideal for lateral charge transport, which depends on the
size of the grains in the polycrystalline film.[11,34] This is less relevant when vertical transport across the layers
is required as it is here, unless polycrystalline misorientation leads
to interlayer conduction at grain boundaries. Hence, morphology effects
must play a crucial role in the transport of charge carriers in such
polycrystalline-layered materials.The room-temperature transient
photocurrent response is further investigated by measuring its dynamics
within both the BB (410 nm) and exciton (521 nm) regions. The IO perovskite
exhibits a much faster (100-fold) rise in the photocurrent upon exciton
illumination at 521 nm (Figure a) compared to that upon BB (410 nm) illumination. Similarly,
much faster photocurrent decay is visible from 521 nm illumination
compared to 410 nm illumination (Figure b). Because similar photocurrent magnitudes
are generated under 410 and 521 nm excitation and the absorptions
are similar, this suggests that both photocarrier species contribute
equally to the photocurrents measured in these 2D IO perovskites when
fabricated in configuration 1. However, distribution
of the photocarriers and excitons may be rather different in the two
situations, and most likely excitons are field-ionized in the immediate
vicinity of the contacts (see below).
Figure 3
Transient photocurrent response of CHPI
in configuration 1 showing (a) rise and (b) fall time
profiles with the BB or CT region (410 nm) and exciton (521 nm) illumination
under +1 V bias. Shaded regions show when the laser is OFF. (c) Comparison
of room-temperature photocurrent spectral responses in CHPI and parent
PbI2 thin films.
Transient photocurrent response of CHPI
in configuration 1 showing (a) rise and (b) fall time
profiles with the BB or CT region (410 nm) and exciton (521 nm) illumination
under +1 V bias. Shaded regions show when the laser is OFF. (c) Comparison
of room-temperature photocurrent spectral responses in CHPI and parent
PbI2 thin films.The influence of quantum and dielectric confinement can be
further investigated by comparing the photocurrents from CHPI and
the parent PbI2 compound, integrated as a film within the
same photodetector configuration. This parent network PbI2 material is also a layered direct-band-gap semiconductor (Eg ∼ 2.55 eV), with a layer-to-layer separation
of ∼7 Å.[35] During the formation
of CHPI, PbI2 structurally exfoliates as the organics intercalate
inside the PbI42– extended network, increasing
the layer spacing to >20 Å.[36] Because
the exciton binding energies are substantially lower (∼30 meV)
in the parent PbI2, the optical exciton features are only
observed at low temperature.[37] Room-temperature
photocurrent measurements are performed on samples with PbI2 films as the active layer [Al/PbI2/ITO] and compared
to CHPI (Figure c).
Both devices exhibit a broad photocurrent response in the energy region
(400–500 nm) associated with BB transitions.[38,39] However, unlike CHPI, photocurrent spectra of the PbI2 films do not show any signature of the excitonic features near 521
nm. This experiment confirms the surprising result that the narrow
photocurrent peak in CHPI at 521 nm originates solely from photocarriers
associated with exciton transitions in the 2D organic–inorganic
perovskite well structures. We also confirm that the photocurrent
is linear in illumination power (Figure S1b in the Supporting Information), with only a weak nonlinear component,
suggesting that no cooperative mechanism is involved.[40]To explore the competing roles of electron–hole
photocarriers and exciton photocurrents, the bias-dependent response
is studied in configuration 1 at room temperature, up
to +2.0 V (Figure a). Surprisingly, the photocurrent peak in these 2Dperovskite structures
exhibits strong blue shifts (∼55 meV) at high-bias conditions.[41−43] This observation differs from that in typical inorganic MQW structures,
which show red shifts from the quantum-confined Stark effect.[44,45] To investigate this further, the spectral photocurrent response
is fit using two Gaussian components made up of the broad-band photocurrent
(300–475 nm) and narrow exciton photocurrent at 521 nm (Figure
S2 in the Supporting Information). While
the exciton blue-shifts by 12 nm with increasing applied bias from
0.0 to +2.0 V, its spectral width remains constant. On the other hand,
the broad-band photocurrent shows substantial variation in the spectral
position as well as spectral width. This could potentially be because
more than one mechanism is involved in the generation of photocurrents,
for example, BB absorption, CT absorption, etc. Examining the bias
dependence of the two contributions (Figure b), we find that the threshold bias voltage
(at which the photocurrent flips sign) is 0.35 V higher for excitons,
emphasizing the different mechanisms involved in creating these photocurrents.
In order to better distinguish the different contributions to the
photocurrent and their bias dependence, we also use a singular value
decomposition analysis (Figure S3 in the Supporting Information), which identifies additional contributions from
Stark shifts due to charging, which produces fields on the exciton.
Figure 4
(a) Photocurrent
spectral response with respect to the applied bias voltage for configuration 1. (b) Variation of the photocurrent magnitudes with applied
bias at specific wavelengths extracted from part a.
(a) Photocurrent
spectral response with respect to the applied bias voltage for configuration 1. (b) Variation of the photocurrent magnitudes with applied
bias at specific wavelengths extracted from part a.
Scanning Photocurrent Microscopy
Global illumination of Al/CHPI/ITO reveals information about the
origin of photocurrents, transport (and dynamics) of photogenerated
charge carriers, and exciton photocurrent peak tunability. Localized
illumination, however, offers insight into the photogeneration and
transport mechanisms of photocarriers. Scanning photocurrent microscopy
has recently been utilized to study charge transport along 1D semiconductors
(such as carbon nanotubes, silicon and Nb2O5 nanowires, VO2, etc.) and at their junctions.[46−48] This technique can also give valuable information related to local
band bending and carrier diffusion lengths.[49] Localized low-power-laser (diffraction-limited) irradiation measurements
are performed on the lateral photocurrent arrangement (Al/CHPI/Al)
shown in Figure a
(for fabrication, see Methods in the Supporting Information). The 410 nm diode laser (<50 mW) is focused
through a 40× microscope objective to a spot size of ∼5
μm. Precise scanning of the laser spot across the two metal
contacts is achieved with an XY-piezocontrolled stage, with electrical
contacts made using micropositioner probes.
Figure 5
(a) Lateral-geometry
Al/CHPI/Al photocurrent configuration fabricated on a glass substrate
in (b) a bright-field image. Greenish-blue emission between the two
aluminum contacts is luminescence (λem ∼ 520
nm) due to 410 nm laser spot irradiation as well as laser scattering.
(c) Scanning photocurrent response moving between aluminum contacts,
at applied biases of +5 and −5 V. (d) Schematic energy band
diagrams of Al/CHPI/Al under +5 V applied bias showing the band bending
and photocarrier transport due to light irradiation at the left (+ve)
and right (−ve) terminals.
(a) Lateral-geometry
Al/CHPI/Al photocurrent configuration fabricated on a glass substrate
in (b) a bright-field image. Greenish-blue emission between the two
aluminum contacts is luminescence (λem ∼ 520
nm) due to 410 nm laser spot irradiation as well as laser scattering.
(c) Scanning photocurrent response moving between aluminum contacts,
at applied biases of +5 and −5 V. (d) Schematic energy band
diagrams of Al/CHPI/Al under +5 V applied bias showing the band bending
and photocarrier transport due to light irradiation at the left (+ve)
and right (−ve) terminals.The laser spot spatial position is monitored through a CCD
camera, which tracks the observed bright-green luminescence spot (Figure b). At an applied
potential of +5 V, when the laser spot is scanned from the anode (aluminum;
left) to the cathode (aluminum; right) a strong photocurrent is observed
only at the anode–CHPI interface region (Figure c). This photocurrent
is still observed at the anode–CHPI interfacial region when
the polarities of the aluminum electrodes are exchanged. Additional
experiments confirm that the higher photocurrent is collected only at the anode–CHPI (+ve terminal) interfacial
region.The photoresponse can be explained by considering the
energy band diagram of this Al/CHPI/Al configuration (Figure d). At zero bias, the difference
in the aluminum metal work function and the electron affinity level
of the semiconducting film creates a Schottky potential barrier. When
an external bias is applied, band bending occurs according to the
respective polarities of the aluminum metal electrodes as well as
the type of semiconducting film. At the positively biased side (anode–CHPI
interface), the photogenerated electron and hole pairs are separated
by a strong local electric field. The electrons move toward the positive
terminal (left) and are readily collected. However, holes have to
move across the CHPI film to be collected at the negative terminal
(right). When we instead consider the case with illumination at the
cathode–CHPI interface (right side), the photogenerated holes
are readily collected at the negative aluminum terminal (right), while
the electrons experience a large barrier and have to diffuse across
the film before being collected at the positive terminal (left).Thus, at positive bias there is always a unidirectional flow of carriers,
irrespective of the illumination position. Despite the relatively
low diffusion rate of the holes, the photocurrents at the positive
terminal are always higher than those at the negative terminal (Figure d), which occurs
when the semiconducting channel is of the p-type.[47] Therefore, these scanning photocurrent microscopy measurements
imply that this CHPI 2Dperovskite is a p-type semiconductor. Mitzi
et al. used extensive varieties of related 2D IO perovskites (tin-
and lead-based) in transistors and also found them to be in the p-type,[11,12,50,51] as indeed is also the parent PbI2.[50]
Effect of the Electron- and Hole-Transport
Layers
On the basis of our observations, we conclude that
the energy stored as strongly bound excitons in this 2Dperovskite
may, nevertheless, be harvested in the presence of a suitable interface.
This behavior is conceptually similar to that utilized by photovoltaics
based on organic semiconductors and dyes: pristine organic films achieve
external quantum efficiency (EQE) of the order of 0.1% because of
the low probability of spontaneous thermal dissociation of excitons.[52,53] By contrast, organic heterojunctions introducing a suitable electric
field or potential step, achieved by pairing the organic with a complementary
metal or semiconductor layer, exhibit relatively high exciton dissociation
efficiencies.[54] We therefore adapt our
design to introduce two carrier-selective, nonmetallic interfaces
(p-type spiro-OMeTAD and n-type TiO2), both of which should
have the capability of dissociating a bound e–h pair without
introducing image-dipole or plasmon quenching. To observe the effects
of electron- and hole-transport materials on charge carriers in the
2Dperovskite, the photodetector configurations 2 and 3 are studied. Parts a and c of Figure show the schematic layer structures and
parts b and d of Figure the corresponding cross-sectional SEM images of both configurations
(2 and 3). In configuration 2, CHPI coats a compact TiO2 (c-TiO2) electron-transport layer (ETL) and is
overcoated with spiro-OMeTAD as the hole-transport layer (HTL) and
gold to produce heterojunction configuration [Au/HTL/CHPI/c-TiO2/FTO] (see Methods in the Supporting Information).[4,5] In configuration 3, an additional 500
nm thick mesoporous TiO2 (mp-TiO2) layer is
spun onto the c-TiO2 layer before infiltrating with CHPI
[Au/HTL/CHPI/mp-TiO2/c-TiO2/FTO].[1,2] These structures are inspired by recent progress in the field of
3D perovskite-based solar cells, where device optimization has led
to PCEs exceeding 15% in just a few years.[1−4]
Figure 6
(a) Schematic and (b) cross-sectional
SEM of photodetector device configuration 2 [Au/HTL/CHPI/c-TiO2/FTO]. (c) Schematic and (d) cross-sectional SEM of photodetector
device configuration 3 [Au/HTL/CHPI/mp-TiO2/c-TiO2/FTO]. (e) Energy diagram of 2D perovskite (CHPI)
photodetector configurations 2 and 3 with
no bias.
(a) Schematic and (b) cross-sectional
SEM of photodetector device configuration 2 [Au/HTL/CHPI/c-TiO2/FTO]. (c) Schematic and (d) cross-sectional SEM of photodetector
device configuration 3 [Au/HTL/CHPI/mp-TiO2/c-TiO2/FTO]. (e) Energy diagram of 2Dperovskite (CHPI)
photodetector configurations 2 and 3 with
no bias.The transient photocurrent of
configuration 2 recorded at two different excitation
wavelengths, 450 and 508 nm, corresponding respectively to BB and
exciton transitions, shows a prompt and strongly enhanced photocurrent
compared to the pristine configuration 1 (Figure a). After many ON/OFF cycles,
only a slight degradation in the photocurrent magnitude is observed.
At 0 V bias, the photocurrent corresponding to exciton transitions
(at 508 nm) is larger by a factor of 7 compared to the photocurrent
obtained for BB transitions (at 450 nm). The photocurrent spectral
response, recorded for the visible region of the spectra, again shows
significant enhancement in the narrow exciton band (peaked at 508
nm) compared to the broad-band features associated with BB transitions.
Thus, the addition of carrier-transport layers does not alter this
surprising strength of exciton photocurrent contributions. The narrow
exciton photocurrent peak possesses a fwhm of ∼21 nm, which
shows that, even with the presence of both ETL and HTL, the 2Dperovskite
in the photodetector configuration maintains the MQW structures, resulting
in excitonic features but still facilitating dissociation of the tightly
bound e–h pairs. The current–voltage (I–V) curves represent typical semiconductor
diode-like characteristics with significant enhancement in the generated
photocurrent under 450 and 508 nm illumination (Figure b). The shifts in I–V curves along the negative voltage axis indicate the generation
of photovoltage upon illumination. The exciton photocurrent peak shows
a blue shift of 17 nm compared to configuration 1 (fabricated
with a top gold electrode; Figure c). This blue-shifted exciton photocurrent peak better
matches the absorption spectrum of CHPI, which has an exciton peak
at 506 nm (Figure a). Hence, this suggests that the large exciton photocurrent now
comes from the bulk CHPI within the full thickness of the device.
Figure 7
(a) Transient
photocurrent response of configuration 2 under periodic
ON/OFF illumination of 450 and 508 nm light at 0 V bias. (b) I–V characteristics of configuration 2 under 450 nm, 508 nm exposure, and dark conditions. (c)
Photocurrent spectrum of configuration 2 measured at
0 V bias. The photocurrent spectrum of configuration 1 (with gold top electrode) is added for comparison. (d) Comparison
of the photocurrent spectral response of configuration 2 with a commercially available GaP photodiode.
(a) Transient
photocurrent response of configuration 2 under periodic
ON/OFF illumination of 450 and 508 nm light at 0 V bias. (b) I–V characteristics of configuration 2 under 450 nm, 508 nm exposure, and dark conditions. (c)
Photocurrent spectrum of configuration 2 measured at
0 V bias. The photocurrent spectrum of configuration 1 (with gold top electrode) is added for comparison. (d) Comparison
of the photocurrent spectral response of configuration 2 with a commercially available GaP photodiode.The photodetector in configuration 2 is compared
with a commercial GaP photodiode (FGAP71, Thorlabs). The as-prepared
CHPI-based photodetector configuration 2 was not encapsulated
with any sealing agent or epoxy and all measurements were performed
in air. The photocurrent spectral response of configuration 2 shows an efficiency comparable to that of the GaP photodiode
(Figure d). Thus,
such 2Dperovskite-based photodetectors could be suited to specific
detector applications at wavelengths of around 500 nm. Because previous
work reports wide exciton tunability in these perovskites (achieved
by compositional substitutions of cations and anions as well as varied
layer stackings and variation of the organic moieties; Figure S4 in
the Supporting Information),[25,28,29] photodetectors could be fabricated
with appropriate 2Dperovskite materials for many specific target
spectral regions.To further explore interplane exciton and
carrier transport in 2Dperovskite-based photodetectors, configuration 3 is studied in which a thick layer (∼500 nm) of CHPI/mp-TiO2 is sandwiched between the c-TiO2 and spiro-OMeTAD
layers (Figure c).
The SEM cross-sectional image of configuration 3 (Figure d) shows no clear
CHPI layer between mp-TiO2 and spiro-OMeTAD, indicating
that the 2Dperovskite is well dispersed in the mp-TiO2 layer. Recent studies on 3D perovskite-based solar cells demonstrate
that CH3NH3PbI3 forms closely packed
networks of perovskite cubic unit cells around TiO2 nanoparticle
scaffolds, facilitating extraction of photogenerated electrons to
TiO2, with holes being transferred to spiro-OMeTAD.[1] The situation for layered 2D perovskites is expected
to be similar, with the TiO2 nanoparticles not disturbing
the self-assembled alternate stacking of IO layers. This is further
confirmed by glancing-angle X-ray diffraction (GAXRD) spectra of configuration 3 without top spiro-OMeTAD and gold contacts. The X-ray diffraction
pattern shows the dominance of c-axis-oriented (00l) planes, signifying the presence of a strong layering
arrangement of inorganic and organic sheets (Figure S5 in the Supporting Information). The crystallite size
estimated from Scherrer’s formula using the angular width of
the narrow (001) characteristic peak occurring at 2θ = 5.12°
is found to be 83 nm, which is actually much larger than that for
a CHPI film spin-coated onto glass (12 nm). The crystallite size of
the perovskite depends on the porosity of the mesoporous scaffold,
which can be optimized by varying the nanoparticle size.[55]The photocurrent measured for configuration 3 under 508 nm illumination at 0 V is 3 times larger than
that for configuration 2. The transient photocurrent
shown in Figure a
is recorded under periodic illumination at 508 nm for several cycles
under zero bias conditions. The photocurrent rises very rapidly (submilliseconds)
during the transition from OFF to ON states and rapidly decreases
to zero as soon as the light turns off, much faster than that for
configuration 2. These results are highly reproducible,
and the photocurrent magnitude is found to be completely stable over
many ON/OFF cycles, in contrast to configuration 2. After
the fast anodic spike, the photocurrent slightly decays with a slow
time constant of ∼20 s before settling to a stable photocurrent.
This slow decay in the photocurrent is attributed to the accumulation
of excess electrons on the TiO2 surfaces. Rather than being
trapped or extracted, these electrons undergo competitive recombination
with the holes available at the nearest site in the perovskite. Once
the equilibration of competitive separation and recombination of electron–hole
pairs is attained, the photocurrent remains constant.
Figure 8
(a) Transient photocurrent
response of configurations 2 and 3 under
periodic ON/OFF illumination at 508 nm with 0 V bias. (b) I–V characteristics of heterojunction
photodetector configurations 2 and 3 measured
in the dark (dashed line) and under 100 mW cm–2 (AM1.5G)
photon flux (solid line) [note: the bias polarity is inverted compared
to previous measurements to get a conventional I–V curve]. (c) Corresponding EQE spectra showing improvement
in the efficiency at exciton wavelengths in configuration 3. (d) Room-temperature photocurrent spectra of configuration 3 recorded under different applied potentials (inset shows
schematic). (e) Comparison of normalized photocurrent spectra of configurations 1 (with gold top electrodes), 2, and 3, at +0.5 V bias.
(a) Transient photocurrent
response of configurations 2 and 3 under
periodic ON/OFF illumination at 508 nm with 0 V bias. (b) I–V characteristics of heterojunction
photodetector configurations 2 and 3 measured
in the dark (dashed line) and under 100 mW cm–2 (AM1.5G)
photon flux (solid line) [note: the bias polarity is inverted compared
to previous measurements to get a conventional I–V curve]. (c) Corresponding EQE spectra showing improvement
in the efficiency at exciton wavelengths in configuration 3. (d) Room-temperature photocurrent spectra of configuration 3 recorded under different applied potentials (inset shows
schematic). (e) Comparison of normalized photocurrent spectra of configurations 1 (with gold top electrodes), 2, and 3, at +0.5 V bias.The I–V characteristics of both configurations 2 and 3 are recorded at room temperature under
simulated AM1.5G solar illumination and show typical photodiode behavior.
The open-circuit voltages (Voc) for these
devices are 0.51 and 0.58 V for configurations 2 and 3, respectively (Figure b). The effect of the mp-TiO2 layer is to
enhance the short-circuit current density (Jsc) roughly 9-fold, from 0.11 to 1.03 mA cm–2. Configuration 3 shows a PCE of 0.3%, which is 11 times
higher than that of configuration 2 (0.027%).Room-temperature
EQE measurements were performed for a wide spectral range and are
compared in Figure c. Although the EQE values for configuration 3 are found
to be higher than those for configuration 2 across the
whole spectrum range, this enhancement is stronger at the exciton
wavelength (508 nm) with 10% EQE, which is 8 times higher, and in
the BB transition region, with 36% EQE, which is 9 times higher. The
overall improvement in the EQE of configuration 3 can
be attributed to the role of sphericalTiO2 nanoparticles
forming mesoporous structures of high aspect ratios, which promote
electron transfer between PbI4 layers as well as increased
optical scattering, resulting in this significant enhancement in the
device performance.[56,57] Moreover, charge transport within
the perovskite is improved because of the larger grain size, reducing
the number of grain boundaries and making it possible to have single
grains span the space between two TiO2 nanoparticles. These
results thus show the role of TiO2 nanoparticles in improving
the photocurrent efficiencies, which remain a source of considerable
controversy in solar cells based on 3D perovskites.[58]The bias dependencies of the photocurrent spectral
response for both configurations 2 and 3 are studied at room temperature (Figure d,e). At zero bias, both configurations exhibit
a strong exciton photocurrent peak at 508 nm. Unlike configuration 1, changing the applied bias does not change the exciton photocurrent
peak position (508 nm) for configurations 2 and 3. The overall comparison between the normalized photocurrent
spectra for all three structures (Figure e) shows that configuration 1 displays different spectral responses at both exciton and BB transitions,
likely because of the rate-determining collection at the Schottky
aluminum–gold contact, which has high space-charge fields.
The additional peak around 400 nm in configuration 3 is
likely due to the intrinsic photocurrent response of the anatase phase
TiO2 nanoparticles.[59,60] Similar enhancements
are seen for another 2Dperovskite when the TiO2 nanoparticles
are inserted into the active layer (Figure S6 in the Supporting Information).
Conclusion
This
investigation of the room-temperature photocurrent properties of 2D
IO perovskites reveals that excitons strongly contribute to the photocurrents
despite possessing binding energies more than 10-fold larger than
the thermal energies. The p-type CHPI liberates photocarriers at metallic
Schottky aluminum contacts, but charging slows down the photoresponse.
In contrast, using ETL and HTL enhances the extracted photocurrents
by 100-fold, and a further 10-fold gain is found when mixing TiO2 nanoparticles directly into the perovskite layers, although
the 2D exciton layers are not significantly disrupted. We thus conclude
that exciton dissociation must occur within strong local electric
fields, at the material interfaces, or at crystal grain boundaries.
We also find that carrier transport between the >1-nm-spaced QW
sheets is far more efficient in these 2D materials than was expected
from previous considerations, probably because of rapid lateral transport
to grain boundaries or the TiO2 nanoparticles. These results
show that strong excitonic materials may be useful as photovoltaic
materials despite high binding energies and provide useful evidence
in the understanding of the related 3D perovskites.
Authors: T Serkan Kasırga; Dong Sun; Jae H Park; Jim M Coy; Zaiyao Fei; Xiaodong Xu; David H Cobden Journal: Nat Nanotechnol Date: 2012-10-21 Impact factor: 39.213
Authors: Sudeep Maheshwari; Tom J Savenije; Nicolas Renaud; Ferdinand C Grozema Journal: J Phys Chem C Nanomater Interfaces Date: 2018-07-08 Impact factor: 4.126
Authors: Mohammad Rahil; Rashid Malik Ansari; Chandra Prakash; S S Islam; Ambesh Dixit; Shahab Ahmad Journal: Sci Rep Date: 2022-02-09 Impact factor: 4.379