Yury
Smirnov‡
a,
Pierre-Alexis
Repecaud‡
a,
Leonard
Tutsch
b,
Ileana
Florea
c,
Kassio P.S.
Zanoni
d,
Abhyuday
Paliwal
d,
Henk J.
Bolink
d,
Pere Roca
i Cabarrocas
d,
Martin
Bivour
b and
Monica
Morales-Masis
*a
aMESA+ Institute for Nanotechnology, University of Twente, Enschede, AE 7500, Netherlands. E-mail: m.moralesmasis@utwente.nl
bFraunhofer Institute for Solar Energy Systems ISE, 79110 Freiburg, Germany
cLPICM, ÉCole Polytechnique, CNRS, Institut Polytechnique de Paris, Palaiseau 91120, France
dInstituto de Ciencia Molecular, Universidad de Valencia, C/Catedrático J. Beltrán 2, 46980 Paterna, Spain
First published on 1st March 2022
Transparent conducting oxides (TCOs) used in solar cells must be optimized to achieve minimum parasitic absorption losses while providing sufficient lateral conductivity. Low contact resistance with the adjacent device layers and low damage to the substrate during deposition of the TCO are also important requirements to ensure high solar cell efficiencies. Pulsed laser deposition (PLD) has been proposed as an alternative low-damage TCO deposition technique on top of sensitive layers and interfaces in organic and perovskite solar cells but is yet to be studied for the more mature silicon technology. Focusing on the PLD deposition pressure as the key parameter to reduce damage, we developed tin-doped indium oxide (ITO) with a sheet resistance of 60 Ω □−1 at different pressures and implemented it in silicon heterojunction (SHJ) solar cells. Buffer-free semi-transparent perovskite cells with the same PLD ITO electrodes were also fabricated for comparison. While in the perovskite cells increased ITO deposition pressure leads to an improved open circuit voltage and fill factor indicative of damage reduction, SHJ cells with PLD ITO at all conditions maintained a high passivation quality, but increased pressures lead to high series resistance. Transmission electron microscopy and time-of-flight secondary ion mass spectrometry confirmed the formation of a parasitic SiOx at the ITO/a-Si:H interface of the SHJ cell causing a transport barrier. The optimized ITO films with the highest carrier density were able to obtain >21% SHJ efficiency with 75 nm-thick PLD ITO. Moreover, reducing the ITO thickness to ∼45 nm and using TiOx for optical compensation enables fabrication of SHJ devices with reduced indium consumption and efficiencies of >22%.
In this work Sn-doped In2O3 (ITO) films grown using wafer-scale PLD at different deposition pressures but with the same sheet resistance (Rsh) are implemented as both the front electrode and rear electrode in SHJ solar cells. To compare the effects of deposition pressure on other sensitive contact layers, buffer-free semi-transparent perovskite cells (ST-PSC) were fabricated with the same rear PLD ITO electrodes. The results suggest that an increased ITO deposition pressure leads to lower damage at the ITO/organic (BCP/C60) interface in the perovskite cells. For the SHJ cells, no correlation was found between deposition pressure and passivation damage, but high pressures resulted in a high contact resistance. At optimized PLD ITO conditions, combining high pressure during deposition and high free carrier density (Ne) on the film level, leads to efficient proof-of-concept SHJ solar cells. These results motivate further studies of TCO low damage deposition techniques towards achieving low contact resistance when implemented in devices in addition to the optimum trade-off between transparency and conductivity in TCOs.
Fig. 1 displays grazing incidence X-ray diffraction (XRD) patterns of the ITO films deposited on glass and planar Si wafers. All the as-deposited ITO films are amorphous regardless of the deposition pressure and substrate (Fig S1, ESI†). However, a 200 °C annealing step in air for 20 min (similar to the Ag metallization step of the SHJ cells) results in films with different structural properties. While on glass the HP ITO films remain amorphous, both LP and LP with buffer ITO films show (211), (222), (400) and (440) peaks corresponding to the In2O3 bixbyite reference pattern.13
Of note, the LP with buffer ITO films show enhanced crystallinity, as suggested by the higher intensity peaks as compared to the LP films. Following previous reports on ITO crystallization, one can speculate that the LP ITO film is only partially crystallized.14 Interestingly, ITO films deposited on the a-Si:H(n/i)/c-Si/a-Si:H(i/p) stacks remain mainly amorphous, with only the LP with buffer showing In2O3 bixbyite reflections. These results suggest that the thin ITO buffer deposited at 0.1 mbar promotes the crystallization of the ITO, following observation of previous reports,15 which moreover affects the optoelectronic properties of the films as will be described below.
Hall effect measurements of the same ITO films were performed to evaluate the effect of pressure, substrate (glass vs. planar a-Si:H(p/i)/c-Si stacks) and the resulting structural properties on the free carrier density (Ne) and electron mobility (μe). Fig. 2(a) displays the Rsh of the films, all showing ∼60 Ω □−1 in the as-deposited state, which was the target value for the ITO development. Following that Rsh = 1/(eμeNed), with e being the fundamental charge and d the thickness of the ITO fixed at 100 nm, we can see that, while the LP and LP with buffer ITO show Ne above 3 × 1020 cm−3 in the as-deposited state, the HP ITO show Ne below 2.5 × 1020 cm−3. Conversely, μe is higher for the HP ITO reaching values >40 cm2 V−1 s−1, while μe for the LP and LP with buffer ITO films are all below 40 cm2 V−1 s−1. The difference in Ne is likely caused by different oxidation conditions during PLD growth and is possibly defining the observed difference in μe for ITO films. In the case of HP ITO, μe is likely to be limited by dislocation scattering (Ne < 3 × 1020 cm−3),16 whereas LP and LP with buffer ITO (Ne > 3 × 1020 cm−3) are most probably primarily limited by ionized impurities scattering.17 Moreover, electrons tunnel through thin potential barriers formed at grain boundaries18 for films at higher Ne leading to a smaller contribution from dislocation scattering explaining the observed difference in the μe of ITO films.
After the 200 °C annealing step, μe and Ne of all PLD ITO deposited onto the a-Si:H(p/i)/c-Si stacks ITO remain virtually unchanged. Interestingly, similar trends are observed for the LP and LP with buffer ITO on glass, whereas the HP (0.02 mbar) ITO show variations in the properties after annealing. Rsh increases from 60 to 95 Ω □−1 after the heat treatment on glass due to the drop of Ne (from 2.4 to 1.2 × 1020 cm−3). It is important to mention that the reported values represent an average of at least 2 glass samples which have been co-deposited with a SHJ cell stack. The electrical properties of the TCO layers have been previously shown to be dependent on the underlying substrate and to be sensitive towards hydrogen effusion from the hydrogenated a-Si:H layers beneath,19,20 however, this was not observed in our Hall effect measurements on the a-Si:H(p/i)/c-Si(n) stacks. Although this stack seems to be more representative of the device performance, we underline that the developed ITO electrodes were implemented in SHJ cells with a rear emitter design. Therefore, the front current collection would occur from a-Si:H(n/i)/c-Si(n) stack which cannot be reliably measured via the Hall effect due to substantial conduction through the Si substrate in this case.
Optical properties, as shown by the absorptance in Fig. 2(d) and transmittance in Fig. S2 (ESI†), followed the expected trend: a blue shift in the UV due to the Burstein–Moss effect21,22 and increased free carrier absorption (FCA) in the NIR with increased Ne. The lowest FCA and the narrowest optical band gap are observed for the HP film (lowest Ne, highest μe), whereas the highest FCA and widest optical band gap are measured for the LP with the buffer film (highest Ne, lowest μe).
Interestingly, the use of a high-pressure ITO buffer layer promotes ITO crystallization resulting in films with high Ne. This is opposite to an expected increase in μe with enhanced crystallization as demonstrated in other works.15,23 The high Ne instead of high μe of our ITO films with the highest crystallinity indicates that there is a more complex interplay between oxygen vacancies24, grain boundaries16 and ionized impurity scattering,17 in our films. Finally, the optoelectronic properties of the PLD grown ITO films at the three pressure conditions meet the requirements of a front electrode of the SHJ solar cells and/or a rear electrode in ST-PSC, i.e. Rsh < 100 Ω □−1 and low FCA (absorptance below 10% in the spectral range from UV to NIR).25,26 In the following section, the performance of these PLD ITO films on devices will be compared to a sputtered ITO reference for SHJ cells (Rsh ∼ 100 Ω □−1 on textured substrate; Ne ∼ 1.5 × 1020 cm−3, μe ∼ 40 cm2 V−1 s−1) or an opaque Ag electrode for the case of ST-PSC.
Fig. 3 displays the statistical distribution of the main solar cell parameters for devices with different rear ITO electrodes for the forward scan directions measured from the glass side (forward and reversed scan are presented in Fig. S3, ESI†). The results show clear improvements in open-circuit voltage (Voc) and fill factor (FF) with the increase in the deposition pressure of ITO. Cells with LP ITO show a severe drop in Voc and fill factor (FF) as compared to the opaque reference cell with evaporated Ag back contact. Of note, the thin layer deposited at 0.1 mbar for the case of LP with buffer ITO leads to significant improvements in power conversion efficiency (due to enhanced FF and Voc) as compared to cells with LP ITO. Devices with HP and LP with buffer ITO show comparable short-circuit density (Jsc), yet the FF and Voc are higher for the latter, thus leading to gains in PCE. Nevertheless, cells with HP ITO show only a small drop of Voc and FF with respect to the best performing ST-PSC indicative of a good interface formation for the two conditions. The HP ITO results are in agreement with previous reports for solution-processed ST-PSC with PLD IZrO.11 For the cells with LP ITO, an increased barrier height at the ETL/TCO interface may be causing the severe drop of FF and Voc as suggested by Kanda et al.28 Another possible explanation of the deteriorated cell performance is the penetration of the energetic ablated particles in the organic layer29 due to the suppressed thermalization during PLD at low pressures. The PCE of the reference opaque cell is >19% for the champion cell highlighting the high quality of the halide absorber and relevant choice of the transport layers. Overall, the higher Jsc of the reference cell is related to Ag acting as a back reflector in the cells. Following the confirmation of the effect of increasing the ITO deposition pressure on the damage mitigation of the thin organic transport layers in ST-PSCs, we proceeded to study the effect on SHJ cells.
As seen from Fig. 4, a similar drop of τeff from 2 ms to around 1.5 ms is observed for all PLD conditions. Interestingly, the sputtered reference is already deposited at 200 °C which is beneficial for in situ curing of the sputter-induced damage. Nevertheless, we observe the drop of τeff for the case of sputtered ITO as well. As expected, the annealing step at 200 °C recovers the passivation for cell precursors with all transparent electrodes due to the possibility for the a-Si:H network to recover at such elevated temperatures.4,5,30,31 The τeff matches or even slightly exceeds the initial values of a-Si:H coated c-Si wafers (>2 ms) for the case of the HP PLD ITO, whereas the passivation is only slightly improved (1.4 ms vs. 1.2 ms) for the case of sputtered ITO.
Remarkably, the cells with LP with buffer ITO demonstrate the highest efficiency among the ITO PLD devices (average across the 10 cells) of 21%, but lag behind the established reference cells with sputtered ITO by ∼1.2% as displayed in Fig. 5(a). Devices with LP and HP ITO reach average efficiencies of 20% and 16.9%, respectively. As seen from Fig. 5(b and c), the cells with various ITO electrodes display similar Voc values. Slight differences in Jsc follow the trend observed in Section 2.1 being inversely proportional to the ITO absorptance.
The differences in the overall efficiency originate from the variations in FF for the case of PLD ITO. These changes are mainly dominated by the trend observed in the series resistance (Rs) of the different PLD films. As shown in Fig. 5(e), cells with HP ITO display the most significant increase of Rs (4.9 Ω cm−2), while Rs for the cells with LP with buffer ITO is just a bit higher (1.1 Ω cm−2) than for cells with sputtered ITO (0.86 Ω cm−2). Interestingly, devices with LP ITO display Rs of 1.9 Ω cm−2 which is notably higher than the cells with LP with buffer ITO. This confirms the importance of the thin buffer layer deposited at 0.1 mbar defining the structural and optoelectrical properties of the ITO film. These films have the highest Ne among the PLD ITO films and additionally display the highest crystallinity which may influence the ITO work function at the interface.32,33 Conversely, the highest Rs is observed for cells with the PLD ITO with the lowest Ne. It has been previously shown34,35 that the combination of Ne in TCO films and the activation energy of the a-Si:H films plays a significant role in increasing the contact resistivity (ρc) of the TCO/a-Si:H stack. However, we believe that the difference of ∼2 Ω cm−2 in ρc cannot be accounted for by the rather insignificant difference in Ne (1.5 × 1020 cm−3vs. 3.0 × 1020 cm−3 as measured on planar a-Si:H-coated Si wafers). For these Ne, the expected difference in ρc is in the orders of few tens of mΩ cm−2 as calculated by Luderer et al.36 Therefore, a more plausible contribution to the high Rs could be the potential formation of an amorphous silicon oxide layer at the a-Si:H/ITO interface during PLD which is performed at elevated oxygen partial pressures compared to sputtering. This parasitic oxide may hinder the carrier transport and lead to the increased contact resistance3 which is investigated in the next section.
To further verify this hypothesis, a batch of SHJ cells with only the front electrode grown via PLD was fabricated (the rear ITO was deposited by sputtering). As seen in Fig. 6, Rs drops substantially by ∼2.5 Ω cm−2 (2.4 vs. 4.9 Ω cm−2). Considering that no lateral transport is needed for the rear contact, this value can be considered as an upper bound for the contribution from the vertical transport, i.e. a good estimation for the ρc of the hole contact stack in the presence of HP ITO. The remaining difference of 1.6 Ω cm−2 in Rs between the double-sided sputtered reference (0.8 Ω cm−2) and only front HP ITO provides, in its turn, an estimation for the ρc of the electron contact stack with HP ITO. These values are high for contacts for SHJ cells but match reasonably well for the case of parasitic oxide hindering the transport of other passivating contacts, such as the TCO/poly-Si contact.3
Chemical mapping of the ITO/a-Si:H(i/n) interface was furthermore performed via time-of-flight secondary ion mass spectrometry (ToF-SIMS) and high-resolution energy dispersive X-ray spectroscopy (EDX) under a scanning transmission electron microscope (STEM). Fig. 7(a and b) show the ToF-SIMS depth profile resulting from ablation using a Cs+ source from the HP ITO towards the c-Si both before and after annealing. It should be noted that the annealed states resemble the situation in the solar cell for which JV measurements have been performed after annealing at 200 °C. One measurement frame was performed after every ablation while tracking In2O3−, Si−, H− (Fig. 7(a)) and SiHO2−/SiO3In− (Fig. 7(b)) signals, respectively, with a quadrupole mass spectrometer. SIMS measurement data for LP ITO and HP ITO are presented in Fig. S4 (ESI†). Si− and In2O3− signals do not change upon annealing for any samples and therefore allow identification of the ITO/a-Si:H interface. H− is observed for all samples before and after annealing suggesting the presence of H− in ITO already in the as-deposited state. In contrast to what has been shown by Cruz et al.20 or Ritzau et al.,39 we do not observe additional H− diffusion into the ITO layer from the a-Si:H. This agrees with the Hall effect data, showing that Ne does not change upon annealing of the ITO/a-Si:H planar stacks. SIMS measurements also allowed detection of SiO3In− and SiHO2− signals which are indicative of oxygen presence. Fig. 7(b) and Fig. S4 (ESI†) show that the SiO3In− and SiHO2− signals are only present in the vicinity of the TCO/a-Si:H interface, both before and after annealing. The high intensity of the SiHO2− signal at the TCO/a-Si:H interface indicates the oxidation of the a-Si:H surface during ITO deposition. In order to compare the SiOx layer for the three PLD conditions, before and after annealing, SiO3In− and SiHO2− signals were extracted and plotted independently for each sample in Fig. 7(c and d). The full width at half maximum (FWHM) and the area of these two signals were measured before and after annealing and are reported in Table S1 (ESI†). The results indicate that the SiOx layer is present for all as-deposited samples with a similar thickness independent of the PLD deposition pressure.
For both the SiHO2− and SiO3In− signals, the only significant change in FWHM is observed for the stack with HP ITO, showing broadening of the peak after annealing. This suggests possible oxygen migration at the ITO/a-Si:H interface, increasing the SiOx barrier width after annealing. We observe this only for the HP ITO sample, which is the amorphous film before and after annealing. The density of the film or even its possible higher oxygen content (due to higher p(O2) during the deposition process) might be the cause of this effect. The observation also agrees with the higher Rs for the SHJ cells with the HP as ITO reported in Section 2.1. The ToF-SIMS measurements, the same as the Hall effect measurements, were all performed in the ITO/a-Si:H(n/i)/c-Si planar stacks. To verify the presence of the SiOx also on the cells analyzed in Fig. 5 (textured wafers instead of planar), scanning transmission electron microscope high-angle annular dark field (STEM-HAADF) EDX was performed on FIB prepared lamellas taken directly from the cells. The contrast in STEM imaging of the amorphous layers next to the HP ITO films in Fig. 7(e) suggests the presence of ∼1.2 nm a-SiOx next to the a-Si:H thin film. The EDX chemical mapping corresponding to the zoomed area (Fig. 7(f)) indicates the oxygen (green) signal between the indium (pink) and silicon (blue) layers. Identical analysis for the LP ITO and LP ITO with the buffer is displayed in Fig. S5 (ESI†). The increase in the O− signal prior to indium and tin signals is clearly observed for all ITO samples in the STEM-HAADF EDX line scan profile recorded across the a-Si:H/ITO interface (as shown in Fig. S5(g–i), ESI†). Interestingly, the a-SiOx layer is present for cells with ITO by PLD as confirmed by both STEM and ToF-SIMS measurements. The absence of hydrogen effusion into the ITO layers observed by ToF-SIMS may suggest that the thin a-SiOx also acts as the hydrogen blocking layer. However, the presence of this a-SiOx thin layer only leads to severe degradation of FF for cells with HP ITO. This may also be indicative of a thicker/denser parasitic oxide layer for the case of HP ITO.3 Nevertheless, distinguishing a minor difference in the thicknesses of the SiOx for each of the pressure conditions from the local EDX/TEM measurements is challenging and cannot be easily decoupled from other effects such as the crystallinity of the ITO layers and/or its Ne as discussed in Section 2.4.
Optical properties of the ITO films were measured on a UV-Vis-NIR spectrophotometer PerkinElmer Lambda 950S using an integrating sphere. Absorptance (A), defined as A = 1 − TT − TR, where TT is the total transmittance and TR is the total reflectance, of the films on glass. Sheet resistance (Rsh), free carrier density (Ne) and electron Hall mobility (μe) were determined using a Hall Effect measurement setup in the van der Pauw configuration, using 1 × 1 cm2 pre-diced samples. The structural properties of the films were investigated using an Xpert Pro diffractometer (Panalytical) in grazing incidence (GI-XRD) configuration were the incident angle is ω = 0.6°. The ITO thickness was determined by measuring the step height on glass samples with a Dektak stylus profilometer. Time-of-flight secondary ion mass spectrometry (ToF-SIMS) was performed by TESCAN analytics. Ablation was done using a Cs+ source on a 200 μm2 area. The process was performed such that one measurement frame was performed after every ablation frame while tracking H−/In2O3−/Si−/SiHO2− and SiO3In− signals with a quadrupole mass spectrometer.
Chemical analyses were performed in the scanning transmission electron microscope high-angle annular dark field (STEM-HAADF) imaging mode of a 200 kV Titan-Themis TEM/STEM electron microscope equipped with a Cs probe corrector and a ChemiSTEM Super-X detector. Prior to the analysis, the FIB technique was used for the preparation of cross-section lamellas of the considered sample. STEM-HAADF EDX chemical mapping was performed by considering the following elements of interest: the silicon Kα-1.73 keV ionization present in the substrate, the a-SiOx layer and the a-Si:H layer, the oxygen Kα-0.523 keV ionization edge coming also from the thermal a-SiOx and the indium L-3.28 keV ionization edge from the ITO layer.
Solar cells and lifetime test structures were fabricated on random pyramid textured 1 Ω cm, and 180 μm thick n-type FZ silicon wafers at Fraunhofer ISE. The monofacial solar cells were fabricated in the rear-emitter design and metallized at the front and rear side via screen printing of an Ag paste cured at 200 °C in a belt furnace. The a-Si:H layers are deposited by plasma-enhanced chemical vapor deposition (PECVD) using mixtures of SiH4, H2, TMB, and PH3. These precursors were later shipped to the University of Twente for PLD ITO. The reference ITO samples were deposited inline via DC magnetron sputtering from a rotary 97/3 wt% In2O3/SnO2 target with a deposition substrate temperature of 190 °C. The power of 4.4 kW was distributed along the 75 cm long target, and the deposition pressure was kept at 4 × 10−3 mbar in 5% O2 in an Ar atmosphere.
Semi-transparent perovskite solar cells (ST-PSC) were fabricated by thermal evaporation in vacuum chambers at 10−6 mbar, which are integrated in a nitrogen-filled glovebox (H2O and O2 < 0.1 ppm) at the University of Valencia. The vacuum chambers are equipped with temperature-controlled evaporation sources (Creaphys) fitted with ceramic crucibles, directed upward. Individual quartz crystal microbalance (QCM) sensors monitored the deposition rate of each evaporation source. As mentioned in Section 2.2, the evaporated perovskite solar cell stack consisted of glass/ITO (160 nm)/MoO3 (6 nm)/TaTm (10 nm)/MAPbI3 (500 nm)/C60 (25 nm)/BCP (7 nm). The deposition of the perovskite and charge transport layers followed the same procedure described in our previous publications.43,44 The ST-PSC substrates were later shipped to the University of Twente for rear transparent ITO electrode fabrication by PLD. For the ITO PLD deposition, the substrates were aligned to shadow masks to obtain the electrode layout indicated in Fig. S6 (ESI†) with sixteen rectangular pixels of 0.0825 cm2, eight on each side of the substrate, allowing for significant statistics. No silver grid lines surrounding the PLD-ITO contacts were used for semi-transparent cells in this study. An Ag grid for the reference opaque cells was fabricated by thermal evaporation at the University of Valencia.
Footnotes |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/d1ma01225h |
‡ These authors contributed equally to this work. |
This journal is © The Royal Society of Chemistry 2022 |