Yan Wanga,
Theodore D. C. Hobson
a,
Jack E. N. Swallowa,
Shona McNab
b,
John O’Sullivana,
Anastasia H. Soeriyadia,
Xinya Niua,
Rebekah C. Fraser
c,
Akash Dasguptac,
Soumyajit Maitraa,
Pietro P. Altermatta,
Robert S. Weatherup
a,
Matthew Wright
a and
Ruy S. Bonilla
*a
aDepartment of Materials, University of Oxford, Oxford, OX1 3PH, UK. E-mail: sebastian.bonilla@materials.ox.ac.uk
bSchool of Photovoltaic and Renewable Energy Engineering, University of New South Wales, Sydney 2052, Australia
cDepartment of Physics, University of Oxford, Oxford, OX1 3PU, UK
First published on 3rd February 2025
High-efficiency solar cell architectures, including silicon heterojunction (SHJ) and perovskite/silicon tandems, rely heavily on the unique properties of transparent conducting oxides (TCOs). The push towards terawatt-scale PV manufacturing means it is increasingly desirable to develop indium-free TCOs to facilitate the upscaled manufacturing of high-efficiency cell designs. Aluminium-doped ZnO (AZO) deposited by atomic layer deposition (ALD) has emerged as a promising candidate due to its combination of optical transparency and electrical conductivity. In addition, AZO has also been shown to passivate the c-Si surface. The ability for one material to provide all three properties without requiring any indium is advantageous in single junction and tandem solar devices. Herein, we demonstrate exceptional silicon surface passivation using AZO/AlOx stacks deposited with ALD, with a J0 < 1 fA cm−2 and corresponding implied open circuit voltage (iVOC) of 740 mV. We provide a comprehensive analysis of the role of ALD precursor dosing to achieve optimised performance. A broad range of characterisation approaches were used to probe the structural, compositional, and chemical properties of AZO films. These indicated that the passivation properties are governed by a delicate interplay between the Zn and Al concentrations in the film, highlighting the importance of precise process control. Optical modelling in a single junction SHJ architecture indicates these AZO films are close in performance to high-mobility indium-containing TCOs. The insights provided by this work may help to further the case of indium-free TCOs, which is critical for upscaled production of high-efficiency solar cells.
Most commonly used TCOs in the solar industry contain indium. Indium-based TCOs, such as tin-doped indium oxide (ITO) and tungsten-doped indium oxide (IWO), tend to have high free carrier mobility, allowing for simultaneous high transparency in the visible range and sufficient conductivity for PV devices.5 However, indium is scarce, and using it in TCOs limits TW-scale deployment of PV.11 Hence, PV cells dependent on indium cannot contribute significantly to climate change mitigation. Currently, ongoing research aims to find alternative TCO materials that are earth-abundant while providing the necessary properties for high-efficiency PV devices. One of the promising indium-free TCO alternatives is doped zinc oxide (ZnO).12 Doping ZnO with aluminium (AZO) provides sufficient conductivity for TCO functionality in solar cells. Researchers have also used a variety of deposition techniques to fabricate ZnO, including spray pyrolysis,13 chemical vapor deposition (CVD),14 pulsed laser deposition (PLD),15,16 atomic layer deposition (ALD),17–19 sputtering,20,21 and sol–gel processing.22 Among these, ALD has recently demonstrated several crucial advantages, such as atomic-level thickness control, excellent spatial uniformity, industrial scalability, and doping tailoring.23 Furthermore, ALD-ZnO materials also show promising properties for device integration, including interface passivation, good optical coupling, and processing compatibility.24
Besides transparency and conductivity, PV devices require outstanding surface passivation. Minimising interface recombination losses remains one of the major hurdles in the pathway to ultra-high-efficiency solar cells. We use two parameters to quantify passivation: implied open circuit voltage (iVOC) and saturation current density (J0). iVOC represents the maximum open-circuit voltage (VOC) possible in a solar cell, assuming unity ideality factor in the diode equation. It is calculated from quasi-steady-state (QSS) or transient photoconductance decay (PCD), or photoluminescence (PL) measurements of the solar absorber before charge-extracting electrodes are applied. The QSS PCD measurement is well established25 and uses the recorded average excess carrier concentration (Δn) to infer the voltage performance of the cell under 1 sun (AM1.5G) standard illumination conditions. A high iVOC indicates good passivation quality and is closely correlated with higher solar cell efficiency. For instance, silicon solar cells with iVOC values reaching 730–750 mV correspond to high open-circuit voltage in complete cells, leading to efficiencies above 25%.26–28
The J0 current density characterises the total recombination losses, both in the bulk, the surfaces, and metal contacts of the solar cell. Lower J0 values indicate reduced recombination and, thus better passivation quality. For instance, in well-passivated silicon solar cells, J0 values below 10 fA cm−2 are required for efficiencies to exceed 25%.29,30
Traditionally, the purpose of a TCO is to achieve high transmission of light into the absorber while having sufficient conductivity to extract photo-generated electrons towards the metal contacts with minimal resistive losses. However, TCOs may also function as a passivation layer, for example, on the crystalline silicon (c-Si) surface31,32 or the charge transport layer interface in a perovskite cell.33,34 Recent reports have demonstrated that excellent passivation of a c-Si surface is possible using SiOx/AZO/AlOx. Macco et al. showed significant advancements in the use of AZO as a transparent, passivating and conductive layer for solar cells, demonstrating the potential for iVOC as high as 728 mV.32 This improvement was largely attributed to ALD deposition. The use of supercycle growth leads to a layered structure of dopants embedded in the host ZnO matrix, rather than being isotropically distributed.35 This non-uniform distribution can influence field-effect passivation by affecting the distribution of charge carriers at the surface, which impacts recombination. Therefore, understanding how ALD preparation conditions affect electrical conductivity and passivation behaviour is crucial for exploiting all functionalities in AZO films for solar cell applications.
Previous studies have demonstrated that excellent carrier transport properties were achievable using dimethylaluminum isopropoxide (DMAI) as the Al precursor in AZO films on Si passivated with a-Si.36 This success was primarily attributed to the steric hindrance of the larger isopropoxyl ligand (OiPr, approximately 4.9 Å in size).37 The Al atoms from DMAI are spaced farther apart during deposition compared to smaller precursors like trimethylaluminum (TMA). The increased spacing can prevent unwanted clustering of Al atoms on the ZnO surface, thus decreasing inactive regions where the Al atoms cannot effectively substitute into the ZnO lattice so that a higher doping efficiency can be achieved. Therefore, the DMAI precursor results in enhanced charge carrier mobility.38 In comparison, the more common TMA precursor was shown to be ineffective at shielding surface area and sterically hindering further reactions between adjacent –OH surface groups and incoming precursor molecules.37 In TMA, the methyl ligand CH3 is approximately 2.6 Å in size. Lower doping efficiency of Al from TMA compared with DMAI would mean lower carrier densities from ineffective Al atoms. These inactive dopants can act as scattering centres, leading to low mobility.
This work demonstrates that a combination of favourable transparent conducting electrode (TCE) properties and improved surface passivation is possible using TMA as the Al precursor for AZO, provided the dosing conditions are carefully monitored and optimised. We achieved an optimised ALD recipe yielding outstanding surface passivation, with the lowest reported J0 of 0.87 fA cm−2 corresponding to iVOC of 740 mV. Our optimised AZO achieves a stringent combination of functions: lateral conductivity across a nanolayer thinner than 40 nm, effective chemical and field-effect passivation of the Si surface, and low optical losses via well-matched refractive index and low absorption.
We present the impact that precursor dosing pressures have on the passivation properties, and we use such pressures as the tuning parameter to achieve the best passivation performance. We also investigated the interface properties and AZO/AlOx passivation mechanisms to establish the contributions of interface chemistry and field effect to optimised performance. This work highlights the impact and insights into how ALD precursors affect AZO film deposition and influence surface passivation and optoelectronic properties. Our work paves the way for future mass production of solar cells using earth-abundant TCO materials that provide high transparency, conductivity, and passivation.
Symmetrical SiOx/AZO/AlOx passivation stacks were fabricated on n-type Si, as illustrated in Fig. 1a. While the AZO layer can be exploited as a transparent conductor, the central role we explore is the recombination losses at the interface. The top AlOx served as a capping layer for hydrogen passivation purposes.32 The SiOx was chemically grown by RCA2, while the AZO and AlOx layers were grown bifacially on the c-Si wafer, ensuring uniform and equivalent passivation characteristics on both sides of the Si specimen. Additionally, the AZO and AlOx are grown sequentially inside the same thermal ALD system, demonstrating high process compatibility.
In our AZO process development, we evaluated the surface passivation of sample batches deposited over the span of a year. We found significant discrepancies in the passivation across different batches, which prompted a review of the synthesis conditions. We examined the gas dosing and found that the precursor gas ratios during ALD deposition were the primary descriptor correlating to the changes in AZO passivation properties. Careful monitoring and reproducibility of precursor dosing emerged as the key to achieving high surface passivation. To exemplify our yearlong findings, this work describes four recipes designed to investigate how deposition conditions influence surface passivation on n-type Si.
In this work, we vary the flow of gas precursors H2O, diethylzinc (DEZ) and TMA, such that four distinct recipes with varying gas partial pressures are achieved. The gas pressure profiles for the four recipes are shown in Fig. 1b. Modulating the precursor gas flow allows for the formation of H2O-deficient (blue curve), Zn-deficient (green curve), and Al-rich (purple curve) AZO films. The recipe enabling the highest passivation AZO is labelled “optimised”, shown as the orange curve. The absolute peak precursor pressures for each of the recipes are shown in Table 1, along with the H2O:
DEZ
:
TMA ratios.
Group | H2O pressure (mTorr) | DEZ pressure (mTorr) | TMA pressure (mTorr) | Ratio H2O![]() ![]() ![]() ![]() |
---|---|---|---|---|
Al-rich | 0.20 | 0.15 | 0.15 | 4![]() ![]() ![]() ![]() |
Zn-deficient | 0.20 | 0.125 | 0.125 | 4![]() ![]() ![]() ![]() |
Optimised | 0.20 | 0.15 | 0.125 | 4![]() ![]() ![]() ![]() |
H2O-deficient | 0.10 | 0.15 | 0.125 | 2![]() ![]() ![]() ![]() |
Fig. 2a shows the effective lifetime as a function of excess minority carrier density for the champion sample for each recipe. Each sample received a 20 min anneal at 500 °C, in a box furnace in ambient atmosphere, followed by a 10 min anneal on a hotplate at 450 °C. Table S1 (ESI†) displays the average and standard deviation iVOC for 5 samples fabricated and measured per condition. Table S2 (ESI†) shows the extraction of J0 and iVOC values (calculated using the models described in the ESI†) of the effective lifetime data on the champion samples from each profile.
The optimised passivation performance was achieved with a precursor pressure ratio H2O:
Zn
:
Al of 4
:
3
:
2.5, represented by the orange curve in Fig. 1b. The corresponding lifetime for the optimised ratio at 1015 cm−3 excess carrier density (ECD) is 3.38 ms. The ALD recipe used to synthesise this sample is subsequently referred to as ‘optimised’ since recipes were optimised for carrier lifetime. Fig. 2b displays a photoluminescence image for the champion sample for the optimised recipe, indicating acceptable uniformity of the achieved passivation. We note that a common reason for deficient passivation in a given sample could result from a lack of spatial uniformity across the sample area, arising from contamination in the ALD chamber. Fig. 2c illustrates the effect of post annealing at 450 °C, on a hotplate, after the initial 500 °C anneal for 20 min in a box furnace. At the hotplate annealing time of 20 minutes (following the furnace step), the maximum iVOC of above 741 mV was observed, while the iVOC after 10 minutes was marginally lower, at 738 mV, with this step providing the most significant increase in iVOC. 10 minutes of hotplate annealing was selected for the standard recipe as it allowed the rapid synthesis of samples for improved statistics, with iVOC values only marginally lower than the maximum achieved. We can also observe from Fig. 2c that longer hotplate annealing degrades the iVOC above the annealing time of 20 minutes. Possible explanations include the hydrogen effusion from samples or the growth of ZnO crystallites as reported for ALD TiOX.39 The lifetime curves were modelled to extract the surface recombination current density (J0s) for each specimen. A J0s of 0.87 fA cm−2 on each side was achieved for the optimised recipe. The effective lifetime and J0s as a function of ECD is plotted in Fig. S1a and b (ESI†), while the extracted iVOC is shown in Fig. S1c (ESI†). A corresponding iVOC is among the highest recorded for AZO passivation schemes, while the J0 is the lowest recorded.40–42 We note that our wafers are industrially compatible 135 mm thick n-type silicon. The passivation mechanism of the optimised sample was investigated further using surface photo-voltage measurements. Fig. S2 (ESI†) shows a modest negative charge concentration in the region of 1 × 1011–1 × 1012 q cm−2, fitting with the band bending extracted from the XPS discussed in the next section. To achieve a lifetime value of >3 ms, a defect density at the mid bandgap of Dit,mg < 1 × 1011 cm−2 is expected.43,44
The Al-rich recipe achieved a lifetime similar to the optimised recipe, with an identical iVOC of 740 mV, a lower lifetime at 1015 cm−3 ECD of 3.25 ms, and a slightly higher J0 of 0.88 fA cm−2. However, changing the recipe to be either Zn-deficient or H2O-deficient has a significant impact on the lifetime. The corresponding lifetime for these cases at 1015 cm−3 ECD was 1.62 ms and 1.12 ms, respectively. The iVOC was 733 mV and 727 mV for Zn-deficient or H2O-deficient recipes, respectively. Varying the precursor flow in the recipe impacts the amount of Al dopant incorporated into the film, which in turn may influence its structural and compositional properties. The differences in dopant concentration can affect the film's crystallinity, defect density, band bending, and overall uniformity, which may affect the passivation performance. Therefore, it is essential to examine how these variations alter the microstructure and elemental distribution, providing insight into the mechanisms that drive the observed differences in lifetime, J0, and iVOC across the different recipes.
Fig. 3ci presents a high-resolution transmission electron microscope (HRTEM) micrograph of a cross-section in the optimised recipe, showing the detailed nanolayer arrangement across the SiOx/AZO/AlOx stack. The nano-crystallites are visible in the AZO and are embedded in an amorphous AZO matrix, indicating the possible presence of phase boundary defects, which could act as sites of charge trapping or scattering, affecting the electronic properties. The elemental distribution zoom-in map was obtained via EDS (Fig. 3cii), revealing the spatial concentration of key elements: O (red), Si (green), Zn (yellow), and Al (blue). There is a consistent distribution of Zn, Al, and O within the AZO matrix, with sharp transitions at the c-Si interface, confirming high film uniformity. This film control is crucial for ensuring effective passivation and confirms successful Al incorporation via ALD. Atomic fraction profiles were obtained from the averaged EDS micrograph and are shown in Fig. 3ciii. The Al concentrations gradually taper off near the surface, indicating the well-distributed doping process in the AZO film.
The XRD and HRTEM results indicate high structural and compositional integrity for the optimised nanolayer AZO films. It is clear that the optimised ALD process (4:
3
:
2.5 ratio of H2O
:
Zn
:
Al) leads to excellent film conformality, a continuous interfacial SiOx, and controlled Al doping. The XRD data suggests that the slight densification after annealing improves the crystallinity without altering the overall phase. Additionally, the uniform Al distribution observed in the elemental analysis is expected to deliver effective doping, which increases the n/p charge carrier ratio at the Si surface via the field effect mechanism, improving passivation.
To further elucidate the role of Al incorporation in AZO films, X-ray photoelectron spectroscopy (XPS) analysis was conducted to examine the Al concentration across different precursor pressure profiles. XPS allows for a more detailed investigation into the chemical composition and distribution of Al within the films, thereby complementing the microstructural insights from HRTEM and XRD. AZO films prepared for XPS were deposited to a thickness of 50 nm and annealed under the same conditions as samples for lifetime measurements, without the AlOx capping layer so that the isolated AZO layer could be measured. XPS surveys (see Fig. S3, ESI†) exhibited Zn, O and Al core levels, as well as carbon, suggesting some surface contamination. The sample surfaces were then sputtered with an Ar+ ion gun and a second survey (see ESI†) showed the carbon peak had disappeared while the other core levels increased in intensity, indicating that surface contamination was removed but the AZO layer was not sputtered through.
The extracted Al 2p/Zn 3p3/2 ratios of core level intensities are shown in Fig. 4, demonstrating significant differences depending on the precursor purge pressures used. The core level peak fitting is shown for all samples in Fig. S4 (ESI†). These values could not be translated into absolute concentrations, as the relative sensitivity factors (RSF) for the measurement system were not known. EDS results would suggest these correspond to Al concentrations on the order of 5 at% while the difference in the ratio of the Zn and Al core levels is intended to provide a more robust fractional comparison between samples.
The XPS analysis demonstrates that the Al 2p/Zn 3p3/2 ratio does not linearly correlate with the partial pressure of the Al precursor, but rather is influenced more significantly by the Zn precursor purge pressure. Interestingly, the Zn-deficient sample, which exhibited the highest Al 2p/Zn 3p3/2 ratio, did not exhibit superior passivation (when compared to the effective lifetime curves in Fig. 2a), reinforcing the notion that optimised passivation is not merely a function of higher Al content but depends on a delicate balance between Zn and Al concentrations. Furthermore, the observation of a higher Al 2p/Zn 3p3/2 ratio after surface sputtering suggests that the bulk of the AZO film contains more Al than the air-exposed surface.
The combined structural, compositional, and chemical analyses provide a comprehensive picture of AZO chemistry. They suggest that effective passivation correlates with optimised Al doping, where both concentration and distribution within the ZnO matrix are relevant. The interaction between the Al and Zn precursors during deposition is crucial for tuning the material's properties, emphasizing the importance of precise ALD process control to optimise structural quality and passivation performance.
Hall effect measurements of AZO films with varying precursor pressure profiles were carried out in the same configuration as the vdP test. Fig. 5b shows the electron mobility (left axis, pink triangles) and carrier concentration (right axis, cyan hexagons). The optimised sample exhibits the highest mobility of approximately 80 cm2 V−1 s−1 and the lowest carrier concentration of 1.5 × 1019 cm−3. The Al-rich sample shows the lowest mobility and the highest carrier concentration. The H2O-deficient sample, compared to the Zn-deficient sample, exhibits higher carrier concentration. This likely arises from the reduction in oxygen precursor, which can increase oxygen vacancies, generate a large number of unpaired electrons on the surface, enhance the number of active sites, and thus increase the free carrier density.47
Fig. 5c illustrates the effect that annealing (450 °C, in air) has on the resistivity (measured by vdP) of the optimised sample. As the annealing time increases from 0 minutes (as-deposited) to 20 minutes, the resistivity steadily increases from 7 mΩ-cm to 72 mΩ-cm. This trend suggests that extended annealing might decrease free carrier concentration, which may be due to a reduction in oxygen vacancies.48–50 In our work, the AlOx capping layer was not present to allow resistivity measurements. However, Macco et al. have found that, when capped by the AlOx, the resistivity does not degrade during post-deposition annealing.32
The Al-concentration (as estimated from XPS) does not directly correlate to the carrier density measured via the Hall effect, suggesting differences in dopant activation, and that the efficiency of Al incorporation and activation varies depending on the specific synthesis regime. This may indicate a relatively inefficient dopant incorporation process when using TMA rather than DMAI, as was reported by Macco et al.37 Although the impressive carrier lifetimes demonstrated in this work suggest that TMA may have advantages for surface passivation.
We also investigated the optical properties of AZO nanolayers by Ultraviolet–visible (UV-vis) spectrophotometry. Transmission curves are shown in Fig. 6a, covering the wavelength range from 200 nm to 1200 nm. For wavelengths >600 nm, the transmittance remains above 98% for all samples, indicating good transparency. Notably, the optimised sample (orange curve) demonstrates the highest transmittance, while the H2O-deficient sample (blue curve) shows reduced transmittance, particularly in the UV region (<400 nm). The Al-rich samples exhibit the lowest transmittance across the spectrum, which is in good correlation with high carrier concentration due to the many-body band gap renormalisation effect.51,52 In highly doped n-type semiconductors, such as the Al-rich AZO, an increase in free electron concentration fills the lower energy states of the conduction band. As a result, photons with lower energy (longer wavelengths) cannot excite electrons into the conduction band, effectively “shifting” the absorption edge to higher energies. Meanwhile, the high carrier concentration increases free carrier absorption, where free electrons interact with incident light and cause lower energy photons to be absorbed. This explains why the Al-rich sample, with its elevated electron density, shows the lowest optical transparency across the measured spectrum.
In Fig. 6b, Tauc plots are used to determine the direct optical bandgap of the AZO samples. The bandgap values are extracted by fitting the linear region of the plot (αhν)2 versus photon energy and extrapolating to the intercept at (αhν)2 = 0. All the samples appear to have bandgaps clustered around 3.25 eV, with only slight variations. This suggests that while the precursor ratio affects the material properties, the differences in bandgap among these four samples are small. However, it can be observed from Fig. 6b that the Al-rich sample has the lowest measured optical bandgap of <3.25 eV.
Along with the valence band positions determined from XPS (see Fig. S5, ESI†) the band structures of each sample type (relative to the Fermi energy) are shown in Fig. 6c. The valence band positions are based on a linear extrapolation of the valence band edge from XPS, and the conduction band position is the inferred position from the optical bandgap values. Since these materials are expected to be degenerately-doped, we would expect that Eg = Ef − EV. For all cases but the optimised case, the bandgap inferred from XPS and the optical methods are aligned, implying degenerate doping, and in the case of the optimised sample, Eg,optical < Ef − EV, also consistent with degenerate doping, but possibly demonstrating the difference in measurement outcomes between absorption and XPS in the case of a partially-filled conduction band. The larger binding energy of the valence band compared to other samples suggests that the optimised sample is more highly doped. From this, we infer a larger offset between the valence bands of AZO and Si in the case of the optimised ALD recipe, which could produce a greater field-effect and so contribute to greater passivation. However, this result is inconsistent with the Hall effect results in Fig. 5b, where the carrier density was lowest in the optimised case and highest in the Al-rich case, and so does not provide a single answer for the improved passivation properties in the optimised case. Reasons for the inconsistency between valence band positions from XPS and carrier densities from the Hall effect could relate to a difference between annealed and non-annealed samples, a native space-charge region at the AZO top surface or Fermi-level shifts as a result of sputter damage-induced surface defects.
Estimates of the valence band offset between the AZO and the Si substrate in the case of the optimised lifetime sample are shown in Fig. 6d. Offsets were estimated from the XPS-extracted valence band maximum of the AZO, and the calculated valence band position for the Si wafer based on its known resistivity (4 Ω-cm) and dopant type (phosphorous). This yielded a valence band maximum 0.86 eV below the Fermi level. A direct measurement of the bulk Si valence band position with XPS was not considered as reliable as the calculation based on doping, since defects on the c-Si surface can significantly shift or pin the Fermi level53 and Fermi level pinning as a result of sputter damage has been reported in other photoemission studies.54 Taken together, these results implied a type II (staggered gap) alignment between the materials, with a valence band offset of 2.52 eV. Meanwhile, the offset as determined by the Kraut method55 (see ESI,† for calculation), with core level shifts at the interface used to determine band bending, implied a valence band offset of 3.25 eV, equal to the AZO bandgap measured by absorption, and so ambiguously suggesting either a type II or type III (broken gap) alignment. Time constraints prevented the measurement of all samples this way, meaning comparisons of the offset could not be made between samples Fig. 6.53 Regardless, a large valence band offset was observed between the AZO and Si, with direct interface measurements (Kraut method) indicating a significantly larger offset than implied by the bulk valence band maximum positions. This large offset may have a positive impact on field-effect passivation but could be detrimental to contact resistance. Comparisons of the offset could not be made across all sample types, but will be a priority for future studies.
The combined electrical and optical analyses reveal certain correlations between the carrier concentration, mobility, resistivity, and transmittance of AZO films and the precursor ratios used during their deposition. The Al-rich sample, with the highest carrier concentration, suffers from reduced mobility and lower optical transmittance, which may result from increased free carrier absorption and the many-body band gap renormalization effect. In contrast, the optimised sample balances carrier concentration and mobility, resulting in low resistivity and high transmittance, making it ideal for both transparent conductive and passivation applications. The Zn-deficient and H2O-deficient samples show higher carrier concentration, lower mobility, and lower optical performance than the optimised one, emphasising the importance of proper DEZ and H2O levels in optimising film properties. This relationship underscores the need to precisely control ALD conditions to tune AZO films for specific optoelectronic applications.
In addition to the precise control of AZO film fabrication conditions, the trade-off between conductivity and transparency regarding TCO thickness is a critical aspect of solar cells and other optoelectronic devices. Therefore, we investigated the AZO film resistivity under different thicknesses and included ESI,† in Fig. S6. Note that all the AZO films were deposited using the optimised recipe. It is clear that increasing thickness leads to increased conductivity.
From ellipsometry, we fitted the n, k, and thickness values of all the samples from different pressure profiles, as listed in Table S3 (ESI†). Fig. S7 (ESI†) illustrates the fitting curve for the optimised recipe. As shown in Table S3 (ESI†), ∼20 nm (Zn-deficient, optimised) and ∼23 nm AZO (Al-rich, H2O-deficient) samples were analysed in ellipsometry, leading to a variation of a magnitude of 10−2 in the k value at 600 nm wavelength. However, the total transmittance metric does not comprehensively describe device performance as it disregards the interference effects. Therefore, we simulate and find optimised thicknesses for AZO layers that account for all-optical phenomena. Using n and k values from Table S2 (ESI†), we simulated the expected optimised Jsc with AM 1.5G illumination and 100% EQE, with all simulation details provided in the ESI.† Fig. 7 presents a contour plot of the maximum achievable efficiency for a silicon heterojunction cell, incorporating different TCEs, assuming only optical, Auger and series resistance losses are present. Due to varying optical coupling at different TCE thicknesses, a MgF anti-reflection layer is incorporated to provide a just comparison between TCEs.
The x-axis shows the TCO sheet resistance (Ω sq−1), while the y-axis displays the normalised short-circuit current density (Jsc/Jsc,max). A variety of TCEs, including AZO, hydrogen-doped indium oxide (H:IOx),56 IWO,57 zirconium oxide-doped indium oxide (IZRO),58 ITO59 are evaluated, with varying thicknesses ranging from 20 to 120 nm. AZO films exhibit the best balance of sheet resistance and device current density at thicknesses near 60–80 nm, promising an efficiency potential of >26.5%. Modelled devices using IZRO, H:IOx, and IWO films demonstrate the strongest performance at thicknesses ∼60 nm as well, showing a good balance between device current density and resistance. Additionally, the model indicates that further reducing sheet resistance below 100 Ω sq−1 yields diminishing returns in terms of efficiency, where the films which maximise photon management, and thus current density, enable more substantial gains. This suggests that optimising both the TCE material and thickness is critical for maximizing solar cell performance, with AZO showing potential to achieve performance close to that of high mobility indium-based TCOs such as IZRO, and H:IOx, while matching that of IWO.
The thickness of the thin films was measured using ellipsometry (JA Woollam). The modelling parameters used for AZO were refractive index (n) ranging from 1.6 to 2.1, and extinction coefficient (k) ranging from 0 to 0.4 from 210 to 1690 nm wavelength. XRD (θ–2θ) measurements were carried out using a Rigaku miniflex with a Cu K-α1 source (1.541 nm wavelength), over a range of θ = 10–90°, at 0.05° per second.
XPS was employed to analyse the elemental ratio of Al and Zn in the films based on the integrated intensity of the Zn 3p and Al 2p core level peaks. Monochromated XPS measurements of the core levels were carried out with an Al Kα X-ray source (1486.6 eV), using a hemispherical analyser with the pass energy set to 26 eV. The Al 2p core level was observed to be weak in all samples, consistent with the expected Al concentrations of a few at%. The Al 2p/Zn 3p3/2 ratio was estimated from spectra taken after sputter cleaning, by fitting the core level peaks using CasaXPS to extract the integrated intensity, with the fits shown in Fig. S4 (ESI†). Translating these values to an Al concentration requires knowledge of the RSF which is specific to the XPS instrument used. Because RSF values were not available for the spectrometer used for in this work, the absolute values of concentration could not be known in this case. However, the trends in Al 2p/Zn 3p3/2 ratios between the samples should nevertheless be representative. The ESI,† explores the impacts of sputtering on the estimated Al 2p/Zn 3p3/2 ratios (Fig. S8, ESI†), but due to the possibility of surface contamination, sputter cleaning of samples was considered necessary for accurate results.
The valence band offsets could be estimated from the Kraut method by directly measuring the band bending at the AZO/Si interface. The interface was characterised by in situ sputtering through the AZO layer at 4 kV for 15 min using an Ar+ ion gun, such that a thin (∼1 nm) layer of AZO remained on the Si surface, thin enough that photoelectrons from the Si 2p core level escape through the AZO layer to be measured (Fig. S9, ESI†). In this interface region, the Si and Zn core levels are expected to shift compared to their bulk values by an energy equal to the shift in Si and AZO valence bands at the interface55 (the exact calculation is described in the ESI,† eqn (S1)). Therefore, we measured the position of the Zn 3p and Si 3p core levels at this interface region. The AZO valence band position at the interface was determined from the bulk AZO valence band, shifted by the difference between the bulk and interface Zn 3p core levels. Meanwhile, the Si interface valence band position was determined by adding a fixed value of 98.95 eV to the binding energy of the Si 2p core level, as this is well-defined for Si.61 The bulk valence band for the Si was then determined from its known doping level using tools available on PVLighthouse.62 The difference between the interface and bulk valence band positions corresponded to the interface band bending, and provided an estimate of the valence band offset between AZO and Si that took account of this phenomenon. This was only performed for the optimised lifetime sample, due to constraints on equipment access which prevented measurement of all sample types.
To characterise charge concentration in the AZO layer the surface photovoltage (SPV) was measured using a KP Technology Scanning Kelvin Probe (SKP5050) and a 10 mW cm−2 halogen lamp. A 1 × 1 cm map containing 36 points was measured using a 2 mm gold probe. The analysis of the charge was carried out using software available at https://github.com/OxfordInterfacesLab/. To complement the SPV measurements, the band bending at the Si surface was extracted using the Si 2p core level spectra obtained from XPS.
PCD lifetime measurements were conducted at room temperature using a Sinton WCT-120 lifetime tester, which were operated in an ambient air environment. In addition, PL imaging was utilised to evaluate the surface passivation uniformity of the AZO/AlOx stacks. The sheet resistance of AZO was measured using the van der Pauw method with gold metal probes in direct contact with the AZO surface, as close to the edge as possible. Under a perpendicular magnetic field of 0.3 T, carrier concentration and mobility were determined by measuring the Hall effect technique. For both van der Pauw and Hall effect measurements, signal generation and data acquisition were conducted using a Keysight B2901A Source Measuring Unit.
A Cary 5000 UV-vis spectrophotometer was utilised to investigate the optical properties of the AZO, from which the optical band gap was estimated using a Tauc plot. Tauc plots of the film's optical absorption were constructed to extract optical bandgaps, which were then combined with XPS results to create a complete model of the electronic band alignment at AZO-Si interfaces. Transmission measurements were carried out on single-sided 40-nm-thick AZO samples deposited on fused quartz substrates (to enable measurements at UV wavelengths) over a wavelength range of 200 to 1200 nm (to capture the relevant spectral features).
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d4ya00552j |
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