Screen-printing provides an economically attractive means for making Ag electrical contacts to Si solar cells, but the use of Ag substantiates a significant manufacturing cost, and the glass frit used in the paste to enable contact formation contains Pb. To achieve optimal electrical performance and to develop pastes with alternative, abundant and non-toxic materials, a better understanding the contact formation process during firing is required. Here, we use in situ X-ray diffraction during firing to reveal the reaction sequence. The findings suggest that between 500 and 650 °C PbO in the frit etches the SiNx antireflective-coating on the solar cell, exposing the Si surface. Then, above 650 °C, Ag+ dissolves into the molten glass frit – key for enabling deposition of metallic Ag on the emitter surface and precipitation of Ag nanocrystals within the glass. Ultimately, this work clarifies contact formation mechanisms and suggests approaches for development of inexpensive, nontoxic solar cell contacting pastes.
By far the most commercially viable option for photovoltaic energy generation, crystalline silicon (c-Si) continues to dominate the industry with over 90% market share. Optimally designed silver (Ag) front-contacts in the majority of c-Si solar cells utilize narrow grid lines (approximate width of 50 μm) to minimize shading loss and achieve high current, high fill factor, and hence, high photo-conversion efficiency. While screen-printing provides an economically attractive means for making these contacts, owing to suitability for high-volume manufacturing, the use of Ag adds significantly to the solar cell cost. Furthermore, despite more than three decades of use in photovoltaic manufacturing, the mechanism of contact formation during the firing of screen-printed contacts remains a subject of debate. Achieving optimal firing conditions to minimize contact resistance, and to develop new pastes with alternative materials (that is, earth-abundant and non-toxic), requires a detailed understanding of the contact formation process. In situ X-ray diffraction (XRD) data obtained during rapid-thermal processing (RTP) of Ag-paste materials reveal that there are multiple competing anti-reflective layer burn-through and Si oxidation reactions occurring with different temperature thresholds. The primary reactive species responsible for burn-through is lead-oxide (PbO), and these PbO driven redox reactions lead to liquid Pb formation and reversible Ag–Pb alloying during firing. Our in situ experiments also elucidate factors affecting dissolution of Ag into the frit and subsequent nanocrystal precipitation – key for achieving low contact resistance.
Typically, screen-printing contacts onto the n-type emitter of a p-type c-Si solar cell employs a paste consisting of Ag particles, organic binders and metal-oxide glass frit. The frit, usually a PbO-based borosilicate glass, promotes a series of reactions allowing electrical contact to the emitter after deposition of the silicon-nitride (SiNx) anti-reflective and passivation layer during contact firing. Although the frit has long been known to enable this process1, conflicting arguments bring into question the specific role of the frit to enable SiNx burn-through and the mechanism of Ag transport to the c-Si surface. Hence, the actual electrical contact formation pathway remains scarcely understood – largely because previous investigations lacked in situ measurement capabilities with the temporal-resolution and operating temperature range necessary to observe these processes in real-time.
Reactions responsible for contact formation occur during rapid heating, with ramp-rates of 50–100 °C s−1, at temperatures of 500–800 °C. In general, the Ag-paste is well known to penetrate the SiNx layer during firing by oxidation, and the resulting silicon-oxide (SiO2) reaction product becomes incorporated into the molten frit. However, the associated oxidation reaction remains in question, since this can occur in one of several ways. The two most frequently cited arguments suggest either that SiNx is oxidized by PbO in the frit by2,3,4:
The second case is perhaps less obvious, since Ag2O itself readily decomposes under thermal activation, and so may not seem an obvious reactant at contact firing temperatures. However, Ag2O becomes more stable when bound in certain glasses, and therefore, technically both reactions (1) and (2) are thermodynamically feasible. In situ results presented in this work reveal the dominant SiNx burn-through reaction.
After SiNx opening, Ag contacts the Si emitter. Electrical conduction in fired contacts relies largely on tunneling through a layer of re-solidified glass frit, which forms between the c-Si surface and Ag bulk during firing. Distributed precipitation of Ag and Pb nanocrystals within the glass enables the tunneling9,10,11. Minimizing the glass intermediate layer thickness, inducing Ag sintering and promoting a controlled amount of Ag deposition on the c-Si surface (without spike-shunting the junction), are said to impart low contact resistance12. Here, certain additional details remain in question. For instance, the means by which Ag deposits onto the emitter is not obvious. According to some authors the deposition of Ag on the emitter requires the Ag to first oxidize by:
Not all agree with the Ag2O-based deposition model. Schubert (ref. 15) and Horteis16 argue that Pb formed in reaction 1 lowers the Ag–Si interaction temperature such that when the molten system phase separates upon cooling Ag deposits on the Si surface and within the glass layer. Sopori et al.17 agree with an Ag–Si alloy-assisted contact formation mechanism, and suggest involvement of other metal solvent species to further depress the melting temperature. In addition, the extent of Pb formation, argued to assist in Ag sintering, has been questioned. Thus, ambiguity persists regarding details of metal transport and precipitation, the extent of Ag–Pb alloying, the extent of Ag–Pb–Si alloying if any occurs at all, and therefore the keys for achieving low contact resistance.
Here, direct observation of SiN etching by PbO and Ag2O during different stages of firing using in situ XRD reveals the burn-through reaction and contact formation sequence. Studies on Ag, frit, c-Si and SiN model systems show a strong dependence of Pb formation, and hence Ag–Pb alloying, on oxygen (O2) partial pressure during firing. In addition, Ag dissolution into the glass frit, and hence the resulting abundance of Ag precipitate formation, shows a strong O2-dependence. This investigation finds the Ag redox reactions only occur with sufficient O2 at temperatures higher than 650 °C – negating a role of Ag in opening of the antireflective-coating at lower temperatures. Our findings also explain increased Pb formation observed when firing in a N2 atmosphere compared with air. Understanding the temperature thresholds for each of these competing mechanisms accurately clarifies the nature of screen-printed, fast-fired contacts.
Powder model system
Model systems containing Ag nanocrystals, PbO-based frit, SiNx and c-Si, in varying combinations, have been fired in an air or nitrogen (N2) atmosphere and characterized using an in situ XRD/RTP apparatus18. Use of powder model systems enabled characteristic XRD data acquisition with short collection intervals (<1 s), with high signal-to-noise achievable due to high interface area between reactants of interest within the sampled volume. This allowed detection of varying reaction species abundance with high sensitivity during rapid heating and cooling with temperature profiles analogous to solar cell contact firing conditions. This provides a unique opportunity to observe the reaction sequence in real time; such detailed analysis is impossible to perform on an actual Ag contact on a solar cell during firing in a belt-furnace. Results at the end of this section show that the powder mixture model systems fired by RTP in the present study behave analogous to fast-fired contacts made by screen-printing with conventional Ag pastes. Sample preparation and measurement procedures are explained further in the Methods section.
XRD patterns measured during firing of a frit/SiNx (1:1 molar ratio) mixture in air to 800 °C (Fig. 1a) demonstrate the in situ measurement capability. The frit and amorphous-SiNx generate only weak, broad diffraction, in the initial patterns. However, sharp crystalline-Pb peaks emerge after firing, as the system cools below 327 °C (the melting temperature of Pb), which substantiates evidence of reaction 1. Results from analogous measurements on Ag/frit/SiNx mixtures (Fig. 1b), fired to 500, 600, 700 and 800 °C, in air and N2, provide insights concerning the temperature threshold to initiate SiNx etching, the accompanying Pb formation, and hence the extent of Ag–Pb alloying during contact firing.
As shown in Fig. 1b, which plots the ratio of Pb(111) integrated intensity to that of Ag(111), varying amounts of Pb form depending on both the maximum temperature and the firing atmosphere. Pb is not detected upon heating to 500 °C, whereas heating to 600 °C induces measurable Pb in both air and N2. Trend-lines show the amount of Pb increasing progressively with maximum firing temperature. Heating in N2 promotes Pb formation significantly compared with firing in air. Analogous behavior is observed in experiments with Ag/frit/c-Si, wherein PbO oxidizes c-Si by:
Enhanced Pb formation in N2 is explained by irreversible PbO reduction. In air, when Pb forms by reaction 1, it tends to react with O2, or Ag2O in the frit if present, and oxidize back to PbO by:
respectively. Thus, it seems regeneration of PbO by reactions 6 and 7 allows complete SiNx etching despite a very small loading of PbO in the Ag paste (about 2 wt.%), as these reactions perpetuate the burn-through process.
Burn-through reaction sequence revealed
Figure 2 shows diffraction patterns obtained from an Ag/frit/SiNx/Si mixture at different stages of firing. The Si diffraction decreases during heating between 550 and 750 °C, and does not recover upon cooling. This suggests oxidation of c-Si by Ag2O (reaction 4) and/or PbO (reaction 5). The Ag peaks initially narrow during temperature ramping as a consequence of Ag grain growth by sintering and ripening. Then on further heating to temperatures above 650 °C the Ag peak intensity diminishes, and a diffuse peak emerges near the Ag (111) peak (that is, at Q≅2.7 Å−1). The emerging diffuse peak is attributed to scattering from an amorphous phase, such as liquid metal (possibly Pb or Ag–Pb alloy), which is not present at room temperature and becomes most intense at the max temperature (825 °C) where the Ag peak intensity is a minimum. On cooling, the diffuse peak disappears while the Ag peaks gain intensity and broaden. Most likely, Ag peak broadening reflects contributions from newly formed Ag nanocrystals that precipitate within the glass during cooling. Pb peaks appear below 327 °C.
Loss of Ag diffraction intensity during temperature ramping most likely follows from one of two possible mechanisms: Pb formed by redox reaction with SiNx alloys and melts Ag, or Ag oxidizes and dissolves into the molten frit by reaction 3. In fact, the present study finds that both mechanisms occur, though with different onset temperatures. Examining the intensity trends versus time and temperature allows decoupling of the competing mechanisms. Figure 3 shows the corresponding temperature profile versus time along with Ag, Si and Pb integrated intensities. The Si diffraction intensity begins to decrease at about 10 s (500 °C). Then, the Ag peak intensity begins to diminish 5 s later, at about 14 s (650 °C). As the Ag signal begins to drop, the rate of Si signal loss accelerates markedly. Loss of Si signal results from Si oxidation by either PbO or Ag2O in the frit. Ag dissolution into the molten frit by reaction 3 must occur before etching by Ag2O (reaction 4). Since the Si signal decreases before the onset of Ag intensity loss, the low temperature oxidation (<650 °C) must be dominated by reaction with PbO in the frit (that is, by reaction 1). The observation of Pb diffraction upon cooling below 320 °C supports this interpretation, as this confirms formation of Pb.
Excellent agreement between the onset of Ag intensity decline and increased rate of Si oxidation at 15 s (650 °C) suggests a change in the dominant oxidation reaction during temperature ramping – most likely the onset of Si etching by Ag2O (reaction 4). Indeed, with Ag being the most noble metal in the system, Si oxidation by Ag2O, if present, should dominate given its thermodynamic favorability compared to reaction 1 (ref. 4).
Involvement of Ag in SiNx burn-through unlikely
Examining the nature of Ag dissolution into PbO-based frit under varying temperature conditions negates the possibility of Ag participation in SiNx removal during the early stages of contact firing. To test this, Ag/frit mixtures (5 wt.% Ag) were isothermally annealed at 600 and 700 °C for 10 s. As shown in Fig. 4, annealing at 600 °C induces only a modest increase in Ag(111) intensity, probably due to grain growth. On the other hand, at 700 °C, the Ag intensity decreases and only 30% of the initial intensity remains after 10 s. The loss of Ag diffraction intensity implies about 70% Ag dissolution into the frit by reaction 3. Therefore, Ag dissolution into the frit must occur with a temperature threshold between 600 °C and 700 °C, and hence, oxidation of SiNx or Si (observed onset temperature is approximately 500 °C) below this temperature range cannot involve Ag+ ions. The majority of SiNx oxidation during temperature ramping must therefore be attributed to redox reactions with PbO.
Monitoring the Ag peak intensity during firing reveals the extent of Ag dissolution into the glass under varying conditions. Notably, the response of an Ag/frit/SiNx/Si mixture strongly depends on whether firing occurs in air or N2 (Fig. 5). During heating, the Ag peaks initially become sharper as a consequence of grain growth, and the intensity increases slightly. Then, above 650 °C (about 15 s), the Ag intensity diminishes continuously with increasing temperature up to the maximum temperature of 810 °C (about 20 s). In both cases, air and N2 atmosphere, the Ag peak intensity recovers during cooling, albeit to a different extent. In air, as applies in solar cell manufacturing, the Ag signal intensity decreases to approximately 50% at maximum temperature, and then recovers to about 75% of the initial value on cooling. On the other hand, when firing in N2, the Ag signal intensity drops to just 10% of the initial value at the maximum temperature, and then recovers completely upon cooling.
The different behavior in air versus N2 reflects the different forms of Ag during firing, respectively. According to the equilibrium Ag–Pb phase diagram, metallic Pb formed by redox reactions between PbO and SiNx readily forms a liquid alloy with Ag in this temperature range. As was previously shown, more Pb forms in N2 due to irreversible reduction of PbO (Fig. 1b). Hence more Ag–Pb alloying occurs in N2, which is almost entirely reversible due to low miscibility of Ag and Pb solid phases at lower temperatures. On the other hand, Fig. 4 showed that Ag dissolves readily into the glass in the presence of O2 above 650 °C. Thus, in the case of firing in air, the dip in Ag signal reflects both Ag–Pb alloying and Ag dissolution, whereas only the former occurs in N2. In air, some of the Ag signal recovers as Ag nanocrystals precipitate within the glass upon cooling as a consequence of the temperature-dependent solubility. However, weak scattering from nanocrystals having a diameter below 2 nm, as are commonly seen in cross-sections of fired contacts11,12,13,14, and Ag remaining bound as Ag+ within the glass, are both consistent with lower Ag signal detected after firing in air.
Before considering implications of these results on screen-printed solar cell contacts, it is important to show that the model systems used in the present work behave representatively. Figure 6 shows a cross-section SEM of our model frit system with inverted Ag pyramids penetrating the surface of the c-Si substrate beneath the Ag/frit/SiNx mixture after firing. The Ag pyramid formation observed here is analogous to that observed in numerous prior studies on fired Ag contacts3,7,13,15,16. Therefore, our frit, powder mixtures and firing conditions clearly mimic the screen-printed contact firing process. Interestingly, in this case, the mixture contained a larger proportion of frit (1:1 frit/Ag) compared with common Ag pastes used in solar cell contacts (typically lower than 0.1:1), which seems to have induced a larger characteristic Ag pyramid size compared with most other studies.
A complete picture of the contact formation process, consistent with all previous findings and informed by the present in situ results, emerges as follows: during firing, above 500 °C, the frit melts and wets the Ag/SiNx interface. Between 500 and 650 °C, PbO in the frit reacts with and penetrates the SiNx anti-reflective layer by reaction 1, as shown in Fig. 7a. Pb formed during the burn-through process alloys with and assists in liquid-phase assisted sintering of Ag (Fig. 7b). Above 650 °C, Ag dissolves into the frit and diffuses towards the emitter surface. In the vicinity of the Si emitter surface, Ag ions are consumed by redox reaction 4, which oxidizes Si to SiO2 and deposits metallic Ag on the emitter surface (Fig. 7c). SiO2 formed by reaction 4 is incorporated into the molten frit. On cooling, the solubility of Ag in the melt decreases and nanocrystals precipitate from within the glass matrix. Kinetic constraints limit grain growth during fast cooling, resulting in a high density of distributed nanocrystals within the glass intermediate layer (Fig. 7d).
In summary, Ohmic contacts with low resistivity result when Ag crystals form within a thin glass intermediate layer and on the emitter surface; thus, in general, it would seem optimal contacts result with adequate heating to achieve complete SiNx opening and abundant Ag precipitation within the glass. At the same time, over-firing must be avoided both to prevent excessive Ag deposition onto the emitter – Ag spikes – which can shunt the pn-junction in extreme cases, and to minimize SiO2 generation, which increases the thickness of the glass layer and diminishes carrier tunneling.
In the larger effort to replace costly Ag and toxic Pb in the solar cell manufacturing sector, the present study offers several insights. To replace Ag with an alternative, low-resistivity metal, assuming suitable work-function alignment for contacting Si, analogous use will require the metal have variable solubility in a frit system within a comparable temperature range (below 800 °C). The PbO-based frit may be replaced by a frit system containing another metal-oxide that alloys with the primary contact metal upon metal-oxide reduction and provides a low glass transition temperature. This is a necessary condition to achieve wetting and adhesion at the contact interface. The frit must contain a reactive species with a negative redox potential in relation to SiNx, and preferably to both SiNx and Si. Ultimately, metal solubility and transport kinetics enabling nanocrystal precipitation within the glass upon cooling, which allows carrier tunneling (that is, ohmic contact formation), depends strongly on the frit composition. Thus, the metal and accompanying frit used in the paste must be developed in tandem.
Ag, frit, SiNx and c-Si model systems in this study have been characterized as powder mixtures. Our model, controlled PbO-based frit was synthesized following ref. 15 by quenching a molten mixture of PbO (60 mol%), SiO2 (30 mol%) and B2O3 (10 mol%), and then milling to form a powder. Ag nanocrystals and SiNx powder was purchased from Sigma-Aldrich, and c-Si nanocrystals were from Nanostructured and Amorphous Materials, Inc. Samples of varying composition were mixed to desired proportions in dry form, and then deposited onto 20 × 20 mm Si wafer substrates using isopropyl alcohol as a dispersing agent. Multiple samples were characterized for each test condition to ensure the reliability of the data.
Measurement and heating
Our model systems were fired at heating rates around 100 °C s−1 and characterized by XRD in real-time using a synchrotron-mounted, RTP apparatus, equipped with a Pilatus, Dectris 300 K area detector, with 250 ms integration time (4 Hz sampling frequency). Specifics of the in situ XRD/RTP apparatus can be found elsewhere18. Briefly, the in situ RTP chamber was gold-coated aluminium enclosure with four high-power quartz-tungsten-halide lamps (750 W each). The chamber is sealed and plumbed to allow atmosphere control. Al coated Kapton windows were used to allow high X-ray transmission while containing heat during thermal processing. The RTP chamber body was water cooled by means of a chiller. Firing under N2 atmosphere was accomplished by purging the RTP chamber for 5 min prior to heating. In situ temperature measurements were obtained using a thermocouple, and cross-referenced based on calculations using the Ag diffraction signal (that is, the temperature dependence of the Ag lattice). This method provides a high level of accuracy in temperature measurement.
Analysis of in situ XRD datasets was accomplished by fitting peaks with Pearson VII functions. The integrated area of the diffraction peak for a given phase corresponds directly with its abundance, which allowed extraction of phase-evolution trends versus time for the individual species of interest.
Cross-section SEM was performed using an FEI Nova NanoSEM, with a working-distance of 4.4 mm, accelerating potential of 10 kV and 1.3 mA operating current.
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This project is funded through the Bridging Research Interactions through collaborating the Development Grants in Energy (BRIDGE) program under the SunShot initiative of the Department of Energy (DE-EE0005951). Sample preparation and SEM analysis were performed at the National Renewable Energy Laboratory, which is operated under the prime contract no. DE-AC36-08GO28308. In situ characterization was performed at the Stanford Synchrotron Radiation Laboratory, a national user facility operated by Stanford University on behalf of the US Department of Energy, Office of Basic Energy Sciences, under contract no. DE-AC02-76SF00515. We thank Bobby To at NREL for performing the SEM analysis, and Ron Marks and Bart Johnson at SSRL for assistance with beam line 7-2.
The authors declare no competing financial interests.
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Fields, J., Ahmad, M., Pool, V. et al. The formation mechanism for printed silver-contacts for silicon solar cells. Nat Commun 7, 11143 (2016). https://doi.org/10.1038/ncomms11143
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