Jia
Guo
a,
Andrey
Berenov
a and
Stephen J.
Skinner
*ab
aDepartment of Materials, Imperial College London, Exhibition Road, London, SW7 2AZ, UK. E-mail: s.skinner@imperial.ac.uk
bInternational Institute for Carbon Neutral Energy Research, Kyushu University, Fukuoka, Japan
First published on 8th July 2024
Exsolution, an innovative method for fabricating perovskite-based oxides decorated with metal nanoparticles, has garnered significant interest in the fields of catalyst fabrication and electrochemical devices. Although dopant exsolution from single perovskite structures has been extensively studied, the exsolution behaviour of double perovskite structures remains insufficiently understood. In this study, we synthesized B-site double perovskite Ru-doped lanthanum nickel titanates with a 7.5 at% A-site deficiency, and systematically investigated the exsolution process that formed nickel metal nanoparticles on the material surface, across a broad reduction temperature range of 350–1000 °C. Both Ex situ and in situ characterization revealed that small, uniform Ni nanoparticles exsolved at low temperatures, whereas the exsolution of ruthenium required higher reduction temperatures beyond 1000 °C. Within the reduction temperature range of 350–500 °C, a notable finding is the reconstruction of exsolved nanoparticles, implying that Ni particles exist in a thermodynamically metastable state. Electrochemical impedance spectroscopy (EIS) showed a decreased area specific resistance (ASR) during the progress of exsolution. The increase in current density of a full solid oxide cell (SOC) in electrolysis mode and the doubling of peak power density in fuel cell mode attributed to the exsolution of Ni nanoparticles highlight the potential application of metal exsolution in electrode materials for SOCs.
Exsolution includes multiple steps including reduction-induced oxygen vacancy generation within the oxide lattice, subsequent cation migration, nucleation, and nanoparticle growth.6,7 Studies on exsolution gained particular attention after Neagu et al.8 proposed controlling and tuning exsolved nanoparticles, promoted through the presence of A-site deficiency in a perovskite lattice. The presence of A-site deficiency facilitates the spontaneous exsolution of localized B-site ‘excess’ to restore local stoichiometry, and also suppresses the structural decomposition of the perovskite into the component oxides. A subsequent investigation into the interface between exsolved Ni nanoparticles and the lanthanum strontium titanate bulk substrate revealed a unique ‘socketed’ structure, which contributed to high thermal stability and excellent coking resistance, without sacrificing catalytic activity.9 These findings prompted a surge of interest in exsolved nanoparticles across diverse applications in catalyst development and electrochemical devices, including SOCs,10–18 water splitting catalysis,19–27 ammonia reaction catalysis,28–35 hydrocarbon reforming36–48 and CO2 electrolysis.49–61
The exsolution process was widely believed to be influenced by both internal and external factors. Intrinsic factors include defects, dopants, elemental composition, defect concentrations, strain, and facet effects, with defects such as A-site deficiency playing a pivotal role.7,8 A-site deficiency promotes the generation of oxygen vacancies, facilitating the exsolution of B-site cations62,63 and serve as active sites for nanoparticle nucleation.64 The host lattice and dopants influence the type, morphology, and population of exsolved nanoparticles, while strain and facets affect cation and oxygen vacancy formation, thus impacting exsolution behaviour.8,9,65–67 Among the extrinsic factors, reduction temperature is of paramount importance, and it can be readily managed. Tang et al.68 found that Rh cation exsolution from La0.43Ca0.37Rh0.01Ti0.99O3 preferred to nucleate at lower temperatures (500–700 °C), while particle growth occurred above 700 °C. Similarly, Cao et al.69 employed in situ transmission electron microscopy (TEM) to observe the exsolution process of Ni cations from LaNiO3 over time. Ni exsolution onset was noted at 600 °C with a preference for exsolution at grain boundary positions. Consequently, the exploration of external parameters such as reduction temperature is critical for understanding their impact on modulating the morphology and distribution of exsolved nanoparticles.
Double perovskite oxides, especially A2BB′O6, where A = rare earth, B, B′ = transition metal oxides, exhibits a distinctive crystal structure capable of hosting different elements at the B-site. This structural characteristic renders them highly applicable in SOCs. Yang et al.70 applied Co-substituted Sr2Fe1.5Mo0.5O6−δ as the anode of SOFCs. Exsolution of Co metal nanoparticles greatly enhanced peak power density and the stability of anode materials, in which degradation was negligible for 190 hours in syngas and 300 hours in methane. Similarly, Wu et al.71 investigated the performance of the Sr1.9Fe1.5Mo0.4Cu0.1O6−δ double perovskite anode with the exsolution of Fe and Cu phases, showing a great enhancement in power density at 800 °C of up to 1.2 W cm−2 in an electrolyte-supported SOFC. Yet, the exsolution phenomenon of metal nanoparticles from double perovskites and the influence of intrinsic and extrinsic factors still poses a challenge. Despite being a topic of interest, only a few studies have investigated this, for example, Du et al.72 studied Co–Fe exsolution from the Sr2FeMo0.65Co0.35O6−δ, proposing the similarities of lattice structure of the metal phase and perovskites reduced the interfacial energy and stabilized the exsolved nanoparticles, whereas the impact of external factors on morphology remains unexplored.
In our previous work,73 a low-temperature exsolution between 350–500 °C was observed in A-site deficient La1.85NiRuO6−δ double perovskite samples, while the reduction temperature was found to have an impact on the particle size and distribution. However, the influence of the B-site cation ratio on this process remains insufficiently explored. To better separate the inherent B-site cation exsolution and the dopant exsolution, in this work, Ru-doped lanthanum nickel titanate double perovskites were adopted and their exsolution behaviour explored with reduction temperatures ranging from 350 °C to 1000 °C. The morphology of the materials reduced at high temperature (800 °C) and low temperature (450 °C) were studied, while in situ scanning transmission electron microscopy (STEM) coupled with energy dispersive X-ray (EDX) analysis was utilized to reveal the morphology changes of the double perovskite samples during the heating and reduction process. The electrochemical impedance spectra (EIS) reflecting the exsolution behaviour at different reduction temperatures and I–V curves of single SOCs were also studied, suggesting the potential of the nanoparticle decorated double perovskite as SOC electrodes.
The electrochemical performance of the symmetrical cell (L1.85NTR/LSGM/L1.85NTR) was assessed through electrochemical impedance spectroscopy (EIS) to investigate exsolution processes at specific temperatures. A two-probe geometry was implemented using Pt mesh current collectors attached to opposite sides of the symmetrical cell. A frequency response analyser (Solartron Modulab XM ECS) was connected to the configuration, operating within a frequency range of 1 MHz to 50 mHz. The impedance spectra were measured while supplying 5% H2/Ar gas at a rate of 200 ml min−1 to the symmetrical cell. The Zview software (Version 3.5 by Scribner Associates, USA) was employed for the analysis of acquired EIS spectra. Full cell I–V curves and impedance spectra were obtained by placing the L1.85NTR/Hionic™ Electrolyte/LSM-GDC single cell in a rig based on an alumina tube sealed with ceramic sealant (AREMCO, lot No. 668-1263). Measurements were carried out at 850 °C with a thermocouple placed next to the sample to make sure thermal equilibrium was achieved. 50 ml min−1 hydrogen with 3% H2O was fed to the L1.85NTR electrode whilst the LSM-GDC electrode was kept in static air during the measurement. Similar two probe connections and EIS measurements were adopted, and a Solartron Modulab XM ECS was used to conduct the impedance measurements and DC controlled linear sweep voltammetry. Thermogravimetric analysis (Netzsch STA 449c F5) was utilized to understand material stability as a function of temperature under a flowing 5%H2/Ar atmosphere. After a correction run with an empty crucible, approximately 40 mg of the sample was loaded into a Pt crucible and heated to 1000 °C at a rate of 10 °C min−1. The change in mass was subsequently analysed using Netzsch Proteus software.
Similarly, XRD and Rietveld refinement were employed to study the 7.5 at% A-site deficient phase, denoted as L1.85NTR. As with L2NT and L2NTR, space group P21/n based on reference ICSD186433,78 was employed to analyse the XRD pattern of the A-site deficient double perovskite L1.85NTR using Rietveld refinement, as illustrated in Fig. 1c and S2 (ESI†). The green arrows indicate two subtle features in Fig. S2 (ESI†), which were attributed to Cu Kβ diffraction peaks. These peaks arose due to the unavoidable incomplete filtering of the X-ray source and were excluded during the refinement fitting process. For Rietveld refinement, we incorporated constraints into the calculations of the XRD profiles, as detailed in the ESI. The outcomes of the Rietveld refinement are provided in Table S3 (ESI†). The refined lattice parameters were found to be a = 5.550(1) Å, b = 5.559(1) Å, c = 7.844(1) Å, and β = 90.046(1)°. The reduction in lattice dimensions and the increase in the β angle, as compared to the Le Bail refined data for the stoichiometric phase L2NTR, indicated that the introduction of A-site vacancies contributed to the contraction of the lattice volume. The ordering of B-site cations was quantified as S = 0.616 using eqn (S1) (ESI†), which suggested partial disordering of the B-site cations. Additionally, according to Table S3 (ESI†), the refined La cation occupancy exhibited a slightly higher value than the intended amount, implying a deficiency of 5.6 at%. ICP-OES results (Table S2, ESI†) showed a lower amount of A-site deficiency which might be attributed to unresolved phases depicted in Fig. S2 (ESI†) and the occurrence of local B-site enrichment.
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Fig. 1 XRD patterns of the as-prepared L1.85NTR pristine, and L1.85NTR samples reduced at 450 °C and 800 °C in wet 5% H2/Ar (a) and zoomed in detailed region from 43° to 51° 2θ postion (b); (c) XRD pattern and Rietveld refinement plots of as-prepared L1.85NTR parent phase. The factors of agreement are Rp = 4.95, Rwp = 6.41, Rexp = 4.11 and χ2 = 2.43; (d) XRD pattern and Rietveld refinement profiles of L1.85NR reduced at 800 °C. The factors of agreement are Rp = 5.59, Rwp = 7.08, Rexp = 4.12 and χ2 = 2.95. Lattice parameters of nickel metal phase were refined based on reference structure ICSD64989.79 Lattice parameters of lanthanum oxide phase were refined based on reference structure ICSD28555;80 SEM images of (e) as prepared and (f) reduced L1.85NTR sample at 800 °C for 3 hours. The inset image is the enlarged display of the reduced sample. |
Subsequently, the L1.85NTR sample underwent a reduction treatment in a wet 5% H2/Ar atmosphere. Various reduction temperatures were employed to assess the materials' stability under reducing conditions. The corresponding XRD patterns are presented in Fig. 1a and b, with additional details in Fig. S3 (ESI†). It can be inferred that the titanium-based sample maintained its double perovskite structure up to 1000 °C. However, a subtle peak at the 30° 2θ position indicated the presence of a small amount of La2O3 in the sample reduced at temperatures exceeding 800 °C (Fig. S3, ESI†). This observation is commonly linked to side reactions and exsolution, suggesting a slight decomposition of the double perovskite structure.81,82 Moreover, a peak at the 44.5° 2θ position was detected in the reduced samples, closely aligned with the Ni metal phase,79 signifying the occurrence of exsolution during the reduction process.
Rietveld refinement was applied to the XRD pattern of the L1.85NTR sample reduced at 800 °C (Fig. 1d). As illustrated in Fig. S4 (ESI†), subtle peaks attributed to a slight amount of La2O3 phase were observed at 29.96° and 29.05°. Therefore, both Ni and La2O3 phases were incorporated in the refinement, despite the less prominent peak intensity of La2O3 compared to the XRD patterns of L1.85NTR samples reduced at 900 °C and 1000 °C. The refined lattice and atomic parameters of the double perovskite phase reduced at 800 °C are outlined in Table S3 (ESI†). The lattice parameters of the double perovskite phase remained consistent with those of the as-prepared sample, while the atomic occupancies suggested a slightly greater B-site disordering and La-occupancy. This indicates a propensity to restore A-site stoichiometry through the exsolution process, as observed in previous studies.6,8 The refined lattice parameters of the Ni metal phase, 3.52395(7) Å, agreed with the reported reference ICSD 64989,79 confirming the exsolution of Ni. The refinement results revealed that the reduced sample contained 1.58(5) wt% Ni metal and 0.28(2) wt% lanthanum oxides. This finding implies that, under a reducing atmosphere, most of the A-site deficient sample experiences exsolution rather than decomposition into metal oxides.
Through the study of the sample's surface morphology after reduction at 800 °C in a wet 5% H2/Ar environment for 3 hours by SEM, nano-sized particles were observed evenly distributed on the surface of the oxide bulk, compared to the pristine sample (Fig. 1e and f). This suggested the occurrence of exsolution in the L1.85NTR sample during reduction.
To gain insight into the exsolution process at varying reduction temperatures, SEM images of the L1.85NTR sample reduced at 800 °C and 450 °C (as depicted in Fig. S5 and S6, ESI†) were analysed using ImageJ software.83 Specifically, the inset images in Fig. 2c and d display one of the selected areas for particle size analysis, deliberately excluding large grain fragments. The outcomes of particle size distribution analysis are presented in Fig. 2e and f. As anticipated, the sample reduced at the higher temperature (800 °C) exhibited larger particle sizes. In total, 208 particles from four areas (4.9 × 104 nm2) of the sample reduced at 800 °C were analysed, with particle density of 420 μm−2. The average size of the exsolved nanoparticles in the L1.85NTR sample reduced at 800 °C was approximately 15.8 nm, corroborating findings from TEM and STEM imaging. The majority of the sizes of exsolved nanoparticles following reduction in a wet 5% H2/Ar environment for 3 hours fell within the range of 10 to 20 nm. In contrast, the sample reduced at 450 °C exhibited smaller exsolved nanoparticles with higher particle density (1300 μm−2) in comparison to the samples reduced at 800 °C. A total of 125 particles from four areas covering an area of 9.6 × 103 nm2 were analysed, yielding an average size of approximately 8.7 nm. The size distribution in Fig. 2f reveals that 67 out of the 125 particles measured between 5 to 10 nm, displaying a relatively narrower distribution than observed in the L1.85NTR sample reduced at 800 °C. This observation suggests a more uniform morphology for the exsolved nanoparticles at the lower temperature. The increasing particle size and broadened size distribution from 450 °C to 800 °C implies particle-growth dominated exsolution in this temperature range.
To further investigate the phenomenon of Ru-exsolution, STEM-EDX examination was conducted on the L1.85NTR sample that underwent reduction above 800 °C in a wet 5% H2/Ar environment. Fig. 3 displays the STEM-EDX analysis performed on two distinct particles situated on the surface of the L1.85NTR sample, which was reduced at 1000 °C for 3 hours in the same wet 5% H2/Ar atmosphere. Fig. 3a prominently shows the occurrence of Ru exsolution, manifesting as particles with sizes ranging from approximately 2.5 to 3 nm. Notably, there was an absence of Ni enrichment within these exsolved nanoparticles. In contrast, Fig. 3b offers a depiction of Ni particle exsolution, with these particles measuring around 35 nm in size. These observations highlight the distinctive characteristics of ruthenium exsolution within lanthanum nickel titanates from nickel exsolution. Specifically, the exsolution process of Ru cations demands higher reduction temperatures. This behaviour can be attributed to the gradual migration of transition metal cations, particularly Ru cations, within the perovskite structure.84 This sluggish diffusion contrasts to the behaviour observed in ruthenates,73 where Ru cations were more widely distributed within the material. This indicates the need for elevated temperatures, such as 1000 °C in a wet 5% H2/Ar environment, to promote the diffusion/exsolution of Ru cations from the interior of the parent L1.85NTR perovskite structure to its surface.
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Fig. 3 STEM images and EDX maps of two distinct regions (a) and (b) of the L1.85NTR sample reduced at 1000 °C in a wet 5% H2/Ar for 3 hours. Scale bar: (a) 5 nm; (b) 10 nm. |
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Fig. 4 (a) TG curves and corresponding temperature profiles as a function of time, encompassing both the heating and dwelling phases; (b) TG and DTG curves as a function of increasing temperature, ranging from room temperature (RT) to 1000 °C. (c) STEM-ABF, STEM-ADF, STEM-MAADF, STEM-HAADF images and maps of the quenched L1.85NTR after reduction at 350 °C. Same area with the in situ observation in Fig. S8.† STEM-ABF, STEM-ADF, STEM-MAADF, STEM-HAADF images and EDX maps of different areas in the quenched L1.85NTR after reduction at 500 °C (d) and 800° (e). |
Prior to reaching 1000 °C, two distinct phases of mass loss became evident as illustrated in Fig. 4a and b. The mass loss attributed to surface-adsorbed moisture was negligible, as indicated by the absence of noticeable weight change within the temperature range of room temperature to 250 °C.85–87 The DTG curve indicated that the first peak of maximum mass loss occurred around 427 °C, followed by a broader mass loss phase centred at approximately 665 °C. The exsolution of Ni nanoparticles was confirmed through the characterization of the L1.85NTR sample reduced at 450 °C and 800 °C. Both mass loss steps were linked to the exsolution process, resulting from the loss of oxygen anions in the perovskite structure.88,89 As the temperature increased, the first plateau emerged at around 500 °C, accompanied by a 0.36 wt% mass loss. Subsequently, when the temperature surpassed 600 °C, a continuous mass loss was observed, akin to the reported exsolution behaviour of La(Sr)Cr0.85Ni0.15O3−δ (ref. 90) and La0.6Sr0.4FeO3−d.86 The loss of oxygen was deduced from the TG curve, as depicted in eqn (S2) (ESI),† revealing an oxygen loss of approximately 0.25 mol per mol of L1.85NTR for the sample reduced at 800 °C. Consequently, in conjunction with the outcomes of Rietveld refinement (Fig. 1d) and Table S4 (ESI†), the reduction process at 800 °C can be summarized as follows:
However, precisely determining the oxygen stoichiometry of the resulting La1.910NiTi0.9Ru0.1O6−y double perovskite remains challenging due to the uncertainty surrounding the exsolution behaviour of Ni cations or Ni–O species.
Ex situ microscopy characterization disclosed that exsolution occurred not only at high temperatures but also at relatively lower temperatures. Thermogravimetric analysis indicated two stages of mass loss, signifying two distinct exsolution stages. Thus, in situ STEM was employed to examine the evolution of the sample's morphology. The Protochips Fusion Select E-chips and rod were utilized to attain the elevated temperatures necessary for the exsolution process. In contrast to the experimental conditions, high vacuum (∼10−7 torr, equivalent to ∼1.33 × 10−5 Pascal) was employed as the reducing environment in the TEM equipment. To thoroughly investigate the evolution of L1.85NTR during the exsolution process, a heating procedure was employed, involving gradual temperature increments to minimize vibrations caused by rapid heating of the sample and rod. The thermal cycle applied to the sample is outlined in Fig. S8 (ESI†). Additionally, to analyse the chemical composition of the exsolved nanoparticles during thermal treatment, STEM-EDX analysis was conducted after swiftly quenching the sample to room temperature. Both heating and quenching rates were set at 5 °C s−1.
In alignment with the ex situ characterization, the STEM-EDX analysis of the sample, quenched between heating stages, unveiled the presence of exsolved Ni nanoparticles, along with a progressive enlargement in particle size (as illustrated in Fig. 4c–e). As depicted in Fig. 4c, the dot contrasts situated at the edge of the bulk grain exhibited measurements of approximately 3–3.5 nm. Fig. 4d presented STEM images and EDX maps of exsolved nanoparticles quenched from 500 °C, showcasing particles ranging in size from 3.1 nm to 5.5 nm. Upon reaching 800 °C, fully developed spherical nanoparticles with socket structures became evident. The spherical particle depicted in Fig. 4e had an approximate diameter of 9 nm. Notably, since the in situ growth of these nanoparticles took place under vacuum conditions rather than in a hydrogen atmosphere, the measured diameters of the Ni particles appeared to be slightly smaller than those depicted in Fig. 2c–f.
An intriguing observation of morphology reconstruction was observed during the in situ reduction of L1.85NTR (depicted in Fig. S9, ESI†), showing STEM-ADF images of the initial sample and the sample at various temperatures: 350 °C, 450 °C, and 800 °C. At a reduction temperature of 350 °C, three distinct bright dots, marked by arrows, are discernible on the surface of the sample grain, diverging from the initial pristine sample. These particles in this region are exactly those shown in Fig. 4c, corroborating their Ni metal composition in line with the ex situ observations. As illustrated in Fig. S9b,† when the temperature reaches 450 °C, nanoparticles indicated by the green arrows reincorporate or dissolve into the bulk, vanishing from microscopic observation. This phenomenon indicates a reconstruction of both the sample's surface morphology and the exsolved nanoparticles, concomitant with mass movement within the bulk oxide materials. The nanoparticles nucleation and growth on the surface of ceramic oxides involves the interplay of segregation energy, surface energy and lattice mismatching on each facet.9,64–66,91 This reconstruction likely arises from exsolution as a dynamic process, continuously modifying the surface morphology until the exsolved nanoclusters/nanoparticles achieve both an energetically favourable state and a critical size for further growth. In a related study, Cao et al.64 computed the theoretical critical size of Ni nanocrystals to be approximately 1.5 nm. In our specific case, STEM-EDX analysis (Fig. 4c) demonstrated nanoparticle sizes of 3–3.5 nm, equivalent to 12–15 atomic diameters.
Another facet observed under in situ conditions, providing additional evidence for the nucleation and growth of particles, is illustrated in Fig. 5. Two types of nanoparticles were evident on the surface of the bulk grain reduced at 950 °C. One type comprised small nanoparticles, akin to those seen in Fig. 4c–e and S9 (ESI†), with sizes of around 3 nm, equivalent to 12 atomic diameters. The other type, highlighted by the green circle in Fig. 5, exhibited larger particle sizes of about 17 nm. The larger particles were indicative of particle growth, while the smaller particles might remain in a metastable state, potentially rejoining the bulk or merging with neighbouring larger particles through Ostwald ripening as the reduction temperature/time are extended.64,92 The nucleation and reconstruction of exsolved Ni nanoparticles offer insights into the two-step exsolution process depicted in Fig. 4a and b, reflecting the TG behaviour of L1.85NTR during reduction.
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Fig. 5 In situ STEM-ADF image of the L1.85NTR sample measured at 950 °C in high vacuum. The green arrows highlight the exsolved nanoparticles/nuclei with smaller size. |
Fig. 6a reveals two intricate arcs spanning from high to low frequencies, as depicted in the spectra recorded at 343 °C. The gradual progression observed in the ten spectra over a span of five hours implies a subtle decline in impedance as the exsolution process unfolds. This trend seems to stabilize after 30 minutes of measurement at this temperature. Interestingly, an unexpected phenomenon was observed as the temperature increased to 437 °C: during the reduction process, the low-frequency impedance arc exhibited a slight increase (Fig. 6b). Upon further elevating the temperature beyond 500 °C, the impedance arcs demonstrated a more pronounced reduction, as evident in Fig. S10a and b (ESI†). In contrast to the observations in Fig. 6a, the spectra obtained at 528 °C and 710 °C indicated that the exsolution persisted for a longer duration. The spectra acquired at 528 °C appeared to stabilize after 4 hours of reduction, while the spectra captured at 710 °C (depicted in Fig. S10b, ESI†) continued to decrease until the reduction was extended to 5 hours. This suggested that the limited amount of Ni cations located at the B-site were exsolved at lower temperature and is highly dependent on the reduction temperature.
Two R/CPE (resistor and constant phase element) components were employed to simulate the frequency-dependent impedance responses. This was performed on the symmetric cell response after reduction at 800 °C for 4 hours (Fig. S10c, ESI†). The details of this analysis can be found in Table S6 (ESI†). Specifically, the low-frequency arc was associated with the electrode–electrolyte interface, implying an enhancement in conductivity at this interface, likely stemming from the advancement of Ni cation exsolution. In light of the earlier in situ observations conducted using TEM and TGA, an unusual behaviour of the L1.85NTR electrode was identified within a relatively low temperature range, approximately 400–450 °C. This phenomenon could potentially account for the observed rise in impedance at 437 °C. The reconstruction of nanoparticles, accompanied by the incorporation of Ni into the structure, alongside the loss of smaller nanoparticles, might impede the desorption of hydrogen and consequently lead to increased polarization resistance within this temperature range.
Full cell testing was conducted to evaluate the electrochemical performance of the L1.85NTR as a fuel electrode in SOCs and to assess the impact of Ni nanoparticle exsolution. Fig. 6c displays the I–V curve of the single cell L1.85NTR/Hionic™ Electrolyte/LSM-GDC measured at 850 °C. Consistent with the in situ EIS measurements, decrease of the impedance of a single cell confirmed the progression of Ni nanoparticle exsolution (Fig. S12, ESI†). After a 30 minute reduction, the impedance of the single cell decreased from approximately 37.3 Ω cm2 to 11.3 Ω cm2, indicating a reduction in the polarization resistance due to the exsolution of Ni nanoparticles. Compared to the impedance spectrum of symmetric cells measured at 800 °C (Fig. S10c, ESI,† the real axis intercept of the single cell spectra is smaller. This is primarily attributed to the lower resistance of the thin Hionic™ electrolyte at 850 °C. However, the single cell after reduction in wet hydrogen for 30 minutes exhibited higher polarization resistance compared to the spectrum of the symmetric cell (Fig. S10c, ESI†). This higher polarization resistance is likely due to complex reactions involving higher activation resistance of the cathode-side oxygen reduction reaction, interfacial resistance at the LSM-GDC/electrolyte interface, contributions from the LSM-GDC cathode resistance, and gas diffusion polarization. Following a 3 hour reduction of the L1.85NTR fuel electrode, the current density increased from 27 mA cm−2 at an applied voltage of 1.5 V to 59 mA cm−2, indicating an enhancement in the performance of the cell in SOEC mode. For SOFC mode, the peak power densities doubled after 3 hours of reduction and exsolution of the Ni nanoparticles (from 10 mW cm−2 to 25 mW cm−2). Whilst this is a low overall cell performance these data underscore the significant potential of metal nanoparticles in the electrode for improving the performance of both SOFCs and SOECs.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d4na00349g |
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