Yinlong Zhua,
Ye Linb,
Xuan Shencd,
Jaka Sunarsoe,
Wei Zhou*f,
Shanshan Jianga,
Dong Suc,
Fanglin Chenb and
Zongping Shao*g
aState Key Laboratory of Materials-Oriented Chemical Engineering, College of Chemistry & Chemical Engineering, Nanjing Tech University, No. 5 Xin Mofan Road, Nanjing 210009, P.R. China
bDepartment of Mechanical Engineering, University of South Carolina, Columbia, South Carolina 29208, USA
cCenter for Functional Nanomaterials, Brookhaven National Laboratory, Upton, NY 11973, USA
dNational Laboratory of Solid State Microstructures, Department of Materials Science and Engineering, Nanjing University, Nanjing 210093, P.R. China
eDepartment of Chemistry, University of Waterloo, 200 University Avenue West, Waterloo, Ontario N2L 3G1, Canada
fSchool of Chemical Engineering, The University of Queensland, Brisbane, Queensland 4072, Australia. E-mail: wei.zhou@uq.edu.au
gState Key Laboratory of Materials-Oriented Chemical Engineering, College of Energy, Nanjing Tech University, No. 5 Xin Mofan Road, Nanjing 210009, P.R. China. E-mail: shaozp@njtech.edu.cn; Fax: +86-25-83172256
First published on 21st August 2014
The creation of A-site cation defects within a perovskite oxide can substantially alter the structure and properties of its stoichiometric analogue. In this work, we demonstrate that by vacating 2 and 5% of A-site cations from SrNb0.1Co0.9O3−δ (SNC1.00) perovskites (Sr1−sNb0.1Co0.9O3−δ, s = 0.02 and 0.05; denoted as SNC0.98 and SNC0.95, respectively), a Jahn–Teller (JT) distortion with varying extents takes place, leading to the formation of a modified crystal lattice within a the perovskite framework. Electrical conductivity, electrochemical performance, chemical compatibility and microstructure of Sr1−sNb0.1Co0.9O3−δ as cathodes for solid oxide fuel cells were evaluated. Among SNC1.00, SNC0.98 and SNC0.95, SNC0.95 (P4/mmm symmetry (#123)) which exhibits a large JT distortion in conjunction with charge-ordering of cobalt (Co) shows the best oxygen reduction reaction (ORR) activity at low temperature while SNC0.98 (P4mm symmetry (#99)), which displays a local JT distortion, shows the poorest performance.
ABO3 perovskite-type mixed oxide-ionic and electronic conductors (MIECs) are among excellent cathode candidates for low-temperature SOFCs.1–8 Up to a reasonable limit, these perovskite oxides can fine-tune their structure (so that their original framework is maintained) to accommodate a mismatch of the equilibrium bond lengths between (and within) the A and B sites, cation and/or anion vacancies, as well as the formation of A- or B-site cation ordering structures.9 In this context, one strategy has been devised to enhance their oxygen reduction kinetics, e.g. by introducing A-site defects. Several A-site deficient perovskites, namely La0.6Sr0.4−sCo0.2Fe0.8O3−δ,10 (Pr0.6Sr0.4)1−sCo0.2Fe0.8O3−δ,11 La1−sFe0.4Ni0.6O3−δ,12,13 (Ba0.5Sr0.5)1−xCo0.8Fe0.2O3−δ,14 Ba1−xCo0.9−yFeyNb0.1O3−δ,15,16 and PrBa1−sCo2O5+δ (ref. 17) have been investigated as cathode materials for SOFCs. The physical and chemical properties of A-site deficient perovskites are often substantially different from those of the stoichiometric ones. The introduction of A-site defects tends to create additional oxygen vacancies which facilitate oxygen ionic transport and enhance the ORR activity.18 However, these oxygen vacancies may also interfere with the electron transport, reducing the electronic conductivity of the materials.19 We found a novel A-site deficient perovskite, Sr0.95Nb0.1Co0.9O3−δ (SNC0.95) which exhibits substantially improved ORR activity at low temperatures relative to its stoichiometric analogue, SrNb0.1Co0.9O3−δ (SNC1.00). SNC0.95 features simultaneous enhancement in oxygen vacancy concentration and electrical conductivity,20 the responsible mechanism of which has not yet been clarified. Here, we show that the Sr1−sNb0.1Co0.9O3−δ perovskites (s = 0.02 and 0.05; denoted as SNC0.98 and SNC0.95, respectively) exhibit different crystal structures due to the varying extent of Jahn–Teller (JT) distortions. The effects of crystal structure on the electrical conductivity, electrochemical performance, chemical compatibility and microstructure of the resultant cathode materials are examined. SNC0.95 (P4/mmm crystal structure) shows improved ORR activity at low temperature whereas SNC0.98 (P4mm structure) shows diminished performance. Sr1−sNb0.1Co0.9O3−δ perovskites represents a deviation from the general notion of increased concentration of oxygen vacancies leading to enhanced ORR activity.20–22 Instead, the crystal structure seems to play a more determining role towards its electrochemical performance.
The chemical compatibility between the cathode and the SDC electrolyte materials was examined. Sr1−sNb0.1Co0.9O3−δ–SDC powders mixtures (1:
1 weight ratio) were calcined at 1000 °C for 2 h in air atmosphere. The phase composition of the mixture after calcinations was analysed by powder X-ray diffraction (XRD, D8 Advance, Bruker, Germany) at room temperature.
The oxygen non-stoichiometry and the valence states of cobalt at room temperature were determined by iodometric titration. In brief, approximately 0.1 g of powder was dissolved in a 6 mol L−1 HCl solution in a nitrogen atmosphere to prevent the oxidation of I− ions (from KI) by air, followed by titration with a standard thiosulfate (S2O32−) solution. The oxygen non-stoichiometry and the valence states of cobalt at high temperatures were measured by thermogravimetric analysis (TGA, Model STA 449 F3, NETZSCH) in a synthetic air atmosphere from room temperature to 1000 °C. The heating and cooling rates were 10 °C min−1.
The cathode powders were packed into rectangular bars with dimensions of 2 mm × 5 mm × 20 mm and sintered at 1200 °C for 5 h in air for electrical conductivity testing. All bars used for measurements had densities of >93% of their theoretical values. Electrical conductivity was measured using a four-probe DC technique with silver coating layer as electrodes. The current and voltage were measured using a Keithley 2420 source meter; the data was collected at a 25 °C interval between 450 and 800 °C in an air atmosphere.
Raman spectra were recorded in a backscattering mode at room temperature using a LABRAM inVia micro-Raman system equipped with an optical microscope containing a 50× objective lens. The radiation source was a He–Ne laser (λ = 514 nm) operated at 1% power, which was focused on a 5 μm spot at 40 mW. Before measurement, the micro-Raman system was calibrated using the 520 cm−1 peak of polycrystalline Si.
Transmission electron microscopy (TEM) was conducted at 220 kV with a Philips T30F field emission instrument equipped with a 2k-CCD camera and JEOL 2100F TEM equipped with a Schottky field-emission gun (FEG), with Cs = 1.0 mm operated at 200 kV. Double tilting was applied to find the right zone axis as required. The morphologies of the cathode and cathode/electrolyte interface were obtained using an environmental scanning electron microscope (ESEM, QUANTA-2000). The selected area electron diffraction (SAED) simulation patterns based on the XRD refinements results were obtained using the CrystalMaker (2.5.1) and SingleCrystal (2.0.1) software.24
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Fig. 1 (a) X-ray diffraction patterns of SNC1.00, SNC0.98 and SNC0.95 powders calcined at 1200 °C; (b) magnified XRD patterns around 2θ = 47°, 58.5° and 68.5°. |
To avoid complications from the second phase, we limit our scope to SNC1.00, SNC0.98, and SNC0.95. SNC0.95 has a tetragonal structure, the symmetry of which can be described by the P4/mmm space group (#123). This is implied by the line splitting of peaks at approximately 47°, 58.5° and 68.5°, which was not observed in SNC1.00 and SNC0.98 (Fig. 1b). Raman spectroscopy was used to probe the symmetry of the crystal structure of SNC1.00, SNC0.98, and SNC0.95 (Fig. 2). No vibrational modes were observed for SNC1.00, indicating high symmetry, i.e., a Pmm cubic symmetry.25 Six modes were identified for SNC0.95, in agreement with the symmetry of the P4/mmm space group.26 We further confirmed the cubic and tetragonal lattice for SNC1.00 and SNC0.95, respectively, by high resolution (HR) TEM and selected area electron diffraction (SAED) (Fig. 3). The HRTEM image and the corresponding SAED pattern of SNC1.00 are indeed characteristic of the primitive cubic perovskite symmetry best described by Pm
m space group (#221) with a = ap = 3.9 Å. For SNC0.95, the reconstruction of the reciprocal space from the SAED pattern revealed a tetragonal cell with a ≈ ap and c ≈ 2ap, compatible with the P4/mmm space group. The doubled cell parameter value with respect to the primitive perovskite cell is clearly indicated on the HRTEM image and the corresponding SAED pattern.
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Fig. 3 HRTEM images of (a) SNC1.00 and (c) SNC0.95; SAED images of (b) SNC1.00 and (d) SNC0.95.20 |
The structure of SNC0.98 cannot be directly identified by XRD. SNC1.00 and SNC0.98 powders showed similar XRD patterns but distinct Raman vibrational modes (Fig. 2). The broad band at ∼590 cm−1 in the spectrum of SNC0.98 was indicative of degradation of ideal cubic symmetry; most likely attributed to a local JT distortion.27 The JT distortion may lead to a tetragonal distortion in the CoO6 octahedra.27 Slight decrease in the symmetry of the diffraction peaks (Fig. 1b) implies the likelihood of a P4mm symmetry, as is the case of BaTiO3 perovskite.28 We refined the structure of SNC0.98 using model based on centrosymmetric Pmm, noncentrosymmetric P4mm and centrosymmetric P4/mmm space group. P4mm space group (#99) model gave the lowest residuals among the three models (Table S1†). Low electrical conductivity SNC0.98 seems to somewhat correlate with the noncentrosymmetric structure as suggested by the following conductivity results. The phase stability was then probed using high-temperature (HT)-XRD (Fig. 4). The splitting of the peaks at 47°, 58.5° and 68° is retained up to 800 °C; ruling out the possible phase transformation during SOFC operation.
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Fig. 4 (a) HT-XRD patterns of the SNC0.98 powder between room temperature to 800 °C. (b) Magnified XRD patterns around 2θ = 47°, 58.5° and 68.5°. |
HRTEM was used to examine the crystal structure of SNC0.98. Fig. 5 indicates identical lattice structure between SNC0.98 and SNC1.00. It is not possible to confidently distinguish P4mm from Pmm symmetry using HRTEM and SAED results, considering the relatively weak tetragonal distortion as reflected by the ratio of c/a of only 1.003 (for P4mm symmetry).29 This is particularly apparent upon comparing the Fast Fourier Transform (FFT) images with the simulated electron diffraction spots (Fig. 5d–f to g–i).
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Fig. 5 HRTEM images (a–c); Fast Fourier Transform (FFT) images (d–f) of [100], [110], [111] zone axes for SNC0.98 and the simulated diffraction patterns of (g) [100], (h) [110], (i) [111] zone axes for SNC0.98 in P4mm space group with lattice parameters listed in Table S2.† |
Lattice parameters of SNC1.00, SNC0.98 and SNC0.95 were obtained by Rietveld refinement (Fig. S2 and Table S2†). Introduction of A-site defects in Sr1−sNb0.1Co0.9O3−δ perovskites led to lattice expansion for both SNC0.98 and SNC0.95. The (Co,Nb)–O bond lengths and O–(Co,Nb)–O angles in SNC1.00, SNC0.98 and SNC0.95 are listed in Table 1. The crystal structure transitions from Pmm to P4mm and P4/mmm are depicted schematically in Fig. 6. The P4mm structure exemplified a tetragonal distortion of the cubic perovskite, resulting in a difference of (Co,Nb)–O1 and (Co,Nb)–O1* bond lengths. As a result, (Co,Nb)–O1* bond can be visualised to be excluded from an originally symmetric (Co,Nb)O6 octahedron (imagine taking out O1* from one of the opposing apex) so that the repeating unit becomes a distorted (Co,Nb)O5 square pyramid which shares corner with other units (in the same layer). For 0.05 A-site deficiency case, although each (Co,Nb)–O1* and (Co,Nb)–O1 bond shows similar bond length value (1.8810 Å and 2.0075 Å, respectively), they are distributed periodically in two different (Co,Nb)O6 octahedron, forming an overall framework described by P4/mmm symmetry. Perhaps, the doubling of the lattice in SNC0.95 originates from long-range ordering of oxygen vacancies along the c axis, which brings about the charge-ordering between Co4+ and Co3+ cations. Charge ordering is a phase transition observed mostly in strongly correlated materials such as transition metal oxides.30–32 Strong interaction between electrons in these materials lead to localised charges on different sites and thus, a disproportionation and an ordered superlattice.33 Here, two types of (Co,Nb)O6 octahedron exist within the P4/mmm framework; the elongated one e.g. (Co,Nb)1O6 octahedron containing two stacked (Co,Nb)1–O2 bonds of 2.0075 Å length each (as the 4-fold axis) while the shortened one e.g. (Co,Nb)2O6 octahedron containing two stacked (Co,Nb)2–O2 bonds of 1.8810 Å length each (also as 4-fold axis). In both cases, the square centre of the octahedron is symmetrical as reflected by 4 equivalent bond length of (Co,Nb)1–O1 and (Co,Nb)2–O3 (e.g. 1.9348 Å). Since the average valence for Co is 3.2+ (Table 2), the charge-ordering hypothesis signifies an average oxidation state of Co3+ at (Co,Nb)1O6 sites and Co3.4+ at (Co,Nb)2O6 sites, assuming a full charge disproportionation. A similar structure was also noticed earlier in a SrSb0.1Co0.9O3−δ perovskite.34
SNC1.00 | |||
(Co,Nb)–O × 6 | 1.936(3) | O–(Co,Nb)–O | 180° |
SNC0.98 | |||
(Co,Nb)–O1 | 1.837(0) | O1–(Co,Nb)–O1* | 180° |
(Co,Nb)–O1* | 2.055(2) | ||
(Co,Nb)O2 × 4 | 1.986(9) | O2–(Co,Nb)–O2 | 154.92° |
SNC0.95 | |||
(Co,Nb)1–O2 × 2 | 2.007(5) | O2–(Co,Nb)1–O2 | 180° |
(Co,Nb)2–O2 × 2 | 1.881(0) | O2–(Co,Nb)2–O2 | 180° |
(Co,Nb)1–O1 × 4 | 1.934(8) | O1–(Co,Nb)1–O1 | 180° |
(Co,Nb)2–O3 × 4 | 1.934(8) | O3–(Co,Nb)2–O3 | 180° |
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Fig. 6 Schematic of the structure transition from Pm![]() |
Sample | δ | Valence states of cobalt |
---|---|---|
SNC1.00 | 0.24 | 3.3 |
SNC0.98 | 0.38 | 3.0 |
SNC0.95 | 0.35 | 3.2 |
We speculate that the JT distortion offsets the increased energy of the perovskite system induced by a 2% A-site deficiency. Nonetheless, increasing the deficiency to 5% cannot be compensated by slight (local) JT distortion. SNC0.95 shows substantial JT distortion reflected by (Co,Nb)1O6 with elongated axial bond and (Co,Nb)2O6 with shortened axial bond. Both distortions will lower the energy for a system with one eg electron (for (Co,Nb)1O6 the z2 orbital is lowered and x2–y2 orbital for (Co,Nb)2O6 just the opposite direction, and in both cases the lowest eg orbital is singly occupied). Therefore, besides the JT distortion, the elastic energy would be further minimised by such an ordering with shorter and longer bond lengths.22,35,36
Within the perovskite, each O2− is surrounded by 4 A-site cations and 2 B-site cations. The formation of one A-site vacancy necessitates a change in the local coordination number (CN) from 6 to 5 for O2−. Given that no O2− ions with CN = 5 is possible,37 the distortions of the oxygen sublattice somehow need to be compensated by modifying the perovskite structure. La1/3NbO3, for example can accommodate a large A-site deficiency since Nb–O has a high degree of covalence to stabilise the Nb–O network.38 However, for transition metal cations which can easily change their oxidation states (such as Co), a stable CoO6 octahedron is difficult to obtain (upon subjected to A-site deficient). Konysheva et al. provides simple prediction criteria to estimate the extent of the A-site deficiency in perovskites based on the average 〈B–O〉 bond energy and metal (A,B)–oxygen bond energy (〈ABE〉) within the perovskite lattice.38 In our case, Co is partially replaced with 10% Nb to enhance the stability of the B-site octahedral network. The 〈B–O〉 bond energy for A(Nb5+0.1Co3+0.9)O3−δ perovskites is −207 kJ mol−1, suggesting the maximum defect concentration of 0.06 (ESI, Fig. S3†). Nonetheless, when the 〈ABE〉 value is applied as the prediction descriptor (the properties of the particular A-site cations are involved in this prediction), the A-site deficiency is unattainable in Sr1−sNb0.1Co0.9O3−δ; given the more positive value of 〈ABE〉 in SNC0.95 (−287 kJ mol−1, ESI, Fig. S4†). The obtainment of 5% A-site deficient (SNC0.95) perovskite phase here highlights the fact that the stability of B-site octahedron provides a more dominant role.
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SNC0.98 has the largest oxygen vacancy concentration in the temperature range studied. Fig. 8 displays the electrical conductivities of SNC1.00, SNC0.98 and SNC0.95 between 450–800 °C. Whilst reduced electrical conductivity of SNC0.98 (relative to SNC1.00) is consistent with its higher concentration of oxygen vacancies, SNC0.95 deviates from this trend. Despite its larger concentration of oxygen vacancies, in fact, the electrical conductivity of SNC0.95 exhibits values between 276–117 S cm−1,20 higher than those of 265–83 S cm−1 for SNC1.00. This synergistic effect is perhaps related to its intrinsic structure with P4/mmm symmetry. It is very likely that the charge ordering of Co favours rapid electron transport in SNC0.95.
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Fig. 8 Electrical conductivities of SNC1.00, SNC0.98 and SNC0.95 (ref. 20) between 450–800 °C. |
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Fig. 9 XRD patterns of SNC1.00-SDC, SNC0.98-SDC and SNC0.95–SDC20 mixed powders (1![]() ![]() |
The microstructures of the Sr1−sNb0.1Co0.9O3−δ cathodes are shown in Fig. 10. Firm attachment between the cathode and electrolyte suggests good thermal compatibility between Sr1−sNb0.1Co0.9O3−δ perovskites and SDC. The grain sizes and pore structures look very similar for the three cathodes, which dismisses microstructural effects on the electrochemical performance.
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Fig. 11 Electrochemical impedance spectra of SNC1.00, SNC0.98 and SNC0.95 cathodes between 550–650 °C. |
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Fig. 12 Temperature dependent ASRs of Sr1−sNb0.1Co0.9O3−δ cathodes tested between 500 and 750 °C. Error bars represent standard deviations of three independent measurements. |
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c4ra06191h |
This journal is © The Royal Society of Chemistry 2014 |