Luca Angelo
Betti
a,
Lisa Rita
Magnaghi
*a,
Aldo
Bosetti
b,
Raffaella
Biesuz
a and
Lorenzo
Malavasi
*a
aDepartment of Chemistry, University of Pavia and INSTM, Viale Taramelli 16, Pavia, Italy. E-mail: lisarita.magnaghi@unipv.it; lorenzo.malavasi@unipv.it
bEni, Renewable, New Energies and Material Science Research Center, Via Fauser 4 28100, Novara, Italy
First published on 1st May 2024
Nowadays, the existence of high entropy perovskite (HEP) oxides is well established and, since their discovery, they have found application in several technological fields. The main advantage provided by these materials, with the general formula ABO3, is the possibility of widely tuning their properties by acting on the chemical composition. The study of stability, fields of existence, and solubility limits in a systematic way remains lacking in comparison with continuous application research, despite the presence of large datasets and computational studies. In the present work, we aimed at investigating the structure and solubility limits of two series of HEPs including five different cations on the perovskite B-site, namely La(CrMnFeCoNi)O3 and La(CrMnFeCoZn)O3, exploring a full range of compositions beyond the classical equimolar phases usually investigated. This has been accomplished by the design of experiment strategy to investigate the influence of the B-site composition on phase stability, crystal structure, and oxygen non-stoichiometry for the two systems providing a solid tool for researchers to predict such properties on the whole compositional space of the two HEPs.
Among the relatively vast examples of high entropy oxides (HEOs) explored to date, a clear understanding has emerged, i.e. the configurational entropy plays a dominant role in determining the Gibbs free energy of formation.7,10,11 This entropy effectively compensates for any positive enthalpic contributions, showcasing the pivotal influence of configurational entropy in stabilizing these high-entropy materials.12,13 The configurational entropy of a system experiences a notable increase as the number of different elements distributed over the cation lattice site rises, reaching its maximum when all constituent elements are present in equimolar amounts.14 Beyond the intriguing structural implications, this distinct design concept not only highlights the significance of configurational entropy but also presents an opportunity for fine-tuning of materials functional properties.5,15,16 The equimolar distribution of diverse elements creates a unique environment wherein the interplay of configurational entropy and elemental composition contributes to the overall stability and properties of the high-entropy materials. This nuanced understanding not only expands our comprehension of the thermodynamic aspects but also opens avenues for tailoring functional characteristics in a controlled manner, providing a promising platform for the development of materials with finely tuned and optimized properties.17–22 Most of these studies are based on a computational or machine learning approach where potential chemistries are interpolated and compared in order to predict the structure and performance of a huge number of materials. However, only equimolar quantities with a high number of cations are mostly considered in these approaches leaving the experimental part deficient, often without real feedback, and failing in emphasizing the influence and synergy between cations.23–25
To address some of these issues, in the current investigation we focused on the rational characterisation of ABO3 perovskites in which B sites are occupied by a combination of Cr, Mn Fe, Co and either Ni or Zn in order to unveil the effect of the type and quantity of cations (moving beyond equimolar compositions) occupying B sites on specific perovskite properties, such as the phase composition, structural geometry, and oxygen non-stoichiometry. This has been evaluated by means of the design of experiment tool. Concurrently, relying on a suitable training set of perovskites whose compositions have been selected by D-optimal design, polynomial models are developed and validated to allow the prediction and optimisation of the properties of interest within the entire experimental domain.
As mentioned above, the materials under scrutiny encompass compositions ranging from two- to six-element mixtures. Despite the proximity of these elements in the periodic table, their inclusion introduces variability in redox capacities and oxygen vacancies within the material structures. A key distinction between the two sets lies in the behavior of Ni and Zn: Ni has the capacity to be oxidized to Ni3+, whereas Zn can only exist in the Zn2+ oxidation state. This difference leads to the generation of vacancies, compelling other elements to adapt to the presence of Zn as a dopant within the structure. Additionally, a common dataset is considered, comprising samples that exclude both nickel and zinc. Leveraging chemometric analysis, we systematically mapped all conceivable combinations of these cations. This mapping encompasses a spectrum ranging from end-members, characterized by samples with only one cation on the A site and one on the B site, to more complex members featuring five cations on the B site. Through this comprehensive compositional space mapping, we gain insights into the influence of each cation on the structural aspects and oxygen vacancies. Furthermore, we unravel the intricate synergy that emerges when these elements coexist within the material matrix. This rigorous experimental and chemometric approach not only sheds light on the structural intricacies of the studied compositions but also contributes to a deeper understanding of how different cations collaborate and influence the properties of high-entropy materials in a controlled and deliberate manner.
Depending on the type of variables, the response trend and the model equation postulated, different mathematical tools enable us to appropriately investigate any system, from the simplest cases to the most complex ones, but for further information on these techniques the readers should refer to the dedicated literature.26–30 DOE has to be considered as an adaptable stepwise approach that, starting with the problem identification, leads to response modelling and prediction.31 The workflow followed for the rational characterisation of multicomponent ABO3 perovskites is summarised in Fig. 1 and will be discussed in detail in the following sections and in the Experimental section (ESI†).
y = bCrxCr + bMnxMn + bFexFe + bCoxCo + bMxM + bCrMnxCrxMn + bCrFexCrxFe + bCrCoxCrxCo + bCrMxCrxM + bMnFexMnxFe + bMnCoxMnxCo + bMnMxMnxM + bFeCoxFexCo + bFeMxFexM + bCoMxCoxM + bCrMnFexCrxMnxFe + bCrMnCoxCrxMnxCo + bCrMnMxCrxMnxM + bCrFeCoxCrxFexCo + bCrFeMxCrxFexM + bCrCoMxCrxCoxM + bMnFeCoxMnxFexCo + bMnFeMxMnxFexM + bMnCoMxMnxCoxM + bFenCoMxFexCoxM | (1) |
It glaringly appears that samples extracted from cp to train the model depend on the terms included in the polynomial model, both in term of numerosity, i.e. the more the number of terms included, the more the amount of samples required, and location in the domain, i.e. linear terms only require mono-cation samples while 2-cations and 3-cations interactions require the corresponding combinations. Once computed the candidate point matrix and the polynomial model, D-optimal design is employed to extract the best subset of training experiments from cp; being out of the purpose of this paper to describe in detail the algorithm besides this tool, only a qualitative description of the approach will be provided.36 The algorithm iteratively identifies the best training set according to the D-optimality criterion, which means maximising the coefficients significance, their mutual independence and the information that can be extracted from the data. D-optimality is represented by a mathematical parameter that has to be normalized based on the number of experiments, since obviously a higher number of experiments always leads to higher information. The normalized parameter associated with the D-optimal set of training samples per each number of experiments is reported in Fig. S1 (ESI†) and the best compromises between extractable information and experimental effort are identified as the local maxima. In this case, 26-experimental solution, reported in Table S2 (ESI†), undoubtedly represents the preferable set of training experiments.
Just looking at the values obtained (Table S2, ESI†), we notice that Ni-containing perovskites are all single-phase, except for LaNiO3, while Zn is much less soluble and results in several non-homogeneous materials, even for low Zn molar fractions. The difference between the two metals required a different approach, as summarised in Fig. 1.
For Ni-containing perovskites, according to the Rietveld refinement results on the 26 samples of the training set (Table S2, ESI†), the experimental domain is reduced to samples with Ni content below or equal firstly to 0.9, then to 0.8. In both cases, the cp in Table S1 (ESI†) is adapted to the new domains excluding samples out of these limits (Table S1, seventh and eight columns, ESI†) and the samples to be added to the first training set (Table S2, ESI†) are selected again according to D-optimality criterion. This latter tool is generally referred to as D-optimal design by addition and is often employed to amend or expand existing matrices whenever necessary.35 The computed expanded training is reported in Table S3 (ESI†) and graphically represented in Fig. 3a in a pseudo-ternary domain in which the axes represent the molar fraction of Cr + Co, Mn + Fe and Ni. This Figure includes the results of the synthesis and structural characterization of the additional samples included in the expanded training set (results reported in Table S3, ESI†). At a glance, we can observe that single-phase samples (green) are obtained in almost the entire domain except for samples with Ni molar fraction equal to 1 and 0.9. Therefore, we can assume that single-phase perovskites are obtained for Ni content below or equal to 0.8.
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Fig. 3 (a) Training samples (Table S3, ESI†) represented is a pseudo-ternary domain in which the axes are associated to the molar fraction of Cr + Co, Mn + Fe and Ni. Single-phase samples are labelled in green while the others in red; (b) training samples (Table S4, ESI†) represented is a pseudo-ternary domain in which the axis are associated to the molar fraction of Cr + Co, Mn + Fe and Zn. Single-phase samples are labelled in green while the others in red. |
As can be appreciated by the results of the structural refinements reported in Table S2 (ESI†) for the La(Cr,Mn,Fe,Co,Zn)O3 perovskites, the Zn solubility is much lower and strongly dependent on the other cations present and therefore we cannot perform a roughly estimation, as done in the case of Ni, but solubility should be modelled by Design of Experiments. Also in this case, D-optimal design by addition is applied to better investigate the region with Zn content below 0.5, since for higher Zn content single-phase materials are almost never achieved (see Table S2, ESI†). Analysing the percentage of perovskite for the expanded training set, reported in Table S4 (ESI†) and represented in Fig. 3b, we can confirm that single-phase materials are obtained only for low content of Zn but also the other cations do influence the stability of the phase.
The ternary plot in Fig. 4 highlights the main points already hinted above: firstly, Zn solubility in the perovskite system strongly depends on the other cations included in the crystal and, secondly, Co and Fe exhibit the lower stabilisation effect while the presence of Cr and Mn allows to obtain single-phase materials for higher Zn amounts. In fact, phase pure La(Fe,Co,Zn)O3 perovskites (ternary plot in the left upper part of Fig. 4) are predicted only for Zn molar fraction below 0.4, or even 0.2 for high Co contents, while the stability domain becomes wider replacing Fe with Cr (right upper plot), or even more with Mn (left lower plot). To conclude, La(Cr,Mn,Zn)O3 perovskites is predicted to be single-phase for Zn content up to 0.5 thanks to the presence of the two most stabilising cations.
Sample | Formula | Cr | Mn | Fe | Co | Ni | Crystal System | δ |
---|---|---|---|---|---|---|---|---|
P1 | LaCrO3 | 1 | 0 | 0 | 0 | 0 | Orthorhombic | 0.003 |
P2 | La(CrMn)0.5O3 | 0.5 | 0.5 | 0 | 0 | 0 | Orthorhombic | 0.006 |
P3 | La(CrFe)0.5O3 | 0.5 | 0 | 0.5 | 0 | 0 | Orthorhombic | 0.002 |
P4a | La(CrCo)0.5O3 | 0.5 | 0 | 0 | 0.5 | 0 | Trigonal | 0.027 |
P4b | La(CrCo)0.5O3 | 0.5 | 0 | 0 | 0.5 | 0 | Trigonal | 0.027 |
P5a | LaCr0.4(FeCo)0.3O3 | 0.4 | 0 | 0.3 | 0.3 | 0 | Orthorhombic | 0.005 |
P5b | LaCr0.4(FeCo)0.3O3 | 0.4 | 0 | 0.3 | 0.3 | 0 | Orthorhombic | 0.008 |
P5c | LaCr0.4(FeCo)0.3O3 | 0.4 | 0 | 0.3 | 0.3 | 0 | Orthorhombic | 0.002 |
P6 | LaMn0.4(CrFe)0.3O3 | 0.3 | 0.4 | 0.3 | 0 | 0 | Orthorhombic | 0.011 |
P7 | LaMn0.4(CrCo)0.3O3 | 0.3 | 0.4 | 0 | 0.3 | 0 | Orthorhombic | 0.002 |
P8 | LaMnO3 | 0 | 1 | 0 | 0 | 0 | Orthorhombic | 0.006 |
P9a | La(MnFe)0.5O3 | 0 | 0.5 | 0.5 | 0 | 0 | Orthorhombic | 0.021 |
P9b | La(MnFe)0.5O3 | 0 | 0.5 | 0.5 | 0 | 0 | Orthorhombic | 0.018 |
P9c | La(MnFe)0.5O3 | 0 | 0.5 | 0.5 | 0 | 0 | Orthorhombic | 0.020 |
P10 | La(MnFe)0.5O3 | 0 | 0.5 | 0 | 0.5 | 0 | Orthorhombic | 0.003 |
P11 | LaMn0.4(FeCo)0.3O3 | 0 | 0.4 | 0.3 | 0.3 | 0 | Orthorhombic | 0.003 |
P12 | LaFeO3 | 0 | 0 | 1 | 0 | 0 | Orthorhombic | 0.003 |
P13 | La(FeCo)0.5O3 | 0 | 0 | 0.5 | 0.5 | 0 | Trigonal | 0.021 |
P14 | LaCoO3 | 0 | 0 | 0 | 1 | 0 | Trigonal | 0.003 |
P15a | LaMn0.6Co0.4O3 | 0 | 0.6 | 0 | 0.4 | 0 | Orthorhombic | 0.024 |
P15b | LaMn0.6Co0.4O3 | 0 | 0.6 | 0 | 0.4 | 0 | Orthorhombic | 0.017 |
P16 | LaMn0.1Fe0.9O3 | 0 | 0.1 | 0.9 | 0 | 0 | Orthorhombic | 0.009 |
P17 | LaMn0.1Fe0.4Co0.5O3 | 0 | 0.1 | 0.4 | 0.5 | 0 | Trigonal | 0.003 |
P18 | LaMn0.1Co0.9O3 | 0 | 0.1 | 0 | 0.9 | 0 | Trigonal | 0.000 |
PN1a | LaMn0.4(CrNi)0.3O3 | 0.3 | 0.4 | 0 | 0 | 0.3 | Orthorhombic | 0.003 |
PN1b | LaMn0.4(CrNi)0.3O3 | 0.3 | 0.4 | 0 | 0 | 0.3 | Orthorhombic | 0.003 |
PN1c | LaMn0.4(CrNi)0.3O3 | 0.3 | 0.4 | 0 | 0 | 0.3 | Orthorhombic | 0.008 |
PN2 | LaCo0.4(CrNi)0.3O3 | 0.3 | 0 | 0 | 0.4 | 0.3 | Trigonal | 0.002 |
PN3 | LaCo0.4(MnNi)0.3O3 | 0 | 0.3 | 0 | 0.4 | 0.3 | Trigonal | 0.015 |
PN4 | LaFe0.4(CoNi)0.3O3 | 0 | 0 | 0.4 | 0.3 | 0.3 | Orthorhombic | 0.015 |
PN5 | LaNi0.4(CrFe)0.3O3 | 0.3 | 0 | 0.3 | 0 | 0.4 | Orthorhombic | 0.005 |
PN6 | LaNi0.4(CrCo)0.3O3 | 0.3 | 0 | 0 | 0.3 | 0.4 | Trigonal | 0.008 |
PN7 | LaNi0.4(MnFe)0.3O3 | 0 | 0.3 | 0.3 | 0 | 0.4 | Orthorhombic | 0.003 |
PN8 | La(CrNi)0.5O3 | 0.5 | 0 | 0 | 0 | 0.5 | Orthorhombic | 0.002 |
PN9 | La(MnNi)0.5O3 | 0 | 0.5 | 0 | 0 | 0.5 | Orthorhombic | 0.002 |
PN10 | La(FeNi)0.5O3 | 0 | 0 | 0.5 | 0 | 0.5 | Orthorhombic | 0.014 |
PN11 | La(CoNi)0.5O3 | 0 | 0 | 0 | 0.5 | 0.5 | Trigonal | 0.017 |
PN15 | LaFe0.4Co0.1Ni0.5O3 | 0 | 0 | 0.4 | 0.1 | 0.5 | Trigonal | 0.008 |
PN16 | LaFe0.1Co0.4Ni0.5O4 | 0 | 0 | 0.1 | 0.4 | 0.5 | Trigonal | 0.009 |
PN17a | La(CrMn)0.1Co0.2Ni0.6O3 | 0.1 | 0.1 | 0 | 0.2 | 0.6 | Trigonal | 0.006 |
PN17b | La(CrMn)0.1Co0.2Ni0.6O3 | 0.1 | 0.1 | 0 | 0.2 | 0.6 | Trigonal | 0.006 |
PN18a | LaFe0.1Co0.3Ni0.6O3 | 0 | 0 | 0.1 | 0.3 | 0.6 | Trigonal | 0.002 |
PN18b | LaFe0.1Co0.3Ni0.6O3 | 0 | 0 | 0.1 | 0.3 | 0.6 | Trigonal | 0.003 |
PN19a | La(FeCo)0.2Ni0.6O3 | 0 | 0 | 0.2 | 0.2 | 0.6 | Trigonal | 0.000 |
PN19b | La(FeCo)0.2Ni0.6O3 | 0 | 0 | 0.2 | 0.2 | 0.6 | Trigonal | 0.003 |
PN20 | LaMn0.2Co0.1Ni0.7O3 | 0 | 0.2 | 0 | 0.1 | 0.7 | Trigonal | 0.008 |
PN21a | LaCr0.2Ni0.8O3 | 0.2 | 0 | 0 | 0 | 0.8 | Trigonal | 0.001 |
PN21b | LaCr0.2Ni0.8O3 | 0.2 | 0 | 0 | 0 | 0.8 | Trigonal | 0.001 |
Sample | Formula | Cr | Mn | Fe | Co | Zn | Crystal System | δ |
---|---|---|---|---|---|---|---|---|
P1 | LaCrO3 | 1 | 0 | 0 | 0 | 0 | Orthorhombic | 0.003 |
P2 | La(CrMn)0.5O3 | 0.5 | 0.5 | 0 | 0 | 0 | Orthorhombic | 0.006 |
P3 | La(CrFe)0.5O3 | 0.5 | 0 | 0.5 | 0 | 0 | Orthorhombic | 0.002 |
P4a | La(CrCo)0.5O3 | 0.5 | 0 | 0 | 0.5 | 0 | Trigonal | 0.027 |
P4b | La(CrCo)0.5O3 | 0.5 | 0 | 0 | 0.5 | 0 | Trigonal | 0.027 |
P5a | LaCr0.4(FeCo)0.3O3 | 0.4 | 0 | 0.3 | 0.3 | 0 | Orthorhombic | 0.005 |
P5b | LaCr0.4(FeCo)0.3O3 | 0.4 | 0 | 0.3 | 0.3 | 0 | Orthorhombic | 0.008 |
P5c | LaCr0.4(FeCo)0.3O3 | 0.4 | 0 | 0.3 | 0.3 | 0 | Orthorhombic | 0.002 |
P6 | LaMn0.4(CrFe)0.3O3 | 0.3 | 0.4 | 0.3 | 0 | 0 | Orthorhombic | 0.011 |
P7 | LaMn0.4(CrCo)0.3O3 | 0.3 | 0.4 | 0 | 0.3 | 0 | Orthorhombic | 0.002 |
P8 | LaMnO3 | 0 | 1 | 0 | 0 | 0 | Orthorhombic | 0.006 |
P9a | La(MnFe)0.5O3 | 0 | 0.5 | 0.5 | 0 | 0 | Orthorhombic | 0.021 |
P9b | La(MnFe)0.5O3 | 0 | 0.5 | 0.5 | 0 | 0 | Orthorhombic | 0.018 |
P9c | La(MnFe)0.5O3 | 0 | 0.5 | 0.5 | 0 | 0 | Orthorhombic | 0.020 |
P10 | La(MnFe)0.5O3 | 0 | 0.5 | 0 | 0.5 | 0 | Orthorhombic | 0.003 |
P11 | LaMn0.4(FeCo)0.3O3 | 0 | 0.4 | 0.3 | 0.3 | 0 | Orthorhombic | 0.003 |
P12 | LaFeO3 | 0 | 0 | 1 | 0 | 0 | Orthorhombic | 0.003 |
P13 | La(FeCo)0.5O3 | 0 | 0 | 0.5 | 0.5 | 0 | Trigonal | 0.021 |
P14 | LaCoO3 | 0 | 0 | 0 | 1 | 0 | Trigonal | 0.003 |
P15a | LaMn0.6Co0.4O3 | 0 | 0.6 | 0 | 0.4 | 0 | Orthorhombic | 0.024 |
P15b | LaMn0.6Co0.4O3 | 0 | 0.6 | 0 | 0.4 | 0 | Orthorhombic | 0.017 |
P16 | LaMn0.1Fe0.9O3 | 0 | 0.1 | 0.9 | 0 | 0 | Orthorhombic | 0.009 |
P17 | LaMn0.1Fe0.4Co0.5O3 | 0 | 0.1 | 0.4 | 0.5 | 0 | Trigonal | 0.003 |
P18 | LaMn0.1Co0.9O3 | 0 | 0.1 | 0 | 0.9 | 0 | Trigonal | 0.000 |
PZ13 | LaCr0.3Mn0.5Zn0.2O3 | 0.3 | 0.5 | 0 | 0 | 0.2 | Orthorhombic | 0.017 |
PZ14 | LaCr0.3Fe0.4Co0.1Zn0.2O3 | 0.3 | 0 | 0.4 | 0.1 | 0.2 | Orthorhombic | 0.012 |
PZ15 | LaMn0.7Fe0.1Zn0.2O3 | 0 | 0.7 | 0.1 | 0 | 0.2 | Orthorhombic | 0.006 |
PZ16a | LaCr0.7Zn0.3O3 | 0.7 | 0 | 0 | 0 | 0.3 | Orthorhombic | 0.041 |
PZ16b | LaCr0.7Zn0.3O3 | 0.7 | 0 | 0 | 0 | 0.3 | Orthorhombic | 0.035 |
PZ17a | LaCr0.4(FeZn)0.3O3 | 0.4 | 0 | 0.3 | 0 | 0.3 | Orthorhombic | 0.070 |
PZ17b | LaCr0.4(FeZn)0.3O3 | 0.4 | 0 | 0.3 | 0 | 0.3 | Orthorhombic | 0.056 |
PZ1 | LaMn0.4(CrZn)0.3O3 | 0.3 | 0.4 | 0 | 0 | 0.3 | Orthorhombic | 0.011 |
PZ18 | La(CrMn)0.3Fe0.1Zn0.3O3 | 0.3 | 0.3 | 0.1 | 0 | 0.3 | Orthorhombic | 0.012 |
PZ21a | LaMn0.4(CoZn)0.3O3 | 0 | 0.4 | 0 | 0.3 | 0.3 | Orthorhombic | 0.060 |
PZ21b | LaMn0.4(CoZn)0.3O3 | 0 | 0.4 | 0 | 0.3 | 0.3 | Orthorhombic | 0.065 |
PZ24 | LaCr0.3Mn0.2Co0.1Zn0.3O3 | 0.3 | 0.2 | 0 | 0.1 | 0.4 | Orthorhombic | 0.008 |
PZ25a | LaMn0.5Co0.1Zn0.4O3 | 0 | 0.5 | 0 | 0.1 | 0.4 | Orthorhombic | 0.023 |
PZ25b | LaMn0.5Co0.1Zn0.4O3 | 0 | 0.5 | 0 | 0.1 | 0.4 | Orthorhombic | 0.020 |
PZ25c | LaMn0.5Co0.1Zn0.4O3 | 0 | 0.5 | 0 | 0.1 | 0.4 | Orthorhombic | 0.021 |
PZ9 | La(MnZn)0.5O3 | 0 | 0.5 | 0 | 0 | 0.5 | Orthorhombic | 0.012 |
The first property of interest is the perovskite crystal system that can be either orthorhombic or trigonal for the investigated materials: this property has been further studied only for Ni-containing perovskites since, as it glaringly appears looking at the crystal system of samples in Table 2, single-phase Zn-containing perovskites exhibit only orthorhombic geometry. Before presenting the results, the following clarification must be made: common design of experiment tools, as those described so far, can model only quantitative, numerical responses while, in this case, the perovskites crystal system is undoubtedly a qualitative, dichotomic response since no copresence of the two geometries is ever detected but the materials exhibit either an orthorhombic or a trigonal phase. To model this response, we codify the experimental response for single-phase training samples on a 0–1 scale (1 for orthorhombic and 0 for trigonal) and we use these fictitious values to calculate the coefficients by MLR. Then, both the fitted and predicted data are decodified assigning orthorhombic geometry to values above 0.55, trigonal geometry to those below 0.45 and leaving a non-assigned region for intermediate values between 0.45 and 0.55. The computed coefficients, reported in Table S7 (ESI†) and depicted in Fig. S3a (ESI†), appropriately describes the distinction between the two geometries in the training set (E.V. = 85.25%, s = 0.19) with the fitted crystal system corresponding to the experimental one for all the samples, except for one per each geometry located in the non-assigned region, as summarised in Fig. S3b (ESI†). Also validation is successful since all the geometries are corrected predicted (Fig. S3c, ESI†).
As already presented before, a preliminary analysis of the results can be performed relying on coefficients significance: in this case, the highest significance (***, 99.9% C.L.) is associated with the linear terms, except for Co, and the interaction between Mn and Ni, the latter strongly promoting orthorhombic geometry. Still relevant (**, 99% C.L.) are Ni interactions with Cr or Fe, again promoting orthorhombic geometry, and with Mn and Co together, in this case leading to trigonal phase. Lastly, the lower effect (*, 95% C.L.) is attributed to the 2-cation interactions involving Co that promote either orthorhombic (Mn + Co, Ni + Co) or trigonal geometry (Cr + Co, Fe + Co) depending on the other cations involved. To better visualize all the effects involved, Fig. 5 reports some partial representations of the predicted crystal system, limiting the representation to ternary compositions including Ni and two other cations and plotting also the training samples referring to the given ternary composition, with both experimental and predicted values coloured according to the same colourmap. We can immediately observe that trigonal geometry is occurring in presence of Co and Ni while Cr, Mn and Fe promote the orthorhombic one. In addition, the trigonal geometry is occurring for lower contents of Ni and Co when Cr and Fe are added as third cations; in other words, Cr and Fe are less efficient than Mn in promoting orthorhombic geometry. Oppositely, when Co is excluded from the ternary composition and Ni is added to Mn and Fe or Cr, orthorhombic geometry undoubtedly occurs almost in the entire experimental domain, except for Ni content above 0.7.
The calculated coefficients are reported in Tables S8 and S9 (ESI†) and graphically depicted in Fig. S4a and S5a (ESI†), for Ni and Zn-containing perovskites, respectively. The first assumption made from these results is that both the models fit satisfactorily the experimental data (E.V.= 57.73%, s = 0.005 in the case of Ni; E.V.= 90.93%, s = 0.005 in the case of Zn), consequently showing a good agreement between experimental and fitted δ, as glaringly appears from Fig. S4b and S5b (ESI†), for Ni and Zn-containing perovskites, respectively. Moving to the analysis of the coefficients, in both the models none of the linear terms is found significant, thus suggesting that mono-cation perovskites exhibit similar non-stoichiometry while several interactions significantly affect this property, both including two and three cations, as presented in Fig. S4a and S5a (ESI†). The validation is successful in both cases since the RMSEPs (0.005 in the case of Ni; 0.006 in the case of Zn) are statistically equal to the fitting residuals standard deviation (calculated F = 1.17, tabulated F0.05,6,23 = 2.53 in the case of Ni; calculated F = 1.14, tabulated F0.05,6,15 = 2.79 in the case of Zn).
The last and the most important step of the analysis involves the discussion of the response trend in the domain of interest: as already mentioned above, the δ values can be predicted in the entire 5-cation domain but this domain cannot be completely represented in 2D or 3D plots. For this reason, only partial representations of ternary compositions of interest are presented to better visualise the relationship between oxygen non-stoichiometry and perovskites composition. In Fig. 6 is presented the case of Ni-containing perovskites, limiting the highest content of Ni to 0.8, when present, as a consequence of the previously presented estimation of the stability domain. As can be inferred from Fig. 6, the highest non-stoichiometry is registered for binary combinations of Co and Cr or Fe, even with lower values. In contrast, samples containing higher content of Mn and, even more, Ni exhibit a generally low δ. Therefore, limiting the investigation to La(CrMnFeCoNi)O3 systems, oxygen non-stoichiometry is maximised in lower left plot, which means for ternary combinations of Co, Cr and Fe, especially for high Co contents while all the other regions are less favourable.
Oxygen non-stoichiometry trend for Zn-containing systems is presented in Fig. 7. To overcome the issue associated with low Zn solubility in the perovskite structure, the results of the stability domain modelling discussed in the previous sections are overlapped to response trend as gradient white regions according to the predicted percentage of the perovskite (95, 90 and 85% as reported in the plots). In this way, the δ trend is shown in the stability domain and in the regions corresponding to low percentage of secondary phases (white gradient) while the remaining areas are not described. The first aspect to be underlined is that Zn-containing perovskites exhibit much higher δ values with a maximum at around 0.08 while no values above 0.03 have been registered in the case of Ni-containing systems. As a consequence, the colourmaps in Fig. 6 and 7 are different and adapted to the specific system under investigation. Also in this case Co exerts the highest positive contribution, followed by Zn, Cr and eventually Mn, while Fe has no positive effect on this property. Therefore, the preferable domain regions to maximise this oxygen non-stoichiometry are the ternary combinations of Co, Zn and Cr or Mn, presented in the central and right upper plots, taking into account also the absence of secondary phases. In contrast, when Co or Zn or both the cations are excluded from the material, the oxygen non-stoichiometry suddenly drops, as presented in the lower panel of Fig. 7.
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Fig. 7 Predicted oxygen non-stoichiometry for Zn-containing perovskites for La(Fe,Co,Zn)O3 (left upper plot), La(Cr,Co,Zn)O3 (central upper plot), La(Mn,Co,Zn)O3 (right upper plot), La(Cr,Mn,Zn)O3 (left lower plot), La(Cr,Mn,Co)O3 (central lower plot) and La(Cr,Mn,Fe)O3 (right lower plot) and experimental values for the monophasic training samples, all coloured according to the colourmap reported next to the ternary plots. For Zn-containing plots, the stability domain represented in Fig. 3 are overlapped to the oxygen non-stoichiometry trend. |
The need of using two different colourmaps for Ni and Zn-containing perovskites does not allow to clearly understand if the models developed for the two different cases show a good agreement in predicting those perovskites included in both the domains, i.e. perovskites not containing either Ni or Zn. To clarify this point and to further confirm the validity of our approach and results, the δ values for samples in the candidate point lists (Table S1, ESI†) including neither Ni nor Zn, and thus in common between the two experimental domains, are predicted using both the models and are plotted in Fig. S6 (ESI†). Since the points perfectly lie on the y = x line, a good agreement is achieved between the prediction of the two models on the candidate points in common, thus confirming the validity and robustness of the fittings.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d4tc00993b |
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