research papers
accessUnveiling the ambient-condition structure of Sr2FeIrO6: a triclinic phase through synchrotron-based X-ray techniques and high pressure
aInstituto de Diseño para la Fabricación y Producción Automatizada, MALTA Consolider Team, Universitat Politècnica de València, 46022 València, Spain, bEuropean Synchrotron Radiation Facility, 38043 Grenoble, France, cDepartamento de Física Aplicada-ICMUV, MALTA Consolider Team, Universitat de València, Dr. Moliner 50, Burjassot, 46100 Valencia, Spain, dDepartamento CITIMAC, Universidad de Cantabria, Avda. Los Castros 48, 39005 Santander, Spain, eCELLS – ALBA Synchrotron, E-08290 Cerdanyola del Vallès, Barcelona, Spain, and fInstituto de Ciencia de Materiales de Madrid, CSIC, C/Sor Juana Inés de la Cruz 3, 28049 Madrid, Spain
*Correspondence e-mail: [email protected], [email protected]
Double perovskites with the formula A2BB′O6, such as Sr2FeIrO6, are being explored as unique platforms for unveiling diverse structural, electronic and magnetic properties. Inclusion of 3d and 5d transition metals in the B and B′ sites, as in Sr2FeIrO6, enables the study of electron correlation and spin–orbit coupling effects to tailor promising properties. The structure of Sr2FeIrO6 under ambient conditions has been widely debated, with theoretical and experimental studies suggesting several potential structures. This uncertainty complicates the understanding of its magnetic and electronic behaviours. High-pressure X-ray diffraction measurements, complemented by high-resolution powder X-ray diffraction studies under ambient conditions, have provided a definitive structural characterization of Sr2FeIrO6, crucial for interpreting its properties and guiding future research.
Keywords: Sr2FeIrO6; double perovskites; structural characterization; materials science; high-pressure powder diffraction; inorganic chemistry.
CCDC reference: 2457253
1. Introduction
Double perovskites with the formula A2BB′O6 have garnered significant interest due to the capability to accommodate different elements, with varying oxidation states, in A, B and B′ sites. This flexibility enables the design of materials with diverse structural, electronic and magnetic properties, and showing emerging exotic phenomena such as tunnelling-type magnetoresistance in Sr2FeMoO6 (Kobayashi et al., 1998
), half metallicity in A2CrWO6 (A = Ca, Sr, Ba) (Philipp et al., 2003
), the ferromagnetic insulator state in Y2CoMnO6 (Das & Choudhary, 2021
), ferrimagnetism in A2CrOsO6 (A = Sr, Ca) (Morrow et al., 2016
), the magneto-caloric effect in Nd2BMnO6 (B = Co, Ni) (Li et al., 2021
) and the spin-glass state in Sr2FeCoO6 (Pradheesh et al., 2012a
; Pradheesh et al., 2012b
). These features emerge through the interplay of 3d and 5d transition metals in B and B′ sites. Among these, Sr2FeIrO6 is particularly noteworthy due to the intriguing magnetic and structural phenomena arising from the combination of Fe and Ir, driven by strong spin–orbit coupling (SOC) and effects.
The structure of A2BB′O6 double perovskites has been the subject of numerous studies, where the mismatch in the sizes of the cations is revealed to be a crucial factor, evaluated through the t (Goldschmidt, 1926
):
where the ri's represent the ionic radii of A, B, B′ and O atoms. The lower the value of the mismatch, the less symmetric the structure becomes due to the high degree of tilt allowed for the B(B′)O6 octahedra, generally following the sequence [with their Glazer's notation (GN)] for double perovskites (Howard et al., 2003
): Fm3m, a0a0a0 > I4/m, a0a0c− > I2/m, a0b−b− > P21/n, a−a−c+ > I1, a−b−c− (Kharkwal et al., 2020
; Vasala & Karppinen, 2015
). In this particular case, Sr2FeIrO6 is a double perovskite compound with antisite disorder between Fe and Ir ions (i.e. occupation of Fe atoms in Ir sites and vice versa) within a distorted perovskite lattice. The structure of Sr2FeIrO6 at room temperature has been the subject of significant debate in the literature. Theoretical calculations suggest that the triclinic I1 structure and the monoclinic P21/n or I2/m structures have very similar total energy values, making it challenging to determine the most stable structure solely through computational means (Roy & Kanungo, 2022
). Experimental studies have also demonstrated uncertainty regarding the room-temperature structure, with some prioritizing monoclinic structures (Qasim et al., 2013
; Bufaiçal et al., 2016
; Laguna-Marco et al., 2015
; Retuerto et al., 2021
) whereas other studies have suggested that the most stable structure is triclinic under ambient conditions (Battle et al., 1999
; Kharkwal & Pramanik, 2018
). Resolving this structural ambiguity is crucial for understanding the material's properties and aligning scientific findings in the literature.
A review of the existing literature reveals that a triclinic phase in double perovskites, with the GN a−b−c− (different out-of-phase tilt angles along the a, b and c axes), is relatively uncommon and has primarily been observed in systems like Sr2BMoO6 (where B = Fe, Co, Ni, Zn, Ti, Mg) (Vasala et al., 2010
; Alarcon et al., 2012
; Marrero-López et al., 2009
). Conversely, for Sr2BIrO6 compounds, a monoclinic P21/n phase, with the GN a−a−c+ (same out-of-phase tilt angles along the a and b axes, different from an in-phase tilt angle along the c axis) predominates particularly for B = Ce, Ca, In, Sc, Lu, Ni, Tb and Y (Harada et al., 2000
; Jung & Demazeau, 1995
; Kayser et al., 2015
; Wakeshima et al., 1999
; Kayser et al., 2013
; Zhou et al., 2005
; Ranjbar et al., 2015
). In double perovskites where one of the B sites is fixed as Fe and the secondary cation is varied, such as in Sr2FeBO6, a tetragonal I4/m phase, with the GN a0a0c− (no tilt along the a and b axes and an out-of-phase tilt along the c axis), is often found, especially for B = Co, Re, Nb, Sb and Os (Pradheesh et al., 2012a
; Pradheesh et al., 2012b
; Nakamura & Oikawa, 2003
; Rosas et al., 2019
; Faik et al., 2010
; Retuerto et al., 2009
). These patterns hint at a possible dependence of the symmetry of the structure on the nature of both B and B′ ions, further complicating the structural determination of Sr2FeIrO6.
The exact structure of Sr2FeIrO6 under ambient conditions has been contested, leading to differing interpretations and reported properties. Previous studies have used various experimental techniques, such as X-ray diffraction (XRD) and neutron diffraction, to propose different structural models. Theoretical studies add complexity by indicating that multiple structures are energetically comparable. This hinders a comprehensive understanding of the material's magnetic and electronic behaviours, which are highly dependent on the precise arrangement of atoms in the crystal lattice.
Here, we address and resolve this controversy through synchrotron-based studies utilizing high-resolution powder X-ray diffraction (HR-PXRD) and high-pressure powder X-ray diffraction (HP-PXRD). Our synchrotron-based investigations provide a more accurate and definitive structural characterization of Sr2FeIrO6 than previous works. Through HR-PXRD and HP-PXRD techniques, we can distinguish between the competing structural models and establish the most accurate description of the at room temperature. This resolution of the structural ambiguity is pivotal for accurately interpreting the physical properties of the material and for guiding future research and applications involving Sr2FeIrO6 and its related double perovskites.
2. Experimental
2.1. Sample preparation
A polycrystalline sample of Sr2FeIrO6 was prepared by wet chemistry methods followed by annealing treatments. Stoichiometric amounts of Sr(NO3)2 (99%), IrO2 (99.9%) and FeC2O4·2H2O (99%) were dissolved in an aqueous solution of citric acid (10% w/w) and 1 ml of nitric acid to facilitate the dissolution of the starting materials. IrO2 was not dissolved in the solution but remained in suspension under magnetic stirring. The resulting suspension was gently heated until the organic resins formed, ensuring a homogeneous distribution of the involved cations. After evaporation, the resins were dried at 140°C and then heated at 600°C for 12 h (with a heating rate of 2°C min−1) to decompose the organic materials and eliminate the nitrates. This treatment produced highly reactive precursor materials, which were then heated in air at 1100°C for 12 h to obtain a phase-pure sample.
2.2. High-angular-resolution X-ray diffraction
HR-PXRD experiments were performed at the powder diffraction end station of the MSPD beamline at the Spanish ALBA synchrotron, using a high-angular-resolution multianalyzer (MAD) setup. The samples were contained in 0.3 mm diameter borosilicate capillaries, which were rotated during the collection time, and transmission geometry was used. The operating wavelength was calibrated using a NIST standard silicon sample, NIST Si640D (λ = 0.4138 Å). Given the strong X-ray absorption of iridium, a 0.3 mm diameter capillary was specifically chosen to achieve a reasonable sample absorption of μR = 1.1. Using the MAD setup, the analyser crystals act as additional tiny aperture slits and thus limit peak broadening induced by residual divergence of the beam impinging on the sample, by the size of the sample and the slight displacement of the sample due to wobbling. In this way, the highest angular resolution is obtained with the beamline configuration (Fauth et al., 2013
). The angular range covered was up to 40°.
2.3. High-pressure angular-dispersive X-ray diffraction
HP experiments were conducted using a membrane-type diamond-anvil cell with IIA-type diamonds, 350 µm in size. A pre-indented stainless-steel gasket with a hole diameter of 150 µm was used as a pressure chamber. We employed a 4:1 methanol–ethanol mixture as a pressure-transmitting medium, which remains quasi-hydrostatic up to 10 GPa (Klotz et al., 2009
). Pressure measurements were performed using the Cu equation of state (Dewaele et al., 2004
). HP-PXRD experiments were carried out at the BL04-MSPD beamline of the ALBA-CELLS synchrotron (Fauth et al., 2013
), utilizing a monochromatic wavelength of 0.4642 Å and a spot size of 20 µm × 20 µm full width at half-maximum. A Rayonix SX165 CCD image plate was used to collect the diffraction patterns, which were integrated into conventional XRD patterns using DIOPTAS (Prescher & Prakapenka, 2015
). The GSAS-II software (Toby & Von Dreele, 2013
) was employed to perform Rietveld and Le Bail fits on powder diffractograms. Atomic positions were not refined for the high-pressure data due to limited data quality; instead, the ambient-pressure atomic coordinates were used as a fixed model for profile fitting of the high-pressure patterns. Thus, no additional atomic coordinate values are reported under high pressure. The angular range covered was up to 20°.
3. Theoretical calculations
First-principles electronic structure calculations were conducted using the density functional theory (DFT) framework implemented in the Vienna Ab initio Simulation Package (VASP). To avoid atomic disorder, all mixed Fe/Ir sites were modelled as idealized positions occupied exclusively by either Fe or Ir atoms, at 2f and 2g sites, respectively (Kresse & Furthmüller, 1996a
; Kresse & Furthmüller, 1996b
; Kresse & Joubert, 1999
). Projected augmented wave potentials (Blöchl, 1994
) were used to describe valence electrons of Sr (4s2 4p6 5s2), Fe (3d6 4s2), Ir (5d7 6s2) and O (2s2 2p4) atoms. We used Liechtenstein's approximation to include the on-site Coulomb (U) and exchange (J) interaction in our DFT + U calculations. For Fe ions, these values were fixed to U = 4.40 and J = 3.0 eV (Serrate et al., 2006
), and for Ir ions U = 2 eV (Liechtenstein et al., 1995
). Spin-polarized calculations were performed with the generalized gradient approximation of Perdew–Burke–Ernzerhof revised for solids (PBEsol) (Perdew et al., 2008
) for the exchange and correlation energy, which provided crystal structural parameters that closely match the experimental values. The unit-cell geometries and atomic positions were optimized using the conjugate-gradient algorithm (Teter et al., 1989
; Bylander et al., 1990
). Our preliminary tests, including SOC, indicated changes in lattice parameters and atomic positions of approximately 0.1% or less. Given the negligible impact and the difficulty of achieving convergence with SOC, we chose to omit SOC in this work. A plane-wave kinetic-energy cutoff of 550 eV was set, along with a dense Monkhorst–Pack grid (Monkhorst & Pack, 1976
) with an 8 × 8 × 7 k-point sampling mesh to ensure the total energy converged to around 10−6 eV, with stress tensor deviations from a diagonal hydrostatic form being less than 1 kbar (0.1 GPa). All the structures were visualized using the VESTA program (Momma & Izumi, 2011
).
4. Results and discussion
4.1. Indexing
The HR-PXRD pattern of Sr2FeIrO6 (from our phase-pure, highly crystalline sample) was indexed to evaluate candidate structures reported in the literature. We tested a triclinic model (space group I1) against two monoclinic models (space groups I2/m and P21/n) via the M20 figure of merit, developed by de Wolff (1968
), with the resulting values given in Table 1
. The triclinic model yielded the highest indexing quality, with a de Wolff M20 figure of merit of 172, compared with 153 for I2/m and 57 for P21/n. This superior M20 value indicates that the triclinic lattice parameters provide the best fit to the observed diffraction peaks. Consistently, Le Bail profile fits for each model showed that, while all three structures could reproduce the main diffraction features, the triclinic model produced the lowest residuals and best agreement factors. In contrast, the monoclinic models showed slightly higher misfit. These results firmly point to a triclinic unit cell as the correct description of Sr2FeIrO6 under ambient conditions, even before considering Rietveld refinement.
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4.2. Rietveld refinement under ambient conditions
using the experimental HR-PXRD pattern was performed using the triclinic I1 model (Fig. 1
). The F2meas versus F2obs plot from this HR-PXRD pattern is included in Fig. S1 of the supporting information. The refinement process yielded an Rwp of 13%. This relatively high Rwp value can be attributed to the complexity of the triclinic structure, which involves 25 variables: three lattice parameters, a, b and c; three angles, α, β and γ; three O atomic positions with the three fractional coordinates free; fractional occupancies between Fe and Ir atomic positions in 2f and 2g sites (Fig. 1
, right); and eight isotropic atomic displacement parameters (see Table 2
). The significant number of parameters required for an accurate fit underscores the intricate nature of the triclinic structure. The fractional occupancies obtained from the Rietveld refinement are in agreement with results obtained in the literature with values that vary between 10 and 20%. The resulting crystallographic data have been deposited at the Cambridge Crystallographic Data Centre (CCDC deposition No. 2457253).
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| Figure 1 Perspective view of the triclinic structure of Sr2FeIrO6 in I1 (left panel) and the Sr2FeIrO6 structure oriented along the b axis (right panel). In the right panel, Sr atoms have been removed for easier visualization. One inequivalent Sr atom occupies the 4i sites, as do the three inequivalent O atoms. In two inequivalent positions, in 2f and 2g sites, high fractional occupancies of Fe and Ir are found, respectively. Further clarifications are given in the main text. |
In addition to the a comparative analysis of Le Bail fits was conducted to evaluate the plausibility of the three proposed structures for Sr2FeIrO6: the triclinic I1 structure, and both monoclinic P21/n and I2/m structures, obtaining similar results to those reported by Kharkwal et al. (2020
). This comparative analysis between the experimental XRD patterns and each of the three structures with the related residuals is depicted in Fig. 2
. The residuals were found to be similar across all three fits. However, the triclinic structure exhibited the smallest residuals and the lowest quality factors, making it the most plausible structure. Despite this, the residuals for the monoclinic P21/n and I2/m structures were not significantly higher, suggesting that these structures cannot be entirely ruled out. Additionally, the experimental lattice parameters and volume for the P21/n and I2/m structures from Le Bail fits are given in Table 2
along with their theoretical values. To allow a direct comparison of the lattice parameters and unit-cell volume, the three space groups have been presented in their non-standard settings. Although this approach may go against certain data-validation checks performed by checkCIF/PLATON (Spek, 2009
), it provides a consistent structural framework for comparison. For the triclinic model, a PLAT155 alert arises because it is not reported in its Niggli-reduced cell, whereas for the monoclinic P21/n and I2/m models, a PLAT157 alert is reported since, by convention, the monoclinic angle β is required to be larger than 90º. The lattice parameters a, b and c of the three models agree nicely. One detail to remark on is that the β angles in the monoclinic P21/n and I2/m models are predicted to be higher than 90º, unlike our experimental values, which are lower than 90º. These experimental values agree with those reported for the monoclinic P21/n and I2/m models by Bufaiçal et al. (2016
) of 89.951 (1)° and 89.72 (1)°, respectively. The present refinements highlight the inherent complexity in accurately determining the symmetry of the crystal structure of Sr2FeIrO6, providing no evidence of higher-symmetry space groups under ambient conditions. Instead, prior HR-XRD studies and our own data support the low-symmetry triclinic model (Page et al., 2018
). The small differences in residuals among the three proposed structures indicate that the structure under ambient conditions is not straightforward to ascertain. This ambiguity necessitates the use of new tools to resolve it.
| Figure 2 Le Bail fits of the HR-XRD pattern of Sr2FeIrO6 using an (a) triclinic I1, (b) monoclinic P21/n and (c) monoclinic I2/m structure. |
4.3. High pressure behaviour
To provide additional proof of the actual structure of Sr2FeIrO6 under ambient conditions, we performed a synchrotron-based HP-PXRD experiment [Fig. 3
(a)]. The XRD patterns obtained under varying pressure conditions were analysed using Rietveld refinement, considering the structural factors with fixed atomic positions, i.e. by refining all the structural parameters except the oxygen atomic positions, due to the limitation of the 2θ range for the HP measurements. The results helped us to derive the pressure–volume equation of state and monitor the evolution of the lattice parameters and angles under high pressure. In the supporting information, Fig. S2 contains three representative 2D diffraction images at 1.4, 10 and 15.3 GPa [panels (a), (c) and (e)], with their respective Rietveld refinements [panels (b), (d) and (f)]. As can be seen, no rings from the stainless-steel gasket were observed through the whole pressure range studied, and no abrupt changes in the peak broadening above 10 GPa were seen that would indicate that the 4:1 methanol–ethanol pressure-transmitting medium had solidified.
| Figure 3 (a) XRD patterns of Sr2FeIrO6 at different pressures stacked and vertically shifted for clarity. HP evolution of Bragg peaks around (b) 6°, (c) 12.5° and (d) 8.8°. |
During the fitting process, it became evident that the monoclinic structures were insufficient to describe the evolution of the experimental diffraction patterns throughout the entire pressure cycle. At pressures below 7 GPa, both monoclinic structures provided satisfactory fits to the diffraction patterns. However, as the pressure increased beyond 7 GPa, noticeable splits in some Bragg reflections indicated the inadequacy of these models in describing the structural changes accurately [as shown in Figs. 3
(b), 3
(c) and 3
(d)]. These splits suggest the presence of additional structural complexities not captured by simpler monoclinic symmetries. Moreover, theoretical calculations for both monoclinic structures reveal no indication of a second-order phase transition, consistent with the smooth evolution of the reflection peaks. The theoretically simulated enthalpy versus pressure curves for the three proposed structures (Fig. 4
) indicate that they have similar energies, with all lines overlapping within the calculation uncertainties. When the triclinic structure was employed from the beginning, the variation of lattice parameters displayed a smooth and continuous evolution with pressure, as illustrated in the experimental and theoretical normalized lattice parameters in Fig. 5
(a). Neither the experimental nor theoretical pressure dependence of the volume show any anomaly, as depicted in Fig. 5
(b). This critical observation indicated a more accurate representation of the actual structural changes occurring in Sr2FeIrO6. The absence of abrupt changes or anomalies in the normalized lattice parameter trends provided compelling evidence for the triclinic nature of the structure under all examined pressures. Further comparisons can be made by calculating the third-order Birch–Murnaghan equation of state (BM3-EoS) for Sr2FeIrO6, the parameters of which can be found in Table 3
. The BM3-EoS was calculated using the free software EoSfit (Angel et al., 2014
).
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| Figure 4 HP dependence of theoretically simulated enthalpy for the three structures proposed in the literature. |
| Figure 5 (a) Evolution of the normalized lattice parameters (and angles) under HP (inset) of the Sr2FeIrO6 structure in the I1, and (b) pressure dependence of the volume. Experimental data are represented as symbols and the theoretical calculations as solid lines. The region of quasi-hydrostatic conditions up to ∼10 GPa for the 4:1 methanol–ethanol mixture pressure-transmitting medium is shaded in the plots. |
The theoretically simulated data gave rise to a bulk modulus, B0,theor, at 0 GPa of 167.5 (1) GPa with a first pressure derivative of the bulk modulus, B′0,theor, of 4.0 (1). Experimentally, these parameters are B0,exp = 137.1 (1) GPa and B′0,exp = 7.1 (1). To compare B0,exp with B0,theor and the strong correlation between B0 and B′0, we fixed B′0,exp to the value given by the theoretical calculations, attaining a B0,exp value of 151.7 (1) GPa, showing a good agreement between both techniques.
It is noteworthy that the smooth evolution of normalized lattice parameters for the triclinic model in the whole pressure range up to 15.3 GPa contrasts sharply with the need for a above 7 GPa when using the monoclinic models. Regarding the axial compressibilities derived from the linearized 3BM-EoS given in Table 3
, the a and c axes exhibit similar pressure behaviour, both experimentally and theoretically. It is the b axis which, experimentally, is slightly softer as theoretically predicted but, on average, the a and b axes are more compressible than the longer c axis. This comparison serves as additional support for the triclinic model in the pressure range evaluated. As additional proof of a triclinic stucture being consistent with the data in the pressure range studied, we plotted the pressure evolution of the experimental and theoretical Fe—O and Ir—O distances, shown in Fig. 6
. Even though the experimental bond distances from HR-PRXRD show a certain offset with respect to the high-pressure data, this does not hamper our comparison of the experimental and theoretical high-pressure trends. Experimental and theoretical Fe—O bond distances compress at a similar rate. However, this does not happen for Ir—O bond distances, which are less compressible according to the trends predicted by our theoretical calculations than the experimental trends. Regardless of this, both experimental and theoretical bond distances share a common feature: Fe(Ir)—O3 bond distances directed along the c axis are less compressible than the Fe(Ir)—O1, O2 bond distances located near the ab plane, a statement that supports a lower axial compressibility of the c axis than those of the a and b axes, as shown in Table 3
. This can be easily explained by observing the SrO12 dodecahedron arrays that are placed along the c axis that govern its compressibility.
| | Figure 6 Evolution of the experimental and theoretical (a) Fe—O and (b) Ir—O bond distances under HP of the Sr2FeIrO6 structure in the I1. Experimental data are represented as symbols and the theoretical calculations as solid lines. Experimental Fe(Ir)—O bond distances represent the Fe(Ir) atoms in the atomic sites 2f(2g) with a fractional occupancy of 82.6%. The region of quasi-hydrostatic conditions up to ∼10 GPa for the 4:1 methanol–ethanol mixture pressure-transmitting medium is shaded in the plots. |
The necessity of introducing a in these simpler monoclinic models highlights their inability to fully capture the structural intricacies of Sr2FeIrO6 under high pressure. In contrast, the triclinic model's capacity to explain the diffraction patterns without requiring such transitions underscores its validity. Furthermore, the continuous evolution observed in the triclinic phase model supports the hypothesis that the original structure of Sr2FeIrO6 is triclinic (Fig. 5
). Additionally, attempts to index the 15.3 GPa pattern with higher symmetry cells (monoclinic P21/n or I2/m) were unsuccessful – these cells could not reproduce key peak splittings and yielded significantly larger profile residuals. Neither the calculations nor the experiments provide evidence for a phase transition to a new space group up to 15.3 GPa. In particular, the smooth evolution of the lattice metrics and the absence of any abrupt anomalies suggest that Sr2FeIrO6 maintains the triclinic structure throughout this pressure range. While we cannot absolutely rule out an undetectably subtle symmetry change, our extensive analysis did not reveal any such transition. Thus, we are confident in asserting the robustness of the triclinic model in this pressure range.
The bulk modulus obtained for Sr2FeIrO6 can be contextualized by comparing it with other similar double perovskites. Sr2FeIrO6 has B0,exp = 164 (2) GPa, which is comparable to other members of the double perovskite family, such as Sr2CoMoO6 [B0,exp = 152 (9) GPa (Lufaso et al., 2006
)], Sr2CuWO6 [B0,exp = 185 (14) GPa (Lufaso et al., 2006
)], Sr2CrReO6 [B0,exp = 170 (4) GPa, B0,theor = 172.6 GPa (Olsen et al., 2009
)] and Sr2MnSbO6 [B0,theor = 157.24 GPa (Sosa-Correa et al., 2023
)]. This comparison indicates that Sr2FeIrO6 has experimental and theoretical B0 values that fall within the typical range for double perovskites, suggesting that its compressibility and resistance to volume change under pressure are consistent with those of similar compounds.
In summary, while both monoclinic models can describe the structure of Sr2FeIrO6 at lower pressures, they fail to account for the structural evolution at pressures beyond 7 GPa. The requirement of a above 7 GPa for these models is rendered unnecessary when a triclinic phase is considered from the outset. The smooth variation of normalized lattice parameters in the triclinic model serves as unambiguous proof of the original triclinic structure of Sr2FeIrO6, providing a more comprehensive understanding of its HP behaviour and confirming its triclinic symmetry under all examined conditions. Our results unveil that Sr2FeIrO6 maintains its low-symmetry tilt system (a−b−c− in GN) under pressures up to 15 GPa, a finding which underscores the rigidity of this distortion. This contrasts with many perovskites where pressure induces symmetry elevation; here the triclinic distortions are persistent.
5. Conclusions
In this study, we have confirmed that a triclinic I1 provides a more realistic model for the observed diffraction data of Sr2FeIrO6 compared with the existing models. Our synchrotron-based HR-PXRD and HP-PXRD studies provide compelling evidence that Sr2FeIrO6 adopts a triclinic I1 structure under ambient conditions. This conclusion is supported by the highest M20 figure of merit during the indexing process and the superior quality of achieved using the triclinic model compared with other proposed structures. The analysis also shows that the triclinic structure captures the structural complexity and atomic arrangements more accurately, thus establishing a reliable crystallographic framework for Sr2FeIrO6.
Theoretical DFT calculations further corroborate the experimental findings, revealing minimal energy differences between the proposed triclinic and monoclinic structures, yet favouring the triclinic structure based on better alignment with experimental parameters. By performing HP-PXRD we observed that the normalized lattice parameters evolve smoothly and continuously in the triclinic model, in stark contrast to the anomalies observed when using monoclinic structural models (especially above 7 GPa). Additionally, the increasing Fe(Ir)—O bond distances with pressure evolve smoothly, supporting the triclinic model. This provides robust evidence for the stability of the triclinic phase across a broad range of pressures, eliminating the need for an assumed phase transition that the monoclinic models required at higher pressures. The calculated bulk modulus of Sr2FeIrO6 at ambient pressure, derived from the pressure–volume data using a BM3-EoS, and the axial compressibilities from linearized BM3-EoS show good agreement between theoretical and experimental values. This consistency highlights the reliability of our experimental setup, and the theoretical framework used.
The findings from this research have significant implications for understanding the magnetic and electronic behaviours of Sr2FeIrO6. The precise identification of the triclinic structure clarifies the discrepancies in earlier reports. It provides a more accurate basis for exploring the material's complex SOC and electron correlation effects, which are highly structure-dependent. This work lays the groundwork for future investigations into the exotic magnetic and electronic phenomena inherent in Sr2FeIrO6 and other related double perovskites by establishing the correct structural model. The structural insights gained here are also crucial for guiding the synthesis of these materials for technological uses where specific magnetic or electronic properties are required.
Supporting information
CCDC reference: 2457253
contains datablock P0-Rietveld_v3-todorefinado3.bak0. DOI: https://doi.org/10.1107/S2052252525008218/oz5009sup1.cif
Supporting figures. DOI: https://doi.org/10.1107/S2052252525008218/oz5009sup2.pdf
| Fe0.5Ir0.5O3Sr | β = 90.136 (4)° |
| Mr = 259.65 | γ = 90.127 (3)° |
| Triclinic, ¯I1 | V = 244.95 (1) Å3 |
| a = 5.5716 (3) Å | Z = 4 |
| b = 5.5676 (3) Å | Dx = 7.041 Mg m−3 |
| c = 7.89642 (17) Å | T = 300 K |
| α = 89.763 (3)° |
| Least-squares matrix: full | Profile function: Finger-Cox-Jephcoat function parameters U, V, W, X, Y, SH/L: peak variance(Gauss) = Utan(Th)2+Vtan(Th)+W: peak HW(Lorentz) = X/cos(Th)+Ytan(Th); SH/L = S/L+H/L U, V, W in (centideg)2, X & Y in centideg 359.111, -58.925, 2.974, 0.586, 0.411, 0.002, |
| Rp = 0.093 | 7 parameters |
| Rwp = 0.134 | (Δ/σ)max = 0.099 |
| Rexp = 0.006 | Background function: Background function: "chebyschev" function with 16 terms: 9385.017, 2580.242, 25124.143, -186393.132, -516161.786, 2.333943047e6, 3.439625975e6, -1.2422545252e7, -1.0265731033e7, 3.3013226862e7, 1.5422560934e7, -4.6237913498e7, -1.1321060326e7, 3.2551887016e7, 3.218096032e6, -9.059493051e6, |
| R(F2) = 0.05497 | Preferred orientation correction: March-Dollase correction coef. = 1.000 axis = [0, 0, 1] |
| 10609 data points |
| x | y | z | Uiso*/Ueq | Occ. (<1) | |
| Sr | 0.50000 | 0.50000 | 0.25000 | 0.0027* | |
| Fe | 0.00000 | 0.50000 | 0.00000 | 0.0027* | 0.8258 |
| Ir | 0.50000 | 0.00000 | 0.00000 | 0.0027* | 0.8258 |
| O1 | 0.24642 | 0.24361 | 0.99280 | 0.0100* | |
| O2 | 0.24277 | 0.76305 | 0.01535 | 0.0100* | |
| O3 | 0.54267 | 0.06175 | 0.27082 | 0.0100* | |
| Ir7 | 0.00000 | 0.50000 | 0.00000 | 0.0027* | 0.1742 |
| Fe8 | 0.50000 | 0.00000 | 0.00000 | 0.0027* | 0.1742 |
| Sr—Sri | 3.9482 | Ir—O3 | 2.1797 |
| Sr—Srii | 3.9427 | O1—Srxvii | 2.8566 |
| Sr—Sriii | 3.9427 | O1—Srviii | 2.7985 |
| Sr—Sriv | 3.9482 | O1—Sriv | 2.7732 |
| Sr—Srv | 3.9339 | O1—Srxviii | 2.7205 |
| Sr—Srvi | 3.9339 | O1—Fexvii | 1.9838 |
| Sr—O1vii | 2.8566 | O1—Irxvii | 1.9613 |
| Sr—O1viii | 2.7985 | O2—Sr | 2.7580 |
| Sr—O1iv | 2.7732 | O2—Srxiii | 2.8164 |
| Sr—O1ix | 2.7205 | O2—Sriii | 2.6539 |
| Sr—O2 | 2.7580 | O2—Fe | 1.9953 |
| Sr—O2x | 2.8164 | O2—Irxix | 1.9494 |
| Sr—O2iii | 2.6539 | O3—Sr | 2.4569 |
| Sr—O3 | 2.4569 | O3—Srii | 2.5776 |
| Sr—O3ii | 2.5776 | O3—Fex | 1.8564 |
| Fe—O1vii | 1.9838 | O3—Ir | 2.1797 |
| Fe—O1xi | 1.9838 | Ir7—O1xi | 1.9838 |
| Fe—O2 | 1.9953 | Ir7—O1vii | 1.9838 |
| Fe—O2xii | 1.9953 | Ir7—O2 | 1.9953 |
| Fe—O3v | 1.8564 | Ir7—O2xii | 1.9953 |
| Fe—O3xiii | 1.8564 | Ir7—O3xiii | 1.8564 |
| Ir—O1vii | 1.9613 | Ir7—O3v | 1.8564 |
| Ir—O1xiv | 1.9613 | Fe8—O1xiv | 1.9613 |
| Ir—O2i | 1.9494 | Fe8—O1vii | 1.9613 |
| Ir—O2xv | 1.9494 | Fe8—O2xv | 1.9494 |
| Ir—O3xvi | 2.1797 | Fe8—O2i | 1.9494 |
| O3—Sr—O3ii | 76.931 | O3xiii—Ir7—O3v | 180 |
| Sr—O3—Srii | 103.069 |
| Symmetry codes: (i) −x+1, −y+1, −z; (ii) −x+3/2, −y+1/2, −z+1/2; (iii) −x+1/2, −y+3/2, −z+1/2; (iv) −x+1, −y+1, −z+1; (v) −x+1/2, −y+1/2, −z+1/2; (vi) −x+3/2, −y+3/2, −z+1/2; (vii) x, y, z−1; (viii) −x+1/2, −y+1/2, −z+3/2; (ix) x+1/2, y+1/2, z−1/2; (x) x+1/2, y−1/2, z+1/2; (xi) −x, −y+1, −z+1; (xii) −x, −y+1, −z; (xiii) x−1/2, y+1/2, z−1/2; (xiv) −x+1, −y, −z+1; (xv) x, y−1, z; (xvi) −x+1, −y, −z; (xvii) x, y, z+1; (xviii) x−1/2, y−1/2, z+1/2; (xix) x, y+1, z. |
Funding information
This publication is part of the project MALTA Consolider Team network (grant No. RED2022-134388-T), financed by MINECO/AEI/10.13039/501100003329; by I+D+i projects (grant Nos. PID2021-125927NB-C21, PID2021-125927NA-C22, PID2022-138076NB-C42, PID2022-138076NB-C44), financed by MCIN/AEI/10.13039/501100011033; by projects CIPROM/2021/075 (GREENMAT) and MFA/2022/025 (ARCANGEL), financed by Generalitat Valenciana. VM thanks the MICINN for the Beatriz Galindo distinguished researcher program (BG20/00077). VPCG and TMGS thank Primeros proyectos de investigacion 2022 (PAID-06-22), en el marco de ayudas del Vicerrectorado de Investigación de la Universitat Politécnica de Valencia. We also thank ALBA synchrotron light source for funded experiments 2023027484 and 2022025730 at the MSPD-BL04 beamline.
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