research papers
accessRevisiting the structures and phase transitions of PrNiO3 nickelate using symmetry-mode analysis
aInstituto de Ciencia de Materiales de Madrid, CSIC, Cantoblanco, Madrid, 28049, Spain, bLaboratory of Electromechanical Systems (LASEM), National Engineering School of Sfax, BPW 3038, Sfax, Tunisia, and cEuropean Synchrotron Radiation Facility (ESRF), 71 Avenue des Martyrs, Grenoble, 38000, France
*Correspondence e-mail: [email protected], [email protected]
We have investigated the complete sequence of temperature-induced structural phase transitions in PrNiO3 using high-angular-resolution synchrotron X-ray diffraction and symmetry-adapted distortion-mode analysis. By employing a high-purity sample synthesized under high pressure (3.5 GPa at 1073 K), we resolve the monoclinic (P21/n) → orthorhombic (Pbnm) → rhombohedral (R3c) evolution over an extended temperature range (10–900 K). Beyond confirming the role of oxygen stretching modes in the insulator–metal transition at ∼130 K, we show that these phonon modes also govern the high-temperature metallic–metallic transition at ∼750 K. This work provides a comprehensive mode-resolved picture of both insulator and metallic regimes in PrNiO3 and highlights the central role of phonon-mediated processes in driving charge disproportionation and lattice symmetry breaking across all the crystalline phases.
Keywords: RNiO3 perovskites; phase transitions; symmetry-mode analysis; metal–insulator transitions.
1. Introduction
Nickelates with the formula RNiO3 (R represents a rare earth element, such as La, Pr, Nd, Sm etc.) are complex oxide materials that have attracted increasing interest in solid-state physics and materials science research (Medarde, 1997
; Tomioka et al., 2021
; Catalano et al., 2018
; Jaramillo et al., 2014
; Gawryluk et al., 2019
; Klein et al., 2021
; Catalan, 2008
; Wang et al., 2019
). These compounds belong to the perovskite family, characterized by a unique crystal structure that provides exceptional electronic, magnetic and optical properties. The rare earth nickelate perovskites exhibit a variety of intriguing phenomena, such as metal–insulator transitions at characteristic temperatures TIM, unusual magnetic properties, and strong coupling between structural, electronic and spin degrees of freedom (Medarde et al., 1997
; Rodrigues et al., 2023
, 2024
; Alonso et al., 2000
). These characteristics make RNiO3 promising candidates for applications in advanced electronic devices such as catalysts, sensors, actuators, resistive memories and energy conversion devices (Xin et al., 2020
; Pandiyan et al., 2023
; Retuerto et al., 2017
; Junita et al., 2022
). The ability to tune their properties by varying the ionic radius of the rare earth element, applying external stresses or introducing additional doping provides a wide range of possibilities for engineering new functionalities in multifunctional materials.
Rare earth nickelates RNiO3 are electron-correlated materials, where the interplay between charge and spin order leads to a rich phase diagram, passing through antiferromagnetic insulators to paramagnetic metals. As initially described by Demazeau et al. (1971
), these materials enjoyed a renaissance of interest after the discovery of a thermally driven insulator–metal (IM) transition depending on the rare earth ionic size. In the case of small-sized rare earths (R = Ho–Lu, Y), it was demonstrated that the symmetry of the lattice varies from orthorhombic (Pbnm) to monoclinic (
P21/n) at TIM (Fernández-Díaz et al., 2001
; Kobayashi et al., 2015
; Massa et al., 2015
; Alonso et al., 2000
; Muñoz et al., 2009
) to produce two chemically and crystallographically distinct Ni sites in the insulating regime, whereas the parent compound LaNiO3 is metallic and rhombohedral over its entire temperature range. For Pr and Nd, the IM transition coincides with the antiferromagnetic ordering temperature , whereas for the medium-sized rare earths (R = Sm–Dy)
and
are different.
Among all the nickelates RNiO3, PrNiO3 occupies a unique position. It hosts all three archetypal perovskite structures (
P21/n, Pbnm and ) accessible via temperature tuning. Remarkably, PrNiO3 exhibits a simultaneous insulator–metal and antiferromagnetic transition at ∼130 K (
), coinciding with a monoclinic to orthorhombic symmetry change, and an unusual increase in unit-cell volume upon cooling. Such a transition is believed to be stabilized by charge disproportionation, being a phonon-mediated mechanism that could potentially suppress Jahn–Teller effects. However, the interplay between lattice dynamics and electronic ordering remains poorly understood. The temperature-induced Pbnm to
phase transition also remains largely uncharacterized, occurring in the metallic state of PrNiO3 above 750 K (Rodrigues et al., 2024
).
The phase transition
P21/n to Pbnm, which is simultaneously observed upon the metallization of Ni perovskites upon warming, has been analyzed in terms of symmetry-adapted distortion modes (Gawryluk et al., 2019
). This analysis allowed identification of the contribution of the different symmetry modes to the global distortion over a broad temperature range (Perez-Mato et al., 2010a
). Moreover, it showed that the structural changes at the metal-to-insulator (MI) transition, traditionally described in terms of the evolution of the interatomic distances and angles, appear as abrupt increases of all non-zero mode amplitudes at =
≃ 130 K, accompanied by the appearance of new modes below this temperature. These observations suggest the existence of a hidden symmetry in the insulating phase, which might be due to the theoretically predicted existence of polar distortions induced by the non-centrosymmetric magnetic order (Giovannetti et al., 2009
; Perez-Mato et al., 2016
). However, the underlying mechanisms of the Pbnm to transition have not previously been analyzed using symmetry-adapted distortion modes. This is partly since the high-quality structural data necessary for this analysis have only recently become available for PrNiO3 through the recent work of our group (Rodrigues et al., 2024
).
In this paper, we revisit the evolution of distortion modes across the structural phase transitions of PrNiO3 nickelate, mainly addressing the metal–metal transition (Pbnm to ). A ceramic sample was prepared at 3.5 GPa under in situ O2 pressure provided by the decomposition of KClO3, yielding a material with a crystallinity which exceeds those currently prepared at 200 bar O2 pressure (Gainza et al., 2021
). The transition sequence monoclinic (
P21/n) → orthorhombic (Pbnm) → rhombohedral () was identified in our specimen, examined with high-resolution synchrotron X-ray diffraction data (SXRD) and symmetry-adapted distortion-mode analysis.
2. Methods and notation
2.1. Experimental techniques
High-quality PrNiO3 powder was synthesized via high-pressure solid-state reaction (Gainza et al., 2021
). Stoichiometric amounts of Pr6O11 and Ni(OH)2 were mixed with 30 wt% KClO4, which generates in situ oxygen to oxidize Ni to the 3+ state. The mixture was sealed in a 5 mm diameter gold capsule, placed in a graphite heater and treated in a Rockland Research piston-cylinder press at 3.5 GPa and 1073 K for 30 min, and then quenched to room temperature. Residual KCl and unreacted oxides were removed by washing in dilute HNO3.
High-angular-resolution temperature-dependent SXRD measurements (λ = 0.35418 Å) were carried out on beamline ID22 (Fitch et al., 2023
) at the ESRF using a Dectris EIGER2 X 2M-W CdTe detector in position-sensitive mode, covering a 2θ range of 1–40° with an angular resolution of 0.002°. PrNiO3 powder was placed into a 0.5 mm diameter quartz capillary and continuously rotated to minimize orientation effects. The temperature dataset was collected in the range between 10 and 900 K with 10 min equilibration per point (Rodrigues et al., 2024
) using a Dynaflow cryostat (T < 300 K) and hot blower system (T > 300 K). The setup enabled precise tracking of diffraction peak splitting and distortion linked to structural transitions.
The SXRD data were analyzed by Rietveld refinement using the FullProf program (Rodríguez-Carvajal, 1993
), with a pseudo-Voigt function employed to model the peak profiles. The refined parameters included scale factors, zero-point offset, background coefficients, asymmetry corrections, lattice constants, atomic positions, site occupancies and isotropic displacement parameters.
2.2. Notation
Understanding a material's properties often relies on its electronic and phonon band structures, which are mapped within the first Brillouin zone (BZ). For a simple cubic lattice, key high-symmetry points within this reciprocal-space unit cell are crucial, namely , X, M and R. The
point sits at the BZ center (0, 0, 0). The X point at (½, 0, 0) denotes the center of a BZ face. The M point at (½, ½, 0) is found at the center of a BZ edge. The R point at (½, ½, ½) defines a BZ corner.
In Glazer's notation, a general symbol () represents the tilt magnitudes along the pseudo-cubic directions x, y and z, respectively. The superscript # may have three values to describe no tilt (#, 0) and in-phase (#, +) and out-of-phase (#, −) octahedral tilting of the neighboring octahedral layers (Glazer, 1972
, 1975
). For instance, the aristotype unit cell has the Glazer symbol (), while (
) denotes out-of-phase tilts of equal magnitude along all the pseudo-cubic axes.
3. Structural transitions in PrNiO3
3.1. Summary of structural analysis
PrNiO3 undergoes a sequence of structural transitions driven by temperature and pressure. Below ∼130 K it adopts a monoclinic
P21/n structure with charge disproportionation and antiferromagnetic order. As the temperature increases, it transitions to an orthorhombic Pbnm phase around 130 K, coinciding with a metal–insulator transition and the collapse of Ni site splitting. Above ∼700 K, PrNiO3 enters a rhombohedral phase, associated with increased orbital overlap and metallic behavior. Similar transitions occur under pressure, with orthorhombic–rhombohedral coexistence between 6 and 12 GPa (Rodrigues et al., 2024
; Zhou et al., 2004
). Table 1
details the experimental conditions and reported transition temperatures for PrNiO3.
|
In Fig. 1
, we present representative SXRD patterns and corresponding Rietveld refinements of the three mentioned PrNiO3 structures that occur in the temperature interval of 10–900 K at ambient pressure. A characteristic feature of the monoclinic phase is the diffraction peak doublet (224 and 224 reflections) at around 15.1° (2θ) [inset of Fig. 1
(a)]. The occurrence of this doublet is linked to the charge disproportionation on Ni sites, and thus to the generation of two distinct crystallographic Ni sites with different charges (Ni13+δ and Ni23−δ). This doublet is not observed in the orthorhombic phase or for temperatures above [inset of Fig. 1
(b)]. In the orthorhombic lattice, the charge disproportionation on the Ni site collapses, resulting in a single Ni site with a uniform valence of 3+. Above 700 K, we found that a high-symmetry phase with a rhombohedral lattice is stabilized, as attested by the disappearance of the orthorhombic characteristic peaks [Fig. 1
(c)]. All the refined parameters for the three phases are listed in Tables S1–S3 in the supporting information.
|
Figure 1
Typical high-angular-resolution SXRD profiles for PrNiO3 (red open circles) and corresponding Rietveld refinements (black lines) at (a) 10 K for the P21/n (monoclinic) phase, (b) 295 K for the Pbnm (orthorhombic) phase and (c) 900 K for the |
3.2. Distortion-mode analysis across the phase transitions
To better understand the mechanism of the phase transitions in PrNiO3, we used symmetry-mode analysis (also known as distortion-mode analysis). We computed the amplitudes and polarization vectors of the symmetry-adapted modes for the low-symmetry distorted phase (subgroup H) with respect to the high-symmetry phase (aristotype, supergroup G) using the Amplimodes algorithm available at the Bilbao Crystallographic Server (Perez-Mato et al., 2010a
; Aroyo et al., 2006
; Perez-Mato et al., 2010b
). Because the structural transitions in PrNiO3 exhibit group–subgroup relations between low-symmetry (i.e.
P21/n, Pbnm and ) and high-symmetry structures, the low-symmetry distorted unit cell can be written as `frozen' modes using irreducible representations (here referred to as irreps) of the high-symmetry space group. The high-symmetry unit cell can be hypothetical (or virtual). Here, we choose the aristotype space group (
), which does not present any structural distortion, such as octahedral rotation, cationic displacement or orbital ordering (Glazer, 1972
). The initial point of the analysis consists of writing the atomic positions of the low-symmetry phases (r; subgroup H) with respect to the atomic positions of the aristotype (r0; supergroup G), being the last ones described in the unit-cell basis of the subgroup H, as follows:
where stands for distinct elements within the asymmetric unit and i ranges from 1 to
(number of atoms). For the description of the structural evolution, the displacement vectors
are linearly decomposed in terms of the basis vectors of the irreps obtained from the group–subgroup analysis as follows:
where denotes the polarization vector (or basis vector) of the irrep
and m the possible independent modes for each
, while the amplitude
denotes the distortion magnitude of each distortion mode. A rough estimation of the uncertainty in the distortion amplitudes
, considering typical errors of ∼10−5 in both atomic positions (x, y, z) and lattice parameters (a, b, c), gives
, i.e. essentially of the order of ∼10−5 per unit-norm mode vector, with an increase of only a few percent from the lattice parameter contributions.
To perform the symmetry-mode decomposition, we used the experimentally determined structures defined in
P21/n, Pbnm and space groups, as reported by Rodrigues et al. (2024
), constituting the subgroup H, while the high-symmetry supergroup G contains the unit cell . For this high symmetry, we took the virtual aristotype cubic structure belonging to space group
(No. 221), where Pr is located on 1b (½, ½, ½), Ni on 1a (0, 0, 0) and O on 3d (½, 0, 0). The irreps are labeled using the k vector designation in the first BZ of the cubic unit cell, i.e.
, X, M and R. Since Ni is at the origin of the aristotype unit cell, we shifted the atomic coordinates in both monoclinic and orthorhombic lattices to have at least one Ni at the origin. Prior to the group-theory calculations, both monoclinic and orthorhombic lattices were converted to their respective standard sets,
P21/c and Pnma, respectively, using the CIF2Standard tool (Kroumova et al., 2003
). The decomposition to represent the low-symmetry phases using the irreps of the supergroup G () space group leads to the Wyckoff site splitting in Table 2
. The symmetry-mode amplitudes are listed in Table 3
. On the basis of such a splitting description, the number and symmetry vectors of the distortion modes can be calculated for each distorted phase.
|
||||||||||||||||||||||||||||||||||||||||||||||||||
|
||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
We started the symmetry-mode analysis from the rhombohedral phase, for which the static displacements for the aristotype symmetry lowering come from one frozen mode along the direction [111], wavevector k = (½, ½, ½), of the pseudo-cubic unit cell. It results from an out-of-phase octahedral [NiO6] tilt with Glazer's symbol (
) [see the mode representation in Fig. 2
(c)]. The irrep
R4+ shows precisely the out-of-phase tilt along the c direction of the hexagonal cell, i.e. parallel to the pseudo-cubic direction [111]. The tilts lead to trigonal distortion of the rhombohedral phase and an additional degree of freedom for the oxygen fractional coordinate on 18e sites (x, 0, ¼) compared with the aristotype unit cell (Table 2
).
|
Figure 2
Schematic representation of the atomic displacements (polarization vectors) of symmetry-adapted modes for describing the symmetry-lowering transitions (a) |
In the orthorhombic phase, more degrees of freedom are enabled due to the Wyckoff site splitting resulting from seven distortion modes, as represented by five irreps, namely
R4+,
R5+,
M2+,
M3+ and
X5+ in Table 2
. Pr site 1b enables two distortion modes [ +
] on Pr site 4c within the orthorhombic lattice. Their respective polarization vectors are mainly described by Pr translations along the a and b axes, respectively [Fig. 2
(b)]. The oxygen 3d site splitting leads to five modes [ +
+
+
+
] on O sites 4c and 8d of the Pbnm phase. From the symmetry-mode amplitudes in Table 3
, we note that the orthorhombic distortion is mainly induced by the modes
R4+ (0.529 Å) and
M3+ (0.334 Å) which describe the out-of-phase () and in-phase (
) rotations of neighboring octahedra, respectively, to account for the Glazer symbol
of the orthorhombic lattice. The polarization vectors of the distortion mode
M2+ mimic an asymmetric octahedral stretching confined to the ab plane but exhibiting a low amplitude of 0.013 Å, and therefore having less impact on the global orthorhombic distortion and showing the minor role of any possible orbital ordering (Zhou & Goodenough, 2004
; Mazin et al., 2007
).
In the monoclinic phase, 12 distortion modes as written by eight irreps, namely
R1+,
R3+,
R4+,
R5+,
M2+,
M3+,
M5+ and
X5+ in Table 2
, are allowed. In addition to the irreps from the orthorhombic distortion, four more [,
,
and
] are needed to account for the charge disproportionation and, consequently, the charge ordering at long range of the monoclinic phase. In Fig. 2
(a), we see that the
M5+ mode is an additional rotation of adjacent octahedra that accounts for the Glazer symbol of the monoclinic unit cell. The polarization vectors of
R1+ and
R3+ describe symmetric and asymmetric octahedral stretching modes with quite similar amplitudes of 0.062 and 0.042 Å, respectively, meaning that the charge disproportion below
may be driven by oxygen stretching (breathing) modes. The asymmetric stretching is also known as Jahn–Teller-type mode because it distorts the octahedral cage to induce apical and basal oxygen splitting. Consequently, the charge transfer 2Ni3+ → Ni13+δ + Ni23−δ can be thought of as a phonon-mediated process, the oxygen stretching modes being essential to its progress.
Using the temperature-dependent crystal structure of PrNiO3 in the broad range 10–900 K, we have analyzed the evolution of the symmetry-mode amplitudes across the phase transitions in the temperature range 10–900 K, as plotted in Fig. 3
. The amplitudes are normalized with respect to the primitive unit cell of the aristotype cubic cell. All the mode amplitudes vanish for temperatures above 700 K except for
R4+, which is the sole mode for describing the rhombohedral distortion along the pseudo-cubic direction [111]. Below 700 K, the highest-amplitude modes
R4+ and
M3+ show a nearly temperature-independent behavior, with slight anomalies at possibly induced by the
M5+ mode which also rotates the adjacent octahedral layers toward the monoclinic distortion. The mode amplitudes encompassing Pr atoms [
R5+ and
X5+] enhance the distortion when the temperature decreases and
R5+ has a subtle change near
. Interesting trends can be observed for the stretching modes
R1+,
R3+ and
M2+, in view of their pronounced jumps at the onset of the insulator–metal transition.
|
Figure 3
Temperature dependence of the symmetry-mode amplitudes across the transitions |
In our previous work (Rodrigues et al., 2023
), we found strong evidence for spin–phonon coupling below in PrNiO3 using X-ray absorption spectroscopy. The Debye–Waller exponent of the Ni—O pair bond indicated a softening behavior below the IM transition, attributed to the coupling of the Ni magnetic lattice and the stretching vibrational modes of the nickel octahedra. On the basis of the analysis presented here, we can now say that charge disproportionation is mediated by oxygen stretching modes, a hypothesis that was also raised recently (Gawryluk et al., 2019
). Our results demonstrate that both charge transfer and magnetic ordering are intimately entangled with phonon-mediated processes.
4. Conclusions
Our study presents a full symmetry-mode decomposition analysis of PrNiO3 across its temperature-induced structural phase transitions, enabled by high-quality and high-resolution SXRD data collected between 10 and 900 K. We identify oxygen stretching and Jahn–Teller-like modes as the primary drivers of charge disproportionation at ∼130 K (metal–insulator transition) and show that these distortions persist and evolve through the high-temperature orthorhombic to rhombohedral transition. The transition to the phase is characterized by the disappearance of all modes except a single octahedral [NiO6] tilt.
These results establish that phonon-mediated lattice distortions not only drive electronic and magnetic transitions but also govern structural evolution in both insulating and metallic states, offering a unified framework to understand phase competition in electron-correlated nickelates.
Supporting information
Additional tables with structural parameters. DOI: https://doi.org/10.1107/S1600576725009380/hat5010sup1.pdf
Funding information
The following funding is acknowledged: Ministerio de Ciencia, Innovación y Universidades (grant No. PID2021-122477OB-I00).
References
Acosta-Alejandro, M., de León, J. M., Medarde, M., Lacorre, P., Konder, K. & Montano, P. A. (2008). Phys. Rev. B 77, 085107.
Google Scholar
Alonso, J., Martínez-Lope, M., Casais, M., García-Muñoz, J. & Fernández-Díaz, M. T. (2000). Phys. Rev. B 61, 1756–1763.
CrossRef
ICSD
CAS
Google Scholar
Aroyo, M. I., Perez-Mato, J. M., Capillas, C., Kroumova, E., Ivantchev, S., Madariaga, G., Kirov, A. & Wondratschek, H. (2006). Z. Kristallogr. Cryst. Mater. 221, 15–27.
Web of Science
CrossRef
CAS
Google Scholar
Catalan, G. (2008). Phase Transit. 81, 729–749.
CrossRef
CAS
Google Scholar
Catalano, S., Gibert, M., Fowlie, J., Íñiguez, J., Triscone, J.-M. & Kreisel, J. (2018). Rep. Prog. Phys. 81, 046501.
CrossRef
PubMed
Google Scholar
Demazeau, G., Marbeuf, A., Pouchard, M. & Hagenmuller, P. (1971). J. Solid State Chem. 3, 582–589.
CrossRef
ICSD
CAS
Google Scholar
Fernández-Díaz, M. T., Alonso, J. A., Martínez-Lope, M. J., Casais, M. T. & García-Muñoz, J. L. (2001). Phys. Rev. B 64, 144417.
Google Scholar
Fitch, A., Dejoie, C., Covacci, E., Confalonieri, G., Grendal, O., Claustre, L., Guillou, P., Kieffer, J., de Nolf, W., Petitdemange, S., Ruat, M. & Watier, Y. (2023). J. Synchrotron Rad. 30, 1003–1012.
Web of Science
CrossRef
CAS
IUCr Journals
Google Scholar
Gainza, J., Serrano-Sánchez, F., Rodrigues, J. E. F. S., Nemes, N. M., Martínez, J. L. & Alonso, J. A. (2021). Materials 14, 1946.
CrossRef
PubMed
Google Scholar
García-Muñoz, J. L., Rodríguez-Carvajal, J., Lacorre, P. & Torrance, J. B. (1992). Phys. Rev. B 46, 4414–4425.
Google Scholar
Gawryluk, D. J., Klein, Y. M., Shang, T., Sheptyakov, D., Keller, L., Casati, N., Lacorre, P., Fernández-Díaz, M. T., Rodríguez-Carvajal, J. & Medarde, M. (2019). Phys. Rev. B 100, 205137.
CrossRef
Google Scholar
Giovannetti, G., Kumar, S., Khomskii, D., Picozzi, S. & van den Brink, J. (2009). Phys. Rev. Lett. 103, 156401.
CrossRef
PubMed
Google Scholar
Glazer, A. M. (1972). Acta Cryst. B28, 3384–3392.
CrossRef
CAS
IUCr Journals
Web of Science
Google Scholar
Glazer, A. M. (1975). Acta Cryst. A31, 756–762.
CrossRef
CAS
IUCr Journals
Web of Science
Google Scholar
Huang, T. C., Parrish, W., Toraya, H., Lacorre, P. & Torrance, J. B. (1990). Mater. Res. Bull. 25, 1091–1098.
CrossRef
ICSD
CAS
Google Scholar
Jaramillo, R., Ha, S. D., Silevitch, D. M. & Ramanathan, S. (2014). Nat. Phys. 10, 304–307.
CrossRef
CAS
Google Scholar
Junita, J., Jayalakshmi, D. & Rodney, J. D. (2022). Int. J. Hydrogen Energy 47, 30602–30612.
Google Scholar
Klein, Y. M., Kozłowski, M., Linden, A., Lacorre, P., Medarde, M. & Gawryluk, D. J. (2021). Cryst. Growth Des. 21, 4230–4241.
Web of Science
CrossRef
ICSD
CAS
Google Scholar
Kobayashi, H., Ikeda, S., Yoda, Y., Hirao, N., Ohishi, Y., Alonso, J. A., Martinez-Lope, M. J., Lengsdorf, R., Khomskii, D. I. & Abd-Elmeguid, M. M. (2015). Phys. Rev. B 91, 195148.
CrossRef
Google Scholar
Kroumova, E., Aroyo, M. I., Perez-Mato, J. M., Kirov, A., Capillas, C., Ivantchev, S. & Wondratschek, H. (2003). Phase Transit. 76, 155–170.
Web of Science
CrossRef
CAS
Google Scholar
Massa, N. E., Ramos, A. Y., Tolentino, H. C. N., Sousa-Neto, N. M., Fonseca, J. & Alonso, J. A. (2015). Mater. Res. Expr. 2, 126301.
CrossRef
Google Scholar
Mazin, I. I., Khomskii, D. I., Lengsdorf, R., Alonso, J. A., Marshall, W. G., Ibberson, R. M., Podlesnyak, A., Martínez-Lope, M. J. & Abd-Elmeguid, M. M. (2007). Phys. Rev. Lett. 98, 176406.
CrossRef
Google Scholar
Medarde, M., Fernández-Díaz, M. T. & Lacorre, P. (2008). Phys. Rev. B 78, 212101.
CrossRef
Google Scholar
Medarde, M., Fontaine, A., García-Muñoz, J. L., Rodríguez-Carvajal, J., de Santis, M., Sacchi, M., Rossi, G. & Lacorre, P. (1992). Phys. Rev. B 46, 14975–14984.
CrossRef
CAS
Google Scholar
Medarde, M., Lacorre, P., Conder, K., Rodríguez-Carvajal, J., Rosenkranz, S., Fauth, F. & Furrer, A. (1997). Physica B 241–243, 751–757.
CrossRef
CAS
Google Scholar
Medarde, M. L. (1997). J. Phys. Condens. Matter 9, 1679–1707.
CrossRef
CAS
Google Scholar
Muñoz, A., Alonso, J. A., Martínez-Lope, M. J. & Fernández-Díaz, M. T. (2009). J. Solid State Chem. 182, 1982–1989.
Google Scholar
Pandiyan, R., Vinothkumar, V., Chen, S.-M., Prasad, G. V. & Kim, T. H. (2023). Surf. Interfaces 38, 102805.
CrossRef
Google Scholar
Perez-Mato, J. M., Gallego, S. V., Elcoro, L., Tasci, E. & Aroyo, M. I. (2016). J. Phys. Condens. Matter 28, 286001.
PubMed
Google Scholar
Perez-Mato, J. M., Orobengoa, D. & Aroyo, M. I. (2010a). Acta Cryst. A66, 558–590.
CrossRef
IUCr Journals
Google Scholar
Perez-Mato, J. M., Orobengoa, D., Aroyo, M. I. & Elcoro, L. (2010b). J. Phys. Conf. Ser. 226, 012011.
Google Scholar
Retuerto, M., Pereira, A. G., Pérez-Alonso, F. J., Peña, M. A., Fierro, J. L. G., Alonso, J. A., Fernández-Díaz, M. T., Pascual, L. & Rojas, S. (2017). Appl. Catal. Environ. 203, 363–371.
CrossRef
CAS
Google Scholar
Rodrigues, J. E., Rosa, A. D., Gainza, J., Silva, R. S., Mijit, E., Garbarino, G., Irifune, T., Shinmei, T., Dejoie, C., Nemes, N. M., Martínez, J. L., Mezouar, M., Alonso, J. A. & Mathon, O. (2024). Chem. Mater. 36, 596–608.
CrossRef
ICSD
CAS
Google Scholar
Rodrigues, J. E., Rosa, A. D., López-Sánchez, J., Sebastiani-Tofano, E., Nemes, N. M., Martínez, J. L., Alonso, J. A. & Mathon, O. (2023). J. Mater. Chem. C 11, 462–471.
CrossRef
CAS
Google Scholar
Rodríguez-Carvajal, J. (1993). Phys. B 192, 55–69.
Google Scholar
Tomioka, Y., Ito, T., Maruyama, E., Kimura, S. & Shindo, I. (2021). J. Phys. Soc. Jpn 90, 034704.
CrossRef
Google Scholar
Wang, C., Chang, C.-H., Huang, A., Wang, P.-C., Wu, P.-C., Yang, L., Xu, C., Pandey, P., Zeng, M., Böttger, R., Jeng, H.-T., Zeng, Y.-J., Helm, M., Chu, Y.-H., Ganesh, R. & Zhou, S. (2019). Phys. Rev. Mater. 3, 053801.
CrossRef
Google Scholar
Xin, C., Sun, Z., Yuan, B., Wei, Z., Li, H., Hu, Z. & Jin, G. (2020). J. Alloys Compd. 815, 152351.
CrossRef
ICSD
Google Scholar
Zhou, J. & Goodenough, J. B. (2004). Phys. Rev. B 69, 153105.
Google Scholar
Zhou, J., Goodenough, J. B. & Dabrowski, B. (2004). Phys. Rev. B 70, 081102.
Google Scholar
This is an open-access article distributed under the terms of the Creative Commons Attribution (CC-BY) Licence, which permits unrestricted use, distribution, and reproduction in any medium, provided the original authors and source are cited.
access
journal menu



