research papers\(\def\hfill{\hskip 5em}\def\hfil{\hskip 3em}\def\eqno#1{\hfil {#1}}\)

Journal logoSTRUCTURAL SCIENCE
CRYSTAL ENGINEERING
MATERIALS
ISSN: 2052-5206

The varying temperature- and pressure-induced phase transition pathways in hybrid improper ferroelectric Sr3Sn2O7

crossmark logo

aDepartment of Chemistry, University of Warwick, Gibbet Hill, Coventry, CV4 7AL, United Kingdom, bDepartment of Physics, University of Warwick, Gibbet Hill, Coventry, CV4 7AL, United Kingdom, cKeck Center for Quantum Magnetism, Rutgers University, Piscataway, New Jersey, 07928, USA, and dDiamond Light Source Ltd, Harwell Science and Innovation Campus, Didcot, OX11 0DE, United Kingdom
*Correspondence e-mail: m.senn@warwick.ac.uk

Edited by O. V. Yakubovich, Moscow State University, Russian Federation (Received 5 February 2025; accepted 14 March 2025; online 14 April 2025)

A variable-temperature and pressure single-crystal diffraction study of hybrid improper ferroelectric Sr3Sn2O7 is reported. In combination with symmetry analysis, we reveal that the application of pressure and temperature induce distinct phase transition pathways, driven by a differing response of the octahedral rotations to these stimuli. Contrary to what has been previously predicted, we observe the ferroelectric to paraelectric phase transition between 10.17(18) and 12.13(14) GPa, meaning the hybrid improper ferroelectric phase remains stable to significantly higher pressures than expected.

1. Introduction

Ferroelectric materials, which display a spontaneous electrical polarization that is reversible by an external electric field, are fundamental to many technological applications such as non-volatile memory and sensing devices (Scott, 2007[Scott, J. F. (2007). Science, 315, 954-959.]). Polarization in conventional proper ferroelectrics like BaTiO3 and Pb(Zr/Ti)O3 arises through a single primary lattice distortion/instability. However, hybrid improper ferroelectrics (HIFs) have recently emerged as an intriguing alternative (Benedek & Fennie, 2011[Benedek, N. A. & Fennie, C. J. (2011). Phys. Rev. Lett. 106, 107204.]; Bousquet et al., 2008[Bousquet, E., Dawber, M., Stucki, N., Lichtensteiger, C., Hermet, P., Gariglio, S., Triscone, J.-M. & Ghosez, P. (2008). Nature, 452, 732-736.]; Oh et al., 2015[Oh, Y. S., Luo, X., Huang, F.-T., Wang, Y. & Cheong, S.-W. (2015). Nat. Mater. 14, 407-413.]). In these materials, polarization arises indirectly as a result of a trilinear coupling mechanism between two non-polar structural distortions and a polar mode, generating an overall polar structure. This expands the range of materials that can exhibit ferroelectricity and, additionally, negates the strict chemical requirements that often restrict proper ferroelectrics from becoming multiferroic. Hybrid improper ferroelectricity is prototypical to layered perovskites, such as Ruddlesden–Popper (RP) perovskites which have a structure consisting of n perovskite layers intercalated with a rock-salt-like layer. Here, the two non-polar structural distortions are the tilting and rotation of the oxygen octahedra, highlighted in Fig. 1[link]. This mechanism, where polarization is a secondary rather than primary order parameter, can provide a rich platform for manipulating polarization through the interplay of structural degrees of freedom.

[Figure 1]
Figure 1
(a) Relationship between the phases generated from the I4/mmm aristotype through combinations of the [{\rm X}_{2}^{+}], [{\rm X}_{1}^{-}] and [{\rm X}_{3}^{-}] irreps. (b) Rotation and tilting of SnO6 octahedra, highlighting the hybrid improper coupling of the octahedral distortions, [{\rm X}_{2}^{+}] and [{\rm X}_{3}^{-}] to the polar mode, Γ[{}_{5}^{-}] in A21am, and, similarly, the trilinear coupling between [{\rm X}_{3}^{-}], [{\rm X}_{1}^{-}] and the antiferroelectric mode, [{\rm M}_{5}^{+}] in Pnab. (c) Crystal structures of the phases of Sr3Sn2O7 that have been experimentally observed by temperature (Yoshida et al., 2018[Ablitt, C., Craddock, S., Senn, M. S., Mostofi, A. A. & Bristowe, N. C. (2017). npj Comput. Mater. 3, 44.]) and pressure, showing the different order parameter directions. Sr displacements are indicated by blue and red arrows with crosses indicating no displacement. This results in an antiferroelectric distortion ([{\rm M}_{5}^{+}]) for Pnab and a polar distortion (Γ[{}_{5}^{-}]) for A21am.

External stimuli such as temperature and pressure can be utilized to directly control the structural distortions which allows for exploration of the ferroelectric mechanism with a view to how the structure may be adapted to tune the ferroelectric character of HIFs for technological use. Variable-temperature studies on n = 2 RP phases (RP2) (Senn et al., 2015[Senn, M., Bombardi, A., Murray, C., Vecchini, C., Scherillo, A., Luo, X. & Cheong, S. (2015). Phys. Rev. Lett. 114, 035701.]; Kratochvilova et al., 2019[Kratochvilova, M., Huang, F.-T., Diaz, M. F., Klicpera, M., Day, S. J., Thompson, S. P., Oh, Y.-S., Gao, B., Cheong, S.-W. & Park, J.-G. (2019). J. Appl. Phys. 125, 244102.]; Yoshida et al., 2018[Yoshida, S., Akamatsu, H., Tsuji, R., Hernandez, O., Padmanabhan, H., Sen Gupta, A., Gibbs, A. S., Mibu, K., Murai, S., Rondinelli, J. M., Gopalan, V., Tanaka, K. & Fujita, K. (2018). J. Am. Chem. Soc. 140, 15690-15700.]; Pomiro et al., 2020[Pomiro, F., Ablitt, C., Bristowe, N. C., Mostofi, A. A., Won, C., Cheong, S.-W. & Senn, M. S. (2020). Phys. Rev. B, 102, 014101.]) have shown that numerous phases are accessible through different combinations of octahedral distortions, where phases with a lower tolerance factor tend to have a greater degree of octahedral rotations and tilting. Whilst it is typically understood that hydrostatic pressure suppresses polarization in proper ferroelectrics (Ishidate et al., 1997[Ishidate, T., Abe, S., Takahashi, H. & Môri, N. (1997). Phys. Rev. Lett. 78, 2397-2400.]; Bousquet & Ghosez, 2006[Bousquet, E. & Ghosez, P. (2006). Phys. Rev. B, 74, 180101.]), in HIFs pressure can, instead, act to enhance polarization. Additionally, we have recently demonstrated by a combined experimental high-pressure powder X-ray diffraction and density functional theory (DFT) study that, for Ca3Ti2O7 (Clarke et al., 2024[Clarke, G., Daisenberger, D., Luo, X., Cheong, S. W., Bristowe, N. C. & Senn, M. S. (2024). Phys. Rev. B, 109, 094107.]), the amplitude of the octahedral rotations is increased by external pressure which, in turn, enhances the polarization by the trilinear coupling mechanism.

Sr3Sn2O7 is a desirable candidate for the technological realization of HIFs as it is ferroelectric at room temperature and exhibits a small polarization switching field (Xu et al., 2020[Xu, X., Wang, Y., Huang, F.-T., Du, K., Nowadnick, E. A. & Cheong, S.-W. (2020). Adv. Funct. Mater. 30, 2003623.]). The temperature-induced phase transitions of Sr3Sn2O7 have been previously studied by X-ray and powder neutron diffraction which revealed a complex series of phase transitions from the polar ground state A21am phase to a non-polar Pnab phase at 410 K, with subsequent transitions to Acaa and I4/mmm at around 700 and 900 K, respectively (Yoshida et al., 2018[Yoshida, S., Akamatsu, H., Tsuji, R., Hernandez, O., Padmanabhan, H., Sen Gupta, A., Gibbs, A. S., Mibu, K., Murai, S., Rondinelli, J. M., Gopalan, V., Tanaka, K. & Fujita, K. (2018). J. Am. Chem. Soc. 140, 15690-15700.]). Another study (Smith et al., 2021[Smith, K. A., Ramkumar, S. P., Harms, N. C., Clune, A. J., Xu, X., Cheong, S.-W., Liu, Z., Nowadnick, E. A. & Musfeldt, J. L. (2021). Phys. Rev. B, 104, 064106.]), using infrared spectroscopy (IR) and interpreted with the aid of DFT, suggested that the same sequence of phase transitions is induced by increasing pressure, with these transitions occurring at approximately 2, 15 and 18 GPa. It should be noted that this sequence is unique to Sr3Sn2O7.

The structural differences between these phases can be visualized as distortions acting on the tetragonal aristotype I4/mmm, as shown in Fig. 1[link]. The A21am phase arises as a consequence of the hybrid improper mechanism whereby an in-phase rotation and an out-of-phase tilt of the SnO6 octahedra, transforming as irreducible representations [{\rm X}_{2}^{+}] (a; 0) and [{\rm X}_{3}^{-}] (b; 0), respectively, couple to a polar displacement with irrep Γ[{}_{5}^{-}]. The Pnab phase also exhibits a trilinear coupling term which instead arises due to the combination of the out-of-phase tilt, [{\rm X}_{3}^{-}] (a; 0), and an out-of-phase rotation, [{\rm X}_{1}^{-}] (0; b) with an antiferrodistortive displacement, [{\rm M}_{5}^{+}]. Despite the out-of-phase tilt, [{\rm X}_{3}^{-}], remaining in both phases, there is no pathway along which the [{\rm X}_{2}^{+}] transforms directly and continuously into [{\rm X}_{1}^{-}]. As such, this transition would be first-order, as there is no group–subgroup relationship. Finally, the Acaa phase only exhibits the out-of-phase rotation, [{\rm X}_{1}^{-}] (a; 0).

Although the pressure-dependent response of the octahedral distortions in Sr3Sn2O7 has been investigated previously by first principle calculations (Ramkumar & Nowadnick, 2021[Ramkumar, S. P. & Nowadnick, E. A. (2021). Phys. Rev. B, 104, 144105.]), it has not been directly investigated experimentally.

In this work, we investigate the evolution of the structure of Sr3Sn2O7 as a function of temperature and pressure. We perform variable-temperature single-crystal X-ray diffraction between 100 and 480 K, allowing us to access a phase transition from A21am to Pnab and confirming the previously published transition. We also undertake the first single-crystal high-pressure X-ray diffraction experiment at ambient temperature using a diamond anvil cell to achieve pressures up to 31 GPa. In contrast to the previously reported phase transitions from IR spectroscopy (Smith et al., 2021[Smith, K. A., Ramkumar, S. P., Harms, N. C., Clune, A. J., Xu, X., Cheong, S.-W., Liu, Z., Nowadnick, E. A. & Musfeldt, J. L. (2021). Phys. Rev. B, 104, 064106.]), we do not find evidence for a phase transition from A21am to Pnab. Instead, we observed a transition directly from A21am to Acaa at around 12 GPa with no further transition to I4/mmm up to the limit of our experiment. To investigate the response of the octahedral distortions to temperature and pressure, we utilize symmetry-adapted distortion analysis. Our results show clearly that while both increasing temperature and pressure act to suppress the amplitude of the octahedral tilting, [{\rm X}_{3}^{-}], the two physical control parameters produce an opposite response with respect to the octahedral rotations, [{\rm X}_{2}^{+}] and [{\rm X}_{1}^{-}], providing a likely explanation for the different phase transition pathways that are observed.

2. Methods

2.1. Sample growth

Single crystals of Sr3Sn2O7 were grown using a laser floating zone furnace, as described by Xu et al. (2020[Xu, X., Wang, Y., Huang, F.-T., Du, K., Nowadnick, E. A. & Cheong, S.-W. (2020). Adv. Funct. Mater. 30, 2003623.]).

2.2. Variable-temperature XRD

A polarized light microscope was used to select a crystal that did not possess rotated orthorhombic twin domains which was confirmed by routine in-house diffraction screening. Images showing orthorhombic twin domains are included in the supporting information (Fig. S1). The single crystal of dimensions 50 × 50 × 15 µm was mounted using Fomblin-Y on a Mitigen cryoloop. Variable-temperature single-crystal X-ray diffraction measurements were collected in Experimental Hutch 1 (EH1) at Beamline I19 of the Diamond Light Source using a wavelength of λ = 0.6889 Å (corresponding to a beam energy of approximately 18.0 keV). Measurements were collected on heating from 100 K to 480 K and on cooling from 480 K to 300 K.

Indexing, integration and refinalization were performed using CrysAlisPRO (Rigaku, 2023[Rigaku (2023). CrysAlisPro. Rigaku Oxford Diffraction, Yarnton, England.]). Data were reduced initially in P1 with no rejection conditions applied to eliminate any bias. The structure was initially solved for the 100 K collection in A21am using SHELXT (Sheldrick, 2015b[Sheldrick, G. M. (2015b). Acta Cryst. A71, 3-8.]) and subsequent temperatures by isomorphous replacement, each refined to convergence using SHELXL (Sheldrick, 2015a[Sheldrick, G. M. (2015a). Acta Cryst. C71, 3-8.]) implemented through Olex2 (Dolomanov et al., 2009[Dolomanov, O. V., Bourhis, L. J., Gildea, R. J., Howard, J. A. K. & Puschmann, H. (2009). J. Appl. Cryst. 42, 339-341.]). The presence of inversion twinning in the A21am phase was accounted for with the twin law, ([−1 0 0], [0 −1 0], [0 0 −1]) for which the batch scale factor (BASF) was refined to approximately 0.50.

Once a suitable model was established and the space group confirmed, data reduction was repeated with the appropriate symmetry expectations and the lattice parameters extracted.

2.3. High-pressure XRD

A single crystal of dimensions 50 × 30 × 15 µm was loaded into a LeToullec style four-pin membrane diamond anvil cell (DAC) equipped with Boehler-Almax anvils with 400 µm culets and a rhenium gasket which was preindented to 50 µm with a 250 µm diameter sample chamber spark eroded into the indent. Care was, again, taken to ensure that the sample did not possess orthorhombic twinning. Helium was used as a pressure transmitting medium to ensure the sample was compressed under hydrostatic conditions with a ruby sphere used as a pressure indicator, measured by fluorescence (Syassen, 2008[Syassen, K. (2008). High Pressure Res. 28, 75-126.]). Single-crystal X-ray diffraction measurements were performed using a four-axis Newport diffractometer equipped with a Dectris Eiger CdTe detector, operating at a wavelength of λ = 0.4859 Å (corresponding to a beam energy of approximately 25.5 keV), in Experimental Hutch 2 (EH2) at Beamline I19 of the Diamond Light Source. Measurements were taking at intervals from ambient pressure to 30.1 (2) GPa, as detailed in the results section below.

Data reduction followed similarly as for the variable-temperature data. As is typical in high-pressure experiments, the data are incomplete on account of the body of the DAC reducing the reciprocal space available. This is exacerbated by the cell having a decreased opening angle (φ/2 = 23°) to allow higher pressures to be reached, while the c axis is particularly poorly defined on account of the orientation of the plate-like crystal within the DAC and a high mosaicity observed along c. Suitable models were identified based on the variable-temperature study and other common distorted RP2 structures (A21am, Pnab, Acaa, P4/nbm and I4/mmm) and generated using ISODISTORT. Each model was tested by refining to convergence using SHELXL, implemented through Olex2.

The distances between apical oxygens and Sn (O–Sn–O) were restrained to be similar with an e.s.d. of 0.2 Å to maintain chemical and physical sensibility of the model. Atomic displacement parameters were refined isotropically, with oxygens restrained to be similar. These restraints were necessary to obtain self-consistent, physically sensible, fully converged refinements for the final models.

3. Results

3.1. Variable-temperature XRD

Single-crystal X-ray diffraction data were collected on heating from 100 to 480 K and on cooling from 480 to 300 K. Within this temperature range, only the A21am and Pnab phases were accessible. Fig. 2[link] shows the temperature-dependent evolution of the lattice parameters, where a significant discontinuity is clear upon heating to above 400 K. A hysteresis of 10 K is observed for this transition between heating and cooling. We, therefore, confirm a first-order structural phase transition from A21am to Pnab, in agreement with previous work (Yoshida et al., 2018[Yoshida, S., Akamatsu, H., Tsuji, R., Hernandez, O., Padmanabhan, H., Sen Gupta, A., Gibbs, A. S., Mibu, K., Murai, S., Rondinelli, J. M., Gopalan, V., Tanaka, K. & Fujita, K. (2018). J. Am. Chem. Soc. 140, 15690-15700.]).

[Figure 2]
Figure 2
Lattice parameters as a function of temperature on heating and cooling. Blue and green backgrounds indicate the A21am and Pnab phases, respectively, with the region between 400 and 410 K showing hysteresis.

To further investigate and confirm the high-temperature phase as Pnab, we can assess the adherence to certain reflection conditions. Observation of super-structure reflections, given by k + l = odd, corresponding to the violation of A-centering would corroborate a change in centering. Fig. 3[link](a) shows that, from 100 to 400 K, there is negligible intensity in k + l = odd reflections and so A centering is indeed present. However, upon heating to 410 K, there is a clear change to P centering as intensity is generated for this class of reflections, similar to the classes corresponding to violation of B and C centering conditions.

[Figure 3]
Figure 3
(a) The sum of the squares of each hkl reflection where k + l, h + l, h + k = odd, normalized by k + l, h + l, h + k = even, respectively. Excluding reflections where h, k, l = 0. (b) Distortion mode amplitudes as a function of temperature with inset showing hybrid improper coupling in the A21am phase. Blue and green indicate the A21am and Pnab phases, respectively.

To explore the evolution of the atomic level structure, the structures were decomposed in terms of symmetry-adapted displacements using ISODISTORT (Campbell et al., 2006[Campbell, B. J., Stokes, H. T., Tanner, D. E. & Hatch, D. M. (2006). J. Appl. Cryst. 39, 607-614.]; Stokes et al., 2013[Stokes, H. T., Hatch, D. M. & Campbell, B. J. (2013). ISODISTORT, ISOTROPY Software Suite. https://iso.byu.edu.]), as shown in Fig. 3[link](b). The amplitude of the octahedral tilt, [{\rm X}_{3}^{-}], and rotation, [{\rm X}_{2}^{+}], both decrease steadily as a function of temperature. For HIFs, it is a specific prediction that the amplitude of the polar distortion should be linearly proportional to the product of the amplitude of the driving order parameters (Q) (Benedek & Fennie, 2011[Benedek, N. A. & Fennie, C. J. (2011). Phys. Rev. Lett. 106, 107204.]). To test the validity of the assumption that Sr3Sn2O7 is indeed strictly a HIF, we hence plot Q(Γ[{}_{5}^{-}]) against Q(X 2+)Q(X[_{3}^{-}]), shown in Fig. 3[link](b). A strong linear trend with an intercept close to zero is shown [y = 1.83 (14)x − 0.10 (3)], demonstrating that the polarization is driven directly by the octahedral rotations and tilts and that there is no appreciable proper contribution to the ferroelectric polarization. This is at odds to what has been observed for Ca3Ti2O7, where an appreciable proper contribution to the polarization is expected based on DFT calculations (Clarke et al., 2024[Clarke, G., Daisenberger, D., Luo, X., Cheong, S. W., Bristowe, N. C. & Senn, M. S. (2024). Phys. Rev. B, 109, 094107.]).

Above the phase transition temperature, the improper coupling to the polar distortions is necessarily turned off and replaced by a coupling to the antipolar displacements, [{\rm M}_{5}^{+}]. This coupling is shown in the supporting information (Fig. S2). The amplitudes of both [{\rm X}_{3}^{-}] and [{\rm X}_{1}^{-}] decrease steadily with increasing temperature, as to be expected as we approach the vicinity of the entropically stabilized undistorted I4/mmm aristotype.

3.2. High-pressure XRD

We collected high-pressure single-crystal X-ray diffraction data between ambient pressure and 30.1 (2) GPa. Fig. 4[link] shows how the a and b lattice parameters and volume evolve throughout this pressure range. In contrast to previous work using IR spectroscopy (Smith et al., 2021[Smith, K. A., Ramkumar, S. P., Harms, N. C., Clune, A. J., Xu, X., Cheong, S.-W., Liu, Z., Nowadnick, E. A. & Musfeldt, J. L. (2021). Phys. Rev. B, 104, 064106.]), there does not appear to be any evidence of a phase transition from A21am to Pnab at around 2 GPa that would manifest itself in a discontinuity in the lattice parameters. However, there is a large discontinuity at approximately 11 GPa.

[Figure 4]
Figure 4
Pressure dependence of the a and b lattice parameters and volume. Inset shows b/a lattice parameter ratio. Blue and pink backgrounds indicate A21am and Acaa phases, respectively. The first data point at 0 GPa was collected in cell but prior to gas-loading with He. Pressure error bars are smaller than size of markers.

To identify these phases, models were tested in A21am, Pnab, P4/nbm and Acaa (and I4/mmm for higher pressures). Between 0 and 10.17 (18) GPa, a structural model refined in A21am provides the best fit. The Pnab and P42/nbm models tested provided significantly worse fitting statistics or would not converge without additional constraints. Further details are provided in Tables S4–S6.

From 10.17 (18) to 30.1 (2) GPa, Acaa provides the most reasonable fit. The inset of Fig. 4[link] shows that there is a significant decrease in the degree of orthorhombicity as the b/a ratio decreases to values close to one in this pressure range. This has been demonstrated previously for the Acaa phase in the variable-temperature diffraction study (Yoshida et al., 2018[Yoshida, S., Akamatsu, H., Tsuji, R., Hernandez, O., Padmanabhan, H., Sen Gupta, A., Gibbs, A. S., Mibu, K., Murai, S., Rondinelli, J. M., Gopalan, V., Tanaka, K. & Fujita, K. (2018). J. Am. Chem. Soc. 140, 15690-15700.]).

In the region between 12.13 (14) and 13.20 (18) GPa, both the A21am and Acaa models converge successfully, which could indicate a region of phase coexistence. Interestingly, despite the fact that orthorhombic twinning is not present in the A21am phase, it appears in the Acaa phase. This provides further evidence that the phase transition is not continuous in either of the order parameters. As shown in Fig. 5[link], between 12.13 (14) and 13.20 (18) GPa, the twin fraction {refined via the BASF in SHELXL with the twin law ([0 1 0], [−1 0 0], [0 0 1])} refines to approximately 0.5, consistent with the same region where both A21am and Acaa models converge successfully. This twin fraction then increases to around 0.7 beyond this, corresponding to 30% of the A-centered domain [X[_{1}^{-}] (a; 0)] and 70% of the B-centered domain [X[_{1}^{-}] (0; a)]. This may occur to relieve strain in the Acaa phase but it may, instead, indicate that it is easier to nucleate the [{\rm X}_{1}^{-}] along (0; a) compared to (a; 0) to alleviate competition with the rotation (X 2+) in A21am.

[Figure 5]
Figure 5
Pressure-dependent evolution of BASF within the Acaa phase. Pressure error bars are smaller than size of markers.

To further investigate the evolution of the atomic structure under pressure, the ferroelectric phase was decomposed in terms of symmetric-adapted displacements, as shown in Fig. 6[link], using ISODISTORT and AMPLIMODES (Orobengoa et al., 2009[Orobengoa, D., Capillas, C., Aroyo, M. I. & Perez-Mato, J. M. (2009). J. Appl. Cryst. 42, 820-833.]; Perez-Mato et al., 2010[Perez-Mato, J. M., Orobengoa, D. & Aroyo, M. I. (2010). Acta Cryst. A66, 558-590.]). The noise and outliers in these data, which we attribute to the inherent complications of the high-pressure experiment, particularly the limited data completeness, illustrate the difficulty in refining the subtle structural distortions associated with the octahedral rotation and tilting that are dominated by oxygen displacements. However, the results still provide a useful upper and lower bound for what should be expected for the pressure-dependent evolution of the octahedral rotation and tilt modes. As the pressure increases, the amplitude of all modes remains relatively constant, exhibiting a shallow gradient with a confidence interval that encompasses both negative and positive values. This is broadly in line with computational predictions by Ramkumar & Nowadnick (2021[Ramkumar, S. P. & Nowadnick, E. A. (2021). Phys. Rev. B, 104, 144105.]) which shows a slight decrease in all distortions modes within the same 0 to 10 GPa pressure range. Regardless of the overall trends, the persistence of the polar mode, Γ[{}_{5}^{-}], indicates that the ferroelectric, A21am, is stable to much higher pressures than was previously inferred from the IR study.

[Figure 6]
Figure 6
Distortion mode amplitudes as a function of pressure for A21am phase, showing the rotation, [{\rm X}_{2}^{+}], and tilt, [{\rm X}_{3}^{-}], and polar, Γ[{}_{5}^{-}], modes. Darker and lighter markers indicate a lower and higher uncertainty, respectively. A weighted linear regression was performed based on errors generated through AMPLIMODES with shaded regions showing the confidence interval of one sigma.

Fig. 7[link] shows how the out-of-phase rotation, [{\rm X}_{1}^{-}], of the Acaa phase evolves above 10 GPa. The amplitude increases steadily and linearly with pressure, suggesting that the Acaa phase is continuing to be stabilized relative to the aristotype symmetry. Accordingly, we do not necessarily expect a further phase transition to the aristotype symmetry I4/mmm. From refinements, no transition from Acaa to I4/mmm was identified, even to the limit of our experiment at 30.1 (2) GPa.

[Figure 7]
Figure 7
Evolution of the out-of-phase rotation, [{\rm X}_{1}^{-}], as a function of pressure for Acaa phase. A weighted linear regression was performed based on errors generated from AMPLIMODES.

Compressibility parameters were calculated using PASCal (Cliffe & Goodwin, 2012[Cliffe, M. J. & Goodwin, A. L. (2012). J. Appl. Cryst. 45, 1321-1329.]) also provide evidence to this conclusion. These data are tabulated in the supporting information (Table S7). For both the A21am and Acaa phases, the c axis is more compressible than the a and b axes and, additionally, the c axis is more compressible in Acaa than in A21am. Together, this failure to recover the I4/mmm phase at high pressure is consistent with the observed uniaxial negative thermal expansion in isosymmetric RP2, Ca3Mn2O7, which we have found is related to the unusually high anisotropic compressibility mediated by the octahedral rotations in these phases (Senn et al., 2016[Senn, M. S., Murray, C. A., Luo, X., Wang, L., Huang, F.-T., Cheong, S.-W., Bombardi, A., Ablitt, C., Mostofi, A. A. & Bristowe, N. C. (2016). J. Am. Chem. Soc. 138, 5479-5482.]; Ablitt et al., 2017[Ablitt, C., Craddock, S., Senn, M. S., Mostofi, A. A. & Bristowe, N. C. (2017). npj Comput. Mater. 3, 44.]; Ablitt et al., 2018[Ablitt, C., Mostofi, A. A., Bristowe, N. C. & Senn, M. S. (2018). Front. Chem. 6, 455.]).

We find that our results do not follow the trend that the application of pressure induces the same sequence of phase transitions as with increasing temperature. The effect of pressure and temperature on the structural distortions in the ferroelectric, A21am, phase also differs slightly from each other. Whilst increasing temperature causes a distinct decrease in the tilting and rotation modes and, therefore, a decrease in the polar mode, the pressure-dependent trends are much more marginal. Compared to Ca3Ti2O7, where the amplitude of the rotation increases faster than the amplitude of the tilt decreases (Clarke et al., 2024[Clarke, G., Daisenberger, D., Luo, X., Cheong, S. W., Bristowe, N. C. & Senn, M. S. (2024). Phys. Rev. B, 109, 094107.]), this does not appear to be the case for Sr3Sn2O7.

Finally, we note that while our results appear to contradict the IR results (Smith et al., 2021[Smith, K. A., Ramkumar, S. P., Harms, N. C., Clune, A. J., Xu, X., Cheong, S.-W., Liu, Z., Nowadnick, E. A. & Musfeldt, J. L. (2021). Phys. Rev. B, 104, 064106.]), in the same study the authors report ground state DFT energies which appear to show that Acaa, not Pnab, is the stable high-pressure phase. The differences in the experimental phase transitions reported could be as a result of the pressure transmitting medium used. Although the exact hydrostatic limit of petroleum jelly, as used in the IR study, has not been previously reported, we speculate that it is much lower than 4 GPa, in line with the limits of similar media (Klotz et al., 2009[Klotz, S., Chervin, J.-C., Munsch, P. & Le Marchand, G. (2009). J. Phys. D Appl. Phys. 42, 075413.]). As the differences between the structures are subtle, they are likely very sensitive to non-hydrostatic conditions. Understanding the discrepancy between results derived from crystallographic studies and those of a spectroscopic nature would require substantial further investigation.

Acknowledgements

EL thanks Matt Edwards and Sarah Barnett for assistance in data collection at beamline I19 of the Diamond Light Source. EL thanks the University of Warwick for a PhD studentship through the Warwick Centre for Doctoral Training in Analytical Science.

Conflict of interest

No conflicts of interest.

Data availability

All CIFs underpinning the results presented here are available as part of the supporting information.

Funding information

The following funding is acknowledged: Royal Society (grant No. UF160265 to Mark S. Senn; grant No. URF\R\231012); Engineering and Physical Sciences Research Council (grant No. EP/S027106/1 to Mark S. Senn); US Department of Energy (award No. DE-FG02-07ER46382 to Sang-Wook Cheong); Diamond Light Source (award No. CY36775; award No. CY26668).

References

First citationAblitt, C., Craddock, S., Senn, M. S., Mostofi, A. A. & Bristowe, N. C. (2017). npj Comput. Mater. 3, 44.  CrossRef Google Scholar
First citationAblitt, C., Mostofi, A. A., Bristowe, N. C. & Senn, M. S. (2018). Front. Chem. 6, 455.  CrossRef PubMed Google Scholar
First citationBenedek, N. A. & Fennie, C. J. (2011). Phys. Rev. Lett. 106, 107204.  Web of Science CrossRef PubMed Google Scholar
First citationBousquet, E., Dawber, M., Stucki, N., Lichtensteiger, C., Hermet, P., Gariglio, S., Triscone, J.-M. & Ghosez, P. (2008). Nature, 452, 732–736.  Web of Science CrossRef PubMed CAS Google Scholar
First citationBousquet, E. & Ghosez, P. (2006). Phys. Rev. B, 74, 180101.  CrossRef Google Scholar
First citationCampbell, B. J., Stokes, H. T., Tanner, D. E. & Hatch, D. M. (2006). J. Appl. Cryst. 39, 607–614.  Web of Science CrossRef CAS IUCr Journals Google Scholar
First citationClarke, G., Daisenberger, D., Luo, X., Cheong, S. W., Bristowe, N. C. & Senn, M. S. (2024). Phys. Rev. B, 109, 094107.  CrossRef Google Scholar
First citationCliffe, M. J. & Goodwin, A. L. (2012). J. Appl. Cryst. 45, 1321–1329.  Web of Science CrossRef CAS IUCr Journals Google Scholar
First citationDolomanov, O. V., Bourhis, L. J., Gildea, R. J., Howard, J. A. K. & Puschmann, H. (2009). J. Appl. Cryst. 42, 339–341.  Web of Science CrossRef CAS IUCr Journals Google Scholar
First citationIshidate, T., Abe, S., Takahashi, H. & Môri, N. (1997). Phys. Rev. Lett. 78, 2397–2400.  CrossRef CAS Google Scholar
First citationKlotz, S., Chervin, J.-C., Munsch, P. & Le Marchand, G. (2009). J. Phys. D Appl. Phys. 42, 075413.  Web of Science CrossRef Google Scholar
First citationKratochvilova, M., Huang, F.-T., Diaz, M. F., Klicpera, M., Day, S. J., Thompson, S. P., Oh, Y.-S., Gao, B., Cheong, S.-W. & Park, J.-G. (2019). J. Appl. Phys. 125, 244102.  CrossRef Google Scholar
First citationOh, Y. S., Luo, X., Huang, F.-T., Wang, Y. & Cheong, S.-W. (2015). Nat. Mater. 14, 407–413.  CrossRef CAS PubMed Google Scholar
First citationOrobengoa, D., Capillas, C., Aroyo, M. I. & Perez-Mato, J. M. (2009). J. Appl. Cryst. 42, 820–833.  Web of Science CrossRef CAS IUCr Journals Google Scholar
First citationPerez-Mato, J. M., Orobengoa, D. & Aroyo, M. I. (2010). Acta Cryst. A66, 558–590.  Web of Science CrossRef CAS IUCr Journals Google Scholar
First citationPomiro, F., Ablitt, C., Bristowe, N. C., Mostofi, A. A., Won, C., Cheong, S.-W. & Senn, M. S. (2020). Phys. Rev. B, 102, 014101.  CrossRef Google Scholar
First citationRamkumar, S. P. & Nowadnick, E. A. (2021). Phys. Rev. B, 104, 144105.  CrossRef Google Scholar
First citationRigaku (2023). CrysAlisPro. Rigaku Oxford Diffraction, Yarnton, England.  Google Scholar
First citationScott, J. F. (2007). Science, 315, 954–959.  Web of Science CrossRef PubMed CAS Google Scholar
First citationSenn, M., Bombardi, A., Murray, C., Vecchini, C., Scherillo, A., Luo, X. & Cheong, S. (2015). Phys. Rev. Lett. 114, 035701.  CrossRef PubMed Google Scholar
First citationSenn, M. S., Murray, C. A., Luo, X., Wang, L., Huang, F.-T., Cheong, S.-W., Bombardi, A., Ablitt, C., Mostofi, A. A. & Bristowe, N. C. (2016). J. Am. Chem. Soc. 138, 5479–5482.  Web of Science CrossRef ICSD CAS PubMed Google Scholar
First citationSheldrick, G. M. (2015a). Acta Cryst. C71, 3–8.  Web of Science CrossRef IUCr Journals Google Scholar
First citationSheldrick, G. M. (2015b). Acta Cryst. A71, 3–8.  Web of Science CrossRef IUCr Journals Google Scholar
First citationSmith, K. A., Ramkumar, S. P., Harms, N. C., Clune, A. J., Xu, X., Cheong, S.-W., Liu, Z., Nowadnick, E. A. & Musfeldt, J. L. (2021). Phys. Rev. B, 104, 064106.  CrossRef Google Scholar
First citationStokes, H. T., Hatch, D. M. & Campbell, B. J. (2013). ISODISTORT, ISOTROPY Software Suite. https://iso.byu.eduGoogle Scholar
First citationSyassen, K. (2008). High Pressure Res. 28, 75–126.  Web of Science CrossRef CAS Google Scholar
First citationXu, X., Wang, Y., Huang, F.-T., Du, K., Nowadnick, E. A. & Cheong, S.-W. (2020). Adv. Funct. Mater. 30, 2003623.  Google Scholar
First citationYoshida, S., Akamatsu, H., Tsuji, R., Hernandez, O., Padmanabhan, H., Sen Gupta, A., Gibbs, A. S., Mibu, K., Murai, S., Rondinelli, J. M., Gopalan, V., Tanaka, K. & Fujita, K. (2018). J. Am. Chem. Soc. 140, 15690–15700.  CAS PubMed 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.

Journal logoSTRUCTURAL SCIENCE
CRYSTAL ENGINEERING
MATERIALS
ISSN: 2052-5206
Follow Acta Cryst. B
Sign up for e-alerts
Follow Acta Cryst. on Twitter
Follow us on facebook
Sign up for RSS feeds