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Spin structures and band gap reduction of high-pressure triple perovskite Mn3MnTa2O9

Elena Solana-Madruga *a, Clemens Ritter b, Olivier Mentré a and Ángel M. Arévalo-López *a
aUniv. Lille, CNRS, Centrale Lille, ENSCL, Univ. Artois, UMR 8181 – UCCS – Unité de Catalyse et Chimie du Solide, F-59000 Lille, France. E-mail: elena.solanamadruga@univ-lille.fr; angel.arevalo-lopez@univ-lille.fr
bInstitut Laue-Langevin, Avenue des Martyrs 71, 32042, Grenoble Cedex, France

Received 6th September 2021 , Accepted 7th October 2021

First published on 8th October 2021


Abstract

Herein we report the second transition-metal-only triple perovskite Mn3MnTa2O9, from high pressure-high temperature transformation of Mn4Ta2O9. It shows 1[thin space (1/6-em)]:[thin space (1/6-em)]2 Mn[thin space (1/6-em)]:[thin space (1/6-em)]Ta B-site order and a complex antiferromagnetic behavior with a collinear structure that modulates into a spin density wave. The high pressure phase presents a 25% band gap reduction compared to its multiferroic precursor, recoverable above 625 °C.


Introduction

The flexibility of transition metal (TM) perovskite oxides (ABO3, Pv) allows accommodation of a wide variety of elements into both A and B sites and thus tuning of their promising technological applications.1,2 Different types of cation ordered derivatives can also be obtained and their physical properties enhanced, for instance Sr2FeMoO6 (double perovskite DPv, 1[thin space (1/6-em)]:[thin space (1/6-em)]1 B-site ordering), where the Fe–Mo cation order promotes its room temperature colossal magnetoresistance.3 Exotic perovskites with small TM ions at the A-sites are usually stabilized under high-pressure, as in CaCu3Fe2Re2O12 (quadruple perovskite QPv with 1[thin space (1/6-em)]:[thin space (1/6-em)]3 A and 1[thin space (1/6-em)]:[thin space (1/6-em)]1 B site ordering).4

The growing family of A-site manganites is under intensive study, since the stabilization of Mn into the A-site in the perovskite structure via high-pressure (HP) provides a rich playground of potential spin, orbital and charge orders. Among them, simple (Pv, only MnVO3),5 double (DPv, e.g. Mn2FeReO6),6 doubly ordered (also known as double DDPv, e.g. MnRMnSbO6 with R = rare earth),7 quadruple (QPv, e.g. MnMn3Mn4O12)8,9 and only very recently triple (TPv, only Mn3MnNb2O9 with 1[thin space (1/6-em)]:[thin space (1/6-em)]2 B site ordering)10 perovskite phases have been reported.

In the present study we prepared at high pressure and temperature Mn3MnTa2O9, the second transition-metal-only A3BB′2O9 triple perovskite, from the room pressure (RP) magnetoelectric Mn4Ta2O9 at 8 GPa and 1100 °C. A comparative study with the closely related HP-Mn3MnNb2O9 is presented here. Both isostructural compounds have a complex magnetic behavior, with three subsequent transitions at TN = 52 K, TM = 30.5 K and TL = 6 K for Ta (52.1, 27.8 and 4.8 K respectively for the Nb compound), where Mn2+ spins order into a collinear antiferromagnetic (AFM) structure that modulates into a spin density wave (SDW) and locks-in at lower temperature as revealed by neutron powder diffraction (NPD). The band gap as measured from UV-vis and calculated from DFT for the new HP-Mn3MnTa2O9 shows a reduction of 25% when compared to its room pressure precursor and we argue that this is due to the change in connectivity between both polymorphs offering a promising approach to adjust to ideal values for photovoltaic applications.

Results and discussion

Structural characterization was performed from the Rietveld fit against high resolution NPD data (λ = 1.54 Å, collected on D20 @ ILL). Fig. 1a shows the structural features of the TPv model refined using Full Prof suite11 and summarized in Table 1. HP-Mn3MnTa2O9 crystallizes with the acentric monoclinic Cc symmetry with a = 9.8992(3) Å, b = 5.3267(2) Å, c = 13.2472(5) Å and β = 92.736(3)° cell parameters. As for HP-Mn3MnNb2O9,10 the C2/c symmetry was tested and found in worse agreement (ESI), the superstructure peaks (200), (002) and (110) support the refined Cc model (ESI Fig. SF1). The refined structure shows perfect 1[thin space (1/6-em)]:[thin space (1/6-em)]2 cation order between Mn2+ (Mn2, blue) and Ta5+ (Ta1 and Ta2, orange) among the B sites (being isostructural to HP-Mn3MnNb2O9), see Fig. 1b. Mn–O distances up to 3.5 Å confirm octahedral coordination for Mn2, with all bond lengths between 1.99 Å and 2.28 Å. Otherwise, Mn1 (black), Mn3 (red) and Mn4 (green) show 12-, 11- and 10-fold coordination respectively, according to their location into A sites of the TPv structure. The structural distortion parameters, including abc tilt angles (Φ1 = 18.90°, Φ2 = 23.20° and Φ3 = 24.25°) and polyhedral distortions (quadratic elongation and bond angle variance, see Table 1) are of the same order of magnitude as those observed for the related HP-Mn3MnNb2O9 TPv.10 This suggests that A-site manganites with 1[thin space (1/6-em)]:[thin space (1/6-em)]2 B-site order could generally stabilize much greater distortions with respect to Pv, DPv and QPv materials (SF2, ESI). Bond Valence Sum (BVS) calculations confirm nominal Mn2+ and Ta5+ oxidation states, with compensated mismatches among the B-site cations reflecting the strain in the structure and the necessity to stabilize it at high pressure.
image file: d1tc04231a-f1.tif
Fig. 1 (a) Rietveld fit against 300 K high resolution NPD data of HP-Mn3MnTa2O9. (b) Refined TPv crystal structure. One (11-2) plane with the B-site order of Mn2 and Ta is shown on the left panel and 12-, 11- and 10-fold coordination polyhedra of Mn A sites on the right panel.
Table 1 Atomic positions (all Wyckoff 4a sites fully occupied) of HP-Mn3MnTa2O9 refined from the 300 K high resolution NPD data. Space group Cc and cell parameters a = 9.8992(3) Å, b = 5.3267(2) Å, c = 13.2472(5) Å and β = 92.736(3)°. Thermal parameters constrained for cations and anions refine to 0.53 (5) and 0.54(2) Å2 respectively
Site x y z
a Mn3 site used as a cell reference.
Mn1 0.728(2) 0.494(4) 0.428(1)
Mn2 0.440(3) 0.479(3) 0.476(2)
Mn3a 0.394 0.5 0.757
Mn4 0.551(2) −0.012(4) 0.589(1)
Ta1 0.105(1) 0.508(3) 0.823(1)
Ta2 0.770(1) 0.511(2) 0.652(1)
O1 0.724(2) 0.698(2) 0.776(1)
O2 0.194(1) 0.687(2) 0.697(1)
O3 0.111(1) 0.864(3) 0.070(1)
O4 0.853(1) 0.337(2) 0.538(1)
O5 0.514(1) 0.688(2) 0.367(1)
O6 0.563(1) 0.186(2) 0.449(1)
O7 0.767(1) 0.864(3) 0.395(1)
O8 0.450(2) 0.885(1) 0.744(1)
O9 0.387(1) 0.294(2) 0.624(1)

Mn1 Mn2 Mn3 Mn4 Ta1 Ta2
λ 1.086 1.016 1.089 1.060 1.009 1.012
103Δ 10.4 37.7 5.6 8.1 4.1 3.8
σ 2 (deg2) 254.2 46.5 266.2 182.6 20.7 31.3
BVS 1.94 2.45 2.03 2.07 4.67 4.71


A comparative study of the crystal structures of HP-Mn3MnB′2O9 with B′ = Ta and Nb (see Table 2) indicates their main differences concern coordination numbers of MnA sites and tilt angles. Higher A-site coordination is found for B′ = Ta, supporting the perovskite-related structure. Smaller Φ1 and Φ2 while larger Φ3 values compared with those in HP-Mn3MnNb2O9, agree with the relative lattice parameters, two of which are longer for HP-Mn3MnTa2O9. Similar unit cell volumes reflect the close synthesis conditions for both compounds, coherently with their equivalent ionic radii (0.64 Å for both Nb5+ and Ta5+).12 This is also reflected in similar global distortion parameters which confirms their close stability, suggesting other related high pressure compounds should be accessible from HPHT phase transition from the A4B2O9 niobates and tantalates first reported by Bertaut et al.13 Consequently, new complex HP-TPv are currently under study.

Table 2 Compared main structural features of HP-Mn3MnB′2O9 (B′ = Nb, Ta)
B′ Nb Ta
MnA coordination 10, 10, 8 12, 11, 10
Φ 1, Φ2, Φ3 (°) 20, 25, 16 19, 23, 24
a (Å) 9.9054(5) 9.8992(3)
b (Å) 5.3097(2) 5.3267(2)
c (Å) 13.2052(7) 13.2472(5)
β (°) 92.772(6) 92.736(3)
V3) 693.72(3) 697.73(5)


Magnetic susceptibility data (top panel in Fig. 2) show two clear magnetic transitions at TN = 52 K and TM = 30.5 K. These transitions are also observed as λ peaks in heat capacity measurements (see SF2, ESI for derivative curves and TN and TM assignment). A low temperature anomaly (TL = 6 K) is assigned to a lock-in transition of the modulated magnetic phase, in accordance to NPD results as described below (Fig. 2 middle and bottom panels). Curie–Weiss fit to the inverse susceptibility above 150 K results in an effective magnetic moment of 6.0(1) μB/Mn2+, in good agreement with the expected value of 5.92 μB/Mn2+, and θ = −237(1) K, suggesting dominant AFM interactions with strong magnetic frustration (f = |θ|/TN = 4.6(1). A similar behavior was observed for HP-Mn3MnNb2O9, the main difference between both compounds being the clear lambda-like transition observed in the Nb compound at TL. Here, this lock-in is more evident from NPD data (vide infra) while the derivative of heat capacity data (SF2, ESI) shows a broad maximum.


image file: d1tc04231a-f2.tif
Fig. 2 Temperature dependence of magnetic susceptibility and heat capacity (top panel), neutron diffraction (middle) and refined propagation vector and magnetic moment (bottom). Dashed lines mark TN, TM and TL transition temperatures. Green lines in bottom panel show the fit of k vectors to a critical law. μmax stand for maximum values in the SDW phase and μav for averaged (μ/2π) magnetic moments.

The thermal evolution of NPD data (λ = 2.41 Å, D20@ILL) focused on the 24–36° 2θ region is depicted in the middle panel of Fig. 2. These data confirm that HP-Mn3MnTa2O9 undergoes an AFM transition below 54 K, marked with a dashed line. A coherent increase of the intensity of these magnetic peaks is observed down to 32 K (both TM and TN show a 2 K difference respect to bulk properties, usual from experimental details), where the magnetic susceptibility describes a maximum, and a sharp transition occurs, involving the immediate shift of the magnetic peaks. All magnetic peaks in the TN > T > TM temperature range can be indexed with the propagation vector k0 = [0 0 0], where it develops a collinear magnetic structure with all magnetic moments along the easy c axis. This magnetic structure refined from NPD data collected at 40 K is shown in Fig. 3a. It describes AFM (101) planes of MnA sites (black dashed lines). MnB (blue) sites align AFM with Mn1 (black), according to dominant direct d5–d5 interactions through octahedral face sharing.14 The need for FM interactions between MnB and Mn3 (red)/Mn4 (green) A sites induces magnetic frustration. Below TM, the magnetic frustration of MnB sites (vide infra), induces a sinusoidal modulation of the magnetic moments into a complex SDW magnetic structure with kM = [kx 0 kz]. This modulation involves the continuous evolution of the propagation vector towards kx = 1/3 and kz = −1/6, where they are locked below 10 K (Fig. 2 bottom panel). Averaged magnetic moments (μav = μ/2π) evolve progressively throughout the complete temperature range, reaching a maximum value of 3.81(1) μB. This value corresponds to 76.2% of the ideal 2S = 5 value for Mn2+, in line with the change in magnetic entropy estimated from heat capacity (see ESI).


image file: d1tc04231a-f3.tif
Fig. 3 (a) Magnetic structure of HP-Mn3MnTa2O9 at 40 K with k0 = [0 0 0]. AFM (101) MnA planes (red–green–black) are highlighted with black dashed lines. Orange spheres represent Ta sites and the dashed purple and orange boxes highlight sections of the nuclear cell with different sine patterns at low temperature. (b) Schematic representation of UU0DD0 and sinusoidal waves at 1.5 K with kL = [1/3 0 −1/6], where Mn2 (blue)/Mn3 (red) and Mn1 (black)/Mn4 (green) waves with closer propagation are coupled for simplicity. A single unit is shown for Mn1/Mn4 sites while longer sections are shown for Mn2/Mn3. Magnetic phase factors (relative shifts of the waves) are indicated.

The low temperature magnetic structure, schematized in Fig. 3b, can be described as a SDW with kL = [1/3 0 −1/6] and magnetic moments modulated along the c easy axis, varying between zero and saturated values of 5.1 (1) μB. Two different types of sine waves propagating along the a axis alternate along c, showing up–up-0-down–down-0 (UU0DD0) and 3up–3down (sinusoidal) patterns. Similarly complex frustrated magnetic structures are reported in the only oxynitride A-site manganite with Ta, MnTaO2N.15 The magnetic frustration between A and B sites is the driving force for the modulation of these unusual SDW in A-site manganites with TPv structure (see below and ESI for details).

The most distinctive point of both TPv HP-Mn3MnB′2O9 phases (B′ = Ta and Nb) is their magnetic frustration. While the Nb compound showed a larger frustration index (6.42), its collinear k0 phase was dominant down to lower TM = 27.8 K. As a result, the magnetic moment of Mn2+ spins increased in this k0 phase for HP-Mn3MnNb2O9 to maximum values of 2.68(1) μB before modulating into the SDW, while the Ta compound reported here reaches only 2.50(1) μB in the collinear phase. The reason for the earlier modulation of the magnetic moments in HP-Mn3MnTa2O9 compared to the Nb analogue is the larger constraint function,16i.e. the energy ratio between the ground SDW and the hypothetical non-modulated collinear phases. The energy of both magnetic phases can be estimated using a classical spin description as Ef (k0) = Σ Jij*si*sj, where Jij is the spin exchange parameter and si and sj are the magnetic moments of i and j sites. Considering a hypothetical AFM non-modulated phase at low temperature with all equivalent (μav) magnetic moments 2.50 μB, Ef(k0) = 1350*J. The spin modulation minimizes the number of frustrated (FM MnB–MnA) interactions in the kL phase, which decrease from 12 to 5 in each unit cell (see SF4, ESI). Therefore, accounting for the 18 cells per magnetic cell and the different magnetic moments in the UU0DD0 waves (4.33 μB) and in the sinusoidal waves (5 or 2.5 μB), the estimated Ef(kL) = 1177.2*J. The ratio F = Ef(k0)/Ef(kL) = 1.15, suggests maximum values of 2.2 μB/Mn2+ would be reached in the hypothetical non-modulated structure to keep the same energy, while the modulation of the magnetic moments allows their partial saturation with averaged moments near 80% of their ideal value. Therefore, the magnetic frustration between A and B sites is confirmed to be the driving force for the modulation of these unusual SDW in A-site manganites with TPv structure. A similar estimation for HP-Mn3MnNb2O9 results in F = 1.32, thus showing a larger frustration.

High temperature XRD studies revealed the reversibility of the structural phase transition back to the room pressure polymorph Mn4Ta2O9 upon heating HP-Mn3MnTa2O9 at room pressure. As shown in Fig. 4a, it is a first order transition starting at 625 °C and completed at 780 °C. A comparison between both structures is presented in Fig. 4a. The corner-sharing B-site scaffold for the HP TPv phase is highlighted (blue MnBO6 and orange TaO6 octahedra). Compared with Mn4Ta2O9, the main structural difference is the antiphase rotation between the TaO6 octahedra ending up in the characteristic face sharing in the room pressure polymorph. These changes in connectivity have a strong effect in the optical properties.


image file: d1tc04231a-f4.tif
Fig. 4 (a) XRD thermodiffraction patterns showing a room pressure phase transition from the Cc TPv structure of HP-Mn3MnTa2O9 to the P[3 with combining macron]c1 structure of Mn4Ta2O9. The transition temperature range (625–780 °C) is delimited with dashed lines. Projections along [010] of HP-Mn3MnTa2O9 (left) and [100] of Mn4Ta2O9 (right) structures compared below. (b) UV-Vis data showing 25% band gap reduction. (c) Density of states calculated for the room (left) and high-pressure (right) polymorphs.

Kubelka–Munk plots of our experimental UV-vis reflectance spectra (Fig. 4b) show a ΔEgap = 0.9 eV from the Mn4Ta2O9 precursor (Egap = 3.5 eV) to the Mn3MnTa2O9 TPv high pressure phase (Egap = 2.6 eV). DFT+U (U = 5 eV) calculations in a ferromagnetic configuration were performed for both polymorphs (Fig. 4c). A Egap = 2.4 eV was obtained for RP-Mn4Ta2O9 in accordance with previous reports.17 HP-Mn3MnTa2O9 shows a reduced Egap = 1.5 eV. Although both calculated gaps are underestimated by ≈1 eV from their experimental values, they show the same ΔE = 0.9 eV gap shift. Moreover, the Egap reduction in Mn3MnTa2O9 is mainly due to the Ta octahedra, lying at the bottom of the conduction band that shows a red shift. This is commonly related to the change in connectivity between both polymorphs, the denser being prone to easier carrier hopping. The most critical structural reorganization involves the collapsing of face-sharing electron-blocking Ta2O9 dimers (d(Ta–Ta) = 3.08 Å) and edge-sharing Ta–Mn links (d(Ta−Mn) = 3.17 Å) in the RP form, for face sharing Mn–Ta bridges (d(Mn–Ta) = 3.03 Å) in the HP-polymorph, more prompt to delocalization. Mn3TeO6 also shows a similar reduction in the band gap between the room (Egap = 2.6 eV) and the high-pressure polymorphs (Egap = 1.8 eV).18 The differences between both structures in Mn3TeO6 are also due to a drastic structural reorganization of the polyhedral connectivity. A similar explanation has been found for the gap variation between light-harvesting lead iodide perovskite-derived compounds.19 In the case of the here discussed modifications of RP-Mn4Ta2O9 and HP-Mn3MnTa2O9, the gap reduction is mainly promoted by the change in the TaO6 octahedra connectivity.

Conclusions

In conclusion a new HP-Mn3MnTa2O9 A-site manganite with TPv structure and 1[thin space (1/6-em)]:[thin space (1/6-em)]2 B-site order of Mn and Ta has been prepared under HPHT conditions. This is notable as it represents only the second transition-metal-only compound ever reported to show this Cc structure, suggesting a new complete family of functional oxides is accessible. The complex magnetic behavior arises from highly frustrated Mn–Mn interactions giving rise to an unusual SDW with propagation vector k = [1/3 0 −1/6] locked at low temperatures, dictated by the B-site cation order and reflecting the key role of the triangular antiferromagnetic sublattices. The metastable HP-Mn3MnTa2O9 TPv polymorph transforms back into the ambient Mn4Ta2O9 structure above 625 °C. The connectivity changes between the room- and the high-pressure polymorph promotes a band gap reduction as observed in UV-vis measurements and further confirmed by DFT calculations.

Author contributions

The study was designed by A. M. A. L. Synthesis was performed by E. S. M. Bulk magnetism and heat capacity data were measured and analyzed by E. S. M. and A. M. A. L. Neutron diffraction data were collected and analyzed by E. S. M., A. M. A. L. and C. R. DFT calculations were performed by O. M. The paper was written by E. S. M. and A. M. A. L. with collaborations from all authors.

Conflicts of interest

There are no conflicts to declare.

Acknowledgements

We thank support from ANR AMANTS project (19-CE08-0002-01) and the ILL for beamtime at D20 (doi: 10.5291/ILL-DATA.EASY-858) The Chevreul Institute (FR 2638), Region Hauts-de-France, and FEDER are acknowledged for funding the X-ray diffractometers, the “LEGO” multianvil-press and the PPMS magnetometer.

Notes and references

  1. S. Vasala and M. Karppinen, Prog. Solid State Chem., 2015, 43, 1–36 Search PubMed.
  2. A. T. Mulder, N. A. Benedek, J. M. Rondinelli and C. J. Fennie, Adv. Funct. Mater., 2013, 23, 4810–4820 Search PubMed.
  3. K.-I. Kobayashi, T. Kimura, H. Sawada, K. Terakura and Y. Tokura, Nature, 1998, 395, 677–680 Search PubMed.
  4. W.-t. Chen, M. Mizumaki, H. Seki, M. S. Senn, T. Saito, D. Kan, J. P. Attfield and Y. Shimakawa, Nat. Commun., 2014, 5, 3909 Search PubMed.
  5. M. Markkula, A. M. Arévalo-López, A. Kusmartseva, J. A. Rodgers, C. Ritter, H. Wu and J. P. Attfield, Phys. Rev. B: Condens. Matter Mater. Phys., 2011, 84, 094450 Search PubMed.
  6. A. M. Arévalo-López, G. M. McNally and J. P. Attfield, Angew. Chem., Int. Ed., 2015, 54, 12074–12077 Search PubMed.
  7. E. Solana-Madruga, A. M. Arévalo-López, A. J. Dos santos-García, E. Urones-Garrote, D. Ávila-Brande, R. Sáez-Puche and J. P. Attfield, Angew. Chem., Int. Ed., 2016, 55, 9340–9344 Search PubMed.
  8. S. V. Ovsyannikov, A. M. Abakumov, A. A. Tsirlin, W. Schnelle, R. Egoavil, J. Verbeeck, G. Van Tendeloo, K. V. Glazyrin, M. Hanfland and L. Dubrovinsky, Angew. Chem., Int. Ed., 2013, 52, 1494–1498 Search PubMed.
  9. D. D. Khalyavin, R. D. Johnson, P. Manuel, A. A. Tsirlin, A. M. Abakumov, D. P. Kozlenko, Y. Sun, L. Dubrovinsky and S. V. Ovsyannikov, Phys. Rev. B, 2018, 98, 014426 Search PubMed.
  10. E. Solana-Madruga, C. Ritter, C. Aguilar-Maldonado, O. Mentré, J. P. Attfield and Á. M. Arévalo-López, Chem. Commun., 2021, 57, 8441–8444 Search PubMed.
  11. J. Rodriguez-Carvajal, Phys. B, 1993, 192, 55–69 Search PubMed.
  12. R. D. Shannon and C. T. Prewitt, Acta Crystallogr., Sect. B: Struct. Crystallogr. Cryst. Chem., 1969, 25, 925–946 Search PubMed.
  13. E. F. Bertaut, L. Corliss and F. Forrat, J. Phys. Chem. Solids, 1961, 21, 234–251 Search PubMed.
  14. J. B. Goodenough, Magnetism and the Chemical Bond, New Wiley, New York, 1963, pp. 180–181 Search PubMed.
  15. C. Tassel, Y. Kuno, Y. Goto, T. Yamamoto, C. M. Brown, J. Hester, K. Fujita, M. Higashi, R. Abe, K. Tanaka, Y. Kobayashi and H. Kageyama, Angew. Chem., Int. Ed., 2015, 54, 516–521 Search PubMed.
  16. D. Dai and M. H. Whangbo, J. Chem. Phys., 2004, 121, 672–680 Search PubMed.
  17. N. Narayanan, A. Senyshyn, D. Mikhailova, T. Faske, T. Lu, Z. Liu, B. Weise, H. Ehrenberg, R. A. Mole, W. D. Hutchison, H. Fuess, G. J. McIntyre, Y. Liu and D. Yu, Phys. Rev. B, 2018, 98, 134438 Search PubMed.
  18. Á. M. Arévalo-López, E. Solana-Madruga, C. Aguilar-Maldonado, C. Ritter, O. Mentré and J. P. Attfield, Chem. Commun., 2019, 55, 14470–14473 Search PubMed.
  19. M. E. Kamminga, G. A. de Wijs, R. W. A. Havenith, G. R. Blake and T. T. M. Palstra, Inorg. Chem., 2017, 56, 8408–8414 Search PubMed.

Footnote

Electronic supplementary information (ESI) available: Supporting figures and tables. See DOI: 10.1039/d1tc04231a

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