journal article·2024-02-01Open access

Picometer atomic displacements behind ferroelectricity in the commensurate low-temperature phase in multiferroic YMn2O5

Tina Weigel, Carsten Richter, Melanie Nentwich, Erik Mehner, Valentin Garbe, Laurence Bouchenoire, Dmitri Novikov, Dirk C. Meyer, Matthias Zschornak

Physical Review B· Volume 109· Issue 5

Abstract

Multiferroics are rare materials that exhibit an interaction of ferroelectricity and magnetism. One such multiferroic material is the $\mathrm{Mn}$-based mullite ${\mathrm{YMn}}2{\mathrm{O}}5$. ${\mathrm{YMn}}2{\mathrm{O}}5$ undergoes several low-temperature phases, and the origin of ferroelectricity in the commensurate phase remains open. Changes in the Mn spin configuration are believed to be the main driving force, which can be induced by magnetostriction caused by symmetric exchange, the antisymmetric inverse Dzyaloshinskii-Moriya interaction, or a combination of both. These mechanisms are accompanied by specific displacements of ions in the structure. The space group $Pbam\phantom{\rule{0.16em}{0ex}}(55)$ of the paraelectric phase does not allow polar displacements. Moreover, conventional structure analysis has been unsuccessful in refining the charge structure in a lower symmetric phase due to its limited sensitivity in resolving the expected positional displacements. To shed light on this controversial discussion, our goal was to resolve potential ionic displacements within a polar space group by employing the new resonantly suppressed diffraction method, which is highly sensitive to minuscule structural changes in the (sub)picometer range. In this paper, we present the first refined structure model of the commensurate phase in ${\mathrm{YMn}}2{\mathrm{O}}5$ using the lower symmetric space group $Pb{2}1m$, allowing polarization in the $b$ direction. We observed a significant displacement of the Mn ions and the partial structure of oxygen, resulting in a calculated spontaneous polarization ${P}S=(1.3\ifmmode\pm\else\textpm\fi{}0.4)\phantom{\rule{0.16em}{0ex}}\mathrm{mC}\phantom{\rule{0.16em}{0ex}}{\mathrm{m}}^{\ensuremath{-}2}$, which is in good agreement with our measured value ${P}S=(0.88\ifmmode\pm\else\textpm\fi{}0.06)\phantom{\rule{0.16em}{0ex}}\mathrm{mC}\phantom{\rule{0.16em}{0ex}}{\mathrm{m}}^{\ensuremath{-}2}$. Importantly, we confirm that ${P}S$ predominantly arises from an ionic contribution induced by magnetostriction. These results hold great interest not only for all multiferroic Mn-based mullites, but also for other multiferroic materials where ferroelectricity arises from their magnetic order. Furthermore, a precise understanding of the ionic movement induced by magnetism will aid in the material tuning process to enhance or create multiferroic properties.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Multiferroics and related materials · Ferroelectric and Piezoelectric Materials · Magnetic and transport properties of perovskites and related materials

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Institute of Experimental Physics, Technical University Bergakademie Freiberg, 09596 Freiberg, Germany

Leibniz-Institut für Kristallzüchtung, 12489 Berlin, Germany

Deutsches Elektronen-Synchrotron DESY, 22607 Hamburg, Germany

Institute of Applied Physics, Technical University Bergakademie Freiberg, 09596 Freiberg, Germany

XMaS/BM28, European Synchrotron Radiation Facility, 38043 Grenoble, France

University of Liverpool, Department of Physics, Liverpool L69 7ZE, England, United Kingdom

Funding

Deutsche Forschungsgemeinschaft

References (100+)

Show source-provided references
1. 10.1186/s11671-019-2961-710.1186/s11671-019-2961-7 ↗
2. 10.1038/nmat186010.1038/nmat1860 ↗
3. 10.1063/1.487051110.1063/1.4870511 ↗
4. 10.1063/1.219811110.1063/1.2198111 ↗
5. 10.1063/1.366203710.1063/1.3662037 ↗
6. 10.1103/Physics.2.2010.1103/Physics.2.20 ↗
7. H. Schneider · 200510.1002/3527607358 ↗
8. 10.1107/S002188981103897010.1107/S0021889811038970 ↗
9. 10.1103/PhysRevB.82.01440910.1103/PhysRevB.82.014409 ↗
10. 10.1021/acs.est.1c0892210.1021/acs.est.1c08922 ↗
11. 10.1039/D1TC06106B10.1039/D1TC06106B ↗
12. 10.4209/aaqr.22030210.4209/aaqr.220302 ↗
13. 10.1103/PhysRevB.84.10441610.1103/PhysRevB.84.104416 ↗
14. I. Kagomiya · J. Phys. Soc. Jpn. · 2001 · 70 · 145
15. 10.1080/0015019070145460210.1080/00150190701454602 ↗
16. T. Weißbach · Untersuchungen zu Kristallstruktur und Magnetismus von Übergangsmetalloxiden mittels Dichtefunktionaltheorie und kristallographischer experimenteller Techniken · 2010
17. 10.1143/JPSJ.73.159310.1143/JPSJ.73.1593 ↗
18. 10.1080/0015019021478810.1080/00150190214788 ↗
19. 10.1016/j.jmmm.2008.11.05110.1016/j.jmmm.2008.11.051 ↗
20. 10.1103/PhysRevB.72.22442510.1103/PhysRevB.72.224425 ↗
21. 10.1103/PhysRevLett.96.09760110.1103/PhysRevLett.96.097601 ↗
22. 10.1103/PhysRevLett.100.22760310.1103/PhysRevLett.100.227603 ↗
23. 10.1103/PhysRevLett.93.17740210.1103/PhysRevLett.93.177402 ↗
24. 10.1103/PhysRevB.77.13443410.1103/PhysRevB.77.134434 ↗
25. 10.1143/JPSJ.76.07470610.1143/JPSJ.76.074706 ↗
26. 10.1103/PhysRevLett.98.02720210.1103/PhysRevLett.98.027202 ↗
27. 10.1103/PhysRevB.96.04111710.1103/PhysRevB.96.041117 ↗
28. 10.1103/PhysRevB.88.14040310.1103/PhysRevB.88.140403 ↗
29. 10.1103/PhysRevB.84.05444410.1103/PhysRevB.84.054444 ↗
30. 10.1007/s11467-011-0201-410.1007/s11467-011-0201-4 ↗
31. 10.1016/j.physb.2006.05.17910.1016/j.physb.2006.05.179 ↗
32. 10.3938/jkps.51.82810.3938/jkps.51.828 ↗
33. 10.1088/0953-8984/20/43/43420610.1088/0953-8984/20/43/434206 ↗
34. 10.1038/nmat180410.1038/nmat1804 ↗
35. 10.1103/PhysRevB.92.06041010.1103/PhysRevB.92.060410 ↗
36. 10.1143/JPSJ.79.05470510.1143/JPSJ.79.054705 ↗
37. 10.1063/1.217586610.1063/1.2175866 ↗
38. 10.1063/1.221949410.1063/1.2219494 ↗
39. 10.1103/PhysRevB.78.24511510.1103/PhysRevB.78.245115 ↗
40. 10.1016/j.jmmm.2008.11.05010.1016/j.jmmm.2008.11.050 ↗
41. 10.1016/j.ssc.2012.09.02510.1016/j.ssc.2012.09.025 ↗
42. Y. Noda · J. Korean Phys. Soc. · 2003 · 42 · S1192
43. 10.1134/1.158195110.1134/1.1581951 ↗
44. 10.1103/PhysRevLett.101.06720510.1103/PhysRevLett.101.067205 ↗
45. 10.1103/PhysRevB.79.02040410.1103/PhysRevB.79.020404 ↗
46. 10.1080/0015019039020634710.1080/00150190390206347 ↗
47. 10.1016/j.jeurceramsoc.2009.05.03510.1016/j.jeurceramsoc.2009.05.035 ↗
48. 10.1088/0953-8984/8/15/01610.1088/0953-8984/8/15/016 ↗
49. 10.1103/PhysRevLett.107.05720110.1103/PhysRevLett.107.057201 ↗
50. 10.1038/s41467-017-02599-610.1038/s41467-017-02599-6 ↗
51. J. Attfield · 1996
52. 10.1140/epjd/e2007-00015-y10.1140/epjd/e2007-00015-y ↗
53. 10.1103/PhysRevB.89.09411010.1103/PhysRevB.89.094110 ↗
54. 10.1002/crat.20130043010.1002/crat.201300430 ↗
55. 10.1103/PhysRevB.64.19513310.1103/PhysRevB.64.195133 ↗
56. 10.1103/PhysRevLett.80.193210.1103/PhysRevLett.80.1932 ↗
57. 10.1107/S010876730000342110.1107/S0108767300003421 ↗
58. 10.1103/PhysRevLett.102.03720510.1103/PhysRevLett.102.037205 ↗
59. 10.1103/PhysRevB.73.10040910.1103/PhysRevB.73.100409 ↗
60. 10.1103/PhysRevB.88.02410410.1103/PhysRevB.88.024104 ↗
61. 10.1016/j.physc.2010.02.00210.1016/j.physc.2010.02.002 ↗
62. 10.1016/j.materresbull.2007.10.02910.1016/j.materresbull.2007.10.029 ↗
63. 10.1107/S090904950202234310.1107/S0909049502022343 ↗
64. 10.1107/S010876739600569710.1107/S0108767396005697 ↗
65. 2012
66. E. R. Dobrovinskaya · 2009
67. 10.1088/1742-6596/150/4/04201310.1088/1742-6596/150/4/042013 ↗
68. 10.1143/JPSJ.77.06470610.1143/JPSJ.77.064706 ↗
69. 10.1103/PhysRevB.77.22010410.1103/PhysRevB.77.220104 ↗
70. 10.1107/S090904950101539410.1107/S0909049501015394 ↗
71. 10.1006/adnd.1993.101310.1006/adnd.1993.1013 ↗
72. 10.1007/BF0134031510.1007/BF01340315 ↗
73. 10.1107/S160057752300967010.1107/S1600577523009670 ↗
74. 10.1086/15487010.1086/154870 ↗
75. 10.3390/cryst1007058010.3390/cryst10070580 ↗
76. 10.1107/S010876739000027710.1107/S0108767390000277 ↗
77. 10.1103/PhysRevLett.114.11760110.1103/PhysRevLett.114.117601 ↗
78. 10.1103/PhysRevB.71.21440210.1103/PhysRevB.71.214402 ↗
79. 10.1103/PhysRevB.99.24510910.1103/PhysRevB.99.245109 ↗
80. 10.1103/PhysRevB.93.06441510.1103/PhysRevB.93.064415 ↗
81. 10.1088/0953-8984/20/48/48521610.1088/0953-8984/20/48/485216 ↗
82. 10.1103/PhysRevB.105.21441310.1103/PhysRevB.105.214413 ↗
83. 10.1103/PhysRevLett.99.17720210.1103/PhysRevLett.99.177202 ↗
84. 10.1103/PhysRevB.77.13411310.1103/PhysRevB.77.134113 ↗
85. 10.1140/epjb/e2006-00318-310.1140/epjb/e2006-00318-3 ↗
86. 10.1103/PhysRevB.108.05410510.1103/PhysRevB.108.054105 ↗
87. 10.1103/PhysRevB.83.22010310.1103/PhysRevB.83.220103 ↗
88. 10.1103/RevModPhys.66.89910.1103/RevModPhys.66.899 ↗
89. 10.1103/PhysRevB.47.165110.1103/PhysRevB.47.1651 ↗
90. 10.1103/PhysRevB.48.444210.1103/PhysRevB.48.4442 ↗
91. 10.1140/epjst/e2012-01614-y10.1140/epjst/e2012-01614-y ↗
92. 10.1103/PhysRevB.100.10410610.1103/PhysRevB.100.104106 ↗
93. 10.1155/2013/49707310.1155/2013/497073 ↗
94. 10.1021/acsami.5b0091110.1021/acsami.5b00911 ↗
95. 10.1103/PhysRevLett.95.08720510.1103/PhysRevLett.95.087205 ↗
96. 10.1039/C3MH00073G10.1039/C3MH00073G ↗
97. 10.1038/s41578-021-00375-z10.1038/s41578-021-00375-z ↗
98. IUCr · 2002
99. I. Kagomiya · 2000
100. P. J. Brown · 2006