journal article·2019-10-16

Effect of confinement and octahedral rotations on the electronic, magnetic, and thermoelectric properties of correlated SrXO3/SrTiO3(001) superlattices ( X=V , Cr, or Mn)

Manish Verma, Benjamin Geisler, Rossitza Pentcheva

Physical Review B· Volume 100· Issue 16
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Abstract

By using density functional theory calculations with an on-site Coulomb repulsion term combined with Boltzmann transport theory, we explore the effect of ${t}2g$ orbital occupation on the electronic, magnetic, and thermoelectric properties of ${(\mathrm{Sr}X{\mathrm{O}}3)}1/{({\mathrm{SrTiO}}3)}n(001)$ superlattices with $n=1,3$ and $X=\mathrm{V}$, Cr, and Mn. In order to disentangle the effect of quantum confinement and octahedral rotations and to account for a wider temperature range, $P4/mmm$ (untilted) and $P{2}1/c$ (tilted) phases are considered. We find that the ground-state superlattice geometries always display finite octahedral rotations, which drive an orbital reconstruction and a concomitant metal-to-insulator transition in confined ${\mathrm{SrVO}}3$ and ${\mathrm{SrCrO}}3$ single layers with ferro- and antiferromagnetic spin alignments, respectively. On the other hand, the confined ${\mathrm{SrMnO}}3$ single layer exhibits electronic properties similar to bulk. We show that confinement enhances the thermoelectric properties, particularly for ${\mathrm{SrVO}}3$ and ${\mathrm{SrCrO}}3$ due to the emergent Mott phase. Large room-temperature Seebeck coefficients are obtained for the tilted superlattices, ranging from 500 to $600\phantom{\rule{0.28em}{0ex}}\ensuremath{\mu}\mathrm{V}/\mathrm{K}$ near the band edges. The estimated attainable power factors of $27.9\phantom{\rule{0.28em}{0ex}}(26.6)\phantom{\rule{0.28em}{0ex}}\ensuremath{\mu}\mathrm{W}\phantom{\rule{0.16em}{0ex}}{\mathrm{K}}^{\ensuremath{-}2}\phantom{\rule{0.16em}{0ex}}{\mathrm{cm}}^{\ensuremath{-}1}$ in plane for the ${({\mathrm{SrCrO}}3)}1/{({\mathrm{SrTiO}}3)}1(001)$ superlattice with $P4/mmm\phantom{\rule{0.28em}{0ex}}(P{2}1/c)$ symmetry and $28.1\phantom{\rule{0.28em}{0ex}}\ensuremath{\mu}\mathrm{W}\phantom{\rule{0.16em}{0ex}}{\mathrm{K}}^{\ensuremath{-}2}\phantom{\rule{0.16em}{0ex}}{\mathrm{cm}}^{\ensuremath{-}1}$ cross plane for the ${({\mathrm{SrMnO}}3)}1/{({\mathrm{SrTiO}}3)}1(001)$ superlattice with $P{2}1/c$ symmetry compare favorably with some of the best-performing oxide thermoelectrics. This demonstrates that the idea to use quantum confinement to enhance the thermoelectric response in correlated transition-metal oxide superlattices [Phys. Rev. Mater. 2, 055403 (2018)] can be applied to a broader class of materials combinations.
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Research context

OpenAlex topics: Magnetic and transport properties of perovskites and related materials · Electronic and Structural Properties of Oxides · Advanced Condensed Matter Physics

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References (80)

Show source-provided references
1. 10.1557/jmr.2011.10810.1557/jmr.2011.108 ↗
2. S. Hébert · 2010
3. 10.1103/PhysRevLett.80.477510.1103/PhysRevLett.80.4775 ↗
4. 10.1103/PhysRevB.61.799610.1103/PhysRevB.61.7996 ↗
5. 10.1038/natrevmats.2017.5310.1038/natrevmats.2017.53 ↗
6. 10.1103/PhysRevLett.104.17660110.1103/PhysRevLett.104.176601 ↗
7. 10.1103/PhysRevLett.108.19660110.1103/PhysRevLett.108.196601 ↗
8. 10.1063/1.494171110.1063/1.4941711 ↗
9. 10.1103/PhysRevB.94.04512210.1103/PhysRevB.94.045122 ↗
10. 10.1021/acs.chemmater.6b0044710.1021/acs.chemmater.6b00447 ↗
11. 10.1103/PhysRevB.92.23514010.1103/PhysRevB.92.235140 ↗
12. 10.1063/1.11020710.1063/1.110207 ↗
13. 10.1038/nmat322310.1038/nmat3223 ↗
14. 10.1126/science.118186210.1126/science.1181862 ↗
15. 10.1038/nmat322510.1038/nmat3225 ↗
16. 10.1146/annurev-matsci-070115-03205710.1146/annurev-matsci-070115-032057 ↗
17. 10.1088/0022-3727/49/43/43300110.1088/0022-3727/49/43/433001 ↗
18. 10.1038/ncomms767810.1038/ncomms7678 ↗
19. 10.1021/acs.jpcc.6b0763410.1021/acs.jpcc.6b07634 ↗
20. 10.1103/PhysRevB.86.19530110.1103/PhysRevB.86.195301 ↗
21. 10.1103/PhysRevB.95.12530110.1103/PhysRevB.95.125301 ↗
22. 10.1103/PhysRevMaterials.2.05540310.1103/PhysRevMaterials.2.055403 ↗
23. 10.1103/PhysRevApplied.11.04404710.1103/PhysRevApplied.11.044047 ↗
24. 10.1103/PhysRevB.84.19545010.1103/PhysRevB.84.195450 ↗
25. 10.1103/PhysRevB.88.04531010.1103/PhysRevB.88.045310 ↗
26. 10.1038/nmat182110.1038/nmat1821 ↗
27. 10.1063/1.347139810.1063/1.3471398 ↗
28. 10.1103/PhysRevB.63.11310410.1103/PhysRevB.63.113104 ↗
29. 10.1063/1.184772310.1063/1.1847723 ↗
30. 10.1103/PhysRevMaterials.2.05100210.1103/PhysRevMaterials.2.051002 ↗
31. 10.1103/PhysRev.140.A113310.1103/PhysRev.140.A1133 ↗
32. P. Blaha · 2001
33. 10.1103/PhysRevLett.100.13640610.1103/PhysRevLett.100.136406 ↗
34. 10.1103/PhysRevB.48.1692910.1103/PhysRevB.48.16929 ↗
35. 10.1103/PhysRevB.81.24511710.1103/PhysRevB.81.245117 ↗
36. 10.1103/PhysRevB.80.12513310.1103/PhysRevB.80.125133 ↗
37. 10.1038/srep0790910.1038/srep07909 ↗
38. 10.1103/PhysRevB.13.518810.1103/PhysRevB.13.5188 ↗
39. 10.1016/j.cpc.2006.03.00710.1016/j.cpc.2006.03.007 ↗
40. 10.1103/PhysRevB.33.55110.1103/PhysRevB.33.551 ↗
41. 10.1103/PhysRevB.92.14441810.1103/PhysRevB.92.144418 ↗
42. 10.1103/PhysRevB.89.18442210.1103/PhysRevB.89.184422 ↗
43. 10.1103/PhysRevB.89.09441010.1103/PhysRevB.89.094410 ↗
44. 10.1103/PhysRev.177.85810.1103/PhysRev.177.858 ↗
45. 10.1016/j.jallcom.2006.02.02610.1016/j.jallcom.2006.02.026 ↗
46. 10.1016/0022-4596(71)90035-110.1016/0022-4596(71)90035-1 ↗
47. 10.1016/0022-4596(75)90029-810.1016/0022-4596(75)90029-8 ↗
48. 10.1016/0038-1098(91)90546-810.1016/0038-1098(91)90546-8 ↗
49. 10.1016/0038-1098(94)00834-Y10.1016/0038-1098(94)00834-Y ↗
50. 10.1103/PhysRevLett.104.14760110.1103/PhysRevLett.104.147601 ↗
51. 10.1016/S0925-8388(02)01349-X10.1016/S0925-8388(02)01349-X ↗
52. 10.1103/PhysRevB.58.437210.1103/PhysRevB.58.4372 ↗
53. 10.1016/0038-1098(67)90088-910.1016/0038-1098(67)90088-9 ↗
54. 10.1103/PhysRevB.84.12511410.1103/PhysRevB.84.125114 ↗
55. 10.1103/PhysRevLett.99.25570110.1103/PhysRevLett.99.255701 ↗
56. 10.1016/j.physb.2012.01.12610.1016/j.physb.2012.01.126 ↗
57. 10.1088/0953-8984/27/24/24560510.1088/0953-8984/27/24/245605 ↗
58. 10.1103/PhysRevB.64.13441210.1103/PhysRevB.64.134412 ↗
59. 10.1016/j.jssc.2007.03.02010.1016/j.jssc.2007.03.020 ↗
60. 10.1143/JPSJ.37.27510.1143/JPSJ.37.275 ↗
61. 10.1103/PhysRevB.74.14410210.1103/PhysRevB.74.144102 ↗
62. 10.1016/0025-5408(85)90101-110.1016/0025-5408(85)90101-1 ↗
63. 10.1006/jssc.1999.821810.1006/jssc.1999.8218 ↗
64. 10.1103/PhysRevB.92.02441910.1103/PhysRevB.92.024419 ↗
65. 10.1103/PhysRevB.94.10410110.1103/PhysRevB.94.104101 ↗
66. 10.1016/j.tsf.2017.08.05210.1016/j.tsf.2017.08.052 ↗
67. 10.1103/PhysRevLett.99.19640410.1103/PhysRevLett.99.196404 ↗
68. 10.1103/PhysRevLett.98.17640610.1103/PhysRevLett.98.176406 ↗
69. 10.1103/PhysRevMaterials.2.03500110.1103/PhysRevMaterials.2.035001 ↗
70. 10.1103/PhysRevB.88.11543310.1103/PhysRevB.88.115433 ↗
71. 10.1051/jp1:199214510.1051/jp1:1992145 ↗
72. 10.1051/jp1:199424910.1051/jp1:1994249 ↗
73. 10.1103/PhysRevLett.99.12640210.1103/PhysRevLett.99.126402 ↗
74. 10.1103/PhysRevB.61.252510.1103/PhysRevB.61.2525 ↗
75. 10.1103/PhysRevB.51.1394210.1103/PhysRevB.51.13942 ↗
76. 10.1103/PhysRevB.58.375510.1103/PhysRevB.58.3755 ↗
77. 10.1103/PhysRevB.65.17411210.1103/PhysRevB.65.174112 ↗
78. 10.1103/PhysRevB.69.07511010.1103/PhysRevB.69.075110 ↗
79. 10.1103/PhysRevB.73.09444010.1103/PhysRevB.73.094440 ↗
80. 10.1103/PhysRevMaterials.1.06540510.1103/PhysRevMaterials.1.065405 ↗