journal article·2021-03-25Open access

Experimental and Theoretical Study of the Electronic Structures of Lanthanide Indium Perovskites LnInO3

P. Hartley, R. G. Egdell, K. H. L. Zhang, M. V. Hohmann, L. F. J. Piper, D. J. Morgan, D. O. Scanlon, B. A. D. Williamson, A. Regoutz

The Journal of Physical Chemistry C· Volume 125· Issue 11

Abstract

High Resolution Image Download MS PowerPoint Slide Ternary lanthanide indium oxides LnInO 3 (Ln = La, Pr, Nd, Sm) were synthesized by high-temperature solid-state reaction and characterized by X-ray powder diffraction. Rietveld refinement of the powder patterns showed the LnInO 3 materials to be orthorhombic perovskites belonging to the space group Pnma, based on almost-regular InO 6 octahedra and highly distorted LnO 12 polyhedra. Experimental structural data were compared with results from density functional theory (DFT) calculations employing a hybrid Hamiltonian. Valence region X-ray photoelectron and K-shell X-ray emission and absorption spectra of the LnInO 3 compounds were simulated with the aid of the DFT calculations. Photoionization of lanthanide 4f orbitals gives rise to a complex final-state multiplet structure in the valence region for the 4f n compounds PrInO 3, NdInO 3, and SmInO 3, and the overall photoemission spectral profiles were shown to be a superposition of final-state 4f n –1 terms onto the cross-section weighted partial densities of states from the other orbitals. The occupied 4f states are stabilized in moving across the series Pr–Nd–Sm. Band gaps were measured using diffuse reflectance spectroscopy. These results demonstrated that the band gap of LaInO 3 is 4.32 eV, in agreement with DFT calculations. This is significantly larger than a band gap of 2.2 eV first proposed in 1967 and based on the idea that In 4d states lie above the top of the O 2p valence band. However, both DFT and X-ray spectroscopy show that In 4d is a shallow core level located well below the bottom of the valence band. Band gaps greater than 4 eV were observed for NdInO 3 and SmInO 3, but a lower gap of 3.6 eV for PrInO 3 was shown to arise from the occupied Pr 4f states lying above the main O 2p valence band.
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OpenAlex topics: Magnetic and transport properties of perovskites and related materials · Electronic and Structural Properties of Oxides · ZnO doping and properties

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Affiliations

Department of Chemistry, Inorganic Chemistry Laboratory, University of Oxford, South Parks Road, Oxford OX1 3QR, U.K.

State Key Laboratory of Physical Chemistry of Solid Surfaces, College of Chemistry and Chemical Engineering, Xiamen University, Xiamen 361005, People’s Republic of China

Institute of Materials Science, Surface Science Division, Technische Universität Darmstadt, Darmstadt 64287, Germany

WMG, The University of Warwick, Coventry CV4 7AL, U.K.

Department of Applied Physics & Astronomy, Binghamton University, State University of New York, Binghamton, New York 13902, United States

Cardiff Catalysis Institute, School of Chemistry, Cardiff University, Park Place, Cardiff CF10 3AT, U.K.

Department of Chemistry, University College London, 20 Gordon Street, London WC1H 0AJ, U.K.

Thomas Young Centre, University College London, Gower Street, London WC1E 6BT, U.K.

Diamond Light Source Ltd., Diamond House, Harwell Science and Innovation Campus, Didcot, Oxfordshire OX11 0DE, U.K.

Department of Materials Science and Engineering, Norwegian University of Science and Technology (NTNU), Trondheim 7491, Norway

Funding

Engineering and Physical Sciences Research Council · Norges Forskningsr?d · Advanced Light Source

References (80)

Show source-provided references
1. 10.1021/ic102386e10.1021/ic102386e ↗
2. 10.1016/j.jlumin.2017.05.06410.1016/j.jlumin.2017.05.064 ↗
3. 10.1016/j.jlumin.2018.10.09010.1016/j.jlumin.2018.10.090 ↗
4. 10.1016/s0022-3697(02)00358-x10.1016/s0022-3697(02)00358-x ↗
5. 10.1016/j.jpowsour.2012.08.09110.1016/j.jpowsour.2012.08.091 ↗
6. 10.1166/jnn.2015.1154010.1166/jnn.2015.11540 ↗
7. 10.1016/j.jpowsour.2013.10.05410.1016/j.jpowsour.2013.10.054 ↗
8. 10.1016/j.physb.2014.08.03610.1016/j.physb.2014.08.036 ↗
9. 10.1007/s11581-015-1461-810.1007/s11581-015-1461-8 ↗
10. 10.1016/j.rser.2016.12.08610.1016/j.rser.2016.12.086 ↗
11. 10.1063/1.491358710.1063/1.4913587 ↗
12. 10.1063/1.495996010.1063/1.4959960 ↗
13. 10.1063/1.504636810.1063/1.5046368 ↗
14. 10.1063/1.508405810.1063/1.5084058 ↗
15. 10.1038/s41598-019-52772-810.1038/s41598-019-52772-8 ↗
16. 10.1103/physrevapplied.13.06406610.1103/physrevapplied.13.064066 ↗
17. 10.1038/nature0230810.1038/nature02308 ↗
18. 10.1021/cm503896h10.1021/cm503896h ↗
19. 10.1107/s056773947600155110.1107/s0567739476001551 ↗
20. 10.1039/c7dt04849a10.1039/c7dt04849a ↗
21. 10.1016/0022-1902(76)90011-710.1016/0022-1902(76)90011-7 ↗
22. 10.1088/0953-8984/23/33/33421110.1088/0953-8984/23/33/334211 ↗
23. 10.1021/cm901127r10.1021/cm901127r ↗
24. 10.1021/nl102403t10.1021/nl102403t ↗
25. 10.1103/physrevb.82.16531210.1103/physrevb.82.165312 ↗
26. 10.1021/nn301382j10.1021/nn301382j ↗
27. 10.1016/j.jcrysgro.2010.10.14310.1016/j.jcrysgro.2010.10.143 ↗
28. 10.1016/0025-5408(67)90061-x10.1016/0025-5408(67)90061-x ↗
29. 10.1063/1.307052410.1063/1.3070524 ↗
30. 10.1103/physrevb.75.15320510.1103/physrevb.75.153205 ↗
31. 10.1103/physrevlett.100.16740210.1103/physrevlett.100.167402 ↗
32. 10.1103/physrevb.81.16520710.1103/physrevb.81.165207 ↗
33. 10.1143/jjap.40.323110.1143/jjap.40.3231 ↗
34. 10.1143/jjap.36.555110.1143/jjap.36.5551 ↗
35. 10.1063/1.497786310.1063/1.4977863 ↗
36. 10.1080/14786435.2020.177820310.1080/14786435.2020.1778203 ↗
37. 10.1007/s13369-020-04576-610.1007/s13369-020-04576-6 ↗
38. 10.1103/physrevlett.96.15740310.1103/physrevlett.96.157403 ↗
39. 10.1063/1.114092910.1063/1.1140929 ↗
40. 10.1103/physrevb.47.55810.1103/physrevb.47.558 ↗
41. 10.1103/physrevb.49.1425110.1103/physrevb.49.14251 ↗
42. 10.1103/physrevb.54.1116910.1103/physrevb.54.11169 ↗
43. 10.1016/0927-0256(96)00008-010.1016/0927-0256(96)00008-0 ↗
44. 10.1103/physrevlett.77.386510.1103/physrevlett.77.3865 ↗
45. 10.1103/physrevb.50.1795310.1103/physrevb.50.17953 ↗
46. 10.1063/1.240466310.1063/1.2404663 ↗
47. 10.21105/joss.0071710.21105/joss.00717 ↗
48. 10.1107/s010827010302480610.1107/s0108270103024806 ↗
49. 10.1039/c4dt03881a10.1039/c4dt03881a ↗
50. 10.1107/s056774087200797610.1107/s0567740872007976 ↗
51. 10.1107/s010876819500610010.1107/s0108768195006100 ↗
52. 10.1107/s010876819800197910.1107/s0108768198001979 ↗
53. 10.1063/1.494236610.1063/1.4942366 ↗
54. 10.1080/14786435.2016.118910010.1080/14786435.2016.1189100 ↗
55. 10.1016/0092-640x(85)90016-610.1016/0092-640x(85)90016-6 ↗
56. 10.1016/0009-2614(73)89501-610.1016/0009-2614(73)89501-6 ↗
57. 10.1088/0305-4608/11/1/01410.1088/0305-4608/11/1/014 ↗
58. 10.1088/0305-4608/13/3/02110.1088/0305-4608/13/3/021 ↗
59. 10.1016/0009-2614(79)80458-310.1016/0009-2614(79)80458-3 ↗
60. 10.1103/physrevb.68.16510410.1103/physrevb.68.165104 ↗
61. 10.1016/j.cplett.2004.09.14510.1016/j.cplett.2004.09.145 ↗
62. 10.1088/0953-8984/10/38/00610.1088/0953-8984/10/38/006 ↗
63. 10.1021/acs.jpcc.8b0862310.1021/acs.jpcc.8b08623 ↗
64. 10.1103/physrevb.77.15511510.1103/physrevb.77.155115 ↗
65. 10.1063/1.481651110.1063/1.4816511 ↗
66. 10.1021/acs.jpcc.8b1057310.1021/acs.jpcc.8b10573 ↗
67. 10.1021/ic034551c10.1021/ic034551c ↗
68. 10.1557/jmr.2007.025910.1557/jmr.2007.0259 ↗
69. 10.1143/apex.5.06110210.1143/apex.5.061102 ↗
70. 10.1063/1.502942210.1063/1.5029422 ↗
71. 10.1103/physrevb.79.20521110.1103/physrevb.79.205211 ↗
72. 10.1103/physrevlett.41.175010.1103/physrevlett.41.1750 ↗
73. 10.1103/physrevb.51.683310.1103/physrevb.51.6833 ↗
74. 10.1016/0079-6786(71)90018-510.1016/0079-6786(71)90018-5 ↗
75. 10.1088/0022-3719/16/32/01410.1088/0022-3719/16/32/014 ↗
76. 10.1088/0022-3719/16/32/01310.1088/0022-3719/16/32/013 ↗
77. 10.1103/physrevb.87.16120110.1103/physrevb.87.161201 ↗
78. 10.1103/physrevlett.116.02760210.1103/physrevlett.116.027602 ↗
79. 10.1103/physrevlett.110.05680310.1103/physrevlett.110.056803 ↗
80. 10.1103/physrevb.77.15510710.1103/physrevb.77.155107 ↗