journal article·2016-03-03

Octahedral Rotation Preferences in Perovskite Iodides and Bromides

Joshua Young, James M. Rondinelli

Publisher page

Abstract

Phase transitions in ABX3 perovskites are often accompanied by rigid rotations of the corner-connected BX6 octahedral network. Although the mechanisms for the preferred rotation patterns of perovskite oxides are fairly well recognized, the same cannot be said of halide variants (i.e., X = Cl, Br, or I), several of which undergo an unusual displacive transition to a tetragonal phase exhibiting in-phase rotations about one axis (a(0)a(0)c(+) in Glazer notation). To discern the chemical factors stabilizing this unique phase, we investigated a series of 12 perovskite bromides and iodides using density functional theory calculations and compared them with similar oxides. We find that in-phase tilting provides a better arrangement of the larger bromide and iodide anions, which minimizes the electrostatic interactions, improves the bond valence of the A-site cations, and enhances the covalency between the A-site metal and Br(-) or I(-) ions. The opposite effect is present in the oxides, with out-of-phase tilting maximizing these factors.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Perovskite Materials and Applications · Solid-state spectroscopy and crystallography · Magnetic and transport properties of perovskites and related materials

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

Affiliations

Department of Materials Science and Engineering, Drexel University, Philadelphia, Pennsylvania 19104, United States

Department of Materials Science and Engineering, Northwestern University, Evanston, Illinois 60208, United States

Funding

Basic Energy Sciences · Division of Materials Research

References (47)

Show source-provided references
1. 10.1021/cs500606g10.1021/cs500606g ↗
2. 10.1557/mrs.2012.4910.1557/mrs.2012.49 ↗
3. 10.1021/jz402016210.1021/jz4020162 ↗
4. 10.1039/C4TA05033A10.1039/C4TA05033A ↗
5. 10.1002/adma.20140314010.1002/adma.201403140 ↗
6. 10.1126/science.125405010.1126/science.1254050 ↗
7. 10.1002/adma.20140199110.1002/adma.201401991 ↗
8. 10.1039/C5TA02950C10.1039/C5TA02950C ↗
9. 10.1038/ncomms675710.1038/ncomms6757 ↗
10. 10.1021/acs.jpcc.5b0744610.1021/acs.jpcc.5b07446 ↗
11. 10.1246/cl.1991.80110.1246/cl.1991.801 ↗
12. 10.1021/ja301539s10.1021/ja301539s ↗
13. 10.1107/S056774087200797610.1107/S0567740872007976 ↗
14. 10.1016/0038-1098(95)00625-710.1016/0038-1098(95)00625-7 ↗
15. 10.1016/0022-4596(74)90088-710.1016/0022-4596(74)90088-7 ↗
16. 10.1088/0022-3719/19/14/00510.1088/0022-3719/19/14/005 ↗
17. 10.1143/JPSJ.37.139310.1143/JPSJ.37.1393 ↗
18. 10.1107/S010876810101528210.1107/S0108768101015282 ↗
19. 10.1080/0015019740823795610.1080/00150197408237956 ↗
20. 10.1107/S010876819800963X10.1107/S010876819800963X ↗
21. 10.1088/0953-8984/16/16/00410.1088/0953-8984/16/16/004 ↗
22. 10.1103/PhysRev.136.B86410.1103/PhysRev.136.B864 ↗
23. 10.1103/PhysRev.140.A113310.1103/PhysRev.140.A1133 ↗
24. 10.1103/PhysRevLett.106.10720410.1103/PhysRevLett.106.107204 ↗
25. 10.1002/adma.20110467410.1002/adma.201104674 ↗
26. 10.1088/0953-8984/27/28/28320210.1088/0953-8984/27/28/283202 ↗
27. 10.1103/PhysRevB.50.1795310.1103/PhysRevB.50.17953 ↗
28. 10.1103/PhysRevLett.100.13640610.1103/PhysRevLett.100.136406 ↗
29. 10.1103/PhysRevB.47.55810.1103/PhysRevB.47.558 ↗
30. 10.1016/0927-0256(96)00008-010.1016/0927-0256(96)00008-0 ↗
31. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
32. 10.1002/zaac.1988559010110.1002/zaac.19885590101 ↗
33. 10.1002/zaac.1989571010610.1002/zaac.19895710106 ↗
34. 10.1524/zkri.1995.210.1.6410.1524/zkri.1995.210.1.64 ↗
35. 10.1016/j.jpcs.2008.05.00710.1016/j.jpcs.2008.05.007 ↗
36. 10.1002/zaac.1987545021710.1002/zaac.19875450217 ↗
37. 10.1016/j.ssi.2008.11.01910.1016/j.ssi.2008.11.019 ↗
38. 10.1103/PhysRevB.81.05411510.1103/PhysRevB.81.054115 ↗
39. 10.1103/PhysRev.177.85810.1103/PhysRev.177.858 ↗
40. 10.1107/S010876739400560X10.1107/S010876739400560X ↗
41. 10.1103/PhysRevB.86.14410710.1103/PhysRevB.86.144107 ↗
42. 10.1039/C4TA00435C10.1039/C4TA00435C ↗
43. 10.1107/S010876819601071310.1107/S0108768196010713 ↗
44. 10.1107/S010876819601205010.1107/S0108768196012050 ↗
45. 10.1107/S010876810302666110.1107/S0108768103026661 ↗
46. 10.1107/S010876730402449310.1107/S0108767304024493 ↗
47. 10.1007/BF0150752710.1007/BF01507527 ↗