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Slater Insulator in Iridate Perovskites with Strong Spin-Orbit Coupling.

Authors :
Cui, Q.
Cheng, J.-G.
Fan, W.
Taylor, A. E.
Calder, S.
McGuire, M. A.
Yan, J.-Q.
Meyers, D.
Li, X.
Cai, Y. Q.
Jiao, Y. Y.
Choi, Y.
Haskel, D.
Gotou, H.
Uwatoko, Y.
Chakhalian, J.
Christianson, A. D.
Yunoki, S.
Goodenough, J. B.
Zhou, J.-S.
Source :
Physical Review Letters. 10/21/2016, Vol. 117 Issue 17, p1-1. 1p.
Publication Year :
2016

Abstract

The perovskite SrIrO3 is an exotic narrow-band metal owing to a confluence of the strengths of the spin-orbit coupling (SOC) and the electron-electron correlations. It has been proposed that topological and magnetic insulating phases can be achieved by tuning the SOC, Hubbard interactions, and/or lattice symmetry. Here, we report that the substitution of nonmagnetic, isovalent Sn4+ for Ir4+ in the SrIr1-xSnxO3 perovskites synthesized under high pressure leads to a metal-insulator transition to an antiferromagnetic (AF) phase at TN=225 K. The continuous change of the cell volume as detected by x-ray diffraction and the κ-shape transition of the specific heat on cooling through TN demonstrate that the metal-insulator transition is of second order. Neutron powder diffraction results indicate that the Sn substitution enlarges an octahedral-site distortion that reduces the SOC relative to the spin-spin exchange interaction and results in the type-G AF spin ordering below TN. Measurement of high-temperature magnetic susceptibility shows the evolution of magnetic coupling in the paramagnetic phase typical of weak itinerant-electron magnetism in the Sn-substituted samples. A reduced structural symmetry in the magnetically ordered phase leads to an electron gap opening at the Brillouin zone boundary below TN in the same way as proposed by Slater. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00319007
Volume :
117
Issue :
17
Database :
Academic Search Index
Journal :
Physical Review Letters
Publication Type :
Academic Journal
Accession number :
119148427
Full Text :
https://doi.org/10.1103/PhysRevLett.117.176603