Back to Search Start Over

Electronic structure and exchange interactions of insulating double perovskite La2CuRuO6.

Authors :
Panda, S. K.
Kvashnin, Y. O.
Sanyal, B.
Dasgupta, I.
Eriksson, O.
Source :
Physical Review B. Aug2016, Vol. 94 Issue 6, p1-1. 1p.
Publication Year :
2016

Abstract

We have performed first-principles calculations of the electronic and magnetic properties of insulating double perovskite compound La2CuRuO6 (LCRO) which has recently been reported to exhibit intriguing magnetic properties. We derived a tight-binding Hamiltonian for LCRO based on the Nth-order muffin-tin orbital (NMTO) downfolding technique. The computed on-site energies and hopping integrals are used to estimate the dominant exchange interactions employing an extended Kugel-Khomskii model. This way the dominant exchange paths were identified and a low-energy spin model was proposed. The Green function method based on the magnetic force theorem has also been used to extract the exchange interactions to provide a more accurate estimation and to justify the model calculations. Our results show that the nearest neighbor (NN) Cu-Ru magnetic interactions are very much direction dependent and a strong antiferromagnetic next nearest neighbor Ru-Ru interaction along the crystallographic b axis is responsible for the magnetic frustration observed experimentally in this system. We argue that due to the broken symmetry, NN Cu-Ru interaction becomes stronger along one direction than the other, which essentially reduces the amount of frustration and helps the system to achieve an antiferromagnetic ground state at low temperature. A detailed microscopic explanation of the exchange mechanism is discussed. We also find that spin-orbit coupling effect is significant and causes a canting of the Ru spin with respect to the Cu moments. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
24699950
Volume :
94
Issue :
6
Database :
Academic Search Index
Journal :
Physical Review B
Publication Type :
Academic Journal
Accession number :
119148212
Full Text :
https://doi.org/10.1103/PhysRevB.94.064427