Bulletin of the American Physical Society
APS March Meeting 2018
Volume 63, Number 1
Monday–Friday, March 5–9, 2018; Los Angeles, California
Session X10: 4d/5d materials I
8:00 AM–11:00 AM,
Friday, March 9, 2018
LACC
Room: 301B
Sponsoring
Unit:
DMP
Chair: Adam Aczel, Oak Ridge National Laboratory
Abstract ID: BAPS.2018.MAR.X10.1
Abstract: X10.00001 : Stability of the anti-ferromagnetic state in the hole and electron doped Sr2IrO4
8:00 AM–8:12 AM
Presenter:
Sayantika Bhowal
(Physics and Astronomy, University of Missouri)
Authors:
Sayantika Bhowal
(Physics and Astronomy, University of Missouri)
Jamshid Kurdestany
(Physics and Astronomy, University of Missouri)
Sashi Satpathy
(Physics and Astronomy, University of Missouri)
The realization of the spin-orbit coupling (SOC) driven jeff = 1/2 anti-ferromagnetic (AFM) Mott insulating state in Sr2IrO4 has generated a huge interest in the field of 5d transition metal oxides. Recently, much work has been done on the electron and hole doped materials, particularly because doping can reveal many properties of the underlying structure. In this context, we have studied a minimal model, an extended (t-t'-t'') Hubbard model on a square lattice (in terms of which the upper and lower Hubbard bands can be described) using the Hartree-Fock mean field theory to understand the quantum many-body instabilities of the AFM state in the doped relativistic Mott insulator Sr2IrO4. Our results for the relevant parameters required to describe the material show that the AFM state is stable for a range of both electron and hole doping concentration. Interestingly, a mixed phase of metallic and insulating regions leading to percolative conduction occurs in case of hole doping. Our analysis of the stability of the AFM state in the doped extended Hubbard model of the present work, with respect to the transverse perturbations shows that the sign of the third nearest neighbor interaction plays a crucial role in determining the stability of the AFM state away from half-filling.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.MAR.X10.1
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