In-plane magnetic anisotropy in strontium iridate Sr2IrO4
Source abstract
Abstract
Magnetic anisotropy in strontium iridate ($\mathrm{S}{\mathrm{r}}2\mathrm{Ir}{\mathrm{O}}4$) is found to be large because of the strong spin-orbit interactions. In our work, we studied the in-plane magnetic anisotropy of $\mathrm{S}{\mathrm{r}}2\mathrm{Ir}{\mathrm{O}}4$ and traced the anisotropic exchange interactions between the isospins in the crystal. The magnetic-field--dependent torque \ensuremath{\tau}($H$) showed a prominent transition from the canted antiferromagnetic state to the weak ferromagnetic (WFM) state. A comprehensive analysis was conducted to examine the isotropic and anisotropic regimes and probe the easy magnetization axis along the $ab$ plane. The angle-dependent torque \ensuremath{\tau}(\ensuremath{\theta}) revealed a deviation from the sinusoidal behavior, and small differences in hysteresis were observed around 0\ifmmode^\circ\else\textdegree\fi{} and 90\ifmmode^\circ\else\textdegree\fi{} in the low-magnetic-field regime. This indicates that the orientation of the easy axis of the FM component is along the $b$ axis, where the antiferromagnetic to WFM spin-flop transition occurs. We compared the coefficients of the magnetic susceptibility tensors and captured the anisotropy of the material. The in-plane \ensuremath{\tau}(\ensuremath{\theta}) revealed a tendency toward isotropic behavior for fields with values above the field value of the WFM transition.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Advanced Condensed Matter Physics · Multiferroics and related materials · Physics of Superconductivity and Magnetism
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (26)
Show source-provided references
1. 10.1126/science.108285710.1126/science.1082857 ↗
2. 10.1103/PhysRevLett.95.19720210.1103/PhysRevLett.95.197202 ↗
3. 10.1103/PhysRevB.79.02040310.1103/PhysRevB.79.020403 ↗
4. 10.1038/ncomms231610.1038/ncomms2316 ↗
5. 10.1103/PhysRevB.49.919810.1103/PhysRevB.49.9198 ↗
6. 10.1103/PhysRevLett.69.227610.1103/PhysRevLett.69.2276 ↗
7. 10.1103/PhysRevB.60.1217710.1103/PhysRevB.60.12177 ↗
8. 10.1098/rsta.2013.014810.1098/rsta.2013.0148 ↗
9. 10.1103/PhysRevX.4.04103410.1103/PhysRevX.4.041034 ↗
10. 10.1126/science.116710610.1126/science.1167106 ↗
11. 10.1103/PhysRevLett.106.13640210.1103/PhysRevLett.106.136402 ↗
12. 10.1103/PhysRevLett.102.01720510.1103/PhysRevLett.102.017205 ↗
13. 10.1103/PhysRevLett.101.07640210.1103/PhysRevLett.101.076402 ↗
14. 10.1103/PhysRevLett.112.05640210.1103/PhysRevLett.112.056402 ↗
15. 10.1103/PhysRevLett.107.12720510.1103/PhysRevLett.107.127205 ↗
16. 10.1103/PhysRevLett.105.02720410.1103/PhysRevLett.105.027204 ↗
17. 10.1103/PhysRevB.83.20510110.1103/PhysRevB.83.205101 ↗
18. 10.1103/PhysRevB.89.03510910.1103/PhysRevB.89.035109 ↗
19. 10.1088/0953-8984/28/32/32LT0110.1088/0953-8984/28/32/32LT01 ↗
20. 10.1103/PhysRevB.91.15511310.1103/PhysRevB.91.155113 ↗
21. 10.1103/PhysRevLett.116.13640110.1103/PhysRevLett.116.136401 ↗
22. 10.1103/PhysRevB.93.09440610.1103/PhysRevB.93.094406 ↗
23. 10.1088/0953-8984/28/12/12600310.1088/0953-8984/28/12/126003 ↗
24. 10.1088/0953-8984/22/2/02600610.1088/0953-8984/22/2/026006 ↗
25. 10.1088/0953-8984/17/48/01710.1088/0953-8984/17/48/017 ↗
26. 10.1016/j.jmmm.2013.05.02210.1016/j.jmmm.2013.05.022 ↗