Theoretical prediction of antiferromagnetism in layered perovskite Sr2TcO4
Source abstract
Abstract
We theoretically investigate the magnetic properties of ${\mathrm{Sr}}2{\mathrm{TcO}}4$, a $4d$ transition-metal layered perovskite of the ${\mathrm{K}}2{\mathrm{NiF}}4$ type with half-filled ${t}2g$ states. The effect of local Coulomb repulsion between the ${t}2g$ orbitals is included within the density-functional theory (DFT) + $U$ and DFT + dynamical mean-field theory (DMFT) methods. The DFT + DMFT predicts paramagnetic ${\mathrm{Sr}}2{\mathrm{TcO}}4$ to be close to the Mott insulator-to-metal transition, similarly to the cubic compound ${\mathrm{SrTcO}}3$. The intersite exchange interactions computed within the DFT + DMFT framework point to a strong antiferromagnetic coupling between the neighboring Tc sites within the layer. We then evaluate the N\'eel temperature ${T}N$ within a classical Monte Carlo approach including dipolar interactions, which stabilize the magnetic order in the frustrated ${\mathrm{K}}2{\mathrm{NiF}}4$ lattice structure. Our approach is validated by applying it to a set of layered and cubic perovskites, for which we obtain ${T}N$ in fair agreement with experiment. Within the same approach we obtain the ${T}N$ of ${\mathrm{Sr}}2{\mathrm{TcO}}4$ to be about 450 K. We explore also the effect of anisotropy in exchange interactions due to spin-orbit coupling. These lead to a somewhat higher transition temperature, 550 K.
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Research context
OpenAlex topics: Magnetic and transport properties of perovskites and related materials · Advanced Condensed Matter Physics · Physics of Superconductivity and Magnetism
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (57)
Show source-provided references
1. 10.1103/PhysRevLett.106.06720110.1103/PhysRevLett.106.067201 ↗
2. 10.1021/ja109431t10.1021/ja109431t ↗
3. 10.1103/PhysRevLett.107.25640110.1103/PhysRevLett.107.256401 ↗
4. 10.1103/PhysRevB.83.22040210.1103/PhysRevB.83.220402 ↗
5. 10.1103/PhysRevLett.108.19720210.1103/PhysRevLett.108.197202 ↗
6. 10.1103/PhysRevB.86.10440610.1103/PhysRevB.86.104406 ↗
7. 10.1016/j.physleta.2012.08.00410.1016/j.physleta.2012.08.004 ↗
8. 10.1142/S021798491450049310.1142/S0217984914500493 ↗
9. 10.1146/annurev-conmatphys-020911-12504510.1146/annurev-conmatphys-020911-125045 ↗
10. W. Pies · 1977
11. 10.1016/j.proche.2012.10.09510.1016/j.proche.2012.10.095 ↗
12. 10.1103/PhysRevLett.17.113310.1103/PhysRevLett.17.1133 ↗
13. 10.1103/PhysRevB.39.234410.1103/PhysRevB.39.2344 ↗
14. 10.1103/PhysRevB.11.204210.1103/PhysRevB.11.2042 ↗
15. 10.1103/PhysRevLett.77.279010.1103/PhysRevLett.77.2790 ↗
16. 10.1103/PhysRevLett.94.21720110.1103/PhysRevLett.94.217201 ↗
17. 10.1103/PhysRev.164.73610.1103/PhysRev.164.736 ↗
18. 10.1103/PhysRevB.1.221110.1103/PhysRevB.1.2211 ↗
19. 10.1103/PhysRevB.76.02443310.1103/PhysRevB.76.024433 ↗
20. 10.1103/PhysRevB.15.429210.1103/PhysRevB.15.4292 ↗
21. 10.1103/PhysRevB.63.14040110.1103/PhysRevB.63.140401 ↗
22. 10.1107/S002188981103897010.1107/S0021889811038970 ↗
23. D. P. Landau · 200910.1017/CBO9780511994944 ↗
24. 10.1103/PhysRevB.59.1357710.1103/PhysRevB.59.13577 ↗
25. P. Blaha · 2001
26. 10.1103/PhysRevB.86.16510510.1103/PhysRevB.86.165105 ↗
27. 10.1103/PhysRevB.48.1692910.1103/PhysRevB.48.16929 ↗
28. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
29. 10.1016/j.cpc.2015.04.02310.1016/j.cpc.2015.04.023 ↗
30. 10.1016/j.cpc.2016.03.01410.1016/j.cpc.2016.03.014 ↗
31. 10.1103/PhysRevB.80.08510110.1103/PhysRevB.80.085101 ↗
32. 10.1103/PhysRevB.84.05452910.1103/PhysRevB.84.054529 ↗
33. 10.1016/j.cpc.2015.10.02310.1016/j.cpc.2015.10.023 ↗
34. 10.1103/PhysRevB.84.07514510.1103/PhysRevB.84.075145 ↗
35. 10.1103/RevModPhys.83.34910.1103/RevModPhys.83.349 ↗
36. 10.1103/PhysRevB.74.15510710.1103/PhysRevB.74.155107 ↗
37. 10.1103/PhysRevB.86.15515810.1103/PhysRevB.86.155158 ↗
38. 10.1080/0026897630010046110.1080/00268976300100461 ↗
39. 10.1088/0953-8984/16/47/01610.1088/0953-8984/16/47/016 ↗
40. 10.1103/PhysRevB.19.469110.1103/PhysRevB.19.4691 ↗
41. 10.1103/PhysRevB.25.576610.1103/PhysRevB.25.5766 ↗
42. 10.1016/0304-8853(87)90721-910.1016/0304-8853(87)90721-9 ↗
43. 10.1103/PhysRevLett.90.08720510.1103/PhysRevLett.90.087205 ↗
44. 10.1103/PhysRevB.70.12511510.1103/PhysRevB.70.125115 ↗
45. 10.1103/PhysRevB.61.890610.1103/PhysRevB.61.8906 ↗
46. 10.1103/PhysRevLett.97.26640310.1103/PhysRevLett.97.266403 ↗
47. 10.1103/PhysRevB.94.11511710.1103/PhysRevB.94.115117 ↗
48. 10.1098/rspa.1963.020410.1098/rspa.1963.0204 ↗
49. 10.1103/PhysRevLett.106.09640110.1103/PhysRevLett.106.096401 ↗
50. 10.1080/0001873970010155810.1080/00018739700101558 ↗
51. 10.1103/PhysRev.166.51410.1103/PhysRev.166.514 ↗
52. 10.1063/1.275116510.1063/1.2751165 ↗
53. 10.1016/0022-4596(81)90469-210.1016/0022-4596(81)90469-2 ↗
54. 10.1103/PhysRevB.47.502710.1103/PhysRevB.47.5027 ↗
55. 10.1103/RevModPhys.70.89710.1103/RevModPhys.70.897 ↗
56. 10.1002/ange.20131011010.1002/ange.201310110 ↗
57. 10.1021/ic500265t10.1021/ic500265t ↗