Effects of anisotropy in spin molecular-orbital coupling on effective spin models of trinuclear organometallic complexes
Source abstract
Abstract
We consider layered decorated honeycomb lattices at two-thirds filling, as realized in some trinuclear organometallic complexes. Localized $S=1$ moments with a single-spin anisotropy emerge from the interplay of Coulomb repulsion and spin molecular-orbit coupling (SMOC). Magnetic anisotropies with bond-dependent exchange couplings occur in the honeycomb layers when the direct intracluster exchange and the spin molecular-orbital coupling are both present. We find that the effective spin exchange model within the layers is an XXZ + ${120}^{\ensuremath{\circ}}$ honeycomb quantum compass model. The intrinsic nonspherical symmetry of the multinuclear complexes leads to very different transverse and longitudinal spin molecular-orbital couplings, which greatly enhances the single-spin and exchange coupling anisotropies. The interlayer coupling is described by an XXZ model with anisotropic biquadratic terms. As the correlation strength increases the system becomes increasingly one-dimensional. Thus, if the ratio of SMOC to the interlayer hopping is small this stabilizes the Haldane phase. However, as the ratio increases there is a quantum phase transition to the topologically trivial ``$D$ phase.'' We also predict a quantum phase transition from a Haldane phase to a magnetically ordered phase at sufficiently strong external magnetic fields.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Advanced Condensed Matter Physics · Physics of Superconductivity and Magnetism · Theoretical and Computational Physics
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (58)
Show source-provided references
1. 10.1146/annurev-conmatphys-020911-12513810.1146/annurev-conmatphys-020911-125138 ↗
2. 10.1038/nphys160610.1038/nphys1606 ↗
3. 10.1103/RevModPhys.87.110.1103/RevModPhys.87.1 ↗
4. 10.1103/PhysRevLett.102.01720510.1103/PhysRevLett.102.017205 ↗
5. 10.1103/PhysRevB.89.03514310.1103/PhysRevB.89.035143 ↗
6. 10.1103/PhysRevB.90.15512610.1103/PhysRevB.90.155126 ↗
7. 10.1016/j.aop.2005.10.00510.1016/j.aop.2005.10.005 ↗
8. 10.1103/PhysRevLett.119.05720210.1103/PhysRevLett.119.057202 ↗
9. 10.1103/PhysRevB.95.06040410.1103/PhysRevB.95.060404 ↗
10. 10.1103/PhysRevLett.119.08720410.1103/PhysRevLett.119.087204 ↗
11. 10.1021/om00120a00610.1021/om00120a006 ↗
12. 10.1103/PhysRevB.95.11510910.1103/PhysRevB.95.115109 ↗
13. 10.1103/PhysRevB.95.15512010.1103/PhysRevB.95.155120 ↗
14. 10.1103/PhysRevB.94.20510910.1103/PhysRevB.94.205109 ↗
15. 10.1103/PhysRevB.95.09443210.1103/PhysRevB.95.094432 ↗
16. 10.1103/PhysRevB.96.09990210.1103/PhysRevB.96.099902 ↗
17. 10.1103/PhysRevB.91.12514010.1103/PhysRevB.91.125140 ↗
18. 10.1103/PhysRevB.81.20511510.1103/PhysRevB.81.205115 ↗
19. 10.1103/PhysRevLett.95.14680210.1103/PhysRevLett.95.146802 ↗
20. 10.1103/PhysRevLett.99.24720310.1103/PhysRevLett.99.247203 ↗
21. 10.1021/acs.jpcc.6b0508110.1021/acs.jpcc.6b05081 ↗
22. 10.1063/1.498514410.1063/1.4985144 ↗
23. 10.1103/PhysRevLett.110.19680110.1103/PhysRevLett.110.196801 ↗
24. 10.1038/ncomms245110.1038/ncomms2451 ↗
25. 10.1038/nmat332910.1038/nmat3329 ↗
26. 10.1103/PhysRevX.5.01101310.1103/PhysRevX.5.011013 ↗
27. 10.1103/PhysRevB.93.24513410.1103/PhysRevB.93.245134 ↗
28. 10.1103/PhysRevB.94.21441810.1103/PhysRevB.94.214418 ↗
29. 10.1103/PhysRevLett.113.26720410.1103/PhysRevLett.113.267204 ↗
30. 10.1103/PhysRevB.90.03512010.1103/PhysRevB.90.035120 ↗
31. 10.1143/PTPS.160.15510.1143/PTPS.160.155 ↗
32. 10.1088/1367-2630/14/7/07301510.1088/1367-2630/14/7/073015 ↗
33. 10.1063/1.182904710.1063/1.1829047 ↗
34. 10.1016/j.ccr.2015.02.00810.1016/j.ccr.2015.02.008 ↗
35. 10.1103/PhysRevB.52.1023910.1103/PhysRevB.52.10239 ↗
36. 10.1103/PhysRev.120.9110.1103/PhysRev.120.91 ↗
37. 10.1103/PhysRevLett.69.83610.1103/PhysRevLett.69.836 ↗
38. 10.1088/0022-3719/10/10/00210.1088/0022-3719/10/10/002 ↗
39. 10.1103/PhysRev.157.29510.1103/PhysRev.157.295 ↗
40. 10.1103/PhysRevLett.59.79910.1103/PhysRevLett.59.799 ↗
41. 10.1103/PhysRevB.48.384410.1103/PhysRevB.48.3844 ↗
42. 10.1016/0375-9601(83)90631-X10.1016/0375-9601(83)90631-X ↗
43. 10.1103/PhysRevLett.50.115310.1103/PhysRevLett.50.1153 ↗
44. 10.1103/PhysRevLett.63.79010.1103/PhysRevLett.63.790 ↗
45. 10.1103/PhysRevB.85.07512510.1103/PhysRevB.85.075125 ↗
46. 10.1103/PhysRevB.79.05441210.1103/PhysRevB.79.054412 ↗
47. 10.1103/PhysRevB.84.22040210.1103/PhysRevB.84.220402 ↗
48. 10.1088/0953-8984/25/40/40600210.1088/0953-8984/25/40/406002 ↗
49. 10.1103/PhysRevA.77.01231110.1103/PhysRevA.77.012311 ↗
50. 10.7566/JPSCP.3.01200510.7566/JPSCP.3.012005 ↗
51. 10.1103/PhysRevB.42.453710.1103/PhysRevB.42.4537 ↗
52. 10.1103/PhysRevB.41.669710.1103/PhysRevB.41.6697 ↗
53. 10.1103/PhysRevB.75.14040310.1103/PhysRevB.75.140403 ↗
54. 10.1103/PhysRevB.92.06041210.1103/PhysRevB.92.060412 ↗
55. 10.1103/PhysRevB.94.14440910.1103/PhysRevB.94.144409 ↗
56. 10.1103/PhysRevB.92.19511010.1103/PhysRevB.92.195110 ↗
57. 10.1103/PhysRevB.78.14040510.1103/PhysRevB.78.140405 ↗
58. 10.1103/PhysRevLett.118.26720110.1103/PhysRevLett.118.267201 ↗