journal article·2017-11-10Open access

Effects of anisotropy in spin molecular-orbital coupling on effective spin models of trinuclear organometallic complexes

J. Merino, A. C. Jacko, A. L. Khosla, B. J. Powell

Physical Review B· Volume 96· Issue 20

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.
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Research context

OpenAlex topics: Advanced Condensed Matter Physics · Physics of Superconductivity and Magnetism · Theoretical and Computational Physics

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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 ↗