Heisenberg antiferromagnet on the Husimi lattice
Source abstract
Abstract
We perform a systematic study of the antiferromagnetic Heisenberg model on the Husimi lattice using numerical tensor-network methods based on projected entangled simplex states. The nature of the ground state varies strongly with the spin quantum number $S$. For $S=\frac{1}{2}$, it is an algebraic (gapless) quantum spin liquid. For $S=1$, it is a gapped, nonmagnetic state with spontaneous breaking of triangle symmetry (a trimerized simplex-solid state). For $S=2$, it is a simplex-solid state with a spin gap and no symmetry breaking; both integer-spin simplex-solid states are characterized by specific degeneracies in the entanglement spectrum. For $S=\frac{3}{2}$, and indeed for all spin values $S\ensuremath{\ge}\frac{5}{2}$, the ground states have ${120}^{\ensuremath{\circ}}$ antiferromagnetic order. In a finite magnetic field, we find that, irrespective of the value of $S$, there is always a plateau in the magnetization at $m=\frac{1}{3}$.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Quantum many-body systems · Physics of Superconductivity and Magnetism · Advanced Condensed Matter Physics
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (67)
Show source-provided references
1. 10.1016/0375-9601(83)90631-X10.1016/0375-9601(83)90631-X ↗
2. 10.1103/PhysRevLett.50.115310.1103/PhysRevLett.50.1153 ↗
3. 10.1016/0003-4916(61)90115-410.1016/0003-4916(61)90115-4 ↗
4. 10.1007/BF0040030410.1007/BF00400304 ↗
5. 10.1103/PhysRevLett.59.79910.1103/PhysRevLett.59.799 ↗
6. 10.1007/BF0121802110.1007/BF01218021 ↗
7. 10.1103/PhysRevB.40.470910.1103/PhysRevB.40.4709 ↗
8. 10.1103/PhysRevB.77.24511910.1103/PhysRevB.77.245119 ↗
9. 10.1103/PhysRevB.80.15513110.1103/PhysRevB.80.155131 ↗
10. 10.1103/PhysRevB.83.03510710.1103/PhysRevB.83.035107 ↗
11. 10.1103/PhysRevB.84.23512810.1103/PhysRevB.84.235128 ↗
12. 10.1103/PhysRevB.84.16513910.1103/PhysRevB.84.165139 ↗
13. 10.1103/PhysRevB.87.15511410.1103/PhysRevB.87.155114 ↗
14. 10.1103/PhysRevB.69.10443110.1103/PhysRevB.69.104431 ↗
15. 10.1103/PhysRevB.77.10440410.1103/PhysRevB.77.104404 ↗
16. 10.1103/PhysRevX.4.01102510.1103/PhysRevX.4.011025 ↗
17. 10.1103/PhysRevB.42.843610.1103/PhysRevB.42.8436 ↗
18. 10.1063/1.34783010.1063/1.347830 ↗
19. 10.1103/PhysRevB.68.21441510.1103/PhysRevB.68.214415 ↗
20. 10.1103/PhysRevB.76.18040710.1103/PhysRevB.76.180407 ↗
21. 10.1103/PhysRevB.77.14441510.1103/PhysRevB.77.144415 ↗
22. 10.1103/PhysRevLett.104.18720310.1103/PhysRevLett.104.187203 ↗
23. 10.1103/PhysRevB.83.10040410.1103/PhysRevB.83.100404 ↗
24. 10.1103/PhysRevB.45.1237710.1103/PhysRevB.45.12377 ↗
25. 10.1103/PhysRevLett.101.11720310.1103/PhysRevLett.101.117203 ↗
26. 10.1126/science.120108010.1126/science.1201080 ↗
27. 10.1103/PhysRevLett.109.06720110.1103/PhysRevLett.109.067201 ↗
28. 10.1038/nphys246510.1038/nphys2465 ↗
29. 10.1103/PhysRevLett.98.11720510.1103/PhysRevLett.98.117205 ↗
30. 10.1103/PhysRevB.87.06040510.1103/PhysRevB.87.060405 ↗
31. 10.7566/JPSJ.84.06370510.7566/JPSJ.84.063705 ↗
32. 10.1103/PhysRevB.93.06040710.1103/PhysRevB.93.060407 ↗
33. 10.1143/JPSJ.69.400310.1143/JPSJ.69.4003 ↗
34. 10.1103/PhysRevB.89.17441110.1103/PhysRevB.89.174411 ↗
35. 10.1088/0953-8984/21/45/45600910.1088/0953-8984/21/45/456009 ↗
36. 10.1103/PhysRevB.91.06040310.1103/PhysRevB.91.060403 ↗
37. 10.1103/PhysRevB.91.10040710.1103/PhysRevB.91.100407 ↗
38. 10.1103/PhysRevB.84.22442810.1103/PhysRevB.84.224428 ↗
39. 10.1063/1.174772510.1063/1.1747725 ↗
40. 10.1139/p01-09710.1139/p01-097 ↗
41. 10.1103/PhysRevLett.101.09060310.1103/PhysRevLett.101.090603 ↗
42. 10.1103/PhysRevB.86.19513710.1103/PhysRevB.86.195137 ↗
43. 10.1103/PhysRevB.48.1364710.1103/PhysRevB.48.13647 ↗
44. 10.1103/PhysRevLett.103.18720310.1103/PhysRevLett.103.187203 ↗
45. 10.1063/1.169874210.1063/1.1698742 ↗
46. 10.1073/pnas.39.4.31510.1073/pnas.39.4.315 ↗
47. 10.2307/236930610.2307/2369306 ↗
48. 10.1051/jp1:199311510.1051/jp1:1993115 ↗
49. 10.1016/j.physa.2012.01.03810.1016/j.physa.2012.01.038 ↗
50. M. Takigawa · 2011
51. 10.1103/PhysRevLett.103.16060110.1103/PhysRevLett.103.160601 ↗
52. 10.1103/PhysRevB.81.17441110.1103/PhysRevB.81.174411 ↗
53. 10.1103/PhysRevLett.91.14790210.1103/PhysRevLett.91.147902 ↗
54. 10.1103/PhysRevLett.93.04050210.1103/PhysRevLett.93.040502 ↗
55. 10.1103/PhysRevB.88.03513810.1103/PhysRevB.88.035138 ↗
56. 10.1103/PhysRevB.86.04513910.1103/PhysRevB.86.045139 ↗
57. 10.1137/S089547989630569610.1137/S0895479896305696 ↗
58. 10.1103/PhysRevLett.101.01050410.1103/PhysRevLett.101.010504 ↗
59. 10.1140/epjb/e2014-50391-x10.1140/epjb/e2014-50391-x ↗
60. 10.1103/PhysRevB.89.05442610.1103/PhysRevB.89.054426 ↗
61. 10.1103/PhysRevLett.17.113310.1103/PhysRevLett.17.1133 ↗
62. 10.1103/PhysRevB.88.24511810.1103/PhysRevB.88.245118 ↗
63. 10.1103/PhysRevB.88.14441610.1103/PhysRevB.88.144416 ↗
64. 10.1038/ncomms328710.1038/ncomms3287 ↗
65. 10.1103/PhysRevLett.78.198410.1103/PhysRevLett.78.1984 ↗
66. 10.1103/PhysRevLett.90.23640110.1103/PhysRevLett.90.236401 ↗
67. 10.1103/PhysRevB.53.1400410.1103/PhysRevB.53.14004 ↗