journal article·2016-09-09

Itinerant magnetic phases and quantum Lifshitz transitions in a three-dimensional repulsively interacting Fermi gas with spin-orbit coupling

Shang-Shun Zhang, Jinwu Ye, Wu-Ming Liu

Physical Review B· Volume 94· Issue 11
Publisher page

Abstract

Magnetic phenomena in itinerant electron systems have been at the forefront of materials science. Here we show that the Weyl spin-orbit coupling (SOC) in three-dimensional repulsively interacting itinerant Fermi systems opens up a platform to host new itinerant magnetic phases, excitations, and phase transitions. A putative ferromagnetic state (FM) is always unstable against a stripe spiral spin density wave (S-SDW) or a stripe longitudinal SDW (LSDW) at small or large SOC strengths, respectively. The stripe-ordering wave vector is given by the nesting momentum of the two SOC-split Fermi surfaces with the same or opposite helicities at small or large SOC strengths, respectively. The LSDW is accompanied by a charge density wave (CDW) with half of its pitch. The transition from the paramagnet to the SSDW or LSDW+CDW is described by quantum Lifshitz-type actions, in sharp contrast to the Hertz-Millis types for itinerant electron systems without SOC. The collective excitations and Fermi surface reconstructions inside the SSDW and LSDW+CDW are also studied. The effects of a harmonic trap in cold-atom experiments are briefly discussed. In view of recent ground-breaking experimental advances in generating two-dimensional SOC in cold atoms, these phenomena can be observed in current or near-future cold-atom experiments even at very weak interactions. They may also be relevant to some itinerant magnetic materials with a strong SOC.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Cold Atom Physics and Bose-Einstein Condensates · Advanced Condensed Matter Physics · Physics of Superconductivity and Magnetism

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

References (70)

Show source-provided references
1. 10.1103/PhysRevLett.83.373710.1103/PhysRevLett.83.3737 ↗
2. 10.1103/RevModPhys.82.304510.1103/RevModPhys.82.3045 ↗
3. 10.1103/RevModPhys.83.105710.1103/RevModPhys.83.1057 ↗
4. 10.1038/nature0988710.1038/nature09887 ↗
5. 10.1103/PhysRevLett.109.09530110.1103/PhysRevLett.109.095301 ↗
6. 10.1103/PhysRevLett.109.09530210.1103/PhysRevLett.109.095302 ↗
7. 10.1103/RevModPhys.83.152310.1103/RevModPhys.83.1523 ↗
8. 10.1038/ncomms1089710.1038/ncomms10897 ↗
9. 10.1038/nphys367210.1038/nphys3672 ↗
10. 10.1103/PhysRevLett.116.03530110.1103/PhysRevLett.116.035301 ↗
11. 10.1103/PhysRevB.83.09451510.1103/PhysRevB.83.094515 ↗
12. 10.1103/PhysRevB.84.01451210.1103/PhysRevB.84.014512 ↗
13. 10.1103/PhysRevA.90.05360310.1103/PhysRevA.90.053603 ↗
14. 10.1103/PhysRevB.85.20512610.1103/PhysRevB.85.205126 ↗
15. 10.1103/PhysRevA.87.06362310.1103/PhysRevA.87.063623 ↗
16. 10.1038/srep0211910.1038/srep02119 ↗
17. 10.1103/PhysRevA.92.04360910.1103/PhysRevA.92.043609 ↗
18. 10.1103/PhysRevB.94.02440910.1103/PhysRevB.94.024409 ↗
19. 10.1080/1478644330946224110.1080/14786443309462241 ↗
20. 10.1103/PhysRevB.14.116510.1103/PhysRevB.14.1165 ↗
21. 10.1103/PhysRevB.48.718310.1103/PhysRevB.48.7183 ↗
22. 10.1103/PhysRevB.51.899610.1103/PhysRevB.51.8996 ↗
23. 10.1103/PhysRevB.57.142210.1103/PhysRevB.57.1422 ↗
24. 10.1103/RevModPhys.75.120110.1103/RevModPhys.75.1201 ↗
25. 10.1016/j.nuclphysb.2008.06.01710.1016/j.nuclphysb.2008.06.017 ↗
26. 10.1126/science.117711210.1126/science.1177112 ↗
27. 10.1103/PhysRevLett.95.23040310.1103/PhysRevLett.95.230403 ↗
28. 10.1103/PhysRevLett.106.05040210.1103/PhysRevLett.106.050402 ↗
29. 10.1103/PhysRevLett.105.03040510.1103/PhysRevLett.105.030405 ↗
30. 10.1103/PhysRevLett.106.01040210.1103/PhysRevLett.106.010402 ↗
31. 10.1103/PhysRevLett.108.24040410.1103/PhysRevLett.108.240404 ↗
32. 10.1038/nature0647310.1038/nature06473 ↗
33. 10.1038/nature0824410.1038/nature08244 ↗
34. 10.1126/science.110922010.1126/science.1109220 ↗
35. 10.1126/science.121498710.1126/science.1214987 ↗
36. 10.1103/PhysRevLett.82.87110.1103/PhysRevLett.82.871 ↗
37. 10.1103/PhysRevLett.82.456910.1103/PhysRevLett.82.4569 ↗
38. 10.1103/PhysRevLett.83.287610.1103/PhysRevLett.83.2876 ↗
39. 10.1103/PhysRevLett.88.12040710.1103/PhysRevLett.88.120407 ↗
40. 10.1103/PhysRevLett.101.13530110.1103/PhysRevLett.101.135301 ↗
41. 10.1038/nphys147610.1038/nphys1476 ↗
42. 10.1103/PhysRevA.83.05160410.1103/PhysRevA.83.051604 ↗
43. 10.1016/j.aop.2012.09.00610.1016/j.aop.2012.09.006 ↗
44. 10.1103/PhysRevA.87.06363410.1103/PhysRevA.87.063634 ↗
45. 10.1103/PhysRevLett.108.23530110.1103/PhysRevLett.108.235301 ↗
46. S. A. Brazovskii · Sov. Phys. JETP · 1975 · 41 · 85
47. P. M. Chaikin · 199510.1017/CBO9780511813467 ↗
48. 10.1103/PhysRevB.76.18410410.1103/PhysRevB.76.184104 ↗
49. 10.1103/PhysRevLett.97.12530210.1103/PhysRevLett.97.125302 ↗
50. 10.1209/0295-5075/82/1600110.1209/0295-5075/82/16001 ↗
51. 10.1007/s10909-010-0184-510.1007/s10909-010-0184-5 ↗
52. 10.1007/s10909-012-0657-910.1007/s10909-012-0657-9 ↗
53. 10.1103/PhysRevLett.98.23680210.1103/PhysRevLett.98.236802 ↗
54. 10.1103/PhysRevLett.97.23680310.1103/PhysRevLett.97.236803 ↗
55. 10.1016/j.aop.2007.06.00610.1016/j.aop.2007.06.006 ↗
56. 10.1007/s10909-009-0056-z10.1007/s10909-009-0056-z ↗
57. 10.1103/PhysRevA.84.02361110.1103/PhysRevA.84.023611 ↗
58. 10.1103/RevModPhys.66.110.1103/RevModPhys.66.1 ↗
59. 10.1007/s00257005039910.1007/s002570050399 ↗
60. 10.1103/PhysRevB.69.03511110.1103/PhysRevB.69.035111 ↗
61. 10.1103/PhysRevLett.105.15160210.1103/PhysRevLett.105.151602 ↗
62. 10.1103/PhysRevB.44.1017310.1103/PhysRevB.44.10173 ↗
63. 10.1103/PhysRevB.65.21450510.1103/PhysRevB.65.214505 ↗
64. 10.1103/PhysRevLett.10.15910.1103/PhysRevLett.10.159 ↗
65. 10.1103/PhysRev.137.A172610.1103/PhysRev.137.A1726 ↗
66. 10.1143/PTP.30.27510.1143/PTP.30.275 ↗
67. 10.1103/PhysRevB.49.1326710.1103/PhysRevB.49.13267 ↗
68. A. Auerbach · 199410.1007/978-1-4612-0869-3 ↗
69. 10.1063/1.294589310.1063/1.2945893 ↗
70. S. Sachdev · 1999