Nematic Bogoliubov Fermi surfaces from magnetic toroidal order in FeSe 1 − x S x
Source abstract
Abstract
Recently it has been shown experimentally that the superconducting state of ${\mathrm{FeSe}}_{1\ensuremath{-}x}{\mathrm{S}}x$ exhibits Bogoliubov Fermi surfaces for $x>0.17$. These Bogoliubov Fermi surfaces appear together with broken time-reversal symmetry and surprisingly demonstrate nematic behavior in a structurally tetragonal phase. Here, through a comprehensive analysis that deduces the structure of Bogoliubov Fermi surfaces from all symmetry-allowed types of translation invariant broken time-reversal symmetry, we find that the origin of nematic Bogoliubov Fermi surfaces is due to magnetic toroidal order that belongs to an ${E}u$ irreducible representation of the ${D}4h$ point group. We further show that this magnetic toroidal order appears as a consequence of either static N\'eel antiferromagnetic order or due to the formation of a spontaneous pair density wave superconducting order. Finally, we reveal that independent of the presence of Bogoliubov Fermi surfaces, supercurrents will induce N\'eel magnetic order in many Fe-based superconductors.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Iron-based superconductors research · Physics of Superconductivity and Magnetism · Rare-earth and actinide compounds
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
University of Wisconsin–Milwaukee
Funding
U.S. Department of Energy · Basic Energy Sciences
References (70)
Show source-provided references
1. 10.1103/PhysRevLett.118.12700110.1103/PhysRevLett.118.127001 ↗
2. 10.1103/PhysRevB.98.22450910.1103/PhysRevB.98.224509 ↗
3. 10.1103/PhysRevB.102.02050110.1103/PhysRevB.102.020501 ↗
4. 10.1103/PhysRevB.102.02450510.1103/PhysRevB.102.024505 ↗
5. 10.1103/PhysRevB.104.09451810.1103/PhysRevB.104.094518 ↗
6. 10.1021/ja063355c10.1021/ja063355c ↗
7. 10.1073/pnas.080732510510.1073/pnas.0807325105 ↗
8. 10.7566/JPSJ.89.10200210.7566/JPSJ.89.102002 ↗
9. 10.3390/sym1209140210.3390/sym12091402 ↗
10. 10.3389/fphy.2020.59450010.3389/fphy.2020.594500 ↗
11. 10.1039/b813076k10.1039/b813076k ↗
12. 10.1016/j.ssc.2009.02.01110.1016/j.ssc.2009.02.011 ↗
13. 10.1103/PhysRevLett.103.05700210.1103/PhysRevLett.103.057002 ↗
14. 10.1143/JPSJ.78.07471210.1143/JPSJ.78.074712 ↗
15. 10.1038/ncomms575610.1038/ncomms5756 ↗
16. 10.1103/PhysRevB.92.12110810.1103/PhysRevB.92.121108 ↗
17. 10.1103/PhysRevB.92.23511310.1103/PhysRevB.92.235113 ↗
18. 10.1073/pnas.160580611310.1073/pnas.1605806113 ↗
19. 10.1073/pnas.171733111510.1073/pnas.1717331115 ↗
20. 10.1126/sciadv.aar641910.1126/sciadv.aar6419 ↗
21. 10.1038/s42005-023-01289-810.1038/s42005-023-01289-8 ↗
22. 10.1073/pnas.220827612010.1073/pnas.2208276120 ↗
23. 10.1103/PhysRevB.96.15510510.1103/PhysRevB.96.155105 ↗
24. 10.1103/PhysRevLett.125.23700410.1103/PhysRevLett.125.237004 ↗
25. 10.1103/PhysRevB.99.13451310.1103/PhysRevB.99.134513 ↗
26. 10.1103/PhysRevB.100.22450510.1103/PhysRevB.100.224505 ↗
27. 10.1103/PhysRevB.96.09452610.1103/PhysRevB.96.094526 ↗
28. 10.1038/s41467-020-14357-210.1038/s41467-020-14357-2 ↗
29. 10.1103/PhysRevB.102.06450410.1103/PhysRevB.102.064504 ↗
30. 10.1016/0370-1573(90)90042-Z10.1016/0370-1573(90)90042-Z ↗
31. 10.1088/0022-3727/38/8/R0110.1088/0022-3727/38/8/R01 ↗
32. 10.1103/PhysRevB.76.21440410.1103/PhysRevB.76.214404 ↗
33. 10.1088/0953-8984/20/43/43420310.1088/0953-8984/20/43/434203 ↗
34. 10.3367/UFNe.0179.200911d.117510.3367/UFNe.0179.200911d.1175 ↗
35. 10.1103/PhysRevB.90.02443210.1103/PhysRevB.90.024432 ↗
36. 10.1103/PhysRevB.92.09443110.1103/PhysRevB.92.094431 ↗
37. 10.1016/j.jssc.2018.12.03510.1016/j.jssc.2018.12.035 ↗
38. 10.7566/JPSJ.87.03370910.7566/JPSJ.87.033709 ↗
39. 10.1103/PhysRevB.98.16511010.1103/PhysRevB.98.165110 ↗
40. 10.1103/PhysRevB.106.02440510.1103/PhysRevB.106.024405 ↗
41. 10.1103/PhysRevB.105.15515710.1103/PhysRevB.105.155157 ↗
42. 10.1038/s41586-023-06072-x10.1038/s41586-023-06072-x ↗
43. 10.1038/ncomms1218210.1038/ncomms12182 ↗
44. 10.1038/s42005-019-0107-y10.1038/s42005-019-0107-y ↗
45. 10.1016/j.mattod.2020.07.00510.1016/j.mattod.2020.07.005 ↗
46. 10.1103/PhysRevB.91.05450210.1103/PhysRevB.91.054502 ↗
47. 10.1038/s42005-022-00804-710.1038/s42005-022-00804-7 ↗
48. 10.1103/PhysRevB.109.02450210.1103/PhysRevB.109.024502 ↗
49. I. Tamm · Phys. Z. Sowjetunion · 1932 · 1 · 733
50. 10.1038/nphys243810.1038/nphys2438 ↗
51. 10.1063/1.486555710.1063/1.4865557 ↗
52. 10.1103/RevModPhys.87.85510.1103/RevModPhys.87.855 ↗
53. 10.1016/j.matpr.2020.04.50310.1016/j.matpr.2020.04.503 ↗
54. 10.1038/s42005-018-0006-710.1038/s42005-018-0006-7 ↗
55. 10.1021/acsnano.3c0287610.1021/acsnano.3c02876 ↗
56. 10.1103/PhysRevLett.130.04670210.1103/PhysRevLett.130.046702 ↗
57. 10.1103/PhysRevLett.119.26700110.1103/PhysRevLett.119.267001 ↗
58. V. P. Mineev · Zh. Eksp. Teor. Fiz · 1994 · 105 · 747
59. 10.1088/1361-6633/80/3/03650110.1088/1361-6633/80/3/036501 ↗
60. 10.1073/pnas.211050111910.1073/pnas.2110501119 ↗
61. 10.1038/ncomms1284310.1038/ncomms12843 ↗
62. 10.1103/PhysRevB.106.18450710.1103/PhysRevB.106.184507 ↗
63. 10.1103/PhysRevLett.131.01600210.1103/PhysRevLett.131.016002 ↗
64. 10.1007/s11433-023-2122-410.1007/s11433-023-2122-4 ↗
65. 10.1038/s41467-023-38956-x10.1038/s41467-023-38956-x ↗
66. 10.1073/pnas.211954811910.1073/pnas.2119548119 ↗
67. 10.1088/1367-2630/ac676610.1088/1367-2630/ac6766 ↗
68. 10.1103/PhysRevLett.128.03700110.1103/PhysRevLett.128.037001 ↗
69. 10.1038/s41567-022-01699-510.1038/s41567-022-01699-5 ↗
70. 10.1103/PhysRevB.108.22450610.1103/PhysRevB.108.224506 ↗