Accurate magneto-optical determination of radius of topological nodal-ring semimetals
Source abstract
Abstract
The shape of the Fermi surface of topological nodal-ring semimetals at low carrier concentrations is characterized by the ring radius $b/\ensuremath{\hbar}{v}F$. This peculiar topological property may not have a clear signature in measurable physical quantities. We demonstrate an accurate and definitive method to determine the radius of topological nodal-ring semimetals. Under a magnetic field along the ring axis, the axial magneto-optical response (${\ensuremath{\sigma}}zz$) has a giant peak. The position of this ultrastrong response is at the frequency of exactly $2b$ and is independent of the strength of the magnetic field. The amplitude of the peak response is many times stronger than that of any other inter-Landau level transitions if the magnetic energy is greater than $b$ and is similar strength if $b$ is greater than the magnetic energy. The origin of the ultrastrong response is that the axial magnetic transition is governed by selection rules completely different to those governing ${\ensuremath{\sigma}}xx$ where the giant response is absent [R. Y. Chen et al., Phys. Rev. Lett. 115, 176404 (2015)]. The present work provides a method to accurately determine parameters of the topological properties of semimetals.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Topological Materials and Phenomena · Graphene research and applications · 2D Materials and Applications
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (55)
Show source-provided references
1. T. T. Heikkilä · Pisma Zh. Eksp. Teor. Fiz. · 2011 · 93 · 63
2. 10.1134/S002136401102007X10.1134/S002136401102007X ↗
3. 10.1103/PhysRevB.84.23512610.1103/PhysRevB.84.235126 ↗
4. 10.1038/ncomms1169610.1038/ncomms11696 ↗
5. 10.1038/s41535-017-0074-z10.1038/s41535-017-0074-z ↗
6. 10.1103/RevModPhys.88.03500510.1103/RevModPhys.88.035005 ↗
7. 10.1146/annurev-conmatphys-031016-02522510.1146/annurev-conmatphys-031016-025225 ↗
8. 10.1146/annurev-conmatphys-031016-02545810.1146/annurev-conmatphys-031016-025458 ↗
9. 10.1103/RevModPhys.90.01500110.1103/RevModPhys.90.015001 ↗
10. 10.1007/s11467-016-0630-110.1007/s11467-016-0630-1 ↗
11. 10.1103/PhysRevB.92.08120110.1103/PhysRevB.92.081201 ↗
12. 10.1088/1674-1056/25/11/11710610.1088/1674-1056/25/11/117106 ↗
13. 10.1080/23746149.2017.141463110.1080/23746149.2017.1414631 ↗
14. 10.1103/PhysRevLett.115.03680610.1103/PhysRevLett.115.036806 ↗
15. 10.1103/PhysRevB.93.20513210.1103/PhysRevB.93.205132 ↗
16. 10.1103/PhysRevB.93.04520110.1103/PhysRevB.93.045201 ↗
17. 10.1103/PhysRevLett.120.14660210.1103/PhysRevLett.120.146602 ↗
18. 10.1103/PhysRevB.97.16511810.1103/PhysRevB.97.165118 ↗
19. 10.1103/PhysRevB.97.20510710.1103/PhysRevB.97.205107 ↗
20. 10.1103/PhysRevLett.117.01660210.1103/PhysRevLett.117.016602 ↗
21. 10.1103/PhysRevLett.121.25660210.1103/PhysRevLett.121.256602 ↗
22. 10.1016/j.scib.2018.04.01110.1016/j.scib.2018.04.011 ↗
23. 10.1103/PhysRevB.92.04512610.1103/PhysRevB.92.045126 ↗
24. 10.1103/PhysRevLett.115.02640310.1103/PhysRevLett.115.026403 ↗
25. 10.1103/PhysRevB.97.16510410.1103/PhysRevB.97.165104 ↗
26. 10.1140/epjb/e2018-80717-510.1140/epjb/e2018-80717-5 ↗
27. 10.1103/PhysRevLett.121.16680210.1103/PhysRevLett.121.166802 ↗
28. 10.1103/PhysRevB.95.07513810.1103/PhysRevB.95.075138 ↗
29. 10.1103/PhysRevB.96.23510310.1103/PhysRevB.96.235103 ↗
30. 10.1103/PhysRevB.98.07511510.1103/PhysRevB.98.075115 ↗
31. 10.1103/PhysRevB.97.11520410.1103/PhysRevB.97.115204 ↗
32. 10.1103/PhysRevB.97.16111310.1103/PhysRevB.97.161113 ↗
33. 10.1103/PhysRevLett.120.14660110.1103/PhysRevLett.120.146601 ↗
34. 10.1103/PhysRevB.97.23541810.1103/PhysRevB.97.235418 ↗
35. 10.1103/PhysRevB.95.23510410.1103/PhysRevB.95.235104 ↗
36. 10.1103/PhysRevB.96.04111310.1103/PhysRevB.96.041113 ↗
37. 10.1103/PhysRevB.95.07542610.1103/PhysRevB.95.075426 ↗
38. 10.1103/PhysRevB.84.06050410.1103/PhysRevB.84.060504 ↗
39. 10.1103/PhysRevB.93.02050610.1103/PhysRevB.93.020506 ↗
40. 10.1103/PhysRevB.95.06050610.1103/PhysRevB.95.060506 ↗
41. 10.1103/PhysRevB.95.09450210.1103/PhysRevB.95.094502 ↗
42. 10.1103/PhysRevLett.113.04640110.1103/PhysRevLett.113.046401 ↗
43. 10.1126/science.aaa929710.1126/science.aaa9297 ↗
44. 10.1103/PhysRevLett.113.18720210.1103/PhysRevLett.113.187202 ↗
45. 10.1103/PhysRevB.87.24513110.1103/PhysRevB.87.245131 ↗
46. 10.1103/PhysRevB.96.08514710.1103/PhysRevB.96.085147 ↗
47. 10.1103/PhysRevB.94.22430510.1103/PhysRevB.94.224305 ↗
48. 10.1103/PhysRevB.96.15515010.1103/PhysRevB.96.155150 ↗
49. 10.1088/1361-648X/29/4/04530110.1088/1361-648X/29/4/045301 ↗
50. 10.1103/PhysRevB.95.21420310.1103/PhysRevB.95.214203 ↗
51. 10.1103/PhysRevLett.119.14740210.1103/PhysRevLett.119.147402 ↗
52. 10.1103/PhysRevLett.115.17640410.1103/PhysRevLett.115.176404 ↗
53. 10.1140/epjb/e2017-70739-x10.1140/epjb/e2017-70739-x ↗
54. 10.1103/PhysRevB.86.08514910.1103/PhysRevB.86.085149 ↗
55. 10.1103/PhysRevB.93.08513810.1103/PhysRevB.93.085138 ↗