Electric and spin current vortices in altermagnets
Source abstract
Abstract
Altermagnets are collinear magnets exhibiting momentum-dependent spin splitting and vanishing net magnetization. Using semiclassical Boltzmann and lattice Keldysh approaches, the authors demonstrate here that altermagnets support swirling electric and spin currents. The patterns of these currents are controlled by the relative orientation of altermagnetic nodal planes and sample boundaries. Unlike previous proposals considering the hydrodynamic transport regime, swirling currents appear even in the Ohmic regime and rely exclusively on altermagnetic spin splitting, with no swirls found in ferromagnets.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Magnetic properties of thin films · Magnetic Properties of Alloys · Advanced Condensed Matter Physics
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Bogolyubov Institute for Theoretical Physics
Norwegian University of Science and Technology
Taras Shevchenko National Kyiv University
University of Missouri
Funding
Norges Forskningsråd · Department of Physics and Astronomy of the NAS of Ukraine
References (75)
Show source-provided references
1. 10.1039/C5CP07806G10.1039/C5CP07806G ↗
2. 10.1126/sciadv.aaz880910.1126/sciadv.aaz8809 ↗
3. 10.7566/JPSJ.88.12370210.7566/JPSJ.88.123702 ↗
4. 10.1103/PhysRevB.99.18443210.1103/PhysRevB.99.184432 ↗
5. 10.1103/PhysRevB.102.01442210.1103/PhysRevB.102.014422 ↗
6. 10.1103/PhysRevMaterials.5.01440910.1103/PhysRevMaterials.5.014409 ↗
7. 10.1038/s41467-021-23127-710.1038/s41467-021-23127-7 ↗
8. 10.1103/PhysRevX.12.04050110.1103/PhysRevX.12.040501 ↗
9. 10.1103/PhysRevX.12.03104210.1103/PhysRevX.12.031042 ↗
10. 10.1103/PhysRevX.12.04000210.1103/PhysRevX.12.040002 ↗
11. 10.1002/adfm.20240932710.1002/adfm.202409327 ↗
12. 10.1038/s44306-024-00066-910.1038/s44306-024-00066-9 ↗
13. 10.1126/sciadv.adj488310.1126/sciadv.adj4883 ↗
14. 10.1038/s41586-023-06907-710.1038/s41586-023-06907-7 ↗
15. 10.1103/PhysRevLett.132.03670210.1103/PhysRevLett.132.036702 ↗
16. 10.1103/PhysRevB.109.11510210.1103/PhysRevB.109.115102 ↗
17. 10.1002/advs.20240652910.1002/advs.202406529 ↗
18. 10.1103/PhysRevLett.133.20640110.1103/PhysRevLett.133.206401 ↗
19. 10.1038/s41567-025-02864-210.1038/s41567-025-02864-2 ↗
20. 10.1038/s41567-025-02822-y10.1038/s41567-025-02822-y ↗
21. 10.1103/PhysRevLett.132.17670110.1103/PhysRevLett.132.176701 ↗
22. 10.1103/PhysRevLett.130.03670210.1103/PhysRevLett.130.036702 ↗
23. 10.1038/s41467-024-48493-w10.1038/s41467-024-48493-w ↗
24. 10.1103/PhysRevB.109.22443010.1103/PhysRevB.109.224430 ↗
25. 10.1103/PhysRevB.55.806010.1103/PhysRevB.55.8060 ↗
26. 10.1103/PhysRevB.102.07511210.1103/PhysRevB.102.075112 ↗
27. 10.1103/PhysRevApplied.15.02405710.1103/PhysRevApplied.15.024057 ↗
28. 10.1103/PhysRevLett.133.21660210.1103/PhysRevLett.133.216602 ↗
29. 10.1016/0022-3697(58)90076-310.1016/0022-3697(58)90076-3 ↗
30. 10.1103/PhysRev.120.9110.1103/PhysRev.120.91 ↗
31. 10.1002/adma.20250501910.1002/adma.202505019 ↗
32. 10.1038/s41467-019-12229-y10.1038/s41467-019-12229-y ↗
33. 10.1103/PhysRevLett.126.12770110.1103/PhysRevLett.126.127701 ↗
34. 10.1103/PhysRevLett.129.13720110.1103/PhysRevLett.129.137201 ↗
35. 10.1103/PhysRevB.110.04514710.1103/PhysRevB.110.045147 ↗
36. 10.1515/nanoph-2019-020910.1515/nanoph-2019-0209 ↗
37. 10.1103/RevModPhys.92.01500410.1103/RevModPhys.92.015004 ↗
38. A. P. Baddorf · 2007
39. 10.1103/PhysRevLett.55.179010.1103/PhysRevLett.55.1790 ↗
40. 10.1038/3506653310.1038/35066533 ↗
41. As we verify in Sec. S1.B.2 (see Supplemental Material [46]), a model with sublattice degrees of freedom leads to the same structure of the response tensor.
42. The spin-dependent effective chemical potential can be achieved by applying a weak magnetic field via the Zeeman term. In 2D systems, orbital effects can be ignored if the field is in the plane of the material.
43. 10.1103/PhysRevB.96.02040110.1103/PhysRevB.96.020401 ↗
44. See Supplemental Material at http://link.aps.org/supplemental/10.1103/3sw6-y8vf for the details of the calculations in the kinetic and Keldysh formalisms, the discussion of g- and i-wave altermagnets, analytical and numerical results for a ribbon with fixed current boundary conditions, and the discussion of the spin-flipping scattering, which includes Refs. [70, 71, 72, 73, 74, 75].
45. L. D. Landau · 2013
46. A different configuration of the contacts where the source and drain are located at the same surface is considered in the Supplemental Material [46].
47. Mathematica (Wolfram Research, Inc., Champaign, IL, 2025), https://www.wolfram.com/mathematica/.
48. M. I. D'Yakonov · Sov. J. Expt. Theor. Phys. Lett. · 1971 · 13 · 467
49. 10.1103/PhysRevLett.83.183410.1103/PhysRevLett.83.1834 ↗
50. 10.1109/TMAG.2013.226294710.1109/TMAG.2013.2262947 ↗
51. 10.1103/RevModPhys.77.137510.1103/RevModPhys.77.1375 ↗
52. 10.1038/s41586-020-2507-210.1038/s41586-020-2507-2 ↗
53. 10.1038/s41567-021-01341-w10.1038/s41567-021-01341-w ↗
54. 10.1038/s41586-022-05002-710.1038/s41586-022-05002-7 ↗
55. 10.1103/PhysRevLett.129.08770110.1103/PhysRevLett.129.087701 ↗
56. 10.1038/s41586-022-04794-y10.1038/s41586-022-04794-y ↗
57. 10.1142/9789811279461_000710.1142/9789811279461_0007 ↗
58. 10.1103/PhysRevB.73.07530310.1103/PhysRevB.73.075303 ↗
59. 10.1103/PhysRevB.111.17443110.1103/PhysRevB.111.174431 ↗
60. While the recent studies suggest that RuO2 is nonmagnetic [76, 77, 78], it may support altermagnetism in thin films due to strain [19, 79].
61. 10.1103/PhysRevX.12.01102810.1103/PhysRevX.12.011028 ↗
62. 10.1038/s41467-024-45951-310.1038/s41467-024-45951-3 ↗
63. 10.1103/PhysRevApplied.13.04404310.1103/PhysRevApplied.13.044043 ↗
64. 10.1038/s42254-021-00380-910.1038/s42254-021-00380-9 ↗
65. 10.1063/1.498652510.1063/1.4986525 ↗
66. 10.1038/nature0727910.1038/nature07279 ↗
67. 10.1103/PhysRevB.110.14441210.1103/PhysRevB.110.144412 ↗
68. 10.1103/3k12-246710.1103/3k12-2467 ↗
69. 10.1103/PhysRevLett.134.08670110.1103/PhysRevLett.134.086701 ↗
70. 10.1103/pbbr-hwz410.1103/pbbr-hwz4 ↗
71. 10.1126/science.aad020110.1126/science.aad0201 ↗
72. 10.1103/PhysRevB.92.16543310.1103/PhysRevB.92.165433 ↗
73. 10.1103/PhysRevLett.132.16670210.1103/PhysRevLett.132.166702 ↗
74. 10.1038/s44306-024-00055-y10.1038/s44306-024-00055-y ↗
75. 10.1088/1361-648X/adad2a10.1088/1361-648X/adad2a ↗