Shape of magnetic domain walls formed by coupling to mobile charges
Source abstract
Abstract
Magnetic domain walls, which are crucially important in both fundamental physics and technical applications, often have a preference in their form due to many different origins, such as the crystalline shape, lattice symmetry, and magnetic anisotropy. We theoretically investigate yet another origin stemming from the coupling to mobile charges in itinerant magnets. Performing a large-scale numerical simulation in a minimal model for itinerant magnets, i.e., the Kondo lattice model with classical localized spins, we show that the shape of magnetic domain walls depends on the electronic band structure and electron filling. While N\'eel and ${120}^{\ensuremath{\circ}}$ antiferromagnetic states do not show a strong preference in the shape of domain walls, noncoplanar spin states with scalar chiral ordering have distinct directional preferences of the domain walls depending on the electron filling. We find that the directional preference is rationalized by the wave-number dependence of the effective magnetic interactions induced by the mobile charges, which are set by the band structure and electron filling. We also observe that, in the noncoplanar chiral states, an electric current is induced along the domain walls owing to the spin Berry phase mechanism, with different spatial distributions depending on whether the bulk state is metallic or insulating.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Physics of Superconductivity and Magnetism · Advanced Condensed Matter Physics · Topological Materials and Phenomena
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (48)
Show source-provided references
1. 10.1103/RevModPhys.21.54110.1103/RevModPhys.21.541 ↗
2. S. Chikazumi · 199710.1093/oso/9780198517764.001.0001 ↗
3. 10.1063/1.171034410.1063/1.1710344 ↗
4. 10.1103/PhysRevB.51.985510.1103/PhysRevB.51.9855 ↗
5. 10.1103/PhysRevLett.77.158010.1103/PhysRevLett.77.1580 ↗
6. 10.1103/PhysRevLett.78.377310.1103/PhysRevLett.78.3773 ↗
7. 10.1103/PhysRevLett.79.511010.1103/PhysRevLett.79.5110 ↗
8. 10.1016/j.physrep.2008.07.00310.1016/j.physrep.2008.07.003 ↗
9. 10.1080/71371603310.1080/713716033 ↗
10. 10.1038/nmat237310.1038/nmat2373 ↗
11. 10.1103/PhysRevLett.92.07720510.1103/PhysRevLett.92.077205 ↗
12. 10.1038/nature0244110.1038/nature02441 ↗
13. 10.1016/0304-8853(96)00062-510.1016/0304-8853(96)00062-5 ↗
14. 10.1103/PhysRevB.83.17444710.1103/PhysRevB.83.174447 ↗
15. 10.1103/PhysRevLett.107.13680410.1103/PhysRevLett.107.136804 ↗
16. 10.1103/PhysRevB.54.935310.1103/PhysRevB.54.9353 ↗
17. 10.1103/PhysRevLett.95.02660110.1103/PhysRevLett.95.026601 ↗
18. 10.7566/JPSJ.84.08370110.7566/JPSJ.84.083701 ↗
19. 10.1103/PhysRevLett.114.14720510.1103/PhysRevLett.114.147205 ↗
20. 10.1103/PhysRevB.83.20510110.1103/PhysRevB.83.205101 ↗
21. 10.1103/PhysRevX.4.02103510.1103/PhysRevX.4.021035 ↗
22. 10.1103/PhysRevB.93.19514610.1103/PhysRevB.93.195146 ↗
23. 10.7566/JPSJ.82.02370610.7566/JPSJ.82.023706 ↗
24. 10.1103/PhysRevB.89.07512710.1103/PhysRevB.89.075127 ↗
25. 10.1103/PhysRevB.92.12111010.1103/PhysRevB.92.121110 ↗
26. 10.1126/science.aac828910.1126/science.aac8289 ↗
27. 10.1103/PhysRevB.88.23510110.1103/PhysRevB.88.235101 ↗
28. 10.1103/PhysRevLett.101.15640210.1103/PhysRevLett.101.156402 ↗
29. 10.1143/JPSJ.79.08371110.1143/JPSJ.79.083711 ↗
30. 10.1103/PhysRevLett.69.323210.1103/PhysRevLett.69.3232 ↗
31. 10.1103/PhysRevLett.83.373710.1103/PhysRevLett.83.3737 ↗
32. 10.1103/PhysRevLett.65.246210.1103/PhysRevLett.65.2462 ↗
33. 10.1103/PhysRev.82.40310.1103/PhysRev.82.403 ↗
34. 10.1103/PhysRev.100.67510.1103/PhysRev.100.675 ↗
35. 10.1103/PhysRev.96.9910.1103/PhysRev.96.99 ↗
36. 10.1143/PTP.16.4510.1143/PTP.16.45 ↗
37. 10.1103/PhysRev.106.89310.1103/PhysRev.106.893 ↗
38. 10.1103/RevModPhys.78.27510.1103/RevModPhys.78.275 ↗
39. 10.1002/nla.77910.1002/nla.779 ↗
40. L. D. Landau · Phys. Z. Sowjetunion · 1935 · 8 · 153
41. 10.1109/TMAG.2004.83674010.1109/TMAG.2004.836740 ↗
42. 10.1088/0953-8984/20/31/31520310.1088/0953-8984/20/31/315203 ↗
43. 10.1088/0953-8984/22/17/17600110.1088/0953-8984/22/17/176001 ↗
44. 10.1103/PhysRevLett.80.84510.1103/PhysRevLett.80.845 ↗
45. 10.1103/PhysRevLett.73.103910.1103/PhysRevLett.73.1039 ↗
46. 10.1103/PhysRevLett.108.09640110.1103/PhysRevLett.108.096401 ↗
47. 10.1103/PhysRevB.90.06040210.1103/PhysRevB.90.060402 ↗
48. 10.7566/JPSJ.83.07370610.7566/JPSJ.83.073706 ↗