journal article·2019-12-24

Nonlinear domain-mode ferromagnetic resonances in garnet films with perpendicular anisotropy

N. Vukadinovic, J. Ben Youssef

Physical Review B· Volume 100· Issue 22
Publisher page

Abstract

The zero-field domain-mode ferromagnetic resonances (DM-FMRs) in the weakly nonlinear regime have been investigated for garnet films with a perpendicular anisotropy supporting parallel stripe domains by means of broadband microwave measurements, and analytical and numerical approaches. First, the perpendicular ferromagnetic resonance (FMR) in the saturated state is considered as a reference case. A redshift of the resonance frequency and a broadening of the resonance line are experimentally observed for increasing the input microwave power. These power-dependent characteristics are nicely reproduced by an analytical model taking into account the linear polarization of the pumping field and a nonlinear Gilbert-type damping parameter. Then, the effect of the stripe domain pattern is analyzed. A redshift and a line broadening are also experimentally revealed both for the acoustic and the optical modes with an anisotropic character between the two modes. Numerical simulations based on the DM-FMR model extended in the nonlinear regime and including a nonlinear Gilbert-type damping parameter account quantitatively for the power dependences of the DM resonance frequency shifts and the DM resonance linewidths. These results highlight the requirement of a nonlinear damping term for explaining the FMR and DM-FMR spectra in the weakly nonlinear regime within the framework of the phenomenological approach of magnetization dynamics.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Magneto-Optical Properties and Applications · Magnetic properties of thin films · Photonic Crystals and Applications

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

References (55)

Show source-provided references
1. J. Smit · Philips. Res. Rep. · 1955 · 10 · 113
2. 10.1103/PhysRev.105.6210.1103/PhysRev.105.62 ↗
3. 10.1002/pssa.221051011610.1002/pssa.2210510116 ↗
4. 10.1063/1.33071010.1063/1.330710 ↗
5. 10.1109/TMAG.1982.106203110.1109/TMAG.1982.1062031 ↗
6. 10.1016/0304-8853(88)90058-310.1016/0304-8853(88)90058-3 ↗
7. 10.1007/BF0033175810.1007/BF00331758 ↗
8. 10.1016/0304-8853(95)00118-210.1016/0304-8853(95)00118-2 ↗
9. 10.1002/pssa.221157011710.1002/pssa.2211570117 ↗
10. 10.1103/PhysRevB.79.18440510.1103/PhysRevB.79.184405 ↗
11. 10.1103/PhysRevB.85.18441810.1103/PhysRevB.85.184418 ↗
12. 10.1063/1.36487710.1063/1.364877 ↗
13. 10.1103/PhysRevB.69.17440210.1103/PhysRevB.69.174402 ↗
14. 10.1103/PhysRevB.63.17443710.1103/PhysRevB.63.174437 ↗
15. 10.1063/1.217254410.1063/1.2172544 ↗
16. 10.1103/PhysRevLett.94.05720210.1103/PhysRevLett.94.057202 ↗
17. 10.1103/PhysRevLett.94.21720410.1103/PhysRevLett.94.217204 ↗
18. 10.1103/PhysRevB.76.22440110.1103/PhysRevB.76.224401 ↗
19. 10.1103/PhysRevB.89.21441210.1103/PhysRevB.89.214412 ↗
20. 10.1103/PhysRevB.75.01442010.1103/PhysRevB.75.014420 ↗
21. 10.1103/PhysRevB.78.18441110.1103/PhysRevB.78.184411 ↗
22. 10.1103/RevModPhys.25.8910.1103/RevModPhys.25.89 ↗
23. 10.1063/1.32491610.1063/1.324916 ↗
24. 10.1063/1.32709410.1063/1.327094 ↗
25. 10.1016/0022-3697(57)90010-010.1016/0022-3697(57)90010-0 ↗
26. 10.1103/PhysRevB.75.01444010.1103/PhysRevB.75.014440 ↗
27. 10.1103/PhysRevB.92.21440810.1103/PhysRevB.92.214408 ↗
28. 10.1063/1.165523210.1063/1.1655232 ↗
29. 10.1016/0304-8853(90)90100-510.1016/0304-8853(90)90100-5 ↗
30. C. Kooy · Philips Res. Rep. · 1960 · 15 · 7
31. 10.1103/PhysRevB.71.01441010.1103/PhysRevB.71.014410 ↗
32. 10.1109/20.80914410.1109/20.809144 ↗
33. 10.15407/ujpe59.02.014110.15407/ujpe59.02.0141 ↗
34. 10.1063/1.33898810.1063/1.338988 ↗
35. 10.1016/0304-8853(91)90635-N10.1016/0304-8853(91)90635-N ↗
36. V. S. L'vov · 1994
37. G. V. Skrotskii · Sov. Phys. JETP · 1959 · 35 · 1035
38. 10.1103/PhysRevLett.86.72410.1103/PhysRevLett.86.724 ↗
39. 10.1109/TMAG.2017.270264110.1109/TMAG.2017.2702641 ↗
40. A. G. Gurevich · 1996
41. 10.1103/PhysRevB.99.06440510.1103/PhysRevB.99.064405 ↗
42. 10.1063/1.169950310.1063/1.1699503 ↗
43. 10.1134/S106378501009017810.1134/S1063785010090178 ↗
44. 10.1063/1.32333910.1063/1.323339 ↗
45. 10.1007/BF0092820310.1007/BF00928203 ↗
46. 10.1134/1.113135410.1134/1.1131354 ↗
47. 10.1103/PhysRevLett.85.281710.1103/PhysRevLett.85.2817 ↗
48. 10.1016/0304-8853(75)90159-610.1016/0304-8853(75)90159-6 ↗
49. 10.1063/1.34235410.1063/1.342354 ↗
50. 10.1103/PhysRevB.91.06442610.1103/PhysRevB.91.064426 ↗
51. 10.1103/PhysRevB.80.18442210.1103/PhysRevB.80.184422 ↗
52. 10.1103/PhysRevB.75.14040510.1103/PhysRevB.75.140405 ↗
53. 10.1103/PhysRevB.96.02442110.1103/PhysRevB.96.024421 ↗
54. 10.1038/s41565-019-0429-710.1038/s41565-019-0429-7 ↗
55. A. I. Pil'shchikov · Sov. Phys. JETP · 1974 · 39 · 328