Off-stoichiometry effect on magnetic damping in thin films of Heusler alloy Co2MnSi
Source abstract
Abstract
We investigated the effect of off-stoichiometry on the Gilbert magnetic damping constant (\ensuremath{\alpha}) of Heusler alloy $\mathrm{C}{\mathrm{o}}2\mathrm{MnSi}$ (CMS) thin films by employing time-resolved magneto-optical Kerr effect (TR-MOKE) measurements along with first-principles calculations based on the linear-response theory for magnetic damping. Because of the contribution of extrinsic damping arising from two-magnon scattering, the effective \ensuremath{\alpha} (${\ensuremath{\alpha}}_{\mathrm{eff}}$) extracted from the TR-MOKE responses showed dependences on the in-plane magnetic-field angle (${\ensuremath{\theta}}_{\mathrm{H}}$) and the field strength ($H$). Then, we obtained the smallest ${\ensuremath{\alpha}}_{\mathrm{eff}}$ (${\ensuremath{\alpha}}0$) for each sample under the most reduced contribution from two-magnon scattering realized through varying ${\ensuremath{\theta}}_{\mathrm{H}}$ and $H$ values, which is the closest value to \ensuremath{\alpha}. The thus obtained ${\ensuremath{\alpha}}0$ values of epitaxially grown off-stoichiometric $\mathrm{C}{\mathrm{o}}2\mathrm{M}{\mathrm{n}}_{\ensuremath{\beta}}\mathrm{S}{\mathrm{i}}_{\ensuremath{\gamma}}$ ($\ensuremath{\gamma}=0.82$) films with various (Mn + Si) compositions, $(\ensuremath{\beta}+\ensuremath{\gamma})$, decreased with increasing $(\ensuremath{\beta}+\ensuremath{\gamma})$ from ${\ensuremath{\alpha}}0=0.0057$ for (Mn + Si)-deficient $(\ensuremath{\beta}+\ensuremath{\gamma})=1.44$ to ${\ensuremath{\alpha}}0=0.0036$ for $(\ensuremath{\beta}+\ensuremath{\gamma})=1.90$ being close to the stoichiometric one of $(\ensuremath{\beta}+\ensuremath{\gamma})=2.0$ at 300 K. It was also demonstrated that a half-metallic (Mn+Si)-rich CMS film with $\ensuremath{\beta}=1.30$ and $\ensuremath{\gamma}=0.90$ showed a low ${\ensuremath{\alpha}}0$ of 0.0035. The dependence of ${\ensuremath{\alpha}}0$ on $(\ensuremath{\beta}+\ensuremath{\gamma})$ in $\mathrm{C}{\mathrm{o}}2\mathrm{M}{\mathrm{n}}_{\ensuremath{\beta}}\mathrm{S}{\mathrm{i}}_{\ensuremath{\gamma}}$ ($\ensuremath{\gamma}=0.82$) was well explained by the first-principles calculations. Through the systematic investigations of off-stoichiometric CMS with various values of $(\ensuremath{\beta}+\ensuremath{\gamma})$, it was clarified that the total density of states (DOS) at the Fermi level, $D({E}_{\mathrm{F}})$, plays the key role for determining the damping constant of CMS. Furthermore, it was revealed that the reduced minority-spin DOS at ${E}_{\mathrm{F}}$, caused by decreasing harmful $\mathrm{C}{\mathrm{o}}_{\mathrm{Mn}}$ antisites, is essential for reducing the damping constant of CMS. These findings demonstrate that appropriately controlling off-stoichiometry and film composition is thus promising for achieving half-metallicity and a low \ensuremath{\alpha} simultaneously for CMS thin films.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Heusler alloys: electronic and magnetic properties · Magnetic properties of thin films · Magnetic Properties and Applications
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (94)
Show source-provided references
1. 10.1103/RevModPhys.76.32310.1103/RevModPhys.76.323 ↗
2. 10.1103/PhysRevLett.50.202410.1103/PhysRevLett.50.2024 ↗
3. 10.1016/j.progsolidstchem.2011.02.00110.1016/j.progsolidstchem.2011.02.001 ↗
4. 10.1103/PhysRevB.28.174510.1103/PhysRevB.28.1745 ↗
5. 10.1143/JPSJ.64.215210.1143/JPSJ.64.2152 ↗
6. 10.1103/PhysRevB.66.09442110.1103/PhysRevB.66.094421 ↗
7. 10.1103/PhysRevB.66.17442910.1103/PhysRevB.66.174429 ↗
8. 10.1016/S0022-3697(71)80180-410.1016/S0022-3697(71)80180-4 ↗
9. 10.1063/1.216286710.1063/1.2162867 ↗
10. 10.1063/1.237839710.1063/1.2378397 ↗
11. 10.1063/1.327292610.1063/1.3272926 ↗
12. 10.1088/0953-8984/22/16/16421210.1088/0953-8984/22/16/164212 ↗
13. 10.1103/PhysRevB.81.14040210.1103/PhysRevB.81.140402 ↗
14. 10.1063/1.475577310.1063/1.4755773 ↗
15. 10.1103/PhysRevB.89.01442810.1103/PhysRevB.89.014428 ↗
16. 10.1088/0022-3727/48/16/16400110.1088/0022-3727/48/16/164001 ↗
17. 10.1103/PhysRevB.93.13440310.1103/PhysRevB.93.134403 ↗
18. 10.1063/1.299064710.1063/1.2990647 ↗
19. 10.1103/PhysRevB.82.09444410.1103/PhysRevB.82.094444 ↗
20. 10.1063/1.500024410.1063/1.5000244 ↗
21. 10.1103/PhysRevB.78.12130310.1103/PhysRevB.78.121303 ↗
22. 10.1103/PhysRevB.87.23520510.1103/PhysRevB.87.235205 ↗
23. 10.1063/1.481727010.1063/1.4817270 ↗
24. 10.1103/PhysRevB.91.14041010.1103/PhysRevB.91.140410 ↗
25. 10.1038/ncomms497410.1038/ncomms4974 ↗
26. 10.1016/0304-8853(96)00062-510.1016/0304-8853(96)00062-5 ↗
27. 10.1038/nmat331110.1038/nmat3311 ↗
28. 10.1139/p70-36110.1139/p70-361 ↗
29. 10.1007/BF0158762110.1007/BF01587621 ↗
30. 10.1103/PhysRevB.76.13441610.1103/PhysRevB.76.134416 ↗
31. 10.1103/PhysRevLett.99.02720410.1103/PhysRevLett.99.027204 ↗
32. 10.1103/PhysRevLett.101.03720710.1103/PhysRevLett.101.037207 ↗
33. 10.1103/PhysRevLett.107.06660310.1103/PhysRevLett.107.066603 ↗
34. 10.1103/PhysRevB.87.01443010.1103/PhysRevB.87.014430 ↗
35. 10.1143/JJAP.45.388910.1143/JJAP.45.3889 ↗
36. 10.1103/PhysRevLett.98.11760110.1103/PhysRevLett.98.117601 ↗
37. 10.1063/1.484537510.1063/1.4845375 ↗
38. 10.1038/nphys377010.1038/nphys3770 ↗
39. 10.1063/1.306760710.1063/1.3067607 ↗
40. 10.1063/1.310598210.1063/1.3105982 ↗
41. 10.1103/PhysRevB.81.09440210.1103/PhysRevB.81.094402 ↗
42. 10.1088/0022-3727/46/19/19500110.1088/0022-3727/46/19/195001 ↗
43. 10.1063/1.482465410.1063/1.4824654 ↗
44. 10.1063/1.489394910.1063/1.4893949 ↗
45. 10.1063/1.490079210.1063/1.4900792 ↗
46. 10.1088/0022-3727/48/16/16401210.1088/0022-3727/48/16/164012 ↗
47. 10.1103/PhysRevB.92.05443310.1103/PhysRevB.92.054433 ↗
48. 10.1088/0022-3727/49/6/06500510.1088/0022-3727/49/6/065005 ↗
49. 10.1103/PhysRevB.93.09441010.1103/PhysRevB.93.094410 ↗
50. 10.1103/PhysRevB.93.09441710.1103/PhysRevB.93.094417 ↗
51. 10.1063/1.496070510.1063/1.4960705 ↗
52. 10.1103/PhysRevB.97.09442010.1103/PhysRevB.97.094420 ↗
53. 10.1063/1.503034110.1063/1.5030341 ↗
54. 10.1063/1.315726710.1063/1.3157267 ↗
55. 10.1088/0022-3727/48/16/16401110.1088/0022-3727/48/16/164011 ↗
56. 10.1103/PhysRevB.95.09442510.1103/PhysRevB.95.094425 ↗
57. 10.1103/PhysRevB.69.09442310.1103/PhysRevB.69.094423 ↗
58. 10.1103/PhysRevB.69.14441310.1103/PhysRevB.69.144413 ↗
59. 10.1103/PhysRevB.94.09442810.1103/PhysRevB.94.094428 ↗
60. 10.1103/PhysRevB.85.06440710.1103/PhysRevB.85.064407 ↗
61. 10.1103/PhysRevB.82.18441910.1103/PhysRevB.82.184419 ↗
62. 10.1103/PhysRevB.86.14441210.1103/PhysRevB.86.144412 ↗
63. 10.1063/1.492153810.1063/1.4921538 ↗
64. 10.1007/s00339-013-7565-y10.1007/s00339-013-7565-y ↗
65. 10.1103/PhysRevB.89.12511610.1103/PhysRevB.89.125116 ↗
66. 10.1088/0022-3727/48/16/16400210.1088/0022-3727/48/16/164002 ↗
67. 10.1088/0022-3727/49/19/19500210.1088/0022-3727/49/19/195002 ↗
68. 10.1063/1.33499110.1063/1.334991 ↗
69. 10.1103/PhysRevB.85.05441210.1103/PhysRevB.85.054412 ↗
70. 10.1103/PhysRevLett.88.22720110.1103/PhysRevLett.88.227201 ↗
71. 10.1103/PhysRevLett.95.03740110.1103/PhysRevLett.95.037401 ↗
72. 10.1063/1.284375610.1063/1.2843756 ↗
73. 10.1016/j.jmmm.2009.09.05910.1016/j.jmmm.2009.09.059 ↗
74. 10.1109/TMAG.2006.87885010.1109/TMAG.2006.878850 ↗
75. 10.1088/0034-4885/74/9/09650110.1088/0034-4885/74/9/096501 ↗
76. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
77. 10.1103/PhysRevB.79.09440710.1103/PhysRevB.79.094407 ↗
78. L. D. Landau · 1967
79. 10.1109/TMAG.2004.83674010.1109/TMAG.2004.836740 ↗
80. 10.1063/1.190093910.1063/1.1900939 ↗
81. 10.1103/PhysRevB.60.739510.1103/PhysRevB.60.7395 ↗
82. 10.1103/PhysRevLett.90.22760110.1103/PhysRevLett.90.227601 ↗
83. 10.1103/PhysRevB.81.17441410.1103/PhysRevB.81.174414 ↗
84. 10.1038/s41567-018-0053-810.1038/s41567-018-0053-8 ↗
85. 10.1103/PhysRevB.73.14442410.1103/PhysRevB.73.144424 ↗
86. 10.1103/PhysRevB.76.10441610.1103/PhysRevB.76.104416 ↗
87. 10.1103/PhysRevB.87.18443110.1103/PhysRevB.87.184431 ↗
88. 10.1103/PhysRevB.67.20542110.1103/PhysRevB.67.205421 ↗
89. 10.1063/1.491890910.1063/1.4918909 ↗
90. 10.1103/PhysRevLett.88.11760110.1103/PhysRevLett.88.117601 ↗
91. 10.1103/PhysRevB.66.22440310.1103/PhysRevB.66.224403 ↗
92. 10.1103/PhysRevB.77.16511710.1103/PhysRevB.77.165117 ↗
93. 10.1063/1.144729410.1063/1.1447294 ↗
94. 10.1103/PhysRevB.91.16513210.1103/PhysRevB.91.165132 ↗