Magnetocrystalline anisotropy of Fe and Co slabs and clusters onSrTiO3by first-principles
Source abstract
Abstract
In this paper, we present a detailed theoretical investigation of the electronic and magnetic properties of ferromagnetic slabs and clusters deposited on ${\mathrm{SrTiO}}3$ via first-principles calculations, with a particular emphasis on the magnetocrystalline anisotropy (MCA). We found that in the case of Fe ultrathin films deposited on ${\mathrm{SrTiO}}3$ the effect of the interface is to quench the MCA whereas for Co we observe a spin reorientation from in-plane to out-of-plane as compared to the free surface. We also find a strong enhancement of MCA for small clusters upon deposition on a ${\mathrm{SrTiO}}3$ substrate. The origin of this enhancement of MCA is attributed to the hybridization between the substrate and the $d$ orbitals of the cluster extending in-plane for Fe and out-of-plane for Co. As a consequence, we predict that the Fe nanocrystals (even rather small) should be magnetically stable and are thus good potential candidates for magnetic storage devices.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Magnetic and transport properties of perovskites and related materials · Electronic and Structural Properties of Oxides · Advanced Condensed Matter Physics
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (35)
Show source-provided references
1. 10.1063/1.306416210.1063/1.3064162 ↗
2. 10.1063/1.291316310.1063/1.2913163 ↗
3. 10.1063/1.326574010.1063/1.3265740 ↗
4. 10.1103/PhysRevLett.100.08720410.1103/PhysRevLett.100.087204 ↗
5. 10.1103/PhysRevLett.99.22660210.1103/PhysRevLett.99.226602 ↗
6. 10.1103/PhysRevLett.81.522910.1103/PhysRevLett.81.5229 ↗
7. 10.1103/PhysRevB.49.1288810.1103/PhysRevB.49.12888 ↗
8. 10.1103/PhysRevB.86.10443610.1103/PhysRevB.86.104436 ↗
9. 10.1063/1.148312210.1063/1.1483122 ↗
10. 10.1038/nmat280410.1038/nmat2804 ↗
11. 10.1103/PhysRevB.84.05440110.1103/PhysRevB.84.054401 ↗
12. 10.1126/science.125284110.1126/science.1252841 ↗
13. 10.1126/science.121413110.1126/science.1214131 ↗
14. 10.1126/science.125440210.1126/science.1254402 ↗
15. 10.1103/PhysRevB.88.21441310.1103/PhysRevB.88.214413 ↗
16. 10.1103/PhysRevB.90.20540910.1103/PhysRevB.90.205409 ↗
17. 10.1063/1.200837510.1063/1.2008375 ↗
18. 10.1088/0953-8984/21/39/39550210.1088/0953-8984/21/39/395502 ↗
19. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
20. 10.1103/PhysRevB.77.09411210.1103/PhysRevB.77.094112 ↗
21. 10.1103/PhysRevLett.82.428810.1103/PhysRevLett.82.4288 ↗
22. 10.1126/science.286.5439.50710.1126/science.286.5439.507 ↗
23. 10.1103/PhysRevB.65.02040110.1103/PhysRevB.65.020401 ↗
24. 10.1103/PhysRevB.88.18442310.1103/PhysRevB.88.184423 ↗
25. 10.1103/PhysRevLett.114.24720310.1103/PhysRevLett.114.247203 ↗
26. 10.1103/PhysRevB.38.802210.1103/PhysRevB.38.8022 ↗
27. 10.1103/PhysRevB.39.86510.1103/PhysRevB.39.865 ↗
28. 10.1103/PhysRevB.50.998910.1103/PhysRevB.50.9989 ↗
29. 10.1088/0953-8984/18/29/01810.1088/0953-8984/18/29/018 ↗
30. 10.1103/PhysRevLett.102.24720310.1103/PhysRevLett.102.247203 ↗
31. 10.1103/PhysRevB.86.18440710.1103/PhysRevB.86.184407 ↗
32. 10.1103/PhysRevB.48.1692910.1103/PhysRevB.48.16929 ↗
33. 10.1140/epjb/e2007-00043-510.1140/epjb/e2007-00043-5 ↗
34. 10.1103/PhysRevB.76.02441210.1103/PhysRevB.76.024412 ↗
35. 10.1103/PhysRevLett.115.25720110.1103/PhysRevLett.115.257201 ↗