Giant interfacial perpendicular magnetic anisotropy in Fe/CuInGaSe beyond Fe/MgO
arXiv:1707.02694 · doi:10.1103/PhysRevB.96.174401
Abstract
We study interfacial magnetocrystalline anisotropies in various Fe/semiconductor heterostructures by means of first-principles calculations. We find that many of those systems show perpendicular magnetic anisotropy (PMA) with a positive value of the interfacial anisotropy constant . In particular, the Fe/CuInSe interface has a large of , which is about 1.6 times larger than that of Fe/MgO known as a typical system with relatively large PMA. We also find that the values of in almost all the systems studied in this work follow the well-known Bruno's relation, which indicates that minority-spin states around the Fermi level provide dominant contributions to the interfacial magnetocrystalline anisotropies. Detailed analyses of the local density of states and wave-vector-resolved anisotropy energy clarify that the large in Fe/CuInSe is attributed to the preferable -orbital configurations around the Fermi level in the minority-spin states of the interfacial Fe atoms. Moreover, we have shown that the locations of interfacial Se atoms are the key for such orbital configurations of the interfacial Fe atoms.
8 pages, 8 figures, 1 table