Hernando A, Crespo P, García M A
Instituto de Magnetismo Aplicado, RENFE-UCM-CSIC, and Departamento de Física de Materiales UCM, P.O. Box 155, Las Rozas, Madrid 28230, Spain.
Phys Rev Lett. 2006 Feb 10;96(5):057206. doi: 10.1103/PhysRevLett.96.057206. Epub 2006 Feb 7.
The origin of orbital magnetism recently observed in different nanostructured films and particles is discussed as a consequence of spin-orbit coupling. It is shown that contact potentials induced at the thin film surface by broken symmetries, as domain boundaries in self-assembled monolayers, lead to orbital states that in some cases are of large radius. The component of the angular momentum normal to the surface can reach very high values that decrease the total energy by decreasing spin-orbit interaction energy. Intraorbital ferromagnetic spin correlations induce orbital momenta alignment. The estimated values of the magnetic moments per atom are in good agreement with the experimental observations in thiol capped gold films and nanoparticles.
讨论了最近在不同纳米结构薄膜和颗粒中观察到的轨道磁性的起源,这是自旋轨道耦合的结果。结果表明,由对称性破缺(如自组装单分子层中的畴边界)在薄膜表面诱导的接触电势会导致在某些情况下具有大半径的轨道状态。垂直于表面的角动量分量可以达到非常高的值,通过降低自旋轨道相互作用能来降低总能量。轨道内铁磁自旋相关性会引起轨道动量排列。每个原子的磁矩估计值与硫醇包覆的金薄膜和纳米颗粒的实验观测结果吻合良好。