Department of Physics and Astronomy, University of Wyoming, Laramie, WY 82071, USA.
J Phys Condens Matter. 2013 Mar 27;25(12):125802. doi: 10.1088/0953-8984/25/12/125802. Epub 2013 Mar 1.
The investigation of a series of oxygen-deficient EuO thin films provided strong evidence that the doped electrons form magnetic polarons with the nearby Eu2+ 4f spins; this is responsible for the enhanced Curie temperature observed near 140 K. Unlike in the previous magnetic polaron models proposed for the metal-to-insulator transition in EuO, the exchange coupling J between the doped electron and its neighboring 4f spins is antiferromagnetic. The model explains satisfactorily the fact that the ordering temperature of the magnetic polarons occurs at ~140 K, independently of the oxygen vacancy concentration, and the contradiction that electron doping increases T(c) and yet reduces the red shift in the optical absorption. The magnetic polarons are coupled antiferromagnetically to the Eu2+ local moments that are ordered in the Heisenberg ferromagnet below 69 K. This coupling was observable in the vicinity of 69 K. We discuss how, with increasing concentration of the oxygen vacancies, their behaviors evolve from those of isolated superparamagnetic polarons to those of percolating magnetic polarons with a finite coercivity.
对一系列缺氧 EuO 薄膜的研究提供了有力的证据,表明掺杂电子与附近的 Eu2+ 4f 自旋形成磁性极化子;这是导致在接近 140 K 时观察到居里温度增强的原因。与之前提出的用于解释 EuO 中金属-绝缘体转变的磁性极化子模型不同,掺杂电子与其相邻 4f 自旋之间的交换耦合 J 是反铁磁的。该模型令人满意地解释了以下事实:磁性极化子的有序温度发生在~140 K,与氧空位浓度无关,以及电子掺杂增加 T(c),但降低了光学吸收的红移。磁性极化子与 Heisenberg 铁磁体中有序的 Eu2+ 局域磁矩反铁磁耦合,低于 69 K。这种耦合在接近 69 K 时是可以观察到的。我们讨论了随着氧空位浓度的增加,它们的行为如何从孤立的超顺磁极化子演变为具有有限矫顽力的渗流磁性极化子。