arXivDaily arXiv每日学术速递 周一至周五更新
arXiv周末暂无论文更新,休息一下吧,周末愉快~~
arXiv 1208.5635cond-mat.str-el
收藏

具有Rashba自旋-轨道相互作用的二维基质中的两个Anderson杂质

Two Anderson impurities in a 2D host with Rashba spin-orbit interaction

T. I. Ivanov

摘要:

本文用修正的微扰理论研究了具有附加Rashba自旋轨道相互作用的二维双杂质Anderson模型。我们构造的杂质格林函数精确地再现了前四个谱矩。我们讨论了偶/奇近藤峰的高度和宽度作为杂质间距离和Rashba能量$E_R$(Rashba自旋轨道相互作用的强度)的函数。对于小的杂质分离的近藤温度显示出非单调依赖于$E_R$是不同的,在偶数和奇数通道。我们预测Kondo温度与$E_R$几乎只有线性关系,而不是与$E_R$呈指数关系

英文摘要:

We have studied the two-dimensional two-impurity Anderson model with additional Rashba spin-orbit interaction by means of the modified perturbation theory. The impurity Green's functions we have constructed exactly reproduce the first four spectral moments. We discuss the height and the width of the even/odd Kondo peaks as functions of the inter-impurity distance and the Rashba energy $E_R$ (the strength of the Rashba spin-orbit interaction). For small impurity separations the Kondo temperature shows a non-monotonic dependence on $E_R$ being different in the even and the odd channel. We predict that the Kondo temperature has only almost linear dependence on $E_R$ and not an exponential increase with $E_R$

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

↑