非中心对称超导体的序参量宇称混合效应:比热与自旋磁化率(英文)

在非中心对称超导体中,反对称的自旋-轨道耦合会导致自旋单态配对与三重态配对的混合.这里主要关注重费米子超导体CePt3Si,研究自旋-轨道耦合以及宇称混合对该系统比热和自旋磁化率的影响,得到了与实验可以比拟的理论结果.

Rashba自旋轨道耦合对电子自旋磁化率的影响

研究了哈伯德强关联系统中,Rashba自旋轨道耦合(R-SOC)对二维正方晶格的自旋磁化率的影响.在线性响应理论中,自旋磁化率可以表示为推迟格林函数.对它所遵守的运动方程做哈特利-福克近似(HFA)和无规位相近似(RPA),再通过数值求解可得自旋磁化率.结果表明:没有R-SOC的静态磁化率Reχ(q,ω=0)随着库伦排斥势U的增大而增大,随温度T的增大而减小,库伦排斥势和温度对动态磁化率Reχ(q,ω=0)也有相似的影响.在加入R-SOC后,自旋轨道耦合的自旋磁化率实部在q=0附近形成了平底,而且平底宽度随VSO的增加而增大.同时自旋磁化率的虚部在平底边沿上呈现剧烈起伏.该效应可作为材料的自旋轨道耦合的显著标志.

Pauli Spin Paramagnetism and Electronic Specific Heat in Generalised d-Dimensions

The variations of pauli spin paramagnetic susceptibility and the electronic specific heat of solids, are caiculated as functions of temperature following the free electron approximation, in generalised d-dimensions. The results are compared and become consistent with that obtained in susceptibility becomes independent of temperature only in three dimensions. Interestingly, the Pauli spin paramagnetic two dimensions.