Department of Physics, University of California, Berkeley, Berkeley, California 94720, USA.
Phys Rev Lett. 2010 Jul 9;105(2):026805. doi: 10.1103/PhysRevLett.105.026805.
The photocurrent in an optically active metal is known to contain a component that switches sign with the helicity of the incident radiation. At low frequencies, this current depends on the orbital Berry phase of the Bloch electrons via the "anomalous velocity" of Karplus and Luttinger. We consider quantum wells in which the parent material, such as GaAs, is not optically active and the relevant Berry phase only arises as a result of quantum confinement. Using an envelope approximation that is supported by numerical tight-binding results, it is shown that the Berry-phase contribution is determined for realistic wells by a cubic Berry phase intrinsic to the bulk material, the well width, and the well direction. These results for the Berry-phase effect suggest that it may already have been observed in quantum well experiments.
已知光活性金属中的光电流包含一个与入射辐射的螺旋性符号相反的分量。在低频下,该电流通过 Karplus 和 Luttinger 的“异常速度”,依赖于 Bloch 电子的轨道 Berry 相位。我们考虑量子阱,其中母体材料(如 GaAs)没有光活性,相关的 Berry 相位仅由于量子限制而产生。使用数值紧束缚结果支持的包络近似,表明 Berry 相贡献由体材料的立方 Berry 相、阱宽和阱方向的内在特性决定。这些 Berry 相效应的结果表明,它可能已经在量子阱实验中被观察到。