arXiv · cond-mat/0410420
Semiclassical Time Evolution of the Holes from Luttinger Hamiltonian
Abstract
We study the semi-classical motion of holes by exact numerical solution of the Luttinger model. The trajectories obtained for the heavy and light holes agree well with the higher order corrections to the abelian and the non-abelian adiabatic theories in Ref. [1] [S. Murakami et al., Science 301, 1378(2003)], respectively. It is found that the hole trajectories contain rapid oscillations reminiscent of the "Zitterbewegung" of relativistic electrons. We also comment on the non-conservation of helicity of the light holes.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Z. F. Jiang, R. D. Li, Shou-Cheng Zhang, W. M. Liu. 2004-10-17. Semiclassical Time Evolution of the Holes from Luttinger Hamiltonian. https://doi.org/10.1103/physrevb.72.045201
Cite the original work for its findings. Save a collection to share your selection of sources.