Orbital and spin contributions to the -tensors in metal nanoparticles
arXiv:cond-mat/0312278 · doi:10.1103/PhysRevB.69.045411
Abstract
We present a theoretical study of the mesoscopic fluctuations of -tensors in a metal nanoparticle. The calculations were performed using a semi-realistic tight-binding model, which contains both spin and orbital contributions to the -tensors. The results depend on the product of the spin-orbit scattering time and the mean-level spacing , but are otherwise weakly affected by the specific shape of a {\it generic} nanoparticle. We find that the spin contribution to the -tensors agrees with Random Matrix Theory (RMT) predictions. On the other hand, in the strong spin-orbit coupling limit , the orbital contribution depends crucially on the space character of the quasi-particle wavefunctions: it levels off at a small value for states of character but is strongly enhanced for states of character. Our numerical results demonstrate that when orbital coupling to the field is included, RMT predictions overestimate the typical -factor of orbitals that have dominant -character. This finding points to a possible source of the puzzling discrepancy between theory and experiment.
arXiv comment21 pages, 6 figures; accepted for publication in Physical Review B
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