Electric Field-Induced Kerr Rotation on Metallic Surfaces
Farzad Mahfouzi, Mark D. Stiles, Paul M. Haney
TL;DR
This work addresses electric-field-induced Kerr rotation at metallic Pt surfaces by combining density functional theory with a nonlocal optical-conductivity framework and Maxwell scattering. It identifies two microscopic mechanisms—extrinsic bias-driven orbital accumulation (orbital Edelstein effect) and intrinsic surface-localized Pockels-like changes in wavefunctions—both contributing within a surface-proximal region of a few nanometers. In Pt films, these contributions are found to be comparable in magnitude but produce distinct polarization signatures, with extrinsic Kerr angles for $s$- and $p$-polarized light nearly equal and intrinsic Kerr angles opposite in sign. The results, including an effective surface-localization length shorter than 1 nm for the electro-optically active region, agree well with experimental Pt data and underscore the necessity of a nonlocal electro-optical description to capture surface boundary effects in metallic systems.
Abstract
We use a combination of density functional theory calculations and optical modeling to establish that the electric field-induced Kerr rotation in metallic thin films has contributions from both non-equilibrium orbital moment accumulation (arising from the orbital Edelstein effect) and a heretofore overlooked surface Pockels effect. The Kerr rotation associated with orbital accumulation has been studied in previous works and is largely due to the dc electric field-induced change of the electron distribution function. In contrast, the surface Pockels effect is largely due to the dc field-induced change to the wave functions. Both of these contributions arise from the dual mirror symmetry breaking from the surface and from the dc applied field. Our calculations show that the resulting Kerr rotation is due to the dc electric field modification of the optical conductivity within a couple of nanometers from the surface, consistent with the dependence on the local mirror symmetry breaking at the surface. For thin films of Pt, our calculations show that the relative contributions of the orbital Edelstein and surface Pockels effects are comparable, and that they have different effects on Kerr rotation of $s$ and $p$ polarized light, $θ_K^s$ and $θ_K^p$. The orbital Edelstein effect yields similar values of $θ_K^s$ and $θ_K^p$, while the surface Pockels effect leads to opposing values of $θ_K^s$ and $θ_K^p$.
