Rashba Spin-Orbit Coupling and Nonlocal Correlations in Disordered 2D Systems
Yongtai Li, Gour Jana, Chinedu E. Ekuma
TL;DR
The paper extends the dynamical cluster approximation to include Rashba spin–orbit coupling, enabling a nonlocal mean-field study of disorder and SOC in 2D systems. By analyzing the average density of states, momentum-resolved self-energy, and return probability, it demonstrates SOC-induced delocalization effects and the crucial role of nonlocal correlations in shaping spin-dependent interference within the symplectic universality class. The extended DCA–SOC approach aligns well with numerically exact kernel polynomial method results, validating its accuracy and efficiency for exploring disordered, spin–orbit-coupled systems and paving the way for future multiorbital and strongly correlated extensions. However, like other mean-field methods, it cannot capture the Anderson localization transition itself, motivating future incorporation of typical-medium extensions (TMDCA) for ALT physics and transport studies.
Abstract
We present an extension of the dynamical cluster approximation (DCA) that incorporates Rashba spin-orbit coupling (SOC) to investigate the interplay between disorder, spin-orbit interaction, and nonlocal spatial correlations in disordered two-dimensional systems. By analyzing the average density of states, momentum-resolved self-energy, and return probability, we demonstrate how Rashba SOC and nonlocal correlations jointly modify single-particle properties and spin-dependent interference. The method captures key features of the symplectic universality class, including SOC-induced delocalization signatures at finite times. We benchmark the DCA results against those obtained from the numerically exact kernel polynomial method, finding good agreement. This validates the computationally efficient, mean-field-based DCA framework as a robust tool for exploring disorder, spin-orbit coupling, and nonlocal correlation effects in low-dimensional systems, and paves the way for simulating multiorbital and strongly correlated systems that were previously inaccessible due to computational limitations.
