Microscopic mechanism for asymmetric charge distribution in Rashba-type surface states and the origin of the the energy splitting scale
Beomyoung Kim, Panjin Kim, Wonsig Jung, Yeongkwan Kim, Yoonyoung Koh,, Wonshik Kyung, Joonbum Park, Masaharu Matsunami, Shin-ichi Kimura, Jun Sung, Kim, Jung Hoon Han, and Changyoung Kim

TL;DR
This paper investigates the microscopic origins of Rashba-type band splitting, revealing how asymmetric charge distribution arises from local orbital angular momentum and crystal momentum interlocking, and how the energy scale shifts from atomic SOC to electrostatic energy.
Contribution
It introduces an effective Hamiltonian model that explains the evolution of orbital angular momentum states and the energy scale of band splitting in Rashba systems, validated by experiments and first-principles calculations.
Findings
Asymmetric charge distribution forms due to interlocked OAM and crystal momentum.
Energy scale of band splitting shifts from atomic SOC to electrostatic energy with increasing SOC.
Model successfully explains spin and OAM structures in Au(111) and Bi2Te2Se systems.
Abstract
Microscopic mechanism for the Rashba-type band splitting is examined in detail. We show how asymmetric charge distribution is formed when local orbital angular momentum (OAM) and crystal momentum get interlocked due to surface effects. An electrostatic energy term in the Hamiltonian appears when such OAM and crystal momentum dependent asymmetric charge distribution is placed in an electric field produced from an inversion symmetry breaking (ISB). Analysis by using an effective Hamiltonian shows that, as the atomic spin-orbit coupling (SOC) strength increases from weak to strong, originally OAM-quenched states evolve into well-defined chiral OAM states and then to total angular momentum J-states. In addition, the energy scale of the band splitting changes from atomic SOC energy to electrostatic energy. To confirm the validity of the model, we study OAM and spin structures of Au(111)…
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