The steady-state orbital angular momentum accumulation at a Hall strip edge is proportional to the edge current profile with a Dyakonov-Perel-like decay time, plus new non-local terms for non-Ohmic flows.
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Orbital Hall Effect and Angular Momentum Dynamics in Confined Geometries
The steady-state orbital angular momentum accumulation at a Hall strip edge is proportional to the edge current profile with a Dyakonov-Perel-like decay time, plus new non-local terms for non-Ohmic flows.