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Energy as a function of dimensionless spin–orbit coupling parameter β for the case where the oscillator potential is deformed

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posted on 2013-06-24, 00:00 authored by O V Marchukov, A G Volosniev, D V Fedorov, A S Jensen, N T Zinner

Figure 2. Energy as a function of dimensionless spin–orbit coupling parameter β for the case where the oscillator potential is deformed. The left panel has \gamma =\frac{\omega _x}{\omega _y} = 2 and the right panel has γ = 3.

Abstract

We consider a spin–orbit coupled system of particles in an external trap that is represented by a deformed harmonic oscillator potential. The spin–orbit interaction is a Rashba interaction that does not commute with the trapping potential and requires a full numerical treatment in order to obtain the spectrum. The effect of a Zeeman term is also considered. Our results demonstrate that variable spectral gaps occur as a function of strength of the Rashba interaction and deformation of the harmonic trapping potential. The single-particle density of states and the critical strength for superfluidity vary tremendously with the interaction parameter. The strong variations with Rashba coupling and deformation imply that the few- and many-body physics of spin–orbit coupled systems can be manipulated by variation of these parameters.

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