2013
DOI: 10.1088/0953-4075/46/13/134002
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Single-branch theory of ultracold Fermi gases with artificial Rashba spin–orbit coupling

Abstract: We consider interacting ultracold fermions subject to Rashba spin-orbit coupling. We construct a single-branch interacting theory for the Fermi gas when the system is dilute enough so that the positive helicity branch is not occupied at all in the non-interacting ground state. We show that the theory is renormalizable in perturbation theory and therefore yields a model of polarized fermions that avoids a multi-channel treatment of the problem. Our results open the path towards a much more straightforward appro… Show more

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Cited by 4 publications
(6 citation statements)
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References 31 publications
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“…This is a typical situation that also occurs, for instance, in the study of the ferromagnetic transition [34] in repulsive Fermi gases [35][36][37] and is resolved by going beyond first-order perturbation theory, which can result in an apparent first-order transition [37,38], or using nonperturbative methods [39,40], which predict a second-order phase transition and are in good agreement with Monte Carlo simulations [41]. Our findings are the natural starting point for higher order corrections [31] and nonperturbative treatments, and can still be improved at the mean-field level [42]. Moreover, if, as our results suggest, the transition to finite momentum is continuous, the critical point can be obtained by calculating only the second-order response function F(ξ,z) but with improved treatments of the interactions.…”
Section: O) the Extra Hartree Shift Of Eq (22) Is Easily Calculatedsupporting
confidence: 69%
See 1 more Smart Citation
“…This is a typical situation that also occurs, for instance, in the study of the ferromagnetic transition [34] in repulsive Fermi gases [35][36][37] and is resolved by going beyond first-order perturbation theory, which can result in an apparent first-order transition [37,38], or using nonperturbative methods [39,40], which predict a second-order phase transition and are in good agreement with Monte Carlo simulations [41]. Our findings are the natural starting point for higher order corrections [31] and nonperturbative treatments, and can still be improved at the mean-field level [42]. Moreover, if, as our results suggest, the transition to finite momentum is continuous, the critical point can be obtained by calculating only the second-order response function F(ξ,z) but with improved treatments of the interactions.…”
Section: O) the Extra Hartree Shift Of Eq (22) Is Easily Calculatedsupporting
confidence: 69%
“…The dimensionless interaction parameter ξ = mg/4πh 2 [30] must here be compared with the only dimensionless parameter z of the noninteracting gas. The typical interaction energy gρ/4 [31] should be smaller than the Fermi energy E F = πh 2 ρz/2m, which gives ξ < z/2.…”
Section: Weakly Interacting Fermi Gasmentioning
confidence: 98%
“…Refs. [274][275][276] describe how interactions are modified in the presence of strong Rashba coupling, offering a relation between physical scattering lengths and mean-field interactions.…”
Section: Interacting Fermi Gases With Socmentioning
confidence: 99%
“…Next, the paper by Maldonado-Mundo et al [2] studies ultracold Fermi gases with artificial Rashba spin-orbit coupling in a 2D gas. Anderson and Charles [3], in contrast, discuss a three-dimensional spin-orbit coupling in a trap.…”
mentioning
confidence: 99%