2012
DOI: 10.1103/physreva.85.012701
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Hartree shift in unitary Fermi gases

Abstract: The Hartree energy shift is calculated for a unitary Fermi gas. By including the momentum dependence of the scattering amplitude explicitly, the Hartree energy shift remains finite even at unitarity. Extending the theory also for spin-imbalanced systems allows calculation of polaron properties. The results are in good agreement with more involved theories and experiments.Comment: 31 pages, many figure

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Cited by 22 publications
(30 citation statements)
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“…The plot reveals the strong momentum dependence of the self-energy, particularly close to unitarity k F a = ±∞. The momentum dependence is easily understood32 when considering the two-body on-shell scattering amplitude, which for the contact interaction pseudopotential isFor large relative momenta , the scattering amplitude is suppressed. Hence, high momentum atoms will interact very weakly with atoms in the Fermi sea and the self-energy is suppressed.…”
Section: Resultsmentioning
confidence: 90%
See 1 more Smart Citation
“…The plot reveals the strong momentum dependence of the self-energy, particularly close to unitarity k F a = ±∞. The momentum dependence is easily understood32 when considering the two-body on-shell scattering amplitude, which for the contact interaction pseudopotential isFor large relative momenta , the scattering amplitude is suppressed. Hence, high momentum atoms will interact very weakly with atoms in the Fermi sea and the self-energy is suppressed.…”
Section: Resultsmentioning
confidence: 90%
“…In particular, the imaginary part of the self-energy no longer changes sign at the Fermi surface32. To avoid the problem, we neglect the imaginary part obtained from the Brueckner-Goldstone self-energy altogether and instead use a fixed imaginary part.…”
Section: Methodsmentioning
confidence: 99%
“…In this paper, we numerically calculate χ n within the framework of an extended T -matrix approximation (ETMA) [21][22][23][24][25] which has been developed to evaluate the spin susceptibility χ s in the BCS-BEC crossover region. An advantage of ETMA is that one may quantitatively describe the self-energy shift, which is also referred as "Hartree shift" in the previous work [26][27][28]. We compare our results with the recent experiment on a 6 Li Fermi gas, to clarify effects of quantum fluctuations in the whole BCS-BEC crossover region at T = 0.…”
Section: Introductionmentioning
confidence: 71%
“…The Hartree energy [the term proportional to densities n ↑(↓) (r)] is known to be ill behaved in the strongly interacting regime [27,28], causing large perturbations in the density profiles by compressing the gas. In BdG theory the problem manifests already well before the actual divergence of the scattering length: the kinetic-energy cost of adding one more atom to the center of the trap would be…”
Section: Methodsmentioning
confidence: 99%