Large-N expansion for unitary superfluid Fermi gases

dc.creatorVeillette, M. Y.
dc.creatorSheehy, D. E.
dc.creatorRadzihovsky, L.
dc.date2006-10-28
dc.date2007-05-14
dc.date.accessioned2026-07-07T12:37:43Z
dc.date.available2026-07-07T12:37:43Z
dc.descriptionWe analyze strongly interacting Fermi gases in the unitary regime by considering the generalization to an arbitrary number N of spin-1/2 fermion flavors with Sp(2N) symmetry. For N=\infty this problem is exactly solved by the BCS-BEC mean-field theory, with corrections small in the parameter 1/N. The large-N expansion provides a systematic way to determine corrections to mean-field predictions, allowing the calculation of a variety of thermodynamic quantities at (and in the proximity to) unitarity, including the energy, the pairing gap, and upper-critical polarization (in the case of a polarized gas) for the normal to superfluid instability. For the physical case of N=1, among other quantities, we predict in the unitarity regime, the energy of the gas to be ξ=0.28 times that for the non-interacting gas and the pairing gap to be 0.52 times the Fermi energy.
dc.description13 pages
dc.identifierhttps://arxiv.org/abs/cond-mat/0610798
dc.identifierhttp://arxiv.org/abs/cond-mat/0610798
dc.identifierPhys.Rev.A75:043614,2007
dc.identifierdoi:10.1103/PhysRevA.75.043614
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/218534
dc.subjectOther Condensed Matter
dc.titleLarge-N expansion for unitary superfluid Fermi gases
dc.typetext

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