Unitary polarized Fermi gas under adiabatic rotation

dc.creatorBausmerth, I.
dc.creatorRecati, A.
dc.creatorStringari, S.
dc.date2008-06-11
dc.date2008-12-03
dc.date.accessioned2026-07-07T12:08:29Z
dc.date.available2026-07-07T12:08:29Z
dc.descriptionWe discuss the effect of an adiabatic rotation on the phase separation between the superfluid and normal component of a trapped polarized Fermi gas at unitarity and zero temperature, under the assumption that quantized vortices are not formed. We show that the Chandrasekhar-Clogston limit $n_{\downarrow}/\n_{\uparrow}$ characterizing the local polarization in the normal phase at the interface is enhanced by the rotation as a consequence of the centrifugal effect. The density profiles (local and column integral) of the two spin species are calculated as a function of the angular velocity for different values of the polarization. The critical value of the angular velocity at which the superfluid exhibits a spontaneous quadrupole deformation is also calculated for the unpolarized case.
dc.description8 pages, 11 figures, discussion added according to referee report, final version as published
dc.identifierhttps://arxiv.org/abs/0806.1885
dc.identifierhttp://arxiv.org/abs/0806.1885
dc.identifierPhysical Review A 78, 063603 (2008)
dc.identifierdoi:10.1103/PhysRevA.78.063603
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/209335
dc.subjectOther Condensed Matter
dc.titleUnitary polarized Fermi gas under adiabatic rotation
dc.typetext

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