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Colliding clouds of strongly interacting spin-polarized fermions

Edward Taylor, Shizhong Zhang, William Schneider, and Mohit Randeria
Phys. Rev. A 84, 063622 – Published 16 December 2011

Abstract

Motivated by a recent experiment at MIT, we consider the collision of two clouds of spin-polarized atomic Fermi gases close to a Feshbach resonance. We explain why two dilute gas clouds, with underlying attractive interactions between their constituents, bounce off each other in the strongly interacting regime. Our hydrodynamic analysis, in excellent agreement with experiment, gives strong evidence for a metastable many-body state with effective repulsive interactions.

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  • Received 14 July 2011

DOI:https://doi.org/10.1103/PhysRevA.84.063622

©2011 American Physical Society

Authors & Affiliations

Edward Taylor, Shizhong Zhang, William Schneider, and Mohit Randeria

  • Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA

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Issue

Vol. 84, Iss. 6 — December 2011

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Images

  • Figure 1
    Figure 1
    Schematic of the colliding cloud experiment.Reuse & Permissions
  • Figure 2
    Figure 2
    Time dependence of the center-of-mass positions z¯σ of the two spin clouds at unitarity, with the red (upper) and blue (lower) curves denoting the two spin species. We use the upper-branch energy functional (see text), with εF0 corresponding to N=7.5×105 atoms, trap anisotropy ω/ωz=10, and damping γ̃=1. Initially the two clouds are displaced from the trap center by the axial Thomas-Fermi radius, z¯(t=0)=Rz,z¯(t=0)=Rz with initial axial width δz(0)=Rz equal to its equilibrium value.Reuse & Permissions
  • Figure 3
    Figure 3
    Time dependence of the center-of-mass positions z¯σ of the two spin clouds for kF(0)as=2. The parameters are the same as in Fig. 2.Reuse & Permissions
  • Figure 4
    Figure 4
    Time dependence of the center-of-mass positions z¯σ of the two spin clouds for kF(0)as=0.5. The parameters are the same as in Fig. 2.Reuse & Permissions
  • Figure 5
    Figure 5
    The single-particle energy in the upper branch, obtained from lowest-order constraint variational method. The energy is in units of 3/5εF. (a) Energy as a function of the polarization P for various values of kFas as indicated. (b) Energy as a function of the interaction parameter kFas for various values of polarization P as indicated. (c) Phase diagram of the interacting two-component Fermi gases. The two vertical red dashed lines indicates the separation between three phases. For 1/(kFas)>1.124, the system is in the Fermi liquid (FL) phase. For 1.124>1/(kFas)>0.91, the system is in the partially polarized phase (PP), and for 1/(kFas)<0.91, the system is fully polarized (FP).Reuse & Permissions
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