A rapid scattering-length sweep in a near-unitary Fermi gas produces an early-time attractor that is visible only in the joint (E, Π) state space, not in a single-variable curve.
Hydrodynamics with spacetime-dependent scattering length
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abstract
Hydrodynamics provides a concise but powerful description of long-time and long-distance physics of correlated systems out of thermodynamic equilibrium. Here we construct hydrodynamic equations for nonrelativistic particles with a spacetime-dependent scattering length and show that it enters constitutive relations uniquely so as to represent the fluid expansion and contraction in both normal and superfluid phases. As a consequence, we find that a leading dissipative correction to the contact density due to the spacetime-dependent scattering length is proportional to the bulk viscosity ($\zeta_2$ in the superfluid phase). Also, when the scattering length is slowly varied over time in a uniform system, the entropy density is found to be produced even without fluid flows in proportion to the bulk viscosity, which may be useful as a novel probe to measure the bulk viscosity in ultracold-atom experiments.
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Experimentally accessible drive-induced attractor in a Fermi gas near unitarity
A rapid scattering-length sweep in a near-unitary Fermi gas produces an early-time attractor that is visible only in the joint (E, Π) state space, not in a single-variable curve.