“…Having obtained a low entropy band insulating state, we now tune an onsite attractive interaction U of the Hubbard type (using, e.g., a Feshbach resonance 36 37 ) to drive the band insulating state into a superfluid state 25 38 39 40 41 42 43 . The emergent superfluid state can be modeled by the action
where
stands for the fermion Grassman variable associated with momentum
, sublattice flavour α , β = A , B ; σ is the spin label, τ is the imaginary time, N is the number of unit cells of the homogeneous system, and
is a 2 × 2 matrix, defined as
…”