Equilibration and prethermalization in the Bose-Hubbard and Fermi-Hubbard models
arXiv:1311.2212 · doi:10.1103/PhysRevA.89.033616
Abstract
We study the Bose and Fermi Hubbard model in the (formal) limit of large coordination numbers . Via an expansion into powers of , we establish a hierarchy of correlations which facilitates an approximate analytical derivation of the time-evolution of the reduced density matrices for one and two sites etc. With this method, we study the quantum dynamics (starting in the ground state) after a quantum quench, i.e., after suddenly switching the tunneling rate from zero to a finite value, which is still in the Mott regime. We find that the reduced density matrices approach a (quasi) equilibrium state after some time. For one lattice site, this state can be described by a thermal state (within the accuracy of our approximation). However, the (quasi) equilibrium state of the reduced density matrices for two sites including the correlations cannot be described by a thermal state. Thus, real thermalization (if it occurs) should take much longer time. This behavior has already been observed in other scenarios and is sometimes called ``pre-thermalization.'' Finally, we compare our results to numerical simulations for finite lattices in one and two dimensions and find qualitative agreement.
arXiv admin note: substantial text overlap with arXiv:1203.2164
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