Space-time first-order correlations of an open Bose-Hubbard model with incoherent pump and loss

TL;DR

This paper studies the steady-state correlations of an open driven-dissipative Bose-Hubbard model, revealing how dissipation and interactions influence spectral properties and correlation decay in a non-thermal quantum regime.

Contribution

It provides an exact diagonalization analysis of space-time correlations in a driven-dissipative Bose-Hubbard system, highlighting the effects of interactions, hopping, and dissipation on spectral features.

Findings

Decay width of correlations is renormalized by interactions and hopping.

Spectral function shows dispersive and doublon branches.

Driven-dissipative steady state differs from ground state and high-temperature equilibrium.

Abstract

We investigate the correlation properties in the steady state of driven-dissipative interacting bosonic systems in the quantum regime, as for example non-linear photonic cavities. Specifically, we consider the Bose-Hubbard model on a periodic chain and with spatially homogeneous one-body loss and pump within the Markovian approximation. The steady state is non-thermal and is formally equivalent to an infinite-temperature state with finite chemical potential set by the dissipative parameters. While there is no effect of interactions on the steady state, we observe a nontrivial behaviour of the space-time two-point correlation function, obtained by exact diagonalisation. In particular, we find that the decay width of the propagator is not only renormalised at increasing interactions, as it is the case of a single non-linear resonator, but also at increasing hopping strength. Furthermore, we numerically predict at large interactions a plateau value of the decay rate which goes beyond perturbative results in the interaction strength. We then compute the full spectral function, finding that it contains both a dispersive free-particle like dispersion at low energy and a doublon branch at energy corresponding to the on-site interactions. We compare with the corresponding calculation for the ground state of a closed quantum system and show that the driven-dissipative nature -- determining both the steady state and the dynamical evolution -- changes the low-lying part of the spectrum, where noticeably, the dispersion is quadratic instead of linear at small wavevectors. Finally, we compare to a high temperature grand-canonical equilibrium state and show the difference with respect to the open system stemming from the additional degree of freedom of the dissipation that allows one to vary the width of the dispersion lines.