Superconductor-Insulator transition in a two-orbital attractive Hubbard model with Hund's exchange
arXiv:2505.08597 · doi:10.1103/svwm-6n4c
Abstract
We study a two-orbital attractive Hubbard model with a repulsive Hund's exchange coupling as an idealized model for a two-band superconductor. This framework is motivated by a system where a large isotropic electron-phonon coupling drives the on-site Hubbard repulsion negative, while leaving the exchange term unaffected. We focus on the intra-orbital (intra-band) singlet superconducting phase and we solve the model at zero temperature and half-filling using Dynamical Mean-Field Theory. Already at , the two-orbital model features a superconductor-insulator transition as grows, as opposed to the single-orbital case which remains superconducting for any . We find that a finite strengthens the effect of the attractive , both in the normal state and, more significantly, in the superconducting state. However, this pushes the system towards an effectively stronger coupling, hence to a faster transition to the insulating state. Remarkably, the transition from a superconductor to an insulator occurs with a vanishing quasi-particle weight and in a scenario that recalls strongly correlated superconductivity close to a Mott transition, even though the present model is dominated by attractive interactions.
arXiv comment8 pages, 6 figures
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