2020
DOI: 10.1103/physrevlett.124.147203
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Dynamical Sign Reversal of Magnetic Correlations in Dissipative Hubbard Models

Abstract: In quantum magnetism, the virtual exchange of particles mediates an interaction between spins. Here we show that an inelastic Hubbard interaction fundamentally alters the magnetism of the Hubbard model due to dissipation in spin-exchange processes, leading to sign reversal of magnetic correlations in dissipative quantum dynamics. This mechanism is applicable to both fermionic and bosonic Mott insulators, and can naturally be realized with ultracold atoms undergoing two-body inelastic collisions. The dynamical … Show more

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Cited by 70 publications
(60 citation statements)
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“…The study, that has the merit of highlighting in a transparent way the fermionisation induced by strong two-body losses, does not produce any prediction for the dynamics of the population of the gas. Finally, we mention the existence of a conspicuous literature focusing on the problem of two-body losses in one-dimensional fermionic gases [38][39][40][41].…”
Section: Introductionmentioning
confidence: 99%
“…The study, that has the merit of highlighting in a transparent way the fermionisation induced by strong two-body losses, does not produce any prediction for the dynamics of the population of the gas. Finally, we mention the existence of a conspicuous literature focusing on the problem of two-body losses in one-dimensional fermionic gases [38][39][40][41].…”
Section: Introductionmentioning
confidence: 99%
“…Non-Hermitian XXZ model NH spin models in the presence of dissipation have been proposed as prototypical dissipative quantum systems which are relevant to experiments in ultracold atoms [11,17,80]. However, NH many-body phenomena in dissipative spin systems are less explored [11,17], compared to the other dissipative spin models that can be mapped to noninteracting NH systems or to those in the master equation frameworks [80][81][82][83]. Here we follow Ref.…”
Section: Modelmentioning
confidence: 99%
“…For simplicity, we assume U ↑↑ = U ↓↓ ≡ U and γ ↑↑ = γ ↓↓ ≡ γ. Then, after the second-order perturbation theory with respect to t h , the effective NH Hamiltonian reduces to the NH XXZ model [17,88]…”
Section: Modelmentioning
confidence: 99%
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