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Superradiant strongly correlated quantum states in cavity Hubbard model

Kang Wang, Wei-Xuan Chang, Cheng-Yu Bi, Zi Cai, Zi-Xiang Li

Abstract

In cavity quantum materials, entangling strongly correlated electrons with quantum light provides a unique opportunity to explore novel quantum phases and phase transitions absent in conventional solid-state materials. In this study, we develop a sign-problem-free fermion-photon hybrid Quantum Monte Carlo (QMC) algorithm, and use it to systematically investigate the ground-state phase diagram of a two-dimensional cavity Hubbard model. It is shown that the interplay between the electron correlation and photon condensation gives rise to intriguing quantum phases ({\it e.g.} superradiant antiferromagnetic and chiral/$π$-flux states), and different quantum phase transitions, such as a first-order superradiant phase transition and a continuous phase transition with Gross-Neveu universality class. The methodology can be readily generalized to more complicated cavity strongly correlated models.

Superradiant strongly correlated quantum states in cavity Hubbard model

Abstract

In cavity quantum materials, entangling strongly correlated electrons with quantum light provides a unique opportunity to explore novel quantum phases and phase transitions absent in conventional solid-state materials. In this study, we develop a sign-problem-free fermion-photon hybrid Quantum Monte Carlo (QMC) algorithm, and use it to systematically investigate the ground-state phase diagram of a two-dimensional cavity Hubbard model. It is shown that the interplay between the electron correlation and photon condensation gives rise to intriguing quantum phases ({\it e.g.} superradiant antiferromagnetic and chiral/-flux states), and different quantum phase transitions, such as a first-order superradiant phase transition and a continuous phase transition with Gross-Neveu universality class. The methodology can be readily generalized to more complicated cavity strongly correlated models.
Paper Structure (4 sections, 29 equations, 8 figures)

This paper contains 4 sections, 29 equations, 8 figures.

Figures (8)

  • Figure 1: (a) Schematic illustration of a two-dimensional Hubbard model embedded in a gyrotropic cavity. (b)Ground-state phase diagram of the cavity Hubbard model in terms of light-matter coupling $g$ and Hubbard interaction $U/t$. Dashed and solid denote first-order and second-order AFM transitions, respectively. The label GNU marks the second-order phase transition with Gross-Neveu universality class.
  • Figure 2: Superradiant phase transition at $U=0$. (a) Squared effective gauge flux $\langle \hat{\Phi}^2 \rangle=\frac{g^2}{N}\langle \hat{X}^2 \rangle$ per plaquette as a function of light-matter coupling $g$. The discontinuous jump at $g_c\approx 2.8$ signals a first-order photon condensation transition. (b) Edge current correlation function. The finite negative value for $g>g_c$ indicates chiral edge currents induced by the emergent magnetic flux.
  • Figure 3: Effects of finite Hubbard interaction. (a) and (b) AFM structure factor $S(\pi,\pi)$ and squared effective flux $\langle \Phi^2 \rangle$ as functions of $U$ at $g = 4.0$. The simultaneous discontinuous jumps in both quantities are the hallmark of a single first-order transition. (c) Correlation-length ratio $R_s$ as a function of $U$ at $g = 6.0$ for different system sizes. The crossing of curves for different $L$, shown in the inset, signals a continuous AFM transition at $U \approx 6.4t$. (d) Squared effective flux $\langle \Phi^2 \rangle$ at $g = 6.0$, showing a first-order photon condensation transition at $U\approx 8.6t$. (e) and (f) Histogram of probability distribution of the $S(\pi,\pi)$ at $U = 6.4$ (close to the AFM transition) and $\langle \Phi^2 \rangle$ at $U = 8.15$ (close to the superradiant transition) for $L=12$ system, the former displays a unimodal distribution characteristic of a continuous (second-order) phase transition, while the latter exhibits a bimodal distribution characteristic of a first-order phase transition, $g$ is fixed as $g=6.0$ and the dashed line indicates the average value. (g) and (h) Finite-size scaling of the AFM structure factor $S(\pi,\pi)$ and the squared effective flux $\langle \Phi^2 \rangle$ for different system sizes at $g = 6.0, U=7.4$, confirming the coexistence of AFM order and photon condensation in the intermediate interaction regime.
  • Figure 4: Finite-size scaling analysis of the continuous AFM transition at $g=6.0$. Data collapse of the (a) AFM structure factor $S(\pi,\pi)L^{2\beta/\nu}$ and (b) correlation-length ratio $R_s$ as functions of the scaling variable $(U/U_c-1)L^{1/\nu}$. The critical point here is $U_c\approx6.4$. The critical exponents used for the collapse, $\nu = 1.021, \beta=0.743$, are taken from the established values for the chiral Heisenberg Gross-Neveu universality class Sorella16PRX.
  • Figure 5: Evolution of physical observables as a function of interaction strength $U$ for different light-matter coupling values $g=2.0, 4.0, 6.0,$ and $10.0$ (arranged from top to bottom). From left to right, each column displays: the squared effective flux $\langle\Phi^2\rangle$, the antiferromagnetic spin structure factor $S(\pi,\pi)$, and the dimensionless correlation-length ratio $R_s$. These results provide further evidence for the competition between magnetic and photonic orders across different parameter regimes.
  • ...and 3 more figures