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Quantum phase transition driven by competing intralayer and interlayer hopping in bilayer nickelates

Xiaoyu Zhu, Wei Qin, Ping Cui, Zhenyu Zhang

TL;DR

This work addresses how superconductivity arises in bilayer nickelates under non-thermal tuning by examining a minimal bilayer Hubbard model focused on the Ni-$d_{3z^2-r^2}$ orbital. Using DMRG on a bilayer lattice with doping $\delta=1/8$ and $U=8t$, the authors identify a quantum phase transition controlled by the ratio $t_1/t$ near $0.5$, separating a quasi-long-range SDW phase from a Luther-Emery phase where superconductivity is enhanced and CDW correlations emerge. The transition features the opening of a spin gap, a shift in central charge from $c\approx 2$ to $c\approx 1$, and a move from SDW-dominated order to uniform extended-$s$-wave superconductivity with interlayer singlet pairing; PDW tendencies are noted in the SDW regime. The results provide a microscopic link between lattice anisotropy and superconductivity, suggesting that pressure or strain tuning and possible hybridization with the $d_{x^2-y^2}$ orbital could further elevate the superconducting transition temperature in bilayer nickelates.

Abstract

Bilayer nickelates exhibit high-temperature superconductivity under proper hydrostatic pressure or epitaxial strain, signifying the emergence of quantum phase transitions whose physical mechanisms remain unclear. Using a minimal bilayer Hubbard model incorporating only the Ni-$d_{3z^2-r^2}$ orbitals, we demonstrate that a phase transition naturally arises from tuning the ratio of intralayer to interlayer hopping amplitudes. The transition point separates regimes with a rich interplay between superconducting and density-wave orders. In the regime of weaker intralayer hopping, the ground state is characterized by quasi-long-range spin-density-wave order. As the intralayer hopping increases, the system undergoes a transition marked by the opening of a finite spin gap and the disappearance of spin-density-wave order. Meanwhile, superconductivity is dramatically enhanced, accompanied by the emergence of quasi-long-range charge-density-wave order, indicating that the system enters Luther-Emery phase. This quantum phase transition, driven by the competition between intralayer and interlayer hopping, provides a plausible microscopic explanation for the experimentally observed correlation between the superconducting transition temperature and ratio of out-of-plane to in-plane lattice constants. Our findings reveal a possible link between the suppression of spin-density-wave order and the prominence of superconducting order, which may assist future efforts to optimize experimental conditions for further enhancing superconductivity in bilayer nickelates.

Quantum phase transition driven by competing intralayer and interlayer hopping in bilayer nickelates

TL;DR

This work addresses how superconductivity arises in bilayer nickelates under non-thermal tuning by examining a minimal bilayer Hubbard model focused on the Ni- orbital. Using DMRG on a bilayer lattice with doping and , the authors identify a quantum phase transition controlled by the ratio near , separating a quasi-long-range SDW phase from a Luther-Emery phase where superconductivity is enhanced and CDW correlations emerge. The transition features the opening of a spin gap, a shift in central charge from to , and a move from SDW-dominated order to uniform extended--wave superconductivity with interlayer singlet pairing; PDW tendencies are noted in the SDW regime. The results provide a microscopic link between lattice anisotropy and superconductivity, suggesting that pressure or strain tuning and possible hybridization with the orbital could further elevate the superconducting transition temperature in bilayer nickelates.

Abstract

Bilayer nickelates exhibit high-temperature superconductivity under proper hydrostatic pressure or epitaxial strain, signifying the emergence of quantum phase transitions whose physical mechanisms remain unclear. Using a minimal bilayer Hubbard model incorporating only the Ni- orbitals, we demonstrate that a phase transition naturally arises from tuning the ratio of intralayer to interlayer hopping amplitudes. The transition point separates regimes with a rich interplay between superconducting and density-wave orders. In the regime of weaker intralayer hopping, the ground state is characterized by quasi-long-range spin-density-wave order. As the intralayer hopping increases, the system undergoes a transition marked by the opening of a finite spin gap and the disappearance of spin-density-wave order. Meanwhile, superconductivity is dramatically enhanced, accompanied by the emergence of quasi-long-range charge-density-wave order, indicating that the system enters Luther-Emery phase. This quantum phase transition, driven by the competition between intralayer and interlayer hopping, provides a plausible microscopic explanation for the experimentally observed correlation between the superconducting transition temperature and ratio of out-of-plane to in-plane lattice constants. Our findings reveal a possible link between the suppression of spin-density-wave order and the prominence of superconducting order, which may assist future efforts to optimize experimental conditions for further enhancing superconductivity in bilayer nickelates.

Paper Structure

This paper contains 15 sections, 13 equations, 12 figures, 1 table.

Figures (12)

  • Figure 1: (a) Schematic of the bilayer Hubbard model. Circles of different colors indicate electron sites in different layers. The strong interlayer hopping $t$ is indicated by thick lines while the weak intralayer hopping $t_1$ is shown in thin lines. (b) Three types of dimers relevant to ground states in the weak $t_1$ regime. (c) Two distinct phases separated by a quantum phase transition at $t_1\approx 0.5t$, calculated for onsite Hubbard interaction $U = 8t$ and doping $\delta = 1/8$. The dashed line indicates the dimer limit ($t_1=0$), where the multiply degenerate ground states only involve the three types of dimers in (b). SDW is the shorthand for spin density wave, and LE denotes Luther-Emery liquid, which features competing superconductivity and charge density wave.
  • Figure 2: (a) Charge-density profiles along the $x$ direction for $t_1=0.2t$, $0.4t$, and $0.6t$. (b) Oscillation amplitude $A$ as a function of $t_1/t$. (c) Spatial profiles of spin-spin correlation $\langle D_x\rangle$ within each dimer at $t_1=0.2t$, $0.4t$, and $0.6t$. (d) Evolution of the averaged $\langle D_x \rangle$ with $t_1/t$. The blue dashed line marks the average value in the dimer limit. These plots are obtained on a bilayer $96\times 2$ lattice.
  • Figure 3: (a) and (b) Charge (c), spin (s), and pairing (sc) correlation functions plotted in the log-log scales. Dashed lines represent power-law or exponential fits to the envelope function $f(x)$. $K$ denotes the decay exponent of the power-law fitting, and $\xi$ is the decay length in the exponential case. (c) Dependence of decay exponents on $t_1/t$. The dashed line indicates $K_c^A$, extracted from the charge-density profile. (d) Oscillation coefficient $B$ in $P(x)$ as a function of $t_1/t$. $|B|>1$ indicates that the correlation functions change signs periodically. These results are obtained from simulations on a $96\times 2$ bilayer lattice.
  • Figure 4: (a) Charge structure factor. A peak appears in the LE phase ($t_1=0.6t$) at $(\pi/2,0,0)$. (b) Spin structure factor. The peak shows only in the SDW phase ($t_1=0.3t$) at $(\pi/2,0,0)$. (c) Pair structure factor. There is a singular point in the SDW phase at $(k_x,k_y) = (\pi/2,0)$. In the LE phase, the singularity only occurs at $(0,0)$. (d) Momentum distribution function. The effective Fermi point $k_F$, where $\tilde{n}_{\sigma}$ becomes singular, lies at $k_x = 3\pi/4$.
  • Figure 5: Scalings of the charge gap $\Delta_c$ and spin gap $\Delta_s$ with $1/N_x$. The insets show the variations of extrapolated gaps with $t_1/t$ in the thermodynamic limit. After the transition, the spin gap becomes finite while the charge gap remains zero. The truncation error is fixed at $\epsilon = 1.0\times 10^{-7}$.
  • ...and 7 more figures