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Unified description of cuprate superconductors using four-band dd-pp model

Hiroshi Watanabe1,2 [email protected]    Tomonori Shirakawa3,4    Kazuhiro Seki5    Hirofumi Sakakibara2,6,7    Takao Kotani6,7    Hiroaki Ikeda8    Seiji Yunoki2,3,4,5 1Research Organization of Science and Technology, Ritsumeikan University, Shiga 525-8577, Japan
2Computational Condensed Matter Physics Laboratory, RIKEN Cluster for Pioneering Research (CPR), Saitama 351-0198, Japan
3Computational Materials Science Research Team, RIKEN Center for Computational Science (R-CCS), Hyogo 650-0047, Japan
4Quantum Computational Science Research Team, RIKEN Center for Quantum Computing (RQC), Saitama 351-0198, Japan
5Computational Quantum Matter Research Team, RIKEN Center for Emergent Matter Science (CEMS), Saitama 351-0198, Japan
6Advanced Mechanical and Electronic System Research Center (AMES), Faculty of Engineering, Tottori University, Tottori 680-8552, Japan
7Center of Spintronics Research Network (CSRN), Graduate School of Engineering Science, Osaka University, Osaka, 560-8531, Japan
8Department of Physics, Ritsumeikan University, Shiga 525-8577, Japan
Abstract

In the 35 years since the discovery of cuprate superconductors, we have not yet reached a unified understanding of their properties, including their material dependence of the superconducting transition temperature TcT_{\text{c}}. The preceding theoretical and experimental studies have provided an overall picture of the phase diagram, and some important parameters for the TcT_{\text{c}}, such as the contribution of the Cu dz2d_{z^{2}} orbital to the Fermi surface and the site-energy difference Δdp\Delta_{dp} between the Cu dx2y2d_{x^{2}-y^{2}} and O pp orbitals. However, they are somewhat empirical and limited in scope, always including exceptions, and do not provide a comprehensive view of the series of cuprates. Here we propose a four-band dd-pp model as a minimal model to study material dependence in cuprates. Using the variational Monte Carlo method, we theoretically investigate the phase diagram for the La2CuO4 and HgBa2CuO4 systems and the correlation between the key parameters and the superconductivity. Our results comprehensively account for the empirical correlation between TcT_{\text{c}} and model parameters, and thus can provide a guideline for new material design. We also show that the effect of the nearest-neighbor dd-dd Coulomb interaction VddV_{dd} is actually quite important for the stability of superconductivity and phase competition.

I INTRODUCTION

The discovery of superconductivity in cuprates has brought about the significant progress in strongly-correlated electron systems [1]. Along with the high superconducting transition temperature TcT_{\text{c}}, cuprates show anomalous phases and phenomena such as the Mott metal-insulator transition, pseudogap phenomena, and antiferromagnetic (AF) and charge-density-wave (or stripe) phases [2, 3]. Recently, nematic order [4] and ferromagnetic fluctuation [5, 6] have also been observed experimentally. These newly observed experiments being constantly reported with the underlying, possibly exotic, physics have continued to attract many researchers’ interests over 35 years since the first high-TcT_{\text{c}} cuprate superconductor was synthesized.

It has been widely believed that the strong AF spin fluctuation characteristic to the two-dimensional square lattice structure triggers the various anomalous phenomena in cuprates [7, 8, 9, 10]. On the basis of this picture, the effective one-band Hubbard model [11] has been studied with various numerical methods extensively [12, 13]. It succeeded to describe the important physics in cuprates not only for the ground state but also for the excited state. The angle-resolved photoemission spectroscopy (ARPES) experiments show that the Fermi surface consists of only one energy band mainly derived from the Cu dx2y2d_{x^{2}-y^{2}} orbital [14] and thus the one-band models are justified as long as the low-energy physics is concerned.

However, recent theoretical and experimental development sheds light on the importance of the orbital degree of freedom in cuprates. For example, material dependence of TcT_{\text{c}} is difficult to discuss within the one-band models. The previous studies of the one-band models generally discussed the material dependence via the shape of different Fermi surfaces originated by different hopping integrals, e.g., the nearest-neighbor hopping tt and the next nearest-neighbor hopping tt^{\prime}. Indeed, such treatment allowed us to capture the overall feature for the difference between hole-doped and electron-doped systems [15]. However, the material dependence of TcT_{\text{c}} for the hole-doped systems has not been able to be explained properly. Experimentally, TcT_{\text{c}} becomes higher with larger |t/t||t^{\prime}/t|, i.e., more rounded Fermi surface [16]. On the contrary, it is predicted theoretically that in most one-band models, TcT_{\text{c}} is reduced because of poor nesting properties in rounded Fermi surfaces [17, 18]. A clue to resolving this contradiction can be found by seriously considering the orbital degrees of freedom, especially, the Cu dz2d_{z^{2}} orbital [18, 19, 20]. The study for the two-orbital model shows that the contribution of the dz2d_{z^{2}} orbital to the Fermi surface, which is strong in low TcT_{\text{c}} materials, works against the dx2y2d_{x^{2}-y^{2}}-wave superconductivity [18]. This picture can explain the material dependence of TcT_{\text{c}}. Indeed, a recent ARPES experiment directly observed the hybridization gap between the dz2d_{z^{2}} and dx2y2d_{x^{2}-y^{2}} orbitals and pointed out the importance of the multiorbital effect on superconductivity [21].

Another extension to a multiorbital model is the introduction of the O pp orbitals. A minimal model that includes the Cu dx2y2d_{x^{2}-y^{2}}, O pxp_{x}, and O pyp_{y} orbitals in the CuO2 plane is known as the (three-band) dd-pp model or the Emery model [22]. The three-band dd-pp model has been studied with various numerical methods [23, 24, 25, 26, 27, 29, 28, 30, 31, 32, 33, 34, 35, 36, 37, 38, 39, 40, 41, 42, 43, 44, 45, 46, 47] as much as the one-band models. In these studies, the site-energy difference Δdp\Delta_{dp} between the Cu dx2y2d_{x^{2}-y^{2}} and O px/yp_{x/y} orbitals is found to be an important parameter for understanding the material dependence of TcT_{\text{c}}. For example, the three-band dd-pp model can successfully reproduce the negative correlation between Δdp\Delta_{dp} and TcT_{\text{c}} [34], namely, a smaller Δdp\Delta_{dp} leads to a higher TcT_{\text{c}}. Furthermore, the role of the O pp orbitals in the superconducting pairing [37, 41, 43, 44, 47], stripe order [26, 38], loop current [29, 30, 33], and nematic order [33, 36, 39, 40] has been discussed with the three-band dd-pp model. However, it is still difficult to correctly capture the correlation between Fermi surface topology and TcT_{\text{c}} within the three-band dd-pp model [28, 34].

In this paper, we study a four-band dd-pp model composed of the Cu dx2y2d_{x^{2}-y^{2}} and dz2d_{z^{2}} orbitals and the O pxp_{x} and pyp_{y} orbitals, which can be expected to resolve the problems mentioned above. As typical examples of single-layer hole-doped cuprates, we consider La2CuO4 and HgBa2CuO4 systems. We construct the tight-binding model for these systems based on the first-principles calculation and examine the effect of Coulomb interaction by the variational Monte Carlo (VMC) method. We show that the material dependence of TcT_{\text{c}} is well explained with two key parameters, the site energy εdz2\varepsilon_{d_{z^{2}}} of the Cu dz2d_{z^{2}} orbital and the site-energy difference Δdp\Delta_{dp} between the Cu dx2y2d_{x^{2}-y^{2}} and O px/yp_{x/y} orbitals, which is consistent with the empirical relation. We thus propose that the present four-band dd-pp model is a minimal model that can properly describe the material dependence of cuprate superconductors. Furthermore, we also study the effect of the nearest-neighbor dd-dd Coulomb interaction VddV_{dd}, which has not been discussed in detail previously. We show that VddV_{dd} substantially affects the stability of superconductivity and the phase competition among various phases, suggesting an important parameter for the effective model of cuprates. In addition, we find that VddV_{dd} induces a crossover from a Slater insulator to a Mott insulator at the undoped limit.

The rest of this paper is organized as follows. In Sec. II, a four-band dd-pp model on the two-dimensional square lattice is introduced. The VMC method and the variational wave functions are also explained in Sec. II. The numerical results are then provided in Sec. III. The tight-binding energy bands for the La2CuO4 and HgBa2CuO4 systems, obtained on the basis of the first-principles calculation, are first shown in Sec. III.1. The material and doping dependences of a superconducting correlation function are then examined and the role of two key parameters εdz2\varepsilon_{d_{z^{2}}} and Δdp\Delta_{dp} are clarified in Sec. III.2. The effect of the nearest-neighbor dd-dd Coulomb interaction VddV_{dd} is investigated in Sec. III.3. The phase competition among superconductivity and other phases is briefly discussed in Sec. III.4. Finally, the paper concludes with a summary in Sec. IV. The details of the variational wave functions are described in Appendix.

II MODEL AND METHOD

II.1 Four-band dd-pp model

As an effective low-energy model of cuprates, we consider a four-band dd-pp model on the two-dimensional square lattice (see Fig. 1) defined by the following Hamiltonian:

H=Hkin+HintHdc.H=H_{\text{kin}}+H_{\text{int}}-H_{\text{dc}}. (1)

Here, the kinetic term HkinH_{\text{kin}} is described by

Hkin\displaystyle H_{\text{kin}} =i,j,σα,βtijαβciασcjβσ\displaystyle=\sum_{i,j,\sigma}\sum_{\alpha,\beta}t^{\alpha\beta}_{ij}c^{\dagger}_{i\alpha\sigma}c_{j\beta\sigma} (2)
=k,σmEm(k)akmσakmσ,\displaystyle=\sum_{\textbf{k},\sigma}\sum_{m}E_{m}(\textbf{k})a^{\dagger}_{\textbf{k}m\sigma}a_{\textbf{k}m\sigma}, (3)

where Eq. (2) is the kinetic term in an orbital representation and Eq. (3) is in a band representation. ciασc^{\dagger}_{i\alpha\sigma} (ciασc_{i\alpha\sigma}) is a creation (annihilation) operator of an electron at site ii with spin σ(=,)\sigma\,(=\uparrow,\downarrow) and orbital α(=1,2,3,4)\alpha\,(=1,2,3,4) corresponding to (dx2y2d_{x^{2}-y^{2}}, dz2d_{z^{2}}, pxp_{x}, pyp_{y}), respectively. tijαβt^{\alpha\beta}_{ij} denotes a hopping integral between orbital α\alpha at site ii and orbital β\beta at site jj. tiiααt^{\alpha\alpha}_{ii} is a site energy εα\varepsilon_{\alpha} for orbital α\alpha at site ii. Equation (3) is obtained by diagonalizing Eq. (2), and the energy eigenvalue Em(k)E_{m}(\textbf{k}) is characterized by the wave vector k and the energy band index m(=1,2,3,4)m\,(=1,2,3,4). akmσa^{\dagger}_{\textbf{k}m\sigma} (akmσa_{\textbf{k}m\sigma}) is a creation (annihilation) operator of the corresponding energy band with spin σ\sigma. The undoped parent compounds of cuprates correspond to one hole (i.e., seven electrons) per unit cell in this model, which is conventionally referred to as half filling, and hereafter we denote the carrier density as the number δ\delta of holes per unit cell that are introduced into the system at half filling.

Refer to caption
Figure 1: (a) Schematic lattice structure of the four-band dd-pp model, forming the two-dimensional square lattice. Each Cu site contains dx2y2d_{x^{2}-y^{2}} and dz2d_{z^{2}} orbitals, while there is either pxp_{x} or pyp_{y} orbital on O sites. The lattice constant between the nearest-neighbor Cu sites is set to be one, i.e., primitive translation vectors |ex|=|ey|=1|\textbf{e}_{x}|=|\textbf{e}_{y}|=1. (b) Phase convention for the Cu dx2y2d_{x^{2}-y^{2}} orbital and the O pxp_{x} and pyp_{y} orbitals. Solid (open) ovals indicate the positive (negative) phase. The hopping integral between the dx2y2d_{x^{2}-y^{2}} and px/yp_{x/y} orbitals, t1t_{1}, is shown with the sign. The definitions of other hopping integrals (t2t6t_{2}-t_{6}) are described in Appendix A.1.

The Coulomb interaction term HintH_{\text{int}} is composed of eight terms,

Hint\displaystyle H_{\text{int}} =Udi(nid1nid1+nid2nid2)\displaystyle=U_{d}\sum_{i}\left(n^{d_{1}}_{i\uparrow}n^{d_{1}}_{i\downarrow}+n^{d_{2}}_{i\uparrow}n^{d_{2}}_{i\downarrow}\right)
+(UdJ2)inid1nid22JiSid1Sid2\displaystyle+\left(U^{\prime}_{d}-\frac{J}{2}\right)\sum_{i}n^{d_{1}}_{i}n^{d_{2}}_{i}-2J\sum_{i}\textbf{S}^{d_{1}}_{i}\cdot\textbf{S}^{d_{2}}_{i}
Ji(ci1ci1ci2ci2+ci2ci2ci1ci1)\displaystyle-J^{\prime}\sum_{i}\left(c^{\dagger}_{i1\uparrow}c^{\dagger}_{i1\downarrow}c_{i2\uparrow}c_{i2\downarrow}+c^{\dagger}_{i2\uparrow}c^{\dagger}_{i2\downarrow}c_{i1\uparrow}c_{i1\downarrow}\right)
+Upi(nipxnipx+nipynipy)+Vdpi,jnidnjpx/y\displaystyle+U_{p}\sum_{i}\left(n^{p_{x}}_{i\uparrow}n^{p_{x}}_{i\downarrow}+n^{p_{y}}_{i\uparrow}n^{p_{y}}_{i\downarrow}\right)+V_{dp}\sum_{\left<i,j\right>}n^{d}_{i}n^{p_{x/y}}_{j}
+Vppi,jnipxnjpy+Vddi,jnidnjd.\displaystyle+V_{pp}\sum_{\left<i,j\right>}n^{p_{x}}_{i}n^{p_{y}}_{j}+V_{dd}\sum_{\left<i,j\right>}n^{d}_{i}n^{d}_{j}. (4)

Here, niα=niα+niαn^{\alpha}_{i}=n^{\alpha}_{i\uparrow}+n^{\alpha}_{i\downarrow} with niσα=ciασciασn^{\alpha}_{i\sigma}=c^{\dagger}_{i\alpha\sigma}c_{i\alpha\sigma} is the number operator and Siα\textbf{S}^{\alpha}_{i} is the spin angular momentum operator at site ii with orbital α\alpha. d1d_{1} and d2d_{2} are abbreviations for dx2y2d_{x^{2}-y^{2}} and dz2d_{z^{2}} orbitals, respectively, and nid=nid1+nid2n^{d}_{i}=n^{d_{1}}_{i}+n^{d_{2}}_{i}. Ud,Ud,J,U_{d},U_{d}^{\prime},J, and JJ^{\prime} represent on-site intraorbital, interorbital, Hund’s coupling, and pair-hopping interactions between dd orbitals, respectively. In this study, we set J=JJ^{\prime}=J and Ud=Ud+2JU_{d}=U^{\prime}_{d}+2J [48]. The on-site intraorbital Coulomb interaction within pp orbitals, UpU_{p}, is also introduced. The last three terms in HintH_{\text{int}} take into account the intersite Coulomb interactions between nearest-neighbor orbitals, Vdp,Vpp,V_{dp},V_{pp}, and VddV_{dd}, as shown in Fig. 2, where the sum i,j\sum_{\left<i,j\right>} runs over all pairs of nearest-neighbor orbitals located at site ii and jj.

Refer to caption
Figure 2: The Coulomb interaction parameters between nearest-neighbor orbitals. Solid (open) circles represent Cu (O) atoms.

In addition, the following double counting correction term HdcH_{\text{dc}} is introduced,

Hdc=[{Ud+2(UdJ2)+16Vdd}nd0+8Vdpnp0]indi+{(Up+8Vpp)np0+8Vdpnd0}i(nipx+nipy),H_{\text{dc}}=\biggl{[}\left\{U_{d}+2\left(U^{\prime}_{d}-\frac{J}{2}\right)+16V_{dd}\right\}\langle n^{d}\rangle_{0}\ \\ +8V_{dp}\left<n^{p}\right>_{0}\biggr{]}\sum_{i}n^{d}_{i}\\ +\left\{(U_{p}+8V_{pp})\left<n^{p}\right>_{0}+8V_{dp}\langle n^{d}\rangle_{0}\right\}\sum_{i}(n^{p_{x}}_{i}+n^{p_{y}}_{i}), (5)

where nd0=1NSinid\langle n^{d}\rangle_{0}=\frac{1}{N_{\text{S}}}\sum_{i}\langle n^{d}_{i}\rangle and np0=1NSi(nipx+nipy)\left<n^{p}\right>_{0}=\frac{1}{N_{\text{S}}}\sum_{i}\langle(n^{p_{x}}_{i}+n^{p_{y}}_{i})\rangle are the average electron density of the dd and pp orbitals in the noninteracting limit and NSN_{\text{S}} is the total number of unit cells. When we apply a many-body calculation method to a multiorbital model, the site energy of each orbital is shifted due to the interaction effect. However, such energy shifts have already been included in the energy band of the tight-binding model constructed from the first-principles calculation. This is a so-called double counting problem and should be treated with care especially in the dd-pp model [49]. Here, we subtract the term HdcH_{\text{dc}} from the Hamiltonian to correct the energy shift. This is one of the reasonable treatments to avoid the double counting.

Table 1: The tight-binding parameters for the La2CuO4 and HgBa2CuO4 systems in eV units estimated on the basis of maximally localized Wannier orbitals from the first-principles LDA calculation. For comparison, the tight-binding parameters for the La2CuO4 system with reference to the QSGW method are also shown (denoted as “revised”). The definitions of tit_{i} and εα\varepsilon_{\alpha} are described in Appendix A.1. Δdp=εdx2y2εp\Delta_{dp}=\varepsilon_{d_{x^{2}-y^{2}}}-\varepsilon_{p}, i.e., the site-energy difference between the Cu dx2y2d_{x^{2}-y^{2}} and O px/yp_{x/y} orbitals.
t1t_{1} t2t_{2} t3t_{3} t4t_{4} t5t_{5} t6t_{6} εdx2y2\varepsilon_{d_{x^{2}-y^{2}}} εdz2\varepsilon_{d_{z^{2}}} εpx/y\varepsilon_{p_{x/y}} Δdp\Delta_{dp}
La2CuO4 1.42 0.61 0.07 0.65 0.05 0.07 -0.87 -0.11 -3.13 2.26
La2CuO4(revised) 1.42 0.61 0.07 0.51 0.03 0.07 -0.87 -0.68 -3.13 2.26
HgBa2CuO4 1.26 0.65 0.13 0.33 0.00 0.05 -1.41 -1.68 -3.25 1.84
Refer to caption
Figure 3: The energy dispersions and projected density of states onto the dx2y2d_{x^{2}-y^{2}}, dz2d_{z^{2}}, and px/yp_{x/y} orbitals for the noninteracting tight-binding models for (a) La2CuO4, (b) La2CuO4(revised), and (c) HgBa2CuO4 systems. The tight-binding parameters are given in Table 1. Fermi energy (defined as zero energy) is set to be the case of 15% hole doping (δ\delta=0.15). The high symmetric momenta are indicated as Γ=(0,0)\Gamma=(0,0), M=(π,π)\text{M}=(\pi,\pi), and X=(π,0)\text{X}=(\pi,0).

II.2 VMC method

The effect of Coulomb interaction is treated using a VMC method [50, 51, 52]. The trial wave function considered here is a Gutzwiller-Jastrow type composed of four parts,

|Ψ=PG(2)PJcPJs|Φ.\left|\Psi\right>=P^{(2)}_{\text{G}}P_{\text{J}_{\text{c}}}P_{\text{J}_{\text{s}}}\left|\Phi\right>. (6)

|Φ\left|\Phi\right> is a one-body part constructed by diagonalizing the one-body Hamiltonian including the off-diagonal elements {ρiα}\{\rho^{\alpha}_{i}\}, {miα}\{m^{\alpha}_{i}\}, and {Δijαβ}\{\Delta^{\alpha\beta}_{ij}\}, which induce long-range ordering of charge, spin, and superconductivity, respectively. The renormalized hopping integrals {t~ijαβ}\{\tilde{t}^{\alpha\beta}_{ij}\} are also included in |Φ\left|\Phi\right> as variational parameters. The explicit forms of them are described in Appendix.

The Gutzwiller factor

PG(2)=i,γ[egγ|γγ|i]P^{(2)}_{\text{G}}=\prod_{i,\gamma}\bigl{[}\text{e}^{-g_{\gamma}}\left|\gamma\right>\left<\gamma\right|_{i}\bigr{]} (7)

is extended to two-orbital systems [53, 54]. In PG(2)P^{(2)}_{\text{G}}, possible 16 patterns of charge and spin configuration of the dx2y2d_{x^{2}-y^{2}} and dz2d_{z^{2}} orbitals at each site |γ\left|\gamma\right>, i.e., |0=|0 0\left|0\right>=\left|0\;0\right>, |1=|0\left|1\right>=\left|0\uparrow\right>, \cdots, |15=|\left|15\right>=\left|\uparrow\downarrow\;\uparrow\downarrow\right>, are differently weighted with egγ\text{e}^{-g_{\gamma}} and {gγ}\{g_{\gamma}\} are optimized as variational parameters.

The remaining operators

PJc=exp[i,jα,βvijαβcniαnjβ]P_{\text{J}_{\text{c}}}=\exp\Bigl{[}-\sum_{i,j}\sum_{\alpha,\beta}v^{\text{c}}_{ij\alpha\beta}n^{\alpha}_{i}n^{\beta}_{j}\Bigr{]} (8)

and

PJs=exp[i,jα,βvijαβssiαzsjβz]P_{\text{J}_{\text{s}}}=\exp\Bigl{[}-\sum_{i,j}\sum_{\alpha,\beta}v^{\text{s}}_{ij\alpha\beta}s^{z}_{i\alpha}s^{z}_{j\beta}\Bigr{]} (9)

are charge and spin Jastrow factors, which control long-range charge and spin correlations, respectively. siαzs^{z}_{i\alpha} is the zz component of the spin angular momentum operator at site ii with orbital α\alpha. We set viiαβc=viiαβs=0v^{\text{c}}_{ii\alpha\beta}=v^{\text{s}}_{ii\alpha\beta}=0 for α,β=d1,d2\alpha,\beta=d_{1},d_{2} because the on-site correlation between the dx2y2d_{x^{2}-y^{2}} and dz2d_{z^{2}} orbitals are already taken into account in PG(2)P^{(2)}_{\text{G}}.

In this paper, we focus mainly on the superconducting correlation functions to examine where the superconductivity appears in the phase diagram. The detailed studies on other competing orders will be discussed elsewhere. The variational parameters in |Ψ\left|\Psi\right> are therefore {t~ijαβ}\{\tilde{t}^{\alpha\beta}_{ij}\}, {Δijαβ}\{\Delta^{\alpha\beta}_{ij}\}, {gγ}\{g_{\gamma}\}, {vijαβc}\{v^{\text{c}}_{ij\alpha\beta}\}, and {vijαβs}\{v^{\text{s}}_{ij\alpha\beta}\}. They are simultaneously optimized using stochastic reconfiguration method [55]. We show results for NSN_{\text{S}}=24×\times24=576 unit cells (and thus 576×\times4=2304 orbitals in total), which is large enough to avoid finite size effects. The antiperiodic boundary conditions are set for both xx and yy directions of the primitive lattice vectors.

III RESULTS

III.1 Band structures of La2CuO4 and HgBa2CuO4

First, we discuss the material dependence of the band structure. As a typical example of single-layer hole-doped cuprates, we study the La2CuO4 and HgBa2CuO4 systems. We construct maximally localized Wannier orbitals [56, 57] from the first-principles calculation in the local-density approximation (LDA) with ecalj package [58] and fit them with the hopping integrals tit_{i} (i=16i=1-6) and the site energy of each orbital εα\varepsilon_{\alpha}. The parameter sets determined for these systems are listed in Table 1 and the explicit form of the tight-binding model is described in Appendix A.1. Note that the estimated site energy of the Cu dz2d_{z^{2}} orbital, εdz2\varepsilon_{d_{z^{2}}}, and the hybridization between the Cu dz2d_{z^{2}} and O px/yp_{x/y} orbitals, t4t_{4}, depend significantly on the method of first-principles calculation. In fact, the estimated εdz2\varepsilon_{d_{z^{2}}} is much lower in the quasiparticle self-consistent GWGW (QSGW) method [61, 62, 63] than in the conventional LDA calculation [64]. To clarify the effect, we also consider another parameter set of La system with reference to the QSGW band structure (labeled as “revised”), where the site energy εdz2\varepsilon_{d_{z^{2}}} is lower and t4t_{4} is also slightly smaller than those estimated on the basis of the LDA calculation (See Table 1).

Figure 3 shows the noninteracting tight-binding energy bands for La and Hg systems. We can notice the clear difference among them: (i) The density of states (DOS) of the dz2d_{z^{2}} component is extended from 0 to -2 eV in the La system [Fig. 3(a)], while it is almost localized around -2 eV in the Hg system [Fig. 3(c)]. This is because the dz2d_{z^{2}} orbital is hybridized with the px/yp_{x/y} orbital in the La system much more strongly than in the Hg system. The dz2d_{z^{2}} electrons obtain the itinerancy through the hybridization and therefore the dz2d_{z^{2}} component of the La system is more extended than that of the Hg system. The revised version of the La system is located somewhere in between [Fig. 3(b)]. (ii) The site-energy difference between the dx2y2d_{x^{2}-y^{2}} and px/yp_{x/y} orbitals, Δdp=εdx2y2εp\Delta_{dp}=\varepsilon_{d_{x^{2}-y^{2}}}-\varepsilon_{p}, is larger in the La system than in the Hg system. This affects the occupancy of each orbital and thus the strength of the electron correlation. For example, when Δdp(>0)\Delta_{dp}\,(>0) is small, the energy band crossing the Fermi energy contains more component of the px/yp_{x/y} orbital, in which the intraorbital Coulomb interaction is smaller.

Starting from these energy band structures, we shall investigate the ground state property of the La and Hg systems using the VMC method. We assume that the tight-binding parameters remain unchanged with hole doping. The Coulomb interaction parameters are set as (Ud,Ud,J,Up,Vdp,Vpp)=(8.0,6.4,0.8,4.0,2.0,1.6)t1(U_{d},U^{\prime}_{d},J,U_{p},V_{dp},V_{pp})=(8.0,6.4,0.8,4.0,2.0,1.6)\;t_{1} for both La and Hg systems with reference to Ref. [65]. Note that the values for the La system are larger in eV units because of the larger t1t_{1}. In the following, we set t1t_{1} as a unit of energy. We first set Vdd=0V_{dd}=0 and then discuss the effect of finite VddV_{dd}. As shown in Sec. III.3, we find that even small VddV_{dd} can substantially affect the property of the system.

III.2 Superconducting correlation function

III.2.1 Overview

To discuss the material dependence of superconductivity, we calculate the superconducting correlation function defined as

Pdd(r)=1NSiτ,τfττ(dd)<Δτ(Ri)Δτ(Ri+r)>,P^{dd}(\textbf{r})=\frac{1}{N_{\text{S}}}\sum_{i}\sum_{\tau,\tau^{\prime}}f^{(dd)}_{\tau\tau^{\prime}}\bigl{<}\Delta^{\dagger}_{\tau}(\textbf{R}_{i})\Delta_{\tau^{\prime}}(\textbf{R}_{i}+\textbf{r})\bigr{>}, (10)

where Δτ(Ri)\Delta^{\dagger}_{\tau}(\textbf{R}_{i}) is a creation operator of singlet pairs between nearest-neighbor dx2y2d_{x^{2}-y^{2}} orbitals,

Δτ(Ri)=12(ci1ci+τ1+ci+τ1ci1),\Delta^{\dagger}_{\tau}(\textbf{R}_{i})=\frac{1}{\sqrt{2}}(c^{\dagger}_{i1\uparrow}c^{\dagger}_{i+\tau 1\downarrow}+c^{\dagger}_{i+\tau 1\uparrow}c^{\dagger}_{i1\downarrow}), (11)

and τ\tau runs over four nearest-neighbor Cu sites (τ=±𝐞x,±𝐞y\tau=\pm\mathbf{e}_{x},\pm\mathbf{e}_{y}). fττ(dd)f^{(dd)}_{\tau\tau^{\prime}} is a form factor of a superconducting gap function with dx2y2d_{x^{2}-y^{2}} symmetry, namely, fττ(dd)=1f^{(dd)}_{\tau\tau^{\prime}}=1 for ττ\tau\parallel\tau^{\prime} and 1-1 for ττ\tau\perp\tau^{\prime}. \langle\cdots\rangle denotes Ψ||Ψ/Ψ|Ψ\langle\Psi|\cdots|\Psi\rangle/\langle\Psi|\Psi\rangle for the optimized variational wave function |Ψ|\Psi\rangle. If Pdd(r)P^{dd}(\textbf{r}) is saturated to a finite value for r=|𝐫|r=|\mathbf{r}|\rightarrow\infty, superconducting long-range order exists.

Refer to caption
Figure 4: (a) Superconducting correlation function Pdd(r)P^{dd}(r) and Pdp(r)P^{dp}(r) for the Hg system at a hole doping rate δ=0.153\delta=0.153. The sign change of (b) dd-dd and (c) dd-pp pairings. Cu (O) sites are indicated by solid (open) circles in (b) and (c).

Figure 4(a) shows the behavior of Pdd(r=|r|)P^{dd}(r=|\textbf{r}|) for the Hg system at a hole doping rate δ=0.153\delta=0.153. It shows good convergence for r4r\gtrsim 4 and reveals that the superconducting long-range order certainly exists. The sign of the dd-dd pairing in a real space is shown in Fig. 4(b). It is positive in the xx direction and negative in the yy direction, reflecting the dx2y2d_{x^{2}-y^{2}}-wave symmetry expected in cuprate superconductors. We also calculate the superconducting correlation function for pairing formed between the dx2y2d_{x^{2}-y^{2}} and px/yp_{x/y} orbitals Pdp(r)P^{dp}(r), which is defined in the same way as Pdd(r)P^{dd}(r) except that ci+τ1σc^{\dagger}_{i+\tau 1\sigma} in Eq. (11) is replaced with ci+τ23(4)σc^{\dagger}_{i+\frac{\tau}{2}3(4)\sigma} for τ=±ex(y)\tau=\pm\textbf{e}_{x(y)}. Although the value is one order of magnitude smaller than Pdd(r)P^{dd}(r) [see Fig. 4(a)], Pdp(r)P^{dp}(r) is also saturated to a finite value, indicative of the long-range order of dd-pp pairing. Note that the sign of the dd-pp pairing changes alternatively along both xx and yy directions and thus shows pp-like symmetry as shown in Fig. 4(c). This is due to the phase convention of pxp_{x} and pyp_{y} orbitals adopted here [see Fig. 1(b)] and is consistent with the dx2y2d_{x^{2}-y^{2}} pairing symmetry [66]. It is also compatible with the preceding study of the three-band dd-pp model [45]. This kind of real space or orbital representation is useful for the analysis of cuprate superconductors [43, 44, 47] because the pairing length is expected to be very short [67].

Refer to caption
Figure 5: PddP^{dd} as a function of the hole doping rate δ\delta for the three systems.

III.2.2 Material dependence: Effect of dz2d_{z^{2}} orbital

Let us now examine the material and doping dependence of the superconducting correlation function. We take the converged value of Pdd(r)P^{dd}(r\rightarrow\infty) as a strength of superconductivity PddP^{dd}. Figure 5 shows the doping dependence of PddP^{dd} for the La, La(revised), and Hg systems. For all cases, PddP^{dd} displays a dome shape as a function of the hole doping rate δ\delta. At δ=0\delta=0, the system is insulating due to the strong correlation effect and thus Pdd=0P^{dd}=0. As δ\delta increases, mobile carriers are introduced into the system and the mobility of the Cooper pair increases. On the other hand, the strength of the dd-dd pairing itself is reduced by doping because the electron correlation effect is also reduced. The balance between these two factors results in the dome-shaped behavior of PddP^{dd}. This picture is expected to be universal for all hole-doped cuprate superconductors.

Refer to caption
Figure 6: Total and α\alpha orbital components of momentum distribution function for the La system at (a) δ=0.153\delta=0.153 (superconducting phase) and (b) δ=0.181\delta=0.181 (paramagnetic metallic phase). The high symmetric momenta are indicated as Γ=(0,0)\Gamma=(0,0), M=(π,π)\text{M}=(\pi,\pi), and X=(π,0)\text{X}=(\pi,0).

Next, let us study the importance of the orbital character near the Fermi energy in the material dependence of superconductivity. Generally, a large DOS at the Fermi energy is favorable for superconductivity due to the large energy gain of gap opening. However, a detailed structure of the DOS, namely, the orbital character and 𝐤\mathbf{k} dependence should be carefully investigated. For this purpose, we calculate the following momentum distribution function of holes,

nα(k)=12σckασckασ,n^{\alpha}(\textbf{k})=\frac{1}{2}\sum_{\sigma}\langle c_{\textbf{k}\alpha\sigma}c^{\dagger}_{\textbf{k}\alpha\sigma}\rangle, (12)

where ckασc^{\dagger}_{\textbf{k}\alpha\sigma} (ckασc_{\textbf{k}\alpha\sigma}) is a Fourier transform of ciασc^{\dagger}_{i\alpha\sigma} (ciασc_{i\alpha\sigma}) in Eq. (2). Figure 6 shows nα(k)n^{\alpha}(\textbf{k}) for the La system at the superconducting phase (δ=0.153\delta=0.153) and the paramagnetic metallic phase (δ=0.181\delta=0.181). The discontinuities around the X point and in the middle of the Γ\Gamma-M line in Fig. 6(b) for the paramagnetic metallic phase indicate the existence of Fermi surface. Since the node of the superconducting gap runs along the Γ\Gamma-M line, a discontinuity also exists in the superconducting phase, as shown in Fig. 6(a). We can observe that the dz2d_{z^{2}} component has large weight around the X point, exhibiting a peak structure in nα(k)n^{\alpha}(\textbf{k}), where the superconducting gap becomes the largest (so-called “hot spot”). This feature is expected to be unfavorable for superconductivity because the AF spin fluctuation, which promotes the dx2y2d_{x^{2}-y^{2}}-wave pairing, is suppressed when the Cu dz2d_{z^{2}} orbital contributes to the formation of the Fermi surface [68].

Refer to caption
Figure 7: (a) δ\delta dependence of the ratio RR of the dz2d_{z^{2}} component to the total at the X point for the three systems. Solid (open) symbols represent the superconducting (paramagnetic metallic) phase. (b) δ\delta dependence of the quasiparticle renormalization factor zz for the three systems. Symbols are the same with those in (a).

To investigate the effect of the dz2d_{z^{2}} component, the ratio of the dz2d_{z^{2}} component to the total at the X point, R=ndz2(X)/ntot(X)R=n^{d_{z^{2}}}(\text{X})/n^{\text{tot}}(\text{X}), is calculated in Fig 7(a). For the La system, the ratio RR increases with increasing δ\delta and shows rapid enhancement for δ>0.16\delta>0.16. It coincides with the sudden disappearance of PddP^{dd} for δ>0.16\delta>0.16 shown in Fig. 5. On the other hand, RR for the La(revised) system is much smaller than that of the La system, because εdz2\varepsilon_{d_{z^{2}}} is lower and the hybridization between the dz2d_{z^{2}} and dx2y2d_{x^{2}-y^{2}} orbitals via the px/yp_{x/y} orbitals is smaller. As a result, the superconducting phase is extended to a larger value of δ\delta and a smooth dome shape is observed in PddP^{dd} vs. δ\delta as shown in Fig. 5. For the Hg system, RR is much more suppressed because the dz2d_{z^{2}}-orbital based band is almost localized and detached from the dx2y2d_{x^{2}-y^{2}}-orbital based band [see Fig. 3(c)]. This is an ideal condition for superconductivity [18] and therefore PddP^{dd} becomes largest for the Hg system.

These results conclude that superconductivity is more enhanced when the dz2d_{z^{2}}-orbital based band is deeply sinking and its contribution to the low-energy physics is small. Therefore, the material dependence of superconductivity is understood only by incorporating the dz2d_{z^{2}} orbital explicitly into a model such as our model, which is a remarkable advantage over the usual one-band Hubbard and tt-JJ models, and even the three-band dd-pp model.

PddP^{dd} calculated here corresponds to the square of the superconducting order parameter and is closely related to the superconducting transition temperature TcT_{\text{c}}. The critical doping rate δc\delta_{\text{c}} for the La system, where PddP^{dd} becomes zero, seems to be too small (0.16\sim 0.16) compared with the experimental value (δc=0.250.3\delta_{\text{c}}=0.25-0.3). Furthermore, the sudden disappearance of PddP^{dd} is also unrealistic. It can be inferred that the actual value of εdz2\varepsilon_{d_{z^{2}}} is much lower than the value estimated from the LDA calculation. Indeed, as shown in Table 1, the value of εdz2\varepsilon_{d_{z^{2}}} with reference to the QSGW calculation is much lower. Furthermore, the QSGW band structure [64] can well explain the resonant inelastic X-ray scattering experiment [69]. We expect that the revised band structure shown in Fig. 3(b) properly includes the correction for the LDA calculation and gives more realistic result for the La system.

III.2.3 Material dependence: Effect of apical oxygen height

From the viewpoint of the actual lattice structure, εdz2\varepsilon_{d_{z^{2}}} is governed by the apical oxygen height, i.e., the distance between the apical oxygen and the copper: The larger the apical oxygen height is, the lower εdz2\varepsilon_{d_{z^{2}}} is with respect to εdx2y2\varepsilon_{d_{x^{2}-y^{2}}}, because of the crystal field effect [70, 68]. In addition, a larger apical oxygen height leads to a lower site energy εpz\varepsilon_{p_{z}} of the apical oxygen due to the decrease of a crystal field effect, which in turn lowers the εdz2\varepsilon_{d_{z^{2}}} through the hybridization between pzp_{z} and dz2d_{z^{2}} orbitals despite the increase of the distance between apical oxygen and the copper. Therefore, our result suggests that a larger apical oxygen height leads to a higher TcT_{\text{c}} through a lower εdz2\varepsilon_{d_{z^{2}}}. Indeed, the experimentally observed apical oxygen height of the Hg system is larger than that of the La system. This tendency is also consistent with the so-called Maekawa’s plot [71], where a lower εpz\varepsilon_{p_{z}} is related to a higher TcT_{\text{c}}. Although the model itself does not explicitly include the pzp_{z} orbital of the apical oxygen, the present four-band dd-pp model properly incorporates the effect of the apical oxygen height via adjusting the site energy εdz2\varepsilon_{d_{z^{2}}}.

III.2.4 Material dependence: Effect of Δdp\Delta_{dp}

We also show in Fig. 7(b) the quasiparticle renormalization factor zz estimated from the jumps in the total momentum distribution function ntot(k)n^{\text{tot}}(\textbf{k}) along the nodal direction of the dx2y2d_{x^{2}-y^{2}}-wave superconducting gap. At δ=0\delta=0, the system is insulating and thus z=0z=0. With increasing δ\delta, zz increases according to the decrease of the electron correlation effect. We find that zz for the La system is smaller than that for the Hg system, indicating that the electron correlation effect is stronger in the La system. This can be attributed to the larger Δdp=εdx2y2εp\Delta_{dp}=\varepsilon_{d_{x^{2}-y^{2}}}-\varepsilon_{p} for the La system, which results in the larger dd-orbital occupancy of holes when it is doped. The electron correlation has a dual effect: One is to enhance the superconducting pairing and the other is to reduce the mobility of Cooper pairs. In the present case, the latter effect would be dominant and thus PddP^{dd} for the La system is suppressed compared with the Hg system. This tendency is consistent with the negative correlation between Δdp\Delta_{dp} and TcT_{\text{c}} as mentioned in Sec. I.

Refer to caption
Figure 8: Ground state phase diagram for the Hg system at δ=0\delta=0 (a) within the paramagnetic phase and (b) with the AF phase. The dotted curve in (b) corresponds to the solid curve in (a). Green stars in (a) and (b) represent the parameters used in Fig. 9.

III.3 Effect of VddV_{dd}

Now we discuss the effect of the Coulomb interaction between nearest-neighbor dd orbitals, VddV_{dd}. VddV_{dd} is expected to be smaller than other Coulomb interactions, Ud,Ud,Up,VdpU_{d},U^{\prime}_{d},U_{p},V_{dp}, and VppV_{pp} [65]. However, VddV_{dd} directly affects the charge and spin correlations between nearest-neighbor dd electrons, which dominate the properties of cuprate superconductors. As discussed in this section, we verify that the superconductivity in the model studied here is more sensitive to the value of VddV_{dd} than other Coulomb interactions. Hereafter, we treat only UdU_{d} and VddV_{dd} as independent parameters, and set other Coulomb interactions as (Ud,J,Up,Vdp,Vpp)=(0.8,0.1,0.5,0.25,0.2)Ud(U^{\prime}_{d},J,U_{p},V_{dp},V_{pp})=(0.8,0.1,0.5,0.25,0.2)\;U_{d} with reference to Ref. [65]

Refer to caption
Figure 9: PddP^{dd} as a function of the hole doping rate δ\delta at Ud/t1=8U_{d}/t_{1}=8 and Vdd/t1=0,0.3,0.6V_{dd}/t_{1}=0,0.3,0.6 for the Hg system.

Figure 8(a) shows the ground state phase diagram for the Hg system at δ=0\delta=0 within the paramagnetic phase. When Vdd=0V_{dd}=0, a metal-insulator transition occurs at Ud/t16.3U_{d}/t_{1}\sim 6.3, assuming the paramagnetic phase. The metal-insulator transition is detected by monitoring the jump in the total momentum distribution function ntot(k)n^{\text{tot}}(\textbf{k}) as well as the long-range behavior of the charge Jastrow factor PJcP_{\text{J}_{\text{c}}} [72]. This transition is a Mott metal-insulator transition because δ=0\delta=0 corresponds to the case with one hole per unit cell, nhole=1n_{\text{hole}}=1, where the system cannot be a band insulator. With the introduction of small but finite VddV_{dd} (one order of magnitude smaller than UdU_{d}), the metallic region is substantially enlarged. This is understood because the densities of empty sites and doubly-occupied sites increase to reduce the energy loss of VddV_{dd}, thus effectively weakening UdU_{d} by VddV_{dd}, and then the insulating phase is destabilized.

It is noteworthy that the AF insulator is always more stable than the paramagnetic insulator in the present parameter space. With increasing UdU_{d}, the system undergoes the phase transition from the metallic phase to a Slater-type AF insulator [a blue line in Fig. 8(b)], followed by the crossover to a Mott-type AF insulator [a red dotted line in Fig. 8(b)]. Here, a Slater-type AF insulator is an insulator that becomes metallic without AF order, while a Mott-type AF insulator is an insulator that remains insulating without AF order. The crossover line in Fig. 8(b) is hence identical with the paramagnetic metal-insulator transition line in Fig. 8(a). As explained next, it is crucially important for the appearance of high-TcT_{\text{c}} superconductivity whether the AF insulator in the parent compounds (δ\delta=0) is Slater-type or Mott-type [31, 32, 73, 72].

Next we study the effect of VddV_{dd} on superconductivity. Figure 9 shows the superconducting correlation function PddP^{dd} at Ud/t1=8U_{d}/t_{1}=8 and Vdd/t1=0,0.3,V_{dd}/t_{1}=0,0.3, and 0.6 for the Hg system. As VddV_{dd} increases, PddP^{dd} is suppressed and the peak position is moved to a smaller value of δ\delta. In particular, a significant suppression is observed when Vdd/t1=0.6V_{dd}/t_{1}=0.6. In this case, PddP^{dd} vs. δ\delta does not show a dome-shaped behavior but instead an almost monotonic decrease, which rather reminds us of electron-doped cuprates [74, 75]. This observation of PddP^{dd} vs. δ\delta corresponds to the fact that the system is out of the Mott insulator region at δ=0\delta=0 (see Fig. 8). The view of a “doped Mott insulator” is thus no longer valid. Similar claims have been made in the study of one-band Hubbard models [76, 77]. Our result suggests that it is essential to start from the Mott insulator region at δ=0\delta=0 to reproduce the dome-shaped behavior observed experimentally in hole-doped cuprates. This can be considered as a good criterion for choosing the reasonable Coulomb interaction parameters of an effective model for cuprates.

III.4 Phase competition

Finally, we briefly discuss the competition between superconductivity and other phases. The energy comparison among various phases in the ground state is a subtle problem and depends significantly on the numerical methods. The VMC method used here tends to overestimate the magnetic long-range ordered phases, although it is much improved as compared with a mean-field type approximation. In fact, we find that the AF phase and the stripe phase with both spin and charge modulations have lower variational energies than dx2y2d_{x^{2}-y^{2}}-wave superconductivity for δ<0.3\delta<0.3. Nevertheless, we believe that the present results capture the essence of the material dependence of cuprate superconductors and the conclusion is unchanged, when the improved wave functions incorporating the quantum fluctuations suppress these overestimated competing orders. We also note that the effect of VddV_{dd} is also important for the phase competition. This is because most of the competing phases including the phase separation are governed by the correlation between nearest-neighbor dd electrons. This is also the case in the one-band Hubbard model [78, 79]. The detailed ground state phase diagram, including various competing phases, for the four-band dd-pp model is left for a future study.

IV DISCUSSION AND SUMMARY

To obtain the unified description of cuprate superconductors, we have studied the four-band dd-pp model for the La2CuO4 and HgBa2CuO4 systems. We have shown that a lower εdz2\varepsilon_{d_{z^{2}}} with respect to εdx2y2\varepsilon_{d_{x^{2}-y^{2}}} and a smaller Δdp(>0)\Delta_{dp}(>0) lead to a higher TcT_{\text{c}}. The former results in a more localized dz2d_{z^{2}}-orbital based band that do not interfere the superconductivity. The latter results in a larger zz, namely, a weaker electron correlation effect, which promotes the itinerancy of mobile carriers and thus enhances superconductivity. The present four-band dd-pp model covers these two factors, beyond the usual one-band and even three-band dd-pp models. Therefore, this model is considered to be a minimal model that can properly describe the material dependence of cuprate superconductors, and thus it can also provide a valuable guideline to design new materials with a higher TcT_{\text{c}}.

The effect of VddV_{dd} has also been investigated. Although the value of VddV_{dd} is small compared with other Coulomb interaction parameters, it substantially affects the ground state property of the system. VddV_{dd} weakens the effective UdU_{d} and induces the paramagnetic metal-insulator transition, or the crossover from a Slater insulator to a Mott insulator. The stability of superconductivity is also affected by VddV_{dd}. Considering the doping dependence, we have to start from the Mott insulator region at δ=0\delta=0 to obtain the stable superconductivity and the dome-shaped dependence of PddP^{dd} as a function of δ\delta. Therefore, the appropriate estimation of VddV_{dd} is important for the modelling of cuprates, as in other strongly-correlated electron systems where various phases compete.

Acknowledgements.
The authors thank K. Kuroki for useful discussions. The computation has been done using the facilities of the Supercomputer Center, Institute for Solid State Physics, University of Tokyo and the supercomputer system HOKUSAI in RIKEN. This work was supported by a Grant-in-Aid for Scientific Research on Innovative Areas “Quantum Liquid Crystals” (KAKENHI Grant No. JP19H05825) from JSPS of Japan, and also supported by JSPS KAKENHI (Grant Nos. JP21H04446, JP20K03847, JP19K23433, JP19H01842, and JP18H01183).

*

Appendix A Construction of the trial wave function

Here, we describe the details of the trial wave function together with the noninteracting tight-binding model obtained on the basis of the first-principles calculations in Sec. III.1. The construction of the trial wave function is the most important part for the VMC method. Depending on the trial state, both real and k space representations are used.

A.1 Noninteracting energy band

First, we describe how to construct the noninteracting tight-binding energy band discussed in Sec. III.1. The noninteracting energy band is obtained by diagonalizing the following one-body Hamiltonian:

Hkin\displaystyle H_{\text{kin}} =k,σ(ck1σ,ck2σ,ck3σ,ck4σ)(t11t21t31t41t21t22t32t42t31t32t33t43t41t42t43t44)(ck1σck2σck3σck4σ)\displaystyle=\sum_{\textbf{k},\sigma}\left(c_{\textbf{k}1\sigma}^{\dagger},c_{\textbf{k}2\sigma}^{\dagger},c_{\textbf{k}3\sigma}^{\dagger},c_{\textbf{k}4\sigma}^{\dagger}\right)\begin{pmatrix}t_{11}&t^{*}_{21}&t^{*}_{31}&t^{*}_{41}\\ t_{21}&t_{22}&t^{*}_{32}&t^{*}_{42}\\ t_{31}&t_{32}&t_{33}&t^{*}_{43}\\ t_{41}&t_{42}&t_{43}&t_{44}\end{pmatrix}\begin{pmatrix}c_{\textbf{k}1\sigma}\\ c_{\textbf{k}2\sigma}\\ c_{\textbf{k}3\sigma}\\ c_{\textbf{k}4\sigma}\end{pmatrix} (13)
=k,σmEm(k)akmσakmσ\displaystyle=\sum_{\textbf{k},\sigma}\sum_{m}E_{m}(\textbf{k})a^{\dagger}_{\textbf{k}m\sigma}a_{\textbf{k}m\sigma} (14)

with the hopping matrix elements given as

t11\displaystyle t_{11} =εdx2y2,\displaystyle=\varepsilon_{d_{x^{2}-y^{2}}}, (15)
t21\displaystyle t_{21} =0,\displaystyle=0, (16)
t22\displaystyle t_{22} =εdz22t5(coskx+cosky),\displaystyle=\varepsilon_{d_{z^{2}}}-2t_{5}(\cos k_{x}+\cos k_{y}), (17)
t31\displaystyle t_{31} =2it1sin12kx,\displaystyle=2\text{i}t_{1}\sin\frac{1}{2}k_{x}, (18)
t32\displaystyle t_{32} =2it4sin12kx,\displaystyle=-2\text{i}t_{4}\sin\frac{1}{2}k_{x}, (19)
t33\displaystyle t_{33} =εpx+2t3coskx+2t6[cos(kx+ky)+cos(kxky)],\displaystyle=\varepsilon_{p_{x}}+2t_{3}\cos k_{x}+2t_{6}[\cos(k_{x}+k_{y})+\cos(k_{x}-k_{y})], (20)
t41\displaystyle t_{41} =2it1sin12ky,\displaystyle=-2\text{i}t_{1}\sin\frac{1}{2}k_{y}, (21)
t42\displaystyle t_{42} =2it4sin12ky,\displaystyle=-2\text{i}t_{4}\sin\frac{1}{2}k_{y}, (22)
t43\displaystyle t_{43} =2t2[cos(12kx+12ky)cos(12kx12ky)],\displaystyle=2t_{2}\left[\cos\left(\frac{1}{2}k_{x}+\frac{1}{2}k_{y}\right)-\cos\left(\frac{1}{2}k_{x}-\frac{1}{2}k_{y}\right)\right], (23)
t44\displaystyle t_{44} =εpy+2t3cosky+2t6[cos(kx+ky)+cos(kxky)],\displaystyle=\varepsilon_{p_{y}}+2t_{3}\cos k_{y}+2t_{6}[\cos(k_{x}+k_{y})+\cos(k_{x}-k_{y})], (24)

where ckασc^{\dagger}_{\textbf{k}\alpha\sigma} (ckασc_{\textbf{k}\alpha\sigma}) is a creation (annihilation) operator of an electron with momentum k, spin σ(=,)\sigma\,(=\uparrow,\downarrow), and orbital α(=1,2,3,4)\alpha\,(=1,2,3,4) corresponding to (dx2y2d_{x^{2}-y^{2}}, dz2d_{z^{2}}, pxp_{x}, pyp_{y}), respectively. The bonds between nearest-neighbor Cu sites are set as unit vectors (|ex|=|ey|=1|\textbf{e}_{x}|=|\textbf{e}_{y}|=1) and the bonds between nearest-neighbor Cu and O sites are one-half of them (see Fig. 1). The hopping integrals tit_{i} (i=16i=1-6) and the site energy of each orbital εα\varepsilon_{\alpha} are determined by fitting the band structures that are obtained by the LDA or QSGW calculation. The specific values for the La, La(revised), and Hg systems are listed in Table 1. Equation (14) is obtained by diagonalizing the Hamiltonian matrix in Eq. (13) and is the same with Eq. (3) in Sec. II.1. Em(k)E_{m}(\textbf{k}) is the noninteracting energy band characterized by the wave vector k and the energy band index m(=1,2,3,4)m\,(=1,2,3,4) with akmσa^{\dagger}_{\textbf{k}m\sigma} (akmσa_{\textbf{k}m\sigma}) being a creation (annihilation) operator of the corresponding energy band with spin σ\sigma.

A.2 Trial wave function

A.2.1 Superconductivity

To construct the trial wave function for superconductivity, we employ the Bogoliubov de-Gennes (BdG) type Hamiltonian in real space [80], i.e.,

HBdG=i,jα,β(ciα,ciα)(TijαβΔijαβΔjiαβTjiαβ)(cjβcjβ).H_{\text{BdG}}=\sum_{i,j}\sum_{\alpha,\beta}\left(c^{\dagger}_{i\alpha\uparrow},c_{i\alpha\downarrow}\right)\begin{pmatrix}T^{\alpha\beta}_{ij\uparrow}&\Delta^{\alpha\beta}_{ij}\\ \Delta^{\alpha\beta*}_{ji}&-T^{\alpha\beta}_{ji\downarrow}\end{pmatrix}\begin{pmatrix}c_{j\beta\uparrow}\\ c^{\dagger}_{j\beta\downarrow}\end{pmatrix}. (25)

Here, TijσαβT^{\alpha\beta}_{ij\sigma} is obtained from the Fourier transform of the matrix in Eq. (13) with renormalized hopping integrals t~i\tilde{t}_{i} and also includes the chemical potential term. The chemical potential μ\mu is set to the Fermi energy in the noninteracting limit. Δijαβ\Delta^{\alpha\beta}_{ij} corresponds to an anomalous part that describes the superconducting pairing in real space. Therefore, the variational parameters to be optimized in |Φ\left|\Phi\right> are t~i\tilde{t}_{i} (i=26i=2-6) and {Δijαβ}\{\Delta^{\alpha\beta}_{ij}\} with t~1=t1\tilde{t}_{1}=t_{1} being fixed as a unit of energy. In this study, we consider the pairing between nearest-neighbor orbitals, dd-dd, dd-pxp_{x}, dd-pyp_{y}, pxp_{x}-pxp_{x}, and pyp_{y}-pyp_{y}, where dd denotes the dx2y2d_{x^{2}-y^{2}} orbital. In the paramagnetic phase, we simply set Δijαβ=0\Delta^{\alpha\beta}_{ij}=0.

We can also construct the trial wave function with the band (k space) representation, where Δmn(k)<akmakn>\Delta^{mn}(\textbf{k})\propto\bigl{<}a_{\textbf{k}m\uparrow}a_{-\textbf{k}n\downarrow}\bigr{>} is the variational parameter. However, we find that the trial wave function with the real space representation always gives lower (i.e., better) energy than that with the band representation, especially, for large Coulomb interaction parameters. This is because the Coulomb interaction depends on the orbital, not on the band, and thus the trial wave function with the real space (orbital) representation gives the better result.

A.2.2 Uniform spin AF and stripe phases

As mentioned in Sec. II.2, various long-range orderings of charge and spin can be described by introducing {ρiα}\{\rho^{\alpha}_{i}\} and {miα}\{m^{\alpha}_{i}\}. A uniform spin AF phase with A and B sublattices for the orbital α\alpha is expressed with the staggered potential

miα={sσmαfor A sublattice+sσmαfor B sublatticem^{\alpha}_{i}=\begin{cases}-s_{\sigma}m^{\alpha}&\text{for A sublattice}\\ +s_{\sigma}m^{\alpha}&\text{for B sublattice}\end{cases} (26)

where sσ=1(1)s_{\sigma}=1(-1) for σ=()\sigma=\uparrow(\downarrow). For a stripe phase with charge and spin periodicities λcα=2π/qcα\lambda^{\alpha}_{\text{c}}=2\pi/q^{\alpha}_{\text{c}} and λsα=2π/qsα\lambda^{\alpha}_{\text{s}}=2\pi/q^{\alpha}_{\text{s}}, respectively, the following potentials with spatial modulation in the xx direction should be introduced:

ρiα=ραcos[qcα(xixcα)]\rho^{\alpha}_{i}=\rho^{\alpha}\cos[q^{\alpha}_{\text{c}}(x_{i}-x^{\alpha}_{\text{c}})] (27)

and

miα=(1)xi+yimαsin[qsα(xixsα)],m^{\alpha}_{i}=(-1)^{x_{i}+y_{i}}m^{\alpha}\sin[q^{\alpha}_{\text{s}}(x_{i}-x^{\alpha}_{\text{s}})], (28)

where xcαx^{\alpha}_{\text{c}} and xsαx^{\alpha}_{\text{s}} control the relative phases of charge and spin orderings, respectively. For example, the stripe phase observed around δ=1/8\delta=1/8 in several cuprate superconductors corresponds to λc=4\lambda_{\text{c}}=4 and λs=8\lambda_{\text{s}}=8, although the orbital dependence and relative phase are still under debate.

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