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Topologically protected two-fluid edge states

K. L. Zhang    Z. Song [email protected] School of Physics, Nankai University, Tianjin 300071, China
Abstract

Edge states reveal the nontrivial topology of energy band in the bulk. As localized states at boundaries, many-body edge states may obey a special symmetry that is broken in the bulk. When local particle-particle interaction is induced, they may support a particular property. We consider an extended two-dimensional Su-Schrieffer-Heeger Hubbard model and examine the appearance of η\eta-pairing states, which are excited eigenstates related to superconductivity. In the absence of Hubbard interaction, the energy band is characterized by topologically invariant polarization in association with edge states. In the presence of on-site Hubbard interaction, η\eta-pairing edge states appear in the topologically nontrivial phase, resulting in the condensation of pairs at the boundary. In addition, as Hamiltonian eigenstates, the edge states contain paired fermions and unpaired fermions. Neither affects the other; they act as two-fluid states. From numerical simulations of many-body scattering processes, a clear manifestation and experimental detection scheme of topologically protected two-fluid edge states are provided.

I Introduction

Topology in matter permits the existence of edge states, which have a strong immunity to distortions of the underlying architecture. Although they are believed to be inherited from the topology of the bulk, these edge states present some properties only around the boundary and are forbidden in the bulk. Topological insulator in condensed matter physics is a well-known example of this phenomenon. Although such a system is an insulator in the bulk, it permits electron conductance along the edges, resulting in quantized Hall conductance [1, 2, 3, 4]. In general, the strong interaction between fermions can affect the topology of a fermion system and break the bulk-boundary correspondence (BBC) [5]. Nevertheless, recent work [6] shows that quantum spin system also exhibits BBC even in a thermal state. This indicates that although the BBC reveals a nontrivial topology of the energy band, it has a particular feature in the presence of interaction.

Beyond the realm of the well-known topological insulator, recent studies on the twisted bilayer graphene (TBG) show that at a series of magic twist angles, the moiré pattern yields the flat low-energy bands that promise strong electronic correlations [7, 8, 9]. The interplay of lattice geometry and many-body interactions induces exotic quantum states including superconducting [10, 11] and correlated insulating [12] behaviors, which have been achieved in experiments [13, 14]. An interesting question is whether such exotic quantum states exist in a topological system, where the energy band of edge states plays the same role as the moiré flat band, in the presence of strong electronic correlations. The η\eta pairing proposed by Yang [15] is a promising mechanism to address this problem. In the absence of Hubbard interaction UU, an η\eta pair has zero energy in a bipartite lattice, thus the flat band appears when considering multiple η\eta pairs formed by electrons with momentums 𝐤\mathbf{k} and 𝝅𝐤\boldsymbol{\pi}-\mathbf{k} [15]. There are two common grounds between the flat bands of TBG and that of many-body edge states: They are formed by breaking the translational symmetry and have the potential to enhance electronic correlations. Importantly, such paired states become long lived in the presence of strong Hubbard repulsion [16, 17, 18, 19]. In addition, recent theoretical works [20, 21] suggest that the η\eta-pairing states can be induced by pulse irradiation or heating. On the other hand, as a phenomenological theory, the two-fluid model was proposed several decades ago to explain the behavior of superfluid helium [22, 23] and a conventional superconductor [24]. It postulates that a superconductor possesses two parallel channels, one superconducting and one normal. Although it is a useful tool, so far two-fluid states have yet to be investigated in the framework of quantum mechanics, appearing as a many-body Hamiltonian eigenstate. For instance, even the usual BCS wave function [25] is not an eigenstate of a Hamiltonian system with a local potential energy.

In this paper, we consider an extended two-dimensional (2D) Su-Schrieffer-Heeger (SSH) [26] model with on-site Hubbard interaction UU. Specifically, we examine the appearance of η\eta-pairing edge states [see Fig. 1(a)]. In the absence of Hubbard interaction, the energy band is characterized by topologically invariant polarization in association with edge states. When UU switches on, the bulk states do not support the formation of η\eta pairs, which appear only at the edge and possess an off-diagonal long-range order (ODLRO) [27] in the topologically nontrivial phase. We further propose a concept of topologically protected two-fluid edge states. As many-body eigenstates of a 2D SSH Hubbard model, the two-fluid edge states contain two components: η\eta-pairing fermions and unpaired fermions, which do not affect each other. The signature of the two-fluid edge states is observable in the dynamic behavior of resonant transmission. Based on the non-Hermitian quantum mechanics [28, 29, 30, 31, 32], we also develop a method to resolve the scattering problem involving multiple interacting fermions.

The remainder of this paper is organized as follows. In Sec. II, we introduce the concept of two-fluid states by a Hubbard model. In Sec. III, we demonstrate the existence of topological η\eta-paring edge states in an extended 2D SSH Hubbard model, which also supports two-fluid edge states and the properties are studied in Sec. IV through dynamics of resonant transmission. In Sec. V, we summarize our results.

Refer to caption
Figure 1: (a) Schematic of the lattice with cylindrical boundary condition. The lattice supports η\eta-pairing edge states, whereas the bulk states are unpaired fermions. (b) Details of the lattice, which is an extended 2D SSH Hubbard model depicted by the Hamiltonian in Eq. (9). The black and red dots represent sublattices A and B, respectively. The solid and dashed lines represent the nearest-neighbor and next-nearest-neighbor hopping, respectively.

II Model and two-fluid states

We begin with the Hamiltonian model of a general form and a brief summary of related results. The Hamiltonian is in the following form

H=H0+Hintra,H=H_{0}+H_{\mathrm{intra}}, (1)

on two sublattices A\mathrm{A} and B\mathrm{B}. Here H0H_{0} is the Hamiltonian of a simple Hubbard model with bipartite lattice symmetry

H0=𝐫A,𝐫Bσ=,t𝐫𝐫c𝐫,σc𝐫,σ+H.c.+U𝐫ABn𝐫,n𝐫,,H_{0}=\sum_{\mathbf{r}\in\mathrm{A},\mathbf{r}^{\prime}\in\mathrm{B}}\sum_{\sigma=\uparrow,\downarrow}t_{\mathbf{rr}^{\prime}}c_{\mathbf{r},\sigma}^{\dagger}c_{\mathbf{r}^{\prime},\sigma}+\text{{H.c.}}+U\sum_{\mathbf{r}\in\mathrm{A}\cup\mathrm{B}}n_{\mathbf{r},\uparrow}n_{\mathbf{r},\downarrow}, (2)

where the operator c𝐫,σc_{\mathbf{r},\sigma} (c𝐫,σc_{\mathbf{r},\sigma}^{\dagger}) is the usual annihilation (creation) operator of a fermion with spin σ{,}\sigma\in\left\{\uparrow,\downarrow\right\} at site 𝐫\mathbf{r}, and n𝐫,σ=c𝐫,σc𝐫,σn_{\mathbf{r},\sigma}=c_{\mathbf{r},\sigma}^{\dagger}c_{\mathbf{r},\sigma} is the number operator for a particle of spin σ\sigma on site 𝐫\mathbf{r}. As many previous studies [16, 17, 18, 19, 20, 21], here the interaction is purely on-site. Nevertheless, the weak nearest-neighbor interaction does not break the paired states [33] considered below. Unlike almost all studies on the η\eta-pairing states, we consider an extra term HintraH_{\mathrm{intra}}, representing the intrasublattice hopping. This term breaks the bipartite symmetry of H0H_{0}.

We first review well-established model properties of H0H_{0} that are crucial to our conclusion (see Appendix A for more details). First, H0H_{0} possesses SU(2) symmetry characterized by the generators s+=(s)=𝐫s𝐫+s^{+}=\left(s^{-}\right)^{\dagger}=\sum_{\mathbf{r}}s_{\mathbf{r}}^{+} and sz=𝐫s𝐫zs^{z}=\sum_{\mathbf{r}}s_{\mathbf{r}}^{z}, where s𝐫+=c𝐫,c𝐫,s_{\mathbf{r}}^{+}=c_{\mathbf{r},\uparrow}^{\dagger}c_{\mathbf{r},\downarrow} and s𝐫z=(n𝐫,n𝐫,)/2s_{\mathbf{r}}^{z}=\left(n_{\mathbf{r},\uparrow}-n_{\mathbf{r},\downarrow}\right)/2. Second, one can define the following operators

η+=(η)=𝐫η𝐫+,ηz=𝐫η𝐫z,\eta^{+}=\left(\eta^{-}\right)^{\dagger}=\sum_{\mathbf{r}}\eta_{\mathbf{r}}^{+},\quad\eta^{z}=\sum_{\mathbf{r}}\eta_{\mathbf{r}}^{z}, (3)

with η𝐫+=c𝐫,c𝐫,\eta_{\mathbf{r}}^{+}=c_{\mathbf{r},\uparrow}^{\dagger}c_{\mathbf{r},\downarrow}^{{\dagger}} (c𝐫,c𝐫,-c_{\mathbf{r},\uparrow}^{\dagger}c_{\mathbf{r},\downarrow}^{{\dagger}}) for 𝐫A\mathbf{r}\in A (𝐫B\mathbf{r}\in B), and η𝐫z=(n𝐫,+n𝐫,1)/2\eta_{\mathbf{r}}^{z}=\left(n_{\mathbf{r},\uparrow}+n_{\mathbf{r},\downarrow}-1\right)/2, satisfying commutation relation [η𝐫+,[\eta_{\mathbf{r}}^{+}, η𝐫]=2η𝐫z\eta_{\mathbf{r}}^{-}]=2\eta_{\mathbf{r}}^{z} and [η𝐫z,[\eta_{\mathbf{r}}^{z}, η𝐫±]=±η𝐫±\eta_{\mathbf{r}}^{\pm}]=\pm\eta_{\mathbf{r}}^{\pm}. Straightforward algebra shows that

[H0Uηz,η±]=[H0,ηz]=0,\left[H_{0}-U\eta^{z},\eta^{\pm}\right]=\left[H_{0},\eta^{z}\right]=0, (4)

which is guaranteed by the bipartite lattice symmetry. These two properties allow the construction of two types of eigenstates of H0H_{0}: ferromagnetic (FM) and antiferromagnetic (AFM).

An mm-fermion FM eigenstate with energy {𝐤}mε𝐤\sum_{\left\{\mathbf{k}\right\}}^{m}\varepsilon_{\mathbf{k}} can be expressed as follows:

|ψFM(m,l)=(s)(ml)/2{𝐤}mc𝐤,|Vac,\left|\psi_{\mathrm{FM}}(m,l)\right\rangle=\left(s^{-}\right)^{\left(m-l\right)/2}\prod_{\left\{\mathbf{k}\right\}}^{m}c_{\mathbf{k},\uparrow}^{\dagger}\left|\mathrm{Vac}\right\rangle, (5)

where |Vac\left|\mathrm{Vac}\right\rangle is the vacuum state of the fermion c𝐫,σc_{\mathbf{r},\sigma}, and c𝐤,c_{\mathbf{k},\uparrow}^{\dagger} is the eigenmode of H0H_{0} with U=0U=0 —that is, [c𝐤,σ,H0(U=0)]=ε𝐤c𝐤,σ[c_{\mathbf{k},\sigma}^{\dagger},H_{0}(U=0)]=-\varepsilon_{\mathbf{k}}c_{\mathbf{k},\sigma}^{\dagger}. Eigenstate |ψFM(m,l)\left|\psi_{\mathrm{FM}}(m,l)\right\rangle is a saturated FM state, given that it is also an eigenstate of s2s^{2} and szs^{z}, with eigenvalues m(m/2+1)/2m\left(m/2+1\right)/2 and l/2,l/2, respectively.

An nn-pair AFM eigenstate can be expressed as

|ψAFM(n)=(η+)n|Vac,\left|\psi_{\mathrm{AFM}}(n)\right\rangle=\left(\eta^{+}\right)^{n}\left|\mathrm{Vac}\right\rangle, (6)

which obeys H0|ψAFM(n)=nU|ψAFM(n)H_{0}\left|\psi_{\mathrm{AFM}}(n)\right\rangle=nU\left|\psi_{\mathrm{AFM}}(n)\right\rangle and s2|ψAFM(n)=0s^{2}\left|\psi_{\mathrm{AFM}}(n)\right\rangle=0. Obviously, an η\eta-pairing state is spin singlet. Unlike all other spin singlet states, an AFM η\eta-pairing eigenstate is independent of the detailed structure of the bipartite lattice, regardless of whether it contains short-, long-, or even infinite-range hopping terms. This feature is characterized by a correlator related to the off-diagonal element of the reduced density matrix of the system [27, 15].

Importantly, there is a mixture of two types of states, referred to as two-fluid state

|ψ2F(n,m,l)=(η+)n(s)(ml)/2{𝐤}mc𝐤,|Vac,\left|\psi_{\mathrm{2F}}(n,m,l)\right\rangle=\left(\eta^{+}\right)^{n}\left(s^{-}\right)^{\left(m-l\right)/2}\prod_{\left\{\mathbf{k}\right\}}^{m}c_{\mathbf{k},\uparrow}^{\dagger}\left|\mathrm{Vac}\right\rangle, (7)

which is a common eigenstate of H0H_{0}, s2s^{2} and szs^{z} with eigenvalues {𝐤}mε𝐤+nU\sum_{\left\{\mathbf{k}\right\}}^{m}\varepsilon_{\mathbf{k}}+nU, m(m/2+1)/2m\left(m/2+1\right)/2 and l/2,l/2, respectively. States |ψ2F(n,m,l)\left|\psi_{\mathrm{2F}}(n,m,l)\right\rangle are demonstrated to be related to ODLRO and superconductivity for finite n/Nn/N in a large-NN limit [27, 34, 35], where NN is the total number of lattice sites. In a comparison of states |ψAFM(n)\left|\psi_{\mathrm{AFM}}(n)\right\rangle and |ψFM(m,l)\left|\psi_{\mathrm{FM}}(m,l)\right\rangle, the first is a condensation of pairs, acting as a Bose-Einstein condensate, whereas the second is a free electron gas, acting as a normal conductor. Notably, eigenstate |ψ2F(n,m,l)\left|\psi_{\mathrm{2F}}(n,m,l)\right\rangle contains two components, paired and single electrons, and no scattering occurs between single electrons and η\eta pairs. This mechanism suggests the presence of resonant transmission channels for a Hubbard cluster in the state |ψAFM(n)\left|\psi_{\mathrm{AFM}}(n)\right\rangle as a scattering center. This can be verified by examining the scattering dynamics of an input Gaussian wave packet with resonant energy. Here we emphasize that the bipartite symmetry plays an important role in the formation of the AFM η\eta-pairing states and the two-fluid states.

We wish to determine what happens in the presence of HintraH_{\mathrm{intra}}. Obviously, the paired states are suppressed in general. However, the foregoing analysis remains true if there exists an invariant subspace spanned by a set of many-body states {|ψp}\left\{\left|\psi_{\mathrm{p}}\right\rangle\right\}, satisfying

Hintra|ψp=0.H_{\mathrm{intra}}\left|\psi_{\mathrm{p}}\right\rangle=0. (8)

We refer to these types of states as conditional η\eta-pairing states. Furthermore, it would be interesting when states {|ψp}\left\{\left|\psi_{\mathrm{p}}\right\rangle\right\} have special physical significant because an η\eta-pairing state has ODLRO or superconductivity. We will consider a concrete example in which states {|ψp}\left\{\left|\psi_{\mathrm{p}}\right\rangle\right\} are topologically protected edge states. These conditional η\eta-pairing states permit the existence of two-fluid edge states, which support not only the superconductivity but also a single-fermion transmission channel at the system boundary.

III Topological η\eta-pairing edge states

We consider an extended 2D SSH Hubbard model on an Nx×NyN_{x}\times N_{y} square lattice, as presented in the schematic in Fig. 1(b). The Hamiltonian consists of two parts

H2D=H0+HintraH_{2\text{{D}}}=H_{\text{{0}}}+H_{\mathrm{intra}} (9)

with H0=3𝐫,σ(txcx,y,σcx+1,y,σH_{\text{{0}}}=3\sum_{\mathbf{r},\sigma}(t_{x}c_{x,y,\sigma}^{{\dagger}}c_{x+1,y,\sigma} +cx,y,σcx,y+1,σ+H.c.)+U𝐫n𝐫,n𝐫,+c_{x,y,\sigma}^{{\dagger}}c_{x,y+1,\sigma}+\mathrm{H.c.})+U\sum_{\mathbf{r}}n_{\mathbf{r},\uparrow}n_{\mathbf{r},\downarrow} and Hintra=𝐫,σtx(cx,y,σcx+1,y+1,σH_{\mathrm{intra}}=\sum_{\mathbf{r},\sigma}t_{x}(c_{x,y,\sigma}^{{\dagger}}c_{x+1,y+1,\sigma} +cx,y,σcx+1,y1,σ)+H.c.+c_{x,y,\sigma}^{{\dagger}}c_{x+1,y-1,\sigma})+\mathrm{H.c.}. Here, xx and yy [𝐫=(x,y)\mathbf{r}=\left(x,y\right)] are the lattice indexes in the x^\hat{x} and y^\hat{y} directions, respectively, and the parameter tx=λ(x mod 2)t_{x}=\lambda^{\left(x\text{ }\mathrm{mod}\text{ }2\right)}. The hopping term HintraH_{\mathrm{intra}} breaks the bipartite lattice symmetry, as indicated by the dashed lines in Fig. 1(b).

We first focus on the interaction-free case with U=0U=0, where a single parameter λ\lambda controls the topological quantum phase. The system is in the topologically nontrivial phase within |λ|<1\left|\lambda\right|<1 (see Appendix B). With the open boundary condition in x^\hat{x} direction [see Fig. 1(a)] and in the large-NxN_{x} limit, the system supports two degenerate edge modes

|ψky,σL\displaystyle|\psi_{k_{y},\sigma}^{\mathrm{L}}\rangle =\displaystyle= Ωx(λ)x1ax,ky,σ|Vac,\displaystyle\Omega\sum_{x}\left(-\lambda\right)^{x-1}a_{x,k_{y},\sigma}^{{\dagger}}\left|\mathrm{Vac}\right\rangle,
|ψky,σR\displaystyle|\psi_{k_{y},\sigma}^{\mathrm{R}}\rangle =\displaystyle= Ωx(λ)Nxxbx,ky,σ|Vac,\displaystyle\Omega\sum_{x}\left(-\lambda\right)^{N_{x}-x}b_{x,k_{y},\sigma}^{{\dagger}}\left|\mathrm{Vac}\right\rangle, (10)

with the eigenenergy EL/R=6coskyE^{\mathrm{L}/\mathrm{R}}=6\cos k_{y} and the normalization constant Ω=1λ2\Omega=\sqrt{1-\lambda^{2}}. Here, (ax,ky,σ,bx,ky,σ)\left(a_{x,k_{y},\sigma},b_{x,k_{y},\sigma}\right) =Ny1/2y(c2x1,y,σ,c2x,y,σ)eikyy=N_{y}^{-1/2}\sum_{y}\left(c_{2x-1,y,\sigma},c_{2x,y,\sigma}\right)e^{-ik_{y}y}, and this transformation does not break the bipartite lattice symmetry. We note that

Hintra|ψky,σL/R=0,H_{\mathrm{intra}}|\psi_{k_{y},\sigma}^{\mathrm{L/R}}\rangle=0, (11)

which indicates that edge states {|ψky,σL/R}\{|\psi_{k_{y},\sigma}^{\mathrm{L/R}}\rangle\} span an invariant subspace with bipartite lattice symmetry and make possible the formation of η\eta-pairing eigenstates when UU is switched on. Notably, Eq. (11) still holds when disordered perturbation is introduced. This indicates that the η\eta-pairing edge states are topologically protected. In the trivial phase |λ|>1\left|\lambda\right|>1, or when periodic boundary condition in both directions are taken, these paired eigenstates are absent. This is another important characterization of topological system.

Refer to caption
Figure 2: Numerical results of the correlator C(1,y)C\left(1,y\right) defined in Eq. (12) for systems with different numbers of fermions and parameters λ\lambda. The lattice sizes and Hubbard interaction strengths are all (Nx,Ny)=(5,4)(N_{x},N_{y})=(5,4) and U=1.5U=1.5. The number of fermions in (a) and (b) is two (\uparrow\downarrow) and four (\uparrow\uparrow\downarrow\downarrow), respectively. For comparison, the correlators for a bipartite chain are also plotted (dashed lines). The corresponding energies are indicated to the right of each line.

To verify the existence of the η\eta-pairing edge states |ψedge|\psi_{\text{{edge}}}\rangle, we study the system H2DH_{2\text{{D}}} in two- and four-fermion subspaces with Hubbard interaction UU through exact diagonalization. To characterize the η\eta-pairing edge states, we introduce the following correlator [27, 15]

C(y,y)=ψedge|ηx=1,yηx=1,y|ψedge,C\left(y^{\prime},y\right)=\langle\psi_{\text{{edge}}}|\eta_{x=1,y^{\prime}}^{{\dagger}}\eta_{x=1,y}|\psi_{\text{{edge}}}\rangle, (12)

where ηx,y=(1)ycx,y,cx,y,\eta_{x,y}=\left(-1\right)^{y}c_{x,y,\downarrow}c_{x,y,\uparrow}. The lattice index xx is fixed at the left end in Eq. (12), because the lattice possesses inversion symmetry, and for an edge state, the correlator should vanish in the bulk. For the eigenstate |ψedge|\psi_{\text{{edge}}}\rangle possessing ODLRO, the correlator C(y,y)C\left(y^{\prime},y\right) is a constant when |yy|\left|y^{\prime}-y\right| increases. This is a characteristic of superconductivity. When λ0\lambda\approx 0, the presence of η\eta-pairing edge states is clear; the two chains at the boundaries, which support the edge states, are isolated from the bulk of the cylinder, and the boundary chains can be regarded as approximate bipartite lattices. For the η\eta-pairing state |ψ(n)=(η)n|vac\left|\psi(n)\right\rangle=(\eta^{{\dagger}})^{n}|\mathrm{vac}\rangle in a bipartite lattice, the correlator is [15]

C(y,y)=n(Nyn)Ny(Ny1),yy.C\left(y^{\prime},y\right)=\frac{n\left(N_{y}-n\right)}{N_{y}\left(N_{y}-1\right)},y^{\prime}\neq y. (13)

This bipartite lattice corresponds to the isolated chain with NyN_{y} sites at the boundary.

The η\eta-pairing edge states are bound pairs localized at the boundary, which have substantial pairing energy and near-zero kinetic energy; thus, the pair density at the boundary 𝒩edge=yψedge|n1,y,n1,y,|ψedge\mathcal{N}_{\text{{edge}}}=\sum_{y}\langle\psi_{\text{{edge}}}|n_{1,y,\uparrow}n_{1,y,\downarrow}|\psi_{\text{{edge}}}\rangle is useful in the search for the η\eta-pairing edge states. One can search for η\eta-pairing edge states in eigenstates with large 𝒩edge\mathcal{N}_{\text{{edge}}}. We perform the numerical calculation for systems with different numbers of particles and parameters λ\lambda.

The numerical results of the correlator C(y,y)C\left(y^{\prime},y\right) for the η\eta-pairing edge states are shown in Fig. 2. The corresponding local particle density is presented in Appendix C. The lattice size of the system is set as (Nx,Ny)=(5,4)(N_{x},N_{y})=(5,4), where NxN_{x} is truncated to an odd number such that the edge states appear in only one boundary. The interaction strength is U=1.5U=1.5, and the number of particles are two (one spin up and one spin down, marked as \uparrow\downarrow), and four (\uparrow\uparrow\downarrow\downarrow) for Figs. 2(a) and (b), respectively. In the invariant subspaces of two and four fermions, there exist only one η\eta-pairing state with one-pairing and two-pairing, respectively. A higher filling ratio will involve the bulk fermions, which have no contribution to the ODLRO. The correlators of a uniform chain in Eq. (13) are plotted as a comparison. One can see that until λ=0.4\lambda=0.4, these two states have the long-range correlation of C(1,y)C\left(1,y\right). The comparison between the energies of two and four fermions indicates that there is no interaction between the paired fermions in small λ\lambda limit, which is equivalent to finite |λ|<1\left|\lambda\right|<1 with large NxN_{x}. In Appendix C, we also give the numerical results of three fermions, and the approximate results of even- and odd-number fermions in a larger system. In these cases, the previous conclusions are still valid.

IV Resonant transmission

In the preceding section, we demonstrate the existence of the η\eta-pairing edge states from the correlator. A natural question is that whether system H2DH_{\mathrm{2D}} supports a two-fluid state containing single fermions and η\eta pairs localized at the boundary of the system. We attempt to answer this question and demonstrate the properties of the two-fluid edge states.

Particle beam scattering is a conventional technique for detecting the nature of matter [36]. Because no scattering occurs between the single fermions and η\eta pairs, resonant transmission provides a means to present the features of two-fluid edge states. The detection of resonant transmission for a many-body state is somewhat challenging, both theoretically and experimentally. Nevertheless, exceptional point (EP) [30, 31, 32] dynamics in non-Hermitian quantum mechanics can reduce the difficulty of the calculation. For a system with parameters at EP, two or more eigenvalues along with their associated eigenstates become identical, leading to unidirectional dynamics. This allows us to employ EP dynamics to simulate the perfect resonant transmission of particles. It can shorten the lengths of the input and output leads, and the scattering process in a Hermitian system can be effectively treated as the dynamics of a non-Hermitian system (see Appendix D). In the following, we present the resonant transmission dynamics of the two-fluid edge states. For comparison, the scattering dynamics between a single fermion and an FM edge state are also examined.

Refer to caption
Figure 3: (a) Resonant transmission process. (b) Ordinary scattering process. The top panel is a schematic of the two processes. The bottom panel presents the corresponding numerical results of fidelity defined in Eq. (15) at time t=1000t=1000 as a function of μ\mu for U=1.5U=1.5 and 33, as well as the particle density ρ𝐑(t)\rho_{\mathbf{R}}(t) and the pair density 𝒩𝐑(t)\mathcal{N}_{\mathbf{R}}(t) defined in Eqs. (16) and (17) for parameters μ=0\mu=0 and U=1.5U=1.5. The other parameters are (Nx,Ny)=(5,4)(N_{x},N_{y})=(5,4), λ=0.2\lambda=0.2 and J=0.1J=0.1. The scales of the Hamiltonian and time tt are taken as dimensionless.

We consider the dynamics in a non-Hermitian system, which consists of the 2D SSH Hubbard model H2DH_{2\text{{D}}} and two extra sites (with indexes j=1j=-1 and 11), connected by the unidirectional hopping

HNH\displaystyle H_{\text{{NH}}} =\displaystyle= H2D+Jσ=,(cα,σc1,σ+c1,σcβ,σ)\displaystyle H_{2\text{{D}}}+J\sum_{\sigma=\uparrow,\downarrow}\left(c_{\alpha,\sigma}^{\dagger}c_{-1,\sigma}+c_{1,\sigma}^{\dagger}c_{\beta,\sigma}\right) (14)
+μσ=,j=±1cj,σcj,σ,\displaystyle+\mu\sum_{\sigma=\uparrow,\downarrow}\sum_{j=\pm 1}c_{j,\sigma}^{\dagger}c_{j,\sigma},

where cα,σc_{\alpha,\sigma}^{\dagger} and cβ,σc_{\beta,\sigma} are fermion operators at the edge of the cylinder H2DH_{2\text{{D}}}. A schematic of the system configuration is presented in Appendix D. When μ=EL/R=6cosky\mu=E^{\mathrm{L/R}}=6\cos k_{y} is considered, a Jordan block with order of three should appear in single-particle subspace (see Appendix D). For the many-body case, if the two-fluid states remain eigenstates of H2DH_{2\text{{D}}}, it still supports the Jordan block with order of three. This can be verified by examining the dynamic process. We take the initial state as |ψ(0)=c1,|ψedgea\left|\psi(0)\right\rangle=c_{-1,\uparrow}^{\dagger}|\psi_{\text{{edge}}}^{\mathrm{a}}\rangle, with the AFM η\eta-pairing edge state |ψedgea|\psi_{\text{{edge}}}^{\mathrm{a}}\rangle satisfying s2|ψedgea=0s^{2}|\psi_{\text{{edge}}}^{\mathrm{a}}\rangle=0, and calculate the time evolution |ψ(t)=eiHNHt|ψ(0)/|eiHNHt|ψ(0)|\left|\psi(t)\right\rangle=e^{-iH_{\text{{NH}}}t}\left|\psi(0)\right\rangle/|e^{-iH_{\text{{NH}}}t}\left|\psi(0)\right\rangle|. The expected final state is |ψfinal=c1,|ψedgea\left|\psi_{\mathrm{final}}\right\rangle=c_{1,\uparrow}^{\dagger}|\psi_{\text{{edge}}}^{\mathrm{a}}\rangle when resonant transmission occurs. Here, the numerical computations are performed by using a uniform mesh in conducting time discretization.

To characterize the procedure, we introduce three quantities: the fidelity between the expected state and the evolved state

F(t)=|ψfinal|ψ(t)|;F(t)=\left|\left\langle\psi_{\mathrm{final}}\right.\left|\psi(t)\right\rangle\right|; (15)

the particle density of the evolved state at different spatial regions

ρ𝐑(t)=𝐫=𝐑σ=,ψ(t)|n𝐫,σ|ψ(t),\rho_{\mathbf{R}}(t)=\sum_{\mathbf{r=R}}\sum_{\sigma=\uparrow,\downarrow}\left\langle\psi(t)\right|n_{\mathbf{r},\sigma}\left|\psi(t)\right\rangle, (16)

where 𝐑=𝐑1\mathbf{R}=\mathbf{R}_{-1} and 𝐑1\mathbf{R}_{1} respectively represent the extra sites with indexes j=1j=-1 and 11, and 𝐑=𝐑C\mathbf{R}=\mathbf{R}_{\mathrm{C}} represents the sites of the scattering center H2DH_{2\text{{D}}}; and the pair density

𝒩𝐑(t)=𝐫=𝐑ψ(t)|n𝐫,n𝐫,|ψ(t).\mathcal{N}_{\mathbf{R}}(t)=\sum_{\mathbf{r=R}}\left\langle\psi(t)\right|n_{\mathbf{r},\uparrow}n_{\mathbf{r},\downarrow}\left|\psi(t)\right\rangle. (17)

Figure. 3(a) presents the numerical results of the fidelity after a sufficiently long time as a function of μ\mu, and the two other quantities as functions of time tt. As expected, the peaks appear at μ=6\mu=-6, 0 and 66, where the single fermion is resonantly transmitted from site 𝐑1\mathbf{R}_{-1} to site 𝐑1\mathbf{R}_{1}. This can also be seen in the particle density ρ𝐑(t)\rho_{\mathbf{R}}(t) and the pair density 𝒩𝐑(t)\mathcal{N}_{\mathbf{R}}(t) for μ=0\mu=0 and U=1.5U=1.5.

For comparison, in Fig. 3(b), we consider the time evolution of another initial state |ψ(0)=c1,|ψedgeb\left|\psi(0)\right\rangle=c_{-1,\uparrow}^{\dagger}|\psi_{\text{{edge}}}^{\mathrm{b}}\rangle, with the FM edge state |ψedgeb|\psi_{\text{{edge}}}^{\mathrm{b}}\rangle satisfyings2|ψedgeb=2\ s^{2}|\psi_{\text{{edge}}}^{\mathrm{b}}\rangle=2, sz|ψedgeb=0s_{z}|\psi_{\text{{edge}}}^{\mathrm{b}}\rangle=0, and the state |ψfinal=c1,|ψedgeb\left|\psi_{\mathrm{final}}\right\rangle=c_{1,\uparrow}^{\dagger}|\psi_{\text{{edge}}}^{\mathrm{b}}\rangle. The numerical results indicate that the single fermion is scattered by the FM\mathrm{FM} state |ψedgeb|\psi_{\text{{edge}}}^{\mathrm{b}}\rangle at any μ\mu value due to the Hubbard interaction. When μ=0\mu=0 and U=1.5U=1.5, two fermions are transmitted to site 𝐑1\mathbf{R}_{1} after a sufficiently long time.

V Summary

We present a concept of topologically protected two-fluid edge states and a means for their detection. We demonstrate the existence of such states in the 2D SSH Hubbard model, which provides an analog to the topological insulator. Such a material behaves as a conductor in its interior but possesses a surface containing superconducting states. In other words, the condensation of η\eta pairs can exist only on the surface of the material. We also determine that a two-fluid state can be formed as a many-body eigenstate of a realistic Hubbard model. By employing EP dynamics, a technique of the numerical simulation is developed to overcome the computational difficulty in the scattering problem of many-body system, which involve numerous basis vectors. It is expected to measure the resonant transmission in experiment via peaks in transmission coefficient [37, 38]. At present, the possible experimental implementation to explore the two-fluid edge states is ultracold fermions in an optical lattice [39].

Acknowledgements.
This work was supported by National Natural Science Foundation of China (under Grant No. 11874225).

Appendix

In this Appendix, we present A. Symmetries, FM and AFM eigenstates for H0H_{0}; B. Solution of the extended 2D SSH model; C. More exact numerical results and approximate numerical results; and D. Non-Hermitian description of resonant transmission.

A Symmetries, FM and AFM eigenstates for H0H_{0}

Considering the Hubbard Hamiltonian H0H_{0} in the main text, one can defined two sets of pseudo-spin operators (s±,szs^{\pm},s^{z}) and (η±,ηz\eta^{\pm},\eta^{z}). The first set is

s+\displaystyle s^{+} =\displaystyle= (s)=𝐫s𝐫+,\displaystyle\left(s^{-}\right)^{\dagger}=\sum_{\mathbf{r}}s_{\mathbf{r}}^{+},
sz\displaystyle s^{z} =\displaystyle= 𝐫s𝐫z,\displaystyle\sum_{\mathbf{r}}s_{\mathbf{r}}^{z}, (A1)

where the local operators s𝐫+=c𝐫,c𝐫,s_{\mathbf{r}}^{+}=c_{\mathbf{r},\uparrow}^{\dagger}c_{\mathbf{r},\downarrow} and s𝐫z=(n𝐫,n𝐫,)/2s_{\mathbf{r}}^{z}=\left(n_{\mathbf{r},\uparrow}-n_{\mathbf{r},\downarrow}\right)/2 obey the Lie algebra, i.e., [s𝐫+,[s_{\mathbf{r}}^{+}, s𝐫]=2s𝐫zs_{\mathbf{r}}^{-}]=2s_{\mathbf{r}}^{z}, and [s𝐫z,[s_{\mathbf{r}}^{z}, s𝐫±]=±s𝐫±s_{\mathbf{r}}^{\pm}]=\pm s_{\mathbf{r}}^{\pm}. The second set is

η+\displaystyle\eta^{+} =\displaystyle= (η)=𝐫η𝐫+,\displaystyle\left(\eta^{-}\right)^{\dagger}=\sum_{\mathbf{r}}\eta_{\mathbf{r}}^{+},
ηz\displaystyle\eta^{z} =\displaystyle= 𝐫η𝐫z,\displaystyle\sum_{\mathbf{r}}\eta_{\mathbf{r}}^{z}, (A2)

with η𝐫+=c𝐫,c𝐫,\eta_{\mathbf{r}}^{+}=c_{\mathbf{r},\uparrow}^{\dagger}c_{\mathbf{r},\downarrow}^{{\dagger}} (c𝐫,c𝐫,-c_{\mathbf{r},\uparrow}^{\dagger}c_{\mathbf{r},\downarrow}^{{\dagger}}) for 𝐫A\mathbf{r}\in A (𝐫B\mathbf{r}\in B), and η𝐫z=(n𝐫,+n𝐫,1)/2\eta_{\mathbf{r}}^{z}=\left(n_{\mathbf{r},\uparrow}+n_{\mathbf{r},\downarrow}-1\right)/2 satisfying commutation relation [η𝐫+,[\eta_{\mathbf{r}}^{+}, η𝐫]=2η𝐫z\eta_{\mathbf{r}}^{-}]=2\eta_{\mathbf{r}}^{z}, and [η𝐫z,[\eta_{\mathbf{r}}^{z}, η𝐫±]=±η𝐫±\eta_{\mathbf{r}}^{\pm}]=\pm\eta_{\mathbf{r}}^{\pm}. Straightforward algebra shows the symmetries of H0H_{0}:

[H0,s±]=[H0,sz]=0,\left[H_{0},s^{\pm}\right]=\left[H_{0},s^{z}\right]=0, (A3)

and

[H0Uηz,η±]=[H0,ηz]=0,\left[H_{0}-U\eta^{z},\eta^{\pm}\right]=\left[H_{0},\eta^{z}\right]=0, (A4)

which will be employed to construct eigenstates of the Hamiltonian.

Starting from the diagonalization form of H0H_{0} with zero UU,

H0(U=0)=𝐤,σ=,ε𝐤c𝐤,σc𝐤,σ,H_{0}(U=0)=\sum_{\mathbf{k},\sigma=\uparrow,\downarrow}\varepsilon_{\mathbf{k}}c_{\mathbf{k},\sigma}^{\dagger}c_{\mathbf{k},\sigma}, (A5)

one can construct an mm-fermion FM eigenstate of H0(U0)H_{0}(U\neq 0)

|ψFM(m,m)={𝐤}mc𝐤,|Vac,\left|\psi_{\mathrm{FM}}(m,m)\right\rangle=\prod_{\left\{\mathbf{k}\right\}}^{m}c_{\mathbf{k},\uparrow}^{\dagger}\left|\mathrm{Vac}\right\rangle, (A6)

with |Vac\left|\mathrm{Vac}\right\rangle being the vacuum state of fermion c𝐫,σc_{\mathbf{r},\sigma}, since the UU term has no effect on the fermions with aligned spin polarization. The symmetry in Eq. (A3) permits the existence of eigenstates

|ψFM(m,l)=(s)(ml)/2{𝐤}mc𝐤,|Vac,\left|\psi_{\mathrm{FM}}(m,l)\right\rangle=\left(s^{-}\right)^{\left(m-l\right)/2}\prod_{\left\{\mathbf{k}\right\}}^{m}c_{\mathbf{k},\uparrow}^{\dagger}\left|\mathrm{Vac}\right\rangle, (A7)

with l=m,m+2,,m4,m2,ml=-m,-m+2,...,m-4,m-2,m, which obeys

H0|ψFM(m,l)={𝐤}mε𝐤|ψFM(m,l).H_{0}\left|\psi_{\mathrm{FM}}(m,l)\right\rangle=\sum_{\left\{\mathbf{\ k}\right\}}^{m}\varepsilon_{\mathbf{k}}\left|\psi_{\mathrm{FM}}(m,l)\right\rangle. (A8)

These states are referred to as FM states since they obey

s2|ψFM(m,l)=m2(m2+1)|ψFM(m,l),s^{2}\left|\psi_{\mathrm{FM}}(m,l)\right\rangle=\frac{m}{2}(\frac{m}{2}+1)\left|\psi_{\mathrm{FM}}(m,l)\right\rangle, (A9)

and

sz|ψFM(m,l)=l2|ψFM(m,l).s^{z}\left|\psi_{\mathrm{FM}}(m,l)\right\rangle=\frac{l}{2}\left|\psi_{\mathrm{FM}}(m,l)\right\rangle. (A10)

Similarly, one can construct a set of AFM eigenstates based on the symmetry in Eq. (A4). An nn-pair has the form

|ψAFM(n)=(η+)n|Vac,\left|\psi_{\mathrm{AFM}}(n)\right\rangle=\left(\eta^{+}\right)^{n}\left|\mathrm{Vac}\right\rangle, (A11)

which obeys

H0|ψAFM(n)=nU|ψAFM(n),H_{0}\left|\psi_{\mathrm{AFM}}(n)\right\rangle=nU\left|\psi_{\mathrm{AFM}}(n)\right\rangle, (A12)

and

s2|ψAFM(n)=0.s^{2}\left|\psi_{\mathrm{AFM}}(n)\right\rangle=0. (A13)

Obviously, an η\eta-pairing state is spin singlet. In the main text, a two-fluid eigenstates is constructed based on the above two types of states.

B Solution of the extended 2D SSH model

Taking the periodic boundary condition in both directions, the interaction-free 2D SSH Hamiltonian in 𝐤\mathbf{k} space can be written as

H2D(U=0)=𝐤σ=,(a𝐤,σb𝐤,σ)h𝐤(a𝐤,σb𝐤,σ),H_{2\text{{D}}}(U=0)=\sum_{\mathbf{k}}\sum_{\sigma=\uparrow,\downarrow}\left(\begin{array}[]{cc}a_{\mathbf{k,}\sigma}^{{\dagger}}&b_{\mathbf{k,}\sigma}^{{\dagger}}\end{array}\right)h_{\mathbf{k}}\left(\begin{array}[]{c}a_{\mathbf{k,}\sigma}\\ b_{\mathbf{k,}\sigma}\end{array}\right), (B1)

where the core matrix is

h𝐤=(6coskyϑ𝐤ϑ𝐤6cosky),h_{\mathbf{k}}=\left(\begin{array}[]{cc}6\cos k_{y}&\vartheta_{\mathbf{k}}\\ \vartheta_{\mathbf{k}}^{\ast}&6\cos k_{y}\end{array}\right), (B2)

with ϑ𝐤=(λ+eikx)(3+2cosky)\vartheta_{\mathbf{k}}=\left(\lambda+e^{-ik_{x}}\right)\left(3+2\cos k_{y}\right), based on the Fourier transformation

(a𝐤,σ,b𝐤,σ)=(NxNy)1/2𝐫(c2x1,y,σ,c2x,y,σ)ei𝐤𝐫.\left(a_{\mathbf{k,}\sigma},b_{\mathbf{k,}\sigma}\right)=\left(N_{x}N_{y}\right)^{-1/2}\sum_{\mathbf{r}}\left(c_{2x-1,y,\sigma},c_{2x,y,\sigma}\right)e^{-i\mathbf{k\cdot r}}. (B3)

We note that the system satisfies time reversal symmetry and is invariant under the inversion symmetry

𝒯h𝐤𝒯1=h𝐤,Rh𝐤R1=h𝐤,\mathcal{T}h_{\mathbf{k}}\mathcal{T}^{-1}\mathcal{=}h_{-\mathbf{k}},Rh_{\mathbf{k}}R^{-1}=h_{-\mathbf{k}}, (B4)

where 𝒯=K\mathcal{T}=K is conjugation operator and R=(0110)R=\left(\begin{array}[]{cc}0&1\\ 1&0\end{array}\right). The eigenvectors of h𝐤h_{\mathbf{k}} are

|ψ𝐤±=12(±eiθ𝐤1),\left|\psi_{\mathbf{k}}^{\pm}\right\rangle=\frac{1}{\sqrt{2}}\left(\begin{array}[]{c}\pm e^{i\theta_{\mathbf{k}}}\\ 1\end{array}\right), (B5)

with θ𝐤=arg(ϑ𝐤)\theta_{\mathbf{k}}=\arg\left(\vartheta_{\mathbf{k}}\right) and the corresponding eigenvalues

E𝐤±=6cosky±|3+2cosky|Λ𝐤.E_{\mathbf{k}}^{\pm}=6\cos k_{y}\pm\left|3+2\cos k_{y}\right|\Lambda_{\mathbf{k}}. (B6)

Here factor Λ𝐤=λ2+1+2λcoskx\Lambda_{\mathbf{k}}=\sqrt{\lambda^{2}+1+2\lambda\cos k_{x}} determines the pseudo band gap, which vanishes at kx=0,πk_{x}=0,\pi when taking λ=±1\lambda=\pm 1.

Refer to caption
Figure 4: Numerical results for local particle density ρ(𝐫)\rho\left(\mathbf{r}\right) defined in Eq. (C1) for the systems with different numbers of fermions and parameters λ\lambda . The lattices size and Hubbard interaction strength are all (Nx,Ny)=(5,4)(N_{x},N_{y})=(5,4) and U=1.5U=1.5. The numbers of fermions are two (\uparrow\downarrow) and four (\uparrow\uparrow\downarrow\downarrow) for (a) and (b), respectively.

Under cylindrical boundary condition (taking open boundary condition in xx direction), this model supports topological edge states protected by time reversal symmetry and inversion symmetry. We introduce the wave polarization to characterize the topological phase transition [40, 41]

𝐏±=1(2π)2BZ𝐀𝐤±𝑑kx𝑑ky,\mathbf{P}^{\pm}=\frac{1}{\left(2\pi\right)^{2}}\iint_{\mathrm{BZ}}\mathbf{A}_{\mathbf{k}}^{\pm}dk_{x}dk_{y}, (B7)

where 𝐀𝐤±=ψ𝐤±|i𝐤|ψ𝐤±\mathbf{A}_{\mathbf{k}}^{\pm}=\langle\psi_{\mathbf{k}}^{\pm}|i\partial_{\mathbf{k}}|\psi_{\mathbf{k}}^{\pm}\rangle is the Berry connection, and the integral region is in the first Brillouin zone. We simply have

𝐀𝐤±=12x^kxθ𝐤,\mathbf{A}_{\mathbf{k}}^{\pm}=-\frac{1}{2}\hat{x}\partial_{k_{x}}\theta_{\mathbf{k}}, (B8)

and

𝐏±=12x^𝒲=12x^{1,|λ|<10,|λ|>1.\mathbf{P}^{\pm}=-\frac{1}{2}\hat{x}\mathcal{W}=\frac{1}{2}\hat{x}\left\{\begin{array}[]{cc}1,&\left|\lambda\right|<1\\ 0,&\left|\lambda\right|>1\end{array}\right.. (B9)

The topological characterization is obvious since

𝒲=12πππkxarg(ϑ𝐤)dkx\mathcal{W}=\frac{1}{2\pi}\int_{-\pi}^{\pi}\partial_{k_{x}}\arg\left(\vartheta_{\mathbf{k}}\right)dk_{x} (B10)

is essentially the winding number.

In the topologically nontrivial phase |λ|<1\left|\lambda\right|<1, we have nonzero polarization 𝐏±=(1/2,0)\mathbf{P}^{\pm}=\left(1/2,0\right), thus it is expected to observe the topological edge state in the boundary of xx direction when the cylindrical boundary condition is taken. In fact, it can be checked that in the large-NxN_{x} limit, the system supports two degenerate edge modes

|ψky,σL\displaystyle|\psi_{k_{y},\sigma}^{\mathrm{L}}\rangle =\displaystyle= Ωx(λ)x1ax,ky,σ|Vac,\displaystyle\Omega\sum_{x}\left(-\lambda\right)^{x-1}a_{x,k_{y},\sigma}^{{\dagger}}|\mathrm{Vac}\rangle,
|ψky,σR\displaystyle|\psi_{k_{y},\sigma}^{\mathrm{R}}\rangle =\displaystyle= Ωx(λ)Nxxbx,ky,σ|Vac,\displaystyle\Omega\sum_{x}\left(-\lambda\right)^{N_{x}-x}b_{x,k_{y},\sigma}^{{\dagger}}|\mathrm{Vac}\rangle, (B11)

with the eigenenergy EL/R=6coskyE^{\mathrm{L}/\mathrm{R}}=6\cos k_{y} and the normalization constant Ω=1λ2\Omega=\sqrt{1-\lambda^{2}}, where the inverse transformation is (ax,ky,σ,bx,ky,σ)=Ny1/2y(c2x1,y,σ,c2x,y,σ)eikyy\left(a_{x,k_{y},\sigma},b_{x,k_{y},\sigma}\right)=N_{y}^{-1/2}\sum_{y}\left(c_{2x-1,y,\sigma},c_{2x,y,\sigma}\right)e^{-ik_{y}y}.

C More exact numerical results and approximate numerical results

Refer to caption
Figure 5: Numerical results of the local particle density ρ(𝐫)\rho\left(\mathbf{r}\right) and correlator C(1,y)C\left(1,y\right) for the system with 33 (\uparrow\uparrow\downarrow) fermions obtained from exact diagonalization. The lattices size and Hubbard interaction strength are all (Nx,Ny)=(5,4)(N_{x},N_{y})=(5,4) and U=1.5U=1.5.
Refer to caption
Figure 6: Comparison of energy Ep+eE_{\mathrm{p+e}} with Ep+EeE_{\mathrm{p}}+E_{\mathrm{e}} obtained form exact diagonalization (a) as function of λ\lambda with fixed U=1.5U=1.5; (b) as function of UU with fixed λ=0.2\lambda=0.2. The lattices size is (Nx,Ny)=(5,4)(N_{x},N_{y})=(5,4).
Refer to caption
Figure 7: Numerical results obtained from the effective Hamiltonian in the subspace of edge states. (a1) and (b1) are local particle density ρ(𝐫)\rho\left(\mathbf{r}\right). (a2) and (b2) show correlator C(1,y)C\left(1,y\right) for the systems with different numbers of fermions and parameters λ\lambda. The lattices size and Hubbard interaction strength are all (Nx,Ny)=(11,8)(N_{x},N_{y})=(11,8) and U=1.5U=1.5. The numbers of fermions are 88 (444\uparrow 4\downarrow) and 99 (545\uparrow 4\downarrow ); the energies are E=6.00E=6.00 and E=10.24E=10.24, for (a) and (b), respectively.

To visualize the distribution of the fermions of a state in real space, we calculate the local particle density

ρ(𝐫)=σ=,ψedge|n𝐫,σ|ψ edge .\rho\left(\mathbf{r}\right)=\sum_{\sigma=\uparrow,\downarrow}\langle\psi_{\text{{edge}}}|n_{\mathbf{r},\sigma}|\psi_{\text{{\ edge }}}\rangle. (C1)

The numerical results of the local particle density ρ(𝐫)\rho\left(\mathbf{r}\right) for the η\eta-pairing edge states with two and four fermions are presented in Figs. 4(a) and 4(b), which respectively correspond to the cases considered in Figs. 2(a) and 2(b) of the main text. In Fig. 5, we present the numerical results of the three-fermion (\uparrow\uparrow\downarrow) case. It indicates that the three-fermion η\eta-pairing edge state also has off-diagonal long-range order. This is the simplest two-fluid edge state. We can gain some intuition in term of energy. We choose one of the three-fermion edge states with energy Ep+eE_{\mathrm{p+e}} from the numerical data. In Fig. 6, we present the comparison between the energy Ep+eE_{\mathrm{p+e}} and Ep+EeE_{\mathrm{p}}+E_{\mathrm{e}}, as functions of λ\lambda [Fig. 6(a)] and UU [Fig. 6(b)], where EpE_{\mathrm{p}} is the energy of η\eta-pairing edge state in two-fermion subspace and EeE_{\mathrm{e}} is the energy of a single-fermion edge state. It indicates that the energy Ep+eE_{\mathrm{p+e}} has the form of Ep+EeE_{\mathrm{p}}+E_{\mathrm{e}} for small λ\lambda or large UU. This suggests the existence of the two-fluid edge states in certain parameter region.

To handle a larger system, we can write the matrix of effective Hamiltonian in the edge-states subspace. For the extended 2D SSH Hubbard model with zero UU, there are two kinds of single-particle states: edge states |ψky,σL/R|\psi_{k_{y},\sigma}^{\mathrm{L/R}}\rangle and bulk states |ψky,σbulk|\psi_{k_{y},\sigma}^{\mathrm{bulk}}\rangle, in the topologically nontrivial phase with |λ|<1\left|\lambda\right|<1. The wave function of an edge state exponential decay from edge to bulk, then the spatial overlap of these two states tends to zero in the thermodynamic limit, that is |ψky,σL/R|n𝐫,σ|ψky,σbulk|0|\langle\psi_{k_{y},\sigma}^{\mathrm{\ L/R}}|n_{\mathbf{r},\sigma}|\psi_{k_{y}^{\prime},\sigma}^{\mathrm{bulk}}\rangle|\rightarrow 0 for any 𝐫\mathbf{r}. Since the Hubbard interaction U𝐫n𝐫,n𝐫,U\sum_{\mathbf{r}}n_{\mathbf{r},\uparrow}n_{\mathbf{r},\downarrow} is local, when it is switched on, it does not hybridize these two kinds of states approximately, that is 𝐫|n𝐫,σn𝐫,σ|ψky,σL/R|ψky,σbulk|0\sum_{\mathbf{r}}|n_{\mathbf{r},\sigma}n_{\mathbf{r},\sigma^{\prime}}|\psi_{k_{y},\sigma}^{\mathrm{L/R}}\rangle|\psi_{k_{y}^{\prime},\sigma^{\prime}}^{\mathrm{bulk}}\rangle|\approx 0 (σσ)\left(\sigma\neq\sigma^{\prime}\right). The main hybridization occurs between the bulk states, or the edge states. Notably, this approximation is more effective when NxN_{x} is larger. Then we can consider the physics in the invariant subspace of edge states {|ψky,σL/R}\{|\psi_{k_{y},\sigma}^{\mathrm{L/R}}\rangle\}, which has bipartite lattice symmetry that ensures the formation of two-fluid edge states. Based on this approximation, the η\eta-pairing edge states in a larger system can be calculated approximately. In Figs. 7 (a) and 7(b), we present the numerical results with 88 and 99 fermions on the lattice with size (Nx,Ny)=(11,8)(N_{x},N_{y})=(11,8), respectively, obtained from the effective Hamiltonian in the subspace of edge states. We can see that for the cases of more fermions in a larger system, the η\eta-pairing and two-fluid edge states with off-diagonal long-range order still exist.

D Non-Hermitian description of resonant transmission

In this section, we establish a connection between the resonant transmission of a scattering center and the EP dynamics of a non-Hermitian system, which is consisted with the scattering center and two extra sites. Two systems are schematically illustrated in Fig. 8(a) and 8(b). We consider a general scattering system by a single-particle Hamiltonian

Refer to caption
Figure 8: (a) Schematic illustration of the Hermitian system HscattH_{\mathrm{scatt}} in Eq. (D1). The orange arrows represent the wave of resonant transmission. (b) Schematic illustration of the effective non-Hermitian system HeffH_{\mathrm{eff}} in Eq. (D5). The black arrows indicate the unidirectional hoppings. The gray areas represent two identical scattering centers HcH_{\mathrm{c}}.
Refer to caption
Figure 9: Schematic illustration of the configuration of the non-Hermitian Hamiltonian HNHH_{\text{{NH}}} considered in the main text. The blue dots represent two extra sites with on-site potential of strength μ\mu. The arrows indicate the unidirectional hopping of strength JJ.
Hscatt=HLd+Hc,H_{\mathrm{scatt}}=H_{\mathrm{Ld}}+H_{\mathrm{c}}, (D1)

where HLdH_{\mathrm{Ld}} represents the two leads,

HLd\displaystyle H_{\mathrm{Ld}} =\displaystyle= Jj=1(|jj1|+|jj+1|)\displaystyle J\sum_{j=1}^{\infty}\left(\left|-j\right\rangle\left\langle-j-1\right|+\left|j\right\rangle\left\langle j+1\right|\right)
+J(|1α|+|1α|)+H.c.+μ|j|=1|jj|,\displaystyle+J\left(\left|-1\right\rangle\left\langle\alpha\right|+\left|1\right\rangle\left\langle\alpha\right|\right)+\mathrm{\ H.c.}+\mu\sum_{\left|j\right|=1}^{\infty}\left|j\right\rangle\left\langle j\right|,

while HcH_{\mathrm{c}} is a scattering center of NN sites,

Hc=q=1Nεq|ϕqϕq|.H_{\mathrm{c}}=\sum_{q=1}^{N}\varepsilon_{q}\left|\phi_{q}\right\rangle\left\langle\phi_{q}\right|. (D3)

Here α\alpha represents a site in the cluster HcH_{\mathrm{c}} connecting to the left and right leads. |ϕq\left|\phi_{q}\right\rangle denotes the normalized eigenstate of HcH_{\mathrm{c}} with energy εq\varepsilon_{q}. Now we consider the case, in which HcH_{\mathrm{c}} has an isolated energy level at q=ρq=\rho, satisfying μ=ερ\mu=\varepsilon_{\rho} and |ερερ±1|J\left|\varepsilon_{\rho}-\varepsilon_{\rho\pm 1}\right|\gg J. It can be checked that the state |ψπ/2|\psi_{\pi/2}\rangle in the form

|ψπ/2={eiπj/2|j,|j|1γ|ϕρ,j{c},|\psi_{\pi/2}\rangle=\left\{\begin{array}[]{cc}e^{-i\pi j/2}\left|j\right\rangle,&\left|j\right|\geqslant 1\\ \gamma\left|\phi_{\rho}\right\rangle,&j\in\left\{\mathrm{c}\right\}\end{array}\right., (D4)

is an eigenstate of HscattH_{\mathrm{scatt}} with energy ερ\varepsilon_{\rho}. where {c}\left\{\mathrm{c}\right\} denotes the set of index for the sites of scattering center. Here γ\gamma is a complex number, determined by α|ϕρ=γ1\left\langle\alpha\right|\phi_{\rho}\rangle=\gamma^{-1}.

In parallel, we consider a non-Hermitian Hamiltonian

Heff\displaystyle H_{\mathrm{eff}} =\displaystyle= J(|α1|+|1α|)\displaystyle J\left(\left|\alpha\right\rangle\left\langle-1\right|+\left|1\right\rangle\left\langle\alpha\right|\right) (D5)
+q=1Nεq|ϕqϕq|+μj=±1|jj|,\displaystyle+\sum_{q=1}^{N}\varepsilon_{q}\left|\phi_{q}\right\rangle\left\langle\phi_{q}\right|+\mu\sum_{j=\pm 1}\left|j\right\rangle\left\langle j\right|,

which contains two unidirectional hopping terms. For the isolated energy level with |ερερ±1|J\left|\varepsilon_{\rho}-\varepsilon_{\rho\pm 1}\right|\gg J, it reduces to

Heff\displaystyle H_{\mathrm{eff}} \displaystyle\approx J(|α1|+|1α|)\displaystyle J\left(\left|\alpha\right\rangle\left\langle-1\right|+\left|1\right\rangle\left\langle\alpha\right|\right) (D6)
+ερ|ϕρϕρ|+μj=±1|jj|.\displaystyle+\varepsilon_{\rho}\left|\phi_{\rho}\right\rangle\left\langle\phi_{\rho}\right|+\mu\sum_{j=\pm 1}\left|j\right\rangle\left\langle j\right|.

Under the resonant condition μ=ερ\mu=\varepsilon_{\rho} the dynamics is governed by the Jordan block with order of three

MJB=(μ00Jμ00Jμ).M_{\mathrm{JB}}=\left(\begin{array}[]{ccc}\mu&0&0\\ J&\mu&0\\ 0&J&\mu\end{array}\right). (D7)

For initial state |ψ(0)=|1=(1,0,0)T\left|\psi(0)\right\rangle=\left|-1\right\rangle=\left(1,0,0\right)^{\mathrm{T}}, the final state is |ψ()=|1=(0,0,1)T\left|\psi(\infty)\right\rangle=\left|1\right\rangle=\left(0,0,1\right)^{\mathrm{T}}, due to the fact

exp(iMJBt)\displaystyle\exp\left(-iM_{\mathrm{JB}}t\right)
=\displaystyle= exp(iμt)[1i(MJBμ)t12(MJBμ)2t2],\displaystyle\exp\left(-i\mu t\right)\left[1-i\left(M_{\mathrm{JB}}-\mu\right)t-\frac{1}{2}\left(M_{\mathrm{JB}}-\mu\right)^{2}t^{2}\right],

and

exp(iMJBt)(100)=exp(iμt)(1iJt12J2t2).\exp\left(-iM_{\mathrm{JB}}t\right)\left(\begin{array}[]{c}1\\ 0\\ 0\end{array}\right)=\exp\left(-i\mu t\right)\left(\begin{array}[]{c}1\\ -iJt\\ -\frac{1}{2}J^{2}t^{2}\end{array}\right). (D8)

A straightforward implication of the result is that this process accords with the resonant transmission, i.e., the particle is perfectly transported from the left to the right.

Nevertheless, we would like to point that no matter if it is resonant or not, the Jordan block always exists, but with different order. Here we consider the case of μ\mu deviate from ερ\varepsilon_{\rho}, and the dynamics is governed by the matrix

M=(μ00Jερ00Jμ).M=\left(\begin{array}[]{ccc}\mu&0&0\\ J&\varepsilon_{\rho}&0\\ 0&J&\mu\end{array}\right)\text{.} (D9)

Here matrix MM can be related to the Jordan block with order of two, which is (μ001μ000ερ)\left(\begin{array}[]{ccc}\mu&0&0\\ 1&\mu&0\\ 0&0&\varepsilon_{\rho}\end{array}\right), by Jordan decomposition. The time evolution is

exp(iMt)(100)=exp(iμt)(1ςτς2[τ+i(ερμ)t]),\exp\left(-iMt\right)\left(\begin{array}[]{c}1\\ 0\\ 0\end{array}\right)=\exp\left(-i\mu t\right)\left(\begin{array}[]{c}1\\ \varsigma\tau\\ \varsigma^{2}\left[\tau+i\left(\varepsilon_{\rho}-\mu\right)t\right]\end{array}\right), (D10)

where ς=J/(ερμ)\varsigma=J/\left(\varepsilon_{\rho}-\mu\right) and τ=exp[i(ερμ)t]1\tau=\exp\left[-i\left(\varepsilon_{\rho}-\mu\right)t\right]-1.

It indicates that in the resonant case, the evolved state converges to the target state more rapidly. In other word, to distinguish two different processes, we can observe the fidelity between the evolved state and the target state for two different dynamics processes at the same sufficiently long time tt.

In Fig. 9, we present the schematic illustration of the system configuration of the Hamiltonian in Eq. (13) of the main text.

References