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Continuous phase transition induced by non-Hermiticity in the quantum contact process model

Wen-Bin He 111These two authors contributed equally to the work Beijing Computational Science Research Center, Beijing, 100193, China Quantum Systems Unit, Okinawa Institute of Science and Technology Graduate University, 904-0495 Okinawa, Japan    Jiasen Jin 222These two authors contributed equally to the work School of Physics, Dalian University of Technology, Dalian 116024, China    Fernando Iemini Instituto de Física, Universidade Federal Fluminense, 24210-346 Niterói, Brazil The Abdus Salam International Center for Theoretical Physics, Strada Costiera 11, 34151 Trieste, Italy.    Hai-Qing Lin Beijing Computational Science Research Center, Beijing, 100193, China School of Physics, Zhejiang University, Hangzhou, 310030, China. fernandoiemini@gmail.com haiqing0@csrc.ac.cn submissions@iop.org
Abstract

Non-Hermitian quantum system recently have attracted a lots of attentions theoretically and experimentally. However, the results based on the single-particle picture may not apply to understand the property of non-Hermitian many-body system. How the property of quantum many-body system especially the phase transition will be affected by the non-Hermiticity remains unclear. Here we study non-Hermitian quantum contact process (QCP) model, whose effective Hamiltonian is derived from Lindbladian master equation. We show that there is a continuous phase transition induced by the non-Hermiticity in QCP. We also determine the critical exponents β\beta of order parameter, γ\gamma of susceptibility and study the correlation and entanglement near phase transition point. We observe that the order parameter and susceptibility display infinitely singularity even for finite size system, since non-Hermiticity endow many-body system with different singular behaviour from classical phase transition. Moreover our results show that the phase transition have no counterpart in Hermitian case and belongs to completely different universality class.

1 Introduction

Non-Hermitian physics currently has attracted considerable attentions [1, 2], which greatly extend the knowledge about quantum system. For example, the complex energy coalesce at exceptional point(EP)[2, 3, 4, 5]; The wave function localize at the edge of quantum system, which is now named as non-Hermitian skin effect[3, 4, 6, 7]. Actually, quantum systems almost are subjected to environment. It is more appropriate to consider the quantum system to be non-Hermitian(NH). Recently, it was found that driven-dissipative non-Hermitian system can provide one method to control quantum system, for instance, directional amplification [8, 9, 10, 11]. Non-Hermiticity can impose great influence on the properties of the topological non-trivial system. It needs generalized Brillouin zone to establish a generalized Bloch band theory [4, 12, 13]. Non-Hermiticity can also induce phase transition without gap[14] and non-Hermitian many-body localization [15]. Non-Hermitian quantum system needs more effort to be studied, understood and utilized.

Though we have understood several interesting property of non-Hermitian quantum system which based on single-particle picture, it is an important issue to understand that how non-Hermiticity affect many-body system, especially the phase transition of many-body system. The theory of phase transition provide people profound understanding to the status of the matter. When non-Hermiticity comes into quantum many-body system, whether non-Hermiticity can induce phase transition, and if the phase transition exists how to classify this type of phase transition. These questions remain being elusive. Moreover, what the relation is between the phase transition induced by non-Hermiticity and their Hermitian counterpart. As the primary motivation to answer above questions, we are going to explore the phase transition induced by non-Hermiticity in quantum contact process model.

In this work, we consider the open system whose dynamics governed by Lindbladian master equation. We use effective Hamiltonian to describe the property of non-Hermitian quantum system. Then we choose quantum contact process(QCP) model as research object, which breaks U(1)U(1) symmetry. We combine analytical method for special case of spin number L=2L=2 and exact diagonalization(ED) for general LL to compute energy spectrum, the order parameter MxM^{x}, susceptibility χ\chi, correlation, and entanglement entropy. The results of this work show that there is continuous phase transition within the non-Hermitian QCP model. We extract the critical exponents, β\beta of order parameter, γ\gamma of susceptibility. We reveal the transition from quasi long-rang order to short-range order and entanglement properties near critical point. Finally, we compare the results of non-Hermitian QCP model with Hermitian counterpart, which shows the phase transition in non-Hermitian QCP model have no correspondence in Hermitian case. By looking at the critical exponents, the results in our work may indicate the phase transition belongs a new universality class. Moreover, even for finite size system, we notice non-Hermiticity endow many-body system with different singular behaviour from classical phase transition. Our results can extend the knowledge about the phase transition of non-Hermitian quantum matter.

2 Non-Hermitian QCP model

For the open quantum many-body systems, its dynamics usually can be determined by Lindbladian master equation [16] as

ρ˙(t)=i[H^0,ρ(t)]+kL𝒟k[ρ(t)].\dot{\rho}(t)=-i[\hat{H}_{0},\rho(t)]+\sum_{k}^{L}{{\cal D}_{k}[\rho(t)]}. (1)

where H^0\hat{H}_{0} is Hamiltonian governing the coherent evolution of the system. The dissipation superoperator 𝒟α[ρ(t)]=L^kρ(t)L^k,12{L^kL^k,ρ(t)}{\cal D}_{\alpha}[\rho(t)]=\hat{L}^{k}\rho(t)\hat{L}^{k,\dagger}-\frac{1}{2}\{\hat{L}^{k^{\dagger}}\hat{L}^{k},\rho(t)\} is defined by the following Lindbladian jump operator, L^k=Γσk\hat{L}^{k}=\sqrt{\Gamma}\sigma_{-}^{k} which impose local spin decaying channels. In the absence of quantum jumps during a time interval, the term Lkρ(t)LkL^{k}\rho(t)L^{k\dagger}, which describes the state transition, can be omitted[1, 17]. This corresponds to postselection [17, 18]in the experiment, which target on succeed measurement results. In this case, the quantum system is considered to undergo a non-unitary time evolution governed by an effective Hamiltonian which is derived from the master equation(1) as follows

H^eff=H^0i2k=1LL^kL^k.\hat{H}_{\rm eff}=\hat{H}_{0}-\frac{i}{2}\sum_{k=1}^{L}\hat{L}^{k^{\dagger}}\hat{L}^{k}. (2)

In following discussion, we omit subscript for the non-Hermitian Hamiltonian. Since the Lindbladian operator above, we are interested in exploring the properties of non-Hermitian many-body system which is described by the effective Hamiltonian as

H^=H^0i2Γk=1Lσ^+kσ^k.\hat{H}=\hat{H}_{0}-\frac{i}{2}\Gamma\sum_{k=1}^{L}\hat{\sigma}_{+}^{k}\hat{\sigma}_{-}^{k}. (3)

From above formula, which gives out the non-Hermitian Hamiltonian of a class of spin many-body system with jump operator of L^k=Γσk\hat{L}^{k}=\sqrt{\Gamma}\sigma_{-}^{k}, it can be found that dissipation imposes imaginary field along zz-direction by looking at formula σ+kσk=(σzk+I)/2\sigma_{+}^{k}\sigma_{-}^{k}=(\sigma_{z}^{k}+I)/2. We look back at the knowledge about the general matrix. There are the left and right eigen-energy and eigenvectors with the non-Hermitian effective Hamiltonian, which are denoted by

H^|ϕRi=Ei|ϕRi,\displaystyle\hat{H}|\phi_{R}^{i}\rangle=E_{i}|\phi_{R}^{i}\rangle, (4)
ϕLi|H^=EiϕLi|,\displaystyle\langle\phi_{L}^{i}|\hat{H}=E_{i}\langle\phi_{L}^{i}|, (5)

with eigenvalues EiE_{i}\in\mathbb{C}. The left and right eigenvectors satisfy bi-orthonormal relation and completeness relation [19]

ϕLi|ϕRj=δijϕLj|ϕRj,\displaystyle\langle\phi_{L}^{i}|\phi_{R}^{j}\rangle=\delta_{ij}\langle\phi_{L}^{j}|\phi_{R}^{j}\rangle, (6)
j|ϕRjϕLj|ϕLj|ϕRj=I.\displaystyle\sum_{j}\frac{|\phi_{R}^{j}\rangle\langle\phi_{L}^{j}|}{\langle\phi_{L}^{j}|\phi_{R}^{j}\rangle}=I. (7)

The properties of eigen-energy and eigenvectors of non-Hermitian are completely different from the Hermitian case, which endow non-Hermitian system with interesting new physics. When at least two eigen-energies coalesce with each other, exceptional point(EP) emerges[3, 4, 16, 19, 20, 21]. In order to obtain EP with our model in Eq(3), original Hamiltonian H0H_{0} must not conserve spin polarization. If [H^0,kσzk]=0\left[\hat{H}_{0},\sum_{k}\sigma_{z}^{k}\right]=0 holds, the non-Hermitian term in Eq(3) can only give us trivial complex energy. Such that we choose quantum contact process(QCP) model in 1D as research object

H^0=Ωk=1L(σ^xkσ^nk+1+σ^nkσ^xk+1),\hat{H}_{0}=\Omega\sum_{k=1}^{L}\left(\hat{\sigma}_{x}^{k}\hat{\sigma}_{n}^{k+1}+\hat{\sigma}_{n}^{k}\hat{\sigma}_{x}^{k+1}\right), (8)

with σ^nk=σ^+kσ^k\hat{\sigma}_{n}^{k}=\hat{\sigma}_{+}^{k}\hat{\sigma}_{-}^{k} and LL the number of spins in the system. QCP model has been widely studied in open many-body system, such as quantum epidemic dynamics [22, 23], experimental realization by Rydberg atom [24]. We arrive at non-Hermitian Hamiltonian as

H^=ΩkL(σ^xkσ^nk+1+σ^nkσ^xk+1)i2Γ^k=1Lσ^+kσ^k,\hat{H}=\Omega\sum_{k}^{L}\left(\hat{\sigma}_{x}^{k}\hat{\sigma}_{n}^{k+1}+\hat{\sigma}_{n}^{k}\hat{\sigma}_{x}^{k+1}\right)-\frac{i}{2}\Gamma\hat{\sum}_{k=1}^{L}\hat{\sigma}_{+}^{k}\hat{\sigma}_{-}^{k}, (9)

which determines non-Hermitian physics in our model. For convenience with following discussion, we set Ω=1\Omega=1 to make the parameter of Hamiltonian dimensionless. In our work, we always use periodic boundary condition.

Refer to caption
Figure 1: The subplots (a)(b)(c)(d), distribution pattern of complex energy spectrum for four different Γ\Gamma; The lowest and highest seven real part (e) and their imaginary part (f) of energy spectrum EE vary with Γ\Gamma. Ω=1,L=10\Omega=1,L=10.

We firstly look at the complex energy spectrum of the non-Hermitian system for two spins case L=2L=2. We obtain four eigen-energies as E1=0(trivial)E_{1}=0\quad(\rm trivial), E2=iΓ/2E_{2}=-i\Gamma/2, E3,4=i3Γ4±1432Ω2Γ2E_{3,4}=\frac{-i3\Gamma}{4}\pm\frac{1}{4}\sqrt{32\Omega^{2}-\Gamma^{2}}, please see the [25] for the matrix and eigenvectors for L=2L=2. It is easy to determine the EP as Γc=32Ω\Gamma_{c}=\sqrt{32}\Omega, where E3E_{3} and E4E_{4} coalesce with each other. For many-body case, we look at the energy spectrum changing with dissipation strength Γ\Gamma by exact diagonalization(ED). We used brute-force diagonalization up to N=12N=12 as eig of matlab, and diagonalization based on Lanczos method for ground state up to N=16N=16 as eigs of matlab. See Fig. 1 subplots(a-d), energy spectrum changes with Γ\Gamma from distributing on complex plane of EE to distributing on imaginary axis. Moreover, the real part of the energy varies with dissipation strength Γ\Gamma from finite values to zero at around Γ14\Gamma\sim 14, whose singularity looks like the order parameter of second-order phase transition [26]; while there is split with the imaginary part of energy. We also notice that iH^effi\hat{H}_{eff} satisfies pseudo-Hermiticity [1] by transforming Hamiltonian and energy spectrum

H^effiH^eff\displaystyle\hat{H}_{eff}\rightarrow i\hat{H}_{eff}
(±Ere+iEim)(±iEreEim)\displaystyle(\pm E_{re}+iE_{im})\rightarrow(\pm iE_{re}-E_{im})

which results in that the eigenvalues appear in complex conjugate pairs at left of EP and the spectrum are entirely real at right of EP. These analysis show that HeffH_{eff} of NH QCP has anti-PT symmetry breaking [27, 28, 29] near EP. The singularity of the real part energy and anti-PT breaking indicates a transition in the energy spectrum of the non-Hermitian model (9), as a complex-imaginary transition.

In order to understand the complex-imaginary transition better, we are going to analyse the phase transition by studying the order parameter and susceptibility. But here we need to make preparation by defining the ground state of non-Hermitian many-body system. Ground states: we define the ”ground state” |ψR/L|\psi_{R/L}\rangle as the state ψ0\psi_{0} associated to the energy E0E_{0} with minimum real part as did in literatures [14, 30]. The state with smallest real part can map to traditional ground state through continuation between the non-Hermitian case and Hermitian case, which can be observed within short time evolution in the absence of quantum jump[15, 14] due to its imaginary part. The state with largest imaginary part corresponds to the steady state that can be observed within long time evolution [21, 20]. By continuation we mean that the non-Hermitian Hamiltonian becomes the Hermitian case when the dissipation Γ\Gamma tends to zero and the chosen ”ground state” recover to the traditional one, namely the state corresponds to the smallest real energy. The former satisfies the requirement of continuation while the latter does not. When the system crosses to right side of the exceptional point, since energies become imaginary such that above definition of ground state become invalid, we track the continuity and analyticity of energy and observables to choose the ground state. Concretely, the ground state should keep the continuity of imaginary part of ground state from left side to right side of EP firstly. After reaching right side of EP, we use continuity and analyticity of observables to determine the ground state. In following part, we will reveal the phase transition induced by non-Hermiticity in our model in detail.

Refer to caption
Figure 2: (a)The spin polarization along xx-axis direction Mx=kσxkM^{x}=\left\langle\sum_{k}\sigma^{k}_{x}\right\rangle of ground state vary with Γ\Gamma for different system size LL; (b) the absolute value of MxM^{x} near critical point V.S dissipation strength in logarithmic scale. The scaling exponent of Mx|Γc(L)Γ|βM^{x}\sim-|\Gamma_{c}(L)-\Gamma|^{\beta} is fitted out for different system size, see the Table.(1). Ω=1\Omega=1.
Table 1: The critical points,critical exponents of order parameter of spin polarization along x-direction MxM^{x} for different system size LL. normr\mathrm{normr} stands for norm of residuals.
LL 4 5 6 7 8 9 10
Γc(L)\Gamma{c}(L) 13.4396 13.6116 13.6969 13.7424 13.7720 13.7898 13.8016
β\beta 0.5102 0.5209 0.5303 0.5117 0.5261 0.5251 0.5026
normr\mathrm{normr} 0.0336 0.0582 0.0953 0.0108 0.0319 0.0383 0.0122
LL 11 12 13 14 15 16
Γc(L)\Gamma{c}(L) 13.8106 13.8169 13.8223 13.8259 13.8289 13.8312
β\beta 0.5069 0.4968 0.5178 0.5120 0.5201 0.5122
normr\mathrm{normr} 0.0111 0.0687 0.0063 0.0129 0.0504 0.0181

3 The observables and critical exponents

Generally, we use right ground eigenstate to compute the observables

O=ψR|O^|ψR,O=\langle\psi_{R}|\hat{O}|\psi_{R}\rangle, (10)

which can make sure that observables are always real. In fact, it can give the same results by using right eigenstate and using left-right eigenstate, see Fig.10 in appendix [25]. In order to compute the susceptibility of system, we impose a small probe magnetic field along the zz-axis,

H^H^δh/2kσ^zk=H^δhk(σ^+kσ^kI/2).\hat{H}\rightarrow\hat{H}-\delta h/2\sum_{k}\hat{\sigma}_{z}^{k}=\hat{H}-\delta h\sum_{k}(\hat{\sigma}_{+}^{k}\hat{\sigma}_{-}^{k}-I/2). (11)

The spin polarization Mα=ψR|kσ^αk|ψRM^{\alpha}=\langle\psi_{R}|\sum_{k}\hat{\sigma}_{\alpha}^{k}|\psi_{R}\rangle for general direction α=x,y,z\alpha=x,y,z. In our work, we choose spin polarization along xx-axis MxM^{x} as order parameter. The susceptibility can be given by the differential,

χ=(Mz(δh)Mz(0))/2δh.\chi=(M^{z}(\delta h)-M^{z}(0))/2\delta h. (12)

The non-analytical behaviour of order parameter and susceptibility can help us to reveal the property of phase transition for non-Hermitian QCP model.

As shown in Fig. 2, order parameter MxM^{x} vary with dissipation strength Γ\Gamma for different spin number up to L=16L=16 in linear axis (a) and logarithmic axis (b). The critical points for different system size are determined when MxM^{x} becomes zero. While in Fig. 2(b) the data almost collapse into one straight line in logarithmic scale, we extract the critical exponents β\beta for different spin number according to scaling function

Mx|Γc(L)Γ|β.M^{x}\sim-|\Gamma_{c}(L)-\Gamma|^{\beta}. (13)

The critical points for different system size gradually converge to true critical point. In Table.1, we list critical points and critical exponents for system size from L=4L=4 to L=16L=16. And normr\mathrm{normr} stands for norm of residuals, which quantifies the error for fitting our data to the scaling function in logarithmic axis. All critical exponents for different system sizes are nearly the same. After taking average of critical exponents of different LL, the critical exponent of order parameter is estimated as β¯0.51\bar{\beta}\approx 0.51. In fact, we can look at theoretical results of special case L=2L=2 to check numerical results. The order parameter can be written as

Mx2Γc(2)Γc(2)ΓΓc(2)Γ,M^{x}\sim\sqrt{2\Gamma_{c}(2)}\sqrt{\Gamma_{c}(2)-\Gamma}\sim\sqrt{\Gamma_{c}(2)-\Gamma}, (14)

here Γc(2)=32Ω\Gamma_{c}(2)=\sqrt{32}\Omega mean the EP for L=2L=2, see appendix [25] for details. This theoretical analysis confirm numerical results of critical exponent. From above analysis, we can confidently claim the true critical exponent for thermodynamic limit β=1/2\beta=1/2 [31]. The results of order parameter MxM^{x} confirm the analysis by energy spectrum in Fig. 1, namely there is continuous phase transition induced by non-Hermiticity in QCP model. To be added, we observe the non-analytical behaviour of order parameter for finite size system even L=2L=2. While, for classical phase transition of Hermitian models, non-analytical behaviour of order parameter appears in thermodynamic limit. When system size is finite, order parameter become smooth near critical point. In reference [20], the authors noticed similar behaviours. The non-analytical behaviour of order parameter for finite system size in our work may be related to non-Hermiticity, which is very different from classical phase transition of Hermitian case.

Table 2: The critical points, critical exponents and amplitude of susceptibility for different system size LL.
LL 4 5 6 7 8
Γc(L)\Gamma{c}(L) 13.4388 13.6092 13.6949 13.7418 13.7704
γ\gamma 1.5198 1.5829 1.4975 1.5049 1.4986
χ0104\chi_{0}*10^{-4} 0.2972 0.2614 0.3377 0.3384 0.3573
normr\mathrm{normr} 0.0009 0.0061 0.0001 0.0001 0.0003
LL 9 10 11 12
Γc(L)\Gamma{c}(L) 13.7887 13.8010 13.8105 13.8168
γ\gamma 1.5273 1.4969 1.4999 1.5731
χ0104\chi_{0}*10^{-4} 0.3337 0.3907 0.3809 0.2833
normr\mathrm{normr} 0.0008 0.0022 0.0002 0.0110
Refer to caption
Figure 3: The susceptibility χ\chi vary with Γ\Gamma in linear scale(a) and vary with ΓΓc(L)\Gamma-\Gamma_{c}(L) in logarithmic scale(b) for different size L=[4,5,6,7,8,9,10,11,12]L=[4,5,6,7,8,9,10,11,12] . By linear fitting in logarithmic scaling of formula χ=χ0/(ΓΓc(L))γ\chi=\chi_{0}/(\Gamma-\Gamma_{c}(L))^{\gamma}, the critical points, the scaling exponents γ\gamma and amplitude χ0\chi_{0} in the table.2.

We also study the magnetic susceptibility χ\chi along zz-direction, see Fig. 3. We show susceptibility vary with dissipation Γ\Gamma for different spin number up to L=12L=12 in linear axis (a) and logarithmic axis (b). We can also observe that the susceptibility tends to infinite divergence for finite size system rather than finite peak for classical phase transition. As increasing system size, susceptibility strongly diverges near critical points in Fig. 3(a). Moreover these diverging data can collapse into one straight line in logarithmic scale in Fig. 3(b) except the data of small size L=4L=4 with small error. The critical exponent of susceptibility is extracted according to scaling relation

χ=χ0/(ΓΓc(L))γ.\chi=\chi_{0}/(\Gamma-\Gamma_{c}(L))^{\gamma}. (15)

In Table.2, we list critical points, critical exponents and amplitude of susceptibility for different system size. By comparing the critical points of Table.1 and Table.2, both results of Γc(L))\Gamma_{c}(L)) precisely agree with each other with negligible error. The critical exponents γ\gamma are close to each other near 1.51.5. After taking average of critical exponents γ\gamma, mean value of critical exponent is estimated as γ¯1.52\bar{\gamma}\approx 1.52. Usually, EP is sensitive to disorder [32]. In appendix.C, we consider the non-Hermitian QCP model with random potentials and two spins case. The results indicate that the critical exponent changes even if under weak perturbation, the deviation from β=0.5\beta=0.5 is slight within 5%5\% as shown in Fig. 17 of Appendix.C

Refer to caption
Figure 4: The correlation function Δσ1xσnx\Delta\sigma^{x}_{1}\sigma^{x}_{n} (a) vary with spin site nn for four different Γ\Gamma with system size L=16L=16. Von Neumann entropy SvnS_{vn}(b) vary with Γ\Gamma for half-partition of different system size LL.
Refer to caption
Figure 5: Entanglement entropy SvnS_{vn} (a) for half-partition vary with system size LL and (b) for LAL_{A}-partition vary with LAL_{A} with L=16L=16. The dissipation strength Γ=12.0,13.0,14,15.0\Gamma=12.0,13.0,14,15.0.

4 Correlation and entanglement

In order to understanding the correlation and entanglement near phase transition, we study the correlation function of spin chain with open boundary

Δσ1xσnx=σ^x1σ^xnσ^x1σ^xn.\Delta\sigma^{x}_{1}\sigma^{x}_{n}=\langle\hat{\sigma}_{x}^{1}\hat{\sigma}_{x}^{n}\rangle-\langle\hat{\sigma}_{x}^{1}\rangle\langle\hat{\sigma}_{x}^{n}\rangle. (16)

we also look at Von Neumann entropy SvnS_{vn} of subsystem-AA by partitioning system as L=LA+LBL=L_{A}+L_{B}

Svn=Tr[ρAlnρA]=nλnlnλn,S_{vn}=-\Tr[\rho_{A}\ln\rho_{A}]=-\sum_{n}\lambda_{n}\ln\lambda_{n}, (17)

where reduced density matrix of AA is ρA=TrB[|ψRψR|]\rho_{A}=\Tr_{B}[|\psi_{R}\rangle\langle\psi_{R}|] of ground state |ψR|\psi_{R}\rangle, and {λn}\{\lambda_{n}\} are the eigenvalues of ρA\rho_{A}. During calculation, we define the half-partition as

LA={L/2,mod(L,2)=0(L+1)/2,mod(L,2)=1L_{A}=\left\{\begin{array}[]{ccc}L/2&,&\mod(L,2)=0\\ (L+1)/2&,&\mod(L,2)=1\\ \end{array}\right. (18)

we also used the right eigenstate to make sure that correlation function and Von Neumann entropy are real numbers in the non-Hermitian model.

As seen in fig.4(a), the correlation functions vary with spin site nn for parameters Γ=12,13\Gamma=12,13(red and blue lines) at left side and Γ=14.5,15\Gamma=14.5,15(cyan and pink lines) right side of critical point. Correlations have quasi long-range decay at left side of critical point and nearly exponential decay at right side of critical point. The system at left side seem be quasi long-range ordering (see similar case [20]). Meanwhile, system at right side has short-range ordering. The correlation at left and right side of critical point decay in completely different form regardless of boundary condition, as fig.13 in appendix left panel for periodic boundary and right for open boundary .

As seen in Fig.4(b), entanglement entropy decays with Γ\Gamma for different LL. Non-analytical peaks indicate a NH phase transition for the system from a higher to a lower entangled state. For ground state of NH-QCP model, entanglement characterize the continuous phase transition by non-analytical peak. At same time, we consider two cases to study entanglement entropy, first one: LL changes from 44 to 1616 for half-partition LA=L/2L_{A}=L/2 and second one: LAL_{A} changes from 11 to L/2L/2 for fixed L=16L=16. In Fig.5, we also found the results that entanglement entropy SvnS_{vn} almost (a) do not change with LL for half- partition and (b) do not vary with LAL_{A} for LAL_{A} ranging from 11 to L/2L/2 when Γ[12.0,13.0,14,15.0]\Gamma\in[12.0,13.0,14,15.0] is near Γc\Gamma_{c}. These results reveal that entanglement entropy in NH-QCP model satisfies area law since the surface of spin chain is two spins as Hermitian model in 1D.

By summarizing above results, we have obtained the critical exponents β\beta, γ\gamma for the phase transition in non-Hermitian QCP model. As far as we know, β\beta in our model is same as mean field results; While γ\gamma in our work are different from the known critical exponents. Since the phase transition is related with the coalescence of energy spectrum at EP, non-Hermiticity can endow non-Hermitian many-body system with new critical behaviour, such as shown in Fig. 2. 3. The analysis about critical exponents of β\beta, γ\gamma reveal that the phase transition in non-Hermitian QCP is independent of system size. But the critical points serve as function of system size LL, and correlation length must be constrained by LL. The critical behaviour is governed by the long-wavelength fluctuations such that the critical exponents are universal. For finite size, singularity of phase transition in this work accompany with finite correlation length. This peculiar behaviour should be derived from the singular behaviour of EP for non-Hermitian system. The phase transition for non-Hermitian many-body system may be beyond the classification for Hermitian many-body system.

Refer to caption
Figure 6: subplot(a): By setting real part of Γ\Gamma as zeros, the susceptibility vary with Γim\Gamma_{im} for ground eigenstates of non-Hermitian QCP model. Subplot(b):By setting imaginary part of Γ\Gamma as zeros, the susceptibility of Hermitian QCP model vary with Γre\Gamma_{re} for ground eigenstates. The critical exponent for Hermitian model is γ0.57\gamma\sim 0.57. Subplots(c)(d). The nupn_{up} number of up-spin and order parameter MxM^{x} vary with Γre\Gamma_{re}. L=12L=12, Ω=1\Omega=1.

5 Comparison with Hermitian counterpart.

We compare the results of our model with its Hermitian counterpart by generalizing parameter to complex value iΓΓre+iΓimi\Gamma\rightarrow\Gamma_{\rm re}+i\Gamma_{\rm im} in Eq.(9). The Hamiltonian becomes

H^=Ωk(σ^xkσ^nk+1+σ^nkσ^xk+1)12(Γre+iΓim)k=1Lσ^+kσ^k,\hat{H}=\Omega\sum_{k}\left(\hat{\sigma}_{x}^{k}\hat{\sigma}_{n}^{k+1}+\hat{\sigma}_{n}^{k}\hat{\sigma}_{x}^{k+1}\right)-\frac{1}{2}(\Gamma_{\rm re}+i\Gamma_{\rm im})\sum_{k=1}^{L}\hat{\sigma}_{+}^{k}\hat{\sigma}_{-}^{k}, (19)

where we define Γ=Γre+iΓim\Gamma=\Gamma_{\rm re}+i\Gamma_{\rm im}. When Γ\Gamma taking real part Γre\Gamma_{\rm re}, it corresponds to Hermitian case; While Γ\Gamma taking imaginary part iΓimi\Gamma_{\rm im}, it corresponds to non-Hermitian case in this work. In Fig. 6, we show the susceptibility of non-Hermitian case (a) and Hermitian counterpart(b). By numerical fitting, the critical exponents γ\gamma for both case are respectively near 1.5,0.571.5,0.57. From the difference of critical exponent γ\gamma, it indicates that the continuous phase transition in non-Hermitian QCP model is different from its Hermitian counterpart. By looking at the number of up-spin(c)and order parameter(d) for Hermitian case, these observables discontinuously jump at critical point Γrec4\Gamma_{\rm re}^{c}\sim-4, which imply first-order phase transition with Hermitian QCP model.

We include complementary results of Hermitian model in Figs.7.8. As Fig.7 of numerical results shows, the lowest five energy levels vary with Γre\Gamma_{\rm re}. There is level crossing point at Γre=4Ω\Gamma_{\rm re}=-4\Omega for Hermitian QCP. As shown in Fig.8, the number of up-spin and order parameter which are rescaled with LL vary with Γre\Gamma_{\rm re} for different system sizes, indicating that the jump heights are proportional to system size LL. There are sudden jumps with both observables near critical point. All results for different system size collapse into same curve.

Symmetry analysis: We transform the Hamiltonian of Hermitian case by using σnk=(σzk+1)/2\sigma_{n}^{k}=(\sigma_{z}^{k}+1)/2

H^\displaystyle\hat{H} =Ω2k(σ^xkσ^zk+1+σ^zkσ^xk+1)+Ωkσ^xk\displaystyle=\frac{\Omega}{2}\sum_{k}\left(\hat{\sigma}_{x}^{k}\hat{\sigma}_{z}^{k+1}+\hat{\sigma}_{z}^{k}\hat{\sigma}_{x}^{k+1}\right)+\Omega\sum_{k}\hat{\sigma}_{x}^{k} (20)
\displaystyle- 14Γrek=1Lσ^zk+const.\displaystyle\frac{1}{4}\Gamma_{\rm re}\sum_{k=1}^{L}\hat{\sigma}_{z}^{k}+const.

We notice that in the interaction terms the xx and zz directions play a symmetric role. On the other hand, the external fields (second and third terms) break this symmetry. The symmetric point is Γre=4Ω\Gamma_{\rm re}=-4\Omega, which agrees with critical point in Figs.7.8 by numerics. We can conclude that order parameter MxM^{x} of ground state has sudden jump at two side of critical point hence first-order phase transition with Hermitian counterpart.

In fact, by summarizing the results of critical exponent, we think that phase transition in non-Hermitian QCP model belongs to new universality class from previous known’s. Non-Hermitian many-body system break the Hermitian conjugation symmetry. This type of phase transition is induced by the non-Hermiticity. Moreover, exceptional point is continuous and non-analytical behaviour mathematically for finite size system even L=2L=2. At EP, non-Hermiticity alters the property of ground state hence the non-analytical behaviour of order parameter and singularity of susceptibility. It is uniqueness of non-Hermitian system comparing with regular phase transition of Hermitian counterpart.

Refer to caption
Figure 7: The lowest five energy levels vary with real part of parameter Γre\Gamma_{re} for Hermitian case. L=16L=16, Ω=1\Omega=1.
Refer to caption
Figure 8: The results for Hermitian model. subfig(a):The rescaled nupn_{up} vary with Γre\Gamma_{re} for ground eigenstates of Hermitian QCP model for different system size LL. subfig(b): rescaled MxM^{x} vary with Γre\Gamma_{re} for different system size LL. Ω=1\Omega=1.

6 Conclusion

We have studied the phase transition in non-Hermitian QCP model. We have determined the critical exponents β\beta, γ\gamma which may indicate that the phase transition in non-Hermitian QCP model belongs to new universality class. Our results can help people to understand the property of non-Hermitian many-body system. Moreover, our results can stimulate more study about the phase transition of non-Hermitian many-body system. As for outlook, the dynamics of non-Hermitian system will be interesting topic since non-unitary evolution is completely different from the unitary evolution of Hermitian model, like [33, 34]. Renormalization group can be used to reveal the difference and relation of phase transition between the Hermitian model and non-Hermitian model [35]. It may be feasible to utilize Rydberg atom[24, 36] to simulate the non-Hermitian QCP model in our work to observe the continuous phase transition experimentally even for simple case of two spins.

7 Acknowledgements.

We gratefully thank Profs.Rosario Fazio and Stefano Chesi for their inspiring discussions and suggestions. W.B.H. acknowledges support from NSAF U1930402. J.J. acknowledges support from the National Natural Science Foundation of China (NSFC) via Grant No. 11975064. F.I. acknowledges the financial support of the Brazilian funding agencies National Council for Scientific and Technological Development-CNPq(Grant No. 308205/2019 − 7) and FAPERJ (Grant No. E-26/211.318/2019 and E-26/201.365/2022). H.Q. Lin acknowledges financial support from NSAF U1930402 and NSFC 12088101 and computational resources from the Beijing Computational Science Research Center.

8 Data availability

The data that support the findings of this study are available upon reasonable request from the authors.

Appendix A The notations and observables of non-Hermitian QCP

In this part, we introduce the notations used in main text and show more supplementary results.

Energy gap. We define the energy gap as following,

Δ=minn0|EnE0|.\Delta=\min_{n\neq 0}|E_{n}-E_{0}|. (21)

In Fig.9, the energy gap for no-Hermitian Hamiltonian vary with dissipation strength for L=10L=10, which indicates the gap closing at critical point.

Observables. Generally, we use right eigenstate of ground state to compute the observables:

O=ψR|O^|ψR.O=\langle\psi_{R}|\hat{O}|\psi_{R}\rangle. (22)

such as, number of spin-up

nup=ψR|kσ^+kσ^k|ψR.n_{\rm up}=\langle\psi_{R}|\sum_{k}\hat{\sigma}_{+}^{k}\hat{\sigma}_{-}^{k}|\psi_{R}\rangle. (23)

In this way, the observables and susceptibility are always real which is conformal to experimental detection. We can also use the left and right eigenstates of ground state to define the observable

OLR=ψL|O^|ψR.O_{LR}=\langle\psi_{L}|\hat{O}|\psi_{R}\rangle. (24)

Such as, magnetization Mα=ψR/L|kσ^αk/2|ψRM^{\alpha}=\langle\psi_{R/L}|\sum_{k}\hat{\sigma}_{\alpha}^{k}/2|\psi_{R}\rangle for α=x,y,z\alpha=x,y,z.

We denote the susceptibility computed by two formulas (22) and (24) as χ\chi and χLR\chi_{LR} respectively. We think that χ\chi and χLR\chi_{LR} both have the same function to characterize the property of phase transitions, see Fig.10. Near critical point, χ\chi is very close to the real part of χLR\chi_{LR}.

In Fig.11, we show susceptibility χ\chi vary with dissipation strength for different system size. The singular point help us determine the critical points as shown in Tabs. 1.2.

In Fig.12, we show the extrapolation of the critical points Γc(L)\Gamma_{c}(L) and the system size LL. According to numerical results, the critical points of thermodynamic limit LL\rightarrow\infty is Γc13.845\Gamma_{c}\sim 13.845.

Refer to caption
Figure 9: The energy gap Δ\Delta vary with Γ\Gamma for ground state L=10L=10, Ω=1\Omega=1.
Refer to caption
Figure 10: subfig(a):The susceptibility vary with Γ\Gamma for right ground eigenstates of non-Hermitian QCP model. subfig(b):The susceptibility vary with Γ\Gamma for right and left ground eigenstates of non-Hermitian QCP model. L=10L=10, Ω=1\Omega=1.
Refer to caption
Figure 11: The susceptibility vary with Γ\Gamma for ground eigenstates for different LL, Ω=1\Omega=1. The black dash lines indicate the critical points Γc(L)\Gamma_{c}(L) of each spin number, which are 13.4388,13.6949,13.770,13.801,13.816813.4388,13.6949,13.770,13.801,13.8168. We assume susceptibility satisfy scaling law χ1/(ΓΓc)γ\chi\sim 1/(\Gamma-\Gamma_{c})^{\gamma}. By using the right data of Γc(L)\Gamma_{c}(L) which are larger than the critical point of each cluster size, the critical exponents of each cluster can be extracted.

Correlation. As seeing Fig.13, the correlation function vary with position nn for periodic(left panel) and open(right panel) boundary condition.

Refer to caption
Figure 12: The extrapolation of critical points Γc(L)\Gamma_{c}(L) of order parameter MxM^{x} for system size up to L=16L=16. We extract the true critical point Γc13.845\Gamma_{c}\sim 13.845.

Appendix B non-Hermitian case of L=2L=2

We look at the particular and simpler case of L=2L=2 spins, which can provide theoretical information about phase transition. It is easy to explicitly write matrix of the effective Hamiltonian

Heff=(iΓΩΩ0ΩiΓ/200Ω0iΓ/200000).H_{\rm eff}=\left(\begin{array}[]{cccc}-i\Gamma&\Omega&\Omega&0\\ \Omega&-i\Gamma/2&0&0\\ \Omega&0&-i\Gamma/2&0\\ 0&0&0&0\\ \end{array}\right). (25)

The eigenvalues are given by

E1=0(trivial),\displaystyle E_{1}=0\quad(\rm trivial),
E2=iΓ/2,\displaystyle E_{2}=-i\Gamma/2,
E3,4=i3Γ4±1432Ω2Γ2.\displaystyle E_{3,4}=\frac{-i3\Gamma}{4}\pm\frac{1}{4}\sqrt{32\Omega^{2}-\Gamma^{2}}.

Here, we only give out right eigenstates |ψRi|\psi_{R}^{i}\rangle since we use right eigenstates to compute the observables

|ψR1\displaystyle|\psi_{R}^{1}\rangle =\displaystyle= (0,0,0,1)T,\displaystyle\left(0,0,0,1\right)^{T},
|ψR2\displaystyle|\psi_{R}^{2}\rangle =\displaystyle= (0,1,1,0)T,\displaystyle\left(0,1,-1,0\right)^{T}, (26)
|ψR3,4\displaystyle|\psi_{R}^{3,4}\rangle =\displaystyle= 12Ω2+Γ2+|λ|2+2ΓIm(λ)\displaystyle\frac{1}{\sqrt{2\Omega^{2}+\Gamma^{2}+|\lambda|^{2}+2\Gamma Im(\lambda)}}
(2Ω,(λ+iΓ)/2,(λ+iΓ)/2,0)T.\displaystyle\left(\sqrt{2}\Omega,(\lambda+i\Gamma)/\sqrt{2},(\lambda+i\Gamma)/\sqrt{2},0\right)^{T}.

where, for last two wave functions, we remark that eigenvalue λ\lambda take E3,4E_{3,4}. The exceptional point(EP) is located at

Γc=32Ω.\Gamma_{c}=\sqrt{32}\Omega. (28)

When the dissipation Γ\Gamma exceed the Γc\Gamma_{c}, all non-trivial eigenvalues EE become the purely imaginary. Meanwhile, the ground state is |ψR4|\psi_{R}^{4}\rangle since E4E_{4} has minimum real part.

The order parameter: Mx=ψR4|σx|ψR4M^{x}=\langle\psi_{R}^{4}|\sigma^{x}|\psi_{R}^{4}\rangle, where σx=kσxk\sigma^{x}=\sum_{k}\sigma^{k}_{x} can be written as matrix form

σx=(0110100110010110).\sigma^{x}=\left(\begin{array}[]{cccc}0&1&1&0\\ 1&0&0&1\\ 1&0&0&1\\ 0&1&1&0\\ \end{array}\right). (29)

We obtain the results of MxM^{x}

Mx=Ω32Ω2Γ22Ω2+Γ2+|λ|2+2ΓIm(λ).M^{x}=\frac{-\Omega\sqrt{32\Omega^{2}-\Gamma^{2}}}{2\Omega^{2}+\Gamma^{2}+|\lambda|^{2}+2\Gamma Im(\lambda)}. (30)

When dissipation tends to exceptional point |ΓΓc|0|\Gamma-\Gamma_{c}|\rightarrow 0, the order parameter can be written as Mx2ΓcΓcΓΓcΓM^{x}\sim\sqrt{2\Gamma_{c}}\sqrt{\Gamma_{c}-\Gamma}\sim\sqrt{\Gamma_{c}-\Gamma}. Such that the critical exponent β=1/2\beta=1/2

Refer to caption
Figure 13: Correlation function for periodic(left) and open(right) boundary. L=12L=12. The correlation length for Γ=14.5\Gamma=14.5,Γ=15.0\Gamma=15.0 are 0.58790.5879,0.53040.5304.

Appendix C Influence of perturbation to critical exponent

Here, we added imaginary random potential perturbation zz-direction with Hamiltonian,which can keep energy change from complex to imaginary

H^=ΩkL(σ^xkσ^nk+1+σ^nkσ^xk+1)i2Γk=1Lσ^+kσ^k+ik=1Lhkσ^+kσ^k,\hat{H}=\Omega\sum_{k}^{L}\left(\hat{\sigma}_{x}^{k}\hat{\sigma}_{n}^{k+1}+\hat{\sigma}_{n}^{k}\hat{\sigma}_{x}^{k+1}\right)-\frac{i}{2}\Gamma\sum_{k=1}^{L}\hat{\sigma}_{+}^{k}\hat{\sigma}_{-}^{k}+i\sum_{k=1}^{L}h_{k}\hat{\sigma}_{+}^{k}\hat{\sigma}_{-}^{k}, (31)

where random disorder hk[w/2,w/2]h_{k}\in[-w/2,w/2] and sampling number NrandNrand. We computed the energy and order parameter MxM^{x} of ground state of of each sampling as in fig. 14, finally averaged the results of all sampling in fig.15 as

Mx=1Nrandn=1Nrandψ0(w)n|M^x|ψ0(w)n.M^{x}=\frac{1}{Nrand}\sum_{n=1}^{Nrand}\langle\psi_{0}(w)_{n}|\hat{M}^{x}|\psi_{0}(w)_{n}\rangle. (32)

The results of one time sampling in fig.14, there is exceptional point and critical exponent is close to 0.50.5. After averaging the results over all sampling, order parameter also change from finite value to zeros. Exceptional point is easy to be destroyed by random potential perturbation, see the upper subplots of fig.15. The critical exponent slightly deviates from 0.50.5 of fig.15(lower subplots) with uncertainty.

Refer to caption
Figure 14: The results of one time sampling. The energy(upper subplots) and the order parameter MxM^{x} of w=0.1w=0.1 near critical point vary with dissipation(lower Left) and its logarithmic scale(lower Right). The critical exponent is extracted as β0.5118\beta\sim 0.5118. L=10,Ω=1L=10,\Omega=1.
Refer to caption
Figure 15: Non-Hermitian qcp model of Eq.31: The averaged energy(upper subplots) and the order parameter MxM^{x} of w=0.1w=0.1 vary with dissipation(lower Left) and its logarithmic scale(lower Right). The critical exponent is extracted as β0.5348±0.0399\beta\sim 0.5348\pm 0.0399. L=10,Ω=1,Nrand=500L=10,\Omega=1,Nrand=500.

We also consider the special case a two spins system with imaginary random potential, the perturbed Hamiltonian is given as follows,

H^=Ω(σ^x1σ^n2+σ^n1σ^x2)i2Γk=12σ^+kσ^k+i(h1σ^+1σ^1+h2σ^+2σ^2).\hat{H}=\Omega\left(\hat{\sigma}_{x}^{1}\hat{\sigma}_{n}^{2}+\hat{\sigma}_{n}^{1}\hat{\sigma}_{x}^{2}\right)-\frac{i}{2}\Gamma\sum_{k=1}^{2}\hat{\sigma}_{+}^{k}\hat{\sigma}_{-}^{k}+i(h_{1}\hat{\sigma}_{+}^{1}\hat{\sigma}_{-}^{1}+h_{2}\hat{\sigma}_{+}^{2}\hat{\sigma}_{-}^{2}). (33)

For convenience, we set Ω=1\Omega=1 as the rescaling unit of system’s parameter. The matrix of HH is given by

H=(i(γ1+γ2)1101iγ10010iγ200000),H=\left(\begin{array}[]{cccc}i(\gamma_{1}+\gamma_{2})&1&1&0\\ 1&i\gamma_{1}&0&0\\ 1&0&i\gamma_{2}&0\\ 0&0&0&0\\ \end{array}\right), (34)

here define γ1=h1Γ/2\gamma_{1}=h_{1}-\Gamma/2 and γ2=h2Γ/2\gamma_{2}=h_{2}-\Gamma/2. Apart from trivial eigenvalue E=0E=0, the characteristic equation of remained three eigenvalues as |EH|=0|E-H|=0 satisfy cubic equation

(Ei(γ1+γ2))(Eiγ1)(Eiγ2)(2Ei(γ1+γ2))=0\displaystyle(E-i(\gamma_{1}+\gamma_{2}))(E-i\gamma_{1})(E-i\gamma_{2})-(2E-i(\gamma_{1}+\gamma_{2}))=0 (35)
E32i(γ1+γ2)E[(γ1+γ2)2+γ1γ2+2]E\displaystyle E^{3}-2i(\gamma_{1}+\gamma_{2})E-[(\gamma_{1}+\gamma_{2})^{2}+\gamma_{1}\gamma_{2}+2]E
+i[(γ1+γ2)+γ1γ2(γ1+γ2)]=0\displaystyle+i[(\gamma_{1}+\gamma_{2})+\gamma_{1}\gamma_{2}(\gamma_{1}+\gamma_{2})]=0 .

Only for balanced perturbation h1=h2h_{1}=h_{2}, above Eq.(35) can reduce to quadratic equation. Usually random potentials are different that break translation symmetry, eigen-equation changes from square to cubic. The solution formula of cubic equation is too complicated to analysis. The order of characteristic equation is sensitive to the perturbation field.

Fig.16(a)(b) show the real and imaginary parts of the energy vary with dissipation for three sets of perturbation fields. There is tiny difference with the energy between the case without(blue dash line) and with(red solid line and cyan dash line) perturbation. Fig.16(c) shows the scaling fitting of energy coalescence. The critical exponents of two sets of perturbation slightly deviate from the results without perturbation. In order understand how perturbation influence the critical exponent, we computed the relation of critical exponent and perturbation field. Fig.17 show the critical point(a) and critical exponent(b) of energy coalescence vary with perturbation field difference |h1h2||h_{1}-h_{2}|. The critical exponents saturate to 0.490.49.

Refer to caption
Refer to caption
Figure 16: The real(a) and imaginary(b) part of energy. Blue lines: h1=h2=0h_{1}=h_{2}=0, red lines h1=0,h2=0.1h_{1}=0,h_{2}=-0.1 and cyan lines h1=0.2,h2=0.1h_{1}=0.2,h_{2}=0.1. L=2,Ω=1L=2,\Omega=1. (c). The critical exponents are respectively β[0.5004,4.817,0.5047]\beta\sim[0.5004,4.817,0.5047]. L=2,Ω=1L=2,\Omega=1.
Refer to caption
Figure 17: The scaling fitting. The critical point(a) and critical exponents β\beta (b) vary with field difference. The parameters h1=0,h2[0:0.1:1],L=2,Ω=1h_{1}=0,h_{2}\in-[0:0.1:1],L=2,\Omega=1. The errorbar indicate the error of numerical fitting.

Appendix D Hermitian cases of L=2L=2

It is easy to explicitly write the Hamiltonian of Eq.(19) for simple case L=2L=2

H=(ΓΩΩ0ΩΓ/200Ω0Γ/200000).H=\left(\begin{array}[]{cccc}-\Gamma&\Omega&\Omega&0\\ \Omega&-\Gamma/2&0&0\\ \Omega&0&-\Gamma/2&0\\ 0&0&0&0\\ \end{array}\right). (36)

The eigenvalues are given by

E1=0(trivial),\displaystyle E_{1}=0\quad(\rm trivial),
E2=Γ/2,\displaystyle E_{2}=-\Gamma/2,
E3,4=3Γ4±1432Ω2+Γ2.\displaystyle E_{3,4}=\frac{-3\Gamma}{4}\pm\frac{1}{4}\sqrt{32\Omega^{2}+\Gamma^{2}}.

If there is an exceptional point, 32Ω2+Γ2=32Ω2+Γre2Γim2+i2ΓreΓim=032\Omega^{2}+\Gamma^{2}=32\Omega^{2}+\Gamma_{re}^{2}-\Gamma_{im}^{2}+i2\Gamma_{re}\Gamma_{im}=0. We can solve it

32Ω2+Γre2Γim2=0,&ΓreΓim=0.32\Omega^{2}+\Gamma_{re}^{2}-\Gamma_{im}^{2}=0,\quad\&\quad\Gamma_{re}\Gamma_{im}=0. (37)

Only for Γre=0\Gamma_{re}=0 there is a reasonable solution, but recovers the results of Eq.(9). Through the above analysis, for general non-zero Γre\Gamma_{\rm re} and Γim\Gamma_{\rm im} there are no exceptional points of energy coalescence.

If Γ\Gamma is real value, the eigenvalues

E1=0(trivial),\displaystyle E_{1}=0\quad(\rm trivial),
E2=Γre/2,\displaystyle E_{2}=-\Gamma_{re}/2,
E3,4=3Γre4±1432Ω2+Γre2.\displaystyle E_{3,4}=\frac{-3\Gamma_{re}}{4}\pm\frac{1}{4}\sqrt{32\Omega^{2}+\Gamma_{re}^{2}}.

eigen-states are given as

|ψR1\displaystyle|\psi_{R}^{1}\rangle =\displaystyle= (0,0,0,1)T,\displaystyle\left(0,0,0,1\right)^{T},
|ψR2\displaystyle|\psi_{R}^{2}\rangle =\displaystyle= (0,1,1,0)T,\displaystyle\left(0,1,-1,0\right)^{T}, (38)
|ψR3,4\displaystyle|\psi_{R}^{3,4}\rangle =\displaystyle= 12Ω2+(E+Γre)2\displaystyle\frac{1}{\sqrt{2\Omega^{2}+(E+\Gamma_{\rm re})^{2}}} (39)
(2Ω,(E+Γre)/2,(E+Γre)/2,0)T.\displaystyle\left(\sqrt{2}\Omega,(E+\Gamma_{\rm re})/\sqrt{2},(E+\Gamma_{\rm re})/\sqrt{2},0\right)^{T}.

Where EE takes E3,4E_{3,4} for real Γ\Gamma. If Γ\Gamma is real and Γim=0,Γre<0\Gamma_{\rm im}=0,\,\Gamma_{\rm re}<0, let E1=E4E_{1}=E_{4} for the Hermitian model since E2>0,E3>0E_{2}>0,\,E_{3}>0. We obtain that

Γre2=4Ω2.\Gamma_{\rm re}^{2}=4\Omega^{2}. (40)

The solution is Γre=2Ω=Γc\Gamma_{\rm re}=-2\Omega=\Gamma_{c}, which is the energy level crossing point for the Hermitian model. Near critical point, E1<E4E_{1}<E_{4} for Γre<Γc\Gamma_{\rm re}<\Gamma_{c}, while E4<E1E_{4}<E_{1} for Γre>Γc\Gamma_{\rm re}>\Gamma_{c}.

The order parameter MxM^{x} of ground state can be given as

Mx(Γre<Γc)=ψR1|σx|ψR1=0,M^{x}(\Gamma_{\rm re}<\Gamma_{c})=\langle\psi_{R}^{1}|\sigma^{x}|\psi_{R}^{1}\rangle=0, (41)

and

Mx(Γre>Γc)=ψR4|σx|ψR4=2Ω(E+Γre)2Ω2+(E+Γre)2.M^{x}(\Gamma_{\rm re}>\Gamma_{c})=\langle\psi_{R}^{4}|\sigma^{x}|\psi_{R}^{4}\rangle=\frac{2\Omega(E+\Gamma_{\rm re})}{2\Omega^{2}+(E+\Gamma_{\rm re})^{2}}. (42)

which tends to 2ΩΓc/(2Ω2+Γc2)<02\Omega\Gamma_{c}/(2\Omega^{2}+\Gamma_{c}^{2})<0 for ΓreΓc+\Gamma_{\rm re}\rightarrow\Gamma_{c}^{+}, that the theoretical analysis agree with the results in Fig.8.

References

  • [1] Yuto Ashida, Zongping Gong, and Masahito Ueda, Non-Hermitian physics, Advances in Physics 69 249 (2020).
  • [2] Emil J. Bergholtz, Jan Carl Budich, and Flore K. Kunst, Rev. Mod. Phys. 93, 015005(2021).
  • [3] N. Hatano and D. R. Nelson, Phys. Rev. Lett. 77, 570 (1996).
  • [4] Shunyu Yao and Zhong Wang, Phys. Rev. Lett. 121, 086803(2018).
  • [5] Robin Schafer, J.C.Budich, and David J. Luitz,Symmetry protected exceptional points of interacting fermions,Phys. Rev. Research 4,033181(2020).
  • [6] Linhu Li, Ching Hua Lee, Sen Mu and Jiangbin Gong, Nat.Comm.11,5491 (2020).
  • [7] L. Xiao, T. Deng, K. Wang, G. Zhu, Z. Wang, W. Yi, and P. Xue, Non-Hermitian bulk-boundary correspondence in quantum dynamics, Nat. Phys. 16, 761 (2020).
  • [8] Clara C. Wanjura, Matteo Brunelli,and Andreas Nunnenkamp Topological framework for directional amplification in driven-dissipative cavity arrays, Nat. Comm. 11, 3149 (2020).
  • [9] Clara C. Wanjura, Matteo Brunelli, and Andreas Nunnenkamp Topological framework for directional amplification in driven-dissipative cavity arrays, Phys.Rev.Lett. 127,213601(2021).
  • [10] Diego Porras and Samuel Fernandez-Lorenzo,Topological Amplification in Photonic Lattices, Phys. Rev. Lett. 122, 143901(2019).
  • [11] Tomas Ramos, Juan Jose Garcia-Ripoll, and Diego Porras, Topological input-output theory for directional amplification, Phys. Rev. A 103, 033513(2021).
  • [12] Shunyu Yao, Fei Song, and Zhong Wang, Non-Hermitian Chern Bands, Phys. Rev. Lett.121,136802(2018).
  • [13] Kazuki Yokomizo and Shuichi Murakami, Non-Bloch Band Theory of Non-Hermitian Systems, Phys. Rev. Lett. 123, 066404(2019).
  • [14] Norifumi Matsumoto, Kohei Kawabata, Yuto Ashida, Shunsuke Furukawa, and Masahito Ueda, Continuous Phase Transition without Gap Closing in Non-Hermitian Quantum Many-Body Systems, Phys. Rev. Lett. 125, 260601(2020).
  • [15] Ryusuke Hamazaki, Kohei Kawabata, and Masahito Ueda, Phys. Rev. Lett. 123, 090603(2019).
  • [16] H. P. Breuer, and F. Petruccione, Theory of Open Quantum Systems, Oxford University Press, Oxford, (2002).
  • [17] Andrew.J. Daley Quantum trajectories and open many-body quantum systems, Adv. Phys. 63, 77 (2014).
  • [18] Shengshi Pang and Todd.A.Brun, Improving the Precision of Weak Measurements by Postselection Measurement, Phys.Rev.Lett. 115, 120401(2015).
  • [19] W D Heiss The physics of exceptional points, J. Phys. A: Math. Theor. 45, 444016(2012).
  • [20] Tony E. Lee and Ching-Kit Chan, Heralded Magnetism in Non-Hermitian Atomic Systems, Phys.Rev.X.4, 041001(2014).
  • [21] Tony E. Lee, Florentin Reiter, and Nimrod Moiseyev,Entanglement and Spin Squeezing in Non-Hermitian Phase Transitions, Phys. Rev. Lett. 113, 250401(2014).
  • [22] Federico Carollo, Edward Gillman, Hendrik Weimer, and Igor Lesanovsky,Critical Behavior of the Quantum Contact Process in One Dimension, Phys. Rev. Lett. 123, 100604 (2019).
  • [23] T. M. Wintermantel, M. Buchhold, S. Shevate, M. Morgado, Y. Wang, G. Lochead, S. Diehl, and S. Whitlock,Epidemic growth and Griffiths effects on an emergent network of excited atoms Nat Commun 12 103 (2021).
  • [24] Ricardo Gutiérrez, Cristiano Simonelli, Matteo Archimi, Francesco Castellucci, Ennio Arimondo, Donatella Ciampini, Matteo Marcuzzi, Igor Lesanovsky, and Oliver Morsch, Phys. Rev. A 96, 041602(R) (2017).
  • [25] Appendix for more details.
  • [26] S. Sachdev, Quantum Phase Transitions (Cambridge University Press, Cambridge, England, 2001).
  • [27] Ramy El-Ganainy, Konstantinos G. Makris, Mercedeh Khajavikhan, Ziad H. Musslimani, Stefan Rotter and Demetrios N. Christodoulides, Non-Hermitian physics and PT symmetry, Nat.Phys.14, 11–19 (2018).
  • [28] S.K. Özdemir, S. Rotter, F. Nori and L. Yang , Parity–time symmetry and exceptional points in photonics, Nature Materials. 18, 783–798 (2019).
  • [29] Y. Yang, Yi-Pu Wang, J. W. Rao, Y. S. Gui, B. M. Yao, W. Lu, and C.-M. Hu, Unconventional Singularity in Anti-Parity-Time Symmetric Cavity Magnonics, Phys. Rev. Lett. 125, 147202(2020).
  • [30] Weitao Chen, Liangtao Peng, Hantao Lu, Xiancong Lu, Phys. Rev. B 105, 075126(2022).
  • [31] Bo-Bo Wei and Liang Jin, Universal Critical Behaviours in Non-Hermitian Phase Transitions, Scientific Reports. 7,7165 (2017) .
  • [32] Cem Yuce and Hamidreza Ramezani, Robust exceptional points in disordered systems, 2019 EPL 126 17002.
  • [33] Taiki Haga, Masaya Nakagawa, Ryusuke Hamazaki, and Masahito Ueda,Liouvillian Skin Effect: Slowing Down of Relaxation Processes without Gap Closing, Phys. Rev. Lett. 127, 070402(2021).
  • [34] Takahiro Orito, Ken-Ichiro Imura,Unusual diffusion and entanglement dynamics in non-Hermitian disordered many-body systems,Phys. Rev. B 105, 024303(2022) .
  • [35] Kohei Kawabata1, and Shinsei Ryu,Nonunitary Scaling Theory of Non-Hermitian Localization, Phys.Rev.Lett.126,166801(2021).
  • [36] A. Browaeys and T. Lahaye, Many-body physics with individually controlled Rydberg atoms, Nat. Phys. 16, 132 (2020)