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Dynamic generation of nonequilibrium superconducting states in Kitaev chain

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

A non-equilibrium state shares macroscopic properties, such as conductivity and superconductivity, with a static state when the two states exhibit an identical average value of an observable over a period. We studied the quench dynamics of a Kitaev chain on the basis of two types of order parameters associated with two channels of pairing: local pairing in real space and Bardeen-Cooper-Schrieffer (BCS)-like pairing in momentum space. On the basis of the exact solution, we found that the two order parameters were identical for the ground state, which indicated a balance between the two pairing channels and would help determine the quantum phase diagram. However, for a non-equilibrium state obtained through time evolution from an initially prepared vacuum state, the two parameters varied; however, both parameters could still help determine the phase diagram. In the region of nontrivial topological phases, non-equilibrium states favored BCS-like pairing. This paper presents an alternative approach to dynamically generate a superconducting state from a trivial empty state and illuminates the pairing mechanism.

I   Introduction

The topic of non-equilibrium phenomena in quantum many-body systems is fundamental and compelling in condensed matter physics. In conventional theory, quantum phase transitions occur at zero temperature, and a phase diagram refers, in particular, to the ground state of a system. However, it is obviously that the ground state is intimately related to the excited states for a certain class of systems since they all stem from a same time-independent Hamiltonian. For instance, for a Hamiltonian written in pseudospin form k𝐁k𝐬k\sum_{k}\mathbf{B}_{k}\mathbf{\cdot s}_{k}, the ground state is determined by the field distribution 𝐁k/|𝐁k|\mathbf{B}_{k}/\left|\mathbf{B}_{k}\right| ZG , which can be extracted from any eigenstates in the tensor product form. In this sense, non-equilibrium phenomena within the prethermalization regime can probably reflect the phase diagram from an alternative aspect. A well-known probe of many-body quantum dynamics is quantum quench, in which a many-body system is initially prepared in a state that is typically the ground state of some simple Hamiltonian and subsequently evolves with a different Hamiltonian. In a conventional framework, the properties of prequench and postquench Hamiltonians are extracted from the evolved states instead of the ground state. The use of nonequilibrium many-body dynamics presents an alternative approach for accessing a new exotic quantum state with an energy level considerably different from that of the ground state Choi ; Else ; Khemani ; Lindner ; Kaneko ; Tindall ; YXMPRA ; ZXZPRB2 ; TK ; JT1 ; JT2 . Advancements in atomic physics, quantum optics, and nanoscience have allowed the development of artificial systems with high accuracy Jochim ; Greiner . Thus, theoretical models can be simulated and realized experimentally. Direct simulation of a simple model is useful not only for solving key challenges in condensed matter physics but also in the engineering design of quantum devices. Notably, the availability of an experimentally controllable fermion system provides an unprecedented opportunity to explore nonequilibrium dynamics in interacting many-body systems.

In addition, it has recently been established that experiments with various materials and excitation conditions have witnessed phenomena with no equilibrium analog or accessibility of chemical substitution, including superconducting-like phases AC ; DF ; MM ; TS , charge density waves (CDW) LS ; HM ; AK and excitonic condensation YM . Therefore, how to stabilize a system in a non-equilibrium superconducting phase with a long lifetime is a great challenge and is at the forefront of current research. Among various non-equilibrium protocols, the generation of the η\eta-pairing-like state plays a pivotal role in which the existence of doublon and holes facilitate the superconductivity SK ; TK ; JT ; FP ; RF1 ; RF2 ; SE ; JL ; TK2 ; ZXZPRB2 ; ZXZPRB3 ; JT1 ; JT2 .

In the present paper, we report our theoretical investigation of nonequilibrium dynamics in a paradigmatic quantum many-body model—the Kitaev chain. Comparing to the previous works on the Hubbard model, the intial state is an easily prepared state YXMPRA and quenched Hamiltonian is time-independent with parameters covering rich phase diagram in the present work. The Kitaev chain is a lattice model of a p-wave superconducting wire, which realizes Majorana zero modes at the ends of the chain Kitaev . Unpaired Majorana modes have been exponentially localized at the ends of open Kitaev chains Sarma ; Stern ; Alicea . The primary feature of this model originates from the pairing term, which violates the conservation of the fermion number but preserves its parity, leading to a superconducting state. In general, most studies on this model have centered on the ground state or the dynamical quantum phase transitions related to the ground state MH ; LZ . The strength of the pairing interactions has an important role in giving rise to a gapped superconducting state. However, knowledge regarding the pair in each quantum phase remains limited. Specifically, the nearest-neighbor (NN) pair creation (annihilation) term is subtle for the formation of a pair. It results in an NN pair in real space. By contrast, the Hamiltonian in k-space indicates that it also contributes to Bardeen-Cooper-Schrieffer (BCS)-like pairing in momentum space, which involves two particles with opposite momentum. In addition, distinct features originate from the pair term in not only statics but also dynamics. To determine the features of a given state, we introduced two types of order parameters associated with two channels of pairing: local pairing in real space and BCS-like pairing in momentum space. On the basis of the exact solution, we found that the two order parameters were identical for the ground state and could help determine the quantum phase diagram. This revealed an unprecedented feature of the ground state that helps balance between two types of pairing channels. The primary aim of this study was to obtain pertinent information regarding the nonequilibrium state. In this study, acquisition of a vacuum state by the quench process, in which a prequench Hamiltonian has infinite chemical potential, was considered to be the ground state. We investigated evolved states under the postquench Hamiltonian with parameters covering the entire region and found two types of order parameters that were different but could help determine the quantum phase diagram. Our results yield two key findings: a superconducting state can be dynamically generated from a trivial state, and the difference between two types of order parameters for a nonequilibrium state indicates the generation of various superconducting states from the ground state, thus expanding the variety of the state of matter that is associated with different channels of pairing.

This paper is organized as follows. In Sec. II, we present the model and introduce two types of order parameters to investigate the feature of superconducting state. In Subsecs. II.1 and II.2, we calculate the order parameters in kk space and real space for the ground state, respectively. In Sec. III, we investigate the features of dynamic behavior of the system. Finally, we give a summary and discussion in Section IV. Some details of the derivations are given in Appendix.

Refer to caption
Figure 1: (a) Phase diagram of the Hamiltonian in Eq. (1) on the μΔ\mu-\Delta plane. The sky blue, green and pink regions correspond to the winding numbers 1,1, 0 and 1-1, respectively. Red lines indicate phase-transition lines. The four colored dots a-d represent the typical sets of parameters at which the order parameters, as shown in Fig. 3. (b) and (c), present the profiles of ζg\zeta_{g} defined in Eq. (10) at the lines Δ=0.6\Delta=0.6 and μ=0.6\mu=0.6, respectively. They indicate that ζg\zeta_{g} is independent of μ\mu in topologically non-trivial regions and is non-analytic at the phase boundary. The other parameters are N=2000N=2000 and J=1J=1.
Refer to caption
Figure 2: Three-dimensional plots of the (a) order parameter of the ground state ζg\zeta_{g} obtained from Eq. (10); (b) partial derivative of ζg\zeta_{g} with respect to μ,\mu, μζg;\partial_{\mu}\zeta_{g}; and (c) partial derivative of ζg\zeta_{g} with respect to Δ,\Delta, Δζg,\partial_{\Delta}\zeta_{g}, as the functions of μ\mu and Δ\Delta for case N=4000N=4000. The results indicate that second-order quantum phase transitions occur at phase boundaries. Therefore, the analytical behavior of the order parameter can identify the phase diagram. The other parameter is J=1J=1.
Refer to caption
Figure 3: (a) plots of the time-averaged analytical expressions for (1) ζ\zeta and (2) η\eta obtained from Eqs. (35) and (33). The four colored dots represent the dots a-d in Fig. 1(a). (b) Profiles of (1) ζ(t)\zeta(t) and (2) η(t)\eta(t) obtained from Eqs. (22) and (23) as the function of time for case N=4000N=4000 with four sets of parameters (μ(\mu and Δ)\Delta) indicated by dots a-d as shown in Fig. 1(a). The colored arrows are the stable values ζ(t)\zeta(t) and η(t)\eta(t) tend to. The colored dots represent ζ¯\overline{\zeta} and η¯\overline{\eta} obtained from Eqs. (35) and (33) (c) Plots of dispersion E=±εkE=\pm\varepsilon_{k} and DOS D(E)D(E) for the systems with the same sets of parameters in (b1) and (b2) with the same colors. We can see that both ζ(t)\zeta(t) and η(t)\eta(t) exhibit damping oscillations around their stable values. The frequency and decay rate of amplitude are associated with the energy difference δE\delta E between the highest peaks and maximum of DOS. The amplitude decays slower if DOS has a higher peak. A larger value of δE\delta E indicates a higher oscillation frequency. The other parameter is J=1J=1.
Refer to caption
Figure 4: Plots of ln[δη(t)]\ln[\delta\eta(t)] as functions of ln(t)\ln(t) with four sets of parameters (μ\mu and Δ\Delta) indicated by dots a-d as shown in Fig. 1(a) . δη(t)\delta\eta(t) is defined in Eq. (27). The slope of the green line in (a) and (b) is 0.5 while in (c) and (d) is 1.
Refer to caption
Figure 5: Three-dimensional plots of the average order parameters (a) η¯\overline{\eta} and (b) ζ¯\overline{\zeta} obtained from Eqs. (29) and (30) as the function of μ\mu and Δ\Delta for case N=4000N=4000 in the first quadrant. The patterns are not dependent on the quadrant. The two quantities vary, but both can identify the phase boundary at μ=1\mu=1 and Δ=0\Delta=0 (|μ|<1)(\left|\mu\right|<1) (also refer to Fig. 6). The other parameter is J=1J=1.
Refer to caption
Figure 6: Three-dimensional plots of (a) μη¯\partial_{\mu}\overline{\eta}, (b) μζ¯\partial_{\mu}\overline{\zeta}, (c) Δη¯\partial_{\Delta}\overline{\eta} and (d) Δζ¯\partial_{\Delta}\overline{\zeta} as the function of μ\mu and Δ\Delta for case N=4000N=4000 in the first quadrant; the forms of η¯\overline{\eta} and ζ¯\overline{\zeta} are obtained from Eqs. (29) and (30). The aforementioned four quantities can identify the phase boundary at μ=1\mu=1 and Δ=0\Delta=0 (|μ|<1)(\left|\mu\right|<1). The other parameter is J=1J=1.
Refer to caption
Figure 7: Profiles of ζ¯\overline{\zeta} and η¯\overline{\eta} obtained from Eqs. (29) and (30) at lines (a1) Δ=0.6\Delta=0.6 and (b1) μ=0.6\mu=0.6. The corresponding partial derivatives of η¯\overline{\eta} and ζ¯\overline{\zeta} (a2) μη¯\partial_{\mu}\overline{\eta}, (a3) μζ¯\partial_{\mu}\overline{\zeta}, (b2) Δη¯\partial_{\Delta}\overline{\eta} and (b3) Δζ¯\partial_{\Delta}\overline{\zeta} for finite sizes N=100N=100, 200200, 400400 and 1000,1000, respectively. In (a2) and (a3), the values of μη¯(μ=1)\partial_{\mu}\overline{\eta}\left(\mu=1\right) and μζ¯(μ=1+)\partial_{\mu}\overline{\zeta}\left(\mu=1^{+}\right) increase rapidly with increasing NN, indicating the divergence of μη¯\partial_{\mu}\overline{\eta} and μζ¯\partial_{\mu}\overline{\zeta} at phase boundary |μ|=1\left|\mu\right|=1 in the large NN limit. (b2) and (b3) indicate that Δη¯\partial_{\Delta}\overline{\eta} is discontinuous and Δζ¯\partial_{\Delta}\overline{\zeta} is divergent at the phase boundary |Δ|=0\left|\Delta\right|=0 in the large NN limit. The other parameter used for numerical calculations is J=1J=1.

II Model and order parameters

We consider the following fermionic Hamiltonian on a lattice of length NN

H\displaystyle H =\displaystyle= j=1N[Jcjcj+1Δcjcj+1+H.c.\displaystyle\sum\limits_{j=1}^{N}[-Jc_{j}^{{\dagger}}c_{j+1}-\Delta c_{j}^{{\dagger}}c_{j+1}^{{\dagger}}+\mathrm{H.c.} (1)
+μ(2nj1)],\displaystyle+\mu\left(2n_{j}-1\right)],

where cjc_{j}^{{\dagger}} (cj)(c_{j}) is a fermionic creation (annihilation) operator on site jj, nj=cjcjn_{j}=c_{j}^{{\dagger}}c_{j}, JJ the tunneling rate, μ\mu the chemical potential, and Δ\Delta the strength of the pp-wave pair creation (annihilation). cN+1=c1c_{N+1}=c_{1} is defined for periodic boundary condition. The Hamiltonian in Eq. (1) has a rich phase diagram that describes a spin-polarized pp-wave superconductor in one dimension. This system has a topological phase in which a zero- energy Majorana mode is located at each end of a long chain. It is the fermionized version of the well-known one-dimensional transverse-field Ising model Pfeuty , which is one of the simplest solvable models that exhibits quantum criticality and phase transition with spontaneous symmetry breaking SachdevBook .Several studies have been conducted with a focus on long-range Kitaev chains, in which the superconducting pairing term decays with distance as a power law TPCHOY ; AGG ; DV1 ; DV2 ; OV ; LL ; UB .

This study centered on the dynamics of a system with NN superconducting pairing term, which warrants further-systematic studies, such as those on long-range correlations. The Hamiltonian can be exactly solved based on Fourier transformation (see Appendix A). The ground-state wave function can be expressed as

|G=π>k>0|φke,\left|\text{{G}}\right\rangle=\prod_{\pi>k>0}\left|\varphi_{k\mathrm{e}}^{-}\right\rangle, (2)

with groundstate energy

Eg=π>k>0εk.E_{\mathrm{g}}=-\sum_{\pi>k>0}\varepsilon_{k}. (3)

Accordingly, the phase diagram can be obtained from |G\left|\text{{G}}\right\rangle and EgE_{\mathrm{g}}, with the phase boundaries

μ=±1, and Δ=0, for |μ|<1.\mu=\pm 1\text{, and }\Delta=0\text{, for }\left|\mu\right|<1. (4)

These lines separate four regions in the parameter space, representing different phases with winding numbers CKC ; NL N=0N=0, and ±1\pm 1, respectively. Fig. 1(a) depicts the phase diagram. The phase diagram indicates that the chemical potential μ\mu has a subtle role in the ground state. It restricts the value of |μ|\left|\mu\right| to maintain the non-trivial phases. The might be because the sufficiently large |μ|\left|\mu\right| suppresses pair creation. Thus the number of pairs is higher in nontrivial phases than in trivial phases which leads to the following two questions. First, how to quantify the amount of pairs in each phase? Second, what are the features of the pairing in real or momentum space. The answers are the main part of our goals in this work.

To answer the questions, we explore the features of a superconducting state by introducing two types of order parameters BP . Two operators η^l\widehat{\eta}_{l} and ζ^k\widehat{\zeta}_{k} characterize pairing channels in real space with

η^l=2πodd r>01r(clcl+rclcl+r),\widehat{\eta}_{l}=\frac{2}{\pi}\sum\limits_{\text{odd }r>0}\frac{1}{r}\left(c_{l}c_{l+r}-c_{l}^{{\dagger}}c_{l+r}^{{\dagger}}\right), (5)

and kk space with

ζ^k=i(ckckckck).\widehat{\zeta}_{k}=i\left(c_{-k}c_{k}-c_{k}^{{\dagger}}c_{-k}^{{\dagger}}\right). (6)

For a given state |ψ\left|\psi\right\rangle, the quantity |ψ|η^l|ψ||\left\langle\psi\right|\widehat{\eta}_{l}\left|\psi\right\rangle| helps measure the rate of transition for a pair located around the llth site, whereas |ψ|ζ^k|ψ||\left\langle\psi\right|\widehat{\zeta}_{k}\left|\psi\right\rangle| helps measure the rate of transition for a pair at the kk channel. The corresponding order parameters are defined on the basis of the average magnitude over all channels, as expressed in

η=1Nl|ψ|η^l|ψ|,\eta=\frac{1}{N}\sum_{l}|\left\langle\psi\right|\widehat{\eta}_{l}\left|\psi\right\rangle|, (7)

and

ζ=1Nπ>k>0|ψ|ζ^k|ψ|.\zeta=\frac{1}{N}\sum_{\pi>k>0}|\left\langle\psi\right|\widehat{\zeta}_{k}\left|\psi\right\rangle|. (8)

Nonzero η\eta and ζ\zeta indicate that the state |ψ\left|\psi\right\rangle is a superconducting state. In general, η\eta and ζ\zeta have different values for a given state. In the following subsections, we describe the analytical expressions of η\eta and ζ\zeta for the ground states of the system in different regions and their behaviors at phase boundaries.

II.1 Pairing in kk space

The order parameter of the ground state is expressed as

ζg=1Nπ>k>0|G|ζ^k|G|=1Nπ>k>0|φke|ζ^k|φke|.\zeta_{\mathrm{g}}=\frac{1}{N}\sum_{\pi>k>0}\left|\left\langle\text{{G}}\right|\widehat{\zeta}_{k}\left|\text{{G}}\right\rangle\right|=\frac{1}{N}\sum_{\pi>k>0}\left|\left\langle\varphi_{k\mathrm{e}}^{-}\right|\widehat{\zeta}_{k}\left|\varphi_{k\mathrm{e}}^{-}\right\rangle\right|. (9)

Direct derivation shows that the order parameter is

ζg=2|Δ|Nπ>k>0|sinkεk|=|Δ|π0πsinkεkdk\zeta_{\mathrm{g}}=\frac{2\left|\Delta\right|}{N}\sum_{\pi>k>0}\left|\frac{\sin k}{\varepsilon_{k}}\right|=\frac{\left|\Delta\right|}{\pi}\int_{0}^{\pi}\frac{\sin k}{\varepsilon_{k}}\mathrm{d}k (10)

in the large NN limit, which can be expressed explicitly in the following regions. (i) When |μ|>1\left|\mu\right|>1, the order parameter is

ζg=|Δ|2π1Δ2ln||μ|+1Δ2|μ|1Δ2|\zeta_{\mathrm{g}}=\frac{\left|\Delta\right|}{2\pi\sqrt{1-\Delta^{2}}}\ln\left|\frac{\left|\mu\right|+\sqrt{1-\Delta^{2}}}{\left|\mu\right|-\sqrt{1-\Delta^{2}}}\right| (11)

for |Δ|1\left|\Delta\right|\neq 1 but (|μ|π)1\left(\left|\mu\right|\pi\right)^{-1} at |Δ|=1\left|\Delta\right|=1. (ii) When |μ|1\left|\mu\right|\leqslant 1, the order parameter is

ζg=|Δ|2π1Δ2ln|1+1Δ211Δ2|\zeta_{\mathrm{g}}=\frac{\left|\Delta\right|}{2\pi\sqrt{1-\Delta^{2}}}\ln\left|\frac{1+\sqrt{1-\Delta^{2}}}{1-\sqrt{1-\Delta^{2}}}\right| (12)

for |Δ|1\left|\Delta\right|\neq 1 but π1\pi^{-1} at |Δ|=1\left|\Delta\right|=1. This suggests that when |μ|1,\left|\mu\right|\leqslant 1, ζg\zeta_{\mathrm{g}} is not dependent on μ\mu. Unexpectedly, the number of pairs is determined using only the parameter Δ\Delta in non-trivial phases. The underlying mechanism is an open question in this work. By contrast, when |μ|>1\left|\mu\right|>1ζg\zeta_{\mathrm{g}} decays as |μ|\left|\mu\right| increases. Specifically, it decays linearly with |μ|1\left|\mu\right|-1 for small |μ|1\left|\mu\right|-1 and as |μ|1\left|\mu\right|^{-1} for large |μ|\left|\mu\right|.

Nevertheless, we can only understand this result mathematically from an example in classical Electromagnetics. We consider a charged conducting ellipsoid with the surface equations

(xμ)2+y2+z2Δ2=1.(x-\mu)^{2}+\frac{y^{2}+z^{2}}{\Delta^{2}}=1. (13)

The total charge is Q=4|Δ|Q=4\left|\Delta\right|. Then surface charge density distribution along the xx axis is

σ=1π|Δ|[(xμ)2+R2Δ4]12.\sigma=\frac{1}{\pi\left|\Delta\right|}\left[(x-\mu)^{2}+\frac{R^{2}}{\Delta^{4}}\right]^{-\frac{1}{2}}. (14)

And the electric potential at the origin is

Φ=|Δ|2π0πsinθ(Δsinθ)2+(cosθμ)2𝑑θ,\Phi=\frac{\left|\Delta\right|}{2\pi}\int_{0}^{\pi}\frac{\sin\theta}{\sqrt{\left(\Delta\sin\theta\right)^{2}+(\cos\theta-\mu)^{2}}}d\theta, (15)

where

tanθ=RΔ(xμ).\tan\theta=\frac{R}{\Delta\left(x-\mu\right)}. (16)

Regardless of the integration, the physics tells us that Φ\Phi is always constant when the origin lies inside the ellipsoid (|μ|<1\left|\mu\right|<1). We note that the expression of Φ\Phi is identical to the Eq. (10).

II.2 Pairing in real space

The following order parameter

ηg=1Nl|G|η^l|G|\eta_{\mathrm{g}}=\frac{1}{N}\sum_{l}\left|\left\langle\text{{G}}\right|\widehat{\eta}_{l}\left|\text{{G}}\right\rangle\right| (17)

is identical to ζg\zeta_{\mathrm{g}}. The fact that G|η^l|G=G|η^l+1|G\left\langle\text{{G}}\right|\widehat{\eta}_{l}\left|\text{{G}}\right\rangle=\left\langle\text{{G}}\right|\widehat{\eta}_{l+1}\left|\text{{G}}\right\rangle indicates that

ηg=|G|l1Nη^l|G|.\eta_{\mathrm{g}}=\left|\left\langle\text{{G}}\right|\sum_{l}\frac{1}{N}\widehat{\eta}_{l}\left|\text{{G}}\right\rangle\right|. (18)

Applying Fourier transformation in Eq. (A1) in the large NN limit, the following equation can be obtained:

ηg=ζg=1Nπ>k>0|G|i(ckckckck)|G|.\eta_{\mathrm{g}}=\zeta_{\mathrm{g}}=\frac{1}{N}\sum_{\pi>k>0}\left|\left\langle\text{{G}}\right|i\left(c_{-k}c_{k}-c_{k}^{{\dagger}}c_{-k}^{{\dagger}}\right)\left|\text{{G}}\right\rangle\right|. (19)

This is the primary finding of the present study. It appears that the ground state favors a balance between the two types of pairing. However, not all states can maintain such a balance. Thus, the aformentioned queries are resolved. Regarding the first query, two types of order parameters are deliberately selected to quantify the number of pairs in two aspects. Regarding the second query, the equality of the two quantities ηg\eta_{\mathrm{g}} and ζg\zeta_{\mathrm{g}} for the ground state itself is a key feature of the ground state.

In particular, the analytical behavior of ηg\eta_{\mathrm{g}} (ζg\zeta_{\mathrm{g}}) as function of (Δ,μ)\left(\Delta,\mu\right) can identify the phase diagram (see Appendix B). It is found that second-order quantum phase transitions occur at phase boundaries. The first-order derivatives of two parameters with respect to Δ\Delta or μ\mu are discontinuous, and then result in the divergence of the corresponding second-order derivatives. The profiles of ζg(μ,Δ)\zeta_{\mathrm{g}}\left(\mu,\Delta\right) at the line Δ=0.6\Delta=0.6 and μ=0.6\mu=0.6 are presented in Figs. 1(b) and 1(c), respectively. ζg\zeta_{\mathrm{g}} and its partial derivatives with respect to μ\mu and Δ\Delta for a finite NN lattice in the first quadrant of the μΔ\mu-\Delta plane are shown in Figs. 2(a)-2(c). Numerical data for the finite system reveal that the divergence at phase boundaries is demonstrated by peaks.

III Non-equilibrium stationary state

In this section, we present the features of the dynamic behavior of the system. It relates to the time evolution |ψ(t)\left|\psi(t)\right\rangle for a particular initial state

|ψ(0)=π>k>0|0k|0k,\left|\psi(0)\right\rangle=\prod_{\pi>k>0}\left|0\right\rangle_{k}\left|0\right\rangle_{-k}, (20)

which is essentially an empty state j=1N|0j\prod_{j=1}^{N}\left|0\right\rangle_{j} for fermion in real space. The evolved state

|ψ(t)\displaystyle\left|\psi(t)\right\rangle =\displaystyle= eiHt|ψ(0)=π>k>0eiHkt|0k|0k\displaystyle e^{-iHt}\left|\psi(0)\right\rangle=\prod_{\pi>k>0}e^{-iH_{k}t}\left|0\right\rangle_{k}\left|0\right\rangle_{-k} (21)
=\displaystyle= π>k>0sin(εkt)εk{2Δsink|1k|1k\displaystyle\prod_{\pi>k>0}\frac{\sin\left(\varepsilon_{k}t\right)}{\varepsilon_{k}}\{-2\Delta\sin k\left|1\right\rangle_{k}\left|1\right\rangle_{-k}
+[εkcot(εkt)i2(coskμ)]|0k|0k},\displaystyle+\left[\varepsilon_{k}\cot\left(\varepsilon_{k}t\right)-i2\left(\cos k-\mu\right)\right]\left|0\right\rangle_{k}\left|0\right\rangle_{-k}\},

may trend toward a stationary state after a sufficiently long time. The non-equilibrium stationary state driven by HH is intimately associated with the phase diagram of the ground state (Fig. 1(a)). We focus on the time-dependent order parameters for the evolved state |ψ(t)\left|\psi(t)\right\rangle. Based on the fact that |ψ(t)\left|\psi(t)\right\rangle represents the eigenstates of the operator TT, the following explicit forms can be obtained:

η(t)\displaystyle\eta(t) =\displaystyle= 1Nl|ψ(t)|η^l|ψ(t)|\displaystyle\frac{1}{N}\sum_{l}\left|\left\langle\psi(t)\right|\widehat{\eta}_{l}\left|\psi(t)\right\rangle\right| (22)
=\displaystyle= 2N|π>k>0F(k)sin2(εkt)|,\displaystyle\frac{2}{N}\left|\sum_{\pi>k>0}F(k)\sin^{2}\left(\varepsilon_{k}t\right)\right|,

and

ζ(t)\displaystyle\zeta(t) =\displaystyle= 1Nπ>k>0|ψ(t)|ζ^k|ψ(t)|\displaystyle\frac{1}{N}\sum_{\pi>k>0}\left|\left\langle\psi(t)\right|\widehat{\zeta}_{k}\left|\psi(t)\right\rangle\right| (23)
=\displaystyle= 2Nπ>k>0|F(k)|sin2(εkt),\displaystyle\frac{2}{N}\sum_{\pi>k>0}\left|F(k)\right|\sin^{2}\left(\varepsilon_{k}t\right),

where the key function is

F(k)=(coskμ)Δsink(coskμ)2+Δ2sin2k.F(k)=\frac{\left(\cos k-\mu\right)\Delta\sin k}{\left(\cos k-\mu\right)^{2}+\Delta^{2}\sin^{2}k}. (24)

Figs. 3(b1) and 3(b2) present ζ(t)\zeta(t) and η(t)\eta(t) as the function of time for finite-size systems with several typical system parameters (μ,Δ)\left(\mu,\Delta\right). As expected, both quantities become steady after a long period. ζ(t)\zeta(t) and η(t)\eta(t) behave as damping oscillations around a certain equilibrium position. The quasi frequencies and decay rates can be evaluated through a saddle point integration in the continuum limit AS ; AAM ; SA . We rewrite η(t)\eta\left(t\right) in the form

η(t)=|η()δη(t)|\eta\left(t\right)=\left|\eta\left(\infty\right)-\delta\eta\left(t\right)\right| (25)

where

η()\displaystyle\eta\left(\infty\right) =\displaystyle= 12π0πF(k)dk,\displaystyle\frac{1}{2\pi}\int_{0}^{\pi}F\left(k\right)\mathrm{d}k, (26)
δη(t)\displaystyle\delta\eta\left(t\right) =\displaystyle= 12π0πF(k)cos(2εkt)dk.\displaystyle\frac{1}{2\pi}\int_{0}^{\pi}F\left(k\right)\cos\left(2\varepsilon_{k}t\right)\mathrm{d}k. (27)

The results depends on the location k0k_{0} of the extrema εk\varepsilon_{k}. (i) In this case with k00,πk_{0}\neq 0,\pi, we have quasi frequency ω2εk0\omega\approx 2\varepsilon_{k_{0}} and δη(t)t0.5\delta\eta\left(t\right)\sim t^{-0.5}. (ii) In this case with k0=0,πk_{0}=0,\pi, we have quasi frequency ω2εk0=0\omega\approx 2\varepsilon_{k_{0}=0} and δη(t)t1\delta\eta\left(t\right)\sim t^{-1}. Similar analysis can be applied to ζ(t)\zeta\left(t\right). These results accord with the plots in Fig. 4.

On the other hand, such behaviors can also be understood by a simple picture, when the spectrum contains higher degeneracy, which relates to the peak of the density of state (DOS) of the system. The DOS at energy level EE is generally defined as

D(E)=λdN(E)dED\left(E\right)=\lambda\frac{\text{d}N\left(E\right)}{\text{d}E} (28)

where dN(E)N\left(E\right) indicates the number of energy levels that appear in the interval [E,E+dE],\left[E,E+dE\right], with the normalization factor λ=1N\lambda=\frac{1}{N}. Figs. 3(c1)-3(c4), depict the energy levels and DOS as the functions of momentum kk and EE, respectively. When the peaks of D(E)D\left(E\right) appear, the quasi frequency is related to the energy band gap δE\delta E, which is the distance between two peaks.

No matter what mechanism of the decay, ζ(t)\zeta(t) and η(t)\eta(t) approach to their stable values, which can be obtained from

η¯=limT1T0Tη(t)dt=1N|π>k>0F(k)|,\overline{\eta}=\lim_{T\rightarrow\infty}\frac{1}{T}\int_{0}^{T}\eta(t)\mathrm{d}t=\frac{1}{N}\left|\sum_{\pi>k>0}F(k)\right|, (29)

and

ζ¯=limT1T0Tζ(t)dt=1Nπ>k>0|F(k)|.\overline{\zeta}=\lim_{T\rightarrow\infty}\frac{1}{T}\int_{0}^{T}\zeta(t)\mathrm{d}t=\frac{1}{N}\sum_{\pi>k>0}\left|F(k)\right|. (30)

It is two types of summation for the same function F(k)F(k). In the large NN limit, η¯\overline{\eta} and ζ¯\overline{\zeta} can be expressed as the integral equations:

η¯=12π|0πF(k)dk|,\overline{\eta}=\frac{1}{2\pi}\left|\int_{0}^{\pi}F(k)\mathrm{d}k\right|, (31)

and

ζ¯=12π0π|F(k)|dk.\overline{\zeta}=\frac{1}{2\pi}\int_{0}^{\pi}\left|F(k)\right|\mathrm{d}k\mathbf{.} (32)

Straightforward derivations lead to the development of analytical expressions

η¯=|Δ|2π(1Δ2)ln||μ|+1|μ|1|Λ(μ,Δ),\overline{\eta}=\frac{\left|\Delta\right|}{2\pi\left(1-\Delta^{2}\right)}\ln\left|\frac{\left|\mu\right|+1}{\left|\mu\right|-1}\right|-\Lambda\left(\mu,\Delta\right), (33)

where Λ=μΔπ1(1Δ2)1\Lambda=\mu\Delta\pi^{-1}\left(1-\Delta^{2}\right)^{-1} at μ2+Δ2=1\mu^{2}+\Delta^{2}=1, and

Λ(μ,Δ)\displaystyle\Lambda\left(\mu,\Delta\right) =\displaystyle= Δ2|μ|2π(1Δ2)μ2+Δ21\displaystyle\frac{\Delta^{2}\left|\mu\right|}{2\pi\left(1-\Delta^{2}\right)\sqrt{\mu^{2}+\Delta^{2}-1}} (34)
×ln|μ2+Δ21+|Δ|μ2+Δ21|Δ||,\displaystyle\times\ln\left|\frac{\sqrt{\mu^{2}+\Delta^{2}-1}+\left|\Delta\right|}{\sqrt{\mu^{2}+\Delta^{2}-1}-\left|\Delta\right|}\right|,

when μ2+Δ21\mu^{2}+\Delta^{2}\neq 1. Conversely,

ζ¯={η¯|μ|1|Δ|ln(|Δ|)π(Δ21)|μ|<1.\overline{\zeta}=\left\{\begin{array}[]{cc}\overline{\eta}&\left|\mu\right|\geqslant 1\\ \frac{\left|\Delta\right|\ln\left(\left|\Delta\right|\right)}{\pi\left(\Delta^{2}-1\right)}&\left|\mu\right|<1\end{array}\right.. (35)

the time-averaged analytical expressions for η\eta and ζ\zeta obtained from Eqs. (33) and (35) are shown graphically in Fig. 3(a).

Similar to the static order parameters, analytical behavior of ζ¯\overline{\zeta} and η¯\overline{\eta} as function of (Δ,μ)\left(\Delta,\mu\right) can still identify the phase diagram (see Appendix B). Fig. 5 shows the average order parameters ζ¯\overline{\zeta} and η¯\overline{\eta} obtained from Eqs. (29) and (30) as the function of μ\mu and Δ\Delta for the case N=4000N=4000 in the first quadrant of the μΔ\mu-\Delta plane. Fig. 6 presents μη¯,\partial_{\mu}\overline{\eta}, μζ¯\partial_{\mu}\overline{\zeta}, Δη¯,\partial_{\Delta}\overline{\eta}, and Δζ¯\partial_{\Delta}\overline{\zeta}, the partial dervatives of ζ¯\overline{\zeta} and η¯\overline{\eta} with respect to μ\mu and Δ\Delta, for finite system. Fig. 7(a1)-7(a3) show the profiles of ζ¯(μ,Δ)\overline{\zeta}\left(\mu,\Delta\right), η¯(μ,Δ)\overline{\eta}\left(\mu,\Delta\right), μη¯\partial_{\mu}\overline{\eta} and μζ¯\partial_{\mu}\overline{\zeta} at the line Δ=0.6.\Delta=0.6. Fig. 7(b1)-7(b3) present the profiles of ζ¯(μ,Δ)\overline{\zeta}\left(\mu,\Delta\right), η¯(μ,Δ)\overline{\eta}\left(\mu,\Delta\right), Δη¯\partial_{\Delta}\overline{\eta} and Δζ¯\partial_{\Delta}\overline{\zeta} at the line μ=0.6\mu=0.6, indicating that four quantities, μη¯,\partial_{\mu}\overline{\eta}, μζ¯\partial_{\mu}\overline{\zeta}, Δη¯,\partial_{\Delta}\overline{\eta}, and Δζ¯\partial_{\Delta}\overline{\zeta}, can identify the phase boundary at μ=1\mu=1 and Δ=0\Delta=0 (μ<1)(\mu<1). Compared with ηg\eta_{\mathrm{g}} and ζg,\zeta_{\mathrm{g}}, which are always identical in all regions, ζ¯\overline{\zeta} and η¯\overline{\eta} vary in non-trivial regions, providing quantitative description of the pairing mechanism for a non-equilibrium state. Moreover, the non-equilibrium state is also a superconducting state because the values of ζ¯\overline{\zeta} and η¯\overline{\eta} have the same order as those of ζg\zeta_{\mathrm{g}} and ηg\eta_{\mathrm{g}}. The fact that ζ¯>η¯\overline{\zeta}>\overline{\eta} indicates that BCS-like pairing in momentum space is favored. Before ending this work, we would like to point out that the obtained results depend on the initial state. For example, consider an initial state in the form

|ψ(0)=k{ka}|1k|0kk{kb}|0k|1k,\left|\psi(0)\right\rangle=\prod\limits_{k\in\left\{k_{a}\right\}}\left|1\right\rangle_{k}\left|0\right\rangle_{-k}\prod\limits_{k\in\left\{k_{b}\right\}}\left|0\right\rangle_{k}\left|1\right\rangle_{-k}, (36)

with {ka}{kb}(0,π)\left\{k_{a}\right\}\oplus\left\{k_{b}\right\}\in\left(0,\pi\right), which is the eigenstate of HH with arbitrary parameters (J,Δ,μ)\left(J,\Delta,\mu\right) due to the fact

Hk|1k|0k=Hk|0k|1k=0,H_{k}\left|1\right\rangle_{k}\left|0\right\rangle_{-k}=H_{k}\left|0\right\rangle_{k}\left|1\right\rangle_{-k}=0, (37)

from the Appendix A. We find that

lη^l|ψ(0)=π>k>0ζ^k|ψ(0)=0,\sum_{l}\widehat{\eta}_{l}\left|\psi(0)\right\rangle=\sum_{\pi>k>0}\widehat{\zeta}_{k}\left|\psi(0)\right\rangle=0, (38)

which result in η¯=ζ¯=0\overline{\eta}=\overline{\zeta}=0, indicating that quantities η¯\overline{\eta} and ζ¯\overline{\zeta}\ cannot indicate the phase diagram.

IV Summary

In summary, we have studied the quench dynamics of a Kitaev chain by introducing two types of order parameters that characterize two different pairing mechanisms, namely local pairing in real space and BCS-like pairing in momentum space. We have shown exactly that the ground states over the entire parameter region support the identical values of them, indicating a balance between the two types of pairing channels; This is an unprecedented feature of the ground state. The balance is disturbed in a non-equilibrium state when the post-quench Hamiltonian is in a topologically non-trivial phase, whereas it is maintained in a topologically trivial phase. Furthermore, non-equilibrium superconducting states favor the BCS-like pairing. —Our findings present an alternative approach to generate a superconducting state from a trivial empty state and illuminate the pairing mechanism.

Acknowledgment

We acknowledge the support of NSFC (Grants No. 11874225).

Appendix A Solution and phase diagram

The Hamiltonian (1) is exactly solvable because of the translational symmetry of the system, i.e., [T,H]=0\left[T,H\right]=0, where TT is the translational operator, which is defined by TclT1=cl+1Tc_{l}T^{-1}=c_{l+1}. Taking the Fourier transformation

cj=1Nkeikjck,c_{j}=\frac{1}{\sqrt{N}}\sum\limits_{k}e^{ikj}c_{k}, (A1)

of the Hamiltonian (1), with wave vector k(π,π]k\in(-\pi,\pi], we can obtain the following equation:

H\displaystyle H =\displaystyle= k[(2Jcosk+2μ)ckck\displaystyle\sum_{k}[\left(-2J\cos k+2\mu\right)c_{k}^{{\dagger}}c_{k} (A2)
+iΔsink(ckck+ckck)μ].\displaystyle+i\Delta\sin k\left(c_{-k}c_{k}+c_{-k}^{{\dagger}}c_{k}^{{\dagger}}\right)-\mu].

For ease of further analysis, the JJ value can be considered to be 11 and the Hamiltonian can be expressed through the Nambu representation

H\displaystyle H =\displaystyle= π>k>0Hk,\displaystyle\sum_{\pi>k>0}H_{k}, (A3)
Hk\displaystyle H_{k} =\displaystyle= 2(ckck)(coskμiΔsinkiΔsinkμcosk)(ckck),\displaystyle-2\left(\begin{array}[]{cc}c_{k}^{{\dagger}}&c_{-k}\end{array}\right)\left(\begin{array}[]{cc}\cos k-\mu&i\Delta\sin k\\ -i\Delta\sin k&\mu-\cos k\end{array}\right)\left(\begin{array}[]{c}c_{k}\\ c_{-k}^{{\dagger}}\end{array}\right), (A9)

where the Hamiltonian HkH_{k} in each invariant subspace satisfies the commutation relation

[Hk,Hk]=0.\left[H_{k},H_{k^{\prime}}\right]=0. (A10)

This allows us to treat the diagonalization and dynamics governed by HkH_{k} individually. For a given kk, the Hamiltonian HkH_{k} in the basis (|0k|0k,|1k|1k,|1k|0k,|0k|1k\left|0\right\rangle_{k}\left|0\right\rangle_{-k},\left|1\right\rangle_{k}\left|1\right\rangle_{-k},\left|1\right\rangle_{k}\left|0\right\rangle_{-k},\left|0\right\rangle_{k}\left|1\right\rangle_{-k}) is expressed as a 4×44\times 4 matrix

hk=2(coskμiΔsink00iΔsinkμcosk0000000000),h_{k}=2\left(\begin{array}[]{cccc}\cos k-\mu&i\Delta\sin k&0&0\\ -i\Delta\sin k&\mu-\cos k&0&0\\ 0&0&0&0\\ 0&0&0&0\end{array}\right), (A11)

where |1k=ck|0k\left|1\right\rangle_{k}=c_{k}^{{\dagger}}\left|0\right\rangle_{k} and ck|0k=0c_{k}\left|0\right\rangle_{k}=0. The eigenstates |φkλ±\left|\varphi_{k\mathrm{\lambda}}^{\pm}\right\rangle [λ=e\mathrm{\lambda}=\mathrm{e} (o)\mathrm{(o)} denotes the even (odd) parity of the particle number] are

|φke±\displaystyle\left|\varphi_{k\mathrm{e}}^{\pm}\right\rangle =\displaystyle= 1Ω±(ak±|0k|0k+|1k|1k),\displaystyle\frac{1}{\Omega^{\pm}}\left(a_{k}^{\pm}\left|0\right\rangle_{k}\left|0\right\rangle_{-k}+\left|1\right\rangle_{k}\left|1\right\rangle_{-k}\right), (A12)
|φko+\displaystyle\left|\varphi_{k\mathrm{o}}^{+}\right\rangle =\displaystyle= |1k|0k,|φko=|0k|1k,\displaystyle\left|1\right\rangle_{k}\left|0\right\rangle_{-k},\left|\varphi_{k\mathrm{o}}^{-}\right\rangle=\left|0\right\rangle_{k}\left|1\right\rangle_{-k}, (A13)

where Ω±=1+|ak±|2\Omega^{\pm}=\sqrt{1+\left|a_{k}^{\pm}\right|^{2}} is the normalization coefficient in the context of Dirac inner product with

ak±=icoskμ+ϵke±/2Δsink,a_{k}^{\pm}=i\frac{\cos k-\mu+\epsilon_{k\mathrm{e}}^{\pm}/2}{\Delta\sin k}, (A14)

and corresponding energies are

ϵke±=±εk,ϵko±=0,\epsilon_{k\mathrm{e}}^{\pm}=\pm\varepsilon_{k},\epsilon_{k\mathrm{o}}^{\pm}=0, (A15)

with

εk=2(μcosk)2+Δ2sin2k.\varepsilon_{k}=2\sqrt{\left(\mu-\cos k\right)^{2}+\Delta^{2}\sin^{2}k}. (A16)

Accordingly, the ground-state wave function can be expressed as

|G=π>k>0|φke.\left|\text{{G}}\right\rangle=\prod_{\pi>k>0}\left|\varphi_{k\mathrm{e}}^{-}\right\rangle. (A17)

|G\left|\text{{G}}\right\rangle is the eigenstate of TT, obeying T|G=eiΩ|GT\left|\text{{G}}\right\rangle=e^{i\Omega}\left|\text{{G}}\right\rangle, where Ω\Omega is a real number. Furthermore, the phase-transition lines (phase boundary) can be determined using min(εk)=0(\varepsilon_{k})=0, which results in the gapless lines

μ=±1, and Δ=0, for |μ|<1.\mu=\pm 1\text{, and }\Delta=0\text{, for }\left|\mu\right|<1. (A18)

These lines separate four regions in the parameter space, representing different phases with winding numbers CKC ; NL N=0N=0, and ±1\pm 1, respectively.

Appendix B Analytical behavior of static and dynamic order parameters

The analytical behavior of ηg\eta_{\mathrm{g}} (ζg\zeta_{\mathrm{g}}) as the function of (Δ and μ)\left(\Delta\text{ and }\mu\right) can identify the phase diagram. On the basis of the aforementioned euqations, we found that second-order quantum phase transitions occur at phase boundaries. Around lines |μ|=1\left|\mu\right|=1, we have μζg=0\partial_{\mu}\zeta_{\mathrm{g}}=0 at μ=±1\mu=\pm 1^{\mp} but μζg=2π1Δ1\partial_{\mu}\zeta_{\mathrm{g}}=\mp 2\pi^{-1}\Delta^{-1} at μ=±1±\mu=\pm 1^{\pm}. Then, μ2ζg\partial_{\mu}^{2}\zeta_{\mathrm{g}} diverges at these two lines. We have

ζg|Δ0\displaystyle\zeta_{\mathrm{g}}|_{\Delta\rightarrow 0} \displaystyle\approx 2π1Δln|Δ|,\displaystyle-2\pi^{-1}\Delta\ln\left|\Delta\right|, (B 1)
Δζg|Δ0\displaystyle\partial_{\Delta}\zeta_{\mathrm{g}}|_{\Delta\rightarrow 0} \displaystyle\approx 2π1ln|Δ|,\displaystyle-2\pi^{-1}\ln\left|\Delta\right|, (B 2)
Δ2ζg|Δ0\displaystyle\partial_{\Delta}^{2}\zeta_{\mathrm{g}}|_{\Delta\rightarrow 0} \displaystyle\approx 2π1Δ1,\displaystyle-2\pi^{-1}\Delta^{-1}, (B 3)

around the segment |Δ|=0\left|\Delta\right|=0 (|μ|1)(\left|\mu\right|\leqslant 1).

Similarly, the analytic expressions of ζ¯\overline{\zeta} and η¯\overline{\eta} help us investigate their analytical behaviors. (i) Around lines |μ|=1\left|\mu\right|=1, we have

μη¯=±12π|Δ|ln4Δ2|μ21|,\partial_{\mu}\overline{\eta}=\pm\frac{1}{2\pi\left|\Delta\right|}\ln\frac{4\Delta^{2}}{\left|\mu^{2}-1\right|}, (B 4)

which is divergent at the phase boundary μ=±1\mu=\pm 1. By contrast, when μ±1±,\mu\approx\pm 1^{\pm}, we have

μζ¯±12π|Δ|ln4Δ2|μ21|,\partial_{\mu}\overline{\zeta}\approx\pm\frac{1}{2\pi\left|\Delta\right|}\ln\frac{4\Delta^{2}}{\left|\mu^{2}-1\right|}, (B 5)

which is divergent. However, we have μζ¯=0\partial_{\mu}\overline{\zeta}=0 at |μ|=1\left|\mu\right|=1^{-}. Therefore, μζ¯\partial_{\mu}\overline{\zeta} is discontinuous at the lines |μ|=1\left|\mu\right|=1. (ii) Around the segment |Δ|=0\left|\Delta\right|=0 (|μ|<1\left|\mu\right|<1), we have

Δη¯±0.5π1[ln(||μ|+1|)ln(||μ|1|)]\partial_{\Delta}\overline{\eta}\approx\pm 0.5\pi^{-1}\left[\ln\left(\left|\left|\mu\right|+1\right|\right)-\ln\left(\left|\left|\mu\right|-1\right|\right)\right] (B 6)

for Δ=0±\Delta=0^{\pm}, resulting in the divergent Δ2η¯\partial_{\Delta}^{2}\overline{\eta}. By contrast, we have

Δζ¯π1ln(|Δ|)\partial_{\Delta}\overline{\zeta}\approx\mp\pi^{-1}\ln\left(\left|\Delta\right|\right) (B 7)

for Δ=0±\Delta=0^{\pm}. It is divergent at the phase boundary |Δ|=0\left|\Delta\right|=0. In summary, μη¯,\partial_{\mu}\overline{\eta}, μζ¯\partial_{\mu}\overline{\zeta}, Δη¯,\partial_{\Delta}\overline{\eta}, and Δζ¯\partial_{\Delta}\overline{\zeta}, can identify the phase boundary at μ=1\mu=1 and Δ=0\Delta=0 (μ<1)(\mu<1). Compared with ηg\eta_{\mathrm{g}} and ζg,\zeta_{\mathrm{g}}, which are always identical in all regions, ζ¯\overline{\zeta} and η¯\overline{\eta} vary in non-trivial regions, providing quantitative description of the pairing mechanism for a non-equilibrium state. Moreover, the non-equilibrium state is also a superconducting state because the values of ζ¯\overline{\zeta} and η¯\overline{\eta} have the same order as those of ζg\zeta_{\mathrm{g}} and ηg\eta_{\mathrm{g}}. The fact that ζ¯>η¯\overline{\zeta}>\overline{\eta} indicates that BCS-like pairing in momentum space is favored.

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