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A linearly implicit energy-preserving exponential time differencing scheme for the fractional nonlinear Schrödinger equation

  • In this paper, we present a new method to solve the fractional nonlinear Schrödinger equation. Our approach combines the invariant energy quadratization method with the exponential time differencing method, resulting in a linearly-implicit energy-preserving scheme. To achieve this, we introduce an auxiliary variable to derive an equivalent system with a modified energy conservation law. The proposed scheme uses stabilized exponential time differencing approximations for time integration and Fourier pseudo-spectral discretization in space to obtain a linearly-implicit, fully-discrete scheme. Compared to the original energy-preserving exponential integrator scheme, our approach is more efficient as it does not require nonlinear iterations. Numerical experiments confirm the effectiveness of our scheme in conserving energy and its efficiency in long-time computations.

    Citation: Tingting Ma, Yayun Fu, Yuehua He, Wenjie Yang. A linearly implicit energy-preserving exponential time differencing scheme for the fractional nonlinear Schrödinger equation[J]. Networks and Heterogeneous Media, 2023, 18(3): 1105-1117. doi: 10.3934/nhm.2023048

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  • In this paper, we present a new method to solve the fractional nonlinear Schrödinger equation. Our approach combines the invariant energy quadratization method with the exponential time differencing method, resulting in a linearly-implicit energy-preserving scheme. To achieve this, we introduce an auxiliary variable to derive an equivalent system with a modified energy conservation law. The proposed scheme uses stabilized exponential time differencing approximations for time integration and Fourier pseudo-spectral discretization in space to obtain a linearly-implicit, fully-discrete scheme. Compared to the original energy-preserving exponential integrator scheme, our approach is more efficient as it does not require nonlinear iterations. Numerical experiments confirm the effectiveness of our scheme in conserving energy and its efficiency in long-time computations.



    In 2000, Laskin, a Canadian scholar, explored non-Brownian motion as a possible approach to deriving the path integral. He expanded on Feynmann's path integral by incorporating Levy paths, as documented in his works [11,12], which allowed for the modification of the Schrödinger equation. By utilizing the non-local Laplacian operator (Δ)α/2(1<α2), he established the Schrödinger model [13], which accurately describes the quantum state variations of non-local physical systems over time, surpassing the classical Schrödinger equation. The model has been successfully applied to various fields [9,15,23]. This paper focuses on the fractional nonlinear Schrödinger (NLS) equation with the form

    iu(x,t)t(Δ)α2u(x,t)+β|u(x,t)|2u(x,t)=0,  xΩR2,  t(0,T], (1.1)
    u(x,0)=u0(x),  xΩ, (1.2)

    where 1<α2, i2=1, u0(x) is a given smooth function, β is a real positive constant. The fractional Laplacian (Δ)α2 with period 2L can be defined by [22]

    (Δ)α2u(x,t)=k1Zk2Z|υ2k1+υ2k2|α2ˆukeiυk(x+L), with  ˆuk=1(2L)2Ωu(x,t)eiυk(x+L)dx, (1.3)

    where υk1=k1πL, υk2=k2πL, υk(x+L)=υk1(x+L)+υk2(y+L). By setting u=p+iq, we can rewrite system (1.1) as a pair of real-valued equations

    pt=(Δ)α2qβ(p2+q2)q, (1.4)
    qt=(Δ)α2p+β(p2+q2)p. (1.5)

    Guo et al. derive the equation possessing the energy conservation law [6], namely

    H(p,q)=12Ω[((Δ)α4p)2+((Δ)α4q)2]dxβ4Ω(p2+q2)2dx, (1.6)

    where H is energy function. From variational derivative formula [4], systems (1.4) and (1.5) can be rewritten as as an Hamiltonian system

    dzdt=J1δHδz,  with  z=(p,q)T,  J=(0110).

    It is widely acknowledged that conserving energy is crucial in establishing the existence and uniqueness of solutions for PDEs [3,19]. Traditional methods fail to maintain these conservation laws, making structure-preserving algorithms essential for the numerical analysis of classical differential equations. Recently, researchers have been exploring structure-preserving numerical schemes for fractional equations [18], with a focus on the fractional NLS equation. For example, Li et al. [16] developed a fast conservative finite element scheme for the strongly coupled fractional NLS equation. Wang et al. [20,21] also presented different schemes that can exactly conserve energy for various fractional NLS equations. Additional related research can be found in [4] and the references therein. However, most structure-preserving schemes for the fractional NLS equation are fully implicit, requiring iterations to solve algebraic systems at each time step. This leads to a substantial number of calculations.

    In [2], the exponential integrators scheme was studied in depth. This scheme has a unique advantage in that it accurately evaluates the contribution of the linear part, allowing for stable and precise computations even when dealing with highly rigid linear terms. As a result, this scheme has been successfully applied to Hamiltonian PDEs [17] and has been found to permit larger step sizes and achieve greater accuracy than non-exponential schemes. Additionally, the invariant energy quadratization (IEQ) method, developed by Yang and colleagues, has been used to create efficient and accurate linearly-implicit schemes for certain gradient models [5] and conservative differential equations [1,10]. For example, in [1], a linearly implicit scheme for the fractional NLS equation was developed using the IEQ method. However, practical computations using these schemes still require smaller step sizes, making them computationally expensive for long-time numerical simulations. To address these challenges, we propose a novel approach that combines the exponential time differencing method with the IEQ approach to develop an efficient linearly-implicit energy-preserving scheme for the fractional NLS equation. Surprisingly, there has been little research in this area to date. The main goal of this paper is to develop a linearly-implicit exponential integrator scheme for this equation, using the IEQ method. Our contributions can be summarized as follows: (i) we introduce the Hamiltonian form of the equation; (ii) we combine the IEQ method and the exponential integrators technique to develop a linearly implicit scheme that conserves energy; (iii) we demonstrate that the construction process of the proposed scheme can be extended to develop conservative schemes for other differential equations. Moreover, our numerical results show that the scheme inherits the modified energy and has better numerical stability than traditional energy-preserving schemes in practical computations.

    The paper is arranged as follows. In Section 2, we obtain a new equivalent system with modified energy via the IEQ method. In Section 3, we construct a linearly-implicit exponential integrator scheme for solving the fractional NLS equation, and prove that the proposed scheme can preserve the discrete energy. A numerical example is presented in Section 4 to illustrate the theoretical results. We draw some conclusions in Section 5.

    In this Section, we utilize the IEQ idea to transform Eqs (1.4) and (1.5) into an equivalent system. Following the idea of the IEQ approach, we introduce an auxiliary variable w:=w(t)=G(p,q)+C0, where G(p,q)=β4(p2+q2)2, by choosing a sufficiently large constant C0, the well-posedness of w is ensured. This results in a modified formalism for the Hamiltonian energy (1.6).

    E(t)=12Ω[((Δ)α4p)2+((Δ)α4q)2]dxΩw2dx, (2.1)

    and the corresponding fractional NLS systems (1.4) and (1.5) can be written as

    pt=(Δ)α2qβ(p2+q2)qG(p,q)+C0w, (2.2)
    qt=(Δ)α2p+β(p2+q2)pG(p,q)+C0w, (2.3)
    wt=β(p2+q2)ppt+β(p2+q2)qqt2G(p,q)+C0, (2.4)

    with the consistent initial condition p0=p0(x,0)=Re(u0(x)),q0=q0(x,0)=Im(u0(x)),w0=G(p0,q0)+C0, and the periodic boundary condition. It is easy to prove the systems (2.2)–(2.4) possesses the modified energy

    E(t)=E(0). (2.5)

    For positive even integers Nx, Ny and N, we define: hx:=2LNx,hy:=2LNy, and set time step τ=TN. The spatial grid points are given: Ωh={(xi,yj)| i=0,1,,Nx1;j=0,1,,Ny1}, where xi=L+ihx,0iNx1,yj=L+jhy,0jNy1. Let Uh={u|u=(u0,0,,uNx1,0,u0,1,,uNx1,1, ,u0,Ny1,,uNx1,Ny1)T}. For u,vUh, we define

    u,vh=hxhyNx1i=0Ny1j=0ui,jˉvi,j,   u=u,u12h,  u=sup(xi,yj)Ωh|ui,j|,

    where ˉvi,j is the conjugate of vi,j, and we introduce some operators

    δtun=un+1unτ, un+1/2=un+1+un2,  ˆun+1/2=3unun12.

    Let (xi,yj)Ωh be the Fourier collocation points. Using the interpolation polynomial INp(x,y) to approximate pN(x,y) of the function p(x,y), and we have

    INp(x,y)=pN(x,y)=Nx/2k1=Nx/2Ny/2k2=Ny/2˜pk1,k2eik1μ(x+L)eik2μ(y+L),

    where μ=πL, and the coefficient

    ˜pk1,k2=1Nxck11Nyck2Nx1i=0Ny1j=0p(xi,yj)eik1μ(x+L)eik2μ(y+L),

    with ck1=1 for |k1|<Nx/2, ck2=1 for |k2|<Ny/2, ck1=2 for k1=±Nx/2, and ck2=2 for k2=±Ny/2.

    Then the (Δ)α2 on p(xi,yj) can be discretized by [8]

    (Dαp)i,j:=(Δ)α2pN(xi,yj)=1NxNyNx1k1=0Ny1k2=0d(s)k1,k2(Nx1i=0Ny1j=0pi,je2πi(ik1+jk2)/Nx)e2πi(ik1+jk2)/Ny, (3.1)

    where

    d(α)k1,k2={μα(k21+k22)α/2,0k1Nx/2,0k2Ny/2,μα(k21+(k2N2)2)α/2,0k1Nx/2,Ny/2k2Ny1,μα((k1N1)2+k22)α/2,Nx/2k1Nx1,0k2Ny/2,μα((k1N1)2+(k2N2)2)α/2,Nx/2k1Nx1,Ny/2k2Ny1.

    Especially for N=Nx=Ny, the negative definite and symmetric matrix Ds is given

    Ds=(FF)1Λ(FF),Λ=diag(d(s)),

    where F is a orthogonal matrix with the entries

    (F)j,k=1N[e2πi(j1)(k1)N],k=1,2,,N.

    One can observe that the expression (FF)1Λ(FF)p can be efficiently calculated in O(N2logN) operations using the built-in function ifft2(Λ.fft2(p)) in Matlab.

    By applying the Fourier pseudo-spectral to Eqs (2.2)–(2.4), we obtain

    pt=Dαqg2(p,q)G(p,q)+C0w, (3.2)
    qt=Dαp+g1(p,q)G(p,q)+C0w, (3.3)
    wt=g1(p,q)pt+g2(p,q)qt2G(p,q)+C0, (3.4)

    where g1(p,q)=β(p2+q2)p, g2(p,q)=β(p2+q2)q.

    Let

    z(t)=(p(t),q(t))T,f(p(t),q(t),w(t))=(g1(p,q)G(p,q)+C0w,g2(p,q)G(p,q)+C0w)T,
    S=(OIIO),D=(DαOODα),

    then, systems (3.2)–(3.4) can be rewritten as

    zt=SDz(t)+Sf (3.5)
    wt=g1(p,q)pt+g2(p,q)qt2G(p,q)+C0. (3.6)

    Let V=τSD, then integrating systems (3.5) and (3.6) from tn to tn+1, we can obtain

    zn+1=exp(V)zn+τ10exp[(1ξ)V]Sf(p(tn+ξτ),q(tn+ξτ),w(tn+ξτ))dξ, (3.7)
    wn+1=wn+τ10g1(p(tn+ξτ),q(tn+ξτ))pt+g2(p(tn+ξτ),q(tn+ξτ))qt2G(p(tn+ξτ),q(tn+ξτ))+C0dξ. (3.8)

    Then, we can use f(p(tn+ξτ),q(tn+ξτ),w(tn+ξτ)) and

    g1(p(tn+ξτ),q(tn+ξτ))pt+g2(p(tn+ξτ),q(tn+ξτ))qt2G(p(tn+ξτ),q(tn+ξτ))+C0

    to approximate f(ˆpn+12,ˆqn+12,wn+12) and

    g1(ˆpn+12,ˆqn+12)δtpn+g2(ˆpn+12,ˆqn+12)δtqn2G(ˆpn+12,ˆqn+12)+C0,

    respectively, and obtain the following new scheme

    zn+1=exp(V)zn+τϕ(V)Sf(ˆpn+12,ˆqn+12,wn+12), (3.9)
    wn+1=wn+τg1(ˆpn+12,ˆqn+12)δtpn+g2(ˆpn+12,ˆqn+12)δtqn2G(ˆpn+12,ˆqn+12)+C0, (3.10)

    where

    ϕ(V)=10exp[(1ξ)V]dξ,
    f(ˆpn+12,ˆqn+12,wn+12)=(g1(ˆpn+12,ˆqn+12)wn+12G(ˆpn+12,ˆqn+12)+C0,g2(ˆpn+12,ˆqn+12)wn+12G(ˆpn+12,ˆqn+12)+C0)T,  n=1,2,.

    Remark 3.1. It should be noted that the proposed schemes (3.9) and (3.10) are a three level method, therefore, we can calculate the z1 and w1 by using the z0 instead of ˆz12 for the first step.

    Theorem 3.1. Schemes (3.4) and (3.5) conserve the modified energy

    En+1=En, with  En=12(zn)TDzn+(wn)2,  n=0,1,.

    To this end, we first give some lemmas.

    Lemma 3.1. [7] Assuming that g(x) is a sufficiently smooth function, in the vicinity of zero, with 0 being a removable singularity, we can define g(0) as the limit of g(x) as x approaches zero.

    g(x)=k=0gk(0)k!xk,

    and for a matrix A, the matrix valued function is defined by g(A)=k=0gk(0)k!Ak.

    Lemma 3.2. [17] If D is a symmetric matrix and τ is a non-negative scalar, then the matrix A defined by A=exp(V)TDexp(V)D is a nilpotent matrix, where V=τSD and S is a skew-symmetric matrix.

    Next, we show that the proposed scheme can preserve the modified energy.

    Proof. If D is a singular matrix, let {Dϵ} be a series of symmetric and nonsingular matrices, which converge to D when ϵ0. We assume znϵ,wnϵ satisfy the perturbed scheme

    zn+1ϵ=exp(Vϵ)znϵ+τg(Vϵ)Sf(ˆzn+12ϵ,wn+12ϵ), (3.11)
    wn+1ϵ=wnϵ+τg1(^pϵn+12,^qϵn+12)δtpϵn+g2(^pϵn+12,^qϵn+12)δtqϵn2G(^pϵn+12,^qϵn+12)+C0, (3.12)

    where Vϵ=τSDϵ, n=0,1,. Then, we denote

    ˜fϵ:=D1ϵfϵ=D1ϵf(ˆzn+12ϵ,wn+12ϵ),

    and rewrite En as

    Enϵ=12(znϵ)TDϵznϵ+(wnϵ)2. (3.13)

    According to Eq (3.4), we have

    12(zn+1ϵ)TDϵzn+1ϵ=12[(znϵ)Texp(Vϵ)T+τfTϵSTϕ(Vϵ)T]Dϵ[exp(Vϵ)znϵ+τϕ(Vϵ)Sfϵ]=12(znϵ)Texp(Vϵ)TDϵexp(Vϵ)znϵ+(znϵ)Texp(Vϵ)TDϵ[exp(Vϵ)I]˜fϵ+12˜fTϵ[exp(Vϵ)TI]Dϵ[exp(Vϵ)I]˜fϵ=12[(znϵ)Texp(Vϵ)T+τfTϵSTϕ(Vϵ)T]Dϵ[exp(Vϵ)znϵ+τϕ(Vϵ)Sfϵ]=12(znϵ)Texp(Vϵ)TDϵexp(Vϵ)znϵ+(znϵ)Texp(Vϵ)TDϵ[exp(Vϵ)I]˜fϵ+12˜fTϵ[exp(Vϵ)TI]Dϵ[exp(Vϵ)I]˜fϵ. (3.14)

    On the other hand, from Eq (3.12), we have

    (wn+1ϵ)2(wnϵ)2=g1(^pϵn+12,^qϵn+12)(pn+1ϵpnϵ)+g2(^pϵn+12,^qϵn+12)(qn+1ϵqnϵ)2G(^pϵn+12,^qϵn+12)+C0wn+12ϵ=((zn+1ϵ)T(znϵ)T)fϵ=(znϵ)T[exp(Vϵ)TI]fϵ+τfTϵSTϕ(Vϵ)Tfϵ=(znϵ)T[exp(Vϵ)TI]D˜fϵ+τfTϵSTϕ(Vϵ)TD˜fϵ=(znϵ)T[exp(Vϵ)TDϵDϵ]˜fϵ+˜fTϵVTϵϕ(Vϵ)TDϵ˜fϵ=(znϵ)T[exp(Vϵ)TDϵDϵ]˜fϵ+˜fTϵ[exp(Vϵ)TDϵDϵ]˜fϵ. (3.15)

    This together with Eq (3.9), we can deduce

    En+1ϵEnϵ=12(zn+1ϵ)TDϵzn+1ϵ12(znϵ)TDϵznϵ+(wn+1ϵ)2(wnϵ)2=12(znϵ)T[exp(Vϵ)TDϵexp(Vϵ)Dϵ]znϵ+(znϵ)T[exp(Vϵ)TDϵexp(Vϵ)Dϵ]˜fϵ+12˜fTϵ[exp(Vϵ)TDϵexp(Vϵ)Dϵ]˜fϵ+12˜fTϵ[exp(Vϵ)TDϵDϵexp(Vϵ)]˜fϵ=12˜fTϵBϵ˜fϵ+12(znϵ+˜fϵ)TAϵ(znϵ+˜fϵ)=0, (3.16)

    where

    Bϵ=exp(Vϵ)TDϵDϵexp(Vϵ),
    Aϵ=exp(Vϵ)TDϵexp(Vϵ)Dϵ.

    The last equality is based on Lemma 3.1 and the skew symmetry of the matrix B. Thus, from Eq (3.9), when ϵ0,znϵzn,wnϵwn, we obtain En+1=En.

    If D is a nonsingular matrix, the proof is similar to above process, for brevity, we omit it. The proof is completed.

    Two examples are given to confirm the efficiency, conservation and stability of the proposed scheme. We use the formula

    Rate=ln(error1/error2)ln(τ1/τ2) (4.1)

    to evaluate the convergence rate, where τi,errori,(i=1,2) are step sizes and L-norm errors with the step size τi, respectively. The relative energy error is defined as

    REn=|EnE0E0|,   RHn=|HnH0H0|, (4.2)

    where En and En denote the conservation laws at tn=nτ.

    Example 4.1. Considering the equation with

    u(x,0)=exp(x2)exp(ix),   xΩ=[40,40]. (4.3)

    The exact solution is not given, we use

    e=u(h,τ)u(h,τ2),

    to obtain numerical errors.

    In the follow-up of the article, the E-IEQ is the developed scheme in our work, CN-IEQ is a linearly implicit Crank-Nicolson IEQ scheme [1], E-AVF scheme is a fully-implicit exponential AVF scheme, and the E-SAV scheme [14] represents a linearly implicit exponential scheme based on the SAV approach. Yet the general, we first take α=1.8 to demonstrate the accuracy, efficiency and conservation properties of E-IEQ scheme. In Table 1, numerical errors and convergence orders implies that four schemes have second-order accuracy in the time. Noting that 'NaN' implies the CN-IEQ scheme cannot be implemented with a large time step, but the E-IEQ scheme can. Figure 1 shows that linearly implicit schemes are more efficient than the E-AVF scheme, and the E-IEQ scheme is most efficient of the four schemes.

    Table 1.  Temporal accuracy of different schemes with, h=80/512.
    Scheme τ=140 τ=180 τ=1160 τ=1320
    CN-IEQ e NaN NaN 9.81e-03 2.54e-03
    Rate * * * 1.95
    E-IEQ e 3.32e-02 7.64e-03 1.82e-04 4.46e-04
    Rate * 2.12 2.07 2.03
    E-SAV [14] e 2.91e-02 7.26e-03 1.81e-03 4.53e-04
    Rate * 2.00 2.00 2.00
    EAVF [17] e 1.68e-02 4.19e-03 1.04e-03 2.62e-04
    Rate * 1.99 2.00 2.00

     | Show Table
    DownLoad: CSV
    Figure 1.  The numerical error versus the CPU time using the four numerical schemes.

    In Figure 2, the relative errors of the modified energy and original energy of the equation are presented. From the results, we can see three linearly implicit schemes only can conserve the modified energy, the E-AVF scheme can preserve the inherent energy of the equation. Finally, we focus on the correlation between the fractional order α and the soliton's shape. Figure 3 displays numerical outcomes for various α values. It is evident that α has a significant impact on the soliton's form. As α shifts from 1.3 to 2, the soliton's appearance changes dramatically. The findings reveal that the solitary wave can endure stable propagation under finite initial circumstances, even after long periods of propagation.

    Figure 2.  Relative errors of conservation laws for different schemes with h=80/512,τ=0.01.
    Figure 3.  Evolution of the solitons with N=512,τ=0.01 for different order α.

    Example 4.2. We consider the equation on (x,y)=(π,π)×(π,π) and has the form

    u(x,y,t)=Aexp(i(λ1x+λ2yωt)), (4.4)

    with

    ω=(λ12+λ22)α2β|A|2. (4.5)

    where the amplitude A=1, the wave numbers λ1=λ2=2 and β=2.

    This example takes α=1.4,1.7,2. Figure 4 shows that the proposed scheme has second-order in time. We then run a long-time simulation till T=50 and plot the relative energy deviation in Figure 5 which indicates that the new scheme can preserve the modified energy exactly in discrete scene.

    Figure 4.  Convergence orders in time for different order α with h=2π/16.
    Figure 5.  Convergence orders in time for different order α with h=2π/16.

    In this paper, we introduce a unique technique to solve the fractional nonlinear Schrödinger equation while conserving energy. We achieve this through a combination of the invariant energy quadratization method and the exponential time differencing method. Our proposed scheme is highly efficient and performs well even with large time steps during long-time computations. In discrete settings, the modified energy is precisely preserved. To demonstrate our approach, we present a numerical example. Furthermore, this technique can be applied to other fractional Hamiltonian PDEs, including the fractional nonlinear wave equation and the fractional Klein-Gordon-Schrödinger equation, by following a similar process.

    The research is supported by the National Natural Science Foundation of China (No. 12001471).

    The authors declare there is no conflict of interest.



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