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Soliton solutions of conformable time-fractional perturbed Radhakrishnan-Kundu-Lakshmanan equation

  • In this paper, our main purpose is to study the soliton solutions of conformable time-fractional perturbed Radhakrishnan-Kundu-Lakshmanan equation. New soliton solutions have been obtained by the extended (G/G)-expansion method, first integral method and complete discrimination system for the polynomial method, respectively. The solutions we obtained mainly include hyperbolic function solutions, solitary wave solutions, Jacobi elliptic function solutions, trigonometric function solutions and rational function solutions. Moreover, we draw its three-dimensional graph.

    Citation: Chun Huang, Zhao Li. Soliton solutions of conformable time-fractional perturbed Radhakrishnan-Kundu-Lakshmanan equation[J]. AIMS Mathematics, 2022, 7(8): 14460-14473. doi: 10.3934/math.2022797

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  • In this paper, our main purpose is to study the soliton solutions of conformable time-fractional perturbed Radhakrishnan-Kundu-Lakshmanan equation. New soliton solutions have been obtained by the extended (G/G)-expansion method, first integral method and complete discrimination system for the polynomial method, respectively. The solutions we obtained mainly include hyperbolic function solutions, solitary wave solutions, Jacobi elliptic function solutions, trigonometric function solutions and rational function solutions. Moreover, we draw its three-dimensional graph.



    Due to the wide application in the fields of physics, communication and engineering, the study of soliton solutions of the Radhakrishnan-Kundu-Lakshmanan (RKL) equation has attracted much attention[1,2,3,4,5,6,7]. Especially in nonlinear optical fibers, the RKL equation usually describes the propagation of optical pulses, which is represented by the higher-order nonlinear Schrödinger equation. In recent years, many powerful mathematical methods have been proposed to derive soliton solutions [8,9,10,11,12,13,14,15,16,17,18,19,20,21] for the RKL equation, such as the first integral method[22], the generalized exponential rational function method [23], the Laplace-Adomian decomposition method [24], the dynamical system method[25], the Painlevé analysis[26], the auxiliary equation method and extended simple equation method[27], the modified simple equation and exp(φ(q)) method [28].

    In the paper, we consider the fractional perturbed Radhakrishnan-Kundu-Lakshmanan (FPRKL) equation[29,30,31,32]:

    iDαtϕ+aϕxx+b|ϕ|2ϕiδϕxiλ(|ϕ|2ϕ)xiσ(|ϕ|2)xϕiγϕxxx=0, 0<α1, (1.1)

    where ϕ is the complex-valued wave function.

    Definition 1.1. Let ψ:[0,)R. Then, the conformable fractional derivative of ψ of order α is defined as

    Dαtψ(t)=limε0ψ(t+εt1α  )ψ(t)ε, (1.2)

    for all t>0 and α(0,1]. Further, some properties of conformable fractional derivative is given

    (i) Dαt(tδ)=μtδα, δR.

    (ii) Dαt(ψ(t)+φ(t))=Dαtψ(t)+Dαtφ(t).

    (iii) Dαt(ψφ)(t)=t1αφ(t)α1φ(t)Dαt(ψ(t))|t=φ(t).

    This article is arranged as follows. In Section 2, we employ three different methods to solve the FPRKL equation. In Section 3, we draw three-dimensional graph of Eq (1.1). In Section 4, we give a brief conclusion.

    Making the complex transformation

    ϕ(x,t)=u(ξ)eiτ, ξ=μ(xνtαα), τ=kx+ϖtαα+θ. (2.1)

    Substituting Eq (2.1) into Eq (1.1), separating into real and imaginary parts yields

    μ2(a3kγ)u+(bkλ)u3(ϖ+ak2+δkγk3)u=0, (2.2)
    μ2γu+(ν+2ak+δ3k2γ)u+(3λ+2σ)u2u=0. (2.3)

    Integrating Eq (2.3) once, we have

    3μ2γu+3(ν+2ak+δ3k2γ)u+(3λ+2σ)u3=0. (2.4)

    Since the function U satisfies both Eq (2.3) and Eq (2.4), the following constraint condition is obtained

    a+3kγ3γ=ϖ+ak2+δkγk3ν+2ak+δ+3k2γ=bkλ3λ+2σ. (2.5)

    So, k and c in Eq (2.5) can be obtained

    k=3bγ+2aσ+3aλ6γ(λ+σ), ν=γ(ϖ+ak2+δkγk3)a+3kγ(2ak+δ+3γk2). (2.6)

    Balancing u3 and u in Eq (2.4), we have N=1. So, the solution form of Eq (2.4) is

    u(ξ)=a1(GG)+a0+a1(GG)1. (2.7)

    Here G=G(ξ) satisfies the following nonlinear ordinary differential equation

    GG=A(G)2+BGG+CG2, (2.8)

    where A, B, C are real parameters, Eq (2.8) satisfies the following equation

    G(ξ)G(ξ)={B2(1A)+Δ12(1A)C1sinhΔ12ξ+C2coshΔ12ξC1coshΔ12ξ+C2sinhΔ12ξ,when Δ1=B24(A1)C>0,A1,β2(1A)+Δ22(1A)C1sinΔ22ξ+C2cosΔ22ξC1cosΔ22ξ+C2sinΔ22ξ,when Δ2=4(A1)CB2>0,A1,11A(C1C1ξ+C2+B2),when  4(A1)CB2=0,A1. (2.9)

    Then we can obtain a nonlinear algebraic equations.

    (GG)3: 6μ2γ(A1)2a1(3λ+2σ)a31=0.

    (GG)2: 9μ2γB(A1)2a13(3λ+2σ)a21a0=0.

    (GG)1: 3μ2γ[2C(A1)+B2]a13(ν+2ak+δ+3k2γ)a13(3λ+2σ)(a20a1+a21a1)=0.

    (GG)0: 3μ2γ[BCa1+B(A1)a1]3(ν+2ak+δ+3k2γ)a0(3λ+2σ)(6a20a1a1+a30)=0.

    (GG)1: 3μ2γ[2C(A1)+B2]a13(ν+2ak+δ+3k2γ)a13(3λ+2σ)(a20a1+a21a1)=0.

    (GG)2: 9μ2γB(A1)a13(3λ+2σ)a21a0=0.

    (GG)3: 6μ2γC2a1(3λ+2σ)a31=0.

    Next, we get the following the results:

    Case 1.1. a1=±6μ2γ(A1)23λ+2σ, a0=±μ2γ[B2+2C(A1)](ν+2ak+δ+3k2γ)3λ+2σ, a1=0,

    γ=μ2γ[B2+2C(A1)]+2(ν+2ak+δ+3k2γ)6μ2(A1)C.

    Case 1.2. a1=0, a0=±μ2γ[B2+2C(A1)](ν+2ak+δ+3k2γ)3λ+2σ, a1=±6μ2γC23λ+2σ,

    γ=μ2γ[B2+2C(A1)]+2(ν+2ak+δ+3k2γ)6μ2(A1)C.

    Family 1. When A1, Δ1=B2+4C4AC>0, we obtain

    ϕ1(x,t)={±μ2γ[B2+2C(A1)](ν+2ak+δ+3k2γ)3λ+2σ±3μ2γB22(3λ+2σ)±3μ2γ(B2+4C4AC)2(3λ+2σ)(C1sinhB2+4C4AC2ξ+C2coshB2+4C4AC2ξC1coshB2+4C4AC2ξ+C2sinhB2+4C4AC2ξ)}ei(kx+ϖtαα+θ). (2.10)
    ϕ2(x,t)={±μ2γ[B2+2C(A1)](ν+2ak+δ+3k2γ)3λ+2σ±6μ2γC23λ+2σ[B2+4C4AC2(1A)(C1sinhB2+4C4AC2ξ+C2coshB2+4C4AC2ξC1coshB2+4C4AC2ξ+C2sinhB2+4C4AC2ξ)+B2(1A)]1}ei(kx+ϖtαα+θ), (2.11)

    where C1 and C2 are arbitrary constants.

    Especially, if C10, and C2=0 in Eq (2.7), we have

    ϕ11(x,t)={±μ2γ[B2+2C(A1)](ν+2ak+δ+3k2γ)3λ+2σ±3μ2γB23λ+2σ±3μ2γC2(B2+4C4AC)2(3λ+2σ)tanhB2+4C4AC2ξ}ei(kx+ϖtαα+θ). (2.12)
    ϕ12(x,t)={±μ2γ[B2+2C(A1)](ν+2ak+δ+3k2γ)3λ+2σ±3μ2γB23λ+2σ±3μ2γC2(B2+4C4AC)2(3λ+2σ)cothB2+4C4AC2ξ}ei(kx+ϖtαα+θ). (2.13)
    ϕ21(x,t)={±μ2γ[B2+2C(A1)](ν+2ak+δ+3k2γ)3λ+2σ±6μ2γC23λ+2σ[B2+4C4AC2(1A)tanhB2+4C4AC2ξ+B2(1A)]1}ei(kx+ϖtαα+θ). (2.14)
    ϕ22(x,t)={±μ2γ[B2+2C(A1)](ν+2ak+δ+3k2γ)3λ+2σ±6μ2γC23λ+2σ[B2+4C4AC2(1A)cothB2+4C4AC2ξ+B2(1A)]1}ei(kx+ϖtαα+θ). (2.15)

    Family 2. When A1, and Δ2=B2+4C4AC<0, we obtain

    ϕ3(x,t)={±μ2γ[B2+2C(A1)](ν+2ak+δ+3k2γ)3λ+2σ±3μ2γB22(3λ+2σ)±3μ2γ(4ACB24C)2(3λ+2σ)(C1sin4ACB24C2ξ+C2cos4ACB24C2ξC1cos4ACB24C2ξ+C2sin4ACB24C2ξ)}ei(kx+ϖtαα+θ). (2.16)
    ϕ4(x,t)={±μ2γ[B2+2C(A1)](ν+2ak+δ+3k2γ)3λ+2σ±6μ2γC23λ+2σ[B2+4C4AC2(1A)(C1sin4ACB24C2ξ+C2cos4ACB24C2ξC1cos4ACB24C2ξ+C2sin4ACB24C2ξ)+B2(1A)]1}ei(kx+ϖtαα+θ). (2.17)

    Family 3. When A1, and B2+4C4AC=0, we obtain the rational function solution of Eq (1.1) as

    ϕ5(t,x,y)={±μ2γ[B2+2C(A1)](ν+2ak+δ+3k2γ)3λ+2σ±6μ2γ3λ+2σ(C1C1ξ+C2+B2)}ei(kx+ϖtαα+θ). (2.18)
    ϕ6(t,x,y)={±μ2γ[B2+2C(A1)](ν+2ak+δ+3k2γ)3λ+2σ±6μ2γC2(1A)23λ+2σ(C1C1ξ+C2+B2)1}ei(kx+ϖtαα+θ). (2.19)

    Now, Eq (2.4) is equivalent to the following of two dimensional system

    {Xξ(ξ)=Y(ξ),Yξ(ξ)=ν+3ak+δ+3k2γμ2γX(ξ)+3λ+2σ3μ2γX(ξ)3, (2.20)

    where Q(X,Y)=mi=0ai(X)Yi,

    P(X(ξ),Y(ξ))=mi=0ai(X)Yi=0, (2.21)

    Then, based on the division theorem, there exists a polynomial g(X)+h(X)Y in C[X,Y] such that

    dQdξ=QXdXdξ+QYdYdξ=[g(X)+h(X)Y(ξ)]mi=0ai(X)Yi(ξ). (2.22)

    Case 2.1. If m=1.

    Substituting Eq (2.21) into Eq (2.22) and calculating the coefficients of Yi(ξ)=(i=0,1,2) both sides of Eq (2.22), we have

    g(X)a0(X)=a1(X)[(ν+3ak+δ3k2γ)μ2γX(ξ)(3λ+2σ)3μ2γX(ξ)3]. (2.23)
    da0(X)dX=g(X)a1(X)+h(X)a0(X). (2.24)
    da1(X)dX=h(X)a1(X). (2.25)

    Since ai(X)(i=0,1) are polynomials, then we obtain when deg(g(X))=1

    g(X)=A1(X)+B0. (2.26)
    a0(X)=12A1(X)2+B0(X)+A0. (2.27)

    Substitutinga0(X),a1(X),g(X) into Eq (2.23) and setting all the coefficients of powers X to be zero, then, we obtain

    A1=±2(3λ+2σ)3μ2γ,B0=0,A0=±ν+3ak+δ3k2γ23(3λ+2σ)μ2γ. (2.28)

    Using the conditions Eq (2.28) in Eq (2.21), we obtain

    X(ξ)=±ν+3ak+δ3k2γ23(3λ+2σ)μ2γ(3λ+2σ)6μ2γX2(ξ). (2.29)

    Combining Eq (2.29) with Eq (2.20), we obtain the exact solution for FPRKL equation which can be written as

    Type 1. If c+3ak+δ3k2γγ<0,(3λ+2σ)γ<0, we get

    ϕ7(x,t)=±ν+3ak+δ3k2γ3λ+2σtanh(ν+3ak+δ3k2γ2μ2γξεlnξ02)ei(kx+ϖtαα+θ),if ξ0>0. (2.30)
    ϕ8(x,t)=±ν+3ak+δ3k2γ3λ+2σcoth(ν+3ak+δ3k2γ2μ2γξεlnξ02)ei(kx+ϖtαα+θ),if ξ0<0. (2.31)
    ϕ9(x,t)=±ν+3ak+δ3k2γ3λ+2σei(kx+ϖtαα+θ),if ξ0=0. (2.32)

    Type 2. If c+3ak+δ3k2γγ>0,(3λ+2σ)γ>0, we get

    ϕ10(x,t)=±ν+3ak+δ3k2γ3λ+2σtan(ν+3ak+δ3k2γ2μ2γξ+ξ0)ei(kx+ϖtαα+θ). (2.33)
    ϕ11(x,t)=±ν+3ak+δ3k2γ3λ+2σcot(ν+3ak+δ3k2γ2μ2γξ+ξ0)ei(kx+ϖtαα+θ). (2.34)

    Type 3. If ν+3ak+δ3k2γγ=0,(3λ+2σ)γ<0, we get

    ϕ12(x,t)=±13λ+2σ6μ2γξ+ξ0ei(kx+ϖtαα+θ). (2.35)

    Case 2.2. If m=2.

    Comparing the coefficients of Yi(ξ)=(0,1,2,3) on both sides of Eq (2.22), we obtain

    g(X)a0(X)=a1(X)[(ν+3ak+δ3k2γ)μ2γX(ξ)(3λ+2σ)3μ2γX(ξ)3]. (2.36)
    da0(X)dX+2a2(X)[ν+3ak+δ3k2γμ2γX(ξ)+(3λ+2σ)3μ2γX(ξ)3]=g(X)a1(X)+h(X)a0(X). (2.37)
    da1(X)dX=h(X)a1(X)+g(X)a2(X). (2.38)
    da2(X)dX=h(X)a2(X). (2.39)

    Balancing the degrees of g(X) and a1(X), we get deg(g(X))=1, deg(a1(X))=2, then

    g(X)=A1(X)+B0. (2.40)
    a1(X)=12A1(X)2+B0(X)+A0,A10, (2.41)

    where A1,A0,B0 are all constants to be determined.

    Now, Eq (2.37) becomes

    a0(X)=[3λ+2σ6μ2γ+18A21]X(ξ)4+12A1B0X(ξ)3+[ν+3ak+δ3k2γμ2γ+12A1A0+12B20]X(ξ)2+A0B0X(ξ)+d, (2.42)

    where d is the constant of integration.

    Substituting a0(X),g(X),a1(X) into Eq (2.36) and setting all the coefficients of powers X to be zero, we obtain

    A1=±22(3λ+2σ)3μ2γ, B0=0,A0=±6(ν+3ak+δ3k2γ)(3λ+2σ)μ2γ,d=(ν+3ak+δ3k2γ)22(3λ+2σ)μ2γ. (2.43)

    From Eq (2.43) into Eq (2.21), we obtain

    X(ξ)=±6(ν+3ak+δ3k2γ)2(3λ+2σ)μ2γ±2(3λ+2σ)3μ2γX2(ξ). (2.44)

    This shows that the two cases m=1 and m=2 give the same solutions.

    Multiplying u on both sides of Eq (2.4), and again integrating it on ξ, we can get

    (u)2=a4u4+a2u2+a0, (2.45)

    where a4=3λ+2σ6μ2γ, a2=ν+2ak+δ3k2γμ2γ, and a0 is the constant.

    Making the transformation ψ=±(2(3λ+2σ)3μ2γ)13u, ξ1=(2(3λ+2σ)3μ2γ)13ξ, Eq (2.45) becomes

    (ψ)2=ψ(ψ2+p1ψ+p0), (2.46)

    where p1=4(ν+2ak+δ3k2γ)μ2γ(2(3λ+2σ)3μ2γ)23, p0=4a0(2(3λ+2σ)3μ2γ)13.

    Integrating Eq (2.46), we have

    ±(ξ1ξ0)=duψ(ψ2+p1ψ+p0), (2.47)

    where ξ0 is the integration constant.

    Suppose that Δ=p214p0 and G(ψ)=ψ2+p1ψ+p0, there are four cases for the solutions of Eq (2.4).

    Case 3.1. Δ=0.

    When ψ>0, we have

    ±(ξ1ξ0)=dψψ(ψ+p12). (2.48)

    If p1<0, the corresponding solutions are

    ϕ16(x,t)=±[3(ν+2ak+δ3k2γ)3λ+2σ]12tanh{[18(ν+2ak+δ3k2γ)μ2γ(3λ+2σ)2]16[(2(3λ+2σ)3μ2γ)13ξξ0]}ei(kx+ϖtαα+θ). (2.49)
    ϕ17(x,t)=±[3(ν+2ak+δ3k2γ)3λ+2σ]12coth{[18(ν+2ak+δ3k2γ)μ2γ(3λ+2σ)2]16[(2(3λ+2σ)3μ2γ)13ξξ0]}ei(kx+ϖtαα+θ). (2.50)

    If p1>0, the corresponding solutions are

    ϕ18(x,t)=±[3(ν+2ak+δ3k2γ)3λ+2σ]12tan{[18(ν+2ak+δ3k2γ)μ2γ(3λ+2σ)2]16[(2(3λ+2σ)3μ2γ)13ξξ0]}ei(kx+ϖtαα+θ). (2.51)

    If p1=0, we get the corresponding solutions

    ϕ19(x,t)=1[2(3λ+2σ)3μ2γ]12ξ[2(3λ+2σ)3μ2γ]16ξ0ei(kx+ϖtαα+θ). (2.52)

    Case 3.2. Δ>0 and p0=0. As for ψ>p1, we have

    ±(ξ1ξ0)=dψψψ+p1. (2.53)

    If p1>0, the solutions are given as follows

    ϕ20(x,t)=±[3(ν+2ak+δ3k2γ)3λ+2σ]12{tanh2[(18(ν+2ak+δ3k2γ)μ2γ(3λ+2σ)2)16((2(3λ+2σ)3μ2γ)13ξξ0)]1}ei(kx+ϖtαα+θ). (2.54)
    ϕ21(x,t)=±[3(ν+2ak+δ3k2γ)3λ+2σ]12{coth2[(18(ν+2ak+δ3k2γ)μ2γ(3λ+2σ)2)16((2(3λ+2σ)3μ2γ)13ξξ0)]1}ei(kx+ϖtαα+θ). (2.55)

    If p1<0, the solutions are given as follows

    ϕ22(x,t)=±[3(ν+2ak+δ3k2γ)3λ+2σ]12{tan2[(18(ν+2ak+δ3k2γ)μ2γ(3λ+2σ)2)16((2(3λ+2σ)3μ2γ)13ξξ0)]1}ei(kx+ϖtαα+θ). (2.56)

    Case 3.3. Δ>0, p00.

    Suppose that λ1<λ2<λ3, λ1, λ2 and λ3 are two roots of G(ψ)=0. Here we make the transformation ψ=λ1+(λ2λ1)sin2φ, it is clear that

    ±(ξ1ξ0)=2λ3λ1dψ1m21sin2φ, (2.57)

    where m21=λ2λ1λ3λ1. We get the corresponding solutions

    ϕ23(x,t)=±[3μ2γ2(3λ+2σ)]16{λ1+(λ2λ1)sn2[λ3λ12((2(3λ+2σ)3μ2γ)13ξξ0),m1]}12ei(kx+ϖtαα+θ). (2.58)

    If ψ>λ3, we take the following transformation ψ=λ2sin2φ+λ3cos2φ, the corresponding solutions are

    ϕ24(x,t)=±[3μ2γ2(3λ+2σ)]16{λ2sn2(λ3λ1((2(3λ+2σ)3μ2γ)13ξξ0)/2,m1)γcn2(λ3λ1((2(3λ+2σ)3μ2γ)13ξξ0)/2,m1)}12ei(kx+ϖtαα+θ). (2.59)

    Case 3.4. Δ<0, taking the transformation ψ=p0tan2φ2 it is clear that

    ±2(ξ1ξ0)=p140dψ1m22sin2φ, (2.60)

    where m22=12(1p12p0). we get the corresponding solutions

    ϕ25(x,t)=±(6μ2γa03λ+2σ)14{21+cn[(192a30μ2γ3λ+2σ)112((2(3λ+2σ)3μ2γ)13ξξ0),m2]1}12ei(kx+ϖtαα+θ). (2.61)

    In this section, the numerical simulations of some remarkable solutions for the FPRKL equation are presented. By the (G/G)-expansion method, we obtained the solution ϕ11(x,t) and ϕ12(x,t) shown in Figure 1. The graphical solutions ϕ10(x,t) and ϕ11(x,t) are shown in Figure 2. Moreover, the graphical solutions ϕ16(x,t) and ϕ17(x,t) are shown in Figure 3.

    Figure 1.  The hyperbolic function solutions of Eq (1.1), when ϖ=2, λ=1, δ=1, σ=1, k=1,μ=3,a=1,γ=1,A=1,B=2,C=1,α=12, (a)the hyperbolic function solutions ϕ11(x,t), (b) the hyperbolic function solutions ϕ12(x,t).
    Figure 2.  The trigonometric function solutions of Eq (1.1), when λ=1, δ=1, σ=1, μ=1,a=1,γ=1,b=223, (a)the trigonometric function solutions ϕ10(x,t), (b)the trigonometric function solutions ϕ11(x,t).
    Figure 3.  The hyperbolic function solutions of Eq (1.1), when λ=1, γ=1, δ=1, σ=1,a=1,b=143,μ=1,ξ0=0, (a)the hyperbolic function solutions ϕ16(x,t), (b) the hyperbolic function solutions ϕ17(x,t).

    In this article, we have investigated the exact solutions to the FPRKL equation by three different methods. Many exact solutions have been obtained. In the paper, we get all the traveling wave solutions, which have not been seen in other literature. These solutions might be further useful and effective to study more about the various forms of solitary waves in physics. We have noticed that the proposed complete discrimination system for the polynomial method gives much more new and general exact solutions than the other two suggested methods. In future work, we will consider the bifurcation, phase diagrams and exact solutions of the FPRKL equation.

    This work was supported by Science Research Fund of Education Department of Sichuan Province of China under grant No.18ZB0537 and Scientific Research Funds of Sichuan Vocational and Technical College under grant No.2022YZB009.

    The author declare no conflict of interest.



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