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Review

State of the art in carbon taxes: a review of the global conclusions

  • Received: 28 September 2020 Accepted: 20 November 2020 Published: 24 November 2020
  • JEL Codes: H23, P48, Q01, Q38, Q50, Q54

  • Carbon taxes have been advocated as a key economic measure for the reduction of greenhouse gas emissions. The basis of this proposition,is the economic theory that applying a tax on carbon dioxide emissions is the "optimal" solution to addressing the market failure of externalities. In moving from theory to practice,the evidence from comprehensive global assessments,over the last three decades,covering actual policy experience and empirical study of policy effects,requires evolution and refinement of the theory. Carbon taxes are not adopted at the scale,coverage or price level necessary to effectively reduce emissions in line with the Paris Agreement. A persistent "implementation gap" has arisen,largely due to the political and social challenges that accompany taxation. Assessments of policy experience in key sectors of built environment,transport and industry,highlight the critical role of regulation,standards and technology among broader policy programmes. While a carbon tax can provide simplicity and scope,it is not sufficient on its own. Consistent with this finding,recent modelling innovations show that taxes can be employed as part of a portfolio of best practice policies and measures,for deep reduction of emissions. Portfolios can facilitate application of a lower,more "moderate" carbon tax,which enhances the social acceptability and political feasibility of the tax itself. When designing a tax,revenue recycling can help with policy resistance,delivering the "double dividend" of economic and climate gains,and addressing distributional considerations. A carbon tax may be useful to complement the broader portfolio of policies and measures accepted as necessary for long-term transition and transformation. It can offer support and prevent rebounds,but is not a substitute for the fundamental systems change that is at the core of addressing urgent sustainability crises.

    Citation: Tadhg O'Mahony. State of the art in carbon taxes: a review of the global conclusions[J]. Green Finance, 2020, 2(4): 409-423. doi: 10.3934/GF.2020022

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  • Carbon taxes have been advocated as a key economic measure for the reduction of greenhouse gas emissions. The basis of this proposition,is the economic theory that applying a tax on carbon dioxide emissions is the "optimal" solution to addressing the market failure of externalities. In moving from theory to practice,the evidence from comprehensive global assessments,over the last three decades,covering actual policy experience and empirical study of policy effects,requires evolution and refinement of the theory. Carbon taxes are not adopted at the scale,coverage or price level necessary to effectively reduce emissions in line with the Paris Agreement. A persistent "implementation gap" has arisen,largely due to the political and social challenges that accompany taxation. Assessments of policy experience in key sectors of built environment,transport and industry,highlight the critical role of regulation,standards and technology among broader policy programmes. While a carbon tax can provide simplicity and scope,it is not sufficient on its own. Consistent with this finding,recent modelling innovations show that taxes can be employed as part of a portfolio of best practice policies and measures,for deep reduction of emissions. Portfolios can facilitate application of a lower,more "moderate" carbon tax,which enhances the social acceptability and political feasibility of the tax itself. When designing a tax,revenue recycling can help with policy resistance,delivering the "double dividend" of economic and climate gains,and addressing distributional considerations. A carbon tax may be useful to complement the broader portfolio of policies and measures accepted as necessary for long-term transition and transformation. It can offer support and prevent rebounds,but is not a substitute for the fundamental systems change that is at the core of addressing urgent sustainability crises.


    Hirota and Ito [1] proposed the following Sawada-Kotera equation to theoretically study the resonances of solitons in one dimension,

    ut+b(15u3+15uuxx+uxxxx)x=0, (1.1)

    which has a non-vanishing boundary condition

    u|x==constant. (1.2)

    Replace u by u+a15b and apply the Galilei transformation to remove ux, then Eq (1.1) changes to the KdV-Sawada-Kotera equation [2]

    ut+a(3u2+uxx)x+b(15u3+15uuxx+uxxxx)x=0, (1.3)

    where a, b are constants. It is a linear combination of the Sawada-Kotera equation and the KdV equation, with considering a=0, Eq (1.3) reduces to the Sawada-Kotera equation, when b=0, Eq (1.3) reduces to the KdV equation. In the past few years, many achievements have been made in the study of KdV-Sawada-Kotera equation. About this equation, conservation laws are investigated by Konno [3], and traveling wave solutions are discovered in [4]. Quasi-periodic wave and exact solitary wave solutions to the KdV-Sawada-Kotera equation are obtained [5].

    As we know, nonlinear differential equations (NLDEs) are widely utilized in fluid dynamics, solid state physics, plasma physics, biology, nonlinear optics, chemistry and so on. The study to exact solutions of various NLDEs is extremely important in modern mathematics with ramifications to some areas of physics, mathematics and other sciences. There are many systematic methods to seek exact solutions of NLDEs, for example, Hirota bilinear method [6,7], modified simple equation method [8], generalized (G/G)-expansion method [9,10], modified Kudryashov method [11,12], exp function method [13,14], modified extended tanh method [15,16], sine-Gordon expansion method [17,18], extended sine-Gordon expansion method [19,20], complex method [21,22,23,24] and exp(ψ(z))-expansion method [25,26,27,28].

    Eremenko showed that all meromorphic solutions of the Kuramoto Sivashinsky equation are elliptic function and its degeneration in [29]. After that, Laurent series were applied by Kudryashov et al. [30,31] to obtain meromorphic exact solutions to certain nonlinear differential equations. On the basis of their work, Yuan et al. [32,33] established the complex method combining the theories of complex analysis and complex differential equations. It is a powerful approach to obtain exact solutions for NLDEs that admit p,q condition or are Briot-Bouquet (BB) equations [34]. Following their work, we propose the extended complex method to get meromorphic exact solutions for NLDEs which neither admit p,q condition nor BB equations. Therefore, the extended complex method is an enhancement of the complex method and should deal with more NLDEs in applied sciences.

    The exp(ψ(z))-expansion approach is an effectual technique to seek analytical solutions for NLDEs. A lot of researchers, for instance, Jafari, Khan, Roshid, etc [25,26,27,28], made good use of this method to study NLDEs. In this article, we utilize two different systematic methods mentioned above to seek meromorphic exact solutions of the KdV-Sawada-Kotera equation. Dynamic behaviors of the solutions are shown by some graphs in which the profiles of Weierstrass elliptic function solutions have never been shown in former literatures.

    Consider the following nonlinear PDE:

    P(u,ux,ut,uxx,utt,)=0, (2.1)

    where P is a polynomial consisted by the unknown function u(x,t) as well as its partial derivatives.

    Step 1. Reduce Eq (2.1) to the ODE

    F(u,u,u,u,)=0, (2.2)

    by traveling wave transform

    u(x,t)=u(z),z=kx+rt.

    Step 2. Assume that Eq (2.2) has exact solutions as follows:

    u(z)=mτ=0Bτ(exp(ψ(z)))τ, (2.3)

    where Bτ(0τm) are constants to be determined latter, such that Bm0 and ψ=ψ(z) admits the following ODE:

    ψ(z)=γ+exp(ψ(z))+μexp(ψ(z)). (2.4)

    The solutions of Eq (2.4) are given in the following.

    When γ24μ>0, μ0,

    ψ(z)=ln((γ24μ)tanh(γ24μ2(z+c))γ2μ), (2.5)
    ψ(z)=ln((γ24μ)coth(γ24μ2(z+c))γ2μ). (2.6)

    When γ24μ<0, μ0,

    ψ(z)=ln((4μγ2)tan((4μγ2)2(z+c))γ2μ), (2.7)
    ψ(z)=ln((4μγ2)cot((4μγ2)2(z+c))γ2μ). (2.8)

    When γ24μ>0, γ0, μ=0,

    ψ(z)=ln(γexp(γ(z+c))1). (2.9)

    When γ24μ=0, γ0, μ0,

    ψ(z)=ln(2(γ(z+c)+2)γ2(z+c)). (2.10)

    When γ24μ=0, γ=0, μ=0,

    ψ(z)=ln(z+c). (2.11)

    In Eqs (2.5)–(2.11), Bm0,γ,μ,c are constants. Taking the homogeneous balance between nonlinear terms and highest order derivatives of Eq (2.2) yields the positive integer m.

    Step 3. Insert Eq (2.3) into Eq (2.2) and collect the function exp(ψ(z)) to yield the polynomial to exp(ψ(z)). Letting all coefficients with same power of exp(ψ(z)) be zero to obtain a system of algebraic equations. Solving these equations, we achieve the values of Bm0,γ,μ and substitute them into Eq (2.3) as well as Eqs (2.5)–(2.11) to accomplish the determination for analytical solutions of the original PDE.

    Substituting

    u(x,t)=u(z),z=kx+rt,

    into Eq (1.3) and then integrating it we obtain

    ru+3kau2+k3au+15kbu3+15k3buu+k5bu+ζ=0. (3.1)

    where ζ is the integration constant.

    Taking the homogeneous balance between u and uu in Eq (3.1) to yields

    u(z)=B0+B1exp(ψ(z))+B2(exp(ψ(z)))2, (3.2)

    where B20, B1 and B0 are constants.

    Substituting u,uu,u,u3,u2,u into Eq.(3.1) and equating the coefficients about exp(ψ(z)) to zero, we obtain

    e0(ψ(z)):
    k5bB1γ3μ+14k5bB2γ2μ2+8k5bB1γμ2+16k5bB2μ3+15k3bB0B1μγ
    +30k3bB0B2μ2+ak3B1μγ+2ak3B22μ+15kbB03+3kaB20+rB0+ζ=0,
    e1(ψ(z)):
    B1bγ4k5+30B2bγ3k5μ+22B1bγ2k5μ+120B2bγk5μ2+30k3bB0B1μ
    +15B0B1bγ2k3+90B0B2bγk3μ+15B12bγk3μ+30B1B2bk3μ2+16B1bk5μ2
    +B1aγ2k3+6B2aγk3μ+2ak3B1μ+45B20B1bk+6B0B1ak+B1r=0,
    e2(ψ(z)):
    16B2bγ4k5+15B1bγ3k5+232B2bγ2k5μ+60B1bγk5μ+136B2bk5μ2
    +60B0B2bγ2k3+15B12bγ2k3+105B1B2bγk3μ+30B22bk3μ2+45B0B1bγk3
    +120B0B2bk3μ+30B21bk3μ+4B2aγ2k3+3B1aγk3+8B2ak3μ+45B20B2bk
    +45B0B21bk+6B0B2ak+3B21ak+B2r=0,
    e3(ψ(z)):
    130B2bγ3k5+50B1bγ2k5+440B2bγk5μ+75B1B2bγ2k3+40B1bk5μ
    +90B22bγk3μ+150B0B2bγk3+45B21bγk3+30B0B1bk3+10B2aγk3
    +150B1B2bk3μ+90B0B1B2bk+15B31bk+2B1ak3+6B1B2ak=0,
    e4(ψ(z)):
    330B2bγ2k5+60B1bγk5+60B22bγ2k3+240B2bk5μ+195B1B2bγk3
    +90B0B2bk3+30B21bk3+45B0B22bk+45B21B2bk+6B2ak3+3B22ak
    +120B22bk3μ=0,
    e5(ψ(z)):
    336B2bγk5+24B1bk5+150B22bγk3+120B1B2bk3+45B1B22bk=0,
    e6(ψ(z)):
    120B2bk5+90B22bk3+15B32bk=0.

    We solve the above algebraic equations and derive two different families:

    Family 1:

    B2=4k2,B1=4γk2,B0=5k2b(γ2+8μ)+a15b,r=k(5k4b2(γ24μ)2a2)5b, (3.3)

    where γ and μ are arbitrary constants.

    Substituting Eq (3.3) into Eq (3.2) yields

    u(z)=5k2b(γ2+8μ)+a15b4k2γexp(ψ(z))4k2(exp(ψ(z)))2. (3.4)

    Applying Eqs (2.5)–(2.11) into Eq (3.4) respectively, we get the following exact solutions of the KdV-Sawada-Kotera equation.

    Family 1.1: When γ24μ>0, μ0,

    u11(z)=5k2b(γ2+8μ)+a15b+8k2γμ(γ24μ)tanh(γ24μ2(z+c))+γ
    16k2μ2((γ24μ)tanh(γ24μ2(z+c))+γ)2,
    u12(z)=5k2b(γ2+8μ)+a15b+8k2γμ(γ24μ)coth(γ24μ2(z+c))+γ
    16k2μ2((γ24μ)coth(γ24μ2(z+c))+γ)2.

    Family 1.2: When γ24μ<0, μ0,

    u13(z)=5k2b(γ2+8μ)+a15b8k2γμ(4μγ2)tan(4μγ22(z+c))γ
    16k2μ2((4μγ2)tan(4μγ22(z+c))γ)2,
    u14(z)=5k2b(γ2+8μ)+a15b8k2γμ(4μγ2)cot(4μγ22(z+c))γ
    16k2μ2((4μγ2)cot(4μγ22(z+c))γ)2.

    Family 1.3: When γ24μ>0, γ0, μ=0,

    u15(z)=5k2bγ2+a15b4k2γ2exp(γ(z+c))14k2γ2(exp(γ(z+c))1)2.

    Family 1.4: When γ24μ=0, γ0, μ0,

    u16(z)=60k2bμ+a15b+2k2γ3(z+c)γ(z+c)+2k2γ4(z+c)2(γ(z+c)+2)2.

    Family 1.5: When γ24μ=0, γ=0, μ=0,

    u17(z)=a15b4k2(z+c)2.

    Family 2:

    B2=2k2,B1=2γk2,B0=2a+5k2b(γ2+8μ)30b,r=k(4a2+5k4b2(γ24μ)2)20b, (3.5)

    where γ and μ are arbitrary.

    Substituting Eq (3.5) into Eq (3.2) yields

    u(z)=2a+5k2b(γ2+8μ)30b2k2γexp(ψ(z))2k2(exp(ψ(z)))2. (3.6)

    Applying Eqs (2.5)–(2.11) into Eq (3.6) respectively, we get the following exact solutions of the KdV-Sawada-Kotera equation.

    Family 2.1: When γ24μ>0, μ0,

    u21(z)=2a+5k2b(γ2+8μ)30b+4k2γμ(γ24μ)tanh(γ24μ2(z+c))+γ
    8k2μ2((γ24μ)tanh(γ24μ2(z+c))+γ)2,
    u22(z)=2a+5k2b(γ2+8μ)30b+4k2γμ(γ24μ)coth(γ24μ2(z+c))+γ
    8k2μ2((γ24μ)coth(γ24μ2(z+c))+γ)2.

    Family 2.2: When γ24μ<0, μ0,

    u23(z)=2a+5k2b(γ2+8μ)30b4k2γμ(4μγ2)tan(4μγ22(z+c))γ
    8k2μ2((4μγ2)tan(4μγ22(z+c))γ)2,
    u24(z)=2a+5k2b(γ2+8μ)30b4k2γμ(4μγ2)cot(4μγ22(z+c))γ
    8k2μ2((4μγ2)cot(4μγ22(z+c))γ)2.

    Family 2.3: When γ24μ>0, γ0, μ=0,

    u25(z)=2a+5k2bγ230b2k2γ2exp(γ(z+c))12k2γ2(exp(γ(z+c))1)2.

    Family 2.4: When γ24μ=0, γ0, μ0,

    u26(z)=a+30k2bμ15b+k2γ3(z+c)γ(z+c)+2k2γ4(z+c)22(γ(z+c)+2)2.

    Family 2.5: When γ24μ=0, γ=0, μ=0,

    u27(z)=a15b2k2(z+c)2.

    Figures 16 show the properties of the solutions.

    Figure 1.  The 3D and 2D surfaces of u11(z) by considering the values γ=4, μ=3, k=1, r=1, c=1, b=1, a=215 and t=0 for the 2D graphic.
    Figure 2.  The 3D and 2D surfaces of u12(z) by considering the values γ=4, μ=3, k=1, r=1, c=1, b=1, a=215 and t=0 for the 2D graphic.
    Figure 3.  The 3D and 2D surfaces of u13(z) by considering the values γ=4, μ=5, k=1, r=1, c=1, b=1, a=295 and t=0 for the 2D graphic.
    Figure 4.  The 3D and 2D surfaces of u14(z) by considering the values γ=4, μ=5, k=1, r=1, c=1, b=1, a=295 and t=0 for the 2D graphic.
    Figure 5.  The 3D and 2D surfaces of u15(z) by considering the values γ=1, μ=0, k=1, r=1, c=1, b=1, a=20 and t=0 for the 2D graphic.
    Figure 6.  The 3D and 2D surfaces of u16(z) by considering the values γ=1, μ=14, k=1, r=1, c=1, b=1, a=30 and t=0 for the 2D graphic.

    Step 1. Substitute the transformation I:u(x,t)U(z), (x,t)z into a nonlinear PDE to yield an ODE

    G(U,U,U,)=0. (4.1)

    Step 2. Determination of the weak p,q condition.

    Assume that the meromorphic solutions U of Eq (4.1) have at least one pole and let q,pN. Substitute the Laurent series

    U(z)=k=qTkzk,Tq0,q>0, (4.2)

    into Eq (4.1) to determine p distinct Laurent principal parts

    1k=qTkzk,

    then we say that the weak p,q condition of Eq (4.1) holds.

    It is know that Weierstrass elliptic function (z):=(z,g2,g3) has double periods and satisfies:

    ((z))2=4(z)3g2(z)g3,

    and it admit an addition formula [35] as follows:

    (zz0)=(z)+14[(z)+(z0)(z)(z0)]2(z0).

    Step 3. Substituting the indeterminate forms

    U(z)=h1i=1qj=2(1)jβij(j1)!dj2dzj2(14((z)+Di(z)Ci)2(z))+h1i=1βi12(z)+Di(z)Ci
    +qj=2(1)jβhj(j1)!dj2dzj2(z)+β0, (4.3)
    U(z)=hi=1qj=1βij(zzi)j+β0, (4.4)
    U(eαz)=hi=1qj=1βij(eαzeαzi)j+β0, (4.5)

    into Eq (4.1) respectively yields a set of algebraic equations, and then solving these equations, we achieve elliptic function solutions, simply periodic solutions and rational function solutions with a pole at z=0, in which D2i=4C3ig2Cig3, βij are determined by (4.2), and hi=1βi1=0, and R(z), R(eαz)(αC) have h(p) distinct poles of multiplicity q.

    Step 4. Derive the meromorphic solutions at arbitrary pole, and insert the inverse transform I1 back to the meromorphic solutions to obtain exact solutions of the given PDE.

    Inserting (4.2) into Eq.(3.1) yields

    T2=4k2,T1=0,T0=a15b,T1=0,T2=5rbka2300k3b2,

    and

    T2=2k2,T1=0,T0=a15b,T1=0,T2=ka25rb150k3b2,

    Therefore we know that p=2,q=2, then the weak 2,2 condition of Eq (3.1) hold.

    By the weak 2,2 condition and (4.3), we have the form of the elliptic solutions of Eq (3.1)

    U10(z)=β2(z)+β20,

    with pole at z=0.

    Substituting U10(z) into Eq (3.1) yields

    4i=1c1ii1(z)=0, (5.1)

    where

    c11=12k5bβ2g3152k3bβ2β20g2+15kbβ320+3kaβ22012ak3β2g2+rβ20+ζ,
    c12=18k5bβ2g2152k3bβ22g2+45kbβ2β220+6kaβ2β20+rβ2,
    c13=90k3bβ2β20+6ak3β2+45bkβ22β20+3akβ22,
    c14=120bk5β2+90bk3β22+15bkβ32.

    Equate the coefficients of all powers of (z) in Eq (5.1) to zero to achieve one set of algebraic equations:

    c11=0,c12=0,c13=0,c14=0.

    Solve the above equations, then

    β2=4k2,β20=a15b,g2=a2k5br60b2k5,g3=2a3k+225ζb215abr10800b3k7,

    and

    β2=2k2,β20=a15b,g2=5bra2k15b2k5,g3=2a3k+225ζb215abr5400b3k7,

    then

    U11,0(z)=4k2(z)a15b,

    and

    U12,0(z)=2k2(z)a15b.

    Thus, elliptic solutions of Eq (3.1) with arbitrary pole are

    U11(z)=4k2(zz0)a15b,

    and

    U12(z)=2k2(zz0)a15b,

    where z0C.

    Use the addition formula to U11(z) and U12(z), then

    U11(z)=4k2(z)k2((z)+D(z)C)2+60k2bCa15b,

    and

    U12(z)=2k2(z)k22((z)+D(z)C)2+30k2bCa15b,

    where C2=4D3g2Dg3. g2=a2k5bμ60b2k5,g3=2a3k+225ζb215abμ10800b3k7 in the former case, g2=5bra2k15b2k5,g3=2a3k+225ζb215abr5400b3k7 in the latter case.

    By (4.4) and the weak 2,2 condition, we have the indeterminate form of rational solutions

    U20(z)=β12z2+β11z+β10,

    with pole at z=0.

    Substituting U20(z) into Eq (3.1) yields

    7i=1c2izi7=0, (5.2)

    where

    c21=120bk5β12+90bk3β122+15bkβ123,
    c22=24bk5β11+120bk3β11β12+45bkβ11β122,
    c23=90bk3β10β12+30bk3β112+6ak3β12+45bkβ10β122+45bkβ112β12+3akβ122,
    c24=30bk3β10β11+2ak3β11+90bkβ10β11β12+15bkβ113+6akβ11β12,
    c25=45bkβ102β12+45bkβ10β112+6akβ10β12+3akβ112+rβ12,
    c26=45bkβ102β11+6akβ10β11+rβ11,
    c27=15kbβ103+3kaβ102+rβ10+ζ.

    Equate the coefficients of all powers of z in Eq (5.2) to zero to achieve a system of algebraic equations:

    c21=0,c22=0,c23=0,c24=0,c25=0,c26=0,c27=0.

    Solving the above equations, we get

    β12=4k2,β11=0,β10=a15b,

    and

    β12=2k2,β11=0,β10=a15b,

    then

    U21,0(z)=4k2z2a15b,

    and

    U22,0(z)=2k2z2a15b,

    where r=ka25b, ζ=ka3225b2.

    Insert U(z)=R(η) into Eq (3.1) to yield

    k5bα4(R(4)η4+6Rη3+7Rη2+Rη)+15k3bα2R(ηR+η2R)
    +15kbR3+3kaR2+ak3α2(ηR+η2R)+rR+ζ=0, (5.3)

    where η=eαz (αC).

    Substituting

    U30(z)=b12(eαz1)2+b11eαz1+b10,

    into the Eq (5.3), we have

    7i=1c3iα2e(7i)αz(eαz1)6=0, (5.4)

    in which

    c31=15bkb310+3akb210+rb10+ζ,
    c32=α4bk5b11+15α2bk3b10b11+aα2k3b1190bkb310+45bkb210b1118akb210
    +6akb10b116rb10+rb116ζ,
    c33=10α4bk5b11+16α4bk5b1230α2bk3b10b11+60α2bk3b10b12+15α2bk3b211
    2aα2k3b11+4aα2k3b12+225bkb103225bkb102b11+45bkb102b12+45bkb10b211
    +45akb21030akb10b11+6akb10b12+3kab211+15rb105rb11+rb12+15ζ,
    c34=66α4bk5b1290α2bk3b10b1215α2bk3b112+75α2bk3b11b126aα2k3b12
    300bkb310+450bkb210b11180bkb210b12180bkb10b211+90bkb10b11b12+15kbb311
    +60akb10b1124akb10b1212kab211+6akb11b1220rb10+10rb114rb1220ζ
    60akb210,
    c35=10α4bk5b11+36α4bk5b12+30α2bk3b10b1115α2bk3b21130α2bk3b11b12
    +60α2bk3b212+2aα2k3b11+225bkb310450bkb210b11+270bkb210b12+270bkb10b211
    270bkb10b11b12+45bkb10b21245kbb311+45bkb211b12+45akb21060akb10b11
    +36akb10b12+18kab21118akb11b12+3kab212+15rb1010rb11+6rb12+15ζ,
    c36=α4bk5b11+2α4bk5b1215α2bk3b10b11+30α2bk3b10b12+15α2bk3b211
    45α2bk3b11b12+30α2bk3b212aα2k3b11+2aα2k3b1290bkb310+18akb11b12
    +225bkb210b11180bkb210b12180bkb10b211+270bkb10b11b12+45kbb3116rb10
    90bkb211b12+45bkb11b21218akb210+30akb10b1124akb10b126kab212+5rb11
    12kab21190bkb10b2124rb126ζ,
    c37=15bkb31045bkb210b11+45bkb210b12+45bkb10b21190bkb10b11b12+45bkb10b212
    15kbb311+45bkb211b1245bkb11b212+15kbb312+3akb1026akb10b11+6akb10b12
    +3kab2116akb11b12+3kab212+rb10rb11+rb12+ζ.

    Equate the coefficients of all powers about eαz in Eq (5.4) to zero to achieve a system of algebraic equations:

    c31=0,c32=0,c33=0,c34=0,c35=0,c36=0,c37=0.

    Solving the above equations, we get

    b12=4k2α2,b11=4k2α2,b10=5k2bα2+a15b,
    r=(5α4b2k4+a2)k5b,ζ=(10α4b2k45aα2bk2+a2)k(5α2bk2+a)225b2,

    and

    b12=2k2α2,b11=2k2α2,b10=5k2bα2+a15b,
    r=(5α4b2k4+a2)k5b,ζ=(10α4b2k45aα2bk2+a2)k(5α2bk2+a)225b2.

    So simply periodic solutions of Eq (3.1) with pole at z=0 are

    U31,0(z)=4k2α2(eαz1)24k2α2(eαz1)5k2bα2+a15b
    =4k2α2eαz(eαz1)25k2bα2+a15b
    =k2α2coth2αz2+10k2bα2a15b,

    and

    U32,0(z)=2k2α2(eαz1)22k2α2(eαz1)5k2bα2+a15b
    =2k2α2eαz(eαz1)25k2bα2+a15b
    =k2α22coth2αz2+5k2bα22a30b.

    Similar to U30(z), we substitute

    U40(z)=b12(eαz+1)2+b11eαz+1+b10,

    into the Eq (5.3) to yield

    b12=4k2α2,b11=4k2α2,b10=5k2bα2+a15b,
    r=(5α4b2k4+a2)k5b,ζ=(10α4b2k45aα2bk2+a2)k(5α2bk2+a)225b2,

    and

    b12=2k2α2,b11=2k2α2,b10=5k2bα2+a15b,
    r=(5α4b2k4+a2)k5b,ζ=(10α4b2k45aα2bk2+a2)k(5α2bk2+a)225b2,

    then

    U41,0(z)=4k2α2(eαz+1)2+4k2α2(eαz+1)5k2bα2+a15b
    =4k2α2eαz(eαz+1)25k2bα2+a15b
    =k2α2tanh2αz2a10k2bα215b,

    and

    U42,0(z)=2k2α2(eαz+1)2+2k2α2(eαz+1)5k2bα2+a15b
    =2k2α2eαz(eαz+1)25k2bα2+a15b
    =k2α22tanh2αz22a5k2bα230b.

    Substituting

    U50(z)=b14(eαz1)2+b13(eαz+1)2+b12eαz1+b11eαz+1+b10,

    into the Eq (5.3) to yield

    b144k2α2,b13=4k2α2,b12=4k2α2,b11=4k2α2,b10=2(5k2bα2+a)15b,
    r=(5α4b2k4+a2)k5b,ζ=(10α4b2k45aα2bk2+a2)k(5α2bk2+a)225b2,

    and

    b142k2α2,b13=2k2α2,b12=2k2α2,b11=2k2α2,b10=2(5k2bα2+a)15b,
    r=(5α4b2k4+a2)k5b,ζ=(10α4b2k45aα2bk2+a2)k(5α2bk2+a)225b2,

    then

    U51,0(z)=4k2α2(eαz1)24k2α2(eαz+1)24k2α2(eαz1)+4k2α2(eαz+1)2(5k2bα2+a)15b
    =4k2α2eαz(eαz1)2+4k2α2eαz(eαz+1)22(5k2bα2+a)15b,

    and

    U52,0(z)=2k2α2(eαz1)22k2α2(eαz+1)22k2α2(eαz1)+2k2α2(eαz+1)2(5k2bα2+a)15b
    =2k2α2eαz(eαz1)2+2k2α2eαz(eαz+1)22(5k2bα2+a)15b.

    Collecting meromorphic solutions of Eq (3.1) in above procedures, we have the following solutions with arbitrary pole:

    (1)U11(z)=4k2(z)k2((z)+D(z)C)2+60k2bCa15b,
    (2)U12(z)=2k2(z)k22((z)+D(z)C)2+30k2bCa15b,

    where C2=4D3g2Dg3, g2=a2k5bμ60b2k5,g3=2a3k+225ζb215abμ10800b3k7 in the former case, g2=5bra2k15b2k5,g3=2a3k+225ζb215abr5400b3k7 in the latter case;

    (3)U21(z)=4k2(zz0)2a15b,
    (4)U22(z)=2k2(zz0)2a15b,

    where r=ka25b, ζ=ka3225b2;

    (5)U31(z)=k2α2coth2α(zz0)2+10k2bα2a15b,
    (6)U32(z)=k2α22coth2α(zz0)2+5k2bα22a30b,
    (7)U41(z)=k2α2tanh2α(zz0)2a10k2bα215b,
    (8)U42(z)=k2α22tanh2α(zz0)22a5k2bα230b,
    (9)U51(z)=4k2α2eα(zz0)(eα(zz0)1)2+4k2α2eα(zz0)(eα(zz0)+1)22(5k2bα2+a)15b,
    (10)U52(z)=2k2α2eα(zz0)(eα(zz0)1)2+2k2α2eα(zz0)(eα(zz0)+1)22(5k2bα2+a)15b,

    where r=(5α4b2k4+a2)k5b,ζ=(10α4b2k45aα2bk2+a2)k(5α2bk2+a)225b2.

    Figures 711 show the properties of the solutions.

    Figure 7.  The 3D and 2D surfaces of U11(z) by considering the values k=0.28, r=0.42, a=3.79, b=4.97, D=0.032, μ=1.32, ζ=0.071 and t=0 for the 2D graphic.
    Figure 8.  The 3D and 2D surfaces of U12(z) by considering the valuesk=0.28, r=0.42, a=3.79, b=4.97, D=0.032, μ=1.32, ζ=0.071 and t=0 for the 2D graphic.
    Figure 9.  The 3D and 2D surfaces of U22(z) by considering the values k=1, r=1, b=1, a=15, z0=1 and t=0 for the 2D graphic.
    Figure 10.  The 3D and 2D surfaces of U32(z) by considering the values k=1, r=1, b=1, a=5, α=2, z0=5 and t=0 for the 2D graphic.
    Figure 11.  The 3D and 2D surfaces of U42(z) by considering the values k=1, r=1, b=1, a=5, α=2, z0=5 and t=0 for the 2D graphic.

    In this paper, we derive meromorphic exact solutions to the KdV-Sawada-Kotera equation via two different systematic methods. Five types of solutions are constructed, including hyperbolic, trigonometric, exponential, elliptic and rational function solutions. Dynamic behaviors of these solutions are given by some graphs. Observing from the figures, we know that the obtained solutions are soliton solutions. Among of them, figures 3, 7 and 8 show multiple soliton solutions, and others show singular soliton solutions. The graphs of Weierstrass elliptic function solutions U11(z) and U12(z) are more interesting and have never been shown in other literatures. We can use the ideas of this study to other differential equations in complexity and nonlinear science.

    This research is supported by the NSFC (11901111); Visiting Scholar Program of Chern Institute of Mathematics.

    The authors declare no conflict of interest.



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