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doi:10.1155/2012/236875

Research Article

Exact Traveling Wave Solutions of

Explicit Type, Implicit Type, and Parametric Type for K m, n Equation

Xianbin Wu,

1

Weiguo Rui,

2

and Xiaochun Hong

3

1Junior College, Zhejiang Wanli University, Ningbo 315100, China

2College of Mathematics, Honghe University, Mengzi, Yunnan 661100, China

3College of Statistics and Mathematics, Yunnan University of Finance and Economics, Kunming, Yunnan 650221, China

Correspondence should be addressed to Weiguo Rui,weiguorhhu@yahoo.com.cn Received 9 December 2011; Accepted 22 January 2012

Academic Editor: J. Biazar

Copyrightq2012 Xianbin Wu et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

By using the integral bifurcation method, we study the nonlinearKm, nequation for all possible values ofmandn. Some new exact traveling wave solutions of explicit type, implicit type, and parametric type are obtained. These exact solutions include peculiar compacton solutions, singular periodic wave solutions, compacton-like periodic wave solutions, periodic blowup solutions, smooth soliton solutions, and kink and antikink wave solutions. The great parts of them are different from the results in existing references. In order to show their dynamic profiles intuitively, the solutions ofKn, n,K2n−1, n,K3n−2, n,K4n−3, n, andKm,1equations are chosen to illustrate with the concrete features.

1. Introduction

In this paper, we will investigate some new traveling-wave phenomena of the following non- linear dispersiveKm, nequation1:

utσumx unxxx0, m >1, n≥1, 1.1

wheremandnare integers andσis a real parameter. This is a family of fully KdV equations.

When σ 1, 1.1as a role of nonlinear dispersion in the formation of patterns in liquid drops was studied by Rosenau and Hyman1. In2–6, the studies show that the model

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equation1.1supports compact solitary structure. In3, especially Rosenau’s study shows that the branch i.e.,σ1supports compact solitary waves and the branch−i.e.,σ−1 supports motion of kinks, solitons with spikes, cusps or peaks. In7,8, Wazwaz developed new solitary wave solutions of1.1with compact support and solitary patterns with cusps or infinite slopes under σ ±1, respectively. In 9, by using the extend decomposition method, Zhu and L ¨u obtained exact special solutions with solitary patterns for 1.1. In 10, by using homotopy perturbation method HPM, Domairry et al. studied the1.1;

under particular cases, they obtained some numerical and exact compacton solutions of the nonlinear dispersive K2,2 and K3,3 equations with initial conditions. In 11, by variational iteration method, Tian and Yin obtained new solitary solutions for nonlinear dispersive equations Km, n; under particular values of m and n, they obtained shock- peakon solutions forK2,2equation and shock-compacton solutions forK3,3equation.

In 12, the nonlinear equation Km, n is studied by Wazwaz for all possible values of mand n. In 13, by using Adomian decomposition method, Zhu and Gao obtained new solitary-wave special solutions with compact support for 1.1. In 14, by using a new method which is different from the Adomian decomposition method, Shang studied 1.1 and obtained new exact solitary-wave solutions with compact. In15,16, 1-soliton solutions of the Km, n equation with generalized evolution are obtained by Biswas. In 17, the bright and dark soliton solutions for Km, n equation with t-dependent coefficients are obtained by Triki and Wazwaz, especially, whenm n, theKn, nequation was studied by many authors; see18–24and references cited therein. Defocusing branch, Deng et al.

25obtained exact solitary and periodic traveling wave solutions ofK2,2equation. Also, under some particular values ofmandn, many authors considered some particular cases of Km, nequation. Ismail and Taha26implemented a finite difference method and a finite element method to study two types of equationsK2,2andK3,3. A single compacton as well as the interaction of compactons has been numerically studied. Then, Ismail27made an extension to the work in 26, applied a finite difference method on K2,3 equation, and obtained numerical solutions of K2,3 equation28. Frutos and Lopez-Marcos 29 presented a finite difference method for the numerical integration ofK2,2equation. Zhou and Tian 30 studied soliton solution of K2,2 equation. Xu and Tian 31 investigated the peaked wave solutions of K2,2 equation. Zhou et al. 32 obtained kink-like wave solutions and antikink-like wave solutions of K2,2 equation. He and Meng 33 obtain some new exact explicit peakon and smooth periodic wave solutions of theK3,2equation by the bifurcation method of planar systems and qualitative theory of polynomial differential system.

From the aforementioned references, and references cited therein, it has been shown that1.1is a very important physical and engineering model. This is a main reason for us to study it again. In this paper, by using the integral bifurcation method34–36, we mainly investigate some new exact solutions such as explicit solutions of Jacobian elliptic function type with low-power, implicit solutions of Jacobian elliptic function type, periodic solutions of parametric type, and so forth. We also investigate some new traveling wave phenomena and their dynamic properties.

The rest of this paper is organized as follows. In Section2, we will derive the equivalent two-dimensional planar system of 1.1 and its first integral. In Section 3, by using the integral bifurcation method, we will obtain some new traveling wave solutions and discuss their dynamic properties; some phenomena of new traveling waves are illustrated with the concrete features.

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2. The Equivalent Two-Dimensional Planar System to 1.1 and Its First Integral Equations

We make a transformationut, x φξwithξxvt, where thevis a nonzero constant as wave velocity. Thus,1.1can be reduced to the following ODE:

−vφσ φm

φn

0. 2.1

Integrating2.1once and setting the integral constant as zero yields

−vφσφmnn−1φn−2 φ2

n−1φ 0. 2.2

Letφ dφ/dξ y. Equation2.2can be reduced to a 2D planar system:

y, dy

σφmnn−1φn−2y2

n−1 , 2.3

where φ /0. Obviously, the solutions of 2.2 include the solutions of 2.3 and constant solutionφ 0. We notice that the second equation in2.3is not continuous whenφ 0;

that is, the functionφξis not defined by the singular lineφ 0. Therefore, we make the following transformation:

dξnφn−1dτ, 2.4

whereτis a free parameter. Under the transformation2.4,2.3, andφ0 combine to make one 2D system as follows:

n−1y, dy

σφmnn−1φn−2y2. 2.5 Clearly,2.5is equivalent to2.2. It is easy to know that2.3and2.5have the same first integral as follows:

y2 h 2v/n1φn1−2σ/nnm

2n−2 , 2.6

wherehis an integral constant. From2.6, we define a function as follows:

H φ, y

2n−2y2

nmφmn− 2v

n1φn1h. 2.7

It is easy to verify that2.5satisfies

1

n−1

∂H

∂y, dy

− 1 2φn−1

∂H

∂φ. 2.8

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Therefore, 2.5 is a Hamiltonian system and 1/2φn−1 is an integral factor. In fact, 2.7 can be rewritten as the form H E T, where E 1/2My2 1/2Mφ2 and T 2σ/nmn−2v/n1φn1 withM 2nφ2n−2.Edenotes kinetic energy, and T denotes potential energy. Especially, when n 1, M becomes a constant 2. In this case, the kinetic energyEonly depends on movement velocityφof particle; it does not depend on potential functionφ. So, according to Theorem 3.2 in 37, it is easy to know that2.5 is a stable and nonsingular system whenn 1; in this case its solutions have not singular characters. Whenn >1,2.5becomes a singular system; in this case some solutions of2.5 have singular characters.

For the equilibrium points of the system2.5, we have the following conclusion.

Case 1. Whenmis even number,2.5has two equilibrium pointsO0,0andA0v/σ1/m−1,0. From2.7, we obtain

hOH0,0 0, hA0 − 2vm−1 mnn1

v σ

n1/m−1

. 2.9

Case 2. Whenmis odd number andσv > 0,2.5has three equilibrium pointsO0,0and A1,2±v/σ1/m−1,0. From2.7, we also obtainhO H0,0 0 and

hA1− 2m−1v mnn1

v σ

n1/m−1

, hA2 −1n2 2m−1v mnn1

v σ

n1/m−1

. 2.10 Obviously, if nis odd, then hA1 hA2. Ifnis even, thenhA1/hA2. ThenhO H0,0 0 whethermis odd number or even number.

3. Exact Solutions of Explicit Type, Implicit Type, and Parametric Type and Their Properties

3.1. Exact Solutions and Their Properties of 1.1underhhO

TakinghhO 0,2.6can be reduced to

y2 2v/n1φn1−2σ/nnm

2n−2 . 3.1

iWhenmn >1,3.1can be rewritten as

y±

2nv/n1φn1σφ2n

n−1 . 3.2

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Substituting3.2into the first expression in2.5yields

±φ

2nv

n1φn−1σ φn−12

. 3.3

Noticing that equation 2nv/n1φn−1σφn−12 0 has two roots φ 0 andφ 2nv/n1σ1/n−1, we take2nv/n1σ1/n−1,0as the initial value. Using this initial value, integrating3.2yields

φ

2nv/n1σ1/n1

φ

2nv/n1φn−1σ

φn−12 ± τ

0

dτ. 3.4

After completing the aforementioned integral, we solve this equation; thus we obtain

φ 2nn1v

n2n−12v2τ2 n12σ 1/n−1

. 3.5

Substituting3.5into2.4, then integrating it yields

ξ 2n

n−1√

σarctan

nn−1v n1√

στ

, σ >0,

ξ− 2n

n−1√

−σtanh−1

nn−1v n1√

−στ

, σ <0.

3.6

Thus, we respectively obtain a periodic wave solution and solitary wave solution of parametric type for the equationKn, nas follows:

uφτ 2nn1v

n2n−12v2τ2 n12σ 1/n−1

,

ξ 2n

n−1√

σarctan

nn−1v n1√

στ

, σ >0,

3.7

uφτ 2nn1v

n2n−12v2τ2 n12σ 1/n−1

,

ξ− 2n

n−1√

−σtanh−1

nn−1v n1√

−στ

, σ <0.

3.8

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On the other hand,3.1can be rewritten as

y±

2nv/n1φn−1σφ2n−1

n−2 . 3.9

Using2nv/n1σ1/n−1,0as the initial value, substituting3.9into the first expression in2.3directly, we obtain an integral equation as follows:

φ

2nv/n1σ1/n−1

n−2

2nv/n1φn−1σφ2n−1 ±

ξ

0

dξ. 3.10

Completing the aforementioned integral equation, then solving it, we obtain a periodic solu- tion and a hyperbolic function solution as follows:

ux, t φξ

2nv

n1σcos2n−1√ σ

2n ξ

1/n−1

, σ >0, 3.11

ux, t φξ

2nv

n1σcosh2n−1√

−σ

2n ξ

1/n−1

, σ <0. 3.12

Obviously, the solution3.7is equal to the solution3.11; also the solution3.8is equal to the solution3.12. Similarly, taking the0,0as initial value, substituting3.9into the first expression in2.3, then integrating them, we obtain another periodic solution and another hyperbolic function solution ofKn, nequation as follows.

ux, t φξ

2nv

n1σsin2n−1√ σ

2n ξ

1/n−1

, σ >0, 3.13

ux, t φξ

2nv

n1σsinh2n−1√

−σ

2n ξ

1/n−1

, σ <0. 3.14

In fact, the solutions3.11and3.13have been appeared in35, so we do not list similar solutions anymore at here. Next, we discuss a interesting problem as follows.

When σ > 0, from3.11 and 3.13, we can construct two compacton solutions as follows:

⎧⎪

⎪⎨

⎪⎪

ux, t φξ

2nv

n1σcos2n−1√ σ

2n ξ

1/n−1

, σ >0, −

n−1 ≤ξ n−1,

0, otherwise,

3.15

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0 0.5 1 1.5 2 2.5

2 4 6

−6 −4 −2 ξ a n2

0.6 0.7 0.8 0.9 1 1.1

0 1 2 3

−3 −2 −1 ξ bn15

0.97 0.975 0.98 0.985 0.99 0.995 1

0 1 2 3

−3 −2 −1 ξ cn400

Figure 1: The solutionuin3.15shows a shape of compacton for parametersv2,andσ1.

⎧⎪

⎪⎨

⎪⎪

ux, t φξ

2nv

n1σsin2n−1√ σ

2n ξ

1/n−1

, σ >0, 0≤ξ≤ 2nπ n−1,

0, otherwise.

3.16

The shape of compacton solutions3.15and3.16changes gradually as the value of param- eternincreases. For example, whenn2,15,400, respectively, the shapes of compacton so- lution3.15are shown in Figure1.

iiWhenn1, m >1,3.1can be directly reduced to

y±φ

v− 2σ

m1φm−1. 3.17

Equation3.17 is a nonsingular equation. Using2σ/m1vn−1,0as initial value and then substituting3.17into the first expression in2.3directly, we obtain a smooth solitary wave solution and a periodic wave solution ofKm,1equation as follows:

ux, t φξ

m1v

2σ sech2m−1√ v

2 ξ

1/m−1

, v >0, 3.18

ux, t φξ

m1v

2σ sec2m−1√

−v

2 ξ

1/m−1

, v <0. 3.19

Also, the shape of solitary wave solution3.18changes gradually as the value of parameter mincreases. Whenm 2,20,200, respectively, its shapes of compacton solution3.18are shown in Figure2.

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0.5 1 1.5 2

0 1 2 3

−3 −2 −1 ξ am2

0.2 0.4 0.6 0.8 1

0 1 2 3

−3 −2 −1 ξ b m20

0.2 0.4 0.6 0.8 1

0 1 2

−2 −1 ξ cn200

Figure 2: The solutionuin3.18shows a shape of compacton for parametersv2,andσ1.

iiiWhennis even number andm2n−1,3.1can be reduced to

y±

2nv/n1φn−1−2nσ/3n−1φ3n−1

n−2 . 3.20

It is easy to know that2nv/n1φn−1−2nσ/3n−1φ3n−10 has three rootsφ0 and φ α, γwithα, γ ±

3n−1v/n1σ1/n−1whenσv >0. In fact,γ −α. Using these three roots as initial value, respectively, then substituting3.20into the first expression in 2.3, we obtain three integral equations as follows:

φ

α

n−2

2nv/n1φn−1−2nσ/3n−1φ3n−1 ± ξ

0

dξ, 0

φ

n−2

2nv/n1φn−1−2nσ/3n−1φ3n−1 ± ξ

0

dξ.

γ

φ

n−2

2nv/n1φn−1−2nσ/3n−1φ3n−1 ± ξ

0

dξ,

3.21

Completing the previous three integral equations, then solving them, we obtain three periodic solutions of Jacobian elliptic function forK2n−1, nequation as follows:

ux, t φξ αnc2

n−1√ 2α 2n ξ, 1

√2

1/n−1

, neven number, 3.22

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0 1 2 3 4 5 6

5 10 15

−15 −10 −5 ξ

aPeriodic blowup wave

5 10 15

−15 −10 −5

−1.2

−1

−0.8

−0.6

−0.4

−0.2 0 ξ

b Periodic cusp wave

0 5 10

−10 −5

−6

−5

−4

−3

−2

−1 ξ

c Periodic blowup wave Figure 3: Three periodic waves of solutions3.22,3.23, and3.24for parametersn4, v2,andσ1.

ux, t φξ

⎢⎣−αsn2

n−1√ 2α

/2n ξ,1/√

2 2dn2

n−1√ 2α

/2n ξ,1/√

2

⎥⎦

1/n−1

, neven number, 3.23

ux, t φξ

γ nc2

n−1√ 2α

/2n ξ,1/√

21/n−1

, neven number. 3.24

The solutions3.22and3.24show two shapes of periodic wave with blowup form, which are shown in Figures3aand3c. The solution3.23shows a shape of periodic cusp wave, which is shown in Figure3b.

ivWhenm3n−2, n >1,3.1can be directly reduced to

y±

2nv/n1φn−1−2nσ/4n−2 φn−14

n−2 . 3.25

It is easy to know that the function2nσ/4n−2a−φn−1φn−1−0φn−1n−1c 2nσ/4n−2a−φn−1φn−1 −0φn−1b12a21, where b1 cc/2 −a/2, a21

−c−c2/4 3a2/4. Usinga1/n−1,0and0,0as initial values, respectively, substituting 3.25into the first expression in2.3, we obtain four elliptic integral equations as follows.

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1Whenσ >0, v >0,

φ

0

n−1 aφn−1

φn−1−0

φn−1b1

2

a21 ±n−1 n

2nσ 4n−2

ξ

0

dξ. 3.26

2Whenσ >0, v <0,

φ

a1/n−1

n−1 φn−1a

φn−1−0

φn−1b1

2

a21 ±n−1 n

2nσ 4n−2

ξ

0

dξ. 3.27

3Whenσ <0, v <0,

φ

0

n−1 aφn−1

φn−1−0

φn−1b1

2

a21 ±n−1 n

2nσ 2−4n

ξ

0

dξ. 3.28

4Whenσ <0, v >0,

φ

a1/n−1

n−1 φn−1a

φn−1−0

φn−1b1

2

a21 ±n−1 n

2nσ 2−4n

ξ

0

dξ. 3.29

Corresponding to 3.26, 3.27, 3.28, and 3.29, respectively, we obtain four periodic solutions of elliptic function type forK3n−2, nequation as follows:

ux, t φξ

⎢⎣ aB

1−cn

n−1/gn

2nσ/4n−2ξ,√ 6

3−√ 3

/12 AB A−Bcn

n−1/gn

2nσ/4n−2ξ,√ 6

3−√ 3

/12

⎥⎦

1/n−1

,

3.30

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0.6 0.7 0.8 0.9 1 1.1

−10 −8 −6 −4 −2 0 2 4 6 8 10 ξ

a n10, σ1, v2

1 1.1 1.2 1.3 1.4

0 10 20

−20 −10 ξ

bn9, σ3, v0.1

Figure 4: Two different periodic waves on solutions3.30and3.31for given parameters.

ux, t φξ

⎢⎣ aB

1cn

n−1/gn

2nσ/4n−2ξ,√ 6−√

2 /4 BA ABcn

n−1/gn

2nσ/4n−2ξ,√ 6−√

2 /4

⎥⎦

1/n−1

,

3.31 ux, t φξ

⎢⎣ aB

1−cn

n−1/gn

2nσ/2n−4ξ,√ 6

3−√ 3

/12 AB ABcn

n−1/gn

2nσ/2n−4ξ,√ 6

3−√ 3

/12

⎥⎦

1/n−1

,

3.32 ux, t φξ

⎢⎣ aB

1cn

n−1/gn

2nσ/2−4nξ,√ 6−√

2 /4 BA ABcn

n−1/gn

2nσ/2−4nξ,√ 6−√

2 /4

⎥⎦

1/n−1

,

3.33 whereA

a−b12a21

3a, B

0−b12a21 a,andg 1/√

AB4

27/3awith a3

4n−2v/n1σgiven previously.

The solution3.30shows a shape of periodic wave with blowup form, which is shown in Figure4a. The solution3.31shows s shape of compacton-like periodic wave, which is shown in Figure4b. The profile of solution3.32is similar to that of solution3.30. Also the profile of solution3.33is similar to that of solution3.31. So we omit the graphs of their profiles here.

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vWhenm k−1n−k2, n >1, k >4,3.1can be directly reduced to

y±

2nv/n1φn−1−2nσ/kn−1 2φkn−1

n−2 . 3.34

Suppose thatφ0 φ0 is one of roots for equation2nv/n1φn−1 −2nσ/kn−1 2φkn−10. Clearly, the 0 is its one root. Anyone solution ofKk−1n−k2, nequation can be obtained theoretically from the following integral equations:

φ

φ0

n−1

2nv/n1φn−1−2nσ/kn−1 2

φn−1k ±n−1

n ξ. 3.35

The left integral of3.35is called hyperelliptic integral forφn−1when the degreekis greater than four. Letφn−1z. Thus,3.35can be reduced to

z

z01/n−1

dz

2nv/n1z−2nσ/kn−1 2zk ±n−1

n ξ. 3.36

In fact, we cannot obtain exact solutions by3.36when the degreekis grater than five. But we can obtain exact solutions by3.36whenk 5, v −σn1/kn−1 2, andσ < 0.

Under these particular conditions, takingφ0z01/n−10 as initial value,3.36becomes Z

0

dz

zz5 ±n−1 n

σn1

5n−3 ξ. 3.37

Letz 1/2ρ−

ρ2−4, andz 1Z2/Z2 . We obtain−dz/z√

z 1/21/

ρ2 1/

ρ−2and 0< Z≤1. Thus,3.37can be transformed to

1 2

⎢⎣

z

ρ2

ρ2−2

z

ρ−2

ρ2−2

⎥⎦±n−1 n

σn1

5n−3 ξ. 3.38

Completing3.38and refunded the variablez φn−1, we obtain two implicit solutions of elliptic function type forK4n−3, nequation as follows:

sn−1

⎝ √

22 φn−12,

2−√

2 2√

2

⎠sn−1

#$

$% √ 22 φn−1

2,

2√ 2 2√ 2

⎠ Ω1,2 ξ, 3.39

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whereΩ1,2 ±n−1/n2 2 −σn1/5n−3. The solutions also can be rewritten as

F

⎝sin−1

22 φn−12,

2−√

2 2√

2

F

⎝sin−1

#$

$% √ 22 φn−1

2,

2√ 2 2√ 2

⎠ Ω1,2 ξ, 3.40

where the functionFϕ, k EllipticFϕ, kis the incomplete Elliptic integral of the first kind.

The two solutions in 3.40 are asymptotically stable. Under Ω1 n −

1/n2 √

2

−σn1/5n−3,φ → 0 as ξ → ∞. Under Ω2 −n − 1/n2

√2

−σn1/5n−3,φ → 0 as ξ → −∞. The graphs of their profiles are shown in Figure5.

3.2. Exact Solutions and Their Properties of 1.1underh /0

In this subsection, under the conditionsh hA0,andh hA1, h hA2, we will investigate exact solutions of1.1and discuss their properties. Whenh /0,2.6can be reduced to

y±

h 2nv/n1φn1−2nσ/nnm

n−1 . 3.41

Substituting3.41into the first expression of2.3yields φ

φ

n

h 2nv/n1φn1−2nσ/nnm ±ξ, 3.42

whereφis one of roots for equationh2nv/n1φn1−2nσ/nnm0. However we cannot obtain any exact solutions by3.42when the degreesmand nare more great, because we cannot obtain coincidence relationship among different degreesn, n1 andn m. But, we can always obtain some exact solutions when the degreemnis not greater than four. For example, by using3.42directly, we can also obtain many exact solutions ofK2,1 andK3,1equations; see the next computation and discussion.

iIfmn2, then3.41can be reduced to

y±

h 4v/3φ3σφ4

. 3.43

Takingh hA0|mn2 −v4/6σ3as Hamiltonian quantity, substituting3.43andm n 2 into the first expression of2.5yields

v4/6σ3

4v/3φ3σφ4

±dτ. 3.44

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2 3 4 5 6 7 8 9

0.4 0.6 0.8 1 1.2 1.4

x

φ

a Asymptotically stable wave

2 3 4 5 6 7 8 9

−1 −0.8 −0.6 −0.4 −0.2 0 0.2 x

φ

b Asymptotically stable wave

Figure 5: Waveforms of two asymptotically stable solutions in3.40whenn4, σ−1,andt1.

Then−v4/6σ3 4v/3φ3σφ40 has four roots, two real roots, and two complex roots as follows:

a, b v σ

1 3 μ

6 ±1 6

8−3

42√ 21/3

−6 42√

2−1/3 16

μ

,

c, c v σ

1 3 −μ

6 ±i1 6

−83 42√

21/3 6

42√ 2−1/3

16 μ

,

3.45

withμ

4342√

21/3642√ 2−1/3.

1Whenσ >0 anda > φ > b, takingbas initial value, then integrating3.44yields

φ

b

aφ

φb φc

φc ±√ σ

τ

0

dτ. 3.46

Solving the aforementioned integral equation yields

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φ aBbA AB

⎢⎣1α1cn ABσ τ, k 1αcn

ABσ τ, k⎥⎦, 3.47

whereα1 bA−aB/aBbA, α A−B/ABand k 1/2

a−b2−A−B2/AB withA

a−cc/22−c−c2/4andB

b−cc/22−c−c2/4 Sub- stituting3.47andn2 into2.4yields

ξ 2aBbA AB

ABσ α1

αu1 αα1

α1α2

Π

ϕ, α2 α2−1, k

αf1

, 3.48

whereu1sn−1

ABστ, k Fϕ, k, ϕamu1arcsin√

ABστ, α2/1, theΠϕ, α22− 1, kis an elliptic integral of the third kind, and the functionf1satisfies the following three cases, respectively:

f1

1−α2

k2k2α2arctan

k2k2α2 1−α2 sd√

ABσ τ, k

, if α2

α2−1 < k2, sd√

ABστ, k, if α2

α2−1 k2,

1 2

α2−1 k2k2α2

×ln k2k2α2dn√

ABστ, k

α2−1sn√

ABστ, k k2k2α2dn√

ABστ, k−√

α2−1sn√

ABστ, k

, if α2 α2−1 > k2.

In the previous three cases,k2 1−k2. Thus, by using3.47and3.48, we obtain a parametric solution of Jacobian elliptic function forK2,2equation as follows:

φ aBbA AB

⎢⎣1α1cn√

ABσ τ, k 1αcn

ABσ τ, k

⎥⎦,

ξ 2aBbA AB

ABσ α1

αu1 αα1

α1α2

Π

ϕ, α2 α2−1, k

αf1

.

3.49

2Whenσ <0 andb < a < φ <∞, takingaas initial value, integrating3.44yields

φ

a

φa

φb φc

φc ±√

−σ τ

0

dτ. 3.50

(16)

Solving the aforementioned integral equation yields

φ aBbA BA

⎢⎣1α&1cn√

−ABσ τ,k&

1αcn& √

−ABσ τ,k&

⎥⎦, 3.51

whereα&1 aBbA/aBbA,α& AB/BA,k& 1/2

AB2 a−b2/AB,and AandBare given in case1. Substituting3.51andn2 into2.4yields

ξ aBbA B−A

−ABσ

× α&1

&

αu&1 α&−α&1

&

α1α&2

Π

&

ϕ, α&2

&

α2−1,k&

α&f&1

,

3.52

whereu&1sn−1

−ABστ,k & Fϕ, k,& ϕ&amu&1arcsin√

−ABστ, α&2/1,Πϕ,& α&2/&α2− 1,k& is an elliptic integral of the third kind, and the functionf&1satisfies the following three cases, respectively:

&

f1

1−α&2

&

k2k&2α&2arctan

k&2k&2α&2 1−α&2 sd√

−ABσ τ,k&

, if α&2

α&2−1 <k&2, sd√

−ABστ,k,& if α&2

α&2−1 k&2,

1 2

α&2−1

&

k2k&2α&2

×ln

⎢⎣

k&2&k2α&2dn√

−ABστ,k & √

&

α2−1sn√

−ABστ,k&

k&2&k2α2dn√

−ABστ,k& −√

&

α2−1sn√

−ABστ,k&

⎥⎦, if α&2

&

α2−1 >k&2.

In the previous three cases,k&2 1−&k2. Thus, by using 3.51and3.52, we obtain another parametric solution of Jacobian elliptic function forK2,2equation as follows:

aBbA BA

⎢⎣1α&1cn√

−ABσ τ, k&

1αcn& √

−ABσ τ, k&

⎥⎦,

ξ aBbA B−A

−ABσ

&

α1

&

αu&1 α&−α&1

&

α1α&2

Π

&

ϕ, α&2

&

α2−1,k&

α&f&1

.

3.53

In addition, whenh <−v4/6σ3,h 4v/3φ3σφ4 0 has four complex roots; in this case, we cannot obtain any useful results forK2,2equation. Whenh >−v4/6σ3, the case is very

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0.57 0.58 0.59 0.6 0.61 0.62 0.63

0 0.1 0.2 0.3

−0.3 −0.2 −0.1

aPeculiar compacton wave

0 0.1 0.2 0.3

0.1 0.2 0.3

−0.3 −0.2 −0.1

−0.3

−0.2

−0.1 τ

bBounded region of independent variableξ Figure 6: Peculiar compacton wave and its bounded region of independent variableξ.

similar to 3.52; that is, the equationh 4v/3φ3σφ4 0 has two real roots and two complex roots. So we omit the discussions for these parts of results.

In order to describe the dynamic properties of the traveling wave solutions 3.49 and3.53intuitively, as an example, we draw profile figure of solution3.53by using the software Maple, whenv4,and σ−2, see Figure6a.

Figure6ashows a shape of peculiar compacton wave; its independent variableξis bounded regioni.e.,|ξ|< α11; see Figure6b. From Figure6a, we find that its shape is very similar to that of the solitary wave, but it is not solitary wave because when|ξ| ≥α11, u≡0. So, this is a new compacton.

iiUnderm 2, n 1, takingh hA0|m2,n1 −v3/3σ2 as Hamiltonian quantity, 3.42can be reduced to

φ

φ

−v3/3σ2 2−2σ/3φ3

±ξ, 3.54

whereφis one of roots for the equation−v3/3σ22−2σ/3φ30. Clearly, this equation has three real roots, one single root−v/2σand two double rootsv/σ, v/σ. Ifσ >0, then the function

−v3/3σ2 2−2σ/3φ3

2σ/3|φ−v/σ|

−v/2σ−φ; ifσ <0, then the function

−v3/3σ2 2−2σ/3φ3

−2σ/3|φ−v/σ|

v/2σ φ. In these two conditions, takingφ −v/2σas initial value and completing the3.54, we obtain a periodic solution and a solitary wave solutions forK2,1as follows:

ux, t φξ v

2σ 3v 2σtan2

1 2

, v >0,

ux, t φξ v

2σ − 3v 2σtanh2

1 2

√−vξ

, v <0.

3.55

(18)

Similarly, taking φ v/σ as initial value, we obtain two periodic solutions forK2,1as follows:

ux, t φξ v 2σ− 3v

2σtan2 π

4 ±1 2

, v >0. 3.56

iiiUnderm2, n1, taking arbitrary constanthas Hamiltonian quantity,3.42can be reduced to

φ

φ

−2σ/3

φ32q ±ξ, 3.57

where p −3v/2σ,q −3h/2σ.Write Δ q2/4 p3/27 9v4/64σ4 − v36hσ2 3/1728σ9. It is easy to know thatΔ 0 ashhA0|m2,n1 −v3/3σ2; this case is same as caseii. So, we only discuss the caseΔ<0 in the next.

Whenh, σ,andvsatisfyΔ < 0,φ32q 0 has three real rootsz1, z2, and z3 such as

v/2σ cosθ/3,

v/2σcosθ/32π/3, and

v/2σ cosθ/34π/3withθ arccos3h/2σ

3/v3 andv/σ >0. Under these conditions, taking thez1, z2,andz3as initial values replacingφ, respectively,3.57can be reduced to the following three integral equations:

φ

z1

φz1

φz2

φz3 ±

−2σ

3 ξ

σ <0, z3< z2 < z1< φ <, φ

z2

z1φ

φz2

φz3 ±

2σ 3 ξ

σ >0, z3< z2< φ < z1

, φ

z3

z1φ

φz2

φz3 ±

3 ξ

σ >0, z3< φ < z2< z1

.

3.58

Integrating the3.58, then solving them, respectively, we obtain three periodic solu- tions of elliptic function type forK2,1as follows:

uxvt φξ z1z2sn2ω1ξ, k1

cn2ω1ξ, k1 , 3.59

uxvt φξ z2z3k22sn2ω2ξ, k2

dn2ω2ξ, k2 , 3.60

uxvt φξ z3 z2z3sn2ω2ξ, k1, 3.61

where ω1 1/2

−2σ/3z1z3, k1

z2z3/z1z3, ω2 1/2

2σ/3z1z3, andk2

z1z2/z1z3.

(19)

ivWhen m 3, n 1, taking the constant h hA1 hA2|m3,n1 −v/2σ as Hamiltonian quantity,3.42can be reduced to

φ

φ

v/σ−φ2 ±

σ

2ξ σ <0, v <0. 3.62

Clearly, v/σ − φ2 0 has two real roots

v/σ and−

v/σ. Taking φ v/σ

v/σ/2 0 as initial value, solving 3.62, we obtain a kink wave solution and an antikink wave solution forK3,1as follows:

uxvt φξ ± v

σtanh

v 2ξ

, 3.63

wherev <0 shows that the waves defined by3.63are reverse traveling waves.

vUnderm3, n1, taking arbitrary constanthas Hamiltonian quantity andh / − v2/2σ,3.42can be reduced to

φ

φ

φ4−2v/σφ2−2h/σ ±

σ

2ξ σ <0, v <0, 3.64

or

φ

φ

φ4−2v/σφ2−2h/σ ± σ

2ξ σ >0, v >0. 3.65

Clearly,φ4−2v/σφ2−2h/σ 0 has four real rootsr1,2,3,4±

v/σ±

v222h/σifσ <

0, v <0,and 0< h <−v2/2σorσ >0, v >0, and −v2/2σ< h <0; it has two real roots s1,2 ±

v/σ±

v222h/σand two complex rootss, s ±i

|v/σ−

v222h/σ|if σ < 0, v < 0,andh < 0 orσ >0, v > 0, andh > 0; it has not any real roots ifσ < 0, v <

0,and h >−v2/2σorσ >0, v >0, andh <−v2/2σ.

1Under the conditionsσ < 0, v < 0,and 0 < h < −v2/2σ orσ > 0, v > 0,and− v2/2σ < h <0, takingφr1as an initial value,3.64and3.65can be reduced to

φ

r1

φr1

φr2

φr3

φr4 ±

σ 2ξ, r1

φ

r1φ

φr2

φr3

φr4 ± σ

2ξ,

3.66

(20)

wherer1 > r2> r3 > r4. Solving the integral equations3.66, we obtain two periodic solutions of Jacobian elliptic function forK3,1equation as follows:

uxvt φξ r1r2r4r2r1r4sn2

Ω1ξ,k&1 r2r4−r1r4sn2

Ω1ξ,k&1

φ < r1

, 3.67

whereΩ1 1/2

−σ/2r1r3r2r4,k&1

r2r3r1r4/r1r3r2r4, uxvt φξ r1r2r4 r4r1r2sn2

Ω2ξ,k&2 r2r4−r1r2sn2

Ω2ξ,k&2

r2< φ < r1

, 3.68

whereΩ2 1/2

σ/2r1r3r2r4,and&k2

r1r2r3r4/r1r3r2r4. The case for takingφ r2, r3, r4as initial values can be similarly discussed; here we omit these discussions because these results are very similar to the solutions3.67and3.68.

2Under the conditions σ < 0, v < 0, andh < 0 or σ > 0, v > 0, andh > 0, respectively takingφs1, s2as initial value,3.64and3.65can be reduced to

φ

s1

φs1

φs2 φs

φs ±

σ 2ξ, φ

s2

s1φ φs2

φs

φs ± σ

2ξ.

3.69

Solving the aforementioned two integral equations, we obtain two periodic solutions of Jacobian elliptic function forK3,1equation as follows:

uxvt φξ s1B&−s2A&

s1B&s2A&

cn

1/&g −σ/2ξ,k&3

&

BA&

&

AB&

cn

1/g& −σ/2ξ,k&3

,

uxvt φξ s1B&s2A&

s2A&−s1B&

cn1/&g

σ/2ξ,k&4

&

BA&

&

AB&

cn 1/g&

σ/2ξ,k&4 ,

3.70

whereg& 1/

&

AB,& k&3

A&B& 2−s1s22/4A&B,& k&4

s1s22A&−B& 2/4A&B&

withA&

s1b&12a&21,B&

s2−&b12a&21,a&21−s−s2/4|v/σ−

v222h/σ|,&b1 ss/20, ands1 ands2are given previously.

Among these aforementioned solutions, 3.59 shows a shape of solitary wave for given parametersv 4, andσ 1 which is shown in Figure7a. Equation3.60shows a shape of smooth periodic wave for given parametersv2, σ1,andh4 which is shown in Figure 7b. Also 3.61 shows a shape of smooth periodic wave for given parameters

(21)

0 1 2

−4 −3 −2 −1

−4

−3

−2

−1

1 2 3 4

ξ

aBright soliton

0 0.2 0.4 0.6 0.8

−10 −5 5 10

ξ

b Smooth periodic wave

0 5 10

−10 −5 ξ

−0.35

−0.3

−0.25

−0.2

−0.15

−0.1

c Smooth periodic wave

0 0.5 1

2 4 6

−6 −4 −2

−0.5 ξ

−1

dAntikink wave

0 0.5 1

2 4 6

−6 −4 −2

−0.5 ξ

−1 e Kink wave

2 4 6

−6 −4 −2

ξ 30

20 10 0

−10

−20

−30

fSingular periodic wave Figure 7: The graphs of six kinds of waveforms for solutions3.59,3.60,3.61,3.63, and3.68.

v2, σ1,and h0.4 which is shown in Figure7c. Equation3.63shows two shapes of kink wave and antikink wave for given parametersv −4,andσ −2 which are shown in Figures 7d–7e. Equation 3.68 shows a shape of singular periodic wave for given parametersv−10, σ −1,and h48 which is shown in Figure7f.

4. Conclusion

In this work, by using the integral bifurcation method, we study the nonlinear Km, n equation for all possible values ofmandn. Some travelling wave solutions such as normal compactons, peculiar compacton, smooth solitary waves, smooth periodic waves, periodic blowup waves, singular periodic waves, compacton-like periodic waves, asymptotically stable waves, and kink and antikink waves are obtained. In order to show their dynamic properties intuitively, the solutions ofKn, n,K2n−1, n,K3n−2, n,K4n−3, n, and Km,1equations are chosen to illustrate with the concrete features; using software Maple, we display their profiles by graphs; see Figures1–7. These phenomena of traveling waves are different from those in existing literatures and they are very interesting. Although we do not know how they are relevant to the real physical or engineering problem for the moment, these interesting phenomena will attract us to study them further in the future works.

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