Research Article A New Method with a Different Auxiliary Equation to

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Hindawi Publishing Corporation
Advances in Mathematical Physics
Volume 2013, Article ID 890784, 11 pages
http://dx.doi.org/10.1155/2013/890784
Research Article
A New Method with a Different Auxiliary Equation to
Obtain Solitary Wave Solutions for Nonlinear Partial
Differential Equations
Bülent Kiliç and Hasan Bulut
Department of Mathematics, Firat University, 23119 Elazig, Turkey
Correspondence should be addressed to Hasan Bulut; hbulut@firat.edu.tr
Received 3 February 2013; Revised 22 April 2013; Accepted 23 April 2013
Academic Editor: Dumitru Baleanu
Copyright © 2013 B. KilicΜ§ and H. Bulut. 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.
A new method with a different auxiliary equation from the Riccati equation is used for constructing exact travelling wave solutions
of nonlinear partial differential equations. The main idea of this method is to take full advantage of a different auxilliary equation
from the Riccati equation which has more new solutions. More new solitary solutions are obtained for the RLW Burgers and Hirota
Satsuma coupled equations.
1. Introduction
In the recent years, remarkable progress has been made in
the construction of the exact solutions for nonlinear partial
differential equations, which have been a basic concern for
both mathematicians and physicists [1–3].We do not attempt
to characterize the general form of nonlinear dispersive
wave equations [4, 5]. When an original nonlinear equation
is directly calculated, the solution will preserve the actual
physical characters of solutions [6]. The studies in finding
exact solutions to nonlinear differential equation (NPDE),
when they exist, are very important for the understanding
of most nonlinear physical phenomena. There are many
studies which obtain explicit solutions for nonlinear differential equations. Many explicit exact methods have been
introduced in literature [7–21]. Some of them are generalized
Miura transformation, Darboux transformation, Cole-Hopf
transformation, Hirota’s dependent variable transformation,
the inverse scattering transform and the Bäcklund transformation, tanh method, sine-cosine method, Painleve method,
homogeneous balance method (HB), similarity reduction
method, improved tanh method and so on.
In this article, the first section presents the scope of the
study as an introduction. In the second section contains
analyze of a new method and balance term definition. In the
third section, we will obtain wave solutions of RLW Burgers
and Hirota Satsuma coupled equations by using a new
method. In the last section, we implement the conclusion.
2. Method and Its Applications
Let us simply describe the method [22]. Consider a given
partial differential equation in two variables
𝐻 (𝑒, 𝑒𝑑 , 𝑒π‘₯ , 𝑒π‘₯π‘₯ , . . .) = 0.
(1)
The fact that the solutions of many nonlinear equations can
be expressed as a finite series of solutions of the auxiliary
equation motivates us to seek for the solutions of (1) in the
form
π‘š
𝑒 (π‘₯, 𝑑) = πœ†∑ [π‘Žπ‘– 𝐹(πœ‰)𝑖 + π‘Ž−𝑖 𝐹(πœ‰)−𝑖 ] ,
(2)
𝑖=0
where, πœ‰ = π‘˜(π‘₯ − 𝑐𝑑), π‘˜ and 𝑐 are the wave number and
the wave speed respectively, π‘š is a positive integer that can
be determined by balancing the linear term of highest order
with the nonlinear term in (1), πœ† is balancing coefficient
that will be defined in a new “Balance term” definition and
π‘Ž0 , π‘Ž1 , π‘Ž2 , . . . are parameters to be determined. Substituting
(2) into (1) yields a set of algebraic equations for π‘Ž0 , π‘Ž1 , π‘Ž2 , . . .
because all coefficients of 𝐹 have to vanish. From these
2
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0.4
0.1
0
−0.1
−0.2
−0.3
−5
0.2
4
4
0
−5
2
2
0
0
0
5
0
5
(a)
(b)
Figure 1: Graph of the solution 𝑒(π‘₯, 𝑑) from left to the right for (13) and (14).
0
0.5
−0.05
4
−0.1
−5
4
0
−5
2
2
0
0
5
0
5
(a)
0
(b)
Figure 2: Graph of the solution 𝑒(π‘₯, 𝑑) from left to the right for (15) and (16).
relations π‘Ž0 , π‘Ž1 , π‘Ž2 , . . . can be determined. The main idea of
our method is to take full advantage of the new auxiliary
equation. The desired auxiliary equation presents as following
𝐹󸀠 =
𝐴
+ 𝐡𝐹 + 𝐢𝐹3 ,
𝐹
In the following we present a new approach to the
“Balance term” definition.
(3)
where 𝑑𝐹/π‘‘πœ‰ = 𝐹󸀠 and 𝐴, 𝐡, 𝐢 are constants.
Case 1. If 𝐴 = −1/4, 𝐡 = 1/2, 𝐢 = −1/2 then (3) has the
solution 𝐹 = 1/√1 + tan(πœ‰) + sec(πœ‰).
Case 2. If 𝐴 = 1/4, 𝐡 = −1/2, 𝐢 = 0 then (3)
has the solutions 𝐹 = 1/√1 + csc β„Ž(πœ‰) + coth(πœ‰) or 𝐹 =
1/√1 + 𝑖 sec β„Ž(πœ‰) + tanh(πœ‰).
Case 3. If 𝐴 = 1/2, 𝐡 = −1,𝐢 = 0 then (3) has the solutions
𝐹 = 1/√1 + cot β„Ž(πœ‰) or
𝐹=
1
√1 + tanh (πœ‰)
.
Remark 1. Depending on the 𝐴, 𝐡 and 𝐢 coefficients in the
(3), it could be reached only three cases.
(4)
Definition 2. When (1) is transformed with 𝑒(π‘₯, 𝑑) = 𝑒(πœ‰),
πœ‰ = π‘˜(π‘₯ − 𝑐𝑑), where π‘˜ and 𝑐 are real constants, we get a
nonlinear ordinary differential equation for 𝑒(πœ‰) as following
𝑄󸀠 (𝑒, π‘˜π‘π‘’σΈ€  , π‘˜π‘’σΈ€  , π‘˜2 𝑒󸀠󸀠 , . . .) = 0.
(5)
Let 𝑒(𝑝) is the highest order derivative linear term and π‘’π‘ž 𝑒(π‘Ÿ)
is the highest nonlinear term in (5) and 𝐹󸀠 = π‘˜0 + π‘˜1 𝐹 +
π‘˜2 𝐹2 + ⋅ ⋅ ⋅ + π‘˜π‘› 𝐹𝑛 is the auxiliary equation that is used to solve
the nonlinear partial differential equation then the “Balance
term” π‘š can be decided by the balancing the nonlinear term
π‘’π‘ž 𝑒(π‘Ÿ) and the linear term 𝑒(𝑝) with acceptances of 𝑒 ≅ πœ†πΉπ‘–
and 𝐹󸀠 ≅ 𝐹𝑛 where 𝑛 is integer (𝑛 =ΜΈ 1)and πœ† is the balance
coefficient that can be determined later.
Advances in Mathematical Physics
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0
20
−20
4
−40
−5
4
10
0
−5
2
2
0
0
0
5
5
(a)
0
(b)
0
2
−5
4
−10
−5
0
4
−2
−5
2
2
0
0
5
0
5
(c)
0
(d)
Figure 3: Graph of the solutions 𝑒(π‘₯, 𝑑) and V(π‘₯, 𝑑) corresponding to the value 𝑏0 = 1 from left to the right for (22), (3), and (23).
Example 1. For the KdV equation with the transform
𝑒(π‘₯, 𝑑) = 𝑒(πœ‰), πœ‰ = π‘₯ − 𝑐𝑑 we have the ordinary differential
equation as following
σΈ€ 
σΈ€ 
−𝑐𝑒 + 6𝑒𝑒 + 𝑒
σΈ€ σΈ€ σΈ€ 
= 0.
(6)
By the balancing linear term 𝑒󸀠󸀠󸀠 with nonlinear term 𝑒𝑒󸀠
σΈ€ 
𝑒󸀠󸀠 = (πœ†π‘šπΉπ‘š+𝑛−1 ) = πœ†π‘š (π‘š + 𝑛 − 1) πΉπ‘š+𝑛−2 𝐹󸀠
= πœ†π‘š (π‘š + 𝑛 − 1) πΉπ‘š+𝑛−2 𝐹𝑛 = πœ†π‘š (π‘š + 𝑛 − 1) πΉπ‘š+2𝑛−2 ,
π‘š+2𝑛−2 σΈ€ 
)
πœ† = (π‘š + 𝑛 − 1) (π‘š + 2𝑛 − 2) ,
π‘š = 2 (𝑛 − 1) .
(8)
3. Application of the Method
Example 2. Let’s consider RLW Burgers equation
= πœ†π‘š (π‘š + 𝑛 − 1) (π‘š + 2𝑛 − 2) πΉπ‘š+2𝑛−3 𝐹󸀠
= πœ†π‘š (π‘š + 𝑛 − 1) (π‘š + 2𝑛 − 2) 𝐹
πœ†2 π‘šπΉ2π‘š+𝑛−1 = πœ†π‘š (π‘š + 𝑛 − 1) (π‘š + 2𝑛 − 2) πΉπ‘š+3𝑛−3 ,
If it is noticed that our new balance term π‘š (π‘š = 2(𝑛 − 1))
is connected to 𝑛. Namely our new balance term definition is
connected to chosen auxiliary equation.
σΈ€ 
𝑒󸀠 = (πœ†πΉπ‘š ) = πœ†π‘šπΉπ‘š−1 𝐹󸀠 = πœ†π‘šπΉπ‘š−1 𝐹𝑛 = πœ†π‘šπΉπ‘š+𝑛−1 ,
𝑒󸀠󸀠󸀠 = (πœ†π‘š (π‘š + 𝑛 − 1) 𝐹
we have the equations above and the equating 𝑒𝑒󸀠 to 𝑒󸀠󸀠󸀠
𝑒𝑑 + 𝑒π‘₯ + 12𝑒𝑒π‘₯ − 𝑒π‘₯π‘₯ − 𝑒π‘₯π‘₯𝑑 = 0,
(9)
π‘š+2𝑛−3 𝑛
𝐹
with the transform 𝑒(π‘₯, 𝑑) = 𝑒(πœ‰), πœ‰ = π‘₯ − 𝑐𝑑 we have the
following equation
= πœ†π‘š (π‘š + 𝑛 − 1) (π‘š + 2𝑛 − 2) πΉπ‘š+3𝑛−3 ,
𝑒𝑒󸀠 = πœ†πΉπ‘š πœ†π‘šπΉπ‘š+𝑛−1 = πœ†2 π‘šπΉ2π‘š+𝑛−1
(7)
−𝑐𝑒󸀠 + 𝑒󸀠 + 12𝑒𝑒󸀠 − 𝑒󸀠󸀠 + 𝑐𝑒󸀠󸀠󸀠 = 0.
(10)
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0.4
0.5
4
0
−5
0.2
4
0
−0.2
−5
2
2
0
0
5
0
0
5
(a)
(b)
1
0
0.5
−1
4
−2
−3
−5
0
−0.5
4
−5
2
2
0
0
5
0
5
(c)
0
(d)
Figure 4: Graph of the solutions 𝑒(π‘₯, 𝑑) and V(π‘₯, 𝑑) corresponding to the value 𝑏0 = 1 from left to the right for (25) and (26).
From the Definition 2 we have the balance term of RLW Burgers equation by using the auxiliary equation (3) for “Case 1”,
is equal to 4. Therefore, we may choose the following ansatz:
(−
3π‘Ž−4 27π‘π‘Ž−4
2
2
+ 9π‘Ž−3
−
− 24π‘Ž−4
2
2
+
𝑒 (π‘₯, 𝑑) = 48 (π‘Ž−4 𝐹−4 + π‘Ž−3 𝐹−3 + π‘Ž−2 𝐹−2 + π‘Ž−1 𝐹−1
(11)
(−
+π‘Ž0 + π‘Ž1 𝐹 + π‘Ž2 𝐹2 + π‘Ž3 𝐹3 + π‘Ž4 𝐹4 ) .
Substituting (11) into (10) along with (3) and using Mathematica yields a system of equations w.r.t. 𝐹𝑖 . Setting the
coefficients of 𝐹𝑖 in the obtained system of equations to zero,
we can deduce the following set of algebraic polynomials with
the respect unknowns π‘Ž0 , π‘Ž1 , π‘Ž2 , . . . for the Case 1:
(
105π‘π‘Ž−3
+ 21π‘Ž−4 π‘Ž−3 ) = 0,
64
15π‘Ž−3 225π‘π‘Ž−3
−
− 42π‘Ž−4 π‘Ž−3 + 15π‘Ž−3 π‘Ž−2
16
32
+
15π‘π‘Ž−1
+ 15π‘Ž−4 π‘Ž−1 ) = 0,
64
2
2
(6π‘Ž−4 + 28π‘π‘Ž−4 + 24π‘Ž−4
− 18π‘Ž−3
−
π‘Ž−2
− 3π‘π‘Ž−2
2
2
−36π‘Ž−4 π‘Ž−2 + 6π‘Ž−2
+ 12π‘Ž−3 π‘Ž−1 + 12π‘Ž−4 π‘Ž0 ) = 0,
(
2
3π‘π‘Ž−4 + 12π‘Ž−4
= 0,
3π‘π‘Ž−2
+ 18π‘Ž−4 π‘Ž−2 ) = 0,
4
15π‘Ž−3 429π‘π‘Ž−3
+
+ 42π‘Ž−4 π‘Ž−3 − 30π‘Ž−3 π‘Ž−2
4
32
−
3π‘Ž−1 27π‘π‘Ž−1
−
− 30π‘Ž−4 π‘Ž−1 + 9π‘Ž−2 π‘Ž−1
16
32
+9π‘Ž−3 π‘Ž0 −
3π‘π‘Ž1
+ 9π‘Ž−4 π‘Ž1 ) = 0,
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5
2
(8π‘Ž−4 + 20π‘π‘Ž−4 − 3π‘Ž−2 − 4π‘π‘Ž−2 + 12π‘Ž−2
(6π‘Ž12 − π‘Ž2 + 4π‘π‘Ž2 + 12π‘Ž0 π‘Ž2 − 6π‘Ž22
2
+ 24π‘Ž−3 π‘Ž−1 − 6π‘Ž−1
+ 24π‘Ž−4 π‘Ž0
+ 12π‘Ž−1 π‘Ž3 − 12π‘Ž1 π‘Ž3 + 2π‘Ž4 − 10π‘π‘Ž4
−12π‘Ž−2 π‘Ž0 − 12π‘Ž−3 π‘Ž1 − 12π‘Ž−4 π‘Ž2 ) = 0,
+12π‘Ž−2 π‘Ž4 − 12π‘Ž0 π‘Ž4 ) = 0,
2
+ 2π‘Ž−2
(−10π‘Ž−4 − 32π‘π‘Ž−4 + 18π‘Ž−3
2
+ 5π‘π‘Ž−2 + 36π‘Ž−4 π‘Ž−2 − 12π‘Ž−2
− 24π‘Ž−3 π‘Ž−1 +
2
3π‘Ž−1
π‘Ž
3π‘π‘Ž−1 π‘Ž1 35π‘π‘Ž1
3
(− π‘π‘Ž−3 + −1 −
+
−
8
4
8
2
16
− 6π‘Ž0 π‘Ž1 − 6π‘Ž−1 π‘Ž2 + 18π‘Ž1 π‘Ž2 − 3π‘Ž3
− 24π‘Ž−4 π‘Ž0
27π‘π‘Ž3
− 6π‘Ž−2 π‘Ž3 + 18π‘Ž0 π‘Ž3 − 15π‘Ž2 π‘Ž3
2
+
+6π‘Ž−2 π‘Ž0 + 6π‘Ž−3 π‘Ž1 + 6π‘Ž−4 π‘Ž2 ) = 0,
(−6π‘Ž−3 −
27π‘π‘Ž−3
3π‘Ž
+ 30π‘Ž−3 π‘Ž−2 + −1
2
4
35π‘π‘Ž−1
+
+ 30π‘Ž−4 π‘Ž−1 − 18π‘Ž−2 π‘Ž−1
32
− 18π‘Ž−3 π‘Ž0 + 3π‘Ž−1 π‘Ž0 +
π‘Ž1 3π‘π‘Ž1
+
16
32
−6π‘Ž−3 π‘Ž4 + 18π‘Ž−1 π‘Ž4 − 15π‘Ž1 π‘Ž4 ) = 0,
(−6π‘Ž12 + 2π‘Ž2 − 10π‘π‘Ž2 − 12π‘Ž0 π‘Ž2 + 12π‘Ž22
− 12π‘Ž−1 π‘Ž3 + 24π‘Ž1 π‘Ž3 − 9π‘Ž32 − 6π‘Ž4 + 32π‘π‘Ž4
−12π‘Ž−2 π‘Ž4 + 24π‘Ž0 π‘Ž4 − 18π‘Ž2 π‘Ž4 ) = 0,
− 18π‘Ž−4 π‘Ž1 + 3π‘Ž−2 π‘Ž1 + 3π‘Ž−3 π‘Ž2
+
(
(−
3π‘π‘Ž3
+ 3π‘Ž−4 π‘Ž3 ) = 0,
64
(
9π‘Ž−3 105π‘π‘Ž−3
π‘π‘Ž
+
− π‘Ž−1 − −1 + 18π‘Ž−2 π‘Ž−1
2
16
2
π‘Ž
π‘π‘Ž
+ 18π‘Ž−3 π‘Ž0 − 6π‘Ž−1 π‘Ž0 − 1 + 1
4
32
+ 18π‘Ž−4 π‘Ž1 − 6π‘Ž−2 π‘Ž1 − 3π‘Ž0 π‘Ž1
−6π‘Ž−4 π‘Ž3 − 3π‘Ž−2 π‘Ž3 − 3π‘Ž−3 π‘Ž4 ) = 0,
(− 2π‘Ž−4 − 6π‘π‘Ž−4 + 2π‘Ž−2 + π‘π‘Ž−2 +
2
6π‘Ž−1
π‘π‘Ž2
2
π‘Ž4
+ 12π‘Ž−4 π‘Ž2 − 6π‘Ž0 π‘Ž2 − 6π‘Ž−1 π‘Ž3 −
2
+ 12π‘Ž−2 π‘Ž0 + 12π‘Ž−3 π‘Ž1 − 3π‘Ž12 −
+
3π‘π‘Ž4
− 6π‘Ž−2 π‘Ž4 ) = 0,
2
3π‘Ž
9π‘π‘Ž−3 π‘Ž−1 π‘π‘Ž−1
(− −3 −
+
−
+ 6π‘Ž−1 π‘Ž0
4
8
2
16
π‘π‘Ž
+ 1 + 6π‘Ž−2 π‘Ž1 + 6π‘Ž0 π‘Ž1 + 6π‘Ž−3 π‘Ž2
2
3π‘Ž
105π‘π‘Ž3
+ 6π‘Ž−1 π‘Ž2 − 9π‘Ž1 π‘Ž2 + 3 −
4
32
+ 6π‘Ž−4 π‘Ž3 + 6π‘Ž−2 π‘Ž3 − 9π‘Ž0 π‘Ž3
+6π‘Ž−3 π‘Ž4 − 9π‘Ž−1 π‘Ž4 ) = 0,
3π‘π‘Ž−1 3π‘Ž1 27π‘π‘Ž1
9π‘Ž
−
+
− 18π‘Ž1 π‘Ž2 + 3
8
4
8
2
429π‘π‘Ž3
− 18π‘Ž0 π‘Ž3 + 30π‘Ž2 π‘Ž3
16
−
−18π‘Ž−1 π‘Ž4 + 30π‘Ž1 π‘Ž4 − 21π‘Ž3 π‘Ž4 ) = 0,
(−
3π‘Ž
9π‘π‘Ž3
− 6π‘Ž−3 π‘Ž2 − 3π‘Ž−1 π‘Ž2 − 3 +
16
32
105π‘π‘Ž3
− 42π‘Ž3 π‘Ž4 ) = 0,
8
15π‘π‘Ž1 15π‘Ž3 225π‘π‘Ž3
−
+
8
4
8
−30π‘Ž2 π‘Ž3 − 30π‘Ž1 π‘Ž4 + 42π‘Ž3 π‘Ž4 ) = 0,
(−24π‘π‘Ž4 − 24π‘Ž42 ) = 0,
(−2π‘Ž2 + 12π‘π‘Ž2 − 12π‘Ž22 − 24π‘Ž1 π‘Ž3
+ 18π‘Ž32 + 8π‘Ž4 − 56π‘π‘Ž4 − 24π‘Ž0 π‘Ž4
+36π‘Ž2 π‘Ž4 − 12π‘Ž42 ) = 0,
(−6π‘π‘Ž2 − 18π‘Ž32 − 6π‘Ž4
+54π‘π‘Ž4 − 36π‘Ž2 π‘Ž4 + 24π‘Ž42 ) = 0.
(12)
From the system of (12) we have
(i)
π‘Ž0 = −
11
𝑖
− ,
60 12
π‘Ž1 = π‘Ž2 = π‘Ž3 = π‘Ž4 = π‘Ž−1 = π‘Ž−3 = 0,
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π‘Ž−2 =
π‘Ž−4
1
𝑖
+ ,
10 10
𝑖
=− ,
20
(
𝑖
𝑐= ,
5
9π‘Ž−3 135π‘π‘Ž−3
−
+ 30π‘Ž−3 π‘Ž−2
4
16
𝑒 (π‘₯, 𝑑)
= −(
11 + 5𝑖
1+𝑖
)+(
)
60
10
−9π‘Ž−2 π‘Ž−1 − 9π‘Ž−3 π‘Ž0 ) = 0,
(−2π‘Ž−4 + 6π‘π‘Ž−4 + π‘Ž−2 − 3π‘π‘Ž−2
−2
1
)
×(
√1 + sec [π‘₯ − (𝑖/5) 𝑑] + tan [π‘₯ − (𝑖/5) 𝑑]
2
2
+ 12π‘Ž−2
+ 24π‘Ž−3 π‘Ž−1 − 3π‘Ž−1
−4
−
3π‘Ž−1 27π‘π‘Ž−1
+
+ 30π‘Ž−4 π‘Ž−1
16
32
−
+24π‘Ž−4 π‘Ž0 − 6π‘Ž−2 π‘Ž0 ) = 0,
𝑖
1
(
) .
20 √1 + sec [π‘₯ − (𝑖/5) 𝑑] + tan [π‘₯ − (𝑖/5) 𝑑]
(−
(13)
3π‘Ž−3 15π‘π‘Ž−3 π‘Ž−1 9π‘π‘Ž−1
+
+
−
4
8
4
16
+18π‘Ž−2 π‘Ž−1 + 18π‘Ž−3 π‘Ž0 − 3π‘Ž−1 π‘Ž0 ) = 0,
(ii)
π‘Ž0 =
1 + 5𝑖
,
60
𝑐 = −π‘Ž4 ,
(−
π‘Ž1 = π‘Ž−2 = π‘Ž3 = π‘Ž−4 = π‘Ž−1 = π‘Ž−3 = 0,
π‘Ž2 = −
1+𝑖
,
5
2
+ 12π‘Ž−2 π‘Ž0 ) = 0,
(6π‘Ž−1
𝑖
π‘Ž4 = ± ,
5
(
1 + 5𝑖 1 + 𝑖
−
60
5
𝑒 (π‘₯, 𝑑) =
(15)
From the system of (15) we have
(i)
2
π‘Ž0 = π‘Ž−1 = 0,
4
𝑖
𝑖
𝑖
+ (√ 1 + sec [π‘₯ + 𝑑] + tan [π‘₯ + 𝑑]) .
5
5
5
From the Definition 2 we have the balance term of RLW
Burgers equation by using the auxiliary equation (3) for “Case
2”, is equal to −4 then we have the following system of
equations
π‘Ž−3 = 0,
1
,
20
1
𝑐=− ,
5
−2
1
1
=− (
)
5 √1 + 𝑖 sech [π‘₯ + (1/5) 𝑑] + tanh [π‘₯ + (1/5) 𝑑]
−4
3π‘Ž
27π‘π‘Ž−4
2
2
(− −4 +
− 9π‘Ž−3
+ 24π‘Ž−4
2
2
3π‘π‘Ž−2
− 18π‘Ž−4 π‘Ž−2 ) = 0,
4
15π‘Ž−3 225π‘π‘Ž−3
+
+ 42π‘Ž−4 π‘Ž−3 − 15π‘Ž−3 π‘Ž−2
16
32
+
1
1
(
) ,
20 √1 + 𝑖 sech [π‘₯ + (1/5) 𝑑] + tanh [π‘₯ + (1/5) 𝑑]
(16)
or
𝑒 (π‘₯, 𝑑)
1
1
=− (
)
5 √1 + csch [π‘₯ + (1/5) 𝑑] + coth [π‘₯ + (1/5) 𝑑]
15π‘π‘Ž−1
−
− 15π‘Ž−4 π‘Ž−1 ) = 0,
64
2
(4π‘Ž−4 − 18π‘π‘Ž−4 + 18π‘Ž−3
−
π‘Ž−4 =
1
π‘Ž−2 = − ,
5
𝑒 (π‘₯, 𝑑)
2
= 0,
−3π‘π‘Ž−4 − 12π‘Ž−4
(−
π‘Ž−1 3π‘π‘Ž−1
−
+ 6π‘Ž−1 π‘Ž0 ) = 0.
4
8
(14)
𝑖
𝑖
× (√ 1 + sec [π‘₯ + 𝑑] + tan [π‘₯ + 𝑑])
5
5
−
105
π‘π‘Ž − 21π‘Ž−4 π‘Ž−3 ) = 0,
64 −3
π‘Ž−2
2
2
+ 3π‘π‘Ž−2 + 36π‘Ž−4 π‘Ž−2 − 6π‘Ž−2
− 12π‘Ž−3 π‘Ž−1 −12π‘Ž−4 π‘Ž0 ) = 0,
−2
−4
1
1
+ (
) .
20 √1 + csch [π‘₯ + (1/5) 𝑑] + coth [π‘₯ + (1/5) 𝑑]
(17)
Advances in Mathematical Physics
7
Example 3. Let’s consider Hirota Satsuma coupled equation
π‘Ž1 π‘π‘Ž1 3π‘Ž0 π‘Ž1 9π‘Ž1 π‘Ž2
−
−
+
2
2
2
4
(−
1
𝑒𝑑 − 3𝑒𝑒π‘₯ + 6VVπ‘₯ − 𝑒π‘₯π‘₯π‘₯ = 0,
2
+
(18)
V𝑑 + 3𝑒Vπ‘₯ + Vπ‘₯π‘₯π‘₯ = 0,
129π‘Ž3 3π‘π‘Ž3 9π‘Ž0 π‘Ž3
+
+
64
4
4
+ 3𝑏0 𝑏1 −
(−
with the transform 𝑒(π‘₯, 𝑑) = 𝑒(πœ‰), V(π‘₯, 𝑑) = V(πœ‰), πœ‰ = π‘₯ − 𝑐𝑑 we
have
3π‘Ž12 5π‘Ž2
−
− π‘π‘Ž2 − 3π‘Ž0 π‘Ž2
2
2
+
σΈ€ 
−𝑐V + 3𝑒V + V
σΈ€ σΈ€ σΈ€ 
(19)
−6𝑏1 𝑏3 − 6𝑏0 𝑏4 ) = 0,
= 0.
(
From the Definition 2 we have the balance term of Hirota
Satsuma coupled equation by using the auxiliary equation (3)
for “Case 1”, is equal to 4 for 𝑒 and V. Therefore, we may choose
the following ansatz:
2
3
43π‘Ž1 π‘π‘Ž1 3π‘Ž0 π‘Ž1 9π‘Ž1 π‘Ž2
+
+
−
32
2
2
2
−
15π‘Ž3 3π‘π‘Ž3 9π‘Ž0 π‘Ž3 15π‘Ž2 π‘Ž3
−
−
+
2
2
2
4
+
15π‘Ž1 π‘Ž4
− 3𝑏0 𝑏1 + 9𝑏1 𝑏2
4
+9𝑏0 𝑏3 −
4
𝑒 (π‘₯, 𝑑) = 48 (π‘Ž0 + π‘Ž1 𝐹 + π‘Ž2 𝐹 + π‘Ž3 𝐹 + π‘Ž4 𝐹 ) ,
V (π‘₯, 𝑑) = 48 (𝑏0 + 𝑏1 𝐹 + 𝑏2 𝐹2 + 𝑏3 𝐹3 + 𝑏4 𝐹4 ) .
(20)
(
Substituting (20) into (19) along with (3) and using Mathematica yields a system of equations w.r.t. 𝐹𝑖 . Setting the
coefficients of 𝐹𝑖 in the obtained system of equations to zero,
we can deduce the following set of algebraic polynomials with
the respect unknowns π‘Ž0 , π‘Ž1 , π‘Ž2 , . . . for the Case 1:
3π‘Ž
3π‘Ž
(− 1 − 3 ) = 0,
64 128
3π‘Ž π‘Ž
9π‘Ž
3𝑏 𝑏
7π‘Ž
π‘π‘Ž
( 1 + 1 + 0 1 − 3 − 0 1 ) = 0,
64
4
4
64
2
3π‘Ž12 π‘Ž2 π‘π‘Ž2 3π‘Ž0 π‘Ž2
+
+
+
4
2
2
2
−
3π‘Ž4 3𝑏12
−
− 3𝑏0 𝑏2 ) = 0,
4
2
15𝑏2 𝑏3 15𝑏1 𝑏4
−
) = 0,
2
2
3π‘Ž12 11π‘Ž2
+
+ π‘π‘Ž2 + 3π‘Ž0 π‘Ž2 − 3π‘Ž22
2
2
− 6π‘Ž1 π‘Ž3 +
9π‘Ž32
− 17π‘Ž4 − 2π‘π‘Ž4
4
− 6π‘Ž0 π‘Ž4 +
9π‘Ž2 π‘Ž4
− 3𝑏12 − 6𝑏0 𝑏2
2
+ 6𝑏22 + 12𝑏1 𝑏3 −
9𝑏32
2
+12𝑏0 𝑏4 − 9𝑏2 𝑏4 ) = 0,
3π‘Ž1
= 0,
128
(
3π‘Ž22
11π‘Ž4
+ 3π‘Ž1 π‘Ž3 +
+ π‘π‘Ž4
2
2
+ 3π‘Ž0 π‘Ž4 + 3𝑏12 + 6𝑏0 𝑏2 − 3𝑏22
1
−𝑐𝑒󸀠 − 3𝑒𝑒󸀠 + 6VVσΈ€  − 𝑒󸀠󸀠󸀠 = 0,
2
σΈ€ 
9𝑏1 𝑏2 9𝑏0 𝑏3
−
) = 0,
2
2
(
105π‘Ž3 21π‘Ž3 π‘Ž4
+
− 21𝑏3 𝑏4 ) = 0,
16
2
(−
27π‘Ž1 9π‘Ž1 π‘Ž2 453π‘Ž3 3π‘π‘Ž3
+
+
+
16
2
32
2
+
9π‘Ž0 π‘Ž3 15π‘Ž2 π‘Ž3 15π‘Ž1 π‘Ž4
−
−
2
2
2
+
21π‘Ž3 π‘Ž4
− 9𝑏1 𝑏2 − 9𝑏0 𝑏3
4
+15𝑏2 𝑏3 + 15𝑏1 𝑏4 −
21𝑏3 𝑏4
) = 0,
2
8
Advances in Mathematical Physics
(
15π‘Ž1 225π‘Ž3 15π‘Ž2 π‘Ž3
−
+
16
16
2
+
−2𝑐𝑏4 + 6π‘Ž0 𝑏4 − 3π‘Ž2 𝑏4 ) = 0,
15π‘Ž1 π‘Ž4 21π‘Ž3 π‘Ž4
−
− 15𝑏2 𝑏3
2
2
−15𝑏1 𝑏4 + 21𝑏3 𝑏4 ) = 0,
(12π‘Ž4 + 6π‘Ž42 − 12𝑏42 ) = 0,
(−6π‘Ž2 +
3π‘Ž22
9π‘Ž2
+ 6π‘Ž1 π‘Ž3 − 3
2
+ 29π‘Ž4 + 2π‘π‘Ž4 + 6π‘Ž0 π‘Ž4
− 9π‘Ž2 π‘Ž4 + 3π‘Ž42 − 6𝑏22
(−
(
27𝑏1 3π‘Ž2 𝑏1 3π‘Ž4 𝑏1
−
+
− 3π‘Ž1 𝑏2
8
2
2
+ 3π‘Ž3 𝑏2 −
+
(−
− 12𝑏1 𝑏3 + 9𝑏32 − 12𝑏0 𝑏4
+18𝑏2 𝑏4 −
6𝑏42 )
3𝑏
= 0 − 1 = 0,
64
−
𝑐𝑏1 3π‘Ž0 𝑏1 3π‘Ž2 𝑏1 3π‘Ž1 𝑏2
+
−
−
2
2
4
2
(−6𝑏2 − 3π‘Ž4 𝑏2 −
9π‘Ž3 𝑏3
+ 54𝑏4
2
−6π‘Ž2 𝑏4 + 6π‘Ž4 𝑏4 ) = 0,
3π‘Ž1 𝑏1 3π‘Ž3 𝑏1
−
+ 5𝑏2 − 𝑐𝑏2
2
4
+ 3π‘Ž0 𝑏2 −
9π‘Ž1 𝑏3 9π‘Ž3 𝑏3
+
− 58𝑏4 + 2𝑐𝑏4
2
2
−6π‘Ž0 𝑏4 + 6π‘Ž2 𝑏4 − 3π‘Ž4 𝑏4 ) = 0,
129𝑏3 3𝑐𝑏3 9π‘Ž0 𝑏3
+
−
) = 0,
32
4
4
(
9π‘Ž2 𝑏3 9π‘Ž4 𝑏3
+
− 6π‘Ž1 𝑏4 + 6π‘Ž3 𝑏4 ) = 0,
2
2
3
(− π‘Ž3 𝑏1 + 12𝑏2 − 3π‘Ž2 𝑏2 + 3π‘Ž4 𝑏2
2
3π‘Ž 𝑏
𝑐𝑏
3𝑏
3
(− π‘Ž1 𝑏1 − 𝑏2 + 2 − 0 2 + 4 ) = 0,
4
2
2
2
−
9π‘Ž2 𝑏3 9π‘Ž4 𝑏3
−
+ 6π‘Ž1 𝑏4 − 3π‘Ž3 𝑏4 ) = 0,
2
4
(−24𝑏4 − 6π‘Ž4 𝑏4 ) = 0,
7𝑏1 𝑐𝑏1 3π‘Ž0 𝑏1 9𝑏3
+
−
+
) = 0,
32
4
4
32
(𝑏1 −
453𝑏3 3𝑐𝑏3 9π‘Ž0 𝑏3
+
−
16
2
2
225𝑏3
15𝑏1 3π‘Ž4 𝑏1
−
− 3π‘Ž3 𝑏2 +
8
2
8
−
3𝑏
3𝑏
( 1 + 3 ) = 0,
32
64
(−
105𝑏3 9π‘Ž4 𝑏3
−
− 6π‘Ž3 𝑏4 ) = 0,
8
2
(3π‘Ž2 +
3π‘Ž2 𝑏2 9π‘Ž1 𝑏3
−
2
4
9π‘Ž32
− 27π‘Ž4 + 9π‘Ž2 π‘Ž4 − 6π‘Ž42
2
−9𝑏32 − 18𝑏2 𝑏4 + 12𝑏42 ) = 0.
−11𝑏4 + 𝑐𝑏4 − 3π‘Ž0 𝑏4 ) = 0,
(21)
3π‘Ž 𝑏
43𝑏
𝑐𝑏
3π‘Ž 𝑏
(− 1 + 1 − 0 1 + 2 1
16
2
2
2
−
3π‘Ž 𝑏
3π‘Ž4 𝑏1
+ 3π‘Ž1 𝑏2 − 3 2 + 15𝑏3
4
2
−
3𝑐𝑏3 9π‘Ž0 𝑏3 9π‘Ž2 𝑏3
+
−
− 3π‘Ž1 𝑏4 ) = 0,
2
2
4
3π‘Ž 𝑏
3
(− π‘Ž1 𝑏1 + 3 1 − 11𝑏2 + 𝑐𝑏2
2
2
− 3π‘Ž0 𝑏2 + 3π‘Ž2 𝑏2 −
+
3π‘Ž4 𝑏2
2
9π‘Ž1 𝑏3 9π‘Ž3 𝑏3
−
+ 34𝑏4
2
4
From the system of (21) we have
(i)
𝑐=
1
(5 − 6𝑏0 ) ,
4
π‘Ž1 = π‘Ž3 = 0,
π‘Ž0 =
1
(−5 − 2𝑏0 ) ,
4
𝑏1 = 𝑏3 = 0,
π‘Ž2 = 4,
𝑏2 = −2,
π‘Ž4 = −4,
𝑏4 = 2,
Advances in Mathematical Physics
𝑒 (π‘₯, 𝑑) =
9
1
(−5 − 2𝑏0 )
4
𝑏2
2
V (π‘₯, 𝑑) = −
+ 4 (((1 + sec [π‘₯ −
+ tan [π‘₯ −
− 𝑏2 (((1 + sec [π‘₯ −
−1
2
−1
4
−1/2
1
(5 − 6𝑏0 ) 𝑑]) ) )
4
− 4 (((1 + sec [π‘₯ −
+ tan [π‘₯ −
1
(5 − 6𝑏0 ) 𝑑]
4
−1
1
(5 − 6𝑏0 ) 𝑑]
4
From the Definition 2 we have the balance term of Hirota
Satsuma coupled equation by using the auxiliary equation (3)
for “Case 2”, is equal to −4 then we have the following system
of equations
V (π‘₯, 𝑑) = 𝑏0
3π‘Ž−4
2
2
− 6𝑏−4
= 0,
+ 3π‘Ž−4
2
1
(5 − 6𝑏0 ) 𝑑]
4
(
−1
−1/2
1
+ tan [π‘₯ − (5 − 6𝑏0 ) 𝑑]) ) )
4
+ 2 (((1 + sec [π‘₯ −
2
105π‘Ž−3 21
21
+ π‘Ž−4 π‘Ž−3 − 𝑏−4 𝑏−3 ) = 0,
128
4
2
(−
1
(5 − 6𝑏0 ) 𝑑]
4
(−
4
−1
π‘Ž−1 π‘π‘Ž−1 3
−
− π‘Ž−1 π‘Ž0 + 3𝑏−1 ) = 0,
16
2
2
9π‘Ž2
27π‘Ž−4
3π‘Ž
9
2
+ −3 + −2 + π‘Ž−4 π‘Ž−2
− 6π‘Ž−4
4
4
8
2
2
+12𝑏−4
−
−1/2
1
+ tan [π‘₯ − (5 − 6𝑏0 ) 𝑑]) ) ) .
4
(22)
(−
(ii)
𝑐=
1
(−1 − 3𝑏22 ) ,
4
π‘Ž1 = π‘Ž3 = 0,
π‘Ž2 = 2,
π‘Ž0 =
1
(−3 − 𝑏22 ) ,
4
𝑏1 = 𝑏3 = 𝑏4 = 0,
𝑏2 =ΜΈ 0,
(
π‘Ž4 = −2,
1
𝑒 (π‘₯, 𝑑) = (−3 − 𝑏22 )
4
+ 2 (((1 + sec [π‘₯ −
225π‘Ž−3 21
15
− π‘Ž−4 π‘Ž−3 + π‘Ž−3 π‘Ž−2
64
2
4
+
15π‘Ž−1 15
+ π‘Ž−4 π‘Ž−1 + 21𝑏−4 𝑏−3
128
4
−
15
15
𝑏 𝑏 − 𝑏 𝑏 ) = 0,
2 −3 −2 2 −4 −1
2
3π‘Ž−2
+ 3π‘Ž−3 π‘Ž−1 + 3π‘Ž−4 π‘Ž0 − 6𝑏−4
2
2
2
+9𝑏−3
+ 18𝑏−4 𝑏−2 − 3𝑏−2
− 6𝑏−3 𝑏−1 ) = 0,
1
(−1 − 3𝑏22 ) 𝑑]
4
−1
− 2 (((1 + sec [π‘₯ −
2
9𝑏−3
− 9𝑏−4 𝑏−2 ) = 0,
2
9π‘Ž2
19π‘Ž−4
3π‘Ž
+ π‘π‘Ž−4 − −3 − −2 − 9π‘Ž−4 π‘Ž−2
2
2
2
+
−1/2
1
+ tan [π‘₯ − (−1 − 3𝑏22 ) 𝑑]) ) )
4
2
(
147π‘Ž−3 3π‘π‘Ž−3 15
+
− π‘Ž−3 π‘Ž−2
32
4
2
−
1
(−1 − 3𝑏22 ) 𝑑]
4
−1
2
−1/2
1
+ tan [π‘₯ − (−1 − 3𝑏22 ) 𝑑]) ) ) .
4
(23)
−1/2
1
(5 − 6𝑏0 ) 𝑑]) ) ) ,
4
− 2 (((1 + sec [π‘₯ −
1
(−1 − 3𝑏22 ) 𝑑]
4
4
−1/2
1
+ tan [π‘₯ − (−1 − 3𝑏22 ) 𝑑]) ) ) ,
4
27π‘Ž−1 15
9
− π‘Ž−4 π‘Ž−1 + π‘Ž−2 π‘Ž−1
64
2
4
9𝑏
9
+ π‘Ž−3 π‘Ž0 − −3 + 15𝑏−3 𝑏−2
4
2
9
+15𝑏−4 𝑏−1 − 𝑏−2 𝑏−1 ) = 0,
2
10
Advances in Mathematical Physics
(−
9
(8𝑏−4 − 2𝑐𝑏−4 + 6π‘Ž0 𝑏−4 + π‘Ž−1 𝑏−3
2
27π‘Ž−3 3π‘π‘Ž−3 13π‘Ž−1 π‘π‘Ž−1
−
+
+
16
2
32
4
9
9
3
− π‘Ž−2 π‘Ž−1 − π‘Ž−3 π‘Ž0 + π‘Ž−1 π‘Ž0
2
2
4
+9𝑏−3 −
−
3𝑏−1
+ 9𝑏−2 𝑏−1 ) = 0,
2
(− 4π‘Ž−4 − 2π‘π‘Ž−4 +
3
3
3
− π‘Ž0 𝑏−2 + π‘Ž−3 𝑏−1 − π‘Ž−1 𝑏−1 ) = 0,
2
2
4
7π‘Ž−2 π‘π‘Ž−2
+
4
2
2
− 3π‘Ž−2
− 6π‘Ž−3 π‘Ž−1 +
3
(𝑏−2 − 𝑐𝑏−2 + 3π‘Ž0 𝑏−2 + π‘Ž−1 𝑏−1 ) = 0,
2
2
3π‘Ž−1
4
(
3
− 6π‘Ž−4 π‘Ž0 + π‘Ž−2 π‘Ž0 + 12𝑏−4
2
27𝑏−3 3𝑐𝑏−3 9
−
+ π‘Ž0 𝑏−3 + 3π‘Ž−1 𝑏−2
8
2
2
−
3𝑏2
2
−3𝑏−2 + 6𝑏−2
+ 12𝑏−3 𝑏−1 − −1 ) = 0,
2
(−
π‘Ž−2
2
) = 0,
− π‘π‘Ž−2 −
− 3π‘Ž−2 π‘Ž0 + 6𝑏−2 + 3𝑏−1
2
2
(−3π‘Ž−3 𝑏−4 −
(
105𝑏−3 9
− π‘Ž−4 𝑏−3 ) = 0,
64
4
From the system of (3) we have
(i)
π‘Ž−1 = π‘Ž−3 = 𝑏−1 = 𝑏−3 = 0,
3𝑏
9
3
− π‘Ž−3 𝑏−3 − −2 − π‘Ž−4 𝑏−2 ) = 0,
4
4
2
𝑏−2 = ±1,
225𝑏−3
32
15𝑏−1 3
− π‘Ž−4 𝑏−1 ) = 0,
64
4
( − 19𝑏−4 + 𝑐𝑏−4 + 6π‘Ž−2 𝑏−4 − 3π‘Ž0 𝑏−4
9
9
+ π‘Ž−3 𝑏−3 − π‘Ž−1 𝑏−3 + 3𝑏−2
2
4
3
3
+3π‘Ž−4 𝑏−2 − π‘Ž−2 𝑏−2 − π‘Ž−3 𝑏−1 ) = 0,
2
4
(6π‘Ž−1 𝑏−4 −
147𝑏−3 3𝑐𝑏−3
+
16
4
9
9
+ π‘Ž−2 𝑏−3 − π‘Ž0 𝑏−3
2
4
27𝑏−1
3
+ 3π‘Ž−3 𝑏−2 − π‘Ž−1 𝑏−2 +
2
32
3
3
+ π‘Ž−4 𝑏−1 − π‘Ž−2 𝑏−1 ) = 0,
2
4
𝑏−4 = −
π‘Ž−4 = −1,
9
9
3
+ π‘Ž−4 𝑏−3 − π‘Ž−2 𝑏−3 − π‘Ž−3 𝑏−2
2
4
2
−
𝑏−1 𝑐𝑏−1 3
−
+ π‘Ž0 𝑏−1 ) = 0.
8
2
2
(24)
27𝑏−4
+ 6π‘Ž−4 𝑏−4 − 3π‘Ž−2 𝑏−4
2
(6π‘Ž−3 𝑏−4 − 3π‘Ž−1 𝑏−4 +
13𝑏−1 𝑐𝑏−1 3
3
+
+ π‘Ž−2 𝑏−1 − π‘Ž0 𝑏−1 ) = 0,
16
4
2
4
(
2
3π‘Ž−1
−3𝑏−4 − 3π‘Ž−4 𝑏−4 = 0,
7𝑏−2 𝑐𝑏−2
+
+ 3π‘Ž−2 𝑏−2
2
2
π‘Ž0 =
𝑐=
𝑏−2
,
2
π‘Ž−2 = 2,
1
(1 + 6𝑏−2 ) ,
4
1
(−1 + 2𝑏−2 ) ,
4
𝑒 (π‘₯, 𝑑)
1
1
= +2 (
)
4
√1 + 𝑖 sech [π‘₯ − (7/4) 𝑑] + tanh [π‘₯ − (7/4) 𝑑]
−2
−4
1
−(
) ,
√1 + 𝑖 sech [π‘₯ − (7/4) 𝑑] + tanh [π‘₯ − (7/4) 𝑑]
V (π‘₯, 𝑑)
−2
= 𝑏0 + (
1
)
√1 + 𝑖 sech [π‘₯ − (7/4) 𝑑] + tanh [π‘₯ − (7/4) 𝑑]
−4
1
1
− (
) ,
2 √1 + 𝑖 sech [π‘₯ − (7/4) 𝑑] + tanh [π‘₯ − (7/4) 𝑑]
(25)
Advances in Mathematical Physics
11
or
𝑒 (π‘₯, 𝑑)
=
1
1
)
+2(
4
√1 + csch [π‘₯ − (7/4) 𝑑] + coth[π‘₯ − (7/4) 𝑑]
−2
−4
1
−(
) ,
√1 + csch [π‘₯ − (7/4) 𝑑] + coth [π‘₯ − (7/4) 𝑑]
V (π‘₯, 𝑑)
−2
= 𝑏0 + (
1
)
√1 + csch [π‘₯ − (7/4) 𝑑] + coth [π‘₯ − (7/4) 𝑑]
−4
1
1
− (
) .
2 √1 + csch [π‘₯ − (7/4) 𝑑] + coth [π‘₯ − (7/4) 𝑑]
(26)
Figures 1, 2, 3 and 4 gives to us 3D graphics for RLW Burgers
and RLW Burgers and Hirota Satsuma coupled equations.
4. Conclusion
We have presented a new method and balance term definition
and used it to solve the RLW Burgers and Hirota Satsuma
coupled equations. In fact, this method is readily applicable
to a large variety of nonlinear PDEs. First, all the nonlinear
PDEs which can be solved by the other methods can be
solved by our method. Second, we used only the special
solutions of (3). If we use other solutions of (3), we can obtain
more travelling wave solutions. Third it is a computerizable
method, which allow us to perform complicated and tedious
algebraic calculation on computer and so our balance term
definition is effectively useful for any to chosen auxiliary
equation.
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