Startseite Mathematik Reductions and conservation laws for BBM and modified BBM equations
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Reductions and conservation laws for BBM and modified BBM equations

  • Maryam Khorshidi , Mehdi Nadjafikhah EMAIL logo , Hossein Jafari und Maysaa Al Qurashi
Veröffentlicht/Copyright: 30. Dezember 2016

Abstract

In this paper, the classical Lie theory is applied to study the Benjamin-Bona-Mahony (BBM) and modified Benjamin-Bona-Mahony equations (MBBM) to obtain their symmetries, invariant solutions, symmetry reductions and differential invariants. By observation of the the adjoint representation of Mentioned symmetry groups on their Lie algebras, we find the primary classification (optimal system) of their group-invariant solutions which provides new exact solutions to BBM and MBBM equations. Finally, conservation laws of the BBM and MBBM equations are presented. Some aspects of their symmetry properties are given too.

MSC 2010: 70H33; 34K17; 70G65

1 Introduction

Finding the exact solutions of nonlinear evolution equations (NEEs) plays a fundamental role in the study of nonlinear phenomena in physics and applied mathematics[16]. Solving these types of partial differential equations by using symmetry methods was originally developed by S. Lie and, without any doubt, this is one of the most effective algorithmic ways for analyzing and solving linear and nonlinear differential equations [1, 2]. During the last few decades some semi analytical methods have been developed for solving these type of equations.

One such NEEs is Benjamin-Bona-Mahony (BBM) equation

ut+uxa(u2)xbuxxt=0,(1)

first introduced by Benjamin et al. (1972), as an improvement of the Korteweg-de Vries equation (KdV), and it is well known in applied sciences, where a and b are arbitrary constants. Originally KdV derived to describe shallow water waves of long wavelength and small amplitude. BBM and KdV are useful for modelling surface waves of long wavelength in liquids, acoustic-gravity waves in compressible fluids, hydromagnetics waves in cold plasma and acoustic waves in anharmonic crystals [3, 4, 710]. Peregrine also derived the BBM equations to regularized long-wave equation [11]. Another equation in this article that we will study is the nonlinear dispersive modified Benjamin- Bona- Mahony equation (MBBM)

ut+ux+au2ux+uxxx=0,(2)

where a is an arbitrary constant, which was first derived to describe an approximation for surface long waves in nonlinear dispersive media. This equation can also characterize the hydro-magnetic wave in cold plasma, acoustic-gravity waves in compressible fluids and acoustic waves in an-harmonic crystals. Physical applications and mathematical properties of these equations have been discussed in other papers [3, 4, 7, 10]. Khalique presented some result regarding BBM equation and we cover all of them [12].

This paper is organized as follows: Section 2 is devoted to some concepts needed to construct Lie point symmetries and general form of infinitesimal generators of BBM and MBBM equations and exact solutions associated with the symmetries. We will find an optimal system of one-dimensional subalgebras for symmetry algebras of these systems in Section 3. In Section 4, we compute the invariants associated with the symmetry operators by integrating the characteristic equations to reduced BBM and MBBM equations and differential invariant are exhibited. Finally in the last section, conservation laws of BBM and MBBM equations are obtained.

2 Calculation of symmetry groups

Suppose (x,un) is a differential equation defined over the total space M=X×U, whose coordinates represent the independent and dependent variables and the derivatives of dependent variables up to order n, that is called the n-th order jet space on the underlying space X×U. If f(x):XU is a smooth real-valued function whit p independent variables, the n-jet or n-th prolongation of f is

Pr(n)f:XU(n),

a typical point in U(n) will be denoted by U(n), with q.C(p + n, n) different components uJα=Jfα(x), where J=(j1,,jk),1<_jk<_p and 0≤kn, note uα refers to component uα of u itself. The graph of Pr(n)f(x) lies in the n-jet space M(n)=X×U×U1×U2××Un and from this point of view, a smooth solution of the given system of differential equations is a smooth function u = f(x) such that

ΔV(x,u(n))=0,V=1,,l.(3)

A local group transformation acting on M is given by one parameter Lie group

G:I×MMIR,
(ε,(x,u))φ(ε)=(x1+ξ1(x,u)+O(ε2),xp+εξp(x,u)+O(ε2),u1+εη1(x,u)+O(ε2),,uq+εηq(x,u)+O(ε2)).

Let C-curve be the graph of G on M, that at each it's point the tangent vector

v=φ˙(ε)=dφdε|ε=0=i=1pξi(x,u)xi+α=1qηα(x,u)uα,

is infinitesimal transformation of G in g that acts on X×U×U(1).G is a symmetry group of (3), which transforms solutions of the system to other solutions. For determining symmetry group through the classical infinitesimal symmetry condition, we must check the following system

Pr(n)v[ΔV(x,u(n))]V=1,,l=0,wheneverΔV(x,+u(n))=0,(4)

where Pr(n)v called n-th prolongation of v is

Prnv=v+α=1qJDJφαi=1pξiuiα+i=1pξiuJ,iαuJα,(5)

where J = (j1,…, jk) with 1≤kp is a multi-indices, and Di represents the total derivative with respect to the i-th independent variable xj[1, 13].

Theorem 2.1

LetX=ξ1(x,t,u)x+ξ2(x,t,u)t+φ(x,t,u)ube an infinitesimal generator of the classical Lie point symmetry groups forBBMandMBBMequations; then we have, respectively

ξ1=c1,ξ2=c2t+c3,φ=12c22ac2ua,(6)

and

ξ1=13(x+2t)c1+c2,ξ2=c1t+c3,φ=13c1u,(7)

wherecisfori = 1,2,3 are arbitrary constants.

Proof

At first applying the invariance condition (4) for Eq. (1), we have

X(3)[ut+uxa(u2)xbuxxt]=0,(8)

where X(3) is the third prolongation obtained using (5), with the following form

X(3)=X+J=(j1,,jk)[DJ(φξ1uxξ2ut)+ξ1uJ,x+ξ2uJ,t]uJ,(9)

where DJ=Dj1Djk and Q depend on x, t, u and first order derivatives of u. Substituting (9) into (8) and introducing the relation ut=ux+a(u2)x+buxxt to eliminate ut we are left with a polynomial equation involving the various derivatives of u(x, t) whose coefficients are certain derivatives of ξ1, ξ2 and φ. We can equate the individual coefficients to zero, and have the complete set of determining equations as below:

ξx1=ξu1=ξt1=0,ξx2=ξtt2=ξu2=0,φ=12(2au1)ξt2a.

By solving these equation we obtain (6). For MBBM, applying above approach to Eq. (2) leads to the complete set of determining equations

ξu1=ξx2=ξtt2=ξu2=0,ξt1=23ξt2,ξx1=13ξt2,φ=13ξt2u,(10)

and solving (10) leads to (7). □

Corollary 2.2

The Lie algebras of infinitesimal projectable symmetries ofBBMand MBBM equations are spanned by the vectorfields in (11) and (12), respectively

X1=x,X2=t,X3=2att+(12au)u,(11)

{\it and}

Y1=x,Y2=t,Y3=(x+2t)x+3tuu.(12)

The commutator tables of Lie algebras gBBM and gMBBM for BBM and MBBM equations are given in Table 1 and 2 respectively, where the entry in the i-th row and j -th column is defined as [Xj, Xj] = XjXj−XjXj. The relations between these vector fields in Table 1 and 2 say that the Lie algebras gBBM and gMBBM are solvable, because in gBBM, we have

g(1)=[g,g]=X2,g(2)=[g(1),g(1)]={0},andgR×a(2).
Table 1

The commutator table of gBBM

[Xi, Xj]X1X2X3
X1000
X2002aX2
X30−2aX20
Table 2

The commutator table of gMBBM

[Yi}, Yj]Y1Y2Y3
Y100Y1
y2002Y1
y3Y1−2Y10

Similarly, in gMBBM we have

g(1)=Y1,g(2)=0.

To obtain the group transformation, which is generated by the infinitesimal generators (11) and (12), we need to solve the following systems of first order ordinary differential equations for each of them, separately

dτ~(s)ds=η(x~(s),t~(s),u~(s)),τ~(0)=τ,

where η = ξ12,φ and τ = x, t, u. Consequently, we conclude the following theorems:

Theorem 2.3

Ifgi(s) is the one parameter group generated by (11), then

g1:(x,t,u)(x+s,t,u),g2:(x,t,u)(x,t+s,u),g3:(x,t,u)(x,exp(2as)t,1+exp(2as)(2au1)2a).(13)
Theorem 2.4

Ifgi(s) is the one parameter group generated by (12), then

g1:(x,t,u)(x+s,t,u),g2:(x,t,u)(x,t+s,u),g3:(x,t,u)(62t6s+exp(s)(x+2t+6),t+3s,uexp(s)).(14)

In general a family of solutions, called group-invariant solutions, will correspond to each parameter subgroup of the full symmetry group of a system.

Theorem 2.5

Ifu = f(x, t) is a solution ofBBMequatin, so are the functions

u1=f(xϵ,t),u2=f(x,tϵ),u3=1exp(2aϵ)+2aexp(2aϵ)f(x,texp(2aϵ))2a.
Theorem 2.6

Ifu = f(x, t) is a solution of MBBM equation, so are the functions

u1=f(xϵ,t),u2=f(x,tϵ),u3=exp(ϵ)f(x+66exp(ϵ)2texp(ϵ)+6sexp(ϵ)+2texp(ϵ),t3ϵ).

3 Classification of group invariant solutions

The Lie group theory plays an important role in finding the exact solutions of differential equations and any transformation in the full symmetry group will take a solution to another solution, so it is sufficient to find invariant solutions which are not related to transformations in the full symmetry group. There are a set of group-invariant solutions for every s-parameter subgroup of the full symmetry group G. Since for every full symmetry group there are infinite number of such subgroups, it's very difficult to know all of them. The problem of finding an optimal system of subgroups is equivalent to finding an optimal system of subalgebras. For one-dimensional subalgebras, this classification problem is essentially the same as the problem of classifying the orbits of the adjoint representations. Therefore, by taking a general element in the Lie algebra and subjecting it to various adjoint transformations we simplify it as much as possible, because two connected s-dimensional subqroups of the Lie group G are conjugate if and only if their subalgebras are conjugate subalgebras [1, 2].

The adjoint action is given by the Lie series

Ad(exp(sXi)Xj)=XjsLXi(Xj)+s22LXi2(Xj),

where LA(B) = adA(B) = [A, B] is the commutator for the Lie algebra, s is a parameter and i, j = 1,2,3. Adjoint representation of infinitesimal symmetries of BBM and MBBM equations are shown in Table 3 and 4.

Table 3

Adjoint representation (BBM equation)

AdX1X2X3
X1X1X2X3
X2X1X2X3 − 2asX2
X3X1(1 + 2as)X2X3
Table 4

Adjoint representation (MBBM equation)

AdY1Y2Y3
Y1Y1Y2Y3sY1
Y2Y1Y2Y3 − 2sY1
Y3(1 + s)Y1Y2 + 2sY1Y3
Theorem 3.1

One-dimensional optimal system of BBM equation is provided by these vector fields

1:αX1+X3,2:X1+βX2,3:X2.(15)
Proof

Let X = a1X1 + a2X2 + a3X3 be a nonzero vector field of gBBM. We will simplify as many of the coefficients ai, i = 1,2,3 as possible through proper adjoint applications on X. We demonstrate our aim as follows:

  1. At first, assume that a3 ≠ 0. We can scale X if necessary and assume that a3 = 1, so we get X = a1X1 + a2X2 + X3, using the Table 3, if we act on X with Ad(exp(sX2), the coefficient of X2 can vanish:

    X=a1X1+X3,

    which by any applying Ad doesn't change.

  2. II. Now assume that a3 = 0 and a1 ≠ 0, by scaling X, we can assume that a1 = 1. Now by the action of Ad(exp)(sXi) i = 1,2,3, the coefficient doesn't change, so we have

    X=X1+βX2,
  3. III. Another case is a1 = 0 and a2 ≠ 0. By any scaling it doesn't change, so

    X=X2.

There is not any more possible case and the proof is complete. □

we can proof

Theorem 3.2

One-dimensional optimal system of MBBM equation is provided by these vector fields

1:αY2+Y3,2:Y1+βY2,3:Y2.(16)

According to our optimal systems of one-dimensional subalgebras of the full symmetry algebra g, we only need to find group-invariant solutions for one-parameter subgroups generated by (15) and (16).

4 Symmetry reduction and differential invariants for BBM and MBBM equations

The fundamental theorem on group-invariant solutions roughly states that the solutions which are invariant under a given r-parameter symmetry group of the system can all be found by solving a system of differential equations involving r fewer independent variables than the original system. Assume G is a symmetry group that acts regularly on Δ, that is a system of differential equation defined on an open subset MX × U, the space of independent and dependent variables. The reduced system Δ/G is a differential equation on M/G by p + q − s functionally independent invariant on M, that determine global coordinates on M/G, where s denotes the dimension of the orbits of G.

We can now compute the invariants associated with the symmetry operators (15) and (16) by integrating the characteristic equations. In continuation, we will find some group-invariant solutions for both BBM and MBBM equations. For example, take operator t, so we have dx0=dt1=du0 and the corresponding invariants are I1 = x, I2 = u and a similarity solution of the form y = y(x) . Now substitute it into (1) and (2) respectively, to determine the form of the function y. Finally we have y′ − 2ayy′ = 0 and y′ + ay2y′ + y′′′ = 0 as reduced equations of BBM and MBBM. Solving these ODEs leads to a solutions for BBM and MBBM. For example, by solving y′ − 2ayy′ = 0, we have

u(x,t)=12a+candu(x,t)=c,

where c is an arbitrary constant. Another results are in Table 5, 6, 7 and 8.

Table 5

Reduction of BBM equation

operatoryvu
X1tuv(y)
X2xuv(y)
X3xt(1 − 2au)12a(1v(y)t)
αX1 + X32aαxlntt(1 − 2au)12a(1v(y)t)
X1 + βX2βxtuv(y)
Table 6

Reduced equations (BBM equation)

operatorsimilarity reduced equations
X1vY = 0
X2vY − 2avyv(y) = 0
X312at2(v(y)v(y)vybvyy)=0
αX1 + X312at2(vy+v(y)2aα(vyv(y)2abα(vyyyvyy))=0
X1 + βX2−vy + βvY − 2vYv(y) + 2vyyy = 0
Table 7

Reduction of MBBM equation

operatoryvu
Y1tuv(y)
Y2xuv(y)
y33 ln(x + 2t) − tlnu+t3exp(v)(y)t3)
αY2 + Y3(α + 3) ln (x + 2t) − tlnu+t3+αexp(v)(y)t3+α)
Y1 + βY2βx − tuv(y)
Table 8

Reduced equations (MBBM equation)

operatorsimilarity reduced equations
Y1vy = 0
Y2vy + av2(y)vy + vyyy = 0
Y3exp(v(y)t3)(vy(6x+2t1)13+3vyx+2t+3avyx+2texp(2(v(y)t3))+1(x+2t)3(81vyvyy27vy227vyy+27vy3+27vyyy+6vyy)
αY2 + Y3exp(v(y)tα+3)(vy(2α+6x+2t)1α+3+α+3x+2tvy+aα+3x+2texp(v(y)(tα+3)vy+α+3(x+2t)33(α+3)vyy+(α+3)2vyyy+2(α+3)2vyvyy+2vy2(α+3)vy2(α+3)vy+(α+3)2vyy+(α+3)2vy2))
Y1 + βY2−vy + βvy + v(y)2vy + β3vyyy

Now we turn the whole procedure around and ask the complementary question: What is the most general type of differential equation which admits a given group as a group of symmetries? For an answer we introduce differential invariants, that play an important role in this procedure. Let SΔMn be the corresponding subvariety to Δ(x, un), so SΔ is invariant under the n-th prolongation Pr(n)(G) . Furthermore, there is an equivalent equation Δ~=0 describing the subvariety SΔ, where Δ~ depends only on the invariants of the group action Pr(n)(G) . An n-th order differential invariant of G is a smooth function η : MnR, depending on x, u and derivatives of u such that η is invariant on the prolonged group action Pr(n)(G), namely

η(Pr(n)g.(x,u(n)))=η(x,u(n)),(x,u(n))MngG.

If G is a symmetry group for a system of PDEs with functionally differential invariants, we can rewrite the system in terms of these invariants. To calculate differential invariants of a system the following systems of PDEs must be solved

Ix,It,tItuIu,I1x,I1t,tI1tuI1uuxI1uX2utI1ut,I2x,I2t,tI2tux2I2ux22uxtI2uxt3ut2I2ut2,(17)

where I, I1 and I2 are smooth functions of (x, t, u), (x, t, u, ux, ut) and (x, t, u, ux, ut, uxx, uxt, utt) respectively. The solutions of (17) for (1) and (2) are shown in 9 and 10. Note in Table 10, m = LambertW((2t+x+6)6exp((2t+x+6)6)) that LambertW(x).exp(LambertW(x)) = x.

Table 9

Differential invariants for BBM equation

vector fieldordinary1st order2nd order3nd order
v1t, uux, utuxx, uxt, uttuxxx, uxxt, uxtt, uttt
v2x, uux, utuxx, uxt, uttuxxx, uxxt, uxtt, uttt
v3x,(2au1)t2auxt, utt2uxxt, uxtt2, uttt3uxxx, uxxt, uxtt, uttt
Table 10

Differential invariants for MBBM equation

vector fieldup to 3nd order
v1t, u, ux, ut, uxx, uxt, utt, uxxx, uxxt, uxtt, uttt
v2x, u, ux, ut, uxx, uxt, utt, uxxx, uxxt, uxtt, uttt
v3exp(−t/3)(2t + x + 6), mux, m3uxx, −m2(2uxxuxt), m4uxxx, −m3(2uxxxuxxt), mu, −m(2uxut), m(4uxx − 4uxt + utt), m2(4uxxx - 4uxxt) + uxtt, −m(8uxxx − 12uxxt + 6uxttuttt)

5 Conservation laws for BBM and MBBM equations

A conservation law of differential equation Δ(x, u(n)) = 0 is a divergence expression

DivP=D1P1++DpPp=0,

which vanishes for all solutions of the system. Here P = (P1(x, u(n)),..., Pp(x, u(n))) is a p-tuple of smooth functions of x = (x1,..., xp), u = (u1,..., uq) and derivative of u on the jet space X × U(n); this requires

P(x, u(n)) to be constant for all solutions of the system. Thus a conservation law for a system is equivalent to the classical notion of a first integral or constant of the motion of the system. This definition in characteristic form is

DivP=Q.ΔwhereQ=(Q1,,QL),

L-tuple Q is characteristic of this conservation law. In general, the characteristics are determined up to the equivalence and are not unique. In other words, if Q and Q¯ are characteristics of one conservation law, then also is QQ¯ and is called trivial characteristic, and two characteristics Q and QQ¯ are equivalent. The Euler operator is defined as bellow:

Eα=J=(j1,,jk)(D)J/uJα,1αq,1jkp,k0.
Theorem 5.1

(Theorem 1.3.2, [1, 5]). The equationsEαF(x,U,U,,US)0, hold for arbitraryU(x)if and only if for some functionsΨj(x,U,U,,Us1),i=1,qwe haveF(x,U,U,,US)DjΨj(x,U,U,,Us1)

Theorem 5.2

(Theorem 1.3.3, [5]). A local conservation law for the system ΔV(x, u(n)) is a set of non-singular local multipliersΛv(x,U,U,,Ur),v=1,,l, if and only if

Eα(Λv(x,U,U,,Ur)Δv(x,u(n)))0,1αq,(18)

for an arbitrary functionU(x)

To find all local conservation law multipliers for the system (1) and (2) of the form ξ(x, t, u, ux, uxx, uxt, utt) and η(x, t, u, ux, uxx, uxt, utt), the determining equations (18) become

Eα[ξ(x,t,U,Ux,Uxx,Uxt,Utt)[Ut+Ux2aUUxbUxxt]0,(19)
Eα[η(x,t,U,Ux,Uxx,Uxt,Utt)[Ut+Ux+aU2Ux+Uxxx]]0,(20)

where U(x, t) is an arbitrary function. The solutions of (19) and (20) or the set of local multipliers of all nontrivial local conservation laws for BBM and MBBM equations are

ξ=c3uxt+abc3u2+c1u+c2andη=112a(18c3uxt+a2(3c3u5+(12tc1+4c2)u3)+a(6c3u3+12c5+u(6c3ux2+12c1(tx)+12c4)+12uxx(3tc1+c2+c3u2))),

where ci, i = 1, 2, 3, 4, 5 are arbitrary constants. So local multipliers are given by:

ξ1=1,ξ2=u,ξ3=uxt+au2,
η1=1,η2=u,η3=uxx+a3u3,η4=3tuxx+atu3+tuxu,
η5=12u(u2ux2+a2u4)+u2uxx32auxt.

Each pair of the local multipliers ξ and φ determine a nontrivial local conservation law for BBM and MBBM equations, respectively, that in characteristic form are

DtΨ1+Dxφ1ξ.(Ut+Ux2aUUxbUxxt),

and

DtΨ2+Dxφ2η.(Ut+Ux+aU2Ux+Uxxx).

To calculate Ψ1, φ1, Ψ2 and φ2, we must apply integration of an expression in multi-dimensions involving arbitrary functions and its derivatives, which is very complicated, but we can do it by the homotopy operator tool (explicit formula) [15].

Definition 5.3

(Hu(x,t)(x)f,Hu(x,t)(t)f)that are defined as below, are the components of a 2-dimensional homotopy operator

Hu(x,t)(m)f=01j=1qIuj(m)f[λu]dλλ,wherem=x,t,(21)

the x-integrand, Iu(x,t)j(x)f and x-integrand, Iu(x,t)j(t)f are

Iuj(x)f=k1=1M1jk2=0M2ji1=0k11i2=0k2B(x)uxi1ti2j(Dx)k1i11(Dt)k2i2fuxk1tk2j,
Iuj˙(t)f=k1=0M1jk2=1M2ji1=0k1i2=0k21B(t)uxi1ti2j(Dx)k1i1(Dt)k2i21fuxk1tk2j,

whereM1j,M2jare the order off inujwith respect to x and t respectively, and

B(x)=B(i1,i2,k1,k2)=C(i1+i2,i1)C(k1+k2i1i21,k1i11)C(k1+k2,k1),B(t)=B(i2,i1,k2,k1).

The results of applying (21) for BBM and MBBM are in Table 11.

Table 11

Integrands

Ψ=Hu(x,t)f(x)φ=Hu(xt)f(t)
ξ = 1

ξ = u

ξ=uxt+abu2
uau223buxt

12u223au323buuxt+13buxut3buxt2+a3bu3a22bu4au2uxtb12ut(uxxttuxxt)+14ut(ut+ux)+14u(uxtutt)+b6uxuxtt
u13buxx

12u2+16bux213buuxx14u(uxtuxx)+b12uuxxxt+14ux(ut+ux)b12uxuxxt+a3bu3b6uxxuxt
η = 1u+13au3+uxxu
η = u12u2+14au4+uuxx12ux212u2
η=uxx+a3u312(a6u4+a29a2u6uuxt+uxut+ux2+23au3uxx+uxx2)12uuxx+112au4
η=3tuxx+atu3+tuxu12atu2(u2+13au4+2u3uxx)+12(tu2xu212axu43tuuxt+3tuxut+xux2+3tuxx2uux)uuxx(xt)+tux214tau4+12tu212xu2+32tuuxx
η=a4u5+u2uxx+12u332auxt12ux2u18u2(52uxut+au4+u22ux2au2ux2+4uxx2)38a(ut2+uxut+uxxxut+uuxt+uutt+uuxxxt)+34auxuxxt+12uuxx(12au4+u2ux2)+132a2u8+18ux434uxt(uxxa+712u3)18u2(13au4+u2+72u3uxx+12ux2)38a(uuxtuuxxuuxxxx+uxut+ux2+uxuxxx)

Thus we have a set of conservation laws for BBM and MBBM equations, as shown below:

Dx(uau223buxt)+Dt(u13buxx)=0,Dx(12u223au323buuxt+13buxut)+Dt(12u2+16bux213buuxx)=0,Dx(3buxt2+a3bu3+14u(uxtutt)a22bu4au2uxtb12ut(uxxttuxxt)+14ut(ut+ux)+b6uxuxtt)+Dt(a3bu3+14u(uxtuxx)+b12uuxxxt+14ux(ut+ux)b12uxuxxtb6uxxuxt)=0,

and

Dx(u+13au3+uxx)+Dt(u)=0,Dx(12u2+14au4+uuxx12ux2)+Dt(12u2)=0,Dx(12(a6u4+a29a2u6uuxt+uxut+ux2+23au3uxx+uxx2))+Dt(12uuxx+112au4)=0,Dx(12atu2(u2+13au4+2u3uxx)uuxx(xt)+tux2+12(tu2xu212axu43tuuxt+3tuxut+xux2+3tuxx2uux))+Dt(32tuuxx+14tau4+12tu212xu2)=0,Dx(18u2(52uxut+au4+u22ux2au2ux2+4uxx2)+132a2u834uxt(uxxa+712u3)38a(ut2+uxut+uxxxut+uuxt+uutt+uuxxxt)+34auxuxxt+12uuxx(12au4+u2ux2)+18ux4)+Dt(18u2(13au4+u2+72u3uxx+12ux2)38a(uuxtuuxxuuxxxx+uxut+ux2+uxuxxx))=0.

6 Conclusion

In this paper we use the classical Lie point symmetry method for the Benjamin-Bona-Mahony (BBM) and Modified Benjamin-Bona-Mahony (MBBM) equations. We obtained the general form of infinitesimal generators of BBM and MBBM equations, the exact solutions associated with the symmetries, the optimal system of one-dimensional sub-algebras for symmetry algebras of these systems, the invariants associated with the symmetry operators by integrating the characteristic equations to reducted BBM and MBBM equations, and the differential invariants and conservation laws of BBM and MBBM equations.

Acknowledgement

The second author would like to thank Mr. Saeed Dodangeh to his contribution to this project.

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Received: 2016-8-4
Accepted: 2016-10-28
Published Online: 2016-12-30
Published in Print: 2016-1-1

© 2016 Khorshidi et al.

This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 3.0 License.

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