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Solution of Time-Fractional Navier-Stokes Equation by Using
Homotopy Analysis Method
A.A. Ragab1, K.M. Hemida2, M.S. Mohamed3 and M.A. Abd El Salam4 Mathematics Department, Faculty of Science
Al-Azhar University Nasr City (11884), Cairo, Egypt
1E-mail: [email protected]
2E-mail: [email protected]
3E-mail: m s [email protected]
4E-mail: mohamed [email protected] (Received: 26-8-12 / Accepted: 18-10-12)
Abstract
The homotopy analysis method (HAM) is used to obtain an approximate solution of the nonlinear time fractional Navier-Stokes equation by introducing the fractional derivative in the caputo’s sense. Convergence of the solution and effects for the method are discussed within comparing the obtained results with exact solution of the corresponding nonlinear problem, which indicated that the proposed method is very effective and simple. The HAM contains a certain aux- iliary parameter h which provides us with a simple way to adjust and control the convergence region and rate of convergence of the series solution. It also suggests that both the homotopy perturbation method (HPM), Adomian decom- position method (ADM) and variational iteration method (VIM) are special cases of the HAM.
Keywords: Homotopy analysis method, fractional partial differential equa- tion
1 Introduction
Nonlinear partial differential equations (NPDEs) are encountered in such var- ious fields as physics, chemistry, biology, mathematics and engineering. Many important phenomena in various field are will describe and generalize by an ordinary or partial fractional differential equations.
Recently, El-Shahed and Salem [8] have generalized the classical Navier–
Stokes equations by replacing the first time derivative by a fractional derivative of orderα ,0 < α ≤ 1. They used Laplace transform, Fourier sine transform and finite Hankel transforms to obtain exact solutions for three different special cases.
This model is generalized by replacing the first-time derivative by a frac- tional derivative of orderα ,0< α≤1. The time-fractional model for Navier–
Stokes equations has the following form Dtαu+ (u· ∇)u=−1
ρ∇P +ν∇2u, (1.1)
Where t is the time, u is the velocity vector,P is the pressure, ν is the kine- matics viscosity andρ is the density.
2 Basic Definitions
In this section we give some definitions and properties of the fractional calcu- lus. The fractional calculus is a name for the theory of integrals and derivatives of arbitrary order. Various definitions of fractional integration and differentia- tion are found in [1], [3], [7], and [12], such as Grunwald-Letnikov’s definition, Riemann-Liouville definition, and Caputo’s definition and generalized function approach. For the purpose of this paper, the Caputo’s definition of the frac- tional differentiation will be used, taking the advantage of Caputo’s approach that the initial conditions for fractional differential equation with Caputo’s derivatives take on the traditional form as for integer-order differential equa- tion.
Definition 2.1. Areal functionh(t),t >0, is said to be in the spaceCµ, µ ∈ R , if there exists a real number p > µ , such that h(t) = tph1(t) , where h1(t) ∈ C(0,∞) , and it is said to be in the space Cµn if and only if h(n) ∈ Cµ , n ∈ N
Definition 2.2. The Riemann-Liouville fractional integral operator (Jα) of orderα ≥0, of a functionh ∈ Cµ , µ≥ −1 is defined as
Jαh(t) = 1 Γ (α)
Z t
0
(t−τ)α−1h(τ)dτ] (2.1)
J0h(t) =h(t)
Γ (α) is the well known gamma function. Some of the Jα properties of the operator which we will need here are as follows:
JαJβh(t) =Jα+βh(t), JαJβh(t) =JβJαh(t), Jαtγ = Γ (γ+ 1)
Γ (α+γ+ 1) tγ+α . Definition 2.3. The fractional derivative (Dα) of h(t) in the Caputo’s sense is defined as follows
Dαh(t) = 1 Γ (n−α)
Z t
0
(t−τ)n−α−1h(τ)dτ (2.2) for
n−1< α < n, n ∈ N , t >0 , h ∈ Cn−1
The following are two basic properties of Caputo’s fractional Derivative [?]
Let h ∈ Cn−1 , n ∈ N then Dαh , 0 ≤ α ≤ n is well defined and Dαh ∈C−1
Let−1< α < n , n ∈ N and h ∈ Cnµ , µ≥ −1 then
(JαDα)h(t) =h(t)−
n−1
X
k=0
h(k) 0+ tk
k! (2.3)
3 The Homotopy Analysis Method (HAM)
The HAM [10] is applied to the nonlinear homogeneous fractional equation with a general form
N[u(r, t)] = 0. (3.1)
WhereN is a nonlinear operator for the problem,r and t denote independent variables andu(r;t) is an unknown function. By means of the HAM, one first constructs the zero-order deformation equation
(1−q)L(∈(r, t, q)−u0(r, t)) =qhH(r, t)N[∈(r, t)]. (3.2) Whereq is the embedding parameter,q ∈[0, 1], h6= 0 is an auxiliary param- eter, H(r;t) 6= 0 is an auxiliary function ,L is an auxiliary linear operator, u0(r, t) is an initial guess.
Obviously, when q= 0 andq = 1, it holds that
∈(r, t,0) =u0(r, t),∈(r, t,1) = u(r, t). (3.3)
Liao [10] expanded ∈ (x, t, q) in Taylor series with respect to the embedding parameterq, as follows:
∈(r, t, q) =u0(r, t) +
∞
X
m=1
um(r, t)qm. (3.4) Where
um(r, t) = 1 m!
∂m ∈(r, t, q)
∂qm q=0
. (3.5)
Assume that the auxiliary linear operator, the initial guess, the auxiliary pa- rameterh and the auxiliary functionH(x, t) are selected such that the series (3.4) is convergent atq = 1 ,then we have from (3.4)
u(r, t) =u0(r, t) +
∞
X
m=1
um(r, t). (3.6)
Let us define the vector
−
→un(t) = {u0(r, t), u1(r, t), u2(r, t), . . . un(r, t)}. (3.7) Differentiating (3.2)mtimes with respect to q, then settingq = 0 and dividing bym!, that the mth-order deformation equation
L(um(r, t)−χmum−1(r, t)) = hH(r, t)Rm(−→um−1). (3.8) Where
Rm(−→um−1) = 1 (m−1)!
∂m−1 N[∈(r, t, q)]
∂qm−1
q=0
. (3.9)
And
χm =
0 m≤1
1 m >1 (3.10)
The mth-order deformation Eq. (3.8) becomes linear and it can be easily solved, especially by means of symbolic computation software such as Mathe- matica, Maple, Matlab.
4 Time Fractional Navier-Stokes Equation
The Navier-Stokes equation (1.1) in cylindrical coordinates for unsteady one dimensional motion of a viscous fluid is given by
Dαtu=P +ν(∂2u
∂r2 +1 r
∂u
∂r). (4.1)
4.1 Application 1
Firstly, we consider
Dαtu=P + ∂2u
∂r2 +1 r
∂u
∂r. (4.2)
With initial condition
u(r,0) = 1−r2. (4.3)
According to the (HAM), and apply (HAM) as [4], [5] and [6] we choose the auxiliary operator as
L[∈(r, t;q)] =Dαt ∈(r, t, q). (4.4) With property L[c] = 0 where c is a constant.
We define a nonlinear operator as
N[∈(r, t, q)] =Dtα∈(r, t, q)− ∂2 ∈(r, t, q)
∂r2 − 1 r
∂ ∈(r, t, q)
∂r −P. (4.5) In order to obey the rule of solution expression and the rule of the coefficient periodicity [9], the auxiliary function can be determined uniquelyH(x, t) = 1, and
Rm(−→um−1) = Dtαum−1− ∂2
∂r2u
m−1
− 1 r
∂
∂rum−1−P (1−χm). (4.6) Now the solution of the mth-order deformation equations (3.8) for m ≥ 1 becomes
um(r, t) = χmum−1(r, t) +hL−1Rm(−→um−1). (4.7) So, the first few terms of the solution are
u0(r, t) = 1−r2 u1(r, t) = −h(−4 +P)tα Γ[1 +α]
u2(r, t) = −h(1 +h)(−4 +P)tα
Γ[1 +α] u3(r, t) = −h(1 +h)2(−4 +P)tα Γ[1 +α]
u4(r, t) = −h(1 +h)3(−4 +P)tα Γ[1 +α]
Then, we can conclude that
u(r, t) = u0(r, t) +u1(r, t) +u2(r, t) +u3(r, t) +u4(r, t). . . Then
u(r, t) = 1−r2−h(−4 +P)tα Γ[1 +α]
1 + (1 +h) + (1 +h)2+ (1 +h)3. . .
. (4.8)
Using the Geometric series as in [4], when the series tends to infinity and h must be less than 0, the solution becomes independent of h and takes the following form
u(r, t) = 1−r2+ (−4 +P)tα
Γ[1 +α] (4.9)
Which represent the exact solution of equation (4.2), also the solution is the same as S. Momani and Z. Odibat [11], and Fig. 1 and 2 shows the evolution results for the time-fractional Eq. (4.2) when α= 1 and α= 0.5 respectively.
It is easy to conclude that the solution continuously depends on the time- fractional derivative.
Fig.1 (α= 1) Fig.2 (α = 0.5)
4.2 Application 2
Consider the equation in the form Dtαu= ∂2u
∂r2 + 1 r
∂u
∂r. (4.10)
Subject to the initial condition
u(r,0) =r. (4.11)
Similarly, choosing
N[∈(r, t, q)] = Dtα ∈(x, t, q)−∂2 ∈(r, t, q)
∂r2 − 1 r
∂ ∈(r, t, q)
∂r . (4.12)
Then,
Rm(−→um−1) =Dαtum−1 − ∂2
∂r2u
m−1− 1 r
∂
∂rum−1. (4.13) So, first terms of the series are
u0(r, t) =r
u1(r, t) =− htα rΓ[1 +α]
u2(r, t) =−h(1 +h)tα
rΓ[1 +α] + h2t2α r3Γ[1 + 2α]
u3(r, t) =−h(1 +h)2tα
rΓ[1 +α] +h2(1 +h)t2α
r3Γ [1 + 2α] − 9h3t3α r5Γ[1 + 3α]
u4(r, t) =−h(1 +h)3tα
rΓ[1 +α] +3h2(1 +h)2t2α
r3Γ [1 + 2α] −3h3(1 +h)9t3α
r5Γ[1 + 3α] + 9h425t4α r7Γ[1 + 4α]
Then, we can conclude that
u(r, t) = u0(r, t) +u1(r, t) +u2(r, t) +u3(r, t) +. . . Or
u(r, t) =r− htα rΓ[1 +α]
1 + (1 +h) + (1 +h)2 + (1 +h)3. . . + h2t2α
r3Γ[1 + 2α]
1 + 2 (1 +h) + 3(1 +h)2+. . .
− 9h3t3α r5Γ[1 + 3α]
1 + 3 (1 +h) + 6(1 +h)2+. . . +. . .
As the series tends to infinity (using Geometric series as [4] where h must be less than 0), the solution becomes independent of h and takes the following form
u(r, t) =r+ tα
rΓ[1 +α] + t2α
r3Γ[1 + 2α] + 9t3α
r5Γ[1 + 3α] + 25t4α r7Γ[1 + 4α]. . . Therefore the solution is
u(r, t) =r+
∞
X
n=1
12×32× · · · ×(2n−3)2 r2n−1
tnα Γ(nα+ 1) Which is the same solution given by S. Momani and Z. Odibat [11].
Atα= 1 we have
u(r, t) = r+
∞
X
n=1
12×32× · · · ×(2n−3)2 r2n−1
tn n!
Which is the same solution given by Biazar et al. [2].
Fig. 3 and 4 shows the evolution results for the time-fractional Eq. (4.10) whenα = 1 andα= 0.5, respectively.
Fig.1 (α= 1) Fig.2 (α = 0.5)
5 Conclusion
In this paper, the homotopy analysis method (HAM) is applied to obtain the solution of time-fractional Navier–Stokes equation in cylindrical coordinates.
The results show that (HAM) is powerful and efficient techniques in finding exact and approximate solutions for nonlinear fractional partial differential equations.
The (HAM) provides us with a convenient way to control the convergence of approximation series which is a fundamental qualitative difference in analysis between (HAM) and other method. Thus the auxiliary parameter h plays an important role within the frame of the (HAM). Mathematica has been used for computations in this paper.
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