
Citation: M. Hamid, T. Zubair, M. Usman, R. U. Haq. Numerical investigation of fractional-order unsteady natural convective radiating flow of nanofluid in a vertical channel[J]. AIMS Mathematics, 2019, 4(5): 1416-1429. doi: 10.3934/math.2019.5.1416
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The exponential growth of natural convection radiating flow has gained a considerable attention in the developing research area. Many numerical, theoretical and experimental investigation has been made for natural convection radiating flow of viscous fluids in vertical cylinders, in a channel and over an infinite plate. Fujii et al. [1] experimentally analyzed the natural-convection transfer of heat from the external surface of a vertical cylinder to liquids. Fujii and Imura [2] provided an experimental investigation about concerning natural-convection heat transfer from a plate with arbitrary inclination. In their study they restricted the boundary layer flow to 2D (two-dimensional). Ezzat, [3] examined the heat transport and MHD thermoelectric flow of non-Newtonian fluid with fractional derivative. Arshad et al. [4] studied the natural convection heat transfer from a bounded assembly of thin non-horizontal cylinders. Their work was purely reported an experimental study of natural convection. Eldabe et al. [5] numerically examines the influence of viscous dissipation on free convection heat and mass transfer of MHD non-Newtonian fluid flow through a porous medium. Rubbab et al. [6] analyzed the natural convection flow near a vertical plate. Ellahi [7] analytically examined the impacts of temperature dependent viscosity and MHD flow of nanofluid in a pipe. Natural convection flow along an isothermal vertical flat plate with temperature dependent viscosity and heat generation examined by Molla et al. [8]. Ezzat et al. [9] described the heat and mass transfer through a MHD time-depended viscoelastic fluid enclosed by infinite vertical plates. The simulations are performed via Laplace-transform method (LTM) and behavior of concentration, temperature, velocity, electric and induced magnetic field distributions have been analyzed via set of graphs. Sheri and Thumma [10] studied the heat transfer enhancement in MHD free convection flow over vertical plate utilizing nanofluids. The readers are referred to see [11,12,13,14,15] for some recent literature related to combined analysis of MHD natural convection in different fluid problems.
The field of fluid mechanics gained a worthy consecration after the Choi contribution [16,17]. He was the pioneer who worked on improvement of the thermal conductivity of the fluids. According to his idea there is an appropriate quantity of nanoparticles inside the traditional fluids. He named the term as nanofluids. The experimental outcomes reconfirm that thermal properties of traditional fluids can be enhanced by using Choi idea. After this ground breaking innovation this domain gained a significant importance and a lot of work reported in the literature. Dinarvand et al. [18] studied the Buongiorno's model for double-diffusive mixed convective stagnation-point flow of a nanofluid considering diffusiophoresis effect of binary base fluid. Three dimensional mesoscopic simulation of magnetic field effect on natural convection of nanofluid studied by Sheikholeslami and Ellahi [19]. Sheikholeslami and Ganji [20] analyzed the nanofluid convective heat transfer. They used both numerical and analytical approaches to investigate the said nanofluid model. Usman et al. [21] used an analytical technique (DTM) to investigate the unsteady nanofluid flow and heat transfer. Hassan et al. [22] conducted a model study for both magnetic and non-magnetic particles in nanofluid over a wedge and presented a comparative analysis. Mohyud-Din [23] reported the influence of Marangoni convection and thermal radiation effects on CNT-Water flow of nanofluid. A least squares technique is adopted to present the analysis for said flow model while findings are asserted with the help of graphical sets. The thermal boundary thickness and temperature both enhanced while increase the nanoparticle friction. It is reported that the velocity of the fluid is decreased for both kinds of CNTs. Hamid et al. [24] examined the heat and mass transport for MHD time-dependent flow of nanofluid in the presence of natural convection, thermal radiation and heat sink/source. The solution of reduced nonlinear PDEs is obtained via Crank-Nicolson finite difference scheme. The small values of time with increasing Reynolds number an enhanced velocity distribution is perceived. The temperature profile is dropped for Biot numbers while enhanced for higher values of Reynolds, Brownian motion, thermophoresis, and heat source numbers. An inclusive study associated to nanofluids via various aspects can be find in [25,26,27,28,29].
Previously, the fractional calculus theory has gained extensive concern because of its large range of applications in various areas of engineering and physics [30]. The fractional calculus has been exploited with ample success in the description of complex dynamics such as wave, viscoelastic and relaxation behaviors. In fractional calculus due to development of operator a straightforward technique for presenting fractional derivatives into models of linear viscous is to change the first derivative in the constitutive equation of the natural convection model with an α∈0, 1 order fractional derivative. The fractional calculus provides some noticeable contributions in relating frequent technological and scientific situations such as capacitor theory, viscoelasticity, electrical circuits, electro-analytical chemistry, diffusion and neurology [31,32]. Different methods have been proposed by various authors to tackle non-linearity of fractional differential equations [33,34,35,36]. Although there is a comprehensive research literature available on the fluid flows, many mathematical models employed the fractional calculus to solve a variety of applied fluid flow problems. We are citing some recent literate related to said domain [37,38,39,40].
The present work is an extension of [40] in which we analyzed the unsteady natural convection radiating flow in an open ended vertical channel beside the magnetic effects. The channel is stationary with non-uniform temperature. We utilized a fractional calculus approach for the constitutive relationship of a fluid model. The finite difference approach [41] along with Crank Nicolson method [42] has been successfully applied [13,28]. The careful literature survey witnesses that this scheme has never been reported in the literary. The physical changes are discussed with the help of graphical plots. The expression for both velocity field and temperature distribution has been made via said scheme. Finally, a detailed discussion about the influence of various related dimensionless parameters upon the flow properties disclosed our work.
Let us examine the effects of heat transfer of unsteady, one dimensional, naturally convected, and viscous flow. It is also consider that the fluid is enclosed between two non-uniform, stagnant and parallel walls separated by distance d, x and y- axis are considered along flow direction and normal to flow direction respectively. Assume that the temperature of wall and fluid has constant value T∞. Furthermore, temperature of plate reserved at y = 0 and t > 0 is preserved as initial temperature T∞ and natural convection current is produced because the temperature of wall kept at y = d is raised up and is considered Tw. Applied Magnetic field is considered constant and electric field is pondered as zero. The induced magnetic field is neglected due to small Reynolds number. In view of Boussinesq approximation, flow can be explained with the help of following partial differential equations [40]
∂u∂t=νnf∂2u∂y2+gρnfβnf(T−T∞)+1ρnf(J×B)x, | (1) |
(ρCP)nf∂T∂t=knf∂2T∂y2−∂qr∂y, | (2) |
where u(y,t),T(y,t),g,νnf,ρnf,βnf,σnf,(CP)nf,knf,J are the velocity along x-axis, temperature along x-axis, gravitational acceleration, kinematics viscosity for nano-fluid, density of nano-fluid, heat transfer constant for nano-fluid, electrical conductivity for nano-fluid, heat capacity of for nano-fluid, thermal conductivity for nano-fluid, current density respectively and also defined as [12].
νnf=μnfρnf,μnf=μf(1−ϕ)2.5,ρnf=ρf((1−ϕ)+ϕρsρf), | (3a) |
(ρcp)nf=(1−ϕ)(ρcp)f+ϕ(ρcp)s,(ρβ)nf=(1−ϕ)(ρβ)f+ϕ(ρβ)s | (3b) |
where ρf, ρs, βf, βs, μnf, μf and ϕ are density of fluid, density of solid particle, heat transfer constant for fluid, heat transfer constant for solid particle, viscosity of nano-fluid, viscosity of fluid, viscosity of solid particle and solid volume fraction respectively.
The value of current density is
J=σnf(E+V×B), | (4) |
where E is the electric field. Cogley et al. [43], shows that [30]:
∂qr∂y=4(T−T∞)∫∞0kλw(debλdt)wdλ, | (5) |
where kλ, ebλ, w are the absorption coefficient, plank function and value at the wall y = d. Substituting the values from Eqs (4) and (5) into Eqs (1) and (2), once obtained
∂u∂t=νnf∂2u∂y2+gρnfβnf(T−T∞)−σB20ρnfu, | (6) |
(ρcP)nf∂T∂t=knf∂2T∂y2−4(T−T∞)I, | (7) |
where I=∫∞0kλw(debλdt)wdλ..
The associated initial and boundary condition of problem (6)–(7) are
u(y,0)=u(0,t)=u(1,t)=0,T(y,0)=T(0,t)=T∞,T(1,t)=Tw. |
Introducing the transformation for Eqs (6) and (7) is given by
u=νfdU,t=d2vft∗,y=dY,T−T∞=(Tw−T∞)T∗. | (8) |
Using (3) and (8), once obtained
[(1−ϕ)+ϕρsρf]∂U∂t∗=1(1−ϕ)2.5∂2U∂Y2+GrT∗[(1−ϕ)+ϕ(ρβ)s(ρβ)f]−M2U, | (9) |
[(1−ϕ)+ϕ(ρβ)s(ρβ)f]Pr∂T∗∂t∗=knfkf∂2T∗∂Y2−RT∗,y∈[0,1],t≥0, | (10) |
where Gr, M2, Pr and R are the Grashof number, Hartmann number, Prandtl number and radiation parameter and is defined as
Gr=gβf(Tw−T∞)d3ν2f,M2=σB20d2μf,Pr=μf(cP)fkf,R=4Id2kf. |
After applying the above transformations boundary condition reduces as:
u(y,0)=0,u(0,t)=0,u(1,t)=0,T(y,0)=0,T(0,t)=0,T(1,t)=1. |
The Caputo time fractional form of Eqs (9) and (10) are explained as
[(1−ϕ)+ϕρsρf]Dαtu(y,t)=1(1−ϕ)2.5∂2u∂y2+GrT[(1−ϕ)+ϕ(ρβ)s(ρβ)f]−M2u, | (11) |
[(1−ϕ)+ϕ(ρβ)s(ρβ)f]PrDαtT(y,t)=knfkf∂2T∂y2−RT, | (12) |
where DαtT(y,t){1Γ(1−α)∫t01(t−τ)α∂T(y,τ)∂τdτ,0<α<1,∂T(y,t)∂t,α=1..
In this section, we introduce the well-known Crank-Nicholson finite difference scheme for the numerical solution of the following fractional partial differential equations:
ρnfρf∂α∂tαu(y,t)=1(1−ϕ)2.5∂2∂y2u(y,t)−M2u(y,t)+(ρβ)nf(ρβ)fGrT(y,t), | (13) |
(ρcp)nf(ρcp)fPr∂α∂tαT(y,t)=knfkf∂2∂y2T(y,t)−RT(y,t), | (14) |
along with the boundary conditions associated with (13–14). In above 0 < α≤1 is Caputo derivative of fractional order. Consider that the above fractional-order system has sufficiently smooth and has a unique. Assume that xj = jh, 0≤j≤M with Mh = 1 and tn = nτ, 0≤n≤N. Here h and τ indicates the space and time step length, M and N are represents the number of grids point. Fractional order derivate can discretize as [41]:
DαtQ(y,t)=1ταΓ(2−α)[Qn+1j−Qnj+n∑i=1(Qn−i+1j−Qn−ij)((i+1)1−α−i1−α)]+O(τ), |
and the second order derivative using Crank-Nicholson idea can be discretize as under:
∂2∂y2Q(y,t)=12h2[(Qn+1j+1−2Qn+1j+Qn+1j−1)+(Qnj+1−2Qnj+Qnj−1)]+O(h2). |
Using the above discretize formulas, system (12–13) takes the following form:
−ω˜u˜un+1j+1+(ϑ˜u+2ω˜u)˜un+1j−ω˜u˜un+1j−1=ω˜u˜unj+1+(ϑ˜u−2ω˜u−M2)˜unj+ω˜u˜unj−1+(ρβ)nf(ρβ)fGr˜Tnj−ϑ˜u∑ni=1(˜un−i+1j−˜un−ij)bi,
−ω˜T˜Tn+1j+1+(ϑ˜T+2ω˜T)˜Tn+1j−ω˜T˜Tn+1j−1=ω˜T˜Tnj+1+(ϑ˜T−2ω˜T−R)˜Tnj+ω˜T˜Tnj−1−ϑ˜T∑ni=1(˜Tn−i+1j−˜Tn−ij)bi,
where ω˜u=1(1−ϕ)2.512h2,ϑ˜u=ρnfρf1ταΓ(2−α),ω˜T=knfkf12h2,ϑ˜T=(ρcp)nf(ρcp)fPrταΓ(2−α),bi=((i+1)1−α−i1−α).
A1v1=Bv0+(ρβ)nf(ρβ)fGrCv0, |
for n≥1,
An+1vn+1=Bn+1vn+sn+11vn+sn+12vn−1+…+sn+1nv1+bn+1v0+(ρβ)nf(ρβ)fGrCvn. |
In above An+1,Bn+1,vn,sn+1n,C and bn+1 are represents the block matrices which defined as follow:
An+1=[A˜un+1OOA˜Tn+1],Bn+1=[B˜un+1OOB˜Tn+1],C=[OIOO],sn+1n=[cTnOOdTn]n+1,vn=[uT]n,bn+1=[bTnOObTn]n+1, |
where the matrices A˜un+1,A˜Tn+1,B˜un+1,B˜Tn+1,B˜un+1,cTn,dTn,I and bTn present in [31] and u and T are given as:
un=[un1,un2,un3,…,unM−2,unM−1]T,Tn=[Tn1,Tn2,Tn3,…,TnM−2,TnM−1]T. |
This section explore the behavior of non-dimensional velocity and temperature profiles under the influence of the various physical parameters for various values of α. Figures 1-7 are plotted along with comprehensive discussion for the purpose.
In Figures 1 and 2 are plotted to explain the behavior of velocity of nano- fluid (Copper Cu and Aluminum oxide Al2O3 based) for different values of fractional parameter "α" as well as Grashof number "Gr", Hartmann number "M", time "t" and solid volume fraction "ϕ". Figure 1(a) is plotted against the variation of Grashof number "Gr" for the numerous values of "α". It is observed that velocity profiles demonstrate the increasing behavior with the increase in both Grashof number "Gr" and parameter "α". For the small value of Grashof number the effect of parameter "α" is insignificant and vice versa. Effect of Hartman number "M" and parameter "α" on velocity profile plotted in Figure 1(b). Decreasing behavior of velocity field is detected for different values of Hartmann number "M". This is because the increasing values of Hartmann number "M" corresponds the increaser the magnitude of magnetic field. That is why, magnetic forces against the flow process is increasing which become the cause to decrease the velocity of nano- fluid (Copper Cu and Aluminum oxide Al2O3-based). Behavior of the velocity profile due to the variation in Prandtl number "Pr" and parameter "α". Again similar behavior is achieved under the impact of Prandtl number "Pr" as we got in previous figure that is velocity profiles decreases gradually as Prandtl number "Pr" increases. Dominant effect of parameter "α" can be seen for the least value of Prandtl number "Pr". Effect of time "t" and parameter "α" analyze in Figure 2(b). Velocity field increases gradually as time increase. Behavior of velocity for different values of fractional parameter "α" and solid volume fraction "ϕ" is present in Figure 3.
Observation shows that velocity is decreasing gradually while we are increasing the values of fractional parameter α and solid volume fraction "ϕ". From Figures 1–3, we observed that velocity profiles have dominant values for the case of Cu-based nanofluid as compare to Al2O3-based nanofluid.
To scrutinize the variation in temperature distribution against the different values of time "t", radiation parameter "R", Prandtl number "Pr" and solid volume fraction "ϕ" Figures 4-8 are portrayed for both Copper (Cu) and Aluminum oxide (Al2O3) based nanofluid.
Figure 4 shows the effect of time "t" and parameter "α" on the temperature field. It is found that temperature profiles increases as upsurge the values of time "t". On the other hand, for the small value of "α" behavior of temperature profile is linear. Effect of radiation parameter "R" with the numerous values of "α" deliberated in Figure 5.
Temperature profiles decreases as increasing the radiation parameter. Dominant effect of radiation parameter "R" can be seen at the center of channel. Also, temperature increases as parameter "α" decreases gradually. Behavior of Prandtl number "Pr" and "α" on the dimensionless temperature profile demonstrated in Figure 8. Enhancement in Prandtl number decrease the temperature distribution gradually. Lastly, effect of solid volume fraction "ϕ" and parameter "α" on temperature distribution pondered in Figure 7. Here temperature of the fluid enhanced as enhancing both parameters. From Figures 4-7, we observe that temperature profiles have dominant values for the case of Cu-based nanofluid as compare to Al2O3 based nanofluid. Figure 8(a–b) is plotted to demonstrate the comparison of proposed finite difference scheme with published work [30]. Figure 8(a) clearly exhibit that the obtained solutions are excellent agreement with published work. The main advantage of the proposed method that it is accurate and can be extended for nonlinear problem. Figure 8(b) shows the comparison of temperature profile for different values of time and fractional-order parameter α, it can be noted that for all values of α and t the achieved solutions shows the good agreement with analytical solutions [30]. Table 1 is constructed for the estimation of L2, L∞ and RMS norms using the following relations.
α | Norms | t=0.1 | t=0.5 | t=0.9 |
0.4 | L2 | 2.65×10-2 | 3.28×10-3 | 1.50×10-3 |
L∞ | 2.64×10-2 | 3.27×10-3 | 1.49×10-3 | |
RMS | 5.90×10-3 | 7.33×10-4 | 3.37×10-4 | |
0.7 | L2 | 1.80×10-2 | 1.78×10-3 | 6.45×10-4 |
L∞ | 1.79×10-2 | 1.77×10-3 | 6.44×10-4 | |
RMS | 4.02×10-3 | 3.98×10-4 | 1.44×10-4 | |
1.0 | L2 | 5.07×10-2 | 3.90×10-4 | 3.82×10-5 |
L∞ | 5.06×10-2 | 3.90×10-4 | 3.82×10-5 | |
RMS | 1.13×10-2 | 8.73×10-5 | 8.55×10-6 |
Ej=Tj−˜Tj,L∞=maxj|Ej|,L2=√M∑j=1|E2j|,RMS=√1MM∑j=1|E2j|. |
It concluded that proposed method is accurate, stable and well-matched to tackle this problem and also can be extended fractional-order nonlinear problem of physical nature.
In the presence of magnetic effects, we analyzed the unsteady natural convection radiating flow in an open ended vertical channel. We assumed the channel is stationary with non-uniform temperature. The finite difference approach coupled with Crank Nicolson method has been successfully applied to obtain the solution of said fluid model. Hence, key findings of our study are stated below:
● The temperature decreased due to increase in fractional parameter and radiative parameter R.
● The temperature increased when we enhanced the value of time.
● The velocity of the fluid decreased while enhancing the radiative parameter R as well as Prandtl number Pr.
● The Grashof number Gr enhanced the velocity of the fluid while fluid velocity decreased with the passage of time t.
● For lesser values of time t, while increase in the fractional parameter α the velocity of the fluid increases but after some critical values of time tc the behavior is reverse.
The corresponding author is grateful for the support of Peking University through the Boya Post-doctoral Fellowship. The first author is thankful to Prof. Wei Wang and Chinese scholarship council for providing him an opportunity to study in China and research-oriented environment.
The authors declare that there is no conflict of interests.
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α | Norms | t=0.1 | t=0.5 | t=0.9 |
0.4 | L2 | 2.65×10-2 | 3.28×10-3 | 1.50×10-3 |
L∞ | 2.64×10-2 | 3.27×10-3 | 1.49×10-3 | |
RMS | 5.90×10-3 | 7.33×10-4 | 3.37×10-4 | |
0.7 | L2 | 1.80×10-2 | 1.78×10-3 | 6.45×10-4 |
L∞ | 1.79×10-2 | 1.77×10-3 | 6.44×10-4 | |
RMS | 4.02×10-3 | 3.98×10-4 | 1.44×10-4 | |
1.0 | L2 | 5.07×10-2 | 3.90×10-4 | 3.82×10-5 |
L∞ | 5.06×10-2 | 3.90×10-4 | 3.82×10-5 | |
RMS | 1.13×10-2 | 8.73×10-5 | 8.55×10-6 |
α | Norms | t=0.1 | t=0.5 | t=0.9 |
0.4 | L2 | 2.65×10-2 | 3.28×10-3 | 1.50×10-3 |
L∞ | 2.64×10-2 | 3.27×10-3 | 1.49×10-3 | |
RMS | 5.90×10-3 | 7.33×10-4 | 3.37×10-4 | |
0.7 | L2 | 1.80×10-2 | 1.78×10-3 | 6.45×10-4 |
L∞ | 1.79×10-2 | 1.77×10-3 | 6.44×10-4 | |
RMS | 4.02×10-3 | 3.98×10-4 | 1.44×10-4 | |
1.0 | L2 | 5.07×10-2 | 3.90×10-4 | 3.82×10-5 |
L∞ | 5.06×10-2 | 3.90×10-4 | 3.82×10-5 | |
RMS | 1.13×10-2 | 8.73×10-5 | 8.55×10-6 |