Exact solutions for free convection flow of generalized Jeffrey fluid: A Caputo-Fabrizio fractional model

Exact solutions for free convection flow of generalized Jeffrey fluid: A Caputo-Fabrizio fractional model

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Alexandria Engineering Journal (2017) xxx, xxx–xxx

H O S T E D BY

Alexandria University

Alexandria Engineering Journal www.elsevier.com/locate/aej www.sciencedirect.com

ORIGINAL ARTICLE

Exact solutions for free convection flow of generalized Jeffrey fluid: A Caputo-Fabrizio fractional model Muhammad Saqib a, Farhad Ali a,*, Ilyas Khan b, Nadeem Ahmad Sheikh a, Syed Aftab Alam Jan a, Samiulhaq c a

Department of Mathematics, City University of Science and Information Technology, Peshawar 25000, Pakistan Basic Engineering Sciences Department, College of Engineering Majmaah University, Majmaah 11952, Saudi Arabia c Department of Mathematics, Islamia College University, Peshawar 25000, Pakistan b

Received 29 December 2016; revised 22 February 2017; accepted 4 March 2017

KEYWORDS Caputo-Fabrizio fractional derivatives; Generalized Jeffrey fluid; Free convection; The Laplace transform; Exact solutions

Abstract The present article reports the applications of Caputo-Fabrizio time-fractional derivatives. This article generalizes the idea of free convection flow of Jeffrey fluid over a vertical static plate. The free convection is caused due to the temperature gradient. Therefore, heat transfer is considered for free convection. The classical model for Jeffrey fluid is written in dimensionless form with the help of non-dimensional variables. Furthermore, the dimensionless model is converted into a fractional model called as a generalized Jeffrey fluid model. The governing equations of generalized Jeffrey fluid model have been solved analytically using the Laplace transform technique. The recovery of existing solutions in the open literature is possible through this work in terms of classical Jeffrey fluid, fractional Newtonian fluid as well as classical Newtonian fluid. For various embedded parameters, the physics of velocity and temperature profiles is studied by means of numerical computation. This report provides a detailed discussion as well as a graphical representation of the obtained results. Ó 2017 Faculty of Engineering, Alexandria University. Production and hosting by Elsevier B.V. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).

1. Introduction In 1695, L’Hospital raised a question in a letter [1] to Leibniz about the particular notation that he had used the nth derivatives of a function Dn gðrÞ=Drn , in his publication, what would be the result if n ¼ 1=2. Leibniz responds an apparent paradox * Corresponding author. E-mail address: [email protected] (F. Ali). Peer review under responsibility of Faculty of Engineering, Alexandria University.

from which one-day useful consequences will be drawn. In these words, fractional calculus was born [2]. In the recent past, fractional calculus has applications almost in every field of science, mathematics, and engineering. Some of the fields where fractional calculus has made a valuable impact included viscoelasticity, electrochemistry, electrical engineering, mechanics, signal and image processing, control theory, mechatronics and physics [3]. During the last 60 years, the concept of using fractional calculus in the development of constitutive equations for materials with memory has been proposed

http://dx.doi.org/10.1016/j.aej.2017.03.017 1110-0168 Ó 2017 Faculty of Engineering, Alexandria University. Production and hosting by Elsevier B.V. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/). Please cite this article in press as: M. Saqib et al., Exact solutions for free convection flow of generalized Jeffrey fluid: A Caputo-Fabrizio fractional model, Alexandria Eng. J. (2017), http://dx.doi.org/10.1016/j.aej.2017.03.017

2 many times [4]. Bagley and Torvik [5] contributed to give a review of the applications of fractional calculus to viscoelasticity. Viscoelasticity of a material is defined as when it deforms exhibits both viscous and elastic behaviors through storage of mechanical energy and simultaneous dissipation. Mainardi [6] investigated the connections among fractional calculus, wave motion, and linear viscoelasticity. Makris et al. [7], presented a general boundary element modeling for the prediction of dynamic response of viscoelastic fluids. The generalized constitutive equations are formulated with fractional order derivatives. The proposed models are valid for the fluid motions with infinitesimally small displacement gradient and for fluids with linear viscoelastic behavior. Many scholars have used the concept of fractional calculus in their study, see [8–13] and the references therein. The famous definitions of fractional derivatives in fractional calculus are Riemann-Lioville, Grunwald-Letnikov, Caputo, Oldhan and Spanier, Miller and Ross and Kolwankar and Gangal [12]. Mostly Riemann-Liouville and Caputo fractional derivative are used [13,14]. Tan and Xu [15] studied the flow of generalized second-grade fluid using the definition of Riemann-Lioville fractional derivatives and obtained the exact analytic solutions with help of the Laplace transform. Wenchang et al. [16] applied the Riemann-Liouville fractional derivative approach to the flow of generalized Maxwell fluid between two parallel plates. Shahid [17], used the approach of Caputo fractional derivatives for the study of heat and mass transfer in MHD flow over an oscillating plate. Vieru et al. [18] analyzed the time-fractional free convection flow of generalized viscous fluid using the concept of Caputo fractional derivatives. Khan et al. [19] developed a mathematical model for generalized Casson fluid with Caputo fractional operator. However, there are some discrepancies in applications of these operators. In the case of Riemann-Liouville fractional derivatives, the derivative of a constant is not zero and the Laplace transform contains terms without physical significance. On the other hand, the kernel of the Caputo fractional derivatives is a singular function. To overcome this shortcoming, Caputo and Fabrizio developed a new approach without singularities [20]. The Caputo-Fabrizio time-fractional derivatives are convenient in the application of the Laplace transform. To develop a fractional model often, in the governing equations of the classical fluid model the time derivatives can be replaced with fractional derivatives of order a. Shah and Khan [21] applied the idea of the Caputo-Fabrizio fractional derivatives to generalize the starting flow of second grade fluid over a vertical plate and obtained the exact solutions using the Laplace transform technique. Some other recent studies can be found in [22–27] and the references therein. Non-Newtonian fluids have received the attention of the researchers due to their industrial and engineering applications, for instance, in dying of paper, plastics manufacturing, textile industry, food processing, wire and blade coating and movement of biological fluids [28]. Among them, the one that is widely used is the Jeffrey fluid model. The exact analysis of free convection flow of Jeffery fluid has been performed by Khan [29]. Zin et al. [30] considered the thermal radiation effect on the convective flow of Jeffery fluid with ramped wall temperature. Zeeshan and Majeed [31], studied the magnetic dipole effect on the convective flow of Jeffery fluid, past a porous plate with suction and injection. Some interesting and recent studies can be found in [32–41] and the references

M. Saqib et al. therein. Motivated from the above discussed literature, we have chosen Jeffery fluid model for the present analysis. More exactly, the aim of the present work was to generalize the work of Khan [29]. We have converted the classical model to fractional model called as generalized Jeffrey fluid model using the fractional derivative operator of Caputo-Fabrizio. The closed form solutions have been obtained using the Laplace transform. Closed form solutions are important for many reasons. They provide a standard for checking the accuracies of many approximate methods such as numerical or asymptotic. Also, these solutions can be used as a benchmark by numerical solvers and experimentalists for checking the stability of their solutions. 2. Governing equations The momentum and energy equations for incompressible Jeffrey fluid [29] are given as under the following:   @uðy; tÞ l @ @ 2 uðy; tÞ q ¼ 1 þ k2 þ qgbT ðT  T1 Þ; ð1Þ @t 1 þ k1 @t @y2 qcp

@Tðy; tÞ @ 2 Tðy; tÞ ¼k ; @t @y2

ð2Þ

subjected to the following initial and boundary conditions: uðy; 0Þ ¼ 0; Tðy; 0Þ ¼ T1 ; for all y > 0;

ð3Þ

 for t > 0 : for t > 0

uð0; tÞ ¼ 0; Tð0; tÞ ¼ Tw ; uð1; tÞ ¼ 0; Tðy; tÞ ¼ T1 ;

ð4Þ

Here uðy; tÞ is the velocity of Jeffrey fluid in x-direction, l is dynamic viscosity, k1 ; k2 are Jeffery fluid parameters, q is constant density, g is gravitational acceleration, bT is volumetric thermal expansion, Tðy; tÞ is the temperature, cp is the specific heat capacity, k is the thermal conductivity, Tw is the wall temperature and T1 is the ambient temperature as shown in Fig. 1. Introducing the non-dimensional variables: u U0 U2 T  T1 y; t ¼ 0 t; h ¼ ; y ¼ ; m m Tw  T1 U0 into Eqs. (1)(4)we obtained (‘‘*” signs are dropped to minimize

u ¼

complexity):

  @uðy; tÞ 1 @ @ 2 uðy; tÞ 1þk þ Grh; ¼ @t 1 þ k1 @t @y2

ð5Þ

@hðy; tÞ 1 @ 2 hðy; tÞ ¼ ; @t Pr @y2

ð6Þ

uð0; tÞ ¼ 0; hðy; 0Þ ¼ 0;

ð7Þ

uð0; tÞ ¼ 0; hð0; tÞ ¼ 1; uð1; tÞ ¼ 0; hð1; tÞ ¼ 0; where k ¼

k2 U20 m

 :

; Gr ¼ mgbT ðTUw3T1 Þ and Pr ¼ 0

ð8Þ lcp k

are the Jeffrey

fluid parameter, thermal Grashof number and Prandtl number respectively. In order to develop a time fractional model for the convective flow of an incompressible generalized Jeffrey fluid we

Please cite this article in press as: M. Saqib et al., Exact solutions for free convection flow of generalized Jeffrey fluid: A Caputo-Fabrizio fractional model, Alexandria Eng. J. (2017), http://dx.doi.org/10.1016/j.aej.2017.03.017

Exact solutions for free convection flow of generalized Jeffrey fluid

3

Pr1 ¼ a0 Pr and c ¼ a0 a: Solution of Eq. (14) in light of (13) is given by the following: hðy; qÞ ¼ Wðy; q; Pr1 ; c; 0Þ; where Wðg; q; m0 ; m1 ; m2 Þ ¼

ð15Þ

 rffiffiffiffiffiffiffiffiffiffiffiffiffiffi 1 m0 q : exp g q  m2 q þ m1

ð16Þ

Inverting the Laplace transform of Eq. (16), we have the following:  rffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi m0 m2 Wðg; t; m0 ; m1 ; m2 Þ ¼ exp m2 t  g m1 þ m2   Z 2m0 1 sinðgsÞ s 2 m1 t  ds exp  m0 þ s2 p 0 sðm0 þ s2 Þ Z 2m0 m2 1 sinðgsÞ  s m p ½ m þ ðm1 þ m2 Þs2  0 2 0   s2 m1 t  exp  ds: ð17Þ m0 þ s2

Figure 1

replace form:

@ ð:Þ @t

Taking the Laplace transform of Eq. (9) using initial condition from (7) and boundary conditions from (8), we arrived the following:  qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi GrðqþcÞ2 ð1þk1 Þ ð1þk1 Þa0 q uðy; qÞ ¼ Pr1 q2 fð1þa exp y ð1þa 0 kÞqcgfðqþcÞð1þk1 Þqg 0 kÞqþc ð18Þ  qffiffiffiffiffiffiffi GrðqþcÞ2 ð1þk1 Þ Pr1 q  Pr1 q2 fð1þa0 kÞqcgfðqþcÞð1þk1 Þqg exp y qþc ;

Physical geometry and coordinate system.

with

Dat ð:Þ

in Eqs. (5) and (6), which takes the

Dat uðy; tÞ ¼

1 @ 2 uðy; tÞ ð1 þ kDat Þ þ Grh; 1 þ k1 @y2

Dat hðy; tÞ ¼

1 @ hðy; tÞ ; Pr @y2

ð9Þ

for simplicity Eq. (18) can be written as follows: sffiffiffiffiffiffiffiffiffiffiffiffiffi!   d1 d2 d3 b0 q exp y uðy; qÞ ¼ þ  q þ b1 q2 q q þ a1 sffiffiffiffiffiffiffiffiffiffiffi!   d1 d2 d3 Pr1 q ; exp y  2þ  qþc q q q þ a1

ð19Þ

2

ð10Þ

here Dat ð:Þ is the Caputo-Fabrizio time fractional operator [20] and can be defined as follows:   Z t 1 aðt  sÞ 0 f ðsÞds; for 0 < a < 1: exp Dat fðtÞ ¼ 1a 0 1a ð11Þ 3. Exact solutions Applying the Laplace transform, using corresponding initial condition from (7) Eq. (10) takes the form:    1 q 1 d2 hðy; qÞ hðy; qÞ ¼ ; ð12Þ a 1  a q þ 1a Pr dy2 with transformed boundary conditions: 1 hð0; qÞ ¼ ; hð1; qÞ ¼ 0: q

ð13Þ

with

ð1þk1 Þ cð1þk1 Þ b0 ¼ a01þa ; b1 ¼ 1þac 0 k ; d1 ¼ Gr 1þk ; 0k 1 Pr1 1 Pr1 ð1a0 kÞ ; d2 ¼ Grð1 þ k1 Þ 1þkð1þk Pr Þ2 1

d3 ¼ Grð1 þ k1 Þ ½1þk

1

ðPr1 a0 kÞ2 2 1 Pr1 ð1þa0 kÞð1þk1 Pr1 Þ

1 Pr1 ; a1 ¼ c 1þk1þk : 1 Pr1 ð1þa0 kÞ

The more suitable but equivalent form of Eq. (19) is given as under the following: uðy; qÞ ¼ d1 vðy; q; b0 ; b1 Þ þ d2 Wðy; q; b0 ; b1 ; 0Þ  d3 Wðy; q; b0 ; b1 ; a1 Þ d1 vðy; q; Pr1 ; cÞ  d2 Wðy; q; Pr1 ; c; 0Þ þ d3 Wðy; q; Pr1 ; c; a1 Þ; ð20Þ

where vðg; q; m0 ; m1 Þ ¼

 rffiffiffiffiffiffiffiffiffiffiffiffiffiffi 1 m0 q ; exp g q2 q þ m1

with the Laplace inverse Z t Wðg; s; m0 ; m1 ; 0Þds: vðg; t; m0 ; m1 Þ ¼

ð21Þ

ð22Þ

0

1 ; Eq. (12) implies the following: Let us denote a0 ¼ 1a

d2 hðy; qÞ Pr1 q  hðy; qÞ ¼ 0; qþc dy2

where

Upon taking the Laplace inverse of Eq. (20), we have the following: ð14Þ

uðy; tÞ ¼ d1 vðy; t; b0 ; b1 Þ þ d2 Wðy; t; b0 ; b1 ; 0Þ  d3 Wðy; t; b0 ; b1 ; a1 Þ d1 vðy; t; Pr1 ; cÞ  d2 Wðy; t; Pr1 ; c; 0Þ þ d3 Wðy; t; Pr1 ; c; a1 Þ: ð23Þ

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Figure 2

Velocity plot for various values of k when Gr ¼ 10 and Pr ¼ 10.

4. Special cases

4.1. Classical solutions for velocity profile

The following special cases may be recovered from the general solutions (23).

Using the property of the Caputo–Fabrizio fractional derivative, when ða ! 1 ) a0 ! 1Þ, Eq. (23) is reduced to the cor-

Please cite this article in press as: M. Saqib et al., Exact solutions for free convection flow of generalized Jeffrey fluid: A Caputo-Fabrizio fractional model, Alexandria Eng. J. (2017), http://dx.doi.org/10.1016/j.aej.2017.03.017

Exact solutions for free convection flow of generalized Jeffrey fluid

Figure 3

5

Velocity plot for various values of Gr when k = 1.5 and Pr ¼ 10.

responding classical velocity profile for the Jeffrey fluid as follows: uðy; tÞ ¼ d1 vðy; t; b0 ; b1 Þ þ d2 Wðy; t; b0 ; b1 ; 0Þ  d3 Wðy; t; b0 ; b1 ; a1 Þ pffiffiffiffiffi pffiffiffiffiffi pffiffiffiffiffi d1 /ðy Pr; tÞ  d2 Uðy Pr; t; 0Þ þ d3 Uðy Pr; t; a1 Þ; ð24Þ

with 1 þ k1 1 1 þ k1 kð1 þ k1 Þ ; ; b1 ¼ a1 ¼ ; d1 ¼ ; d2 ¼  k Pr k Pr d3 ¼ kPrð1 þ k1 Þ a1 ; b0 ¼

where

Please cite this article in press as: M. Saqib et al., Exact solutions for free convection flow of generalized Jeffrey fluid: A Caputo-Fabrizio fractional model, Alexandria Eng. J. (2017), http://dx.doi.org/10.1016/j.aej.2017.03.017

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M. Saqib et al.

Figure 4

/ðg; tÞ ¼

Velocity plot for various values of Pr when k = 1.5 and Gr ¼ 10.

rffiffiffi     g2 g t g2 erf c pffiffi  g tþ e 4t ; 2 p 2 t

Uðg; t;m4 Þ ¼

e

m4 t

2



pffiffiffiffi g m4

e



ð25Þ

   pffiffiffiffi pffiffiffiffiffiffiffiffi pffiffiffiffiffiffiffiffi g g erf c pffiffi  m4 t þ eg m4 erf c pffiffi þ m4 t : 2 t 2 t ð26Þ

The obtained solutions in Eq. (24) are equivalent to the solutions obtained by Khan [29, Eq. (31)]. 4.2. Velocity profile for fractional Newtonian fluid For k1 ¼ k ¼ 0, Eq. (23) is reduced to the fractional Newtonian which is given as under the following:

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Exact solutions for free convection flow of generalized Jeffrey fluid

Figure 5

Temperature plot for various values of t and a.

Figure 6

Temperature profile for various Pr and t.

uðy; tÞ ¼ d1 vðy; t; b0 ; b1 Þ þ d2 Wðy; t; b0 ; b1 ; 0Þ  d1 vðy; t; Pr1 ; cÞ  d2 Wðy; t; Pr1 ; c; 0Þ;

ð27Þ

with b0 ¼ a0; b1 ¼ a1 ¼ c; d1 ¼

c 1 and d2 ¼ : 1  Pr1 1  Pr1

4.3. Velocity profile for classical Newtonian fluid When a ! 1 ) a0 ! 1; Eq. (27) represents the following classical Newtonian fluid: pffiffiffiffiffi uðy; tÞ ¼ Gr1 /ðy; tÞ  Gr1 /ðy Pr; tÞ; ð28Þ where Gr1 ¼

7

Gr : Pr  1

5. Skin friction and Nusselt number The dimensionless form of skin friction ðfsÞ and Nusselt number ðNuÞ is given as under the following:



1 a @uðy; tÞ

fs ¼ ð1 þ kDt Þ 1 þ k1 @y y¼0 Nu ¼ 

@hðy; tÞ

@y y¼0

ð29Þ

ð30Þ

6. Results and discussion A new definition of fractional derivatives namely the CaputoFabrizio fractional derivatives is applied and the closed form solutions for velocity and temperature distributions are obtained using the Laplace transform method. The influence of various embedded parameters such as fractional parameter a, Jeffrey fluid parameter k, thermal Grashof number Gr and Prandtl number Pr is analyzed for different values of t on velocity distribution. Temperature profile is studied for a; Pr and t. Figs. 2–4 depict the variation of a on velocity profile. The effect of a is significantly near the static vertical plate. It is interesting to observe that for small values of t the fractional modeled fluid flows faster than the classical modeled fluid. In

Please cite this article in press as: M. Saqib et al., Exact solutions for free convection flow of generalized Jeffrey fluid: A Caputo-Fabrizio fractional model, Alexandria Eng. J. (2017), http://dx.doi.org/10.1016/j.aej.2017.03.017

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Figure 7

Figure 8

Temperature profile for various values of Pr.

Comparison Plot for classical Jeffery fluid.

addition, when we take larger values of t the classical modeled fluid flows faster than the fractional modeled fluid. Furthermore, for short time the fluid velocity decays to zero asymptotically earlier as compared to larger time.

Fig. 2 shows the influence of k on the fluid velocity. Physically, k gives rise to viscous forces or increases the nonNewtonian behavior and as a result, the thickness of momentum boundary layer increases. Due to this reason the fluid velocity decreases. The velocity of the fluid is independent of Pr when Gr ¼ 0: This case is not considered here because in the present study the velocity is just because of buoyancy forces (free convection) and we sketch our graphs with the positive values of Gr. In Fig. 3 the velocity profiles for different values of Gr are presented. Clearly, the velocity increases with an increase in Gr due to the fact that larger values of Gr enhance the buoyancy forces. Pr is a non-dimensional number which shows the relationship between thermal and momentum boundary layers. The velocity distribution for various values of Pr is plotted in Fig. 4, which shows that the velocity is a decreasing function of Pr. The physics behind these phenomena is that, larger the values of Pr, thicker will be the momentum boundary layer. Consequently, the fluid flow is reduced. In order to show the effect of a; t and Pr on the temperature profile, Figs. 5–7 are plotted. Fig. 5 shows the influence of a on the temperature profile for two different values of t: For smaller value when t ¼ 0:2 the classical temperature is less than fractional temperature. On the other hand, when we choose t ¼ 2 (larger time) then this effect reverses. The effect of Pr

Please cite this article in press as: M. Saqib et al., Exact solutions for free convection flow of generalized Jeffrey fluid: A Caputo-Fabrizio fractional model, Alexandria Eng. J. (2017), http://dx.doi.org/10.1016/j.aej.2017.03.017

Exact solutions for free convection flow of generalized Jeffrey fluid Table 1

9

Variation in skin friction for different values of a.

a

t

k1

k

Pr

Gr

fs

0.2 0.5 0.7 1.00

5 5 5 5

0.5 0.5 0.5 0.5

0.5 0.5 0.5 0.5

1.5 1.5 1.5 1.5

10 10 10 10

3.500 1.754 1.028 0.559

Table 2

Variation in Nusselt number for different values of a.

a

t

Pr

Nu

0.2 0.5 0.7 1.00

5 5 5 5

10 10 10 10

2.082 1.208 0.977 0.400

is studied on temperature distribution as shown in Fig. 6. It is found that temperature decreases with increasing values of Pr; in addition the thickness of thermal boundary layer decreases. For smaller values of Pr the thermal conductivity increases; therefore, heat is able to defuse away from the heated plate more rapidly than for larger values of Pr. In Fig. 7 a comparison between classical and fractional temperate is provided. It is found that for larger values of t fractional temperature rapidly decays to zero asymptotically as compared to classical temperature but this behavior is opposite in case of smaller values of t. In Fig. 8 a comparison is provided between the classical solutions obtained in Eq. (24) of the present analysis to the solutions obtained by Khan [29, Eq. (31)]. The figure shows a strong agreement that both the solutions are equivalent. Table 1 exhibits variation in skin friction for different values of a when t ¼ 5: From the table it can be clearly observed that for large values of a, skin friction decreases which shows a strong agreement with that of velocity profiles. Table 2 presents variations in the rate of heat transfer in a. It is noticed that the rate of heat transfer decreases with increase in a which is quite opposite to that of temperature distribution. 7. Concluding remarks A fractional model has been developed for generalized Jeffrey fluid using the definition of Caputo-Fabrizio fractional derivatives. Exact solutions have been obtained with the help of the Laplace transform technique. The influence of various embedded parameters has been studied graphically. Based on the present analysis, the summarized key findings are as follows:  Fractional fluid flows faster than classical fluid for smaller values of t whereas this effect is opposite in the case of larger values of t.  The fluid velocity decreases with increasing values of k and Pr.  The fluid velocity enhances with enhancement in Gr.  It is noticed that temperature reduces for greater values of Pr.  Skin friction and rate of heat transfer decrease with increasing a.

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Please cite this article in press as: M. Saqib et al., Exact solutions for free convection flow of generalized Jeffrey fluid: A Caputo-Fabrizio fractional model, Alexandria Eng. J. (2017), http://dx.doi.org/10.1016/j.aej.2017.03.017