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https://doi.org/10.1007/s12043-019-1837-9

Chemically reactive flow of thixotropic nanofluid with thermal radiation

MADIHA RASHID1,∗, TASAWAR HAYAT1,2, KIRAN RAFIQUE1and AHMED ALSAEDI2

1Department of Mathematics, Quaid-I-Azam University 45320, Islamabad 44000, Pakistan

2Nonlinear Analysis and Applied Mathematics (NAAM) Research Group, Department of Mathematics, Faculty of Science, King Abdulaziz University, Jeddah 21589, Saudi Arabia

Corresponding author. E-mail: madiha.rashid@math.qau.edu.pk

MS received 25 October 2018; revised 5 May 2019; accepted 31 May 2019

Abstract. This article addresses the flow of a thixotropic liquid with nanomaterials due to a stretching sheet of variable thickness. The stimulus effects of the heat source/sink and first-order chemical reaction are retained.

Convective conditions of heat and mass transfer are also considered at the boundary. Unlike the classical consideration, the linear thermal radiation aspect is examined. The influence of emergent flow, heat and mass parameters on velocity, concentration and temperature fields are shown graphically. It is also noted that the velocity of the fluid significantly favours the non-Newtonian parameters. For higher values of radiation and heat source/sink parameter, the temperature rises. Moreover, a novel investigation on heat and mass transfer rates subject to nanomaterials (i.e. Brownian motion and thermophoresis) in the liquid has been carried out. Nonlinear systems are solved by the optimal homotopy analysis method (OHAM). Convergence analysis has been executed and the optimal values are computed. The main advantage of the proposed technique is that it can be directly utilised in highly nonlinear systems without using discretisation, linearisation and round-off errors. The table shows the results of the error analysis.

Keywords. Thixotropic nanofluid; porous medium; thermal radiation; convective boundary conditions; first-order chemical reaction; heat source/sink.

PACS Nos 44.40.+a; 44.90.+c; 82.30.−b

1. Introduction

Nanofluid is a uniform suspension of ultrafine nano- sized particles (metallic/non-metallic/nanofibres) with the typical size less than 100 nm of diameter in base fluids, such as water, ethylene, toluene and oil. Some common nanoparticles are copper, aluminium, silver [1], silicon [2], diamond [3], titanium [4] and car- bon nanotubes [5] which tend to enhance thermal conductivity. Experimental investigation revealed that the thermal performance of nanofluids depends on particle material, particle shape, particle volume frac- tion, temperature, particle size and base fluid material.

Nanofluids have attained great importance in many engineering and biological fields such as catalysis, electronics, solar cells, medicines, glass industry, mate- rial manufacturing, laser cutting, plasma, etc. Choi [6] initiated the basic mechanism of nanofluids to

enhance their thermal characteristics. Buongiorno [7]

observed enhanced thermal conductivities with the insertion of Brownian motion and thermophoresis prop- erties in a flow. Babu and Sandeep [8] worked on nanofluids with thermophoresis and Brownian motion aspects due to stretching sheets. A review of the ther- mal conductivity of various nanofluids was done by Ahmadi et al [9]. Uddin et al [10] studied the con- vective flow of nanofluids. For further details, see refs [1–5,11,12].

Nowadays, the boundary layer flow of non-Newtonian fluids is a hot topic of research and such fluids can be used in fibre technology, coating of wires, ketchup, slurries, drilling muds, shampoo, apple sauce, synovial fluid and heather honey. Non-Newtonian fluids exhibit a nonlinear relationship between shear stress and strain rate. The thixotropic fluid model is one of these models.

The thixotropic fluid exhibits a reduction in viscosity 0123456789().: V,-vol

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over time at a constant shear rate. Sadeqi et al [13]

elaborated the Blasius flow of thixotropic materials.

Deus and Dupim [14] investigated the behaviour of thixotropic fluids. Shehzad et al [15] worked on the chemically reactive flow of thixotropic fluids subject to stretching sheets. In a doubly stratified medium, the flow analysis of thixotropic nanomaterials with mag- netic field effects is discussed by Hayat et al [16].

Zubair et al [17] elaborated the flow of thixotropic fluid with the Cattaneo–Christov heat flux model. A comparison of non-thixotropic and thixotropic mate- rials in a tube is presented by Abedi et al [18].

Qayyum et al [19] presented the flow of thixotropic nanofluids subject to a stretched surface of variable thickness.

Heat and mass transport in the flow of an incom- pressible fluid due to the stretching surface has been extensively investigated by many researchers. Recently, an attempt has been made to introduce variable thick- nesses on stretching surfaces. Due to the acceleration or deceleration of the surface, the thickness of the stretched surface may decrease or increase depending on the value of the power index of velocity. Presently, fluid flow sub- ject to stretching surfaces with variable thicknesses is an important area of research. This is due to its relevance in the industrial and engineering sectors, particularly in civil, marine, aeronautical and architectural engineer- ing. It also helps in refining the utilisation of the material.

Fanget al[20] introduced flow due to a stretched sheet of variable thickness. The flow of the thixotropic fluid with nanomaterials subject to a nonlinear stretching surface of variable thickness is modelled by Hayatet al [21].

Danielet al[22] studied the radiative flow of nanoflu- ids towards a nonlinear stretching sheet with variable thickness. A fragment’s mass distribution scaling rela- tion with variable thickness is elaborated by Zhang et al[23]. Hayatet al[24] described the MHD effects on the Al2O3−water nanofluid due to the rotating disk with variable thickness. The flow of the Maxwell fluid by a stretching sheet with variable thickness is studied by Liu and Liu [25].

The main aim of this study is to explore the flow of thixotropic nanofluid by a stretching sheet of vari- able thickness with a heat source/sink. The effects of thermal radiation and chemical reaction are also highlighted. The relevant problems are formulated.

The governing nonlinear framework is solved by the optimal homotopy analysis method (OHAM) [26–

32]. Based on the aforementioned literature survey, the flow of the thixotropic nanofluid on a stretch- ing surface with variable thickness is discussed for the first time. The immediate applications are in the melting of plastics, engine cooling and paper production.

Figure 1. Flow geometry.

2. Modelling

Consider the chemically reactive flow of a thixotropic nanofluid due to a stretching surface of variable thickness. The flow caused by the nonlinear stretching surface is restricted to the domainy >0. The stretching velocity of the sheet isuw(x)=a(x+b)n (nbeing the power-law index). The flow fills the porous medium. In this analysis, contributions due to thermophoresis and Brownian movements are studied. Heat transfer anal- ysis is performed in the presence of thermal radiation and heat generation/absorption effects. Figure 1plots the physical description.

The problem statements are:

u

∂x + v

∂y =0, (1)

ρ

u∂u

∂x+v∂u

∂y

2u

∂y2

−6Ra

u

∂y 2

2u

∂y2μ Ku

+4Rb

⎢⎢

⎢⎢

⎢⎢

⎢⎢

⎢⎢

⎢⎢

⎢⎣ u

∂y

2u

∂y2

ˆ u 2u

∂x∂y +v∂2u

∂y2

+ u

∂y 2

u 3u

∂x∂y2 +v∂3u

∂y3+∂uˆ

∂y

2u

∂x∂y

+v

∂y

2u

∂y2

⎥⎥

⎥⎥

⎥⎥

⎥⎥

⎥⎥

⎥⎥

⎥⎦ ,

⎫⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎬

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎭ (2)

(3)

u∂T

∂x +v∂T

∂y =α 2T

∂y2

⎣DB ∂C

∂y

∂T

∂y

+ D

T

T

∂T

∂y 2

− 1 ρCp

f

∂q

∂y + Qh ρCp

f

(TT),

⎫⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎭

(3)

u∂C

∂x +v∂C

∂y = DB

2C

∂y2

+ DT T

2T

∂y2

KC(CC), (4)

u =uw=a(x+b)n, v=0, −k∂T

∂y =h

TfT ,

Dm∂C

∂y =km

CfC

aty =δ(x +b)(1−n)/2,

u →0, T =T, C =C asy→ ∞,

⎫⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎭ (5) whereu,vare the velocity components parallel to thex andydirections, respectively,uwis the stretching veloc- ity,C is the volume fraction of the nanoparticles,T is the temperature,ρis the fluid density,RaandRbare the material constants,α = k/(ρC)p is the thermal diffu- sivity,kis the thermal conductivity,(ρC)pis the specific heat,kmis the mass transfer coefficient,D

T is the ther- mophoresis diffusion coefficient,τ =(ρC)p/(ρC)f is the heat capacity ratio, K is the permeability of porous space,his the heat transfer coefficient,DBis the Brown- ian diffusion coefficient andKCis the chemical reaction rate coefficient. By utilising Rosseland’s concept, the radiative heat fluxq is

q = −4σ∂T4

3k∂y , (6)

whereσandkare Stefan–Boltzmann and Rosseland’s mean absorption coefficients. Temperature is expanded aboutTinto the Taylor series

T4 ∼=4T3T −3T4. (7) Now eq. (3) is reduced to

u∂T

∂x +v∂T

∂y =α 2T

∂y2

⎣DB ∂C

∂y

∂T

∂y

+ D

T

T

∂T

∂y 2

× 1 ρCp

f

16σT3 3

2T

∂y2 + Qh

ρCp

f

(TT).

⎫⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎬

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎭ (8) Considering

u =a(x+b)nF˜(ξ),

v = −

n+1 2

νa(x+b)n1

×

F˜(ξ)+ n−1 n+1ξF˜(ξ)

,

ξ = y

n+1 2

a

ν(x+b)n1, (ξ)˜ =

TT TfT

,

φ(ξ)˜ =

CC CfC

,

⎫⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎭ (9) eq. (1) is trivially satisfied while eqs (2), (4), (5) and (8) give

F˜− 2n

n+1F˜2+ ˜FF˜ +K a(x)

n+1

2 F˜2F˜

− 2

n+1DaF˜

+K b(x)

⎢⎢

⎢⎢

⎢⎢

⎢⎢

⎢⎢

⎢⎢

n+1 2

3n−1 2

F˜4

n+1

2 F˜F˜2F˜iv

n+1

2 2

F˜F˜F˜2 +

n+1 2

5n−3 2

F˜F˜2F˜

⎥⎥

⎥⎥

⎥⎥

⎥⎥

⎥⎥

⎥⎥

=0,

⎫⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎬

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎭ (10) 1

Pr(1+R)˜+N b˜φ˜+N t˜2

+ ˜F˜+Q˜ =0, (11) φ˜+

N t N b

˜+ScF˜φ˜LcScφ˜ =0, (12)

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F˜(λ)=λ1−n

1+n, F˜(λ)=1, F˜(∞)=0, ˜(λ)= −γ1[1− ˜(λ)], (∞)˜ =0, φ˜(λ)= −γ2[1− ˜φ(λ)], φ(∞)˜ =0.

⎫⎪

⎪⎪

⎪⎪

⎪⎭

(13)

Letting

F˜ = ˜f(ξλ)= ˜f(η), ˜ = ˜θ(ξλ)= ˜θ(η),

φ˜ = ˜ϕ(ξλ)= ˜ϕ(η). (14)

we have f˜− 2n

n+1f˜2+ ˜f f˜+K a(x) n+1

2 f˜2f˜

− 2

n+1Daf˜

+K b(x)

⎢⎢

⎢⎢

⎢⎢

⎢⎢

⎢⎢

⎢⎢

⎢⎣

n+1 2

3n−1 2

f˜4

n+1

2 f˜f˜2f˜iv

n+1

2 2

f˜f˜f˜2 +

n+1 2

5n−3 2

f˜f˜2f˜

⎥⎥

⎥⎥

⎥⎥

⎥⎥

⎥⎥

⎥⎥

⎥⎦

=0,

⎫⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎭ (15) 1

Pr(1+R)θ˜+N bθ˜ϕ˜+N tθ˜2+ ˜˜+˜=0,

(16) φ˜+

N t N b

θ˜+Scf˜ϕ˜LcScϕ˜ =0, (17)

f˜(0)=λ 1−n

1+n

, f˜(0)=1, f˜(∞)=0, θ˜(0)= −γ1[1− ˜θ(0)], θ(∞)˜ =0,

˜

ϕ(0)= −γ2[1− ˜ϕ(0)], ϕ(∞)˜ =0.

⎫⎪

⎪⎪

⎪⎬

⎪⎪

⎪⎪

⎭ (18) HereKaandKbare the non-Newtonian parameters,γ1

is the thermal Biot number,γ2is the concentration Biot number, Pr is the Prandtl number, Da is the porosity parameter, Sc is the Schmidt number, Ris the radiation parameter,Nbis the Brownian motion parameter,Q is the heat generation/absorption parameter,Ntis the ther- mophoresis parameter,Lcis the reaction-rate parameter andλis the variable thickness index. These values are

K a = 6a3Ra(x+b)3n−1

ρν2 ,

K b= −4a4Rb(x+b)4n2

ρν2 ,

γ1 = h

k

((n+1)/2)(a/ν)(x+b)n1,

γ2 = km

Dm

((n+1)/2)(a/ν)(x+b)n1, Pr=

μCp

f

kf ,

Da= υ

a K(x +b)n−1, Sc= ν DB, R = 4σT3

kfk ,N b= τDB(CfC)

ν ,

Q= Qh

a(x +b)n−1 ρCp

f

, N t = τDT(TfT) νT

,

Lc= KC

a(x +b)n1, λ=δ

a(x+b)(1n)/2

2ν .

⎫⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎬

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎪⎪

⎭ (19) 3. Physical quantities of curiosity

3.1 Skin friction coefficient

Mathematically, the coefficient of skin friction is defined as

Cfx = τw 1

2ρu2w, (20)

where wall shear stressw)is expressed as τw=

μ−2Ra

u

∂y 2

u

∂y

y=λ(x+b)(1−n)/2

. (21)

Re1x/2Cf =

n+1 2

×

f˜(0)+

n+1 2

K a

3 (f˜(0))3

. (22) 3.2 Local Nusselt number

Mathematically, Nu= (x+b)qw

kf(TfT), (23)

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where the wall heat flux(qw)is expressed as qw = −kf

⎝1+16σT3 3kfk

∂T

∂y

y=λ(x+b)(1n)/2

, (24) Rex1/2Nu= −

n+1

2 (1+R)θ˜(0). (25) 3.3 Sherwood number

Mathematically, the ratio of convective mass transfer to diffusive mass transport rate is portrayed as

Sh= (x +b)qm

DB(CfC), (26) where the mass flux(qm)is expressed as

jw = −DB

∂C

∂y

y=λ(x+b)(1n)/2

, (27)

Rex1/2Sh= −

n+1

2 ϕ˜(0). (28)

In the above expressions Rex =U0(x+b)n+1f is the local Reynolds number.

4. Solution methodology

4.1 Optimal homotopic solutions

With the aim of computing the solutions, the optimal values are determined using OHAM. We select suitable operators and initial guesses as follows:

Lf˜= ˜f− ˜f, Lθ˜ = ˜θ− ˜θ, Lϕ˜ = ˜ϕ− ˜ϕ (29) with

f˜0(η)=λ 1−n

1+n

+(1−exp(−η)), θ˜0(η)= γ1

1+γ1

exp(−η), ϕ˜ = γ2

1+γ2

exp(−η),(30) and

Lf˜

d1+d2exp(η)+d3exp(−η)

=0, Lθ˜

d4exp(η)+d5exp(−η)

=0, Lϕ˜

d6exp(η)+d7exp(−η)

=0, (31)

wheredi (i=1–7)are arbitrary constants.

Figure 2. Total residual error for thixotropic nanofluid.

4.2 Convergence analysis

In homotopic solutions, convergence is obtained by set- ting the non-zero auxiliary variables h¯

f, h¯θ˜ and h¯ϕ˜. The best optimal values of the convergence control parameters areh¯

f = −1.2617, h¯θ˜ = −1.22107 and

¯

hϕ˜ = −1.04927.Following

emt =e

f

m+eθm˜ +eϕm˜, (32)

e

f

m = 1

k+1

k

l=0

⎣N

f

m

i=0

f(η),

m

i=0

θ(η)˜

η=lδη

2

, (33) emθ˜ = 1

k+1

×

k

l=0

⎣Nθ˜ m

i=0

f(η),

m

i=0

θ(η),˜

m

i=0

˜ ϕ(η)

η=lδη

2

, (34) emϕ˜ = 1

k+1

×

k

l=0

⎣Nϕ˜ m

i=0

f(η),

m

i=0

θ(η),˜

m

i=0

˜ ϕ(η)

η=lδη

2

, (35) where emt represents the total squared residual error, δη = 0.5 and k = 20.Total average squared residual error isemt =0.0284356 (see figure2and table1).

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Table 1. Magnitudes of error with optimal parameterm=2.

m εmf εθm˜ εmϕ˜

2 2.44423×102 3.81685×103 1.76489×104 4 1.04467×102 3.26281×103 6.1928×105 6 6.45867×103 3.03153×103 4.40793×105 8 4.75994×103 2.88080×103 3.85323×105 10 3.87898×103 2.79506×103 3.51377×105 12 3.34876×103 2.73319×103 3.29852×105 14 2.99461×103 2.69118×103 3.16008×105 16 2.74823×103 2.66208×103 3.05774×105 18 2.58425×103 2.64165×103 2.97839×105 20 2.49455×103 2.62736×103 2.91575×105

η

f'(η)

0 2 4 6 8 10 12

0 0.2 0.4 0.6 0.8 1

Ka = 0, 0.2, 0.4, 0.6 λ= 0.1, Da = Kb = 0.3, n = 0.9

Figure 3. f˜(η)againstKa.

η

0 2 4 6 8 10 12

0 0.2 0.4 0.6 0.8 1

Kb = 0.1, 0.4, 0.7, 1.0 λ= 0.1, Da = Ka = 0.3, n = 0.9

f'(η)

Figure 4. f˜(η)againstKb.

η

0 2 4 6 8 10 12

0 0.2 0.4 0.6 0.8 1

Da = 0.2, 0.7, 1.3, 2.0

λ= 0.1, Ka = Kb = 0.3, n = 0.9

f'(η)

Figure 5. f˜(η)againstDa.

0 2 4 η6 8 10 12

0 0.2 0.4 0.6 0.8 1

n = 1, 2, 3, 4

λ= 0.1, Da = Ka = Kb = 0.3

f'(η)

Figure 6. f˜(η)againstn.

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η

θ(η)

0 2 4 6 8 10 12

0 0.05 0.1 0.15 0.2

Nb = 0.1, 0.4, 0.8, 1.1

λ= Lc = 0.1, Nt = Q =γ1=γ2= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = 0.3, Pr = 1.3, Sc = 1

Figure 7. θ(η)˜ againstNb.

η

0 2 4 6 8 10 12

0 0.05 0.1 0.15 0.2

Nt = 0.1, 0.3, 0.5, 0.7

λ= Lc = 0.1, Q =γ1=γ2= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = Nb = 0.3, Pr = 1.3, Sc = 1

θ(η)

Figure 8. θ(η)˜ againstNt.

η

0 2 4 6 8 10 12

0 0.1 0.2 0.3 0.4 0.5

γ1= 0.2, 0.4, 0.6, 0.8

λ= Lc = 0.1, Nt = Q =γ2= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = Nb = 0.3, Pr = 1.3, Sc = 1

θ(η)

Figure 9. θ(η)˜ againstγ1.

η

0 2 4 6 8 10 12

0 0.05 0.1 0.15 0.2

Pr = 1.0, 1.5, 2.0, 2.5

λ= Lc = 0.1, Nt = Q =γ1=γ2= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = Nb = 0.3, Sc = 1

θ(η)

Figure 10. θ(η)˜ against Pr.

η

0 2 4 6 8 10 12

0 0.05 0.1 0.15 0.2 0.25

Q = 0.2, 0.3, 0.4, 0.5

λ= Lc = 0.1, Nt =γ12= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = Nb = 0.3, Pr = 1.3, Sc = 1

θ(η)

Figure 11. θ(η)˜ whenQ>0.

η

0 2 4 6 8 10 12

0 0.05 0.1 0.15 0.2

Q = -0.2, -0.3, -0.4, -0.5

λ= Lc = 0.1, Nt =γ1=γ2= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = Nb = 0.3, Pr = 1.3, Sc = 1

θ(η)

Figure 12. θ(η)˜ whenQ<0.

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η

φ(η)

0 2 4 6 8 10 12

0 0.05 0.1 0.15 0.2 0.25

Nt = 0.1, 0.3, 0.5, 0.7

λ= Lc = 0.1, Q =γ1=γ2= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = Nb = 0.3, Pr = 1.3, Sc = 1

Figure 13. φ(η)˜ againstNt.

0 2 4 η6 8 10 12

0 0.05 0.1 0.15 0.2 0.25

Nb = 0.1, 0.4, 0.8, 1.1

λ= Lc = 0.1, Nt = Q =γ1=γ2= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = 0.3, Pr = 1.3, Sc = 1

φ(η)

Figure 14. φ(η)˜ againstNb.

η

0 2 4 6 8 10 12

0 0.1 0.2 0.3 0.4 0.5

γ2= 0.1, 0.3, 0.5, 0.7

λ= Lc = 0.1, Nt = Q =γ1= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = Nb = 0.3, Pr = 1.3, Sc = 1

φ(η)

Figure 15. φ(η)˜ againstγ2.

η

0 2 4 6 8 10 12

0 0.05 0.1 0.15 0.2

Lc = 0.1, 0.3, 0.5, 0.7

λ= 0.1, Nt = Q =γ1=γ2= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = Nb = 0.3, Pr = 1.3, Sc = 1

φ(η)

Figure 16. φ(η)˜ againstLc.

η

0 2 4 6 8 10 12

0 0.05 0.1 0.15 0.2

Sc = 0.5, 1.0, 1.5, 2.0

λ= Lc = 0.1, Nt = Q =γ1=γ2= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = Nb = 0.3, Pr = 1.3

φ(η)

Figure 17. φ(η)˜ against Sc.

Kb Rex1/2 Cf

0 2 4 6 8 10 12

-1 0 1 2 3 4 5 6

Ka = 0, 0.2, 0.4, 0.6 λ= 0.1, Da = 0.3, n = 0.9

Figure 18. (Rex)1/2Cf againstKa.

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Ka Rex1/2 Cf

0 2 4 6 8 10 12

-1.2 -1 -0.8 -0.6 -0.4 -0.2

Kb = 0.1, 0.4, 0.7, 1.0 λ= 0.1, Da = 0.3, n = 0.9

Figure 19. (Rex)1/2Cf againstKb.

Nt Rex-1/2 Nu

0 2 4 6 8 10 12

0.204 0.207 0.21 0.213

Nb = 0.1, 0.4, 0.8, 1.1 λ= Lc = 0.1, Q =γ12= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = 0.3, Pr = 1.3, Sc = 1

Figure 20. (Rex)1/2Nu againstNb.

5. Discussion

5.1 Velocity

Figures 3 and 4 are plotted to analyse the behaviour of K a =0.0,0.2,0.4,0.6 and K b=0.0,1.4,0.7,1.0 for velocity f˜(η).Here thixotropic parametersKaand Kb significantly favour the velocity f˜(η).Physically, K a,K b<1 leads to a shear thinning case in which the viscosity varies with time. A reduction in fluid viscos- ity is noted for largerKaandKb. Hence fluid velocity increases. From figure5, it can be seen that the veloc- ity field diminishes for larger local porosity parameters (Da=0.2,0.7,1.3,2.2). Due to the presence of porous space, resistance is produced in the liquid flow which is the reason for the reduced fluid velocity. Multiple values

Nb Rex-1/2 Nu

0 2 4 6 8 10 12

0.204 0.207 0.21 0.213

Nt = 0.1, 0.3, 0.5, 0.7 λ= Lc = 0.1, Q =γ1=γ2= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = 0.3, Pr = 1.3, Sc = 1

Figure 21. (Rex)1/2Nu againstNt.

ofnfor the velocity profilef˜(η)are depicted in figure6.

Velocity is enhanced forn >1 near the surface.

5.2 Temperature profile

The influence of the Brownian motion parameter Nb (N b=0.1,0.4,0.8,1.1)onθ(η)˜ is plotted in figure7.

Temperature and thermal layer thickness show an increasing trend for Brownian motion (Nb). Physically, collision of particles occurs for increasing values of the Brownian motion parameter which enhances the irregular motion of nanoparticles. As a consequence, kinetic energy is transformed into heat energy, resulting in temperature enhancement. Figure8depicts an enhancement in temperature for the thermophore- sis motionNt(N t =0.1,0.3,0.5,0.7).It is due to the thermophoresis phenomenon that the temperature of the fluid increases, in which heated particles are pulled away from a hot region to a cold surface. The effect of the thermal Biot numberγ11=0.2,0.4,0.6,0.8)for temperatureθ(η)is plotted in figure9. An increase in γ1 causes a stronger convection which shows a higher temperature profile θ(η). The impact of Prandtl num- ber Pr(Pr=1.0,1.5,2.0,2.5)on temperature θ(η)˜ is plotted in figure10. It is noted that temperature θ(η)˜ shows a decreasing trend for Prandtl number (Pr).

Physically, bigger values of Pr yield weaker thermal diffusivity which corresponds to a decay in temperature.

The impact of the heat generation/absorption parame- ter (Q > 0 or Q < 0) on temperature is plotted in figures11and12. A rise in temperature is observed for higher Q (Q >0). Physically, the internal energy of liquid particles rises for higher values ofQ. Therefore, the temperature increases. A reverse trend is noticed for Q<0.

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λ Rex-1/2 Sh

0 2 4 6 8 10 12

-5.5 -5 -4.5 -4 -3.5 -3 -2.5

γ2= 0.4, 0.8, 1.1, 1.3

Lc = 0.1, Nt= Q =γ1= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = Nb = 0.3, Pr = 1.3, Sc = 1

Figure 22. (Rex)1/2Sh againstγ2. 5.3 Concentration field

Figure13 depicts the effect of thermophoresis motion parameter Nt (N t =0.1,0.3,0.5,0.7) on concentra- tion ϕ(η)˜ . It is noted that the concentration enhances for larger values ofNt. There is no doubt that thermal conductivity increases in the presence of nanoparti- cles. Higher values of Nt enhance fluid thermal con- ductivity. Larger thermal conductivity leads to high concentration. Figure14elucidates the variation ofNb (N b=0.1,0.4,0.8,1.1)forϕ(η).˜ Physically, for larger Nb, collision among the fluid particles rises and the cor- responding concentration decreases. Figure 15 shows the results of the plot to study the variation of con- centrationϕ(η)˜ for larger γ2 2 = 0.1,0.3,0.5,0.7). With an increment in solutal Biot number 2), the resulting coefficient of mass transfer increases. It gives an enhancement in concentration ϕ(η)˜ . Higher values of Lc (Lc=0.1,0.3,0.5,0.7) on concentrationϕ(η)˜ are depicted in figure 16. A larger chemical reaction parameter (Lc) shows a decay in concentration ϕ(η)˜ because the chemical reaction parameter depends on the reaction rate which produces a decay in concentration

˜

ϕ(η). The impact of Schmidt number (Sc=0.5,1.0, 1.5,2.0) on concentrationϕ(η)˜ is shown in figure17.

Physically, Schmidt number (Sc) has an inverse relation with Brownian diffusivity. So a larger Schmidt number (Sc) yields a weaker Brownian diffusivity leading to lower concentrationϕ(η)˜ .

5.4 Skin friction coefficient and local Nusselt and Sherwood numbers

Figures18and19depict the impacts ofKaandKbon surface drag force. The magnitude of the skin friction coefficient shows increasing behaviour for larger values

Nt Rex-1/2 Sh

0 2 4 6 8 10 12

-1.5 -1 -0.5 0

Nb = 0.1, 0.4, 0.8, 1.1

λ= Lc = 0.1, Q =γ1=γ2= 0.2, R = 0.4, n = 0.9 Da = Ka = Kb = 0.3, Pr = 1.3, Sc = 1

Figure 23. (Rex)1/2Sh againstNb.

ofKa while decreasing behaviour forKb. ForNb and Nt, the heat transfer reduces (see figures 20 and 21).

Figures22and23show that the magnitude of Sherwood number increases for largerγ2andNb.

6. Conclusions

In this paper, the use of a thixotropic nanomate- rial towards a nonlinear stretching surface of variable thickness is addressed. In our view, no attempt at analysing the chemically reactive flow of a thixotropic nanofluid through nonlinear thermal radiation under convective conditions has been made. The velocity of fluid particles enhances the variable thickness index and the non-Newtonian parametersKaandKb, while it decays the porosity parameterDa. The temperature and concentration are enhanced through the thermophoresis variable and heat generation parameter. The skin fric- tion coefficient strongly depends on the non-Newtonian parameterKa. The Nusselt number decreases through the Brownian motion parameter and the thermophoresis parameter, respectively. The magnitude of the Sherwood number is enhanced by the Brownian motion parameter and the concentration Biot number.

References

[1] M Rashid, T Hayat and A Alsaedi, Appl. Nanosci.

(2019),https://doi.org/10.1007/s13204-019-00961-2 [2] M Irfan and M Khan,Appl. Nanosci.(2019),https://doi.

org/10.1007/s13204-019-01012-6

[3] F Mashali, E M Languri, J Davidson, D Kerns and G Cunningham, Int. J. Heat Mass Transf. 129, 1123 (2019)

(11)

[4] T Hayat, M Rashid and A Alsaedi, Appl. Nanosci.

(2019),https://doi.org/10.1007/s13204-019-01028-y [5] J H Lee, Y Jung, J H Kim, S J Yang and T J Kang,

Carbon. N. Y.147, 559 (2019)

[6] S U S Choi,Enhancing thermal conductivity of fluids with nanoparticles(ASME, FEC 231/MD, USA, 1995) pp. 99–105

[7] J Buongiorno,J. Heat Transf.128, 240 (2006)

[8] M J Babu and N Sandeep,Adv. Powder Technol.27, 2039 (2016)

[9] M H Ahmadi, A Mirlohi, M A Nazari and R Ghasem- pour,J. Mol. Liq.265, 181 (2018)

[10] M J Uddin, W A Khan and A I M Ismail,Proc. Power Res.7, 60 (2018)

[11] W A Khan, A S Alshomrani, A K Alzahrani, M Khan and M Irfan,Pramana – J. Phys.(2018),https://doi.org/

10.1007/s12043-018-1634-x

[12] T Hayat, K Rafique, T Muhammad, A Alsaedi and M Ayub,Results Physiother.8, 26 (2018)

[13] S Sadeqi, N Khabazi and K Sadeghy,Commun. Nonlin- ear Sci. Numer. Simul.16, 711 (2011)

[14] H P A Deus and G S P Dupim, Phys. Lett. A6, 478 (2013)

[15] S A Shehzad, T Hayat, A Asghar and A Alsaedi,J. Appl.

Fluid Mech.8, 465 (2015)

[16] T Hayat, M Waqas, M I Khan and A Alsaedi,Int. J. Heat Mass Transf.102, 1123 (2016)

[17] M Zubair, M Waqas, T Hayat, M Ayub and A Alsaedi, Results Physiother.8, 1023 (2018)

[18] B Abedi, R Mendes and P R S Me,J. Pet. Sci. Eng.174, 437 (2019)

[19] S Qayyum, T Hayat, A Alsaedi and B Ahmad,Results Physiother.7, 2124 (2017)

[20] T Fang, J Zhang and Y Zhong, Appl. Math. Comput.

218, 7241 (2012)

[21] T Hayat, S Qayyum, A Alsaedi and B Ahmad,Results Physica B: Condens. Matter537, 267 (2018)

[22] Y S Daniel, Z A B Aziz, Z Ismail and F Salah,J. Comput.

Des. Eng.5, 232 (2018)

[23] Z Zhang, F Huang, Y Cao and C Yan, Int. J. Impact Eng.120, 79 (2018)

[24] T Hayat, M Rashid, M I Khan and A Alsaedi,Results Physiother.9, 1618 (2018)

[25] L Liu and F Liu,Appl. Math. Lett.79, 92 (2018) [26] S J Liao,Appl. Math. Comput.147, 499 (2004) [27] J Sui, L Zheng, X Zhang and G Chen,Int. J. Heat Mass

Transf.85, 1023 (2015)

[28] M Irfan, M Khan, W A Khan and M Ayaz,Phys. Lett.

A382, 1992 (2018)

[29] S Gupta, D Kumar and J Singh, Int. J. Heat Mass Transf.118, 378 (2018)

[30] M Rashid, M I Khan, T Hayat, M I Khan and A Alsaedi, J. Mol. Liq.276, 441 (2019)

[31] M Khan, M Irfan and W A Khan,Pramana – J. Phys.

(2018),https://doi.org/10.1007/s12043-018-1690-2 [32] M Khan, M Irfan, W A Khan and M Ayaz, Pra-

mana – J. Phys. (2018), https://doi.org/10.1007/

s12043-018-1579-0389

References

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