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Research Article Analytic Treatment for Electrical MHD Non-Newtonian Fluid Flow over a Stretching Sheet through a Porous Medium Gossaye Aliy Adem Department of Mathematics, University of Gondar, Ethiopia Correspondence should be addressed to Gossaye Aliy Adem; [email protected] Received 25 August 2020; Revised 26 November 2020; Accepted 11 December 2020; Published 28 December 2020 Academic Editor: John D. Clayton Copyright © 2020 Gossaye Aliy Adem. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. In this study, an attempt has been made to investigate the mass and heat transfer eects in a BLF through a porous medium of an electrically conducting viscoelastic uid subject to a transverse magnetic eld in the existence of an external electric eld, heat source/sink, and chemical reaction. It has been considered the eects of the electric eld, viscous and Joule dissipations, radiation, and internal heat generation/absorption. Closed-form solutions for the boundary layer equations of viscoelastic, second-grade, and WaltersBuid models are considered. The method of the solution includes similarity transformation. The converted equations of thermal and mass transport are calculated using the optimal homotopy asymptotic method (OHAM). The solutions of the temperature eld for both prescribed surface temperature (PST) and prescribed surface heat ux (PHF) are found. It is vital to remark that the interaction of the magnetic eld is found to be counterproductive in enhancing velocity and concentration distribution, whereas the presence of chemical reaction, as well as a porous matrix with moderate values of the magnetic parameter, reduces the temperature and concentration elds at all points of the ow domain. 1. Introduction The signicance of uid ow over a stretching surface can be professed for its ever-increasing inexorable applications in industries and in present-day technology. The applications of the stretching sheet problem are such as polymer sheet extrusion from a dye, drawing, thinning and annealing of copper wires, glass ber and paper production, and the cool- ing of a metallic plate in a cooling bath. The production of these sheets needs that the melt issues from a slit and is stretched to get the anticipated thickness. The nal product depends on the rate of cooling in the process and the process of stretching. Sakadis [1] was the rst to investigate the BL manners on a continuous solid surface moving with constant speed. Crane [2] was the rst to attain a stylish analytical solution to the BL equations for the problem of steady 2D ow through a stretching surface in an inactive incompress- ible uid. The work of Sakadis and Crane was extended and studied by several authors (Madaki et al. [3], Zheng et al. [4], Dessie and Kishan [5], and Pal [6]). The rising need for chemical reaction and hydrometallur- gical industries needs the study of heat and mass transfer with chemical reaction. There are several transport processes that are governed by the combined action of buoyancy forces due to both thermal and mass diusion in the presence of chemical reactions and electric eld eects. These processes occur in the nuclear reactor safety and combustion systems, solar collectors, metallurgical and chemical engineering, etc. In real situations, most of the uids used in engineering applications are almost non-Newtonian, specically of the viscoelastic type than the viscous type. Khan [7], Madhu and Kishan [8], Babaelahi et al. [9], Raftari and Vajravelu [10], Goyal and Bhargava [11], and Madhu and Kishan [12] have investigated the ow of viscoelastic uid ow under dif- ferent conditions. Recently, Aliy and Kishan [13] examined the eect of electric eld on MHD viscoelastic nanouid ow and heat transfer over a stretching sheet with convective boundary conditions. They have considered the local nonsi- milarity method and OHAM to solve the resulting equation. Jafar et al. [14] studied the MHD boundary layer ow of a viscoelastic uid past a nonlinearly stretching sheet in the presence of a viscous dissipation eect. Konda et al. [15] investigated the eect of nonuniform heat source/sink on MHD BLF and melting heat transfer of Hindawi Advances in Mathematical Physics Volume 2020, Article ID 8879264, 14 pages https://doi.org/10.1155/2020/8879264

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  • Research ArticleAnalytic Treatment for Electrical MHD Non-Newtonian FluidFlow over a Stretching Sheet through a Porous Medium

    Gossaye Aliy Adem

    Department of Mathematics, University of Gondar, Ethiopia

    Correspondence should be addressed to Gossaye Aliy Adem; [email protected]

    Received 25 August 2020; Revised 26 November 2020; Accepted 11 December 2020; Published 28 December 2020

    Academic Editor: John D. Clayton

    Copyright © 2020 Gossaye Aliy Adem. This is an open access article distributed under the Creative Commons Attribution License,which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

    In this study, an attempt has been made to investigate the mass and heat transfer effects in a BLF through a porous medium of anelectrically conducting viscoelastic fluid subject to a transverse magnetic field in the existence of an external electric field, heatsource/sink, and chemical reaction. It has been considered the effects of the electric field, viscous and Joule dissipations,radiation, and internal heat generation/absorption. Closed-form solutions for the boundary layer equations of viscoelastic,second-grade, and Walters’ B′ fluid models are considered. The method of the solution includes similarity transformation. Theconverted equations of thermal and mass transport are calculated using the optimal homotopy asymptotic method (OHAM).The solutions of the temperature field for both prescribed surface temperature (PST) and prescribed surface heat flux (PHF) arefound. It is vital to remark that the interaction of the magnetic field is found to be counterproductive in enhancing velocity andconcentration distribution, whereas the presence of chemical reaction, as well as a porous matrix with moderate values of themagnetic parameter, reduces the temperature and concentration fields at all points of the flow domain.

    1. Introduction

    The significance of fluid flow over a stretching surface can beprofessed for its ever-increasing inexorable applications inindustries and in present-day technology. The applicationsof the stretching sheet problem are such as polymer sheetextrusion from a dye, drawing, thinning and annealing ofcopper wires, glass fiber and paper production, and the cool-ing of a metallic plate in a cooling bath. The production ofthese sheets needs that the melt issues from a slit and isstretched to get the anticipated thickness. The final productdepends on the rate of cooling in the process and the processof stretching. Sakadis [1] was the first to investigate the BLmanners on a continuous solid surface moving with constantspeed. Crane [2] was the first to attain a stylish analyticalsolution to the BL equations for the problem of steady 2Dflow through a stretching surface in an inactive incompress-ible fluid. The work of Sakadis and Crane was extended andstudied by several authors (Madaki et al. [3], Zheng et al.[4], Dessie and Kishan [5], and Pal [6]).

    The rising need for chemical reaction and hydrometallur-gical industries needs the study of heat and mass transfer

    with chemical reaction. There are several transport processesthat are governed by the combined action of buoyancy forcesdue to both thermal and mass diffusion in the presence ofchemical reactions and electric field effects. These processesoccur in the nuclear reactor safety and combustion systems,solar collectors, metallurgical and chemical engineering, etc.

    In real situations, most of the fluids used in engineeringapplications are almost non-Newtonian, specifically of theviscoelastic type than the viscous type. Khan [7], Madhuand Kishan [8], Babaelahi et al. [9], Raftari and Vajravelu[10], Goyal and Bhargava [11], and Madhu and Kishan [12]have investigated the flow of viscoelastic fluid flow under dif-ferent conditions. Recently, Aliy and Kishan [13] examinedthe effect of electric field on MHD viscoelastic nanofluid flowand heat transfer over a stretching sheet with convectiveboundary conditions. They have considered the local nonsi-milarity method and OHAM to solve the resulting equation.Jafar et al. [14] studied the MHD boundary layer flow of aviscoelastic fluid past a nonlinearly stretching sheet in thepresence of a viscous dissipation effect.

    Konda et al. [15] investigated the effect of nonuniformheat source/sink on MHD BLF and melting heat transfer of

    HindawiAdvances in Mathematical PhysicsVolume 2020, Article ID 8879264, 14 pageshttps://doi.org/10.1155/2020/8879264

    https://orcid.org/0000-0002-2971-4889https://creativecommons.org/licenses/by/4.0/https://doi.org/10.1155/2020/8879264

  • Williamson nanofluid in a porous medium. Hayat et al. [16]studied the effects of the chemical reaction of an unsteady 3Dflow of the couple stress fluid over a stretching surface.Gireesha et al. [17] have studied the BLF and heat transferof a dusty fluid flow over a stretching sheet in the existenceof nonuniform heat source/sink and radiation. Parsa et al.[18] investigated the MHD boundary-layer flow over astretching surface with internal heat generation or absorp-tion. The thermal radiation effect was studied by differentresearchers (Weidman [19], Abel and Nandeppanavar [20],and Madaki et al. [21]).

    OHAM is an approximate analytical technique that isdirected forward to employ on a different type of problem,and the presence of any small or large parameters is notimportant. Marinca et al. [22] initially introduced the basicconcept of this method in 2008. OHAM reduces the extentof the computational domain. It is a reliable analytical tech-nique and has already been successfully applied to variousnonlinear coupled differential equations occurring in science,engineering, and other fields of study. Marinca and Herisanuapplied OHAM on the different problems (see, [23–25]).Many researchers applied OHAM to study fluid flow prob-lems [26–29]. Recently, Gossaye and Kishan [13, 30, 31]applied the OHAM to the problem arisen from electricalMHD non-Newtonian fluid flows over a stretching sheet,and Khan et al. [32] used OHAM for Lane-Emden andEmden-Fowler initial and boundary value problems.

    The novelty of the present study is starred due to thefollowing aspects.

    (i) Inclusion of electric field is justified since, for aremarkable enhancement in the value of the electricfield, the struggle among fluid particles rises, andhence, the Lorentz force inclines to speed up the bodyforces, and it leads to escalating in the flow velocityand thicker momentum boundary layer. And also,we observed that the concentration of the fluid isaffected by a large amount of an electric field.

    (ii) The dimensionless ordinary differential equationswith the corresponding boundary conditions aresolved by using the approximate analytic techniqueOHAM.

    The aim of this paper is to investigate the effect of electricfield and thermal radiation on MHD viscoelastic fluid flowover a stretching surface through a porous medium with aheat source/sink. The strongly nonlinear differentialequations are solved using the approximate analytic methodOHAM. The effects of different governing parameters onvelocity, temperature, and concentration profiles are dis-played graphically and argued extensively. Moreover, theskin-friction coefficient is also exhibited using a table.

    2. Formulation of the Problem

    Consider a steady 2D boundary layer flow of an electricallyconducting, viscoelastic fluid past a stretching surfaceembedded in a porous medium, the flow being confined to.

    Two equal and opposite forces are applied along the axis,and hence, the surface is stretched, keeping the origin fixed.Assuming that a uniformmagnetic field of strength is appliedalong that produces the magnetic effect in the direction.

    The Lorentz force is given by J × B, where J = σðE +V× BÞ, the Joule current J can be expressed as J = σðE + V ×BÞ, σ stands for the electrical conductivity, V = ðu, vÞ denotesthe velocity of the fluid, and B = ð0, B0, 0Þ and E = ð0, 0,−E0Þare the transverse magnetic field and electric field vectors,correspondingly. The magnetic field and electric field areapplied perpendicular to the flow, and hence, the Reynoldsnumber is selected small. The induced magnetic field is insig-nificant for small magnetic Reynolds number because it issmaller when compared to the applied magnetic field. Underthe usual BL conventions, the equations of continuity,momentum, energy, and concentration for the flow ofviscoelastic fluid are:

    ∂v∂y

    +∂u∂x

    = 0, ð1Þ

    v∂u∂y

    + u∂u∂x

    = υ∂2u∂y2

    −uσB20ρ

    +uv

    Kp′

    !+k0ρ

    ∂∂x

    u∂2u∂y2

    !

    + v∂3u∂y3

    +∂3u∂y3

    v +∂u∂y

    ∂2u∂y∂x

    !+σ

    ρB0E0,

    ð2Þ

    u∂T∂x

    + v∂T∂y

    � �ρCp − k

    ∂2T∂y2

    − μ∂u∂y

    � �2

    = k0∂u∂y

    ∂∂y

    u∂u∂x

    + v∂u∂y

    � �� �

    + σB20u2 −

    ∂qr∂y

    + q T − T∞ð Þ,

    ð3Þ

    u∂C∂x

    + v∂C∂y

    + Kc′ C − C∞ð Þ =D∂2C∂y2

    : ð4Þ

    The approximation of Rosseland for thermal radiationgives qr = −ð4/3Þððσ∗/3k1Þð∂T4/∂yÞÞ. It is assumed that thetemperature variation within the flow is such that may beexpanded in a Taylor series. Expanding T4 about T∞ andneglecting the higher-order terms, we have T4 = 4TðT∞Þ3− 3ðT∞Þ4,

    ∂qr∂y

    = −163

    σ∗T3∞ρCpk1

    ∂2T∂y2

    !: ð5Þ

    Taking the above equation and substituting it intoequation (3), one can get

    2 Advances in Mathematical Physics

  • u∂T∂x

    + v∂T∂y

    = α∂2T∂y2

    ρCp

    ∂u∂y

    � �2+

    16σ∗T3∞3ρCpk1

    !∂2T∂y2

    + T − T∞ð Þq

    ρCp+σB20ρCp

    u2 +k0ρCp

    � ∂u∂y

    ∂∂y

    u∂u∂x

    + v∂u∂y

    � �� �:

    ð6Þ

    The boundary conditions are

    u = uw = ax, v = vw, T = Tw xð Þ = T∞ +AxL

    � �2PST caseð Þ,

    Hw xð Þ = −k∂T∂y

    � �= B

    xL

    � �2PHF caseð Þ,

    C = Cw xð Þ = C∞ + a0xL

    � �2,mw = −D

    ∂C∂y

    � �= a1x2 as y→ 0,

    u = 0,∂u∂y

    = 0, T → T∞, C→ C∞ as y→∞:

    8>>>>>>>>>>>>><>>>>>>>>>>>>>:

    ð7Þ

    3. Solution of the Flow Field

    Equations (1) and (2) disclose self-similar solutions of thetype given below

    f =ψ

    υffiffiffiffiffiffiffiRex

    p , η = yx

    ffiffiffiffiffiffiffiRex

    p, ð8Þ

    where f represents the dimensionless stream function, ηdenotes the similarity variable, Rex = uwx/υ represents thelocal Reynolds number, and ψðx, yÞ symbolizes the streamfunction satisfying the continuity equation (1). Substitutingequation (8) in equation (2), we get

    f ′′′ + f f ′′ − f ′� �2

    + Rc 2f ′ f ′′′ − f ′′� �2

    − f f iv� �

    − M +1Kp

    !f ′ +ME1 = 0,

    ð9Þ

    where Rc = k0a/μ is the viscoelastic parameter,M = σB20/ρa isthe magnetic parameter, E1 = E0/uwB0 is the electric fieldparameter, and Kp = aKp′/υ is the nondimensional permeabil-ity parameter.

    The BCs are:

    f 0ð Þ = f w, f ′ 0ð Þ = 1, f ′ ∞ð Þ = 0, f ′′ ∞ð Þ = 0, ð10Þ

    where f w = −vwffiffiffiffiffiffiffiRex

    p/uw is the suction/injection parameter,

    and f w > 0 and f w < 0 represent suction and injection,respectively.

    Now, we apply OHAM to the nonlinear ODE (9) with theBCs (10) under the following assumption

    f = f0 + pf 1 + p2 f2, g = g0 + pg1 + p

    2g2,

    G =G0 + pG1 + p2G2, h = h0 + ph1 + p

    2h2,

    H1 pð Þ = C1p + C2p2,H2 pð Þ = C3p + C4p2,H3 pð Þ = C5p + C6p2,H4 pð Þ = C7p + C8p2,

    ð11Þ

    where the parameter p ∈ ½0, 1�, HiðpÞ, i = 1, 2, 3, 4 is anauxiliary function which is different from zero, andCj, ðj = 1, 2, 3, 4, 5, 6Þ are constants.

    And also, assume the following

    L = f ′ + f ′′,

    N = f ′′′ + f f ′′ − f ′� �2

    + Rc 2f ′ f ′′′ − f ′′� �2

    − f f iv� �

    − M +1Kp

    !f ′ +ME1 − f ′ − f ′′,

    ð12Þ

    whereN and L are the nonlinear and linear operators, respec-tively. Hence, the OHAM family of equations is given by

    H1 pð Þ − f ′� �2

    + Rc 2f ′ f ′′′ − f ′′� �2

    − f f iv� ��

    − M +1Kp

    !f ′ +ME1 + f ′′′ + f f ′′

    − f ′ + f ′′� �

    1 − pð Þ = 0:

    ð13Þ

    Using the BCs (10) and comparing the coefficients of thesame powers of p-terms, we can get the hypothesis below:

    Equating the coefficients of the zero-order equation p0,we obtain

    f0 ′′ + f0 ′ = 0, f0 0ð Þ = f w, f0 ′ 0ð Þ = 1, f0 ′ ∞ð Þ = 0, f0 ′′ ∞ð Þ = 0:ð14Þ

    Equating the coefficients of the first-order equation p1,we obtain

    − f0 ′� �2

    + Rc 2f0 ′ f0 ′′′ − f0 ′′� �2

    − f0 f0iv

    � ��

    − M +1Kp

    !f0 ′ +ME1 + f0 ′′′ + f0 f0 ′′

    �C1 − f1 ′ − f1 ′′

    + f0 ′′ + f0 ′ = 0,ð15Þ

    f1 0ð Þ = 0, f1 ′ 0ð Þ = 0, f1 ′ ∞ð Þ = 0, f1 ′′ ∞ð Þ = 0: ð16Þ

    3Advances in Mathematical Physics

  • Equating the second-order equation p2, we obtain

    f2 ′′ + f2 ′ = C1 Rc 2f1 ′ f0 ′′′ + 2f0 ′ f1 ′′′ − 2f0 ′′f1 ′′ − f1 f0iv − f0 f1iv� �h

    − M +1Kp

    !f1 ′ +ME1 + f1 ′′′ + f1 f0 ′′ + f0 f1 ′′

    − 2f0 ′ f1 ′i+ f1 ′ + f1 ′′ + C2

    � − f0 ′� �2

    + Rc 2f0 ′ f0 ′′′ − f0 ′′� �2

    − f0 f0iv

    � ��

    − M +1Kp

    !f0 ′ +ME1 + f0 ′′′ + f0 f0 ′′

    �,

    f2 0ð Þ = 0, f2 ′ 0ð Þ = 0, f2 ′ ∞ð Þ = 0, f2 ′′ ∞ð Þ = 0: ð17Þ

    After solving the ODEs (14) and (15) with the corre-sponding boundary conditions, we obtain

    f0 = e−η −1 + eη + eη f wð Þ,

    f1 = −1Kp

    c1e−2η −eη + e2η − eη f wKp + e2η f wKp − e

    ηKpM

    + e2ηKpM − eηE1KpM + e2ηE1KpM − KpRc + eηKpRc− eη f wKpRc + e

    2η f wKpRc − eηη − eη f wKpη − e

    ηKpMη

    − e2ηE1KpMη − eηKpRcη − e

    η f wKpRcη

    :

    ð18Þ

    We cannot write the third term f2 here because of itsbeing large. Hence, the solution f ðη, CiÞ in terms of theparameters can be written as:

    f η, Cið Þ = f0 ηð Þ + f1 η, Cið Þ + f2 η, Cið Þ, i = 1, 2: ð19Þ

    For equation (19), we define its residual equation in theform given below

    R1 η, Cið Þ = f ′′′ + f f ′′ − f ′� �2

    + Rc 2f ′ f ′′′ − f ′′� �2

    − f f iv� �

    − M +1Kp

    !f ′ +ME1:

    ð20Þ

    The unknown convergence parameters C1 andC2 will beoptimally well-known using the conditions given below

    ∂J1 Cið Þ∂C1

    =∂J1 Cið Þ∂C2

    = 0, where J1 Cið Þ =ð0:10R21 η, Cið Þdη:

    ð21Þ

    Taking particular cases when Kp = 100, Rc = 0:5,M = 2,E1 = 0:1, and f w = 1, the convergence parameters are asfollows

    C1 = 0:14227123495837554, C2 = −0:0985828777094099:ð22Þ

    Hence, the approximate analytical solution is given as

    f ηð Þ = e−η −1 + 2eηð Þ − 0:28454246991511e−2η� −0:25 − 2:6eη + 2:85e2η − 3:eηη + 0:1e2ηη

    + 0:666666666666e−3η 0:0012650690185363315ð− 0:2435248057116105eη − 0:6482617721497719e2η

    + 0:8905215088428458e3η − 0:09108496933461585eηη− 1:0292483892015603e2ηη − 0:01118281798120787e3ηη− 0:3597856288717327e2ηη2

    :

    ð23Þ

    The shear stress at the wall is defined as

    τw = μ∂u∂y

    � �y=0

    = μaxffiffiffiffiffiffiffiffiffiffiffiffiffiffi

    a

    υf ′′ 0ð Þ

    s: ð24Þ

    The nondimensional form of skin friction coefficient atthe well is

    f ′′ 0ð Þ = −Cf Re1/2x : ð25Þ

    4. Heat Transfer Analysis

    4.1. Case I: Prescribed Surface Temperature (PST). In theprescribed surface temperature case, introducing nondimen-sional quantities as given below

    g ηð Þ = T − T∞Tw − T∞

    , Pr =υ

    α, Ec =

    a2L2

    ACp, Rc =

    ak0μ

    ,Q

    =q

    aρCp, Rd =

    16σ∗T3∞3kk1

    ,ð26Þ

    and using equation (7) equation (6) become

    Rd + 1ð Þg′′ + Pr f g′ + Q − 2f ′� �

    g + Ec f ′′� �2��

    + Rcf ′′ f ′ f ′′ − f f ′′′� �

    + M +1Kp

    !f ′� �2��

    = 0,

    ð27Þ

    with the BCs given below

    g 0ð Þ = 1, g ∞ð Þ = 0: ð28Þ

    Now let us apply the OHAM to the nonlinear ODE (27)using the following assumption

    4 Advances in Mathematical Physics

  • L = g′ + g, N = Rd + 1ð Þg′′ + Pr� f g′ + Q − 2f ′

    � �g + Ec f ′′

    � �2+ Rcf ′′ f ′ f ′′ − f f ′′′

    � ���

    + M +1Kp

    !f ′� �2��

    − g′ + g� �

    ,

    ð29Þ

    whereN and L are the nonlinear and linear operators, respec-tively. Hence, the OHAM family of equations is given by

    g′ + g� �

    1 − pð Þ =H2 pð Þ Rd + 1ð Þg′′ + Pr f g′ + Q − 2f ′� �

    g��

    + Ec f ′′� �2

    + Rcf ′′ f ′ f ′′ − f f ′′′� ��

    + M +1Kp

    !f ′� �2���

    :

    ð30Þ

    Using the BCs (7) and comparing the coefficients of thesame powers of p-terms in the above equation, one can havethe following:

    Equating the coefficients of the zero-order equation p0,we obtain

    g0 ′ + g0 = 0, g0 0ð Þ = 1, g0 ∞ð Þ = 0: ð31Þ

    Equating the coefficients of the first-order equation p1,we get

    g1 ′ + g1 = g0 ′ + g0 + C3 Rd + 1ð Þg0 ′′ + Pr f0g0 ′ + Q − 2f0 ′� �

    g0��

    + Ec Rcf0 ′′ f0 ′ f0 ′′ − f0 f0 ′′′� �

    + M +1Kp

    !f0′� �2

    + f0′′

    � �2!��, g1 0ð Þ = 0, g1 ∞ð Þ = 0:

    ð32Þ

    Equating the coefficients of the second-order equation p2,we get

    g2 ′ + g2 = g1 ′ + g1 + C3� Rd + 1ð Þg1 ′′ + Pr f1g0 ′ + f0g1 ′ + Q − 2f1 ′

    � �g1

    ��

    + Ec

    Rcf0 ′′ f1 ′ f0 ′′ + f0 ′ f1 ′′ − f1 f0 ′′′ − f0 f1 ′′′� �

    + 2f1 ′′f0 ′′

    2 M +1Kp

    !f1 ′ f0 ′ + Rcf1 ′′ f0 ′ f0 ′′ − f0 f0 ′′′

    � �0BBBB@

    1CCCCA��

    + C4 Rd + 1ð Þg0 ′′ + Pr f0g0 ′ + Q − 2f0 ′� �

    g0��

    + Ec Rcf0 ′′ f0 ′ f0 ′′ − f0 f0 ′′′� �

    + M +1Kp

    !f0′� �2

    + f0′′

    � �2!��,

    ð33Þ

    g2ð0Þ = 0.and g2ð∞Þ = 0.

    After solving the ODEs (31), (34), and (36) with the cor-responding boundary conditions, we obtain

    g0 = e−η, ð34Þ

    g1 =1

    2KpC3e

    −3η −2eηEcPr + 2e2ηEcPr + 2eηKp Pr − 2e2ηKp Pr

    − 2eηEcKp Pr + 2e2ηEcKp Pr − 2eηEcKpM Pr+ 2e2ηEcKpM Pr + EcKpPrRc − 2eηEcf wKpPrRc+ 2e2ηEcf wKpPrRc + 2e

    2ηKpη − 2e2ηKp Pr η− 2e2η f wKp Pr η + 2e

    2ηKp Pr Qη + 2e2ηKpRdη− e2ηEcKpPrRc

    :

    ð35Þ

    We cannot write the third-term g2 here because of itbeing large. Hence, the solution gðη, CiÞ in terms of theparameters can be written as:

    g η, Cið Þ = g0 ηð Þ + g1 η, Cið Þ + g2 η, Cið Þ, i = 1, 2, 3, 4: ð36Þ

    For equation (36), we define its residual equation in theform

    R2 η, Cið Þ = Rd + 1ð Þg′′ + Pr f g′ + Q − 2f ′� �

    g�

    + Ec Rcf ′′ f ′ f ′′ − f f ′′′� �

    + M +1Kp

    !

    � f ′� �2

    + f ′′� �2!�

    :

    ð37Þ

    The unknown convergence parameters C3 andC4 can beoptimally obtained from the following expressed conditionsgiven below

    ∂J2 Cið Þ∂C1

    =∂J2 Cið Þ∂C2

    =∂J2 Cið Þ∂C3

    =∂J2 Cið Þ∂C4

    = 0, where J2 Cið Þ

    =ð0:10R22 η, Cið Þdη:

    ð38Þ

    In the particular case when Rc = Kp = 0:5, E1 = Ec = 0:1,f w = 1,M = Pr = 2,Q = Rd = 0:2, one can obtain the resultsof the convergence parameters. Hence, the values are calcu-lated and obtained below

    C1 = 0:14227123495837554, C2 = −0:0985828777094099,

    C3 = 0:33085325050763764, C4 = −0:17615393227116716:ð39Þ

    5Advances in Mathematical Physics

  • After substituting all the parameters, we get

    g ηð Þ = e−η + e−3η 0:016542662525381883 + 0:2977679254568738eηð− 0:31431058798225564e2η − 0:7940478012183303e2ηη

    + 0:3333333333333333e−4η

    � −0:018007022418104122 + 0:09855963046417679eηð− 1:262581048766744e2η + 1:1820284407206736e3η

    − 1:2401935466956018e2ηη − 0:08408331700268e3ηη+ 0:9175253256056694e3ηη2

    :

    ð40Þ

    The local Nusselt number for PST case is given by

    Nux Re−1/2x = −g′ 0ð Þ: ð41Þ

    4.2. Case II: Prescribed Heat Flux (PHF). In the prescribedheat flux case, introducing the similarity variable T = T∞ +GðηÞðBx2/kL2Þ ffiffiffiffiffiffiffiυ/ap and using equation (7), equation (6)becomes

    Rd + 1ð ÞG′′ + Pr f G′ + Q − 2f ′� �

    G + Ec f ′′� �2

    + Rcf ′′��

    � f ′ f ′′ − f f ′′′� �

    + M +1Kp

    !f ′� �2��

    = 0,

    ð42Þ

    with the boundary conditions

    G′ 0ð Þ = −1, G ∞ð Þ = 0: ð43Þ

    Now, let us apply the OHAM to the nonlinear ODE (42)using the following assumption

    L = G + G′, N = Rd + 1ð ÞG′′ + Pr f G′ + Q − 2f ′� �

    G + Ec�

    � f ′′� �2

    + Rcf ′′ f ′ f ′′ − f f ′′′� ��

    + M +1Kp

    !f ′� �2��

    − G′ +G� �

    ,

    ð44Þ

    whereN and L are the nonlinear and linear operators, respec-tively. Hence, the OHAM family of equations is given by

    G′ + G� �

    1 − pð Þ =H3 pð Þ Rd + 1ð ÞG′′ + Pr f G′ + Q − 2f ′� �

    G��

    + Ec f ′′� �2

    + Rcf ′′ f ′ f ′′ − f f ′′′� ��

    + M +1Kp

    !f ′� �2���

    :

    ð45Þ

    Using the BCs (7) and comparing the coefficients of thesame powers of p-terms in the above equation, one can havethe following:

    Equating the coefficients of the zero-order equation p0,we obtain

    G0 ′ + G0 = 0, G0 ′ 0ð Þ = −1, G0 ∞ð Þ = 0: ð46Þ

    Equating the coefficients of the first-order equation p1,we get

    G1 ′ +G1 =G0 ′ +G0 + C5 Rd + 1ð ÞG0 ′′ + Pr f0G0 ′ + Q − 2f0 ′� �

    G0��

    + Ec Rcf0 ′′ f0 ′ f0 ′′ − f0 f0 ′′′� �

    + M +1Kp

    !f0′� �2

    + f0′′

    � �2!��, G1 ′ 0ð Þ = 0,G1 ∞ð Þ = 0:

    ð47Þ

    Equating the coefficients of the second-order equation p2,we get

    G2 ′ +G2 =G1 ′ +G1 + C5� Rd + 1ð ÞG1 ′′ + Pr f1G0 ′ + f0G1 ′ + Q − 2f1 ′

    � �G1

    ��

    + Ec

    Rcf0 ′′ f1 ′ f0 ′′ + f0 ′ f1 ′′ − f1 f0 ′′′ − f0 f1 ′′′� �

    + 2f1 ′′f0 ′′

    2 M +1Kp

    !f1 ′ f0 ′ + Rcf1 ′′ f0 ′ f0 ′′ − f0 f0 ′′′

    � �0BBBB@

    1CCCCA��

    + C6 Rd + 1ð ÞG0 ′′ + Pr f0G0 ′ + Q − 2f0 ′� �

    G0��

    + Ec Rcf0 ′′ f0 ′ f0 ′′ − f0 f0 ′′′� �

    + M +1Kp

    !f0′� �2

    + f0′′

    � �2 !��,

    ð48Þ

    G2′ð0Þ = 0 and G2ð∞Þ = 0.After solving the ODEs (46), (47), and (48) with the

    corresponding boundary conditions, we obtain

    G0 = e−η,

    G1 =1

    2KpC5e

    −3η 2e2ηKp − 2eηEcPr + 4e2ηEcPr + 2eηKp Pr

    − 6e2ηKp Pr − 2eηEcKp Pr + 4e2ηEcKp Pr− 2e2η f wKp Pr − 2e

    ηEcKpM Pr + 4e2ηEcKpM Pr+ EcKpPrRc − 3e2ηEcKpPrRc − 2eηEcf wKpPrRc+ 4e2ηEcf wKpPrRc + 2e

    2ηKpRd + 2e2ηKpη− 2e2ηKp Pr η − 2e2η f wKp Pr η + 2e

    2ηKp Pr Qη+ 2e2ηKpRdη

    + 2e2ηKp Pr Q:

    ð49Þ

    We cannot write the third term G2 here because of itbeing large. Hence, the solution Gðη, CiÞ in terms of theparameters can be written as:

    G η, Cið Þ =G0 ηð Þ + G1 η, Cið Þ +G2 η, Cið Þ, i = 1, 2, 5, 6: ð50Þ

    For equation (50), we define its residual equation in theform

    6 Advances in Mathematical Physics

  • R3 η, Cið Þ = Rd + 1ð ÞG′′ + Pr f G′ + Q − 2f ′� �

    G�

    + Ec Rcf ′′ f ′ f ′′ − f f ′′′� �

    + M +1Kp

    !

    � f ′� �2

    + f ′′� �2!�

    :

    ð51Þ

    The unknown convergence parameters C3 andC4 can beoptimally obtained from the following expressed conditionsgiven below

    ∂J3 Cið Þ∂C1

    =∂J3 Cið Þ∂C2

    =∂J3 Cið Þ∂C5

    =∂J3 Cið Þ∂C6

    = 0, where J3 Cið Þ =ð0:10R23 η, Cið Þdη:

    ð52Þ

    In a particular case when Rc = Kp = 0:5, E1 = Ec = 0:1,f w = 1,M = Pr = 2,Q = Rd = 0:2, one can obtain the resultsof the convergence parameters. Hence, the values are calcu-lated and obtained below

    C1 = 0:14227123495837554, C2 = −0:0985828777094099,

    C5 = 0:10515520472075117, C6 = 0:006461970319935396:ð53Þ

    After substituting all the parameters, we get

    G ηð Þ = e−η + e−3η 0:005257760236037559ð+ 0:09463968424867605eη − 0:45742514053526756e2η

    − 0:2523724913298028e2ηη

    + 0:3333333333333333e−4η

    � −0:0033498458336746195 + 0:029901242487034338eηð+ 0:16239147539668197e2η − 0:5480934455483598e3η

    − 0:05241128156726507e2ηη − 0:09459486906132786e3ηη+ 0:08656147506726386e3ηη2

    :

    ð54Þ

    The local Nusselt number for the PHF case is given by

    Nux Re−1/2x =1

    G 0ð Þ : ð55Þ

    5. Mass Transfer Analysis

    Introducing the similarity variables C − C∞ = hðηÞða1x2/DÞffiffiffiffiffiffiffiυ/a

    pand using equation (7) in equation (4), we obtain the

    following

    h′′ + Sc f h′ − f ′h − Kch� �

    = 0, ð56Þ

    with boundary condition

    h′ 0ð Þ = −1, h ∞ð Þ = 0: ð57Þ

    Now, let us apply the OHAM to the nonlinear ODE (56)using the following assumption

    L = h′ + h,N = h′′ + Sc f h′ − f ′h −Kch� �

    − h + h′� �

    ,

    ð58Þ

    where L and N stands for the linear and nonlinear oper-ators. Consequently, the OHAM family of equations is writ-ten as

    h′ + h� �

    1 − pð Þ =H4 pð Þ h′′ + Sc f h′ − f ′h −Kch� �� �

    :

    ð59Þ

    Using the BCs (7) and comparing the coefficients of thesame powers of p-terms, one can have the following:

    Equating the coefficients of the zero-order equation p0,one can obtain

    h0 ′ + h0 = 0, h0 ′ 0ð Þ = −1, h0 ∞ð Þ = 0: ð60Þ

    Equating the coefficients of the first-order equation p1,we get

    h1 ′ + h1 = h0 ′ + h0 + C7 h0 ′′ + Sc f0h0 ′ − f0 ′h0 −Kch0� �� �

    ,

    ð61Þ

    h1 ′ 0ð Þ = 0, h1 ∞ð Þ = 0: ð62Þ

    Equating the coefficients of the second-order equation p2,we get

    1.0

    0.8

    0.6

    0.4

    0.2

    0.0

    f′ (𝜂

    )

    𝜂

    fw = –1, 0, 1

    Kp = 100

    Kp = 0.5

    0 1 2 3 4 75 6

    Figure 1: Velocity profiles (second-grade fluid) for different valuesof f w when M = 0:5 andRc = 1.

    7Advances in Mathematical Physics

  • h2 ′ + h2 = h1 ′ + h1 + C7 h1 ′′ + Sc f0h1 ′ + f1h0 ′ − f1 ′h0��

    − f0 ′h1 −Kch1��

    + C8 h0 ′′ + Sc f0h0 ′ − f0 ′h0��

    −Kch0��

    , h2 ′ 0ð Þ = 0, h2 ∞ð Þ = 0::ð63Þ

    After solving the ODEs (60), (61), and (63) with thecorresponding boundary conditions, we obtain

    h0 = e−η:

    h1 = −C7e−η −1 + Sc + f wSc + KcScð Þ 1 + ηð Þ:ð64Þ

    We cannot write the third term h2 here because of itbeing large. Hence, the solution hðη, CiÞ in terms of theparameters can be written as:

    h η, Cið Þ = h0 ηð Þ + h1 η, Cið Þ + h2 η, Cið Þ, i = 1, 2, 7, 8: ð65Þ

    For equation (65), we define its residual equation in theform

    R4 η, Cið Þ = h′′ + Sc f h′ − f ′h −Kch� �

    : ð66Þ

    The unknown convergence parameters C3 andC4 can beoptimally obtained from the following expressed conditionsgiven below

    ∂J4 Cið Þ∂C1

    =∂J4 Cið Þ∂C2

    =∂J4 Cið Þ∂C7

    =∂J4 Cið Þ∂C8

    = 0, where J4 Cið Þ =ð0:10R24 η, Cið Þdη:

    ð67Þ

    In the particular case when Rc = Kp = 0:5, E1 = Sc = 0:1,f w = Kc = 1,M = 2, one can obtain the results of the conver-gence parameters. Hence, the values are calculated as

    C1 = 0:14227123495837554, C2 = −0:0985828777094099,

    C7 = 1:0547354705428924, C8 = 0:7632828804603283:ð68Þ

    After substituting all the parameters, we get the approxi-mate analytic solution as given below

    h ηð Þ = e−η + 0:7383148293800247e−η 1 + ηð Þ + e−3η� −0:0037514629487135163 + 0:16790779466661795eηð+ 0:17398430721442748e2η + 0:4985455077015227e2ηη+ 0:2710538084617421e2ηη2

    :

    ð69Þ

    1.0

    0.8

    0.6

    0.4

    0.2

    0.00 1 2 3 4 5

    Kp = 100

    Kp = 0.5

    Rc = –0.2, 0. 0.2f′ (𝜂

    )

    𝜂

    Figure 2: Velocity profiles for dissimilar values of Rc when M = 1and f w = 0.

    0.8

    0.6

    0.4

    0.2

    1.0

    0.20 1 2 3 4 5 6

    M = 0, 0.4, 0.8

    Kp = 0.5

    Kp = 100

    𝜂

    f′ (𝜂

    )

    Figure 3: Velocity profile for dissimilar values of M whenRc = 0:2, f w = E1 = 0.

    0.8

    0.6

    0.4

    0.2

    1.0

    0.02 4 60 8

    E1 = 0, 0.1, 0.2

    fw = 1

    fw = –1

    f′ (𝜂

    )

    𝜂

    Figure 4: Velocity profile for different values of E1 when Rc = 0:5,M = 1, andKp = 100.

    8 Advances in Mathematical Physics

  • 1.0

    0.8

    0.6

    0.4

    0.2

    0.0

    g (𝜂

    )

    Rc = –0.4, –0.2, 0, 0.3, 0.5

    0 1 2 3 4 5 6𝜂

    (a)

    0.8

    0.6

    0.4

    0.2

    0.0

    G (𝜂

    )

    Rc = –0.4, –0.2, 0, 0.3, 0.5

    𝜂

    0 1 2 3 4 5 6

    (b)

    Figure 5: Temperature profiles for various values of Rcwhen Pr = 3,M = Rd = 1, Ec = E1 = 0:1,Q = 0 and f w = 0: (a) g in the PST case and (b)G in the PHF case.

    0 2 4 6 8

    1.0

    0.8

    0.6

    0.4

    0.2

    0.0

    𝜂

    g (𝜂

    )

    fw = –1fw = 1

    Ec = 0.1, 0.4, 0.6

    (a)

    1.5

    1.0

    0.5

    0.00 2 4 6 8

    𝜂

    G (𝜂

    )

    fw = –1fw = 1

    Ec = 0.1, 0.4, 0.6

    (b)

    Figure 6: Temperature profiles for various values of Ecwith Pr = 2,M = 1, Rc = 0:5, E1 = 0:1,Q = 0:2 and Rd = 1: (a) g in the PST case and (b)G in the PHF case.

    Rd = 0.1, 0.8, 1.5

    0.0

    0.2

    0.4

    0.6

    0.8

    1.0

    0 2 4 6 8

    g (𝜂

    )

    𝜂

    fw = –1fw = 1

    (a)

    Rd = 0.1, 0.8, 1.5

    1.5

    1.0

    0.5

    0.0

    G (𝜂

    )

    𝜂

    0 2 4 6 8

    fw = –1

    fw = 1

    (b)

    Figure 7: Temperature profiles for Rc = 0:5, E1 = 0:1,M = 1, Kp = 100,Q = 0:2, Ec = 0:6, and Pr = 2: (a) PST case and (b) PHF case.

    9Advances in Mathematical Physics

  • The local Sherwood number can be expressed as

    Shx Re−1/2x = −h′ 0ð Þ: ð70Þ

    6. Result and Discussion

    In the course of the discussion, the following aspects arehighlighted:

    (i) Effect of electric field and permeability of themedium on flow characteristics

    (ii) Effect of diffusion species as well as the first-orderchemical reaction

    (iii) Relative response of two viscoelastic models to tem-perature and velocity distribution in the existence ofuniform porous matrix

    (iv) The dimensionless ODEs (9), (27), (36), and (56)with the corresponding boundary conditions aresolved by using the approximate analytic techniqueOHAM

    It is important to note that Rc > 0, Rc < 0, Rc = 0represent second grade, Walters B′, and viscous fluids,respectively.

    Figure 1 displays the velocity distribution of second-grade fluid for suction (f w > 0), injection (f w < 0), andimpermeable plate (f w = 0) in the presence (Kp = 0:5) andabsence (Kp = 100) of the porous matrix. The porousmedium (Kp = 0:5) lessens the primary velocity at all pointsas a result of resistive force accessible by the porous mediumwhich results in thinning of BL. Further, it is motivating tonote that the suction at the plate decreases the velocity. Con-sequently, it is decided that the combined effect of porous

    Q = –2, –1, 0, 0.5, 1

    0 1 2 3 654𝜂

    0.0

    0.2

    0.4

    0.6

    0.8

    1.0

    g (𝜂

    )

    Kp = 0.5Kp = 100

    (a)

    Q = –2, –1, 0, 0.5, 1

    0 1 2 3 654𝜂

    0.0

    0.2

    0.4

    0.6

    0.8

    1.0

    1.2

    G (𝜂

    )

    Kp = 0.5Kp = 100

    (b)

    Figure 8: Temperature profiles for various values of Q with Pr = 2,M = Rd = 1, Ec = E1 = 0:1 and Rc = 0:5, and f w = 0: (a) g in the PST caseand (b) G in the PHF case.

    M = 0, 1, 2

    0.8

    1.0

    0.6

    0.4

    0.2

    0.00 1 2 3 4 5 6

    g (𝜂

    )

    𝜂

    Kp = 0.5Kp = 100

    (a)

    1.0

    0.8

    0.6

    0.4

    0.2

    0.0

    G (𝜂

    )

    0 1 2 3 4 5 6

    Kp = 0.5

    Kp = 100

    𝜂

    M = 0, 1, 2

    (b)

    Figure 9: Temperature profiles for various values of M when Rc = 0:5, E1 = Ec = 0:1, f w = 0, Pr = 2 and Q = Rd = 0:2: (a) g in the PST caseand (b) G in the PHF case.

    10 Advances in Mathematical Physics

  • matrix and suction is encouraging the thinning of BL whichfavors the stability of the flow.

    Figure 2 displays the velocity profiles for Walters B′ðRc= −0:2Þ viscous (Rc = 0) and second-grade flow (Rc = 0:2).It is perceived that velocity achieves low value in the case ofWalters’ B′ model, in the presence of a porous medium. Vis-coelastic flows are disposed to instabilities as a result ofnonlinearity in the constitutive equations. Instabilities aremainly driven by the fluid normal stresses (elasticity) or bythe nature of the boundary conditions. Therefore, the elasticproperty ofWalters’ flowmodel in combination with the per-meability of the porous medium reduces the BL thicknessand hence decreases the instability.

    The variation of the velocity field for various values ofMis illustrated in Figure 3. One can easily understand from thefigure that the velocity significantly declines with a rise in thevalues of M in the absence of an electric field (ðE1 = 0Þ). It isclear that the magnetic field depends on the Lorentz force,which is stronger for a greater magnetic field. Due to the

    nonexistence of an electric field, the Lorentz force raises thefrictional force, which acts as a delaying force that opposesthe viscoelastic fluid flow.

    The effect of E1 on f ′ðηÞ is portrayed in Figure 4. As themagnitudes of E1 boost up, the velocity BL rises nearer to thestretching plate. For remarkable enhancement in the value ofE1, the struggle among the fluid particles rises, and hence, theLorentz force inclines to speed up the body forces, and itleads to escalating in the flow velocity and thicker momen-tum boundary layer. The electric field has the same impactfor the case of injection and suction as demonstrated in thefigure.

    Figures 5(a) and 5(b) display the temperature distribu-tion in cases of PST and PHF cases, respectively, without suc-tion/ injection. The effect of elasticity of the fluid subject tothe present study on temperature distribution is opposite tothat of the viscoelastic parameter that is the temperaturedeclines at all points, and this is further contributed by theWalters B′ model. Both the cases of PHF and PST show asimilar effect.

    Figures 6(a) and 6(b) demonstrate the effects of theEckert number for second-grade fluid in the presence of suc-tion/injection in both PST and PHF cases. The dissipation ofenergy of the flow pattern is measured by the Eckert number.It is seen that an increase in Ec increases the temperature andhence increases the thermal BL thickness. This leads to areduction in the rate of heat transfer from the plate surface.

    0 1 2 3 4 5 6 7𝜂

    h (𝜂) Kc = 0, 0.5, 1

    fw = –1

    fw = 1

    2.0

    1.5

    1.0

    0.5

    0.0

    Figure 11: Concentration profile for various values of Kc when Rc= 0:5, E1 = 0:1,M = 2, Sc = 0:6 and Kp = 100.

    0 1 2 3 4 5

    𝜂

    1.5

    1.0

    0.5

    0.0

    h (𝜂

    )

    E1 = 0.1, 2, 4, 6

    Figure 12: Concentration profile for various values of E1 when Rc= 0:5, Kc = 1, f w = 0,M = 2, Sc = 0:2 and Kp = 100.

    Table 1: Comparison of the values of f ′′ð0Þ when E1 = f w = 0 andKp = 100.

    M Rc Nayak et al. [33] Present result1 -0.5 -2.00499 -2.00328365944

    0.5 -0.5 -1.73781 -1.73779734058

    1 0.5 -1.15758 -1.14375034720

    1 1 -1.00250 -1.00098308049

    0.5 1 -0.86891 -0.86969982367

    0.5 0.5 -1.00333 -1.00284187010

    Sc = 0.1, 0.3, 0.5

    2.0

    1.5

    1.0

    0.5

    0.0

    h (𝜂

    )

    𝜂

    fw = –1

    fw = 1

    0 1 2 3 4 5 6 7

    Figure 10: Concentration profile for various values of Sc when Rc= 0:5, E1 = 0:1,M = 2, Kc = 1 and Kp = 100.

    11Advances in Mathematical Physics

  • The same effect is observed in the case of injection andsuction.

    Figures 7(a) and 7(b) describe the effect of the radiationparameter in the case of second-grade fluid. It is perceivedthat an increase in Rd increases the temperature of the fluidlayer and the processes get accelerated in both cases ofsuction and injection. The rise in temperature with anincrease in radiation parameter causes growth in tempera-ture gradient of the wall in both PST and PHF cases.

    Figures 8(a) and 8(b) display the outcome of the internalheat generation/absorption parameter Q on the temperaturedistribution gðηÞ (PST) and GðηÞ (PHF) in the case ofsecond-grade fluid. This displays that a rise in heat sourcestrength (Q > 0) increases the temperature. This is becauseof the generation of the heat in thermal BL which causesthe temperature to escalate. In the same way, the heat sinkcauses temperature absorption resulting in a decline in tem-perature. The outcome holds good for both PHF and PST.The role of a porous matrix is to accelerate/decelerate theprocess in case of source/sink, respectively.

    From Figures 9(a) and 9(b), it is observed that the impactof the magnetic field parameterM is to raise the temperatureprofile with the increase in the magnetic field in the presenceas well as in the absence of porous matrix. Physically, apply-ing the magnetic field heats up the fluid and thus lessens theheat transfer rates from the wall causing rises in fluid temper-ature distributions.

    Figure 10 exhibits the graph of concentration profiles forvarious values of Schmidt number Sc for the case of suctionand injection. We observed that the concentration declineswith a rise in the Schmidt number Sc for both cases. Thus,for higher values of the Schmidt number, the concentrationof chemically reactive species is larger and lower for smallvalues of Sc. Figure 11 displayed the influence of the chemicalreaction parameter Kc for the case of suction and injection.The concentration profile hðηÞ decreases with an incrementof chemical reaction parameter. From Figure 12, we observedthat the fluid concentration decreases for a large amount ofan electric field parameter E1 . The rate of mass transfer atsheet increases because of an increment in the value of theelectric field.

    We examined the skin friction coefficient f ′′ð0Þ with theaid of a table. Table 1 is computed to validate the present ana-lytic solution in a limiting case. It is observed that the presentlimiting results have a good match with the previouslypublished results.

    7. Conclusions

    In this paper, we investigated the impact of electric field, heatsource/sink, and chemical reaction on the MHD boundarylayer flow of non-Newtonian fluid over a stretching surface.By using similarity transformations, the governing PDEswere converted into the dimensionless ordinary differentialequations. We solved the transformed equations analyticallyusing OHAM. The graphical illustrations of our results fromthe influence of relevant parameters on temperature, concen-tration, and velocity profiles are argued in depth. Some of the

    specific conclusions which have been derived from the studycan be concluded as follows:

    (i) The optimal homotopy asymptotic method is clear,effective, reliable, and efficient

    (ii) Controlling and adjusting the convergence of theseries solution using the convergence parametersare very simple

    (iii) Porous matrix performing as an insulator to thevertical surface averts energy loss because of freeconvection which in turn improves the velocity

    (iv) The existence of porous matrix and elasticity of thefluid overwhelms the resistive force of the magneticfield, and hence, the velocity rises due to the pres-ence of both

    (v) The occurrence of elasticity also leads to rising thetemperature at all points regardless of the presen-ce/absence of porous matrix

    (vi) The slow rate of thermal diffusion in the existenceof the magnetic field and porous matrix causesthinning of the thermal BL thickness

    (vii) The variation in temperature is more sensitive onthe account of heat flux

    (viii) The existence of chemical reaction and porousmatrix with moderate values of the magneticparameter in case of heavier species lessens theconcentration level

    Nomenclature

    Kp: Permeability parameterM: Magnetic parameterB0: Magnetic field strengthQ: Heat source/sink parameterT0: Temperature of the fieldP: Pressure nondimensional timeqr : Radiative heat fluxRd: Radiation parameterEc: Eckert numberCf : Skin friction coefficientk0: Modulus of the viscoelastic fluidmw: Rate of mass fluxK1: Mean absorption coefficientk: Thermal conductivityRc: Viscoelastic parameterPr: Prandtl numberSc: Schmidt numberT : Nondimensional temperatureD: Molecular diffusivityCp: Specific heatqw: Wall heat fluxE1: Electric field parameterT1: Temperature far from sheetTw: Wall temperature

    12 Advances in Mathematical Physics

  • Kc: Chemical reaction parameterA, B, E0, E1: Constants.

    Greek Letters

    α: Thermal diffusivityσ: Electrical conductivityυ: Kinematics viscosityρ: Density of the fluidσ∗: Stefan–Boltzmann constantτw: Wall shear stress.

    Abbreviation

    BLF: Boundary layer flowOHAM: Optimal homotopy asymptotic method2D: Two dimensionalMHD: MagnetohydrodynamicBC: Boundary conditionBL: Boundary layer3D: Three dimensionalODE: Ordinary differential equation.

    Data Availability

    No data support for this particular research.

    Conflicts of Interest

    The author declared no potential conflicts of interest withrespect to the research, authorship, and/or publication of thisarticle.

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    14 Advances in Mathematical Physics

    Analytic Treatment for Electrical MHD Non-Newtonian Fluid Flow over a Stretching Sheet through a Porous Medium1. Introduction2. Formulation of the Problem3. Solution of the Flow Field4. Heat Transfer Analysis4.1. Case I: Prescribed Surface Temperature (PST)4.2. Case II: Prescribed Heat Flux (PHF)

    5. Mass Transfer Analysis6. Result and Discussion7. ConclusionsNomenclatureData AvailabilityConflicts of Interest