Unsteady Magnetohydrodynamics (MHD) Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate

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Unsteady Magnetohydrodynamics (MHD) Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate
Copyright © 2023 by American Scientific Publishers                                             Journal of Nanofluids
                        All rights reserved.                                                                        Vol. 12, pp. 280–287, 2023
                        Printed in the United States of America                                                       (www.aspbs.com/jon)

          Unsteady Magnetohydrodynamics (MHD) Natural
          Convective Flow of Nanofluids Over an Infinite
          Perpendicular Absorbent Plate
          Ch. H. K. Gopal∗ , M. Sudhakar, and S. Masthan Rao
          Department of Mathematics and Humanities, RVR & JC College of Engineering, Chowdavaram, Guntur 522019,
          Andhra Pradesh, India

          The magnetic fields played the significant roles in plentiful field they are, biologically, chemically, mechanically
          as well as medically all investigations. In clinical as well as medical investigation the magnets were extremely
          imperative to create 3-dimensional images of anatomical as well as diagnostics significance from nuclear mag-
          netic resonances signal. In views of those applications, the purpose of present research is to the unsteady
          MHD convective flow past a moving vertical porous plate in nanofluids in the presence of a uniform transverse
          magnetic field has been carried out. The governing equations are solved using Laplace transform technique
          and the solutions are presented in closed form. The numerical computations of velocity and nanofluid temper-
          ature the rate of heat transfer and the shear stress at the plate are presented graphically for several values
ARTICLE

          of the pertinent parameters. An increase in radiation parameter leads to decrease the fluid velocity as well as
          temperature in the boundary layer region. The velocity enhances with increasing permeability parameter. An
          increase in Grashof number and an increase in time lead to increase the fluid temperature. The rate of heat
          transfer at the plate is found to be higher for Cu-water nanofluid. The shear stress at the plate for Cu-water
                                           IP: 5.10.31.151 On: Thu, 11 May 2023 10:35:21
          nanofluid is found to be lower. TheCopyright:
                                                present study   has many
                                                           American       applications
                                                                     Scientific        in engineering devices.
                                                                                Publishers
                                                          Delivered by Ingenta
          KEYWORDS: Natural Convection, MHD Flows, Nanofluid, Thermal Radiation, Vertical Plate.

          1. INTRODUCTION                                                      Emery.1 Rajesh et al.2 researched the consequences of ther-
          Nanoscale particles less than 100 nm have been devel-                mal radiation and chemical reaction in the existence of
          oped through nanotechnology-based procedures. The ther-              Newtonian heating on the transient MHD natural convec-
          mal properties of the base fluid can be enhanced with                tive fluid. Rajesh and Varma3 explored radiation and mass
          nanoparticles to form the stable suspension. The addi-               exchange impacts on MHD natural convective stream past
          tion of small amounts of nanoparticles in metal or metal             an exponentially accelerated vertical plate with mutable
          oxide to fluid has been shown to enhance its thermal                 temperature. Chamkha et al.4 built up a model utilized
          conductivity. Corresponding to existing working fluids,              for the nanofluid consolidates the impacts of Brownian
          nanofluids offer much heat absorbing and heat trans-                 movement and thermophoresis with the Roseland dissem-
          fer properties. Due to its extraordinary applications in             ination estimate. Samad and Rahman5 discussed the inter-
          electronics, communication, and computational systems,               action of thermal radiation with an unsteady MHD flow
          optical devices, etc. research in nanofluids has attracted           through a permeable plate by presenting a time-dependent
          considerable interest in recent years. The wide-ranging              suction. Hamad,6 Krishna et al.,7 Kataria and Mittal,8
          application in physics and engineering especially in the             and Chamkha and Aly9 discussed the unsteady MHD
          design of components and equipment, space technology                 convective flows through porous medium in different phys-
          and gas turbines, etc. thermal radiation on natural con-             ical configurations. Material processing in which mag-
          vection has become extremely relevant. For absorbing                 netic fields are known for their magnificent control of
          and non-absorbing gases, the impact of thermal radiation             electrically-conducting materials is carried discussed the
          on a laminar, Natural convective boundary layer which                role of a magnetic field on the unsteady natural convec-
          flows along a vertical plate was examined by England and             tive nanofluid which stream over a vertical plate. Sheik-
                                                                               holeslami et al.10 examined the heat transfer of Cu–H2 O
           ∗
                                                                               nanofluid in presence of a magnetic field by considering
               Author to whom correspondence should be addressed.
               Email: krishnagopalch@gmail.com                                 the effect of Brownian motion. The motivation behind all
               Received: 5 December 2021                                       the above-presented research considers made on nanoflu-
               Accepted: 10 February 2022                                      ids, was to comprehend and take advantage of nanofluids

          280                             J. Nanofluids 2023, Vol. 12, No. 1   2169-432X/2023/12/280/008         doi:10.1166/jon.2023.1928
Unsteady Magnetohydrodynamics (MHD) Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate
Gopal et al.                           Unsteady MHD Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate

heat transfer mechanism. The viscous dissipation impact         and Chamkha.35 Krishna et al.36 discussed the MHD flow
is also significantly affecting the heat transfer mechanism.    of an electrically conducting second-grade fluid through
The distribution of the temperature in the boundary layer       porous medium over a semi-infinite vertical stretching
is greatly influenced by the viscous dissipation as an inter-   sheet. Krishna et al.37 discussed Hall effects on MHD peri-
nal source of heat-induced by fluid shearing. Khan et al.,11    staltic flow of Jeffrey fluid through porous medium in a
Freidoonimehr et al.,12 and Mustafa et al.13 analysed the       vertical stratum. Krishna et al.38 discussed heat and mass-
influence of unsteady MHD natural convective boundary           transfer effects on an unsteady flow of a chemically react-
layer nanofluid along with a stretching sheet with vis-         ing micropolar fluid over an infinite vertical porous plate
cous dissipation. The influence on MHD nanofluid flow           in the presence of an inclined magnetic field, Hall cur-
of a wedge with permeable slip and the medium was               rent effect, and thermal radiation taken into account. The
investigated by Pandey and Kumar14 and Upreti et al.15          effects of heat and mass transfer on free convective flow of
Rajesh et al.16 established a numerical model for Tran-         micropolar fluid over an infinite vertical porous plate have
sient MHD nanofluid to understand the characteristics of        been discussed by Krishna et al.39 Krishna and Chamkha40
heat transfer in the existence of viscous dissipation. Mishra   have discussed the systematic solution of time-dependent
et al.17 analysed the impact of Ohmic-viscous dissipation       mean velocity on MHD peristaltic rotating flow of an elec-
and slip effects on nanofluid flow over a stretching cylin-     trically conducting couple stress fluid in a uniform elas-
der with suction/injection. Motsumi and Makinde18 stud-         tic porous channel. Krishna and Chamkha41 investigated
ied the impact of thermal radiation and viscous dissipation     the Hall and ion slip effects on the MHD convective flow
on boundary layer flow of nanofluids over a permeable           of elastico-viscous fluid through porous medium between
moving flat plate. Haroun et al.19 examined the unsteady        two rigidly rotating parallel plates with time fluctuating
MHD mixed convection in a nanofluid due to a stretching/        sinusoidal pressure gradient. Krishna et al.42 discussed the
shrinking surface with suction/injection using the spec-        Soret and Joule effects of MHD mixed convective flow of

                                                                                                                                           ARTICLE
tral relaxation method. Farooq et al.20 discussed the influ-    an incompressible and electrically conducting viscous fluid
ence of transpiration and viscous dissipation on entropy        past an infinite vertical porous plate taking Hall effects into
flow over a nonlinear radially stretching disk. Kuznetsov       account. Krishna et al.43 discussed the heat and mass trans-
           21
and Nield have studied the natural convective boundary          fer on unsteady, MHD oscillatory flow of second-grade
                                     IP: 5.10.31.151 On: Thu, 11 May 2023 10:35:21
layer flow of a nanofluid past a vertical   plate. Hamad  and   fluid through
                                         Copyright: American Scientific         a porous medium. Krishna et al.44 investi-
                                                                           Publishers
     22
Pop have investigated the unsteady MHD freeDelivered  convec- bygated  the heat and mass transfer on MHD free convective
                                                                  Ingenta
tion flow of a nanofluid past a vertical permeable flat plate   flow over an infinite non-conducting vertical flat porous
in a rotating frame of reference with constant heat source.     plate.
The effects of magnetic field on free convection flow of a         Chamkha and Khaled45 discussed the problem of cou-
nanofluid past a vertical semi-infinite flat plate were stud-   pled heat and mass transfer by mixed convection in a lin-
ied by Hamad et al.23 Turkyilmazoglu24 has obtained an          early stratified stagnation flow with an externally applied
analytical solution for heat and mass transfer of MHD slip      magnetic field and internal heat generation or absorp-
flow in nanofluids. Nandkeolyar et al.25 have presented the     tion effects. Chamkha et al.46 investigated coupled heat
unsteady hydromagnetic radiative flow of a nanofluid past       and mass transfer by boundary-layer free convection over
a flat plate with ramped temperature.                           a vertical flat plate. The free convection boundary-layer
   Krishna and Chamkha31 investigated the diffusion-            flow over an isothermal inclined plate embedded in a
thermo, radiation-absorption and Hall and ion slip effects      thermally stratified porous medium has been developed
on MHD free convective rotating flow of nano-fluids             by Chamkha.47 Reddy and Chamkha48 discussed Soret
past a semi-infinite permeable moving plate with constant       and Dufour effects on MHD convective flow of Al2 O3 -
heat source. Krishna and Chamkha32 discussed the MHD            Water and TiO2 -Water nanofluids past a stretching sheet in
squeezing flow of a water-based nanofluid through a sat-        porous media. The steady, laminar, MHD flow of a microp-
urated porous medium between two parallel disks, taking         olar fluid past a stretched semi-infinite, vertical and per-
the Hall current into account. Hall and ion slip effects        meable has been explored by Khedr et al.49 Takhar et al.50
on unsteady MHD convective rotating flow of nanoflu-            investigated the unsteady flow and heat transfer on a semi-
ids have been discussed by Krishna and Chamkha.33 The           infinite flat plate with an aligned magnetic field. A study
effects of radiation and Hall current on an unsteady MHD        of natural convective flow, heat transfer and entropy gener-
free convective flow in a vertical channel filled with a        ation in an odd-shaped geometry has presented by Parvin
porous medium have been studied by Krishna et al.34             and Chamkha.51 The effects of nanoparticles diameter and
The heat generation/absorption and thermo-diffusion on          concentration on natural convection heat transfer of a
an unsteady free convective MHD flow of radiating and           nanofluid around a vertical cone embedded in a Darcy
chemically reactive second grade fluid near an infinite         porous medium utilizing the drift-flux model have been
vertical plate through a porous medium and taking the           theoretically investigated Ghalambaz et al.52 Zaraki et al.53
Hall current into account have been studied by Krishna          theoretically explored the problem of natural convection

J. Nanofluids, 12, 280–287, 2023                                                                                                  281
Unsteady Magnetohydrodynamics (MHD) Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate
Unsteady MHD Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate                                Gopal et al.

          boundary layer heat transfer of nanofluids. The effects of              Table I. Thermophysical properties of H2 O, Cu and Ag.
          Joule-heating, chemical reaction and thermal radiation on
                                                                                                              H2 O             Cu               Ag
          unsteady MHD natural convection from a heated vertical
          porous plate in a micropolar fluid have been analyzed by                cp (J/Kg K)              4179               385              235
          Chamkha et al.54                                                         (Kg/m3 )              997.1              8933             10500
                                                                                  k (W/m K)               0.613               401              429
             The purpose of this analysis is to investigate the impacts            × 10−5 (1/K)            21                1.67             1.89
          of radiation and magnetic field on a transient natural                   (S/m)               5.5 × 10−6         59.6 × 106       62.1 × 106
          free convective nanofluid that stream along with a verti-
          cal plate. In this paper, the MHD convective flow past a
          moving vertical porous plate in nanofluids with the pres-           motion. This approximation is exact enough for both drop-
          ence of a uniform transverse magnetic field has been dis-           ping fluids and gases at small values of the temperature
          cussed. With the aid of non-dimensional flow parameters,            difference. As the plate is infinitely long, the velocity and
          the mathematical results of velocity and temperature dis-           temperature fields are functions of y and t alone. The
          tributions are analysed and shown diagrammatically. This            thermophysical properties of the nanofluids are given in
          analysis also highlights the consistency of the numerical           Table I.
          approach using grid independence that is presented in the              It is assumed that induced magnetic field produced by
          tables.                                                             the fluid motion is negligible in comparison with the
                                                                              applied one so that we consider magnetic field B = (0,
          2. FORMULATION AND SOLUTION OF THE                                  0,  B0 ). This assumption is justified, since the magnetic
               PROBLEM                                                        Reynolds     number is very small for metallic liquids and
                                                                              partially ionized fluids. Also, no external electric field is
          We considered the radiation-absorption on the unsteady
                                                                              applied such that the effect of polarization of fluid is neg-
          MHD free convective flow of a nanofluid past an infinite
                                                                              ligible, so we assume E = (0, 0, 0). Under the above
ARTICLE

          vertical flat plate moving with an impulsive motion. Ini-
                                                                              assumptions, the momentum and energy equations in the
          tially the plate is at rest with the ambient temperature T .
          At time t > 0, the plate starts to move in its own plane with       presence of magnetic field and thermal radiation past a
          the velocity u0 in the vertical direction,   where u0 is  con-     moving vertical plate can be expressed as (Krishna and
                                                IP: 5.10.31.151    On:  Thu, 11  May 2023
                                                                              Chamkha     28   10:35:21
                                                                                             and  Das and Jana27 ),
          stant and the temperature of the plate Copyright:
                                                    is raised or American
                                                                 lowered Scientific      Publishers
          to Tw . We choose the x-axis along the plate in theDelivered
                                                                  vertical by Ingenta
                                                                                    u         2 u              f
          direction and y-axis perpendicular to the plate. A uniform            nf     = nf 2 − nf B02 u − u + g nf T − T (1)
                                                                                    t         y                 k
          transverse magnetic field of strength B0 is applied parallel
          to the y-axis. The plate coincides with the plane y = 0 and                           T          2 T q
          the flow being confined to y > 0. The physical model of                       cp nf     = knf 2 − r + Q1 C − C             (2)
                                                                                                 t        y       y
          the problem is as shown in the Figure 1.
                                                                                                         C       2 C
             The assumptions of the present problem are made as                                               =D 2                       (3)
          the following. The pressure gradient is neglected in this                                      t       y
          problem. A radiative heat flux qr is applied in the normal          The important attributes of nanofluid are,
          direction to the plate. The fluid is a water based nanofluid                                f
          containing two types of nanoparticles Cu and Ag. The                             nf =                 = 1 − f + s
          base fluid and the suspended nanoparticles are in thermal                               1 − 2 5 nf
                                                                                                                           
          equilibrium. The density is assumed to be linearly depen-                               cp nf = 1 −       cp f + cp s
          dent on temperature buoyancy forces in the equations of
                                                                                                   nf = 1 −  f +  s
                                                                                                                           
                                                                                                           3  − 1               
                                                                                      nf = f 1 +                            = s
                                                                                                       + 2 −  − 1             f
                                                                                                                                                     (4)

                                                                                  the effective thermal conductivity of the nanofluid29 30
                                                                                  given by
                                                                                                                           
                                                                                                        ks + 2kf − 2 kf − ks
                                                                                             knf = kf                               (5)
                                                                                                        ks + 2kf + kf − ks

                                                                                     The initial and boundary conditions be

          Fig. 1. Physical model.                                                 u=0       T =T       C = C         at t =0 for all y ≥ 0

          282                                                                                                        J. Nanofluids, 12, 280–287, 2023
Unsteady Magnetohydrodynamics (MHD) Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate
Gopal et al.                                Unsteady MHD Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate

           u = u0     T =Tw C =Cw             at t > 0     y=0             To solve the Eqs. (11)–(13) with initial and bound-
                                                                         ary conditions (14) by making use of Laplace transform
           u→0       T → T C → C t > 0 as y → 
                                                                         technique.
                                               (6)
                                                                            Taking Laplace transforms on Eqs. (11)–(13), then the
   The Rosseland approximation26 applies to optically                    transformed equations are,
thick media and gives the net radiation heat flux qr through                                       
                                                                                 2 u             1
the expression as,                                                             a1 2 − s M +   2
                                                                                                     a3 u + Gr a2  = 0      (15)
                                                                                                 K
                                4 ∗ T 4
                       qr = −                                    (7)                                  2 
                                3K ∗ y                                                          a4        − s + Q = 0                  (16)
                                                                                                       2
   It is supposed that, the temperature difference T − T
                                                                                                      d2
within the boundary layer flow is sufficiently small such                                                 − sSc = 0                      (17)
that the term T 4 may be expressed as a linear function                                               d 2
of temperature. This is done by expanding T 4 in a Taylor                   The relevant boundary conditions for ū, ¯ and ¯ are
series about a free stream temperature T , as pursues,
                                                                                                           1            1
                                                                                       u=             =            =        at     =0
     T 4 = T4 + 3T3 T − T + 6T2 T − T 2 + · · ·           (8)                         s              s            s
   Neglecting higher order terms in Eq. (8) ahead of the                           u→0           →0            →0          as      →   (18)
first order in (T − T ), we acquired,                                   Where,
                      T ≈
                        4
                             4T3 T   − 3T4                     (9)                                           
                                                                                           ū        s =           u   t e−st dt

                                                                                                                                                 ARTICLE
                                                                                                            0
  On the utilize of Eqs. (7) and (9), Eq. (2) turns into,                                            
                                      2                                               ¯
                                                                                             s =         t e−st dt
                                ∗ 3
 T         1              16 T  T                                                                 0
     =           knf +                         + Q1 C − C (10)                                    
 t      cp nf               3k∗          y 2                                          ¯
                                                                                        
                                            IP: 5.10.31.151 On: Thu, 11 May 2023 10:35:21       s =         t e−st dt
                                                                                                       0
  Implementing non-dimensional quantities,      Copyright: American Scientific Publishers
                                                            Delivered by Ingenta
                                                                           Transformed solutions of Eqs. (15)–(17) put through the
          u0 y     ∗
                          2
                        u0 t        ∗        u          T − T          boundary requirements (18) are obtained and are provided
       =          t =             u =              =
           vf            vf                 u0          Tw − T         as,
                                                                                                           1 − √sSc
           C − C                       2
                                 f B0 vf                    ∗
                                                        16 T  3                                 s   =    e                       (19)
    =                  M2 =                      Nr =                                                     s
                                                                                                   
          Cw − C                  f u0  2
                                                         3kf k∗                      1        Q           √         Q 1 − √sSc
                                                                          s =         +              e− s +                e      (20)
          f cp             gf vf Tw − T                 ku20                     s Sc −                       Sc −  s 2
   Pr =             Gr =                               K= 2
            kf                       u30                     vf                     
                                                                                                b1              b
          v           vf Q1 Cw − C                                      u   s  =       +              + 2 2
   Sc =          Q=                                                                    s ss − 1            s s − 1
          D              u20 Tw − T                                                               √
                                                                                            b                                 b1     √
                                                                                    + 2 3             e− s+ /a1 −               e− s
  Making use of non-dimensional variables, the governing                              s s −2                           ss −1
Eqs. (2), (3) and (10) reduced to (dropping asterisks),                                      b2          √            b3         √
                                                                                                      − s                     − sSc
                                                                                  −               e         −              e       (21)
         u       2 u                1                                                s 2 s − 1              s 2 s − 2
              = a1 2 − M 2 +                 a3 u + Gr a2        (11)
         t                          K                                    Taking inverse Laplace transforms of Eqs. (19)–(21),
                                 2
                                                                      then, we acquired the solutions for the concentration, tem-
                          = a4 2 + Q                             (12)  perature and velocity fields.
                      t         
                                                                           The shear stress at the surface = 0 measured as,
                                 1 2                                                               
                               =                                  (13)                                   u
                         t      Sc  2                                                          =                                  (22)
  The initial and boundary conditions are,                                                                     =0

                                                                           The Nusselt number in terms of rate of heat transfer at
               u = 0  = 0 t = 0 for all            ≥0
                                                                         the plate = 0 is given by
          u =   = 1  = 1 t > 0 at                =0                                              
                                                                                                    
      u → 0  → 0  → 0 t > 0 as                   →          (14)                          Nu =                            (23)
                                                                                                        =0

J. Nanofluids, 12, 280–287, 2023                                                                                                          283
Unsteady Magnetohydrodynamics (MHD) Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate
Unsteady MHD Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate                                  Gopal et al.

             The Sherwood number in terms of rate of mass transfer
          at the plate = 0 is given by
                                     
                                     
                              Sh =                            (24)
                                         =0

          3. RESULTS AND DISCUSSION
          In order to get a clear insight on the physics of the prob-
          lem, a parametric study is performed and the obtained
          numerical results are elucidated with the help of graphical
          illustrations. We have presented the non-dimensional fluid
          velocity u and the fluid temperature  for several values
          of magnetic parameter M 2 , Grashof number Gr, radiation
          parameter Nr, volume fraction parameter  and time s in           Fig. 3. The velocity profile with K. M = 2, Nr = 0.5,  = 0.05, Gr = 3,
          Figures 2–11. The values of volume fraction of nanoparti-         t = 0.1.
          cles are taken in the range of 0 ≤  ≤ 0 2. The case M = 0
          corresponds to the absence of magnetic field and  = 0 for
          regular fluid. The default values of the other parameters
          are mentioned in the description of the respected figures.
          We consider the non-dimensional velocity distribution for
          nanoparticle (Cu). Due to high density of Cu, for Cu-water
          the dynamic viscosity increases more and leads to a thin-
ARTICLE

          ner boundary layer than other particles. For the cases of
          stationary plate ( = 0) as well as moving plate ( = 1).
             Figure 2 reveals that the fluid velocity u deccelerates for
          increasing values of magnetic parameter      M. The momen-
                                               IP: 5.10.31.151    On: Thu, 11 May 2023 10:35:21
          tum boundary layer thickness decreases   Copyright:  American
                                                     for increasing val- Scientific Publishers
          ues of M for the cases of stationary plate ( = 0)Delivered
                                                                 as well by Ingenta
          as moving plate ( = 1). The velocity profiles are char-
          acterized by distinctive peaks in the immediate vicinity
          of the plate and as M increases these peaks decrease and          Fig. 4. The velocity profile with Nr. M = 2, K = 0.5,  = 0.05, Gr = 3,
                                                                            t = 0.1.
          move gradually downstream. This is due to the fact that
          the magnetic lines of forces move past the plate and the
          fluid which is decelerated by the viscous force, receives         lesser the fluid speed is observed in the entire fluid region.
          a push from the magnetic field which counteracts the vis-         The effect of radiation parameter Nr on the velocity pro-
          cous effects.                                                     files is presented in Figure 4. The fluid velocity u enhances
             Figure 3 depicts that the velocity increases with increas-     as the value of Nr increases for both cases of stationary
          ing permeability parameter K. Lower the permeability              plate ( = 0) as well as moving plate ( = 1). The velocity

          Fig. 2. The velocity profile with M. K = 0.5, Nr = 0.5,  = 0.05, Gr =   Fig. 5. The velocity profile with . M = 2, K = 0.5, Nr = 0.5, Gr = 3,
          3, t = 0.1.                                                              t = 0.1.

          284                                                                                                       J. Nanofluids, 12, 280–287, 2023
Unsteady Magnetohydrodynamics (MHD) Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate
Gopal et al.                                   Unsteady MHD Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate

Fig. 6. The velocity profile with Gr. M = 2, K = 0.5, Nr = 0.5,  =         Fig. 9.    The temperature profile with Nr. Pr = 0.71,  = 0.05, t = 0.1.
0.05, t = 0.1.

                                                                                                                                                          ARTICLE
                                            IP: 5.10.31.151 On: Thu, 11 May 2023 10:35:21
                                                Copyright: American Scientific Publishers
                                                          Delivered by Ingenta

                                                                            Fig. 10.    The temperature profile with . Pr = 0.71, Nr = 0.5, t = 0.1.
Fig. 7. The velocity profile with M. M = 2, K = 0.5, Nr = 0.5,  =
0.05, Gr = 3.                                                               tends to increase inside a boundary layer region. Figure 5
                                                                            depicts the effect of solid volume fraction of nanoparti-
profiles increase sharply near the surface of the plate                     cles on the fluid velocity. The fluid velocity u increases
and after attaining respective maxima’s, the curves settle                  with increasing  for the cases of stationary plate ( = 0)
down to the corresponding asymptotic value. Therefore, Nr                   as well as moving plate ( = 1). It is also revealed that
behaves like a supporting force which accelerates the fluid                 the increase in the values of  results in the increase of
particles near the vicinity of the plate. Also, it is noted that            the momentum boundary layer thickness. Figure 6 shows
momentum boundary layer thickness increases when Nr                         that the velocity u increases with an increase in Grashof

Fig. 8.   The temperature profile with Pr. Nr = 0.5,  = 0.05, t = 0.1.     Fig. 11.    The temperature profile with Pr. Pr = 0.71, Nr = 0.5,  = 0.05.

J. Nanofluids, 12, 280–287, 2023                                                                                                                 285
Unsteady Magnetohydrodynamics (MHD) Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate
Unsteady MHD Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate                           Gopal et al.

          number Gr for the cases of stationary plate ( = 0) as            Table III. Nusselt number.
          well as moving plate ( = 1). This trend is due to the
                                                                            Pr              Nr                            t              Nu
          fact that the positive Grashof number Gr acts like a favor-
          able pressure gradient which accelerates the fluid in the         0.71             1             0.05           0.1         −1.01909
          boundary layer. Consequently, the velocity increases with         3                                                         −2.09480
                                                                            7                                                         −3.19985
          Gr. Grashof number represents the effect of free convec-                          1.5                                       −0.91821
          tion currents. Physically, Gr > 0 means heating of the fluid                       2                                        −0.84237
          of cooling of the boundary surface, Gr < 0 means cool-                                           0.2                        −0.89126
          ing of the fluid of heating of the boundary surface and                                          0.4                        −0.72632
          Gr = 0 corresponds the absence of free convection current.                                                      0.2         −0.72060
                                                                                                                          0.3         −0.58837
          Figure 7 reveals that the fluid velocity u increases as time
          s increases for both cases of stationary plate ( = 0) as
          well as moving plate ( = 1).
                                                                            Table IV. Comparison of the results (y = 0.2,  = 0).
             Figure 8 represents the variation of nanofluid tem-
          perature for Prandtl number Pr. The temperature pro-                                                  Previous work     Present results
          files exhibit that the fluid temperature decreases as Pr          M        K        Nr               Das and Jana27       K→
          increases. This is due to the fact that a higher Prandtl num-     2       0.5        1      0.05        0.522142          0.522145
          ber fluid has relatively low thermal conductivity, which          3                                     0.458448          0.458496
          reduces conduction and there by the thermal boundary              4                                     0.355487          0.355447
          layer thickness; and as a result, temperature decreases.                   1                            0.565894          0.565852
                                                                                    1.5                           0.605221          0.605241
          From Figure 9, an increase in radiation parameter Nr
                                                                                             1.5                  0.587447          0.587463
          means the release of heat energy from the flow region and                            2                  0.622465          0.622447
          so the fluid temperature decreases. This means that, the
ARTICLE

                                                                                                      0.2         0.597995          0.597996
          thermal boundary layer decreases and more uniform tem-                                      0.4         0.650632          0.650621
          perature distribution across the boundary layer. Figure 10
          displays the effect of volume fraction  of nanoparti-
          cles on the temperature distribution.IP:The
                                                   5.10.31.151    On: Thu, 11
                                                       fluid temperature       May 2023 10:35:21
                                                                            asymptotically     to the free stream with zero value far away
                                                   Copyright:   American
          increases as volume fraction parameter  enlarges. Also,        Scientific
                                                                            from the Publishers
                                                                                        plate.
                                                               Delivered by Ingenta
          the thermal boundary layer for Cu-water is greater than              The shear stress at the plate and Nusselt number in
          for pure water ( = 0). This is because copper has high           terms of rate of heat transfer are determined analytically
          thermal conductivity and its addition to the water based          and computationally discussed with reference to governing
          fluid increases the thermal conductivity for the fluid, so the    parameters and are tabulated in Tables II and III. The stress
          thickness of the thermal boundary layer increases. It is also     component reduces with increasing permeability parame-
          observed that with increasing the volume fraction  of the        ter K with increasing radiation parameter Nr, nano particle
          nanoparticles the thermal boundary layer is increased. This       concentration  and enhances with increasing Hartmann
          agrees with the physical behavior of nanoparticles. This          number, thermal Grashof number Gr and time t.
          observation shows that the use of nanofluids will be sig-            Nusselt number reduces with Prandtl number Pr and
          nificance in the cooling and heating processes. Figure 11         accelerates with increasing radiation parameter Nr, nano
          reveals that temperature increases with increasing time s.        particle concentration  and time t. Since the thermal con-
          The fluid temperature is high near the plate and decreases        ductivity of Cu is higher than other nano fluids, the rate of
                                                                            heat transfer is found to be higher for Cu-water nanofluid.
          Table II. Shear stress.                                           Also due to increase in thermal conductivity with the solid
                                                                            volume fraction of nanoparticles. Also, the thermal bound-
          M         K        Nr               Gr         t      x
                                                                            ary layer thickness decreases with increase of nanoparti-
          2        0.5        1      0.05       3        0.2     0.510052   cle volume fraction and in turn the rate of heat transfer
          3                                                      2.983180   increases with increase of volume fraction of nanoparti-
          4                                                      4.218522
                    1                                            0.407968
                                                                            cles. The results are good agreement with results of Das
                   1.5                                           0.333386   and Jana27 (Table IV).
                            1.5                                     0.409731
                             2                                      0.373085
                                       0.2                          0.501324      4. CONCLUSIONS
                                       0.4                          0.483255      To obtain exact solutions for the unsteady natural convec-
                                                  4                 1.655895      tion boundary layer flow of a nanofluid near a moving infi-
                                                  5                 2.114558
                                                                                  nite vertical plate in the presence of a transverse uniform
                                                           0.3      0.652554
                                                           0.4      0.854478      magnetic field. The most important concluding remarks
                                                                                  can be summarized as follows.

          286                                                                                                  J. Nanofluids, 12, 280–287, 2023
Unsteady Magnetohydrodynamics (MHD) Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate
Gopal et al.                                Unsteady MHD Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate

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J. Nanofluids, 12, 280–287, 2023                                                                                                            287
Unsteady Magnetohydrodynamics (MHD) Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate Unsteady Magnetohydrodynamics (MHD) Natural Convective Flow of Nanofluids Over an Infinite Perpendicular Absorbent Plate
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