Sheik-holeslami and Vajravelu [15] investigated the nanofluid flow and heat transfer in a cavity with variable Lorentz forces.. [5]Mohsen Sheikholeslami Kandelousi, Effect of spatially var
Trang 1ORIGINAL ARTICLE
Nanofluid heat transfer between two pipes
considering Brownian motion using AGM
M Sheikholeslami a , * , M Nimafar b , D.D Ganji c
a
Department of Mechanical Engineering, Babol University of Technology, Babol, Iran
bDepartment of Mechanical Engineering, Central Tehran Branch, Islamic Azad University, Tehran, Iran
c
Department of Mechanical Engineering, Sari Branch, Islamic Azad University, Sari, Iran
Received 28 October 2016; revised 19 January 2017; accepted 23 January 2017
KEYWORDS
Nanofluid;
Rotating cylinders;
Magnetic field;
KKL model;
Radiation;
AGM
Abstract Nanofluid flow between two circular cylinders is studied in existence of magnetic field KKL model is applied for nanofluid Thermal radiation effect has been considered in energy equa-tion AGM is selected for solving ODEs Semi analytical procedures are examined for various active parameters namely; aspect ratio, Hartmann number, Eckert number and Reynolds number Results indicate that temperature gradient enhances with rise of Ha, Ec andg but it reduces with augment
of Re Velocity reduces with rise of Lorentz forces but it augments with rise of Reynolds number
Ó 2017 Faculty of Engineering, Alexandria University Production and hosting by Elsevier B.V This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/)
1 Introduction
Magnetohydrodynamic free convection has several
applica-tions In recent decade, nanotechnology has been offered as
novel method for heat transfer improvement MHD nanofluid
free convection in a tilted enclosure has been presented by
Sheremet et al [1] They showed that augment of titled angle
causes convective heat transfer to enhance 3D MHD free
con-vective heat transfer was examined by Sheikholeslami and
Ellahi [2] using LBM Their results revealed that Lorentz
forces causes temperature gradient to reduce Ismael et al [3]
investigated Lorentz forces effect on nanofluid flow in an
enclosure with moving walls Their outputs indicated that
the impact of Lorentz forces reduces with change in direction
of magnetic field Sheikholeslami and Ellahi [4] utilized LBM
to study Fe3O4-water flow for aim of drug delivery They con-cluded that the velocity gradient reduces with rise of magnetic number Influence of non-uniform Lorentz forces on nanofluid flow style has been studied by Sheikholeslami Kandelousi [5]
He concluded that improvement in heat transfer reduces with rise of Kelvin forces New model for nanofluid flow was pre-sented by Hayat et al [6] Sheikholeslami [7] studied the ther-mal radiation effect on nanofluid flow in a cavity with tilted elliptic inner cylinder.
Influence of thermal radiation on magnetohydrodynamic nanofluid motion has been reported by Sheikholeslami et al [8] They concluded that nanofluid concentration gradient aug-ments with rise of radiation parameter Noreen et al [9] exam-ined the motion of nanofluid in a bent channel They showed that curvature can enhance the longitudinal velocity MHD
Fe3O4-water flow in a wavy cavity was examined by Sheik-holeslami and Chamkha [10] Influence of magnetic field on force convection was reported by Sheikholeslami et al [11] Their outputs illustrated that higher lid velocity include more
* Corresponding author
(M Sheikholeslami),m.nimafar@gmail.com(M Nimafar)
Peer review under responsibility of Faculty of Engineering, Alexandria
University
H O S T E D BY
Alexandria University Alexandria Engineering Journal
www.elsevier.com/locate/aej www.sciencedirect.com
http://dx.doi.org/10.1016/j.aej.2017.01.032
Trang 2sensible Kelvin forces effect Bondareva et al [12] utilized
Buongiorno’s mathematical model for magnetic field effect
on transient free convection Sheikholeslami and Rokni [13]
studied the effect of Lorentz forces on free convection in a semi
annulus Bondareva et al [14] was utilized Heatline analysis
for simulating MHD free convection in an open cavity
Sheik-holeslami and Vajravelu [15] investigated the nanofluid flow
and heat transfer in a cavity with variable Lorentz forces
Sher-emet et al [16] investigated magnetic field on free convection of
wavy open cavity They presented the effect of corner heater
on nanofluid flow.
Nonlinear equations can be solved via semi analytical
meth-ods There are several semi analytical methods such as DTM
[17–19] , HPM [20,21] , HAM [22] , ADM [23,24] , OHAM
[25,26] and etc One of the new powerful semi analytical
approaches is AGM Mirgolbabaee et al [27] used AGM for
Duffing-type nonlinear oscillator They showed the accuracy
of this paper Nanofluid flow and heat transfer have been
sim-ulated by several authors in recent decade [28–37,17,38–47]
The chief aim of this paper is to illustrate the effect of
mag-netic field on nanofluid hydrothermal treatment between two
pipes AGM is utilized to solve this problem The roles of
the aspect ratio, radiation parameter, Reynolds number,
Eck-ert number, Hartmann number are presented.
2 Governing formulae Laminar 2D flow in cylindrical coordinate is studied ( Fig 1 ) The governing formulae are as follows:
tnf
@2
v
@r2þ 1 r
@v
@r
v
r2
rnfvB2
knf
r
@
@r r
@T
@r
þ lnf
@v
@r
v r
@qr
@r ¼ ðqCpÞnfv @T
@r ;
qr¼ 4re
3bR
@T4
@y ; T
4ffi 4T3
cT 3T4
r ¼ r1: vðrÞ ¼ X1r1; T ¼ T1
r ¼ r2: vðrÞ ¼ 0; T ¼ T2
ð3Þ ðrÞnf, ðqCpÞnf, ðqbÞnf and ðqnfÞ can be introduced as follows:
rnf
rf
¼ 1 þ 3 ðrp=rf 1Þ/
ðrp=rfþ 2Þ ðrp=rf 1Þ/ ; ðqbÞnf¼ 1 /ÞðqbÞfþ ðqbÞp/;
ðqCpÞnf¼ /ðqCpÞpþ ðqCpÞfð1 /Þ; qnf¼ /qpþ qfð1 /Þ
ð4Þ
ðknfÞ and ðlnfÞ are obtained according to Koo–Kleinstreuer–Li (KKL) model [48] :
knf¼ 3 ðkp=kf 1Þ/
ðkp=kf 1Þ/ þ ðkp=kfþ 2Þ þ 1
þ 5/ 104
cp;fg0ðdp; T; /Þqf
ffiffiffiffiffiffiffiffiffi
jbT
qpdp
s
g0ðdp; T; /Þ ¼ ða1þ a2Ln ðdpÞ þ a5Ln ðdpÞ2
þ a3Ln ð/Þ
þ a4ln ðdpÞLnð/ÞÞLnðTÞ þ ða6þ a7Ln ðdpÞ
þ a10Ln ðdpÞ2
þ a8Ln ð/Þ þ a9ln ðdpÞLnð/ÞÞ
Rf¼ dpð1=kp;eff 1=kpÞ; Rf¼ 4 108km2=W
ð5Þ
Fig 1 Geometry of the problem
Table 1 Thermo physical properties of water and nanoparticles[48]
Nomenclature
v dimensionless velocity
Cp specific heat capacity
B constant applied magnetic field
Pr Prandtl number
Nu Nusselt number
Re Reynolds number
r dimensionless radius
Rd radiation parameter
k thermal conductivity Greek symbols
r electrical conductivity
X constant rotation velocity
g aspect ratio / nanoparticle volume fraction
a thermal diffusivity
h dimensionless temperature
l dynamic viscosity
Trang 3lnf¼ lf
ð1 /Þ2:5þ kBrownian
kf lf
Pr All needed coefficients and properties are illustrated in Tables
1 and 2 [48] The dimensionless forms of above equations are as follows:
@2
v
@r2þ 1
r
@v
@r Ha2 ð1 gÞ2
A5
A2þ 1
r2
!
v Re A1
A2v
@v
@r¼ 0 ð6Þ 1
r
@
@r r@h
@r
þ EcPr A2
A4
@v
@r v
r
þ 4 3A4
Rd @2h
@r2
PrRe A3
A4
v@h
r¼ g : vðrÞ ¼ 1; h ¼ 1
where
r¼ r
r2
; v¼ v
X1r1
; g ¼ r1
r2
; Ha ¼ B0d
ffiffiffiffi
rf
lf
r
; h ¼ T T2
T1 T2
;
Re ¼ qfXr1r2
lf Pr ¼ lfðqCpÞf
qfkf ; Ec ¼ qfðX1r1Þ2
ðqCpÞfDT ;
Rd ¼ 4reT3=ðbRkfÞ; A1¼ qnf
qf; A2¼ lnf
lf ;
A3¼ ðqCpÞnf ðqCpÞf A4¼ knf
kf; A5¼ rnf
rf
ð9Þ
Nu over the hot cylinder is as follows:
Nu ¼ A4@h
@r
3 Basic Idea of AGM
The general forms of equation with its boundary conditions are as follows:
Table 2 The coefficient values of CuO–Water
nanofluids[48]
0
0.2
0.4
0.6
0.8
1
Present work Aberkane et al.
r*
V
Fig 2 Comparison of Aberkane et al.[49]and present results of
velocity profile, forg = 0.5, Ha = 4
Fig 3 Influence of Ha; Re on velocity profile
Trang 4pk: fðu; u0; u00; ; uðmÞÞ ¼ 0; u ¼ uðxÞ ð11Þ
u ðxÞ ¼ u0; u0ðxÞ ¼ u1; ; uðm1ÞðxÞ ¼ um1 at x ¼ 0
uðxÞ ¼ uL 0; u0ðxÞ ¼ uL 1; uðm1ÞðxÞ ¼ uL m1 at x ¼ L
(
ð12Þ
We assume that the solution of this equation is as follows:
u ðxÞ ¼ X
n
i¼0
aixi¼ a0þ a1x1þ a2x2þ þ anxn ð13Þ
The larger n makes larger accuracy of the solution By
inserting Eq (13) into (11) , the residual can be obtained.
According to boundary conditions and values of residual at
boundaries, the constant parameters in Eq (12) can be
obtained.
4 Application of AGM Firstly, we introduce the residuals:
F ¼ @
2
v
@r2þ 1
r
@v
@r Ha2 ð1 gÞ2
A5
A2þ 1
r2
!
v Re A1
A2v
@v
@r¼ 0
G ¼ 1
r
@
@r r@h
@r
þ EcPr A2
A4
@v
@r v
r
þ 4 3A4Rd
@2h
@r2
PrRe A3
A4
v@h
@r¼ 0
ð14Þ
We assume that the solutions of these equations are as follows:
v¼ X
7
i¼0
aiðrÞi; h ¼ X
7
i¼0
Fig 4 Influence of Ha; Re; Ec; Rd on temperature profile
Trang 5According to below equations, all constant parameters can be
obtained.
v¼ vðB:CÞ; h ¼ hðB:CÞ;
F ðB:CÞ ¼ 0; F0ðB:CÞ ¼ 0;
G ðB:CÞ ¼ 0; G0ðB:CÞ ¼ 0
ð16Þ
5 Results and discussion
CuO-water nanofluid flow in an annulus is studied analytically
using AGM Horizontal magnetic field and thermal radiation
impacts are taken into account Influences of effective
param-eters are depicted as graphs AGM outputs are verified with
those of reported by Aberkane et al [49] Fig 2 proved the
accuracy of AGM Fig 3 depicts the influence of Ha; Re on
velocity profile As inertial forces dominate viscous forces,
velocity augments As electromagnetic forces dominate viscous
force, velocity decreases So velocity enhances with rise of Re but it reduces with rise of Ha : Impacts of Ha; Re; Rd; Ec on temperature profile are illustrated in Fig 4 Lorentz forces reduce the velocity and generate secondary flow, and in turn temperature reduces with rise of Ha : Temperature gradient near the inner pipe reduces with rise of Ha ; Rd but it enhances with rise of Re : Higher Ec provides higher viscous dissipation,
so temperature augments with increase of Ec: Fig 5 shows the impacts of Re ; Ec; Rd; g; Ha on Nu Nusselt number augments with rise of Ha ; Rd but it decreases with rise of Re; Ec: Dis-tance between the two pipes reduces with augments of g; so rate
of heat transfer enhances with increase in aspect ratio.
6 Conclusions Effect of radiation heat transfer on nanofluid heat transfer between two pipes is examined in existence of horizontal mag-netic field KKL Model is selected for nanofluid Governing Fig 5 Influence of Re; Ha; Ec; Rd; g on Nusselt number
Trang 6formulae are solved by means of AGM Roles of aspect ratio,
Reynolds number, Eckert number and Hartmann number are
illustrated as graphs Results revealed that temperature
enhances with rise of Eckert number and Reynolds number
but it reduces with augment of Hartmann number and
radia-tion parameter Nusselt number augments with rise of Lorentz
forces but it decreases with rise of viscous dissipation.
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