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Begell House Inc., http://begellhouse.comSpecial Downloaded 2011-3-13 from IP by Dr. Chiu-On Ng (cong) Topics & Reviews in 147.8.84.141 Porous Media — An International Journal, 2 (1): 11–22 (2011) ELECTROHYDRODYNAMIC STABILITY OF COUPLE STRESS FLUID FLOW IN A CHANNEL OCCUPIED BY A POROUS MEDIUM N. Rudraiah,1,2,∗ B. M. Shankar,1 & C. O. Ng3 1 UGC-Centre for Advanced Studies in Fluid Mechanics, Department of Mathematics, Bangalore University, Bangalore, India 2 National Research Institute for Applied Mathematics, Jayanagar, Bangalore, India 3 Department of Mechanical Engineering, The University of Hong Kong, Hong Kong, Republic of China ∗ Address all correspondence to N. Rudraiah E-mail: [email protected] Original Manuscript Submitted: 3/9/2010; Final Draft Received: 7/26/2010 The linear stability of electrohydrodynamic poorly conducting couple stress viscous parallel fluid flow through a porous channel is studied in the presence of a nonuniform transverse electric field using an energy method. Supplemented with a single term Galerkin expansion. The sufficient condition for stability is obtained using the nature of the growth rate as well as sufficiently small values of the Reynolds number, Re. From this condition we show that strengthening or weakening of the stability criterion is dictated by the values of the strength of the electric field, the coefficient of couple stress fluid, and the porous parameter. In particular, it is shown that the interaction of the electric field with couple stress is more effective in stabilizing the poorly conducting couple stress fluid compared with that in an ordinary Newtonian viscous fluid. KEY WORDS: porous medium, stability, couple stress, electrohydrodynamic, nonuniform transverse electric field 1. INTRODUCTION The effective functioning of microfluidic devices in electronics and electrical and mechanical engineering involving fluids, particularly those having vibrations and petroleum products containing organic, inorganic, and other microfluidics, requires the understanding and control of stability of parallel fluid flows. These substances, dissolving in the fluid, make the fluid poorly conducting. The electrical conductivity, σ, of such poorly conducting fluidics, increases with the temperature and the concentration of freely suspended particles. These freely suspended particles in fluid spin, producing microrotation, forming micropolar fluid. According to Eringen (1966) the micropolar fluids may be regarded as non-Newtonian fluids like fluid suspensions. The presence of dust in the atmo- c 2011 by Begell House, Inc. 2151–4798/11/$35.00 ° spheric fluid, the cholesterols, RBC, WBC, and so on, in the physiological fluid; the Hylauronic acid and nutrients in synovial fluid in synovial joints; and the presence of Deuterium–Tritium (DT) in Inertial Fusion Target (IFT) may also be modeled using the micropolar fluid theory of Eringen (1966). This theory takes care of the inertial characteristics of the substructure particles that are allowed to spin and thus undergo microrotation (Peddieson and McNitt, 1970; Ariman et al., 1973; Lukaszewicz 1999; Eringen, 2001). A particular case of micropolar fluid theory, when the microrotation balances the natural vorticity of a poorly conducting fluidics in the presence of an electric field, is called ‘electrohydrodynamic couple stress fluid (EHDCF) (Rudraiah, 1998, 2003). These EHDCFs exhibit a variation of electrical conductivity, ∇σ, increasing with temperature and concen- 11 12 Begell House Inc., http://begellhouse.com Downloaded 2011-3-13 from IP 147.8.84.141 by Dr. Chiu-On Ng (cong) Rudraiah, Shankar, & Ng NOMENCLATURE qi k Ji Ei Tb Cb T0 C0 p V We Re c cr ci l velocity vector (u, v) permeability of a porous medium current density electric field conduction temperature diffusion concentration initial temperature initial concentration pressure applied uniform electric potential electric number, ε0 V 2 /ρu20 h2 Reynolds number, u0 h/ν velocity of perturbed quantities phase velocity growth rate horizontal wavenumber t x, y time space coordinates Greek Symbols ρ density µ viscosity µe effective viscosity β ratio of effective viscosity to the viscosity, µe /µ λ coefficient of couple stress λe effective coefficient of couple stress Λ ratio of coefficient of effective couple stress to the couple stress, λe /λ ρe distribution of charge density σ electrical conductivity αt , αc volumetric coefficient of σ φ electric potential σp porous parameter tration of freely suspended particles, and releasing the charges from the nuclei forming distribution of charge ~ i. density, ρe . These charges induce an electric field, E ~ If need be, we can apply an electric field, Ea , by embedding electrodes of different potentials at the boundaries. ~ =E ~i + E ~ a , produces a current The total electric field, E ~ ~ density, J = σE, according to Ohm’s law and also pro~ This J~ acts as sensing duces an electric force, F~e = ρe E. ~ and the force, Fe , acts as actuation. These two properties make the poorly conducting couple stress fluid act as a smart material (Rudraiah, 2003). This smart couple stress poorly conducting fluid plays a significant role in controlling the stability of parallel flows, which is essential for an effective function of machineries that are used in the practical problems mentioned above. Such smart couple stress poorly conducting fluid also helps to develop the artificial organs at the molecular level and will contribute to the further advancement of physiological studies. These developments play a significant role in human joints, coronary arterial diseases, trachea (i.e., wind pipe), and so on. In the human body, there are three types of joints, namely, freely movable (i.e., diarthrodial), slightly movable (i.e., amphiarthrodial), and immovable (i.e., synarthrodial). The freely movable joints are known as the synovial joints (SJs), and they play a significant role because of their importance in human locomotion. The two important parts of SJs are the cartilage and the rheological nature of synovial fluid (see Fig. 1). The cartilage, a flossy, grayish white substance of about 1–2 mm thickness covering the articulating ends of the bones, plays a significant role in the normal functioning of joints. The synovial fluid (SF) of high viscosity impregnates the movable joints of the body and is contained in the capsules of the joints, normally in volumes of about 0.2–2 mL. It serves as a lubricant between the cartilage surfaces and carries out metabolic functions by providing nutrients to the articular cartilage (AC). Although SF has some resemblance compositionally to blood plasma, it lacks the clotting agents such as fibrinogen. The most important constituent of SF is the hyaluronic acid (HA), which makes the SF have a high viscosity of about 1000 times greater than water. The normal SF is non-Newtonian, exhibiting a decrease in viscosity with an increase in shear rate (Rudraiah, 1998). The most important aspect of SJs is to understand the different Special Topics & Reviews in Porous Media — An International Journal Begell House Inc., http://begellhouse.com Downloaded 2011-3-13 Stability of Couple Stress Fluid Flow from IP 147.8.84.141 by Dr. Chiu-On Ng (cong) Electrohydrodynamic FIG. 1: Synovial joint. aspects, including its lubrication mechanism in human locomotion, because the results obtained may shed light on the understanding of the degenerative changes in SJs that directly affect the normal physiological functioning of an individual. These changes can evolve through the following four types of arthritis: (1) Osteoarthritis, common during old age; (2) traumatic arthritis, occurs due to injuries; (3) rheumatic arthritis, occurs due to diseases; and (4) kinesthesia arthritis, occurs due to an erring gene. Among the recent genetic discoveries reported by the U. S. National Institute of Arthritis is a single genetic flaw that could cause a very common type of arthritis called kinesthesia arthritis. According to the orthopedic surgeons, although it may not be possible to prevent arthritis, there are steps that can be taken to reduce the risk of developing this disease and to slowdown or prevent permanent joint damage. The present measures include reduction in weight (as excess weight puts strain on the joints), doing regular exercise to help the muscles become strong (which will protect and support the joints), and using joint protecting devices and techniques at work (such as proper lifting and posture) to protect muscles and joints. It is known that the above degenerative changes in SJs may be due to physiological and mechanical aspects. One of the physiological aspects is gout, which occurs when the body cannot eliminate the natural substance called uric acid (UA). Volume 02, Number 1, 2011 13 The excess UA forms needle-like crystals in the joints that cause gout, namely, swelling, causing severe pain. The mechanical aspects of degenerative changes in SJs are mainly due to degenerative changes in the cartilage. It is believed (Rudraiah et. al., 2006) that the degenerative changes in ACs will not be naturally recouped using the above-mentioned preventive measures, and when the disorder becomes severe replacement with artificial joints is the only alternative to relieve pain. It is a common observation that artificial joints are manufactured using metals. We know (Ng et. al., 2005) the difficulties in manufacturing metal joints, which are not biocompatible with natural joints. These metal joints will have either rough or smooth surfaces. Both of them are dangerous to the body because they produce stresses, which in turn produce a force that drives the erythrocytes (i.e., RBC) in joints to a particular region where the high concentration of RBC leads to bursting of RBCs, releasing heamoglobin, resulting in a disease called heamolysis due to the loss of heamoglobin. Recently, Ng et al. (2005) have suggested a mechanism of using the smart material of nanostructure to mimic the natural joints as an alternative to metal joints by studying the dispersion of micropolar components in a biological bearing. This force, produced by the metal joints, may also disturb the SF, causing instabilities that in turn may contribute to the malfunctioning of the joints. Further, we note that HA, UA, nutrients, and so on, in the synovial fluid are freely suspended, executing microrotation. In the literature, considerable work has been done to find the effect of this force by studying dispersion phenomena but, to our knowledge, no work has been done on the study of the stability of SF to model it as a couple stress fluid and to understand the degenerative changes in arthritis caused by the instabilities produced by the above-mentioned force. The study of the stability of SF is the main objective of this paper. To achieve this objective, this paper is planned as follows: The required basic equations, corresponding boundary conditions are given in Section 2 on mathematical formulation. The basic state and the stability equations are given in Section 3. The stability analysis is given in Section 4. Results and Discussion are drawn in the Section 5 and conclusions are presented in Section 6. 2. MATHEMATICAL FORMULATION We consider a horizontal poorly conducting couple stress fluid flow through a sparsely packed porous layer bouon both sides by electro-conducting impermeable rigid plates embedded with segmented electrodes located at 14 Begell House Inc., http://begellhouse.com Downloaded 2011-3-13 from IP 147.8.84.141 by Dr. Chiu-On Ng (cong) y = 0 and y = h having different electric potentials φ = (V /h) x at y = 0 and φ = (V /h) (x − x0 ) at y = h, as shown in Fig. 2. For the sake of clarity, we first give the general form of modified basic equations for a poorly conducting couple stress incompressible fluid through a sparsely packed porous medium, modification in the sense of addition of the couple stress and electric force to be obtained from the general form of Maxwell equations. The rheological properties of physiological fluids like synovial fluid in synovial joints and blood flow in arteries reveal that viscosity varies nonlinearly, exhibiting either shear thinning or shear thickening behavior. This is one of the nonNewtonian fluid flow properties that has been studied in the literature (Fung, 1981; Rudraiah, 1998), but their work is absent of the study of microrotation due to freely suspended particles, as explained in Section 1. These are taken into account in this paper using the couple stress fluid as a particular case of micropolar fluid theory, developed by Eringen (1966), as described by Rudraiah et al. (1998). We note that one of the limitations encountered in the continuum theory is the lack of taking into account the microrotation of freely suspended particles in a fluid. For example, HA molecules and other nutrients present in synovial fluid, RBC, WBC, and so on, in blood, DT in (IFT) in the extraction of inertial fusion energy (IFE), and so on, are freely suspended, executing spin. In that case, the microrotation of the microelements must be taken into account in deriving the required basic equations where the microelement motions play a significant role. In such situations, the couple stress theory, a particular case of micropolar fluid, as explained above, is useful. Then, the required basic equations for a couple stress poorly conducting fluid flowing through a sparsely packed porous medium, following Stokes (1968) and Rudraiah et al. (1998), are: The conservation of mass, for an incompressible fluid: Rudraiah, Shankar, & Ng ∂qi =0 ∂xi The conservation of momentum: µ ¶ ∂qi ∂qi ∂p ∂ 2 qi ρ + qj =− + µe 2 ∂t ∂xj ∂xj ∂x µ ¶ i 4 ∂ qi µ λ 1+ qi − λe 4 + ρe Ei − ∂xi k µk (1) (2) where qi = (u, v) is the velocity, ρ is the density, p is the pressure, µe is the effective viscosity, λe is the effective coefficient of couple stress, λ is the coefficient of couple stress, µ is the viscosity of the fluid, k is the permeability of a porous medium, and λ/µ has the dimension of length square. The conservation of charges: ∂ρe ∂Ji + =0 ∂t ∂xj (3) where ρe is the distribution of charge density Ji = ρe qi + σEi (4) where Ji is the current density, which is the sum of convective current, ρe qi , and conduction current, σEi , σ is the electrical conductivity, Ei , is the electric field. These are supplemented with the Maxwell Field equations for a conducting medium: Gauss law ∂Ei ρe (5) = ∂xi ε0 where εo is the dielectric constant for free space. In a poorly conducting fluid, the induced magnetic field is negligible and there is no applied magnetic field; hence, the Faraday law becomes ∂Ei ∂Ej − =0 ∂xj ∂xi (6) That is, the electric field is conservative, so that Ei = − ∂φ ∂xi (7) where ϕis the electric potential. Equation (3), using Eqs. (4) and (1), takes the form ∂ (σEi ) Dρe + =0 Dt ∂xj FIG. 2: Physical configuration. (8) where D/Dt = ∂/∂t + qj (∂/∂xi ). We note that in a poorly conducting fluid σ ¿ 1 and, hence, any perturbation on it is assumed to be negligible and increases with Special Topics & Reviews in Porous Media — An International Journal Begell House Inc., http://begellhouse.com Downloaded 2011-3-13 Stability of Couple Stress Fluid Flow from IP 147.8.84.141 by Dr. Chiu-On Ng (cong) Electrohydrodynamic conduction temperature, Tb , and diffusion concentration, Cb , such that σ = σo [1 + αt (Tb − T0 ) + αc (Cb − Co )] (9) 15 The solutions of Eqs. (13), satisfying conditions (14a) and (14b), are Tb = ∆T y + T0 h and Cb = ∆C y + C0 h (15) Here, σ0 is that of σ at Tb = T0 and Cb = C0 , αt and αc where ∆T = T − T and ∆C = C − C 1 0 1 0 are the volumetric expansion coefficients of σ. The ex- Substituting the solutions given by Eq. (15) into Eq. (9), pressions for Tb and Cb are obtained in Section 3.1. we get σb = σ0 (1 + αh y) ≈ σ0 eαh y 3. THE LINEAR STABILITY EQUATIONS FOR A COUPLE STRESS POORLY CONDUCTING FLUID In this section, we derive the stability equations subject to infinitesimal disturbances superposed on the basic state given in Section 3.1 below. 3.1 Basic State We consider a basic flow in a poorly conducting couple stress fluid and assuming it to be fully developed and unidirectional parallel to the plates driven by a constant pressure gradient ∂pb /∂x. Then, the basic flow, ub , parallel to the boundaries in the x-direction, satisfies the momentum equations ∂pb 0=− ∂x µ µ 1+ − k ∂pb 0=− ∂y ∂ 2 ub ∂ 4 ub + µe − λe + ρeb Ebx 2 ∂y ∂y 4 ¶ λ ub µk + ρeb Eby where the suffix b represents the basic state quantities. The boundary conditions are the no-slip conditions ub = 0 at y = 0 and h (11) at y = 0 and h (12) Further, Tb and Cb in Eq. (9) are the solutions of d2 Tb =0 dy 2 and d 2 Cb =0 dy 2 (17) subject to the boundary conditions φb = Vx h at y = 0 V (x − x0 ) h (18a) at y = h (18b) where V is the applied uniform electric potential. We make quantities in Eqs. (17), (18a), and (18b) dimensionless, using φb , V y y∗ = h φ∗b = ρ∗eb = ε0 ρeb ¡ V ¢, x∗ = h2 x , h (19) ∂ 2 φb ∂ 2 φb ∂φb + + αh =0 2 ∂x ∂y 2 ∂y (20) satisfying the boundary conditions (13) satisfying the conditions φb = x at y = 0 φb = x − x0 Tb = T0 and Cb = C0 at y = 0 (14a) Tb = T1 and Cb = C1 at y = h (14b) Volume 02, Number 1, 2011 ∂ 2 φb ∂ 2 φb ∂φb + + αh =0 2 ∂x ∂y 2 ∂y where the asterisks (*) denote the dimensionless quantities. Substituting Eq. (19) into Eqs. (17), (18a), and (18b), and for simplicity neglecting the asterisks, we get and the couple stress conditions ∂ 2 ub =0 ∂y 2 (16) where αh = αt ∆t/h + αc ∆C/h In a poorly conducting fluid, the frequency of charge distribution is smaller than the corresponding relaxation frequency of the electric field, so that Dρe /Dt in Eq. (8) is negligible compared to ∂ (σEi )/∂xj . Then, from Eq. (8), after neglecting Dρe /Dt and using Eqs. (7) and (16), we get φb = (10) (∵ αh ¿ 1) at y = 1 (21a) (21b) The solution of Eq. (20), satisfying boundary conditions (21a) and (21b), is 16 Begell House Inc., http://begellhouse.com Downloaded 2011-3-13 from IP 147.8.84.141 by Dr. Chiu-On Ng (cong) φb = x − xo (1 − e−αh y ) (1 − e−αh ) (22) The expression for ρeb can be obtained, from Eq. (5), using Eq. (22), as ρeb = − x0 α2h e−αh y (1 − e−αh ) (23) Equation (7), using Eq. (22) becomes Ebx = −1, Eby = Rudraiah, Shankar, & Ng The average velocity, 1 u0 = 2 Z1 ub dy = 0 δ3 (∆3 + ∆4 − ∆7 ) δ6 (29) where the constants ∆i (i = 1 − 7) are given in the Appendix. 3.2 Stability Equations −αh y x0 αh e (1 − e−αh ) (24) We make Eqs. (10)–(12) dimensionless, using pb y ub , p∗b = , y∗ = , u0 ρu20 h ρeb x Eb x∗ = , ρ∗eb = ¡ V ¢ , Eb∗ = ¡ V ¢ h ε0 h2 h u∗b = (25) where u0 is the average velocity and the other quantities are as defined in Eq. (19). Substituting Eq. (25) into Eqs. (10)–(12), using Eqs. (23) and (24), and for simplicity neglecting the asterisks, we get In a two-dimensional, incompressible, homogeneous poorly conducting couple stress fluid flow, with qi = (u, v), the conservation of momentum, given by Eq. (2), takes the form ρe ∂u ∂u ∂u 1 ∂p µe 2 ∇ u + Ex +u +v =− + ∂t ∂x ∂y ρ ∂x ρ ρ µ ¶ µ λe 4 λ 1+ u (30) − ∇ u− ρ ρk µk ρe ∂v ∂v ∂v 1 ∂p µe 2 ∇ v + Ey +u +v =− + ∂t ∂x ∂y ρ ∂y ρ ρ µ ¶ µ λe 4 λ 1+ v (31) − ∇ v− ρ ρk µk Λ ∂ 4 ub ∂ 2 ub − β 2 = −ReP + We ReM e−αh y together with the conservation of mass 2 4 a ∂y ∂y ¶ µ ∂u ∂v σ2p + =0 (32) (26) − σ2p 1 + 2 ub ∂x ∂y a where ∇2 = ∂ 2 /∂x2 + ∂ 2 /∂y 2 , ∇4 = ∂ 4 /∂x4 + p λ/µ is the coefficient of 2∂ 4 /∂ 2 x∂ 2 y + ∂ 4 /∂y 4 where a = h/m; m = the couple stress fluid; β = µe /µ is the ratio of visTo study the electrohydrodynamic stability of coucosities (i.e., Brinkmann viscosity to viscosity of fluid); ple stress poorly conducting fluid in a saturated porous Λ = λe /λ is the ratio of coefficient of effective couple medium, as shown in Fig. 2, we superimpose an infinitesstress to the couple stress P = ∂pb /∂x; Re = u0 h/υ is imal disturbance, denoted by the primes, over the basic the Reynolds number; √ We = ε0 V 2 /ρu20 h2 is the elec- state denoted by suffix ”b” of the form tric number; σp = h/ k is the porous parameter; and u = ub + u0 , v = v 0 , p = pb + p0 , M = x0 α2h /(1 − e−αh ). Physically We represents the Ex = Ebx + Ex0 , Ey = Eby + Ey0 (33) ratio of electric energy to kinetic energy. The required boundary conditions are Substituting Eq. (33) into Eqs. (30)–(32), and linearizing by neglecting the product and higher order of prime 2 ∂ ub ub = = 0 at y = 0 and 1 (27) quantities compared with the basic state, we obtain ∂y 2 ∂u0 ∂u0 ∂ub 1 ∂p0 µe + ub + v0 =− + Solving Eq. (26), using the boundary conditions (27), we ∂t ∂x ∂y ρ ∂x ρ get µ 2 0 ¶ 2 0 λe ∂ u ∂ u 1 × + + (ρeb Ex0 + ρ0e Ebx ) − ub = C1 eδ1 y + C2 e−δ1 y + C3 eδ2 y + C4 e−δ2 y ∂x2 ∂y 2 ρ ρ µ 4 0 ¶ −αh y 2 2 4 0 4 0 We ReP a M e ReP a ∂ u ∂ u ∂ u µ + − (28) × +2 2 2 + − ΛK2 Λ (α4h − K1 α2h + K2 ) ∂x4 ∂x ∂y ∂y 4 ρk ¶ µ λ where the constants Ki (i = 1 and 2), δi (i = 1 − 6), and u0 (34) × 1+ µk Ci (i = 1 − 4) are given in the Appendix. Special Topics & Reviews in Porous Media — An International Journal Begell House Inc., http://begellhouse.com Downloaded 2011-3-13 Stability of Couple Stress Fluid Flow from IP 147.8.84.141 by Dr. Chiu-On Ng (cong) Electrohydrodynamic ∂v 0 ∂v 0 1 ∂p0 µe + ub =− + ∂t ∂x ρ ∂y ρ µ 2 0 ¶ 2 0 ¡ ¢ λe ∂ v ∂ v 1 ρeb Ey0 + ρ0e Eby − × + + 2 2 ∂x ∂y ρ ρ µ 4 0 ¶ 4 0 4 0 ∂ v ∂ v ∂ v µ × +2 2 2 + − ∂x4 ∂x ∂y ∂y 4 ρk ¶ µ λ v0 (35) × 1+ µk ∂u0 ∂v 0 + =0 (36) ∂x ∂y These perturbed equations are made dimensionless using the quantities u v y x , v∗ = , y ∗ = , x∗ = , u∗ = u0 u0 h h ρe p ∗ t E ¡ V ¢ , Ex∗ = ¡ Vx¢ , , t = ³ ´ , ρ∗e = p∗ = h ρu20 ε0 h2 h u0 Ey Ey∗ = ¡ V ¢ (37) h where c = cr + ici is the velocity of perturbed quantities, cr is the phase velocity, ci is the growth rate, and l is the horizontal wavenumber, which is real and positive. If ci > 0, the system is unstable and ci < 0, the system is stable. Equations (38)–(40), using Eq. (41), and after simplification, take the form " Λ β(D2 − l2 ) − ilRe(ub − c) − 2 (D2 − l2 )2 a µ ¶# σ2p σ2p 1+ 2 u = ilRep + ReDub v − Re a − We Re(ρeb Ex + ρe Ebx ) " β(D2 − l2 ) − ilRe(ub − c) − σ2p − Re µ σ2p 1+ 2 a ¶# ∂u ∂u ∂p β + ub + Dub v = − + ∂tµ ∂x ∂x Re ¶ ∂2u ∂2u × + 2 + We (ρeb Ex + ρe Ebx ) ∂x2 ∂y µ 4 ¶ ∂ u ∂4u ∂4u Λ +2 2 2 + 4 − 2 a Re ∂x4 ∂x ∂y ∂y µ ¶ 2 2 σp σp 1+ 2 u − Re a ∂v ∂v ∂p β + ub =− + ∂t ∂x ∂y Re µ 2 ¶ ∂ v ∂2v × + 2 + We (ρeb Ey + ρe Eby ) ∂x2 ∂y µ 4 ¶ ∂ v Λ ∂4v ∂4v − 2 +2 2 2 + 4 a Re ∂x4 ∂x ∂y ∂y µ ¶ 2 2 σp σp 1+ 2 v − Re a Volume 02, Number 1, 2011 y) eil(x−ct) Λ (D2 − l2 )2 a2 ilu + Dv = 0 (43) (44) Eliminating pressure p between Eqs. (42) and (43), by operating D on Eq. (42), multiplying Eq. (43) by il, and then subtracting and expressing u = (i/l)(Dv) and Ey = (−i/l)(DEx ) using, respectively, Eqs. (44) and (5), we get the stability equation (D2 − l2 )2 D2 ub v + iβ v (ub − c) (ub − c) (Dρeb Ex + Dρe Ebx ) Λ (D2 − l2 )3 v + We lRe − 2 a (ub − c) (ub − c) ¢ ¶¡ 2 µ 2 2 D −l σp v=0 − iσ2p 1 + 2 (45) a (ub − c) ¡ ¢ Equation (45), using Ebx = −1, Dρe = − D2 − l2 × Dφ and retaining terms up order α2h since αh ¿ 1, takes the form lRe(D2 − l2 )v − lRe (38) (39) ∂u ∂v + =0 (40) ∂x ∂y where the parameters a, We , σp , β, Λ, and Re are defined in Eq. (26). To discuss the stability of systems (38)–(40), we use the normal mode solution of the form (function of (42) v = ReDp − We Re(ρeb Ey + ρe Eby ) Substituting Eq. (37) into Eqs. (34)–(36), and for simplicity neglecting the asterisks (*) and the primes, we get 17 (41) (D2 − l2 )2 D2 ub v + iβ v (ub − c) (ub − c) ¡ 2 ¢ D − l2 Dφ iΛ (D2 − l2 )3 v + We lRe − 2 a (ub − c) (ub − c) ¢ ¶¡ 2 µ 2 2 D −l σp v=0 − iσ2p 1 + 2 (46) a (ub − c) lRe(D2 − l2 )v − lRe Equation (46) is the required stability equation, which is called the modified form of Orr–Sommerfeld equation 18 Begell House Inc., http://begellhouse.com Downloaded 2011-3-13 from IP 147.8.84.141 by Dr. Chiu-On Ng (cong) Rudraiah, Shankar, & Ng (modified in the sense of incorporating the contribution The second term on the left-hand side of Eq. (48) is the ~ and the couple stress fluid) contribution of the couple stress fluid and the term involvfrom the electric force, ρe E and satisfying the boundary conditions ing We in the first term on the right-hand side of Eq. (48) is the effect of the electric field. v = Dv = D3 v = 0 at y = 0 and 1 (47) Equating the real and imaginary parts of Eq. (48) to zero we respectively, get The conditions on Dv and D3 v are obtained from Qr Eq. (44) using the no-slip and couple stress conditions on (51) cr = 2 (I1 + l2 I02 ) u. To find the conditions for stability or instability of the basic flow, we find (following Rudraiah, 1962, 1963; Drazin and Reid, 2004; Shubha et al., 2008) the nature of c using the energy method. For this, we multiply Eq. (46) by v̄, the complex conjugate of v, and integrating the resulting equation with respect to y from 0 to 1 and using boundary conditions (47) and after simplification, we get ¡ ¢ Λ ¡ ¢ β I22 +2l2 I12 +l4 I02 + 2 I32 +3l2 I22 +3l4 I12 +l6 I02 a ¶ µ 2 ¡ ¢ σ p I12 + l2 I02 = −ilReQ + σ2p 1 + 2 a + ilRec(I12 + l2 I02 ) (48) where Z In2 1 = 0 Z 1 Q= Z + 2 |Dn v| dy (n = 0 − −3) h i 2 2 ub |Dv| + (l2 ub + D2 ub ) |v| dy 0 1 Z v̄DvDub dy − We 0 " µ 2 ¶ 3l Λ 1 Λ 2 I + + β I22 ci = Qi − lRe a2 3 a2 à ! 3l4 Λ + σ2p 2 2 + (2l β + σp ) I12 + a2 ! #! à l2 (l4 Λ + σ4p ) 2 2 2 + l (l β + σp ) I02 + a2 à 4. STABILITY ANALYSIS 0 1 ¡ 2 ¢ D − l2 ÷ (I12 + I 2 I02 ) (52) The nature of stability is determined from Eq. (52) in the following two cases. Case 1: A Sufficient condition for stability, in terms of growth rate ci is obtained, following Joseph (1968), in Result 1. Result 1: Let c be the eigenvalue of Eq. (48). Then, a sufficient condition for stability is N1 ≥ max (We F1 + F0 ) F2 Proof: Eq. (52) can be written as ci = F0 + We F1 − N1 F2 (I12 + l2 I02 ) (53) × Dφv̄ = Qr + iQi R1 where F0 = 0 (vr Dvi − vi Dvr )Dub dy, which is the ¶ µ Z 1( 1 first integral on the right-hand side of Eq. (50); F1 = Qr = Re (Q) = ub |Dv|2 + l2 ub + D2 ub ¢ R1¡ 2 2 0 D − l2 (vi Dφr − vr Dφi ) dy, which is the second 0 ) integral on the right-hand side of Eq. (50); and ¡ 2 ¢ 2 2 × |v| − We D − l (vr Dφr + vi Dφi ) dy (49) ¶ µ 2 3l Λ Λ + β I22 F2 = 2 I32 + a a2 ¶ µ 4 and ¢ 2 3l Λ + σ2p ¡ 2 2 ( + 2l β + σ I1 + p Z 1 a2 ! à ¡ ¢ Qi = Im (Q) = (vr Dvi − vi Dvr ) Dub ¡ ¢ 2 l2 l4 Λ + σ4p 0 2 2 2 + l l β + σp I0 + ) a2 ¡ 2 ¢ + We D − l2 (vi Dφr − vr Dφi ) dy (50) 1 N1 = lRe Special Topics & Reviews in Porous Media — An International Journal Begell House Inc., http://begellhouse.com Downloaded 2011-3-13 Stability of Couple Stress Fluid Flow from IP 147.8.84.141 by Dr. Chiu-On Ng (cong) Electrohydrodynamic 19 Here, F2 is always positive, and F0 and F1 may be posi- and using Schwarz’s inequality, we get tive or negative depending on the signs of the arguments |Im (Q)| ≤ I1 I0 q + B1 in their integral: If N1 ≥ max (F0 + We F1 ) F2 where (54) 0≤y≤1 ci is always negative; hence, the motion is always stable. Inequality (54) gives the sufficient condition for stability; hence, Result 1. In particular, if the basic velocity is uniform, that is, ub = constant, so that Dub = 0 implying F0 = 0, then Eq. (53) becomes ci = We F1 − N1 F2 (I12 + l2 I02 ) If N1 ≥ max We F1 F2 q = max |Dub | (55) Z 1 B1 = We ¯¡ 2 ¯ ¢ ¯ D − l2 (vi Dφr − vr Dφi )¯ dy 0 This gives the upper bound for ci " µ 2 ¶ 3l Λ 1 Λ 2 I + + β I22 ci ≤ (qI0 I1 + B1 ) − lRe a2 3 a2 à ¡ ¢ ¶ µ 4 ¢ 2 l2 l4 Λ + σ4p 3l Λ + σ2p ¡ 2 2 + 2l β + σp I1 + + a2 a2 ! # ¡ ¢ ¡ ¢ + l2 l2 β + σ2p I02 / I12 + l2 I02 (57) ci is always negative; hence, the motion is always stable. Inequality (55) gives the sufficient condition for stability From Eq. (57), it follows that a sufficient condition for for uniform basic velocity. stability is Case 2: In this case, a sufficient condition for stability is " µ 2 ¶ 3l Λ 1 Λ 2 determined in terms of the Reynolds number, Re, as given I + + β I22 Re < in the Result 2. l(qI0 I1 + B1 ) a2 3 a2 ! à à Result 2: A sufficient condition for stability is 4 2 ¡ 2 ¢ l2 (l4 Λ + σ4p ) 3l Λ + σ p 2 2 " + 2l β + σ I + + µ 2 ¶ p 1 a2 a2 3l Λ 1 Λ 2 I3 + + β I22 Re < ! # 2 2 l (qI0 I1 + B1 ) a a ¶ µ 4 + l2 (l2 β + σ2p ) I02 (58) 2 ¢ 2 3l Λ + σp ¡ 2 2 + 2l β + σ I + p 1 a2 ! # à ¡ ¢ Hence, Result 2. ¡ ¢ 2 l2 l4 Λ + σ4p 2 2 2 + l l β + σ I + p 0 a2 5. RESULTS AND DISCUSSION Proof: Following Drazin and Reid (2004), we prove Result 2. We first write Eq. (50) in the form Z i 1 (vDv̄ − v̄Dv)Dub dy Im (Q) = 2 0 Z 1 ¢ ¡ 2 + We D − l2 (vi Dφr − vr Dφi ) dy 0 From Eq. (56) it follows that Z |Im (Q)| ≤ Z + We 1 |v| |Dv| |Dub | dy 0 1 ¯¡ 2 ¯ ¢ ¯ D − l2 (vi Dφr − vr Dφi )¯dy 0 Volume 02, Number 1, 2011 (56) A sufficient condition for stability (ci < 0) is obtained from Eq. (52) as well as in terms of the Reynolds number, Re, given by Eq. (57). The growth rate given by Eq. (52) is also computed numerically using the singleterm Galerkin expansion and the results are depicted graphically. Figure 3 shows that the plot of growth rate ci as a function of horizontal wavenumber l for different values of couple stress parameter, a for fixed values of the electric number, We = 10, Re = 0.8, and porous parameter σp = 0.5. From the Fig. 3, it is clear that an increase in the value of a increases the value of ci because an increase in a is to decrease the viscosity, implying a decrease in resistance to the flow, which in turn promotes instability much faster. 20 Begell House Inc., http://begellhouse.com Downloaded 2011-3-13 from IP 147.8.84.141 by Dr. Chiu-On Ng (cong) FIG. 3: Variation of ci with l for different values of a when We = 10, Re = 0.8, and σp = 0.5. The variation of ci with l for different values of σp with We = 10, Re = 0.8, and a = 10 is shown in Fig. 4. From Fig. 4 it is clear that the effect of σp is to decrease the growth rate, which makes the system more stable. The plausible reason for this is that the decrease in growth rate is due to the resistance offered by the solid particles in the porous media to the fluid. Figure 5 shows that the plot of ci with l for different values of We for fixed values of Re = 0.8, σp = 0.5, and a = 10. From Fig. 5, it may be inferred that for an increase in the value of We decreases the value of ci , and FIG. 4: Variation of ci with l for different values of σp when We = 10, Re = 0.8, and a = 10. Rudraiah, Shankar, & Ng FIG. 5: Variation of ci with l for different values of We when Re = 0.8, σp = 0.5, and a = 10. thus make the system more stable. The reason being that an increase in We is to decrease the kinetic energy and, hence, makes the system more stable. 6. CONCLUSIONS It is known that in the stability of classical Poiseuille flow a sufficient condition for stability is the existence of the point of inflexion. This stability of Poiseuille flow was extended to the electrohydrodynamic stability of an inviscid poorly conducting parallel fluid flow in the presence of an electric field and in the absence of couple stress fluid by Shubha et al. (2008). They have shown that the electrohydrodynamic stability is determined in terms of the electric number rather than the point of inflexion of the basic velocity profile. In contrast to this, in our paper, a sufficient condition for stability is obtained using the nature of growth rate ci as well as a sufficiently small value of Reynolds number, Re. From this we found that strengthening or weakening of a sufficient condition for stability depends on the electric number, We , the coefficient of couple stress fluid, m, and the porous parameter, σp . From these, we conclude that the interaction of the electric field with the couple stress is more effective in stabilizing a poorly conducting couple stress fluid compared with that of ordinary Newtonian viscous fluid. This conclusion on stability analysis helps to understand the degenerative changes in arthritis caused by the instability produced by the force generated by metal joints discussed in the last paragraph of Section 1. Special Topics & Reviews in Porous Media — An International Journal Begell House Inc., http://begellhouse.com Downloaded 2011-3-13 Stability of Couple Stress Fluid Flow from IP 147.8.84.141 by Dr. Chiu-On Ng (cong) Electrohydrodynamic ACKNOWLEDGMENTS 21 nano and smart materials, Proc. of the Workshop on Modeling of Nano and Smart Materials, Jayanagar, Bangalore: Book Paradise, Chap. 2, pp. 4–46, 2003. This work is supported by ISRO under Research Project Nos. ISRO/ RES/2/338/2007-08 and ISRO/RES/2 Rudraiah, N. and Shankar, B. M., Stability of parallel couple /335/2007-08. The financial support of ISRO is gratefully stress viscous fluid flow in a channel, Int. J. App. Math., vol. acknowledged. B. M. S. gratefully acknowledges ISRO 1, pp. 67–78, 2009. for providing JRF under the above projects. The work of Rudraiah, N., Kantha, S., and Manonmani, M. N., Anatomy and C. O. N. was partly supported by the Research Grants biomechanics of synovial joints. Part I, Recent Trends in BaCouncil of the Hong Kong Special Administrative Resic and Applied Anatomy, eds. Thomas, I. M., Srinivasa, K., gion, China, through Project No. KHU 7156/09E. Rajeshwari, T., and Rajangam, S., Karnataka, Bangalore: Rajiv Gandhi University of Health Sciences, pp. 1–9, 1998. REFERENCES Ariman, T., Truk, M. A., and Sylvester, N. D., Microcontinuum fluid mechanics—a review, Int. J. Eng. Sci., vol. 11, pp. 905– 930, 1973. Drazin, P. G., Introduction to Hydrodynamic Stability, Cambridge, U. K.: Cambridge University Press, 2002. Drazin, P. G. and Reid, W. H., Hydrodynamic Stability, Cambridge, U. K.: Cambridge University Press, 2004. Eringen, A. C., Theory of Micropolar Fluids, J. Math. Mech., vol. 16, pp. 1–18, 1966. Eringen, A. C., Microcontinuum Field Theories. II: Fluent Media, New York: Springer, 2001. Fung, Y. C., Biomechanics, New York: Springer, 1981. Rudraiah, N., Ng, C. O., Nagaraj, C., and Nagaraj, H. N., Electrohydrodynamic dispersion of macromolecular components in biological bearing, J. Energy Heat Mass Transfer, vol. 28, pp. 261–280, 2006. Stokes, G. G., On some cases of fluid motion, Trans. Cambridge Philos. Soc., vol. 8, pp. 287–319, 1843. Stokes, V. K., Effects of couple stress in fluid on hydromagnetic channel flow, Phys. Fluids, vol. 11, pp. 1131–1133, 1968. Shivakumara, I. S. and Venkatachalappa, M., Stability of Flows, 3-I, New Delhi, Indis: Tata McGraw-Hill, 2004. Shubha, N., Rudraiah, N., and Chow, K. W., Electrohydrodynamic stability of poorly conducting parallel fluid flow in the presence of transverse electric field, Int. J. Non-Linear Mech., vol. 43, pp. 643–649, 2008. Joseph, D. D., Eigenvalue bounds for the Orr–Sommerfeld equation, J. Fluid Mech., vol. 33, pp. 617–621, 1968. Lin, C. C., The Theory of Hydrodynamic Stability, Cambridge, U.K.: Cambridge University Press, 1955. Lukaszewicz, G., Micropolar Fluids: Theory and Application, Basel, Switzerland: Birkhauser, 1999. Ng, C. O., Rudraiah, N., Nagaraj, C., and Nagaraj, H. N., Electrohydrodynamic dispersion of macromolecular components in nanostructured biological bearing, J. Energy Heat Mass Transfer, vol. 27, pp. 39–64, 2005. Peddieson, J. and McNitt, R. P., Boundary layer theory for a micropolar fluid, Recent Adv. Eng. Sci., vol. 5, pp. 405–476, 1970. Rudraiah, N., Magnetohydrodynamic stability of heterogeneous incompressible nondissipative conducting liquids, Appl. Sci. Res., Sect. B, vol. 11, pp. 105–117, 1962. Rudraiah, N., Magnetohydrodynamic stability of heterogeneous dissipative conducting liquids, Appl. Sci. Res., Sect. B, vol. 11, pp. 118–133, 1963. Rudraiah, N., Anatomy and biomechanics of synovial joints. Part II: Mathematical modeling, Recent Trends in Basic and Applied Anatomy, eds. Thomas, I. M., Srinivasa, K., Rajeshwari, T., and Rajangam, S., Karnataka, Bangalore: Rajiv Gandhi University of Health Sciences, pp. 37–105, 1998. Rudraiah, N., Instabilities of importance in the manufacture of Volume 02, Number 1, 2011 APPENDIX ¡ ¢ σ2 a2 + σ2 βa2 , K2 = , K1 = Λ rΛ q 1 K1 − K12 − 4K2 , δ1 = 2 2 r q 1 K1 + K12 − 4K2 , δ2 = 2 2 δ3 = a2 e−αh P Re, δ4 = K2 M We , δ5 = K2 − K1 α2h + α4h , δ6 = 2K2 δ5 Λ, · µ ½ αh δ1 2 C1 = δ3 (e − e )δ4 αh + eαh (δ5 − δ4 ) ¸ ¾· ¸¶ 2 δ1 αh − 1 + coth(δ1 ) + e (δ4 − e δ5 ) δ2 µ ¶ ÷ δ6 (δ21 − δ22 ) , µ ½ · αh +δ1 2 C2 = − δ3 (e − 1)δ4 αh + δ4 ¸ ¾ ¶ αh +δ1 2 αh (δ5 − δ4 ) δ2 cos ech(δ1 − e δ5 + e 22 Begell House Inc., http://begellhouse.com Downloaded 2011-3-13 from IP 147.8.84.141 by Dr. Chiu-On Ng (cong) µ ¶ 2 2 ÷ δ6 (δ1 − δ2 ) , µ ½ · αh δ2 2 C3 = δ3 (e − e )δ4 αh + eαh (δ5 − δ4 ) ¸ ¾· ¸¶ δ2 αh 2 + e (δ4 − e δ5 ) δ1 − 1 + coth(δ2 ) µ ¶ ÷ δ6 (δ22 − δ21 ) , µ ½ · αh +δ2 2 C4 = − δ3 (e − 1)δ4 αh + δ4 − eαh δ5 ¸ ¾ ¶ αh +δ2 2 +e (δ5 − δ4 ) δ1 cos ech(δ2 ) µ ¶ 2 2 ÷ δ6 (δ2 − δ1 ) , Rudraiah, Shankar, & Ng ∆1 = δ4 + eαh (δ4 − 2δ5 ) , ¡ ¢ ∆2 = 1 + eδ2 ¡ ¢ × δ22 − δ21 , ¡ ¢ eδ2 − 1 ∆1 δ21 , ∆3 = ∆ 2 δ2 ¡ δ ¢£ ¤ e 1 − 1 (eαh + 1) δ4 α2h − ∆1 δ22 , ∆4 = ∆ 2 δ1 µ ¶ δ2 , ∆5 = (eαh + 1) δ4 α3h sinh 2 µ ¶ δ2 αh ∆6 = [δ4 + e (αh δ5 − δ4 )] cosh 2 ¡ ¢ × δ2 δ22 − δ21 , ∆7 = 2eδ2 /2 (∆5 + ∆6 ) αh δ2 ∆2 Special Topics & Reviews in Porous Media — An International Journal