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Volume 2010, Article ID 465835,26pages doi:10.1155/2010/465835

Research Article

Pulsatile Flow of a Two-Fluid Model for Blood Flow through Arterial Stenosis

D. S. Sankar

School of Mathematical Sciences, University Science Malaysia, 11800 Penang, Malaysia

Correspondence should be addressed to D. S. Sankar,sankar ds@yahoo.co.in Received 25 January 2010; Accepted 4 April 2010

Academic Editor: Saad A. Ragab

Copyrightq2010 D. S. Sankar. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Pulsatile flow of a two-fluid model for blood flow through stenosed narrow arteries is studied through a mathematical analysis. Blood is treated as two-phase fluid model with the suspension of all the erythrocytes in the as Herschel-Bulkley fluid and the plasma in the peripheral layer as a Newtonian fluid. Perturbation method is used to solve the system of nonlinear partial differential equations. The expressions for velocity, wall shear stress, plug core radius, flow rate and resistance to flow are obtained. The variations of these flow quantities with stenosis size, yield stress, axial distance, pulsatility and amplitude are analyzed. It is found that pressure drop, plug core radius, wall shear stress and resistance to flow increase as the yield stress or stenosis size increases while all other parameters held constant. It is observed that the percentage of increase in the magnitudes of the wall shear stress and resistance to flow over the uniform diameter tube is considerably very low for the present two-fluid model compared with that of the single-fluid model of the Herschel- Bulkley fluid. Thus, the presence of the peripheral layer helps in the functioning of the diseased arterial system.

1. Introduction

The analysis of blood flow through stenosed arteries is very important because of the fact that the cause and development of many arterial diseases leading to the malfunction of the cardiovascular system are, to a great extent, related to the flow characteristics of blood together with the geometry of the blood vessels. Among the various arterial diseases, the development of arteriosclerosis in blood vessels is quite common which may be attributed to the accumulation of lipids in the arterial wall or pathological changes in the tissue structure 1. Arteries are narrowed by the development of atherosclerotic plaques that protrude into the lumen, resulting in stenosed arteries. When an obstruction is developed in an artery, one of the most serious consequences is the increased resistance and the associated reduction of the blood flow to the particular vascular bed supplied by the artery. Also, the continual flow of blood may lead to shearing of the superficial layer of the plaques, parts of which may be

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deposited in some other blood vessel forming thrombus. Thus, the presence of a stenosis can lead to the serious circulatory disorder.

Several theoretical and experimental attempts have been made to study the blood flow characteristics due to the presence of a stenosis in the arterial lumen of a blood vessel2–10.

It has been reported that the hydrodynamic factors play an important role in the formation of stenosis11,12and hence, the study of the blood flow through a stenosed tube is very important. Many authors have dealt with this problem treating blood as a Newtonian fluid and assuming the flow to be steady13–16. Since the blood flow through narrow arteries is highly pulsatile, more attempts have been made to study the pulsatile flow of blood treating blood as a Newtonian fluid3,6–8,17–19. The Newtonian behavior may be true in larger arteries, but, blood, being a suspension of cells in plasma, exhibits nonNewtonian behavior at low-shear ratesγ <˙ 10/sccin small diameter arteries0.02 mm–0.1 mm; particularly, in diseased state, the actual flow is distinctly pulsatile2,20–25. Several attempts have been made to study the nonNewtonian behavior and pulsatile flow of blood through stenosed tubes2,4,9,10,26–28.

Bugliarello and Sevilla29and Cokelet30have shown experimentally that for blood flowing through narrow blood vessels, there is an outer phaseperipheral layerof plasma Newtonian fluidand an inner phasecore regionof suspension of all the erythrocytes as a nonNewtonian fluid. Their experimentally measured velocity profiles in the tubes confirm the impossibility of representing the velocity distribution by a single-phase fluid model which ignores the presence of the peripheral layer outer layer that plays a crucial role in determining the flow patterns of the system. Thus, for a realistic description of blood flow, perhaps, it is more appropriate to treat blood as a two-phase fluid model consisting of a core regioninner phasecontaining all the erythrocytes as a nonNewtonian fluid and a peripheral layerouter phase of plasma as a Newtonian fluid. Several researchers have studied the two-phase fluid models for blood flow through stenosed arteries treating the fluid in the inner phase as a nonNewtonian fluid and the fluid in the outer phase as a Newtonian fluid25,26,31–33. Srivastava and Saxena25have analyzed a two-phase fluid model for blood flow through stenosed arteries treating the suspension of all the erythrocytes in the core regioninner phaseas a Casson fluid and the plasma in the peripheral layerouter phaseis represented by a Newtonian fluid. In the present model, we study a two-phase fluid model for pulsatile flow of blood through stenosed narrow arteries assuming the fluid in the core region as a Herschel-Bulkley fluid while the fluid in the peripheral region is represented by a Newtonian fluid.

Chaturani and Ponnalagar Samy28and Sankar and Hemalatha2have mentioned that for tube diameter 0.095 mm blood behaves like Herschel-Bulkley fluid rather than power law and Bingham fluids. Iida 34 reports “The velocity profile in the arterioles having diameter less than 0.1 mm are generally explained fairly by the Casson and Herschel-Bulkley fluid models. However, the velocity profile in the arterioles whose diameters less than 0.0650 mm does not conform to the Casson fluid model, but, can still be explained by the Herschel-Bulkley model”. Furthermore, the Herschel-Bulkley fluid model can be reduced to the Newtonian fluid model, power law fluid model and Bingham fluid model for appropriate values of the power law index nand yield index τy. Since the Herschel-Bulkley fluid model’s constitutive equation has one more parameter than the Casson fluid model; one can get more detailed information about the flow characteristics by using the Herschel-Bulkley fluid model. Moreover, the Herschel-Bulkley fluid model could also be used to study the blood flow through larger arteries, since the Newtonian fluid model can be obtained as a particular case of this model. Hence, we felt that it is appropriate to represent the fluid in

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R

Rz R1z

R0 βR0 δp

RP

z Newtonian fluid

Herschel-Bulkley fluid Plug flow

μH, uH δC μN, uN

d L0

L

Figure 1: Flow geometry of an arterial stenosis with peripheral layer.

the core region of the two-phase fluid model by the Herschel-Bulkley fluid model rather than the Casson fluid model. Thus, in this paper, we study a two-phase fluid model for blood flow through mild stenosed narrow arteriesof diameter 0.02 mm–0.1 mmat low-shear rates γ <˙ 10/sectreating the fluid in the core regioninner phaseas a Herschel-Bulkley fluid and the plasma in the peripheral regionouter phaseas a Newtonian fluid.

In this study, the effects of the pulsatility, stenosis, peripheral layer and the nonNew- tonian behavior of blood are analyzed using an analytical solution. Section 2 formulates the problem mathematically and then nondimensionalises the governing equations and boundary conditions. In Section 3, the resulting nonlinear coupled implicit system of differential equations is solved using the perturbation method. The expressions for the velocity, flow rate, wall shear stress, plug core radius, and resistance to flow have been obtained.Section 4analyses the variations of these flow quantities with stenosis height, yield stress, amplitude, power law index and pulsatile Reynolds number through graphs. The estimates of wall shear stress increase factor and the increase in resistance to flow factor are calculated for the two-phase Herschel-bulkley fluid model and single-phase fluid model.

2. Mathematical Formulation

Consider an axially symmetric, laminar, pulsatile and fully developed flow of blood assumed to be incompressiblein thezdirection through a circular artery with an axially symmetric mild stenosis. It is assumed that the walls of the artery are rigid and the blood is represented by a two-phase fluid model with an inner phasecore regionof suspension of all erythrocytes as a Herschel-Bulkley fluid and an outer phaseperipheral layerof plasma as a Newtonian fluid. The geometry of the stenosis is shown inFigure 1. We have used the cylindrical polar coordinatesr, φ, zwhose origin is located on the vesselstenosed artery axis. It can be shown that the radial velocity is negligibly small and can be neglected for a low Reynolds number flow in a tube with mild stenosis. In this case, the basic momentum equations governing the flow are

ρH∂uH

∂t∂p

∂z−1 r

∂rr τH in 0≤rR1z, 2.1

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ρN∂uN

∂t∂p

∂z −1 r

∂rr τN inR1z≤rRz, 2.2

0−∂p

∂r, 2.3

where the shear stress τr z| −τr z sinceτ τH orτ τN. Herschel-Bulkley fluid is a nonNewtonian fluid which is widely used in many areas of fluid dynamics, for example, dam break flows, flow of polymers, blood, and semisolids. Herschel-Bulkley fluid is a nonNewtonian fluid with nonzero yield stress which is generally used in the studies of blood flow through narrow arteries at low-shear rate. Herschel-Bulkley equation is an empirical relation which connects shear stress and shear rate through the viscosity which is given in2.4and 2.5. The relations between the shear stress and the strain rate of the fluids in motion in the core regionfor Herschel-Bulkley fluidand in the peripheral region for Newtonian fluidare given by

τH n

μH ∂uH

∂r

τy ifτHτy, RprR1z, 2.4

∂uH

∂r 0 ifτHτy, 0≤rRp, 2.5 τN μN

∂uN

∂r

ifR1z≤rRz, 2.6

whereuH,uNare the axial component of the fluid’s velocity in the core region and peripheral region; τH, τN are the shear stress of the Herschel-Bulkley fluid and Newtonian fluid;

μH, μNare the viscosities of the Herschel-Bulkley fluid and Newtonian fluid with respective dimensions ML−1T−2nT and ML−1T−1;ρH, ρN are the densities of the Herschel-Bulkley fluid and Newtonian fluid;pis the pressure,t; is the time;τy is the yield stress. From2.5, it is clear that the velocity gradient vanishes in the region where the shear stress is less than the yield stress which implies a plug flow wheneverτHτy. However, the fluid behavior is indicated wheneverτHτy. The geometry of the stenosis in the peripheral region as shown inFigure 1is given by

Rz

⎧⎪

⎪⎪

⎪⎪

⎪⎩

R0 in the normal artery region,

R0δp

2 1cos2π L0

zdL0 2

indzdL0,

2.7

whereRzis the radius of the stenosed artery with peripheral layer,R0 is the radius of the normal artery,L0is the length of the stenosis,dindicates its location, andδpis the maximum depth of the stenosis in the peripheral layer such that δP/R0 1. The geometry of the

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stenosis in the core region as seen inFigure 1is given by

R1z

⎧⎪

⎪⎩

βR0 in the normal artery region,

βR0δC

2 1cos2π L0

zdL0

2

indzdL0, 2.8

whereR1zis the radius of the stenosed core region of the artery,βis the ratio of the central core radius to the normal artery radius, βR0 is the radius of the core region of the normal artery, andδCis the maximum depth of the stenosis in the core region such thatδC/R01.

The boundary conditions are

i τH is finite and ∂uH

∂r 0 atr0, ii τHτN atr R1z,

iii uHuN atr R1z, iv uN0 atrRz.

2.9

Since the pressure gradient is a function ofzandt, we take

∂p

∂z qzf t

, 2.10

whereqz −∂p/∂zz,0,ft 1Asinωt,Ais the amplitude of the flow andωis the angular frequency of the blood flow. Since any periodic function can be expanded in a series of sines of multiple angles using Fourier series, it is reasonable to chooseft 1Asinωt as a good approximation. We introduce the following nondimensional variables

z z

R0, Rz Rz

R0 , R1z R1z

R0 , r r

R0, tωt, d d

R0, L0 L0 R0, qz qz

q0 , uH uH q0R20/4μ0

, uN uN q0R20/4μN

, τH τH

q0R0/2, τN τN q0R0/2,

θ τy

q0R0/2, α2H R20ω ρH

μ0 , α2N R20ω ρN

μN , Rp Rp

R0

, δp δp

R0

, δC δC

R0

,

2.11

where μ0 μH2/q0R0n−1, having the dimension as that of the Newtonian fluid’s viscosity,q0is the negative of the pressure gradient in the normal artery,αH is the pulsatile Reynolds number or generalized Wormersly frequency parameter and whenn 1, we get

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the Wormersly frequency parameterαN of the Newtonian fluid. Using the nondimensional variables,2.1,2.2,2.4,2.5, and2.6reduce, respectively, to

α2H∂uH

∂t 4qzft−2 r

∂rH if 0≤rR1z, 2.12 α2N∂uN

∂t 4qzft−2 r

∂rN if R1z≤rRz, 2.13 τH n

−1 2

∂uH

∂r θ ifτHθ, RprR1z, 2.14

∂uH

∂r 0 ifτHθ, 0≤rRp, 2.15 τN −1

2

∂uN

∂r ifR1z≤rRz, 2.16

whereft 1Asint. The boundary conditionsin dimensionless formare i τH is finite atr0,

ii ∂uH

∂r 0 atr 0, iii τHτN atr R1z, iv uHuN atrR1z,

v uN0 atrRz.

2.17

The geometry of the stenosis in the peripheral regionin dimensionless formis given by

Rz

⎧⎪

⎪⎩

1 in the normal artery region,

1−δp

2

1cos 2π L0

zdL0 2

indzdL0. 2.18

The geometry of the stenosis in the core regionin dimensionless formis given by

R1z

⎧⎨

β in the normal artery region,

βδC

2

1cos 2π L0

zdL0

2

indzdL0. 2.19

The nondimensional volume flow rateQis given by

Q4 Rz

0

ur, z, tr dr, 2.20

whereQQ/πR40q0/8μ0,Qis the volume flow rate.

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3. Method of Solution

When we nondimensionalize the constitutive equations2.1 and 2.2,α2H and α2N occur naturally and these pulsatile Reynolds numbers are time dependent and hence, it is more appropriate to expand2.12–2.16aboutα2Handα2N. The plug core velocityup, the velocity in the core regionuH, the velocity in the peripheral regionuN, the plug core shear stressτp, the shear stress in the core regionτH, the shear stress in the peripheral regionτN, and the plug core radiusRpare expanded as follows in terms of α2H andα2N whereα2H 1 and α2N1:

uPz, t u0Pz, t α2Hu1Pz, t · · · , 3.1 uHr, z, t u0Hr, z, t α2Hu1Hr, z, t · · · , 3.2 uNr, z, t u0Nr, z, t α2Nu1Nr, z, t · · ·, 3.3 τPz, t τ0Pz, t α2Hτ1Pz, t · · · , 3.4 τHr, z, t τ0Hr, z, t α2Hτ1Hr, z, t · · ·, 3.5 τNr, z, t τ0Nr, z, t α2Nτ1Nr, z, t · · ·, 3.6 RPz, t R0Pz, t α2HR1Pz, t · · ·. 3.7

Substituting3.2, 3.5 in 2.12 and then equating the constant terms andα2H terms, we obtain

∂r0H 2qzftr, 3.8

∂u0H

∂t −2 r

∂r1H. 3.9

Applying3.2,3.5in2.14and then equating the constant terms andα2Hterms, one can get

∂u0H

∂r0Hn−1τ0Hnθ, 3.10

∂u1H

∂r 2nτ0Hn−2τ1Hτ0H−n−1θ. 3.11

Using3.3and3.6in2.13and then equating the constant terms andα2Nterms, we get

∂r0N 2qzftr, 3.12

∂u0N

∂t −2 r

∂r1N. 3.13

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On substituting3.3and3.6in2.16and then equating the constant terms andα2N terms, one can obtain

∂u0N

∂r0N, 3.14

∂u1N

∂r1N. 3.15

Using3.1–3.6in2.17and then equating the constant terms andα2Handα2N terms, the boundary conditions are simplified, respectively, to

τ0P, τ1P are finite atr 0, 3.16

∂u0P

∂r 0, ∂u1P

∂r 0 atr 0, 3.17

τ0Hτ0N atr R1z, 3.18

τ1Hτ1N atr R1z, 3.19

u0Hu0N atr R1z, 3.20

u1Hu1N atr R1z, 3.21

u0N 0 atrRz, 3.22

u1N0 atrRz. 3.23

Equations3.8–3.11and3.12–3.15are the system of differential equations which can be solved for the unknownsu0H, u1H, τ0H, τ1Handu0N, u1N, τ0N, τ1N, respectively, with the help of boundary conditions3.16–3.23. Integrating3.8between 0 andR0P and applying the boundary condition3.16, we get

τ0P qzftR0P. 3.24

Integrating3.8betweenR0P andrand then making use of3.24, we get

τ0Hqzftr. 3.25

Integrating3.12betweenR1andrand then using3.18, one can get

τ0Nqzftr. 3.26

Integrating3.14betweenrandRand then making use of3.22, we obtain

u0N qzftR2

1−r R

2

. 3.27

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Integrating3.10betweenrandR1and using the boundary condition3.20, we get

u0H

qzftR R

1−

R1 R

2

2

qzftR1

n R1

1 n1

1−

r R1

n1

k2 R1

1−

r R1

n ,

3.28

wherek2 θ/qzft. The plug core velocityu0Pcan be obtained from3.28by replacing rbyR0P as

u0P

qzftR R

1−

R1

R 2

2

qzftR1

n R1

1 n1

1−

R0p

R1

n1

k2 R1

1−

R0p

R1

n .

3.29

Neglecting the terms with α2H and higher powers of αH in 3.7 and using 3.24, the expression forR0P is obtained as

r|τ0PθR0P θ

qzft

k2. 3.30

Similarly, solving3.9,3.11, 3.13, and 3.15with the help of 3.24–3.29, and using 3.19,3.21and3.23, the expressions forτ1P, τ1H, τ1N, u1H, andu1P can be obtained as

τ1P −1 4

qzftR BR2

k2 R

1−

R1

R 2

qzftR1

n

BR21

n 2n1

k2 R1

−n−1 2

k2 R1

2

n

2n1 k2

R1

n2

,

3.31

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τ1H−1 4

qzftR BR2r

R

1− R1

R 2

qzftR1

n BR21

× n

n1n3

n3 2

r R1

r

R1

n2

−n−1 n2

k2 R1

n2 2

r R1

r

R1

n1

− 3

n22n−2

2n2n3

k2 R1

n3 R1

r

⎤⎦,

3.32

τ1N

qzftR

BRR1 1 4

r R1

−1 8

R1 R

2 R1

r

−1 8

R1 R

2 r R1

3

qzftR1

n

BR21 n 2n3

R1 r

nn−1 2n2

k2 R1

R1 r

− 3

n22n−2

2n2n3

k2 R1

n3 R1

r

⎤⎦,

3.33

u1N−2

qzftR BR2R1

1 8

R R1

1−r

R 2

−1 8

R1 R

3 log

R r

− 1 32

R R1

1−r

R 4

−2

qzftR1

n

BR31log R

r

n

2n3− nn−1 2n2

k2 R1

− 3

n22n−2

2n2n3

k2 R1

n3

,

3.34

u1H−2

qzftR

BR2R1 3 32

R R1

−1 8

R1

R

1 32

R1

R 3

1 8

R1

R 3

log R1

R

2

qzftR1

n

BR31log R1

R

×

n

2n3−nn−1 2n2

k2 R1

− 3

n22n−2

2n2n3

k2 R1

n3

n

qzftR1

n BR1R2

1−

R1

R 2

(11)

× 1 2n1

1−

r R1

n1

−n−1 2n

k2 R1

1−

r R1

n

−2n

qzftR1

2n−1 BR31

× n

2n12

1− r

R1 n1

− n−1 2n1

k2 R1

1−

r R1

n

n

2n12n3

1− r

R1

2n2

n−1

2n26n3 n1n2n32n1

k2 R1

1−

r R1

2n1

− n−1 2n1

k2 R1

1−

r R1

n1

n−12 2n

k2 R1

2 1−

r R1

n

− n−12 2nn2

k2 R1

2 1−

r R1

2n

− 3

n22n−2 2n−1n2n3

k2 R1

n3 1−

r R1

n−1

3n−1

n22n−2 2n−2n2n3

k2 R1

n4 1−

r R1

n−2

,

3.35 u1P −2

qzftR

BR2R1 3 32

R R1

−1 8

R1

R

1 32

R1

R 3

1 8

R1

R 3

log R1

R

2

qzftR1

n

BR31log R1

R

×

n

2n3−nn−1 2n2

k2 R1

− 3

n22n−2

2n2n3

k2 R1

n3

n

qzftR1

n BR1R2

1−

R1

R 2

×

⎣ 1 2n1

⎧⎨

⎩1−

k2 R1

n1

⎭−n−1 2n

k2 R1

1−

k2 R1

n

⎦−2n

qzftR1

2n−1 BR31

×

n 2n12

⎧⎨

⎩1− k2

R1

n1

⎭− n−1 2n1

k2 R1

1−

k2 R1

n

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n 2n12n3

⎧⎨

⎩1− k2

R1

2n2

n−1

2n26n3 n1n2n32n1

k2 R1

⎧⎨

⎩1− k2

R1

2n1

− n−1 2n1

k2 R1

⎧⎨

⎩1− k2

R1

n1

⎭n−12 2n

k2 R1

2 1−

k2 R1

n

− n−12 2nn2

k2 R1

2

⎩1− k2

R1 2n

− 3

n22n−2 2n−1n2n3

k2 R1

n3

⎩1− k2

R1

n−1

3n−1

n22n−2 2n−2n2n3

k2 R1

n4

⎩1− k2

R1 n−2

,

3.36 whereB 1/ftdft/dt. The expression for velocityuH can be easily obtained from 3.2,3.28and 3.35. Similarly, the expressions foruN, τH, and τN can be obtained. The expression for wall shear stressτwcan be obtained by evaluatingτN atr Rand is given below:

τw

τ0Nα2Nτ1N

rR τ0wα2Nτ1w

qzftR α2N

−1 8

qzftR

BR2 1− R1

R 4

α2N

qzftR1

n

2n2n3BR21 R1

R

×

nn2−nn−1n3 k2

R1

−3

n22n−2k2 R1

n3

⎫⎬

.

3.37

From 2.20 and 3.27, 3.28, 3.29, 3.34, 3.35, and 3.36, the volume flow rate is calculated and is given by

Q4

R0P

0

u0Pα2Hu1P

r dr

R1

R0P

u0Hα2Hu1H

r dr

R

R1

u0Nα2u1N

r dr

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4

qzftR R3

1−

R1 R

2

k2

R1

2 1

4

1− R1

R 2

4

qzftR1

n R31 n2n3

⎣n2−nn3 k2

R1

n22n−2k2 R1

n3

2H

qzftR BR2R31

3 32

R R1

−1 8

R1

R

1 32

R1

R 3

1 8

R1

R 3

log R1

R

qzftR1

n

BR51log R1

R

×

⎧⎨

n

2n3−nn−1 2n2

k2 R1

− 3

n22n−2

2n2n3

k2 R1

n3

n

qzftR1

n BR2R31

1−

R1 R

2

×

⎧⎨

⎩ 1

4n3− n−1 4n2

k2 R1

n2n−5

4n2n3

k2 R1

n3

n

qzftR1

2n−1 BR51

×

n

2n2n3− nn−1

4n212n5 n2n32n12n3

k2 R1

nn−12

2n1n2

k2 R1

2

n3−2n2−11n6 2n1n2n3

k2 R1

n3

−n−1

n3−2n2−11n6 2nn2n3

k2 R1

n4

4n514n4−8n3−45n2−3n18 2nn1n2n32n3

k2 R1

2n4

⎦ 4α2N

qzftR BR4R1

× 1

24 R

R1

− 3 32

R1 R

5

96 R1

R 5

− 1 8

R1 R

3

logR1 1−

R1 R

2

qzftR1

n

BR2R31

1− R1

R 2

12 logR1

×

⎧⎨

n

4n3−nn−1 4n2

k2 R1

− 3

n22n−2

4n2n3

k2 R1

n3

. 3.38

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The second approximation to plug core radiusR1P can be obtained by neglecting the terms with α4H and higher powers of αH in3.7in the following manner. The shear stressτH τ0Hα2Hτ1HatrRPis given by

!!!τ0Hα2Hτ1H!!!

rRP θ. 3.39

Equation3.39reflects the fact that on the boundary of the plug core region, the shear stress is the same as the yield stress. Using the Cityplace Taylor’s series ofτ0Handτ1H aboutR0P and usingτ0H|rR0P θ, we get

R1P 1

qzft

−τ1H|rR0P

. 3.40

With the help of3.7,3.30,3.32, and3.40, the expression forRP can be obtained as

RP k2

2HR2 4

qzftR k2

R

1− R1

R 2

nBα2HR21 2n1

qzftR1

n

k2

R1

n2−1 n

k2 R1

2

k2

R1 n2

.

3.41

The resistance to flow in the artery is given by

Λ

qzft

Q . 3.42

WhenR1 R, the present model reduces to the single fluid modelHerschel-Bulkley fluid modeland in such case, the expressions obtained in the present model for velocityuH, shear stressτH,wall shear stressτw,flow rateQ, and plug core radiusRP are in good agreement with those of Sankar and Hemalatha2.

4. Numerical Simulation of Results and Discussion

The objective of the present model is to understand and bring out the salient features of the effects of the pulsatility of the flow, nonNewtonian nature of blood, peripheral layer and stenosis size on various flow quantities. It is generally observed that the typical value of the power law indexnfor blood flow models is taken to lie between 0.9 and 1.1 and we have used the typical value ofnto be 0.95 forn <1 and 1.05 forn >12. Since the value of yield stress is 0.04 dyne/cm2 for blood at a haematocrit of 4035, the nonNewtonian effects are more pronounced as the yield stress value increases, in particular, when it flows through narrow blood vessels. In diseased state, the value of yield stress is quite highalmost five times 28.

In this study, we have used the range from 0.1 to 0.3 for the nondimensional yield stressθ.

To compare the present results with the earlier results, we have used the yield stress value as

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0.01 and 0.04. Though the range of the amplitude A varies from 0 to 1, we use the range from 0.1 to 0.5 to pronounce its effect.

The ratio α αNHbetween the pulsatile Reynolds numbers of the Newtonian fluid and Herschel-Bulkley fluid is called pulsatile Reynolds number ratio. Though the pulsatile Reynolds number ratioαranges from 0 to 1; it is appropriate to assume its value as 0.5 25. Although the pulsatile Reynolds numberαH of the Herschel-Bulkley fluid also ranges from 0 to 1 2, the values 0.5 and 0.25 are used to analyze its effect on the flow quantities. Given the values ofαandαH, the value ofαNcan be obtained fromα αNH. The value of the ratio β of central core radius βR0 to the normal artery radiusR0 in the unobstructed artery is generally taken as 0.95 and 0.98525. Following Shukla et al.26, we have used the relationsR1 βRand δC βδP to estimate R1 andδC. The maximum thickness of the stenosis in the peripheral regionδP is taken in the range from 0.1 to 0.1525.

To compare the present results with the results of Sankar and Hemalatha2for single fluid model, we have used the value 0.2 forδC. To deduce the present model to a single fluid model Newtonian fluid model or Herschel-Bulkley fluid modeland to compare the results with earlier results, we have used the value ofβas 1.

It is observed that in3.38,ft, R, andθare known andQandqzare the unknowns to be determined. A careful analysis of3.38reveals the fact thatqzis the pressure gradient of the steady flow. Thus, if steady flow is assumed, then3.38can be solved forqz 2,10.

For steady flow,3.38reduces to

R2R212 R

R1 2

R2R21 x3

4 n2n3

×"

n2Rn31 xn3nn3θRn21 xn2

n22n−2 θn3#

QSx30,

4.1

where x qz and QS is the steady state flow rate. Equation4.1 can be solved for x numerically for a given value of n, QSand θ. Equation 4.1 has been solved numerically forxusing Newton-Raphson method with variation in the axial direction and yield stress withβ 0.95 andδP 0.1. Throughout the analysis, the steady flow rateQSvalue is taken as 1.0. Only that root which gives the realistic value for plug core radius has been considered there are only two real roots in the range from 0 to 20 and the other root gives values of plug core radius that exceeds the tube radiusR.

4.1. Pressure Gradient

The variation of pressure gradient with axial distance for different fluid models in the core region is shown inFigure 2. It has been observed that the pressure gradient for the Newtonian fluidsingle fluid modelis lower than that of the two fluid models withn 1.05 andθ 0.1 fromz 4 to 4.5 and z 5.5 to 6, and higher than that of the two fluid models from z4.5 toz 5.5 and these ranges are changed with increase in the value of the yield stress θ and a decrease in the value of the power law indexn. The plot for the Newtonian fluid modelsingle phase fluid modelis in good agreement with that in Figure 2 of Sankar and Hemalatha 2. Figure 2 depicts the effects of nonNewtonian nature of blood on pressure gradient.

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0 0.5 1 1.5 2 2.5 3

Pressuregradientqz

4 4.5 5 5.5 6

Axial distancez n0.95, θ0.1 n0.95, θ0.2

n1.05, θ0.1

Power law fluid withn0.95 Newtonian fluidsingle

fluid model withβ1

Figure 2: Variation of pressure gradient with axial direction for different fluids in the core region with δP 0.1.

25 20 15 10 5 0

0 30 60 90 120 150 180 210 240 270 300 330 360 Timet

Pressuredropp

A=0.5,θ=0.1,δP=0.1

A=0.2,θ=0.1,δP=0.1

A=0.5,θ=0.15,δP=0.15 A=0.5,θ=0.15,δP=0.1

Figure 3: Variation of pressure drop in a time cycle for different values ofA,θandδPwith0.95.

4.2. Pressure Drop

The variation of pressure dropΔp across the stenosis, i.e., fromz 4 toz 6in a time cycle for different values ofA,θ, andδP withn β0.95 is depicted inFigure 3. It is clear that the pressure drop increases as timetincreases from 0to 90and then decreases from 90 to 270 and again it increases from 270 to 360. The pressure drop is maximum at 90and minimum at 270. It is also observed that for a given value ofA, the pressure drop increases with the increase of the stenosis heightδP or yield stressθwhen the other parameters held constant. Further, it is noticed that as the amplitude A increases, the pressure drop increases when t lies between 0 and 180 and decreases when t lies between 180 and 360 while θ and δP are held fixed. Figure 3 shows the simultaneous effects of the stenosis size and nonNewtonian nature of blood on pressure drop.

4.3. Plug Core Radius

The variation of plug core radiusRPwith axial distance for different values of the amplitude A and stenosis thicknessδP in the peripheral layerwith0.95,αH 0.5,θ0.1, and t60is shown inFigure 4. It is noted that the plug core radius decreases as the axial variable zvaries from 4 to 5 and it increases as z varies from 5 to 6. It is further observed that for a given value ofδP, the plug core radius decreases with the increase of the amplitudeAand the same behavior is noted as the peripheral layer stenosis thickness increases for a given value

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0.07 0.06 0.05 0.04 0.03 0.02 0.01 0

4 4.5 5 5.5 6

Axial distancez PlugcoreradiusRP

A=0.2,δP=0.1

A=0.5,δP=0.1 A=0.5,δP=0.15

Figure 4: Variation of plug core radius with axial distance for different values of A andδPwith0.95, αH0.5,θ0.1 andt60.

0.16 0.14 0.12 0.1 0.08 0.06 0.04 0.02 0

0 30 60 90 120 150 180 210 240 270 300 330 360

PlugcoreradiusRP αH=0.5,θ=0.15

αH=0.5,θ=0.1

αH=0.1,θ=0.1

Timet

Figure 5: Variation of plug core radius in a time cycle for different values ofαH andθwith0.95, δP 0.1,A0.5,t60andz5.

of the amplitudeA.Figure 4depicts the effects of stenosis height on the plug core radius of the blood vessels.

Figure 5sketches the variation of plug core radius in a time cycle for different values of the pulsatile Reynolds number αH of the Herschel-Bulkley fluid and yield stress θwith 0.95,A0.5,z5,t60, andδP 0.1. It is noted that the plug core radius decreases as timet increases from 0 to 90 and then it increases from 90 to 270 and then again it decreases from 270 to 360. The plug core radius is minimum at t 90 and maximum at t270. It has been observed that for a given value of the pulsatile Reynolds numberαH, the plug core radius increases as the yield stressθincreases. Also, it is noticed that for a given value of yield stressθand with increasing values of the pulsatile Reynolds numberαH, the plug core radius increases whentlies between 0and 90and also between 270and 360and decreases whentlies between 90and 270.Figure 5depicts the simultaneous effects of the pulsatility of the flow and the nonNewtonian nature of the blood on the plug core radius of the two-phase model.

4.4. Wall Shear Stress

Wall shear stress is an important parameter in the studies of the blood flow through arterial stenosis. Accurate predictions of wall shear stress distributions are particularly useful in the

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0 0.5 1 1.5 2 2.5 3

Wallshearstressτw

4 4.5 5 5.5 6

Axial distancez θ0.1,αN0.1

θ0.1,αN0.8

θ0.04,αN0.5,β1 single fluid model

θ0.2,αN0.8

Figure 6: Variation of wall shear stress with axial distance for different valuesθandαNwitht 45, 0.95,A0.5 andδP0.1.

3.5 3 2.5 2 1.5 1 0.5 0

0 30 60 90 120 150 180 210 240 270 300 330 360 Wallshearstressτw

A=0.2,δP=0.1

A=0.5,δP=0.1 A=0.5,δP=0.15

Timet

Figure 7: Variation of wall shear stress in a time cycle for different values ofAandδP withθ 0.1, 0.95,z5 andαN0.5.

understanding of the effects of blood flow on the endothelial cells36, 37. The variation of wall shear stress in the axial direction for different values of yield stressθ and pulsatile Reynolds numberαNof the Newtonian fluid witht45,0.95,A0.5, andδP 0.1 is plotted inFigure 6. It is found that the wall shear stress increases as the axial variable z increases from 4 to 5 and then it decreases symmetrically asz increases further from 5 to 6. For a given value of the pulsatile Reynolds numberαN, the wall shear stress increases considerably with the increase in the values of the yield stressθwhen the other parameters held constant. Also, it is noticed that for a given value of the yield stressθ and increasing values of the pulsatile Reynolds numberαN, the wall shear stress decreases slightly while the other parameters are kept as invariables. It is of interest to note that the plot for the single fluid Herschel-Bulkley model is in good agreement with that in Figure 8 of Sankar and Hemalatha 2.Figure 6shows the effects of pulsatility of the blood flow and nonNewtonian effects of the blood on the wall shear stress of the two-phase model.

Figure 7depicts the variation of wall shear stress in a time cycle for different values of the amplitudeAand peripheral stenosis heightδP withn β 0.95,θ 0.1,αN 0.5 and z 5. It can be easily seen that the wall shear stress increases as time tin degrees increases from 0to 90and then it decreases astincreases from 90to 270and then again it increases astincreases further from 270to 360. The wall shear stress is maximum at 90and

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