Fluid Mechanics: Fundamentals and Applications
Fluid Mechanics: Fundamentals and Applications
4th Edition
ISBN: 9781259696534
Author: Yunus A. Cengel Dr., John M. Cimbala
Publisher: McGraw-Hill Education
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Chapter 9, Problem 93P

An incompressible Newtonian liquid is confined between two concentric circular cylinders of infinite length-a solid inner cylinder of radius R1and a hollow, stationary outer cylinder of radius Rv(Fig. 9-93; the z-axis is out of the page). The inner cylinder rotates at angular velocity ω l . The flow is steady, laminar, and two-dimensional in the r θ -plane. The flow is also ratitionally symmetric, meaning that nothing is a function of coordinate θ and P are functions of radius r only). The flow is also circular, meaning that velocity component ( u θ = 0 everywhere. Generate an exact expression for velocity component u θ as a function of radius r and the other parameters in the problem. You may ignore gravity. (Hint: The result of Prob. 9-92 is useful.)

Chapter 9, Problem 93P, An incompressible Newtonian liquid is confined between two concentric circular cylinders of infinite
FIGURE P9-93

Expert Solution & Answer
Check Mark
To determine

The expression for velocity component uθ.

Answer to Problem 93P

The expression for velocity component uθ is Ri2ωiRo2Ri2(Ro2rr).

Explanation of Solution

Given information:

The flow is steady, laminar, two-dimensional and incompressible. The flow is rotationally symmetric means nothing is function of coordinate θ and the flow is circular means velocity component ur is 0.

The outer cylinder is fixed and angular speed of inner cylinder is ωi, radius of outer cylinder is Ro and radius of inner cylinder is Ri.

Write the expression for continuity equation.

  1r(rur)r+1r(uθ)θ=0   ....... (I)

Here, velocity components are ur and uθ, radius is r and angle is θ.

Write the expression for the θ -component of Navier-Stokes equation.

  [ρ(ur u θr+ u θr u θθ+ u r u θr)]=[1rPθ+μ(1rr(r uθ r) u θ r 2+1 r 2 2 u θ θ 22 r 2 u rθ)+ρgθ]  ......(II)

Here, density is ρ, time is t, dynamic viscosity is μ and gravitational acceleration in θ -direction is gθ.

Calculation:

Substitute 0 for ur and 0 for (uθ)θ in Equation (I).

  1r(0)r+1r(0)=00+0=00=0   ....... (IV)

Since both sides of Equation (IV) are equal, therefore continuity equation is verified.

Substitute 0 for ur, 0 for gθ, 0 for Pθ and 0 for (uθ)θ in Equation (II).

  [ρ(( 0) uθ r+ uθ r( 0)+ (0 )uθ r)]=[1r(0)+μ( 1 r r( r u θr ) uθ r2 + 1 r2 ( 0) 2 r2 ( 0))+ρ(0)]μ(1rr(r u θ r)uθr2)=0(1rr(r u θ r)uθr2)=01r(r2uθr2+uθr)uθr2=0

  2uθr2+1ruθruθr2=01ruθr+1ruθr+2uθr21ruθruθr2=01ruθr+1r(uθr+r2uθr2)1ruθruθr2=01ruθr+1rr(r( u θ r))1ruθruθr2=0

  1r(r(uθ+r( uθ r )))1ruθruθr2=01r2r2(ruθ)1ruθruθr2=01r2r2(ruθ)1r2(ruθr+uθ)=01r2r2(ruθ)1r2r(ruθ)=0

  r(1rr(ruθ))=0   ....... (V)

Change from partial derivative to total derivative in Equation (V).

  ddr(1rddr(ruθ))=0   ....... (VI)

Integrate Equation (VI) with respect to r.

  1rddr(ruθ)=C1ddr(ruθ)=C1r   ...... (VII)

Here arbitrary constant is C1.

Again, Integrate Equation (VII) with respect to r.

  ruθ=C1r22+C2uθ=C1r2+C2r   ....... (VIII)

Here, arbitrary constant is C2.

Substitute 0 for uθ and Ro for r in Equation (VIII).

  0=C1(Ro)2+C2(Ro)C2(Ro)=C1(Ro)2C2=C1Ro22   ...... (IX)

Substitute Riωi for uθ, C1Ro22 for C2 and Ri for r in Equation (VIII).

  Riωi=C1Ri2+( C 1 R o 2 2)RiRiωi=C1Ri2C1Ro22RiRiωi=C1(Ri2Ro22Ri)C1=2Ri2ωiRo2Ri2

Substitute 2Ri2ωiRo2Ri2 for C1 in Equation (IX).

  C2=( 2 R i 2 ω i R o 2 R i 2 )Ro22=Ri2Ro2ωiRo2Ri2

Substitute Ri2Ro2ωiRo2Ri2 for C2 and 2Ri2ωiRo2Ri2 for C1 in Equation (VIII).

  uθ=( 2 R i 2 ω i R o 2 R i 2 )r2+( R i 2 R o 2 ω i R o 2 R i 2 )r=Ri2rωiRo2Ri2+Ri2Ro2ωir(Ro2Ri2)=Ri2ωiRo2Ri2(Ro2rr)

Conclusion:

The expression for velocity component uθ is Ri2ωiRo2Ri2(Ro2rr).

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