Problem #1 Assume: • Incompressible • • • ω1 ∂ 2-D flow ⇒ Vz = 0, = 0 ∂z ∂ Steady ⇒ =0 ∂t Parallel ⇒ Vr = 0 r1 r0 a) Conservation of mass for a 2-D flow is: 1 ∂ 1 ∂ ( r Vr ) + (Vθ ) = 0 r ∂r N r ∂θ =0 ∂ (Vθ ) = 0 ⇒ Vθ does not depend on θ ∂θ ⇒ Vθ = Vθ ( r ) ⇒ b) θ-mometum equation is: K ∂Vθ VV 1 ∂p 2 ∂Vr Vθ + (V ⋅ ∇)Vθ + r θ = − − 2) + ν (∇ 2Vθ + 2 ∂t ∂θ r ρ r ∂θ r N r N N Vr =0 steady Vr =0 In cylindrical coordinates: K ∂ 1 ∂ + Vθ (V ⋅ ∇) = Vr N ∂r r ∂θ =0 Thus, K 1 ∂Vθ =0 (V ⋅ ∇)Vθ + Vθ r N ∂θ =0 from continuity Also, 1 ∂ ∂Vθ 1 ∂ 2Vθ ∇ Vθ = r + 2 2 r ∂r ∂r r ∂θ 2 =0 ω0 Problem #1 Combining all of these results gives: 1 ∂p 1 ∂ ∂Vθ Vθ =ν r − ρ r ∂θ r ∂r ∂r r 2 this side is independent of θ Since the right-hand-side (RHS) is independent of θ , this requires that ∂p = constant for fixed r . But as θ varies from 0 → 2π , it must be equal at ∂θ 0 & 2π , that is p(θ = 0) = p (θ = 2π ) . If not, the solution would be discontinuous. ∂p = 0 ⇐ constant must be zero! Thus, ∂θ The differential equation for Vθ is: V 1 ∂ ∂Vθ (r ) − θ2 = 0 r ∂r ∂r r A little rearranging gives: d 1 d (rVθ ) = 0 dr r dr Integrating once gives: 1 d (rVθ ) = C1 r dr Integrating again gives: rVθ = 1 C1 r 2 + C 2 2 1 C ⇒ Vθ = C1r + 2 r 2 16.100 2002 2 Problem #1 Next, we must apply the no-slip boundary conditions to find Vθ . Specifically, at r = ro , Vθ = ω o ro at r = r1 , Vθ = ω1 r1 because flow velocity equals wall velocity in a viscous flow. So, apply r = ro & r = r1 bc’s: r r ω1 1 − ωo o 1 ro r1 C 1 C = ωo ro = C1ro + 2 2 1 r1 r0 − ro 2 r ⇒ ⇒ 0 r1 C2 1 ω1r1 = C1r1 + r r (ω − ω1 ) r1 C2 = o 1 o 2 r1 r0 − r0 r1 Or, rearranged a little gives: r − ro r r + r1ω1 o Vθ = roωo ro ro r1 r1 − − ro r1 ro r1 r1 r − r r1 c) The radial momentum equation is: K ∂Vr 1 1 ∂p V 2 ∂V + (V ⋅ ∇)Vr − Vθ2 = − + ν ∇ 2Vr − 2r − 2 θ ∂t r r r ∂θ ρ ∂r But Vr = 0 & ∂Vθ = 0 so this reduces to: ∂θ ∂p ρVθ2 = ∂r r Since ρVθ2 r ≥ 0 always, then clearly ∂p ≥ 0. ∂r Thus, pressure increases with r . 16.100 2002 3 Problem #1 d) On the inner cylinder, the moment is a result of the skin friction due to the fluid shear stress. For this flow in which only Vθ ≠ 0 and is only a function of r , the only non-zero shear stress is τ rθ and has the following form: ∂ V ∂Vθ Vθ − = µ r θ ∂r r ∂r r τ rθ = µ =ε rθ , the only non-zero strain 16.100 2002 4 Problem #1 Rotating Cylinders ω1 ωo For the problem you studied in the homework: 1. What direction is the fluid element acceleration? 2. What direction are the net pressure forces on a fluid element? 3. What direction are the net viscous forces on a fluid element? 16.100 2002 5