2. The Navier-Stokes Equation Flashcards
fluid momentum transport, constitutive equation, the navier-stokes equation, hydrostatic and dynamic pressure, boundary conditions, one dimensional flow examples, the reynolds number
Fluid Momentum Transport
Newton’s Second Law
-consider a fixed volume V:
rate of change of momentum in V) = (net inward flow of momentum through S) + (net force acting on V
Fluid Momentum Transport
Rate of Change of Momentum in V
I = ∫ ∂/∂t (ρu_) dV
-or in suffix notation:
Ii = ∫ ∂/∂t (ρui) dV
Fluid Momentum Transport
Net Inward Flow of Momentum Through S
II = - ∫ ∇ . (ρu_u_) dV
-or in suffix notation:
IIi = ∫ ∂/∂xj (ρuiuj) dV
Fluid Momentum Transport
Net Force Acting on V
III = ∫ ρg_ dV (+other volume forces) + ∫ f_ dS
-where f_ is the force density
-or in suffix notation:
IIIi = ∫ ρgi dV + ∫ ∂τji/∂xj dV
Force Density
fi = nj*τji
-where n is the normal and τ is the total stress tensor
Momentum Equation
ρ∂u_/∂t + ρ(u_.∇)u_ = ρg_ + ∇.τ
-where τ is a matrix
-alternatively:
ρDu_/Dt = ρg_ + ∇.τ
Constitutive Equations
Case 1: Ideal Fluid
-for an ideal/inviscid fluid, the only surface force is due to the pressure:
f_ = -Pn_ = n_τ
-or in suffix notation:
fi = -Pni = njτji
-sub into the momentum equation to get the Euler equation:
ρ∂u_/∂t + ρ(u_.∇)u_ = ρg_ + ∇P_
Constitutive Equations
Case 2: Newtonian Fluid
-total stress tensor: τij = -P𝛿ij + σij -where: σij = μ(∂ui/∂xj + ∂uj/∂xi) -so: τij = -P𝛿ij + μ(∂ui/∂xj + ∂uj/∂xi) -sub this into the momentum equation to obtain the Navier-Stokes equation
Navier-Stokes Equation
ρ(∂u_/∂t + (u_.∇)u_
= ρg_ - ∇P + μ∇²u_
Navier-Stokes Equation
In the Absence of Flow
-in the absence of flow the Navier-Stokes equation reduces to: 0_ = ρg_ - ∇P -which is easily solvable: Ph = Po + ρg_.x_ -where Ph is the hydrostatic pressure
Navier-Stokes Equation
Flow Not Driven By Gravity
-if the flow is not driven by gravity, the gravity term in N-S can be absorbed into the pressure term: p = P - Ph => ρ(∂u_/∂t + (u_.∇)u_ = - ∇p + μ∇²u_
Boundary Conditions
Solid Boundary
-for a solid impermeable boundary, fluid velocity at the boundary must be equal to the velocity of the boundary
u_ = U
-force density from the boundary wall on the fluid equal force of fluid on the wall:
f_ = n_ . τ_
Boundary Conditions
Free Surface - Dynamic Boundary Condition
-if the fluid is in contact with air (or a fluid of much lower viscosity) we can ignore the viscosity term σ and say that the only force exerted on the fluid by the air is the atmospheric pressure:
n_ . τ_ = -Pn_ + n_.σ_
= -Patm n_
-consequently there is no force parallel to the surface
-if the position of the surface is given by f(x_,t)=0 and all points on the surface must remain on the surface in time, then:
Df/Dt = 0
-in particular u_ . ∇f = 0
-and ∇f = n_
=>
u_ . n_ = 0
Boundary Between Immiscible Fluids
-at a boundary between two fluids of different viscosities, both the velocity u_ and the force density n_.τ_ must be continuous
-AND is the surface remains fixed in time:
u_.n_ = 0
-consequently the condition that n_.τ_ is continuous reduces to the condition that both P and μ(n_.∇u_) are continuous
Steps to Using the Navier Stokes Equation
- write out in component form
- write out the incompressibiity condition if appropriate
- consider boundary conditions
- cancel terms using the boundary conditions
- the original equations should now be much simplified and solvable