Governing equations on differential form

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The Differential Equations on Conservation Form

Conservation of Mass

Apply Gauss's divergence theorem on the surface integral in Eqn. \ref{eq:governing:cont:int} gives

Ωρ𝐯𝐧dS=Ω(ρ𝐯)dV

Also, if Ω is a fixed control volume

ddtΩρdV=ΩρtdV

The continuity equation can now be written as a single volume integral.

Ω[ρt+(ρ𝐯)]dV=0

Ω is an arbitrary control volume and thus

ρt+(ρ𝐯)=0

which is the continuity equation on partial differential form.

Conservation of Momentum

As for the continuity equation, the surface integral terms are rewritten as volume integrals using Gauss's divergence theorem.

Ω(ρ𝐯𝐧)𝐯dS=Ω(ρ𝐯𝐯)dV

Ωp𝐧dS=ΩpdV

Also, if Ω is a fixed control volume

ddtΩρ𝐯dV=Ωt(ρ𝐯)dV

The momentum equation can now be written as one single volume integral

Ω[t(ρ𝐯)+(ρ𝐯𝐯)+pρ𝐟]dV=0

Ω is an arbitrary control volume and thus

t(ρ𝐯)+(ρ𝐯𝐯)+p=ρ𝐟

which is the momentum equation on partial differential form

Conservation of Energy

Gauss's divergence theorem applied to the surface integral term in the energy equation (Eqn. \ref{eq:governing:energy:int}) gives

Ωρho(𝐯𝐧)dS=Ω(ρho𝐯)dV

Fixed control volume

ddtΩρeodV=Ωt(ρeo)dV

The energy equation can now be written as

Ω[t(ρeo)+(ρho𝐯)ρ𝐟𝐯q˙ρ]dV=0

Ω is an arbitrary control volume and thus

t(ρeo)+(ρho𝐯)=ρ𝐟𝐯+q˙ρ

which is the energy equation on partial differential form

Summary

The governing equations for compressible inviscid flow on partial differential form:

ρt+(ρ𝐯)=0

t(ρ𝐯)+(ρ𝐯𝐯)+p=ρ𝐟

t(ρeo)+(ρho𝐯)=ρ𝐟𝐯+q˙ρ

The Differential Equations on Non-Conservation Form

The Substantial Derivative

The substantial derivative operator is defined as

DDt=t+𝐯

where the first term of the right hand side is the local derivative and the second term is the convective derivative.

Conservation of Mass

If we apply the substantial derivative operator to density we get

DρDt=ρt+𝐯ρ

From before we have the continuity equation on differential form as

ρt+(ρ𝐯)=0

which can be rewritten as

ρt+ρ(𝐯)+𝐯ρ=0

and thus

DρDt+ρ(𝐯)=0

Eqn. \ref{eq:governing:cont:non} says that the mass of a fluid element with a fixed set of fluid particles is constant as the element moves in space.

Conservation of Momentum

We start from the momentum equation on differential form derived above

t(ρ𝐯)+(ρ𝐯𝐯)+p=ρ𝐟

Expanding the first and the second terms gives

ρ𝐯t+𝐯ρt+ρ𝐯𝐯+𝐯(ρ𝐯)+p=ρ𝐟

Collecting terms, we can identify the substantial derivative operator applied to the velocity vector and the continuity equation.

ρ[𝐯t+𝐯𝐯]=D𝐯Dt+𝐯[ρt+ρ𝐯]=0+p=ρ𝐟

which gives us the non-conservation form of the momentum equation

D𝐯Dt+1ρp=𝐟

Conservation of Energy

The last equation on non-conservation differential form is the energy equation. We start by rewriting the energy equation on differential form (Eqn. \ref{eq:governing:energy:pde}), repeated here for convenience

t(ρeo)+(ρho𝐯)=ρ𝐟𝐯+q˙ρ

Total enthalpy, ho, is replaced with total energy, eo

ho=eo+pρ

which gives

t(ρeo)+(ρeo𝐯)+(p𝐯)=ρ𝐟𝐯+q˙ρ

Expanding the two first terms as

ρeot+eoρt+ρ𝐯eo+eo(ρ𝐯)+(p𝐯)=ρ𝐟𝐯+q˙ρ

Collecting terms, we can identify the substantial derivative operator applied on total energy, Deo/Dt and the continuity equation

ρ[eot+𝐯eo]=DeoDt+eo[ρt+(ρ𝐯)]=0+(p𝐯)=ρ𝐟𝐯+q˙ρ

and thus we end up with the energy equation on non-conservation differential form

ρDeoDt+(p𝐯)=ρ𝐟𝐯+q˙ρ

Summary

Continuity:

DρDt+ρ(𝐯)=0

Momentum:

D𝐯Dt+1ρp=𝐟

Energy:

ρDeoDt+(p𝐯)=ρ𝐟𝐯+q˙ρ

Alternative Forms of the Energy Equation

Internal Energy Formulation

Total internal energy is defined as

eo=e+12𝐯𝐯

Inserted in Eqn. \ref{eq:governing:energy:non}, this gives

ρDeDt+ρ𝐯D𝐯Dt+(p𝐯)=ρ𝐟𝐯+q˙ρ

Now, let's replace the substantial derivative D𝐯/Dt using the momentum equation on non-conservation form (Eqn. \ref{eq:governing:mom:non}).

ρDeDt𝐯p+ρ𝐟𝐯+(p𝐯)=ρ𝐟𝐯+q˙ρ

Now, expand the term (p𝐯) gives

ρDeDt𝐯p+𝐯p+p(𝐯)=q˙ρρDeDt+p(𝐯)=q˙ρ

Divide by ρ

DeDt+pρ(𝐯)=q˙

Conservation of mass gives

DρDt+ρ(𝐯)=0𝐯=1ρDρDt

Insert in Eqn. \ref{eq:governing:energy:non:b}

DeDtpρ2DρDt=q˙DeDt+pDDt(1ρ)=q˙

DeDt+pDνDt=q˙

Compare with the first law of thermodynamics: de=δqδw

Enthalpy Formulation

h=e+pρDhDt=DeDt+1ρDpDt+pDDt(1ρ)

with De/Dt from Eqn. \ref{eq:governing:energy:non:b}

DhDt=q˙pDDt(1ρ)+1ρDpDt+pDDt(1ρ)

DhDt=q˙+1ρDpDt

Total Enthalpy Formulation

ho=h+12𝐯𝐯DhoDt=DhDt+𝐯D𝐯Dt

From the momentum equation (Eqn. \ref{eq:governing:mom:non})

D𝐯Dt=𝐟1ρp

which gives

DhoDt=DhDt+𝐯𝐟1ρ𝐯p

Inserting Dh/Dt from Eqn. \ref{eq:governing:energy:non:c} gives

DhoDt=q˙+1ρDpDt+𝐯𝐟1ρ𝐯p=1ρ[DpDt𝐯p]+q˙+𝐯𝐟

The substantial derivative operator applied to pressure

DpDt=pt+𝐯p

and thus

DpDt𝐯p=pt

which gives

DhoDt=1ρpt+q˙+𝐯𝐟

If we assume adiabatic flow without body forces

DhoDt=1ρpt

If we further assume the flow to be steady state we get

DhoDt=0

This means that in a steady-state adiabatic flow without body forces, total enthalpy is constant along a streamline.