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Lecture 15 - Nonlinear Differential Equations

Notations:
Let u=u(x;t), xRn, n2, tR+ and u=(ux1,...,xn) where x=(x1,...xn)

Porous medium Equation:

ut=Δum,m>0ut=Δ(|u|m1u)

If m=1, we have the classical heat equation. With the heat equation, we have the maximum principle.
If u0>0 for some small open set on R then u>0 for t>0. We notice that heat in the heat equation has an infinite speed of propagation.

The physics behind the porous medium equation.

For m=2 we have ut=(u2)xx which is known as the Boussinesq equation. It models flow of a gas in a porous medium where ρ is the density of the gas and v is the velocity.

  1. Conservation of massfρt+div(ρv)=0f(0,1)
  2. Darcy's lawv=ϵμp,ϵ: permeability μ: viscosity p: pressure 
  3. Equation of stateρ=ρ0pγ,0<γ<1

Thus putting everything together we obtain:

fρt=div(p(ϵμp))=ϵμdiv(pρρ01γ)=ϵμ1ρ01γdiv(ρρ1γ1ρ)=ϵμ1ρ01γ11γ+1div(ρ1+1γ)Δρ1+1γ=

If we scale the time

tct

and choose c appropriately we can scale away the constants thus:

ρt=Δρm

Instantaneous point source solution case of the heat solution

ut=Δu,xRn t>0

such that Rnu(x;t)=1, i.e, constant energy and when t=0 we have u(x,0)=δ(x).
Using Fourier transform, we obtain:

φ(x,t)=(4πt)n2e||x||24t

φ is the fundamental solution of the heat equation.

Now if Δu=ut:

u(x,0)=u0(x)u(x,t)=Rnφ(xy,t)u0(y) dy

Notice that if u0>0 in some (ϵ,ϵ)n and 0 elsewhere then u>0 for t>0 and notice that if u0(x)=δ(x) then u(x,t)=φ(x,t)

Self-similar solutions

ut=div(uσu),xRn,t>0u(x,0)=δ(x)

We look for a particular solution:

u(x,t)=tαθ(xtβ)

set ξ=xtβRn . Let us compute α,β and θ:

ut=αtα1θ+tαi=1nβxitβ1θξi=αtα1θβtα1i=1nξiθξiξθ

Thus

div(uσu)=tα(σ+1)2βdivξ(θσθ)

Now we have an equation:

()αtα1θβtα1ξθ=tα(σ+1)2βdivξ(θσθ)

If we require that:

α1=α(σ+1)2β

then we can cancel out the t's on both side of the equation. We also have:

1=Rnu(x,t)dx=Rntαθ(xtβ)dx

With a change of variable we obtain:

1=tα+nβRnθ(ξ)dξ

Now we our second requirement is:

()α+nβ=0

Finally we have equations () and () to solve for α and β:

α=nσn+2β=1σn+2

To obtain θ, I have to solve an Elliptic equation:

div(θσθ)+nσn+2θ+1σn+2ξθ=0

We look for a radial solution:

θ=θ(η),η=||ξ||

In this case, our elliptic equation is reduced to an ODE:

1ηn1(ηn1θσθ)+nσn+2θ+1σn+2θ=0

Which is equivalent to:

(ηn1θσθ)+1σn+2(ηnθ)=0

Integrating once we obtain:

ηn1θσθ+1σn+2ηnθ=const=0

Reducing this equation to:

θσ1θ=1σn+2η

Integrating both sides we obtain our solution:

θ(η)=(σ2(σn+2))1σ(η02η2)+1σ

Remember that Rnθ(ξ) dξ=1 which fixes η0. Thus:

u(x,t)=tαθ(xtβ)=tnσn+2(σ2(σn+2)(η02||x||2t2σn+2))+1σ