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Lecture 15 - Nonlinear Differential Equations

Notations:
Let u=u(x;t), x∈Rn, n≥2, t∈R+ and ∇u=(ux1,...,xn) where x=(x1,...xn)

Porous medium Equation:

ut=Δum,m>0ut=Δ(|u|m−1u)

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=−ϵμ∇p,ϵ: permeability μ: viscosity p: pressure 
  3. Equation of stateρ=ρ0pγ,0<γ<1

Thus putting everything together we obtain:

fρt=−div(p(−ϵμ∇p))=ϵμdiv(p∇ρρ01γ)=ϵμ⋅1ρ01γdiv(ρρ1γ−1∇ρ)=ϵμ1ρ01γ11γ+1div(∇ρ1+1γ)⏟Δρ1+1γ=

If we scale the time

t→ct

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

ρt=Δρm

Instantaneous point source solution case of the heat solution

ut=Δu,x∈Rn 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(x−y,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(uσ∇u),x∈Rn,t>0u(x,0)=δ(x)

We look for a particular solution:

u(x,t)=tαθ(xtβ)

set ξ=xtβ∈Rn . Let us compute α,β and θ:

ut=αtα−1θ+tα∑i=1n−βxit−β−1θξi=αtα−1θ−βtα−1∑i=1nξiθξi⏟ξ⋅∇θ

Thus

div(uσ∇u)=tα(σ+1)−2βdivξ(θσ∇θ)

Now we have an equation:

(∗)αtα−1θ−βtα−1ξ⋅∇θ=tα(σ+1)−2βdivξ(θσ∇θ)

If we require that:

α−1=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+nβ∫Rnθ(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(θσ∇θ)+nσn+2θ+1σn+2ξ⋅∇θ=0

We look for a radial solution:

θ=θ(η),η=||ξ||

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

1ηn−1(ηn−1θσθ′)′+nσn+2θ+1σn+2θ′=0

Which is equivalent to:

(ηn−1θσθ′)′+1σn+2(ηnθ)′=0

Integrating once we obtain:

ηn−1θσθ′+1σn+2ηnθ=const=0

Reducing this equation to:

θσ−1θ′=−1σn+2η

Integrating both sides we obtain our solution:

θ(η)=(σ2(σn+2))1σ(η02−η2)+1σ

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

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