4.3: Inhomogeneous Equations
( \newcommand{\kernel}{\mathrm{null}\,}\)
Here we consider the initial value problem
◻u=w(x,t) on x∈Rn, t∈R1u(x,0)=f(x)ut(x,0)=g(x),
where ◻u:=utt−c2△u. We assume f∈C3, g∈C2 and w∈C1, which are given.
Set u=u1+u2, where u1 is a solution of problem (4.3.1)-(4.3.3) with w:=0 and u2 is the solution where f=0 and g=0 in (4.3.1)-(4.3.3). Since we have explicit solutions u1 in the cases n=1, n=2 and n=3, it remains to solve
◻u=w(x,t) on x∈Rn, t∈R1u(x,0)=0ut(x,0)=0.
The following method is called Duhamel's principle which can be considered as a generalization of the method of variations of constants in the theory of ordinary differential equations.
To solve this problem, we make the ansatz
u(x,t)=∫t0 v(x,t,s) ds,
where v is a function satisfying
◻v=0 for all s
and
v(x,s,s)=0.
From ansatz (???) and assumption (???) we get
ut=v(x,t,t)+∫t0 vt(x,t,s) ds,=∫t0 vt(x,t,s).
It follows ut(x,0)=0. The initial condition u(x,t)=0 is satisfied because of the ansatz (???). From (4.3.12) and ansatz (???) we see that
utt=vt(x,t,t)+∫t0 vtt(x,t,s) ds,△xu=∫t0 △xv(x,t,s) ds.
Therefore, since u is an ansatz for (4.3.5)-(4.3.7),
utt−c2△xu=vt(x,t,t)+∫t0(◻v)(x,t,s) ds=w(x,t).
Thus necessarily vt(x,t,t)=w(x,t), see (???). We have seen that the ansatz provides a solution of (4.3.5)-(4.3.7) if for all s
◻v=0, v(x,s,s)=0, vt(x,s,s)=w(x,s).
Let v∗(x,t,s) be a solution of
◻v=0, v(x,0,s)=0, vt(x,0,s)=w(x,s),
then
$$v(x,t,s):=v^*(x,t-s,s)\]
is a solution of (???).
In the case n=3, where v∗ is given by, see Theorem 4.2,
$$v^*(x,t,s)=\frac{1}{4\pi c^2 t}\int_{\partial B_{ct}(x)}\ w(\xi,s)\ dS_\xi.\]
Then
v(x,t,s)=v∗(x,t−s,s)=14πc2(t−s)∫∂Bc(t−s)(x) w(ξ,s) dSξ.
from ansatz (???) it follows
u(x,t)=∫t0 v(x,t,s) ds=14πc2∫t0 ∫∂Bc(t−s)(x) w(ξ,s)t−s dSξds.
Changing variables by τ=c(t−s) yields
u(x,t)=14πc2∫ct0 ∫∂Bτ(x) w(ξ,t−τ/c)τ dSξdτ=14πc2∫Bct(x) w(ξ,t−r/c)r dξ,
where r=|x−ξ|.
Formulas for the cases n=1 and n=2 follow from formulas for the associated homogeneous equation with inhomogeneous initial values for these cases.
Theorem 4.4. The solution of
◻u=w(x,t), u(x,0)=0, ut(x,0)=0,
where w∈C1, is given by:
Case n=3:
u(x,t)=14πc2∫Bct(x) w(ξ,t−r/c)r dξ,
where r=|x−ξ|, x=(x1,x2,x3), ξ=(ξ1,ξ2,ξ3).
Case n=2:
u(x,t)=14πc∫t0 (∫Bc(t−τ)(x) w(ξ,τ)√c2(t−τ)2−r2 dξ) dτ,
x=(x1,x2), ξ=(ξ1,ξ2).
Case n=1:
u(x,t)=12c∫t0 (∫x+c(t−τ)x−c(t−τ) w(ξ,τ) dξ) dτ.
Remark. The integrand on the right in formula for n=3 is called retarded potential. The integrand is taken not at t, it is taken at an earlier time t−r/c.
Contributors and Attributions
Integrated by Justin Marshall.