The inhomogeneous heat equation on
1 Introduction
In this note I am working out some material following Steve Shkollerβs MAT218: Lecture Notes on Partial Differential Equations. However, I have written out a number of details that were not in the original notes, and may thus have introduced errors that were not in the notes on which this is based.
Write , and for ,
Define
If is a distribution on , is also a distribution on , and in particular, if then is a distribution on . But if , for example, then is an element of , rather than merely being a distribution.
Fix . Let and ; as , we can speak about the value of at every point rather than merely almost all points.
For almost all and for all , define by
and for all define by
In other words, if , then
where
2 Truncation
For each , assume that there is some such that for almost all and for all ,
(1) |
and for all ,
We will thus obtain a formula for . In fact we will not necessarily have , but once we have an expression for we can determine the function space of which it is an element. We will then show that there is some in a certain function space such that for all and .
For all and ,
Then (1) becomes the statement that for almost all and for all ,
If , then , which is a linear ordinary differential equation, whose solution satisfies . Since , . Hence if then . If , then for almost all , . The solution of this is, for all and for all ,
Hence, for all and for all ,
We merely know that is defined for almost all , thus we only know for almost all and for all that exists. We do have that
3 π»ΒΉ
For almost all , multiply (1) by and integrate over . This is,
Integrating by parts this becomes
which is
Writing this using norms,
Integrating from to , for any ,
For almost all ,
It follows that for all (not just almost all )
so, as ,
Let
By the inequality we just established we have, for all ,
By Gronwallβs inequality, we get
As and (these two facts follow from Parsevalβs identity), it follows that
Therefore, if then
By Parsevalβs identity,
hence for all ,
If , then for all . Define by
Thus, for all ,
(2) |
Then, for some ,
It follows that for almost all , there is some whose Fourier coefficients are , and that we have
We have
i.e.
4 π»Β²
Multiply (1) by and integrate over . We get, for almost all ,
As
we have
Integrating from to ,
For almost all ,
It follows that, for all ,
Hence
Using Parsevalβs identity we have, for all ,
hence
so
It follows that, for almost all ,11 1 The reason I see that this follows involves the fact that the intersection of two sets of full measure is itself a set of full measure.
thus .
We have
i.e.
5 Solution
For all we have , and , so for all and all , is defined. The Sobolev embedding tells us that if then . So, being specific, we have . It is a fact that if , , then the partial sums of the Fourier series of converge to in the supremum norm.
For all and for each ,
It follows that, for all ,
On the other hand,
Thus for all , .
We have
Each of the four norms has limit as . Let me work out the first one. For almost all ,
Then using Parsevalβs identity,
Then,
So, for almost all and for almost all ,