Take the Fourier transform in . Since , the transformed heat equation is
Therefore
The given transform pair and the convolution theorem yield the heat-kernel solution
The convolution is
We claim that the -fold convolution is
This is true for . If it holds for and , then
and the convolution vanishes for . This is the gamma density from repeated exponential convolution.
The Fourier transform is
The convolution theorem states
Indeed, Fubini and give
Since , induction immediately verifies
For Parseval identity, take . Then
Using Fourier inversion at zero, which follows from the supplied delta identity,
and the convolution theorem gives
Apply this to . Since
one obtains the Even rational Parseval integral
Insert the transform definitions and use Fubini:
For the indicator of ,
Putting and in the convolution theorem gives
and hence
Use normalized convolution and Fourier coefficients, and define the large spectrum
By the Parseval identity and ,
so .
The convolution theorem gives
If , the part over is at most
because . On the complementary spectrum, and , so the contribution is less than . The required difference is therefore less than .
With the convention in convolution theorem, absolute integrability permits Fubini:
If is orthogonal to every translate of , then the correlation vanishes. By convolution theorem,
almost everywhere. Since vanishes only at one point, a null set, almost everywhere. By Plancherel theorem, . Orthogonal-complement characterization proves density in .