We start off with Maxwell's Equation in the Lorentz gauge:

where we use the metric signature (+,+,+,-) and



The gauge condition for the Lorentz gauge is

Introduce the Green's function at
from some impulse source at

and its Fourier transform


Translational symmetry implies

so that



where
. But



Chose the "retarded" solution, such that the function is zero unless t>t'.




![{\displaystyle ={\frac {1}{(2\pi )^{2}}}{\frac {2}{|\mathbf {r} -\mathbf {r} '|}}{\frac {2\pi }{4}}\left[\delta (|\mathbf {r} -\mathbf {r} '|+c(t-t'))-\delta (|\mathbf {r} -\mathbf {r} '|-c(t-t'))\right]\Theta }](https://wikimedia.org/api/rest_v1/media/math/render/svg/48541628af99cf28e2d003864682e6565eaa5915)
But the term
so that

Now to get the
in the half-space with z>0 with the boundary condition
at
we take the difference:

Now use Green's theorem, with the generating function

![{\displaystyle \int \partial _{\mu }F_{\mu }d^{4}r=\int cdt\int d^{3}r[\partial _{\mu }A\partial ^{\mu }G+A\partial _{\mu }\partial ^{\mu }G_{1}-\partial _{\mu }G\partial ^{\mu }A-G_{1}\partial _{\mu }\partial ^{\mu }A]}](https://wikimedia.org/api/rest_v1/media/math/render/svg/c807a3acf6af188a25a7f51900bfbaecacfcd486)

, let 

Now invoke the divergence theorem on the half space
:
, where the last term is zero by the condition of

To do the t integral, I need to bring out the z derivative. To do this, I first turn it into a z' derivative, using the relation

where 

∴ 
At
, 
If
is independent of position, as in a plane wave propagating along the z axis, then:

This gives us uniform translation of waves at velocity c. More generally:



In our case, we consider only those waves which drop off as
, so

In cylindrical coordinates,
. Without loss of generality, we consider a harmonic solution with a particular frequency ω = kc.


Special Case
Picture an opaque screen with a circular aperture of radius a.
Let
Then 
But


so that
and 
In this particular case, we are dealing with far-field effects only, so
and 
So, 
The integral
is the integral representation of the zero order Bessel function of the first kind with
as the argument. This gives us the equation:

To simplify the math, we make use of the fact that we can represent this Bessel functions as the derivative of a Bessel function of a different order. In general, the formula to compute this derivative is

In this case, we take
and
. So

This gives us the equation
We invoke the principle that the integral of a derivative is the function evaluated at the end points to give us the equation
![{\displaystyle {\mathcal {J}}(r')=2\pi {\frac {e^{ikr'}}{k\sin {\theta }'r'^{2}}}\left[aJ_{1}(ka\sin {\theta }')-0J_{1}(0k\sin {\theta }')\right]=2\pi {\frac {e^{ikr'}}{k\sin {\theta }'r'^{2}}}aJ_{1}(ka\sin {\theta }')}](https://wikimedia.org/api/rest_v1/media/math/render/svg/d2276a013157a101414698ee4e3397b2b8fef3ec)
and 
To find the angle to the first diffraction minimum, we must find the first zero of this amplitude function. This will occur when