Maxwell’s Equations in Differential Forms
To this point, we’ve mostly followed a standard approach to classical electromagnetism, and nothing I’ve said should be all that new to a former physics major, although at some points we’ve infused more mathematical rigor than is typical. But now I want to go in a different direction.
Starting again with Maxwell’s equations, we see all these divergences and curls which, though familiar to many, are really heavy-duty equipment. In particular, they rely on the Riemannian structure on . We want to strip this away to find something that works without this assumption, and as a first step we’ll flip things over into differential forms.
So let’s say that the magnetic field corresponds to a
-form
, while the electric field
corresponds to a
-form
. To avoid confusion between
and the electric constant
, let’s also replace some of our constants with the speed of light —
. At the same time, we’ll replace
with a
-form
. Now Maxwell’s equations look like:
Now I want to juggle around some of these Hodge stars:
Notice that we’re never just using the -form
, but rather the
-form
. Let’s actually go back and use
to represent a
-form, so that
corresponds to the
-form
:
In the static case — where time derivatives are zero — we see how symmetric this new formulation is:
For both the -form
and the
-form
, the exterior derivative vanishes, and the operator
connects the fields to sources of physical charge and current.