Closed and exact differential forms


In mathematics, especially vector calculus and differential topology, a closed form is a differential form α whose exterior derivative is zero, and an exact form is a differential form, α, that is the exterior derivative of another differential form β. Thus, an exact form is in the image of d, and a closed form is in the kernel of d.
For an exact form α, for some differential form β of degree one less than that of α. The form β is called a "potential form" or "primitive" for α. Since the exterior derivative of a closed form is zero, β is not unique, but can be modified by the addition of any closed form of degree one less than that of α.
Because, any exact form is necessarily closed. The question of whether every closed form is exact depends on the topology of the domain of interest. On a contractible domain, every closed form is exact by the Poincaré lemma. More general questions of this kind on an arbitrary differentiable manifold are the subject of de Rham cohomology, which allows one to obtain purely topological information using differential methods.

Examples

A simple example of a form which is closed but not exact is the 1-form given by the derivative of argument on the punctured plane. Since is not actually a function is not an exact form. Still, has vanishing derivative and is therefore closed.
Note that the argument is only defined up to an integer multiple of since a single point can be assigned different arguments,, etc. We can assign arguments in a locally consistent manner around, but not in a globally consistent manner. This is because if we trace a loop from counterclockwise around the origin and back to, the argument increases by. Generally, the argument changes by
over a counter-clockwise oriented loop.
Even though the argument is not technically a function, the different local definitions of at a point differ from one another by constants. Since the derivative at only uses local data, and since functions that differ by a constant have the same derivative, the argument has a globally well-defined derivative "".
The upshot is that is a one-form on that is not actually the derivative of any well-defined function. We say that is not exact. Explicitly, is given as:
which by inspection has derivative zero. Because has vanishing derivative, we say that it is closed.
This form generates the de Rham cohomology group meaning that any closed form is the sum of an exact form and a multiple of where accounts for a non-trivial contour integral around the origin, which is the only obstruction to a closed form on the punctured plane being the derivative of a globally defined function.

Examples in low dimensions

Differential forms in R2 and R3 were well known in the mathematical physics of the nineteenth century. In the plane, 0-forms are just functions, and 2-forms are functions times the basic area element, so that it is the 1-forms
that are of real interest. The formula for the exterior derivative d here is
where the subscripts denote partial derivatives. Therefore the condition for to be closed is
In this case if is a function then
The implication from 'exact' to 'closed' is then a consequence of the symmetry of second derivatives, with respect to x and y.
The gradient theorem asserts that a 1-form is exact if and only if the line integral of the form depends only on the endpoints of the curve, or equivalently,
if the integral around any smooth closed curve is zero.

Vector field analogies

On a Riemannian manifold, or more generally a pseudo-Riemannian manifold, k-forms correspond to k-vector fields, so there is a notion of a vector field corresponding to a closed or exact form.
In 3 dimensions, an exact vector field is called a conservative vector field, meaning that it is the derivative of a 0-form, called the scalar potential. A closed vector field is one whose derivative vanishes, and is called an irrotational vector field.
Thinking of a vector field as a 2-form instead, a closed vector field is one whose derivative vanishes, and is called an incompressible flow. The term incompressible is used because a non-zero divergence corresponds to the presence of sources and sinks in analogy with a fluid.
The concepts of conservative and incompressible vector fields generalize to n dimensions, because gradient and divergence generalize to n dimensions; curl is defined only in three dimensions, thus the concept of irrotational vector field does not generalize in this way.

Poincaré lemma

The Poincaré lemma states that if B is an open ball in Rn, any smooth closed p-form ω defined on B is exact, for any integer p with.
Translating if necessary, it can be assumed that the ball B has centre 0. Let αs be the flow on Rn defined by. For it carries B into itself and induces an action on functions and differential forms.
The derivative of the flow is the vector field X defined on functions f by : it is the radial vector field. The derivative of the flow on forms defines the Lie derivative with respect to X given by. In particular
Now define
By the fundamental theorem of calculus we have that
With being the interior multiplication or contraction by the vector field X, Cartan's formula states that
Using the fact that d commutes with LX, and h, we get:
Setting
leads to the identity
It now follows that if ω is closed, i. e., then, so that ω is exact and the Poincaré lemma is proved.

The same method applies to any open set in Rn that is star-shaped about 0, i.e. any open set containing 0 and invariant under αt for.
Another standard proof of the Poincaré lemma uses the homotopy invariance formula and can be found in,, and. The local form of the homotopy operator is described in and the connection of the lemma with the Maurer-Cartan form is explained in..
This formulation can be phrased in terms of homotopies between open domains U in Rm and V in Rn. If F is a homotopy from x U to V, set Ft = F. For a p-form on V, define
Then
Example: In two dimensions the Poincaré lemma can be proved directly for closed 1-forms and 2-forms as follows.
If is a closed 1-form on, then. If then and. Set
so that. Then must satisfy and. The right hand side here is independent of x since its partial derivative with respect to x is 0. So
and hence
Similarly, if then with. Thus a solution is given by and

Formulation as cohomology

When the difference of two closed forms is an exact form, they are said to be cohomologous to each other. That is, if ζ and η are closed forms, and one can find some β such that
then one says that ζ and η are cohomologous to each other. Exact forms are sometimes said to be cohomologous to zero. The set of all forms cohomologous to a given form is called a de Rham cohomology class; the general study of such classes is known as cohomology. It makes no real sense to ask whether a 0-form is exact, since d increases degree by 1; but the clues from topology suggest that only the zero function should be called "exact". The cohomology classes are identified with locally constant functions.
Using contracting homotopies similar to the one used in the proof of the Poincaré lemma, it can be shown that de Rham cohomology is homotopy-invariant.

Application in electrodynamics

In electrodynamics, the case of the magnetic field produced by a stationary electrical current is important. There one deals with the vector potential of this field. This case corresponds to, and the defining region is the full The current-density vector is It corresponds to the current two-form
For the magnetic field one has analogous results: it corresponds to the induction two-form and can be derived from the vector potential, or the corresponding one-form,
Thereby the vector potential corresponds to the potential one-form
The closedness of the magnetic-induction two-form corresponds to the property of the magnetic field that it is source-free: i.e. that there are no magnetic monopoles.
In a special gauge,, this implies for i = 1, 2, 3
This equation is remarkable, because it corresponds completely to a well-known formula for the electrical field, namely for the electrostatic Coulomb potential of a charge density. At this place one can already guess that
can be unified to quantities with six rsp. four nontrivial components, which is the basis of the relativistic invariance of the Maxwell equations.
If the condition of stationarity is left, on the l.h.s. of the above-mentioned equation one must add, in the equations for to the three space coordinates, as a fourth variable also the time t, whereas on the r.h.s., in the so-called "retarded time", must be used, i.e. it is added to the argument of the current-density. Finally, as before, one integrates over the three primed space coordinates.

Footnotes